diff options
| author | Roger Frank <rfrank@pglaf.org> | 2025-10-14 20:07:19 -0700 |
|---|---|---|
| committer | Roger Frank <rfrank@pglaf.org> | 2025-10-14 20:07:19 -0700 |
| commit | 3b6e8da7ad8c7ab79d7254310de785b7d4d9b369 (patch) | |
| tree | 9269eb72f0560e686ff17ad2f1ac8e3c9298262e /37157-t | |
Diffstat (limited to '37157-t')
| -rw-r--r-- | 37157-t/37157-t.tex | 10208 | ||||
| -rw-r--r-- | 37157-t/images/tb.pdf | bin | 0 -> 2647 bytes | |||
| -rw-r--r-- | 37157-t/old/37157-t.tex | 10206 | ||||
| -rw-r--r-- | 37157-t/old/37157-t.zip | bin | 0 -> 150626 bytes |
4 files changed, 20414 insertions, 0 deletions
diff --git a/37157-t/37157-t.tex b/37157-t/37157-t.tex new file mode 100644 index 0000000..dd19bf5 --- /dev/null +++ b/37157-t/37157-t.tex @@ -0,0 +1,10208 @@ +% %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% % +% % +% The Project Gutenberg EBook of Science and hypothesis, by Henri Poincaré% +% % +% This eBook is for the use of anyone anywhere at no cost and with % +% almost no restrictions whatsoever. You may copy it, give it away or % +% re-use it under the terms of the Project Gutenberg License included % +% with this eBook or online at www.gutenberg.net % +% % +% % +% Title: Science and hypothesis % +% % +% Author: Henri Poincaré % +% % +% Release Date: August 21, 2011 [EBook #37157] % +% Most recently updated: June 11, 2021 % +% % +% Language: English % +% % +% Character set encoding: UTF-8 % +% % +% *** START OF THIS PROJECT GUTENBERG EBOOK SCIENCE AND HYPOTHESIS *** % +% % +% %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% % + +\def\ebook{37157} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% %% +%% Packages and substitutions: %% +%% %% +%% book: Required. %% +%% inputenc: Latin-1 text encoding. Required. %% +%% fontenc: Font encoding, to hyphenate accented words. Required. %% +%% %% +%% ifthen: Logical conditionals. Required. %% +%% %% +%% amsmath: AMS mathematics enhancements. Required. %% +%% amssymb: Additional mathematical symbols. Required. %% +%% %% +%% alltt: Fixed-width font environment. Required. %% +%% %% +%% yfonts: Gothic font on title page. Optional. %% +%% %% +%% footmisc: Start footnote numbering on each page. Required. %% +%% %% +%% graphicx: Standard interface for graphics inclusion. Required. %% +%% %% +%% calc: Length calculations. Required. %% +%% %% +%% fancyhdr: Enhanced running headers and footers. Required. %% +%% %% +%% geometry: Enhanced page layout package. Required. %% +%% hyperref: Hypertext embellishments for pdf output. Required. %% +%% %% +%% %% +%% Producer's Comments: %% +%% %% +%% OCR text for this ebook was obtained on July 30, 2011, from %% +%% http://www.archive.org/details/onriemannstheory00kleiuoft. %% +%% %% +%% Changes to the original are noted in this file as follows: %% +%% 1. \Reword{}{}: Erroneously-translated phrases. No attempt %% +%% was made to compare the French edition with the English %% +%% translation systematically. Instead, incongruous phrases %% +%% in the English edition were compared with the page scans %% +%% at http://gallica.bnf.fr/ark:/12148/bpt6k26745q and the %% +%% wording was modified as appropriate. %% +%% In-line transcriber notes, marked "[** TN: ...]" contain %% +%% the relevant text from the French edition. %% +%% %% +%% 2. \Typo{}{}: Typographical corrections, showing original %% +%% and replacement text side-by-side. %% +%% %% +%% 3. \Chg{}{} and \Add{}: Inconsistent/missing punctuation, %% +%% italicization, and capitalization. %% +%% %% +%% 4. [** TN: ...]: Lengthier miscellaneous comments. %% +%% %% +%% The following hyphenation \Chg{}{}s were made for consistency: %% +%% 1. electrostatic -> electro-static %% +%% 2. thermodynamic -> thermo-dynamic %% +%% 3. re-act[ion] -> react[ion] %% +%% Larmor's spelling "æther" in the introduction is retained. The %% +%% translation uses "ether" uniformly elsewhere. %% +%% %% +%% In Chapter I., equations and expressions that are displayed in %% +%% the French edition (but in-line in the English translation) %% +%% have been displayed. %% +%% %% +%% Fourteen pages of book catalogue at the end have been omitted. %% +%% %% +%% Compilation Flags: %% +%% %% +%% The following behavior may be controlled by boolean flags. %% +%% %% +%% ForPrinting (false by default): %% +%% If false, compile a screen optimized file (one-sided layout, %% +%% blue hyperlinks). If true, print-optimized PDF file: Larger %% +%% text block, two-sided layout, black hyperlinks. %% +%% %% +%% %% +%% PDF pages: 306 (if ForPrinting set to false) %% +%% PDF page size: 4.25 x 5.75" (non-standard) %% +%% %% +%% Summary of log file: %% +%% * One slightly overfull hbox, several harmless underfull hboxes. %% +%% %% +%% Compile History: %% +%% %% +%% August, 2011: (Andrew D. Hwang) %% +%% texlive2007, GNU/Linux %% +%% %% +%% Command block: %% +%% %% +%% pdflatex x3 %% +%% %% +%% %% +%% August 2011: pglatex. %% +%% Compile this project with: %% +%% pdflatex 37157-t.tex ..... THREE times %% +%% %% +%% pdfTeXk, Version 3.141592-1.40.3 (Web2C 7.5.6) %% +%% %% +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\listfiles +\documentclass[12pt,leqno]{book}[2005/09/16] + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%% PACKAGES %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\usepackage[utf8]{inputenc}[2006/05/05] +\usepackage[T1]{fontenc}[2005/09/27] + +\usepackage{ifthen}[2001/05/26] %% Logical conditionals + +\usepackage{amsmath}[2000/07/18] %% Displayed equations +\usepackage{amssymb}[2002/01/22] %% and additional symbols + +\usepackage{alltt}[1997/06/16] %% boilerplate, credits, license + +\IfFileExists{yfonts.sty}{% + \usepackage{yfonts}[2003/01/08] +}{% + \providecommand{\textgoth}[1]{#1}% +} +\usepackage[perpage]{footmisc}[2005/03/17] + +\usepackage{graphicx}[1999/02/16]%% For diagrams + +\usepackage{calc}[2005/08/06] + +\usepackage{fancyhdr} %% For running heads + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%%%% Interlude: Set up PRINTING (default) or SCREEN VIEWING %%%% +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +% ForPrinting=true false (default) +% Asymmetric margins Symmetric margins +% 1 : 1.6 text block aspect ratio 3 : 4 text block aspect ratio +% Black hyperlinks Blue hyperlinks +% Start major marker pages recto No blank verso pages +% +\newboolean{ForPrinting} + +%% UNCOMMENT the next line for a PRINT-OPTIMIZED VERSION of the text %% +%\setboolean{ForPrinting}{true} + +%% Initialize values to ForPrinting=false +\newcommand{\Margins}{hmarginratio=1:1} % Symmetric margins +\newcommand{\HLinkColor}{blue} % Hyperlink color +\newcommand{\PDFPageLayout}{SinglePage} +\newcommand{\TransNote}{Transcriber's Note} +\newcommand{\TransNoteCommon}{% + The camera-quality files for this public-domain ebook may be + downloaded \textit{gratis} at + \begin{center} + \texttt{www.gutenberg.org/ebooks/\ebook}. + \end{center} + + Minor typographical corrections, regularizations, and presentational + changes have been made without comment. + \bigskip + + This ebook was produced using scanned images and OCR text generously + provided by the University of Toronto Robarts Library through the + Internet Archive. + \bigskip +} + +\newcommand{\TransNoteText}{% + \TransNoteCommon + + This PDF file is optimized for screen viewing, but may be recompiled + for printing. Please consult the preamble of the \LaTeX\ source + file for instructions and other particulars. +} +%% Re-set if ForPrinting=true +\ifthenelse{\boolean{ForPrinting}}{% + \renewcommand{\Margins}{hmarginratio=2:3} % Asymmetric margins + \renewcommand{\HLinkColor}{black} % Hyperlink color + \renewcommand{\PDFPageLayout}{TwoPageRight} + \renewcommand{\TransNote}{Transcriber's Note} + \renewcommand{\TransNoteText}{% + \TransNoteCommon + + This PDF file is optimized for printing, but may be recompiled for + screen viewing. Please consult the preamble of the \LaTeX\ source + file for instructions and other particulars. + } +}{% If ForPrinting=false, don't skip to recto + \renewcommand{\cleardoublepage}{\clearpage} +} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%%%% End of PRINTING/SCREEN VIEWING code; back to packages %%%% +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +\ifthenelse{\boolean{ForPrinting}}{% + \setlength{\paperwidth}{8.5in}% + \setlength{\paperheight}{11in}% +% 1:1.6 + \usepackage[body={5in,8in},\Margins]{geometry}[2002/07/08] +}{% + \setlength{\paperwidth}{4.25in}% + \setlength{\paperheight}{5.75in}% + \raggedbottom +% 3:4 + \usepackage[body={4in,4.9in},\Margins,includeheadfoot]{geometry}[2002/07/08] +} + +\providecommand{\ebook}{00000} % Overridden during white-washing +\usepackage[pdftex, + hyperref, + hyperfootnotes=false, + pdftitle={The Project Gutenberg eBook \#\ebook: Science and Hypothesis.}, + pdfkeywords={University of Toronto, The Internet Archive, Henri Poincare, Joseph Larmor, Willian John Greenstreet, Andrew D. Hwang}, + pdfstartview=Fit, % default value + pdfstartpage=1, % default value + pdfpagemode=UseNone, % default value + bookmarks=true, % default value + linktocpage=false, % default value + pdfpagelayout=\PDFPageLayout, + pdfdisplaydoctitle, + pdfpagelabels=true, + bookmarksopen=true, + bookmarksopenlevel=0, + colorlinks=true, + linkcolor=\HLinkColor]{hyperref}[2007/02/07] + + +% Set author here to avoid numerous hyperref warnings from accents +\hypersetup{pdfauthor={Henri Poincaré}} + +%% Fixed-width environment to format PG boilerplate %% +\newenvironment{PGtext}{% +\begin{alltt} +\fontsize{7.2}{9}\ttfamily\selectfont}% +{\end{alltt}} + +%% Re-define the following as, e.g., \newcommand{\Chg}[2]{#1} to revert + +% Translation errors found during digitization +\newcommand{\Reword}[2]{#2} + +% Typographical errors found during digitization +\newcommand{\Typo}[2]{#2} + +% Stylistic changes made for consistency +\newcommand{\Chg}[2]{#2} +\newcommand{\Add}[1]{\Chg{}{#1}} + +%% Miscellaneous global parameters %% +% No hrule in page header +\renewcommand{\headrulewidth}{0pt} + +% Loosen spacing +\setlength{\emergencystretch}{1.25em} +\newcommand{\Loosen}{\spaceskip 0.5em plus 0.75em minus 0.25em} +\hyphenation{extra-ordinary} + +% Scratch pad for length calculations +\newlength{\TmpLen} + +%% Running heads %% +\newcommand{\FlushRunningHeads}{\clearpage\fancyhf{}\cleardoublepage} +\newcommand{\InitRunningHeads}{% + \setlength{\headheight}{15pt} + \pagestyle{fancy} + \thispagestyle{empty} + \ifthenelse{\boolean{ForPrinting}} + {\fancyhead[RO,LE]{\thepage}} + {\fancyhead[R]{\thepage}} +} + +% Uniform style for running heads +\newcommand{\RHeads}[1]{\textsc{\MakeLowercase{#1}}} + +\newcommand{\SetRunningHeads}[2][]{% + \fancyhead[CO]{\RHeads{#2}}% + \ifthenelse{\equal{#1}{}}{% + \fancyhead[CE]{\RHeads{Science and Hypothesis}}% + }{% + \fancyhead[CE]{\RHeads{#2}}% + }% +} + +\ifthenelse{\boolean{ForPrinting}}{% + \newcommand{\ChapTopSkip}{\vspace*{1.5in}}% +}{% + \newcommand{\ChapTopSkip}{}% +} + +\newcommand{\BookMark}[2]{\phantomsection\pdfbookmark[#1]{#2}{#2}} + +%% Major document divisions %% +\newcommand{\PGBoilerPlate}{% + \pagenumbering{Alph} + \pagestyle{empty} + \BookMark{0}{PG Boilerplate.} +} +\newcommand{\FrontMatter}{% + \cleardoublepage + \frontmatter + \BookMark{-1}{Front Matter.} +} +\newcommand{\MainMatter}{% + \FlushRunningHeads + \InitRunningHeads + \mainmatter + \BookMark{-1}{Main Matter.} +} +\newcommand{\BackMatter}{% + \FlushRunningHeads + \InitRunningHeads + \backmatter + \BookMark{-1}{Back Matter.} +} +\newcommand{\PGLicense}{% + \FlushRunningHeads + \pagenumbering{Roman} + \InitRunningHeads + \BookMark{-1}{PG License.} + \SetRunningHeads[both]{License.} +} + +%% ToC formatting %% +\AtBeginDocument{\renewcommand{\contentsname}{% + \protect\thispagestyle{empty}% + \protect\vspace*{-3\baselineskip}% + \protect\SectTitle[\Large]{Contents.}% + \protect\vspace{-\baselineskip} + } +} + +\newcommand{\TableofContents}{% + \FlushRunningHeads + \InitRunningHeads + \SetRunningHeads[both]{Contents.} + \BookMark{0}{Contents.} + \tableofcontents +} + +% For internal use, to determine if we need "PAGE" line +\newcommand{\ToCAnchor}{} +\newcounter{ChapNo} + +% \ToCLine{SecNo}{Title} +\newcommand{\ToCLine}[2]{% + \label{toc:#1}% + \ifthenelse{\not\equal{\pageref{toc:#1}}{\ToCAnchor}}{% + \renewcommand{\ToCAnchor}{\pageref{toc:#1}}% + \noindent\makebox[\textwidth][r]{\scriptsize \null\hfill PAGE}\\% + }{}% + \settowidth{\TmpLen}{999}% + \noindent\strut\parbox[b]{\textwidth-\TmpLen}{\small% + \hangindent4em\textsc{#2}\dotfill}% + \makebox[\TmpLen][r]{\pageref{chap:#1}}% +} + +%% Sectional units %% +% Typographical abstractions +\newcommand{\ChapTitle}[1]{% + \SectTitle[\Large]{#1} + {\centering\includegraphics[width=1in]{./images/tb.pdf}\par\medskip} +} +\newcommand{\SectTitle}[2][\large]{% + \subsection*{\centering\normalfont#1\MakeUppercase{#2}} +} +\newcommand{\SubsectTitle}[2][\normalsize]{% + \subsubsection*{\centering\normalfont#1\MakeUppercase{#2}} +} + +% For internal use +\newboolean{AtPart} +\newcommand{\Part}[2]{% + \setboolean{AtPart}{true} + \FlushRunningHeads + \InitRunningHeads + \BookMark{0}{Part #1 #2} + \addtocontents{toc}{\protect\SectTitle[\protect\small]{PART #1}} + \addtocontents{toc}{\protect\SubsectTitle[\protect\footnotesize]{\protect\textit{#2}}} + \ChapTopSkip + \ifthenelse{\equal{#1}{I.}}{% + \ChapTitle{Science and Hypothesis} + }{} + \SectTitle{PART #1} + \SubsectTitle{\textit{#2}} +} + +% \OtherChapter{Title}: Unnumbered units (preface, etc.) +\newcommand{\OtherChapter}[1]{% + \FlushRunningHeads + \stepcounter{ChapNo}\phantomsection\label{chap:\theChapNo}% + \addtocontents{toc}{\protect\ToCLine{\theChapNo}{#1}}% + \InitRunningHeads + \BookMark{0}{#1} + \SetRunningHeads[both]{#1} + \ChapTopSkip + \ChapTitle{#1} +} + +\newcounter{ChapCount} +\newcommand{\Chapter}[3][]{% + \ifthenelse{\boolean{AtPart}}{% + \setboolean{AtPart}{false}% + }{% + \FlushRunningHeads + \InitRunningHeads + \ChapTopSkip + } + \stepcounter{ChapNo}\phantomsection\label{chap:\theChapNo}% + \stepcounter{ChapCount}\label{chapref:\Roman{ChapCount}}% + \addtocontents{toc}{\protect\SectTitle[\protect\small]{CHAPTER \Roman{ChapCount}.}} + \addtocontents{toc}{\protect\ToCLine{\theChapNo}{#3}}% + \BookMark{1}{Chapter \Roman{ChapCount}: #3} + \ifthenelse{\equal{#1}{}}{% + \SetRunningHeads{#3} + }{% + \SetRunningHeads{#1} + } + \SectTitle{Chapter #2} + \SubsectTitle[\small]{#3} +} +\newcommand{\ChapRef}[1]{\hyperref[chapref:#1]{Chapter~#1}} + +\newcommand{\Section}[1]{\subsection*{\centering\normalsize\normalfont#1}} +\newcommand{\Subsection}[1]{% + \subsubsection*{\centering\small\normalfont\scshape\MakeLowercase{#1}} +} +\newcommand{\Par}[2][]{\par#1\textit{#2}} + +\newcommand{\Dict}[2]{% + \setlength{\TmpLen}{\parindent}% + \vfil + \par\noindent\strut\parbox[t]{0.4\textwidth}{% + \raggedright\hangindent\TmpLen#1\quad\dotfill}\hfill + \parbox[t]{0.55\textwidth}{% + \hangindent\TmpLen#2}% +% \smallskip +} + +\newcommand{\ParSkip}{\hspace*{\parindent}} + +\newcommand{\Signature}[2]{% + \null\hfill#1\ParSkip\break + \ifthenelse{\not\equal{#2}{}}{\smallskip\footnotesize\indent#2\par\normalsize}{} +} + +% Page separators and cross-referencing +\newcommand{\PageSep}[1]{\ignorespaces} + +\newcommand{\Pagelabel}[1]{\phantomsection\label{page:#1}} +\newcommand{\Pageref}[1]{\hyperref[page:#1]{p.~\pageref*{page:#1}}} +\newcommand{\Pagerefs}[2]{% + \ifthenelse{\equal{\pageref*{page:#1}}{\pageref*{page:#2}}}{% + \hyperref[page:#1]{p.~\pageref*{page:#1}}% + }{% Else + pp.~\hyperref[page:#1]{\pageref*{page:#1}},~\hyperref[page:#2]{\pageref*{page:#2}}% + }% +} + +% Miscellaneous semantics and textual conveniences +\newcommand{\Title}[1]{\textit{#1}} +\newcommand{\Foreign}[1]{\textit{#1}} + +\newcommand{\ie}{\Foreign{i.e.}} +\newcommand{\QED}{\text{Q.E.D.}} + +% To denote translator's comments +\newcommand{\Transl}{---[\textsc{Tr}.]} + +\newcommand{\First}[1]{\textsc{#1}} + +\newcommand{\Tag}[1]{#1\quad} + +%% Miscellaneous mathematical formatting %% +\newcommand{\dd}{\partial} +\DeclareInputMath{176}{{}^{\circ}} +\DeclareInputMath{183}{\cdot} + +%% Upright capital letters in math mode +\DeclareMathSymbol{A}{\mathalpha}{operators}{`A} +\DeclareMathSymbol{B}{\mathalpha}{operators}{`B} +\DeclareMathSymbol{C}{\mathalpha}{operators}{`C} +\DeclareMathSymbol{D}{\mathalpha}{operators}{`D} +\DeclareMathSymbol{F}{\mathalpha}{operators}{`F} + +\DeclareMathSymbol{K}{\mathalpha}{operators}{`K} +\DeclareMathSymbol{M}{\mathalpha}{operators}{`M} +\DeclareMathSymbol{N}{\mathalpha}{operators}{`N} + +\DeclareMathSymbol{P}{\mathalpha}{operators}{`P} +\DeclareMathSymbol{Q}{\mathalpha}{operators}{`Q} +\DeclareMathSymbol{R}{\mathalpha}{operators}{`R} +\DeclareMathSymbol{S}{\mathalpha}{operators}{`S} +\DeclareMathSymbol{T}{\mathalpha}{operators}{`T} +\DeclareMathSymbol{U}{\mathalpha}{operators}{`U} + +%%%%%%%%%%%%%%%%%%%%%%%% START OF DOCUMENT %%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{document} +%% PG BOILERPLATE %% +\PGBoilerPlate +\begin{center} +\begin{minipage}{\textwidth} +\small +\begin{PGtext} +The Project Gutenberg EBook of Science and hypothesis, by Henri Poincaré + +This eBook is for the use of anyone anywhere at no cost and with +almost no restrictions whatsoever. You may copy it, give it away or +re-use it under the terms of the Project Gutenberg License included +with this eBook or online at www.gutenberg.net + + +Title: Science and hypothesis + +Author: Henri Poincaré + +Release Date: August 21, 2011 [EBook #37157] +Most recently updated: June 11, 2021 + +Language: English + +Character set encoding: UTF-8 + +*** START OF THIS PROJECT GUTENBERG EBOOK SCIENCE AND HYPOTHESIS *** +\end{PGtext} +\end{minipage} +\end{center} +\newpage +%% Credits and transcriber's note %% +\begin{center} +\begin{minipage}{\textwidth} +\begin{PGtext} +Produced by Andrew D. Hwang +\end{PGtext} +\end{minipage} +\vfill +\end{center} + +\begin{minipage}{0.85\textwidth} +\small +\BookMark{0}{Transcriber's Note.} +\subsection*{\centering\normalfont\scshape% +\normalsize\MakeLowercase{\TransNote}}% + +\raggedright +\TransNoteText +\end{minipage} +%%%%%%%%%%%%%%%%%%%%%%%%%%% FRONT MATTER %%%%%%%%%%%%%%%%%%%%%%%%%% +\PageSep{i} +\FrontMatter +\ifthenelse{\boolean{ForPrinting}}{% +\null\vfill +{\Large SCIENCE AND HYPOTHESIS} +\vfill +\cleardoublepage +}{}% Omit half-title in screen version +\PageSep{ii} +%[Blank page] +\PageSep{iii} +\begin{center} +\huge SCIENCE \\ +AND HYPOTHESIS +\vfill + +\normalsize +{\footnotesize BY} \\ +H. POINCARÉ, \\ +{\scriptsize MEMBER OF THE INSTITUTE OF FRANCE.} +\vfill + +{\small\textsc{With a Preface by}} \\ +\textsc{J. LARMOR, D.Sc., Sec. R.S.}, \\ +{\scriptsize\textit{Lucasian Professor of Mathematics in the University of Cambridge.}} +\vfill\vfill + +\textswab{London and Newcastle-on-Tyne:} \\ +THE WALTER SCOTT PUBLISHING CO., LTD \\ +{\footnotesize NEW YORK: 3 EAST 14TH STREET.} \\ +\oldstylenums{1905}. +\end{center} +\newpage +\PageSep{iv} +%[Blank page] +\PageSep{v} +\TableofContents +\iffalse +CONTENTS. + + PAGE +Translator's Note........................ix + +Introduction.............................xi + +Author's Preface........................xxi + + +PART I. + +NUMBER AND MAGNITUDE. + +CHAPTER I. +On the Nature of Mathematical Reasoning...1 + +CHAPTER II. +Mathematical Magnitude and Experiment....17 + + +PART II. + +SPACE. + +CHAPTER III. +Non-Euclidean Geometries.................35 +\PageSep{vi} + +CHAPTER IV. +Space and Geometry.......................51 + +CHAPTER V. +Experiment and Geometry..................72 + + +PART III. + +FORCE. + +CHAPTER VI. +The Classical Mechanics..................89 + +CHAPTER VII. +Relative and Absolute Motion............111 + +CHAPTER VIII. +Energy and Thermo-dynamics..............123 + + +PART IV. + +NATURE. + +CHAPTER IX. +Hypotheses in Physics...................140 +\PageSep{vii} + +CHAPTER X. +The Theories of Modern Physics..........160 + +CHAPTER XI. +The Calculus of Probabilities...........183 + +CHAPTER XII. +Optics and Electricity..................211 + +CHAPTER XIII. +Electro-dynamics........................225 +\fi +\PageSep{viii} +%[Blank page] +\PageSep{ix} + + +\OtherChapter{Translator's Note.} + +\First{The} translator wishes to express his indebtedness +to Professor Larmor, for kindly consenting +to introduce the author of \Title{Science and Hypothesis} +to English readers; to Dr.~F.~S. Macaulay and +Mr.~C.~S. Jackson,~M.A., who have read the whole +of the proofs and have greatly helped by suggestions; +also to Professor G.~H. Bryan,~F.R.S., who +has read the proofs of \ChapRef{VIII}., and whose +criticisms have been most valuable. + +%[** TN: William John Greenstreet (1861--1930), not identified by name] +\Signature{W.\;J.\;G.}{\textit{February} 1905.} +\PageSep{x} +%[Blank page] +\PageSep{xi} + + +\OtherChapter{Introduction.} + +\First{It} is to be hoped that, as a consequence of the +present active scrutiny of our educational aims +and methods, and of the resulting encouragement +of the study of modern languages, we shall not +remain, as a nation, so much isolated from +ideas and tendencies in continental thought and +literature as we have been in the past. As things +are, however, the translation of this book is +doubtless required; at any rate, it brings vividly +before us an instructive point of view. Though +some of M.~Poincaré's chapters have been collected +from well-known treatises written several years +ago, and indeed are sometimes in detail not quite +up to date, besides occasionally suggesting the +suspicion that his views may possibly have been +modified in the interval, yet their publication in +a compact form has excited a warm welcome in +this country. + +It must be confessed that the English language +\PageSep{xii} +hardly lends itself as a perfect medium for the +rendering of the delicate shades of suggestion +and allusion characteristic of M.~Poincaré's play +around his subject; notwithstanding the excellence +of the translation, loss in this respect is +inevitable. + +There has been of late a growing trend of +opinion, prompted in part by general philosophical +views, in the direction that the theoretical constructions +of physical science are largely factitious, +that instead of presenting a valid image of the +relations of things on which further progress can +be based, they are still little better than a mirage. +The best method of abating this scepticism is to +become acquainted with the real scope and modes +of application of conceptions which, in the popular +language of superficial exposition---and even in +the unguarded and playful paradox of their +authors, intended only for the instructed eye---often +look bizarre enough. But much advantage +will accrue if men of science become their own +epistemologists, and show to the world by critical +exposition in non-technical terms of the results +and methods of their constructive work, that more +than mere instinct is involved in it: the community +has indeed a right to expect as much as +this. +\PageSep{xiii} + +It would be hard to find any one better +qualified for this kind of exposition, either +from the profundity of his own mathematical +achievements, or from the extent and freshness +of his interest in the theories of physical science, +than the author of this book. If an appreciation +might be ventured on as regards the later chapters, +they are, perhaps, intended to present the stern +logical analyst quizzing the cultivator of physical +ideas as to what he is driving at, and whither he +expects to go, rather than any responsible attempt +towards a settled confession of faith. Thus, when +M.~Poincaré allows himself for a moment to +indulge in a process of evaporation of the +Principle of Energy, he is content to sum up: +``Eh bien, quelles que soient les notions nouvelles +que les expériences futures nous donneront sur le +monde, nous sommes sûrs d'avance qu'il y aura +quelque chose qui demeurera constant et que nous +pourrons appeler \Foreign{énergie}'' (\Pageref{166}), and to leave +the matter there for his readers to think it out. +Though hardly necessary in the original French, it +may not now be superfluous to point out that +independent reflection and criticism on the part +of the reader are tacitly implied here as elsewhere. + +An interesting passage is the one devoted to +\PageSep{xiv} +Maxwell's theory of the functions of the æther, +and the comparison of the close-knit theories of +the classical French mathematical physicists with +the somewhat loosely-connected \Foreign{corpus} of ideas by +which Maxwell, the interpreter and successor of +Faraday, has (posthumously) recast the whole +face of physical science. How many times has +that theory been re-written since Maxwell's day? +and yet how little has it been altered in essence, +except by further developments in the problem of +moving bodies, from the form in which he left it! +If, as M.~Poincaré remarks, the French instinct +for precision and lucid demonstration sometimes +finds itself ill at ease with physical theories of +the British school, he as readily admits (\Pagerefs{223}{224}), +and indeed fully appreciates, the advantages +on the other side. Our own mental philosophers +have been shocked at the point of view indicated +by the proposition hazarded by Laplace, that a +sufficiently developed intelligence, if it were made +acquainted with the positions and motions of the +atoms at any instant, could predict all future +history: no amount of demur suffices sometimes +to persuade them that this is not a conception +universally entertained in physical science. It +was not so even in Laplace's own day. From +the point of view of the study of the evolution +\PageSep{xv} +of the sciences, there are few episodes more +instructive than the collision between Laplace +and Young with regard to the theory of capillarity. +The precise and intricate mathematical +analysis of Laplace, starting from fixed preconceptions +regarding atomic forces which were +to remain intact throughout the logical development +of the argument, came into contrast with the +tentative, mobile intuitions of Young; yet the +latter was able to grasp, by sheer direct mental +force, the fruitful though partial analogies of this +recondite class of phenomena with more familiar +operations of nature, and to form a direct picture +of the way things interacted, such as could only +have been illustrated, quite possibly damaged or +obliterated, by premature effort to translate it +into elaborate analytical formulas. The \Foreign{aperçus} +of Young were apparently devoid of all cogency +to Laplace; while Young expressed, doubtless in +too extreme a way, his sense of the inanity of the +array of mathematical logic of his rival. The +subsequent history involved the Nemesis that the +fabric of Laplace was taken down and reconstructed +in the next generation by Poisson; while +the modern cultivator of the subject turns, at any +rate in England, to neither of those expositions +for illumination, but rather finds in the partial +\PageSep{xvi} +and succinct indications of Young the best starting-point +for further effort. + +It seems, however, hard to accept entirely +the distinction suggested (\Pageref{213}) between the +methods of cultivating theoretical physics in +the two countries. To mention only two +transcendent names which stand at the very +front of two of the greatest developments of +physical science of the last century, Carnot and +Fresnel, their procedure was certainly not on the +lines thus described. Possibly it is not devoid of +significance that each of them attained his first +effective recognition from the British school. + +It may, in fact, be maintained that the part +played by mechanical and such-like theories---analogies +if you will---is an essential one. The +reader of this book will appreciate that the human +mind has need of many instruments of comparison +and discovery besides the unrelenting logic of the +infinitesimal calculus. The dynamical basis which +underlies the objects of our most frequent experience +has now been systematised into a great +calculus of exact thought, and traces of new real +relationships may come out more vividly when +considered in terms of our familiar acquaintance +with dynamical systems than when formulated +under the paler shadow of more analytical abstractions. +\PageSep{xvii} +It is even possible for a constructive +physicist to conduct his mental operations entirely +by dynamical images, though Helmholtz, as well +as our author, seems to class a predilection in this +direction as a British trait. A time arrives when, +as in other subjects, ideas have crystallised out +into distinctness; their exact verification and +development then becomes a problem in mathematical +physics. But whether the mechanical +analogies still survive, or new terms are now +introduced devoid of all naïve mechanical bias, +it matters essentially little. The precise determination +of the relations of things in the +rational scheme of nature in which we find +ourselves is the fundamental task, and for its +fulfilment in any direction advantage has to be +taken of our knowledge, even when only partial, +of new aspects and types of relationship which +may have become familiar perhaps in quite +different fields. Nor can it be forgotten that the +most fruitful and fundamental conceptions of +abstract pure mathematics itself have often been +suggested from these mechanical ideas of flux +and force, where the play of intuition is our +most powerful guide. The study of the historical +evolution of physical theories is essential to the +complete understanding of their import. It is in +\PageSep{xviii} +the mental workshop of a Fresnel, a Kelvin, or +a Helmholtz, that profound ideas of the deep +things of Nature are struck out and assume +form; when pondered over and paraphrased by +philosophers we see them react on the conduct +of life: it is the business of criticism to polish +them gradually to the common measure of human +understanding. Oppressed though we are with +the necessity of being specialists, if we are +to know anything thoroughly in these days of +accumulated details, we may at any rate profitably +study the historical evolution of knowledge +over a field wider than our own. + +The aspect of the subject which has here been +dwelt on is that scientific progress, considered +historically, is not a strictly logical process, and +does not proceed by syllogisms. New ideas +emerge dimly into intuition, come into consciousness +from nobody knows where, and become +the material on which the mind operates, forging +them gradually into consistent doctrine, which +can be welded on to existing domains of knowledge. +But this process is never complete: a +crude connection can always be pointed to by a +logician as an indication of the imperfection of +human constructions. + +If intuition plays a part which is so important, +\PageSep{xix} +it is surely necessary that we should possess a firm +grasp of its limitations. In M.~Poincaré's earlier +chapters the reader can gain very pleasantly a +vivid idea of the various and highly complicated +ways of docketing our perceptions of the relations +of external things, all equally valid, that were +open to the human race to develop. Strange to +say, they never tried any of them; and, satisfied +with the very remarkable practical fitness of the +scheme of geometry and dynamics that came +naturally to hand, did not consciously trouble +themselves about the possible existence of others +until recently. Still more recently has it been +found that the good Bishop Berkeley's logical +jibes against the Newtonian ideas of fluxions and +limiting ratios cannot be adequately appeased in +the rigorous mathematical conscience, until our +apparent continuities are resolved mentally into +discrete aggregates which we only partially +apprehend. The irresistible impulse to atomize +everything thus proves to be not merely a disease +of the physicist; a deeper origin, in the nature +of knowledge itself, is suggested. + +Everywhere want of absolute, exact adaptation +can be detected, if pains are taken, between the +various constructions that result from our mental +activity and the impressions which give rise to +\PageSep{xx} +them. The bluntness of our unaided sensual +perceptions, which are the source in part of the +intuitions of the race, is well brought out in this +connection by M.~Poincaré. Is there real contradiction? +Harmony usually proves to be recovered +by shifting our attitude to the phenomena. +All experience leads us to interpret the totality of +things as a consistent cosmos---undergoing evolution, +the naturalists will say---in the large-scale +workings of which we are interested spectators +and explorers, while of the inner relations and +ramifications we only apprehend dim glimpses. +When our formulation of experience is imperfect +or even paradoxical, we learn to attribute the +fault to our point of view, and to expect that +future adaptation will put it right. But Truth +resides in a deep well, and we shall never get +to the bottom. Only, while deriving enjoyment +and insight from M.~Poincaré's Socratic exposition +of the limitations of the human outlook on +the universe, let us beware of counting limitation +as imperfection, and drifting into an inadequate +conception of the wonderful fabric of human +knowledge. + +\Signature{J. LARMOR.}{} +\PageSep{xxi} + + +\OtherChapter{Author's Preface.} + +\First{To} the superficial observer scientific truth is unassailable, +the logic of science is infallible; and if +scientific men sometimes make mistakes, it is +because they have not understood the rules of +the game. Mathematical truths are derived from +a few self-evident propositions, by a chain of +flawless reasonings; they are imposed not only on +us, but on Nature itself. By them the Creator is +fettered, as it were, and His choice is limited to +a relatively small number of solutions. A few +experiments, therefore, will be sufficient to enable +us to determine what choice He has made. From +each experiment a number of consequences will +follow by a series of mathematical deductions, +and in this way each of them will reveal to us a +corner of the universe. This, to the minds of most +people, and to students who are getting their first +ideas of physics, is the origin of certainty in +science. This is what they take to be the rôle of +\PageSep{xxii} +experiment and mathematics. And thus, too, it +was understood a hundred years ago by many +men of science who dreamed of constructing the +world with the aid of the smallest possible amount +of material borrowed from experiment. + +But upon more mature reflection the position +held by hypothesis was seen; it was recognised that +it is as necessary to the experimenter as it is to the +mathematician. And then the doubt arose if all +these constructions are built on solid foundations. +The conclusion was drawn that a breath would +bring them to the ground. This sceptical attitude +does not escape the charge of superficiality. To +doubt everything or to believe everything are two +equally convenient solutions; both dispense with +the necessity of reflection. + +Instead of a summary condemnation we should +examine with the utmost care the rôle of hypothesis; +we shall then recognise not only that it is +necessary, but that in most cases it is legitimate. +We shall also see that there are several kinds of +hypotheses; that some are verifiable, and when +once confirmed by experiment become truths of +great fertility; that others may be useful to us in +fixing our ideas; and finally, that others are +hypotheses only in appearance, and reduce to +definitions or to conventions in disguise. The +\PageSep{xxiii} +latter are to be met with especially in mathematics +and in the sciences to which it is applied. From +them, indeed, the sciences derive their rigour; +such conventions are the result of the unrestricted +activity of the mind, which in this domain recognises +no obstacle. For here the mind may affirm +because it lays down its own laws; but let us +clearly understand that while these laws are +imposed on \emph{our} science, which otherwise could +not exist, they are not imposed on Nature. Are +they then arbitrary? No; for if they were, they +would not be fertile. Experience leaves us our +freedom of choice, but it guides us by helping us to +discern the most convenient path to follow. Our +laws are therefore like those of an absolute +monarch, who is wise and consults his council of +state. Some people have been struck by this +characteristic of free convention which may be +recognised in certain fundamental principles of +the sciences. Some have set no limits to their +generalisations, and at the same time they have +forgotten that there is a difference between liberty +and the purely arbitrary. So that they are compelled +to end in what is called \emph{nominalism}; they +have asked if the \Foreign{savant} is not the dupe of his +own definitions, and if the world he thinks he has +discovered is not simply the creation of his own +\PageSep{xxiv} +caprice.\footnote + {Cf.\ M.~le~Roy: ``Science et Philosophie,'' \Title{Revue de Métaphysique + et de Morale}, 1901.} +Under these conditions science would +retain its certainty, but would not attain its object, +and would become powerless. Now, we daily see +what science is doing for us. This could not be +unless it taught us something about reality; the +aim of science is not things themselves, as the +dogmatists in their simplicity imagine, but the +relations between things; outside those relations +there is no reality knowable. + +Such is the conclusion to which we are led; but +to reach that conclusion we must pass in review +the series of sciences from arithmetic and +geometry to mechanics and experimental physics. +What is the nature of mathematical reasoning? +Is it really deductive, as is commonly supposed? +Careful analysis shows us that it is nothing of the +kind; that it participates to some extent in the +nature of inductive reasoning, and for that reason +it is fruitful. But none the less does it retain its +character of absolute rigour; and this is what +must first be shown. + +When we know more of this instrument which +is placed in the hands of the investigator by +mathematics, we have then to analyse another +fundamental idea, that of mathematical magnitude. +\PageSep{xxv} +Do we find it in nature, or have we ourselves +introduced it? And if the latter be the +case, are we not running a risk of coming to +incorrect conclusions all round? Comparing the +rough data of our senses with that extremely complex +and subtle conception which mathematicians +call magnitude, we are compelled to recognise a +divergence. The framework into which we wish +to make everything fit is one of our own construction; +but we did not construct it at random, we +constructed it by measurement so to speak; and +that is why we can fit the facts into it without +altering their essential qualities. + +Space is another framework which we impose +on the world. Whence are the first principles of +geometry derived? Are they imposed on us by +logic? Lobatschewsky, by inventing non-Euclidean +geometries, has shown that this is not the case. +Is space revealed to us by our senses? No; for +the space revealed to us by our senses is absolutely +different from the space of geometry. Is geometry +derived from experience? Careful discussion will +give the answer---no! We therefore conclude that +the principles of geometry are only conventions; +but these conventions are not arbitrary, and if +transported into another world (which I shall +call the non-Euclidean world, and which I shall +\PageSep{xxvi} +endeavour to describe), we shall find ourselves +compelled to adopt more of them. + +In mechanics we shall be led to analogous conclusions, +and we shall see that the principles of +this science, although more directly based on +experience, still share the conventional character +of the geometrical postulates. So far, nominalism +triumphs; but we now come to the physical +sciences, properly so called, and here the scene +changes. We meet with hypotheses of another +kind, and we fully grasp how fruitful they are. +No doubt at the outset theories seem unsound, +and the history of science shows us how ephemeral +they are; but they do not entirely perish, and of +each of them some traces still remain. It is these +traces which we must try to discover, because in +them and in them alone is the true reality. + +The method of the physical sciences is based +upon the induction which leads us to expect the +recurrence of a phenomenon when the circumstances +which give rise to it are repeated. If all +the circumstances could be simultaneously reproduced, +this principle could be fearlessly applied; +but this never happens; some of the circumstances +will always be missing. Are we absolutely certain +that they are unimportant? Evidently not! It +may be probable, but it cannot be rigorously +\PageSep{xxvii} +certain. Hence the importance of the rôle that is +played in the physical sciences by the law of +probability. The calculus of probabilities is therefore +not merely a recreation, or a guide to the +baccarat player; and we must thoroughly examine +the principles on which it is based. In this connection +I have but very incomplete results to lay +before the reader, for the vague instinct which +enables us to determine probability almost defies +analysis. After a study of the conditions under +which the work of the physicist is carried on, I +have thought it best to show him at work. For +this purpose I have taken instances from the +history of optics and of electricity. We shall thus +see how the ideas of Fresnel and Maxwell took +their rise, and what unconscious hypotheses were +made by Ampère and the other founders of +electro-dynamics. +\PageSep{xxviii} +%[Blank page] +\PageSep{1} +\MainMatter +%[** TN: Commented text is printed by the \Part macro] +% SCIENCE AND HYPOTHESIS. + + +\Part{I.}{Number and Magnitude.} + +\Chapter[Nature of Mathematical Reasoning.]{I.}{On the Nature of Mathematical Reasoning.} + +\Section{I.} + +\First{The} very possibility of mathematical science seems +an insoluble contradiction. If this science is only +deductive in appearance, from whence is derived +that perfect rigour which is challenged by none? +If, on the contrary, all the propositions which it +enunciates may be derived in order by the rules +of formal logic, how is it that mathematics is +not reduced to a gigantic tautology? The syllogism +can teach us nothing essentially new, and +if everything must spring from the principle of +identity, then everything should be capable of +being reduced to that principle. Are we then to +admit that the enunciations of all the theorems +\PageSep{2} +with which so many volumes are filled, are only +indirect ways of saying that A~is~A? + +No doubt we may refer back to axioms which +are at the source of all these reasonings. If it is +felt that they cannot be reduced to the principle of +contradiction, if we decline to see in them any +more than experimental facts which have no part +or lot in mathematical necessity, there is still one +resource left to us: we may class them among +\Foreign{à ~priori} synthetic views. But this is no solution +of the difficulty---it is merely giving it a name; and +even if the nature of the synthetic views had no +longer for us any mystery, the contradiction would +not have disappeared; it would have only been +shirked. Syllogistic reasoning remains incapable +of adding anything to the data that are given it; +the data are reduced to axioms, and that is all we +should find in the conclusions. + +No theorem can be new unless a new axiom +intervenes in its demonstration; reasoning can +only give us immediately evident truths borrowed +from direct intuition; it would only be an intermediary +parasite. Should we not therefore have +reason for asking if the syllogistic apparatus serves +only to disguise what we have borrowed? + +The contradiction will strike us the more if we +open any book on mathematics; on every page the +author announces his intention of generalising some +proposition already known. Does the mathematical +method proceed from the particular to the general, +and, if so, how can it be called deductive? +\PageSep{3} + +Finally, if the science of number were merely +analytical, or could be analytically derived from a +few synthetic intuitions, it seems that a sufficiently +powerful mind could with a single glance perceive +all its truths; nay, one might even hope that some +day a language would be invented simple enough +for these truths to be made evident to any person +of ordinary intelligence. + +Even if these consequences are challenged, it +must be granted that mathematical reasoning has +of itself a kind of creative virtue, and is therefore to +be distinguished from the syllogism. The difference +must be profound. We shall not, for instance, +find the key to the mystery in the frequent use of +the rule by which the same uniform operation +applied to two equal numbers will give identical +results. All these modes of reasoning, whether or +not reducible to the syllogism, properly so called, +retain the analytical character, and \Foreign{ipso facto}, lose +their power. + +\Section{II.} + +The argument is an old one. Let us see how +Leibnitz tried to show that two and two make +four. I assume the number one to be defined, and +also the operation~$x + 1$---\ie, the adding of unity +to a given number~$x$. These definitions, whatever +they may be, do not enter into the subsequent +reasoning. I next define the numbers $2$,~$3$,~$4$ by +the equalities\Chg{:---}{} +%[** TN: Numbered eqns displayed in the French, but not in the English transl.] +\[ +\Tag{(1)} 1 + 1 = 2;\qquad +\Tag{(2)} 2 + 1 = 3;\qquad +\Tag{(3)} 3 + 1 = 4\Chg{,}{;} +\] +and in +\PageSep{4} +the same way I define the operation~$x + 2$ by the +relation\Chg{;}{} +\[ +\Tag{(4)} +x + 2 = (x + 1) + 1. +\] + +Given this, we have\Chg{:---}{} +\begin{alignat*}{2} + 2 + 2 &= (2 + 1) + 1\Chg{;}{,}\ &&\text{(def.~4)\Chg{.}{;}} \\ +(2 + 1) + 1 &= 3 + 1\Add{,} &&\text{(def.~2)\Chg{.}{;}} \\ + 3 + 1 &= 4\Add{,} &&\text{(def.~3)\Chg{.}{;}} \\ +\text{whence } 2 + 2 &= 4\Add{,}&&\quad\QED +\end{alignat*} + +It cannot be denied that this reasoning is purely +analytical. But if we ask a mathematician, he will +reply: ``This is not a demonstration properly so +called; it is a verification.'' We have confined +ourselves to bringing together one or other of two +purely conventional definitions, and we have verified +their identity; nothing new has been learned. +\emph{Verification} differs from proof precisely because it +is analytical, and because it leads to nothing. It +leads to nothing because the conclusion is nothing +but the premisses translated into another language. +A real proof, on the other hand, is fruitful, because +the conclusion is in a sense more general than the +premisses. The equality $2 + 2 = 4$ can be verified +because it is particular. Each individual enunciation +in mathematics may be always verified in +the same way. But if mathematics could be +reduced to a series of such verifications it +would not be a science. A chess-player, for +instance, does not create a science by winning a +piece. There is no science but the science of the +general. It may even be said that the object of +the exact sciences is to dispense with these direct +verifications. +\PageSep{5} + +\Section{III.} + +Let us now see the geometer at work, and try +%[** TN: "surprise" is correct: "...cherchons à surprendre ses procédés."] +to surprise some of his methods. The task is +not without difficulty; it is not enough to open a +book at random and to analyse any proof we may +come across. First of all, geometry must be excluded, +or the question becomes complicated by +difficult problems relating to the rôle of the +postulates, the nature and the origin of the idea +of space. For analogous reasons we cannot +avail ourselves of the infinitesimal calculus. We +must seek mathematical thought where it has +remained pure---\ie, in Arithmetic. But we +still have to choose; in the higher parts of +the theory of numbers the primitive mathematical +ideas have already undergone so profound +an elaboration that it becomes difficult to analyse +them. + +It is therefore at the beginning of Arithmetic +that we must expect to find the explanation we +seek; but it happens that it is precisely in the +proofs of the most elementary theorems that the +authors of classic treatises have displayed the least +precision and rigour. We may not impute this to +them as a crime; they have obeyed a necessity. +Beginners are not prepared for real mathematical +rigour; they would see in it nothing but empty, +tedious subtleties. It would be waste of time to +try to make them more exacting; they have to +pass rapidly and without stopping over the road +\PageSep{6} +which was trodden slowly by the founders of the +science. + +Why is so long a preparation necessary to +habituate oneself to this perfect rigour, which +it would seem should naturally be imposed on +all minds? This is a logical and psychological +problem which is well worthy of study. But we +shall not dwell on it; it is foreign to our subject. +All I wish to insist on is, that we shall fail in our +purpose unless we reconstruct the proofs of the +elementary theorems, and give them, not the rough +form in which they are left so as not to weary the +beginner, but the form which will satisfy the skilled +geometer. + +\Subsection{Definition of Addition.} + +I assume that the operation~$x + 1$ has been +defined; it consists in adding the number~$1$ to a +given number~$x$. Whatever may be said of this +definition, it does not enter into the subsequent +reasoning. + +We now have to define the operation~$x + a$, which +consists in adding the number~$a$ to any given +number~$x$. Suppose that we have defined the +operation +%[** TN: Displayed eqns as in the French; all are inline in the English transl.] +\[ +x + (a - 1); +\] +the operation~$x + a$ will be +defined by the equality\Chg{:}{} +\[ +\Tag{(1)} +x + a = \bigl[x + (a - 1)\bigr] + 1. +\] +We shall know what $x + a$~is when we know what +$x + (a - 1)$ is, and as I have assumed that to start +with we know what $x + 1$~is, we can define +successively and ``by recurrence'' the operations +$x + 2$, $x + 3$,~etc. This definition deserves a moment's +\PageSep{7} +attention; it is of a particular nature which +distinguishes it even at this stage from the purely +logical definition; the equality~(1), in fact, contains +an infinite number of distinct definitions, each +having only one meaning when we know the +meaning of its predecessor. + +\Subsection{Properties of Addition.} + +\Par{Associative.}---I say that +%[** TN: Displayed eqns as in the French; all are inline in the English transl.] +\[ +a + (b + c) = (a + b) + c; +\] +in +fact, the theorem is true for $c = 1$. It may then be +written +\[ +a + (b + 1) = (a + b) + 1; +\] +which, remembering +the difference of notation, is nothing but the equality~(1) +by which I have just defined addition. Assume +the theorem true for $c = \gamma$, I say that it will be true for +$c = \gamma + 1$. Let +\[ +(a + b) + \gamma = a + (b + \gamma)\Chg{,}{;} +\] +it follows that +\[ +\bigl[(a + b) + \gamma\bigr] + 1 = \bigl[a + (b + \gamma)\bigr] + 1; +\] +or by def.~(1)\Chg{---}{,} +\[ +(a + b) + (\gamma + 1) + = a + (b + \gamma + 1) + = a + \bigl[b + (\gamma + 1)\bigr]\Chg{,}{;} +\] +which shows by a series of purely analytical deductions +that the theorem is true for $\gamma + 1$. Being +true for $c = 1$, we see that it is successively true for +$c = 2$, $c = 3$,~etc. + +\Par{Commutative.}---(1)~I say that +%[** TN: Displayed eqns as in the French; all are inline in the English transl.] +\[ +a + 1 = 1 + a. +\] +The +theorem is evidently true for $a = 1$; we can \emph{verify} +by purely analytical reasoning that if it is true for +$a = \gamma$ it will be true for $a = \gamma + 1$.\footnote + {For $(\gamma + 1) + 1 = (1 + \gamma) + 1 = 1 + (\gamma + 1)$.\Transl} +Now, it is true for +$a = 1$, and therefore is true for $a = 2$, $a = 3$, and so +on. This is what is meant by saying that the +proof is demonstrated ``by recurrence.'' + +(2)~I say that +\[ +a + b = b + a. +\] +The theorem has just +\PageSep{8} +been shown to hold good for $b = 1$, and it may be +verified analytically that if it is true for $b = \beta$, it +will be true for $b = \beta + 1$. The proposition is thus +established by recurrence. + +\Subsection{Definition of Multiplication.} + +We shall define multiplication by the equalities\Chg{:}{} +\begin{gather*} +\Tag{(1)} +a × 1 = a\Chg{.}{;} \\ +\Tag{(2)} +a × b = \bigl[a × (b - 1)\bigr] + a. +\end{gather*} +Both of +these include an infinite number of definitions; +having defined~$a × 1$, it enables us to define in +succession $a × 2$, $a × 3$, and so on. + +\Subsection{Properties of Multiplication.} + +\Par{Distributive.}---I say that +%[** TN: Displayed eqns as in the French; all are inline in the English transl.] +\[ +(a + b) × c = (a × c) + (b × c). +\] +We can verify analytically that the theorem +is true for $c = 1$; then if it is true for $c = \gamma$, it will be +true for $c = \gamma + 1$. The proposition is then proved +by recurrence. + +\Par{Commutative.}---(1) I say that +\[ +a × 1 = 1 × a. +\] +The +theorem is obvious for $a = 1$. We can verify +analytically that if it is true for $a = \alpha$, it will be +true for $a = \alpha + 1$. + +(2)~I say that +\[ +a × b = b × a. +\] +The theorem has +just been proved for $b = 1$. We can verify analytically +that if it be true for $b = \beta$ it will be true for +$b = \beta + 1$. + +\Section{IV.} + +This monotonous series of reasonings may now +be laid aside; but their very monotony brings +vividly to light the process, which is uniform, +\PageSep{9} +and is met again at every step. The process is +proof by recurrence. We first show that a +theorem is true for $n = 1$; we then show that if +it is true for~$n - 1$ it is true for~$n$, and we conclude +that it is true for all integers. We have now seen +how it may be used for the proof of the rules of +addition and multiplication---that is to say, for the +rules of the algebraical calculus. This calculus +is an instrument of transformation which lends +itself to many more different combinations than +the simple syllogism; but it is still a purely analytical +instrument, and is incapable of teaching us +anything new. If mathematics had no other instrument, +it would immediately be arrested in its +development; but it has recourse anew to the +same process---\ie, to reasoning by recurrence, and +it can continue its forward march. Then if we +look carefully, we find this mode of reasoning at +every step, either under the simple form which we +have just given to it, or under a more or less modified +form. It is therefore mathematical reasoning +\Foreign{par excellence}, and we must examine it closer. + +\Section{V.} + +The essential characteristic of reasoning by recurrence +is that it contains, condensed, so to +speak, in a single formula, an infinite number of +syllogisms. We shall see this more clearly if we +enunciate the syllogisms one after another. They +follow one another, if one may use the expression, +in a cascade. The following are the hypothetical +\PageSep{10} +syllogisms:---The theorem is true of the number~$1$. +Now, if it is true of~$1$, it is true of~$2$; therefore it is +true of~$2$. Now, if it is true of~$2$, it is true of~$3$; +hence it is true of~$3$, and so on. We see that the +conclusion of each syllogism serves as the minor +of its successor. Further, the majors of all our +syllogisms may be reduced to a single form. If +the theorem is true of~$n - 1$, it is true of~$n$. + +We see, then, that in reasoning by recurrence +we confine ourselves to the enunciation of the +minor of the first syllogism, and the general +formula which contains as particular cases all the +majors. This unending series of syllogisms is thus +reduced to a phrase of a few lines. + +It is now easy to understand why every particular +consequence of a theorem may, as I have +above explained, be verified by purely analytical +processes. If, instead of proving that our theorem +is true for all numbers, we only wish to show that +it is true for the number~$6$ for instance, it will be +enough to establish the first five syllogisms in our +cascade. We shall require~$9$ if we wish to prove +it for the number~$10$; for a greater number we +shall require more still; but however great the +number may be we shall always reach it, and the +analytical verification will always be possible. +But however far we went we should never reach +the general theorem applicable to all numbers, +which alone is the object of science. To reach +it we should require an infinite number of syllogisms, +and we should have to cross an abyss +\PageSep{11} +which the patience of the analyst, restricted to the +resources of formal logic, will never succeed in +crossing. + +I asked at the outset why we cannot conceive of +a mind powerful enough to see at a glance the +whole body of mathematical truth. The answer is +now easy. A chess-player can combine for four or +five moves ahead; but, however extraordinary a +player he may be, he cannot prepare for more than +a finite number of moves. If he applies his faculties +to Arithmetic, he cannot conceive its general +truths by direct intuition alone; to prove even the +smallest theorem he must use reasoning by recurrence, +for that is the only instrument which +enables us to pass from the finite to the infinite. +This instrument is always useful, for it enables us +to leap over as many stages as we wish; it frees +us from the necessity of long, tedious, and +monotonous verifications which would rapidly +become impracticable. Then when we take in +hand the general theorem it becomes indispensable, +for otherwise we should ever be approaching +the analytical verification without ever actually +reaching it. In this domain of Arithmetic we may +think ourselves very far from the infinitesimal +analysis, but the idea of mathematical infinity is +already playing a preponderating part, and without +it there would be no science at all, because there +would be nothing general. +\PageSep{12} + +\Section{VI.} + +The views upon which reasoning by recurrence +is based may be exhibited in other forms; we may +say, for instance, that in any finite collection of +different integers there is always one which is +smaller than any other. We may readily pass from +one enunciation to another, and thus give ourselves +the illusion of having proved that reasoning +by recurrence is legitimate. But we shall +always be brought to a full stop---we shall always +come to an indemonstrable axiom, which will at +bottom be but the proposition we had to prove +translated into another language. We cannot therefore +escape the conclusion that the rule of reasoning +by recurrence is irreducible to the principle of +contradiction. Nor can the rule come to us from +experiment. Experiment may teach us that the +rule is true for the first ten or the first hundred +numbers, for instance; it will not bring us to the +indefinite series of numbers, but only to a more or +less long, but always limited, portion of the series. + +Now, if that were all that is in question, the +principle of contradiction would be sufficient, it +would always enable us to develop as many +syllogisms as we wished. It is only when it is a +question of a single formula to embrace an infinite +number of syllogisms that this principle breaks +down, and there, too, experiment is powerless to +aid. This rule, inaccessible to analytical proof +and to experiment, is the exact type of the \Foreign{à ~priori} +\PageSep{13} +synthetic intuition. On the other hand, we +cannot see in it a convention as in the case of the +postulates of geometry. + +Why then is this view imposed upon us with +such an irresistible weight of evidence? It is +because it is only the affirmation of the power of +the mind which knows it can conceive of the +indefinite repetition of the same act, when the act +is once possible. The mind has a direct intuition +of this power, and experiment can only be for it an +opportunity of using it, and thereby of becoming +conscious of it. + +But it will be said, if the legitimacy of reasoning +by recurrence cannot be established by experiment +alone, is it so with experiment aided by induction? +We see successively that a theorem is true of the +number~$1$, of the number~$2$, of the number~$3$, and +so on---the law is manifest, we say, and it is so on +the same ground that every physical law is true +which is based on a very large but limited number +of observations. + +It cannot escape our notice that here is a +striking analogy with the usual processes of +induction. But an essential difference exists. +Induction applied to the physical sciences is +always uncertain, because it is based on the belief +in a general order of the universe, an order +which is external to us. Mathematical induction---\ie, +proof by recurrence---is, on the contrary, +necessarily imposed on us, because it is only the +affirmation of a property of the mind itself. +\PageSep{14} + +\Section{VII.} + +Mathematicians, as I have said before, always +endeavour to generalise the propositions they have +obtained. To seek no further example, we have +just shown the equality\Chg{,}{} +%[** TN: Displayed eqns as in the French; all are inline in the English transl.] +\[ +a + 1 = 1 + a, +\] +and we then +used it to establish the equality\Chg{,}{} +\[ +a + b = b + a, +\] +which +is obviously more general. Mathematics may, +therefore, like the other sciences, proceed from the +particular to the general. This is a fact which +might otherwise have appeared incomprehensible +to us at the beginning of this study, but which has +no longer anything mysterious about it, since we +have ascertained the analogies between proof by +recurrence and ordinary induction. + +No doubt mathematical recurrent reasoning and +physical inductive reasoning are based on different +foundations, but they move in parallel lines and in +the same direction---namely, from the particular +to the general. + +Let us examine the case a little more closely. +To prove the equality +\[ +\Tag{(1)} +a + 2 = 2 + a, +\] +we need +only apply the rule +\[ +a + 1 = 1 + a\Chg{,}{} +\] +twice, and write +\[ +\Tag{(2)} +a + 2 = a + 1 + 1 = 1 + a + 1 = 1 + 1 + a = 2 + a. +\] + +The equality thus deduced by purely analytical +means is not, however, a simple particular case. It +is something quite different. We may not therefore +even say in the really analytical and deductive +part of mathematical reasoning that we proceed +from the general to the particular in the +ordinary sense of the words. The two sides of +\PageSep{15} +the equality~(2) are merely more complicated +combinations than the two sides of the equality~(1), +and analysis only serves to separate the elements +which enter into these combinations and to +study their relations. + +Mathematicians therefore proceed ``by construction,'' +they ``construct'' more complicated combinations. +When they analyse these combinations, +these aggregates, so to speak, into their primitive +elements, they see the relations of the elements +and deduce the relations of the aggregates themselves. +The process is purely analytical, but it is +not a passing from the general to the particular, +for the aggregates obviously cannot be regarded as +more particular than their elements. + +Great importance has been rightly attached to +this process of ``construction,'' and some claim +to see in it the necessary and sufficient condition +of the progress of the exact sciences. +Necessary, no doubt, but not sufficient! For a +construction to be useful and not mere waste of +mental effort, for it to serve as a stepping-stone to +higher things, it must first of all possess a kind of +unity enabling us to see something more than the +juxtaposition of its elements. Or more accurately, +there must be some advantage in considering the +construction rather than the elements themselves. +What can this advantage be? Why reason on a +polygon, for instance, which is always decomposable +into triangles, and not on elementary +triangles? It is because there are properties of +\PageSep{16} +polygons of any number of sides, and they can be +immediately applied to any particular kind of +polygon. In most cases it is only after long efforts +that those properties can be discovered, by directly +studying the relations of elementary triangles. If +the quadrilateral is anything more than the juxtaposition +of two triangles, it is because it is of the +polygon type. + +A construction only becomes interesting when +it can be placed side by side with other analogous +constructions for forming species of the same +genus. To do this we must necessarily go back +from the particular to the general, ascending one +or more steps. The analytical process ``by +construction'' does not compel us to descend, but +it leaves us at the same level. We can only +ascend by mathematical induction, for from it +alone can we learn something new. Without the +aid of this induction, which in certain respects +differs from, but is as fruitful as, physical induction, +construction would be powerless to create +science. + +Let me observe, in conclusion, that this induction +is only possible if the same operation can +be repeated indefinitely. That is why the theory +of chess can never become a science, for the +different moves of the same piece are limited and +do not resemble each other. +\PageSep{17} + + +\Chapter[Mathematical Magnitude.]{II.}{Mathematical Magnitude and Experiment.} + +\First{If} we want to know what the mathematicians +mean by a continuum, it is useless to appeal to +geometry. The geometer is always seeking, more +or less, to represent to himself the figures he is +studying, but his representations are only instruments +to him; he uses space in his geometry just +as he uses chalk; and further, too much importance +must not be attached to accidents which are +often nothing more than the whiteness of the +chalk. + +The pure analyst has not to dread this pitfall. +He has disengaged mathematics from all extraneous +elements, and he is in a position to answer +our question:---``Tell me exactly what this continuum +is, about which mathematicians reason.'' +Many analysts who reflect on their art have +already done so---M.~Tannery, for instance, in +his \Title{Introduction à la théorie des Fonctions d'une +variable}. + +Let us start with the integers. Between any +two consecutive sets, intercalate one or more intermediary +sets, and then between these sets others +\PageSep{18} +again, and so on indefinitely. We thus get an +unlimited number of terms, and these will be the +numbers which we call fractional, rational, or +commensurable. But this is not yet all; between +these terms, which, be it marked, are already +infinite in number, other terms are intercalated, +and these are called irrational or incommensurable. + +Before going any further, let me make a preliminary +remark. The continuum thus conceived +is no longer a collection of individuals arranged in +a certain order, infinite in number, it is true, but +external the one to the other. This is not the +ordinary conception in which it is supposed that +between the elements of the continuum exists an +intimate connection making of it one whole, in +which the point has no existence previous to the +line, but the line does exist previous to the point. +Multiplicity alone subsists, unity has disappeared---``the +continuum is unity in multiplicity,'' according +to the celebrated formula. The analysts have +even less reason to define their continuum as they +do, since it is always on this that they reason when +they are particularly proud of their rigour. It +is enough to warn the reader that the real +mathematical continuum is quite different from +that of the physicists and from that of the +metaphysicians. + +It may also be said, perhaps, that mathematicians +who are contented with this definition are the +dupes of words, that the nature of each of these +sets should be precisely indicated, that it should +\PageSep{19} +be explained how they are to be intercalated, and +that it should be shown how it is possible to do it. +This, however, would be wrong; the only property +of the sets which comes into the reasoning is that of +preceding or succeeding these or those other sets; +this alone should therefore intervene in the definition. +So we need not concern ourselves with the +manner in which the sets are intercalated, and +no one will doubt the possibility of the operation +if he only remembers that ``possible'' in the +language of geometers simply means exempt from +contradiction. But our definition is not yet complete, +and we come back to it after this rather long +digression. + +\Par{Definition of Incommensurables.}---The mathematicians +of the Berlin school, and Kronecker +in particular, have devoted themselves to constructing +this continuous scale of irrational and +fractional numbers without using any other +materials than the integer. The mathematical +continuum from this point of view would be a +pure creation of the mind in which experiment +would have no part. + +The idea of rational number not seeming to +present to them any difficulty, they have confined +their attention mainly to defining incommensurable +numbers. But before reproducing their definition +here, I must make an observation that will allay +the astonishment which this will not fail to provoke +in readers who are but little familiar with the +habits of geometers. +\PageSep{20} + +Mathematicians do not study objects, but the +relations between objects; to them it is a matter +of indifference if these objects are replaced by +others, provided that the relations do not change. +Matter does not engage their attention, they are +interested by form alone. + +If we did not remember it, we could hardly +understand that Kronecker gives the name of +incommensurable number to a simple symbol---that +is to say, something very different from the +idea we think we ought to have of a quantity +which should be measurable and almost tangible. + +Let us see now what is Kronecker's definition. +Commensurable numbers may be divided into +classes in an infinite number of ways, subject +to the condition that any number whatever +of the first class is greater than any number +of the second. It may happen that among the +numbers of the first class there is one which is +smaller than all the rest; if, for instance, we +arrange in the first class all the numbers greater +than~$2$, and $2$~itself, and in the second class all the +numbers smaller than~$2$, it is clear that $2$~will be +the smallest of all the numbers of the first class. +The number~$2$ may therefore be chosen as the +symbol of this division. + +It may happen, on the contrary, that in the +second class there is one which is greater than all +the rest. This is what takes place, for example, +if the first class comprises all the numbers greater +than~$2$, and if, in the second, are all the numbers +\PageSep{21} +less than~$2$, and $2$~itself. Here again the +number~$2$ might be chosen as the symbol of this +division. + +But it may equally well happen that we can find +neither in the first class a number smaller than all +the rest, nor in the second class a number greater +than all the rest. Suppose, for instance, we +place in the first class all the numbers whose +squares are greater than~$2$, and in the second all +the numbers whose squares are smaller than~$2$. +We know that in neither of them is a number whose +square is equal to~$2$. Evidently there will be in +the first class no number which is smaller than all +the rest, for however near the square of a number +may be to~$2$, we can always find a commensurable +whose square is still nearer to~$2$. From +Kronecker's point of view, the incommensurable +number~$\sqrt{2}$ is nothing but the symbol of this +particular method of division of commensurable +numbers; and to each mode of repartition corresponds +in this way a number, commensurable or +not, which serves as a symbol. But to be satisfied +with this would be to forget the origin of these +symbols; it remains to explain how we have been +led to attribute to them a kind of concrete +existence, and on the other hand, does not the +difficulty begin with fractions? Should we have +the notion of these numbers if we did not previously +know a matter which we conceive as infinitely +divisible---\ie, as a continuum? + +\Par{The Physical Continuum.}---We are next led to ask +\PageSep{22} +if the idea of the mathematical continuum is not +simply drawn from experiment. If that be so, the +rough data of experiment, which are our sensations, +could be measured. We might, indeed, be tempted +to believe that this is so, for in recent times there +has been an attempt to measure them, and a law +has even been formulated, known as Fechner's +law, according to which sensation is proportional +to the logarithm of the stimulus. But if we +examine the experiments by which the endeavour +has been made to establish this law, we shall be +led to a diametrically opposite conclusion. It has, +for instance, been observed that a weight~$A$ of $10$~grammes +and a weight~$B$ of $11$~grammes produced +identical sensations, that the weight~$B$ could no +longer be distinguished from a weight~$C$ of $12$~grammes, +but that the weight~$A$ was readily +distinguished from the weight~$C$. Thus the rough +results of the experiments may be expressed by +the following relations\Chg{:}{} +%[** TN: Not displayed in the English translation] +\[ +A = B,\qquad B = C,\qquad A < C, +\] +which +may be regarded as the formula of the physical +continuum. But here is an intolerable disagreement +with the law of contradiction, and the +necessity of banishing this disagreement has compelled +us to invent the mathematical continuum. +We are therefore forced to conclude that this +notion has been created entirely by the mind, but +it is experiment that has provided the opportunity. +We cannot believe that two quantities which are +equal to a third are not equal to one another, and +we are thus led to suppose that $A$~is different from~$B$, +\PageSep{23} +and $B$~from~$C$, and that if we have not been +aware of this, it is due to the imperfections of our +senses. + +\Par{The Creation of the Mathematical Continuum: First +Stage.}---So far it would suffice, in order to account +for facts, to intercalate between $A$~and~$B$ a small +number of terms which would remain discrete. +What happens now if we have recourse to some +instrument to make up for the weakness of our +senses? If, for example, we use a microscope? +Such terms as $A$~and~$B$, which before were +indistinguishable from one another, appear now +to be distinct: but between $A$~and~$B$, which are +distinct, is intercalated another new term~$D$, +which we can distinguish neither from~$A$ nor from~$B$. +Although we may use the most delicate +methods, the rough results of our experiments +will always present the characters of the physical +continuum with the contradiction which is inherent +in it. We only escape from it by incessantly +intercalating new terms between the terms already +distinguished, and this operation must be pursued +indefinitely. We might conceive that it would be +possible to stop if we could imagine an instrument +powerful enough to decompose the physical continuum +into discrete elements, just as the telescope +resolves the Milky Way into stars. But this we +cannot imagine; it is always with our senses that +we use our instruments; it is with the eye that we +observe the image magnified by the microscope, +and this image must therefore always retain the +\PageSep{24} +characters of visual sensation, and therefore those +of the physical continuum. + +Nothing distinguishes a length directly observed +from half that length doubled by the microscope. +The whole is homogeneous to the part; and there +is a fresh contradiction---or rather there would be +one if the number of the terms were supposed +to be finite; it is clear that the part containing +less terms than the whole cannot be similar to the +whole. The contradiction ceases as soon as the +number of terms is regarded as infinite. There is +nothing, for example, to prevent us from regarding +the aggregate of integers as similar to the aggregate +of even numbers, which is however only a part +of it; in fact, to each integer corresponds another +even number which is its double. But it is not +only to escape this contradiction contained in the +empiric data that the mind is led to create the +concept of a continuum formed of an indefinite +number of terms. + +Here everything takes place just as in the series +of the integers. We have the faculty of conceiving +that a unit may be added to a collection of units. +Thanks to experiment, we have had the opportunity +of exercising this faculty and are conscious of +it; but from this fact we feel that our power is +unlimited, and that we can count indefinitely, +although we have never had to count more than +a finite number of objects. In the same way, as +soon as we have intercalated terms between two +consecutive terms of a series, we feel that this +\PageSep{25} +operation may be continued without limit, and +that, so to speak, there is no intrinsic reason for +stopping. As an abbreviation, I may give the +name of a mathematical continuum of the first +order to every aggregate of terms formed after the +same law as the scale of commensurable numbers. +If, then, we intercalate new sets according to the +laws of incommensurable numbers, we obtain +what may be called a continuum of the second +order. + +\Par{Second Stage.}---We have only taken our first +step. We have explained the origin of continuums +of the first order; we must now see why +this is not sufficient, and why the incommensurable +numbers had to be invented. + +If we try to imagine a line, it must have the +characters of the physical continuum---that is to +say, our representation must have a certain +breadth. Two lines will therefore appear to us +under the form of two narrow bands, and if we +are content with this rough image, it is clear +that where two lines cross they must have some +common part. But the pure geometer makes one +further effort; without entirely renouncing the +aid of his senses, he tries to imagine a line without +breadth and a point without size. This he can +do only by imagining a line as the limit towards +which tends a band that is growing thinner and +thinner, and the point as the limit towards which +is tending an area that is growing smaller and +smaller. Our two bands, however narrow they +\PageSep{26} +may be, will always have a common area; the +smaller they are the smaller it will be, and its +limit is what the geometer calls a point. This is +why it is said that the two lines which cross +must have a common point, and this truth seems +intuitive. + +But a contradiction would be implied if we +conceived of lines as continuums of the first order---\ie, +the lines traced by the geometer should only +give us points, the co-ordinates of which are +rational numbers. The contradiction would be +manifest if we were, for instance, to assert the +existence of lines and circles. It is clear, in fact, +that if the points whose co-ordinates are commensurable +were alone regarded as real, the +in-circle of a square and the diagonal of the +square would not intersect, since the co-ordinates +of the point of intersection are incommensurable. + +Even then we should have only certain incommensurable +numbers, and not all these numbers. + +But let us imagine a line divided into two half-rays +(\Foreign{demi-droites}). Each of these half-rays will +appear to our minds as a band of a certain breadth; +these bands will fit close together, because there +must be no interval between them. The common +part will appear to us to be a point which will still +remain as we imagine the bands to become thinner +and thinner, so that we admit as an intuitive truth +that if a line be divided into two half-rays the +common frontier of these half-rays is a point. +Here we recognise the conception of Kronecker, +\PageSep{27} +in which an incommensurable number was regarded +as the common frontier of two classes of rational +numbers. Such is the origin of the continuum of +the second order, which is the mathematical continuum +properly so called. + +\Par{Summary.}---To sum up, the mind has the faculty +of creating symbols, and it is thus that it has constructed +the mathematical continuum, which is +only a particular system of symbols. The only +limit to its power is the necessity of avoiding all +contradiction; but the mind only makes use of it +when experiment gives a reason for it. + +In the case with which we are concerned, the +reason is given by the idea of the physical continuum, +drawn from the rough data of the senses. +But this idea leads to a series of contradictions +from each of which in turn we must be freed. +In this way we are forced to imagine a more +and more complicated system of symbols. That +on which we shall dwell is not merely exempt +from internal contradiction,---it was so already at +all the steps we have taken,---but it is no longer in +contradiction with the various propositions which +are called intuitive, and which are derived from +more or less elaborate empirical notions. + +\Par{Measurable Magnitude.}---So far we have not +spoken of the measure of magnitudes; we can tell +if any one of them is greater than any other, +but we cannot say that it is two or three times +as large. + +So far, I have only considered the order in which +\PageSep{28} +the terms are arranged; but that is not sufficient +for most applications. We must learn how to +compare the interval which separates any two +terms. On this condition alone will the continuum +become measurable, and the operations +of arithmetic be applicable. This can only be +done by the aid of a new and special convention; +and this convention is, that in such a +case the interval between the terms $A$~and~$B$ is +equal to the interval which separates $C$~and~$D$. +For instance, we started with the integers, and +between two consecutive sets we intercalated $n$~intermediary +sets; by convention we now assume +these new sets to be equidistant. This is one +of the ways of defining the addition of two +magnitudes; for if the interval~$AB$ is by definition +equal to the interval~$CD$, the interval~$AD$ will by +definition be the sum of the intervals $AB$~and~$AC$. +This definition is very largely, but not altogether, +arbitrary. It must satisfy certain conditions---the +commutative and associative laws of addition, for +instance; but, provided the definition we choose +satisfies these laws, the choice is indifferent, and +we need not state it precisely. + +\Par{Remarks.}---We are now in a position to discuss +several important questions. + +(1) Is the creative power of the mind exhausted +by the creation of the mathematical continuum? +The answer is in the negative, and this is shown +in a very striking manner by the work of Du~Bois +Reymond. +\PageSep{29} + +We know that mathematicians distinguish +between infinitesimals of different orders, and that +infinitesimals of the second order are infinitely +small, not only absolutely so, but also in relation +to those of the first order. It is not difficult to +imagine infinitesimals of fractional or even of +irrational order, and here once more we find the +mathematical continuum which has been dealt +with in the preceding pages. Further, there are +infinitesimals which are infinitely small with +reference to those of the first order, and infinitely +large with respect to the order~$1 + \epsilon$, however +small~$\epsilon$ may be. Here, then, are new terms intercalated +in our series; and if I may be permitted to +revert to the terminology used in the preceding +pages, a terminology which is very convenient, +although it has not been consecrated by usage, I +shall say that we have created a kind of continuum +of the third order. + +It is an easy matter to go further, but it is idle +to do so, for we would only be imagining symbols +without any possible application, and no one will +dream of doing that. This continuum of the third +order, to which we are led by the consideration of +the different orders of infinitesimals, is in itself +of but little use and hardly worth quoting. +Geometers look on it as a mere curiosity. The +mind only uses its creative faculty when experiment +requires it. + +(2) When we are once in possession of the +conception of the mathematical continuum, are +\PageSep{30} +we protected from contradictions analogous to +those which gave it birth? No, and the following +is an instance:--- + +He is a \Foreign{savant} indeed who will not take it as +evident that every curve has a tangent; and, in +fact, if we think of a curve and a straight line as +two narrow bands, we can always arrange them in +such a way that they have a common part without +intersecting. Suppose now that the breadth of +the bands diminishes indefinitely: the common +part will still remain, and in the limit, so to speak, +the two lines will have a common point, although +they do not intersect---\ie, they will touch. The +geometer who reasons in this way is only doing +what we have done when we proved that two lines +which intersect have a common point, and his +intuition might also seem to be quite legitimate. +But this is not the case. We can show that there +are curves which have no tangent, if we define +such a curve as an analytical continuum of the +second order. No doubt some artifice analogous +to those we have discussed above would enable us +to get rid of this contradiction, but as the latter is +only met with in very exceptional cases, we need +not trouble to do so. Instead of endeavouring to +reconcile intuition and analysis, we are content to +sacrifice one of them, and as analysis must be +flawless, intuition must go to the wall. + +\Par{The Physical Continuum of several Dimensions.}---We +have discussed above the physical continuum +as it is derived from the immediate evidence of our +\PageSep{31} +senses---or, if the reader prefers, from the rough +results of Fechner's experiments; I have shown +that these results are summed up in the contradictory +formulæ\Chg{:---}{} +\[ +A = B,\qquad B = C,\qquad A < C. +\] + +Let us now see how this notion is generalised, +and how from it may be derived the concept of +continuums of several dimensions. Consider any +two aggregates of sensations. We can either +distinguish between them, or we cannot; just as in +Fechner's experiments the weight of $10$~grammes +could be distinguished from the weight of $12$~grammes, +but not from the weight of $11$~grammes. +This is all that is required to construct the continuum +of several dimensions. + +Let us call one of these aggregates of sensations +an \emph{element}. It will be in a measure analogous to +the \emph{point} of the mathematicians, but will not be, +however, the same thing. We cannot say that +our element has no size, for we cannot distinguish +it from its immediate neighbours, and it is thus +surrounded by a kind of fog. If the astronomical +comparison may be allowed, our ``elements'' +would be like nebulæ, whereas the mathematical +points would be like stars. + +If this be granted, a system of elements will +form a continuum, if we can pass from any one of +them to any other by a series of consecutive +elements such that each cannot be distinguished +from its predecessor. This \emph{linear} series is to the +\emph{line} of the mathematician what the isolated \emph{element} +was to the point. +\PageSep{32} + +Before going further, I must explain what is +meant by a \emph{cut}. Let us consider a continuum~$C$, +and remove from it certain of its elements, which +for a moment we shall regard as no longer belonging +to the continuum. We shall call the aggregate +of elements thus removed a \emph{cut}. By means of this +cut, the continuum~$C$ will be \emph{subdivided} into +several distinct continuums; the aggregate of +elements which remain will cease to form a single +continuum. There will then be on~$C$ two elements, +$A$~and~$B$, which we must look upon as +belonging to two distinct continuums; and we see +that this must be so, because it will be impossible +to find a linear series of consecutive elements of~$C$ +(each of the elements indistinguishable from the +preceding, the first being~$A$ and the last~$B$), \emph{unless +one of the elements of this series is indistinguishable +from one of the elements of the cut}. + +It may happen, on the contrary, that the cut +may not be sufficient to subdivide the continuum~$C$. +To classify the physical continuums, we must +first of all ascertain the nature of the cuts which +must be made in order to subdivide them. If a +physical continuum,~$C$, may be subdivided by a cut +reducing to a finite number of elements, all distinguishable +the one from the other (and therefore +forming neither one continuum nor several continuums), +we shall call~$C$ a continuum \emph{of one +dimension}. If, on the contrary, $C$~can only be subdivided +by cuts which are themselves continuums, +we shall say that $C$~is of several dimensions; if +\PageSep{33} +the cuts are continuums of one dimension, then +we shall say that $C$~has two dimensions; if cuts of +two dimensions are sufficient, we shall say that $C$~is +of three dimensions, and so on. Thus the +notion of the physical continuum of several dimensions +is defined, thanks to the very simple fact, +that two aggregates of sensations may be distinguishable +or indistinguishable. + +\Par{The Mathematical Continuum of Several Dimensions.}---The +conception of the mathematical continuum +of $n$~dimensions may be led up to quite naturally +by a process similar to that which we discussed at +the beginning of this chapter. A point of such a +continuum is defined by a system of $n$~distinct +magnitudes which we call its co-ordinates. + +The magnitudes need not always be measurable; +there is, for instance, one branch of geometry +independent of the measure of magnitudes, in +which we are only concerned with knowing, for +example, if, on a curve~$ABC$, the point~$B$ is +between the points $A$~and~$C$, and in which it is +immaterial whether the arc~$AB$ is equal to or +twice the arc~$BC$. This branch is called \emph{Analysis +Situs}. It contains quite a large body of doctrine +which has attracted the attention of the greatest +geometers, and from which are derived, one from +another, a whole series of remarkable theorems. +What distinguishes these theorems from those of +ordinary geometry is that they are purely qualitative. +They are still true if the figures are copied +by an unskilful draughtsman, with the result that +\PageSep{34} +the proportions are distorted and the straight lines +replaced by lines which are more or less curved. + +As soon as measurement is introduced into the +continuum we have just defined, the continuum +becomes space, and geometry is born. But the +discussion of this is reserved for Part~II. +\PageSep{35} + + +\Part{II.}{Space.} + +\Chapter{III.}{Non-Euclidean Geometries.} + +\First{Every} conclusion presumes premisses. These +premisses are either self-evident and need no +demonstration, or can be established only if based +on other propositions; and, as we cannot go back +in this way to infinity, every deductive science, +and geometry in particular, must rest upon a +certain number of indemonstrable axioms. All +treatises of geometry begin therefore with the +enunciation of these axioms. But there is a +distinction to be drawn between them. Some of +these, for example, ``Things which are equal to +the same thing are equal to one another,'' are not +propositions in geometry but propositions in +analysis. I look upon them as analytical \Foreign{à ~priori} +intuitions, and they concern me no further. But +I must insist on other axioms which are special +to geometry. Of these most treatises explicitly +enunciate three:---(1)~Only one line can pass +through two points; (2)~a straight line is the +\PageSep{36} +shortest distance between two points; (3)~through +one point only one parallel can be drawn to a +given straight line. Although we generally dispense +with proving the second of these axioms, it +would be possible to deduce it from the other two, +and from those much more numerous axioms +which are implicitly admitted without enunciation, +as I shall explain further on. For a long +time a proof of the third axiom known as Euclid's +postulate was sought in vain. It is impossible to +imagine the efforts that have been spent in pursuit +of this chimera. Finally, at the beginning of the +nineteenth century, and almost simultaneously, +%[** TN: Correct ("Hongrois") in the French edition] +two scientists, a Russian and a \Reword{Bulgarian}{Hungarian}, Lobatschewsky +and Bolyai, showed irrefutably that this +proof is impossible. They have nearly rid us of +inventors of geometries without a postulate, and +ever since the Académic des Sciences receives only +about one or two new demonstrations a year. +But the question was not exhausted, and it was +not long before a great step was taken by the +celebrated memoir of Riemann, entitled: \Title{Ueber +die Hypothesen welche der Geometrie zum Grunde +liegen}. This little work has inspired most of the +recent treatises to which I shall later on refer, and +among which I may mention those of Beltrami +and Helmholtz. + +\Par{The Geometry of Lobatschewsky.}---If it were +possible to deduce Euclid's postulate from the +several axioms, it is evident that by rejecting +the postulate and retaining the other axioms we +\PageSep{37} +should be led to contradictory consequences. It +would be, therefore, impossible to found on those +premisses a coherent geometry. Now, this is +precisely what Lobatschewsky has done. He +assumes at the outset that several parallels may +be drawn through a point to a given straight line, +and he retains all the other axioms of Euclid. +From these hypotheses he deduces a series of +theorems between which it is impossible to find +any contradiction, and he constructs a geometry +as impeccable in its logic as Euclidean geometry. +The theorems are very different, however, from +those to which we are accustomed, and at first +will be found a little disconcerting. For instance, +the sum of the angles of a triangle is always less +than two right angles, and the difference between +that sum and two right angles is proportional to +the area of the triangle. It is impossible to construct +a figure similar to a given figure but of +different dimensions. If the circumference of a +circle be divided into $n$~equal parts, and tangents +be drawn at the points of intersection, the $n$~tangents +will form a polygon if the radius of +the circle is small enough, but if the radius is +large enough they will never meet. We need not +multiply these examples. Lobatschewsky's propositions +have no relation to those of Euclid, +but they are none the less logically interconnected. + +\Par{Riemann's Geometry.}---Let us imagine to ourselves +a world only peopled with beings of no +thickness, and suppose these ``infinitely flat'' +\PageSep{38} +animals are all in one and the same plane, from +which they cannot emerge. Let us further admit +that this world is sufficiently distant from other +worlds to be withdrawn from their influence, and +while we are making these hypotheses it will not +cost us much to endow these beings with reasoning +power, and to believe them capable of making +a geometry. In that case they will certainly +attribute to space only two dimensions. But +now suppose that these imaginary animals, while +remaining without thickness, have the form of a +spherical, and not of a plane figure, and are all on +the same sphere, from which they cannot escape. +What kind of a geometry will they construct? In +the first place, it is clear that they will attribute to +space only two dimensions. The straight line to +them will be the shortest distance from one point +on the sphere to another---that is to say, an arc of +a great circle. In a word, their geometry will be +spherical geometry. What they will call space +will be the sphere on which they are confined, and +on which take place all the phenomena with +which they are acquainted. Their space will +therefore be \emph{unbounded}, since on a sphere one may +always walk forward without ever being brought +to a stop, and yet it will be \emph{finite}; the end will +never be found, but the complete tour can be +made. Well, Riemann's geometry is spherical +geometry extended to three dimensions. To construct +it, the German mathematician had first of +all to throw overboard, not only Euclid's postulate +\PageSep{39} +but also the first axiom that \emph{only one line can pass +through two points}. On a sphere, through two +given points, we can \emph{in general} draw only one great +circle which, as we have just seen, would be to +our imaginary beings a straight line. But there +was one exception. If the two given points are +at the ends of a diameter, an infinite number of +great circles can be drawn through them. In +the same way, in Riemann's geometry---at least in +one of its forms---through two points only one +straight line can in general be drawn, but there are +exceptional cases in which through two points +an infinite number of straight lines can be drawn. +So there is a kind of opposition between the +geometries of Riemann and Lobatschewsky. For +instance, the sum of the angles of a triangle is +equal to two right angles in Euclid's geometry, +less than two right angles in that of Lobatschewsky, +and greater than two right angles in that +of Riemann. The number of parallel lines that +can be drawn through a given point to a given +line is one in Euclid's geometry, none in Riemann's, +and an infinite number in the geometry of Lobatschewsky. +Let us add that Riemann's space is +finite, although unbounded in the sense which we +have above attached to these words. + +\Par{Surfaces with Constant Curvature.}---One objection, +however, remains possible. There is no contradiction +between the theorems of Lobatschewsky and +Riemann; but however numerous are the other +consequences that these geometers have deduced +\PageSep{40} +from their hypotheses, they had to arrest their +course before they exhausted them all, for the +number would be infinite; and who can say that +if they had carried their deductions further they +would not have eventually reached some contradiction? +This difficulty does not exist for +Riemann's geometry, provided it is limited to +two dimensions. As we have seen, the two-dimensional +geometry of Riemann, in fact, does +not differ from spherical geometry, which is only a +branch of ordinary geometry, and is therefore outside +all contradiction. Beltrami, by showing that +Lobatschewsky's two-dimensional geometry was +only a branch of ordinary geometry, has equally +refuted the objection as far as it is concerned. +This is the course of his argument: Let us consider +any figure whatever on a surface. Imagine +this figure to be traced on a flexible and inextensible +canvas applied to the surface, in such +a way that when the canvas is displaced and +deformed the different lines of the figure change +their form without changing their length. As a +rule, this flexible and inextensible figure cannot be +displaced without leaving the surface. But there +are certain surfaces for which such a movement +would be possible. They are surfaces of constant +curvature. If we resume the comparison that we +made just now, and imagine beings without thickness +living on one of these surfaces, they will +regard as possible the motion of a figure all the +lines of which remain of a constant length. Such +\PageSep{41} +a movement would appear absurd, on the other +hand, to animals without thickness living on a +surface of variable curvature. These surfaces of +constant curvature are of two kinds. The +curvature of some is \emph{positive}, and they may be +deformed so as to be applied to a sphere. The +geometry of these surfaces is therefore reduced to +spherical geometry---namely, Riemann's. The curvature +of others is \emph{negative}. Beltrami has shown +that the geometry of these surfaces is identical +with that of Lobatschewsky. Thus the two-dimensional +geometries of Riemann and Lobatschewsky +are connected with Euclidean geometry. + +\Par{Interpretation of Non-Euclidean Geometries.}---Thus +vanishes the objection so far as two-dimensional +geometries are concerned. It would be easy to +extend Beltrami's reasoning to three-dimensional +geometries, and minds which do not recoil before +space of four dimensions will see no difficulty in +it; but such minds are few in number. I prefer, +then, to proceed otherwise. Let us consider a +certain plane, which I shall call the fundamental +plane, and let us construct a kind of dictionary by +making a double series of terms written in two +columns, and corresponding each to each, just as +in ordinary dictionaries the words in two languages +which have the same signification correspond to +one another:--- +\Dict{Space}{\raggedright The portion of space situated +above the fundamental +plane.} +\PageSep{42} +\Dict{Plane}{\raggedright Sphere cutting orthogonally +the fundamental plane.} +\Dict{Line}{\raggedright Circle cutting orthogonally +the fundamental plane.} +\Dict{Sphere}{Sphere.} +\Dict{Circle}{Circle.} +\Dict{Angle}{Angle.} +\Dict{Distance between +two points}{Logarithm of the anharmonic +ratio of these two points +and of the intersection +of the fundamental plane +with the circle passing +through these two points +and cutting it orthogonally.} +\Dict{Etc.}{Etc.} + +Let us now take Lobatschewsky's theorems and +translate them by the aid of this dictionary, as we +would translate a German text with the aid of +a German-French dictionary. \emph{We shall then +obtain the theorems of ordinary geometry.} For +instance, Lobatschewsky's theorem: ``The sum of +the angles of a triangle is less than two right +angles,'' may be translated thus: ``If a curvilinear +triangle has for its sides arcs of circles which if +produced would cut orthogonally the fundamental +plane, the sum of the angles of this curvilinear +triangle will be less than two right angles.'' Thus, +however far the consequences of Lobatschewsky's +hypotheses are carried, they will never lead to a +\PageSep{43} +contradiction; in fact, if two of Lobatschewsky's +theorems were contradictory, the translations of +these two theorems made by the aid of our +dictionary would be contradictory also. But +these translations are theorems of ordinary +geometry, and no one doubts that ordinary +geometry is exempt from contradiction. Whence +is the certainty derived, and how far is it justified? +That is a question upon which I cannot enter +here, but it is a very interesting question, and I +think not insoluble. Nothing, therefore, is left of +the objection I formulated above. But this is not +all. Lobatschewsky's geometry being susceptible +of a concrete interpretation, ceases to be a useless +logical exercise, and may be applied. I have no +time here to deal with these applications, nor +with what Herr Klein and myself have done by +using them in the integration of linear equations. +Further, this interpretation is not unique, and +several dictionaries may be constructed analogous +to that above, which will enable us by a simple +translation to convert Lobatschewsky's theorems +into the theorems of ordinary geometry. + +\Par{Implicit Axioms.}---Are the axioms implicitly +enunciated in our text-books the only foundation +of geometry? We may be assured of the contrary +when we see that, when they are abandoned one +after another, there are still left standing some +propositions which are common to the geometries +of Euclid, Lobatschewsky, and Riemann. These +propositions must be based on premisses that +\PageSep{44} +geometers admit without enunciation. It is interesting +to try and extract them from the classical +proofs. + +John Stuart Mill asserted\footnote + {\Title{Logic}, c.~viii., cf.\ Definitions, §5--6.\Transl} +that every definition +contains an axiom, because by defining we implicitly +affirm the existence of the object defined. +That is going rather too far. It is but rarely in +mathematics that a definition is given without +following it up by the proof of the existence of the +object defined, and when this is not done it is +generally because the reader can easily supply +it; and it must not be forgotten that the word +``existence'' has not the same meaning when it +refers to a mathematical entity as when it refers to +a material object. + +A mathematical entity exists provided there is +no contradiction implied in its definition, either in +itself, or with the propositions previously admitted. +But if the observation of John Stuart Mill cannot +be applied to all definitions, it is none the less true +for some of them. A plane is sometimes defined +in the following manner:---The plane is a surface +such that the line which joins any two points +upon it lies wholly on that surface. Now, there is +obviously a new axiom concealed in this definition. +It is true we might change it, and that would be +preferable, but then we should have to enunciate +the axiom explicitly. Other definitions may give +rise to no less important reflections, such as, for +example, that of the equality of two figures. Two +\PageSep{45} +figures are equal when they can be superposed. +To superpose them, one of them must be displaced +until it coincides with the other. But how must +it be displaced? If we asked that question, no +doubt we should be told that it ought to be done +without deforming it, and as an invariable solid is +displaced. The vicious circle would then be evident. +As a matter of fact, this definition defines +nothing. It has no meaning to a being living in a +world in which there are only fluids. If it seems +clear to us, it is because we are accustomed to the +properties of natural solids which do not much +differ from those of the ideal solids, all of whose +dimensions are invariable. However, imperfect as +it may be, this definition implies an axiom. The +possibility of the motion of an invariable figure is +not a self-evident truth. At least it is only so in +the application to Euclid's postulate, and not as an +analytical \Foreign{à ~priori} intuition would be. Moreover, +when we study the definitions and the proofs +of geometry, we see that we are compelled to +admit without proof not only the possibility of +this motion, but also some of its properties. This +first arises in the definition of the straight line. +Many defective definitions have been given, but +the true one is that which is understood in all the +proofs in which the straight line intervenes. ``It +may happen that the motion of an invariable figure +may be such that all the points of a line belonging +to the figure are motionless, while all the points +situate outside that line are in motion. Such a +\PageSep{46} +line would be called a straight line.'' We have +deliberately in this enunciation separated the +definition from the axiom which it implies. Many +proofs such as those of the cases of the equality of +triangles, of the possibility of drawing a perpendicular +from a point to a straight line, assume propositions +the enunciations of which are dispensed +with, for they necessarily imply that it is possible +to move a figure in space in a certain way. + +\Par{The Fourth Geometry.}---Among these explicit +axioms there is one which seems to me to deserve +some attention, because when we abandon it we +can construct a fourth geometry as coherent as +those of Euclid, Lobatschewsky, and Riemann. +To prove that we can always draw a perpendicular +at a point~$A$ to a straight line~$AB$, we consider a +straight line~$AC$ movable about the point~$A$, and +initially identical with the fixed straight line~$AB$. +We then can make it turn about the point~$A$ until +it lies in~$AB$ produced. Thus we assume two +propositions---first, that such a rotation is possible, +and then that it may continue until the two lines +lie the one in the other produced. If the first +point is conceded and the second rejected, we are +led to a series of theorems even stranger than those +of Lobatschewsky and Riemann, but equally free +from contradiction. I shall give only one of these +theorems, and I shall not choose the least remarkable +of them. \emph{A real straight line may be perpendicular +to itself.} + +\Par{Lie's Theorem.}---The number of axioms implicitly +\PageSep{47} +introduced into classical proofs is greater than +necessary, and it would be interesting to reduce +them to a minimum. It may be asked, in the first +place, if this reduction is possible---if the number of +necessary axioms and that of imaginable geometries +is not infinite? A theorem due to Sophus Lie is of +weighty importance in this discussion. It may be +enunciated in the following manner:---Suppose the +following premisses are admitted: (1)~space has $n$~dimensions; +(2)~the movement of an invariable +figure is possible; (3)~$p$~conditions are necessary to +determine the position of this figure in space. + +\emph{The number of geometries compatible with these +premisses will be limited.} I may even add that if $n$~is +given, a superior limit can be assigned to~$p$. If, +therefore, the possibility of the movement is +granted, we can only invent a finite and even +a rather restricted number of three-dimensional +geometries. + +\Par{Riemann's Geometries.}---However, this result +seems contradicted by Riemann, for that scientist +constructs an infinite number of geometries, and +that to which his name is usually attached is only +a particular case of them. All depends, he says, +on the manner in which the length of a curve is +defined. Now, there is an infinite number of ways +of defining this length, and each of them may be +the starting-point of a new geometry. That is +perfectly true, but most of these definitions are incompatible +with the movement of a variable figure +such as we assume to be possible in Lie's theorem. +\PageSep{48} +These geometries of Riemann, so interesting on +various grounds, can never be, therefore, purely +analytical, and would not lend themselves to +proofs analogous to those of Euclid. + +\Par{On the Nature of Axioms.}---Most mathematicians +regard Lobatschewsky's geometry as a mere logical +curiosity. Some of them have, however, gone +further. If several geometries are possible, they +say, is it certain that our geometry is the one that +is true? Experiment no doubt teaches us that the +sum of the angles of a triangle is equal to two +right angles, but this is because the triangles we +deal with are too small. According to Lobatschewsky, +the difference is proportional to the area +of the triangle, and will not this become sensible +when we operate on much larger triangles, and +when our measurements become more accurate? +Euclid's geometry would thus be a provisory +geometry. Now, to discuss this view we must +first of all ask ourselves, what is the nature of +geometrical axioms? Are they synthetic \Foreign{à ~priori} +intuitions, as Kant affirmed? They would then +be imposed upon us with such a force that we +could not conceive of the contrary proposition, nor +could we build upon it a theoretical edifice. There +would be no non-Euclidean geometry. To convince +ourselves of this, let us take a true synthetic +\Foreign{à ~priori} intuition---the following, for instance, which +played an important part in the first chapter:---If +a theorem is true for the number~$1$, and if it has +been proved that it is true of~$n + 1$, provided it is +\PageSep{49} +true of~$n$, it will be true for all positive integers. +Let us next try to get rid of this, and while rejecting +this proposition let us construct a false +arithmetic analogous to non-Euclidean geometry. +We shall not be able to do it. We shall be even +tempted at the outset to look upon these intuitions +as analytical. Besides, to take up again +our fiction of animals without thickness, we can +scarcely admit that these beings, if their minds +are like ours, would adopt the Euclidean geometry, +which would be contradicted by all their experience. +Ought we, then, to conclude that the +axioms of geometry are experimental truths? +But we do not make experiments on ideal lines or +ideal circles; we can only make them on material +objects. On what, therefore, would experiments +serving as a foundation for geometry be based? +The answer is easy. We have seen above that we +constantly reason as if the geometrical figures +behaved like solids. What geometry would borrow +from experiment would be therefore the properties +of these bodies. The properties of light +and its propagation in a straight line have also +given rise to some of the propositions of geometry, +and in particular to those of projective geometry, +so that from that point of view one would be +tempted to say that metrical geometry is the study +of solids, and projective geometry that of light. +But a difficulty remains, and is unsurmountable. +If geometry were an experimental science, it would +not be an exact science. It would be subjected to +\PageSep{5O} +continual revision. Nay, it would from that day +forth be proved to be erroneous, for we know that +no rigorously invariable solid exists. \emph{The geometrical +axioms are therefore neither synthetic \Foreign{à ~priori} +intuitions nor experimental facts.} They are conventions. +Our choice among all possible conventions +is \emph{guided} by experimental facts; but it remains +\emph{free}, and is only limited by the necessity of avoiding +every contradiction, and thus it is that postulates +may remain rigorously true even when the +experimental laws which have determined their +adoption are only approximate. In other words, +\emph{the axioms of geometry} (I do not speak of those of +arithmetic) \emph{are only definitions in disguise}. What, +then, are we to think of the question: Is +Euclidean geometry true? It has no meaning. +We might as well ask if the metric system is true, +and if the old weights and measures are false; if +Cartesian co-ordinates are true and polar co-ordinates +false. One geometry cannot be more +true than another; it can only be more convenient. +Now, Euclidean geometry is, and will remain, the +most convenient: 1st,~because it is the simplest, +and it is not so only because of our mental habits +or because of the kind of direct intuition that we +have of Euclidean space; it is the simplest in +itself, just as a polynomial of the first degree is +simpler than a polynomial of the second degree; +2nd,~because it sufficiently agrees with the properties +of natural solids, those bodies which we +can compare and measure by means of our senses. +\PageSep{51} + + +\Chapter{IV.}{Space and Geometry.} + +\First{Let} us begin with a little paradox. Beings whose +minds were made as ours, and with senses like +ours, but without any preliminary education, +might receive from a suitably-chosen external +world impressions which would lead them to +construct a geometry other than that of Euclid, +and to localise the phenomena of this external +world in a non-Euclidean space, or even in space +of four dimensions. As for us, whose education +has been made by our actual world, if we were +suddenly transported into this new world, we +should have no difficulty in referring phenomena +to our Euclidean space. Perhaps somebody may +appear on the scene some day who will devote his +life to it, and be able to represent to himself the +fourth dimension. + +\Par{Geometrical Space and Representative Space.}---It is +often said that the images we form of external +objects are localised in space, and even that they +can only be formed on this condition. It is also +said that this space, which thus serves as a kind of +framework ready prepared for our sensations and +representations, is identical with the space of the +\PageSep{52} +geometers, having all the properties of that space. +To all clear-headed men who think in this way, +the preceding statement might well appear extraordinary; +but it is as well to see if they are not +the victims of some illusion which closer analysis +may be able to dissipate. In the first place, what +are the properties of space properly so called? +I mean of that space which is the object of +geometry, and which I shall call geometrical +space. The following are some of the more +essential:--- + +1st,~it is continuous; 2nd,~it is infinite; 3rd,~it +is of three dimensions; 4th,~it is homogeneous---that +is to say, all its points are identical one +with another; 5th,~it is isotropic. Compare this +now with the framework of our representations +and sensations, which I may call \emph{representative +space}. + +\Par{Visual Space.}---First of all let us consider a +purely visual impression, due to an image formed +on the back of the retina. A cursory analysis shows +us this image as continuous, but as possessing only +two dimensions, which already distinguishes purely +visual from what may be called geometrical space. +On the other hand, the image is enclosed within +a limited framework; and there is a no less +important difference: \emph{this pure visual space is not +homogeneous}. All the points on the retina, apart +from the images which may be formed, do not +play the same rôle. The yellow spot can in no +way be regarded as identical with a point on the +\PageSep{53} +edge of the retina. Not only does the same object +produce on it much brighter impressions, but in +the whole of the \emph{limited} framework the point +which occupies the centre will not appear identical +with a point near one of the edges. Closer +analysis no doubt would show us that this continuity +of visual space and its two dimensions are +but an illusion. It would make visual space even +more different than before from geometrical space, +but we may treat this remark as incidental. + +However, sight enables us to appreciate distance, +and therefore to perceive a third dimension. +But every one knows that this perception of the +third dimension reduces to a sense of the effort of +accommodation which must be made, and to a +sense of the convergence of the two eyes, that +must take place in order to perceive an object +distinctly. These are muscular sensations quite +different from the visual sensations which have +given us the concept of the two first dimensions. +The third dimension will therefore not appear to us +as playing the same rôle as the two others. What +may be called \emph{complete visual space} is not therefore +an isotropic space. It has, it is true, exactly +three dimensions; which means that the elements +of our visual sensations (those at least which +concur in forming the concept of extension) will +be completely defined if we know three of them; +or, in mathematical language, they will be functions +of three independent variables. But let us +look at the matter a little closer. The third +\PageSep{54} +dimension is revealed to us in two different ways: +by the effort of accommodation, and by the convergence +of the eyes. No doubt these two indications +are always in harmony; there is between +them a constant relation; or, in mathematical +language, the two variables which measure these +two muscular sensations do not appear to us as +independent. Or, again, to avoid an appeal to +mathematical ideas which are already rather too +refined, we may go back to the language of the +preceding chapter and enunciate the same fact as +follows:---If two sensations of convergence $A$~and~$B$ +are indistinguishable, the two sensations of +accommodation $A'$~and~$B'$ which accompany them +respectively will also be indistinguishable. But +that is, so to speak, an experimental fact. Nothing +prevents us \Foreign{à ~priori} from assuming the contrary, +and if the contrary takes place, if these two +muscular sensations both vary independently, we +must take into account one more independent +variable, and complete visual space will appear +to us as a physical continuum of four dimensions. +And so in this there is also a fact of \emph{external} +experiment. Nothing prevents us from assuming +that a being with a mind like ours, with the same +sense-organs as ourselves, may be placed in a world +in which light would only reach him after being +passed through refracting media of complicated +form. The two indications which enable us to +appreciate distances would cease to be connected +by a constant relation. A being educating his +\PageSep{55} +senses in such a world would no doubt attribute +four dimensions to complete visual space. + +\Par{Tactile and Motor Space.}---``Tactile space'' is +more complicated still than visual space, and differs +even more widely from geometrical space. It is +useless to repeat for the sense of touch my remarks +on the sense of sight. But outside the data of +sight and touch there are other sensations which +contribute as much and more than they do to the +genesis of the concept of space. They are those +which everybody knows, which accompany all our +movements, and which we usually call muscular +sensations. The corresponding framework constitutes +what may be called \emph{motor space}. Each +muscle gives rise to a special sensation which may +be increased or diminished so that the aggregate +of our muscular sensations will depend upon as +many variables as we have muscles. From this +point of view \emph{motor space would have as many dimensions +as we have muscles}. I know that it is said +that if the muscular sensations contribute to form +the concept of space, it is because we have the +sense of the \emph{direction} of each movement, and that +this is an integral part of the sensation. If this +were so, and if a muscular sense could not be +aroused unless it were accompanied by this geometrical +sense of direction, geometrical space +would certainly be a form imposed upon our +sensitiveness. But I do not see this at all when +I analyse my sensations. What I do see is that +the sensations which correspond to movements in +\PageSep{56} +the same direction are connected in my mind by a +simple \emph{association of ideas}. It is to this association +that what we call the sense of direction is reduced. +We cannot therefore discover this sense in a single +sensation. This association is extremely complex, +for the contraction of the same muscle may correspond, +according to the position of the limbs, +to very different movements of direction. Moreover, +it is evidently acquired; it is like all +associations of ideas, the result of a \emph{habit}. This +habit itself is the result of a very large number of +\emph{experiments}, and no doubt if the education of our +senses had taken place in a different medium, +where we would have been subjected to different +impressions, then contrary habits would have been +acquired, and our muscular sensations would have +been associated according to other laws. + +\Par{Characteristics of Representative Space.}---Thus representative +space in its triple form---visual, +tactile, and motor---differs essentially from geometrical +space. It is neither homogeneous nor +isotropic; we cannot even say that it is of three +dimensions. It is often said that we ``project'' +into geometrical space the objects of our external +perception; that we ``localise'' them. Now, has +that any meaning, and if so what is that meaning? +Does it mean that we \emph{represent} to ourselves external +objects in geometrical space? Our representations +are only the reproduction of our sensations; +they cannot therefore be arranged in the +same framework---that is to say, in representative +\PageSep{57} +space. It is also just as impossible for us to represent +to ourselves external objects in geometrical +space, as it is impossible for a painter to paint on +a flat surface objects with their three dimensions. +Representative space is only an image of geometrical +space, an image deformed by a kind of +perspective, and we can only represent to ourselves +objects by making them obey the laws of +this perspective. Thus we do not \emph{represent} to ourselves +external bodies in geometrical space, but we +\emph{reason} about these bodies as if they were situated +in geometrical space. When it is said, on the +other hand, that we ``localise'' such an object in +such a point of space, what does it mean? \emph{It +simply means that we represent to ourselves the movements +that must take place to reach that object.} And +it does not mean that to represent to ourselves +these movements they must be projected into +space, and that the concept of space must therefore +pre-exist. When I say that we represent to ourselves +these movements, I only mean that we +represent to ourselves the muscular sensations +which accompany them, and which have no +geometrical character, and which therefore in no +way imply the pre-existence of the concept of +space. + +\Par{Changes of State and Changes of Position.}---But, +it may be said, if the concept of geometrical space +is not imposed upon our minds, and if, on the +other hand, none of our sensations can furnish us +with that concept, how then did it ever come into +\PageSep{58} +existence? This is what we have now to examine, +and it will take some time; but I can sum up in a +few words the attempt at explanation which I am +going to develop. \emph{None of our sensations, if isolated, +could have brought us to the concept of space; we are +brought to it solely by studying the laws by which those +sensations succeed one another.} We see at first that +our impressions are subject to change; but among +the changes that we ascertain, we are very soon +led to make a distinction. Sometimes we say that +the objects, the causes of these impressions, have +changed their state, sometimes that they have +changed their position, that they have only been +displaced. Whether an object changes its state or +only its position, this is always translated for us in +the same manner, \emph{by a modification in an aggregate +of impressions}. How then have we been enabled +to distinguish them? If there were only change +of position, we could restore the primitive aggregate +of impressions by making movements which +would confront us with the movable object in +the same \emph{relative} situation. We thus \emph{correct} the +modification which was produced, and we re-establish +the initial state by an inverse modification. +If, for example, it were a question of the +sight, and if an object be displaced before our +eyes, we can ``follow it with the eye,'' and retain +its image on the same point of the retina by +appropriate movements of the eyeball. These +movements we are conscious of because they are +voluntary, and because they are accompanied by +\PageSep{59} +muscular sensations. But that does not mean +that we represent them to ourselves in geometrical +space. So what characterises change of position, +what distinguishes it from change of state, is that +it can always be \emph{corrected} by this means. It may +therefore happen that we pass from the aggregate +of impressions~$A$ to the aggregate~$B$ in two different +ways. First, involuntarily and without experiencing +muscular sensations---which happens +when it is the object that is displaced; secondly, +voluntarily, and with muscular sensation---which +happens when the object is motionless, but when +we displace ourselves in such a way that the +object has relative motion with respect to us. If +this be so, the translation of the aggregate~$A$ to +the aggregate~$B$ is only a change of position. It +follows that sight and touch could not have given +us the idea of space without the help of the +``muscular sense.'' Not only could this concept +not be derived from a single sensation, or even from +\emph{a series of sensations}; but a \emph{motionless} being could +never have acquired it, because, not being able to +correct by his movements the effects of the change +of position of external objects, he would have had +no reason to distinguish them from changes of +state. Nor would he have been able to acquire +it if his movements had not been voluntary, +or if they were unaccompanied by any sensations +whatever. + +\Par{Conditions of Compensation.}---How is such a +compensation possible in such a way that two +\PageSep{60} +changes, otherwise mutually independent, may be +reciprocally corrected? A mind \emph{already familiar +with geometry} would reason as follows:---If there +is to be compensation, the different parts of the +external object on the one hand, and the different +organs of our senses on the other, must be in the +same \emph{relative} position after the double change. +And for that to be the case, the different parts of +the external body on the one hand, and the different +organs of our senses on the other, must have +the same relative position to each other after the +double change; and so with the different parts of +our body with respect to each other. In other +words, the external object in the first change must +be displaced as an invariable solid would be displaced, +and it must also be so with the whole of our +body in the second change, which is to correct the +first. Under these conditions compensation may +be produced. But we who as yet know nothing of +geometry, whose ideas of space are not yet formed, +we cannot reason in this way---we cannot predict +\Foreign{à ~priori} if compensation is possible. But experiment +shows us that it sometimes does take place, +and we start from this experimental fact in order +to distinguish changes of state from changes of +position. + +\Par{Solid Bodies and Geometry.}---Among surrounding +objects there are some which frequently experience +displacements that may be thus corrected by a +\emph{correlative} movement of our own body---namely, +\emph{solid bodies}. The other objects, whose form is variable, +\PageSep{61} +only in exceptional circumstances undergo +similar displacement (change of position without +change of form). When the displacement of a +body takes place with deformation, we can no +longer by appropriate movements place the organs +of our body in the same \emph{relative} situation with +respect to this body; we can no longer, therefore, +reconstruct the primitive aggregate of impressions. + +It is only later, and after a series of new experiments, +that we learn how to decompose a body of +variable form into smaller elements such that each +is displaced approximately according to the same +laws as solid bodies. We thus distinguish ``deformations'' +from other changes of state. In these +deformations each element undergoes a simple +change of position which may be corrected; but the +modification of the aggregate is more profound, +and can no longer be corrected by a correlative +movement. Such a concept is very complex even +at this stage, and has been relatively slow in +its appearance. It would not have been conceived +at all had not the observation of solid bodies shown +us beforehand how to distinguish changes of +position. + +\emph{If, then, there were no solid bodies in nature there +would be no geometry.} + +Another remark deserves a moment's attention. +Suppose a solid body to occupy successively the +positions $\alpha$~and~$\beta$; in the first position it will give +us an aggregate of impressions~$A$, and in the second +position the aggregate of impressions~$B$. Now let +\PageSep{62} +there be a second solid body, of qualities entirely +different from the first---of different colour, for +instance. Assume it to pass from the position~$\alpha$, +where it gives us the aggregate of impressions~$A'$ to +the position~$\beta$, where it gives the aggregate of +impressions~$B'$. In general, the aggregate~$A$ will +have nothing in common with the aggregate~$A'$, +nor will the aggregate~$B$ have anything in common +with the aggregate~$B'$. The transition from the +aggregate~$A$ to the aggregate~$B$, and that of the +aggregate~$A'$ to the aggregate~$B'$, are therefore +two changes which \emph{in themselves} have in general +nothing in common. Yet we consider both +these changes as displacements; and, further, we +consider them the \emph{same} displacement. How can +this be? It is simply because they may be both +corrected by the \emph{same} correlative movement of our +body. ``Correlative movement,'' therefore, constitutes +the \emph{sole connection} between two phenomena +which otherwise we should never have dreamed of +connecting. + +On the other hand, our body, thanks to the +number of its articulations and muscles, may have +a multitude of different movements, but all are not +capable of ``correcting'' a modification of external +objects; those alone are capable of it in which +our whole body, or at least all those in which +the organs of our senses enter into play are +displaced \Foreign{en bloc}---\ie, without any variation of +their relative positions, as in the case of a solid +body. +\PageSep{63} + +To sum up:\Add{---} + +1. In the first place, we distinguish two categories +of phenomena:---The first involuntary, unaccompanied +by muscular sensations, and attributed to +external objects---they are external changes; the +second, of opposite character and attributed to the +movements of our own body, are internal changes. + +2. We notice that certain changes of each in +these categories may be corrected by a correlative +change of the other category. + +3. We distinguish among external changes those +that have a correlative in the other category---which +we call displacements; and in the same way +we distinguish among the internal changes those +which have a correlative in the first category. + +Thus by means of this reciprocity is defined a +particular class of phenomena called displacements. +\emph{The laws of these phenomena are the object of +geometry.} + +\Par{Law of Homogeneity.}---The first of these laws +is the law of homogeneity. Suppose that by an +external change we pass from the aggregate of +impressions~$A$ to the aggregate~$B$, and that then +this change~$\alpha$ is corrected by a correlative +voluntary movement~$\beta$, so that we are brought +back to the aggregate~$A$. Suppose now that +another external change~$\alpha'$ brings us again from +the aggregate~$A$ to the aggregate~$B$. Experiment +then shows us that this change~$\alpha'$, like the change~$\alpha$, +may be corrected by a voluntary correlative +movement~$\beta'$, and that this movement~$\beta'$ corresponds +\PageSep{64} +to the same muscular sensations as the +movement~$\beta$ which corrected~$\alpha$. + +This fact is usually enunciated as follows:---\emph{Space +is homogeneous and isotropic.} We may also say that a +movement which is once produced may be repeated +a second and a third time, and so on, without any +variation of its properties. In the first chapter, in +which we discussed the nature of mathematical +reasoning, we saw the importance that should be +attached to the possibility of repeating the same +operation indefinitely. The virtue of mathematical +reasoning is due to this repetition; by means of the +law of homogeneity geometrical facts are apprehended. +To be complete, to the law of homogeneity +must be added a multitude of other laws, +into the details of which I do not propose to enter, +but which mathematicians sum up by saying that +these displacements form a ``group.'' + +\Par{The Non-Euclidean World.}---If geometrical space +were a framework imposed on \emph{each} of our representations +considered individually, it would be +impossible to represent to ourselves an image +without this framework, and we should be quite +unable to change our geometry. But this is not +the case; geometry is only the summary of the +laws by which these images succeed each other. +There is nothing, therefore, to prevent us from +imagining a series of representations, similar in +every way to our ordinary representations, but +succeeding one another according to laws which +differ from those to which we are accustomed. We +\PageSep{65} +may thus conceive that beings whose education +has taken place in a medium in which those laws +would be so different, might have a very different +geometry from ours. + +Suppose, for example, a world enclosed in a large +sphere and subject to the following laws:---The +temperature is not uniform; it is greatest at the +centre, and gradually decreases as we move towards +the circumference of the sphere, where it is absolute +zero. The law of this temperature is as follows:---If +$R$~be the radius of the sphere, and $r$~the distance +of the point considered from the centre, the absolute +temperature will be proportional to~$R^{2} - r^{2}$. +Further, I shall suppose that in this world all bodies +have the same co-efficient of dilatation, so that the +linear dilatation of any body is proportional to its +absolute temperature. Finally, I shall assume that +a body transported from one point to another of +different temperature is instantaneously in thermal +equilibrium with its new environment. There is +nothing in these hypotheses either contradictory +or unimaginable. A moving object will become +smaller and smaller as it approaches the circumference +of the sphere. Let us observe, in the first +place, that although from the point of view of our +ordinary geometry this world is finite, to its inhabitants +it will appear infinite. As they approach the +surface of the sphere they become colder, and at +the same time smaller and smaller. The steps +they take are therefore also smaller and smaller, +so that they can never reach the boundary of the +\PageSep{66} +sphere. If to us geometry is only the study of the +laws according to which invariable solids move, to +these imaginary beings it will be the study of the +laws of motion of solids \emph{deformed by the differences +of temperature} alluded to. + +No doubt, in our world, natural solids also experience +variations of form and volume due to +differences of temperature. But in laying the +foundations of geometry we neglect these variations; +for besides being but small they are irregular, +and consequently appear to us to be accidental. +In our hypothetical world this will no longer be +the case, the variations will obey very simple and +regular laws. On the other hand, the different +solid parts of which the bodies of these inhabitants +are composed will undergo the same variations of +form and volume. + +Let me make another hypothesis: suppose that +light passes through media of different refractive +indices, such that the index of refraction is inversely +proportional to~$R^{2} - r^{2}$. Under these conditions it +is clear that the rays of light will no longer be +rectilinear but circular. To justify what has been +said, we have to prove that certain changes in the +position of external objects may be corrected by +correlative movements of the beings which inhabit +this imaginary world; and in such a way as to +restore the primitive aggregate of the impressions +experienced by these sentient beings. Suppose, +for example, that an object is displaced and +deformed, not like an invariable solid, but like a +\PageSep{67} +solid subjected to unequal dilatations in exact conformity +with the law of temperature assumed +above. To use an abbreviation, we shall call such +a movement a non-Euclidean displacement. + +If a sentient being be in the neighbourhood of +such a displacement of the object, his impressions +will be modified; but by moving in a suitable +manner, he may reconstruct them. For this +purpose, all that is required is that the aggregate +of the sentient being and the object, considered as +forming a single body, shall experience one of those +special displacements which I have just called non-Euclidean. +This is possible if we suppose that the +limbs of these beings dilate according to the same +laws as the other bodies of the world they inhabit. + +Although from the point of view of our ordinary +geometry there is a deformation of the bodies in +this displacement, and although their different +parts are no longer in the same relative position, +nevertheless we shall see that the impressions of +the sentient being remain the same as before; in +fact, though the mutual distances of the different +parts have varied, yet the parts which at first were +in contact are still in contact. It follows that +tactile impressions will be unchanged. On the +other hand, from the hypothesis as to refraction +and the curvature of the rays of light, visual impressions +will also be unchanged. These imaginary +beings will therefore be led to classify the phenomena +they observe, and to distinguish among them +the ``changes of position,'' which may be corrected +\PageSep{68} +by a voluntary correlative movement, just as we +do. + +If they construct a geometry, it will not be like +ours, which is the study of the movements of our +invariable solids; it will be the study of the +changes of position which they will have thus +distinguished, and will be ``non-Euclidean displacements,'' +and \emph{this will be non-Euclidean geometry}. +So that beings like ourselves, educated in +such a world, will not have the same geometry as +ours. + +\Par{The World of Four Dimensions.}---Just as we have +pictured to ourselves a non-Euclidean world, so we +may picture a world of four dimensions. + +The sense of light, even with one eye, together +with the muscular sensations relative to the movements +of the eyeball, will suffice to enable us to +conceive of space of three dimensions. The images +of external objects are painted on the retina, which +is a plane of two dimensions; these are \emph{perspectives}. +But as eye and objects are movable, we see in +succession different perspectives of the same body +taken from different points of view. We find at +the same time that the transition from one perspective +to another is often accompanied by +muscular sensations. If the transition from the +perspective~$A$ to the perspective~$B$, and that of the +perspective~$A'$ to the perspective~$B'$ are accompanied +by the same muscular sensations, we +connect them as we do other operations of the +same nature. Then when we study the laws +\PageSep{69} +according to which these operations are combined, +we see that they form a group, which has +the same structure as that of the movements of +invariable solids. Now, we have seen that it is +from the properties of this group that we derive +the idea of geometrical space and that of three +dimensions. We thus understand how these +perspectives gave rise to the conception of three +dimensions, although each perspective is of only +two dimensions,---because \emph{they succeed each other +according to certain laws}. Well, in the same way +that we draw the perspective of a three-dimensional +figure on a plane, so we can draw that of a +four-dimensional figure on a canvas of three (or +two) dimensions. To a geometer this is but child's +play. We can even draw several perspectives of +the same figure from several different points of +view. We can easily represent to ourselves these +perspectives, since they are of only three dimensions. +Imagine that the different perspectives of +one and the same object to occur in succession, +and that the transition from one to the other is +accompanied by muscular sensations. It is understood +that we shall consider two of these transitions +as two operations of the same nature when they +are associated with the same muscular sensations. +There is nothing, then, to prevent us from imagining +that these operations are combined according +to any law we choose---for instance, by forming +a group with the same structure as that of the +movements of an invariable four-dimensional solid. +\PageSep{70} +In this there is nothing that we cannot represent +to ourselves, and, moreover, these sensations are +those which a being would experience who has a +retina of two dimensions, and who may be displaced +in space of four dimensions. In this sense +we may say that we can represent to ourselves the +fourth dimension. + +\Par{Conclusions.}---It is seen that experiment plays a +considerable rôle in the genesis of geometry; but +it would be a mistake to conclude from that that +geometry is, even in part, an experimental science. +If it were experimental, it would only be approximative +and provisory. And what a rough +approximation it would be! Geometry would be +only the study of the movements of solid bodies; +but, in reality, it is not concerned with natural +solids: its object is certain ideal solids, absolutely +invariable, which are but a greatly simplified and +very remote image of them. The concept of these +ideal bodies is entirely mental, and experiment is +but the opportunity which enables us to reach the +idea. The object of geometry is the study of a +particular ``group''; but the general concept of +group pre-exists in our minds, at least potentially. +It is imposed on us not as a form of our sensitiveness, +but as a form of our understanding; only, +from among all possible groups, we must choose +one that will be the \emph{standard}, so to speak, to +which we shall refer natural phenomena. + +Experiment guides us in this choice, which it +does not impose on us. It tells us not what is the +\PageSep{71} +truest, but what is the most convenient geometry. +It will be noticed that my description of these +fantastic worlds has required no language other +than that of ordinary geometry. Then, were we +transported to those worlds, there would be no +need to change that language. Beings educated +there would no doubt find it more convenient to +create a geometry different from ours, and better +adapted to their impressions; but as for us, in the +presence of the same impressions, it is certain that +we should not find it more convenient to make a +change. +\PageSep{72} + + +\Chapter{V.}{Experiment and Geometry.} + +\ParSkip1. I have on several occasions in the preceding +pages tried to show how the principles of geometry +are not experimental facts, and that in particular +Euclid's postulate cannot be proved by experiment. +However convincing the reasons already given +may appear to me, I feel I must dwell upon them, +because there is a profoundly false conception +deeply rooted in many minds. + +2. Think of a material circle, measure its radius +and circumference, and see if the ratio of the two +lengths is equal to~$\pi$. What have we done? We +have made an experiment on the properties of the +matter with which this \emph{roundness} has been realised, +and of which the measure we used is made. + +\Par[3.\ ]{Geometry and Astronomy.}---The same question +may also be asked in another way. If Lobatschewsky's +geometry is true, the parallax of a very +distant star will be finite. If Riemann's is true, it +will be negative. These are the results which +seem within the reach of experiment, and it is +hoped that astronomical observations may enable +%[** TN: "...les trois géométries" in the French edition] +us to decide between the \Reword{two}{three} geometries. But +\PageSep{73} +what we call a straight line in astronomy is simply +the path of a ray of light. If, therefore, we were +to discover negative parallaxes, or to prove that all +parallaxes are higher than a certain limit, we +should have a choice between two conclusions: +we could give up Euclidean geometry, or modify +the laws of optics, and suppose that light is not +rigorously propagated in a straight line. It is +needless to add that every one would look upon +this solution as the more advantageous. Euclidean +geometry, therefore, has nothing to fear from fresh +experiments. + +4. Can we maintain that certain phenomena +which are possible in Euclidean space would be +impossible in non-Euclidean space, so that experiment +in establishing these phenomena would +directly contradict the non-Euclidean hypothesis? +I think that such a question cannot be seriously +asked. To me it is exactly equivalent to the following, +the absurdity of which is obvious:---There +are lengths which can be expressed in metres and +centimetres, but cannot be measured in toises, feet, +and inches; so that experiment, by ascertaining the +existence of these lengths, would directly contradict +this hypothesis, that there are toises divided +into six feet. Let us look at the question a little +more closely. I assume that the straight line in +Euclidean space possesses any two properties, +which I shall call $A$~and~$B$; that in non-Euclidean +space it still possesses the property~$A$, but no +longer possesses the property~$B$; and, finally, I +\PageSep{74} +assume that in both Euclidean and non-Euclidean +space the straight line is the only line that possesses +the property~$A$. If this were so, experiment +would be able to decide between the hypotheses of +Euclid and Lobatschewsky. It would be found +that some concrete object, upon which we can +experiment---for example, a pencil of rays of light---possesses +the property~$A$. We should conclude +that it is rectilinear, and we should then endeavour +to find out if it does, or does not, possess the property~$B$. +But \emph{it is not so}. There exists no +property which can, like this property~$A$, be an +absolute criterion enabling us to recognise the +straight line, and to distinguish it from every +other line. Shall we say, for instance, ``This property +will be the following: the straight line is a +line such that a figure of which this line is a part +can move without the mutual distances of its +points varying, and in such a way that all the +points in this straight line remain fixed''? Now, +this is a property which in either Euclidean or +non-Euclidean space belongs to the straight line, +and belongs to it alone. But how can we ascertain +by experiment if it belongs to any particular +concrete object? Distances must be measured, +and how shall we know that any concrete magnitude +which I have measured with my material +instrument really represents the abstract distance? +We have only removed the difficulty a little farther +off. In reality, the property that I have just +enunciated is not a property of the straight line +\PageSep{75} +alone; it is a property of the straight line and of +distance. For it to serve as an absolute criterion, +we must be able to show, not only that it does not +also belong to any other line than the straight line +and to distance, but also that it does not belong +to any other line than the straight line, and to any +other magnitude than distance. Now, that is not +true, and if we are not convinced by these considerations, +I challenge any one to give me a +concrete experiment which can be interpreted in +the Euclidean system, and which cannot be interpreted +in the system of Lobatschewsky. As I +am well aware that this challenge will never be +accepted, I may conclude that no experiment will +ever be in contradiction with Euclid's postulate; +but, on the other hand, no experiment will ever be +in contradiction with Lobatschewsky's postulate. + +5. But it is not sufficient that the Euclidean +(or non-Euclidean) geometry can ever be directly +contradicted by experiment. Nor could it happen +that it can only agree with experiment by a violation +of the principle of sufficient reason, and of +that of the relativity of space. Let me explain +myself. Consider any material system whatever. +We have to consider on the one hand the ``state'' +of the various bodies of this system---for example, +their temperature, their electric potential,~etc.; +and on the other hand their position in space. +And among the data which enable us to define +this position we distinguish the mutual distances +of these bodies that define their relative positions, +\PageSep{76} +and the conditions which define the absolute position +of the system and its absolute orientation in +space. The law of the phenomena which will be +produced in this system will depend on the state +of these bodies, and on their mutual distances; +but because of the relativity and the inertia of +space, they will not depend on the absolute position +and orientation of the system. In other +words, the state of the bodies and their mutual +distances at any moment will solely depend on +the state of the same bodies and on their mutual +distances at the initial moment, but will in no +way depend on the absolute initial position of +the system and of its absolute initial orientation. +This is what we shall call, for the sake of +abbreviation, \emph{the law of relativity}. + +So far I have spoken as a Euclidean geometer. +But I have said that an experiment, whatever it +may be, requires an interpretation on the Euclidean +hypothesis; it equally requires one on the non-Euclidean +hypothesis. Well, we have made a series +of experiments. We have interpreted them on the +Euclidean hypothesis, and we have recognised +that these experiments thus interpreted do not +violate this ``law of relativity.'' We now interpret +them on the non-Euclidean hypothesis. This is +always possible, only the non-Euclidean distances +of our different bodies in this new interpretation +will not generally be the same as the Euclidean +distances in the primitive interpretation. Will +our experiment interpreted in this new manner +\PageSep{77} +be still in agreement with our ``law of relativity,'' +and if this agreement had not taken place, would +we not still have the right to say that experiment +has proved the falsity of non-Euclidean geometry? +It is easy to see that this is an idle fear. In fact, +to apply the law of relativity in all its rigour, it +must be applied to the entire universe; for if we +were to consider only a part of the universe, and +if the absolute position of this part were to vary, +the distances of the other bodies of the universe +would equally vary; their influence on the part of +the universe considered might therefore increase +or diminish, and this might modify the laws of +the phenomena which take place in it. But if +our system is the entire universe, experiment is +powerless to give us any opinion on its position +and its absolute orientation in space. All that +our instruments, however perfect they may be, +can let us know will be the state of the different +parts of the universe, and their mutual distances. +Hence, our law of relativity may be enunciated as +follows:---The readings that we can make with our +instruments at any given moment will depend +only on the readings that we were able to make +on the same instruments at the initial moment. +Now such an enunciation is independent of all +interpretation by experiments. If the law is true +in the Euclidean interpretation, it will be also true +in the non-Euclidean interpretation. Allow me +to make a short digression on this point. I have +spoken above of the data which define the position +\PageSep{78} +of the different bodies of the system. I might also +have spoken of those which define their velocities. +I should then have to distinguish the velocity with +which the mutual distances of the different bodies +are changing, and on the other hand the velocities +of translation and rotation of the system; that is +to say, the velocities with which its absolute position +and orientation are changing. For the mind +to be fully satisfied, the law of relativity would +have to be enunciated as follows:---The state of +bodies and their mutual distances at any given +moment, as well as the velocities with which +those distances are changing at that moment, +will depend only on the state of those bodies, +on their mutual distances at the initial moment, +and on the velocities with which those distances +were changing at the initial moment. But they +will not depend on the absolute initial position +of the system nor on its absolute orientation, nor +on the velocities with which that absolute position +and orientation were changing at the initial +moment. Unfortunately, the law thus enunciated +does not agree with experiments---at least, as they +are ordinarily interpreted. Suppose a man were +translated to a planet, the sky of which was constantly +covered with a thick curtain of clouds, so +that he could never see the other stars. On that +planet he would live as if it were isolated in space. +But he would notice that it revolves, either by +measuring its ellipticity (which is ordinarily done +by means of astronomical observations, but which +\PageSep{79} +could be done by purely geodesic means), or by +repeating the experiment of Foucault's pendulum. +The absolute rotation of this planet might be +clearly shown in this way. Now, here is a fact +which shocks the philosopher, but which the +physicist is compelled to accept. We know that +from this fact Newton concluded the existence of +absolute space. I myself cannot accept this way +of looking at it. I shall explain why in Part~III., +but for the moment it is not my intention to +discuss this difficulty. I must therefore resign +myself, in the enunciation of the law of relativity, +to including velocities of every kind among the +data which define the state of the bodies. However +that may be, the difficulty is the same for +both Euclid's geometry and for Lobatschewsky's. +I need not therefore trouble about it further, and +I have only mentioned it incidentally. To sum +up, whichever way we look at it, it is impossible +to discover in geometric empiricism a rational +meaning. + +6. Experiments only teach us the relations of +bodies to one another. They do not and cannot +give us the relations of bodies and space, nor the +mutual relations of the different parts of space. +``Yes!'' you reply, ``a single experiment is not +enough, because it only gives us one equation with +several unknowns; but when I have made enough +experiments I shall have enough equations to +calculate all my unknowns.'' If I know the height +of the main-mast, that is not sufficient to enable +\PageSep{80} +me to calculate the age of the captain. When +you have measured every fragment of wood in a +ship you will have many equations, but you will +be no nearer knowing the captain's age. All your +measurements bearing on your fragments of wood +can tell you only what concerns those fragments; +and similarly, your experiments, however numerous +they may be, referring only to the relations of +bodies with one another, will tell you nothing +about the mutual relations of the different parts +of space. + +7. Will you say that if the experiments have +reference to the bodies, they at least have reference +to the geometrical properties of the bodies. First, +what do you understand by the geometrical properties +of bodies? I assume that it is a question +of the relations of the bodies to space. These +properties therefore are not reached by experiments +which only have reference to the relations +of bodies to one another, and that is enough to +show that it is not of those properties that there +can be a question. Let us therefore begin by +making ourselves clear as to the sense of the +phrase: geometrical properties of bodies. When +I say that a body is composed of several parts, I +presume that I am thus enunciating a geometrical +property, and that will be true even if I agree to +give the improper name of points to the very +small parts I am considering. When I say that +this or that part of a certain body is in contact +with this or that part of another body, I am +\PageSep{81} +enunciating a proposition which concerns the +mutual relations of the two bodies, and not their +relations with space. I assume that you will +agree with me that these are not geometrical +properties. I am sure that at least you will +grant that these properties are independent of +all knowledge of metrical geometry. Admitting +this, I suppose that we have a solid body formed +of eight thin iron rods, $oa$, $ob$, $oc$, $od$, $oe$, $of$, $og$, $oh$, +connected at one of their extremities,~$o$. And let +us take a second solid body---for example, a piece +of wood, on which are marked three little spots +of ink which I shall call $\alpha\ \beta\ \gamma$. I now suppose +that we find that we can bring into contact $\Chg{\alpha\ \beta\ \gamma}{\alpha\beta\gamma}$ +with~$ago$; by that I mean $\alpha$~with~$a$, and at the +same time $\beta$~with~$g$, and $\gamma$~with~$o$. Then we can +successively bring into contact $\alpha\beta\gamma$ with $bgo$, $cgo$, +$dgo$, $ego$, $fgo$, then with $aho$, $bho$, $cho$, $dho$, $eho$, $fho$; +and then $\alpha\gamma$ successively with $ab$, $bc$, $cd$, $de$, $ef$, $fa$. +Now these are observations that can be made +without having any idea beforehand as to the +form or the metrical properties of space. They +have no reference whatever to the ``geometrical +properties of bodies.'' These observations will +not be possible if the bodies on which we experiment +move in a group having the same structure +as the Lobatschewskian group (I mean according +to the same laws as solid bodies in Lobatschewsky's +geometry). They therefore suffice to prove that +these bodies move according to the Euclidean +group; or at least that they do not move according +\PageSep{82} +to the Lobatschewskian group. That they may +be compatible with the Euclidean group is easily +seen; for we might make them so if the body~$\alpha\beta\gamma$ +were an invariable solid of our ordinary +geometry in the shape of a right-angled triangle, +and if the points $abcdefgh$ were the vertices of +a polyhedron formed of two regular hexagonal +pyramids of our ordinary geometry having $abcdef$ +as their common base, and having the one~$g$ and +the other~$h$ as their vertices. Suppose now, +instead of the previous observations, we note that +we can as before apply~$\alpha\beta\gamma$ successively to~$ago$, +$bgo$, $cgo$, $dgo$, $ego$, $fgo$, $aho$, $bho$, $cho$, $dho$, $eho$, $fho$, +and then that we can apply~$\alpha\beta$ (and no longer~$\alpha\gamma$) +successively to~$ab$, $bc$, $cd$, $de$, $ef$, and~$fa$. These are +observations that could be made if non-Euclidean +geometry were true. If the bodies~$\alpha\beta\gamma$, $oabcdefgh$ +were invariable solids, if the former were a right-angled +triangle, and the latter a double regular +hexagonal pyramid of suitable dimensions. These +new verifications are therefore impossible if the +bodies move according to the Euclidean group; +but they become possible if we suppose the bodies +to move according to the Lobatschewskian group. +They would therefore suffice to show, if we carried +them out, that the bodies in question do not move +according to the Euclidean group. And so, without +making any hypothesis on the form and the +nature of space, on the relations of the bodies +and space, and without attributing to bodies any +geometrical property, I have made observations +\PageSep{83} +which have enabled me to show in one case that +the bodies experimented upon move according to +a group, the structure of which is Euclidean, and +in the other case, that they move in a group, the +structure of which is Lobatschewskian. It cannot +be said that all the first observations would +constitute an experiment proving that space is +Euclidean, and the second an experiment proving +that space is non-Euclidean; in fact, it might be +imagined (note that I use the word \emph{imagined}) that +there are bodies moving in such a manner as +to render possible the second series of observations: +and the proof is that the first mechanic who came +our way could construct it if he would only take +the trouble. But you must not conclude, however, +that space is non-Euclidean. In the same way, +just as ordinary solid bodies would continue +to exist when the mechanic had constructed the +strange bodies I have just mentioned, he would +have to conclude that space is both Euclidean +and non-Euclidean. Suppose, for instance, that +we have a large sphere of radius~$R$, and that its +temperature decreases from the centre to the +surface of the sphere according to the law of +which I spoke when I was describing the non-Euclidean +world. We might have bodies whose +dilatation is \Typo{negligeable}{negligible}, and which would behave +as ordinary invariable solids; and, on the other +hand, we might have very dilatable bodies, which +would behave as non-Euclidean solids. We +might have two double pyramids~$oabcdefgh$ and +\PageSep{84} +$o'a'b'c'd'e'f'g'h'$, and two triangles $\alpha\beta\gamma$~and~$\alpha'\beta'\gamma'$. +The first double pyramid would be rectilinear, and +the second curvilinear. The triangle~$\alpha\beta\gamma$ would +consist of undilatable matter, and the other of very +dilatable matter. We might therefore make our +first observations with the double pyramid~$o'a'h'$ +and the triangle~$\alpha'\beta'\gamma'$. + +And then the experiment would seem to show---first, +that Euclidean geometry is true, and then +that it is false. Hence, \emph{experiments have reference +not to space but to bodies}. + +\Subsection{Supplement.} + +\ParSkip8. To round the matter off, I ought to speak of +a very delicate question, which will require considerable +development; but I shall confine myself +to summing up what I have written in the \Title{Revue +de Métaphysique et de Morale} and in the \Title{Monist}. +When we say that space has three dimensions, +what do we mean? We have seen the importance +of these ``internal changes'' which are revealed to +us by our muscular sensations. They may serve +to characterise the different attitudes of our body. +Let us take arbitrarily as our origin one of these +attitudes,~$A$. When we pass from this initial +attitude to another attitude~$B$ we experience a +series of muscular sensations, and this series~$S$ of +muscular sensations will define~$B$. Observe, however, +that we shall often look upon two series $S$~and~$S'$ +as defining the same attitude~$B$ (since the +\PageSep{85} +initial and final attitudes $A$~and~$B$ remaining the +same, the intermediary attitudes of the corresponding +sensations may differ). How then can +we recognise the equivalence of these two series? +Because they may serve to compensate for the same +external change, or more generally, because, when +it is a question of compensation for an external +change, one of the series may be replaced by the +other. Among these series we have distinguished +those which can alone compensate for an external +change, and which we have called ``displacements.'' +As we cannot distinguish two displacements which +are very close together, the aggregate of these +displacements presents the characteristics of a +physical continuum. Experience teaches us that +they are the characteristics of a physical continuum +of six dimensions; but we do not know as +yet how many dimensions space itself possesses, so +we must first of all answer another question. +What is a point in space? Every one thinks he +knows, but that is an illusion. What we see when +we try to represent to ourselves a point in space is +a black spot on white paper, a spot of chalk on +a blackboard, always an object. The question +should therefore be understood as follows:---What +do I mean when I say the object~$B$ is at the +point which a moment before was occupied by the +object~$A$? Again, what criterion will enable +me to recognise it? I mean that \emph{although I have +not moved} (my muscular sense tells me this), my +finger, which just now touched the object~$A$, is +\PageSep{86} +now touching the object~$B$. I might have used +other criteria---for instance, another finger or the +sense of sight---but the first criterion is sufficient. +I know that if it answers in the affirmative all +other criteria will give the same answer. I know +it from experiment. I cannot know it \Foreign{à ~priori}. +For the same reason I say that touch cannot +be exercised at a distance; that is another way of +enunciating the same experimental fact. If I +say, on the contrary, that sight is exercised at a +distance, it means that the criterion furnished by +sight may give an affirmative answer while the +others reply in the negative. + +To sum up. For each attitude of my body my +finger determines a point, and it is that and that +only which defines a point in space. To each +attitude corresponds in this way a point. But it +often happens that the same point corresponds to +several different attitudes (in this case we say that +our finger has not moved, but the rest of our body +has). We distinguish, therefore, among changes +of attitude those in which the finger does not +move. How are we led to this? It is because we +often remark that in these changes the object +which is in touch with the finger remains in contact +with it. Let us arrange then in the same +class all the attitudes which are deduced one from +the other by one of the changes that we have thus +distinguished. To all these attitudes of the same +class will correspond the same point in space. +Then to each class will correspond a point, and to +\PageSep{87} +each point a class. Yet it may be said that what +we get from this experiment is not the point, but +the class of changes, or, better still, the corresponding +class of muscular sensations. Thus, when +we say that space has three dimensions, we merely +mean that the aggregate of these classes appears to +us with the characteristics of a physical continuum +of three dimensions. Then if, instead of defining +the points in space with the aid of the first finger, +I use, for example, another finger, would the +results be the same? That is by no means \Foreign{à ~priori} +evident. But, as we have seen, experiment +has shown us that all our criteria are in agreement, +and this enables us to answer in the +affirmative. If we recur to what we have called +displacements, the aggregate of which forms, as +we have seen, a group, we shall be brought to +distinguish those in which a finger does not move; +and by what has preceded, those are the displacements +which characterise a point in space, and +their aggregate will form a sub-group of our +group. To each sub-group of this kind, then, will +correspond a point in space. We might be +tempted to conclude that experiment has taught +us the number of dimensions of space; but in +reality our experiments have referred not to space, +but to our body and its relations with neighbouring +objects. What is more, our experiments +are exceeding crude. In our mind the latent idea +of a certain number of groups pre-existed; these +are the groups with which Lie's theory is concerned. +\PageSep{88} +Which shall we choose to form a kind of +standard by which to compare natural phenomena? +And when this group is chosen, which +of the sub-groups shall we take to characterise a +point in space? Experiment has guided us by +showing us what choice adapts itself best to the +properties of our body; but there its rôle ends. +\PageSep{89} + + +\Part{III.}{Force.} + +\Chapter{VI.}{The Classical Mechanics.} + +\First{The} English teach mechanics as an experimental +science; on the Continent it is taught always more +or less as a deductive and \Foreign{à ~priori} science. The +English are right, no doubt. How is it that the +other method has been persisted in for so long; how +is it that Continental scientists who have tried to +escape from the practice of their predecessors have +in most cases been unsuccessful? On the other +hand, if the principles of mechanics are only of +experimental origin, are they not merely approximate +and provisory? May we not be some day +compelled by new experiments to modify or even +to abandon them? These are the questions which +naturally arise, and the difficulty of solution is +largely due to the fact that treatises on mechanics +do not clearly distinguish between what is experiment, +what is mathematical reasoning, what is +convention, and what is hypothesis. This is not +all. +\PageSep{90} + +1. There is no absolute space, and we only +conceive of relative motion; and yet in most cases +mechanical facts are enunciated as if there is an +absolute space to which they can be referred. + +2. There is no absolute time. When we say that +two periods are equal, the statement has no +meaning, and can only acquire a meaning by a +convention. + +3. Not only have we no direct intuition of the +equality of two periods, but we have not even +direct intuition of the simultaneity of two events +occurring in two different places. I have explained +this in an article entitled ``Mesure du +Temps.''\footnote + {\Title{Revue de Métaphysique et de Morale}, t.~vi., pp.~1--13, January, + 1898.} + +4. Finally, is not our Euclidean geometry in +itself only a kind of convention of language? +Mechanical facts might be enunciated with reference +to a non-Euclidean space which would be +less convenient but quite as legitimate as our +ordinary space; the enunciation would become +more complicated, but it still would be possible. + +Thus, absolute space, absolute time, and even +geometry are not conditions which are imposed on +mechanics. All these things no more existed +before mechanics than the French language can +be logically said to have existed before the truths +which are expressed in French. We might +endeavour to enunciate the fundamental law of +mechanics in a language independent of all these +\PageSep{91} +conventions; and no doubt we should in this way +get a clearer idea of those laws in themselves. +This is what M.~Andrade has tried to do, to +some extent at any rate, in his \Title{Leçons de Mécanique +physique}. Of course the enunciation of these laws +would become much more complicated, because all +these conventions have been adopted for the very +purpose of abbreviating and simplifying the enunciation. +As far as we are concerned, I shall ignore +all these difficulties; not because I disregard +them, far from it; but because they have received +sufficient attention in the first two parts, +of the book. Provisionally, then, we shall admit +absolute time and Euclidean geometry. + +\Par{The Principle of Inertia.}---A body under the +action of no force can only move uniformly in a +straight line. Is this a truth imposed on the mind +\Foreign{à ~priori}? If this be so, how is it that the Greeks +ignored it? How could they have believed that +motion ceases with the cause of motion? or, again, +that every body, if there is nothing to prevent it, +will move in a circle, the noblest of all forms of +motion? + +If it be said that the velocity of a body cannot +change, if there is no reason for it to change, may +we not just as legitimately maintain that the +position of a body cannot change, or that the +curvature of its path cannot change, without the +agency of an external cause? Is, then, the principle +of inertia, which is not an \Foreign{à ~priori} truth, an +experimental fact? Have there ever been experiments +\PageSep{92} +on bodies acted on by no forces? and, if so, +how did we know that no forces were acting? +The usual instance is that of a ball rolling for a +very long time on a marble table; but why do +we say it is under the action of no force? Is it +because it is too remote from all other bodies to +experience any sensible action? It is not further +from the earth than if it were thrown freely into +the air; and we all know that in that case it +would be subject to the attraction of the earth. +Teachers of mechanics usually pass rapidly over +the example of the ball, but they add that the +principle of inertia is verified indirectly by its consequences. +This is very badly expressed; they +evidently mean that various consequences may be +verified by a more general principle, of which the +principle of inertia is only a particular case. I +shall propose for this general principle the +following enunciation:---The acceleration of a +body depends only on its position and that of +neighbouring bodies, and on their velocities. +Mathematicians would say that the movements +of all the material molecules of the universe +depend on differential equations of the second +order. To make it clear that this is really a +generalisation of the law of inertia we may again +have recourse to our imagination. The law of +inertia, as I have said above, is not imposed on us +\Foreign{à ~priori}; other laws would be just as compatible +with the principle of sufficient reason. If a body +is not acted upon by a force, instead of supposing +\PageSep{93} +that its velocity is unchanged we may suppose +that its position or its acceleration is unchanged. + +Let us for a moment suppose that one of these +two laws is a law of nature, and substitute it for +the law of inertia: what will be the natural +generalisation? A moment's reflection will show +us. In the first case, we may suppose that the +velocity of a body depends only on its position and +that of neighbouring bodies; in the second case, +that the variation of the acceleration of a body +depends only on the position of the body and of +neighbouring bodies, on their velocities and +accelerations; or, in mathematical terms, the +differential equations of the motion would be of +the first order in the first case and of the third +order in the second. + +Let us now modify our supposition a little. +Suppose a world analogous to our solar system, +but one in which by a singular chance the orbits +of all the planets have neither eccentricity nor +inclination; and further, I suppose that the +masses of the planets are too small for their +mutual perturbations to be sensible. Astronomers +living in one of these planets would not hesitate to +conclude that the orbit of a star can only be +circular and parallel to a certain plane; the +position of a star at a given moment would then +be sufficient to determine its velocity and path. +The law of inertia which they would adopt would +be the former of the two hypothetical laws I have +mentioned. +\PageSep{94} + +Now, imagine this system to be some day +crossed by a body of vast mass and immense +velocity coming from distant constellations. All +the orbits would be profoundly disturbed. Our +astronomers would not be greatly astonished. +They would guess that this new star is in itself +quite capable of doing all the mischief; but, they +would say, as soon as it has passed by, order will +again be established. No doubt the distances of +the planets from the sun will not be the same as +before the cataclysm, but the orbits will become +circular again as soon as the disturbing cause has +disappeared. It would be only when the perturbing +body is remote, and when the orbits, instead of +being circular are found to be elliptical, that the +astronomers would find out their mistake, and +discover the necessity of reconstructing their +mechanics. + +I have dwelt on these hypotheses, for it seems to +me that we can clearly understand our generalised +law of inertia only by opposing it to a contrary +hypothesis. + +Has this generalised law of inertia been verified +by experiment, and can it be so verified? +When Newton wrote the \Title{Principia}, he certainly +regarded this truth as experimentally acquired and +demonstrated. It was so in his eyes, not only +from the anthropomorphic conception to which I +shall later refer, but also because of the work of +Galileo. It was so proved by the laws of Kepler. +According to those laws, in fact, the path of a +\PageSep{95} +planet is entirely determined by its initial position +and initial velocity; this, indeed, is what our +generalised law of inertia requires. + +For this principle to be only true in appearance---lest +we should fear that some day it must be replaced +by one of the analogous principles which I +opposed to it just now---we must have been led +astray by some amazing chance such as that which +had led into error our imaginary astronomers. +Such an hypothesis is so unlikely that it need not +delay us. No one will believe that there can be +such chances; no doubt the probability that two +eccentricities are both exactly zero is not smaller +than the probability that one is~$0.1$ and the other~$0.2$. +The probability of a simple event is not +smaller than that of a complex one. If, however, +the former does occur, we shall not attribute its +occurrence to chance; we shall not be inclined to +believe that nature has done it deliberately to +deceive us. The hypothesis of an error of this +kind being discarded, we may admit that so far as +astronomy is concerned our law has been verified +by experiment. + +But Astronomy is not the whole of Physics. +May we not fear that some day a new experiment +will falsify the law in some domain of +physics? An experimental law is always subject +to revision; we may always expect to see it replaced +by some other and more exact law. But +no one seriously thinks that the law of which we +speak will ever be abandoned or amended. Why? +\PageSep{96} +Precisely because it will never be submitted to a +decisive test. + +In the first place, for this test to be complete, +all the bodies of the universe must return with +their initial velocities to their initial positions after +a certain time. We ought then to find that they +would resume their original paths. But this test +is impossible; it can be only partially applied, and +even when it is applied there will still be some +bodies which will not return to their original +positions. Thus there will be a ready explanation +of any breaking down of the law. + +Yet this is not all. In Astronomy we \emph{see} the +bodies whose motion we are studying, and in most +cases we grant that they are not subject to the +action of other invisible bodies. Under these conditions, +our law must certainly be either verified or +not. But it is not so in Physics. If physical +phenomena are due to motion, it is to the motion +of molecules which we cannot see. If, then, the +acceleration of bodies we cannot see depends on +something else than the positions or velocities of +other visible bodies or of invisible molecules, the +existence of which we have been led previously +to admit, there is nothing to prevent us from +supposing that this something else is the position +or velocity of other molecules of which we have +not so far suspected the existence. The law +will be safeguarded. Let me express the same +thought in another form in mathematical language. +Suppose we are observing $n$~molecules, and find +\PageSep{97} +that their $3n$~co-ordinates satisfy a system of $3n$~differential +equations of the fourth order (and +not of the second, as required by the law of +inertia). We know that by introducing $3n$~variable +auxiliaries, a system of $3n$~equations of the fourth +order may be reduced to a system of $6n$~equations +of the second order. If, then, we suppose that the +$3n$~auxiliary variables represent the co-ordinates of +$n$~invisible molecules, the result is again conformable +to the law of inertia. To sum up, this law, +verified experimentally in some particular cases, +may be extended fearlessly to the most general +cases; for we know that in these general cases +it can neither be confirmed nor contradicted by +experiment. + +\Par{The Law of Acceleration.}---The acceleration of a +body is equal to the force which acts on it divided +by its mass. + +Can this law be verified by experiment? If so, +we have to measure the three magnitudes mentioned +in the enunciation: acceleration, force, +and mass. I admit that acceleration may be +measured, because I pass over the difficulty +arising from the measurement of time. But how +are we to measure force and mass? We do not +even know what they are. What is mass? +Newton replies: ``The product of the volume and +the density.'' ``It were better to say,'' answer +Thomson and Tait, ``that density is the quotient +of the mass by the volume.'' What is force? +``It is,'' replies Lagrange, ``that which moves or +\PageSep{98} +tends to move a body.'' ``It is,'' according to +Kirchoff, ``the product of the mass and the +acceleration.'' Then why not say that mass is +the quotient of the force by the acceleration? +These difficulties are insurmountable. + +When we say force is the cause of motion, we +are talking metaphysics; and this definition, if we +had to be content with it, would be absolutely +fruitless, would lead to absolutely nothing. For a +definition to be of any use it must tell us how to +measure force; and that is quite sufficient, for it is +by no means necessary to tell what force is in +itself, nor whether it is the cause or the effect of +motion. We must therefore first define what is +meant by the equality of two forces. When are +two forces equal? We are told that it is when +they give the same acceleration to the same mass, +or when acting in opposite directions they are in +equilibrium. This definition is a sham. A force +applied to a body cannot be uncoupled and +applied to another body as an engine is uncoupled +from one train and coupled to another. It is +therefore impossible to say what acceleration such +a force, applied to such a body, would give to +another body if it were applied to it. It is impossible +to tell how two forces which are not +acting in exactly opposite directions would behave +if they were acting in opposite directions. +It is this definition which we try to materialise, as +it were, when we measure a force with a dynamometer +or with a balance. Two forces, $F$~and~$F'$, +\PageSep{99} +which I suppose, for simplicity, to be acting +vertically upwards, are respectively applied to two +bodies, $C$~and~$C'$. I attach a body weighing~$P$ +first to~$C$ and then to~$C'$; if there is equilibrium in +both cases I conclude that the two forces $F$~and~$F'$ +are equal, for they are both equal to the weight +of the body~$P$. But am I certain that the body~$P$ +has kept its weight when I transferred it from the +first body to the second? Far from it. I am +certain of the contrary. I know that the magnitude +of the weight varies from one point to +another, and that it is greater, for instance, at the +pole than at the equator. No doubt the difference +is very small, and we neglect it in practice; but a +definition must have mathematical rigour; this +rigour does not exist. What I say of weight +would apply equally to the force of the spring of +a dynamometer, which would vary according to +temperature and many other circumstances. Nor +is this all. We cannot say that the weight of the +body~$P$ is applied to the body~$C$ and keeps in +equilibrium the force~$F$. What is applied to +the body~$C$ is the action of the body~$P$ on the +body~$C$. On the other hand, the body~$P$ is +acted on by its weight, and by the reaction~$R$ +of the body~$C$ on~$P$ the forces $F$~and~$A$ are +equal, because they are in equilibrium; the forces +$A$~and~$R$ are equal by virtue of the principle +of action and reaction; and finally, the force~$R$ +and the weight~$P$ are equal because they +are in equilibrium. From these three equalities +\PageSep{100} +we deduce the equality of the weight~$P$ and the +force~$F$. + +Thus we are compelled to bring into our definition +of the equality of two forces the principle +of the equality of action and reaction; \emph{hence this +principle can no longer be regarded as an experimental +law but only as a definition}. + +To recognise the equality of two forces we are +then in possession of two rules: the equality of +two forces in equilibrium and the equality of action +and reaction. But, as we have seen, these are not +sufficient, and we are compelled to have recourse +to a third rule, and to admit that certain forces---the +weight of a body, for instance---are constant in +magnitude and direction. But this third rule is +an experimental law. It is only approximately +true: \emph{it is a bad definition}. We are therefore +reduced to Kirchoff's definition: force is the product +of the mass and the acceleration. This law +of Newton in its turn ceases to be regarded as an +experimental law, it is now only a definition. But +as a definition it is insufficient, for we do not +know what mass is. It enables us, no doubt, to +calculate the ratio of two forces applied at +different times to the same body, but it tells us +nothing about the ratio of two forces applied to +two different bodies. To fill up the gap we must +have recourse to Newton's third law, the equality +of action and reaction, still regarded not as +an experimental law but as a definition. Two +bodies, $A$~and~$B$, act on each other; the acceleration +\PageSep{101} +of~$A$, multiplied by the mass of~$A$, is equal to +the action of~$B$ on~$A$; in the same way the +acceleration of~$B$, multiplied by the mass of~$B$ is +equal to the reaction of~$A$ on~$B$. As, by definition, +the action and the reaction are equal, the masses +of $A$~and~$B$ arc respectively in the inverse ratio of +their masses. Thus is the ratio of the two masses +defined, and it is for experiment to verify that the +ratio is constant. + +This would do very well if the two bodies were +alone and could be abstracted from the action of +the rest of the world; but this is by no means +the case. The acceleration of~$A$ is not solely due +to the action of~$B$, but to that of a multitude of +other bodies, $C$,~$D$,~\ldots. To apply the preceding +rule we must decompose the acceleration of~$A$ into +many components, and find out which of these +components is due to the action of~$B$. The +decomposition would still be possible if we +suppose that the action of~$C$ on~$A$ is simply added +to that of~$B$ on~$A$, and that the presence of the +body~$C$ does not in any way modify the action of~$B$ +on~$A$, or that the presence of~$B$ does not modify +the action of~$C$ on~$A$; that is, if we admit that +any two bodies attract each other, that their +mutual action is along their join, and is only dependent +on their distance apart; if, in a word, we +admit the \emph{hypothesis of central forces}. + +We know that to determine the masses of the +heavenly bodies we adopt quite a different principle. +The law of gravitation teaches us that the +\PageSep{102} +attraction of two bodies is proportional to their +masses; if $r$~is their distance apart, $m$~and~$m'$ their +masses, $k$~a constant, then their attraction will be~$kmm'/r^{2}$. +What we are measuring is therefore not +mass, the ratio of the force to the acceleration, but +the attracting mass; not the inertia of the body, +but its attracting power. It is an indirect process, +the use of which is not indispensable theoretically. +We might have said that the attraction is inversely +proportional to the square of the distance, +without being proportional to the product of the +%[** TN: "mais sans que l'on eût f = kmm'"] +masses, that it is equal to~$f/r^{2}$ \Reword{and not to~$kmm'$}{but without having $f = kmm'$}. +If it were so, we should nevertheless, by observing +the \emph{relative} motion of the celestial bodies, be able +to calculate the masses of these bodies. + +But have we any right to admit the hypothesis +of central forces? Is this hypothesis rigorously +accurate? Is it certain that it will never be +falsified by experiment? Who will venture to +make such an assertion? And if we must abandon +this hypothesis, the building which has been so +laboriously erected must fall to the ground. + +We have no longer any right to speak of the +component of the acceleration of~$A$ which is +due to the action of~$B$. We have no means of +distinguishing it from that which is due to the +action of~$C$ or of any other body. The rule +becomes inapplicable in the measurement of +masses. What then is left of the principle of +the equality of action and reaction? If we +reject the hypothesis of central forces this principle +\PageSep{103} +must go too; the geometrical resultant of +all the forces applied to the different bodies of a +system abstracted from all external action will be +zero. In other words, \emph{the motion of the centre of +gravity of this system will be uniform and in a +straight line}. Here would seem to be a means of +defining mass. The position of the centre of +gravity evidently depends on the values given to +the masses; we must select these values so that +the motion of the centre of gravity is uniform +and rectilinear. This will always be possible if +Newton's third law holds good, and it will be in +general possible only in one way. But no system +exists which is abstracted from all external action; +every part of the universe is subject, more or less, +to the action of the other parts. \emph{The law of the +motion of the centre of gravity is only rigorously true +when applied to the whole universe.} + +But then, to obtain the values of the masses +we must find the motion of the centre of gravity +of the universe. The absurdity of this conclusion +is obvious; the motion of the centre of gravity +of the universe will be for ever to us unknown. +Nothing, therefore, is left, and our efforts are +fruitless. There is no escape from the following +definition, which is only a confession of failure: +\emph{Masses are co-efficients which it is found convenient to +introduce into calculations.} + +We could reconstruct our mechanics by giving +to our masses different values. The new mechanics +would be in contradiction neither with +\PageSep{104} +experiment nor with the general principles of +dynamics (the principle of inertia, proportionality +of masses and accelerations, equality of +action and reaction, uniform motion of the centre +of gravity in a straight line, and areas). But the +equations of this mechanics \emph{would not be so simple}. +Let us clearly understand this. It would be only +the first terms which would be less simple---\ie, +those we already know through experiment; +perhaps the small masses could be slightly altered +without the \emph{complete} equations gaining or losing +in simplicity. + +Hertz has inquired if the principles of mechanics +are rigorously true. ``In the opinion of many +physicists it seems inconceivable that experiment +will ever alter the impregnable principles of +mechanics; and yet, what is due to experiment +may always be rectified by experiment.'' From +what we have just seen these fears would appear +to be groundless. The principles of dynamics +appeared to us first as experimental truths, but +we have been compelled to use them as definitions. +It is \emph{by definition} that force is equal to +the product of the mass and the acceleration; +this is a principle which is henceforth beyond +the reach of any future experiment. Thus +it is by definition that action and reaction are +equal and opposite. But then it will be said, +these unverifiable principles are absolutely devoid +of any significance. They cannot be disproved by +experiment, but we can learn from them nothing +\PageSep{105} +of any use to us; what then is the use of studying +dynamics? This somewhat rapid condemnation +would be rather unfair. There is not in Nature any +system \emph{perfectly} isolated, perfectly abstracted from +all external action; but there are systems which +are \emph{nearly} isolated. If we observe such a system, +we can study not only the relative motion of its +different parts with respect to each other, but the +motion of its centre of gravity with respect to the +other parts of the universe. We then find that +the motion of its centre of gravity is \emph{nearly} uniform +and rectilinear in conformity with Newton's Third +Law. This is an experimental fact, which cannot +be invalidated by a more accurate experiment. +What, in fact, would a more accurate experiment +teach us? It would teach us that the law is only +approximately true, and we know that already. +\emph{Thus is explained how experiment may serve as a basis +for the principles of mechanics, and yet will never +invalidate them.} + +\Par{Anthropomorphic Mechanics.}---It will be said that +Kirchoff has only followed the general tendency of +mathematicians towards nominalism; from this his +skill as a physicist has not saved him. He wanted +a definition of a force, and he took the first that +came handy; but we do not require a definition +of force; the idea of force is primitive, irreducible, +indefinable; we all know what it is; of it we have +direct intuition. This direct intuition arises from +the idea of effort which is familiar to us from +childhood. But in the first place, even if this +\PageSep{106} +direct intuition made known to us the real nature +of force in itself, it would prove to be an insufficient +basis for mechanics; it would, moreover, be quite +useless. The important thing is not to know +what force is, but how to measure it. Everything +which does not teach us how to measure it is as +useless to the mechanician as, for instance, the +subjective idea of heat and cold to the student of +heat. This subjective idea cannot be translated +into numbers, and is therefore useless; a scientist +whose skin is an absolutely bad conductor of heat, +and who, therefore, has never felt the sensation +of heat or cold, would read a thermometer in just +the same way as any one else, and would have +enough material to construct the whole of the +theory of heat. + +Now this immediate notion of effort is of no use +to us in the measurement of force. It is clear, for +example, that I shall experience more fatigue in +lifting a weight of $100$~lb.\ than a man who is +accustomed to lifting heavy burdens. But there +is more than this. This notion of effort does not +teach us the nature of force; it is definitively reduced +to a recollection of muscular sensations, and +no one will maintain that the sun experiences +a muscular sensation when it attracts the earth. +All that we can expect to find from it is a symbol, +less precise and less convenient than the arrows +(to denote direction) used by geometers, and quite +as remote from reality. + +Anthropomorphism plays a considerable historic +\PageSep{107} +rôle in the genesis of mechanics; perhaps it may +yet furnish us with a symbol which some minds +may find convenient; but it can be the foundation +of nothing of a really scientific or philosophical +character. + +\Par{The Thread School.}---M.~Andrade, in his \Title{Leçons +de \Typo{Mecanique}{Mécanique} physique}, has modernised anthropomorphic +mechanics. To the school of mechanics +with which Kirchoff is identified, he opposes a +school which is quaintly called the ``Thread +School.'' + +This school tries to reduce everything to the consideration +of certain material systems of negligible +mass, regarded in a state of tension and capable +of transmitting considerable effort to distant +bodies---systems of which the ideal type is the +fine string, wire, or \emph{thread}. A thread which +transmits any force is slightly lengthened in the +direction of that force; the direction of the thread +tells us the direction of the force, and the magnitude +of the force is measured by the lengthening of +the thread. + +%[** TN: "A" variously italicized and not in the original] +{\Loosen We may imagine such an experiment as the +following:}---A body~$A$ is attached to a thread; +at the other extremity of the thread acts a force +which is made to vary until the length of the +thread is increased by~$\alpha$, and the acceleration +of the body~$A$ is recorded. $A$~is then detached, +and a body~$B$ is attached to the same thread, and +the same or another force is made to act until +the increment of length again is~$\alpha$, and the +\PageSep{108} +acceleration of~$B$ is noted. The experiment is +then renewed with both $A$~and~$B$ until the increment +of length is~$\beta$. The four accelerations +observed should be proportional. Here we have +an experimental verification of the law of acceleration +enunciated above. Again, we may consider +a body under the action of several threads in +equal tension, and by experiment we determine +the direction of those threads when the body +is in equilibrium. This is an experimental +verification of the law of the composition of +forces. But, as a matter of fact, what have we +done? We have defined the force acting on the +string by the deformation of the thread, which is +reasonable enough; we have then assumed that if +a body is attached to this thread, the effort which +is transmitted to it by the thread is equal to the +action exercised by the body on the thread; in +fact, we have used the principle of action and +reaction by considering it, not as an experimental +truth, but as the very definition of force. This +definition is quite as conventional as that of +Kirchoff, but it is much less general. + +All the forces are not transmitted by the thread +(and to compare them they would all have to be +transmitted by identical threads). If we even +admitted that the earth is attached to the sun by +an invisible thread, at any rate it will be agreed +that we have no means of measuring the increment +of the thread. Nine times out of ten, in consequence, +our definition will be in default; no +\PageSep{109} +sense of any kind can be attached to it, and we +must fall back on that of Kirchoff. Why then go +on in this roundabout way? You admit a certain +definition of force which has a meaning only in +certain particular cases. In those cases you verify +by experiment that it leads to the law of acceleration. +On the strength of these experiments you +then take the law of acceleration as a definition of +force in all the other cases. + +Would it not be simpler to consider the law of +acceleration as a definition in all cases, and to +regard the experiments in question, not as verifications +of that law, but as verifications of the +principle of action and reaction, or as proving +the deformations of an elastic body depend only +on the forces acting on that body? Without +taking into account the fact that the conditions +in which your definition could be accepted can +only be very imperfectly fulfilled, that a thread is +never without mass, that it is never isolated from +all other forces than the reaction of the bodies +attached to its extremities. + +The ideas expounded by M.~Andrade are none +the less very interesting. If they do not satisfy our +logical requirements, they give us a better view of +the historical genesis of the fundamental ideas of +mechanics. The reflections they suggest show us +how the human mind passed from a naïve +anthropomorphism to the present conception of +science. + +We see that we end with an experiment which +\PageSep{110} +is very particular, and as a matter of fact very +crude, and we start with a perfectly general law, +perfectly precise, the truth of which we regard as +absolute. We have, so to speak, freely conferred +this certainty on it by looking upon it as a convention. + +Are the laws of acceleration and of the composition +of forces only arbitrary conventions? +Conventions, yes; arbitrary, no---they would be +so if we lost sight of the experiments which led the +founders of the science to adopt them, and which, +imperfect as they were, were sufficient to justify +their adoption. It is well from time to time to let +our attention dwell on the experimental origin of +these conventions. +\PageSep{111} + + +\Chapter{VII.}{Relative and Absolute Motion.} + +\Par{The Principle of Relative Motion.}---Sometimes +endeavours have been made to connect the law of +acceleration with a more general principle. The +movement of any system whatever ought to +obey the same laws, whether it is referred to fixed +axes or to the movable axes which are implied +in uniform motion in a straight line. This is +the principle of relative motion; it is imposed +upon us for two reasons: the commonest experiment +confirms it; the consideration of the contrary +hypothesis is singularly repugnant to the mind. + +Let us admit it then, and consider a body under +the action of a force. The relative motion of this +body with respect to an observer moving with a +uniform velocity equal to the initial velocity of the +body, should be identical with what would be its +absolute motion if it started from rest. We conclude +that its acceleration must not depend upon +its absolute velocity, and from that we attempt to +deduce the complete law of acceleration. + +For a long time there have been traces of this +proof in the regulations for the degree of B.~ès~Sc. +\PageSep{112} +It is clear that the attempt has failed. The +obstacle which prevented us from proving the +law of acceleration is that we have no definition +of force. This obstacle subsists in its entirety, +since the principle invoked has not furnished us +with the missing definition. The principle of +relative motion is none the less very interesting, +and deserves to be considered for its own sake. +Let us try to enunciate it in an accurate manner. +We have said above that the accelerations of the +different bodies which form part of an isolated +system only depend on their velocities and their +relative positions, and not on their velocities and +their absolute positions, provided that the movable +axes to which the relative motion is referred +move uniformly in a straight line; or, if it is preferred, +their accelerations depend only on the +differences of their velocities and the differences of +their co-ordinates, and not on the absolute values +of these velocities and co-ordinates. If this principle +is true for relative accelerations, or rather +for differences of acceleration, by combining it +with the law of reaction we shall deduce that it is +true for absolute accelerations. It remains to be +seen how we can prove that differences of acceleration +depend only on differences of velocities +and co-ordinates; or, to speak in mathematical +language, that these differences of co-ordinates +satisfy differential equations of the second order. +Can this proof be deduced from experiment or +from \Foreign{à ~priori} conditions? Remembering what we +\PageSep{113} +have said before, the reader will give his own +answer. Thus enunciated, in fact, the principle of +relative motion curiously resembles what I called +above the generalised principle of inertia; it is not +quite the same thing, since it is a question of +differences of co-ordinates, and not of the co-ordinates +themselves. The new principle teaches +us something more than the old, but the same +discussion applies to it, and would lead to the +same conclusions. We need not recur to it. + +\Par{Newton's Argument.}---Here we find a very important +and even slightly disturbing question. I +have said that the principle of relative motion +was not for us simply a result of experiment; and +that \Foreign{à ~priori} every contrary hypothesis would be +repugnant to the mind. But, then, why is the +principle only true if the motion of the movable +axes is uniform and in a straight line? It seems +that it should be imposed upon us with the same +force if the motion is accelerated, or at any rate +if it reduces to a uniform rotation. In these two +cases, in fact, the principle is not true. I need not +dwell on the case in which the motion of the +axes is in a straight line and not uniform. The +paradox does not bear a moment's examination. +If I am in a railway carriage, and if the train, +striking against any obstacle whatever, is suddenly +stopped, I shall be projected on to the opposite +side, although I have not been directly acted upon +by any force. There is nothing mysterious in +that, and if I have not been subject to the action +\PageSep{114} +of any external force, the train has experienced an +external impact. There can be nothing paradoxical +in the relative motion of two bodies being +disturbed when the motion of one or the other is +modified by an external cause. Nor need I dwell +on the case of relative motion referring to axes +which rotate uniformly. If the sky were for ever +covered with clouds, and if we had no means of +observing the stars, we might, nevertheless, conclude +that the earth turns round. We should be +warned of this fact by the flattening at the poles, +or by the experiment of Foucault's pendulum. +And yet, would there in this case be any meaning +in saying that the earth turns round? If there is +no absolute space, can a thing turn without turning +with respect to something; and, on the other +hand, how can we admit Newton's conclusion and +believe in absolute space? But it is not sufficient +to state that all possible solutions are equally +unpleasant to us. We must analyse in each case +the reason of our dislike, in order to make our +choice with the knowledge of the cause. The +long discussion which follows must, therefore, be +excused. + +Let us resume our imaginary story. Thick +clouds hide the stars from men who cannot observe +them, and even are ignorant of their existence. +How will those men know that the earth turns +round? No doubt, for a longer period than did +our ancestors, they will regard the soil on which +they stand as fixed and immovable! They will +\PageSep{115} +wait a much longer time than we did for the +coming of a Copernicus; but this Copernicus will +come at last. How will he come? In the first +place, the mechanical school of this world would +not run their heads against an absolute contradiction. +In the theory of relative motion we observe, +besides real forces, two imaginary forces, which +we call ordinary centrifugal force and compounded +centrifugal force. Our imaginary scientists can +thus explain everything by looking upon these two +forces as real, and they would not see in this a +contradiction of the generalised principle of inertia, +for these forces would depend, the one on the +relative positions of the different parts of the +system, such as real attractions, and the other on +their relative velocities, as in the case of real +frictions. Many difficulties, however, would before +long awaken their attention. If they succeeded in +realising an isolated system, the centre of gravity +of this system would not have an approximately +rectilinear path. They could invoke, to explain +this fact, the centrifugal forces which they would +regard as real, and which, no doubt, they would +attribute to the mutual actions of the bodies---only +they would not see these forces vanish at great +distances---that is to say, in proportion as the +isolation is better realised. Far from it. Centrifugal +force increases indefinitely with distance. +Already this difficulty would seem to them sufficiently +serious, but it would not detain them for +long. They would soon imagine some very subtle +\PageSep{116} +medium analogous to our ether, in which all +bodies would be bathed, and which would exercise +on them a repulsive action. But that is not +all. Space is symmetrical---yet the laws of +motion would present no symmetry. They should +be able to distinguish between right and left. +They would see, for instance, that cyclones always +turn in the same direction, while for reasons of +symmetry they should turn indifferently in any +direction. If our scientists were able by dint of +much hard work to make their universe perfectly +symmetrical, this symmetry would not subsist, +although there is no apparent reason why it +should be disturbed in one direction more than +in another. They would extract this from the +situation no doubt---they would invent something +which would not be more extraordinary than the +glass spheres of Ptolemy, and would thus go on +accumulating complications until the long-expected +Copernicus would sweep them all away +with a single blow, saying it is much more simple +to admit that the earth turns round. Just as +our Copernicus said to us: ``It is more convenient +to suppose that the earth turns round, because the +laws of astronomy are thus expressed in a more +simple language,'' so he would say to them: ``It +is more convenient to suppose that the earth turns +round, because the laws of mechanics are thus +expressed in much more simple language.\Add{''} That +does not prevent absolute space---that is to say, +the point to which we must refer the earth to +\PageSep{117} +know if it really does turn round---from having +no objective existence. And hence this affirmation: +``the earth turns round,'' has no meaning, +since it cannot be verified by experiment; since +such an experiment not only cannot be realised or +even dreamed of by the most daring Jules Verne, +but cannot even be conceived of without contradiction; +or, in other words, these two propositions, +``the earth turns round,'' and, ``it is more +convenient to suppose that the earth turns round,'' +have one and the same meaning. There is nothing +more in one than in the other. Perhaps they will +not be content with this, and may find it surprising +that among all the hypotheses, or rather all +the conventions, that can be made on this subject +there is one which is more convenient than the +rest? But if we have admitted it without difficulty +when it is a question of the laws of +astronomy, why should we object when it is a +question of the laws of mechanics? We have +seen that the co-ordinates of bodies are determined +by differential equations of the second +order, and that so are the differences of these +co-ordinates. This is what we have called the +generalised principle of inertia, and the principle +of relative motion. If the distances of these +bodies were determined in the same way by +equations of the second order, it seems that the +mind should be entirely satisfied. How far does +the mind receive this satisfaction, and why is it +not content with it? To explain this we had +\PageSep{118} +better take a simple example. I assume a system +analogous to our solar system, but in which fixed +stars foreign to this system cannot be perceived, +so that astronomers can only observe the mutual +distances of planets and the sun, and not the +absolute longitudes of the planets. If we deduce +directly from Newton's law the differential equations +which define the variation of these distances, +these equations will not be of the second order. I +mean that if, outside Newton's law, we knew the +initial values of these distances and of their derivatives +with respect to time---that would not be +sufficient to determine the values of these same +distances at an ulterior moment. A datum would +be still lacking, and this datum might be, for +example, what astronomers call the area-constant. +But here we may look at it from two different +points of view. We may consider two kinds of +constants. In the eyes of the physicist the world +reduces to a series of phenomena depending, on the +one hand, solely on initial phenomena, and, on the +other hand, on the laws connecting consequence +and antecedent. If observation then teaches us +that a certain quantity is a constant, we shall have +a choice of two ways of looking at it. So let us +admit that there is a law which requires that this +quantity shall not vary, but that by chance it has +been found to have had in the beginning of time +this value rather than that, a value that it has +kept ever since. This quantity might then be +called an \emph{accidental} constant. Or again, let us +\PageSep{119} +admit on the contrary that there is a law of nature +which imposes on this quantity this value and not +that. We shall then have what may be called an +\emph{essential} constant. For example, in virtue of the +laws of Newton the duration of the revolution of +the earth must be constant. But if it is $366$~and +something sidereal days, and not $300$~or~$400$, it is +because of some initial chance or other. It is an +\emph{accidental} constant. If, on the other hand, the +exponent of the distance which figures in the +expression of the attractive force is equal to~$-2$ +and not to~$-3$, it is not by chance, but because it +is required by Newton's law. It is an \emph{essential} +constant. I do not know if this manner of giving +to chance its share is legitimate in itself, and if +there is not some artificiality about this distinction; +but it is certain at least that in proportion +as Nature has secrets, she will be strictly arbitrary +and always uncertain in their application. As far +as the area-constant is concerned, we are accustomed +to look upon it as accidental. Is it certain +that our imaginary astronomers would do the +same? If they were able to compare two different +solar systems, they would get the idea that this +constant may assume several different values. But +I supposed at the outset, as I was entitled to do, +that their system would appear isolated, and that +they would see no star which was foreign to their +system. Under these conditions they could only +detect a single constant, which would have an +absolutely invariable, unique value. They would +\PageSep{120} +be led no doubt to look upon it as an essential +constant. + +One word in passing to forestall an objection. +The inhabitants of this imaginary world could +neither observe nor define the area-constant as we +do, because absolute longitudes escape their notice; +but that would not prevent them from being +rapidly led to remark a certain constant which +would be naturally introduced into their equations, +and which would be nothing but what we call the +area-constant. But then what would happen? +If the area-constant is regarded as essential, as +dependent upon a law of nature, then in order to +calculate the distances of the planets at any given +moment it would be sufficient to know the initial +values of these distances and those of their first +derivatives. From this new point of view, distances +will be determined by differential equations +of the second order. Would this completely +satisfy the minds of these astronomers? I think +not. In the first place, they would very soon see +that in differentiating their equations so as to +raise them to a higher order, these equations +would become much more simple, and they would +be especially struck by the difficulty which arises +from symmetry. They would have to admit +different laws, according as the aggregate of the +planets presented the figure of a certain polyhedron +or rather of a regular polyhedron, and these consequences +can only be escaped by regarding the area-constant +as accidental. I have taken this particular +\PageSep{121} +example, because I have imagined astronomers +who would not be in the least concerned with +terrestrial mechanics and whose vision would be +bounded by the solar system. But our conclusions +apply in all cases. Our universe is more +extended than theirs, since we have fixed stars; +but it, too, is very limited, so we might reason on +the whole of our universe just as these astronomers +do on their solar system. We thus see that we +should be definitively led to conclude that the +equations which define distances are of an order +higher than the second. Why should this alarm +us---why do we find it perfectly natural that the +sequence of phenomena depends on initial values +of the first derivatives of these distances, while we +hesitate to admit that they may depend on the +initial values of the second derivatives? It can +only be because of mental habits created in us by +the constant study of the generalised principle of +inertia and of its consequences. The values of the +distances at any given moment depend upon their +initial values, on that of their first derivatives, and +something else. What is that \emph{something else}? If +we do not want it to be merely one of the second +derivatives, we have only the choice of hypotheses. +Suppose, as is usually done, that this something +else is the absolute orientation of the universe in +space, or the rapidity with which this orientation +varies; this may be, it certainly is, the most convenient +solution for the geometer. But it is not +the most satisfactory for the philosopher, because +\PageSep{122} +this orientation does not exist. We may assume +that this something else is the position or the +velocity of some invisible body, and this is what is +done by certain persons, who have even called the +body Alpha, although we are destined to never +know anything about this body except its name. +This is an artifice entirely analogous to that of +which I spoke at the end of the paragraph containing +my reflections on the principle of inertia. +But as a matter of fact the difficulty is artificial. +Provided that the future indications of our instruments +can only depend on the indications which +they have given us, or that they might have +formerly given us, such is all we want, and with +these conditions we may rest satisfied. +\PageSep{123} + + +\Chapter{VIII.}{Energy and Thermo-dynamics.} + +\Par{Energetics.}---The difficulties raised by the classical +mechanics have led certain minds to prefer a +new system which they call Energetics. Energetics +took its rise in consequence of the discovery of the +principle of the conservation of energy. Helmholtz +gave it its definite form. We begin by defining +two quantities which play a fundamental +part in this theory. They are \emph{kinetic energy}, or +\Foreign{vis~viva}, and \emph{potential energy}. Every change +that the bodies of nature can undergo is regulated +by two experimental laws. First, the sum of the +kinetic and potential energies is constant. This +is the principle of the conservation of energy. +Second, if a system of bodies is at~$A$ at the time~$t_{0}$, +and at~$B$ at the time~$t_{1}$, it always passes from the +first position to the second by such a path that +the \emph{mean} value of the difference between the two +kinds of energy in the interval of time which +separates the two epochs $t_{0}$~and~$t_{1}$ is a minimum. +This is Hamilton's principle, and is one of the +forms of the principle of least action. The +energetic theory has the following advantages +\PageSep{124} +over the classical. First, it is less incomplete---that +is to say, the principles of the conservation of +energy and of Hamilton teach us more than the +fundamental principles of the classical theory, and +exclude certain motions which do not occur in +nature and which would be compatible with the +classical theory. Second, it frees us from the +hypothesis of atoms, which it was almost impossible +to avoid with the classical theory. But in +its turn it raises fresh difficulties. The definitions +of the two kinds of energy would raise difficulties +almost as great as those of force and mass in the +first system. However, we can get out of these +difficulties more easily, at any rate in the simplest +cases. Assume an isolated system formed of a +certain number of material points. Assume that +these points are acted upon by forces depending +only on their relative position and their distances +apart, and independent of their velocities. +In virtue of the principle of the conservation of +energy there must be a function of forces. In this +simple case the enunciation of the principle of the +conservation of energy is of extreme simplicity. +A certain quantity, which may be determined by +experiment, must remain constant. This quantity +is the sum of two terms. The first depends only on +the position of the material points, and is independent +of their velocities; the second is proportional +to the squares of these velocities. This +decomposition can only take place in one way. +The first of these terms, which I shall call~$U$, will +\PageSep{125} +be potential energy; the second, which I shall call~$T$, +will be kinetic energy. It is true that if $T + U$ +is constant, so is any function of~$T + U$, $\phi(T + U)$. +But this function $\phi(T + U)$ will not be the sum of +two terms, the one independent of the velocities, +and the other proportional to the square of the +velocities. Among the functions which remain +constant there is only one which enjoys this property. +It is~$T + U$ (or a linear function of~$T + U$\Typo{)}{}, +it matters not which, since this linear function may +always be reduced to~$T + U$ by a change of unit +and of origin\Typo{}{)}. This, then, is what we call energy. +The first term we shall call potential energy, and +the second kinetic energy. The definition of the +two kinds of energy may therefore be carried +through without any ambiguity. + +So it is with the definition of mass. Kinetic +energy, or \Foreign{vis~viva}, is expressed very simply by the +aid of the masses, and of the relative velocities of all +the material points with reference to one of them. +These relative velocities may be observed, and +when we have the expression of the kinetic energy +as a function of these relative velocities, the co-efficients +of this expression will give us the masses. +So in this simple case the fundamental ideas can +be defined without difficulty. But the difficulties +reappear in the more complicated cases if the +forces, instead of depending solely on the distances, +depend also on the velocities. For example, +Weber supposes the mutual action of two +electric molecules to depend not only on their +\PageSep{126} +distance but on their velocity and on their acceleration. +If material points attracted each other +according to an analogous law, $U$~would depend +on the velocity, and it might contain a term +proportional to the square of the velocity. How +can we detect among such terms those that arise +from $T$~or~$U$? and how, therefore, can we distinguish +the two parts of the energy? But there +is more than this. How can we define energy +itself? We have no more reason to take as our +definition $T + U$ rather than any other function of~$T + U$, +when the property which characterised +$T + U$ has disappeared---namely, that of being the +sum of two terms of a particular form. But that +is not all. We must take account, not only of +mechanical energy properly so called, but of the +other forms of energy---heat, chemical energy, +electrical energy,~etc. The principle of the conservation +of energy must be written $T + U + Q =$ +a constant, where $T$~is the sensible kinetic energy, +$U$~the potential energy of position, depending only +on the position of the bodies, $Q$~the internal +molecular energy under the thermal, chemical, or +electrical form. This would be all right if the +three terms were absolutely distinct; if $T$~were +proportional to the square of the velocities, $U$~independent +of these velocities and of the state of +the bodies, $Q$~independent of the velocities and of +the positions of the bodies, and depending only on +their internal state. The expression for the energy +could be decomposed in one way only into three +\PageSep{127} +terms of this form. But this is not the case. Let +us consider electrified bodies. The electro-static +energy due to their mutual action will evidently +depend on their charge---\ie, on their state; +but it will equally depend on their position. +If these bodies are in motion, they will act +electro-dynamically on one another, and the +electro-dynamic energy will depend not only on +their state and their position but on their velocities. +We have therefore no means of making the selection +of the terms which should form part of~$T$, +and~$U$, and~$Q$, and of separating the three parts of +the energy. If $T + U + Q$ is constant, the same is +true of any function whatever, $\phi(T + U + Q)$. + +If $T + U + Q$ were of the particular form that I +have suggested above, no ambiguity would ensue. +Among the functions $\phi(T + U + Q)$ which remain +constant, there is only one that would be of this +particular form, namely the one which I would +agree to call energy. But I have said this is not +rigorously the case. Among the functions that +remain constant there is not one which can +rigorously be placed in this particular form. How +then can we choose from among them that which +should be called energy? We have no longer +any guide in our choice. + +Of the principle of the conservation of energy +there is nothing left then but an enunciation:---\emph{There +is something which remains constant.} In this +form it, in its turn, is outside the bounds of experiment +and reduced to a kind of tautology. It +\PageSep{128} +is clear that if the world is governed by laws +there will be quantities which remain constant. +Like Newton's laws, and for an analogous reason, +the principle of the conservation of energy being +based on experiment, can no longer be invalidated +by it. + +This discussion shows that, in passing from the +classical system to the energetic, an advance has +been made; but it shows, at the same time, that +we have not advanced far enough. + +Another objection seems to be still more serious. +The principle of least action is applicable to reversible +phenomena, but it is by no means satisfactory +as far as irreversible phenomena are concerned. +Helmholtz attempted to extend it to this class +of phenomena, but he did not and could not +succeed. So far as this is concerned all has yet to +be done. The very enunciation of the principle of +least action is objectionable. To move from one +point to another, a material molecule, acted upon +by no force, but compelled to move on a surface, +will take as its path the geodesic line---\ie, the +shortest path. This molecule seems to know the +point to which we want to take it, to foresee +the time that it will take it to reach it by such +a path, and then to know how to choose the most +convenient path. The enunciation of the principle +presents it to us, so to speak, as a living +and free entity. It is clear that it would be better +to replace it by a less objectionable enunciation, +one in which, as philosophers would say, final +\PageSep{129} +effects do not seem to be substituted for acting +causes. + +\Par{Thermo-dynamics.}---The rôle of the two fundamental +principles of thermo-dynamics becomes +daily more important in all branches of natural +philosophy. Abandoning the ambitious theories +of forty years ago, encumbered as they were with +molecular hypotheses, we now try to rest on +thermo-dynamics alone the entire edifice of +mathematical physics. Will the two principles +of Mayer and of Clausius assure to it foundations +solid enough to last for some time? We +all feel it, but whence does our confidence +arise? An eminent physicist said to me one day, +\Foreign{à propos} of the law of errors:---every one stoutly +believes it, because mathematicians imagine that +it is an effect of observation, and observers imagine +that it is a mathematical theorem. And this was +for a long time the case with the principle of the +conservation of energy. It is no longer the same +now. There is no one who does not know that it +is an experimental fact. But then who gives us +the right of attributing to the principle itself more +generality and more precision than to the experiments +which have served to demonstrate it? This +is asking, if it is legitimate to generalise, as we do +every day, empiric data, and I shall not be so +foolhardy as to discuss this question, after so many +philosophers have vainly tried to solve it. One +thing alone is certain. If this permission were +refused to us, science could not exist; or at least +\PageSep{130} +would be reduced to a kind of inventory, to the +ascertaining of isolated facts. It would not longer +be to us of any value, since it could not satisfy our +need of order and harmony, and because it would +be at the same time incapable of prediction. As +the circumstances which have preceded any fact +whatever will never again, in all probability, be +simultaneously reproduced, we already require a +first generalisation to predict whether the fact will +be renewed as soon as the least of these circumstances +is changed. But every proposition may +be generalised in an infinite number of ways. +Among all possible generalisations we must +choose, and we cannot but choose the simplest. +We are therefore led to adopt the same course +as if a simple law were, other things being equal, +more probable than a complex law. A century +ago it was frankly confessed and proclaimed +abroad that Nature loves simplicity; but Nature +has proved the contrary since then on more than +one occasion. We no longer confess this tendency, +and we only keep of it what is indispensable, so +that science may not become impossible. In +formulating a general, simple, and formal law, +based on a comparatively small number of not altogether +consistent experiments, we have only obeyed +a necessity from which the human mind cannot +free itself. But there is something more, and that +is why I dwell on this topic. No one doubts that +Mayer's principle is not called upon to survive all +the particular laws from which it was deduced, in +\PageSep{131} +the same way that Newton's law has survived the +laws of Kepler from which it was derived, and +which are no longer anything but approximations, +if we take perturbations into account. Now why +does this principle thus occupy a kind of privileged +position among physical laws? There are many +reasons for that. At the outset we think that we +cannot reject it, or even doubt its absolute rigour, +without admitting the possibility of perpetual +motion; we certainly feel distrust at such a +prospect, and we believe ourselves less rash in +affirming it than in denying it. That perhaps is +not quite accurate. The impossibility of perpetual +motion only implies the conservation of energy for +reversible phenomena. The imposing simplicity +of Mayer's principle equally contributes to +strengthen our faith. In a law immediately deduced +from experiments, such as Mariotte's law, +this simplicity would rather appear to us a reason +for distrust; but here this is no longer the case. +We take elements which at the first glance are +unconnected; these arrange themselves in an unexpected +order, and form a harmonious whole. +We cannot believe that this unexpected harmony +is a mere result of chance. Our conquest +appears to be valuable to us in proportion to the +efforts it has cost, and we feel the more certain of +having snatched its true secret from Nature in proportion +as Nature has appeared more jealous of our +attempts to discover it. But these are only small +reasons. Before we raise Mayer's law to the +\PageSep{132} +dignity of an absolute principle, a deeper discussion +is necessary. But if we embark on this discussion +we see that this absolute principle is not even easy +to enunciate. In every particular case we clearly +see what energy is, and we can give it at least a +provisory definition; but it is impossible to find +a general definition of it. If we wish to enunciate +the principle in all its generality and apply it to +the universe, we see it vanish, so to speak, and +nothing is left but this---\emph{there is something which +remains constant}. But has this a meaning? In +the determinist hypothesis the state of the universe +is determined by an extremely large number~$n$ +of parameters, which I shall call $x_{1}$,~$x_{2}$, $x_{3}\Add{,}~\ldots\Add{,},~x_{n}$. +As soon as we know at a given moment the values of +these $n$~parameters, we also know their derivatives +with respect to time, and we can therefore calculate +the values of these same parameters at an +anterior or ulterior moment. In other words, +these $n$~parameters specify $n$~differential equations +of the first order. These equations have $n - 1$ +integrals, and therefore there are $n - 1$ functions of +$x_{1}$,~$x_{2}$, $x_{3}\Add{,}~\ldots\Add{,}~x_{n}$, which remain constant. If we +say then, \emph{there is something which remains constant}, +we are only enunciating a tautology. We would +be even embarrassed to decide which among all +our integrals is that which should retain the name +of energy. Besides, it is not in this sense that +Mayer's principle is understood when it is applied +to a limited system. We admit, then, that $p$~of +our $n$~parameters vary independently so that we +\PageSep{133} +have only $n - p$ relations, generally linear, between +our $n$~parameters and their derivatives. Suppose, +for the sake of simplicity, that the sum of the +work done by the external forces is zero, as well +as that of all the quantities of heat given off from +the interior: what will then be the meaning of +our principle? \emph{There is a combination of these $n - p$ +relations, of which the first member is an exact +differential}; and then this differential vanishing +in virtue of our $n - p$ relations, its integral is a +constant, and it is this integral which we call +energy. But how can it be that there are several +parameters whose variations are independent? +That can only take place in the case of external +forces (although we have supposed, for the sake +of simplicity, that the algebraical sum of all the +work done by these forces has vanished). If, +in fact, the system were completely isolated from +all external action, the values of our $n$~parameters +at a given moment would suffice to determine +the state of the system at any ulterior moment +whatever, provided that we still clung to the determinist +hypothesis. We should therefore fall back +on the same difficulty as before. If the future +state of the system is not entirely determined +by its present state, it is because it further depends +on the state of bodies external to the system. +But then, is it likely that there exist among the +parameters~$x$ which define the state of the system of +equations independent of this state of the external +bodies? and if in certain cases we think we can +\PageSep{134} +find them, is it not only because of our ignorance, +and because the influence of these bodies is too +weak for our experiment to be able to detect it? +If the system is not regarded as completely +isolated, it is probable that the rigorously exact +expression of its internal energy will depend upon +the state of the external bodies. Again, I have +supposed above that the sum of all the external +work is zero, and if we wish to be free from +this rather artificial restriction the enunciation +becomes still more difficult. To formulate +Mayer's principle by giving it an absolute +meaning, we must extend it to the whole +universe, and then we find ourselves face to +face with the very difficulty we have endeavoured +to avoid. To sum up, and to use ordinary +language, the law of the conservation of energy +can have only one significance, because there is +in it a property common to all possible properties; +but in the determinist hypothesis there is only one +possible, and then the law has no meaning. In +the indeterminist hypothesis, on the other hand, +it would have a meaning even if we wished to +regard it in an absolute sense. It would appear +as a limitation imposed on freedom. + +But this word warns me that I am wandering +from the subject, and that I am leaving the +domain of mathematics and physics. I check +myself, therefore, and I wish to retain only one +impression of the whole of this discussion, and +that is, that Mayer's law is a form subtle enough +\PageSep{135} +for us to be able to put into it almost anything we +like. I do not mean by that that it corresponds +to no objective reality, nor that it is reduced to +mere tautology; since, in each particular case, and +provided we do not wish to extend it to the +absolute, it has a perfectly clear meaning. This +subtlety is a reason for believing that it will last +long; and as, on the other hand, it will only +disappear to be blended in a higher harmony, +we may work with confidence and utilise it, +certain beforehand that our work will not be +lost. + +Almost everything that I have just said +applies to the principle of Clausius. What +distinguishes it is, that it is expressed by an +inequality. It will be said perhaps that it is +the same with all physical laws, since their +precision is always limited by errors of +observation. But they at least claim to be +first approximations, and we hope to replace +them little by little by more exact laws. If, +on the other hand, the principle of Clausius +reduces to an inequality, this is not caused by +the imperfection of our means of observation, but +by the very nature of the question. + +\Par{General Conclusions on Part~III.}---The principles +of mechanics are therefore presented to us +under two different aspects. On the one hand, +there are truths founded on experiment, and +verified approximately as far as almost isolated +systems are concerned; on the other hand, +\PageSep{136} +there are postulates applicable to the whole of +the universe and regarded as rigorously true. +If these postulates possess a generality and a +certainty which falsify the experimental truths +from which they were deduced, it is because +they reduce in final analysis to a simple convention +that we have a right to make, because +we are certain beforehand that no experiment +can contradict it. This convention, however, is +not absolutely arbitrary; it is not the child +of our caprice. We admit it because certain +experiments have shown us that it will be convenient, +and thus is explained how experiment +has built up the principles of mechanics, and +why, moreover, it cannot reverse them. Take a +comparison with geometry. The fundamental +propositions of geometry, for instance, Euclid's +postulate, are only conventions, and it is quite +as unreasonable to ask if they are true or false +as to ask if the metric system is true or false. +Only, these conventions are convenient, and there +are certain experiments which prove it to us. At +the first glance, the analogy is complete, the rôle +of experiment seems the same. We shall therefore +be tempted to say, either mechanics must +be looked upon as experimental science and then +it should be the same with geometry; or, on the +contrary, geometry is a deductive science, and +then we can say the same of mechanics. Such +a conclusion would be illegitimate. The experiments +which have led us to adopt as more +\PageSep{137} +convenient the fundamental conventions of +geometry refer to bodies which have nothing +in common with those that are studied by +geometry. They refer to the properties of solid +bodies and to the propagation of light in a straight +line. These are mechanical, optical experiments. +In no way can they be regarded as geometrical +experiments. And even the probable reason why +our geometry seems convenient to us is, that our +bodies, our hands, and our limbs enjoy the properties +of solid bodies. Our fundamental experiments are +pre-eminently physiological experiments which +refer, not to the space which is the object that +geometry must study, but to our body---that is to +say, to the instrument which we use for that +study. On the other hand, the fundamental +conventions of mechanics and the experiments +which prove to us that they are convenient, +certainly refer to the same objects or to analogous +objects. Conventional and general principles are +the natural and direct generalisations of experimental +and particular principles. Let it not be +said that I am thus tracing artificial frontiers +between the sciences; that I am separating by +a barrier geometry properly so called from the +study of solid bodies. I might just as well +raise a barrier between experimental mechanics +and the conventional mechanics of general +principles. Who does not see, in fact, that +by separating these two sciences we mutilate +both, and that what will remain of the conventional +\PageSep{138} +mechanics when it is isolated will be but +very little, and can in no way be compared with +that grand body of doctrine which is called +geometry. + +We now understand why the teaching of +mechanics should remain experimental. Thus +only can we be made to understand the genesis +of the science, and that is indispensable for +a complete knowledge of the science itself. +Besides, if we study mechanics, it is in order +to apply it; and we can only apply it if it remains +objective. Now, as we have seen, when principles +gain in generality and certainty they lose in +objectivity. It is therefore especially with the +objective side of principles that we must be +early familiarised, and this can only be by +passing from the particular to the general, instead +of from the general to the particular. + +Principles are conventions and definitions in +disguise. They are, however, deduced from +experimental laws, and these laws have, so to +speak, been erected into principles to which +our mind attributes an absolute value. Some +philosophers have generalised far too much. +They have thought that the principles were +the whole of science, and therefore that the +whole of science was conventional. This paradoxical +doctrine, which is called Nominalism, +cannot stand examination. How can a law +become a principle? It expressed a relation +between two real terms, $A$~and~$B$; but it was +\PageSep{139} +not rigorously true, it was only approximate. +We introduce arbitrarily an intermediate term,~$C$, +more or less imaginary, and $C$~is \emph{by definition} that +which has with~$A$ \emph{exactly} the relation expressed +by the law. So our law is decomposed into an +absolute and rigorous principle which expresses +the relation of~$A$ to~$C$, and an approximate experimental +and revisable law which expresses the +relation of~$C$ to~$B$. But it is clear that however +far this decomposition may be carried, laws will +always remain. We shall now enter into the +domain of laws properly so called. +\PageSep{140} + + +\Part{IV.}{Nature.} + +\Chapter{IX.}{Hypotheses in Physics.} + +\Par{The Rôle of Experiment and Generalisation.}---Exper\-iment +is the sole source of truth. It alone +can teach us something new; it alone can give +us certainty. These are two points that cannot +be questioned. But then, if experiment is everything, +what place is left for mathematical physics? +What can experimental physics do with such an +auxiliary---an auxiliary, moreover, which seems +useless, and even may be dangerous? + +However, mathematical physics exists. It has +rendered undeniable service, and that is a fact +which has to be explained. It is not sufficient +merely to observe; we must use our observations, +and for that purpose we must generalise. This +is what has always been done, only as the recollection +of past errors has made man more and more +circumspect, he has observed more and more and +generalised less and less. Every age has scoffed +at its predecessor, accusing it of having generalised +\PageSep{141} +too boldly and too naïvely. Descartes used to +commiserate the Ionians. Descartes in his turn +makes us smile, and no doubt some day our +children will laugh at us. Is there no way of +getting at once to the gist of the matter, and +thereby escaping the raillery which we foresee? +Cannot we be content with experiment alone? +No, that is impossible; that would be a complete +misunderstanding of the true character of science. +The man of science must work with method. +Science is built up of facts, as a house is built of +stones; but an accumulation of facts is no more a +science than a heap of stones is a house. Most +important of all, the man of science must exhibit +foresight. Carlyle has written somewhere something +after this fashion. ``Nothing but facts are +of importance. John Lackland passed by here. +Here is something that is admirable. Here is a +reality for which I would give all the theories in +the world.''\footnote + {V. \Title{Past and Present}, end of Chapter~I., Book~II.\Transl} +Carlyle was a compatriot of Bacon, +and, like him, he wished to proclaim his worship +of \emph{the God of Things as they are}. + +But Bacon would not have said that. That is +the language of the historian. The physicist +would most likely have said: ``John Lackland +passed by here. It is all the same to me, for he +will not pass this way again.'' + +We all know that there are good and bad +experiments. The latter accumulate in vain. +Whether there are a hundred or a thousand, +\PageSep{142} +one single piece of work by a real master---by a +Pasteur, for example---will be sufficient to sweep +them into oblivion. Bacon would have thoroughly +understood that, for he invented the phrase \Foreign{experimentum +crucis}; but Carlyle would not have understood +it. A fact is a fact. A student has read +such and such a number on his thermometer. +He has taken no precautions. It does not matter; +he has read it, and if it is only the fact which +counts, this is a reality that is as much entitled +to be called a reality as the peregrinations of King +John Lackland. What, then, is a good experiment? +It is that which teaches us something more than +an isolated fact. It is that which enables us to +predict, and to generalise. Without generalisation, +prediction is impossible. The circumstances +under which one has operated will never again +be reproduced simultaneously. The fact observed +will never be repeated. All that can be affirmed +is that under analogous circumstances an analogous +fact will be produced. To predict it, we must +therefore invoke the aid of analogy---that is to say, +even at this stage, we must generalise. However +timid we may be, there must be interpolation. +Experiment only gives us a certain number of +isolated points. They must be connected by a +continuous line, and this is a true generalisation. +But more is done. The curve thus traced will +pass between and near the points observed; it +will not pass through the points themselves. +Thus we are not restricted to generalising our +\PageSep{143} +experiment, we correct it; and the physicist who +would abstain from these corrections, and really +content himself with experiment pure and simple, +would be compelled to enunciate very extraordinary +laws indeed. Detached facts cannot +therefore satisfy us, and that is why our science +must be ordered, or, better still, generalised. + +It is often said that experiments should be made +without preconceived ideas. That is impossible. +Not only would it make every experiment fruitless, +but even if we wished to do so, it could not be +done. Every man has his own conception of the +world, and this he cannot so easily lay aside. We +must, for example, use language, and our language +is necessarily steeped in preconceived ideas. Only +they are unconscious preconceived ideas, which +are a thousand times the most dangerous of all. +Shall we say, that if we cause others to intervene of +which we are fully conscious, that we shall only +aggravate the evil? I do not think so. I am +inclined to think that they will serve as ample +counterpoises---I was almost going to say antidotes. +They will generally disagree, they will enter into +conflict one with another, and \Foreign{ipso~facto}, they will +force us to look at things under different aspects. +This is enough to free us. He is no longer a slave +who can choose his master. + +Thus, by generalisation, every fact observed +enables us to predict a large number of others; +only, we ought not to forget that the first alone +is certain, and that all the others are merely +\PageSep{144} +probable. However solidly founded a prediction +may appear to us, we are never \emph{absolutely} sure that +experiment will not prove it to be baseless if we +set to work to verify it. But the probability of its +accuracy is often so great that practically we may +be content with it. It is far better to predict +without certainty, than never to have predicted +at all. We should never, therefore, disdain to +verify when the opportunity presents itself. But +every experiment is long and difficult, and the +labourers are few, and the number of facts which +we require to predict is enormous; and besides +this mass, the number of direct verifications that +we can make will never be more than a negligible +quantity. Of this little that we can directly attain +we must choose the best. Every experiment must +enable us to make a maximum number of predictions +having the highest possible degree of probability. +The problem is, so to speak, to increase +the output of the scientific machine. I may be +permitted to compare science to a library which +must go on increasing indefinitely; the librarian +has limited funds for his purchases, and he must, +therefore, strain every nerve not to waste them. +Experimental physics has to make the purchases, +and experimental physics alone can enrich the +library. As for mathematical physics, her duty +is to draw up the catalogue. If the catalogue is +well done the library is none the richer for it; but +the reader will be enabled to utilise its riches; +and also by showing the librarian the gaps in his +\PageSep{145} +collection, it will help him to make a judicious +use of his funds, which is all the more important, +inasmuch as those funds are entirely inadequate. +That is the rôle of mathematical physics. It +must direct generalisation, so as to increase what +I called just now the output of science. By what +means it does this, and how it may do it without +danger, is what we have now to examine. + +\Par{The Unity of Nature.}---Let us first of all observe +that every generalisation supposes in a certain +measure a belief in the unity and simplicity of +Nature. As far as the unity is concerned, there +can be no difficulty. If the different parts of the +universe were not as the organs of the same body, +they would not \Chg{re-act}{react} one upon the other; they +would mutually ignore each other, and we in +particular should only know one part. We need +not, therefore, ask if Nature is one, but how she +is one. + +As for the second point, that is not so clear. It +is not certain that Nature is simple. Can we +without danger act as if she were? + +There was a time when the simplicity of +Mariotte's law was an argument in favour of its +accuracy: when Fresnel himself, after having said +in a conversation with Laplace that Nature cares +naught for analytical difficulties, was compelled +to explain his words so as not to give offence to +current opinion. Nowadays, ideas have changed +considerably; but those who do not believe that +natural laws must be simple, are still often obliged +\PageSep{146} +to act as if they did believe it. They cannot +entirely dispense with this necessity without +making all generalisation, and therefore all science, +impossible. It is clear that any fact can be +generalised in an infinite number of ways, and +it is a question of choice. The choice can only +be guided by considerations of simplicity. Let +us take the most ordinary case, that of interpolation. +We draw a continuous line as regularly as +possible between the points given by observation. +Why do we avoid angular points and inflexions +that are too sharp? Why do we not make our +curve describe the most capricious zigzags? It +is because we know beforehand, or think we know, +that the law we have to express cannot be so +complicated as all that. The mass of Jupiter +may be deduced either from the movements of +his satellites, or from the perturbations of the +major planets, or from those of the minor planets. +If we take the mean of the determinations obtained +by these three methods, we find three numbers +very close together, but not quite identical. This +result might be interpreted by supposing that the +gravitation constant is not the same in the three +cases; the observations would be certainly much +better represented. Why do we reject this interpretation? +Not because it is absurd, but because +it is uselessly complicated. We shall only accept +it when we are forced to, and it is not imposed +upon us yet. To sum up, in most cases every law +is held to be simple until the contrary is proved. +\PageSep{147} + +This custom is imposed upon physicists by the +reasons that I have indicated, but how can it be +justified in the presence of discoveries which daily +show us fresh details, richer and more complex? +How can we even reconcile it with the unity of +nature? For if all things are interdependent, +the relations in which so many different objects +intervene can no longer be simple. + +If we study the history of science we see produced +two phenomena which are, so to speak, +each the inverse of the other. Sometimes it is +simplicity which is hidden under what is +apparently complex; sometimes, on the contrary, +it is simplicity which is apparent, and which +conceals extremely complex realities. What is +there more complicated than the disturbed +motions of the planets, and what more simple +than Newton's law? There, as Fresnel said, +Nature playing with analytical difficulties, only +uses simple means, and creates by their combination +I know not what tangled skein. Here it is +the hidden simplicity which must be disentangled. +Examples to the contrary abound. In the kinetic +theory of gases, molecules of tremendous velocity +are discussed, whose paths, deformed by incessant +impacts, have the most capricious shapes, and +plough their way through space in every direction. +The result observable is Mariotte's simple law. +Each individual fact was complicated. The law +of great numbers has re-established simplicity in +the mean. Here the simplicity is only apparent, +\PageSep{148} +and the coarseness of our senses alone prevents us +from seeing the complexity. + +Many phenomena obey a law of proportionality. +But why? Because in these phenomena +there is something which is very small. The +simple law observed is only the translation of +the general analytical rule by which the infinitely +small increment of a function is proportional +to the increment of the variable. As in reality +our increments are not infinitely small, but only +very small, the law of proportionality is only +approximate, and simplicity is only apparent. +What I have just said applies to the law of the +superposition of small movements, which is so +fruitful in its applications and which is the foundation +of optics. + +And Newton's law itself? Its simplicity, so +long undetected, is perhaps only apparent. Who +knows if it be not due to some complicated +mechanism, to the impact of some subtle matter +animated by irregular movements, and if it has +not become simple merely through the play of +averages and large numbers? In any case, it +is difficult not to suppose that the true law contains +complementary terms which may become +sensible at small distances. If in astronomy they +are negligible, and if the law thus regains its +simplicity, it is solely on account of the enormous +distances of the celestial bodies. No doubt, if our +means of investigation became more and more +penetrating, we should discover the simple beneath +\PageSep{149} +the complex, and then the complex from the +simple, and then again the simple beneath the +complex, and so on, without ever being able to +predict what the last term will be. We must stop +somewhere, and for science to be possible we must +stop where we have found simplicity. That is the +only ground on which we can erect the edifice of +our generalisations. But, this simplicity being +only apparent, will the ground be solid enough? +That is what we have now to discover. + +For this purpose let us see what part is played +in our generalisations by the belief in simplicity. +We have verified a simple law in a considerable +number of particular cases. We refuse to admit +that this coincidence, so often repeated, is a result +of mere chance, and we conclude that the law +must be true in the general case. + +Kepler remarks that the positions of a planet +observed by Tycho are all on the same ellipse. +Not for one moment does he think that, by a +singular freak of chance, Tycho had never looked +at the heavens except at the very moment when +the path of the planet happened to cut that +ellipse. What does it matter then if the simplicity +be real or if it hide a complex truth? Whether it +be due to the influence of great numbers which +reduces individual differences to a level, or to the +greatness or the smallness of certain quantities +which allow of certain terms to be neglected---in +no case is it due to chance. This simplicity, real +or apparent, has always a cause. We shall therefore +\PageSep{150} +always be able to reason in the same fashion, +and if a simple law has been observed in several +particular cases, we may legitimately suppose that +it still will be true in analogous cases. To refuse +to admit this would be to attribute an inadmissible +rôle to chance. However, there is a +difference. If the simplicity were real and profound +it would bear the test of the increasing +precision of our methods of measurement. If, +then, we believe Nature to be profoundly simple, +we must conclude that it is an approximate and +not a rigorous simplicity. This is what was +formerly done, but it is what we have no longer +the right to do. The simplicity of Kepler's laws, +for instance, is only apparent; but that does not +prevent them from being applied to almost all +systems analogous to the solar system, though +that prevents them from being rigorously exact. + +\Par{Rôle of Hypothesis.}---Every generalisation is a +hypothesis. Hypothesis therefore plays a necessary +rôle, which no one has ever contested. Only, +it should always be as soon as possible submitted +to verification. It goes without saying that, if it +cannot stand this test, it must be abandoned +without any hesitation. This is, indeed, what +is generally done; but sometimes with a certain +impatience. Ah well!\ this impatience is not +justified. The physicist who has just given up +one of his hypotheses should, on the contrary, +rejoice, for he found an unexpected opportunity of +discovery. His hypothesis, I imagine, had not +\PageSep{151} +been lightly adopted, It took into account all the +known factors which seem capable of intervention +in the phenomenon. If it is not verified, it is +because there is something unexpected and extraordinary +about it, because we are on the point +of finding something unknown and new. Has +the hypothesis thus rejected been sterile? Far +from it. It may be even said that it has rendered +more service than a true hypothesis. Not only +has it been the occasion of a decisive experiment, +but if this experiment had been made by chance, +without the hypothesis, no conclusion could have +been drawn; nothing extraordinary would have +been seen; and only one fact the more would have +been catalogued, without deducing from it the +remotest consequence. + +Now, under what conditions is the use of +hypothesis without danger? The proposal to +submit all to experiment is not sufficient. Some +hypotheses are dangerous,---first and foremost +those which are tacit and unconscious. And +since we make them without knowing them, +we cannot get rid of them. Here again, there +is a service that mathematical physics may +render us. By the precision which is its characteristic, +we are compelled to formulate all the +hypotheses that we would unhesitatingly make +without its aid. Let us also notice that it is +important not to multiply hypotheses indefinitely. +If we construct a theory based upon multiple hypotheses, +and if experiment condemns it, which of +\PageSep{152} +the premisses must be changed? It is impossible +to tell. Conversely, if the experiment succeeds, +must we suppose that it has verified all these +hypotheses at once? Can several unknowns be +determined from a single equation? + +We must also take care to distinguish between +the different kinds of hypotheses. First of all, +there are those which are quite natural and +necessary. It is difficult not to suppose that the +influence of very distant bodies is quite negligible, +that small movements obey a linear law, and that +effect is a continuous function of its cause. I will +say as much for the conditions imposed by +symmetry. All these hypotheses affirm, so to +speak, the common basis of all the theories of +mathematical physics. They are the last that +should be abandoned. There is a second category +of hypotheses which I shall qualify as indifferent. +In most questions the analyst assumes, at the +beginning of his calculations, either that matter is +continuous, or the reverse, that it is formed of +atoms. In either case, his results would have +been the same. On the atomic supposition he has +a little more difficulty in obtaining them---that is +all. If, then, experiment confirms his conclusions, +will he suppose that he has proved, for example, +the real existence of atoms? + +In optical theories two vectors are introduced, +one of which we consider as a velocity and the +other as a vortex. This again is an indifferent +hypothesis, since we should have arrived at the +\PageSep{153} +same conclusions by assuming the former to be +a vortex and the latter to be a velocity. The +success of the experiment cannot prove, therefore, +that the first vector is really a velocity. It only +proves one thing---namely, that it is a vector; +and that is the only hypothesis that has really +been introduced into the premisses. To give it +the concrete appearance that the fallibility of our +minds demands, it was necessary to consider it +either as a velocity or as a vortex. In the same +way, it was necessary to represent it by an~$x$ or a~$y$, +but the result will not prove that we were right +or wrong in regarding it as a velocity; nor will it +prove we are right or wrong in calling it~$x$ and +not~$y$. + +These indifferent hypotheses are never dangerous +provided their characters are not misunderstood. +They may be useful, either as artifices for +calculation, or to assist our understanding by +concrete images, to fix the ideas, as we say. They +need not therefore be rejected. The hypotheses +of the third category are real generalisations. +They must be confirmed or invalidated by experiment. +Whether verified or condemned, they will +always be fruitful; but, for the reasons I have +given, they will only be so if they are not too +numerous. + +\Par{Origin of Mathematical Physics.}---Let us go +further and study more closely the conditions +which have assisted the development of mathematical +physics. We recognise at the outset that +\PageSep{154} +the efforts of men of science have always tended +to resolve the complex phenomenon given directly +by experiment into a very large number of elementary +phenomena, and that in three different +ways. + +First, with respect to time. Instead of embracing +in its entirety the progressive development of a +phenomenon, we simply try to connect each +moment with the one immediately preceding. +We admit that the present state of the world +only depends on the immediate past, without +being directly influenced, so to speak, by the +recollection of a more distant past. Thanks to +this postulate, instead of studying directly the +whole succession of phenomena, we may confine +ourselves to writing down its \emph{differential equation}; +for the laws of Kepler we substitute the law of +Newton. + +Next, we try to decompose the phenomena in +space. What experiment gives us is a confused +aggregate of facts spread over a scene of considerable +extent. We must try to deduce the elementary +phenomenon, which will still be localised in a +very small region of space. + +A few examples perhaps will make my meaning +clearer. If we wished to study in all its complexity +the distribution of temperature in a cooling +solid, we could never do so. This is simply because, +if we only reflect that a point in the solid +can directly impart some of its heat to a neighbouring +point, it will immediately impart that +\PageSep{155} +heat only to the nearest points, and it is but +gradually that the flow of heat will reach other +portions of the solid. The elementary phenomenon +is the interchange of heat between two +contiguous points. It is strictly localised and +relatively simple if, as is natural, we admit that +it is not influenced by the temperature of the +molecules whose distance apart is small. + +I bend a rod: it takes a very complicated form, +the direct investigation of which would be impossible. +But I can attack the problem, however, +if I notice that its flexure is only the resultant of +the deformations of the very small elements of the +rod, and that the deformation of each of these +elements only depends on the forces which are +directly applied to it, and not in the least on +those which may be acting on the other elements. + +In all these examples, which may be increased +without difficulty, it is admitted that there is no +action at a distance or at great distances. That +is an hypothesis. It is not always true, as the law +of gravitation proves. It must therefore be verified. +If it is confirmed, even approximately, it is valuable, +for it helps us to use mathematical physics, +at any rate by successive approximations. If it +does not stand the test, we must seek something +else that is analogous, for there are other means +of arriving at the elementary phenomenon. If +several bodies act simultaneously, it may happen +that their actions are independent, and may be +added one to the other, either as vectors or as scalar +\PageSep{156} +quantities. The elementary phenomenon is then +the action of an isolated body. Or suppose, again, +it is a question of small movements, or more +generally of small variations which obey the well-known +law of mutual or relative independence. +The movement observed will then be decomposed +into simple movements---for example, sound into +its harmonics, and white light into its monochromatic +components. When we have discovered in +which direction to seek for the elementary phenomena, +by what means may we reach it? First, it +will often happen that in order to predict it, or rather +in order to predict what is useful to us, it will not +be necessary to know its mechanism. The law of +great numbers will suffice. Take for example the +propagation of heat. Each molecule radiates towards +its neighbour---we need not inquire according +to what law; and if we make any supposition +in this respect, it will be an indifferent hypothesis, +and therefore useless and unverifiable. In fact, +by the action of averages and thanks to the +symmetry of the medium, all differences are +levelled, and, whatever the hypothesis may be, the +result is always the same. + +The same feature is presented in the theory of +elasticity, and in that of capillarity. The neighbouring +molecules attract and repel each other, we +need not inquire by what law. It is enough for us +that this attraction is sensible at small distances +only, and that the molecules are very numerous, +that the medium is symmetrical, and we have +\PageSep{157} +only to let the law of great numbers come into +play. + +Here again the simplicity of the elementary +phenomenon is hidden beneath the complexity of +the observable resultant phenomenon; but in its +turn this simplicity was only apparent and disguised +a very complex mechanism. Evidently the +best means of reaching the elementary phenomenon +would be experiment. It would be necessary +by experimental artifices to dissociate the +complex system which nature offers for our investigations +and carefully to study the elements as +dissociated as possible; for example, natural white +light would be decomposed into monochromatic +lights by the aid of the prism, and into polarised +lights by the aid of the polariser. Unfortunately, +that is neither always possible nor always sufficient, +and sometimes the mind must run ahead of +experiment. I shall only give one example which +has always struck me rather forcibly. If I decompose +white light, I shall be able to isolate a +portion of the spectrum, but however small it may +be, it will always be a certain width. In the same +way the natural lights which are called \emph{monochromatic} +%[** TN: "nous donnent une raie très fine, mais qui n'est pas cependant infiniment fine"] +give us a very fine \Reword{array, but a y}{ray, but one} which +is not, however, infinitely fine. It might be +supposed that in the experimental study of the +properties of these natural lights, by operating +with finer and finer rays, and passing on at last +to the limit, so to speak, we should eventually +obtain the properties of a rigorously monochromatic +\PageSep{158} +light. That would not be accurate. +I assume that two rays emanate from the same +source, that they are first polarised in planes at +right angles, that they are then brought back +again to the same plane of polarisation, and that +we try to obtain interference. If the light were +\emph{rigorously} monochromatic, there would be interference; +but with our nearly monochromatic +lights, there will be no interference, and that, +however narrow the ray may be. For it to be +otherwise, the ray would have to be several million +times finer than the finest known rays. + +Here then we should be led astray by proceeding +to the limit. The mind has to run ahead of the +experiment, and if it has done so with success, it +is because it has allowed itself to be guided by the +instinct of simplicity. The knowledge of the elementary +fact enables us to state the problem in +the form of an equation. It only remains to deduce +from it by combination the observable and +verifiable complex fact. That is what we call +\emph{integration}, and it is the province of the mathematician. +It might be asked, why in physical +science generalisation so readily takes the +mathematical form. The reason is now easy to +see. It is not only because we have to express +numerical laws; it is because the observable +phenomenon is due to the superposition of a large +number of elementary phenomena which are \emph{all +similar to each other}; and in this way differential +equations are quite naturally introduced. It is +\PageSep{159} +not enough that each elementary phenomenon +should obey simple laws: all those that we have +to combine must obey the same law; then only +is the intervention of mathematics of any use. +Mathematics teaches us, in fact, to combine like +with like. Its object is to divine the result of a +combination without having to reconstruct that +combination element by element. If we have to +repeat the same operation several times, mathematics +enables us to avoid this repetition by telling +the result beforehand by a kind of induction. +This I have explained before in the \hyperref[chapref:I]{chapter on +mathematical reasoning}. But for that purpose +all these operations must be similar; in the contrary +case we must evidently make up our minds +to working them out in full one after the other, +and mathematics will be useless. It is therefore, +thanks to the approximate homogeneity of the +matter studied by physicists, that mathematical +physics came into existence. In the natural +sciences the following conditions are no longer to +be found:---homogeneity, relative independence of +remote parts, simplicity of the elementary fact; +and that is why the student of natural science is +compelled to have recourse to other modes of +generalisation. +\PageSep{160} + + +\Chapter{X.}{The Theories of Modern Physics.} + +\Par{Significance of Physical Theories.}---The ephemeral +nature of scientific theories takes by surprise the +man of the world. Their brief period of prosperity +ended, he sees them abandoned one after another; +he sees ruins piled upon ruins; he predicts that +the theories in fashion to-day will in a short time +succumb in their turn, and he concludes that they +are absolutely in vain. This is what he calls the +\emph{bankruptcy of science}. + +His scepticism is superficial; he does not take +into account the object of scientific theories and +the part they play, or he would understand that +the ruins may be still good for something. No +theory seemed established on firmer ground than +Fresnel's, which attributed light to the movements +of the ether. Then if Maxwell's theory is +to-day preferred, does that mean that Fresnel's +work was in vain? No; for Fresnel's object was +not to know whether there really is an ether, if it +is or is not formed of atoms, if these atoms really +move in this way or that; his object was to +predict optical phenomena. + +This Fresnel's theory enables us to do to-day +\PageSep{161} +as well as it did before Maxwell's time. The +differential equations are always true, they may +be always integrated by the same methods, and +the results of this integration still preserve their +value. It cannot be said that this is reducing +physical theories to simple practical recipes; +these equations express relations, and if the +equations remain true, it is because the relations +preserve their reality. They teach us now, as they +did then, that there is such and such a relation +between this thing and that; only, the something +which we then called \emph{motion}, we now call \emph{electric +current}. But these are merely names of the images +we substituted for the real objects which Nature +will hide for ever from our eyes. The true relations +between these real objects are the only reality we +can attain, and the sole condition is that the same +relations shall exist between these objects as between +the images we are forced to put in their place. If +the relations are known to us, what does it matter +if we think it convenient to replace one image by +another? + +That a given periodic phenomenon (an electric +oscillation, for instance) is really due to the +vibration of a given atom, which, behaving like +a pendulum, is really displaced in this manner or +that, all this is neither certain nor essential. +But that there is between the electric oscillation, +the movement of the pendulum, and all periodic +phenomena an intimate relationship which corresponds +to a profound reality; that this relationship, +\PageSep{162} +this similarity, or rather this parallelism, is continued +in the details; that it is a consequence of +more general principles such as that of the conservation +of energy, and that of least action; this +we may affirm; this is the truth which will ever +remain the same in whatever garb we may see fit +to clothe it. + +Many theories of dispersion have been proposed. +The first were imperfect, and contained but little +truth. Then came that of Helmholtz, and this +in its turn was modified in different ways; its +author himself conceived another theory, founded +on Maxwell's principles. But the remarkable +thing is, that all the scientists who followed +Helmholtz obtain the same equations, although +their starting-points were to all appearance widely +separated. I venture to say that these theories +are all simultaneously true; not merely because +they express a true relation---that between absorption +and abnormal dispersion. In the premisses +of these theories the part that is true is the part +common to all: it is the affirmation of this or +that relation between certain things, which some +call by one name and some by another. + +The kinetic theory of gases has given rise to +many objections, to which it would be difficult +to find an answer were it claimed that the theory +is absolutely true. But all these objections do +not alter the fact that it has been useful, +particularly in revealing to us one true relation +which would otherwise have remained profoundly +\PageSep{163} +hidden---the relation between gaseous and osmotic +pressures. In this sense, then, it may be said to +be true. + +When a physicist finds a contradiction between +two theories which are equally dear to him, he +sometimes says: ``Let us not be troubled, but let +us hold fast to the two ends of the chain, lest +we lose the intermediate links.'' This argument +of the embarrassed theologian would be ridiculous +if we were to attribute to physical theories the +interpretation given them by the man of the +world. In case of contradiction one of them at +least should be considered false. But this is no +longer the case if we only seek in them what +should be sought. It is quite possible that they +both express true relations, and that the contradictions +only exist in the images we have formed +to ourselves of reality. To those who feel that +we are going too far in our limitations of the +domain accessible to the scientist, I reply: These +questions which we forbid you to investigate, +and which you so regret, are not only insoluble, +they are illusory and devoid of meaning. + +Such a philosopher claims that all physics can be +explained by the mutual impact of atoms. If he +simply means that the same relations obtain +between physical phenomena as between the +mutual impact of a large number of billiard +balls---well and good!\ this is verifiable, and +perhaps is true. But he means something more, +and we think we understand him, because we +\PageSep{164} +think we know what an impact is. Why? Simply +because we have often watched a game of billiards. +Are we to understand that God experiences the +same sensations in the contemplation of His +work that we do in watching a game of billiards? +If it is not our intention to give his assertion +this fantastic meaning, and if we do not wish +to give it the more restricted meaning I have +already mentioned, which is the sound meaning, +then it has no meaning at all. Hypotheses of +this kind have therefore only a metaphorical sense. +The scientist should no more banish them than a +poet banishes metaphor; but he ought to know +what they are worth. They may be useful to +give satisfaction to the mind, and they will do +no harm as long as they are only indifferent +hypotheses. + +These considerations explain to us why certain +theories, that were thought to be abandoned and +definitively condemned by experiment, are suddenly +revived from their ashes and begin a new life. +It is because they expressed true relations, and +had not ceased to do so when for some reason or +other we felt it necessary to enunciate the same +relations in another language. Their life had been +latent, as it were. + +Barely fifteen years ago, was there anything +more ridiculous, more quaintly old-fashioned, than +the fluids of Coulomb? And yet, here they are +re-appearing under the name of \emph{electrons}. In what +do these permanently electrified molecules differ +\PageSep{165} +from the electric molecules of Coulomb? It is +true that in the electrons the electricity is supported +by a little, a very little matter; in other +words, they have mass. Yet Coulomb did not +deny mass to his fluids, or if he did, it was with +reluctance. It would be rash to affirm that the +belief in electrons will not also undergo an eclipse, +but it was none the less curious to note this unexpected +renaissance. + +But the most striking example is Carnot's +principle. Carnot established it, starting from +false hypotheses. When it was found that heat +was indestructible, and may be converted into +work, his ideas were completely abandoned; +later, Clausius returned to them, and to him is +due their definitive triumph. In its primitive +form, Carnot's theory expressed in addition to +true relations, other inexact relations, the \Foreign{débris} +of old ideas; but the presence of the latter did +not alter the reality of the others. Clausius had +only to separate them, just as one lops off dead +branches. + +The result was the second fundamental law of +\Chg{thermodynamics}{thermo-dynamics}. The relations were always the +same, although they did not hold, at least to all +appearance, between the same objects. This was +sufficient for the principle to retain its value. +Nor have the reasonings of Carnot perished on +this account; they were applied to an imperfect +conception of matter, but their form---\ie, the +essential part of them, remained correct. What +\PageSep{166} +I have just said throws some light at the same +time on the rôle of general principles, such as +those of the principle of least action or of the +conservation of energy. These principles are of +very great value. They were obtained in the +search for what there was in common in the +enunciation of numerous physical laws; they +thus represent the quintessence of innumerable +observations. However, from their very generality +results a consequence to which I have called +attention in \ChapRef{VIII}.---namely, that they are +no longer capable of verification. As we cannot +give a general definition of energy, the principle +of the conservation of energy simply signifies that +there is a \emph{something} which remains constant. +\Pagelabel{166}% +Whatever fresh notions of the world may be +given us by future experiments, we are certain +beforehand that there is something which remains +constant, and which may be called \emph{energy}. Does +this mean that the principle has no meaning and +vanishes into a tautology? Not at all. It means +that the different things to which we give the +name of \emph{energy} are connected by a true relationship; +it affirms between them a real relation. +But then, if this principle has a meaning, it may +be false; it may be that we have no right to +extend indefinitely its applications, and yet it is +certain beforehand to be verified in the strict +sense of the word. How, then, shall we know +when it has been extended as far as is legitimate? +Simply when it ceases to be useful to us---\ie, +\PageSep{167} +when we can no longer use it to predict correctly +new phenomena. We shall be certain in such a +case that the relation affirmed is no longer real, +for otherwise it would be fruitful; experiment +without directly contradicting a new extension of +the principle will nevertheless have condemned it. + +\Par{Physics and Mechanism.}---Most theorists have a +constant predilection for explanations borrowed +from physics, mechanics, or dynamics. Some +would be satisfied if they could account for all +phenomena by the motion of molecules attracting +one another according to certain laws. Others +are more exact: they would suppress attractions +acting at a distance; their molecules would follow +rectilinear paths, from which they would only be +deviated by impacts. Others again, such as Hertz, +suppress the forces as well, but suppose their +molecules subjected to geometrical connections +analogous, for instance, to those of articulated +systems; thus, they wish to reduce dynamics to a +kind of kinematics. In a word, they all wish to +bend nature into a certain form, and unless they +can do this they cannot be satisfied. Is Nature +flexible enough for this? + +We shall examine this question in \ChapRef{XII}., +\Foreign{à propos} of Maxwell's theory. Every time that the +principles of least action and energy are satisfied, +we shall see that not only is there always a +mechanical explanation possible, but that there +is an unlimited number of such explanations. By +means of a well-known theorem due to Königs, +\PageSep{168} +it may be shown that we can explain everything +in an unlimited number of ways, by connections +after the manner of Hertz, or, again, by central +forces. No doubt it may be just as easily demonstrated +that everything may be explained by +simple impacts. For this, let us bear in mind +that it is not enough to be content with the +ordinary matter of which we are aware by means +of our senses, and the movements of which we +observe directly. We may conceive of ordinary +matter as either composed of atoms, whose internal +movements escape us, our senses being able to +estimate only the displacement of the whole; or +we may imagine one of those subtle fluids, which +under the name of \emph{ether} or other names, have +from all time played so important a rôle in +physical theories. Often we go further, and regard +the ether as the only primitive, or even as the +only true matter. The more moderate consider +ordinary matter to be condensed ether, and +there is nothing startling in this conception; but +others only reduce its importance still further, +and see in matter nothing more than the geometrical +locus of singularities in the ether. Lord +Kelvin, for instance, holds what we call matter +to be only the locus of those points at which the +ether is animated by vortex motions. Riemann +believes it to be locus of those points at which +ether is constantly destroyed; to Wiechert or +Larmor, it is the locus of the points at which +the ether has undergone a kind of torsion of a +\PageSep{169} +very particular kind. Taking any one of these +points of view, I ask by what right do we apply +to the ether the mechanical properties observed +in ordinary matter, which is but false matter? +The ancient fluids, caloric, electricity,~etc., were +abandoned when it was seen that heat is not +indestructible. But they were also laid aside +for another reason, In materialising them, their +individuality was, so to speak, emphasised---gaps +were opened between them; and these gaps had +to be filled in when the sentiment of the unity of +Nature became stronger, and when the intimate +relations which connect all the parts were perceived. +In multiplying the fluids, not only did +the ancient physicists create unnecessary entities, +but they destroyed real ties. It is not enough for +a theory not to affirm false relations; it must not +conceal true relations. + +Does our ether actually exist? We know the +origin of our belief in the ether. If light takes +several years to reach us from a distant star, it +is no longer on the star, nor is it on the earth. +It must be somewhere, and supported, so to speak, +by some material agency. + +The same idea may be expressed in a more +mathematical and more abstract form. What we +note are the changes undergone by the material +molecules. We see, for instance, that the photographic +plate experiences the consequences of a +phenomenon of which the incandescent mass of +a star was the scene several years before. Now, +\PageSep{170} +in ordinary mechanics, the state of the system +under consideration depends only on its state at +the moment immediately preceding; the system +therefore satisfies certain differential equations. +On the other hand, if we did not believe in the +ether, the state of the material universe would +depend not only on the state immediately preceding, +but also on much older states; the system +would satisfy equations of finite differences. The +ether was invented to escape this breaking down +of the laws of general mechanics. + +Still, this would only compel us to fill the +interplanetary space with ether, but not to +make it penetrate into the midst of the material +media. Fizeau's experiment goes further. By +the interference of rays which have passed +through the air or water in motion, it seems to +show us two different media penetrating each +other, and yet being displaced with respect to +each other. The ether is all but in our grasp. +Experiments can be conceived in which we come +closer still to it. Assume that Newton's principle +of the equality of action and \Chg{re-action}{reaction} is not true +if applied to matter \emph{alone}, and that this can be +proved. The geometrical sum of all the forces +applied to all the molecules would no longer be +zero. If we did not wish to change the whole of the +science of mechanics, we should have to introduce +the ether, in order that the action which matter +apparently undergoes should be counterbalanced +by the \Chg{re-action}{reaction} of matter on something. +\PageSep{171} + +Or again, suppose we discover that optical and +electrical phenomena are influenced by the motion +of the earth. It would follow that those phenomena +might reveal to us not only the relative +motion of material bodies, but also what would +seem to be their absolute motion. Again, it would +be necessary to have an ether in order that these +so-called absolute movements should not be their +displacements with respect to empty space, but +with respect to something concrete. + +Will this ever be accomplished? I do not +think so, and I shall explain why; and yet, it is +not absurd, for others have entertained this view. +For instance, if the theory of Lorentz, of which I +shall speak in more detail in \ChapRef{XIII}., were +true, Newton's principle would not apply to matter +\emph{alone}, and the difference would not be very far +from being within reach of experiment. On the +other hand, many experiments have been made +on the influence of the motion of the earth. The +results have always been negative. But if these +experiments have been undertaken, it is because +we have not been certain beforehand; and indeed, +according to current theories, the compensation +would be only approximate, and we might expect +to find accurate methods giving positive results. +I think that such a hope is illusory; it was none +the less interesting to show that a success of this +kind would, in a certain sense, open to us a new +world. + +And now allow me to make a digression; I +\PageSep{172} +must explain why I do not believe, in spite of +Lorentz, that more exact observations will ever +make evident anything else but the relative displacements +of material bodies. Experiments have +been made that should have disclosed the terms +of the first order; the results were nugatory. +Could that have been by chance? No one has +admitted this; a general explanation was sought, +and Lorentz found it. He showed that the terms +of the first order should cancel each other, but +not the terms of the second order. Then more +exact experiments were made, which were also +negative; neither could this be the result of +chance. An explanation was necessary, and was +forthcoming; they always are; hypotheses are +what we lack the least. But this is not enough. +Who is there who does not think that this leaves +to chance far too important a rôle? Would it +not also be a chance that this singular concurrence +should cause a certain circumstance to destroy the +terms of the first order, and that a totally different +but very opportune circumstance should cause +those of the second order to vanish? No; the +same explanation must be found for the two +cases, and everything tends to show that this +explanation would serve equally well for the +terms of the higher order, and that the mutual +destruction of these terms will be rigorous and +absolute. + +\Par{The Present State of Physics.}---Two opposite +tendencies may be distinguished in the history +\PageSep{173} +of the development of physics. On the one hand, +new relations are continually being discovered +between objects which seemed destined to remain +for ever unconnected; scattered facts cease to be +strangers to each other and tend to be marshalled +into an imposing synthesis. The march of science +is towards unity and simplicity. + +On the other hand, new phenomena are continually +being revealed; it will be long before +they can be assigned their place---sometimes it +may happen that to find them a place a corner of +the edifice must be demolished. In the same way, +we are continually perceiving details ever more +varied in the phenomena we know, where our +crude senses used to be unable to detect any lack +of unity. What we thought to be simple becomes +complex, and the march of science seems to be +towards diversity and complication. + +Here, then, are two opposing tendencies, each of +which seems to triumph in turn. Which will win? +If the first wins, science is possible; but nothing +proves this \Foreign{à ~priori}, and it may be that after +unsuccessful efforts to bend Nature to our ideal of +unity in spite of herself, we shall be submerged by +the ever-rising flood of our new riches and compelled +to renounce all idea of classification---to +abandon our ideal, and to reduce science to the +mere recording of innumerable recipes. + +In fact, we can give this question no answer. +All that we can do is to observe the science of +to-day, and compare it with that of yesterday. +\PageSep{174} +No doubt after this examination we shall be in a +position to offer a few conjectures. + +Half-a-century ago hopes ran high indeed. The +unity of force had just been revealed to us by the +discovery of the conservation of energy and of its +transformation. This discovery also showed that +the phenomena of heat could be explained by +molecular movements. Although the nature of +these movements was not exactly known, no one +doubted but that they would be ascertained before +long. As for light, the work seemed entirely completed. +So far as electricity was concerned, there +was not so great an advance. Electricity had just +annexed magnetism. This was a considerable and +a definitive step towards unity. But how was +electricity in its turn to be brought into the +general unity, and how was it to be included in +the general universal mechanism? No one had +the slightest idea. As to the possibility of the inclusion, +all were agreed; they had faith. Finally, +as far as the molecular properties of material +bodies are concerned, the inclusion seemed easier, +but the details were very hazy. In a word, hopes +were vast and strong, but vague. + +To-day, what do we see? In the first place, a +step in advance---immense progress. The relations +between light and electricity are now known; the +three domains of light, electricity, and magnetism, +formerly separated, are now one; and this annexation +seems definitive. + +Nevertheless the conquest has caused us some +\PageSep{175} +sacrifices. Optical phenomena become particular +cases in electric phenomena; as long as the former +remained isolated, it was easy to explain them by +movements which were thought to be known in +all their details. That was easy enough; but any +explanation to be accepted must now cover the +whole domain of electricity. This cannot be done +without difficulty. + +The most satisfactory theory is that of Lorentz; +it is unquestionably the theory that best explains +the known facts, the one that throws into relief +the greatest number of known relations, the one in +which we find most traces of definitive construction. +That it still possesses a serious fault I +have shown above. It is in contradiction with +Newton's law that action and \Chg{re-action}{reaction} are equal +and opposite---or rather, this principle according +to Lorentz cannot be applicable to matter alone; +if it be true, it must take into account the action +of the ether on matter, and the \Chg{re-action}{reaction} of the +matter on the ether. Now, in the new order, it is +very likely that things do not happen in this way. + +However this may be, it is due to Lorentz that +the results of Fizeau on the optics of moving +bodies, the laws of normal and abnormal dispersion +and of absorption are connected with +each other and with the other properties of the +ether, by bonds which no doubt will not be +readily severed. Look at the ease with which the +new Zeeman phenomenon found its place, and +even aided the classification of Faraday's magnetic +\PageSep{176} +rotation, which had defied all Maxwell's efforts. +This facility proves that Lorentz's theory is not a +mere artificial combination which must eventually +find its solvent. It will probably have to be +modified, but not destroyed. + +The only object of Lorentz was to include in a +single whole all the optics and electro-dynamics +of moving bodies; he did not claim to give a +mechanical explanation. Larmor goes further; +keeping the essential part of Lorentz's theory, he +grafts upon it, so to speak, MacCullagh's ideas on +the direction of the movement of the ether. +MacCullagh held that the velocity of the ether +is the same in magnitude and direction as the +magnetic force. Ingenious as is this attempt, the +fault in Lorentz's theory remains, and is even +aggravated. According to Lorentz, we do not +know what the movements of the ether are; and +because we do not know this, we may suppose +them to be movements compensating those of +matter, and re-affirming that action and \Chg{re-action}{reaction} +are equal and opposite. According to Larmor +we know the movements of the ether, and we +can prove that the compensation does not take +place. + +If Larmor has failed, as in my opinion he has, +does it necessarily follow that a mechanical explanation +is impossible? Far from it. I said +above that as long as a phenomenon obeys the +two principles of energy and least action, so long +it allows of an unlimited number of mechanical +\PageSep{177} +explanations. And so with the phenomena of +optics and electricity. + +But this is not enough. For a mechanical +explanation to be good it must be simple; to +choose it from among all the explanations that are +possible there must be other reasons than the +necessity of making a choice. Well, we have no +theory as yet which will satisfy this condition and +consequently be of any use. Are we then to +complain? That would be to forget the end we +seek, which is not the mechanism; the true and +only aim is unity. + +We ought therefore to set some limits to +our ambition. Let us not seek to formulate a +mechanical explanation; let us be content to +show that we can always find one if we wish. In +this we have succeeded. The principle of the +conservation of energy has always been confirmed, +and now it has a fellow in the principle of least +action, stated in the form appropriate to physics. +This has also been verified, at least as far as +concerns the reversible phenomena which obey +Lagrange's equations---in other words, which obey +the most general laws of physics. The irreversible +phenomena are much more difficult to bring into +line; but they, too, are being co-ordinated and +tend to come into the unity. The light which +illuminates them comes from Carnot's principle. +For a long time thermo-dynamics was confined to +the study of the dilatations of bodies and of their +change of state. For some time past it has been +\PageSep{178} +growing bolder, and has considerably extended its +domain. We owe to it the theories of the voltaic +cell and of their thermo-electric phenomena; there +is not a corner in physics which it has not explored, +and it has even attacked chemistry itself. +The same laws hold good; everywhere, disguised +in some form or other, we find Carnot's principle; +everywhere also appears that eminently abstract +concept of entropy which is as universal as the +concept of energy, and like it, seems to conceal a +reality. It seemed that radiant heat must escape, +but recently that, too, has been brought under the +same laws. + +In this way fresh analogies are revealed which +may be often pursued in detail; electric resistance +resembles the viscosity of fluids; hysteresis would +rather be like the friction of solids. In all cases +friction appears to be the type most imitated by +the most diverse irreversible phenomena, and this +relationship is real and profound. + +A strictly mechanical explanation of these +phenomena has also been sought, but, owing to +their nature, it is hardly likely that it will be +found. To find it, it has been necessary to +suppose that the irreversibility is but apparent, that +the elementary phenomena are reversible and obey +the known laws of dynamics. But the elements +are extremely numerous, and become blended +more and more, so that to our crude sight all +appears to tend towards uniformity---\ie, all seems +to progress in the same direction, and that without +\PageSep{179} +hope of return. The apparent irreversibility is +therefore but an effect of the law of great numbers. +Only a being of infinitely subtle senses, such as +Maxwell's demon, could unravel this tangled skein +and turn back the course of the universe. + +This conception, which is connected with the +kinetic theory of gases, has cost great effort and +has not, on the whole, been fruitful; it may +become so. This is not the place to examine if it +leads to contradictions, and if it is in conformity +with the true nature of things. + +Let us notice, however, the original ideas of +M.~Gouy on the Brownian movement. According +to this scientist, this singular movement does not +obey Carnot's principle. The particles which it sets +moving would be smaller than the meshes of that +tightly drawn net; they would thus be ready to +separate them, and thereby to set back the course +of the universe. One can almost see Maxwell's +demon at work.\footnote + {Clerk-Maxwell imagined some supernatural agency at work, + sorting molecules in a gas of uniform temperature into (\textit{a})~those + possessing kinetic energy above the average, (\textit{b})~those possessing + kinetic energy below the average.\Transl} + +To resume, phenomena long known are gradually +being better classified, but new phenomena come +to claim their place, and most of them, like the +Zeeman effect, find it at once. Then we have the +cathode rays, the X-rays, uranium and radium +rays; in fact, a whole world of which none had +suspected the existence. How many unexpected +\PageSep{180} +guests to find a place for! No one can yet predict +the place they will occupy, but I do not believe +they will destroy the general unity: I think that +they will rather complete it. On the one hand, +indeed, the new radiations seem to be connected +with the phenomena of luminosity; not only do +they excite fluorescence, but they sometimes come +into existence under the same conditions as that +property; neither are they unrelated to the cause +which produces the electric spark under the action +of ultra-violet light. Finally, and most important +of all, it is believed that in all these phenomena +there exist ions, animated, it is true, with velocities +far greater than those of electrolytes. All this is +very vague, but it will all become clearer. + +Phosphorescence and the action of light on the +spark were regions rather isolated, and consequently +somewhat neglected by investigators. It is to be +hoped that a new path will now be made which +will facilitate their communications with the +rest of science. Not only do we discover new +phenomena, but those we think we know are +revealed in unlooked-for aspects. In the free ether +the laws preserve their majestic simplicity, but +matter properly so called seems more and more +complex; all we can say of it is but approximate, +and our formulæ are constantly requiring new +terms. + +But the ranks are unbroken, the relations that +we have discovered between objects we thought +simple still hold good between the same objects +\PageSep{181} +when their complexity is recognised, and that +alone is the important thing. Our equations +become, it is true, more and more complicated, so +as to embrace more closely the complexity of +nature; but nothing is changed in the relations +which enable these equations to be derived from +each other. In a word, the form of these equations +persists. Take for instance the laws of reflection. +Fresnel established them by a simple and attractive +theory which experiment seemed to confirm. Subsequently, +more accurate researches have shown +that this verification was but approximate; traces +of elliptic polarisation were detected everywhere. +But it is owing to the first approximation that the +cause of these anomalies was found in the existence +of a transition layer, and all the essentials of +Fresnel's theory have remained. We cannot help +reflecting that all these relations would never have +been noted if there had been doubt in the first +place as to the complexity of the objects they +connect. Long ago it was said: If Tycho had had +instruments ten times as precise, we would never +have had a Kepler, or a Newton, or Astronomy. +It is a misfortune for a science to be born too late, +when the means of observation have become too +perfect. That is what is happening at this moment +with respect to physical chemistry; the founders +are hampered in their general grasp by third and +fourth decimal places; happily they are men of +robust faith. As we get to know the properties +of matter better we see that continuity reigns. +\PageSep{182} +From the work of Andrews and Van~der~Waals, +we see how the transition from the liquid to the +gaseous state is made, and that it is not abrupt. +Similarly, there is no gap between the liquid and +solid states, and in the proceedings of a recent +Congress we see memoirs on the rigidity of liquids +side by side with papers on the flow of solids. + +With this tendency there is no doubt a loss of +simplicity. Such and such an effect was represented +by straight lines; it is now necessary to connect +these lines by more or less complicated curves. +On the other hand, unity is gained. Separate +categories quieted but did not satisfy the mind. + +Finally, a new domain, that of chemistry, has +been invaded by the method of physics, and we see +the birth of physical chemistry. It is still quite +young, but already it has enabled us to connect +such phenomena as electrolysis, osmosis, and the +movements of ions. + +From this cursory exposition what can we conclude? +Taking all things into account, we have +approached the realisation of unity. This has not +been done as quickly as was hoped fifty years ago, +and the path predicted has not always been +followed; but, on the whole, much ground has +been gained. +\PageSep{183} + + +\Chapter{XI.}{The Calculus of Probabilities.} + +\First{No} doubt the reader will be astonished to find +reflections on the calculus of probabilities in such +a volume as this. What has that calculus to do +with physical science? The questions I shall raise---without, +however, giving them a solution---are +naturally raised by the philosopher who is examining +the problems of physics. So far is this the case, +that in the two preceding chapters I have several +times used the words ``probability'' and ``chance.'' +``Predicted facts,'' as I said above, ``can only be +probable.'' However solidly founded a prediction +may appear to be, we are never absolutely +certain that experiment will not prove it false; but +the probability is often so great that practically +it may be accepted. And a little farther on I +added:---``See what a part the belief in simplicity +plays in our generalisations. We have verified a +simple law in a large number of particular cases, +and we refuse to admit that this so-often-repeated +coincidence is a mere effect of chance.'' Thus, in a +multitude of circumstances the physicist is often +in the same position as the gambler who reckons +up his chances. Every time that he reasons by +\PageSep{184} +induction, he more or less consciously requires the +calculus of probabilities, and that is why I am +obliged to open this chapter parenthetically, and to +interrupt our discussion of method in the physical +sciences in order to examine a little closer what this +calculus is worth, and what dependence we may +place upon it. The very name of the calculus of +probabilities is a paradox. Probability as opposed +to certainty is what one does not know, and how +can we calculate the unknown? Yet many eminent +scientists have devoted themselves to this calculus, +and it cannot be denied that science has drawn therefrom +no small advantage. How can we explain +this apparent contradiction? Has probability been +defined? Can it even be defined? And if it cannot, +how can we venture to reason upon it? The +definition, it will be said, is very simple. The +probability of an event is the ratio of the number +of cases favourable to the event to the total number +of possible cases. A simple example will show how +incomplete this definition is:---I throw two dice. +What is the probability that one of the two +at least turns up a~6? Each can turn up in six +different ways; the number of possible cases is +$6 × 6 = 36$. The number of favourable cases is~$11$; +the probability is~$\dfrac{11}{36}$. That is the correct solution. +But why cannot we just as well proceed as follows?---The +points which turn up on the two dice form +$\dfrac{6 × 7}{2} = 21$ different combinations. Among these +combinations, six are favourable; the probability +\PageSep{185} +is~$\dfrac{6}{21}$. Now why is the first method of calculating +the number of possible cases more legitimate than +the second? In any case it is not the definition +that tells us. We are therefore bound to complete +the definition by saying, ``\ldots to the total number +of possible cases, provided the cases are equally +probable.'' So we are compelled to define the +probable by the probable. How can we know +that two possible cases are equally probable? +Will it be by a convention? If we insert at the +beginning of every problem an explicit convention, +well and good! We then have nothing to do but to +apply the rules of arithmetic and algebra, and we +complete our calculation, when our result cannot +be called in question. But if we wish to make the +slightest application of this result, we must prove +that our convention is legitimate, and we shall find +ourselves in the presence of the very difficulty we +thought we had avoided. It may be said that +common-sense is enough to show us the convention +that should be adopted. Alas! M.~Bertrand has +amused himself by discussing the following simple +problem:---``What is the probability that a chord +of a circle may be greater than the side of the +inscribed equilateral triangle?'' The illustrious +geometer successively adopted two conventions +which seemed to be equally imperative in the eyes +of common-sense, and with one convention he finds~$\frac{1}{2}$, +and with the other~$\frac{1}{3}$. The conclusion which +seems to follow from this is that the calculus of +probabilities is a useless science, that the obscure +\PageSep{186} +instinct which we call common-sense, and to which +we appeal for the legitimisation of our conventions, +must be distrusted. But to this conclusion we can +no longer subscribe. We cannot do without that +obscure instinct. Without it, science would be +impossible, and without it we could neither discover +nor apply a law. Have we any right, for instance, +to enunciate Newton's law? No doubt numerous +observations are in agreement with it, but is not +that a simple fact of chance? and how do we know, +besides, that this law which has been true for so +many generations will not be untrue in the next? +To this objection the only answer you can give is: +It is very improbable. But grant the law. By +means of it I can calculate the position of Jupiter +in a year from now. Yet have I any right to say +this? Who can tell if a gigantic mass of enormous +velocity is not going to pass near the solar system +and produce unforeseen perturbations? Here +again the only answer is: It is very improbable. +From this point of view all the sciences would only +be unconscious applications of the calculus of probabilities. +And if this calculus be condemned, then +the whole of the sciences must also be condemned. +I shall not dwell at length on scientific problems +in which the intervention of the calculus of probabilities +is more evident. In the forefront of these +is the problem of interpolation, in which, knowing +a certain number of values of a function, we try +to discover the intermediary values. I may also +mention the celebrated theory of errors of observation, +\PageSep{187} +to which I shall return later; the kinetic +theory of gases, a well-known hypothesis wherein +each gaseous molecule is supposed to describe an +extremely complicated path, but in which, through +the effect of great numbers, the mean phenomena +which are all we observe obey the simple laws of +Mariotte and Gay-Lussac. All these theories are +based upon the laws of great numbers, and the +calculus of probabilities would evidently involve +them in its ruin. It is true that they have only a +particular interest, and that, save as far as interpolation +is concerned, they are sacrifices to which +we might readily be resigned. But I have said +above, it would not be these partial sacrifices that +would be in question; it would be the legitimacy +of the whole of science that would be challenged. +I quite see that it might be said: We do not know, +and yet we must act. As for action, we have not +time to devote ourselves to an inquiry that will +suffice to dispel our ignorance. Besides, such an +inquiry would demand unlimited time. We must +therefore make up our minds without knowing. +This must be often done whatever may happen, +and we must follow the rules although we may +have but little confidence in them. What I know +is, not that such a thing is true, but that the best +course for me is to act as if it were true. The +calculus of probabilities, and therefore science +itself, would be no longer of any practical value. + +Unfortunately the difficulty does not thus disappear. +A gambler wants to try a \Foreign{coup}, and he +\PageSep{188} +asks my advice. If I give it him, I use the +calculus of probabilities; but I shall not guarantee +success. That is what I shall call \emph{subjective probability}. +In this case we might be content with the +explanation of which I have just given a sketch. +But assume that an observer is present at the play, +that he knows of the \Foreign{coup}, and that play goes +on for a long time, and that he makes a summary +of his notes. He will find that events have +taken place in conformity with the laws of the +calculus of probabilities. That is what I shall call +\emph{objective probability}, and it is this phenomenon +which has to be explained. There are numerous +Insurance Societies which apply the rules of the +calculus of probabilities, and they distribute to +their shareholders dividends, the objective reality +of which cannot be contested. In order to explain +them, we must do more than invoke our ignorance +and the necessity of action. Thus, absolute scepticism +is not admissible. We may distrust, but we +cannot condemn \Foreign{en~bloc}. Discussion is necessary. + +\Par[I. ]{Classification of the Problems of Probability.}---In +order to classify the problems which are presented +to us with reference to probabilities, we must look at +them from different points of view, and first of all, +from that of \emph{generality}. I said above that probability +is the ratio of the number of favourable to +the number of possible cases. What for want of a +better term I call generality will increase with the +number of possible cases. This number may be +finite, as, for instance, if we take a throw of the +\PageSep{189} +dice in which the number of possible cases is~$36$. +That is the first degree of generality. But if we +ask, for instance, what is the probability that a +point within a circle is within the inscribed square, +there are as many possible cases as there are points +in the circle---that is to say, an infinite number. +This is the second degree of generality. Generality +can be pushed further still. We may ask the probability +that a function will satisfy a given condition. +There are then as many possible cases as one +can imagine different functions. This is the third +degree of generality, which we reach, for instance, +when we try to find the most probable law after a +finite number of observations. Yet we may place +ourselves at a quite different point of view. If we +were not ignorant there would be no probability, +there could only be certainty. But our ignorance +cannot be absolute, for then there would be no +longer any probability at all. Thus the problems +of probability may be classed according to the +greater or less depth of this ignorance. In mathematics +we may set ourselves problems in probability. +What is the probability that the fifth +decimal of a logarithm taken at random from a +table is a~$9$. There is no hesitation in answering +%[** TN: French edition uses a fraction] +that this probability is~\Reword{$1$-$10$th}{$\frac{1}{10}$}. Here we possess +all the data of the problem. We can calculate +our logarithm without having recourse to the +table, but we need not give ourselves the trouble. +This is the first degree of ignorance. In the +physical sciences our ignorance is already greater. +\PageSep{190} +The state of a system at a given moment depends +on two things---its initial state, and the law +according to which that state varies. If we know +both this law and this initial state, we have a +simple mathematical problem to solve, and we +fall back upon our first degree of ignorance. +Then it often happens that we know the law +and do not know the initial state. It may be +asked, for instance, what is the present distribution +of the minor planets? We know that from +all time they have obeyed the laws of Kepler, +but we do not know what was their initial distribution. +In the kinetic theory of gases we +assume that the gaseous molecules follow rectilinear +paths and obey the laws of impact and +elastic bodies; yet as we know nothing of their +initial velocities, we know nothing of their present +velocities. The calculus of probabilities alone +enables us to predict the mean phenomena which +will result from a combination of these velocities. +This is the second degree of ignorance. Finally +it is possible, that not only the initial conditions +but the laws themselves are unknown. We then +reach the third degree of ignorance, and in general +we can no longer affirm anything at all as to the +probability of a phenomenon. It often happens +that instead of trying to discover an event by +means of a more or less imperfect knowledge of +the law, the events may be known, and we want +to find the law; or that, instead of deducing +effects from causes, we wish to deduce the causes +\PageSep{191} +from the effects. Now, these problems are classified +as \emph{probability of causes}, and are the most interesting +of all from their scientific applications. I play at +\Foreign{écarté} with a gentleman whom I know to be perfectly +honest. What is the chance that he turns +up the king? It is~$\frac{1}{8}$. This is a problem of the +probability of effects. I play with a gentleman +whom I do not know. He has dealt ten times, +and he has turned the king up six times. What +is the chance that he is a sharper? This is a +problem in the probability of causes. It may be +said that it is the essential problem of the experimental +method. I have observed $n$~values of~$x$ +and the corresponding values of~$y$. I have found +that the ratio of the latter to the former is practically +constant. There is the event; what is +the cause? Is it probable that there is a general +law according to which $y$~would be proportional +to~$x$, and that small divergencies are due to errors +of observation? This is the type of question that +we are ever asking, and which we unconsciously +solve whenever we are engaged in scientific work. +I am now going to pass in review these different +categories of problems by discussing in succession +what I have called subjective and objective probability. + +\Par[II. ]{Probability in Mathematics.}---The impossibility +of squaring the circle was shown in~1885, but +before that date all geometers considered this impossibility +as so ``probable'' that the Académie des +Sciences rejected without examination the, alas!\ +\PageSep{192} +too numerous memoirs on this subject that a +few unhappy madmen sent in every year. Was +the Académie wrong? Evidently not, and it +knew perfectly well that by acting in this +manner it did not run the least risk of stifling +a discovery of moment. The Académie could +not have proved that it was right, but it knew +quite well that its instinct did not deceive it. +If you had asked the Academicians, they would +have answered: ``We have compared the probability +that an unknown scientist should have +found out what has been vainly sought for so +long, with the probability that there is one madman +the more on the earth, and the latter has +appeared to us the greater.'' These are very +good reasons, but there is nothing mathematical +about them; they are purely psychological. If +you had pressed them further, they would have +added: ``Why do you expect a particular value of +a transcendental function to be an algebraical +number; if $\pi$~be the root of an algebraical equation, +why do you expect this root to be a period of +%[** TN: sin italicized in the original] +the function~$\sin 2x$, and why is it not the same +with the other roots of the same equation?'' To +sum up, they would have invoked the principle of +sufficient reason in its vaguest form. Yet what +information could they draw from it? At most a +rule of conduct for the employment of their time, +which would be more usefully spent at their +ordinary work than in reading a lucubration +that inspired in them a legitimate distrust. But +\PageSep{193} +what I called above objective probability has +nothing in common with this first problem. It is +otherwise with the second. Let us consider the +first $10,000$ logarithms that we find in a table. +Among these $10,000$ logarithms I take one at +random. What is the probability that its third +decimal is an even number? You will say without +any hesitation that the probability is~$\frac{1}{2}$, and in +fact if you pick out in a table the third decimals +in these $10,000$ numbers you will find nearly as +many even digits as odd. Or, if you prefer it, let +us write $10,000$ numbers corresponding to our +$10,000$ logarithms, writing down for each of these +numbers $+1$~if the third decimal of the corresponding +logarithm is even, and $-1$~if odd; and then +let us take the mean of these $10,000$ numbers. I +do not hesitate to say that the mean of these +$10,000$ units is probably zero, and if I were to +calculate it practically, I would verify that it is +extremely small. But this verification is needless. +I might have rigorously proved that this mean is +smaller than~$0.003$. To prove this result I should +have had to make a rather long calculation for +which there is no room here, and for which I +may refer the reader to an article that I published +in the \Title{Revue générale des Sciences}, April~15th, +1899. The only point to which I wish to +draw attention is the following. In this calculation +I had occasion to rest my case on only two +facts---namely, that the first and second derivatives +of the logarithm remain, in the interval considered, +\PageSep{194} +between certain limits. Hence our first conclusion +is that the property is not only true of the +logarithm but of any continuous function whatever, +since the derivatives of every continuous +function are limited. If I was certain beforehand +of the result, it is because I have often observed +analogous facts for other continuous functions; and +next, it is because I went through in my mind in +a more or less unconscious and imperfect manner +the reasoning which led me to the preceding inequalities, +just as a skilled calculator before finishing +his multiplication takes into account what it +ought to come to approximately. And besides, +since what I call my intuition was only an incomplete +summary of a piece of true reasoning, it is +clear that observation has confirmed my predictions, +and that the objective and subjective probabilities +are in agreement. As a third example I shall +choose the following:---The number~$u$ is taken at +random and $n$~is a given very large integer. What +is the mean value of~$\sin nu$? This problem has +no meaning by itself. To give it one, a convention +is required---namely, we agree that the probability +for the number~$u$ to lie between $a$~and~$a + da$ is +$\phi(a)\, da$; that it is therefore proportional to the +infinitely small interval~$da$, and is equal to this +multiplied by a function~$\phi(a)$, only depending +on~$a$. As for this function I choose it arbitrarily, +but I must assume it to be continuous. The value +of~$\sin nu$ remaining the same when $u$~increases by~$2\pi$, +I may without loss of generality assume that +\PageSep{195} +$u$~lies between $0$~and~$2\pi$, and I shall thus be +led to suppose that $\phi(a)$~is a periodic function +whose period is~$2\pi$. The mean value that we +seek is readily expressed by a simple integral, +and it is easy to show that this integral is smaller +than +%[** TN: Expression displayed in the French edition] +\[ +\frac{2\pi M_{K}}{n^{K}}, +\] +$M_{K}$~being the maximum value of the +$K$th~derivative of~$\phi(u)$. We see then that if the +$K$th~derivative is finite, our mean value will +tend towards zero when $n$~increases indefinitely, +and that more rapidly than~$\dfrac{1}{n^{K+1}}$. + +%[** TN: Paragraph break in the French edition] +The mean +value of~$\sin nu$ when $n$~is very large is therefore +zero. To define this value I required a convention, +but the result remains the same \emph{whatever +that convention may be}. I have imposed upon +myself but slight restrictions when I assumed that +the function~$\phi(a)$ is continuous and periodic, and +these hypotheses are so natural that we may ask +ourselves how they can be escaped. Examination +of the three preceding examples, so different in all +respects, has already given us a glimpse on the +one hand of the rôle of what philosophers call the +principle of sufficient reason, and on the other hand +of the importance of the fact that certain properties +are common to all continuous functions. +The study of probability in the physical sciences +will lead us to the same result. + +\Par[III. ]{Probability in the Physical Sciences.}---We +now come to the problems which are connected +with what I have called the second degree of +\PageSep{196} +ignorance---namely, those in which we know the +law but do not know the initial state of the +system. I could multiply examples, but I shall +take only one. What is the probable present +distribution of the minor planets on the zodiac? +We know they obey the laws of Kepler. We may +even, without changing the nature of the problem, +suppose that their orbits are circular and situated +in the same plane, a plane which we are given. +On the other hand, we know absolutely nothing +about their initial distribution. However, we do +not hesitate to affirm that this distribution is now +nearly uniform. Why? Let $b$~be the longitude +of a minor planet in the initial epoch---that is to +say, the epoch zero. Let $a$~be its mean motion. +Its longitude at the present time---\ie, at the time~$t$ +will be~$at + b$. To say that the present distribution +is uniform is to say that the mean value of +the sines and cosines of multiples of~$at + b$ is zero. +Why do we assert this? Let us represent our +minor planet by a point in a plane---namely, the +point whose co-ordinates are $a$~and~$b$. All these +representative points will be contained in a certain +region of the plane, but as they are very numerous +this region will appear dotted with points. We +know nothing else about the distribution of the +points. Now what do we do when we apply the +calculus of probabilities to such a question as +this? What is the probability that one or more +representative points may be found in a certain +portion of the plane? In our ignorance we are +\PageSep{197} +compelled to make an arbitrary hypothesis. To +explain the nature of this hypothesis I may be +allowed to use, instead of a mathematical formula, +a crude but concrete image. Let us suppose +that over the surface of our plane has been +spread imaginary matter, the density of which is +variable, but varies continuously. We shall then +agree to say that the probable number of representative +points to be found on a certain portion +of the plane is proportional to the quantity of +this imaginary matter which is found there. If +there are, then, two regions of the plane of the +same extent, the probabilities that a representative +point of one of our minor planets is in one or +other of these regions will be as the mean densities +of the imaginary matter in one or other of the +regions. Here then are two distributions, one +real, in which the representative points are very +numerous, very close together, but discrete like the +molecules of matter in the atomic hypothesis; the +other remote from reality, in which our representative +points are replaced by imaginary continuous +matter. We know that the latter cannot be real, +but we are forced to adopt it through our ignorance. +If, again, we had some idea of the real distribution +of the representative points, we could arrange it so +that in a region of some extent the density of this +imaginary continuous matter may be nearly proportional +to the number of representative points, +or, if it is preferred, to the number of atoms which +are contained in that region. Even that is impossible, +\PageSep{198} +and our ignorance is so great that we are +forced to choose arbitrarily the function which +defines the density of our imaginary matter. We +shall be compelled to adopt a hypothesis from +which we can hardly get away; we shall suppose +that this function is continuous. That is +sufficient, as we shall see, to enable us to reach our +conclusion. + +What is at the instant~$t$ the probable distribution +of the minor planets---or rather, what is the +mean value of the sine of the longitude at the +moment~$t$---\ie, of $\sin(at + b)$? We made at the +outset an arbitrary convention, but if we adopt it, +this probable value is entirely defined. Let us +decompose the plane into elements of surface. +Consider the value of $\sin(at + b)$ at the centre of +each of these elements. Multiply this value by the +surface of the element and by the corresponding +density of the imaginary matter. Let us then take +the sum for all the elements of the plane. This +sum, by definition, will be the probable mean +value we seek, which will thus be expressed by a +double integral. It may be thought at first that +this mean value depends on the choice of the +function~$\phi$ which defines the density of the imaginary +matter, and as this function~$\phi$ is arbitrary, we +can, according to the arbitrary choice which we +make, obtain a certain mean value. But this is +not the case. A simple calculation shows us that +our double integral decreases very rapidly as $t$~increases. +Thus, I cannot tell what hypothesis to +\PageSep{199} +make as to the probability of this or that initial +distribution, but when once the hypothesis is +made the result will be the same, and this gets +me out of my difficulty. Whatever the function~$\phi$ +may be, the mean value tends towards zero +as $t$~increases, and as the minor planets have +certainly accomplished a very large number of +revolutions, I may assert that this mean value is +very small. I may give to~$\phi$ any value I choose, +with one restriction: this function must be continuous; +and, in fact, from the point of view of +subjective probability, the choice of a discontinuous +function would have been unreasonable. What +reason could I have, for instance, for supposing +that the initial longitude might be exactly~$0°$, but +that it could not lie between $0°$~and~$1°$? + +The difficulty reappears if we look at it from the +point of view of objective probability; if we pass +from our imaginary distribution in which the supposititious +matter was assumed to be continuous, +to the real distribution in which our representative +points are formed as discrete atoms. The mean +value of $\sin(at + b)$ will be represented quite +simply by +\[ +\frac{1}{n} \sum \sin(at + b), +\] +$n$~being the number of minor planets. Instead of +a double integral referring to a continuous +function, we shall have a sum of discrete terms. +However, no one will seriously doubt that this +mean value is practically very small. Our representative +\PageSep{200} +points being very close together, our +discrete sum will in general differ very little from +an integral. An integral is the limit towards +which a sum of terms tends when the number of +these terms is indefinitely increased. If the terms +are very numerous, the sum will differ very little +from its limit---that is to say, from the integral, +and what I said of the latter will still be true of +the sum itself. But there are exceptions. If, for +instance, for all the minor planets $b = \dfrac{\pi}{2} - at$, the +longitude of all the planets at the time~$t$ would be~$\dfrac{\pi}{2}$, +and the mean value in question would be +evidently unity. For this to be the case at the +time~$0$, the minor planets must have all been +lying on a kind of spiral of peculiar form, with +its spires very close together. All will admit that +such an initial distribution is extremely improbable +(and even if it were realised, the distribution +would not be uniform at the present time---for +example, on the 1st~January 1900; but it would +become so a few years later). Why, then, do we +think this initial distribution improbable? This +must be explained, for if we are wrong in rejecting +as improbable this absurd hypothesis, our inquiry +breaks down, and we can no longer affirm anything +on the subject of the probability of this or +that present distribution. Once more we shall +invoke the principle of sufficient reason, to which +we must always recur. We might admit that at +the beginning the planets were distributed almost +\PageSep{201} +in a straight line. We might admit that they +were irregularly distributed. But it seems to us +that there is no sufficient reason for the unknown +cause that gave them birth to have acted along a +curve so regular and yet so complicated, which +would appear to have been expressly chosen so +that the distribution at the present day would not +be uniform. + +\Par[IV. ]{Rouge et Noir.}---The questions raised by +games of chance, such as roulette, are, fundamentally, +quite analogous to those we have just +%[** TN: "est partagé en un grand mombre de subdivisions égales"] +treated. For example, a wheel is divided into \Reword{thirty-seven}{a large number of} +equal compartments, alternately red and +black. A ball is spun round the wheel, and after +having moved round a number of times, it stops in +front of one of these sub-divisions. The probability +that the division is red is obviously~$\frac{1}{2}$. The needle +describes an angle~$\theta$, including several complete +revolutions. I do not know what is the probability +that the ball is spun with such a force that +this angle should lie between $\theta$~and~$\theta + d\theta$, but I +can make a convention. I can suppose that this +probability is~$\phi(\theta)\, d\theta$. As for the function~$\phi(\theta)$, I +can choose it in an entirely arbitrary manner. I +have nothing to guide me in my choice, but I am +naturally induced to suppose the function to be +continuous. Let $\epsilon$~be a length (measured on the +circumference of the circle of radius unity) of each +red and black compartment. We have to calculate +the integral of~$\phi(\theta)\, d\theta$, extending it on the one +hand to all the red, and on the other hand to all +\PageSep{202} +the black compartments, and to compare the +results. Consider an interval~$2\epsilon$ comprising two +consecutive red and black compartments. Let +$M$~and~$m$ be the maximum and minimum values of +the function~$\phi(\theta)$ in this interval. The integral +extended to the red compartments will be smaller +than~$\sum M\epsilon$; extended to the black it will be greater +than~$\sum m\epsilon$. The difference will therefore be +smaller than $\sum (M - m)\epsilon$. But if the function~$\phi$ is +supposed continuous, and if on the other hand the +interval~$\epsilon$ is very small with respect to the total +angle described by the needle, the difference~$M - m$ +will be very small. The difference of the two +integrals will be therefore very small, and the +probability will be very nearly~$\frac{1}{2}$. We see that +without knowing anything of the function~$\phi$ we +must act as if the probability were~$\frac{1}{2}$. And on +the other hand it explains why, from the +objective point of view, if I watch a certain +number of \Foreign{coups}, observation will give me almost +as many black \Foreign{coups} as red. All the players +know this objective law; but it leads them into a +remarkable error, which has often been exposed, +but into which they are always falling. When +the red has won, for example, six times running, +they bet on black, thinking that they are playing +an absolutely safe game, because they say it is +a very rare thing for the red to win seven times +running. In reality their probability of winning +is still~$\frac{1}{2}$. Observation shows, it is true, that +the series of seven consecutive reds is very rare, +\PageSep{203} +but series of six reds followed by a black are +also very rare. They have noticed the rarity of +the series of seven reds; if they have not remarked +the rarity of six reds and a black, it is only +because such series strike the attention less. + +\Par[V. ]{The Probability of Causes.}---We now come to +the problems of the probability of causes, the +most important from the point of view of +scientific applications. Two stars, for instance, +are very close together on the celestial sphere. Is +this apparent contiguity a mere effect of chance? +Are these stars, although almost on the same +visual ray, situated at very different distances +from the earth, and therefore very far indeed from +one another? or does the apparent correspond +to a real contiguity? This is a problem on the +probability of causes. + +First of all, I recall that at the outset of all +problems of probability of effects that have +occupied our attention up to now, we have had +to use a convention which was more or less +justified; and if in most cases the result was to +a certain extent independent of this convention, +it was only the condition of certain hypotheses +which enabled us \Foreign{à ~priori} to reject discontinuous +functions, for example, or certain absurd conventions. +We shall again find something +analogous to this when we deal with the probability +of causes. An effect may be produced +by the cause~$a$ or by the cause~$b$. The effect +has just been observed. We ask the probability +\PageSep{204} +that it is due to the cause~$a$. This is an \Foreign{à ~posteriori} +probability of cause. But I could not +calculate it, if a convention more or less justified +did not tell me in advance what is the \Foreign{à ~priori} +probability for the cause~$a$ to come into play---I +mean the probability of this event to some one +who had not observed the effect. To make my +meaning clearer, I go back to the game of \Foreign{écarté} +mentioned before. My adversary deals for the +first time and turns up a king. What is the +probability that he is a sharper? The formulæ +ordinarily taught give~$\frac{8}{9}$, a result which is +obviously rather surprising. If we look at it +closer, we see that the conclusion is arrived at +as if, before sitting down at the table, I had +considered that there was one chance in two +that my adversary was not honest. An absurd +hypothesis, because in that case I should certainly +not have played with him; and this explains the +absurdity of the conclusion. The function on +the \Foreign{à ~priori} probability was unjustified, and that +is why the conclusion of the \Foreign{à ~posteriori} probability +led me into an inadmissible result. The importance +of this preliminary convention is obvious. +I shall even add that if none were made, the +problem of the \Foreign{à ~posteriori} probability would have +no meaning. It must be always made either +explicitly or tacitly. + +Let us pass on to an example of a more +scientific character. I require to determine an +experimental law; this law, when discovered, can +\PageSep{205} +be represented by a curve. I make a certain +number of isolated observations, each of which +may be represented by a point. When I have +obtained these different points, I draw a curve +between them as carefully as possible, giving +my curve a regular form, avoiding sharp angles, +accentuated inflexions, and any sudden variation +of the radius of curvature. This curve will represent +to me the probable law, and not only will +it give me the values of the functions intermediary +to those which have been observed, but it also +gives me the observed values more accurately +than direct observation does; that is why I make +the curve pass near the points and not through +the points themselves. + +Here, then, is a problem in the probability of +causes. The effects are the measurements I have +recorded; they depend on the combination of two +causes---the true law of the phenomenon and errors +of observation. Knowing the effects, we have to +find the probability that the phenomenon shall +obey this law or that, and that the observations +have been accompanied by this or that error. +The most probable law, therefore, corresponds to +the curve we have traced, and the most probable +error is represented by the distance of the corresponding +point from that curve. But the +problem has no meaning if before the observations +I had an \Foreign{à ~priori} idea of the probability of +this law or that, or of the chances of error to +which I am exposed. If my instruments are +\PageSep{206} +good (and I knew whether this is so or not before +beginning the observations), I shall not draw the +curve far from the points which represent the +rough measurements. If they are inferior, I may +draw it a little farther from the points, so that I +may get a less sinuous curve; much will be sacrificed +to regularity. + +Why, then, do I draw a curve without sinuosities? +Because I consider \Foreign{à ~priori} a law +represented by a continuous function (or function +the derivatives of which to a high order are small), +as more probable than a law not satisfying those +conditions. But for this conviction the problem +would have no meaning; interpolation would be +impossible; no law could be deduced from a +finite number of observations; science would +cease to exist. + +Fifty years ago physicists considered, other +things being equal, a simple law as more probable +than a complicated law. This principle was even +invoked in favour of Mariotte's law as against +that of Regnault. But this belief is now +repudiated; and yet, how many times are we +compelled to act as though we still held it! +However that may be, what remains of this +tendency is the belief in continuity, and as we +have just seen, if the belief in continuity were +to disappear, experimental science would become +impossible. + +\Par[VI. ]{The Theory of Errors.}---We are thus brought +to consider the theory of errors which is directly +\PageSep{207} +connected with the problem of the probability +of causes. Here again we find \emph{effects}---to wit, +a certain number of irreconcilable observations, +and we try to find the \emph{causes} which are, on the +one hand, the true value of the quantity to be +measured, and, on the other, the error made in +each isolated observation. We must calculate +the probable \Foreign{à ~posteriori} value of each error, and +therefore the probable value of the quantity to be +measured. But, as I have just explained, we +cannot undertake this calculation unless we admit +\Foreign{à ~priori}---\ie, before any observations are made---that +there is a law of the probability of errors. +Is there a law of errors? The law to which +all calculators assent is Gauss's law, that is +represented by a certain transcendental curve +known as the ``bell.'' + +But it is first of all necessary to recall +the classic distinction between systematic and +accidental errors. If the metre with which we +measure a length is too long, the number we get +will be too small, and it will be no use to measure +several times---that is a systematic error. If we +measure with an accurate metre, we may make a +mistake, and find the length sometimes too large +and sometimes too small, and when we take the +mean of a large number of measurements, +the error will tend to grow small. These are +accidental errors. + +It is clear that systematic errors do not satisfy +Gauss's law, but do accidental errors satisfy it? +\PageSep{208} +Numerous proofs have been attempted, almost all +of them crude paralogisms. But starting from +the following hypotheses we may prove Gauss's +law: the error is the result of a very large number +of partial and independent errors; each partial +error is very small and obeys any law of probability +whatever, provided the probability of a +positive error is the same as that of an equal +negative error. It is clear that these conditions +will be often, but not always, fulfilled, and we +may reserve the name of accidental for errors +which satisfy them. + +We see that the method of least squares is not +legitimate in every case; in general, physicists +are more distrustful of it than astronomers. This +is no doubt because the latter, apart from the +systematic errors to which they and the physicists +are subject alike, have to contend with an +extremely important source of error which is +entirely accidental---I mean atmospheric undulations. +So it is very curious to hear a discussion +between a physicist and an astronomer about a +method of observation. The physicist, persuaded +that one good measurement is worth more than +many bad ones, is pre-eminently concerned with +the elimination by means of every precaution of +the final systematic errors; the astronomer retorts: +``But you can only observe a small number of stars, +and accidental errors will not disappear.'' + +What conclusion must we draw? Must we +continue to use the method of least squares? +\PageSep{209} +We must distinguish. We have eliminated all +the systematic errors of which we have any +suspicion; we are quite certain that there are +others still, but we cannot detect them; and yet +we must make up our minds and adopt a definitive +value which will be regarded as the probable +value; and for that purpose it is clear that the +best thing we can do is to apply Gauss's law. +We have only applied a practical rule referring +to subjective probability. And there is no more +to be said. + +Yet we want to go farther and say that not +only the probable value is so much, but that the +probable error in the result is so much. \emph{This +is absolutely invalid}: it would be true only if +we were sure that all the systematic errors +were eliminated, and of that we know absolutely +nothing. We have two series of observations; by +applying the law of least squares we find that the +probable error in the first series is twice as small +as in the second. The second series may, however, +be more accurate than the first, because the +first is perhaps affected by a large systematic +error. All that we can say is, that the first series +is \emph{probably} better than the second because its +accidental error is smaller, and that we have no +reason for affirming that the systematic error is +greater for one of the series than for the other, +our ignorance on this point being absolute. + +\Par[VII. ]{Conclusions.}---In the preceding lines I have +set several problems, and have given no solution. +\PageSep{210} +I do not regret this, for perhaps they will invite +the reader to reflect on these delicate questions. + +However that may be, there are certain points +which seem to be well established. To undertake +the calculation of any probability, and even for +that calculation to have any meaning at all, we +must admit, as a point of departure, an hypothesis +or convention which has always something +arbitrary about it. In the choice of this convention +we can be guided only by the principle +of sufficient reason. Unfortunately, this principle +is very vague and very elastic, and in the cursory +examination we have just made we have seen it +assume different forms. The form under which +we meet it most often is the belief in continuity, +a belief which it would be difficult to justify by +apodeictic reasoning, but without which all science +would be impossible. Finally, the problems to +which the calculus of probabilities may be applied +with profit are those in which the result is independent +of the hypothesis made at the outset, +provided only that this hypothesis satisfies the +condition of continuity. +\PageSep{211} + + +\Chapter{XII.\protect\footnotemark}{Optics And Electricity.} +\footnotetext{This chapter is mainly taken from the prefaces of two of my + books---\Title{Théorie Mathématique de la lumière} (Paris: Naud, 1889), + and \Title{Électricité et Optique} (Paris: Naud, 1901).} + +\Par{Fresnel's Theory.}---The best example that can be +chosen is the theory of light and its relations +to the theory of electricity. It is owing to Fresnel +that the science of optics is more advanced than +any other branch of physics. The theory called the +theory of undulations forms a complete whole, +which is satisfying to the mind; but we must +not ask from it what it cannot give us. The +object of mathematical theories is not to reveal +to us the real nature of things; that would be +an unreasonable claim. Their only object is to +co-ordinate the physical laws with which physical +experiment makes us acquainted, the enunciation +of which, without the aid of mathematics, we +should be unable to effect. Whether the ether +exists or not matters little---let us leave that to +the metaphysicians; what is essential for us is, that +everything happens as if it existed, and that this +hypothesis is found to be suitable for the explanation +of phenomena. After all, have we any other +\PageSep{212} +reason for believing in the existence of material +objects? That, too, is only a convenient hypothesis; +only, it will never cease to be so, while some day, +no doubt, the ether will be thrown aside as useless. + +But at the present moment the laws of optics, +and the equations which translate them into the +language of analysis, hold good---at least as a first +approximation. It will therefore be always useful +to study a theory which brings these equations +into connection. + +The undulatory theory is based on a molecular +hypothesis; this is an advantage to those who +think they can discover the cause under the law. +But others find in it a reason for distrust; and +this distrust seems to me as unfounded as the +illusions of the former. These hypotheses play +but a secondary rôle. They may be sacrificed, +and the sole reason why this is not generally done +is, that it would involve a certain loss of lucidity +in the explanation. In fact, if we look at it a +little closer we shall see that we borrow from +molecular hypotheses but two things---the principle +of the conservation of energy, and the linear form +of the equations, which is the general law of small +movements as of all small variations. This explains +why most of the conclusions of Fresnel +remain unchanged when we adopt the electro-magnetic +theory of light. + +\Par{Maxwell's Theory.}---We all know that it was +Maxwell who connected by a slender tie two +branches of physics---optics and electricity---until +\PageSep{213} +then unsuspected of having anything in common. +Thus blended in a larger aggregate, in a higher +harmony, Fresnel's theory of optics did not perish. +Parts of it are yet alive, and their mutual relations +are still the same. Only, the language which we +use to express them has changed; and, on the +other hand, Maxwell has revealed to us other +relations, hitherto unsuspected, between the +different branches of optics and the domain of +electricity. + +\Pagelabel{213}% +The first time a French reader opens Maxwell's +book, his admiration is tempered with a feeling of +uneasiness, and often of distrust. + +It is only after prolonged study, and at the cost +of much effort, that this feeling disappears. Some +minds of high calibre never lose this feeling. Why +is it so difficult for the ideas of this English +scientist to become acclimatised among us? No +doubt the education received by most enlightened +Frenchmen predisposes them to appreciate precision +and logic more than any other qualities. +In this respect the old theories of mathematical +physics gave us complete satisfaction. All our +masters, from Laplace to Cauchy, proceeded along +the same lines. Starting with clearly enunciated +hypotheses, they deduced from them all their +consequences with mathematical rigour, and then +compared them with experiment. It seemed to +be their aim to give to each of the branches +of physics the same precision as to celestial +mechanics. +\PageSep{214} + +A mind accustomed to admire such models is +not easily satisfied with a theory. Not only will +it not tolerate the least appearance of contradiction, +but it will expect the different parts to be +logically connected with one another, and will +require the number of hypotheses to be reduced +to a minimum. + +This is not all; there will be other demands +which appear to me to be less reasonable. Behind +the matter of which our senses are aware, and +which is made known to us by experiment, such +a thinker will expect to see another kind of matter---the +only true matter in its opinion---which will +no longer have anything but purely geometrical +qualities, and the atoms of which will be mathematical +points subject to the laws of dynamics +alone. And yet he will try to represent to +himself, by an unconscious contradiction, these +invisible and colourless atoms, and therefore +to bring them as close as possible to ordinary +matter. + +Then only will he be thoroughly satisfied, and +he will then imagine that he has penetrated the +secret of the universe. Even if the satisfaction is +fallacious, it is none the less difficult to give it up. +Thus, on opening the pages of Maxwell, a Frenchman +expects to find a theoretical whole, as logical +and as precise as the physical optics that is founded +on the hypothesis of the ether. He is thus preparing +for himself a disappointment which I +should like the reader to avoid; so I will warn +\PageSep{215} +him at once of what he will find and what he will +not find in Maxwell. + +Maxwell does not give a mechanical explanation +of electricity and magnetism; he confines himself +to showing that such an explanation is possible. +He shows that the phenomena of optics are only +a particular case of electro-magnetic phenomena. +From the whole theory of electricity a theory of +light can be immediately deduced. Unfortunately +the converse is not true; it is not always easy to +find a complete explanation of electrical phenomena. +In particular it is not easy if we take +as our starting-point Fresnel's theory; to do so, +no doubt, would be impossible; but none the less +we must ask ourselves if we are compelled to +surrender admirable results which we thought we +had definitively acquired. That seems a step +backwards, and many sound intellects will not +willingly allow of this. + +Should the reader consent to set some bounds +to his hopes, he will still come across other +difficulties. The English scientist does not try +to erect a unique, definitive, and well-arranged +building; he seems to raise rather a large number +of provisional and independent constructions, +between which communication is difficult and +sometimes impossible. Take, for instance, the +chapter in which \Chg{electrostatic}{electro-static} attractions are +explained by the pressures and tensions of the +dielectric medium. This chapter might be suppressed +without the rest of the book being +\PageSep{216} +thereby less clear or less complete, and yet +it contains a theory which is self-sufficient, and +which can be understood without reading a +word of what precedes or follows. But it is +not only independent of the rest of the book; it +is difficult to reconcile it with the fundamental +ideas of the volume. Maxwell does not even +attempt to reconcile it; he merely says: ``I have +not been able to make the next step---namely, to +account by mechanical considerations for these +stresses in the dielectric.'' + +This example will be sufficient to show what +I mean; I could quote many others. Thus, who +would suspect on reading the pages devoted to +magnetic rotatory polarisation that there is an +identity between optical and magnetic phenomena? + +We must not flatter ourselves that we have +avoided every contradiction, but we ought to +make up our minds. Two contradictory theories, +provided that they are kept from overlapping, and +that we do not look to find in them the explanation +of things, may, in fact, be very useful instruments +of research; and perhaps the reading of +Maxwell would be less suggestive if he had not +opened up to us so many new and divergent ways. +But the fundamental idea is masked, as it were. +So far is this the case, that in most works that are +popularised, this idea is the only point which is +left completely untouched. To show the importance +of this, I think I ought to explain in what this +\PageSep{217} +fundamental idea consists; but for that purpose +a short digression is necessary. + +\Par{The Mechanical Explanation of Physical Phenomena.}---In +every physical phenomenon there is a certain +number of parameters which are reached directly +by experiment, and which can be measured. I +shall call them the parameters~$q$. Observation +next teaches us the laws of the variations of these +parameters, and these laws can be generally stated +in the form of differential equations which connect +together the parameters~$q$ and time. What can +be done to give a mechanical interpretation to +such a phenomenon? We may endeavour to +explain it, either by the movements of ordinary +matter, or by those of one or more hypothetical +fluids. These fluids will be considered as formed +of a very large number of isolated molecules~$m$. +When may we say that we have a complete +mechanical explanation of the phenomenon? It +will be, on the one hand, when we know the +differential equations which are satisfied by the +co-ordinates of these hypothetical molecules~$m$, +equations which must, in addition, conform to the +laws of dynamics; and, on the other hand, when we +know the relations which define the co-ordinates +of the molecules~$m$ as functions of the parameters~$q$, +attainable by experiment. These equations, as +I have said, should conform to the principles of +dynamics, and, in particular, to the principle of +the conservation of energy, and to that of least +action. +\PageSep{218} + +The first of these two principles teaches us that +the total energy is constant, and may be divided +into two parts:\Add{---} + +(1) Kinetic energy, or \Foreign{vis~viva}, which depends +on the masses of the hypothetical molecules~$m$, +and on their velocities. This I shall call~$T$. (2)~The +potential energy which depends only on the +co-ordinates of these molecules, and this I shall +call~$U$. It is the sum of the energies $T$~and~$U$ that +is constant. + +Now what are we taught by the principle of +least action? It teaches us that to pass from the +initial position occupied at the instant~$t_{0}$ to +the final position occupied at the instant~$t_{1}$, the +system must describe such a path that in the +interval of time between the instant $t_{0}$~and~$t_{1}$, +the mean value of the action---\ie, the \emph{difference} +between the two energies $T$~and~$U$, must be as +small as possible. The first of these two principles +is, moreover, a consequence of the second. If we +know the functions $T$~and~$U$, this second principle +is sufficient to determine the equations of motion. + +Among the paths which enable us to pass from +one position to another, there is clearly one for +which the mean value of the action is smaller than +for all the others. In addition, there is only\Typo{ }{ one} such +path; and it follows from this, that the principle +of least action is sufficient to determine the path +followed, and therefore the equations of motion. +We thus obtain what are called the equations of +Lagrange. In these equations the independent +\PageSep{219} +variables are the co-ordinates of the hypothetical +molecules~$m$; but I now assume that we take for +the variables the parameters~$q$, which are directly +accessible to experiment. + +The two parts of the energy should then be +expressed as a function of the parameters~$q$ and +their derivatives; it is clear that it is under this +form that they will appear to the experimenter. +The latter will naturally endeavour to define +kinetic and potential energy by the aid of +quantities he can directly observe.\footnote + {We may add that $U$ will depend only on the $q$~parameters, that + $T$~will depend on them and their derivatives with respect to time, + and will be a homogeneous polynomial of the second degree with + respect to these derivatives.} +If this be +granted, the system will always proceed from one +position to another by such a path that the mean +value of the action is a minimum. It matters +little that $T$~and~$U$ are now expressed by the aid +of the parameters~$q$ and their derivatives; it +matters little that it is also by the aid of these +parameters that we define the initial and \Typo{fina}{final} +positions; the principle of least action will always +remain true. + +Now here again, of the whole of the paths which +lead from one position to another, there is one and +only one for which the mean action is a minimum. +The principle of least action is therefore sufficient +for the determination of the differential equations +which define the variations of the parameters~$q$. +The equations thus obtained are another form of +Lagrange's equations. +\PageSep{220} + +To form these equations we need not know the +relations which connect the parameters~$q$ with the +co-ordinates of the hypothetical molecules, nor the +masses of the molecules, nor the expression of~$U$ +as a function of the co-ordinates of these molecules. +All we need know is the expression of~$U$ as a +function of the parameters~$q$, and that of~$T$ as a +function of the parameters~$q$ and their derivatives---\ie, +the expressions of the kinetic and potential +energy in terms of experimental data. + +One of two things must now happen. Either for +a convenient choice of $T$~and~$U$ the Lagrangian +equations, constructed as we have indicated, will +be identical with the differential equations deduced +from experiment, or there will be no functions $T$~and~$U$ +for which this identity takes place. In the +latter case it is clear that no mechanical explanation +is possible. The \emph{necessary} condition for a +mechanical explanation to be possible is therefore +this: that we may choose the functions $T$~and~$U$ so +as to satisfy the principle of least action, and of the +conservation of energy. Besides, this condition is +\emph{sufficient}. Suppose, in fact, that we have found a +function~$U$ of the parameters~$q$, which represents +one of the parts of energy, and that the part of the +energy which we represent by~$T$ is a function of +the parameters~$q$ and their derivatives; that it +is a polynomial of the second degree with respect +to its derivatives, and finally that the Lagrangian +equations formed by the aid of these two functions +$T$~and~$U$ are in conformity with the data of the +\PageSep{221} +experiment. How can we deduce from this a +mechanical explanation? $U$~must be regarded as +the potential energy of a system of which $T$~is the +kinetic energy. There is no difficulty as far as $U$~is +concerned, but can $T$ be regarded as the \Foreign{vis~viva} +of a material system? + +It is easily shown that this is always possible, +and in an unlimited number of ways. I will be +content with referring the reader to the pages of +the preface of my \Title{Électricité et Optique} for further +details. Thus, if the principle of least action +cannot be satisfied, no mechanical explanation is +possible; if it can be satisfied, there is not only one +explanation, but an unlimited number, whence it +follows that since there is one there must be an +unlimited number. + +One more remark. Among the quantities that +may be reached by experiment directly we shall +consider some as the co-ordinates of our hypothetical +molecules, some will be our parameters~$q$, +and the rest will be regarded as dependent not +only on the co-ordinates but on the velocities---or +what comes to the same thing, we look on them as +derivatives of the parameters~$q$, or as combinations +of these parameters and their derivatives. + +Here then a question occurs: among all these +quantities measured experimentally which shall we +choose to represent the parameters~$q$? and which +shall we prefer to regard as the derivatives of these +parameters? This choice remains arbitrary to a +large extent, but a mechanical explanation will be +\PageSep{222} +possible if it is done so as to satisfy the principle of +least action. + +Next, Maxwell asks: Can this choice and that of +the two energies $T$~and~$U$ be made so that electric +phenomena will satisfy this principle? Experiment +shows us that the energy of an electro-magnetic +field decomposes into electro-static and electro-dynamic +energy. Maxwell recognised that if we +regard the former as the potential energy~$U$, and +the latter as the kinetic energy~$T$, and that if on +the other hand we take the electro-static charges +of the conductors as the parameters~$q$, and the intensity +of the currents as derivatives of other +parameters~$q$---under these conditions, Maxwell +has recognised that electric phenomena \Reword{satisfies}{satisfy} the +principle of least action. He was then certain of +a mechanical explanation. If he had expounded +this theory at the beginning of his first volume, +instead of relegating it to a corner of the second, it +would not have escaped the attention of most +readers. If therefore a phenomenon allows of a +complete mechanical explanation, it allows of an +unlimited number of others, which will equally take +into account all the particulars revealed by experiment. +And this is confirmed by the history of +every branch of physics. In Optics, for instance, +Fresnel believed vibration to be perpendicular to +the plane of polarisation; Neumann holds that it is +parallel to that plane. For a long time an \Foreign{experimentum +crucis} was sought for, which would enable +us to decide between these two theories, but in +\PageSep{223} +vain. In the same way, without going out of the +domain of electricity, we find that the theory of +two fluids and the single fluid theory equally +account in a satisfactory manner for all the laws +of electro-statics. All these facts are easily explained, +thanks to the properties of the Lagrange +equations. + +\Pagelabel{223}% +It is easy now to understand Maxwell's fundamental +idea. To demonstrate the possibility of a +mechanical explanation of electricity we need not +trouble to find the explanation itself; we need only +know the expression of the two functions $T$~and~$U$, +which are the two parts of energy, and to form with +these two functions Lagrange's equations, and +then to compare these equations with the experimental +laws. + +How shall we choose from all the possible +explanations one in which the help of experiment +will be wanting? The day will perhaps come +when physicists will no longer concern themselves +with questions which are inaccessible to positive +methods, and will leave them to the metaphysicians. +That day has not yet come; man does not +so easily resign himself to remaining for ever ignorant +of the causes of things. Our choice cannot be +therefore any longer guided by considerations in +which personal appreciation plays too large a part. +There are, however, solutions which all will reject +because of their fantastic nature, and others which +all will prefer because of their simplicity. As +far as magnetism and electricity are concerned, +\PageSep{224} +Maxwell abstained from making any choice. It is +not that he has a systematic contempt for all that +positive methods cannot reach, as may be seen +from the time he has devoted to the kinetic theory +of gases. I may add that if in his \Foreign{magnum opus} he +develops no complete explanation, he has attempted +one in an article in the \Title{Philosophical Magazine}. +The strangeness and the complexity of the +hypotheses he found himself compelled to make, +led him afterwards to withdraw it. + +The same spirit is found throughout his whole +work. He throws into relief the essential---\ie, +what is common to all theories; everything that +suits only a particular theory is passed over almost +in silence. The reader therefore finds himself in +the presence of form nearly devoid of matter, +which at first he is tempted to take as a fugitive +and unassailable phantom. But the efforts he is +thus compelled to make force him to think, and +eventually he sees that there is often something +rather artificial in the theoretical ``aggregates'' +which he once admired. +\Pagelabel{224}% +\PageSep{225} + + +\Chapter{XIII.}{Electro-Dynamics.} + +\First{The} history of electro-dynamics is very instructive +from our point of view. The title of Ampère's +immortal work is, \Title{Théorie des phénomènes electro-dynamiques, +uniquement fondée sur expérience}. He +therefore imagined that he had made no hypotheses; +but as we shall not be long in recognising, he was +mistaken; only, of these hypotheses he was quite +unaware. On the other hand, his successors see +them clearly enough, because their attention is +attracted by the weak points in Ampère's solution. +They made fresh hypotheses, but this time +deliberately. How many times they had to change +them before they reached the classic system, which +is perhaps even now not quite definitive, we shall +see. + +\Par[I. ]{Ampère's Theory.}---In Ampère's experimental +study of the mutual action of currents, he has +operated, and he could operate only, with closed +currents. This was not because he denied the +existence or possibility of open currents. If two +conductors are positively and negatively charged +and brought into communication by a wire, a +current is set up which passes from one to the +\PageSep{226} +other until the two potentials are equal. According +to the ideas of Ampère's time, this was +considered to be an open current; the current was +known to pass from the first conductor to the +second, but they did not know it returned from the +second to the first. All currents of this kind were +therefore considered by Ampère to be open +currents---for instance, the currents of discharge +of a condenser; he was unable to experiment on +them, their duration being too short. Another +kind of open current may be imagined. Suppose +we have two conductors $A$~and~$B$ connected by a +wire~$AMB$. Small conducting masses in motion +are first of all placed in contact with the conductor~$B$, +receive an electric charge, and leaving~$B$ are +set in motion along a path~$BNA$, carrying their +charge with them. On coming into contact with~$A$ +they lose their charge, which then returns to~$B$ +along the wire~$AMB$. Now here we have, in a +sense, a closed circuit, since the electricity describes +the closed circuit~$BNAMB$; but the two parts of +the current are quite different. In the wire~$AMB$ +the electricity is displaced \emph{through} a fixed conductor +like a voltaic current, overcoming an ohmic resistance +and developing heat; we say that it is +displaced by \emph{conduction}. In the part~$BNA$ the +electricity is \emph{carried} by a moving conductor, and is +said to be displaced by \emph{convection}. If therefore the +convection current is considered to be perfectly +analogous to the conduction current, the circuit~$BNAMB$ +is closed; if on the contrary the convection +\PageSep{227} +current is not a ``true current,'' and, for +instance, does not act on the magnet, there is only +the conduction current~$AMB$, which is \emph{open}. For +example, if we connect by a wire the poles of a +Holtz machine, the charged rotating disc transfers +the electricity by convection from one pole to the +other, and it returns to the first pole by conduction +through the wire. But currents of this kind are +very difficult to produce with appreciable intensity; +in fact, with the means at Ampère's disposal we +may almost say it was impossible. + +To sum up, Ampère could conceive of the existence +of two kinds of open currents, but he could +experiment on neither, because they were not +strong enough, or because their duration was too +short. Experiment therefore could only show him +the action of a closed current on a closed current---or +more accurately, the action of a closed current +on a portion of current, because a current can be +made to describe a \emph{closed} circuit, of which part may +be in motion and the other part fixed. The displacements +of the moving part may be studied under the +action of another closed current. On the other +hand, Ampère had no means of studying the action +of an open current either on a closed or on another +open current. + +\Par[1.\ ]{The Case of Closed Currents.}---In the case of +the mutual action of two closed currents, experiment +revealed to Ampère remarkably simple +laws. The following will be useful to us in the +sequel:--- +\PageSep{228} + +(1) \emph{If the intensity of the currents is kept constant}, +and if the two circuits, after having undergone any +displacements and deformations whatever, return +finally to their initial positions, the total work +done by the electro-dynamical actions is zero. In +other words, there is an \emph{electro-dynamical potential} +of the two circuits proportional to the product of +their intensities, and depending on the form and +relative positions of the circuits; the work done +by the electro-dynamical actions is equal to the +change of this potential. + +(2) The action of a closed solenoid is zero. + +(3) The action of a circuit~$C$ on another voltaic +circuit~$C'$ depends only on the ``magnetic field'' +developed by the circuit~$C$. At each point in +space we can, in fact, define in magnitude and +direction a certain force called ``magnetic force,'' +which enjoys the following properties:--- + +(\textit{a}) The force exercised by~$C$ on a magnetic +pole is applied to that pole, and is equal to the +magnetic force multiplied by the magnetic mass +of the pole. + +(\textit{b}) A very short magnetic needle tends to take +the direction of the magnetic force, and the couple +to which it tends to reduce is proportional to the +product of the magnetic force, the magnetic +moment of the needle, and the sine of the dip +of the needle. + +(\textit{c}) If the circuit~$C'$ is displaced, the amount of +the work done by the electro-dynamic action of~$C$ +on~$C'$ will be equal to the increment of ``flow +\PageSep{229} +of magnetic force'' which passes through the +circuit. + +\Par[2.\ ]{Action of a Closed Current on a Portion of +Current.}---Ampère being unable to produce the +open current properly so called, had only one +way of studying the action of a closed current +on a portion of current. This was by operating +on a circuit~$C$ composed of two parts, one movable +and the other fixed. The movable part was, +for instance, a movable wire~$\alpha\beta$, the ends $\alpha$~and~$\beta$ +of which could slide along a fixed wire. In one of +the positions of the movable wire the end~$\alpha$ rested +on the point~$A$, and the end~$\beta$ on the point~$B$ of +the fixed wire. The current ran from~$\alpha$ to~$\beta$---\ie, +from~$A$ to~$B$ along the movable wire, and then +from~$B$ to~$A$ along the fixed wire. \emph{This current +was therefore closed.} + +In the second position, the movable wire +having slipped, the points $\alpha$~and~$\beta$ were respectively +at $A'$~and~$B'$ on the fixed wire. The current +ran from~$\alpha$ to~$\beta$---\ie, from~$A'$ to~$B'$ on the movable +wire, and returned from~$B'$ to~$B$, and +then from~$B$ to~$A$, and then from~$A$ to~$A'$---all on +the fixed wire. This current was also closed. +If a similar circuit be exposed to the action of a +closed current~$C$, the movable part will be displaced +just as if it were acted on by a force. +Ampère \emph{admits} that the force, apparently acting on +the movable part~$AB$, representing the action of~$C$ +on the portion~$\alpha\beta$ of the current, remains the +same whether an open current runs through~$\alpha\beta$, +\PageSep{230} +stopping at $\alpha$~and~$\beta$, or whether a closed current +runs first to~$\beta$ and then returns to~$\alpha$ through the +fixed portion of the circuit. This hypothesis +seemed natural enough, and Ampère innocently +assumed it; nevertheless the hypothesis \emph{is not a +necessity}, for we shall presently see that Helmholtz +rejected it. However that may be, it enabled +Ampère, although he had never produced an open +current, to lay down the laws of the action of a +closed current on an open current, or even on an +element of current. They are simple:\Add{---} + +(1) The force acting on an element of current +is applied to that element; it is normal to the +element and to the magnetic force, and proportional +to that component of the magnetic force +which is normal to the element. + +(2) The action of a closed solenoid on an +element of current is zero. But the electro-dynamic +potential has disappeared---\ie, when a +closed and an open current of constant intensities +return to their initial positions, the total work +done is not zero. + +\Par[3.\ ]{Continuous Rotations.}---The most remarkable +electro-dynamical experiments are those in which +continuous rotations are produced, and which are +called \emph{unipolar induction} experiments. A magnet +may turn about its axis; a current passes first +through a fixed wire and then enters the magnet +by the pole~$N$, for instance, passes through +half the magnet, and emerges by a sliding contact +and re-enters the fixed wire. The magnet +\PageSep{231} +then begins to rotate continuously. This is +Faraday's experiment. How is it possible? If it +were a question of two circuits of invariable form, +$C$~fixed and $C'$~movable about an axis, the latter +would never take up a position of continuous +rotation; in fact, there is an electro-dynamical +potential; there must therefore be a position of +equilibrium when the potential is a maximum. +Continuous rotations are therefore possible only +when the circuit~$C'$ is composed of two parts---one +fixed, and the other movable about an axis, +as in the case of Faraday's experiment. Here +again it is convenient to draw a distinction. The +passage from the fixed to the movable part, or +\Foreign{vice~versâ}, may take place either by simple contact, +the same point of the movable part remaining +constantly in contact with the same point of the +fixed part, or by sliding contact, the same point of +the movable part coming successively into contact +with the different points of the fixed part. + +It is only in the second case that there can +be continuous rotation. This is what then +happens:---the system tends to take up a position +of equilibrium; but, when at the point of reaching +that position, the sliding contact puts the moving +part in contact with a fresh point in the fixed +part; it changes the connexions and therefore the +conditions of equilibrium, so that as the position +of equilibrium is ever eluding, so to speak, the +system which is trying to reach it, rotation may +take place indefinitely. +\PageSep{232} + +Ampère admits that the action of the circuit on +the movable part of~$C'$ is the same as if the fixed +part of~$C'$ did not exist, and therefore as if the +current passing through the movable part were +an open current. He concluded that the action of +a closed on an open current, or \Foreign{vice~versâ}, that of +an open current on a fixed current, may give rise +to continuous rotation. But this conclusion +depends on the hypothesis which I have enunciated, +and to which, as I said above, Helmholtz +declined to subscribe. + +\Par[4.\ ]{Mutual Action of Two Open Currents.}---As far +as the mutual action of two open currents, and in +particular that of two elements of current, is +concerned, all experiment breaks down. Ampère +falls back on hypothesis. He assumes: (1)~that +the mutual action of two elements reduces to a +force acting along their \emph{join}; (2)~that the action +of two closed currents is the resultant of the +mutual actions of their different elements, which +are the same as if these elements were isolated. + +The remarkable thing is that here again Ampère +makes two hypotheses without being aware of it. +However that may be, these two hypotheses, +together with the experiments on closed currents, +suffice to determine completely the law of mutual +action of two elements. But then, most of the +simple laws we have met in the case of closed +currents are no longer true. In the first place, +there is no electro-dynamical potential; nor was +there any, as we have seen, in the case of a closed +\PageSep{233} +current acting on an open current. Next, there +is, properly speaking, no magnetic force; and we +have above defined this force in three different +ways: (1)~By the action on a magnetic pole; +(2)~by the director couple which orientates the +magnetic needle; (3)~by the action on an element +of current. + +In the case with which we are immediately +concerned, not only are these three definitions not +in harmony, but each has lost its meaning:--- + +(1) A magnetic pole is no longer acted on by a +unique force applied to that pole. We have seen, +in fact, the action of an element of current on a +pole is not applied to the pole but to the element; +it may, moreover, be replaced by a force applied to +the pole and by a couple. + +(2) The couple which acts on the magnetic +needle is no longer a simple director couple, for its +moment with respect to the axis of the needle is +not zero. It decomposes into a director couple, +properly so called, and a supplementary couple +which tends to produce the continuous rotation of +which we have spoken above. + +(3) Finally, the force acting on an element of +a current is not normal to that element. In +other words, \emph{the unity of the magnetic force has +disappeared}. + +Let us see in what this unity consists. Two +systems which exercise the same action on a magnetic +pole will also exercise the same action on an +indefinitely small magnetic needle, or on an element +\PageSep{234} +of current placed at the point in space at which the +pole is. Well, this is true if the two systems only +contain closed currents, and according to Ampère +it would not be true if the systems contained open +currents. It is sufficient to remark, for instance, +that if a magnetic pole is placed at~$A$ and an +element at~$B$, the direction of the element being +in~$AB$ produced, this element, which will exercise +no action on the pole, will exercise an action +either on a magnetic needle placed at~$A$, or on +an element of current at~$A$. + +\Par[5.\ ]{Induction.}---We know that the discovery of +electro-dynamical induction followed not long after +the immortal work of Ampère. As long as it is +only a question of closed currents there is no +difficulty, and Helmholtz has even remarked that +the principle of the conservation of energy is +sufficient for us to deduce the laws of induction +from the electro-dynamical laws of Ampère. But +on the condition, as Bertrand has shown,---that +we make a certain number of hypotheses. + +The same principle again enables this deduction +to be made in the case of open currents, although +the result cannot be tested by experiment, since +such currents cannot be produced. + +If we wish to compare this method of analysis +with Ampère's theorem on open currents, we get +results which are calculated to surprise us. In +the first place, induction cannot be deduced from +the variation of the magnetic field by the well-known +formula of scientists and practical men; +\PageSep{235} +in fact, as I have said, properly speaking, there +is no magnetic field. But further, if a circuit~$C$ +is subjected to the induction of a variable voltaic +system~$S$, and if this system~$S$ be displaced and +deformed in any way whatever, so that the +intensity of the currents of this system varies +according to any law whatever, then so long +as after these variations the system eventually +returns to its initial position, it seems natural +to suppose that the \emph{mean} electro-motive force +%[** TN: "induite dans le circuit C est nulle" in the French edition.] +induced in the \Reword{current}{circuit}~$C$ is zero. This is true if +the circuit~$C$ is closed, and if the system~$S$ only +contains closed currents. It is no longer true if +we accept the theory of Ampère, since there would +be open currents. So that not only will induction +no longer be the variation of the flow of magnetic +force in any of the usual senses of the word, but +it cannot be represented by the variation of that +force whatever it may be. + +\Par[II. ]{Helmholtz's Theory.}---I have dwelt upon the +consequences of Ampère's theory and on his +method of explaining the action of open currents. +It is difficult to disregard the paradoxical and +artificial character of the propositions to which +we are thus led. We feel bound to think ``it +cannot be so.'' We may imagine then that +Helmholtz has been led to look for something +else. He rejects the fundamental hypothesis of +Ampère---namely, that the mutual action of two +elements of current reduces to a force along their +join. He admits that an clement of current is not +\PageSep{236} +acted upon by a single force but by a force and a +couple, and this is what gave rise to the celebrated +polemic between Bertrand and Helmholtz. +Helmholtz replaces Ampère's hypothesis by the +following:---Two elements of current always +admit of an electro-dynamic potential, depending +solely upon their position and orientation; and the +work of the forces that they exercise one on the +other is equal to the variation of this potential. +Thus Helmholtz can no more do without +hypothesis than Ampère, but at least he does +not do so without explicitly announcing it. In +the case of closed currents, which alone are +accessible to experiment, the two theories agree; +in all other cases they differ. In the first place, +contrary to what Ampère supposed, the force +which seems to act on the movable portion of +a closed current is not the same as that acting +on the movable portion if it were isolated and +if it constituted an open current. Let us return +to the circuit~$C'$, of which we spoke above, and +which was formed of a movable wire sliding on +a fixed wire. In the only experiment that can be +made the movable portion~$\alpha\beta$ is not isolated, but is +part of a closed circuit. When it passes from~$AB$ +to~$A'B'$, the total electro-dynamic potential +varies for two reasons. First, it has a slight increment +because the potential of~$A'B'$ with respect +to the circuit~$C$ is not the same as that of~$AB$; +secondly, it has a second increment because it +must be increased by the potentials of the elements +\PageSep{237} +$AA'$~and~$B'B$ with respect to~$C$. It is this \emph{double} +increment which represents the work of the force +acting upon the portion~$AB$. If, on the contrary, +$\alpha\beta$~be isolated, the potential would only have the +first increment, and this first increment alone +would measure the work of the force acting on~$AB$. +In the second place, there could be no +continuous rotation without sliding contact, and +in fact, that, as we have seen in the case of closed +currents, is an immediate consequence of the +existence of an electro-dynamic potential. In +Faraday's experiment, if the magnet is fixed, +and if the part of the current external to the +magnet runs along a movable wire, that movable +wire may undergo continuous rotation. But it +does not mean that, if the contacts of the \Typo{weir}{wire} +with the magnet were suppressed, and an open +current were to run along the wire, the wire +would still have a movement of continuous rotation. +I have just said, in fact, that an isolated +element is not acted on in the same way as a +movable element making part of a closed circuit. +But there is another difference. The action of a +solenoid on a closed current is zero according to +experiment and according to the two theories. +Its action on an open current would be zero +according to Ampère, and it would not be +zero according to Helmholtz. From this follows +an important consequence. We have given above +three definitions of the magnetic force. The third +has no meaning here, since an element of current +\PageSep{238} +is no longer acted upon by a single force. Nor +has the first any meaning. What, in fact, is a +magnetic pole? It is the extremity of an +indefinite linear magnet. This magnet may be +replaced by an indefinite solenoid. For the +definition of magnetic force to have any meaning, +the action exercised by an open current on +an indefinite solenoid would only depend on the +position of the extremity of that solenoid---\ie, +that the action of a closed solenoid is zero. Now +we have just seen that this is not the case. On +the other hand, there is nothing to prevent us +from adopting the second definition which is +founded on the measurement of the director +couple which tends to orientate the magnetic +needle; but, if it is adopted, neither the effects +of induction nor electro-dynamic effects will +depend solely on the distribution of the lines +of force in this magnetic field. + +\Par[III. ]{Difficulties raised by these Theories.}---Helmholtz's +theory is an advance on that of Ampère; +it is necessary, however, that every difficulty +should be removed. In both, the name ``magnetic +field'' has no meaning, or, if we give it one by a +more or less artificial convention, the ordinary +laws so familiar to electricians no longer apply; +and it is thus that the electro-motive force induced +in a wire is no longer measured by the number +of lines of force met by that wire. And our +objections do not proceed only from the fact that +it is difficult to give up deeply-rooted habits of +\PageSep{239} +language and thought. There is something more. +If we do not believe in actions at a distance, +electro-dynamic phenomena must be explained by +a modification of the medium. And this medium +is precisely what we call ``magnetic field,'' and +then the electro-magnetic effects should only +depend on that field. All these difficulties arise +from the hypothesis of open currents. + +\Par[IV. ]{Maxwell's Theory.}---Such were the difficulties +raised by the current theories, when Maxwell with +a stroke of the pen caused them to vanish. To +his mind, in fact, all currents are closed currents. +Maxwell admits that if in a dielectric, the electric +field happens to vary, this dielectric becomes the +seat of a particular phenomenon acting on the +galvanometer like a current and called the \emph{current +of displacement}. If, then, two conductors bearing +positive and negative charges are placed in connection +by means of a wire, during the discharge +there is an open current of conduction in that +wire; but there are produced at the same time in +the surrounding dielectric currents of displacement +which close this current of conduction. We +know that Maxwell's theory leads to the explanation +of optical phenomena which would be due to +extremely rapid electrical oscillations. At that +period such a conception was only a daring hypothesis +which could be supported by no experiment; +but after twenty years Maxwell's ideas received the +confirmation of experiment. Hertz succeeded in +producing systems of electric oscillations which +\PageSep{240} +reproduce all the properties of light, and only +differ by the length of their wave---that is to say, +as violet differs from red. In some measure he +made a synthesis of light. It might be said that +Hertz has not directly proved Maxwell's fundamental +idea of the action of the current of +displacement on the galvanometer. That is true +in a sense. What he has shown directly is that +electro-magnetic induction is not instantaneously +propagated, as was supposed, but its speed is the +speed of light. Yet, to suppose there is no current +of displacement, and that induction is with the +speed of light; or, rather, to suppose that the +currents of displacement produce inductive effects, +and that the induction takes place instantaneously---\emph{comes +to the same thing}. This cannot be seen at +the first glance, but it is proved by an analysis +of which I must not even think of giving even a +summary here. + +\Par[V. ]{Rowland's Experiment.}---But, as I have said +above, there are two kinds of open conduction +currents. There are first the currents of discharge +of a condenser, or of any conductor whatever. +There are also cases in which the electric charges +describe a closed contour, being displaced by conduction +in one part of the circuit and by convection +in the other part. The question might be +regarded as solved for open currents of the first +kind; they were closed by currents of displacement. +For open currents of the second kind the +solution appeared still more simple. +\PageSep{241} + +It seemed that if the current were closed it +could only be by the current of convection itself. +For that purpose it was sufficient to admit that a +``convection current''---\ie, a charged conductor in +motion---could act on the galvanometer. But experimental +confirmation was lacking. It appeared +difficult, in fact, to obtain a sufficient intensity +even by increasing as much as possible the charge +and the velocity of the conductors. Rowland, an +extremely skilful experimentalist, was the first to +triumph, or to seem to triumph, over these difficulties. +A disc received a strong \Chg{electrostatic}{electro-static} +charge and a very high speed of rotation. An +astatic magnetic system placed beside the disc +underwent deviations. The experiment was made +twice by Rowland, once in Berlin and once at Baltimore. +It was afterwards repeated by Himstedt. +These physicists even believed that they could +announce that they had succeeded in making +quantitative measurements. For twenty years +Rowland's law was admitted without objection +by all physicists, and, indeed, everything seemed +to confirm it. The spark certainly does produce a +magnetic effect, and does it not seem extremely +likely that the spark discharged is due to particles +taken from one of the electrodes and transferred +to the other electrode with their charge? Is not +the very spectrum of the spark, in which we +recognise the lines of the metal of the electrode, +a proof of it? The spark would then be a real +current of induction. +\PageSep{242} + +On the other hand, it is also admitted that in +an electrolyte the electricity is carried by the ions +in motion. The current in an electrolyte would +therefore also be a current of convection; but it +acts on the magnetic needle. And in the same +way for cathode rays; \Typo{Crooks}{Crookes} attributed these +rays to very subtle matter charged with negative +electricity and moving with very high velocity. +He looked upon them, in other words, as currents +of convection. Now, these cathode rays are +deviated by the magnet. In virtue of the +principle of action and \Chg{re-action}{reaction}, they should in +their turn deviate the magnetic needle. It is +true that Hertz believed he had proved that the +cathodic rays do not carry negative electricity, and +that they do not act on the magnetic needle; but +Hertz was wrong. First of all, Perrin succeeded +in collecting the electricity carried by these rays---electricity +of which Hertz denied the existence; the +German scientist appears to have been deceived +by the effects due to the action of the X-rays, +which were not yet discovered. Afterwards, and +quite recently, the action of the cathodic rays on +the magnetic needle has been brought to light. +Thus all these phenomena looked upon as currents +of convection, electric sparks, electrolytic currents, +cathodic rays, act in the same manner on the +galvanometer and in conformity to Rowland's +law. + +\Par[VI. ]{Lorentz's Theory.}---We need not go much +further. According to Lorentz's theory, currents +\PageSep{243} +of conduction would themselves be true convection +currents. Electricity would remain indissolubly +connected with certain material particles called +\emph{electrons}. The circulation of these electrons +through bodies would produce voltaic currents, +and what would distinguish conductors from +insulators would be that the one could be traversed +by these electrons, while the others would check +the movement of the electrons. Lorentz's theory +is very attractive. It gives a very simple explanation +of certain phenomena, which the earlier +theories---even Maxwell's in its primitive form---could +only deal with in an unsatisfactory manner; +for example, the aberration of light, the partial +impulse of luminous waves, magnetic polarisation, +and Zeeman's experiment. + +A few objections still remained. The phenomena +of an electric system seemed to depend on +the absolute velocity of translation of the centre +of gravity of this system, which is contrary to +the idea that we have of the relativity of space. +Supported by M.~Crémieu, M.~Lippman has presented +this objection in a very striking form. +Imagine two charged conductors with the same +velocity of translation. They are relatively at +rest. However, each of them being equivalent +to a current of convection, they ought to attract +one another, and by measuring this attraction +we could measure their absolute velocity. +``No!'' replied the partisans of Lorentz. ``What +we could measure in that way is not their +\PageSep{244} +absolute velocity, but their relative velocity \emph{with +respect to the ether}, so that the principle of relativity +is safe.'' Whatever there may be in these +objections, the edifice of electro-dynamics seemed, +at any rate in its broad lines, definitively constructed. +Everything was presented under the +most satisfactory aspect. The theories of Ampère +and Helmholtz, which were made for the open +currents that no longer existed, seem to have no +more than purely historic interest, and the inextricable +complications to which these theories +led have been almost forgotten. This quiescence +has been recently disturbed by the experiments of +M.~Crémieu, which have contradicted, or at least +have seemed to contradict, the results formerly +obtained by Rowland. Numerous investigators +have endeavoured to solve the question, and fresh +experiments have been undertaken. What result +will they give? I shall take care not to risk a +prophecy which might be falsified between the +day this book is ready for the press and the day on +which it is placed before the public. +\begin{center} +\vfill +\footnotesize THE END. +\vfill\vfill +\rule{1in}{0.5pt} \\[4pt] +\makebox[0pt][c]{\scriptsize THE WALTER SCOTT PUBLISHING CO., LIMITED, FELLING-ON-TYNE.} +\end{center} + +%%%%%%%%%%%%%%%%%%%%%%%%% GUTENBERG LICENSE %%%%%%%%%%%%%%%%%%%%%%%%%% +\PGLicense +\begin{PGtext} +End of Project Gutenberg's Science and hypothesis, by Henri Poincaré + +*** END OF THIS PROJECT GUTENBERG EBOOK SCIENCE AND HYPOTHESIS *** + +***** This file should be named 37157-t.tex or 37157-t.zip ***** +This and all associated files of various formats will be found in: + http://www.gutenberg.org/3/7/1/5/37157/ + +Produced by Andrew D. Hwang + +Updated editions will replace the previous one--the old editions +will be renamed. + +Creating the works from public domain print editions means that no +one owns a United States copyright in these works, so the Foundation +(and you!) can copy and distribute it in the United States without +permission and without paying copyright royalties. Special rules, +set forth in the General Terms of Use part of this license, apply to +copying and distributing Project Gutenberg-tm electronic works to +protect the PROJECT GUTENBERG-tm concept and trademark. Project +Gutenberg is a registered trademark, and may not be used if you +charge for the eBooks, unless you receive specific permission. If you +do not charge anything for copies of this eBook, complying with the +rules is very easy. You may use this eBook for nearly any purpose +such as creation of derivative works, reports, performances and +research. They may be modified and printed and given away--you may do +practically ANYTHING with public domain eBooks. Redistribution is +subject to the trademark license, especially commercial +redistribution. + + + +*** START: FULL LICENSE *** + +THE FULL PROJECT GUTENBERG LICENSE +PLEASE READ THIS BEFORE YOU DISTRIBUTE OR USE THIS WORK + +To protect the Project Gutenberg-tm mission of promoting the free +distribution of electronic works, by using or distributing this work +(or any other work associated in any way with the phrase "Project +Gutenberg"), you agree to comply with all the terms of the Full Project +Gutenberg-tm License (available with this file or online at +http://gutenberg.net/license). + + +Section 1. General Terms of Use and Redistributing Project Gutenberg-tm +electronic works + +1.A. By reading or using any part of this Project Gutenberg-tm +electronic work, you indicate that you have read, understand, agree to +and accept all the terms of this license and intellectual property +(trademark/copyright) agreement. If you do not agree to abide by all +the terms of this agreement, you must cease using and return or destroy +all copies of Project Gutenberg-tm electronic works in your possession. +If you paid a fee for obtaining a copy of or access to a Project +Gutenberg-tm electronic work and you do not agree to be bound by the +terms of this agreement, you may obtain a refund from the person or +entity to whom you paid the fee as set forth in paragraph 1.E.8. + +1.B. "Project Gutenberg" is a registered trademark. It may only be +used on or associated in any way with an electronic work by people who +agree to be bound by the terms of this agreement. There are a few +things that you can do with most Project Gutenberg-tm electronic works +even without complying with the full terms of this agreement. See +paragraph 1.C below. There are a lot of things you can do with Project +Gutenberg-tm electronic works if you follow the terms of this agreement +and help preserve free future access to Project Gutenberg-tm electronic +works. See paragraph 1.E below. + +1.C. The Project Gutenberg Literary Archive Foundation ("the Foundation" +or PGLAF), owns a compilation copyright in the collection of Project +Gutenberg-tm electronic works. Nearly all the individual works in the +collection are in the public domain in the United States. If an +individual work is in the public domain in the United States and you are +located in the United States, we do not claim a right to prevent you from +copying, distributing, performing, displaying or creating derivative +works based on the work as long as all references to Project Gutenberg +are removed. Of course, we hope that you will support the Project +Gutenberg-tm mission of promoting free access to electronic works by +freely sharing Project Gutenberg-tm works in compliance with the terms of +this agreement for keeping the Project Gutenberg-tm name associated with +the work. You can easily comply with the terms of this agreement by +keeping this work in the same format with its attached full Project +Gutenberg-tm License when you share it without charge with others. + +1.D. The copyright laws of the place where you are located also govern +what you can do with this work. Copyright laws in most countries are in +a constant state of change. If you are outside the United States, check +the laws of your country in addition to the terms of this agreement +before downloading, copying, displaying, performing, distributing or +creating derivative works based on this work or any other Project +Gutenberg-tm work. The Foundation makes no representations concerning +the copyright status of any work in any country outside the United +States. + +1.E. Unless you have removed all references to Project Gutenberg: + +1.E.1. The following sentence, with active links to, or other immediate +access to, the full Project Gutenberg-tm License must appear prominently +whenever any copy of a Project Gutenberg-tm work (any work on which the +phrase "Project Gutenberg" appears, or with which the phrase "Project +Gutenberg" is associated) is accessed, displayed, performed, viewed, +copied or distributed: + +This eBook is for the use of anyone anywhere at no cost and with +almost no restrictions whatsoever. You may copy it, give it away or +re-use it under the terms of the Project Gutenberg License included +with this eBook or online at www.gutenberg.net + +1.E.2. If an individual Project Gutenberg-tm electronic work is derived +from the public domain (does not contain a notice indicating that it is +posted with permission of the copyright holder), the work can be copied +and distributed to anyone in the United States without paying any fees +or charges. If you are redistributing or providing access to a work +with the phrase "Project Gutenberg" associated with or appearing on the +work, you must comply either with the requirements of paragraphs 1.E.1 +through 1.E.7 or obtain permission for the use of the work and the +Project Gutenberg-tm trademark as set forth in paragraphs 1.E.8 or +1.E.9. + +1.E.3. If an individual Project Gutenberg-tm electronic work is posted +with the permission of the copyright holder, your use and distribution +must comply with both paragraphs 1.E.1 through 1.E.7 and any additional +terms imposed by the copyright holder. Additional terms will be linked +to the Project Gutenberg-tm License for all works posted with the +permission of the copyright holder found at the beginning of this work. + +1.E.4. Do not unlink or detach or remove the full Project Gutenberg-tm +License terms from this work, or any files containing a part of this +work or any other work associated with Project Gutenberg-tm. + +1.E.5. Do not copy, display, perform, distribute or redistribute this +electronic work, or any part of this electronic work, without +prominently displaying the sentence set forth in paragraph 1.E.1 with +active links or immediate access to the full terms of the Project +Gutenberg-tm License. + +1.E.6. You may convert to and distribute this work in any binary, +compressed, marked up, nonproprietary or proprietary form, including any +word processing or hypertext form. However, if you provide access to or +distribute copies of a Project Gutenberg-tm work in a format other than +"Plain Vanilla ASCII" or other format used in the official version +posted on the official Project Gutenberg-tm web site (www.gutenberg.net), +you must, at no additional cost, fee or expense to the user, provide a +copy, a means of exporting a copy, or a means of obtaining a copy upon +request, of the work in its original "Plain Vanilla ASCII" or other +form. Any alternate format must include the full Project Gutenberg-tm +License as specified in paragraph 1.E.1. + +1.E.7. Do not charge a fee for access to, viewing, displaying, +performing, copying or distributing any Project Gutenberg-tm works +unless you comply with paragraph 1.E.8 or 1.E.9. + +1.E.8. You may charge a reasonable fee for copies of or providing +access to or distributing Project Gutenberg-tm electronic works provided +that + +- You pay a royalty fee of 20% of the gross profits you derive from + the use of Project Gutenberg-tm works calculated using the method + you already use to calculate your applicable taxes. The fee is + owed to the owner of the Project Gutenberg-tm trademark, but he + has agreed to donate royalties under this paragraph to the + Project Gutenberg Literary Archive Foundation. Royalty payments + must be paid within 60 days following each date on which you + prepare (or are legally required to prepare) your periodic tax + returns. Royalty payments should be clearly marked as such and + sent to the Project Gutenberg Literary Archive Foundation at the + address specified in Section 4, "Information about donations to + the Project Gutenberg Literary Archive Foundation." + +- You provide a full refund of any money paid by a user who notifies + you in writing (or by e-mail) within 30 days of receipt that s/he + does not agree to the terms of the full Project Gutenberg-tm + License. You must require such a user to return or + destroy all copies of the works possessed in a physical medium + and discontinue all use of and all access to other copies of + Project Gutenberg-tm works. + +- You provide, in accordance with paragraph 1.F.3, a full refund of any + money paid for a work or a replacement copy, if a defect in the + electronic work is discovered and reported to you within 90 days + of receipt of the work. + +- You comply with all other terms of this agreement for free + distribution of Project Gutenberg-tm works. + +1.E.9. If you wish to charge a fee or distribute a Project Gutenberg-tm +electronic work or group of works on different terms than are set +forth in this agreement, you must obtain permission in writing from +both the Project Gutenberg Literary Archive Foundation and Michael +Hart, the owner of the Project Gutenberg-tm trademark. Contact the +Foundation as set forth in Section 3 below. + +1.F. + +1.F.1. Project Gutenberg volunteers and employees expend considerable +effort to identify, do copyright research on, transcribe and proofread +public domain works in creating the Project Gutenberg-tm +collection. Despite these efforts, Project Gutenberg-tm electronic +works, and the medium on which they may be stored, may contain +"Defects," such as, but not limited to, incomplete, inaccurate or +corrupt data, transcription errors, a copyright or other intellectual +property infringement, a defective or damaged disk or other medium, a +computer virus, or computer codes that damage or cannot be read by +your equipment. + +1.F.2. LIMITED WARRANTY, DISCLAIMER OF DAMAGES - Except for the "Right +of Replacement or Refund" described in paragraph 1.F.3, the Project +Gutenberg Literary Archive Foundation, the owner of the Project +Gutenberg-tm trademark, and any other party distributing a Project +Gutenberg-tm electronic work under this agreement, disclaim all +liability to you for damages, costs and expenses, including legal +fees. YOU AGREE THAT YOU HAVE NO REMEDIES FOR NEGLIGENCE, STRICT +LIABILITY, BREACH OF WARRANTY OR BREACH OF CONTRACT EXCEPT THOSE +PROVIDED IN PARAGRAPH 1.F.3. YOU AGREE THAT THE FOUNDATION, THE +TRADEMARK OWNER, AND ANY DISTRIBUTOR UNDER THIS AGREEMENT WILL NOT BE +LIABLE TO YOU FOR ACTUAL, DIRECT, INDIRECT, CONSEQUENTIAL, PUNITIVE OR +INCIDENTAL DAMAGES EVEN IF YOU GIVE NOTICE OF THE POSSIBILITY OF SUCH +DAMAGE. + +1.F.3. LIMITED RIGHT OF REPLACEMENT OR REFUND - If you discover a +defect in this electronic work within 90 days of receiving it, you can +receive a refund of the money (if any) you paid for it by sending a +written explanation to the person you received the work from. If you +received the work on a physical medium, you must return the medium with +your written explanation. The person or entity that provided you with +the defective work may elect to provide a replacement copy in lieu of a +refund. If you received the work electronically, the person or entity +providing it to you may choose to give you a second opportunity to +receive the work electronically in lieu of a refund. If the second copy +is also defective, you may demand a refund in writing without further +opportunities to fix the problem. + +1.F.4. Except for the limited right of replacement or refund set forth +in paragraph 1.F.3, this work is provided to you 'AS-IS' WITH NO OTHER +WARRANTIES OF ANY KIND, EXPRESS OR IMPLIED, INCLUDING BUT NOT LIMITED TO +WARRANTIES OF MERCHANTIBILITY OR FITNESS FOR ANY PURPOSE. + +1.F.5. Some states do not allow disclaimers of certain implied +warranties or the exclusion or limitation of certain types of damages. +If any disclaimer or limitation set forth in this agreement violates the +law of the state applicable to this agreement, the agreement shall be +interpreted to make the maximum disclaimer or limitation permitted by +the applicable state law. The invalidity or unenforceability of any +provision of this agreement shall not void the remaining provisions. + +1.F.6. INDEMNITY - You agree to indemnify and hold the Foundation, the +trademark owner, any agent or employee of the Foundation, anyone +providing copies of Project Gutenberg-tm electronic works in accordance +with this agreement, and any volunteers associated with the production, +promotion and distribution of Project Gutenberg-tm electronic works, +harmless from all liability, costs and expenses, including legal fees, +that arise directly or indirectly from any of the following which you do +or cause to occur: (a) distribution of this or any Project Gutenberg-tm +work, (b) alteration, modification, or additions or deletions to any +Project Gutenberg-tm work, and (c) any Defect you cause. + + +Section 2. Information about the Mission of Project Gutenberg-tm + +Project Gutenberg-tm is synonymous with the free distribution of +electronic works in formats readable by the widest variety of computers +including obsolete, old, middle-aged and new computers. It exists +because of the efforts of hundreds of volunteers and donations from +people in all walks of life. + +Volunteers and financial support to provide volunteers with the +assistance they need are critical to reaching Project Gutenberg-tm's +goals and ensuring that the Project Gutenberg-tm collection will +remain freely available for generations to come. In 2001, the Project +Gutenberg Literary Archive Foundation was created to provide a secure +and permanent future for Project Gutenberg-tm and future generations. +To learn more about the Project Gutenberg Literary Archive Foundation +and how your efforts and donations can help, see Sections 3 and 4 +and the Foundation web page at http://www.pglaf.org. + + +Section 3. Information about the Project Gutenberg Literary Archive +Foundation + +The Project Gutenberg Literary Archive Foundation is a non profit +501(c)(3) educational corporation organized under the laws of the +state of Mississippi and granted tax exempt status by the Internal +Revenue Service. The Foundation's EIN or federal tax identification +number is 64-6221541. Its 501(c)(3) letter is posted at +http://pglaf.org/fundraising. Contributions to the Project Gutenberg +Literary Archive Foundation are tax deductible to the full extent +permitted by U.S. federal laws and your state's laws. + +The Foundation's principal office is located at 4557 Melan Dr. S. +Fairbanks, AK, 99712., but its volunteers and employees are scattered +throughout numerous locations. Its business office is located at +809 North 1500 West, Salt Lake City, UT 84116, (801) 596-1887, email +business@pglaf.org. Email contact links and up to date contact +information can be found at the Foundation's web site and official +page at http://pglaf.org + +For additional contact information: + Dr. Gregory B. Newby + Chief Executive and Director + gbnewby@pglaf.org + + +Section 4. Information about Donations to the Project Gutenberg +Literary Archive Foundation + +Project Gutenberg-tm depends upon and cannot survive without wide +spread public support and donations to carry out its mission of +increasing the number of public domain and licensed works that can be +freely distributed in machine readable form accessible by the widest +array of equipment including outdated equipment. Many small donations +($1 to $5,000) are particularly important to maintaining tax exempt +status with the IRS. + +The Foundation is committed to complying with the laws regulating +charities and charitable donations in all 50 states of the United +States. Compliance requirements are not uniform and it takes a +considerable effort, much paperwork and many fees to meet and keep up +with these requirements. We do not solicit donations in locations +where we have not received written confirmation of compliance. To +SEND DONATIONS or determine the status of compliance for any +particular state visit http://pglaf.org + +While we cannot and do not solicit contributions from states where we +have not met the solicitation requirements, we know of no prohibition +against accepting unsolicited donations from donors in such states who +approach us with offers to donate. + +International donations are gratefully accepted, but we cannot make +any statements concerning tax treatment of donations received from +outside the United States. U.S. laws alone swamp our small staff. + +Please check the Project Gutenberg Web pages for current donation +methods and addresses. Donations are accepted in a number of other +ways including including checks, online payments and credit card +donations. To donate, please visit: http://pglaf.org/donate + + +Section 5. General Information About Project Gutenberg-tm electronic +works. + +Professor Michael S. Hart is the originator of the Project Gutenberg-tm +concept of a library of electronic works that could be freely shared +with anyone. For thirty years, he produced and distributed Project +Gutenberg-tm eBooks with only a loose network of volunteer support. + + +Project Gutenberg-tm eBooks are often created from several printed +editions, all of which are confirmed as Public Domain in the U.S. +unless a copyright notice is included. Thus, we do not necessarily +keep eBooks in compliance with any particular paper edition. + + +Most people start at our Web site which has the main PG search facility: + + http://www.gutenberg.net + +This Web site includes information about Project Gutenberg-tm, +including how to make donations to the Project Gutenberg Literary +Archive Foundation, how to help produce our new eBooks, and how to +subscribe to our email newsletter to hear about new eBooks. +\end{PGtext} + +% %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% % +% % +% End of Project Gutenberg's Science and hypothesis, by Henri Poincaré % +% % +% *** END OF THIS PROJECT GUTENBERG EBOOK SCIENCE AND HYPOTHESIS *** % +% % +% ***** This file should be named 37157-t.tex or 37157-t.zip ***** % +% This and all associated files of various formats will be found in: % +% http://www.gutenberg.org/3/7/1/5/37157/ % +% % +% %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% % + +\end{document} +### +@ControlwordReplace = ( + ['\\ie', 'i.e.'], + ['\\QED', 'Q.E.D.'] + ); + +@ControlwordArguments = ( + ['\\Signature', 1, 1, '', ' ', 1, 1, '', ''], + ['\\BookMark', 1, 0, '', '', 1, 0, '', ''], + ['\\First', 1, 1, '', ''], + ['\\Part', 1, 1, 'Part ', ' ', 1, 1, '', ''], + ['\\OtherChapter', 1, 1, '', ''], + ['\\Chapter', 0, 0, '', '', 1, 1, 'Chapter ', ' ', 1, 1, '', ''], + ['\\ChapRef', 1, 1, 'Chapter ', ''], + ['\\hyperref', 0, 0, '', '', 1, 1, '', ''], + ['\\Section', 1, 1, '', ''], + ['\\Subsection', 1, 1, '', ''], + ['\\Par', 0, 1, '', '', 1, 1, '', ''], + ['\\Dict', 1, 1, '', ': ', 1, 1, '', ''], + ['\\Pagelabel', 1, 0, '', ''], + ['\\Pageref', 1, 1, 'p. ', ''], + ['\\Pagerefs', 1, 1, 'pp. ', ', ', 1, 1, '', ''], + ['\\Reword', 1, 0, '', '', 1, 1, '', ''], + ['\\Typo', 1, 0, '', '', 1, 1, '', ''], + ['\\Chg', 1, 0, '', '', 1, 1, '', ''], + ['\\Add', 1, 1, '', ''] + ); +$PageSeparator = qr/^\\PageSep/; +$CustomClean = 'print "\\nCustom cleaning in progress..."; +my $cline = 0; + while ($cline <= $#file) { + $file[$cline] =~ s/--------[^\n]*\n//; # strip page separators + $cline++ + } + print "done\\n";'; +### +This is pdfTeXk, Version 3.141592-1.40.3 (Web2C 7.5.6) (format=pdflatex 2010.5.6) 21 AUG 2011 16:35 +entering extended mode + %&-line parsing enabled. +**37157-t.tex +(./37157-t.tex +LaTeX2e <2005/12/01> +Babel <v3.8h> and hyphenation patterns for english, usenglishmax, dumylang, noh +yphenation, arabic, farsi, croatian, ukrainian, russian, bulgarian, czech, slov +ak, danish, dutch, finnish, basque, french, german, ngerman, ibycus, greek, mon +ogreek, ancientgreek, hungarian, italian, latin, mongolian, norsk, icelandic, i +nterlingua, turkish, coptic, romanian, welsh, serbian, slovenian, estonian, esp +eranto, uppersorbian, indonesian, polish, portuguese, spanish, catalan, galicia +n, swedish, ukenglish, pinyin, loaded. +(/usr/share/texmf-texlive/tex/latex/base/book.cls +Document Class: book 2005/09/16 v1.4f Standard LaTeX document class +(/usr/share/texmf-texlive/tex/latex/base/leqno.clo +File: leqno.clo 1998/08/17 v1.1c Standard LaTeX option (left equation numbers) +) (/usr/share/texmf-texlive/tex/latex/base/bk12.clo +File: bk12.clo 2005/09/16 v1.4f Standard LaTeX file (size option) +) +\c@part=\count79 +\c@chapter=\count80 +\c@section=\count81 +\c@subsection=\count82 +\c@subsubsection=\count83 +\c@paragraph=\count84 +\c@subparagraph=\count85 +\c@figure=\count86 +\c@table=\count87 +\abovecaptionskip=\skip41 +\belowcaptionskip=\skip42 +\bibindent=\dimen102 +) (/usr/share/texmf-texlive/tex/latex/base/inputenc.sty +Package: inputenc 2006/05/05 v1.1b Input encoding file +\inpenc@prehook=\toks14 +\inpenc@posthook=\toks15 +(/usr/share/texmf-texlive/tex/latex/base/latin1.def +File: latin1.def 2006/05/05 v1.1b Input encoding file +)) (/usr/share/texmf-texlive/tex/latex/base/fontenc.sty +Package: fontenc 2005/09/27 v1.99g Standard LaTeX package +(/usr/share/texmf-texlive/tex/latex/base/t1enc.def +File: t1enc.def 2005/09/27 v1.99g Standard LaTeX file +LaTeX Font Info: Redeclaring font encoding T1 on input line 43. +)) (/usr/share/texmf-texlive/tex/latex/base/ifthen.sty +Package: ifthen 2001/05/26 v1.1c Standard LaTeX ifthen package (DPC) +) (/usr/share/texmf-texlive/tex/latex/amsmath/amsmath.sty +Package: amsmath 2000/07/18 v2.13 AMS math features +\@mathmargin=\skip43 +For additional information on amsmath, use the `?' option. +(/usr/share/texmf-texlive/tex/latex/amsmath/amstext.sty +Package: amstext 2000/06/29 v2.01 +(/usr/share/texmf-texlive/tex/latex/amsmath/amsgen.sty +File: amsgen.sty 1999/11/30 v2.0 +\@emptytoks=\toks16 +\ex@=\dimen103 +)) (/usr/share/texmf-texlive/tex/latex/amsmath/amsbsy.sty +Package: amsbsy 1999/11/29 v1.2d +\pmbraise@=\dimen104 +) (/usr/share/texmf-texlive/tex/latex/amsmath/amsopn.sty +Package: amsopn 1999/12/14 v2.01 operator names +) +\inf@bad=\count88 +LaTeX Info: Redefining \frac on input line 211. +\uproot@=\count89 +\leftroot@=\count90 +LaTeX Info: Redefining \overline on input line 307. +\classnum@=\count91 +\DOTSCASE@=\count92 +LaTeX Info: Redefining \ldots on input line 379. +LaTeX Info: Redefining \dots on input line 382. +LaTeX Info: Redefining \cdots on input line 467. +\Mathstrutbox@=\box26 +\strutbox@=\box27 +\big@size=\dimen105 +LaTeX Font Info: Redeclaring font encoding OML on input line 567. +LaTeX Font Info: Redeclaring font encoding OMS on input line 568. +\macc@depth=\count93 +\c@MaxMatrixCols=\count94 +\dotsspace@=\muskip10 +\c@parentequation=\count95 +\dspbrk@lvl=\count96 +\tag@help=\toks17 +\row@=\count97 +\column@=\count98 +\maxfields@=\count99 +\andhelp@=\toks18 +\eqnshift@=\dimen106 +\alignsep@=\dimen107 +\tagshift@=\dimen108 +\tagwidth@=\dimen109 +\totwidth@=\dimen110 +\lineht@=\dimen111 +\@envbody=\toks19 +\multlinegap=\skip44 +\multlinetaggap=\skip45 +\mathdisplay@stack=\toks20 +LaTeX Info: Redefining \[ on input line 2666. +LaTeX Info: Redefining \] on input line 2667. +) (/usr/share/texmf-texlive/tex/latex/amsfonts/amssymb.sty +Package: amssymb 2002/01/22 v2.2d +(/usr/share/texmf-texlive/tex/latex/amsfonts/amsfonts.sty +Package: amsfonts 2001/10/25 v2.2f +\symAMSa=\mathgroup4 +\symAMSb=\mathgroup5 +LaTeX Font Info: Overwriting math alphabet `\mathfrak' in version `bold' +(Font) U/euf/m/n --> U/euf/b/n on input line 132. +)) (/usr/share/texmf-texlive/tex/latex/base/alltt.sty +Package: alltt 1997/06/16 v2.0g defines alltt environment +) (/usr/share/texmf-texlive/tex/latex/yfonts/yfonts.sty +Package: yfonts 2003/01/08 v1.3 (WaS) +) (/usr/share/texmf-texlive/tex/latex/footmisc/footmisc.sty +Package: footmisc 2005/03/17 v5.3d a miscellany of footnote facilities +\FN@temptoken=\toks21 +\footnotemargin=\dimen112 +\c@pp@next@reset=\count100 +\c@@fnserial=\count101 +Package footmisc Info: Declaring symbol style bringhurst on input line 817. +Package footmisc Info: Declaring symbol style chicago on input line 818. +Package footmisc Info: Declaring symbol style wiley on input line 819. +Package footmisc Info: Declaring symbol style lamport-robust on input line 823. + +Package footmisc Info: Declaring symbol style lamport* on input line 831. +Package footmisc Info: Declaring symbol style lamport*-robust on input line 840 +. +) (/usr/share/texmf-texlive/tex/latex/graphics/graphicx.sty +Package: graphicx 1999/02/16 v1.0f Enhanced LaTeX Graphics (DPC,SPQR) +(/usr/share/texmf-texlive/tex/latex/graphics/keyval.sty +Package: keyval 1999/03/16 v1.13 key=value parser (DPC) +\KV@toks@=\toks22 +) (/usr/share/texmf-texlive/tex/latex/graphics/graphics.sty +Package: graphics 2006/02/20 v1.0o Standard LaTeX Graphics (DPC,SPQR) +(/usr/share/texmf-texlive/tex/latex/graphics/trig.sty +Package: trig 1999/03/16 v1.09 sin cos tan (DPC) +) (/etc/texmf/tex/latex/config/graphics.cfg +File: graphics.cfg 2007/01/18 v1.5 graphics configuration of teTeX/TeXLive +) +Package graphics Info: Driver file: pdftex.def on input line 90. +(/usr/share/texmf-texlive/tex/latex/pdftex-def/pdftex.def +File: pdftex.def 2007/01/08 v0.04d Graphics/color for pdfTeX +\Gread@gobject=\count102 +)) +\Gin@req@height=\dimen113 +\Gin@req@width=\dimen114 +) (/usr/share/texmf-texlive/tex/latex/tools/calc.sty +Package: calc 2005/08/06 v4.2 Infix arithmetic (KKT,FJ) +\calc@Acount=\count103 +\calc@Bcount=\count104 +\calc@Adimen=\dimen115 +\calc@Bdimen=\dimen116 +\calc@Askip=\skip46 +\calc@Bskip=\skip47 +LaTeX Info: Redefining \setlength on input line 75. +LaTeX Info: Redefining \addtolength on input line 76. +\calc@Ccount=\count105 +\calc@Cskip=\skip48 +) (/usr/share/texmf-texlive/tex/latex/fancyhdr/fancyhdr.sty +\fancy@headwidth=\skip49 +\f@ncyO@elh=\skip50 +\f@ncyO@erh=\skip51 +\f@ncyO@olh=\skip52 +\f@ncyO@orh=\skip53 +\f@ncyO@elf=\skip54 +\f@ncyO@erf=\skip55 +\f@ncyO@olf=\skip56 +\f@ncyO@orf=\skip57 +) (/usr/share/texmf-texlive/tex/latex/geometry/geometry.sty +Package: geometry 2002/07/08 v3.2 Page Geometry +\Gm@cnth=\count106 +\Gm@cntv=\count107 +\c@Gm@tempcnt=\count108 +\Gm@bindingoffset=\dimen117 +\Gm@wd@mp=\dimen118 +\Gm@odd@mp=\dimen119 +\Gm@even@mp=\dimen120 +\Gm@dimlist=\toks23 +(/usr/share/texmf-texlive/tex/xelatex/xetexconfig/geometry.cfg) + +Package geometry Warning: `tmargin' and `bmargin' result in NEGATIVE (-0.44386p +t). + `height' should be shortened in length. + +) (/usr/share/texmf-texlive/tex/latex/hyperref/hyperref.sty +Package: hyperref 2007/02/07 v6.75r Hypertext links for LaTeX +\@linkdim=\dimen121 +\Hy@linkcounter=\count109 +\Hy@pagecounter=\count110 +(/usr/share/texmf-texlive/tex/latex/hyperref/pd1enc.def +File: pd1enc.def 2007/02/07 v6.75r Hyperref: PDFDocEncoding definition (HO) +) (/etc/texmf/tex/latex/config/hyperref.cfg +File: hyperref.cfg 2002/06/06 v1.2 hyperref configuration of TeXLive +) (/usr/share/texmf-texlive/tex/latex/oberdiek/kvoptions.sty +Package: kvoptions 2006/08/22 v2.4 Connects package keyval with LaTeX options ( +HO) +) +Package hyperref Info: Option `hyperfootnotes' set `false' on input line 2238. +Package hyperref Info: Option `bookmarks' set `true' on input line 2238. +Package hyperref Info: Option `linktocpage' set `false' on input line 2238. +Package hyperref Info: Option `pdfdisplaydoctitle' set `true' on input line 223 +8. +Package hyperref Info: Option `pdfpagelabels' set `true' on input line 2238. +Package hyperref Info: Option `bookmarksopen' set `true' on input line 2238. +Package hyperref Info: Option `colorlinks' set `true' on input line 2238. +Package hyperref Info: Hyper figures OFF on input line 2288. +Package hyperref Info: Link nesting OFF on input line 2293. +Package hyperref Info: Hyper index ON on input line 2296. +Package hyperref Info: Plain pages OFF on input line 2303. +Package hyperref Info: Backreferencing OFF on input line 2308. +Implicit mode ON; LaTeX internals redefined +Package hyperref Info: Bookmarks ON on input line 2444. +(/usr/share/texmf-texlive/tex/latex/ltxmisc/url.sty +\Urlmuskip=\muskip11 +Package: url 2005/06/27 ver 3.2 Verb mode for urls, etc. +) +LaTeX Info: Redefining \url on input line 2599. +\Fld@menulength=\count111 +\Field@Width=\dimen122 +\Fld@charsize=\dimen123 +\Choice@toks=\toks24 +\Field@toks=\toks25 +Package hyperref Info: Hyper figures OFF on input line 3102. +Package hyperref Info: Link nesting OFF on input line 3107. +Package hyperref Info: Hyper index ON on input line 3110. +Package hyperref Info: backreferencing OFF on input line 3117. +Package hyperref Info: Link coloring ON on input line 3120. +\Hy@abspage=\count112 +\c@Item=\count113 +) +*hyperref using driver hpdftex* +(/usr/share/texmf-texlive/tex/latex/hyperref/hpdftex.def +File: hpdftex.def 2007/02/07 v6.75r Hyperref driver for pdfTeX +\Fld@listcount=\count114 +) +\TmpLen=\skip58 +\c@ChapNo=\count115 +\c@ChapCount=\count116 +(./37157-t.aux) +\openout1 = `37157-t.aux'. + +LaTeX Font Info: Checking defaults for OML/cmm/m/it on input line 517. +LaTeX Font Info: ... okay on input line 517. +LaTeX Font Info: Checking defaults for T1/cmr/m/n on input line 517. +LaTeX Font Info: ... okay on input line 517. +LaTeX Font Info: Checking defaults for OT1/cmr/m/n on input line 517. +LaTeX Font Info: ... okay on input line 517. +LaTeX Font Info: Checking defaults for OMS/cmsy/m/n on input line 517. +LaTeX Font Info: ... okay on input line 517. +LaTeX Font Info: Checking defaults for OMX/cmex/m/n on input line 517. +LaTeX Font Info: ... okay on input line 517. +LaTeX Font Info: Checking defaults for U/cmr/m/n on input line 517. +LaTeX Font Info: ... okay on input line 517. +LaTeX Font Info: Checking defaults for LY/yfrak/m/n on input line 517. +LaTeX Font Info: ... okay on input line 517. +LaTeX Font Info: Checking defaults for LYG/ygoth/m/n on input line 517. +LaTeX Font Info: ... okay on input line 517. +LaTeX Font Info: Checking defaults for PD1/pdf/m/n on input line 517. +LaTeX Font Info: ... okay on input line 517. +(/usr/share/texmf/tex/context/base/supp-pdf.tex +[Loading MPS to PDF converter (version 2006.09.02).] +\scratchcounter=\count117 +\scratchdimen=\dimen124 +\scratchbox=\box28 +\nofMPsegments=\count118 +\nofMParguments=\count119 +\everyMPshowfont=\toks26 +\MPscratchCnt=\count120 +\MPscratchDim=\dimen125 +\MPnumerator=\count121 +\everyMPtoPDFconversion=\toks27 +) +-------------------- Geometry parameters +paper: class default +landscape: -- +twocolumn: -- +twoside: true +asymmetric: -- +h-parts: 9.03375pt, 289.07999pt, 9.03375pt +v-parts: -0.17752pt, 415.99635pt, -0.26634pt +hmarginratio: 1:1 +vmarginratio: 2:3 +lines: -- +heightrounded: -- +bindingoffset: 0.0pt +truedimen: -- +includehead: true +includefoot: true +includemp: -- +driver: pdftex +-------------------- Page layout dimensions and switches +\paperwidth 307.14749pt +\paperheight 415.55249pt +\textwidth 289.07999pt +\textheight 354.12256pt +\oddsidemargin -63.23624pt +\evensidemargin -63.23624pt +\topmargin -72.44751pt +\headheight 12.0pt +\headsep 19.8738pt +\footskip 30.0pt +\marginparwidth 98.0pt +\marginparsep 7.0pt +\columnsep 10.0pt +\skip\footins 10.8pt plus 4.0pt minus 2.0pt +\hoffset 0.0pt +\voffset 0.0pt +\mag 1000 +\@twosidetrue \@mparswitchtrue +(1in=72.27pt, 1cm=28.45pt) +----------------------- +(/usr/share/texmf-texlive/tex/latex/graphics/color.sty +Package: color 2005/11/14 v1.0j Standard LaTeX Color (DPC) +(/etc/texmf/tex/latex/config/color.cfg +File: color.cfg 2007/01/18 v1.5 color configuration of teTeX/TeXLive +) +Package color Info: Driver file: pdftex.def on input line 130. +) +Package hyperref Info: Link coloring ON on input line 517. +(/usr/share/texmf-texlive/tex/latex/hyperref/nameref.sty +Package: nameref 2006/12/27 v2.28 Cross-referencing by name of section +(/usr/share/texmf-texlive/tex/latex/oberdiek/refcount.sty +Package: refcount 2006/02/20 v3.0 Data extraction from references (HO) +) +\c@section@level=\count122 +) +LaTeX Info: Redefining \ref on input line 517. +LaTeX Info: Redefining \pageref on input line 517. +(./37157-t.out) (./37157-t.out) +\@outlinefile=\write3 +\openout3 = `37157-t.out'. + +LaTeX Font Info: Try loading font information for T1+cmtt on input line 523. + +(/usr/share/texmf-texlive/tex/latex/base/t1cmtt.fd +File: t1cmtt.fd 1999/05/25 v2.5h Standard LaTeX font definitions +) +LaTeX Font Info: Try loading font information for U+msa on input line 544. +(/usr/share/texmf-texlive/tex/latex/amsfonts/umsa.fd +File: umsa.fd 2002/01/19 v2.2g AMS font definitions +) +LaTeX Font Info: Try loading font information for U+msb on input line 544. +(/usr/share/texmf-texlive/tex/latex/amsfonts/umsb.fd +File: umsb.fd 2002/01/19 v2.2g AMS font definitions +) [1 + +{/var/lib/texmf/fonts/map/pdftex/updmap/pdftex.map}] [2] +LaTeX Font Info: Try loading font information for OML+cmr on input line 597. + +(/usr/share/texmf-texlive/tex/latex/base/omlcmr.fd +File: omlcmr.fd 1999/05/25 v2.5h Standard LaTeX font definitions +) +LaTeX Font Info: Font shape `OML/cmr/m/it' in size <12> not available +(Font) Font shape `OML/cmm/m/it' tried instead on input line 597. +[1 + + +] (./37157-t.toc [2 + + + +] [3]) +\tf@toc=\write4 +\openout4 = `37157-t.toc'. + +[4] <./images/tb.pdf, id=211, 469.755pt x 56.21pt> +File: ./images/tb.pdf Graphic file (type pdf) +<use ./images/tb.pdf> [5 + + + <./images/tb.pdf>] +File: ./images/tb.pdf Graphic file (type pdf) +<use ./images/tb.pdf> [6 + + +] [7] [8] [9] [10] [11] [12] [13] [14] +Underfull \hbox (badness 10000) in paragraph at lines 978--980 + + [] + +[15] +File: ./images/tb.pdf Graphic file (type pdf) +<use ./images/tb.pdf> [16 + + +] [17] [18] [19] [20] [21] [22] +File: ./images/tb.pdf Graphic file (type pdf) +<use ./images/tb.pdf> [1 + + + + + +] [2] [3] [4] [5] [6] [7] [8] [9] [10] [11] [12] [13] [14] [15] [16] [17] +Underfull \hbox (badness 1360) in paragraph at lines 1705--1710 +[]\T1/cmr/m/n/12 No doubt math-e-mat-i-cal re-cur-rent rea-son-ing and + [] + +[18] [19] [20] [21] [22 + + +] [23] [24] [25] [26] [27] [28] +Underfull \hbox (badness 1442) in paragraph at lines 2041--2059 +[]\T1/cmr/m/n/12 Nothing dis-tin-guishes a length di-rectly ob-served + [] + +[29] [30] [31] [32] [33] [34] [35] [36] [37] [38] [39] +Underfull \hbox (badness 1210) in paragraph at lines 2361--2368 +[]\T1/cmr/m/it/12 The Math-e-mat-i-cal Con-tin-uum of Sev-eral Di-men- + [] + +[40] [41] [42 + + +] [43] [44] [45] [46] [47] [48] [49] [50] [51] [52] [53] [54] [55] [56] [57] [5 +8] [59] [60 + + +] [61] [62] [63] [64] [65] [66] [67] [68] [69] [70] [71] [72] [73] [74] +Underfull \hbox (badness 1917) in paragraph at lines 3365--3383 +[]\T1/cmr/m/it/12 The Non-Euclidean World.\T1/cmr/m/n/12 ---If ge-o-met-ri-cal +space + [] + +[75] [76] [77] [78] [79] [80] [81] [82] [83 + + +] [84] [85] [86] [87] [88] [89] [90] [91] [92] [93] [94] [95] [96] [97] [98] [9 +9] [100] [101 + + +] [102] [103] [104] [105] [106] [107] [108] [109] [110] [111] [112] [113] [114] +[115] [116] [117] [118] [119] [120] [121] [122] [123] [124] [125 + + +] [126] [127] [128] [129] [130] [131] [132] [133] [134] [135] [136] [137] [138 + + +] [139] [140] [141] [142] [143] [144] [145] [146] [147] [148] [149] [150] [151] +[152] [153] [154] [155] [156 + + +] [157] [158] [159] [160] [161] [162] [163] [164] [165] [166] [167] [168] [169] +[170] [171] [172] [173] [174] [175] [176] [177] [178 + + +] [179] [180] [181] [182] [183] [184] +Underfull \hbox (badness 1442) in paragraph at lines 6638--6656 +[]\T1/cmr/m/it/12 Physics and Mech-a-nism.\T1/cmr/m/n/12 ---Most the-o-rists ha +ve a + [] + +[185] [186] [187] [188] [189] [190] [191] [192] [193] [194] [195] [196] [197] [ +198] [199] [200] [201] [202] [203] [204 + + +] [205] [206] [207] [208] [209] [210] [211] [212] [213] [214] [215] [216] [217] +[218] [219] [220] [221] [222] [223] [224] [225] [226] [227] [228] [229] [230] [ +231] [232] [233] [234] [235 + + +] [236] [237] [238] [239] [240] [241] [242] [243] [244] [245] [246] [247] [248] +[249] [250] +Underfull \hbox (badness 3250) in paragraph at lines 8568--8620 +[]\T1/cmr/m/n/12 I. \T1/cmr/m/it/12 Am-père's The-ory.\T1/cmr/m/n/12 ---In Am-p +ère's ex-per-i-men-tal + [] + +[251 + + +] [252] [253] [254] [255] [256] +Underfull \hbox (badness 2426) in paragraph at lines 8740--8770 +[]\T1/cmr/m/n/12 3. \T1/cmr/m/it/12 Con-tin-u-ous Ro-ta-tions.\T1/cmr/m/n/12 -- +-The most re-mark-able + [] + +[257] [258] [259] [260] [261] [262] [263] [264] +Overfull \hbox (0.82681pt too wide) in paragraph at lines 9008--9029 +[]\T1/cmr/m/n/12 III. \T1/cmr/m/it/12 Dif-fi-cul-ties raised by these The-o-rie +s.\T1/cmr/m/n/12 ---Helmholtz's + [] + +[265] [266] [267] [268] [269] [270] [271] [272] [1 + + +] [2] [3] [4] [5] [6] [7] [8] [9] [10] (./37157-t.aux) + + *File List* + book.cls 2005/09/16 v1.4f Standard LaTeX document class + leqno.clo 1998/08/17 v1.1c Standard LaTeX option (left equation numbers) + bk12.clo 2005/09/16 v1.4f Standard LaTeX file (size option) +inputenc.sty 2006/05/05 v1.1b Input encoding file + latin1.def 2006/05/05 v1.1b Input encoding file + fontenc.sty + t1enc.def 2005/09/27 v1.99g Standard LaTeX file + ifthen.sty 2001/05/26 v1.1c Standard LaTeX ifthen package (DPC) + amsmath.sty 2000/07/18 v2.13 AMS math features + amstext.sty 2000/06/29 v2.01 + amsgen.sty 1999/11/30 v2.0 + amsbsy.sty 1999/11/29 v1.2d + amsopn.sty 1999/12/14 v2.01 operator names + amssymb.sty 2002/01/22 v2.2d +amsfonts.sty 2001/10/25 v2.2f + alltt.sty 1997/06/16 v2.0g defines alltt environment + yfonts.sty 2003/01/08 v1.3 (WaS) +footmisc.sty 2005/03/17 v5.3d a miscellany of footnote facilities +graphicx.sty 1999/02/16 v1.0f Enhanced LaTeX Graphics (DPC,SPQR) + keyval.sty 1999/03/16 v1.13 key=value parser (DPC) +graphics.sty 2006/02/20 v1.0o Standard LaTeX Graphics (DPC,SPQR) + trig.sty 1999/03/16 v1.09 sin cos tan (DPC) +graphics.cfg 2007/01/18 v1.5 graphics configuration of teTeX/TeXLive + pdftex.def 2007/01/08 v0.04d Graphics/color for pdfTeX + calc.sty 2005/08/06 v4.2 Infix arithmetic (KKT,FJ) +fancyhdr.sty +geometry.sty 2002/07/08 v3.2 Page Geometry +geometry.cfg +hyperref.sty 2007/02/07 v6.75r Hypertext links for LaTeX + pd1enc.def 2007/02/07 v6.75r Hyperref: PDFDocEncoding definition (HO) +hyperref.cfg 2002/06/06 v1.2 hyperref configuration of TeXLive +kvoptions.sty 2006/08/22 v2.4 Connects package keyval with LaTeX options (HO +) + url.sty 2005/06/27 ver 3.2 Verb mode for urls, etc. + hpdftex.def 2007/02/07 v6.75r Hyperref driver for pdfTeX +supp-pdf.tex + color.sty 2005/11/14 v1.0j Standard LaTeX Color (DPC) + color.cfg 2007/01/18 v1.5 color configuration of teTeX/TeXLive + nameref.sty 2006/12/27 v2.28 Cross-referencing by name of section +refcount.sty 2006/02/20 v3.0 Data extraction from references (HO) + 37157-t.out + 37157-t.out + t1cmtt.fd 1999/05/25 v2.5h Standard LaTeX font definitions + umsa.fd 2002/01/19 v2.2g AMS font definitions + umsb.fd 2002/01/19 v2.2g AMS font definitions + omlcmr.fd 1999/05/25 v2.5h Standard LaTeX font definitions +./images/tb.pdf +./images/tb.pdf +./images/tb.pdf +./images/tb.pdf + *********** + + ) +Here is how much of TeX's memory you used: + 5416 strings out of 94074 + 70012 string characters out of 1165154 + 139676 words of memory out of 1500000 + 8147 multiletter control sequences out of 10000+50000 + 29817 words of font info for 77 fonts, out of 1200000 for 2000 + 646 hyphenation exceptions out of 8191 + 29i,12n,46p,258b,493s stack positions out of 5000i,500n,6000p,200000b,5000s +{/usr/share/texmf/fonts/enc/dvips/cm-super/cm-super-t1.enc}</usr/share/texmf- +texlive/fonts/type1/bluesky/cm/cmex10.pfb></usr/share/texmf-texlive/fonts/type1 +/bluesky/cm/cmmi10.pfb></usr/share/texmf-texlive/fonts/type1/bluesky/cm/cmmi12. +pfb></usr/share/texmf-texlive/fonts/type1/bluesky/cm/cmmi8.pfb></usr/share/texm +f-texlive/fonts/type1/bluesky/cm/cmr10.pfb></usr/share/texmf-texlive/fonts/type +1/bluesky/cm/cmr12.pfb></usr/share/texmf-texlive/fonts/type1/bluesky/cm/cmr8.pf +b></usr/share/texmf-texlive/fonts/type1/bluesky/cm/cmsy10.pfb></usr/share/texmf +-texlive/fonts/type1/bluesky/cm/cmsy8.pfb></usr/share/texmf/fonts/type1/public/ +cm-super/sfcc1000.pfb></usr/share/texmf/fonts/type1/public/cm-super/sfcc1095.pf +b></usr/share/texmf/fonts/type1/public/cm-super/sfcc1200.pfb></usr/share/texmf/ +fonts/type1/public/cm-super/sfrm0700.pfb></usr/share/texmf/fonts/type1/public/c +m-super/sfrm0800.pfb></usr/share/texmf/fonts/type1/public/cm-super/sfrm1000.pfb +></usr/share/texmf/fonts/type1/public/cm-super/sfrm1095.pfb></usr/share/texmf/f +onts/type1/public/cm-super/sfrm1200.pfb></usr/share/texmf/fonts/type1/public/cm +-super/sfrm1440.pfb></usr/share/texmf/fonts/type1/public/cm-super/sfrm1728.pfb> +</usr/share/texmf/fonts/type1/public/cm-super/sfrm2488.pfb></usr/share/texmf/fo +nts/type1/public/cm-super/sfti0800.pfb></usr/share/texmf/fonts/type1/public/cm- +super/sfti1000.pfb></usr/share/texmf/fonts/type1/public/cm-super/sfti1095.pfb>< +/usr/share/texmf/fonts/type1/public/cm-super/sfti1200.pfb></usr/share/texmf/fon +ts/type1/public/cm-super/sftt0800.pfb></usr/share/texmf/fonts/type1/public/cm-s +uper/sftt1095.pfb></usr/share/texmf-texlive/fonts/type1/public/gothic/yswab.pfb +> +Output written on 37157-t.pdf (306 pages, 994390 bytes). +PDF statistics: + 1752 PDF objects out of 2073 (max. 8388607) + 453 named destinations out of 1000 (max. 131072) + 230 words of extra memory for PDF output out of 10000 (max. 10000000) + diff --git a/37157-t/images/tb.pdf b/37157-t/images/tb.pdf Binary files differnew file mode 100644 index 0000000..263b9f6 --- /dev/null +++ b/37157-t/images/tb.pdf diff --git a/37157-t/old/37157-t.tex b/37157-t/old/37157-t.tex new file mode 100644 index 0000000..e3d772f --- /dev/null +++ b/37157-t/old/37157-t.tex @@ -0,0 +1,10206 @@ +% %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% % +% % +% The Project Gutenberg EBook of Science and hypothesis, by Henri Poincaré% +% % +% This eBook is for the use of anyone anywhere at no cost and with % +% almost no restrictions whatsoever. You may copy it, give it away or % +% re-use it under the terms of the Project Gutenberg License included % +% with this eBook or online at www.gutenberg.net % +% % +% % +% Title: Science and hypothesis % +% % +% Author: Henri Poincaré % +% % +% Release Date: August 21, 2011 [EBook #37157] % +% % +% Language: English % +% % +% Character set encoding: ISO-8859-1 % +% % +% *** START OF THIS PROJECT GUTENBERG EBOOK SCIENCE AND HYPOTHESIS *** % +% % +% %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% % + +\def\ebook{37157} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% %% +%% Packages and substitutions: %% +%% %% +%% book: Required. %% +%% inputenc: Latin-1 text encoding. Required. %% +%% fontenc: Font encoding, to hyphenate accented words. Required. %% +%% %% +%% ifthen: Logical conditionals. Required. %% +%% %% +%% amsmath: AMS mathematics enhancements. Required. %% +%% amssymb: Additional mathematical symbols. Required. %% +%% %% +%% alltt: Fixed-width font environment. Required. %% +%% %% +%% yfonts: Gothic font on title page. Optional. %% +%% %% +%% footmisc: Start footnote numbering on each page. Required. %% +%% %% +%% graphicx: Standard interface for graphics inclusion. Required. %% +%% %% +%% calc: Length calculations. Required. %% +%% %% +%% fancyhdr: Enhanced running headers and footers. Required. %% +%% %% +%% geometry: Enhanced page layout package. Required. %% +%% hyperref: Hypertext embellishments for pdf output. Required. %% +%% %% +%% %% +%% Producer's Comments: %% +%% %% +%% OCR text for this ebook was obtained on July 30, 2011, from %% +%% http://www.archive.org/details/onriemannstheory00kleiuoft. %% +%% %% +%% Changes to the original are noted in this file as follows: %% +%% 1. \Reword{}{}: Erroneously-translated phrases. No attempt %% +%% was made to compare the French edition with the English %% +%% translation systematically. Instead, incongruous phrases %% +%% in the English edition were compared with the page scans %% +%% at http://gallica.bnf.fr/ark:/12148/bpt6k26745q and the %% +%% wording was modified as appropriate. %% +%% In-line transcriber notes, marked "[** TN: ...]" contain %% +%% the relevant text from the French edition. %% +%% %% +%% 2. \Typo{}{}: Typographical corrections, showing original %% +%% and replacement text side-by-side. %% +%% %% +%% 3. \Chg{}{} and \Add{}: Inconsistent/missing punctuation, %% +%% italicization, and capitalization. %% +%% %% +%% 4. [** TN: ...]: Lengthier miscellaneous comments. %% +%% %% +%% The following hyphenation \Chg{}{}s were made for consistency: %% +%% 1. electrostatic -> electro-static %% +%% 2. thermodynamic -> thermo-dynamic %% +%% 3. re-act[ion] -> react[ion] %% +%% Larmor's spelling "æther" in the introduction is retained. The %% +%% translation uses "ether" uniformly elsewhere. %% +%% %% +%% In Chapter I., equations and expressions that are displayed in %% +%% the French edition (but in-line in the English translation) %% +%% have been displayed. %% +%% %% +%% Fourteen pages of book catalogue at the end have been omitted. %% +%% %% +%% Compilation Flags: %% +%% %% +%% The following behavior may be controlled by boolean flags. %% +%% %% +%% ForPrinting (false by default): %% +%% If false, compile a screen optimized file (one-sided layout, %% +%% blue hyperlinks). If true, print-optimized PDF file: Larger %% +%% text block, two-sided layout, black hyperlinks. %% +%% %% +%% %% +%% PDF pages: 306 (if ForPrinting set to false) %% +%% PDF page size: 4.25 x 5.75" (non-standard) %% +%% %% +%% Summary of log file: %% +%% * One slightly overfull hbox, several harmless underfull hboxes. %% +%% %% +%% Compile History: %% +%% %% +%% August, 2011: (Andrew D. Hwang) %% +%% texlive2007, GNU/Linux %% +%% %% +%% Command block: %% +%% %% +%% pdflatex x3 %% +%% %% +%% %% +%% August 2011: pglatex. %% +%% Compile this project with: %% +%% pdflatex 37157-t.tex ..... THREE times %% +%% %% +%% pdfTeXk, Version 3.141592-1.40.3 (Web2C 7.5.6) %% +%% %% +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\listfiles +\documentclass[12pt,leqno]{book}[2005/09/16] + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%% PACKAGES %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\usepackage[latin1]{inputenc}[2006/05/05] +\usepackage[T1]{fontenc}[2005/09/27] + +\usepackage{ifthen}[2001/05/26] %% Logical conditionals + +\usepackage{amsmath}[2000/07/18] %% Displayed equations +\usepackage{amssymb}[2002/01/22] %% and additional symbols + +\usepackage{alltt}[1997/06/16] %% boilerplate, credits, license + +\IfFileExists{yfonts.sty}{% + \usepackage{yfonts}[2003/01/08] +}{% + \providecommand{\textgoth}[1]{#1}% +} +\usepackage[perpage]{footmisc}[2005/03/17] + +\usepackage{graphicx}[1999/02/16]%% For diagrams + +\usepackage{calc}[2005/08/06] + +\usepackage{fancyhdr} %% For running heads + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%%%% Interlude: Set up PRINTING (default) or SCREEN VIEWING %%%% +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +% ForPrinting=true false (default) +% Asymmetric margins Symmetric margins +% 1 : 1.6 text block aspect ratio 3 : 4 text block aspect ratio +% Black hyperlinks Blue hyperlinks +% Start major marker pages recto No blank verso pages +% +\newboolean{ForPrinting} + +%% UNCOMMENT the next line for a PRINT-OPTIMIZED VERSION of the text %% +%\setboolean{ForPrinting}{true} + +%% Initialize values to ForPrinting=false +\newcommand{\Margins}{hmarginratio=1:1} % Symmetric margins +\newcommand{\HLinkColor}{blue} % Hyperlink color +\newcommand{\PDFPageLayout}{SinglePage} +\newcommand{\TransNote}{Transcriber's Note} +\newcommand{\TransNoteCommon}{% + The camera-quality files for this public-domain ebook may be + downloaded \textit{gratis} at + \begin{center} + \texttt{www.gutenberg.org/ebooks/\ebook}. + \end{center} + + Minor typographical corrections, regularizations, and presentational + changes have been made without comment. + \bigskip + + This ebook was produced using scanned images and OCR text generously + provided by the University of Toronto Robarts Library through the + Internet Archive. + \bigskip +} + +\newcommand{\TransNoteText}{% + \TransNoteCommon + + This PDF file is optimized for screen viewing, but may be recompiled + for printing. Please consult the preamble of the \LaTeX\ source + file for instructions and other particulars. +} +%% Re-set if ForPrinting=true +\ifthenelse{\boolean{ForPrinting}}{% + \renewcommand{\Margins}{hmarginratio=2:3} % Asymmetric margins + \renewcommand{\HLinkColor}{black} % Hyperlink color + \renewcommand{\PDFPageLayout}{TwoPageRight} + \renewcommand{\TransNote}{Transcriber's Note} + \renewcommand{\TransNoteText}{% + \TransNoteCommon + + This PDF file is optimized for printing, but may be recompiled for + screen viewing. Please consult the preamble of the \LaTeX\ source + file for instructions and other particulars. + } +}{% If ForPrinting=false, don't skip to recto + \renewcommand{\cleardoublepage}{\clearpage} +} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%%%% End of PRINTING/SCREEN VIEWING code; back to packages %%%% +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +\ifthenelse{\boolean{ForPrinting}}{% + \setlength{\paperwidth}{8.5in}% + \setlength{\paperheight}{11in}% +% 1:1.6 + \usepackage[body={5in,8in},\Margins]{geometry}[2002/07/08] +}{% + \setlength{\paperwidth}{4.25in}% + \setlength{\paperheight}{5.75in}% + \raggedbottom +% 3:4 + \usepackage[body={4in,4.9in},\Margins,includeheadfoot]{geometry}[2002/07/08] +} + +\providecommand{\ebook}{00000} % Overridden during white-washing +\usepackage[pdftex, + hyperref, + hyperfootnotes=false, + pdftitle={The Project Gutenberg eBook \#\ebook: Science and Hypothesis.}, + pdfkeywords={University of Toronto, The Internet Archive, Henri Poincare, Joseph Larmor, Willian John Greenstreet, Andrew D. Hwang}, + pdfstartview=Fit, % default value + pdfstartpage=1, % default value + pdfpagemode=UseNone, % default value + bookmarks=true, % default value + linktocpage=false, % default value + pdfpagelayout=\PDFPageLayout, + pdfdisplaydoctitle, + pdfpagelabels=true, + bookmarksopen=true, + bookmarksopenlevel=0, + colorlinks=true, + linkcolor=\HLinkColor]{hyperref}[2007/02/07] + + +% Set author here to avoid numerous hyperref warnings from accents +\hypersetup{pdfauthor={Henri Poincaré}} + +%% Fixed-width environment to format PG boilerplate %% +\newenvironment{PGtext}{% +\begin{alltt} +\fontsize{7.2}{9}\ttfamily\selectfont}% +{\end{alltt}} + +%% Re-define the following as, e.g., \newcommand{\Chg}[2]{#1} to revert + +% Translation errors found during digitization +\newcommand{\Reword}[2]{#2} + +% Typographical errors found during digitization +\newcommand{\Typo}[2]{#2} + +% Stylistic changes made for consistency +\newcommand{\Chg}[2]{#2} +\newcommand{\Add}[1]{\Chg{}{#1}} + +%% Miscellaneous global parameters %% +% No hrule in page header +\renewcommand{\headrulewidth}{0pt} + +% Loosen spacing +\setlength{\emergencystretch}{1.25em} +\newcommand{\Loosen}{\spaceskip 0.5em plus 0.75em minus 0.25em} +\hyphenation{extra-ordinary} + +% Scratch pad for length calculations +\newlength{\TmpLen} + +%% Running heads %% +\newcommand{\FlushRunningHeads}{\clearpage\fancyhf{}\cleardoublepage} +\newcommand{\InitRunningHeads}{% + \setlength{\headheight}{15pt} + \pagestyle{fancy} + \thispagestyle{empty} + \ifthenelse{\boolean{ForPrinting}} + {\fancyhead[RO,LE]{\thepage}} + {\fancyhead[R]{\thepage}} +} + +% Uniform style for running heads +\newcommand{\RHeads}[1]{\textsc{\MakeLowercase{#1}}} + +\newcommand{\SetRunningHeads}[2][]{% + \fancyhead[CO]{\RHeads{#2}}% + \ifthenelse{\equal{#1}{}}{% + \fancyhead[CE]{\RHeads{Science and Hypothesis}}% + }{% + \fancyhead[CE]{\RHeads{#2}}% + }% +} + +\ifthenelse{\boolean{ForPrinting}}{% + \newcommand{\ChapTopSkip}{\vspace*{1.5in}}% +}{% + \newcommand{\ChapTopSkip}{}% +} + +\newcommand{\BookMark}[2]{\phantomsection\pdfbookmark[#1]{#2}{#2}} + +%% Major document divisions %% +\newcommand{\PGBoilerPlate}{% + \pagenumbering{Alph} + \pagestyle{empty} + \BookMark{0}{PG Boilerplate.} +} +\newcommand{\FrontMatter}{% + \cleardoublepage + \frontmatter + \BookMark{-1}{Front Matter.} +} +\newcommand{\MainMatter}{% + \FlushRunningHeads + \InitRunningHeads + \mainmatter + \BookMark{-1}{Main Matter.} +} +\newcommand{\BackMatter}{% + \FlushRunningHeads + \InitRunningHeads + \backmatter + \BookMark{-1}{Back Matter.} +} +\newcommand{\PGLicense}{% + \FlushRunningHeads + \pagenumbering{Roman} + \InitRunningHeads + \BookMark{-1}{PG License.} + \SetRunningHeads[both]{License.} +} + +%% ToC formatting %% +\AtBeginDocument{\renewcommand{\contentsname}{% + \protect\thispagestyle{empty}% + \protect\vspace*{-3\baselineskip}% + \protect\SectTitle[\Large]{Contents.}% + \protect\vspace{-\baselineskip} + } +} + +\newcommand{\TableofContents}{% + \FlushRunningHeads + \InitRunningHeads + \SetRunningHeads[both]{Contents.} + \BookMark{0}{Contents.} + \tableofcontents +} + +% For internal use, to determine if we need "PAGE" line +\newcommand{\ToCAnchor}{} +\newcounter{ChapNo} + +% \ToCLine{SecNo}{Title} +\newcommand{\ToCLine}[2]{% + \label{toc:#1}% + \ifthenelse{\not\equal{\pageref{toc:#1}}{\ToCAnchor}}{% + \renewcommand{\ToCAnchor}{\pageref{toc:#1}}% + \noindent\makebox[\textwidth][r]{\scriptsize \null\hfill PAGE}\\% + }{}% + \settowidth{\TmpLen}{999}% + \noindent\strut\parbox[b]{\textwidth-\TmpLen}{\small% + \hangindent4em\textsc{#2}\dotfill}% + \makebox[\TmpLen][r]{\pageref{chap:#1}}% +} + +%% Sectional units %% +% Typographical abstractions +\newcommand{\ChapTitle}[1]{% + \SectTitle[\Large]{#1} + {\centering\includegraphics[width=1in]{./images/tb.pdf}\par\medskip} +} +\newcommand{\SectTitle}[2][\large]{% + \subsection*{\centering\normalfont#1\MakeUppercase{#2}} +} +\newcommand{\SubsectTitle}[2][\normalsize]{% + \subsubsection*{\centering\normalfont#1\MakeUppercase{#2}} +} + +% For internal use +\newboolean{AtPart} +\newcommand{\Part}[2]{% + \setboolean{AtPart}{true} + \FlushRunningHeads + \InitRunningHeads + \BookMark{0}{Part #1 #2} + \addtocontents{toc}{\protect\SectTitle[\protect\small]{PART #1}} + \addtocontents{toc}{\protect\SubsectTitle[\protect\footnotesize]{\protect\textit{#2}}} + \ChapTopSkip + \ifthenelse{\equal{#1}{I.}}{% + \ChapTitle{Science and Hypothesis} + }{} + \SectTitle{PART #1} + \SubsectTitle{\textit{#2}} +} + +% \OtherChapter{Title}: Unnumbered units (preface, etc.) +\newcommand{\OtherChapter}[1]{% + \FlushRunningHeads + \stepcounter{ChapNo}\phantomsection\label{chap:\theChapNo}% + \addtocontents{toc}{\protect\ToCLine{\theChapNo}{#1}}% + \InitRunningHeads + \BookMark{0}{#1} + \SetRunningHeads[both]{#1} + \ChapTopSkip + \ChapTitle{#1} +} + +\newcounter{ChapCount} +\newcommand{\Chapter}[3][]{% + \ifthenelse{\boolean{AtPart}}{% + \setboolean{AtPart}{false}% + }{% + \FlushRunningHeads + \InitRunningHeads + \ChapTopSkip + } + \stepcounter{ChapNo}\phantomsection\label{chap:\theChapNo}% + \stepcounter{ChapCount}\label{chapref:\Roman{ChapCount}}% + \addtocontents{toc}{\protect\SectTitle[\protect\small]{CHAPTER \Roman{ChapCount}.}} + \addtocontents{toc}{\protect\ToCLine{\theChapNo}{#3}}% + \BookMark{1}{Chapter \Roman{ChapCount}: #3} + \ifthenelse{\equal{#1}{}}{% + \SetRunningHeads{#3} + }{% + \SetRunningHeads{#1} + } + \SectTitle{Chapter #2} + \SubsectTitle[\small]{#3} +} +\newcommand{\ChapRef}[1]{\hyperref[chapref:#1]{Chapter~#1}} + +\newcommand{\Section}[1]{\subsection*{\centering\normalsize\normalfont#1}} +\newcommand{\Subsection}[1]{% + \subsubsection*{\centering\small\normalfont\scshape\MakeLowercase{#1}} +} +\newcommand{\Par}[2][]{\par#1\textit{#2}} + +\newcommand{\Dict}[2]{% + \setlength{\TmpLen}{\parindent}% + \vfil + \par\noindent\strut\parbox[t]{0.4\textwidth}{% + \raggedright\hangindent\TmpLen#1\quad\dotfill}\hfill + \parbox[t]{0.55\textwidth}{% + \hangindent\TmpLen#2}% +% \smallskip +} + +\newcommand{\ParSkip}{\hspace*{\parindent}} + +\newcommand{\Signature}[2]{% + \null\hfill#1\ParSkip\break + \ifthenelse{\not\equal{#2}{}}{\smallskip\footnotesize\indent#2\par\normalsize}{} +} + +% Page separators and cross-referencing +\newcommand{\PageSep}[1]{\ignorespaces} + +\newcommand{\Pagelabel}[1]{\phantomsection\label{page:#1}} +\newcommand{\Pageref}[1]{\hyperref[page:#1]{p.~\pageref*{page:#1}}} +\newcommand{\Pagerefs}[2]{% + \ifthenelse{\equal{\pageref*{page:#1}}{\pageref*{page:#2}}}{% + \hyperref[page:#1]{p.~\pageref*{page:#1}}% + }{% Else + pp.~\hyperref[page:#1]{\pageref*{page:#1}},~\hyperref[page:#2]{\pageref*{page:#2}}% + }% +} + +% Miscellaneous semantics and textual conveniences +\newcommand{\Title}[1]{\textit{#1}} +\newcommand{\Foreign}[1]{\textit{#1}} + +\newcommand{\ie}{\Foreign{i.e.}} +\newcommand{\QED}{\text{Q.E.D.}} + +% To denote translator's comments +\newcommand{\Transl}{---[\textsc{Tr}.]} + +\newcommand{\First}[1]{\textsc{#1}} + +\newcommand{\Tag}[1]{#1\quad} + +%% Miscellaneous mathematical formatting %% +\newcommand{\dd}{\partial} +\DeclareInputMath{176}{{}^{\circ}} +\DeclareInputMath{183}{\cdot} + +%% Upright capital letters in math mode +\DeclareMathSymbol{A}{\mathalpha}{operators}{`A} +\DeclareMathSymbol{B}{\mathalpha}{operators}{`B} +\DeclareMathSymbol{C}{\mathalpha}{operators}{`C} +\DeclareMathSymbol{D}{\mathalpha}{operators}{`D} +\DeclareMathSymbol{F}{\mathalpha}{operators}{`F} + +\DeclareMathSymbol{K}{\mathalpha}{operators}{`K} +\DeclareMathSymbol{M}{\mathalpha}{operators}{`M} +\DeclareMathSymbol{N}{\mathalpha}{operators}{`N} + +\DeclareMathSymbol{P}{\mathalpha}{operators}{`P} +\DeclareMathSymbol{Q}{\mathalpha}{operators}{`Q} +\DeclareMathSymbol{R}{\mathalpha}{operators}{`R} +\DeclareMathSymbol{S}{\mathalpha}{operators}{`S} +\DeclareMathSymbol{T}{\mathalpha}{operators}{`T} +\DeclareMathSymbol{U}{\mathalpha}{operators}{`U} + +%%%%%%%%%%%%%%%%%%%%%%%% START OF DOCUMENT %%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{document} +%% PG BOILERPLATE %% +\PGBoilerPlate +\begin{center} +\begin{minipage}{\textwidth} +\small +\begin{PGtext} +The Project Gutenberg EBook of Science and hypothesis, by Henri Poincaré + +This eBook is for the use of anyone anywhere at no cost and with +almost no restrictions whatsoever. You may copy it, give it away or +re-use it under the terms of the Project Gutenberg License included +with this eBook or online at www.gutenberg.net + + +Title: Science and hypothesis + +Author: Henri Poincaré + +Release Date: August 21, 2011 [EBook #37157] + +Language: English + +Character set encoding: ISO-8859-1 + +*** START OF THIS PROJECT GUTENBERG EBOOK SCIENCE AND HYPOTHESIS *** +\end{PGtext} +\end{minipage} +\end{center} +\newpage +%% Credits and transcriber's note %% +\begin{center} +\begin{minipage}{\textwidth} +\begin{PGtext} +Produced by Andrew D. Hwang +\end{PGtext} +\end{minipage} +\vfill +\end{center} + +\begin{minipage}{0.85\textwidth} +\small +\BookMark{0}{Transcriber's Note.} +\subsection*{\centering\normalfont\scshape% +\normalsize\MakeLowercase{\TransNote}}% + +\raggedright +\TransNoteText +\end{minipage} +%%%%%%%%%%%%%%%%%%%%%%%%%%% FRONT MATTER %%%%%%%%%%%%%%%%%%%%%%%%%% +\PageSep{i} +\FrontMatter +\ifthenelse{\boolean{ForPrinting}}{% +\null\vfill +{\Large SCIENCE AND HYPOTHESIS} +\vfill +\cleardoublepage +}{}% Omit half-title in screen version +\PageSep{ii} +%[Blank page] +\PageSep{iii} +\begin{center} +\huge SCIENCE \\ +AND HYPOTHESIS +\vfill + +\normalsize +{\footnotesize BY} \\ +H. POINCARÉ, \\ +{\scriptsize MEMBER OF THE INSTITUTE OF FRANCE.} +\vfill + +{\small\textsc{With a Preface by}} \\ +\textsc{J. LARMOR, D.Sc., Sec. R.S.}, \\ +{\scriptsize\textit{Lucasian Professor of Mathematics in the University of Cambridge.}} +\vfill\vfill + +\textswab{London and Newcastle-on-Tyne:} \\ +THE WALTER SCOTT PUBLISHING CO., LTD \\ +{\footnotesize NEW YORK: 3 EAST 14TH STREET.} \\ +\oldstylenums{1905}. +\end{center} +\newpage +\PageSep{iv} +%[Blank page] +\PageSep{v} +\TableofContents +\iffalse +CONTENTS. + + PAGE +Translator's Note........................ix + +Introduction.............................xi + +Author's Preface........................xxi + + +PART I. + +NUMBER AND MAGNITUDE. + +CHAPTER I. +On the Nature of Mathematical Reasoning...1 + +CHAPTER II. +Mathematical Magnitude and Experiment....17 + + +PART II. + +SPACE. + +CHAPTER III. +Non-Euclidean Geometries.................35 +\PageSep{vi} + +CHAPTER IV. +Space and Geometry.......................51 + +CHAPTER V. +Experiment and Geometry..................72 + + +PART III. + +FORCE. + +CHAPTER VI. +The Classical Mechanics..................89 + +CHAPTER VII. +Relative and Absolute Motion............111 + +CHAPTER VIII. +Energy and Thermo-dynamics..............123 + + +PART IV. + +NATURE. + +CHAPTER IX. +Hypotheses in Physics...................140 +\PageSep{vii} + +CHAPTER X. +The Theories of Modern Physics..........160 + +CHAPTER XI. +The Calculus of Probabilities...........183 + +CHAPTER XII. +Optics and Electricity..................211 + +CHAPTER XIII. +Electro-dynamics........................225 +\fi +\PageSep{viii} +%[Blank page] +\PageSep{ix} + + +\OtherChapter{Translator's Note.} + +\First{The} translator wishes to express his indebtedness +to Professor Larmor, for kindly consenting +to introduce the author of \Title{Science and Hypothesis} +to English readers; to Dr.~F.~S. Macaulay and +Mr.~C.~S. Jackson,~M.A., who have read the whole +of the proofs and have greatly helped by suggestions; +also to Professor G.~H. Bryan,~F.R.S., who +has read the proofs of \ChapRef{VIII}., and whose +criticisms have been most valuable. + +%[** TN: William John Greenstreet (1861--1930), not identified by name] +\Signature{W.\;J.\;G.}{\textit{February} 1905.} +\PageSep{x} +%[Blank page] +\PageSep{xi} + + +\OtherChapter{Introduction.} + +\First{It} is to be hoped that, as a consequence of the +present active scrutiny of our educational aims +and methods, and of the resulting encouragement +of the study of modern languages, we shall not +remain, as a nation, so much isolated from +ideas and tendencies in continental thought and +literature as we have been in the past. As things +are, however, the translation of this book is +doubtless required; at any rate, it brings vividly +before us an instructive point of view. Though +some of M.~Poincaré's chapters have been collected +from well-known treatises written several years +ago, and indeed are sometimes in detail not quite +up to date, besides occasionally suggesting the +suspicion that his views may possibly have been +modified in the interval, yet their publication in +a compact form has excited a warm welcome in +this country. + +It must be confessed that the English language +\PageSep{xii} +hardly lends itself as a perfect medium for the +rendering of the delicate shades of suggestion +and allusion characteristic of M.~Poincaré's play +around his subject; notwithstanding the excellence +of the translation, loss in this respect is +inevitable. + +There has been of late a growing trend of +opinion, prompted in part by general philosophical +views, in the direction that the theoretical constructions +of physical science are largely factitious, +that instead of presenting a valid image of the +relations of things on which further progress can +be based, they are still little better than a mirage. +The best method of abating this scepticism is to +become acquainted with the real scope and modes +of application of conceptions which, in the popular +language of superficial exposition---and even in +the unguarded and playful paradox of their +authors, intended only for the instructed eye---often +look bizarre enough. But much advantage +will accrue if men of science become their own +epistemologists, and show to the world by critical +exposition in non-technical terms of the results +and methods of their constructive work, that more +than mere instinct is involved in it: the community +has indeed a right to expect as much as +this. +\PageSep{xiii} + +It would be hard to find any one better +qualified for this kind of exposition, either +from the profundity of his own mathematical +achievements, or from the extent and freshness +of his interest in the theories of physical science, +than the author of this book. If an appreciation +might be ventured on as regards the later chapters, +they are, perhaps, intended to present the stern +logical analyst quizzing the cultivator of physical +ideas as to what he is driving at, and whither he +expects to go, rather than any responsible attempt +towards a settled confession of faith. Thus, when +M.~Poincaré allows himself for a moment to +indulge in a process of evaporation of the +Principle of Energy, he is content to sum up: +``Eh bien, quelles que soient les notions nouvelles +que les expériences futures nous donneront sur le +monde, nous sommes sûrs d'avance qu'il y aura +quelque chose qui demeurera constant et que nous +pourrons appeler \Foreign{énergie}'' (\Pageref{166}), and to leave +the matter there for his readers to think it out. +Though hardly necessary in the original French, it +may not now be superfluous to point out that +independent reflection and criticism on the part +of the reader are tacitly implied here as elsewhere. + +An interesting passage is the one devoted to +\PageSep{xiv} +Maxwell's theory of the functions of the æther, +and the comparison of the close-knit theories of +the classical French mathematical physicists with +the somewhat loosely-connected \Foreign{corpus} of ideas by +which Maxwell, the interpreter and successor of +Faraday, has (posthumously) recast the whole +face of physical science. How many times has +that theory been re-written since Maxwell's day? +and yet how little has it been altered in essence, +except by further developments in the problem of +moving bodies, from the form in which he left it! +If, as M.~Poincaré remarks, the French instinct +for precision and lucid demonstration sometimes +finds itself ill at ease with physical theories of +the British school, he as readily admits (\Pagerefs{223}{224}), +and indeed fully appreciates, the advantages +on the other side. Our own mental philosophers +have been shocked at the point of view indicated +by the proposition hazarded by Laplace, that a +sufficiently developed intelligence, if it were made +acquainted with the positions and motions of the +atoms at any instant, could predict all future +history: no amount of demur suffices sometimes +to persuade them that this is not a conception +universally entertained in physical science. It +was not so even in Laplace's own day. From +the point of view of the study of the evolution +\PageSep{xv} +of the sciences, there are few episodes more +instructive than the collision between Laplace +and Young with regard to the theory of capillarity. +The precise and intricate mathematical +analysis of Laplace, starting from fixed preconceptions +regarding atomic forces which were +to remain intact throughout the logical development +of the argument, came into contrast with the +tentative, mobile intuitions of Young; yet the +latter was able to grasp, by sheer direct mental +force, the fruitful though partial analogies of this +recondite class of phenomena with more familiar +operations of nature, and to form a direct picture +of the way things interacted, such as could only +have been illustrated, quite possibly damaged or +obliterated, by premature effort to translate it +into elaborate analytical formulas. The \Foreign{aperçus} +of Young were apparently devoid of all cogency +to Laplace; while Young expressed, doubtless in +too extreme a way, his sense of the inanity of the +array of mathematical logic of his rival. The +subsequent history involved the Nemesis that the +fabric of Laplace was taken down and reconstructed +in the next generation by Poisson; while +the modern cultivator of the subject turns, at any +rate in England, to neither of those expositions +for illumination, but rather finds in the partial +\PageSep{xvi} +and succinct indications of Young the best starting-point +for further effort. + +It seems, however, hard to accept entirely +the distinction suggested (\Pageref{213}) between the +methods of cultivating theoretical physics in +the two countries. To mention only two +transcendent names which stand at the very +front of two of the greatest developments of +physical science of the last century, Carnot and +Fresnel, their procedure was certainly not on the +lines thus described. Possibly it is not devoid of +significance that each of them attained his first +effective recognition from the British school. + +It may, in fact, be maintained that the part +played by mechanical and such-like theories---analogies +if you will---is an essential one. The +reader of this book will appreciate that the human +mind has need of many instruments of comparison +and discovery besides the unrelenting logic of the +infinitesimal calculus. The dynamical basis which +underlies the objects of our most frequent experience +has now been systematised into a great +calculus of exact thought, and traces of new real +relationships may come out more vividly when +considered in terms of our familiar acquaintance +with dynamical systems than when formulated +under the paler shadow of more analytical abstractions. +\PageSep{xvii} +It is even possible for a constructive +physicist to conduct his mental operations entirely +by dynamical images, though Helmholtz, as well +as our author, seems to class a predilection in this +direction as a British trait. A time arrives when, +as in other subjects, ideas have crystallised out +into distinctness; their exact verification and +development then becomes a problem in mathematical +physics. But whether the mechanical +analogies still survive, or new terms are now +introduced devoid of all naïve mechanical bias, +it matters essentially little. The precise determination +of the relations of things in the +rational scheme of nature in which we find +ourselves is the fundamental task, and for its +fulfilment in any direction advantage has to be +taken of our knowledge, even when only partial, +of new aspects and types of relationship which +may have become familiar perhaps in quite +different fields. Nor can it be forgotten that the +most fruitful and fundamental conceptions of +abstract pure mathematics itself have often been +suggested from these mechanical ideas of flux +and force, where the play of intuition is our +most powerful guide. The study of the historical +evolution of physical theories is essential to the +complete understanding of their import. It is in +\PageSep{xviii} +the mental workshop of a Fresnel, a Kelvin, or +a Helmholtz, that profound ideas of the deep +things of Nature are struck out and assume +form; when pondered over and paraphrased by +philosophers we see them react on the conduct +of life: it is the business of criticism to polish +them gradually to the common measure of human +understanding. Oppressed though we are with +the necessity of being specialists, if we are +to know anything thoroughly in these days of +accumulated details, we may at any rate profitably +study the historical evolution of knowledge +over a field wider than our own. + +The aspect of the subject which has here been +dwelt on is that scientific progress, considered +historically, is not a strictly logical process, and +does not proceed by syllogisms. New ideas +emerge dimly into intuition, come into consciousness +from nobody knows where, and become +the material on which the mind operates, forging +them gradually into consistent doctrine, which +can be welded on to existing domains of knowledge. +But this process is never complete: a +crude connection can always be pointed to by a +logician as an indication of the imperfection of +human constructions. + +If intuition plays a part which is so important, +\PageSep{xix} +it is surely necessary that we should possess a firm +grasp of its limitations. In M.~Poincaré's earlier +chapters the reader can gain very pleasantly a +vivid idea of the various and highly complicated +ways of docketing our perceptions of the relations +of external things, all equally valid, that were +open to the human race to develop. Strange to +say, they never tried any of them; and, satisfied +with the very remarkable practical fitness of the +scheme of geometry and dynamics that came +naturally to hand, did not consciously trouble +themselves about the possible existence of others +until recently. Still more recently has it been +found that the good Bishop Berkeley's logical +jibes against the Newtonian ideas of fluxions and +limiting ratios cannot be adequately appeased in +the rigorous mathematical conscience, until our +apparent continuities are resolved mentally into +discrete aggregates which we only partially +apprehend. The irresistible impulse to atomize +everything thus proves to be not merely a disease +of the physicist; a deeper origin, in the nature +of knowledge itself, is suggested. + +Everywhere want of absolute, exact adaptation +can be detected, if pains are taken, between the +various constructions that result from our mental +activity and the impressions which give rise to +\PageSep{xx} +them. The bluntness of our unaided sensual +perceptions, which are the source in part of the +intuitions of the race, is well brought out in this +connection by M.~Poincaré. Is there real contradiction? +Harmony usually proves to be recovered +by shifting our attitude to the phenomena. +All experience leads us to interpret the totality of +things as a consistent cosmos---undergoing evolution, +the naturalists will say---in the large-scale +workings of which we are interested spectators +and explorers, while of the inner relations and +ramifications we only apprehend dim glimpses. +When our formulation of experience is imperfect +or even paradoxical, we learn to attribute the +fault to our point of view, and to expect that +future adaptation will put it right. But Truth +resides in a deep well, and we shall never get +to the bottom. Only, while deriving enjoyment +and insight from M.~Poincaré's Socratic exposition +of the limitations of the human outlook on +the universe, let us beware of counting limitation +as imperfection, and drifting into an inadequate +conception of the wonderful fabric of human +knowledge. + +\Signature{J. LARMOR.}{} +\PageSep{xxi} + + +\OtherChapter{Author's Preface.} + +\First{To} the superficial observer scientific truth is unassailable, +the logic of science is infallible; and if +scientific men sometimes make mistakes, it is +because they have not understood the rules of +the game. Mathematical truths are derived from +a few self-evident propositions, by a chain of +flawless reasonings; they are imposed not only on +us, but on Nature itself. By them the Creator is +fettered, as it were, and His choice is limited to +a relatively small number of solutions. A few +experiments, therefore, will be sufficient to enable +us to determine what choice He has made. From +each experiment a number of consequences will +follow by a series of mathematical deductions, +and in this way each of them will reveal to us a +corner of the universe. This, to the minds of most +people, and to students who are getting their first +ideas of physics, is the origin of certainty in +science. This is what they take to be the rôle of +\PageSep{xxii} +experiment and mathematics. And thus, too, it +was understood a hundred years ago by many +men of science who dreamed of constructing the +world with the aid of the smallest possible amount +of material borrowed from experiment. + +But upon more mature reflection the position +held by hypothesis was seen; it was recognised that +it is as necessary to the experimenter as it is to the +mathematician. And then the doubt arose if all +these constructions are built on solid foundations. +The conclusion was drawn that a breath would +bring them to the ground. This sceptical attitude +does not escape the charge of superficiality. To +doubt everything or to believe everything are two +equally convenient solutions; both dispense with +the necessity of reflection. + +Instead of a summary condemnation we should +examine with the utmost care the rôle of hypothesis; +we shall then recognise not only that it is +necessary, but that in most cases it is legitimate. +We shall also see that there are several kinds of +hypotheses; that some are verifiable, and when +once confirmed by experiment become truths of +great fertility; that others may be useful to us in +fixing our ideas; and finally, that others are +hypotheses only in appearance, and reduce to +definitions or to conventions in disguise. The +\PageSep{xxiii} +latter are to be met with especially in mathematics +and in the sciences to which it is applied. From +them, indeed, the sciences derive their rigour; +such conventions are the result of the unrestricted +activity of the mind, which in this domain recognises +no obstacle. For here the mind may affirm +because it lays down its own laws; but let us +clearly understand that while these laws are +imposed on \emph{our} science, which otherwise could +not exist, they are not imposed on Nature. Are +they then arbitrary? No; for if they were, they +would not be fertile. Experience leaves us our +freedom of choice, but it guides us by helping us to +discern the most convenient path to follow. Our +laws are therefore like those of an absolute +monarch, who is wise and consults his council of +state. Some people have been struck by this +characteristic of free convention which may be +recognised in certain fundamental principles of +the sciences. Some have set no limits to their +generalisations, and at the same time they have +forgotten that there is a difference between liberty +and the purely arbitrary. So that they are compelled +to end in what is called \emph{nominalism}; they +have asked if the \Foreign{savant} is not the dupe of his +own definitions, and if the world he thinks he has +discovered is not simply the creation of his own +\PageSep{xxiv} +caprice.\footnote + {Cf.\ M.~le~Roy: ``Science et Philosophie,'' \Title{Revue de Métaphysique + et de Morale}, 1901.} +Under these conditions science would +retain its certainty, but would not attain its object, +and would become powerless. Now, we daily see +what science is doing for us. This could not be +unless it taught us something about reality; the +aim of science is not things themselves, as the +dogmatists in their simplicity imagine, but the +relations between things; outside those relations +there is no reality knowable. + +Such is the conclusion to which we are led; but +to reach that conclusion we must pass in review +the series of sciences from arithmetic and +geometry to mechanics and experimental physics. +What is the nature of mathematical reasoning? +Is it really deductive, as is commonly supposed? +Careful analysis shows us that it is nothing of the +kind; that it participates to some extent in the +nature of inductive reasoning, and for that reason +it is fruitful. But none the less does it retain its +character of absolute rigour; and this is what +must first be shown. + +When we know more of this instrument which +is placed in the hands of the investigator by +mathematics, we have then to analyse another +fundamental idea, that of mathematical magnitude. +\PageSep{xxv} +Do we find it in nature, or have we ourselves +introduced it? And if the latter be the +case, are we not running a risk of coming to +incorrect conclusions all round? Comparing the +rough data of our senses with that extremely complex +and subtle conception which mathematicians +call magnitude, we are compelled to recognise a +divergence. The framework into which we wish +to make everything fit is one of our own construction; +but we did not construct it at random, we +constructed it by measurement so to speak; and +that is why we can fit the facts into it without +altering their essential qualities. + +Space is another framework which we impose +on the world. Whence are the first principles of +geometry derived? Are they imposed on us by +logic? Lobatschewsky, by inventing non-Euclidean +geometries, has shown that this is not the case. +Is space revealed to us by our senses? No; for +the space revealed to us by our senses is absolutely +different from the space of geometry. Is geometry +derived from experience? Careful discussion will +give the answer---no! We therefore conclude that +the principles of geometry are only conventions; +but these conventions are not arbitrary, and if +transported into another world (which I shall +call the non-Euclidean world, and which I shall +\PageSep{xxvi} +endeavour to describe), we shall find ourselves +compelled to adopt more of them. + +In mechanics we shall be led to analogous conclusions, +and we shall see that the principles of +this science, although more directly based on +experience, still share the conventional character +of the geometrical postulates. So far, nominalism +triumphs; but we now come to the physical +sciences, properly so called, and here the scene +changes. We meet with hypotheses of another +kind, and we fully grasp how fruitful they are. +No doubt at the outset theories seem unsound, +and the history of science shows us how ephemeral +they are; but they do not entirely perish, and of +each of them some traces still remain. It is these +traces which we must try to discover, because in +them and in them alone is the true reality. + +The method of the physical sciences is based +upon the induction which leads us to expect the +recurrence of a phenomenon when the circumstances +which give rise to it are repeated. If all +the circumstances could be simultaneously reproduced, +this principle could be fearlessly applied; +but this never happens; some of the circumstances +will always be missing. Are we absolutely certain +that they are unimportant? Evidently not! It +may be probable, but it cannot be rigorously +\PageSep{xxvii} +certain. Hence the importance of the rôle that is +played in the physical sciences by the law of +probability. The calculus of probabilities is therefore +not merely a recreation, or a guide to the +baccarat player; and we must thoroughly examine +the principles on which it is based. In this connection +I have but very incomplete results to lay +before the reader, for the vague instinct which +enables us to determine probability almost defies +analysis. After a study of the conditions under +which the work of the physicist is carried on, I +have thought it best to show him at work. For +this purpose I have taken instances from the +history of optics and of electricity. We shall thus +see how the ideas of Fresnel and Maxwell took +their rise, and what unconscious hypotheses were +made by Ampère and the other founders of +electro-dynamics. +\PageSep{xxviii} +%[Blank page] +\PageSep{1} +\MainMatter +%[** TN: Commented text is printed by the \Part macro] +% SCIENCE AND HYPOTHESIS. + + +\Part{I.}{Number and Magnitude.} + +\Chapter[Nature of Mathematical Reasoning.]{I.}{On the Nature of Mathematical Reasoning.} + +\Section{I.} + +\First{The} very possibility of mathematical science seems +an insoluble contradiction. If this science is only +deductive in appearance, from whence is derived +that perfect rigour which is challenged by none? +If, on the contrary, all the propositions which it +enunciates may be derived in order by the rules +of formal logic, how is it that mathematics is +not reduced to a gigantic tautology? The syllogism +can teach us nothing essentially new, and +if everything must spring from the principle of +identity, then everything should be capable of +being reduced to that principle. Are we then to +admit that the enunciations of all the theorems +\PageSep{2} +with which so many volumes are filled, are only +indirect ways of saying that A~is~A? + +No doubt we may refer back to axioms which +are at the source of all these reasonings. If it is +felt that they cannot be reduced to the principle of +contradiction, if we decline to see in them any +more than experimental facts which have no part +or lot in mathematical necessity, there is still one +resource left to us: we may class them among +\Foreign{à~priori} synthetic views. But this is no solution +of the difficulty---it is merely giving it a name; and +even if the nature of the synthetic views had no +longer for us any mystery, the contradiction would +not have disappeared; it would have only been +shirked. Syllogistic reasoning remains incapable +of adding anything to the data that are given it; +the data are reduced to axioms, and that is all we +should find in the conclusions. + +No theorem can be new unless a new axiom +intervenes in its demonstration; reasoning can +only give us immediately evident truths borrowed +from direct intuition; it would only be an intermediary +parasite. Should we not therefore have +reason for asking if the syllogistic apparatus serves +only to disguise what we have borrowed? + +The contradiction will strike us the more if we +open any book on mathematics; on every page the +author announces his intention of generalising some +proposition already known. Does the mathematical +method proceed from the particular to the general, +and, if so, how can it be called deductive? +\PageSep{3} + +Finally, if the science of number were merely +analytical, or could be analytically derived from a +few synthetic intuitions, it seems that a sufficiently +powerful mind could with a single glance perceive +all its truths; nay, one might even hope that some +day a language would be invented simple enough +for these truths to be made evident to any person +of ordinary intelligence. + +Even if these consequences are challenged, it +must be granted that mathematical reasoning has +of itself a kind of creative virtue, and is therefore to +be distinguished from the syllogism. The difference +must be profound. We shall not, for instance, +find the key to the mystery in the frequent use of +the rule by which the same uniform operation +applied to two equal numbers will give identical +results. All these modes of reasoning, whether or +not reducible to the syllogism, properly so called, +retain the analytical character, and \Foreign{ipso facto}, lose +their power. + +\Section{II.} + +The argument is an old one. Let us see how +Leibnitz tried to show that two and two make +four. I assume the number one to be defined, and +also the operation~$x + 1$---\ie, the adding of unity +to a given number~$x$. These definitions, whatever +they may be, do not enter into the subsequent +reasoning. I next define the numbers $2$,~$3$,~$4$ by +the equalities\Chg{:---}{} +%[** TN: Numbered eqns displayed in the French, but not in the English transl.] +\[ +\Tag{(1)} 1 + 1 = 2;\qquad +\Tag{(2)} 2 + 1 = 3;\qquad +\Tag{(3)} 3 + 1 = 4\Chg{,}{;} +\] +and in +\PageSep{4} +the same way I define the operation~$x + 2$ by the +relation\Chg{;}{} +\[ +\Tag{(4)} +x + 2 = (x + 1) + 1. +\] + +Given this, we have\Chg{:---}{} +\begin{alignat*}{2} + 2 + 2 &= (2 + 1) + 1\Chg{;}{,}\ &&\text{(def.~4)\Chg{.}{;}} \\ +(2 + 1) + 1 &= 3 + 1\Add{,} &&\text{(def.~2)\Chg{.}{;}} \\ + 3 + 1 &= 4\Add{,} &&\text{(def.~3)\Chg{.}{;}} \\ +\text{whence } 2 + 2 &= 4\Add{,}&&\quad\QED +\end{alignat*} + +It cannot be denied that this reasoning is purely +analytical. But if we ask a mathematician, he will +reply: ``This is not a demonstration properly so +called; it is a verification.'' We have confined +ourselves to bringing together one or other of two +purely conventional definitions, and we have verified +their identity; nothing new has been learned. +\emph{Verification} differs from proof precisely because it +is analytical, and because it leads to nothing. It +leads to nothing because the conclusion is nothing +but the premisses translated into another language. +A real proof, on the other hand, is fruitful, because +the conclusion is in a sense more general than the +premisses. The equality $2 + 2 = 4$ can be verified +because it is particular. Each individual enunciation +in mathematics may be always verified in +the same way. But if mathematics could be +reduced to a series of such verifications it +would not be a science. A chess-player, for +instance, does not create a science by winning a +piece. There is no science but the science of the +general. It may even be said that the object of +the exact sciences is to dispense with these direct +verifications. +\PageSep{5} + +\Section{III.} + +Let us now see the geometer at work, and try +%[** TN: "surprise" is correct: "...cherchons à surprendre ses procédés."] +to surprise some of his methods. The task is +not without difficulty; it is not enough to open a +book at random and to analyse any proof we may +come across. First of all, geometry must be excluded, +or the question becomes complicated by +difficult problems relating to the rôle of the +postulates, the nature and the origin of the idea +of space. For analogous reasons we cannot +avail ourselves of the infinitesimal calculus. We +must seek mathematical thought where it has +remained pure---\ie, in Arithmetic. But we +still have to choose; in the higher parts of +the theory of numbers the primitive mathematical +ideas have already undergone so profound +an elaboration that it becomes difficult to analyse +them. + +It is therefore at the beginning of Arithmetic +that we must expect to find the explanation we +seek; but it happens that it is precisely in the +proofs of the most elementary theorems that the +authors of classic treatises have displayed the least +precision and rigour. We may not impute this to +them as a crime; they have obeyed a necessity. +Beginners are not prepared for real mathematical +rigour; they would see in it nothing but empty, +tedious subtleties. It would be waste of time to +try to make them more exacting; they have to +pass rapidly and without stopping over the road +\PageSep{6} +which was trodden slowly by the founders of the +science. + +Why is so long a preparation necessary to +habituate oneself to this perfect rigour, which +it would seem should naturally be imposed on +all minds? This is a logical and psychological +problem which is well worthy of study. But we +shall not dwell on it; it is foreign to our subject. +All I wish to insist on is, that we shall fail in our +purpose unless we reconstruct the proofs of the +elementary theorems, and give them, not the rough +form in which they are left so as not to weary the +beginner, but the form which will satisfy the skilled +geometer. + +\Subsection{Definition of Addition.} + +I assume that the operation~$x + 1$ has been +defined; it consists in adding the number~$1$ to a +given number~$x$. Whatever may be said of this +definition, it does not enter into the subsequent +reasoning. + +We now have to define the operation~$x + a$, which +consists in adding the number~$a$ to any given +number~$x$. Suppose that we have defined the +operation +%[** TN: Displayed eqns as in the French; all are inline in the English transl.] +\[ +x + (a - 1); +\] +the operation~$x + a$ will be +defined by the equality\Chg{:}{} +\[ +\Tag{(1)} +x + a = \bigl[x + (a - 1)\bigr] + 1. +\] +We shall know what $x + a$~is when we know what +$x + (a - 1)$ is, and as I have assumed that to start +with we know what $x + 1$~is, we can define +successively and ``by recurrence'' the operations +$x + 2$, $x + 3$,~etc. This definition deserves a moment's +\PageSep{7} +attention; it is of a particular nature which +distinguishes it even at this stage from the purely +logical definition; the equality~(1), in fact, contains +an infinite number of distinct definitions, each +having only one meaning when we know the +meaning of its predecessor. + +\Subsection{Properties of Addition.} + +\Par{Associative.}---I say that +%[** TN: Displayed eqns as in the French; all are inline in the English transl.] +\[ +a + (b + c) = (a + b) + c; +\] +in +fact, the theorem is true for $c = 1$. It may then be +written +\[ +a + (b + 1) = (a + b) + 1; +\] +which, remembering +the difference of notation, is nothing but the equality~(1) +by which I have just defined addition. Assume +the theorem true for $c = \gamma$, I say that it will be true for +$c = \gamma + 1$. Let +\[ +(a + b) + \gamma = a + (b + \gamma)\Chg{,}{;} +\] +it follows that +\[ +\bigl[(a + b) + \gamma\bigr] + 1 = \bigl[a + (b + \gamma)\bigr] + 1; +\] +or by def.~(1)\Chg{---}{,} +\[ +(a + b) + (\gamma + 1) + = a + (b + \gamma + 1) + = a + \bigl[b + (\gamma + 1)\bigr]\Chg{,}{;} +\] +which shows by a series of purely analytical deductions +that the theorem is true for $\gamma + 1$. Being +true for $c = 1$, we see that it is successively true for +$c = 2$, $c = 3$,~etc. + +\Par{Commutative.}---(1)~I say that +%[** TN: Displayed eqns as in the French; all are inline in the English transl.] +\[ +a + 1 = 1 + a. +\] +The +theorem is evidently true for $a = 1$; we can \emph{verify} +by purely analytical reasoning that if it is true for +$a = \gamma$ it will be true for $a = \gamma + 1$.\footnote + {For $(\gamma + 1) + 1 = (1 + \gamma) + 1 = 1 + (\gamma + 1)$.\Transl} +Now, it is true for +$a = 1$, and therefore is true for $a = 2$, $a = 3$, and so +on. This is what is meant by saying that the +proof is demonstrated ``by recurrence.'' + +(2)~I say that +\[ +a + b = b + a. +\] +The theorem has just +\PageSep{8} +been shown to hold good for $b = 1$, and it may be +verified analytically that if it is true for $b = \beta$, it +will be true for $b = \beta + 1$. The proposition is thus +established by recurrence. + +\Subsection{Definition of Multiplication.} + +We shall define multiplication by the equalities\Chg{:}{} +\begin{gather*} +\Tag{(1)} +a × 1 = a\Chg{.}{;} \\ +\Tag{(2)} +a × b = \bigl[a × (b - 1)\bigr] + a. +\end{gather*} +Both of +these include an infinite number of definitions; +having defined~$a × 1$, it enables us to define in +succession $a × 2$, $a × 3$, and so on. + +\Subsection{Properties of Multiplication.} + +\Par{Distributive.}---I say that +%[** TN: Displayed eqns as in the French; all are inline in the English transl.] +\[ +(a + b) × c = (a × c) + (b × c). +\] +We can verify analytically that the theorem +is true for $c = 1$; then if it is true for $c = \gamma$, it will be +true for $c = \gamma + 1$. The proposition is then proved +by recurrence. + +\Par{Commutative.}---(1) I say that +\[ +a × 1 = 1 × a. +\] +The +theorem is obvious for $a = 1$. We can verify +analytically that if it is true for $a = \alpha$, it will be +true for $a = \alpha + 1$. + +(2)~I say that +\[ +a × b = b × a. +\] +The theorem has +just been proved for $b = 1$. We can verify analytically +that if it be true for $b = \beta$ it will be true for +$b = \beta + 1$. + +\Section{IV.} + +This monotonous series of reasonings may now +be laid aside; but their very monotony brings +vividly to light the process, which is uniform, +\PageSep{9} +and is met again at every step. The process is +proof by recurrence. We first show that a +theorem is true for $n = 1$; we then show that if +it is true for~$n - 1$ it is true for~$n$, and we conclude +that it is true for all integers. We have now seen +how it may be used for the proof of the rules of +addition and multiplication---that is to say, for the +rules of the algebraical calculus. This calculus +is an instrument of transformation which lends +itself to many more different combinations than +the simple syllogism; but it is still a purely analytical +instrument, and is incapable of teaching us +anything new. If mathematics had no other instrument, +it would immediately be arrested in its +development; but it has recourse anew to the +same process---\ie, to reasoning by recurrence, and +it can continue its forward march. Then if we +look carefully, we find this mode of reasoning at +every step, either under the simple form which we +have just given to it, or under a more or less modified +form. It is therefore mathematical reasoning +\Foreign{par excellence}, and we must examine it closer. + +\Section{V.} + +The essential characteristic of reasoning by recurrence +is that it contains, condensed, so to +speak, in a single formula, an infinite number of +syllogisms. We shall see this more clearly if we +enunciate the syllogisms one after another. They +follow one another, if one may use the expression, +in a cascade. The following are the hypothetical +\PageSep{10} +syllogisms:---The theorem is true of the number~$1$. +Now, if it is true of~$1$, it is true of~$2$; therefore it is +true of~$2$. Now, if it is true of~$2$, it is true of~$3$; +hence it is true of~$3$, and so on. We see that the +conclusion of each syllogism serves as the minor +of its successor. Further, the majors of all our +syllogisms may be reduced to a single form. If +the theorem is true of~$n - 1$, it is true of~$n$. + +We see, then, that in reasoning by recurrence +we confine ourselves to the enunciation of the +minor of the first syllogism, and the general +formula which contains as particular cases all the +majors. This unending series of syllogisms is thus +reduced to a phrase of a few lines. + +It is now easy to understand why every particular +consequence of a theorem may, as I have +above explained, be verified by purely analytical +processes. If, instead of proving that our theorem +is true for all numbers, we only wish to show that +it is true for the number~$6$ for instance, it will be +enough to establish the first five syllogisms in our +cascade. We shall require~$9$ if we wish to prove +it for the number~$10$; for a greater number we +shall require more still; but however great the +number may be we shall always reach it, and the +analytical verification will always be possible. +But however far we went we should never reach +the general theorem applicable to all numbers, +which alone is the object of science. To reach +it we should require an infinite number of syllogisms, +and we should have to cross an abyss +\PageSep{11} +which the patience of the analyst, restricted to the +resources of formal logic, will never succeed in +crossing. + +I asked at the outset why we cannot conceive of +a mind powerful enough to see at a glance the +whole body of mathematical truth. The answer is +now easy. A chess-player can combine for four or +five moves ahead; but, however extraordinary a +player he may be, he cannot prepare for more than +a finite number of moves. If he applies his faculties +to Arithmetic, he cannot conceive its general +truths by direct intuition alone; to prove even the +smallest theorem he must use reasoning by recurrence, +for that is the only instrument which +enables us to pass from the finite to the infinite. +This instrument is always useful, for it enables us +to leap over as many stages as we wish; it frees +us from the necessity of long, tedious, and +monotonous verifications which would rapidly +become impracticable. Then when we take in +hand the general theorem it becomes indispensable, +for otherwise we should ever be approaching +the analytical verification without ever actually +reaching it. In this domain of Arithmetic we may +think ourselves very far from the infinitesimal +analysis, but the idea of mathematical infinity is +already playing a preponderating part, and without +it there would be no science at all, because there +would be nothing general. +\PageSep{12} + +\Section{VI.} + +The views upon which reasoning by recurrence +is based may be exhibited in other forms; we may +say, for instance, that in any finite collection of +different integers there is always one which is +smaller than any other. We may readily pass from +one enunciation to another, and thus give ourselves +the illusion of having proved that reasoning +by recurrence is legitimate. But we shall +always be brought to a full stop---we shall always +come to an indemonstrable axiom, which will at +bottom be but the proposition we had to prove +translated into another language. We cannot therefore +escape the conclusion that the rule of reasoning +by recurrence is irreducible to the principle of +contradiction. Nor can the rule come to us from +experiment. Experiment may teach us that the +rule is true for the first ten or the first hundred +numbers, for instance; it will not bring us to the +indefinite series of numbers, but only to a more or +less long, but always limited, portion of the series. + +Now, if that were all that is in question, the +principle of contradiction would be sufficient, it +would always enable us to develop as many +syllogisms as we wished. It is only when it is a +question of a single formula to embrace an infinite +number of syllogisms that this principle breaks +down, and there, too, experiment is powerless to +aid. This rule, inaccessible to analytical proof +and to experiment, is the exact type of the \Foreign{à~priori} +\PageSep{13} +synthetic intuition. On the other hand, we +cannot see in it a convention as in the case of the +postulates of geometry. + +Why then is this view imposed upon us with +such an irresistible weight of evidence? It is +because it is only the affirmation of the power of +the mind which knows it can conceive of the +indefinite repetition of the same act, when the act +is once possible. The mind has a direct intuition +of this power, and experiment can only be for it an +opportunity of using it, and thereby of becoming +conscious of it. + +But it will be said, if the legitimacy of reasoning +by recurrence cannot be established by experiment +alone, is it so with experiment aided by induction? +We see successively that a theorem is true of the +number~$1$, of the number~$2$, of the number~$3$, and +so on---the law is manifest, we say, and it is so on +the same ground that every physical law is true +which is based on a very large but limited number +of observations. + +It cannot escape our notice that here is a +striking analogy with the usual processes of +induction. But an essential difference exists. +Induction applied to the physical sciences is +always uncertain, because it is based on the belief +in a general order of the universe, an order +which is external to us. Mathematical induction---\ie, +proof by recurrence---is, on the contrary, +necessarily imposed on us, because it is only the +affirmation of a property of the mind itself. +\PageSep{14} + +\Section{VII.} + +Mathematicians, as I have said before, always +endeavour to generalise the propositions they have +obtained. To seek no further example, we have +just shown the equality\Chg{,}{} +%[** TN: Displayed eqns as in the French; all are inline in the English transl.] +\[ +a + 1 = 1 + a, +\] +and we then +used it to establish the equality\Chg{,}{} +\[ +a + b = b + a, +\] +which +is obviously more general. Mathematics may, +therefore, like the other sciences, proceed from the +particular to the general. This is a fact which +might otherwise have appeared incomprehensible +to us at the beginning of this study, but which has +no longer anything mysterious about it, since we +have ascertained the analogies between proof by +recurrence and ordinary induction. + +No doubt mathematical recurrent reasoning and +physical inductive reasoning are based on different +foundations, but they move in parallel lines and in +the same direction---namely, from the particular +to the general. + +Let us examine the case a little more closely. +To prove the equality +\[ +\Tag{(1)} +a + 2 = 2 + a, +\] +we need +only apply the rule +\[ +a + 1 = 1 + a\Chg{,}{} +\] +twice, and write +\[ +\Tag{(2)} +a + 2 = a + 1 + 1 = 1 + a + 1 = 1 + 1 + a = 2 + a. +\] + +The equality thus deduced by purely analytical +means is not, however, a simple particular case. It +is something quite different. We may not therefore +even say in the really analytical and deductive +part of mathematical reasoning that we proceed +from the general to the particular in the +ordinary sense of the words. The two sides of +\PageSep{15} +the equality~(2) are merely more complicated +combinations than the two sides of the equality~(1), +and analysis only serves to separate the elements +which enter into these combinations and to +study their relations. + +Mathematicians therefore proceed ``by construction,'' +they ``construct'' more complicated combinations. +When they analyse these combinations, +these aggregates, so to speak, into their primitive +elements, they see the relations of the elements +and deduce the relations of the aggregates themselves. +The process is purely analytical, but it is +not a passing from the general to the particular, +for the aggregates obviously cannot be regarded as +more particular than their elements. + +Great importance has been rightly attached to +this process of ``construction,'' and some claim +to see in it the necessary and sufficient condition +of the progress of the exact sciences. +Necessary, no doubt, but not sufficient! For a +construction to be useful and not mere waste of +mental effort, for it to serve as a stepping-stone to +higher things, it must first of all possess a kind of +unity enabling us to see something more than the +juxtaposition of its elements. Or more accurately, +there must be some advantage in considering the +construction rather than the elements themselves. +What can this advantage be? Why reason on a +polygon, for instance, which is always decomposable +into triangles, and not on elementary +triangles? It is because there are properties of +\PageSep{16} +polygons of any number of sides, and they can be +immediately applied to any particular kind of +polygon. In most cases it is only after long efforts +that those properties can be discovered, by directly +studying the relations of elementary triangles. If +the quadrilateral is anything more than the juxtaposition +of two triangles, it is because it is of the +polygon type. + +A construction only becomes interesting when +it can be placed side by side with other analogous +constructions for forming species of the same +genus. To do this we must necessarily go back +from the particular to the general, ascending one +or more steps. The analytical process ``by +construction'' does not compel us to descend, but +it leaves us at the same level. We can only +ascend by mathematical induction, for from it +alone can we learn something new. Without the +aid of this induction, which in certain respects +differs from, but is as fruitful as, physical induction, +construction would be powerless to create +science. + +Let me observe, in conclusion, that this induction +is only possible if the same operation can +be repeated indefinitely. That is why the theory +of chess can never become a science, for the +different moves of the same piece are limited and +do not resemble each other. +\PageSep{17} + + +\Chapter[Mathematical Magnitude.]{II.}{Mathematical Magnitude and Experiment.} + +\First{If} we want to know what the mathematicians +mean by a continuum, it is useless to appeal to +geometry. The geometer is always seeking, more +or less, to represent to himself the figures he is +studying, but his representations are only instruments +to him; he uses space in his geometry just +as he uses chalk; and further, too much importance +must not be attached to accidents which are +often nothing more than the whiteness of the +chalk. + +The pure analyst has not to dread this pitfall. +He has disengaged mathematics from all extraneous +elements, and he is in a position to answer +our question:---``Tell me exactly what this continuum +is, about which mathematicians reason.'' +Many analysts who reflect on their art have +already done so---M.~Tannery, for instance, in +his \Title{Introduction à la théorie des Fonctions d'une +variable}. + +Let us start with the integers. Between any +two consecutive sets, intercalate one or more intermediary +sets, and then between these sets others +\PageSep{18} +again, and so on indefinitely. We thus get an +unlimited number of terms, and these will be the +numbers which we call fractional, rational, or +commensurable. But this is not yet all; between +these terms, which, be it marked, are already +infinite in number, other terms are intercalated, +and these are called irrational or incommensurable. + +Before going any further, let me make a preliminary +remark. The continuum thus conceived +is no longer a collection of individuals arranged in +a certain order, infinite in number, it is true, but +external the one to the other. This is not the +ordinary conception in which it is supposed that +between the elements of the continuum exists an +intimate connection making of it one whole, in +which the point has no existence previous to the +line, but the line does exist previous to the point. +Multiplicity alone subsists, unity has disappeared---``the +continuum is unity in multiplicity,'' according +to the celebrated formula. The analysts have +even less reason to define their continuum as they +do, since it is always on this that they reason when +they are particularly proud of their rigour. It +is enough to warn the reader that the real +mathematical continuum is quite different from +that of the physicists and from that of the +metaphysicians. + +It may also be said, perhaps, that mathematicians +who are contented with this definition are the +dupes of words, that the nature of each of these +sets should be precisely indicated, that it should +\PageSep{19} +be explained how they are to be intercalated, and +that it should be shown how it is possible to do it. +This, however, would be wrong; the only property +of the sets which comes into the reasoning is that of +preceding or succeeding these or those other sets; +this alone should therefore intervene in the definition. +So we need not concern ourselves with the +manner in which the sets are intercalated, and +no one will doubt the possibility of the operation +if he only remembers that ``possible'' in the +language of geometers simply means exempt from +contradiction. But our definition is not yet complete, +and we come back to it after this rather long +digression. + +\Par{Definition of Incommensurables.}---The mathematicians +of the Berlin school, and Kronecker +in particular, have devoted themselves to constructing +this continuous scale of irrational and +fractional numbers without using any other +materials than the integer. The mathematical +continuum from this point of view would be a +pure creation of the mind in which experiment +would have no part. + +The idea of rational number not seeming to +present to them any difficulty, they have confined +their attention mainly to defining incommensurable +numbers. But before reproducing their definition +here, I must make an observation that will allay +the astonishment which this will not fail to provoke +in readers who are but little familiar with the +habits of geometers. +\PageSep{20} + +Mathematicians do not study objects, but the +relations between objects; to them it is a matter +of indifference if these objects are replaced by +others, provided that the relations do not change. +Matter does not engage their attention, they are +interested by form alone. + +If we did not remember it, we could hardly +understand that Kronecker gives the name of +incommensurable number to a simple symbol---that +is to say, something very different from the +idea we think we ought to have of a quantity +which should be measurable and almost tangible. + +Let us see now what is Kronecker's definition. +Commensurable numbers may be divided into +classes in an infinite number of ways, subject +to the condition that any number whatever +of the first class is greater than any number +of the second. It may happen that among the +numbers of the first class there is one which is +smaller than all the rest; if, for instance, we +arrange in the first class all the numbers greater +than~$2$, and $2$~itself, and in the second class all the +numbers smaller than~$2$, it is clear that $2$~will be +the smallest of all the numbers of the first class. +The number~$2$ may therefore be chosen as the +symbol of this division. + +It may happen, on the contrary, that in the +second class there is one which is greater than all +the rest. This is what takes place, for example, +if the first class comprises all the numbers greater +than~$2$, and if, in the second, are all the numbers +\PageSep{21} +less than~$2$, and $2$~itself. Here again the +number~$2$ might be chosen as the symbol of this +division. + +But it may equally well happen that we can find +neither in the first class a number smaller than all +the rest, nor in the second class a number greater +than all the rest. Suppose, for instance, we +place in the first class all the numbers whose +squares are greater than~$2$, and in the second all +the numbers whose squares are smaller than~$2$. +We know that in neither of them is a number whose +square is equal to~$2$. Evidently there will be in +the first class no number which is smaller than all +the rest, for however near the square of a number +may be to~$2$, we can always find a commensurable +whose square is still nearer to~$2$. From +Kronecker's point of view, the incommensurable +number~$\sqrt{2}$ is nothing but the symbol of this +particular method of division of commensurable +numbers; and to each mode of repartition corresponds +in this way a number, commensurable or +not, which serves as a symbol. But to be satisfied +with this would be to forget the origin of these +symbols; it remains to explain how we have been +led to attribute to them a kind of concrete +existence, and on the other hand, does not the +difficulty begin with fractions? Should we have +the notion of these numbers if we did not previously +know a matter which we conceive as infinitely +divisible---\ie, as a continuum? + +\Par{The Physical Continuum.}---We are next led to ask +\PageSep{22} +if the idea of the mathematical continuum is not +simply drawn from experiment. If that be so, the +rough data of experiment, which are our sensations, +could be measured. We might, indeed, be tempted +to believe that this is so, for in recent times there +has been an attempt to measure them, and a law +has even been formulated, known as Fechner's +law, according to which sensation is proportional +to the logarithm of the stimulus. But if we +examine the experiments by which the endeavour +has been made to establish this law, we shall be +led to a diametrically opposite conclusion. It has, +for instance, been observed that a weight~$A$ of $10$~grammes +and a weight~$B$ of $11$~grammes produced +identical sensations, that the weight~$B$ could no +longer be distinguished from a weight~$C$ of $12$~grammes, +but that the weight~$A$ was readily +distinguished from the weight~$C$. Thus the rough +results of the experiments may be expressed by +the following relations\Chg{:}{} +%[** TN: Not displayed in the English translation] +\[ +A = B,\qquad B = C,\qquad A < C, +\] +which +may be regarded as the formula of the physical +continuum. But here is an intolerable disagreement +with the law of contradiction, and the +necessity of banishing this disagreement has compelled +us to invent the mathematical continuum. +We are therefore forced to conclude that this +notion has been created entirely by the mind, but +it is experiment that has provided the opportunity. +We cannot believe that two quantities which are +equal to a third are not equal to one another, and +we are thus led to suppose that $A$~is different from~$B$, +\PageSep{23} +and $B$~from~$C$, and that if we have not been +aware of this, it is due to the imperfections of our +senses. + +\Par{The Creation of the Mathematical Continuum: First +Stage.}---So far it would suffice, in order to account +for facts, to intercalate between $A$~and~$B$ a small +number of terms which would remain discrete. +What happens now if we have recourse to some +instrument to make up for the weakness of our +senses? If, for example, we use a microscope? +Such terms as $A$~and~$B$, which before were +indistinguishable from one another, appear now +to be distinct: but between $A$~and~$B$, which are +distinct, is intercalated another new term~$D$, +which we can distinguish neither from~$A$ nor from~$B$. +Although we may use the most delicate +methods, the rough results of our experiments +will always present the characters of the physical +continuum with the contradiction which is inherent +in it. We only escape from it by incessantly +intercalating new terms between the terms already +distinguished, and this operation must be pursued +indefinitely. We might conceive that it would be +possible to stop if we could imagine an instrument +powerful enough to decompose the physical continuum +into discrete elements, just as the telescope +resolves the Milky Way into stars. But this we +cannot imagine; it is always with our senses that +we use our instruments; it is with the eye that we +observe the image magnified by the microscope, +and this image must therefore always retain the +\PageSep{24} +characters of visual sensation, and therefore those +of the physical continuum. + +Nothing distinguishes a length directly observed +from half that length doubled by the microscope. +The whole is homogeneous to the part; and there +is a fresh contradiction---or rather there would be +one if the number of the terms were supposed +to be finite; it is clear that the part containing +less terms than the whole cannot be similar to the +whole. The contradiction ceases as soon as the +number of terms is regarded as infinite. There is +nothing, for example, to prevent us from regarding +the aggregate of integers as similar to the aggregate +of even numbers, which is however only a part +of it; in fact, to each integer corresponds another +even number which is its double. But it is not +only to escape this contradiction contained in the +empiric data that the mind is led to create the +concept of a continuum formed of an indefinite +number of terms. + +Here everything takes place just as in the series +of the integers. We have the faculty of conceiving +that a unit may be added to a collection of units. +Thanks to experiment, we have had the opportunity +of exercising this faculty and are conscious of +it; but from this fact we feel that our power is +unlimited, and that we can count indefinitely, +although we have never had to count more than +a finite number of objects. In the same way, as +soon as we have intercalated terms between two +consecutive terms of a series, we feel that this +\PageSep{25} +operation may be continued without limit, and +that, so to speak, there is no intrinsic reason for +stopping. As an abbreviation, I may give the +name of a mathematical continuum of the first +order to every aggregate of terms formed after the +same law as the scale of commensurable numbers. +If, then, we intercalate new sets according to the +laws of incommensurable numbers, we obtain +what may be called a continuum of the second +order. + +\Par{Second Stage.}---We have only taken our first +step. We have explained the origin of continuums +of the first order; we must now see why +this is not sufficient, and why the incommensurable +numbers had to be invented. + +If we try to imagine a line, it must have the +characters of the physical continuum---that is to +say, our representation must have a certain +breadth. Two lines will therefore appear to us +under the form of two narrow bands, and if we +are content with this rough image, it is clear +that where two lines cross they must have some +common part. But the pure geometer makes one +further effort; without entirely renouncing the +aid of his senses, he tries to imagine a line without +breadth and a point without size. This he can +do only by imagining a line as the limit towards +which tends a band that is growing thinner and +thinner, and the point as the limit towards which +is tending an area that is growing smaller and +smaller. Our two bands, however narrow they +\PageSep{26} +may be, will always have a common area; the +smaller they are the smaller it will be, and its +limit is what the geometer calls a point. This is +why it is said that the two lines which cross +must have a common point, and this truth seems +intuitive. + +But a contradiction would be implied if we +conceived of lines as continuums of the first order---\ie, +the lines traced by the geometer should only +give us points, the co-ordinates of which are +rational numbers. The contradiction would be +manifest if we were, for instance, to assert the +existence of lines and circles. It is clear, in fact, +that if the points whose co-ordinates are commensurable +were alone regarded as real, the +in-circle of a square and the diagonal of the +square would not intersect, since the co-ordinates +of the point of intersection are incommensurable. + +Even then we should have only certain incommensurable +numbers, and not all these numbers. + +But let us imagine a line divided into two half-rays +(\Foreign{demi-droites}). Each of these half-rays will +appear to our minds as a band of a certain breadth; +these bands will fit close together, because there +must be no interval between them. The common +part will appear to us to be a point which will still +remain as we imagine the bands to become thinner +and thinner, so that we admit as an intuitive truth +that if a line be divided into two half-rays the +common frontier of these half-rays is a point. +Here we recognise the conception of Kronecker, +\PageSep{27} +in which an incommensurable number was regarded +as the common frontier of two classes of rational +numbers. Such is the origin of the continuum of +the second order, which is the mathematical continuum +properly so called. + +\Par{Summary.}---To sum up, the mind has the faculty +of creating symbols, and it is thus that it has constructed +the mathematical continuum, which is +only a particular system of symbols. The only +limit to its power is the necessity of avoiding all +contradiction; but the mind only makes use of it +when experiment gives a reason for it. + +In the case with which we are concerned, the +reason is given by the idea of the physical continuum, +drawn from the rough data of the senses. +But this idea leads to a series of contradictions +from each of which in turn we must be freed. +In this way we are forced to imagine a more +and more complicated system of symbols. That +on which we shall dwell is not merely exempt +from internal contradiction,---it was so already at +all the steps we have taken,---but it is no longer in +contradiction with the various propositions which +are called intuitive, and which are derived from +more or less elaborate empirical notions. + +\Par{Measurable Magnitude.}---So far we have not +spoken of the measure of magnitudes; we can tell +if any one of them is greater than any other, +but we cannot say that it is two or three times +as large. + +So far, I have only considered the order in which +\PageSep{28} +the terms are arranged; but that is not sufficient +for most applications. We must learn how to +compare the interval which separates any two +terms. On this condition alone will the continuum +become measurable, and the operations +of arithmetic be applicable. This can only be +done by the aid of a new and special convention; +and this convention is, that in such a +case the interval between the terms $A$~and~$B$ is +equal to the interval which separates $C$~and~$D$. +For instance, we started with the integers, and +between two consecutive sets we intercalated $n$~intermediary +sets; by convention we now assume +these new sets to be equidistant. This is one +of the ways of defining the addition of two +magnitudes; for if the interval~$AB$ is by definition +equal to the interval~$CD$, the interval~$AD$ will by +definition be the sum of the intervals $AB$~and~$AC$. +This definition is very largely, but not altogether, +arbitrary. It must satisfy certain conditions---the +commutative and associative laws of addition, for +instance; but, provided the definition we choose +satisfies these laws, the choice is indifferent, and +we need not state it precisely. + +\Par{Remarks.}---We are now in a position to discuss +several important questions. + +(1) Is the creative power of the mind exhausted +by the creation of the mathematical continuum? +The answer is in the negative, and this is shown +in a very striking manner by the work of Du~Bois +Reymond. +\PageSep{29} + +We know that mathematicians distinguish +between infinitesimals of different orders, and that +infinitesimals of the second order are infinitely +small, not only absolutely so, but also in relation +to those of the first order. It is not difficult to +imagine infinitesimals of fractional or even of +irrational order, and here once more we find the +mathematical continuum which has been dealt +with in the preceding pages. Further, there are +infinitesimals which are infinitely small with +reference to those of the first order, and infinitely +large with respect to the order~$1 + \epsilon$, however +small~$\epsilon$ may be. Here, then, are new terms intercalated +in our series; and if I may be permitted to +revert to the terminology used in the preceding +pages, a terminology which is very convenient, +although it has not been consecrated by usage, I +shall say that we have created a kind of continuum +of the third order. + +It is an easy matter to go further, but it is idle +to do so, for we would only be imagining symbols +without any possible application, and no one will +dream of doing that. This continuum of the third +order, to which we are led by the consideration of +the different orders of infinitesimals, is in itself +of but little use and hardly worth quoting. +Geometers look on it as a mere curiosity. The +mind only uses its creative faculty when experiment +requires it. + +(2) When we are once in possession of the +conception of the mathematical continuum, are +\PageSep{30} +we protected from contradictions analogous to +those which gave it birth? No, and the following +is an instance:--- + +He is a \Foreign{savant} indeed who will not take it as +evident that every curve has a tangent; and, in +fact, if we think of a curve and a straight line as +two narrow bands, we can always arrange them in +such a way that they have a common part without +intersecting. Suppose now that the breadth of +the bands diminishes indefinitely: the common +part will still remain, and in the limit, so to speak, +the two lines will have a common point, although +they do not intersect---\ie, they will touch. The +geometer who reasons in this way is only doing +what we have done when we proved that two lines +which intersect have a common point, and his +intuition might also seem to be quite legitimate. +But this is not the case. We can show that there +are curves which have no tangent, if we define +such a curve as an analytical continuum of the +second order. No doubt some artifice analogous +to those we have discussed above would enable us +to get rid of this contradiction, but as the latter is +only met with in very exceptional cases, we need +not trouble to do so. Instead of endeavouring to +reconcile intuition and analysis, we are content to +sacrifice one of them, and as analysis must be +flawless, intuition must go to the wall. + +\Par{The Physical Continuum of several Dimensions.}---We +have discussed above the physical continuum +as it is derived from the immediate evidence of our +\PageSep{31} +senses---or, if the reader prefers, from the rough +results of Fechner's experiments; I have shown +that these results are summed up in the contradictory +formulæ\Chg{:---}{} +\[ +A = B,\qquad B = C,\qquad A < C. +\] + +Let us now see how this notion is generalised, +and how from it may be derived the concept of +continuums of several dimensions. Consider any +two aggregates of sensations. We can either +distinguish between them, or we cannot; just as in +Fechner's experiments the weight of $10$~grammes +could be distinguished from the weight of $12$~grammes, +but not from the weight of $11$~grammes. +This is all that is required to construct the continuum +of several dimensions. + +Let us call one of these aggregates of sensations +an \emph{element}. It will be in a measure analogous to +the \emph{point} of the mathematicians, but will not be, +however, the same thing. We cannot say that +our element has no size, for we cannot distinguish +it from its immediate neighbours, and it is thus +surrounded by a kind of fog. If the astronomical +comparison may be allowed, our ``elements'' +would be like nebulæ, whereas the mathematical +points would be like stars. + +If this be granted, a system of elements will +form a continuum, if we can pass from any one of +them to any other by a series of consecutive +elements such that each cannot be distinguished +from its predecessor. This \emph{linear} series is to the +\emph{line} of the mathematician what the isolated \emph{element} +was to the point. +\PageSep{32} + +Before going further, I must explain what is +meant by a \emph{cut}. Let us consider a continuum~$C$, +and remove from it certain of its elements, which +for a moment we shall regard as no longer belonging +to the continuum. We shall call the aggregate +of elements thus removed a \emph{cut}. By means of this +cut, the continuum~$C$ will be \emph{subdivided} into +several distinct continuums; the aggregate of +elements which remain will cease to form a single +continuum. There will then be on~$C$ two elements, +$A$~and~$B$, which we must look upon as +belonging to two distinct continuums; and we see +that this must be so, because it will be impossible +to find a linear series of consecutive elements of~$C$ +(each of the elements indistinguishable from the +preceding, the first being~$A$ and the last~$B$), \emph{unless +one of the elements of this series is indistinguishable +from one of the elements of the cut}. + +It may happen, on the contrary, that the cut +may not be sufficient to subdivide the continuum~$C$. +To classify the physical continuums, we must +first of all ascertain the nature of the cuts which +must be made in order to subdivide them. If a +physical continuum,~$C$, may be subdivided by a cut +reducing to a finite number of elements, all distinguishable +the one from the other (and therefore +forming neither one continuum nor several continuums), +we shall call~$C$ a continuum \emph{of one +dimension}. If, on the contrary, $C$~can only be subdivided +by cuts which are themselves continuums, +we shall say that $C$~is of several dimensions; if +\PageSep{33} +the cuts are continuums of one dimension, then +we shall say that $C$~has two dimensions; if cuts of +two dimensions are sufficient, we shall say that $C$~is +of three dimensions, and so on. Thus the +notion of the physical continuum of several dimensions +is defined, thanks to the very simple fact, +that two aggregates of sensations may be distinguishable +or indistinguishable. + +\Par{The Mathematical Continuum of Several Dimensions.}---The +conception of the mathematical continuum +of $n$~dimensions may be led up to quite naturally +by a process similar to that which we discussed at +the beginning of this chapter. A point of such a +continuum is defined by a system of $n$~distinct +magnitudes which we call its co-ordinates. + +The magnitudes need not always be measurable; +there is, for instance, one branch of geometry +independent of the measure of magnitudes, in +which we are only concerned with knowing, for +example, if, on a curve~$ABC$, the point~$B$ is +between the points $A$~and~$C$, and in which it is +immaterial whether the arc~$AB$ is equal to or +twice the arc~$BC$. This branch is called \emph{Analysis +Situs}. It contains quite a large body of doctrine +which has attracted the attention of the greatest +geometers, and from which are derived, one from +another, a whole series of remarkable theorems. +What distinguishes these theorems from those of +ordinary geometry is that they are purely qualitative. +They are still true if the figures are copied +by an unskilful draughtsman, with the result that +\PageSep{34} +the proportions are distorted and the straight lines +replaced by lines which are more or less curved. + +As soon as measurement is introduced into the +continuum we have just defined, the continuum +becomes space, and geometry is born. But the +discussion of this is reserved for Part~II. +\PageSep{35} + + +\Part{II.}{Space.} + +\Chapter{III.}{Non-Euclidean Geometries.} + +\First{Every} conclusion presumes premisses. These +premisses are either self-evident and need no +demonstration, or can be established only if based +on other propositions; and, as we cannot go back +in this way to infinity, every deductive science, +and geometry in particular, must rest upon a +certain number of indemonstrable axioms. All +treatises of geometry begin therefore with the +enunciation of these axioms. But there is a +distinction to be drawn between them. Some of +these, for example, ``Things which are equal to +the same thing are equal to one another,'' are not +propositions in geometry but propositions in +analysis. I look upon them as analytical \Foreign{à~priori} +intuitions, and they concern me no further. But +I must insist on other axioms which are special +to geometry. Of these most treatises explicitly +enunciate three:---(1)~Only one line can pass +through two points; (2)~a straight line is the +\PageSep{36} +shortest distance between two points; (3)~through +one point only one parallel can be drawn to a +given straight line. Although we generally dispense +with proving the second of these axioms, it +would be possible to deduce it from the other two, +and from those much more numerous axioms +which are implicitly admitted without enunciation, +as I shall explain further on. For a long +time a proof of the third axiom known as Euclid's +postulate was sought in vain. It is impossible to +imagine the efforts that have been spent in pursuit +of this chimera. Finally, at the beginning of the +nineteenth century, and almost simultaneously, +%[** TN: Correct ("Hongrois") in the French edition] +two scientists, a Russian and a \Reword{Bulgarian}{Hungarian}, Lobatschewsky +and Bolyai, showed irrefutably that this +proof is impossible. They have nearly rid us of +inventors of geometries without a postulate, and +ever since the Académic des Sciences receives only +about one or two new demonstrations a year. +But the question was not exhausted, and it was +not long before a great step was taken by the +celebrated memoir of Riemann, entitled: \Title{Ueber +die Hypothesen welche der Geometrie zum Grunde +liegen}. This little work has inspired most of the +recent treatises to which I shall later on refer, and +among which I may mention those of Beltrami +and Helmholtz. + +\Par{The Geometry of Lobatschewsky.}---If it were +possible to deduce Euclid's postulate from the +several axioms, it is evident that by rejecting +the postulate and retaining the other axioms we +\PageSep{37} +should be led to contradictory consequences. It +would be, therefore, impossible to found on those +premisses a coherent geometry. Now, this is +precisely what Lobatschewsky has done. He +assumes at the outset that several parallels may +be drawn through a point to a given straight line, +and he retains all the other axioms of Euclid. +From these hypotheses he deduces a series of +theorems between which it is impossible to find +any contradiction, and he constructs a geometry +as impeccable in its logic as Euclidean geometry. +The theorems are very different, however, from +those to which we are accustomed, and at first +will be found a little disconcerting. For instance, +the sum of the angles of a triangle is always less +than two right angles, and the difference between +that sum and two right angles is proportional to +the area of the triangle. It is impossible to construct +a figure similar to a given figure but of +different dimensions. If the circumference of a +circle be divided into $n$~equal parts, and tangents +be drawn at the points of intersection, the $n$~tangents +will form a polygon if the radius of +the circle is small enough, but if the radius is +large enough they will never meet. We need not +multiply these examples. Lobatschewsky's propositions +have no relation to those of Euclid, +but they are none the less logically interconnected. + +\Par{Riemann's Geometry.}---Let us imagine to ourselves +a world only peopled with beings of no +thickness, and suppose these ``infinitely flat'' +\PageSep{38} +animals are all in one and the same plane, from +which they cannot emerge. Let us further admit +that this world is sufficiently distant from other +worlds to be withdrawn from their influence, and +while we are making these hypotheses it will not +cost us much to endow these beings with reasoning +power, and to believe them capable of making +a geometry. In that case they will certainly +attribute to space only two dimensions. But +now suppose that these imaginary animals, while +remaining without thickness, have the form of a +spherical, and not of a plane figure, and are all on +the same sphere, from which they cannot escape. +What kind of a geometry will they construct? In +the first place, it is clear that they will attribute to +space only two dimensions. The straight line to +them will be the shortest distance from one point +on the sphere to another---that is to say, an arc of +a great circle. In a word, their geometry will be +spherical geometry. What they will call space +will be the sphere on which they are confined, and +on which take place all the phenomena with +which they are acquainted. Their space will +therefore be \emph{unbounded}, since on a sphere one may +always walk forward without ever being brought +to a stop, and yet it will be \emph{finite}; the end will +never be found, but the complete tour can be +made. Well, Riemann's geometry is spherical +geometry extended to three dimensions. To construct +it, the German mathematician had first of +all to throw overboard, not only Euclid's postulate +\PageSep{39} +but also the first axiom that \emph{only one line can pass +through two points}. On a sphere, through two +given points, we can \emph{in general} draw only one great +circle which, as we have just seen, would be to +our imaginary beings a straight line. But there +was one exception. If the two given points are +at the ends of a diameter, an infinite number of +great circles can be drawn through them. In +the same way, in Riemann's geometry---at least in +one of its forms---through two points only one +straight line can in general be drawn, but there are +exceptional cases in which through two points +an infinite number of straight lines can be drawn. +So there is a kind of opposition between the +geometries of Riemann and Lobatschewsky. For +instance, the sum of the angles of a triangle is +equal to two right angles in Euclid's geometry, +less than two right angles in that of Lobatschewsky, +and greater than two right angles in that +of Riemann. The number of parallel lines that +can be drawn through a given point to a given +line is one in Euclid's geometry, none in Riemann's, +and an infinite number in the geometry of Lobatschewsky. +Let us add that Riemann's space is +finite, although unbounded in the sense which we +have above attached to these words. + +\Par{Surfaces with Constant Curvature.}---One objection, +however, remains possible. There is no contradiction +between the theorems of Lobatschewsky and +Riemann; but however numerous are the other +consequences that these geometers have deduced +\PageSep{40} +from their hypotheses, they had to arrest their +course before they exhausted them all, for the +number would be infinite; and who can say that +if they had carried their deductions further they +would not have eventually reached some contradiction? +This difficulty does not exist for +Riemann's geometry, provided it is limited to +two dimensions. As we have seen, the two-dimensional +geometry of Riemann, in fact, does +not differ from spherical geometry, which is only a +branch of ordinary geometry, and is therefore outside +all contradiction. Beltrami, by showing that +Lobatschewsky's two-dimensional geometry was +only a branch of ordinary geometry, has equally +refuted the objection as far as it is concerned. +This is the course of his argument: Let us consider +any figure whatever on a surface. Imagine +this figure to be traced on a flexible and inextensible +canvas applied to the surface, in such +a way that when the canvas is displaced and +deformed the different lines of the figure change +their form without changing their length. As a +rule, this flexible and inextensible figure cannot be +displaced without leaving the surface. But there +are certain surfaces for which such a movement +would be possible. They are surfaces of constant +curvature. If we resume the comparison that we +made just now, and imagine beings without thickness +living on one of these surfaces, they will +regard as possible the motion of a figure all the +lines of which remain of a constant length. Such +\PageSep{41} +a movement would appear absurd, on the other +hand, to animals without thickness living on a +surface of variable curvature. These surfaces of +constant curvature are of two kinds. The +curvature of some is \emph{positive}, and they may be +deformed so as to be applied to a sphere. The +geometry of these surfaces is therefore reduced to +spherical geometry---namely, Riemann's. The curvature +of others is \emph{negative}. Beltrami has shown +that the geometry of these surfaces is identical +with that of Lobatschewsky. Thus the two-dimensional +geometries of Riemann and Lobatschewsky +are connected with Euclidean geometry. + +\Par{Interpretation of Non-Euclidean Geometries.}---Thus +vanishes the objection so far as two-dimensional +geometries are concerned. It would be easy to +extend Beltrami's reasoning to three-dimensional +geometries, and minds which do not recoil before +space of four dimensions will see no difficulty in +it; but such minds are few in number. I prefer, +then, to proceed otherwise. Let us consider a +certain plane, which I shall call the fundamental +plane, and let us construct a kind of dictionary by +making a double series of terms written in two +columns, and corresponding each to each, just as +in ordinary dictionaries the words in two languages +which have the same signification correspond to +one another:--- +\Dict{Space}{\raggedright The portion of space situated +above the fundamental +plane.} +\PageSep{42} +\Dict{Plane}{\raggedright Sphere cutting orthogonally +the fundamental plane.} +\Dict{Line}{\raggedright Circle cutting orthogonally +the fundamental plane.} +\Dict{Sphere}{Sphere.} +\Dict{Circle}{Circle.} +\Dict{Angle}{Angle.} +\Dict{Distance between +two points}{Logarithm of the anharmonic +ratio of these two points +and of the intersection +of the fundamental plane +with the circle passing +through these two points +and cutting it orthogonally.} +\Dict{Etc.}{Etc.} + +Let us now take Lobatschewsky's theorems and +translate them by the aid of this dictionary, as we +would translate a German text with the aid of +a German-French dictionary. \emph{We shall then +obtain the theorems of ordinary geometry.} For +instance, Lobatschewsky's theorem: ``The sum of +the angles of a triangle is less than two right +angles,'' may be translated thus: ``If a curvilinear +triangle has for its sides arcs of circles which if +produced would cut orthogonally the fundamental +plane, the sum of the angles of this curvilinear +triangle will be less than two right angles.'' Thus, +however far the consequences of Lobatschewsky's +hypotheses are carried, they will never lead to a +\PageSep{43} +contradiction; in fact, if two of Lobatschewsky's +theorems were contradictory, the translations of +these two theorems made by the aid of our +dictionary would be contradictory also. But +these translations are theorems of ordinary +geometry, and no one doubts that ordinary +geometry is exempt from contradiction. Whence +is the certainty derived, and how far is it justified? +That is a question upon which I cannot enter +here, but it is a very interesting question, and I +think not insoluble. Nothing, therefore, is left of +the objection I formulated above. But this is not +all. Lobatschewsky's geometry being susceptible +of a concrete interpretation, ceases to be a useless +logical exercise, and may be applied. I have no +time here to deal with these applications, nor +with what Herr Klein and myself have done by +using them in the integration of linear equations. +Further, this interpretation is not unique, and +several dictionaries may be constructed analogous +to that above, which will enable us by a simple +translation to convert Lobatschewsky's theorems +into the theorems of ordinary geometry. + +\Par{Implicit Axioms.}---Are the axioms implicitly +enunciated in our text-books the only foundation +of geometry? We may be assured of the contrary +when we see that, when they are abandoned one +after another, there are still left standing some +propositions which are common to the geometries +of Euclid, Lobatschewsky, and Riemann. These +propositions must be based on premisses that +\PageSep{44} +geometers admit without enunciation. It is interesting +to try and extract them from the classical +proofs. + +John Stuart Mill asserted\footnote + {\Title{Logic}, c.~viii., cf.\ Definitions, §5--6.\Transl} +that every definition +contains an axiom, because by defining we implicitly +affirm the existence of the object defined. +That is going rather too far. It is but rarely in +mathematics that a definition is given without +following it up by the proof of the existence of the +object defined, and when this is not done it is +generally because the reader can easily supply +it; and it must not be forgotten that the word +``existence'' has not the same meaning when it +refers to a mathematical entity as when it refers to +a material object. + +A mathematical entity exists provided there is +no contradiction implied in its definition, either in +itself, or with the propositions previously admitted. +But if the observation of John Stuart Mill cannot +be applied to all definitions, it is none the less true +for some of them. A plane is sometimes defined +in the following manner:---The plane is a surface +such that the line which joins any two points +upon it lies wholly on that surface. Now, there is +obviously a new axiom concealed in this definition. +It is true we might change it, and that would be +preferable, but then we should have to enunciate +the axiom explicitly. Other definitions may give +rise to no less important reflections, such as, for +example, that of the equality of two figures. Two +\PageSep{45} +figures are equal when they can be superposed. +To superpose them, one of them must be displaced +until it coincides with the other. But how must +it be displaced? If we asked that question, no +doubt we should be told that it ought to be done +without deforming it, and as an invariable solid is +displaced. The vicious circle would then be evident. +As a matter of fact, this definition defines +nothing. It has no meaning to a being living in a +world in which there are only fluids. If it seems +clear to us, it is because we are accustomed to the +properties of natural solids which do not much +differ from those of the ideal solids, all of whose +dimensions are invariable. However, imperfect as +it may be, this definition implies an axiom. The +possibility of the motion of an invariable figure is +not a self-evident truth. At least it is only so in +the application to Euclid's postulate, and not as an +analytical \Foreign{à~priori} intuition would be. Moreover, +when we study the definitions and the proofs +of geometry, we see that we are compelled to +admit without proof not only the possibility of +this motion, but also some of its properties. This +first arises in the definition of the straight line. +Many defective definitions have been given, but +the true one is that which is understood in all the +proofs in which the straight line intervenes. ``It +may happen that the motion of an invariable figure +may be such that all the points of a line belonging +to the figure are motionless, while all the points +situate outside that line are in motion. Such a +\PageSep{46} +line would be called a straight line.'' We have +deliberately in this enunciation separated the +definition from the axiom which it implies. Many +proofs such as those of the cases of the equality of +triangles, of the possibility of drawing a perpendicular +from a point to a straight line, assume propositions +the enunciations of which are dispensed +with, for they necessarily imply that it is possible +to move a figure in space in a certain way. + +\Par{The Fourth Geometry.}---Among these explicit +axioms there is one which seems to me to deserve +some attention, because when we abandon it we +can construct a fourth geometry as coherent as +those of Euclid, Lobatschewsky, and Riemann. +To prove that we can always draw a perpendicular +at a point~$A$ to a straight line~$AB$, we consider a +straight line~$AC$ movable about the point~$A$, and +initially identical with the fixed straight line~$AB$. +We then can make it turn about the point~$A$ until +it lies in~$AB$ produced. Thus we assume two +propositions---first, that such a rotation is possible, +and then that it may continue until the two lines +lie the one in the other produced. If the first +point is conceded and the second rejected, we are +led to a series of theorems even stranger than those +of Lobatschewsky and Riemann, but equally free +from contradiction. I shall give only one of these +theorems, and I shall not choose the least remarkable +of them. \emph{A real straight line may be perpendicular +to itself.} + +\Par{Lie's Theorem.}---The number of axioms implicitly +\PageSep{47} +introduced into classical proofs is greater than +necessary, and it would be interesting to reduce +them to a minimum. It may be asked, in the first +place, if this reduction is possible---if the number of +necessary axioms and that of imaginable geometries +is not infinite? A theorem due to Sophus Lie is of +weighty importance in this discussion. It may be +enunciated in the following manner:---Suppose the +following premisses are admitted: (1)~space has $n$~dimensions; +(2)~the movement of an invariable +figure is possible; (3)~$p$~conditions are necessary to +determine the position of this figure in space. + +\emph{The number of geometries compatible with these +premisses will be limited.} I may even add that if $n$~is +given, a superior limit can be assigned to~$p$. If, +therefore, the possibility of the movement is +granted, we can only invent a finite and even +a rather restricted number of three-dimensional +geometries. + +\Par{Riemann's Geometries.}---However, this result +seems contradicted by Riemann, for that scientist +constructs an infinite number of geometries, and +that to which his name is usually attached is only +a particular case of them. All depends, he says, +on the manner in which the length of a curve is +defined. Now, there is an infinite number of ways +of defining this length, and each of them may be +the starting-point of a new geometry. That is +perfectly true, but most of these definitions are incompatible +with the movement of a variable figure +such as we assume to be possible in Lie's theorem. +\PageSep{48} +These geometries of Riemann, so interesting on +various grounds, can never be, therefore, purely +analytical, and would not lend themselves to +proofs analogous to those of Euclid. + +\Par{On the Nature of Axioms.}---Most mathematicians +regard Lobatschewsky's geometry as a mere logical +curiosity. Some of them have, however, gone +further. If several geometries are possible, they +say, is it certain that our geometry is the one that +is true? Experiment no doubt teaches us that the +sum of the angles of a triangle is equal to two +right angles, but this is because the triangles we +deal with are too small. According to Lobatschewsky, +the difference is proportional to the area +of the triangle, and will not this become sensible +when we operate on much larger triangles, and +when our measurements become more accurate? +Euclid's geometry would thus be a provisory +geometry. Now, to discuss this view we must +first of all ask ourselves, what is the nature of +geometrical axioms? Are they synthetic \Foreign{à~priori} +intuitions, as Kant affirmed? They would then +be imposed upon us with such a force that we +could not conceive of the contrary proposition, nor +could we build upon it a theoretical edifice. There +would be no non-Euclidean geometry. To convince +ourselves of this, let us take a true synthetic +\Foreign{à~priori} intuition---the following, for instance, which +played an important part in the first chapter:---If +a theorem is true for the number~$1$, and if it has +been proved that it is true of~$n + 1$, provided it is +\PageSep{49} +true of~$n$, it will be true for all positive integers. +Let us next try to get rid of this, and while rejecting +this proposition let us construct a false +arithmetic analogous to non-Euclidean geometry. +We shall not be able to do it. We shall be even +tempted at the outset to look upon these intuitions +as analytical. Besides, to take up again +our fiction of animals without thickness, we can +scarcely admit that these beings, if their minds +are like ours, would adopt the Euclidean geometry, +which would be contradicted by all their experience. +Ought we, then, to conclude that the +axioms of geometry are experimental truths? +But we do not make experiments on ideal lines or +ideal circles; we can only make them on material +objects. On what, therefore, would experiments +serving as a foundation for geometry be based? +The answer is easy. We have seen above that we +constantly reason as if the geometrical figures +behaved like solids. What geometry would borrow +from experiment would be therefore the properties +of these bodies. The properties of light +and its propagation in a straight line have also +given rise to some of the propositions of geometry, +and in particular to those of projective geometry, +so that from that point of view one would be +tempted to say that metrical geometry is the study +of solids, and projective geometry that of light. +But a difficulty remains, and is unsurmountable. +If geometry were an experimental science, it would +not be an exact science. It would be subjected to +\PageSep{5O} +continual revision. Nay, it would from that day +forth be proved to be erroneous, for we know that +no rigorously invariable solid exists. \emph{The geometrical +axioms are therefore neither synthetic \Foreign{à~priori} +intuitions nor experimental facts.} They are conventions. +Our choice among all possible conventions +is \emph{guided} by experimental facts; but it remains +\emph{free}, and is only limited by the necessity of avoiding +every contradiction, and thus it is that postulates +may remain rigorously true even when the +experimental laws which have determined their +adoption are only approximate. In other words, +\emph{the axioms of geometry} (I do not speak of those of +arithmetic) \emph{are only definitions in disguise}. What, +then, are we to think of the question: Is +Euclidean geometry true? It has no meaning. +We might as well ask if the metric system is true, +and if the old weights and measures are false; if +Cartesian co-ordinates are true and polar co-ordinates +false. One geometry cannot be more +true than another; it can only be more convenient. +Now, Euclidean geometry is, and will remain, the +most convenient: 1st,~because it is the simplest, +and it is not so only because of our mental habits +or because of the kind of direct intuition that we +have of Euclidean space; it is the simplest in +itself, just as a polynomial of the first degree is +simpler than a polynomial of the second degree; +2nd,~because it sufficiently agrees with the properties +of natural solids, those bodies which we +can compare and measure by means of our senses. +\PageSep{51} + + +\Chapter{IV.}{Space and Geometry.} + +\First{Let} us begin with a little paradox. Beings whose +minds were made as ours, and with senses like +ours, but without any preliminary education, +might receive from a suitably-chosen external +world impressions which would lead them to +construct a geometry other than that of Euclid, +and to localise the phenomena of this external +world in a non-Euclidean space, or even in space +of four dimensions. As for us, whose education +has been made by our actual world, if we were +suddenly transported into this new world, we +should have no difficulty in referring phenomena +to our Euclidean space. Perhaps somebody may +appear on the scene some day who will devote his +life to it, and be able to represent to himself the +fourth dimension. + +\Par{Geometrical Space and Representative Space.}---It is +often said that the images we form of external +objects are localised in space, and even that they +can only be formed on this condition. It is also +said that this space, which thus serves as a kind of +framework ready prepared for our sensations and +representations, is identical with the space of the +\PageSep{52} +geometers, having all the properties of that space. +To all clear-headed men who think in this way, +the preceding statement might well appear extraordinary; +but it is as well to see if they are not +the victims of some illusion which closer analysis +may be able to dissipate. In the first place, what +are the properties of space properly so called? +I mean of that space which is the object of +geometry, and which I shall call geometrical +space. The following are some of the more +essential:--- + +1st,~it is continuous; 2nd,~it is infinite; 3rd,~it +is of three dimensions; 4th,~it is homogeneous---that +is to say, all its points are identical one +with another; 5th,~it is isotropic. Compare this +now with the framework of our representations +and sensations, which I may call \emph{representative +space}. + +\Par{Visual Space.}---First of all let us consider a +purely visual impression, due to an image formed +on the back of the retina. A cursory analysis shows +us this image as continuous, but as possessing only +two dimensions, which already distinguishes purely +visual from what may be called geometrical space. +On the other hand, the image is enclosed within +a limited framework; and there is a no less +important difference: \emph{this pure visual space is not +homogeneous}. All the points on the retina, apart +from the images which may be formed, do not +play the same rôle. The yellow spot can in no +way be regarded as identical with a point on the +\PageSep{53} +edge of the retina. Not only does the same object +produce on it much brighter impressions, but in +the whole of the \emph{limited} framework the point +which occupies the centre will not appear identical +with a point near one of the edges. Closer +analysis no doubt would show us that this continuity +of visual space and its two dimensions are +but an illusion. It would make visual space even +more different than before from geometrical space, +but we may treat this remark as incidental. + +However, sight enables us to appreciate distance, +and therefore to perceive a third dimension. +But every one knows that this perception of the +third dimension reduces to a sense of the effort of +accommodation which must be made, and to a +sense of the convergence of the two eyes, that +must take place in order to perceive an object +distinctly. These are muscular sensations quite +different from the visual sensations which have +given us the concept of the two first dimensions. +The third dimension will therefore not appear to us +as playing the same rôle as the two others. What +may be called \emph{complete visual space} is not therefore +an isotropic space. It has, it is true, exactly +three dimensions; which means that the elements +of our visual sensations (those at least which +concur in forming the concept of extension) will +be completely defined if we know three of them; +or, in mathematical language, they will be functions +of three independent variables. But let us +look at the matter a little closer. The third +\PageSep{54} +dimension is revealed to us in two different ways: +by the effort of accommodation, and by the convergence +of the eyes. No doubt these two indications +are always in harmony; there is between +them a constant relation; or, in mathematical +language, the two variables which measure these +two muscular sensations do not appear to us as +independent. Or, again, to avoid an appeal to +mathematical ideas which are already rather too +refined, we may go back to the language of the +preceding chapter and enunciate the same fact as +follows:---If two sensations of convergence $A$~and~$B$ +are indistinguishable, the two sensations of +accommodation $A'$~and~$B'$ which accompany them +respectively will also be indistinguishable. But +that is, so to speak, an experimental fact. Nothing +prevents us \Foreign{à~priori} from assuming the contrary, +and if the contrary takes place, if these two +muscular sensations both vary independently, we +must take into account one more independent +variable, and complete visual space will appear +to us as a physical continuum of four dimensions. +And so in this there is also a fact of \emph{external} +experiment. Nothing prevents us from assuming +that a being with a mind like ours, with the same +sense-organs as ourselves, may be placed in a world +in which light would only reach him after being +passed through refracting media of complicated +form. The two indications which enable us to +appreciate distances would cease to be connected +by a constant relation. A being educating his +\PageSep{55} +senses in such a world would no doubt attribute +four dimensions to complete visual space. + +\Par{Tactile and Motor Space.}---``Tactile space'' is +more complicated still than visual space, and differs +even more widely from geometrical space. It is +useless to repeat for the sense of touch my remarks +on the sense of sight. But outside the data of +sight and touch there are other sensations which +contribute as much and more than they do to the +genesis of the concept of space. They are those +which everybody knows, which accompany all our +movements, and which we usually call muscular +sensations. The corresponding framework constitutes +what may be called \emph{motor space}. Each +muscle gives rise to a special sensation which may +be increased or diminished so that the aggregate +of our muscular sensations will depend upon as +many variables as we have muscles. From this +point of view \emph{motor space would have as many dimensions +as we have muscles}. I know that it is said +that if the muscular sensations contribute to form +the concept of space, it is because we have the +sense of the \emph{direction} of each movement, and that +this is an integral part of the sensation. If this +were so, and if a muscular sense could not be +aroused unless it were accompanied by this geometrical +sense of direction, geometrical space +would certainly be a form imposed upon our +sensitiveness. But I do not see this at all when +I analyse my sensations. What I do see is that +the sensations which correspond to movements in +\PageSep{56} +the same direction are connected in my mind by a +simple \emph{association of ideas}. It is to this association +that what we call the sense of direction is reduced. +We cannot therefore discover this sense in a single +sensation. This association is extremely complex, +for the contraction of the same muscle may correspond, +according to the position of the limbs, +to very different movements of direction. Moreover, +it is evidently acquired; it is like all +associations of ideas, the result of a \emph{habit}. This +habit itself is the result of a very large number of +\emph{experiments}, and no doubt if the education of our +senses had taken place in a different medium, +where we would have been subjected to different +impressions, then contrary habits would have been +acquired, and our muscular sensations would have +been associated according to other laws. + +\Par{Characteristics of Representative Space.}---Thus representative +space in its triple form---visual, +tactile, and motor---differs essentially from geometrical +space. It is neither homogeneous nor +isotropic; we cannot even say that it is of three +dimensions. It is often said that we ``project'' +into geometrical space the objects of our external +perception; that we ``localise'' them. Now, has +that any meaning, and if so what is that meaning? +Does it mean that we \emph{represent} to ourselves external +objects in geometrical space? Our representations +are only the reproduction of our sensations; +they cannot therefore be arranged in the +same framework---that is to say, in representative +\PageSep{57} +space. It is also just as impossible for us to represent +to ourselves external objects in geometrical +space, as it is impossible for a painter to paint on +a flat surface objects with their three dimensions. +Representative space is only an image of geometrical +space, an image deformed by a kind of +perspective, and we can only represent to ourselves +objects by making them obey the laws of +this perspective. Thus we do not \emph{represent} to ourselves +external bodies in geometrical space, but we +\emph{reason} about these bodies as if they were situated +in geometrical space. When it is said, on the +other hand, that we ``localise'' such an object in +such a point of space, what does it mean? \emph{It +simply means that we represent to ourselves the movements +that must take place to reach that object.} And +it does not mean that to represent to ourselves +these movements they must be projected into +space, and that the concept of space must therefore +pre-exist. When I say that we represent to ourselves +these movements, I only mean that we +represent to ourselves the muscular sensations +which accompany them, and which have no +geometrical character, and which therefore in no +way imply the pre-existence of the concept of +space. + +\Par{Changes of State and Changes of Position.}---But, +it may be said, if the concept of geometrical space +is not imposed upon our minds, and if, on the +other hand, none of our sensations can furnish us +with that concept, how then did it ever come into +\PageSep{58} +existence? This is what we have now to examine, +and it will take some time; but I can sum up in a +few words the attempt at explanation which I am +going to develop. \emph{None of our sensations, if isolated, +could have brought us to the concept of space; we are +brought to it solely by studying the laws by which those +sensations succeed one another.} We see at first that +our impressions are subject to change; but among +the changes that we ascertain, we are very soon +led to make a distinction. Sometimes we say that +the objects, the causes of these impressions, have +changed their state, sometimes that they have +changed their position, that they have only been +displaced. Whether an object changes its state or +only its position, this is always translated for us in +the same manner, \emph{by a modification in an aggregate +of impressions}. How then have we been enabled +to distinguish them? If there were only change +of position, we could restore the primitive aggregate +of impressions by making movements which +would confront us with the movable object in +the same \emph{relative} situation. We thus \emph{correct} the +modification which was produced, and we re-establish +the initial state by an inverse modification. +If, for example, it were a question of the +sight, and if an object be displaced before our +eyes, we can ``follow it with the eye,'' and retain +its image on the same point of the retina by +appropriate movements of the eyeball. These +movements we are conscious of because they are +voluntary, and because they are accompanied by +\PageSep{59} +muscular sensations. But that does not mean +that we represent them to ourselves in geometrical +space. So what characterises change of position, +what distinguishes it from change of state, is that +it can always be \emph{corrected} by this means. It may +therefore happen that we pass from the aggregate +of impressions~$A$ to the aggregate~$B$ in two different +ways. First, involuntarily and without experiencing +muscular sensations---which happens +when it is the object that is displaced; secondly, +voluntarily, and with muscular sensation---which +happens when the object is motionless, but when +we displace ourselves in such a way that the +object has relative motion with respect to us. If +this be so, the translation of the aggregate~$A$ to +the aggregate~$B$ is only a change of position. It +follows that sight and touch could not have given +us the idea of space without the help of the +``muscular sense.'' Not only could this concept +not be derived from a single sensation, or even from +\emph{a series of sensations}; but a \emph{motionless} being could +never have acquired it, because, not being able to +correct by his movements the effects of the change +of position of external objects, he would have had +no reason to distinguish them from changes of +state. Nor would he have been able to acquire +it if his movements had not been voluntary, +or if they were unaccompanied by any sensations +whatever. + +\Par{Conditions of Compensation.}---How is such a +compensation possible in such a way that two +\PageSep{60} +changes, otherwise mutually independent, may be +reciprocally corrected? A mind \emph{already familiar +with geometry} would reason as follows:---If there +is to be compensation, the different parts of the +external object on the one hand, and the different +organs of our senses on the other, must be in the +same \emph{relative} position after the double change. +And for that to be the case, the different parts of +the external body on the one hand, and the different +organs of our senses on the other, must have +the same relative position to each other after the +double change; and so with the different parts of +our body with respect to each other. In other +words, the external object in the first change must +be displaced as an invariable solid would be displaced, +and it must also be so with the whole of our +body in the second change, which is to correct the +first. Under these conditions compensation may +be produced. But we who as yet know nothing of +geometry, whose ideas of space are not yet formed, +we cannot reason in this way---we cannot predict +\Foreign{à~priori} if compensation is possible. But experiment +shows us that it sometimes does take place, +and we start from this experimental fact in order +to distinguish changes of state from changes of +position. + +\Par{Solid Bodies and Geometry.}---Among surrounding +objects there are some which frequently experience +displacements that may be thus corrected by a +\emph{correlative} movement of our own body---namely, +\emph{solid bodies}. The other objects, whose form is variable, +\PageSep{61} +only in exceptional circumstances undergo +similar displacement (change of position without +change of form). When the displacement of a +body takes place with deformation, we can no +longer by appropriate movements place the organs +of our body in the same \emph{relative} situation with +respect to this body; we can no longer, therefore, +reconstruct the primitive aggregate of impressions. + +It is only later, and after a series of new experiments, +that we learn how to decompose a body of +variable form into smaller elements such that each +is displaced approximately according to the same +laws as solid bodies. We thus distinguish ``deformations'' +from other changes of state. In these +deformations each element undergoes a simple +change of position which may be corrected; but the +modification of the aggregate is more profound, +and can no longer be corrected by a correlative +movement. Such a concept is very complex even +at this stage, and has been relatively slow in +its appearance. It would not have been conceived +at all had not the observation of solid bodies shown +us beforehand how to distinguish changes of +position. + +\emph{If, then, there were no solid bodies in nature there +would be no geometry.} + +Another remark deserves a moment's attention. +Suppose a solid body to occupy successively the +positions $\alpha$~and~$\beta$; in the first position it will give +us an aggregate of impressions~$A$, and in the second +position the aggregate of impressions~$B$. Now let +\PageSep{62} +there be a second solid body, of qualities entirely +different from the first---of different colour, for +instance. Assume it to pass from the position~$\alpha$, +where it gives us the aggregate of impressions~$A'$ to +the position~$\beta$, where it gives the aggregate of +impressions~$B'$. In general, the aggregate~$A$ will +have nothing in common with the aggregate~$A'$, +nor will the aggregate~$B$ have anything in common +with the aggregate~$B'$. The transition from the +aggregate~$A$ to the aggregate~$B$, and that of the +aggregate~$A'$ to the aggregate~$B'$, are therefore +two changes which \emph{in themselves} have in general +nothing in common. Yet we consider both +these changes as displacements; and, further, we +consider them the \emph{same} displacement. How can +this be? It is simply because they may be both +corrected by the \emph{same} correlative movement of our +body. ``Correlative movement,'' therefore, constitutes +the \emph{sole connection} between two phenomena +which otherwise we should never have dreamed of +connecting. + +On the other hand, our body, thanks to the +number of its articulations and muscles, may have +a multitude of different movements, but all are not +capable of ``correcting'' a modification of external +objects; those alone are capable of it in which +our whole body, or at least all those in which +the organs of our senses enter into play are +displaced \Foreign{en bloc}---\ie, without any variation of +their relative positions, as in the case of a solid +body. +\PageSep{63} + +To sum up:\Add{---} + +1. In the first place, we distinguish two categories +of phenomena:---The first involuntary, unaccompanied +by muscular sensations, and attributed to +external objects---they are external changes; the +second, of opposite character and attributed to the +movements of our own body, are internal changes. + +2. We notice that certain changes of each in +these categories may be corrected by a correlative +change of the other category. + +3. We distinguish among external changes those +that have a correlative in the other category---which +we call displacements; and in the same way +we distinguish among the internal changes those +which have a correlative in the first category. + +Thus by means of this reciprocity is defined a +particular class of phenomena called displacements. +\emph{The laws of these phenomena are the object of +geometry.} + +\Par{Law of Homogeneity.}---The first of these laws +is the law of homogeneity. Suppose that by an +external change we pass from the aggregate of +impressions~$A$ to the aggregate~$B$, and that then +this change~$\alpha$ is corrected by a correlative +voluntary movement~$\beta$, so that we are brought +back to the aggregate~$A$. Suppose now that +another external change~$\alpha'$ brings us again from +the aggregate~$A$ to the aggregate~$B$. Experiment +then shows us that this change~$\alpha'$, like the change~$\alpha$, +may be corrected by a voluntary correlative +movement~$\beta'$, and that this movement~$\beta'$ corresponds +\PageSep{64} +to the same muscular sensations as the +movement~$\beta$ which corrected~$\alpha$. + +This fact is usually enunciated as follows:---\emph{Space +is homogeneous and isotropic.} We may also say that a +movement which is once produced may be repeated +a second and a third time, and so on, without any +variation of its properties. In the first chapter, in +which we discussed the nature of mathematical +reasoning, we saw the importance that should be +attached to the possibility of repeating the same +operation indefinitely. The virtue of mathematical +reasoning is due to this repetition; by means of the +law of homogeneity geometrical facts are apprehended. +To be complete, to the law of homogeneity +must be added a multitude of other laws, +into the details of which I do not propose to enter, +but which mathematicians sum up by saying that +these displacements form a ``group.'' + +\Par{The Non-Euclidean World.}---If geometrical space +were a framework imposed on \emph{each} of our representations +considered individually, it would be +impossible to represent to ourselves an image +without this framework, and we should be quite +unable to change our geometry. But this is not +the case; geometry is only the summary of the +laws by which these images succeed each other. +There is nothing, therefore, to prevent us from +imagining a series of representations, similar in +every way to our ordinary representations, but +succeeding one another according to laws which +differ from those to which we are accustomed. We +\PageSep{65} +may thus conceive that beings whose education +has taken place in a medium in which those laws +would be so different, might have a very different +geometry from ours. + +Suppose, for example, a world enclosed in a large +sphere and subject to the following laws:---The +temperature is not uniform; it is greatest at the +centre, and gradually decreases as we move towards +the circumference of the sphere, where it is absolute +zero. The law of this temperature is as follows:---If +$R$~be the radius of the sphere, and $r$~the distance +of the point considered from the centre, the absolute +temperature will be proportional to~$R^{2} - r^{2}$. +Further, I shall suppose that in this world all bodies +have the same co-efficient of dilatation, so that the +linear dilatation of any body is proportional to its +absolute temperature. Finally, I shall assume that +a body transported from one point to another of +different temperature is instantaneously in thermal +equilibrium with its new environment. There is +nothing in these hypotheses either contradictory +or unimaginable. A moving object will become +smaller and smaller as it approaches the circumference +of the sphere. Let us observe, in the first +place, that although from the point of view of our +ordinary geometry this world is finite, to its inhabitants +it will appear infinite. As they approach the +surface of the sphere they become colder, and at +the same time smaller and smaller. The steps +they take are therefore also smaller and smaller, +so that they can never reach the boundary of the +\PageSep{66} +sphere. If to us geometry is only the study of the +laws according to which invariable solids move, to +these imaginary beings it will be the study of the +laws of motion of solids \emph{deformed by the differences +of temperature} alluded to. + +No doubt, in our world, natural solids also experience +variations of form and volume due to +differences of temperature. But in laying the +foundations of geometry we neglect these variations; +for besides being but small they are irregular, +and consequently appear to us to be accidental. +In our hypothetical world this will no longer be +the case, the variations will obey very simple and +regular laws. On the other hand, the different +solid parts of which the bodies of these inhabitants +are composed will undergo the same variations of +form and volume. + +Let me make another hypothesis: suppose that +light passes through media of different refractive +indices, such that the index of refraction is inversely +proportional to~$R^{2} - r^{2}$. Under these conditions it +is clear that the rays of light will no longer be +rectilinear but circular. To justify what has been +said, we have to prove that certain changes in the +position of external objects may be corrected by +correlative movements of the beings which inhabit +this imaginary world; and in such a way as to +restore the primitive aggregate of the impressions +experienced by these sentient beings. Suppose, +for example, that an object is displaced and +deformed, not like an invariable solid, but like a +\PageSep{67} +solid subjected to unequal dilatations in exact conformity +with the law of temperature assumed +above. To use an abbreviation, we shall call such +a movement a non-Euclidean displacement. + +If a sentient being be in the neighbourhood of +such a displacement of the object, his impressions +will be modified; but by moving in a suitable +manner, he may reconstruct them. For this +purpose, all that is required is that the aggregate +of the sentient being and the object, considered as +forming a single body, shall experience one of those +special displacements which I have just called non-Euclidean. +This is possible if we suppose that the +limbs of these beings dilate according to the same +laws as the other bodies of the world they inhabit. + +Although from the point of view of our ordinary +geometry there is a deformation of the bodies in +this displacement, and although their different +parts are no longer in the same relative position, +nevertheless we shall see that the impressions of +the sentient being remain the same as before; in +fact, though the mutual distances of the different +parts have varied, yet the parts which at first were +in contact are still in contact. It follows that +tactile impressions will be unchanged. On the +other hand, from the hypothesis as to refraction +and the curvature of the rays of light, visual impressions +will also be unchanged. These imaginary +beings will therefore be led to classify the phenomena +they observe, and to distinguish among them +the ``changes of position,'' which may be corrected +\PageSep{68} +by a voluntary correlative movement, just as we +do. + +If they construct a geometry, it will not be like +ours, which is the study of the movements of our +invariable solids; it will be the study of the +changes of position which they will have thus +distinguished, and will be ``non-Euclidean displacements,'' +and \emph{this will be non-Euclidean geometry}. +So that beings like ourselves, educated in +such a world, will not have the same geometry as +ours. + +\Par{The World of Four Dimensions.}---Just as we have +pictured to ourselves a non-Euclidean world, so we +may picture a world of four dimensions. + +The sense of light, even with one eye, together +with the muscular sensations relative to the movements +of the eyeball, will suffice to enable us to +conceive of space of three dimensions. The images +of external objects are painted on the retina, which +is a plane of two dimensions; these are \emph{perspectives}. +But as eye and objects are movable, we see in +succession different perspectives of the same body +taken from different points of view. We find at +the same time that the transition from one perspective +to another is often accompanied by +muscular sensations. If the transition from the +perspective~$A$ to the perspective~$B$, and that of the +perspective~$A'$ to the perspective~$B'$ are accompanied +by the same muscular sensations, we +connect them as we do other operations of the +same nature. Then when we study the laws +\PageSep{69} +according to which these operations are combined, +we see that they form a group, which has +the same structure as that of the movements of +invariable solids. Now, we have seen that it is +from the properties of this group that we derive +the idea of geometrical space and that of three +dimensions. We thus understand how these +perspectives gave rise to the conception of three +dimensions, although each perspective is of only +two dimensions,---because \emph{they succeed each other +according to certain laws}. Well, in the same way +that we draw the perspective of a three-dimensional +figure on a plane, so we can draw that of a +four-dimensional figure on a canvas of three (or +two) dimensions. To a geometer this is but child's +play. We can even draw several perspectives of +the same figure from several different points of +view. We can easily represent to ourselves these +perspectives, since they are of only three dimensions. +Imagine that the different perspectives of +one and the same object to occur in succession, +and that the transition from one to the other is +accompanied by muscular sensations. It is understood +that we shall consider two of these transitions +as two operations of the same nature when they +are associated with the same muscular sensations. +There is nothing, then, to prevent us from imagining +that these operations are combined according +to any law we choose---for instance, by forming +a group with the same structure as that of the +movements of an invariable four-dimensional solid. +\PageSep{70} +In this there is nothing that we cannot represent +to ourselves, and, moreover, these sensations are +those which a being would experience who has a +retina of two dimensions, and who may be displaced +in space of four dimensions. In this sense +we may say that we can represent to ourselves the +fourth dimension. + +\Par{Conclusions.}---It is seen that experiment plays a +considerable rôle in the genesis of geometry; but +it would be a mistake to conclude from that that +geometry is, even in part, an experimental science. +If it were experimental, it would only be approximative +and provisory. And what a rough +approximation it would be! Geometry would be +only the study of the movements of solid bodies; +but, in reality, it is not concerned with natural +solids: its object is certain ideal solids, absolutely +invariable, which are but a greatly simplified and +very remote image of them. The concept of these +ideal bodies is entirely mental, and experiment is +but the opportunity which enables us to reach the +idea. The object of geometry is the study of a +particular ``group''; but the general concept of +group pre-exists in our minds, at least potentially. +It is imposed on us not as a form of our sensitiveness, +but as a form of our understanding; only, +from among all possible groups, we must choose +one that will be the \emph{standard}, so to speak, to +which we shall refer natural phenomena. + +Experiment guides us in this choice, which it +does not impose on us. It tells us not what is the +\PageSep{71} +truest, but what is the most convenient geometry. +It will be noticed that my description of these +fantastic worlds has required no language other +than that of ordinary geometry. Then, were we +transported to those worlds, there would be no +need to change that language. Beings educated +there would no doubt find it more convenient to +create a geometry different from ours, and better +adapted to their impressions; but as for us, in the +presence of the same impressions, it is certain that +we should not find it more convenient to make a +change. +\PageSep{72} + + +\Chapter{V.}{Experiment and Geometry.} + +\ParSkip1. I have on several occasions in the preceding +pages tried to show how the principles of geometry +are not experimental facts, and that in particular +Euclid's postulate cannot be proved by experiment. +However convincing the reasons already given +may appear to me, I feel I must dwell upon them, +because there is a profoundly false conception +deeply rooted in many minds. + +2. Think of a material circle, measure its radius +and circumference, and see if the ratio of the two +lengths is equal to~$\pi$. What have we done? We +have made an experiment on the properties of the +matter with which this \emph{roundness} has been realised, +and of which the measure we used is made. + +\Par[3.\ ]{Geometry and Astronomy.}---The same question +may also be asked in another way. If Lobatschewsky's +geometry is true, the parallax of a very +distant star will be finite. If Riemann's is true, it +will be negative. These are the results which +seem within the reach of experiment, and it is +hoped that astronomical observations may enable +%[** TN: "...les trois géométries" in the French edition] +us to decide between the \Reword{two}{three} geometries. But +\PageSep{73} +what we call a straight line in astronomy is simply +the path of a ray of light. If, therefore, we were +to discover negative parallaxes, or to prove that all +parallaxes are higher than a certain limit, we +should have a choice between two conclusions: +we could give up Euclidean geometry, or modify +the laws of optics, and suppose that light is not +rigorously propagated in a straight line. It is +needless to add that every one would look upon +this solution as the more advantageous. Euclidean +geometry, therefore, has nothing to fear from fresh +experiments. + +4. Can we maintain that certain phenomena +which are possible in Euclidean space would be +impossible in non-Euclidean space, so that experiment +in establishing these phenomena would +directly contradict the non-Euclidean hypothesis? +I think that such a question cannot be seriously +asked. To me it is exactly equivalent to the following, +the absurdity of which is obvious:---There +are lengths which can be expressed in metres and +centimetres, but cannot be measured in toises, feet, +and inches; so that experiment, by ascertaining the +existence of these lengths, would directly contradict +this hypothesis, that there are toises divided +into six feet. Let us look at the question a little +more closely. I assume that the straight line in +Euclidean space possesses any two properties, +which I shall call $A$~and~$B$; that in non-Euclidean +space it still possesses the property~$A$, but no +longer possesses the property~$B$; and, finally, I +\PageSep{74} +assume that in both Euclidean and non-Euclidean +space the straight line is the only line that possesses +the property~$A$. If this were so, experiment +would be able to decide between the hypotheses of +Euclid and Lobatschewsky. It would be found +that some concrete object, upon which we can +experiment---for example, a pencil of rays of light---possesses +the property~$A$. We should conclude +that it is rectilinear, and we should then endeavour +to find out if it does, or does not, possess the property~$B$. +But \emph{it is not so}. There exists no +property which can, like this property~$A$, be an +absolute criterion enabling us to recognise the +straight line, and to distinguish it from every +other line. Shall we say, for instance, ``This property +will be the following: the straight line is a +line such that a figure of which this line is a part +can move without the mutual distances of its +points varying, and in such a way that all the +points in this straight line remain fixed''? Now, +this is a property which in either Euclidean or +non-Euclidean space belongs to the straight line, +and belongs to it alone. But how can we ascertain +by experiment if it belongs to any particular +concrete object? Distances must be measured, +and how shall we know that any concrete magnitude +which I have measured with my material +instrument really represents the abstract distance? +We have only removed the difficulty a little farther +off. In reality, the property that I have just +enunciated is not a property of the straight line +\PageSep{75} +alone; it is a property of the straight line and of +distance. For it to serve as an absolute criterion, +we must be able to show, not only that it does not +also belong to any other line than the straight line +and to distance, but also that it does not belong +to any other line than the straight line, and to any +other magnitude than distance. Now, that is not +true, and if we are not convinced by these considerations, +I challenge any one to give me a +concrete experiment which can be interpreted in +the Euclidean system, and which cannot be interpreted +in the system of Lobatschewsky. As I +am well aware that this challenge will never be +accepted, I may conclude that no experiment will +ever be in contradiction with Euclid's postulate; +but, on the other hand, no experiment will ever be +in contradiction with Lobatschewsky's postulate. + +5. But it is not sufficient that the Euclidean +(or non-Euclidean) geometry can ever be directly +contradicted by experiment. Nor could it happen +that it can only agree with experiment by a violation +of the principle of sufficient reason, and of +that of the relativity of space. Let me explain +myself. Consider any material system whatever. +We have to consider on the one hand the ``state'' +of the various bodies of this system---for example, +their temperature, their electric potential,~etc.; +and on the other hand their position in space. +And among the data which enable us to define +this position we distinguish the mutual distances +of these bodies that define their relative positions, +\PageSep{76} +and the conditions which define the absolute position +of the system and its absolute orientation in +space. The law of the phenomena which will be +produced in this system will depend on the state +of these bodies, and on their mutual distances; +but because of the relativity and the inertia of +space, they will not depend on the absolute position +and orientation of the system. In other +words, the state of the bodies and their mutual +distances at any moment will solely depend on +the state of the same bodies and on their mutual +distances at the initial moment, but will in no +way depend on the absolute initial position of +the system and of its absolute initial orientation. +This is what we shall call, for the sake of +abbreviation, \emph{the law of relativity}. + +So far I have spoken as a Euclidean geometer. +But I have said that an experiment, whatever it +may be, requires an interpretation on the Euclidean +hypothesis; it equally requires one on the non-Euclidean +hypothesis. Well, we have made a series +of experiments. We have interpreted them on the +Euclidean hypothesis, and we have recognised +that these experiments thus interpreted do not +violate this ``law of relativity.'' We now interpret +them on the non-Euclidean hypothesis. This is +always possible, only the non-Euclidean distances +of our different bodies in this new interpretation +will not generally be the same as the Euclidean +distances in the primitive interpretation. Will +our experiment interpreted in this new manner +\PageSep{77} +be still in agreement with our ``law of relativity,'' +and if this agreement had not taken place, would +we not still have the right to say that experiment +has proved the falsity of non-Euclidean geometry? +It is easy to see that this is an idle fear. In fact, +to apply the law of relativity in all its rigour, it +must be applied to the entire universe; for if we +were to consider only a part of the universe, and +if the absolute position of this part were to vary, +the distances of the other bodies of the universe +would equally vary; their influence on the part of +the universe considered might therefore increase +or diminish, and this might modify the laws of +the phenomena which take place in it. But if +our system is the entire universe, experiment is +powerless to give us any opinion on its position +and its absolute orientation in space. All that +our instruments, however perfect they may be, +can let us know will be the state of the different +parts of the universe, and their mutual distances. +Hence, our law of relativity may be enunciated as +follows:---The readings that we can make with our +instruments at any given moment will depend +only on the readings that we were able to make +on the same instruments at the initial moment. +Now such an enunciation is independent of all +interpretation by experiments. If the law is true +in the Euclidean interpretation, it will be also true +in the non-Euclidean interpretation. Allow me +to make a short digression on this point. I have +spoken above of the data which define the position +\PageSep{78} +of the different bodies of the system. I might also +have spoken of those which define their velocities. +I should then have to distinguish the velocity with +which the mutual distances of the different bodies +are changing, and on the other hand the velocities +of translation and rotation of the system; that is +to say, the velocities with which its absolute position +and orientation are changing. For the mind +to be fully satisfied, the law of relativity would +have to be enunciated as follows:---The state of +bodies and their mutual distances at any given +moment, as well as the velocities with which +those distances are changing at that moment, +will depend only on the state of those bodies, +on their mutual distances at the initial moment, +and on the velocities with which those distances +were changing at the initial moment. But they +will not depend on the absolute initial position +of the system nor on its absolute orientation, nor +on the velocities with which that absolute position +and orientation were changing at the initial +moment. Unfortunately, the law thus enunciated +does not agree with experiments---at least, as they +are ordinarily interpreted. Suppose a man were +translated to a planet, the sky of which was constantly +covered with a thick curtain of clouds, so +that he could never see the other stars. On that +planet he would live as if it were isolated in space. +But he would notice that it revolves, either by +measuring its ellipticity (which is ordinarily done +by means of astronomical observations, but which +\PageSep{79} +could be done by purely geodesic means), or by +repeating the experiment of Foucault's pendulum. +The absolute rotation of this planet might be +clearly shown in this way. Now, here is a fact +which shocks the philosopher, but which the +physicist is compelled to accept. We know that +from this fact Newton concluded the existence of +absolute space. I myself cannot accept this way +of looking at it. I shall explain why in Part~III., +but for the moment it is not my intention to +discuss this difficulty. I must therefore resign +myself, in the enunciation of the law of relativity, +to including velocities of every kind among the +data which define the state of the bodies. However +that may be, the difficulty is the same for +both Euclid's geometry and for Lobatschewsky's. +I need not therefore trouble about it further, and +I have only mentioned it incidentally. To sum +up, whichever way we look at it, it is impossible +to discover in geometric empiricism a rational +meaning. + +6. Experiments only teach us the relations of +bodies to one another. They do not and cannot +give us the relations of bodies and space, nor the +mutual relations of the different parts of space. +``Yes!'' you reply, ``a single experiment is not +enough, because it only gives us one equation with +several unknowns; but when I have made enough +experiments I shall have enough equations to +calculate all my unknowns.'' If I know the height +of the main-mast, that is not sufficient to enable +\PageSep{80} +me to calculate the age of the captain. When +you have measured every fragment of wood in a +ship you will have many equations, but you will +be no nearer knowing the captain's age. All your +measurements bearing on your fragments of wood +can tell you only what concerns those fragments; +and similarly, your experiments, however numerous +they may be, referring only to the relations of +bodies with one another, will tell you nothing +about the mutual relations of the different parts +of space. + +7. Will you say that if the experiments have +reference to the bodies, they at least have reference +to the geometrical properties of the bodies. First, +what do you understand by the geometrical properties +of bodies? I assume that it is a question +of the relations of the bodies to space. These +properties therefore are not reached by experiments +which only have reference to the relations +of bodies to one another, and that is enough to +show that it is not of those properties that there +can be a question. Let us therefore begin by +making ourselves clear as to the sense of the +phrase: geometrical properties of bodies. When +I say that a body is composed of several parts, I +presume that I am thus enunciating a geometrical +property, and that will be true even if I agree to +give the improper name of points to the very +small parts I am considering. When I say that +this or that part of a certain body is in contact +with this or that part of another body, I am +\PageSep{81} +enunciating a proposition which concerns the +mutual relations of the two bodies, and not their +relations with space. I assume that you will +agree with me that these are not geometrical +properties. I am sure that at least you will +grant that these properties are independent of +all knowledge of metrical geometry. Admitting +this, I suppose that we have a solid body formed +of eight thin iron rods, $oa$, $ob$, $oc$, $od$, $oe$, $of$, $og$, $oh$, +connected at one of their extremities,~$o$. And let +us take a second solid body---for example, a piece +of wood, on which are marked three little spots +of ink which I shall call $\alpha\ \beta\ \gamma$. I now suppose +that we find that we can bring into contact $\Chg{\alpha\ \beta\ \gamma}{\alpha\beta\gamma}$ +with~$ago$; by that I mean $\alpha$~with~$a$, and at the +same time $\beta$~with~$g$, and $\gamma$~with~$o$. Then we can +successively bring into contact $\alpha\beta\gamma$ with $bgo$, $cgo$, +$dgo$, $ego$, $fgo$, then with $aho$, $bho$, $cho$, $dho$, $eho$, $fho$; +and then $\alpha\gamma$ successively with $ab$, $bc$, $cd$, $de$, $ef$, $fa$. +Now these are observations that can be made +without having any idea beforehand as to the +form or the metrical properties of space. They +have no reference whatever to the ``geometrical +properties of bodies.'' These observations will +not be possible if the bodies on which we experiment +move in a group having the same structure +as the Lobatschewskian group (I mean according +to the same laws as solid bodies in Lobatschewsky's +geometry). They therefore suffice to prove that +these bodies move according to the Euclidean +group; or at least that they do not move according +\PageSep{82} +to the Lobatschewskian group. That they may +be compatible with the Euclidean group is easily +seen; for we might make them so if the body~$\alpha\beta\gamma$ +were an invariable solid of our ordinary +geometry in the shape of a right-angled triangle, +and if the points $abcdefgh$ were the vertices of +a polyhedron formed of two regular hexagonal +pyramids of our ordinary geometry having $abcdef$ +as their common base, and having the one~$g$ and +the other~$h$ as their vertices. Suppose now, +instead of the previous observations, we note that +we can as before apply~$\alpha\beta\gamma$ successively to~$ago$, +$bgo$, $cgo$, $dgo$, $ego$, $fgo$, $aho$, $bho$, $cho$, $dho$, $eho$, $fho$, +and then that we can apply~$\alpha\beta$ (and no longer~$\alpha\gamma$) +successively to~$ab$, $bc$, $cd$, $de$, $ef$, and~$fa$. These are +observations that could be made if non-Euclidean +geometry were true. If the bodies~$\alpha\beta\gamma$, $oabcdefgh$ +were invariable solids, if the former were a right-angled +triangle, and the latter a double regular +hexagonal pyramid of suitable dimensions. These +new verifications are therefore impossible if the +bodies move according to the Euclidean group; +but they become possible if we suppose the bodies +to move according to the Lobatschewskian group. +They would therefore suffice to show, if we carried +them out, that the bodies in question do not move +according to the Euclidean group. And so, without +making any hypothesis on the form and the +nature of space, on the relations of the bodies +and space, and without attributing to bodies any +geometrical property, I have made observations +\PageSep{83} +which have enabled me to show in one case that +the bodies experimented upon move according to +a group, the structure of which is Euclidean, and +in the other case, that they move in a group, the +structure of which is Lobatschewskian. It cannot +be said that all the first observations would +constitute an experiment proving that space is +Euclidean, and the second an experiment proving +that space is non-Euclidean; in fact, it might be +imagined (note that I use the word \emph{imagined}) that +there are bodies moving in such a manner as +to render possible the second series of observations: +and the proof is that the first mechanic who came +our way could construct it if he would only take +the trouble. But you must not conclude, however, +that space is non-Euclidean. In the same way, +just as ordinary solid bodies would continue +to exist when the mechanic had constructed the +strange bodies I have just mentioned, he would +have to conclude that space is both Euclidean +and non-Euclidean. Suppose, for instance, that +we have a large sphere of radius~$R$, and that its +temperature decreases from the centre to the +surface of the sphere according to the law of +which I spoke when I was describing the non-Euclidean +world. We might have bodies whose +dilatation is \Typo{negligeable}{negligible}, and which would behave +as ordinary invariable solids; and, on the other +hand, we might have very dilatable bodies, which +would behave as non-Euclidean solids. We +might have two double pyramids~$oabcdefgh$ and +\PageSep{84} +$o'a'b'c'd'e'f'g'h'$, and two triangles $\alpha\beta\gamma$~and~$\alpha'\beta'\gamma'$. +The first double pyramid would be rectilinear, and +the second curvilinear. The triangle~$\alpha\beta\gamma$ would +consist of undilatable matter, and the other of very +dilatable matter. We might therefore make our +first observations with the double pyramid~$o'a'h'$ +and the triangle~$\alpha'\beta'\gamma'$. + +And then the experiment would seem to show---first, +that Euclidean geometry is true, and then +that it is false. Hence, \emph{experiments have reference +not to space but to bodies}. + +\Subsection{Supplement.} + +\ParSkip8. To round the matter off, I ought to speak of +a very delicate question, which will require considerable +development; but I shall confine myself +to summing up what I have written in the \Title{Revue +de Métaphysique et de Morale} and in the \Title{Monist}. +When we say that space has three dimensions, +what do we mean? We have seen the importance +of these ``internal changes'' which are revealed to +us by our muscular sensations. They may serve +to characterise the different attitudes of our body. +Let us take arbitrarily as our origin one of these +attitudes,~$A$. When we pass from this initial +attitude to another attitude~$B$ we experience a +series of muscular sensations, and this series~$S$ of +muscular sensations will define~$B$. Observe, however, +that we shall often look upon two series $S$~and~$S'$ +as defining the same attitude~$B$ (since the +\PageSep{85} +initial and final attitudes $A$~and~$B$ remaining the +same, the intermediary attitudes of the corresponding +sensations may differ). How then can +we recognise the equivalence of these two series? +Because they may serve to compensate for the same +external change, or more generally, because, when +it is a question of compensation for an external +change, one of the series may be replaced by the +other. Among these series we have distinguished +those which can alone compensate for an external +change, and which we have called ``displacements.'' +As we cannot distinguish two displacements which +are very close together, the aggregate of these +displacements presents the characteristics of a +physical continuum. Experience teaches us that +they are the characteristics of a physical continuum +of six dimensions; but we do not know as +yet how many dimensions space itself possesses, so +we must first of all answer another question. +What is a point in space? Every one thinks he +knows, but that is an illusion. What we see when +we try to represent to ourselves a point in space is +a black spot on white paper, a spot of chalk on +a blackboard, always an object. The question +should therefore be understood as follows:---What +do I mean when I say the object~$B$ is at the +point which a moment before was occupied by the +object~$A$? Again, what criterion will enable +me to recognise it? I mean that \emph{although I have +not moved} (my muscular sense tells me this), my +finger, which just now touched the object~$A$, is +\PageSep{86} +now touching the object~$B$. I might have used +other criteria---for instance, another finger or the +sense of sight---but the first criterion is sufficient. +I know that if it answers in the affirmative all +other criteria will give the same answer. I know +it from experiment. I cannot know it \Foreign{à~priori}. +For the same reason I say that touch cannot +be exercised at a distance; that is another way of +enunciating the same experimental fact. If I +say, on the contrary, that sight is exercised at a +distance, it means that the criterion furnished by +sight may give an affirmative answer while the +others reply in the negative. + +To sum up. For each attitude of my body my +finger determines a point, and it is that and that +only which defines a point in space. To each +attitude corresponds in this way a point. But it +often happens that the same point corresponds to +several different attitudes (in this case we say that +our finger has not moved, but the rest of our body +has). We distinguish, therefore, among changes +of attitude those in which the finger does not +move. How are we led to this? It is because we +often remark that in these changes the object +which is in touch with the finger remains in contact +with it. Let us arrange then in the same +class all the attitudes which are deduced one from +the other by one of the changes that we have thus +distinguished. To all these attitudes of the same +class will correspond the same point in space. +Then to each class will correspond a point, and to +\PageSep{87} +each point a class. Yet it may be said that what +we get from this experiment is not the point, but +the class of changes, or, better still, the corresponding +class of muscular sensations. Thus, when +we say that space has three dimensions, we merely +mean that the aggregate of these classes appears to +us with the characteristics of a physical continuum +of three dimensions. Then if, instead of defining +the points in space with the aid of the first finger, +I use, for example, another finger, would the +results be the same? That is by no means \Foreign{à~priori} +evident. But, as we have seen, experiment +has shown us that all our criteria are in agreement, +and this enables us to answer in the +affirmative. If we recur to what we have called +displacements, the aggregate of which forms, as +we have seen, a group, we shall be brought to +distinguish those in which a finger does not move; +and by what has preceded, those are the displacements +which characterise a point in space, and +their aggregate will form a sub-group of our +group. To each sub-group of this kind, then, will +correspond a point in space. We might be +tempted to conclude that experiment has taught +us the number of dimensions of space; but in +reality our experiments have referred not to space, +but to our body and its relations with neighbouring +objects. What is more, our experiments +are exceeding crude. In our mind the latent idea +of a certain number of groups pre-existed; these +are the groups with which Lie's theory is concerned. +\PageSep{88} +Which shall we choose to form a kind of +standard by which to compare natural phenomena? +And when this group is chosen, which +of the sub-groups shall we take to characterise a +point in space? Experiment has guided us by +showing us what choice adapts itself best to the +properties of our body; but there its rôle ends. +\PageSep{89} + + +\Part{III.}{Force.} + +\Chapter{VI.}{The Classical Mechanics.} + +\First{The} English teach mechanics as an experimental +science; on the Continent it is taught always more +or less as a deductive and \Foreign{à~priori} science. The +English are right, no doubt. How is it that the +other method has been persisted in for so long; how +is it that Continental scientists who have tried to +escape from the practice of their predecessors have +in most cases been unsuccessful? On the other +hand, if the principles of mechanics are only of +experimental origin, are they not merely approximate +and provisory? May we not be some day +compelled by new experiments to modify or even +to abandon them? These are the questions which +naturally arise, and the difficulty of solution is +largely due to the fact that treatises on mechanics +do not clearly distinguish between what is experiment, +what is mathematical reasoning, what is +convention, and what is hypothesis. This is not +all. +\PageSep{90} + +1. There is no absolute space, and we only +conceive of relative motion; and yet in most cases +mechanical facts are enunciated as if there is an +absolute space to which they can be referred. + +2. There is no absolute time. When we say that +two periods are equal, the statement has no +meaning, and can only acquire a meaning by a +convention. + +3. Not only have we no direct intuition of the +equality of two periods, but we have not even +direct intuition of the simultaneity of two events +occurring in two different places. I have explained +this in an article entitled ``Mesure du +Temps.''\footnote + {\Title{Revue de Métaphysique et de Morale}, t.~vi., pp.~1--13, January, + 1898.} + +4. Finally, is not our Euclidean geometry in +itself only a kind of convention of language? +Mechanical facts might be enunciated with reference +to a non-Euclidean space which would be +less convenient but quite as legitimate as our +ordinary space; the enunciation would become +more complicated, but it still would be possible. + +Thus, absolute space, absolute time, and even +geometry are not conditions which are imposed on +mechanics. All these things no more existed +before mechanics than the French language can +be logically said to have existed before the truths +which are expressed in French. We might +endeavour to enunciate the fundamental law of +mechanics in a language independent of all these +\PageSep{91} +conventions; and no doubt we should in this way +get a clearer idea of those laws in themselves. +This is what M.~Andrade has tried to do, to +some extent at any rate, in his \Title{Leçons de Mécanique +physique}. Of course the enunciation of these laws +would become much more complicated, because all +these conventions have been adopted for the very +purpose of abbreviating and simplifying the enunciation. +As far as we are concerned, I shall ignore +all these difficulties; not because I disregard +them, far from it; but because they have received +sufficient attention in the first two parts, +of the book. Provisionally, then, we shall admit +absolute time and Euclidean geometry. + +\Par{The Principle of Inertia.}---A body under the +action of no force can only move uniformly in a +straight line. Is this a truth imposed on the mind +\Foreign{à~priori}? If this be so, how is it that the Greeks +ignored it? How could they have believed that +motion ceases with the cause of motion? or, again, +that every body, if there is nothing to prevent it, +will move in a circle, the noblest of all forms of +motion? + +If it be said that the velocity of a body cannot +change, if there is no reason for it to change, may +we not just as legitimately maintain that the +position of a body cannot change, or that the +curvature of its path cannot change, without the +agency of an external cause? Is, then, the principle +of inertia, which is not an \Foreign{à~priori} truth, an +experimental fact? Have there ever been experiments +\PageSep{92} +on bodies acted on by no forces? and, if so, +how did we know that no forces were acting? +The usual instance is that of a ball rolling for a +very long time on a marble table; but why do +we say it is under the action of no force? Is it +because it is too remote from all other bodies to +experience any sensible action? It is not further +from the earth than if it were thrown freely into +the air; and we all know that in that case it +would be subject to the attraction of the earth. +Teachers of mechanics usually pass rapidly over +the example of the ball, but they add that the +principle of inertia is verified indirectly by its consequences. +This is very badly expressed; they +evidently mean that various consequences may be +verified by a more general principle, of which the +principle of inertia is only a particular case. I +shall propose for this general principle the +following enunciation:---The acceleration of a +body depends only on its position and that of +neighbouring bodies, and on their velocities. +Mathematicians would say that the movements +of all the material molecules of the universe +depend on differential equations of the second +order. To make it clear that this is really a +generalisation of the law of inertia we may again +have recourse to our imagination. The law of +inertia, as I have said above, is not imposed on us +\Foreign{à~priori}; other laws would be just as compatible +with the principle of sufficient reason. If a body +is not acted upon by a force, instead of supposing +\PageSep{93} +that its velocity is unchanged we may suppose +that its position or its acceleration is unchanged. + +Let us for a moment suppose that one of these +two laws is a law of nature, and substitute it for +the law of inertia: what will be the natural +generalisation? A moment's reflection will show +us. In the first case, we may suppose that the +velocity of a body depends only on its position and +that of neighbouring bodies; in the second case, +that the variation of the acceleration of a body +depends only on the position of the body and of +neighbouring bodies, on their velocities and +accelerations; or, in mathematical terms, the +differential equations of the motion would be of +the first order in the first case and of the third +order in the second. + +Let us now modify our supposition a little. +Suppose a world analogous to our solar system, +but one in which by a singular chance the orbits +of all the planets have neither eccentricity nor +inclination; and further, I suppose that the +masses of the planets are too small for their +mutual perturbations to be sensible. Astronomers +living in one of these planets would not hesitate to +conclude that the orbit of a star can only be +circular and parallel to a certain plane; the +position of a star at a given moment would then +be sufficient to determine its velocity and path. +The law of inertia which they would adopt would +be the former of the two hypothetical laws I have +mentioned. +\PageSep{94} + +Now, imagine this system to be some day +crossed by a body of vast mass and immense +velocity coming from distant constellations. All +the orbits would be profoundly disturbed. Our +astronomers would not be greatly astonished. +They would guess that this new star is in itself +quite capable of doing all the mischief; but, they +would say, as soon as it has passed by, order will +again be established. No doubt the distances of +the planets from the sun will not be the same as +before the cataclysm, but the orbits will become +circular again as soon as the disturbing cause has +disappeared. It would be only when the perturbing +body is remote, and when the orbits, instead of +being circular are found to be elliptical, that the +astronomers would find out their mistake, and +discover the necessity of reconstructing their +mechanics. + +I have dwelt on these hypotheses, for it seems to +me that we can clearly understand our generalised +law of inertia only by opposing it to a contrary +hypothesis. + +Has this generalised law of inertia been verified +by experiment, and can it be so verified? +When Newton wrote the \Title{Principia}, he certainly +regarded this truth as experimentally acquired and +demonstrated. It was so in his eyes, not only +from the anthropomorphic conception to which I +shall later refer, but also because of the work of +Galileo. It was so proved by the laws of Kepler. +According to those laws, in fact, the path of a +\PageSep{95} +planet is entirely determined by its initial position +and initial velocity; this, indeed, is what our +generalised law of inertia requires. + +For this principle to be only true in appearance---lest +we should fear that some day it must be replaced +by one of the analogous principles which I +opposed to it just now---we must have been led +astray by some amazing chance such as that which +had led into error our imaginary astronomers. +Such an hypothesis is so unlikely that it need not +delay us. No one will believe that there can be +such chances; no doubt the probability that two +eccentricities are both exactly zero is not smaller +than the probability that one is~$0.1$ and the other~$0.2$. +The probability of a simple event is not +smaller than that of a complex one. If, however, +the former does occur, we shall not attribute its +occurrence to chance; we shall not be inclined to +believe that nature has done it deliberately to +deceive us. The hypothesis of an error of this +kind being discarded, we may admit that so far as +astronomy is concerned our law has been verified +by experiment. + +But Astronomy is not the whole of Physics. +May we not fear that some day a new experiment +will falsify the law in some domain of +physics? An experimental law is always subject +to revision; we may always expect to see it replaced +by some other and more exact law. But +no one seriously thinks that the law of which we +speak will ever be abandoned or amended. Why? +\PageSep{96} +Precisely because it will never be submitted to a +decisive test. + +In the first place, for this test to be complete, +all the bodies of the universe must return with +their initial velocities to their initial positions after +a certain time. We ought then to find that they +would resume their original paths. But this test +is impossible; it can be only partially applied, and +even when it is applied there will still be some +bodies which will not return to their original +positions. Thus there will be a ready explanation +of any breaking down of the law. + +Yet this is not all. In Astronomy we \emph{see} the +bodies whose motion we are studying, and in most +cases we grant that they are not subject to the +action of other invisible bodies. Under these conditions, +our law must certainly be either verified or +not. But it is not so in Physics. If physical +phenomena are due to motion, it is to the motion +of molecules which we cannot see. If, then, the +acceleration of bodies we cannot see depends on +something else than the positions or velocities of +other visible bodies or of invisible molecules, the +existence of which we have been led previously +to admit, there is nothing to prevent us from +supposing that this something else is the position +or velocity of other molecules of which we have +not so far suspected the existence. The law +will be safeguarded. Let me express the same +thought in another form in mathematical language. +Suppose we are observing $n$~molecules, and find +\PageSep{97} +that their $3n$~co-ordinates satisfy a system of $3n$~differential +equations of the fourth order (and +not of the second, as required by the law of +inertia). We know that by introducing $3n$~variable +auxiliaries, a system of $3n$~equations of the fourth +order may be reduced to a system of $6n$~equations +of the second order. If, then, we suppose that the +$3n$~auxiliary variables represent the co-ordinates of +$n$~invisible molecules, the result is again conformable +to the law of inertia. To sum up, this law, +verified experimentally in some particular cases, +may be extended fearlessly to the most general +cases; for we know that in these general cases +it can neither be confirmed nor contradicted by +experiment. + +\Par{The Law of Acceleration.}---The acceleration of a +body is equal to the force which acts on it divided +by its mass. + +Can this law be verified by experiment? If so, +we have to measure the three magnitudes mentioned +in the enunciation: acceleration, force, +and mass. I admit that acceleration may be +measured, because I pass over the difficulty +arising from the measurement of time. But how +are we to measure force and mass? We do not +even know what they are. What is mass? +Newton replies: ``The product of the volume and +the density.'' ``It were better to say,'' answer +Thomson and Tait, ``that density is the quotient +of the mass by the volume.'' What is force? +``It is,'' replies Lagrange, ``that which moves or +\PageSep{98} +tends to move a body.'' ``It is,'' according to +Kirchoff, ``the product of the mass and the +acceleration.'' Then why not say that mass is +the quotient of the force by the acceleration? +These difficulties are insurmountable. + +When we say force is the cause of motion, we +are talking metaphysics; and this definition, if we +had to be content with it, would be absolutely +fruitless, would lead to absolutely nothing. For a +definition to be of any use it must tell us how to +measure force; and that is quite sufficient, for it is +by no means necessary to tell what force is in +itself, nor whether it is the cause or the effect of +motion. We must therefore first define what is +meant by the equality of two forces. When are +two forces equal? We are told that it is when +they give the same acceleration to the same mass, +or when acting in opposite directions they are in +equilibrium. This definition is a sham. A force +applied to a body cannot be uncoupled and +applied to another body as an engine is uncoupled +from one train and coupled to another. It is +therefore impossible to say what acceleration such +a force, applied to such a body, would give to +another body if it were applied to it. It is impossible +to tell how two forces which are not +acting in exactly opposite directions would behave +if they were acting in opposite directions. +It is this definition which we try to materialise, as +it were, when we measure a force with a dynamometer +or with a balance. Two forces, $F$~and~$F'$, +\PageSep{99} +which I suppose, for simplicity, to be acting +vertically upwards, are respectively applied to two +bodies, $C$~and~$C'$. I attach a body weighing~$P$ +first to~$C$ and then to~$C'$; if there is equilibrium in +both cases I conclude that the two forces $F$~and~$F'$ +are equal, for they are both equal to the weight +of the body~$P$. But am I certain that the body~$P$ +has kept its weight when I transferred it from the +first body to the second? Far from it. I am +certain of the contrary. I know that the magnitude +of the weight varies from one point to +another, and that it is greater, for instance, at the +pole than at the equator. No doubt the difference +is very small, and we neglect it in practice; but a +definition must have mathematical rigour; this +rigour does not exist. What I say of weight +would apply equally to the force of the spring of +a dynamometer, which would vary according to +temperature and many other circumstances. Nor +is this all. We cannot say that the weight of the +body~$P$ is applied to the body~$C$ and keeps in +equilibrium the force~$F$. What is applied to +the body~$C$ is the action of the body~$P$ on the +body~$C$. On the other hand, the body~$P$ is +acted on by its weight, and by the reaction~$R$ +of the body~$C$ on~$P$ the forces $F$~and~$A$ are +equal, because they are in equilibrium; the forces +$A$~and~$R$ are equal by virtue of the principle +of action and reaction; and finally, the force~$R$ +and the weight~$P$ are equal because they +are in equilibrium. From these three equalities +\PageSep{100} +we deduce the equality of the weight~$P$ and the +force~$F$. + +Thus we are compelled to bring into our definition +of the equality of two forces the principle +of the equality of action and reaction; \emph{hence this +principle can no longer be regarded as an experimental +law but only as a definition}. + +To recognise the equality of two forces we are +then in possession of two rules: the equality of +two forces in equilibrium and the equality of action +and reaction. But, as we have seen, these are not +sufficient, and we are compelled to have recourse +to a third rule, and to admit that certain forces---the +weight of a body, for instance---are constant in +magnitude and direction. But this third rule is +an experimental law. It is only approximately +true: \emph{it is a bad definition}. We are therefore +reduced to Kirchoff's definition: force is the product +of the mass and the acceleration. This law +of Newton in its turn ceases to be regarded as an +experimental law, it is now only a definition. But +as a definition it is insufficient, for we do not +know what mass is. It enables us, no doubt, to +calculate the ratio of two forces applied at +different times to the same body, but it tells us +nothing about the ratio of two forces applied to +two different bodies. To fill up the gap we must +have recourse to Newton's third law, the equality +of action and reaction, still regarded not as +an experimental law but as a definition. Two +bodies, $A$~and~$B$, act on each other; the acceleration +\PageSep{101} +of~$A$, multiplied by the mass of~$A$, is equal to +the action of~$B$ on~$A$; in the same way the +acceleration of~$B$, multiplied by the mass of~$B$ is +equal to the reaction of~$A$ on~$B$. As, by definition, +the action and the reaction are equal, the masses +of $A$~and~$B$ arc respectively in the inverse ratio of +their masses. Thus is the ratio of the two masses +defined, and it is for experiment to verify that the +ratio is constant. + +This would do very well if the two bodies were +alone and could be abstracted from the action of +the rest of the world; but this is by no means +the case. The acceleration of~$A$ is not solely due +to the action of~$B$, but to that of a multitude of +other bodies, $C$,~$D$,~\ldots. To apply the preceding +rule we must decompose the acceleration of~$A$ into +many components, and find out which of these +components is due to the action of~$B$. The +decomposition would still be possible if we +suppose that the action of~$C$ on~$A$ is simply added +to that of~$B$ on~$A$, and that the presence of the +body~$C$ does not in any way modify the action of~$B$ +on~$A$, or that the presence of~$B$ does not modify +the action of~$C$ on~$A$; that is, if we admit that +any two bodies attract each other, that their +mutual action is along their join, and is only dependent +on their distance apart; if, in a word, we +admit the \emph{hypothesis of central forces}. + +We know that to determine the masses of the +heavenly bodies we adopt quite a different principle. +The law of gravitation teaches us that the +\PageSep{102} +attraction of two bodies is proportional to their +masses; if $r$~is their distance apart, $m$~and~$m'$ their +masses, $k$~a constant, then their attraction will be~$kmm'/r^{2}$. +What we are measuring is therefore not +mass, the ratio of the force to the acceleration, but +the attracting mass; not the inertia of the body, +but its attracting power. It is an indirect process, +the use of which is not indispensable theoretically. +We might have said that the attraction is inversely +proportional to the square of the distance, +without being proportional to the product of the +%[** TN: "mais sans que l'on eût f = kmm'"] +masses, that it is equal to~$f/r^{2}$ \Reword{and not to~$kmm'$}{but without having $f = kmm'$}. +If it were so, we should nevertheless, by observing +the \emph{relative} motion of the celestial bodies, be able +to calculate the masses of these bodies. + +But have we any right to admit the hypothesis +of central forces? Is this hypothesis rigorously +accurate? Is it certain that it will never be +falsified by experiment? Who will venture to +make such an assertion? And if we must abandon +this hypothesis, the building which has been so +laboriously erected must fall to the ground. + +We have no longer any right to speak of the +component of the acceleration of~$A$ which is +due to the action of~$B$. We have no means of +distinguishing it from that which is due to the +action of~$C$ or of any other body. The rule +becomes inapplicable in the measurement of +masses. What then is left of the principle of +the equality of action and reaction? If we +reject the hypothesis of central forces this principle +\PageSep{103} +must go too; the geometrical resultant of +all the forces applied to the different bodies of a +system abstracted from all external action will be +zero. In other words, \emph{the motion of the centre of +gravity of this system will be uniform and in a +straight line}. Here would seem to be a means of +defining mass. The position of the centre of +gravity evidently depends on the values given to +the masses; we must select these values so that +the motion of the centre of gravity is uniform +and rectilinear. This will always be possible if +Newton's third law holds good, and it will be in +general possible only in one way. But no system +exists which is abstracted from all external action; +every part of the universe is subject, more or less, +to the action of the other parts. \emph{The law of the +motion of the centre of gravity is only rigorously true +when applied to the whole universe.} + +But then, to obtain the values of the masses +we must find the motion of the centre of gravity +of the universe. The absurdity of this conclusion +is obvious; the motion of the centre of gravity +of the universe will be for ever to us unknown. +Nothing, therefore, is left, and our efforts are +fruitless. There is no escape from the following +definition, which is only a confession of failure: +\emph{Masses are co-efficients which it is found convenient to +introduce into calculations.} + +We could reconstruct our mechanics by giving +to our masses different values. The new mechanics +would be in contradiction neither with +\PageSep{104} +experiment nor with the general principles of +dynamics (the principle of inertia, proportionality +of masses and accelerations, equality of +action and reaction, uniform motion of the centre +of gravity in a straight line, and areas). But the +equations of this mechanics \emph{would not be so simple}. +Let us clearly understand this. It would be only +the first terms which would be less simple---\ie, +those we already know through experiment; +perhaps the small masses could be slightly altered +without the \emph{complete} equations gaining or losing +in simplicity. + +Hertz has inquired if the principles of mechanics +are rigorously true. ``In the opinion of many +physicists it seems inconceivable that experiment +will ever alter the impregnable principles of +mechanics; and yet, what is due to experiment +may always be rectified by experiment.'' From +what we have just seen these fears would appear +to be groundless. The principles of dynamics +appeared to us first as experimental truths, but +we have been compelled to use them as definitions. +It is \emph{by definition} that force is equal to +the product of the mass and the acceleration; +this is a principle which is henceforth beyond +the reach of any future experiment. Thus +it is by definition that action and reaction are +equal and opposite. But then it will be said, +these unverifiable principles are absolutely devoid +of any significance. They cannot be disproved by +experiment, but we can learn from them nothing +\PageSep{105} +of any use to us; what then is the use of studying +dynamics? This somewhat rapid condemnation +would be rather unfair. There is not in Nature any +system \emph{perfectly} isolated, perfectly abstracted from +all external action; but there are systems which +are \emph{nearly} isolated. If we observe such a system, +we can study not only the relative motion of its +different parts with respect to each other, but the +motion of its centre of gravity with respect to the +other parts of the universe. We then find that +the motion of its centre of gravity is \emph{nearly} uniform +and rectilinear in conformity with Newton's Third +Law. This is an experimental fact, which cannot +be invalidated by a more accurate experiment. +What, in fact, would a more accurate experiment +teach us? It would teach us that the law is only +approximately true, and we know that already. +\emph{Thus is explained how experiment may serve as a basis +for the principles of mechanics, and yet will never +invalidate them.} + +\Par{Anthropomorphic Mechanics.}---It will be said that +Kirchoff has only followed the general tendency of +mathematicians towards nominalism; from this his +skill as a physicist has not saved him. He wanted +a definition of a force, and he took the first that +came handy; but we do not require a definition +of force; the idea of force is primitive, irreducible, +indefinable; we all know what it is; of it we have +direct intuition. This direct intuition arises from +the idea of effort which is familiar to us from +childhood. But in the first place, even if this +\PageSep{106} +direct intuition made known to us the real nature +of force in itself, it would prove to be an insufficient +basis for mechanics; it would, moreover, be quite +useless. The important thing is not to know +what force is, but how to measure it. Everything +which does not teach us how to measure it is as +useless to the mechanician as, for instance, the +subjective idea of heat and cold to the student of +heat. This subjective idea cannot be translated +into numbers, and is therefore useless; a scientist +whose skin is an absolutely bad conductor of heat, +and who, therefore, has never felt the sensation +of heat or cold, would read a thermometer in just +the same way as any one else, and would have +enough material to construct the whole of the +theory of heat. + +Now this immediate notion of effort is of no use +to us in the measurement of force. It is clear, for +example, that I shall experience more fatigue in +lifting a weight of $100$~lb.\ than a man who is +accustomed to lifting heavy burdens. But there +is more than this. This notion of effort does not +teach us the nature of force; it is definitively reduced +to a recollection of muscular sensations, and +no one will maintain that the sun experiences +a muscular sensation when it attracts the earth. +All that we can expect to find from it is a symbol, +less precise and less convenient than the arrows +(to denote direction) used by geometers, and quite +as remote from reality. + +Anthropomorphism plays a considerable historic +\PageSep{107} +rôle in the genesis of mechanics; perhaps it may +yet furnish us with a symbol which some minds +may find convenient; but it can be the foundation +of nothing of a really scientific or philosophical +character. + +\Par{The Thread School.}---M.~Andrade, in his \Title{Leçons +de \Typo{Mecanique}{Mécanique} physique}, has modernised anthropomorphic +mechanics. To the school of mechanics +with which Kirchoff is identified, he opposes a +school which is quaintly called the ``Thread +School.'' + +This school tries to reduce everything to the consideration +of certain material systems of negligible +mass, regarded in a state of tension and capable +of transmitting considerable effort to distant +bodies---systems of which the ideal type is the +fine string, wire, or \emph{thread}. A thread which +transmits any force is slightly lengthened in the +direction of that force; the direction of the thread +tells us the direction of the force, and the magnitude +of the force is measured by the lengthening of +the thread. + +%[** TN: "A" variously italicized and not in the original] +{\Loosen We may imagine such an experiment as the +following:}---A body~$A$ is attached to a thread; +at the other extremity of the thread acts a force +which is made to vary until the length of the +thread is increased by~$\alpha$, and the acceleration +of the body~$A$ is recorded. $A$~is then detached, +and a body~$B$ is attached to the same thread, and +the same or another force is made to act until +the increment of length again is~$\alpha$, and the +\PageSep{108} +acceleration of~$B$ is noted. The experiment is +then renewed with both $A$~and~$B$ until the increment +of length is~$\beta$. The four accelerations +observed should be proportional. Here we have +an experimental verification of the law of acceleration +enunciated above. Again, we may consider +a body under the action of several threads in +equal tension, and by experiment we determine +the direction of those threads when the body +is in equilibrium. This is an experimental +verification of the law of the composition of +forces. But, as a matter of fact, what have we +done? We have defined the force acting on the +string by the deformation of the thread, which is +reasonable enough; we have then assumed that if +a body is attached to this thread, the effort which +is transmitted to it by the thread is equal to the +action exercised by the body on the thread; in +fact, we have used the principle of action and +reaction by considering it, not as an experimental +truth, but as the very definition of force. This +definition is quite as conventional as that of +Kirchoff, but it is much less general. + +All the forces are not transmitted by the thread +(and to compare them they would all have to be +transmitted by identical threads). If we even +admitted that the earth is attached to the sun by +an invisible thread, at any rate it will be agreed +that we have no means of measuring the increment +of the thread. Nine times out of ten, in consequence, +our definition will be in default; no +\PageSep{109} +sense of any kind can be attached to it, and we +must fall back on that of Kirchoff. Why then go +on in this roundabout way? You admit a certain +definition of force which has a meaning only in +certain particular cases. In those cases you verify +by experiment that it leads to the law of acceleration. +On the strength of these experiments you +then take the law of acceleration as a definition of +force in all the other cases. + +Would it not be simpler to consider the law of +acceleration as a definition in all cases, and to +regard the experiments in question, not as verifications +of that law, but as verifications of the +principle of action and reaction, or as proving +the deformations of an elastic body depend only +on the forces acting on that body? Without +taking into account the fact that the conditions +in which your definition could be accepted can +only be very imperfectly fulfilled, that a thread is +never without mass, that it is never isolated from +all other forces than the reaction of the bodies +attached to its extremities. + +The ideas expounded by M.~Andrade are none +the less very interesting. If they do not satisfy our +logical requirements, they give us a better view of +the historical genesis of the fundamental ideas of +mechanics. The reflections they suggest show us +how the human mind passed from a naïve +anthropomorphism to the present conception of +science. + +We see that we end with an experiment which +\PageSep{110} +is very particular, and as a matter of fact very +crude, and we start with a perfectly general law, +perfectly precise, the truth of which we regard as +absolute. We have, so to speak, freely conferred +this certainty on it by looking upon it as a convention. + +Are the laws of acceleration and of the composition +of forces only arbitrary conventions? +Conventions, yes; arbitrary, no---they would be +so if we lost sight of the experiments which led the +founders of the science to adopt them, and which, +imperfect as they were, were sufficient to justify +their adoption. It is well from time to time to let +our attention dwell on the experimental origin of +these conventions. +\PageSep{111} + + +\Chapter{VII.}{Relative and Absolute Motion.} + +\Par{The Principle of Relative Motion.}---Sometimes +endeavours have been made to connect the law of +acceleration with a more general principle. The +movement of any system whatever ought to +obey the same laws, whether it is referred to fixed +axes or to the movable axes which are implied +in uniform motion in a straight line. This is +the principle of relative motion; it is imposed +upon us for two reasons: the commonest experiment +confirms it; the consideration of the contrary +hypothesis is singularly repugnant to the mind. + +Let us admit it then, and consider a body under +the action of a force. The relative motion of this +body with respect to an observer moving with a +uniform velocity equal to the initial velocity of the +body, should be identical with what would be its +absolute motion if it started from rest. We conclude +that its acceleration must not depend upon +its absolute velocity, and from that we attempt to +deduce the complete law of acceleration. + +For a long time there have been traces of this +proof in the regulations for the degree of B.~ès~Sc. +\PageSep{112} +It is clear that the attempt has failed. The +obstacle which prevented us from proving the +law of acceleration is that we have no definition +of force. This obstacle subsists in its entirety, +since the principle invoked has not furnished us +with the missing definition. The principle of +relative motion is none the less very interesting, +and deserves to be considered for its own sake. +Let us try to enunciate it in an accurate manner. +We have said above that the accelerations of the +different bodies which form part of an isolated +system only depend on their velocities and their +relative positions, and not on their velocities and +their absolute positions, provided that the movable +axes to which the relative motion is referred +move uniformly in a straight line; or, if it is preferred, +their accelerations depend only on the +differences of their velocities and the differences of +their co-ordinates, and not on the absolute values +of these velocities and co-ordinates. If this principle +is true for relative accelerations, or rather +for differences of acceleration, by combining it +with the law of reaction we shall deduce that it is +true for absolute accelerations. It remains to be +seen how we can prove that differences of acceleration +depend only on differences of velocities +and co-ordinates; or, to speak in mathematical +language, that these differences of co-ordinates +satisfy differential equations of the second order. +Can this proof be deduced from experiment or +from \Foreign{à~priori} conditions? Remembering what we +\PageSep{113} +have said before, the reader will give his own +answer. Thus enunciated, in fact, the principle of +relative motion curiously resembles what I called +above the generalised principle of inertia; it is not +quite the same thing, since it is a question of +differences of co-ordinates, and not of the co-ordinates +themselves. The new principle teaches +us something more than the old, but the same +discussion applies to it, and would lead to the +same conclusions. We need not recur to it. + +\Par{Newton's Argument.}---Here we find a very important +and even slightly disturbing question. I +have said that the principle of relative motion +was not for us simply a result of experiment; and +that \Foreign{à~priori} every contrary hypothesis would be +repugnant to the mind. But, then, why is the +principle only true if the motion of the movable +axes is uniform and in a straight line? It seems +that it should be imposed upon us with the same +force if the motion is accelerated, or at any rate +if it reduces to a uniform rotation. In these two +cases, in fact, the principle is not true. I need not +dwell on the case in which the motion of the +axes is in a straight line and not uniform. The +paradox does not bear a moment's examination. +If I am in a railway carriage, and if the train, +striking against any obstacle whatever, is suddenly +stopped, I shall be projected on to the opposite +side, although I have not been directly acted upon +by any force. There is nothing mysterious in +that, and if I have not been subject to the action +\PageSep{114} +of any external force, the train has experienced an +external impact. There can be nothing paradoxical +in the relative motion of two bodies being +disturbed when the motion of one or the other is +modified by an external cause. Nor need I dwell +on the case of relative motion referring to axes +which rotate uniformly. If the sky were for ever +covered with clouds, and if we had no means of +observing the stars, we might, nevertheless, conclude +that the earth turns round. We should be +warned of this fact by the flattening at the poles, +or by the experiment of Foucault's pendulum. +And yet, would there in this case be any meaning +in saying that the earth turns round? If there is +no absolute space, can a thing turn without turning +with respect to something; and, on the other +hand, how can we admit Newton's conclusion and +believe in absolute space? But it is not sufficient +to state that all possible solutions are equally +unpleasant to us. We must analyse in each case +the reason of our dislike, in order to make our +choice with the knowledge of the cause. The +long discussion which follows must, therefore, be +excused. + +Let us resume our imaginary story. Thick +clouds hide the stars from men who cannot observe +them, and even are ignorant of their existence. +How will those men know that the earth turns +round? No doubt, for a longer period than did +our ancestors, they will regard the soil on which +they stand as fixed and immovable! They will +\PageSep{115} +wait a much longer time than we did for the +coming of a Copernicus; but this Copernicus will +come at last. How will he come? In the first +place, the mechanical school of this world would +not run their heads against an absolute contradiction. +In the theory of relative motion we observe, +besides real forces, two imaginary forces, which +we call ordinary centrifugal force and compounded +centrifugal force. Our imaginary scientists can +thus explain everything by looking upon these two +forces as real, and they would not see in this a +contradiction of the generalised principle of inertia, +for these forces would depend, the one on the +relative positions of the different parts of the +system, such as real attractions, and the other on +their relative velocities, as in the case of real +frictions. Many difficulties, however, would before +long awaken their attention. If they succeeded in +realising an isolated system, the centre of gravity +of this system would not have an approximately +rectilinear path. They could invoke, to explain +this fact, the centrifugal forces which they would +regard as real, and which, no doubt, they would +attribute to the mutual actions of the bodies---only +they would not see these forces vanish at great +distances---that is to say, in proportion as the +isolation is better realised. Far from it. Centrifugal +force increases indefinitely with distance. +Already this difficulty would seem to them sufficiently +serious, but it would not detain them for +long. They would soon imagine some very subtle +\PageSep{116} +medium analogous to our ether, in which all +bodies would be bathed, and which would exercise +on them a repulsive action. But that is not +all. Space is symmetrical---yet the laws of +motion would present no symmetry. They should +be able to distinguish between right and left. +They would see, for instance, that cyclones always +turn in the same direction, while for reasons of +symmetry they should turn indifferently in any +direction. If our scientists were able by dint of +much hard work to make their universe perfectly +symmetrical, this symmetry would not subsist, +although there is no apparent reason why it +should be disturbed in one direction more than +in another. They would extract this from the +situation no doubt---they would invent something +which would not be more extraordinary than the +glass spheres of Ptolemy, and would thus go on +accumulating complications until the long-expected +Copernicus would sweep them all away +with a single blow, saying it is much more simple +to admit that the earth turns round. Just as +our Copernicus said to us: ``It is more convenient +to suppose that the earth turns round, because the +laws of astronomy are thus expressed in a more +simple language,'' so he would say to them: ``It +is more convenient to suppose that the earth turns +round, because the laws of mechanics are thus +expressed in much more simple language.\Add{''} That +does not prevent absolute space---that is to say, +the point to which we must refer the earth to +\PageSep{117} +know if it really does turn round---from having +no objective existence. And hence this affirmation: +``the earth turns round,'' has no meaning, +since it cannot be verified by experiment; since +such an experiment not only cannot be realised or +even dreamed of by the most daring Jules Verne, +but cannot even be conceived of without contradiction; +or, in other words, these two propositions, +``the earth turns round,'' and, ``it is more +convenient to suppose that the earth turns round,'' +have one and the same meaning. There is nothing +more in one than in the other. Perhaps they will +not be content with this, and may find it surprising +that among all the hypotheses, or rather all +the conventions, that can be made on this subject +there is one which is more convenient than the +rest? But if we have admitted it without difficulty +when it is a question of the laws of +astronomy, why should we object when it is a +question of the laws of mechanics? We have +seen that the co-ordinates of bodies are determined +by differential equations of the second +order, and that so are the differences of these +co-ordinates. This is what we have called the +generalised principle of inertia, and the principle +of relative motion. If the distances of these +bodies were determined in the same way by +equations of the second order, it seems that the +mind should be entirely satisfied. How far does +the mind receive this satisfaction, and why is it +not content with it? To explain this we had +\PageSep{118} +better take a simple example. I assume a system +analogous to our solar system, but in which fixed +stars foreign to this system cannot be perceived, +so that astronomers can only observe the mutual +distances of planets and the sun, and not the +absolute longitudes of the planets. If we deduce +directly from Newton's law the differential equations +which define the variation of these distances, +these equations will not be of the second order. I +mean that if, outside Newton's law, we knew the +initial values of these distances and of their derivatives +with respect to time---that would not be +sufficient to determine the values of these same +distances at an ulterior moment. A datum would +be still lacking, and this datum might be, for +example, what astronomers call the area-constant. +But here we may look at it from two different +points of view. We may consider two kinds of +constants. In the eyes of the physicist the world +reduces to a series of phenomena depending, on the +one hand, solely on initial phenomena, and, on the +other hand, on the laws connecting consequence +and antecedent. If observation then teaches us +that a certain quantity is a constant, we shall have +a choice of two ways of looking at it. So let us +admit that there is a law which requires that this +quantity shall not vary, but that by chance it has +been found to have had in the beginning of time +this value rather than that, a value that it has +kept ever since. This quantity might then be +called an \emph{accidental} constant. Or again, let us +\PageSep{119} +admit on the contrary that there is a law of nature +which imposes on this quantity this value and not +that. We shall then have what may be called an +\emph{essential} constant. For example, in virtue of the +laws of Newton the duration of the revolution of +the earth must be constant. But if it is $366$~and +something sidereal days, and not $300$~or~$400$, it is +because of some initial chance or other. It is an +\emph{accidental} constant. If, on the other hand, the +exponent of the distance which figures in the +expression of the attractive force is equal to~$-2$ +and not to~$-3$, it is not by chance, but because it +is required by Newton's law. It is an \emph{essential} +constant. I do not know if this manner of giving +to chance its share is legitimate in itself, and if +there is not some artificiality about this distinction; +but it is certain at least that in proportion +as Nature has secrets, she will be strictly arbitrary +and always uncertain in their application. As far +as the area-constant is concerned, we are accustomed +to look upon it as accidental. Is it certain +that our imaginary astronomers would do the +same? If they were able to compare two different +solar systems, they would get the idea that this +constant may assume several different values. But +I supposed at the outset, as I was entitled to do, +that their system would appear isolated, and that +they would see no star which was foreign to their +system. Under these conditions they could only +detect a single constant, which would have an +absolutely invariable, unique value. They would +\PageSep{120} +be led no doubt to look upon it as an essential +constant. + +One word in passing to forestall an objection. +The inhabitants of this imaginary world could +neither observe nor define the area-constant as we +do, because absolute longitudes escape their notice; +but that would not prevent them from being +rapidly led to remark a certain constant which +would be naturally introduced into their equations, +and which would be nothing but what we call the +area-constant. But then what would happen? +If the area-constant is regarded as essential, as +dependent upon a law of nature, then in order to +calculate the distances of the planets at any given +moment it would be sufficient to know the initial +values of these distances and those of their first +derivatives. From this new point of view, distances +will be determined by differential equations +of the second order. Would this completely +satisfy the minds of these astronomers? I think +not. In the first place, they would very soon see +that in differentiating their equations so as to +raise them to a higher order, these equations +would become much more simple, and they would +be especially struck by the difficulty which arises +from symmetry. They would have to admit +different laws, according as the aggregate of the +planets presented the figure of a certain polyhedron +or rather of a regular polyhedron, and these consequences +can only be escaped by regarding the area-constant +as accidental. I have taken this particular +\PageSep{121} +example, because I have imagined astronomers +who would not be in the least concerned with +terrestrial mechanics and whose vision would be +bounded by the solar system. But our conclusions +apply in all cases. Our universe is more +extended than theirs, since we have fixed stars; +but it, too, is very limited, so we might reason on +the whole of our universe just as these astronomers +do on their solar system. We thus see that we +should be definitively led to conclude that the +equations which define distances are of an order +higher than the second. Why should this alarm +us---why do we find it perfectly natural that the +sequence of phenomena depends on initial values +of the first derivatives of these distances, while we +hesitate to admit that they may depend on the +initial values of the second derivatives? It can +only be because of mental habits created in us by +the constant study of the generalised principle of +inertia and of its consequences. The values of the +distances at any given moment depend upon their +initial values, on that of their first derivatives, and +something else. What is that \emph{something else}? If +we do not want it to be merely one of the second +derivatives, we have only the choice of hypotheses. +Suppose, as is usually done, that this something +else is the absolute orientation of the universe in +space, or the rapidity with which this orientation +varies; this may be, it certainly is, the most convenient +solution for the geometer. But it is not +the most satisfactory for the philosopher, because +\PageSep{122} +this orientation does not exist. We may assume +that this something else is the position or the +velocity of some invisible body, and this is what is +done by certain persons, who have even called the +body Alpha, although we are destined to never +know anything about this body except its name. +This is an artifice entirely analogous to that of +which I spoke at the end of the paragraph containing +my reflections on the principle of inertia. +But as a matter of fact the difficulty is artificial. +Provided that the future indications of our instruments +can only depend on the indications which +they have given us, or that they might have +formerly given us, such is all we want, and with +these conditions we may rest satisfied. +\PageSep{123} + + +\Chapter{VIII.}{Energy and Thermo-dynamics.} + +\Par{Energetics.}---The difficulties raised by the classical +mechanics have led certain minds to prefer a +new system which they call Energetics. Energetics +took its rise in consequence of the discovery of the +principle of the conservation of energy. Helmholtz +gave it its definite form. We begin by defining +two quantities which play a fundamental +part in this theory. They are \emph{kinetic energy}, or +\Foreign{vis~viva}, and \emph{potential energy}. Every change +that the bodies of nature can undergo is regulated +by two experimental laws. First, the sum of the +kinetic and potential energies is constant. This +is the principle of the conservation of energy. +Second, if a system of bodies is at~$A$ at the time~$t_{0}$, +and at~$B$ at the time~$t_{1}$, it always passes from the +first position to the second by such a path that +the \emph{mean} value of the difference between the two +kinds of energy in the interval of time which +separates the two epochs $t_{0}$~and~$t_{1}$ is a minimum. +This is Hamilton's principle, and is one of the +forms of the principle of least action. The +energetic theory has the following advantages +\PageSep{124} +over the classical. First, it is less incomplete---that +is to say, the principles of the conservation of +energy and of Hamilton teach us more than the +fundamental principles of the classical theory, and +exclude certain motions which do not occur in +nature and which would be compatible with the +classical theory. Second, it frees us from the +hypothesis of atoms, which it was almost impossible +to avoid with the classical theory. But in +its turn it raises fresh difficulties. The definitions +of the two kinds of energy would raise difficulties +almost as great as those of force and mass in the +first system. However, we can get out of these +difficulties more easily, at any rate in the simplest +cases. Assume an isolated system formed of a +certain number of material points. Assume that +these points are acted upon by forces depending +only on their relative position and their distances +apart, and independent of their velocities. +In virtue of the principle of the conservation of +energy there must be a function of forces. In this +simple case the enunciation of the principle of the +conservation of energy is of extreme simplicity. +A certain quantity, which may be determined by +experiment, must remain constant. This quantity +is the sum of two terms. The first depends only on +the position of the material points, and is independent +of their velocities; the second is proportional +to the squares of these velocities. This +decomposition can only take place in one way. +The first of these terms, which I shall call~$U$, will +\PageSep{125} +be potential energy; the second, which I shall call~$T$, +will be kinetic energy. It is true that if $T + U$ +is constant, so is any function of~$T + U$, $\phi(T + U)$. +But this function $\phi(T + U)$ will not be the sum of +two terms, the one independent of the velocities, +and the other proportional to the square of the +velocities. Among the functions which remain +constant there is only one which enjoys this property. +It is~$T + U$ (or a linear function of~$T + U$\Typo{)}{}, +it matters not which, since this linear function may +always be reduced to~$T + U$ by a change of unit +and of origin\Typo{}{)}. This, then, is what we call energy. +The first term we shall call potential energy, and +the second kinetic energy. The definition of the +two kinds of energy may therefore be carried +through without any ambiguity. + +So it is with the definition of mass. Kinetic +energy, or \Foreign{vis~viva}, is expressed very simply by the +aid of the masses, and of the relative velocities of all +the material points with reference to one of them. +These relative velocities may be observed, and +when we have the expression of the kinetic energy +as a function of these relative velocities, the co-efficients +of this expression will give us the masses. +So in this simple case the fundamental ideas can +be defined without difficulty. But the difficulties +reappear in the more complicated cases if the +forces, instead of depending solely on the distances, +depend also on the velocities. For example, +Weber supposes the mutual action of two +electric molecules to depend not only on their +\PageSep{126} +distance but on their velocity and on their acceleration. +If material points attracted each other +according to an analogous law, $U$~would depend +on the velocity, and it might contain a term +proportional to the square of the velocity. How +can we detect among such terms those that arise +from $T$~or~$U$? and how, therefore, can we distinguish +the two parts of the energy? But there +is more than this. How can we define energy +itself? We have no more reason to take as our +definition $T + U$ rather than any other function of~$T + U$, +when the property which characterised +$T + U$ has disappeared---namely, that of being the +sum of two terms of a particular form. But that +is not all. We must take account, not only of +mechanical energy properly so called, but of the +other forms of energy---heat, chemical energy, +electrical energy,~etc. The principle of the conservation +of energy must be written $T + U + Q =$ +a constant, where $T$~is the sensible kinetic energy, +$U$~the potential energy of position, depending only +on the position of the bodies, $Q$~the internal +molecular energy under the thermal, chemical, or +electrical form. This would be all right if the +three terms were absolutely distinct; if $T$~were +proportional to the square of the velocities, $U$~independent +of these velocities and of the state of +the bodies, $Q$~independent of the velocities and of +the positions of the bodies, and depending only on +their internal state. The expression for the energy +could be decomposed in one way only into three +\PageSep{127} +terms of this form. But this is not the case. Let +us consider electrified bodies. The electro-static +energy due to their mutual action will evidently +depend on their charge---\ie, on their state; +but it will equally depend on their position. +If these bodies are in motion, they will act +electro-dynamically on one another, and the +electro-dynamic energy will depend not only on +their state and their position but on their velocities. +We have therefore no means of making the selection +of the terms which should form part of~$T$, +and~$U$, and~$Q$, and of separating the three parts of +the energy. If $T + U + Q$ is constant, the same is +true of any function whatever, $\phi(T + U + Q)$. + +If $T + U + Q$ were of the particular form that I +have suggested above, no ambiguity would ensue. +Among the functions $\phi(T + U + Q)$ which remain +constant, there is only one that would be of this +particular form, namely the one which I would +agree to call energy. But I have said this is not +rigorously the case. Among the functions that +remain constant there is not one which can +rigorously be placed in this particular form. How +then can we choose from among them that which +should be called energy? We have no longer +any guide in our choice. + +Of the principle of the conservation of energy +there is nothing left then but an enunciation:---\emph{There +is something which remains constant.} In this +form it, in its turn, is outside the bounds of experiment +and reduced to a kind of tautology. It +\PageSep{128} +is clear that if the world is governed by laws +there will be quantities which remain constant. +Like Newton's laws, and for an analogous reason, +the principle of the conservation of energy being +based on experiment, can no longer be invalidated +by it. + +This discussion shows that, in passing from the +classical system to the energetic, an advance has +been made; but it shows, at the same time, that +we have not advanced far enough. + +Another objection seems to be still more serious. +The principle of least action is applicable to reversible +phenomena, but it is by no means satisfactory +as far as irreversible phenomena are concerned. +Helmholtz attempted to extend it to this class +of phenomena, but he did not and could not +succeed. So far as this is concerned all has yet to +be done. The very enunciation of the principle of +least action is objectionable. To move from one +point to another, a material molecule, acted upon +by no force, but compelled to move on a surface, +will take as its path the geodesic line---\ie, the +shortest path. This molecule seems to know the +point to which we want to take it, to foresee +the time that it will take it to reach it by such +a path, and then to know how to choose the most +convenient path. The enunciation of the principle +presents it to us, so to speak, as a living +and free entity. It is clear that it would be better +to replace it by a less objectionable enunciation, +one in which, as philosophers would say, final +\PageSep{129} +effects do not seem to be substituted for acting +causes. + +\Par{Thermo-dynamics.}---The rôle of the two fundamental +principles of thermo-dynamics becomes +daily more important in all branches of natural +philosophy. Abandoning the ambitious theories +of forty years ago, encumbered as they were with +molecular hypotheses, we now try to rest on +thermo-dynamics alone the entire edifice of +mathematical physics. Will the two principles +of Mayer and of Clausius assure to it foundations +solid enough to last for some time? We +all feel it, but whence does our confidence +arise? An eminent physicist said to me one day, +\Foreign{àpropos} of the law of errors:---every one stoutly +believes it, because mathematicians imagine that +it is an effect of observation, and observers imagine +that it is a mathematical theorem. And this was +for a long time the case with the principle of the +conservation of energy. It is no longer the same +now. There is no one who does not know that it +is an experimental fact. But then who gives us +the right of attributing to the principle itself more +generality and more precision than to the experiments +which have served to demonstrate it? This +is asking, if it is legitimate to generalise, as we do +every day, empiric data, and I shall not be so +foolhardy as to discuss this question, after so many +philosophers have vainly tried to solve it. One +thing alone is certain. If this permission were +refused to us, science could not exist; or at least +\PageSep{130} +would be reduced to a kind of inventory, to the +ascertaining of isolated facts. It would not longer +be to us of any value, since it could not satisfy our +need of order and harmony, and because it would +be at the same time incapable of prediction. As +the circumstances which have preceded any fact +whatever will never again, in all probability, be +simultaneously reproduced, we already require a +first generalisation to predict whether the fact will +be renewed as soon as the least of these circumstances +is changed. But every proposition may +be generalised in an infinite number of ways. +Among all possible generalisations we must +choose, and we cannot but choose the simplest. +We are therefore led to adopt the same course +as if a simple law were, other things being equal, +more probable than a complex law. A century +ago it was frankly confessed and proclaimed +abroad that Nature loves simplicity; but Nature +has proved the contrary since then on more than +one occasion. We no longer confess this tendency, +and we only keep of it what is indispensable, so +that science may not become impossible. In +formulating a general, simple, and formal law, +based on a comparatively small number of not altogether +consistent experiments, we have only obeyed +a necessity from which the human mind cannot +free itself. But there is something more, and that +is why I dwell on this topic. No one doubts that +Mayer's principle is not called upon to survive all +the particular laws from which it was deduced, in +\PageSep{131} +the same way that Newton's law has survived the +laws of Kepler from which it was derived, and +which are no longer anything but approximations, +if we take perturbations into account. Now why +does this principle thus occupy a kind of privileged +position among physical laws? There are many +reasons for that. At the outset we think that we +cannot reject it, or even doubt its absolute rigour, +without admitting the possibility of perpetual +motion; we certainly feel distrust at such a +prospect, and we believe ourselves less rash in +affirming it than in denying it. That perhaps is +not quite accurate. The impossibility of perpetual +motion only implies the conservation of energy for +reversible phenomena. The imposing simplicity +of Mayer's principle equally contributes to +strengthen our faith. In a law immediately deduced +from experiments, such as Mariotte's law, +this simplicity would rather appear to us a reason +for distrust; but here this is no longer the case. +We take elements which at the first glance are +unconnected; these arrange themselves in an unexpected +order, and form a harmonious whole. +We cannot believe that this unexpected harmony +is a mere result of chance. Our conquest +appears to be valuable to us in proportion to the +efforts it has cost, and we feel the more certain of +having snatched its true secret from Nature in proportion +as Nature has appeared more jealous of our +attempts to discover it. But these are only small +reasons. Before we raise Mayer's law to the +\PageSep{132} +dignity of an absolute principle, a deeper discussion +is necessary. But if we embark on this discussion +we see that this absolute principle is not even easy +to enunciate. In every particular case we clearly +see what energy is, and we can give it at least a +provisory definition; but it is impossible to find +a general definition of it. If we wish to enunciate +the principle in all its generality and apply it to +the universe, we see it vanish, so to speak, and +nothing is left but this---\emph{there is something which +remains constant}. But has this a meaning? In +the determinist hypothesis the state of the universe +is determined by an extremely large number~$n$ +of parameters, which I shall call $x_{1}$,~$x_{2}$, $x_{3}\Add{,}~\ldots\Add{,},~x_{n}$. +As soon as we know at a given moment the values of +these $n$~parameters, we also know their derivatives +with respect to time, and we can therefore calculate +the values of these same parameters at an +anterior or ulterior moment. In other words, +these $n$~parameters specify $n$~differential equations +of the first order. These equations have $n - 1$ +integrals, and therefore there are $n - 1$ functions of +$x_{1}$,~$x_{2}$, $x_{3}\Add{,}~\ldots\Add{,}~x_{n}$, which remain constant. If we +say then, \emph{there is something which remains constant}, +we are only enunciating a tautology. We would +be even embarrassed to decide which among all +our integrals is that which should retain the name +of energy. Besides, it is not in this sense that +Mayer's principle is understood when it is applied +to a limited system. We admit, then, that $p$~of +our $n$~parameters vary independently so that we +\PageSep{133} +have only $n - p$ relations, generally linear, between +our $n$~parameters and their derivatives. Suppose, +for the sake of simplicity, that the sum of the +work done by the external forces is zero, as well +as that of all the quantities of heat given off from +the interior: what will then be the meaning of +our principle? \emph{There is a combination of these $n - p$ +relations, of which the first member is an exact +differential}; and then this differential vanishing +in virtue of our $n - p$ relations, its integral is a +constant, and it is this integral which we call +energy. But how can it be that there are several +parameters whose variations are independent? +That can only take place in the case of external +forces (although we have supposed, for the sake +of simplicity, that the algebraical sum of all the +work done by these forces has vanished). If, +in fact, the system were completely isolated from +all external action, the values of our $n$~parameters +at a given moment would suffice to determine +the state of the system at any ulterior moment +whatever, provided that we still clung to the determinist +hypothesis. We should therefore fall back +on the same difficulty as before. If the future +state of the system is not entirely determined +by its present state, it is because it further depends +on the state of bodies external to the system. +But then, is it likely that there exist among the +parameters~$x$ which define the state of the system of +equations independent of this state of the external +bodies? and if in certain cases we think we can +\PageSep{134} +find them, is it not only because of our ignorance, +and because the influence of these bodies is too +weak for our experiment to be able to detect it? +If the system is not regarded as completely +isolated, it is probable that the rigorously exact +expression of its internal energy will depend upon +the state of the external bodies. Again, I have +supposed above that the sum of all the external +work is zero, and if we wish to be free from +this rather artificial restriction the enunciation +becomes still more difficult. To formulate +Mayer's principle by giving it an absolute +meaning, we must extend it to the whole +universe, and then we find ourselves face to +face with the very difficulty we have endeavoured +to avoid. To sum up, and to use ordinary +language, the law of the conservation of energy +can have only one significance, because there is +in it a property common to all possible properties; +but in the determinist hypothesis there is only one +possible, and then the law has no meaning. In +the indeterminist hypothesis, on the other hand, +it would have a meaning even if we wished to +regard it in an absolute sense. It would appear +as a limitation imposed on freedom. + +But this word warns me that I am wandering +from the subject, and that I am leaving the +domain of mathematics and physics. I check +myself, therefore, and I wish to retain only one +impression of the whole of this discussion, and +that is, that Mayer's law is a form subtle enough +\PageSep{135} +for us to be able to put into it almost anything we +like. I do not mean by that that it corresponds +to no objective reality, nor that it is reduced to +mere tautology; since, in each particular case, and +provided we do not wish to extend it to the +absolute, it has a perfectly clear meaning. This +subtlety is a reason for believing that it will last +long; and as, on the other hand, it will only +disappear to be blended in a higher harmony, +we may work with confidence and utilise it, +certain beforehand that our work will not be +lost. + +Almost everything that I have just said +applies to the principle of Clausius. What +distinguishes it is, that it is expressed by an +inequality. It will be said perhaps that it is +the same with all physical laws, since their +precision is always limited by errors of +observation. But they at least claim to be +first approximations, and we hope to replace +them little by little by more exact laws. If, +on the other hand, the principle of Clausius +reduces to an inequality, this is not caused by +the imperfection of our means of observation, but +by the very nature of the question. + +\Par{General Conclusions on Part~III.}---The principles +of mechanics are therefore presented to us +under two different aspects. On the one hand, +there are truths founded on experiment, and +verified approximately as far as almost isolated +systems are concerned; on the other hand, +\PageSep{136} +there are postulates applicable to the whole of +the universe and regarded as rigorously true. +If these postulates possess a generality and a +certainty which falsify the experimental truths +from which they were deduced, it is because +they reduce in final analysis to a simple convention +that we have a right to make, because +we are certain beforehand that no experiment +can contradict it. This convention, however, is +not absolutely arbitrary; it is not the child +of our caprice. We admit it because certain +experiments have shown us that it will be convenient, +and thus is explained how experiment +has built up the principles of mechanics, and +why, moreover, it cannot reverse them. Take a +comparison with geometry. The fundamental +propositions of geometry, for instance, Euclid's +postulate, are only conventions, and it is quite +as unreasonable to ask if they are true or false +as to ask if the metric system is true or false. +Only, these conventions are convenient, and there +are certain experiments which prove it to us. At +the first glance, the analogy is complete, the rôle +of experiment seems the same. We shall therefore +be tempted to say, either mechanics must +be looked upon as experimental science and then +it should be the same with geometry; or, on the +contrary, geometry is a deductive science, and +then we can say the same of mechanics. Such +a conclusion would be illegitimate. The experiments +which have led us to adopt as more +\PageSep{137} +convenient the fundamental conventions of +geometry refer to bodies which have nothing +in common with those that are studied by +geometry. They refer to the properties of solid +bodies and to the propagation of light in a straight +line. These are mechanical, optical experiments. +In no way can they be regarded as geometrical +experiments. And even the probable reason why +our geometry seems convenient to us is, that our +bodies, our hands, and our limbs enjoy the properties +of solid bodies. Our fundamental experiments are +pre-eminently physiological experiments which +refer, not to the space which is the object that +geometry must study, but to our body---that is to +say, to the instrument which we use for that +study. On the other hand, the fundamental +conventions of mechanics and the experiments +which prove to us that they are convenient, +certainly refer to the same objects or to analogous +objects. Conventional and general principles are +the natural and direct generalisations of experimental +and particular principles. Let it not be +said that I am thus tracing artificial frontiers +between the sciences; that I am separating by +a barrier geometry properly so called from the +study of solid bodies. I might just as well +raise a barrier between experimental mechanics +and the conventional mechanics of general +principles. Who does not see, in fact, that +by separating these two sciences we mutilate +both, and that what will remain of the conventional +\PageSep{138} +mechanics when it is isolated will be but +very little, and can in no way be compared with +that grand body of doctrine which is called +geometry. + +We now understand why the teaching of +mechanics should remain experimental. Thus +only can we be made to understand the genesis +of the science, and that is indispensable for +a complete knowledge of the science itself. +Besides, if we study mechanics, it is in order +to apply it; and we can only apply it if it remains +objective. Now, as we have seen, when principles +gain in generality and certainty they lose in +objectivity. It is therefore especially with the +objective side of principles that we must be +early familiarised, and this can only be by +passing from the particular to the general, instead +of from the general to the particular. + +Principles are conventions and definitions in +disguise. They are, however, deduced from +experimental laws, and these laws have, so to +speak, been erected into principles to which +our mind attributes an absolute value. Some +philosophers have generalised far too much. +They have thought that the principles were +the whole of science, and therefore that the +whole of science was conventional. This paradoxical +doctrine, which is called Nominalism, +cannot stand examination. How can a law +become a principle? It expressed a relation +between two real terms, $A$~and~$B$; but it was +\PageSep{139} +not rigorously true, it was only approximate. +We introduce arbitrarily an intermediate term,~$C$, +more or less imaginary, and $C$~is \emph{by definition} that +which has with~$A$ \emph{exactly} the relation expressed +by the law. So our law is decomposed into an +absolute and rigorous principle which expresses +the relation of~$A$ to~$C$, and an approximate experimental +and revisable law which expresses the +relation of~$C$ to~$B$. But it is clear that however +far this decomposition may be carried, laws will +always remain. We shall now enter into the +domain of laws properly so called. +\PageSep{140} + + +\Part{IV.}{Nature.} + +\Chapter{IX.}{Hypotheses in Physics.} + +\Par{The Rôle of Experiment and Generalisation.}---Exper\-iment +is the sole source of truth. It alone +can teach us something new; it alone can give +us certainty. These are two points that cannot +be questioned. But then, if experiment is everything, +what place is left for mathematical physics? +What can experimental physics do with such an +auxiliary---an auxiliary, moreover, which seems +useless, and even may be dangerous? + +However, mathematical physics exists. It has +rendered undeniable service, and that is a fact +which has to be explained. It is not sufficient +merely to observe; we must use our observations, +and for that purpose we must generalise. This +is what has always been done, only as the recollection +of past errors has made man more and more +circumspect, he has observed more and more and +generalised less and less. Every age has scoffed +at its predecessor, accusing it of having generalised +\PageSep{141} +too boldly and too naïvely. Descartes used to +commiserate the Ionians. Descartes in his turn +makes us smile, and no doubt some day our +children will laugh at us. Is there no way of +getting at once to the gist of the matter, and +thereby escaping the raillery which we foresee? +Cannot we be content with experiment alone? +No, that is impossible; that would be a complete +misunderstanding of the true character of science. +The man of science must work with method. +Science is built up of facts, as a house is built of +stones; but an accumulation of facts is no more a +science than a heap of stones is a house. Most +important of all, the man of science must exhibit +foresight. Carlyle has written somewhere something +after this fashion. ``Nothing but facts are +of importance. John Lackland passed by here. +Here is something that is admirable. Here is a +reality for which I would give all the theories in +the world.''\footnote + {V. \Title{Past and Present}, end of Chapter~I., Book~II.\Transl} +Carlyle was a compatriot of Bacon, +and, like him, he wished to proclaim his worship +of \emph{the God of Things as they are}. + +But Bacon would not have said that. That is +the language of the historian. The physicist +would most likely have said: ``John Lackland +passed by here. It is all the same to me, for he +will not pass this way again.'' + +We all know that there are good and bad +experiments. The latter accumulate in vain. +Whether there are a hundred or a thousand, +\PageSep{142} +one single piece of work by a real master---by a +Pasteur, for example---will be sufficient to sweep +them into oblivion. Bacon would have thoroughly +understood that, for he invented the phrase \Foreign{experimentum +crucis}; but Carlyle would not have understood +it. A fact is a fact. A student has read +such and such a number on his thermometer. +He has taken no precautions. It does not matter; +he has read it, and if it is only the fact which +counts, this is a reality that is as much entitled +to be called a reality as the peregrinations of King +John Lackland. What, then, is a good experiment? +It is that which teaches us something more than +an isolated fact. It is that which enables us to +predict, and to generalise. Without generalisation, +prediction is impossible. The circumstances +under which one has operated will never again +be reproduced simultaneously. The fact observed +will never be repeated. All that can be affirmed +is that under analogous circumstances an analogous +fact will be produced. To predict it, we must +therefore invoke the aid of analogy---that is to say, +even at this stage, we must generalise. However +timid we may be, there must be interpolation. +Experiment only gives us a certain number of +isolated points. They must be connected by a +continuous line, and this is a true generalisation. +But more is done. The curve thus traced will +pass between and near the points observed; it +will not pass through the points themselves. +Thus we are not restricted to generalising our +\PageSep{143} +experiment, we correct it; and the physicist who +would abstain from these corrections, and really +content himself with experiment pure and simple, +would be compelled to enunciate very extraordinary +laws indeed. Detached facts cannot +therefore satisfy us, and that is why our science +must be ordered, or, better still, generalised. + +It is often said that experiments should be made +without preconceived ideas. That is impossible. +Not only would it make every experiment fruitless, +but even if we wished to do so, it could not be +done. Every man has his own conception of the +world, and this he cannot so easily lay aside. We +must, for example, use language, and our language +is necessarily steeped in preconceived ideas. Only +they are unconscious preconceived ideas, which +are a thousand times the most dangerous of all. +Shall we say, that if we cause others to intervene of +which we are fully conscious, that we shall only +aggravate the evil? I do not think so. I am +inclined to think that they will serve as ample +counterpoises---I was almost going to say antidotes. +They will generally disagree, they will enter into +conflict one with another, and \Foreign{ipso~facto}, they will +force us to look at things under different aspects. +This is enough to free us. He is no longer a slave +who can choose his master. + +Thus, by generalisation, every fact observed +enables us to predict a large number of others; +only, we ought not to forget that the first alone +is certain, and that all the others are merely +\PageSep{144} +probable. However solidly founded a prediction +may appear to us, we are never \emph{absolutely} sure that +experiment will not prove it to be baseless if we +set to work to verify it. But the probability of its +accuracy is often so great that practically we may +be content with it. It is far better to predict +without certainty, than never to have predicted +at all. We should never, therefore, disdain to +verify when the opportunity presents itself. But +every experiment is long and difficult, and the +labourers are few, and the number of facts which +we require to predict is enormous; and besides +this mass, the number of direct verifications that +we can make will never be more than a negligible +quantity. Of this little that we can directly attain +we must choose the best. Every experiment must +enable us to make a maximum number of predictions +having the highest possible degree of probability. +The problem is, so to speak, to increase +the output of the scientific machine. I may be +permitted to compare science to a library which +must go on increasing indefinitely; the librarian +has limited funds for his purchases, and he must, +therefore, strain every nerve not to waste them. +Experimental physics has to make the purchases, +and experimental physics alone can enrich the +library. As for mathematical physics, her duty +is to draw up the catalogue. If the catalogue is +well done the library is none the richer for it; but +the reader will be enabled to utilise its riches; +and also by showing the librarian the gaps in his +\PageSep{145} +collection, it will help him to make a judicious +use of his funds, which is all the more important, +inasmuch as those funds are entirely inadequate. +That is the rôle of mathematical physics. It +must direct generalisation, so as to increase what +I called just now the output of science. By what +means it does this, and how it may do it without +danger, is what we have now to examine. + +\Par{The Unity of Nature.}---Let us first of all observe +that every generalisation supposes in a certain +measure a belief in the unity and simplicity of +Nature. As far as the unity is concerned, there +can be no difficulty. If the different parts of the +universe were not as the organs of the same body, +they would not \Chg{re-act}{react} one upon the other; they +would mutually ignore each other, and we in +particular should only know one part. We need +not, therefore, ask if Nature is one, but how she +is one. + +As for the second point, that is not so clear. It +is not certain that Nature is simple. Can we +without danger act as if she were? + +There was a time when the simplicity of +Mariotte's law was an argument in favour of its +accuracy: when Fresnel himself, after having said +in a conversation with Laplace that Nature cares +naught for analytical difficulties, was compelled +to explain his words so as not to give offence to +current opinion. Nowadays, ideas have changed +considerably; but those who do not believe that +natural laws must be simple, are still often obliged +\PageSep{146} +to act as if they did believe it. They cannot +entirely dispense with this necessity without +making all generalisation, and therefore all science, +impossible. It is clear that any fact can be +generalised in an infinite number of ways, and +it is a question of choice. The choice can only +be guided by considerations of simplicity. Let +us take the most ordinary case, that of interpolation. +We draw a continuous line as regularly as +possible between the points given by observation. +Why do we avoid angular points and inflexions +that are too sharp? Why do we not make our +curve describe the most capricious zigzags? It +is because we know beforehand, or think we know, +that the law we have to express cannot be so +complicated as all that. The mass of Jupiter +may be deduced either from the movements of +his satellites, or from the perturbations of the +major planets, or from those of the minor planets. +If we take the mean of the determinations obtained +by these three methods, we find three numbers +very close together, but not quite identical. This +result might be interpreted by supposing that the +gravitation constant is not the same in the three +cases; the observations would be certainly much +better represented. Why do we reject this interpretation? +Not because it is absurd, but because +it is uselessly complicated. We shall only accept +it when we are forced to, and it is not imposed +upon us yet. To sum up, in most cases every law +is held to be simple until the contrary is proved. +\PageSep{147} + +This custom is imposed upon physicists by the +reasons that I have indicated, but how can it be +justified in the presence of discoveries which daily +show us fresh details, richer and more complex? +How can we even reconcile it with the unity of +nature? For if all things are interdependent, +the relations in which so many different objects +intervene can no longer be simple. + +If we study the history of science we see produced +two phenomena which are, so to speak, +each the inverse of the other. Sometimes it is +simplicity which is hidden under what is +apparently complex; sometimes, on the contrary, +it is simplicity which is apparent, and which +conceals extremely complex realities. What is +there more complicated than the disturbed +motions of the planets, and what more simple +than Newton's law? There, as Fresnel said, +Nature playing with analytical difficulties, only +uses simple means, and creates by their combination +I know not what tangled skein. Here it is +the hidden simplicity which must be disentangled. +Examples to the contrary abound. In the kinetic +theory of gases, molecules of tremendous velocity +are discussed, whose paths, deformed by incessant +impacts, have the most capricious shapes, and +plough their way through space in every direction. +The result observable is Mariotte's simple law. +Each individual fact was complicated. The law +of great numbers has re-established simplicity in +the mean. Here the simplicity is only apparent, +\PageSep{148} +and the coarseness of our senses alone prevents us +from seeing the complexity. + +Many phenomena obey a law of proportionality. +But why? Because in these phenomena +there is something which is very small. The +simple law observed is only the translation of +the general analytical rule by which the infinitely +small increment of a function is proportional +to the increment of the variable. As in reality +our increments are not infinitely small, but only +very small, the law of proportionality is only +approximate, and simplicity is only apparent. +What I have just said applies to the law of the +superposition of small movements, which is so +fruitful in its applications and which is the foundation +of optics. + +And Newton's law itself? Its simplicity, so +long undetected, is perhaps only apparent. Who +knows if it be not due to some complicated +mechanism, to the impact of some subtle matter +animated by irregular movements, and if it has +not become simple merely through the play of +averages and large numbers? In any case, it +is difficult not to suppose that the true law contains +complementary terms which may become +sensible at small distances. If in astronomy they +are negligible, and if the law thus regains its +simplicity, it is solely on account of the enormous +distances of the celestial bodies. No doubt, if our +means of investigation became more and more +penetrating, we should discover the simple beneath +\PageSep{149} +the complex, and then the complex from the +simple, and then again the simple beneath the +complex, and so on, without ever being able to +predict what the last term will be. We must stop +somewhere, and for science to be possible we must +stop where we have found simplicity. That is the +only ground on which we can erect the edifice of +our generalisations. But, this simplicity being +only apparent, will the ground be solid enough? +That is what we have now to discover. + +For this purpose let us see what part is played +in our generalisations by the belief in simplicity. +We have verified a simple law in a considerable +number of particular cases. We refuse to admit +that this coincidence, so often repeated, is a result +of mere chance, and we conclude that the law +must be true in the general case. + +Kepler remarks that the positions of a planet +observed by Tycho are all on the same ellipse. +Not for one moment does he think that, by a +singular freak of chance, Tycho had never looked +at the heavens except at the very moment when +the path of the planet happened to cut that +ellipse. What does it matter then if the simplicity +be real or if it hide a complex truth? Whether it +be due to the influence of great numbers which +reduces individual differences to a level, or to the +greatness or the smallness of certain quantities +which allow of certain terms to be neglected---in +no case is it due to chance. This simplicity, real +or apparent, has always a cause. We shall therefore +\PageSep{150} +always be able to reason in the same fashion, +and if a simple law has been observed in several +particular cases, we may legitimately suppose that +it still will be true in analogous cases. To refuse +to admit this would be to attribute an inadmissible +rôle to chance. However, there is a +difference. If the simplicity were real and profound +it would bear the test of the increasing +precision of our methods of measurement. If, +then, we believe Nature to be profoundly simple, +we must conclude that it is an approximate and +not a rigorous simplicity. This is what was +formerly done, but it is what we have no longer +the right to do. The simplicity of Kepler's laws, +for instance, is only apparent; but that does not +prevent them from being applied to almost all +systems analogous to the solar system, though +that prevents them from being rigorously exact. + +\Par{Rôle of Hypothesis.}---Every generalisation is a +hypothesis. Hypothesis therefore plays a necessary +rôle, which no one has ever contested. Only, +it should always be as soon as possible submitted +to verification. It goes without saying that, if it +cannot stand this test, it must be abandoned +without any hesitation. This is, indeed, what +is generally done; but sometimes with a certain +impatience. Ah well!\ this impatience is not +justified. The physicist who has just given up +one of his hypotheses should, on the contrary, +rejoice, for he found an unexpected opportunity of +discovery. His hypothesis, I imagine, had not +\PageSep{151} +been lightly adopted, It took into account all the +known factors which seem capable of intervention +in the phenomenon. If it is not verified, it is +because there is something unexpected and extraordinary +about it, because we are on the point +of finding something unknown and new. Has +the hypothesis thus rejected been sterile? Far +from it. It may be even said that it has rendered +more service than a true hypothesis. Not only +has it been the occasion of a decisive experiment, +but if this experiment had been made by chance, +without the hypothesis, no conclusion could have +been drawn; nothing extraordinary would have +been seen; and only one fact the more would have +been catalogued, without deducing from it the +remotest consequence. + +Now, under what conditions is the use of +hypothesis without danger? The proposal to +submit all to experiment is not sufficient. Some +hypotheses are dangerous,---first and foremost +those which are tacit and unconscious. And +since we make them without knowing them, +we cannot get rid of them. Here again, there +is a service that mathematical physics may +render us. By the precision which is its characteristic, +we are compelled to formulate all the +hypotheses that we would unhesitatingly make +without its aid. Let us also notice that it is +important not to multiply hypotheses indefinitely. +If we construct a theory based upon multiple hypotheses, +and if experiment condemns it, which of +\PageSep{152} +the premisses must be changed? It is impossible +to tell. Conversely, if the experiment succeeds, +must we suppose that it has verified all these +hypotheses at once? Can several unknowns be +determined from a single equation? + +We must also take care to distinguish between +the different kinds of hypotheses. First of all, +there are those which are quite natural and +necessary. It is difficult not to suppose that the +influence of very distant bodies is quite negligible, +that small movements obey a linear law, and that +effect is a continuous function of its cause. I will +say as much for the conditions imposed by +symmetry. All these hypotheses affirm, so to +speak, the common basis of all the theories of +mathematical physics. They are the last that +should be abandoned. There is a second category +of hypotheses which I shall qualify as indifferent. +In most questions the analyst assumes, at the +beginning of his calculations, either that matter is +continuous, or the reverse, that it is formed of +atoms. In either case, his results would have +been the same. On the atomic supposition he has +a little more difficulty in obtaining them---that is +all. If, then, experiment confirms his conclusions, +will he suppose that he has proved, for example, +the real existence of atoms? + +In optical theories two vectors are introduced, +one of which we consider as a velocity and the +other as a vortex. This again is an indifferent +hypothesis, since we should have arrived at the +\PageSep{153} +same conclusions by assuming the former to be +a vortex and the latter to be a velocity. The +success of the experiment cannot prove, therefore, +that the first vector is really a velocity. It only +proves one thing---namely, that it is a vector; +and that is the only hypothesis that has really +been introduced into the premisses. To give it +the concrete appearance that the fallibility of our +minds demands, it was necessary to consider it +either as a velocity or as a vortex. In the same +way, it was necessary to represent it by an~$x$ or a~$y$, +but the result will not prove that we were right +or wrong in regarding it as a velocity; nor will it +prove we are right or wrong in calling it~$x$ and +not~$y$. + +These indifferent hypotheses are never dangerous +provided their characters are not misunderstood. +They may be useful, either as artifices for +calculation, or to assist our understanding by +concrete images, to fix the ideas, as we say. They +need not therefore be rejected. The hypotheses +of the third category are real generalisations. +They must be confirmed or invalidated by experiment. +Whether verified or condemned, they will +always be fruitful; but, for the reasons I have +given, they will only be so if they are not too +numerous. + +\Par{Origin of Mathematical Physics.}---Let us go +further and study more closely the conditions +which have assisted the development of mathematical +physics. We recognise at the outset that +\PageSep{154} +the efforts of men of science have always tended +to resolve the complex phenomenon given directly +by experiment into a very large number of elementary +phenomena, and that in three different +ways. + +First, with respect to time. Instead of embracing +in its entirety the progressive development of a +phenomenon, we simply try to connect each +moment with the one immediately preceding. +We admit that the present state of the world +only depends on the immediate past, without +being directly influenced, so to speak, by the +recollection of a more distant past. Thanks to +this postulate, instead of studying directly the +whole succession of phenomena, we may confine +ourselves to writing down its \emph{differential equation}; +for the laws of Kepler we substitute the law of +Newton. + +Next, we try to decompose the phenomena in +space. What experiment gives us is a confused +aggregate of facts spread over a scene of considerable +extent. We must try to deduce the elementary +phenomenon, which will still be localised in a +very small region of space. + +A few examples perhaps will make my meaning +clearer. If we wished to study in all its complexity +the distribution of temperature in a cooling +solid, we could never do so. This is simply because, +if we only reflect that a point in the solid +can directly impart some of its heat to a neighbouring +point, it will immediately impart that +\PageSep{155} +heat only to the nearest points, and it is but +gradually that the flow of heat will reach other +portions of the solid. The elementary phenomenon +is the interchange of heat between two +contiguous points. It is strictly localised and +relatively simple if, as is natural, we admit that +it is not influenced by the temperature of the +molecules whose distance apart is small. + +I bend a rod: it takes a very complicated form, +the direct investigation of which would be impossible. +But I can attack the problem, however, +if I notice that its flexure is only the resultant of +the deformations of the very small elements of the +rod, and that the deformation of each of these +elements only depends on the forces which are +directly applied to it, and not in the least on +those which may be acting on the other elements. + +In all these examples, which may be increased +without difficulty, it is admitted that there is no +action at a distance or at great distances. That +is an hypothesis. It is not always true, as the law +of gravitation proves. It must therefore be verified. +If it is confirmed, even approximately, it is valuable, +for it helps us to use mathematical physics, +at any rate by successive approximations. If it +does not stand the test, we must seek something +else that is analogous, for there are other means +of arriving at the elementary phenomenon. If +several bodies act simultaneously, it may happen +that their actions are independent, and may be +added one to the other, either as vectors or as scalar +\PageSep{156} +quantities. The elementary phenomenon is then +the action of an isolated body. Or suppose, again, +it is a question of small movements, or more +generally of small variations which obey the well-known +law of mutual or relative independence. +The movement observed will then be decomposed +into simple movements---for example, sound into +its harmonics, and white light into its monochromatic +components. When we have discovered in +which direction to seek for the elementary phenomena, +by what means may we reach it? First, it +will often happen that in order to predict it, or rather +in order to predict what is useful to us, it will not +be necessary to know its mechanism. The law of +great numbers will suffice. Take for example the +propagation of heat. Each molecule radiates towards +its neighbour---we need not inquire according +to what law; and if we make any supposition +in this respect, it will be an indifferent hypothesis, +and therefore useless and unverifiable. In fact, +by the action of averages and thanks to the +symmetry of the medium, all differences are +levelled, and, whatever the hypothesis may be, the +result is always the same. + +The same feature is presented in the theory of +elasticity, and in that of capillarity. The neighbouring +molecules attract and repel each other, we +need not inquire by what law. It is enough for us +that this attraction is sensible at small distances +only, and that the molecules are very numerous, +that the medium is symmetrical, and we have +\PageSep{157} +only to let the law of great numbers come into +play. + +Here again the simplicity of the elementary +phenomenon is hidden beneath the complexity of +the observable resultant phenomenon; but in its +turn this simplicity was only apparent and disguised +a very complex mechanism. Evidently the +best means of reaching the elementary phenomenon +would be experiment. It would be necessary +by experimental artifices to dissociate the +complex system which nature offers for our investigations +and carefully to study the elements as +dissociated as possible; for example, natural white +light would be decomposed into monochromatic +lights by the aid of the prism, and into polarised +lights by the aid of the polariser. Unfortunately, +that is neither always possible nor always sufficient, +and sometimes the mind must run ahead of +experiment. I shall only give one example which +has always struck me rather forcibly. If I decompose +white light, I shall be able to isolate a +portion of the spectrum, but however small it may +be, it will always be a certain width. In the same +way the natural lights which are called \emph{monochromatic} +%[** TN: "nous donnent une raie très fine, mais qui n'est pas cependant infiniment fine"] +give us a very fine \Reword{array, but a y}{ray, but one} which +is not, however, infinitely fine. It might be +supposed that in the experimental study of the +properties of these natural lights, by operating +with finer and finer rays, and passing on at last +to the limit, so to speak, we should eventually +obtain the properties of a rigorously monochromatic +\PageSep{158} +light. That would not be accurate. +I assume that two rays emanate from the same +source, that they are first polarised in planes at +right angles, that they are then brought back +again to the same plane of polarisation, and that +we try to obtain interference. If the light were +\emph{rigorously} monochromatic, there would be interference; +but with our nearly monochromatic +lights, there will be no interference, and that, +however narrow the ray may be. For it to be +otherwise, the ray would have to be several million +times finer than the finest known rays. + +Here then we should be led astray by proceeding +to the limit. The mind has to run ahead of the +experiment, and if it has done so with success, it +is because it has allowed itself to be guided by the +instinct of simplicity. The knowledge of the elementary +fact enables us to state the problem in +the form of an equation. It only remains to deduce +from it by combination the observable and +verifiable complex fact. That is what we call +\emph{integration}, and it is the province of the mathematician. +It might be asked, why in physical +science generalisation so readily takes the +mathematical form. The reason is now easy to +see. It is not only because we have to express +numerical laws; it is because the observable +phenomenon is due to the superposition of a large +number of elementary phenomena which are \emph{all +similar to each other}; and in this way differential +equations are quite naturally introduced. It is +\PageSep{159} +not enough that each elementary phenomenon +should obey simple laws: all those that we have +to combine must obey the same law; then only +is the intervention of mathematics of any use. +Mathematics teaches us, in fact, to combine like +with like. Its object is to divine the result of a +combination without having to reconstruct that +combination element by element. If we have to +repeat the same operation several times, mathematics +enables us to avoid this repetition by telling +the result beforehand by a kind of induction. +This I have explained before in the \hyperref[chapref:I]{chapter on +mathematical reasoning}. But for that purpose +all these operations must be similar; in the contrary +case we must evidently make up our minds +to working them out in full one after the other, +and mathematics will be useless. It is therefore, +thanks to the approximate homogeneity of the +matter studied by physicists, that mathematical +physics came into existence. In the natural +sciences the following conditions are no longer to +be found:---homogeneity, relative independence of +remote parts, simplicity of the elementary fact; +and that is why the student of natural science is +compelled to have recourse to other modes of +generalisation. +\PageSep{160} + + +\Chapter{X.}{The Theories of Modern Physics.} + +\Par{Significance of Physical Theories.}---The ephemeral +nature of scientific theories takes by surprise the +man of the world. Their brief period of prosperity +ended, he sees them abandoned one after another; +he sees ruins piled upon ruins; he predicts that +the theories in fashion to-day will in a short time +succumb in their turn, and he concludes that they +are absolutely in vain. This is what he calls the +\emph{bankruptcy of science}. + +His scepticism is superficial; he does not take +into account the object of scientific theories and +the part they play, or he would understand that +the ruins may be still good for something. No +theory seemed established on firmer ground than +Fresnel's, which attributed light to the movements +of the ether. Then if Maxwell's theory is +to-day preferred, does that mean that Fresnel's +work was in vain? No; for Fresnel's object was +not to know whether there really is an ether, if it +is or is not formed of atoms, if these atoms really +move in this way or that; his object was to +predict optical phenomena. + +This Fresnel's theory enables us to do to-day +\PageSep{161} +as well as it did before Maxwell's time. The +differential equations are always true, they may +be always integrated by the same methods, and +the results of this integration still preserve their +value. It cannot be said that this is reducing +physical theories to simple practical recipes; +these equations express relations, and if the +equations remain true, it is because the relations +preserve their reality. They teach us now, as they +did then, that there is such and such a relation +between this thing and that; only, the something +which we then called \emph{motion}, we now call \emph{electric +current}. But these are merely names of the images +we substituted for the real objects which Nature +will hide for ever from our eyes. The true relations +between these real objects are the only reality we +can attain, and the sole condition is that the same +relations shall exist between these objects as between +the images we are forced to put in their place. If +the relations are known to us, what does it matter +if we think it convenient to replace one image by +another? + +That a given periodic phenomenon (an electric +oscillation, for instance) is really due to the +vibration of a given atom, which, behaving like +a pendulum, is really displaced in this manner or +that, all this is neither certain nor essential. +But that there is between the electric oscillation, +the movement of the pendulum, and all periodic +phenomena an intimate relationship which corresponds +to a profound reality; that this relationship, +\PageSep{162} +this similarity, or rather this parallelism, is continued +in the details; that it is a consequence of +more general principles such as that of the conservation +of energy, and that of least action; this +we may affirm; this is the truth which will ever +remain the same in whatever garb we may see fit +to clothe it. + +Many theories of dispersion have been proposed. +The first were imperfect, and contained but little +truth. Then came that of Helmholtz, and this +in its turn was modified in different ways; its +author himself conceived another theory, founded +on Maxwell's principles. But the remarkable +thing is, that all the scientists who followed +Helmholtz obtain the same equations, although +their starting-points were to all appearance widely +separated. I venture to say that these theories +are all simultaneously true; not merely because +they express a true relation---that between absorption +and abnormal dispersion. In the premisses +of these theories the part that is true is the part +common to all: it is the affirmation of this or +that relation between certain things, which some +call by one name and some by another. + +The kinetic theory of gases has given rise to +many objections, to which it would be difficult +to find an answer were it claimed that the theory +is absolutely true. But all these objections do +not alter the fact that it has been useful, +particularly in revealing to us one true relation +which would otherwise have remained profoundly +\PageSep{163} +hidden---the relation between gaseous and osmotic +pressures. In this sense, then, it may be said to +be true. + +When a physicist finds a contradiction between +two theories which are equally dear to him, he +sometimes says: ``Let us not be troubled, but let +us hold fast to the two ends of the chain, lest +we lose the intermediate links.'' This argument +of the embarrassed theologian would be ridiculous +if we were to attribute to physical theories the +interpretation given them by the man of the +world. In case of contradiction one of them at +least should be considered false. But this is no +longer the case if we only seek in them what +should be sought. It is quite possible that they +both express true relations, and that the contradictions +only exist in the images we have formed +to ourselves of reality. To those who feel that +we are going too far in our limitations of the +domain accessible to the scientist, I reply: These +questions which we forbid you to investigate, +and which you so regret, are not only insoluble, +they are illusory and devoid of meaning. + +Such a philosopher claims that all physics can be +explained by the mutual impact of atoms. If he +simply means that the same relations obtain +between physical phenomena as between the +mutual impact of a large number of billiard +balls---well and good!\ this is verifiable, and +perhaps is true. But he means something more, +and we think we understand him, because we +\PageSep{164} +think we know what an impact is. Why? Simply +because we have often watched a game of billiards. +Are we to understand that God experiences the +same sensations in the contemplation of His +work that we do in watching a game of billiards? +If it is not our intention to give his assertion +this fantastic meaning, and if we do not wish +to give it the more restricted meaning I have +already mentioned, which is the sound meaning, +then it has no meaning at all. Hypotheses of +this kind have therefore only a metaphorical sense. +The scientist should no more banish them than a +poet banishes metaphor; but he ought to know +what they are worth. They may be useful to +give satisfaction to the mind, and they will do +no harm as long as they are only indifferent +hypotheses. + +These considerations explain to us why certain +theories, that were thought to be abandoned and +definitively condemned by experiment, are suddenly +revived from their ashes and begin a new life. +It is because they expressed true relations, and +had not ceased to do so when for some reason or +other we felt it necessary to enunciate the same +relations in another language. Their life had been +latent, as it were. + +Barely fifteen years ago, was there anything +more ridiculous, more quaintly old-fashioned, than +the fluids of Coulomb? And yet, here they are +re-appearing under the name of \emph{electrons}. In what +do these permanently electrified molecules differ +\PageSep{165} +from the electric molecules of Coulomb? It is +true that in the electrons the electricity is supported +by a little, a very little matter; in other +words, they have mass. Yet Coulomb did not +deny mass to his fluids, or if he did, it was with +reluctance. It would be rash to affirm that the +belief in electrons will not also undergo an eclipse, +but it was none the less curious to note this unexpected +renaissance. + +But the most striking example is Carnot's +principle. Carnot established it, starting from +false hypotheses. When it was found that heat +was indestructible, and may be converted into +work, his ideas were completely abandoned; +later, Clausius returned to them, and to him is +due their definitive triumph. In its primitive +form, Carnot's theory expressed in addition to +true relations, other inexact relations, the \Foreign{débris} +of old ideas; but the presence of the latter did +not alter the reality of the others. Clausius had +only to separate them, just as one lops off dead +branches. + +The result was the second fundamental law of +\Chg{thermodynamics}{thermo-dynamics}. The relations were always the +same, although they did not hold, at least to all +appearance, between the same objects. This was +sufficient for the principle to retain its value. +Nor have the reasonings of Carnot perished on +this account; they were applied to an imperfect +conception of matter, but their form---\ie, the +essential part of them, remained correct. What +\PageSep{166} +I have just said throws some light at the same +time on the rôle of general principles, such as +those of the principle of least action or of the +conservation of energy. These principles are of +very great value. They were obtained in the +search for what there was in common in the +enunciation of numerous physical laws; they +thus represent the quintessence of innumerable +observations. However, from their very generality +results a consequence to which I have called +attention in \ChapRef{VIII}.---namely, that they are +no longer capable of verification. As we cannot +give a general definition of energy, the principle +of the conservation of energy simply signifies that +there is a \emph{something} which remains constant. +\Pagelabel{166}% +Whatever fresh notions of the world may be +given us by future experiments, we are certain +beforehand that there is something which remains +constant, and which may be called \emph{energy}. Does +this mean that the principle has no meaning and +vanishes into a tautology? Not at all. It means +that the different things to which we give the +name of \emph{energy} are connected by a true relationship; +it affirms between them a real relation. +But then, if this principle has a meaning, it may +be false; it may be that we have no right to +extend indefinitely its applications, and yet it is +certain beforehand to be verified in the strict +sense of the word. How, then, shall we know +when it has been extended as far as is legitimate? +Simply when it ceases to be useful to us---\ie, +\PageSep{167} +when we can no longer use it to predict correctly +new phenomena. We shall be certain in such a +case that the relation affirmed is no longer real, +for otherwise it would be fruitful; experiment +without directly contradicting a new extension of +the principle will nevertheless have condemned it. + +\Par{Physics and Mechanism.}---Most theorists have a +constant predilection for explanations borrowed +from physics, mechanics, or dynamics. Some +would be satisfied if they could account for all +phenomena by the motion of molecules attracting +one another according to certain laws. Others +are more exact: they would suppress attractions +acting at a distance; their molecules would follow +rectilinear paths, from which they would only be +deviated by impacts. Others again, such as Hertz, +suppress the forces as well, but suppose their +molecules subjected to geometrical connections +analogous, for instance, to those of articulated +systems; thus, they wish to reduce dynamics to a +kind of kinematics. In a word, they all wish to +bend nature into a certain form, and unless they +can do this they cannot be satisfied. Is Nature +flexible enough for this? + +We shall examine this question in \ChapRef{XII}., +\Foreign{àpropos} of Maxwell's theory. Every time that the +principles of least action and energy are satisfied, +we shall see that not only is there always a +mechanical explanation possible, but that there +is an unlimited number of such explanations. By +means of a well-known theorem due to Königs, +\PageSep{168} +it may be shown that we can explain everything +in an unlimited number of ways, by connections +after the manner of Hertz, or, again, by central +forces. No doubt it may be just as easily demonstrated +that everything may be explained by +simple impacts. For this, let us bear in mind +that it is not enough to be content with the +ordinary matter of which we are aware by means +of our senses, and the movements of which we +observe directly. We may conceive of ordinary +matter as either composed of atoms, whose internal +movements escape us, our senses being able to +estimate only the displacement of the whole; or +we may imagine one of those subtle fluids, which +under the name of \emph{ether} or other names, have +from all time played so important a rôle in +physical theories. Often we go further, and regard +the ether as the only primitive, or even as the +only true matter. The more moderate consider +ordinary matter to be condensed ether, and +there is nothing startling in this conception; but +others only reduce its importance still further, +and see in matter nothing more than the geometrical +locus of singularities in the ether. Lord +Kelvin, for instance, holds what we call matter +to be only the locus of those points at which the +ether is animated by vortex motions. Riemann +believes it to be locus of those points at which +ether is constantly destroyed; to Wiechert or +Larmor, it is the locus of the points at which +the ether has undergone a kind of torsion of a +\PageSep{169} +very particular kind. Taking any one of these +points of view, I ask by what right do we apply +to the ether the mechanical properties observed +in ordinary matter, which is but false matter? +The ancient fluids, caloric, electricity,~etc., were +abandoned when it was seen that heat is not +indestructible. But they were also laid aside +for another reason, In materialising them, their +individuality was, so to speak, emphasised---gaps +were opened between them; and these gaps had +to be filled in when the sentiment of the unity of +Nature became stronger, and when the intimate +relations which connect all the parts were perceived. +In multiplying the fluids, not only did +the ancient physicists create unnecessary entities, +but they destroyed real ties. It is not enough for +a theory not to affirm false relations; it must not +conceal true relations. + +Does our ether actually exist? We know the +origin of our belief in the ether. If light takes +several years to reach us from a distant star, it +is no longer on the star, nor is it on the earth. +It must be somewhere, and supported, so to speak, +by some material agency. + +The same idea may be expressed in a more +mathematical and more abstract form. What we +note are the changes undergone by the material +molecules. We see, for instance, that the photographic +plate experiences the consequences of a +phenomenon of which the incandescent mass of +a star was the scene several years before. Now, +\PageSep{170} +in ordinary mechanics, the state of the system +under consideration depends only on its state at +the moment immediately preceding; the system +therefore satisfies certain differential equations. +On the other hand, if we did not believe in the +ether, the state of the material universe would +depend not only on the state immediately preceding, +but also on much older states; the system +would satisfy equations of finite differences. The +ether was invented to escape this breaking down +of the laws of general mechanics. + +Still, this would only compel us to fill the +interplanetary space with ether, but not to +make it penetrate into the midst of the material +media. Fizeau's experiment goes further. By +the interference of rays which have passed +through the air or water in motion, it seems to +show us two different media penetrating each +other, and yet being displaced with respect to +each other. The ether is all but in our grasp. +Experiments can be conceived in which we come +closer still to it. Assume that Newton's principle +of the equality of action and \Chg{re-action}{reaction} is not true +if applied to matter \emph{alone}, and that this can be +proved. The geometrical sum of all the forces +applied to all the molecules would no longer be +zero. If we did not wish to change the whole of the +science of mechanics, we should have to introduce +the ether, in order that the action which matter +apparently undergoes should be counterbalanced +by the \Chg{re-action}{reaction} of matter on something. +\PageSep{171} + +Or again, suppose we discover that optical and +electrical phenomena are influenced by the motion +of the earth. It would follow that those phenomena +might reveal to us not only the relative +motion of material bodies, but also what would +seem to be their absolute motion. Again, it would +be necessary to have an ether in order that these +so-called absolute movements should not be their +displacements with respect to empty space, but +with respect to something concrete. + +Will this ever be accomplished? I do not +think so, and I shall explain why; and yet, it is +not absurd, for others have entertained this view. +For instance, if the theory of Lorentz, of which I +shall speak in more detail in \ChapRef{XIII}., were +true, Newton's principle would not apply to matter +\emph{alone}, and the difference would not be very far +from being within reach of experiment. On the +other hand, many experiments have been made +on the influence of the motion of the earth. The +results have always been negative. But if these +experiments have been undertaken, it is because +we have not been certain beforehand; and indeed, +according to current theories, the compensation +would be only approximate, and we might expect +to find accurate methods giving positive results. +I think that such a hope is illusory; it was none +the less interesting to show that a success of this +kind would, in a certain sense, open to us a new +world. + +And now allow me to make a digression; I +\PageSep{172} +must explain why I do not believe, in spite of +Lorentz, that more exact observations will ever +make evident anything else but the relative displacements +of material bodies. Experiments have +been made that should have disclosed the terms +of the first order; the results were nugatory. +Could that have been by chance? No one has +admitted this; a general explanation was sought, +and Lorentz found it. He showed that the terms +of the first order should cancel each other, but +not the terms of the second order. Then more +exact experiments were made, which were also +negative; neither could this be the result of +chance. An explanation was necessary, and was +forthcoming; they always are; hypotheses are +what we lack the least. But this is not enough. +Who is there who does not think that this leaves +to chance far too important a rôle? Would it +not also be a chance that this singular concurrence +should cause a certain circumstance to destroy the +terms of the first order, and that a totally different +but very opportune circumstance should cause +those of the second order to vanish? No; the +same explanation must be found for the two +cases, and everything tends to show that this +explanation would serve equally well for the +terms of the higher order, and that the mutual +destruction of these terms will be rigorous and +absolute. + +\Par{The Present State of Physics.}---Two opposite +tendencies may be distinguished in the history +\PageSep{173} +of the development of physics. On the one hand, +new relations are continually being discovered +between objects which seemed destined to remain +for ever unconnected; scattered facts cease to be +strangers to each other and tend to be marshalled +into an imposing synthesis. The march of science +is towards unity and simplicity. + +On the other hand, new phenomena are continually +being revealed; it will be long before +they can be assigned their place---sometimes it +may happen that to find them a place a corner of +the edifice must be demolished. In the same way, +we are continually perceiving details ever more +varied in the phenomena we know, where our +crude senses used to be unable to detect any lack +of unity. What we thought to be simple becomes +complex, and the march of science seems to be +towards diversity and complication. + +Here, then, are two opposing tendencies, each of +which seems to triumph in turn. Which will win? +If the first wins, science is possible; but nothing +proves this \Foreign{à~priori}, and it may be that after +unsuccessful efforts to bend Nature to our ideal of +unity in spite of herself, we shall be submerged by +the ever-rising flood of our new riches and compelled +to renounce all idea of classification---to +abandon our ideal, and to reduce science to the +mere recording of innumerable recipes. + +In fact, we can give this question no answer. +All that we can do is to observe the science of +to-day, and compare it with that of yesterday. +\PageSep{174} +No doubt after this examination we shall be in a +position to offer a few conjectures. + +Half-a-century ago hopes ran high indeed. The +unity of force had just been revealed to us by the +discovery of the conservation of energy and of its +transformation. This discovery also showed that +the phenomena of heat could be explained by +molecular movements. Although the nature of +these movements was not exactly known, no one +doubted but that they would be ascertained before +long. As for light, the work seemed entirely completed. +So far as electricity was concerned, there +was not so great an advance. Electricity had just +annexed magnetism. This was a considerable and +a definitive step towards unity. But how was +electricity in its turn to be brought into the +general unity, and how was it to be included in +the general universal mechanism? No one had +the slightest idea. As to the possibility of the inclusion, +all were agreed; they had faith. Finally, +as far as the molecular properties of material +bodies are concerned, the inclusion seemed easier, +but the details were very hazy. In a word, hopes +were vast and strong, but vague. + +To-day, what do we see? In the first place, a +step in advance---immense progress. The relations +between light and electricity are now known; the +three domains of light, electricity, and magnetism, +formerly separated, are now one; and this annexation +seems definitive. + +Nevertheless the conquest has caused us some +\PageSep{175} +sacrifices. Optical phenomena become particular +cases in electric phenomena; as long as the former +remained isolated, it was easy to explain them by +movements which were thought to be known in +all their details. That was easy enough; but any +explanation to be accepted must now cover the +whole domain of electricity. This cannot be done +without difficulty. + +The most satisfactory theory is that of Lorentz; +it is unquestionably the theory that best explains +the known facts, the one that throws into relief +the greatest number of known relations, the one in +which we find most traces of definitive construction. +That it still possesses a serious fault I +have shown above. It is in contradiction with +Newton's law that action and \Chg{re-action}{reaction} are equal +and opposite---or rather, this principle according +to Lorentz cannot be applicable to matter alone; +if it be true, it must take into account the action +of the ether on matter, and the \Chg{re-action}{reaction} of the +matter on the ether. Now, in the new order, it is +very likely that things do not happen in this way. + +However this may be, it is due to Lorentz that +the results of Fizeau on the optics of moving +bodies, the laws of normal and abnormal dispersion +and of absorption are connected with +each other and with the other properties of the +ether, by bonds which no doubt will not be +readily severed. Look at the ease with which the +new Zeeman phenomenon found its place, and +even aided the classification of Faraday's magnetic +\PageSep{176} +rotation, which had defied all Maxwell's efforts. +This facility proves that Lorentz's theory is not a +mere artificial combination which must eventually +find its solvent. It will probably have to be +modified, but not destroyed. + +The only object of Lorentz was to include in a +single whole all the optics and electro-dynamics +of moving bodies; he did not claim to give a +mechanical explanation. Larmor goes further; +keeping the essential part of Lorentz's theory, he +grafts upon it, so to speak, MacCullagh's ideas on +the direction of the movement of the ether. +MacCullagh held that the velocity of the ether +is the same in magnitude and direction as the +magnetic force. Ingenious as is this attempt, the +fault in Lorentz's theory remains, and is even +aggravated. According to Lorentz, we do not +know what the movements of the ether are; and +because we do not know this, we may suppose +them to be movements compensating those of +matter, and re-affirming that action and \Chg{re-action}{reaction} +are equal and opposite. According to Larmor +we know the movements of the ether, and we +can prove that the compensation does not take +place. + +If Larmor has failed, as in my opinion he has, +does it necessarily follow that a mechanical explanation +is impossible? Far from it. I said +above that as long as a phenomenon obeys the +two principles of energy and least action, so long +it allows of an unlimited number of mechanical +\PageSep{177} +explanations. And so with the phenomena of +optics and electricity. + +But this is not enough. For a mechanical +explanation to be good it must be simple; to +choose it from among all the explanations that are +possible there must be other reasons than the +necessity of making a choice. Well, we have no +theory as yet which will satisfy this condition and +consequently be of any use. Are we then to +complain? That would be to forget the end we +seek, which is not the mechanism; the true and +only aim is unity. + +We ought therefore to set some limits to +our ambition. Let us not seek to formulate a +mechanical explanation; let us be content to +show that we can always find one if we wish. In +this we have succeeded. The principle of the +conservation of energy has always been confirmed, +and now it has a fellow in the principle of least +action, stated in the form appropriate to physics. +This has also been verified, at least as far as +concerns the reversible phenomena which obey +Lagrange's equations---in other words, which obey +the most general laws of physics. The irreversible +phenomena are much more difficult to bring into +line; but they, too, are being co-ordinated and +tend to come into the unity. The light which +illuminates them comes from Carnot's principle. +For a long time thermo-dynamics was confined to +the study of the dilatations of bodies and of their +change of state. For some time past it has been +\PageSep{178} +growing bolder, and has considerably extended its +domain. We owe to it the theories of the voltaic +cell and of their thermo-electric phenomena; there +is not a corner in physics which it has not explored, +and it has even attacked chemistry itself. +The same laws hold good; everywhere, disguised +in some form or other, we find Carnot's principle; +everywhere also appears that eminently abstract +concept of entropy which is as universal as the +concept of energy, and like it, seems to conceal a +reality. It seemed that radiant heat must escape, +but recently that, too, has been brought under the +same laws. + +In this way fresh analogies are revealed which +may be often pursued in detail; electric resistance +resembles the viscosity of fluids; hysteresis would +rather be like the friction of solids. In all cases +friction appears to be the type most imitated by +the most diverse irreversible phenomena, and this +relationship is real and profound. + +A strictly mechanical explanation of these +phenomena has also been sought, but, owing to +their nature, it is hardly likely that it will be +found. To find it, it has been necessary to +suppose that the irreversibility is but apparent, that +the elementary phenomena are reversible and obey +the known laws of dynamics. But the elements +are extremely numerous, and become blended +more and more, so that to our crude sight all +appears to tend towards uniformity---\ie, all seems +to progress in the same direction, and that without +\PageSep{179} +hope of return. The apparent irreversibility is +therefore but an effect of the law of great numbers. +Only a being of infinitely subtle senses, such as +Maxwell's demon, could unravel this tangled skein +and turn back the course of the universe. + +This conception, which is connected with the +kinetic theory of gases, has cost great effort and +has not, on the whole, been fruitful; it may +become so. This is not the place to examine if it +leads to contradictions, and if it is in conformity +with the true nature of things. + +Let us notice, however, the original ideas of +M.~Gouy on the Brownian movement. According +to this scientist, this singular movement does not +obey Carnot's principle. The particles which it sets +moving would be smaller than the meshes of that +tightly drawn net; they would thus be ready to +separate them, and thereby to set back the course +of the universe. One can almost see Maxwell's +demon at work.\footnote + {Clerk-Maxwell imagined some supernatural agency at work, + sorting molecules in a gas of uniform temperature into (\textit{a})~those + possessing kinetic energy above the average, (\textit{b})~those possessing + kinetic energy below the average.\Transl} + +To resume, phenomena long known are gradually +being better classified, but new phenomena come +to claim their place, and most of them, like the +Zeeman effect, find it at once. Then we have the +cathode rays, the X-rays, uranium and radium +rays; in fact, a whole world of which none had +suspected the existence. How many unexpected +\PageSep{180} +guests to find a place for! No one can yet predict +the place they will occupy, but I do not believe +they will destroy the general unity: I think that +they will rather complete it. On the one hand, +indeed, the new radiations seem to be connected +with the phenomena of luminosity; not only do +they excite fluorescence, but they sometimes come +into existence under the same conditions as that +property; neither are they unrelated to the cause +which produces the electric spark under the action +of ultra-violet light. Finally, and most important +of all, it is believed that in all these phenomena +there exist ions, animated, it is true, with velocities +far greater than those of electrolytes. All this is +very vague, but it will all become clearer. + +Phosphorescence and the action of light on the +spark were regions rather isolated, and consequently +somewhat neglected by investigators. It is to be +hoped that a new path will now be made which +will facilitate their communications with the +rest of science. Not only do we discover new +phenomena, but those we think we know are +revealed in unlooked-for aspects. In the free ether +the laws preserve their majestic simplicity, but +matter properly so called seems more and more +complex; all we can say of it is but approximate, +and our formulæ are constantly requiring new +terms. + +But the ranks are unbroken, the relations that +we have discovered between objects we thought +simple still hold good between the same objects +\PageSep{181} +when their complexity is recognised, and that +alone is the important thing. Our equations +become, it is true, more and more complicated, so +as to embrace more closely the complexity of +nature; but nothing is changed in the relations +which enable these equations to be derived from +each other. In a word, the form of these equations +persists. Take for instance the laws of reflection. +Fresnel established them by a simple and attractive +theory which experiment seemed to confirm. Subsequently, +more accurate researches have shown +that this verification was but approximate; traces +of elliptic polarisation were detected everywhere. +But it is owing to the first approximation that the +cause of these anomalies was found in the existence +of a transition layer, and all the essentials of +Fresnel's theory have remained. We cannot help +reflecting that all these relations would never have +been noted if there had been doubt in the first +place as to the complexity of the objects they +connect. Long ago it was said: If Tycho had had +instruments ten times as precise, we would never +have had a Kepler, or a Newton, or Astronomy. +It is a misfortune for a science to be born too late, +when the means of observation have become too +perfect. That is what is happening at this moment +with respect to physical chemistry; the founders +are hampered in their general grasp by third and +fourth decimal places; happily they are men of +robust faith. As we get to know the properties +of matter better we see that continuity reigns. +\PageSep{182} +From the work of Andrews and Van~der~Waals, +we see how the transition from the liquid to the +gaseous state is made, and that it is not abrupt. +Similarly, there is no gap between the liquid and +solid states, and in the proceedings of a recent +Congress we see memoirs on the rigidity of liquids +side by side with papers on the flow of solids. + +With this tendency there is no doubt a loss of +simplicity. Such and such an effect was represented +by straight lines; it is now necessary to connect +these lines by more or less complicated curves. +On the other hand, unity is gained. Separate +categories quieted but did not satisfy the mind. + +Finally, a new domain, that of chemistry, has +been invaded by the method of physics, and we see +the birth of physical chemistry. It is still quite +young, but already it has enabled us to connect +such phenomena as electrolysis, osmosis, and the +movements of ions. + +From this cursory exposition what can we conclude? +Taking all things into account, we have +approached the realisation of unity. This has not +been done as quickly as was hoped fifty years ago, +and the path predicted has not always been +followed; but, on the whole, much ground has +been gained. +\PageSep{183} + + +\Chapter{XI.}{The Calculus of Probabilities.} + +\First{No} doubt the reader will be astonished to find +reflections on the calculus of probabilities in such +a volume as this. What has that calculus to do +with physical science? The questions I shall raise---without, +however, giving them a solution---are +naturally raised by the philosopher who is examining +the problems of physics. So far is this the case, +that in the two preceding chapters I have several +times used the words ``probability'' and ``chance.'' +``Predicted facts,'' as I said above, ``can only be +probable.'' However solidly founded a prediction +may appear to be, we are never absolutely +certain that experiment will not prove it false; but +the probability is often so great that practically +it may be accepted. And a little farther on I +added:---``See what a part the belief in simplicity +plays in our generalisations. We have verified a +simple law in a large number of particular cases, +and we refuse to admit that this so-often-repeated +coincidence is a mere effect of chance.'' Thus, in a +multitude of circumstances the physicist is often +in the same position as the gambler who reckons +up his chances. Every time that he reasons by +\PageSep{184} +induction, he more or less consciously requires the +calculus of probabilities, and that is why I am +obliged to open this chapter parenthetically, and to +interrupt our discussion of method in the physical +sciences in order to examine a little closer what this +calculus is worth, and what dependence we may +place upon it. The very name of the calculus of +probabilities is a paradox. Probability as opposed +to certainty is what one does not know, and how +can we calculate the unknown? Yet many eminent +scientists have devoted themselves to this calculus, +and it cannot be denied that science has drawn therefrom +no small advantage. How can we explain +this apparent contradiction? Has probability been +defined? Can it even be defined? And if it cannot, +how can we venture to reason upon it? The +definition, it will be said, is very simple. The +probability of an event is the ratio of the number +of cases favourable to the event to the total number +of possible cases. A simple example will show how +incomplete this definition is:---I throw two dice. +What is the probability that one of the two +at least turns up a~6? Each can turn up in six +different ways; the number of possible cases is +$6 × 6 = 36$. The number of favourable cases is~$11$; +the probability is~$\dfrac{11}{36}$. That is the correct solution. +But why cannot we just as well proceed as follows?---The +points which turn up on the two dice form +$\dfrac{6 × 7}{2} = 21$ different combinations. Among these +combinations, six are favourable; the probability +\PageSep{185} +is~$\dfrac{6}{21}$. Now why is the first method of calculating +the number of possible cases more legitimate than +the second? In any case it is not the definition +that tells us. We are therefore bound to complete +the definition by saying, ``\ldots to the total number +of possible cases, provided the cases are equally +probable.'' So we are compelled to define the +probable by the probable. How can we know +that two possible cases are equally probable? +Will it be by a convention? If we insert at the +beginning of every problem an explicit convention, +well and good! We then have nothing to do but to +apply the rules of arithmetic and algebra, and we +complete our calculation, when our result cannot +be called in question. But if we wish to make the +slightest application of this result, we must prove +that our convention is legitimate, and we shall find +ourselves in the presence of the very difficulty we +thought we had avoided. It may be said that +common-sense is enough to show us the convention +that should be adopted. Alas! M.~Bertrand has +amused himself by discussing the following simple +problem:---``What is the probability that a chord +of a circle may be greater than the side of the +inscribed equilateral triangle?'' The illustrious +geometer successively adopted two conventions +which seemed to be equally imperative in the eyes +of common-sense, and with one convention he finds~$\frac{1}{2}$, +and with the other~$\frac{1}{3}$. The conclusion which +seems to follow from this is that the calculus of +probabilities is a useless science, that the obscure +\PageSep{186} +instinct which we call common-sense, and to which +we appeal for the legitimisation of our conventions, +must be distrusted. But to this conclusion we can +no longer subscribe. We cannot do without that +obscure instinct. Without it, science would be +impossible, and without it we could neither discover +nor apply a law. Have we any right, for instance, +to enunciate Newton's law? No doubt numerous +observations are in agreement with it, but is not +that a simple fact of chance? and how do we know, +besides, that this law which has been true for so +many generations will not be untrue in the next? +To this objection the only answer you can give is: +It is very improbable. But grant the law. By +means of it I can calculate the position of Jupiter +in a year from now. Yet have I any right to say +this? Who can tell if a gigantic mass of enormous +velocity is not going to pass near the solar system +and produce unforeseen perturbations? Here +again the only answer is: It is very improbable. +From this point of view all the sciences would only +be unconscious applications of the calculus of probabilities. +And if this calculus be condemned, then +the whole of the sciences must also be condemned. +I shall not dwell at length on scientific problems +in which the intervention of the calculus of probabilities +is more evident. In the forefront of these +is the problem of interpolation, in which, knowing +a certain number of values of a function, we try +to discover the intermediary values. I may also +mention the celebrated theory of errors of observation, +\PageSep{187} +to which I shall return later; the kinetic +theory of gases, a well-known hypothesis wherein +each gaseous molecule is supposed to describe an +extremely complicated path, but in which, through +the effect of great numbers, the mean phenomena +which are all we observe obey the simple laws of +Mariotte and Gay-Lussac. All these theories are +based upon the laws of great numbers, and the +calculus of probabilities would evidently involve +them in its ruin. It is true that they have only a +particular interest, and that, save as far as interpolation +is concerned, they are sacrifices to which +we might readily be resigned. But I have said +above, it would not be these partial sacrifices that +would be in question; it would be the legitimacy +of the whole of science that would be challenged. +I quite see that it might be said: We do not know, +and yet we must act. As for action, we have not +time to devote ourselves to an inquiry that will +suffice to dispel our ignorance. Besides, such an +inquiry would demand unlimited time. We must +therefore make up our minds without knowing. +This must be often done whatever may happen, +and we must follow the rules although we may +have but little confidence in them. What I know +is, not that such a thing is true, but that the best +course for me is to act as if it were true. The +calculus of probabilities, and therefore science +itself, would be no longer of any practical value. + +Unfortunately the difficulty does not thus disappear. +A gambler wants to try a \Foreign{coup}, and he +\PageSep{188} +asks my advice. If I give it him, I use the +calculus of probabilities; but I shall not guarantee +success. That is what I shall call \emph{subjective probability}. +In this case we might be content with the +explanation of which I have just given a sketch. +But assume that an observer is present at the play, +that he knows of the \Foreign{coup}, and that play goes +on for a long time, and that he makes a summary +of his notes. He will find that events have +taken place in conformity with the laws of the +calculus of probabilities. That is what I shall call +\emph{objective probability}, and it is this phenomenon +which has to be explained. There are numerous +Insurance Societies which apply the rules of the +calculus of probabilities, and they distribute to +their shareholders dividends, the objective reality +of which cannot be contested. In order to explain +them, we must do more than invoke our ignorance +and the necessity of action. Thus, absolute scepticism +is not admissible. We may distrust, but we +cannot condemn \Foreign{en~bloc}. Discussion is necessary. + +\Par[I. ]{Classification of the Problems of Probability.}---In +order to classify the problems which are presented +to us with reference to probabilities, we must look at +them from different points of view, and first of all, +from that of \emph{generality}. I said above that probability +is the ratio of the number of favourable to +the number of possible cases. What for want of a +better term I call generality will increase with the +number of possible cases. This number may be +finite, as, for instance, if we take a throw of the +\PageSep{189} +dice in which the number of possible cases is~$36$. +That is the first degree of generality. But if we +ask, for instance, what is the probability that a +point within a circle is within the inscribed square, +there are as many possible cases as there are points +in the circle---that is to say, an infinite number. +This is the second degree of generality. Generality +can be pushed further still. We may ask the probability +that a function will satisfy a given condition. +There are then as many possible cases as one +can imagine different functions. This is the third +degree of generality, which we reach, for instance, +when we try to find the most probable law after a +finite number of observations. Yet we may place +ourselves at a quite different point of view. If we +were not ignorant there would be no probability, +there could only be certainty. But our ignorance +cannot be absolute, for then there would be no +longer any probability at all. Thus the problems +of probability may be classed according to the +greater or less depth of this ignorance. In mathematics +we may set ourselves problems in probability. +What is the probability that the fifth +decimal of a logarithm taken at random from a +table is a~$9$. There is no hesitation in answering +%[** TN: French edition uses a fraction] +that this probability is~\Reword{$1$-$10$th}{$\frac{1}{10}$}. Here we possess +all the data of the problem. We can calculate +our logarithm without having recourse to the +table, but we need not give ourselves the trouble. +This is the first degree of ignorance. In the +physical sciences our ignorance is already greater. +\PageSep{190} +The state of a system at a given moment depends +on two things---its initial state, and the law +according to which that state varies. If we know +both this law and this initial state, we have a +simple mathematical problem to solve, and we +fall back upon our first degree of ignorance. +Then it often happens that we know the law +and do not know the initial state. It may be +asked, for instance, what is the present distribution +of the minor planets? We know that from +all time they have obeyed the laws of Kepler, +but we do not know what was their initial distribution. +In the kinetic theory of gases we +assume that the gaseous molecules follow rectilinear +paths and obey the laws of impact and +elastic bodies; yet as we know nothing of their +initial velocities, we know nothing of their present +velocities. The calculus of probabilities alone +enables us to predict the mean phenomena which +will result from a combination of these velocities. +This is the second degree of ignorance. Finally +it is possible, that not only the initial conditions +but the laws themselves are unknown. We then +reach the third degree of ignorance, and in general +we can no longer affirm anything at all as to the +probability of a phenomenon. It often happens +that instead of trying to discover an event by +means of a more or less imperfect knowledge of +the law, the events may be known, and we want +to find the law; or that, instead of deducing +effects from causes, we wish to deduce the causes +\PageSep{191} +from the effects. Now, these problems are classified +as \emph{probability of causes}, and are the most interesting +of all from their scientific applications. I play at +\Foreign{écarté} with a gentleman whom I know to be perfectly +honest. What is the chance that he turns +up the king? It is~$\frac{1}{8}$. This is a problem of the +probability of effects. I play with a gentleman +whom I do not know. He has dealt ten times, +and he has turned the king up six times. What +is the chance that he is a sharper? This is a +problem in the probability of causes. It may be +said that it is the essential problem of the experimental +method. I have observed $n$~values of~$x$ +and the corresponding values of~$y$. I have found +that the ratio of the latter to the former is practically +constant. There is the event; what is +the cause? Is it probable that there is a general +law according to which $y$~would be proportional +to~$x$, and that small divergencies are due to errors +of observation? This is the type of question that +we are ever asking, and which we unconsciously +solve whenever we are engaged in scientific work. +I am now going to pass in review these different +categories of problems by discussing in succession +what I have called subjective and objective probability. + +\Par[II. ]{Probability in Mathematics.}---The impossibility +of squaring the circle was shown in~1885, but +before that date all geometers considered this impossibility +as so ``probable'' that the Académie des +Sciences rejected without examination the, alas!\ +\PageSep{192} +too numerous memoirs on this subject that a +few unhappy madmen sent in every year. Was +the Académie wrong? Evidently not, and it +knew perfectly well that by acting in this +manner it did not run the least risk of stifling +a discovery of moment. The Académie could +not have proved that it was right, but it knew +quite well that its instinct did not deceive it. +If you had asked the Academicians, they would +have answered: ``We have compared the probability +that an unknown scientist should have +found out what has been vainly sought for so +long, with the probability that there is one madman +the more on the earth, and the latter has +appeared to us the greater.'' These are very +good reasons, but there is nothing mathematical +about them; they are purely psychological. If +you had pressed them further, they would have +added: ``Why do you expect a particular value of +a transcendental function to be an algebraical +number; if $\pi$~be the root of an algebraical equation, +why do you expect this root to be a period of +%[** TN: sin italicized in the original] +the function~$\sin 2x$, and why is it not the same +with the other roots of the same equation?'' To +sum up, they would have invoked the principle of +sufficient reason in its vaguest form. Yet what +information could they draw from it? At most a +rule of conduct for the employment of their time, +which would be more usefully spent at their +ordinary work than in reading a lucubration +that inspired in them a legitimate distrust. But +\PageSep{193} +what I called above objective probability has +nothing in common with this first problem. It is +otherwise with the second. Let us consider the +first $10,000$ logarithms that we find in a table. +Among these $10,000$ logarithms I take one at +random. What is the probability that its third +decimal is an even number? You will say without +any hesitation that the probability is~$\frac{1}{2}$, and in +fact if you pick out in a table the third decimals +in these $10,000$ numbers you will find nearly as +many even digits as odd. Or, if you prefer it, let +us write $10,000$ numbers corresponding to our +$10,000$ logarithms, writing down for each of these +numbers $+1$~if the third decimal of the corresponding +logarithm is even, and $-1$~if odd; and then +let us take the mean of these $10,000$ numbers. I +do not hesitate to say that the mean of these +$10,000$ units is probably zero, and if I were to +calculate it practically, I would verify that it is +extremely small. But this verification is needless. +I might have rigorously proved that this mean is +smaller than~$0.003$. To prove this result I should +have had to make a rather long calculation for +which there is no room here, and for which I +may refer the reader to an article that I published +in the \Title{Revue générale des Sciences}, April~15th, +1899. The only point to which I wish to +draw attention is the following. In this calculation +I had occasion to rest my case on only two +facts---namely, that the first and second derivatives +of the logarithm remain, in the interval considered, +\PageSep{194} +between certain limits. Hence our first conclusion +is that the property is not only true of the +logarithm but of any continuous function whatever, +since the derivatives of every continuous +function are limited. If I was certain beforehand +of the result, it is because I have often observed +analogous facts for other continuous functions; and +next, it is because I went through in my mind in +a more or less unconscious and imperfect manner +the reasoning which led me to the preceding inequalities, +just as a skilled calculator before finishing +his multiplication takes into account what it +ought to come to approximately. And besides, +since what I call my intuition was only an incomplete +summary of a piece of true reasoning, it is +clear that observation has confirmed my predictions, +and that the objective and subjective probabilities +are in agreement. As a third example I shall +choose the following:---The number~$u$ is taken at +random and $n$~is a given very large integer. What +is the mean value of~$\sin nu$? This problem has +no meaning by itself. To give it one, a convention +is required---namely, we agree that the probability +for the number~$u$ to lie between $a$~and~$a + da$ is +$\phi(a)\, da$; that it is therefore proportional to the +infinitely small interval~$da$, and is equal to this +multiplied by a function~$\phi(a)$, only depending +on~$a$. As for this function I choose it arbitrarily, +but I must assume it to be continuous. The value +of~$\sin nu$ remaining the same when $u$~increases by~$2\pi$, +I may without loss of generality assume that +\PageSep{195} +$u$~lies between $0$~and~$2\pi$, and I shall thus be +led to suppose that $\phi(a)$~is a periodic function +whose period is~$2\pi$. The mean value that we +seek is readily expressed by a simple integral, +and it is easy to show that this integral is smaller +than +%[** TN: Expression displayed in the French edition] +\[ +\frac{2\pi M_{K}}{n^{K}}, +\] +$M_{K}$~being the maximum value of the +$K$th~derivative of~$\phi(u)$. We see then that if the +$K$th~derivative is finite, our mean value will +tend towards zero when $n$~increases indefinitely, +and that more rapidly than~$\dfrac{1}{n^{K+1}}$. + +%[** TN: Paragraph break in the French edition] +The mean +value of~$\sin nu$ when $n$~is very large is therefore +zero. To define this value I required a convention, +but the result remains the same \emph{whatever +that convention may be}. I have imposed upon +myself but slight restrictions when I assumed that +the function~$\phi(a)$ is continuous and periodic, and +these hypotheses are so natural that we may ask +ourselves how they can be escaped. Examination +of the three preceding examples, so different in all +respects, has already given us a glimpse on the +one hand of the rôle of what philosophers call the +principle of sufficient reason, and on the other hand +of the importance of the fact that certain properties +are common to all continuous functions. +The study of probability in the physical sciences +will lead us to the same result. + +\Par[III. ]{Probability in the Physical Sciences.}---We +now come to the problems which are connected +with what I have called the second degree of +\PageSep{196} +ignorance---namely, those in which we know the +law but do not know the initial state of the +system. I could multiply examples, but I shall +take only one. What is the probable present +distribution of the minor planets on the zodiac? +We know they obey the laws of Kepler. We may +even, without changing the nature of the problem, +suppose that their orbits are circular and situated +in the same plane, a plane which we are given. +On the other hand, we know absolutely nothing +about their initial distribution. However, we do +not hesitate to affirm that this distribution is now +nearly uniform. Why? Let $b$~be the longitude +of a minor planet in the initial epoch---that is to +say, the epoch zero. Let $a$~be its mean motion. +Its longitude at the present time---\ie, at the time~$t$ +will be~$at + b$. To say that the present distribution +is uniform is to say that the mean value of +the sines and cosines of multiples of~$at + b$ is zero. +Why do we assert this? Let us represent our +minor planet by a point in a plane---namely, the +point whose co-ordinates are $a$~and~$b$. All these +representative points will be contained in a certain +region of the plane, but as they are very numerous +this region will appear dotted with points. We +know nothing else about the distribution of the +points. Now what do we do when we apply the +calculus of probabilities to such a question as +this? What is the probability that one or more +representative points may be found in a certain +portion of the plane? In our ignorance we are +\PageSep{197} +compelled to make an arbitrary hypothesis. To +explain the nature of this hypothesis I may be +allowed to use, instead of a mathematical formula, +a crude but concrete image. Let us suppose +that over the surface of our plane has been +spread imaginary matter, the density of which is +variable, but varies continuously. We shall then +agree to say that the probable number of representative +points to be found on a certain portion +of the plane is proportional to the quantity of +this imaginary matter which is found there. If +there are, then, two regions of the plane of the +same extent, the probabilities that a representative +point of one of our minor planets is in one or +other of these regions will be as the mean densities +of the imaginary matter in one or other of the +regions. Here then are two distributions, one +real, in which the representative points are very +numerous, very close together, but discrete like the +molecules of matter in the atomic hypothesis; the +other remote from reality, in which our representative +points are replaced by imaginary continuous +matter. We know that the latter cannot be real, +but we are forced to adopt it through our ignorance. +If, again, we had some idea of the real distribution +of the representative points, we could arrange it so +that in a region of some extent the density of this +imaginary continuous matter may be nearly proportional +to the number of representative points, +or, if it is preferred, to the number of atoms which +are contained in that region. Even that is impossible, +\PageSep{198} +and our ignorance is so great that we are +forced to choose arbitrarily the function which +defines the density of our imaginary matter. We +shall be compelled to adopt a hypothesis from +which we can hardly get away; we shall suppose +that this function is continuous. That is +sufficient, as we shall see, to enable us to reach our +conclusion. + +What is at the instant~$t$ the probable distribution +of the minor planets---or rather, what is the +mean value of the sine of the longitude at the +moment~$t$---\ie, of $\sin(at + b)$? We made at the +outset an arbitrary convention, but if we adopt it, +this probable value is entirely defined. Let us +decompose the plane into elements of surface. +Consider the value of $\sin(at + b)$ at the centre of +each of these elements. Multiply this value by the +surface of the element and by the corresponding +density of the imaginary matter. Let us then take +the sum for all the elements of the plane. This +sum, by definition, will be the probable mean +value we seek, which will thus be expressed by a +double integral. It may be thought at first that +this mean value depends on the choice of the +function~$\phi$ which defines the density of the imaginary +matter, and as this function~$\phi$ is arbitrary, we +can, according to the arbitrary choice which we +make, obtain a certain mean value. But this is +not the case. A simple calculation shows us that +our double integral decreases very rapidly as $t$~increases. +Thus, I cannot tell what hypothesis to +\PageSep{199} +make as to the probability of this or that initial +distribution, but when once the hypothesis is +made the result will be the same, and this gets +me out of my difficulty. Whatever the function~$\phi$ +may be, the mean value tends towards zero +as $t$~increases, and as the minor planets have +certainly accomplished a very large number of +revolutions, I may assert that this mean value is +very small. I may give to~$\phi$ any value I choose, +with one restriction: this function must be continuous; +and, in fact, from the point of view of +subjective probability, the choice of a discontinuous +function would have been unreasonable. What +reason could I have, for instance, for supposing +that the initial longitude might be exactly~$0°$, but +that it could not lie between $0°$~and~$1°$? + +The difficulty reappears if we look at it from the +point of view of objective probability; if we pass +from our imaginary distribution in which the supposititious +matter was assumed to be continuous, +to the real distribution in which our representative +points are formed as discrete atoms. The mean +value of $\sin(at + b)$ will be represented quite +simply by +\[ +\frac{1}{n} \sum \sin(at + b), +\] +$n$~being the number of minor planets. Instead of +a double integral referring to a continuous +function, we shall have a sum of discrete terms. +However, no one will seriously doubt that this +mean value is practically very small. Our representative +\PageSep{200} +points being very close together, our +discrete sum will in general differ very little from +an integral. An integral is the limit towards +which a sum of terms tends when the number of +these terms is indefinitely increased. If the terms +are very numerous, the sum will differ very little +from its limit---that is to say, from the integral, +and what I said of the latter will still be true of +the sum itself. But there are exceptions. If, for +instance, for all the minor planets $b = \dfrac{\pi}{2} - at$, the +longitude of all the planets at the time~$t$ would be~$\dfrac{\pi}{2}$, +and the mean value in question would be +evidently unity. For this to be the case at the +time~$0$, the minor planets must have all been +lying on a kind of spiral of peculiar form, with +its spires very close together. All will admit that +such an initial distribution is extremely improbable +(and even if it were realised, the distribution +would not be uniform at the present time---for +example, on the 1st~January 1900; but it would +become so a few years later). Why, then, do we +think this initial distribution improbable? This +must be explained, for if we are wrong in rejecting +as improbable this absurd hypothesis, our inquiry +breaks down, and we can no longer affirm anything +on the subject of the probability of this or +that present distribution. Once more we shall +invoke the principle of sufficient reason, to which +we must always recur. We might admit that at +the beginning the planets were distributed almost +\PageSep{201} +in a straight line. We might admit that they +were irregularly distributed. But it seems to us +that there is no sufficient reason for the unknown +cause that gave them birth to have acted along a +curve so regular and yet so complicated, which +would appear to have been expressly chosen so +that the distribution at the present day would not +be uniform. + +\Par[IV. ]{Rouge et Noir.}---The questions raised by +games of chance, such as roulette, are, fundamentally, +quite analogous to those we have just +%[** TN: "est partagé en un grand mombre de subdivisions égales"] +treated. For example, a wheel is divided into \Reword{thirty-seven}{a large number of} +equal compartments, alternately red and +black. A ball is spun round the wheel, and after +having moved round a number of times, it stops in +front of one of these sub-divisions. The probability +that the division is red is obviously~$\frac{1}{2}$. The needle +describes an angle~$\theta$, including several complete +revolutions. I do not know what is the probability +that the ball is spun with such a force that +this angle should lie between $\theta$~and~$\theta + d\theta$, but I +can make a convention. I can suppose that this +probability is~$\phi(\theta)\, d\theta$. As for the function~$\phi(\theta)$, I +can choose it in an entirely arbitrary manner. I +have nothing to guide me in my choice, but I am +naturally induced to suppose the function to be +continuous. Let $\epsilon$~be a length (measured on the +circumference of the circle of radius unity) of each +red and black compartment. We have to calculate +the integral of~$\phi(\theta)\, d\theta$, extending it on the one +hand to all the red, and on the other hand to all +\PageSep{202} +the black compartments, and to compare the +results. Consider an interval~$2\epsilon$ comprising two +consecutive red and black compartments. Let +$M$~and~$m$ be the maximum and minimum values of +the function~$\phi(\theta)$ in this interval. The integral +extended to the red compartments will be smaller +than~$\sum M\epsilon$; extended to the black it will be greater +than~$\sum m\epsilon$. The difference will therefore be +smaller than $\sum (M - m)\epsilon$. But if the function~$\phi$ is +supposed continuous, and if on the other hand the +interval~$\epsilon$ is very small with respect to the total +angle described by the needle, the difference~$M - m$ +will be very small. The difference of the two +integrals will be therefore very small, and the +probability will be very nearly~$\frac{1}{2}$. We see that +without knowing anything of the function~$\phi$ we +must act as if the probability were~$\frac{1}{2}$. And on +the other hand it explains why, from the +objective point of view, if I watch a certain +number of \Foreign{coups}, observation will give me almost +as many black \Foreign{coups} as red. All the players +know this objective law; but it leads them into a +remarkable error, which has often been exposed, +but into which they are always falling. When +the red has won, for example, six times running, +they bet on black, thinking that they are playing +an absolutely safe game, because they say it is +a very rare thing for the red to win seven times +running. In reality their probability of winning +is still~$\frac{1}{2}$. Observation shows, it is true, that +the series of seven consecutive reds is very rare, +\PageSep{203} +but series of six reds followed by a black are +also very rare. They have noticed the rarity of +the series of seven reds; if they have not remarked +the rarity of six reds and a black, it is only +because such series strike the attention less. + +\Par[V. ]{The Probability of Causes.}---We now come to +the problems of the probability of causes, the +most important from the point of view of +scientific applications. Two stars, for instance, +are very close together on the celestial sphere. Is +this apparent contiguity a mere effect of chance? +Are these stars, although almost on the same +visual ray, situated at very different distances +from the earth, and therefore very far indeed from +one another? or does the apparent correspond +to a real contiguity? This is a problem on the +probability of causes. + +First of all, I recall that at the outset of all +problems of probability of effects that have +occupied our attention up to now, we have had +to use a convention which was more or less +justified; and if in most cases the result was to +a certain extent independent of this convention, +it was only the condition of certain hypotheses +which enabled us \Foreign{à~priori} to reject discontinuous +functions, for example, or certain absurd conventions. +We shall again find something +analogous to this when we deal with the probability +of causes. An effect may be produced +by the cause~$a$ or by the cause~$b$. The effect +has just been observed. We ask the probability +\PageSep{204} +that it is due to the cause~$a$. This is an \Foreign{à~posteriori} +probability of cause. But I could not +calculate it, if a convention more or less justified +did not tell me in advance what is the \Foreign{à~priori} +probability for the cause~$a$ to come into play---I +mean the probability of this event to some one +who had not observed the effect. To make my +meaning clearer, I go back to the game of \Foreign{écarté} +mentioned before. My adversary deals for the +first time and turns up a king. What is the +probability that he is a sharper? The formulæ +ordinarily taught give~$\frac{8}{9}$, a result which is +obviously rather surprising. If we look at it +closer, we see that the conclusion is arrived at +as if, before sitting down at the table, I had +considered that there was one chance in two +that my adversary was not honest. An absurd +hypothesis, because in that case I should certainly +not have played with him; and this explains the +absurdity of the conclusion. The function on +the \Foreign{à~priori} probability was unjustified, and that +is why the conclusion of the \Foreign{à~posteriori} probability +led me into an inadmissible result. The importance +of this preliminary convention is obvious. +I shall even add that if none were made, the +problem of the \Foreign{à~posteriori} probability would have +no meaning. It must be always made either +explicitly or tacitly. + +Let us pass on to an example of a more +scientific character. I require to determine an +experimental law; this law, when discovered, can +\PageSep{205} +be represented by a curve. I make a certain +number of isolated observations, each of which +may be represented by a point. When I have +obtained these different points, I draw a curve +between them as carefully as possible, giving +my curve a regular form, avoiding sharp angles, +accentuated inflexions, and any sudden variation +of the radius of curvature. This curve will represent +to me the probable law, and not only will +it give me the values of the functions intermediary +to those which have been observed, but it also +gives me the observed values more accurately +than direct observation does; that is why I make +the curve pass near the points and not through +the points themselves. + +Here, then, is a problem in the probability of +causes. The effects are the measurements I have +recorded; they depend on the combination of two +causes---the true law of the phenomenon and errors +of observation. Knowing the effects, we have to +find the probability that the phenomenon shall +obey this law or that, and that the observations +have been accompanied by this or that error. +The most probable law, therefore, corresponds to +the curve we have traced, and the most probable +error is represented by the distance of the corresponding +point from that curve. But the +problem has no meaning if before the observations +I had an \Foreign{à~priori} idea of the probability of +this law or that, or of the chances of error to +which I am exposed. If my instruments are +\PageSep{206} +good (and I knew whether this is so or not before +beginning the observations), I shall not draw the +curve far from the points which represent the +rough measurements. If they are inferior, I may +draw it a little farther from the points, so that I +may get a less sinuous curve; much will be sacrificed +to regularity. + +Why, then, do I draw a curve without sinuosities? +Because I consider \Foreign{à~priori} a law +represented by a continuous function (or function +the derivatives of which to a high order are small), +as more probable than a law not satisfying those +conditions. But for this conviction the problem +would have no meaning; interpolation would be +impossible; no law could be deduced from a +finite number of observations; science would +cease to exist. + +Fifty years ago physicists considered, other +things being equal, a simple law as more probable +than a complicated law. This principle was even +invoked in favour of Mariotte's law as against +that of Regnault. But this belief is now +repudiated; and yet, how many times are we +compelled to act as though we still held it! +However that may be, what remains of this +tendency is the belief in continuity, and as we +have just seen, if the belief in continuity were +to disappear, experimental science would become +impossible. + +\Par[VI. ]{The Theory of Errors.}---We are thus brought +to consider the theory of errors which is directly +\PageSep{207} +connected with the problem of the probability +of causes. Here again we find \emph{effects}---to wit, +a certain number of irreconcilable observations, +and we try to find the \emph{causes} which are, on the +one hand, the true value of the quantity to be +measured, and, on the other, the error made in +each isolated observation. We must calculate +the probable \Foreign{à~posteriori} value of each error, and +therefore the probable value of the quantity to be +measured. But, as I have just explained, we +cannot undertake this calculation unless we admit +\Foreign{à~priori}---\ie, before any observations are made---that +there is a law of the probability of errors. +Is there a law of errors? The law to which +all calculators assent is Gauss's law, that is +represented by a certain transcendental curve +known as the ``bell.'' + +But it is first of all necessary to recall +the classic distinction between systematic and +accidental errors. If the metre with which we +measure a length is too long, the number we get +will be too small, and it will be no use to measure +several times---that is a systematic error. If we +measure with an accurate metre, we may make a +mistake, and find the length sometimes too large +and sometimes too small, and when we take the +mean of a large number of measurements, +the error will tend to grow small. These are +accidental errors. + +It is clear that systematic errors do not satisfy +Gauss's law, but do accidental errors satisfy it? +\PageSep{208} +Numerous proofs have been attempted, almost all +of them crude paralogisms. But starting from +the following hypotheses we may prove Gauss's +law: the error is the result of a very large number +of partial and independent errors; each partial +error is very small and obeys any law of probability +whatever, provided the probability of a +positive error is the same as that of an equal +negative error. It is clear that these conditions +will be often, but not always, fulfilled, and we +may reserve the name of accidental for errors +which satisfy them. + +We see that the method of least squares is not +legitimate in every case; in general, physicists +are more distrustful of it than astronomers. This +is no doubt because the latter, apart from the +systematic errors to which they and the physicists +are subject alike, have to contend with an +extremely important source of error which is +entirely accidental---I mean atmospheric undulations. +So it is very curious to hear a discussion +between a physicist and an astronomer about a +method of observation. The physicist, persuaded +that one good measurement is worth more than +many bad ones, is pre-eminently concerned with +the elimination by means of every precaution of +the final systematic errors; the astronomer retorts: +``But you can only observe a small number of stars, +and accidental errors will not disappear.'' + +What conclusion must we draw? Must we +continue to use the method of least squares? +\PageSep{209} +We must distinguish. We have eliminated all +the systematic errors of which we have any +suspicion; we are quite certain that there are +others still, but we cannot detect them; and yet +we must make up our minds and adopt a definitive +value which will be regarded as the probable +value; and for that purpose it is clear that the +best thing we can do is to apply Gauss's law. +We have only applied a practical rule referring +to subjective probability. And there is no more +to be said. + +Yet we want to go farther and say that not +only the probable value is so much, but that the +probable error in the result is so much. \emph{This +is absolutely invalid}: it would be true only if +we were sure that all the systematic errors +were eliminated, and of that we know absolutely +nothing. We have two series of observations; by +applying the law of least squares we find that the +probable error in the first series is twice as small +as in the second. The second series may, however, +be more accurate than the first, because the +first is perhaps affected by a large systematic +error. All that we can say is, that the first series +is \emph{probably} better than the second because its +accidental error is smaller, and that we have no +reason for affirming that the systematic error is +greater for one of the series than for the other, +our ignorance on this point being absolute. + +\Par[VII. ]{Conclusions.}---In the preceding lines I have +set several problems, and have given no solution. +\PageSep{210} +I do not regret this, for perhaps they will invite +the reader to reflect on these delicate questions. + +However that may be, there are certain points +which seem to be well established. To undertake +the calculation of any probability, and even for +that calculation to have any meaning at all, we +must admit, as a point of departure, an hypothesis +or convention which has always something +arbitrary about it. In the choice of this convention +we can be guided only by the principle +of sufficient reason. Unfortunately, this principle +is very vague and very elastic, and in the cursory +examination we have just made we have seen it +assume different forms. The form under which +we meet it most often is the belief in continuity, +a belief which it would be difficult to justify by +apodeictic reasoning, but without which all science +would be impossible. Finally, the problems to +which the calculus of probabilities may be applied +with profit are those in which the result is independent +of the hypothesis made at the outset, +provided only that this hypothesis satisfies the +condition of continuity. +\PageSep{211} + + +\Chapter{XII.\protect\footnotemark}{Optics And Electricity.} +\footnotetext{This chapter is mainly taken from the prefaces of two of my + books---\Title{Théorie Mathématique de la lumière} (Paris: Naud, 1889), + and \Title{Électricité et Optique} (Paris: Naud, 1901).} + +\Par{Fresnel's Theory.}---The best example that can be +chosen is the theory of light and its relations +to the theory of electricity. It is owing to Fresnel +that the science of optics is more advanced than +any other branch of physics. The theory called the +theory of undulations forms a complete whole, +which is satisfying to the mind; but we must +not ask from it what it cannot give us. The +object of mathematical theories is not to reveal +to us the real nature of things; that would be +an unreasonable claim. Their only object is to +co-ordinate the physical laws with which physical +experiment makes us acquainted, the enunciation +of which, without the aid of mathematics, we +should be unable to effect. Whether the ether +exists or not matters little---let us leave that to +the metaphysicians; what is essential for us is, that +everything happens as if it existed, and that this +hypothesis is found to be suitable for the explanation +of phenomena. After all, have we any other +\PageSep{212} +reason for believing in the existence of material +objects? That, too, is only a convenient hypothesis; +only, it will never cease to be so, while some day, +no doubt, the ether will be thrown aside as useless. + +But at the present moment the laws of optics, +and the equations which translate them into the +language of analysis, hold good---at least as a first +approximation. It will therefore be always useful +to study a theory which brings these equations +into connection. + +The undulatory theory is based on a molecular +hypothesis; this is an advantage to those who +think they can discover the cause under the law. +But others find in it a reason for distrust; and +this distrust seems to me as unfounded as the +illusions of the former. These hypotheses play +but a secondary rôle. They may be sacrificed, +and the sole reason why this is not generally done +is, that it would involve a certain loss of lucidity +in the explanation. In fact, if we look at it a +little closer we shall see that we borrow from +molecular hypotheses but two things---the principle +of the conservation of energy, and the linear form +of the equations, which is the general law of small +movements as of all small variations. This explains +why most of the conclusions of Fresnel +remain unchanged when we adopt the electro-magnetic +theory of light. + +\Par{Maxwell's Theory.}---We all know that it was +Maxwell who connected by a slender tie two +branches of physics---optics and electricity---until +\PageSep{213} +then unsuspected of having anything in common. +Thus blended in a larger aggregate, in a higher +harmony, Fresnel's theory of optics did not perish. +Parts of it are yet alive, and their mutual relations +are still the same. Only, the language which we +use to express them has changed; and, on the +other hand, Maxwell has revealed to us other +relations, hitherto unsuspected, between the +different branches of optics and the domain of +electricity. + +\Pagelabel{213}% +The first time a French reader opens Maxwell's +book, his admiration is tempered with a feeling of +uneasiness, and often of distrust. + +It is only after prolonged study, and at the cost +of much effort, that this feeling disappears. Some +minds of high calibre never lose this feeling. Why +is it so difficult for the ideas of this English +scientist to become acclimatised among us? No +doubt the education received by most enlightened +Frenchmen predisposes them to appreciate precision +and logic more than any other qualities. +In this respect the old theories of mathematical +physics gave us complete satisfaction. All our +masters, from Laplace to Cauchy, proceeded along +the same lines. Starting with clearly enunciated +hypotheses, they deduced from them all their +consequences with mathematical rigour, and then +compared them with experiment. It seemed to +be their aim to give to each of the branches +of physics the same precision as to celestial +mechanics. +\PageSep{214} + +A mind accustomed to admire such models is +not easily satisfied with a theory. Not only will +it not tolerate the least appearance of contradiction, +but it will expect the different parts to be +logically connected with one another, and will +require the number of hypotheses to be reduced +to a minimum. + +This is not all; there will be other demands +which appear to me to be less reasonable. Behind +the matter of which our senses are aware, and +which is made known to us by experiment, such +a thinker will expect to see another kind of matter---the +only true matter in its opinion---which will +no longer have anything but purely geometrical +qualities, and the atoms of which will be mathematical +points subject to the laws of dynamics +alone. And yet he will try to represent to +himself, by an unconscious contradiction, these +invisible and colourless atoms, and therefore +to bring them as close as possible to ordinary +matter. + +Then only will he be thoroughly satisfied, and +he will then imagine that he has penetrated the +secret of the universe. Even if the satisfaction is +fallacious, it is none the less difficult to give it up. +Thus, on opening the pages of Maxwell, a Frenchman +expects to find a theoretical whole, as logical +and as precise as the physical optics that is founded +on the hypothesis of the ether. He is thus preparing +for himself a disappointment which I +should like the reader to avoid; so I will warn +\PageSep{215} +him at once of what he will find and what he will +not find in Maxwell. + +Maxwell does not give a mechanical explanation +of electricity and magnetism; he confines himself +to showing that such an explanation is possible. +He shows that the phenomena of optics are only +a particular case of electro-magnetic phenomena. +From the whole theory of electricity a theory of +light can be immediately deduced. Unfortunately +the converse is not true; it is not always easy to +find a complete explanation of electrical phenomena. +In particular it is not easy if we take +as our starting-point Fresnel's theory; to do so, +no doubt, would be impossible; but none the less +we must ask ourselves if we are compelled to +surrender admirable results which we thought we +had definitively acquired. That seems a step +backwards, and many sound intellects will not +willingly allow of this. + +Should the reader consent to set some bounds +to his hopes, he will still come across other +difficulties. The English scientist does not try +to erect a unique, definitive, and well-arranged +building; he seems to raise rather a large number +of provisional and independent constructions, +between which communication is difficult and +sometimes impossible. Take, for instance, the +chapter in which \Chg{electrostatic}{electro-static} attractions are +explained by the pressures and tensions of the +dielectric medium. This chapter might be suppressed +without the rest of the book being +\PageSep{216} +thereby less clear or less complete, and yet +it contains a theory which is self-sufficient, and +which can be understood without reading a +word of what precedes or follows. But it is +not only independent of the rest of the book; it +is difficult to reconcile it with the fundamental +ideas of the volume. Maxwell does not even +attempt to reconcile it; he merely says: ``I have +not been able to make the next step---namely, to +account by mechanical considerations for these +stresses in the dielectric.'' + +This example will be sufficient to show what +I mean; I could quote many others. Thus, who +would suspect on reading the pages devoted to +magnetic rotatory polarisation that there is an +identity between optical and magnetic phenomena? + +We must not flatter ourselves that we have +avoided every contradiction, but we ought to +make up our minds. Two contradictory theories, +provided that they are kept from overlapping, and +that we do not look to find in them the explanation +of things, may, in fact, be very useful instruments +of research; and perhaps the reading of +Maxwell would be less suggestive if he had not +opened up to us so many new and divergent ways. +But the fundamental idea is masked, as it were. +So far is this the case, that in most works that are +popularised, this idea is the only point which is +left completely untouched. To show the importance +of this, I think I ought to explain in what this +\PageSep{217} +fundamental idea consists; but for that purpose +a short digression is necessary. + +\Par{The Mechanical Explanation of Physical Phenomena.}---In +every physical phenomenon there is a certain +number of parameters which are reached directly +by experiment, and which can be measured. I +shall call them the parameters~$q$. Observation +next teaches us the laws of the variations of these +parameters, and these laws can be generally stated +in the form of differential equations which connect +together the parameters~$q$ and time. What can +be done to give a mechanical interpretation to +such a phenomenon? We may endeavour to +explain it, either by the movements of ordinary +matter, or by those of one or more hypothetical +fluids. These fluids will be considered as formed +of a very large number of isolated molecules~$m$. +When may we say that we have a complete +mechanical explanation of the phenomenon? It +will be, on the one hand, when we know the +differential equations which are satisfied by the +co-ordinates of these hypothetical molecules~$m$, +equations which must, in addition, conform to the +laws of dynamics; and, on the other hand, when we +know the relations which define the co-ordinates +of the molecules~$m$ as functions of the parameters~$q$, +attainable by experiment. These equations, as +I have said, should conform to the principles of +dynamics, and, in particular, to the principle of +the conservation of energy, and to that of least +action. +\PageSep{218} + +The first of these two principles teaches us that +the total energy is constant, and may be divided +into two parts:\Add{---} + +(1) Kinetic energy, or \Foreign{vis~viva}, which depends +on the masses of the hypothetical molecules~$m$, +and on their velocities. This I shall call~$T$. (2)~The +potential energy which depends only on the +co-ordinates of these molecules, and this I shall +call~$U$. It is the sum of the energies $T$~and~$U$ that +is constant. + +Now what are we taught by the principle of +least action? It teaches us that to pass from the +initial position occupied at the instant~$t_{0}$ to +the final position occupied at the instant~$t_{1}$, the +system must describe such a path that in the +interval of time between the instant $t_{0}$~and~$t_{1}$, +the mean value of the action---\ie, the \emph{difference} +between the two energies $T$~and~$U$, must be as +small as possible. The first of these two principles +is, moreover, a consequence of the second. If we +know the functions $T$~and~$U$, this second principle +is sufficient to determine the equations of motion. + +Among the paths which enable us to pass from +one position to another, there is clearly one for +which the mean value of the action is smaller than +for all the others. In addition, there is only\Typo{ }{ one} such +path; and it follows from this, that the principle +of least action is sufficient to determine the path +followed, and therefore the equations of motion. +We thus obtain what are called the equations of +Lagrange. In these equations the independent +\PageSep{219} +variables are the co-ordinates of the hypothetical +molecules~$m$; but I now assume that we take for +the variables the parameters~$q$, which are directly +accessible to experiment. + +The two parts of the energy should then be +expressed as a function of the parameters~$q$ and +their derivatives; it is clear that it is under this +form that they will appear to the experimenter. +The latter will naturally endeavour to define +kinetic and potential energy by the aid of +quantities he can directly observe.\footnote + {We may add that $U$ will depend only on the $q$~parameters, that + $T$~will depend on them and their derivatives with respect to time, + and will be a homogeneous polynomial of the second degree with + respect to these derivatives.} +If this be +granted, the system will always proceed from one +position to another by such a path that the mean +value of the action is a minimum. It matters +little that $T$~and~$U$ are now expressed by the aid +of the parameters~$q$ and their derivatives; it +matters little that it is also by the aid of these +parameters that we define the initial and \Typo{fina}{final} +positions; the principle of least action will always +remain true. + +Now here again, of the whole of the paths which +lead from one position to another, there is one and +only one for which the mean action is a minimum. +The principle of least action is therefore sufficient +for the determination of the differential equations +which define the variations of the parameters~$q$. +The equations thus obtained are another form of +Lagrange's equations. +\PageSep{220} + +To form these equations we need not know the +relations which connect the parameters~$q$ with the +co-ordinates of the hypothetical molecules, nor the +masses of the molecules, nor the expression of~$U$ +as a function of the co-ordinates of these molecules. +All we need know is the expression of~$U$ as a +function of the parameters~$q$, and that of~$T$ as a +function of the parameters~$q$ and their derivatives---\ie, +the expressions of the kinetic and potential +energy in terms of experimental data. + +One of two things must now happen. Either for +a convenient choice of $T$~and~$U$ the Lagrangian +equations, constructed as we have indicated, will +be identical with the differential equations deduced +from experiment, or there will be no functions $T$~and~$U$ +for which this identity takes place. In the +latter case it is clear that no mechanical explanation +is possible. The \emph{necessary} condition for a +mechanical explanation to be possible is therefore +this: that we may choose the functions $T$~and~$U$ so +as to satisfy the principle of least action, and of the +conservation of energy. Besides, this condition is +\emph{sufficient}. Suppose, in fact, that we have found a +function~$U$ of the parameters~$q$, which represents +one of the parts of energy, and that the part of the +energy which we represent by~$T$ is a function of +the parameters~$q$ and their derivatives; that it +is a polynomial of the second degree with respect +to its derivatives, and finally that the Lagrangian +equations formed by the aid of these two functions +$T$~and~$U$ are in conformity with the data of the +\PageSep{221} +experiment. How can we deduce from this a +mechanical explanation? $U$~must be regarded as +the potential energy of a system of which $T$~is the +kinetic energy. There is no difficulty as far as $U$~is +concerned, but can $T$ be regarded as the \Foreign{vis~viva} +of a material system? + +It is easily shown that this is always possible, +and in an unlimited number of ways. I will be +content with referring the reader to the pages of +the preface of my \Title{Électricité et Optique} for further +details. Thus, if the principle of least action +cannot be satisfied, no mechanical explanation is +possible; if it can be satisfied, there is not only one +explanation, but an unlimited number, whence it +follows that since there is one there must be an +unlimited number. + +One more remark. Among the quantities that +may be reached by experiment directly we shall +consider some as the co-ordinates of our hypothetical +molecules, some will be our parameters~$q$, +and the rest will be regarded as dependent not +only on the co-ordinates but on the velocities---or +what comes to the same thing, we look on them as +derivatives of the parameters~$q$, or as combinations +of these parameters and their derivatives. + +Here then a question occurs: among all these +quantities measured experimentally which shall we +choose to represent the parameters~$q$? and which +shall we prefer to regard as the derivatives of these +parameters? This choice remains arbitrary to a +large extent, but a mechanical explanation will be +\PageSep{222} +possible if it is done so as to satisfy the principle of +least action. + +Next, Maxwell asks: Can this choice and that of +the two energies $T$~and~$U$ be made so that electric +phenomena will satisfy this principle? Experiment +shows us that the energy of an electro-magnetic +field decomposes into electro-static and electro-dynamic +energy. Maxwell recognised that if we +regard the former as the potential energy~$U$, and +the latter as the kinetic energy~$T$, and that if on +the other hand we take the electro-static charges +of the conductors as the parameters~$q$, and the intensity +of the currents as derivatives of other +parameters~$q$---under these conditions, Maxwell +has recognised that electric phenomena \Reword{satisfies}{satisfy} the +principle of least action. He was then certain of +a mechanical explanation. If he had expounded +this theory at the beginning of his first volume, +instead of relegating it to a corner of the second, it +would not have escaped the attention of most +readers. If therefore a phenomenon allows of a +complete mechanical explanation, it allows of an +unlimited number of others, which will equally take +into account all the particulars revealed by experiment. +And this is confirmed by the history of +every branch of physics. In Optics, for instance, +Fresnel believed vibration to be perpendicular to +the plane of polarisation; Neumann holds that it is +parallel to that plane. For a long time an \Foreign{experimentum +crucis} was sought for, which would enable +us to decide between these two theories, but in +\PageSep{223} +vain. In the same way, without going out of the +domain of electricity, we find that the theory of +two fluids and the single fluid theory equally +account in a satisfactory manner for all the laws +of electro-statics. All these facts are easily explained, +thanks to the properties of the Lagrange +equations. + +\Pagelabel{223}% +It is easy now to understand Maxwell's fundamental +idea. To demonstrate the possibility of a +mechanical explanation of electricity we need not +trouble to find the explanation itself; we need only +know the expression of the two functions $T$~and~$U$, +which are the two parts of energy, and to form with +these two functions Lagrange's equations, and +then to compare these equations with the experimental +laws. + +How shall we choose from all the possible +explanations one in which the help of experiment +will be wanting? The day will perhaps come +when physicists will no longer concern themselves +with questions which are inaccessible to positive +methods, and will leave them to the metaphysicians. +That day has not yet come; man does not +so easily resign himself to remaining for ever ignorant +of the causes of things. Our choice cannot be +therefore any longer guided by considerations in +which personal appreciation plays too large a part. +There are, however, solutions which all will reject +because of their fantastic nature, and others which +all will prefer because of their simplicity. As +far as magnetism and electricity are concerned, +\PageSep{224} +Maxwell abstained from making any choice. It is +not that he has a systematic contempt for all that +positive methods cannot reach, as may be seen +from the time he has devoted to the kinetic theory +of gases. I may add that if in his \Foreign{magnum opus} he +develops no complete explanation, he has attempted +one in an article in the \Title{Philosophical Magazine}. +The strangeness and the complexity of the +hypotheses he found himself compelled to make, +led him afterwards to withdraw it. + +The same spirit is found throughout his whole +work. He throws into relief the essential---\ie, +what is common to all theories; everything that +suits only a particular theory is passed over almost +in silence. The reader therefore finds himself in +the presence of form nearly devoid of matter, +which at first he is tempted to take as a fugitive +and unassailable phantom. But the efforts he is +thus compelled to make force him to think, and +eventually he sees that there is often something +rather artificial in the theoretical ``aggregates'' +which he once admired. +\Pagelabel{224}% +\PageSep{225} + + +\Chapter{XIII.}{Electro-Dynamics.} + +\First{The} history of electro-dynamics is very instructive +from our point of view. The title of Ampère's +immortal work is, \Title{Théorie des phénomènes electro-dynamiques, +uniquement fondée sur expérience}. He +therefore imagined that he had made no hypotheses; +but as we shall not be long in recognising, he was +mistaken; only, of these hypotheses he was quite +unaware. On the other hand, his successors see +them clearly enough, because their attention is +attracted by the weak points in Ampère's solution. +They made fresh hypotheses, but this time +deliberately. How many times they had to change +them before they reached the classic system, which +is perhaps even now not quite definitive, we shall +see. + +\Par[I. ]{Ampère's Theory.}---In Ampère's experimental +study of the mutual action of currents, he has +operated, and he could operate only, with closed +currents. This was not because he denied the +existence or possibility of open currents. If two +conductors are positively and negatively charged +and brought into communication by a wire, a +current is set up which passes from one to the +\PageSep{226} +other until the two potentials are equal. According +to the ideas of Ampère's time, this was +considered to be an open current; the current was +known to pass from the first conductor to the +second, but they did not know it returned from the +second to the first. All currents of this kind were +therefore considered by Ampère to be open +currents---for instance, the currents of discharge +of a condenser; he was unable to experiment on +them, their duration being too short. Another +kind of open current may be imagined. Suppose +we have two conductors $A$~and~$B$ connected by a +wire~$AMB$. Small conducting masses in motion +are first of all placed in contact with the conductor~$B$, +receive an electric charge, and leaving~$B$ are +set in motion along a path~$BNA$, carrying their +charge with them. On coming into contact with~$A$ +they lose their charge, which then returns to~$B$ +along the wire~$AMB$. Now here we have, in a +sense, a closed circuit, since the electricity describes +the closed circuit~$BNAMB$; but the two parts of +the current are quite different. In the wire~$AMB$ +the electricity is displaced \emph{through} a fixed conductor +like a voltaic current, overcoming an ohmic resistance +and developing heat; we say that it is +displaced by \emph{conduction}. In the part~$BNA$ the +electricity is \emph{carried} by a moving conductor, and is +said to be displaced by \emph{convection}. If therefore the +convection current is considered to be perfectly +analogous to the conduction current, the circuit~$BNAMB$ +is closed; if on the contrary the convection +\PageSep{227} +current is not a ``true current,'' and, for +instance, does not act on the magnet, there is only +the conduction current~$AMB$, which is \emph{open}. For +example, if we connect by a wire the poles of a +Holtz machine, the charged rotating disc transfers +the electricity by convection from one pole to the +other, and it returns to the first pole by conduction +through the wire. But currents of this kind are +very difficult to produce with appreciable intensity; +in fact, with the means at Ampère's disposal we +may almost say it was impossible. + +To sum up, Ampère could conceive of the existence +of two kinds of open currents, but he could +experiment on neither, because they were not +strong enough, or because their duration was too +short. Experiment therefore could only show him +the action of a closed current on a closed current---or +more accurately, the action of a closed current +on a portion of current, because a current can be +made to describe a \emph{closed} circuit, of which part may +be in motion and the other part fixed. The displacements +of the moving part may be studied under the +action of another closed current. On the other +hand, Ampère had no means of studying the action +of an open current either on a closed or on another +open current. + +\Par[1.\ ]{The Case of Closed Currents.}---In the case of +the mutual action of two closed currents, experiment +revealed to Ampère remarkably simple +laws. The following will be useful to us in the +sequel:--- +\PageSep{228} + +(1) \emph{If the intensity of the currents is kept constant}, +and if the two circuits, after having undergone any +displacements and deformations whatever, return +finally to their initial positions, the total work +done by the electro-dynamical actions is zero. In +other words, there is an \emph{electro-dynamical potential} +of the two circuits proportional to the product of +their intensities, and depending on the form and +relative positions of the circuits; the work done +by the electro-dynamical actions is equal to the +change of this potential. + +(2) The action of a closed solenoid is zero. + +(3) The action of a circuit~$C$ on another voltaic +circuit~$C'$ depends only on the ``magnetic field'' +developed by the circuit~$C$. At each point in +space we can, in fact, define in magnitude and +direction a certain force called ``magnetic force,'' +which enjoys the following properties:--- + +(\textit{a}) The force exercised by~$C$ on a magnetic +pole is applied to that pole, and is equal to the +magnetic force multiplied by the magnetic mass +of the pole. + +(\textit{b}) A very short magnetic needle tends to take +the direction of the magnetic force, and the couple +to which it tends to reduce is proportional to the +product of the magnetic force, the magnetic +moment of the needle, and the sine of the dip +of the needle. + +(\textit{c}) If the circuit~$C'$ is displaced, the amount of +the work done by the electro-dynamic action of~$C$ +on~$C'$ will be equal to the increment of ``flow +\PageSep{229} +of magnetic force'' which passes through the +circuit. + +\Par[2.\ ]{Action of a Closed Current on a Portion of +Current.}---Ampère being unable to produce the +open current properly so called, had only one +way of studying the action of a closed current +on a portion of current. This was by operating +on a circuit~$C$ composed of two parts, one movable +and the other fixed. The movable part was, +for instance, a movable wire~$\alpha\beta$, the ends $\alpha$~and~$\beta$ +of which could slide along a fixed wire. In one of +the positions of the movable wire the end~$\alpha$ rested +on the point~$A$, and the end~$\beta$ on the point~$B$ of +the fixed wire. The current ran from~$\alpha$ to~$\beta$---\ie, +from~$A$ to~$B$ along the movable wire, and then +from~$B$ to~$A$ along the fixed wire. \emph{This current +was therefore closed.} + +In the second position, the movable wire +having slipped, the points $\alpha$~and~$\beta$ were respectively +at $A'$~and~$B'$ on the fixed wire. The current +ran from~$\alpha$ to~$\beta$---\ie, from~$A'$ to~$B'$ on the movable +wire, and returned from~$B'$ to~$B$, and +then from~$B$ to~$A$, and then from~$A$ to~$A'$---all on +the fixed wire. This current was also closed. +If a similar circuit be exposed to the action of a +closed current~$C$, the movable part will be displaced +just as if it were acted on by a force. +Ampère \emph{admits} that the force, apparently acting on +the movable part~$AB$, representing the action of~$C$ +on the portion~$\alpha\beta$ of the current, remains the +same whether an open current runs through~$\alpha\beta$, +\PageSep{230} +stopping at $\alpha$~and~$\beta$, or whether a closed current +runs first to~$\beta$ and then returns to~$\alpha$ through the +fixed portion of the circuit. This hypothesis +seemed natural enough, and Ampère innocently +assumed it; nevertheless the hypothesis \emph{is not a +necessity}, for we shall presently see that Helmholtz +rejected it. However that may be, it enabled +Ampère, although he had never produced an open +current, to lay down the laws of the action of a +closed current on an open current, or even on an +element of current. They are simple:\Add{---} + +(1) The force acting on an element of current +is applied to that element; it is normal to the +element and to the magnetic force, and proportional +to that component of the magnetic force +which is normal to the element. + +(2) The action of a closed solenoid on an +element of current is zero. But the electro-dynamic +potential has disappeared---\ie, when a +closed and an open current of constant intensities +return to their initial positions, the total work +done is not zero. + +\Par[3.\ ]{Continuous Rotations.}---The most remarkable +electro-dynamical experiments are those in which +continuous rotations are produced, and which are +called \emph{unipolar induction} experiments. A magnet +may turn about its axis; a current passes first +through a fixed wire and then enters the magnet +by the pole~$N$, for instance, passes through +half the magnet, and emerges by a sliding contact +and re-enters the fixed wire. The magnet +\PageSep{231} +then begins to rotate continuously. This is +Faraday's experiment. How is it possible? If it +were a question of two circuits of invariable form, +$C$~fixed and $C'$~movable about an axis, the latter +would never take up a position of continuous +rotation; in fact, there is an electro-dynamical +potential; there must therefore be a position of +equilibrium when the potential is a maximum. +Continuous rotations are therefore possible only +when the circuit~$C'$ is composed of two parts---one +fixed, and the other movable about an axis, +as in the case of Faraday's experiment. Here +again it is convenient to draw a distinction. The +passage from the fixed to the movable part, or +\Foreign{vice~versâ}, may take place either by simple contact, +the same point of the movable part remaining +constantly in contact with the same point of the +fixed part, or by sliding contact, the same point of +the movable part coming successively into contact +with the different points of the fixed part. + +It is only in the second case that there can +be continuous rotation. This is what then +happens:---the system tends to take up a position +of equilibrium; but, when at the point of reaching +that position, the sliding contact puts the moving +part in contact with a fresh point in the fixed +part; it changes the connexions and therefore the +conditions of equilibrium, so that as the position +of equilibrium is ever eluding, so to speak, the +system which is trying to reach it, rotation may +take place indefinitely. +\PageSep{232} + +Ampère admits that the action of the circuit on +the movable part of~$C'$ is the same as if the fixed +part of~$C'$ did not exist, and therefore as if the +current passing through the movable part were +an open current. He concluded that the action of +a closed on an open current, or \Foreign{vice~versâ}, that of +an open current on a fixed current, may give rise +to continuous rotation. But this conclusion +depends on the hypothesis which I have enunciated, +and to which, as I said above, Helmholtz +declined to subscribe. + +\Par[4.\ ]{Mutual Action of Two Open Currents.}---As far +as the mutual action of two open currents, and in +particular that of two elements of current, is +concerned, all experiment breaks down. Ampère +falls back on hypothesis. He assumes: (1)~that +the mutual action of two elements reduces to a +force acting along their \emph{join}; (2)~that the action +of two closed currents is the resultant of the +mutual actions of their different elements, which +are the same as if these elements were isolated. + +The remarkable thing is that here again Ampère +makes two hypotheses without being aware of it. +However that may be, these two hypotheses, +together with the experiments on closed currents, +suffice to determine completely the law of mutual +action of two elements. But then, most of the +simple laws we have met in the case of closed +currents are no longer true. In the first place, +there is no electro-dynamical potential; nor was +there any, as we have seen, in the case of a closed +\PageSep{233} +current acting on an open current. Next, there +is, properly speaking, no magnetic force; and we +have above defined this force in three different +ways: (1)~By the action on a magnetic pole; +(2)~by the director couple which orientates the +magnetic needle; (3)~by the action on an element +of current. + +In the case with which we are immediately +concerned, not only are these three definitions not +in harmony, but each has lost its meaning:--- + +(1) A magnetic pole is no longer acted on by a +unique force applied to that pole. We have seen, +in fact, the action of an element of current on a +pole is not applied to the pole but to the element; +it may, moreover, be replaced by a force applied to +the pole and by a couple. + +(2) The couple which acts on the magnetic +needle is no longer a simple director couple, for its +moment with respect to the axis of the needle is +not zero. It decomposes into a director couple, +properly so called, and a supplementary couple +which tends to produce the continuous rotation of +which we have spoken above. + +(3) Finally, the force acting on an element of +a current is not normal to that element. In +other words, \emph{the unity of the magnetic force has +disappeared}. + +Let us see in what this unity consists. Two +systems which exercise the same action on a magnetic +pole will also exercise the same action on an +indefinitely small magnetic needle, or on an element +\PageSep{234} +of current placed at the point in space at which the +pole is. Well, this is true if the two systems only +contain closed currents, and according to Ampère +it would not be true if the systems contained open +currents. It is sufficient to remark, for instance, +that if a magnetic pole is placed at~$A$ and an +element at~$B$, the direction of the element being +in~$AB$ produced, this element, which will exercise +no action on the pole, will exercise an action +either on a magnetic needle placed at~$A$, or on +an element of current at~$A$. + +\Par[5.\ ]{Induction.}---We know that the discovery of +electro-dynamical induction followed not long after +the immortal work of Ampère. As long as it is +only a question of closed currents there is no +difficulty, and Helmholtz has even remarked that +the principle of the conservation of energy is +sufficient for us to deduce the laws of induction +from the electro-dynamical laws of Ampère. But +on the condition, as Bertrand has shown,---that +we make a certain number of hypotheses. + +The same principle again enables this deduction +to be made in the case of open currents, although +the result cannot be tested by experiment, since +such currents cannot be produced. + +If we wish to compare this method of analysis +with Ampère's theorem on open currents, we get +results which are calculated to surprise us. In +the first place, induction cannot be deduced from +the variation of the magnetic field by the well-known +formula of scientists and practical men; +\PageSep{235} +in fact, as I have said, properly speaking, there +is no magnetic field. But further, if a circuit~$C$ +is subjected to the induction of a variable voltaic +system~$S$, and if this system~$S$ be displaced and +deformed in any way whatever, so that the +intensity of the currents of this system varies +according to any law whatever, then so long +as after these variations the system eventually +returns to its initial position, it seems natural +to suppose that the \emph{mean} electro-motive force +%[** TN: "induite dans le circuit C est nulle" in the French edition.] +induced in the \Reword{current}{circuit}~$C$ is zero. This is true if +the circuit~$C$ is closed, and if the system~$S$ only +contains closed currents. It is no longer true if +we accept the theory of Ampère, since there would +be open currents. So that not only will induction +no longer be the variation of the flow of magnetic +force in any of the usual senses of the word, but +it cannot be represented by the variation of that +force whatever it may be. + +\Par[II. ]{Helmholtz's Theory.}---I have dwelt upon the +consequences of Ampère's theory and on his +method of explaining the action of open currents. +It is difficult to disregard the paradoxical and +artificial character of the propositions to which +we are thus led. We feel bound to think ``it +cannot be so.'' We may imagine then that +Helmholtz has been led to look for something +else. He rejects the fundamental hypothesis of +Ampère---namely, that the mutual action of two +elements of current reduces to a force along their +join. He admits that an clement of current is not +\PageSep{236} +acted upon by a single force but by a force and a +couple, and this is what gave rise to the celebrated +polemic between Bertrand and Helmholtz. +Helmholtz replaces Ampère's hypothesis by the +following:---Two elements of current always +admit of an electro-dynamic potential, depending +solely upon their position and orientation; and the +work of the forces that they exercise one on the +other is equal to the variation of this potential. +Thus Helmholtz can no more do without +hypothesis than Ampère, but at least he does +not do so without explicitly announcing it. In +the case of closed currents, which alone are +accessible to experiment, the two theories agree; +in all other cases they differ. In the first place, +contrary to what Ampère supposed, the force +which seems to act on the movable portion of +a closed current is not the same as that acting +on the movable portion if it were isolated and +if it constituted an open current. Let us return +to the circuit~$C'$, of which we spoke above, and +which was formed of a movable wire sliding on +a fixed wire. In the only experiment that can be +made the movable portion~$\alpha\beta$ is not isolated, but is +part of a closed circuit. When it passes from~$AB$ +to~$A'B'$, the total electro-dynamic potential +varies for two reasons. First, it has a slight increment +because the potential of~$A'B'$ with respect +to the circuit~$C$ is not the same as that of~$AB$; +secondly, it has a second increment because it +must be increased by the potentials of the elements +\PageSep{237} +$AA'$~and~$B'B$ with respect to~$C$. It is this \emph{double} +increment which represents the work of the force +acting upon the portion~$AB$. If, on the contrary, +$\alpha\beta$~be isolated, the potential would only have the +first increment, and this first increment alone +would measure the work of the force acting on~$AB$. +In the second place, there could be no +continuous rotation without sliding contact, and +in fact, that, as we have seen in the case of closed +currents, is an immediate consequence of the +existence of an electro-dynamic potential. In +Faraday's experiment, if the magnet is fixed, +and if the part of the current external to the +magnet runs along a movable wire, that movable +wire may undergo continuous rotation. But it +does not mean that, if the contacts of the \Typo{weir}{wire} +with the magnet were suppressed, and an open +current were to run along the wire, the wire +would still have a movement of continuous rotation. +I have just said, in fact, that an isolated +element is not acted on in the same way as a +movable element making part of a closed circuit. +But there is another difference. The action of a +solenoid on a closed current is zero according to +experiment and according to the two theories. +Its action on an open current would be zero +according to Ampère, and it would not be +zero according to Helmholtz. From this follows +an important consequence. We have given above +three definitions of the magnetic force. The third +has no meaning here, since an element of current +\PageSep{238} +is no longer acted upon by a single force. Nor +has the first any meaning. What, in fact, is a +magnetic pole? It is the extremity of an +indefinite linear magnet. This magnet may be +replaced by an indefinite solenoid. For the +definition of magnetic force to have any meaning, +the action exercised by an open current on +an indefinite solenoid would only depend on the +position of the extremity of that solenoid---\ie, +that the action of a closed solenoid is zero. Now +we have just seen that this is not the case. On +the other hand, there is nothing to prevent us +from adopting the second definition which is +founded on the measurement of the director +couple which tends to orientate the magnetic +needle; but, if it is adopted, neither the effects +of induction nor electro-dynamic effects will +depend solely on the distribution of the lines +of force in this magnetic field. + +\Par[III. ]{Difficulties raised by these Theories.}---Helmholtz's +theory is an advance on that of Ampère; +it is necessary, however, that every difficulty +should be removed. In both, the name ``magnetic +field'' has no meaning, or, if we give it one by a +more or less artificial convention, the ordinary +laws so familiar to electricians no longer apply; +and it is thus that the electro-motive force induced +in a wire is no longer measured by the number +of lines of force met by that wire. And our +objections do not proceed only from the fact that +it is difficult to give up deeply-rooted habits of +\PageSep{239} +language and thought. There is something more. +If we do not believe in actions at a distance, +electro-dynamic phenomena must be explained by +a modification of the medium. And this medium +is precisely what we call ``magnetic field,'' and +then the electro-magnetic effects should only +depend on that field. All these difficulties arise +from the hypothesis of open currents. + +\Par[IV. ]{Maxwell's Theory.}---Such were the difficulties +raised by the current theories, when Maxwell with +a stroke of the pen caused them to vanish. To +his mind, in fact, all currents are closed currents. +Maxwell admits that if in a dielectric, the electric +field happens to vary, this dielectric becomes the +seat of a particular phenomenon acting on the +galvanometer like a current and called the \emph{current +of displacement}. If, then, two conductors bearing +positive and negative charges are placed in connection +by means of a wire, during the discharge +there is an open current of conduction in that +wire; but there are produced at the same time in +the surrounding dielectric currents of displacement +which close this current of conduction. We +know that Maxwell's theory leads to the explanation +of optical phenomena which would be due to +extremely rapid electrical oscillations. At that +period such a conception was only a daring hypothesis +which could be supported by no experiment; +but after twenty years Maxwell's ideas received the +confirmation of experiment. Hertz succeeded in +producing systems of electric oscillations which +\PageSep{240} +reproduce all the properties of light, and only +differ by the length of their wave---that is to say, +as violet differs from red. In some measure he +made a synthesis of light. It might be said that +Hertz has not directly proved Maxwell's fundamental +idea of the action of the current of +displacement on the galvanometer. That is true +in a sense. What he has shown directly is that +electro-magnetic induction is not instantaneously +propagated, as was supposed, but its speed is the +speed of light. Yet, to suppose there is no current +of displacement, and that induction is with the +speed of light; or, rather, to suppose that the +currents of displacement produce inductive effects, +and that the induction takes place instantaneously---\emph{comes +to the same thing}. This cannot be seen at +the first glance, but it is proved by an analysis +of which I must not even think of giving even a +summary here. + +\Par[V. ]{Rowland's Experiment.}---But, as I have said +above, there are two kinds of open conduction +currents. There are first the currents of discharge +of a condenser, or of any conductor whatever. +There are also cases in which the electric charges +describe a closed contour, being displaced by conduction +in one part of the circuit and by convection +in the other part. The question might be +regarded as solved for open currents of the first +kind; they were closed by currents of displacement. +For open currents of the second kind the +solution appeared still more simple. +\PageSep{241} + +It seemed that if the current were closed it +could only be by the current of convection itself. +For that purpose it was sufficient to admit that a +``convection current''---\ie, a charged conductor in +motion---could act on the galvanometer. But experimental +confirmation was lacking. It appeared +difficult, in fact, to obtain a sufficient intensity +even by increasing as much as possible the charge +and the velocity of the conductors. Rowland, an +extremely skilful experimentalist, was the first to +triumph, or to seem to triumph, over these difficulties. +A disc received a strong \Chg{electrostatic}{electro-static} +charge and a very high speed of rotation. An +astatic magnetic system placed beside the disc +underwent deviations. The experiment was made +twice by Rowland, once in Berlin and once at Baltimore. +It was afterwards repeated by Himstedt. +These physicists even believed that they could +announce that they had succeeded in making +quantitative measurements. For twenty years +Rowland's law was admitted without objection +by all physicists, and, indeed, everything seemed +to confirm it. The spark certainly does produce a +magnetic effect, and does it not seem extremely +likely that the spark discharged is due to particles +taken from one of the electrodes and transferred +to the other electrode with their charge? Is not +the very spectrum of the spark, in which we +recognise the lines of the metal of the electrode, +a proof of it? The spark would then be a real +current of induction. +\PageSep{242} + +On the other hand, it is also admitted that in +an electrolyte the electricity is carried by the ions +in motion. The current in an electrolyte would +therefore also be a current of convection; but it +acts on the magnetic needle. And in the same +way for cathode rays; \Typo{Crooks}{Crookes} attributed these +rays to very subtle matter charged with negative +electricity and moving with very high velocity. +He looked upon them, in other words, as currents +of convection. Now, these cathode rays are +deviated by the magnet. In virtue of the +principle of action and \Chg{re-action}{reaction}, they should in +their turn deviate the magnetic needle. It is +true that Hertz believed he had proved that the +cathodic rays do not carry negative electricity, and +that they do not act on the magnetic needle; but +Hertz was wrong. First of all, Perrin succeeded +in collecting the electricity carried by these rays---electricity +of which Hertz denied the existence; the +German scientist appears to have been deceived +by the effects due to the action of the X-rays, +which were not yet discovered. Afterwards, and +quite recently, the action of the cathodic rays on +the magnetic needle has been brought to light. +Thus all these phenomena looked upon as currents +of convection, electric sparks, electrolytic currents, +cathodic rays, act in the same manner on the +galvanometer and in conformity to Rowland's +law. + +\Par[VI. ]{Lorentz's Theory.}---We need not go much +further. According to Lorentz's theory, currents +\PageSep{243} +of conduction would themselves be true convection +currents. Electricity would remain indissolubly +connected with certain material particles called +\emph{electrons}. The circulation of these electrons +through bodies would produce voltaic currents, +and what would distinguish conductors from +insulators would be that the one could be traversed +by these electrons, while the others would check +the movement of the electrons. Lorentz's theory +is very attractive. It gives a very simple explanation +of certain phenomena, which the earlier +theories---even Maxwell's in its primitive form---could +only deal with in an unsatisfactory manner; +for example, the aberration of light, the partial +impulse of luminous waves, magnetic polarisation, +and Zeeman's experiment. + +A few objections still remained. The phenomena +of an electric system seemed to depend on +the absolute velocity of translation of the centre +of gravity of this system, which is contrary to +the idea that we have of the relativity of space. +Supported by M.~Crémieu, M.~Lippman has presented +this objection in a very striking form. +Imagine two charged conductors with the same +velocity of translation. They are relatively at +rest. However, each of them being equivalent +to a current of convection, they ought to attract +one another, and by measuring this attraction +we could measure their absolute velocity. +``No!'' replied the partisans of Lorentz. ``What +we could measure in that way is not their +\PageSep{244} +absolute velocity, but their relative velocity \emph{with +respect to the ether}, so that the principle of relativity +is safe.'' Whatever there may be in these +objections, the edifice of electro-dynamics seemed, +at any rate in its broad lines, definitively constructed. +Everything was presented under the +most satisfactory aspect. The theories of Ampère +and Helmholtz, which were made for the open +currents that no longer existed, seem to have no +more than purely historic interest, and the inextricable +complications to which these theories +led have been almost forgotten. This quiescence +has been recently disturbed by the experiments of +M.~Crémieu, which have contradicted, or at least +have seemed to contradict, the results formerly +obtained by Rowland. Numerous investigators +have endeavoured to solve the question, and fresh +experiments have been undertaken. What result +will they give? I shall take care not to risk a +prophecy which might be falsified between the +day this book is ready for the press and the day on +which it is placed before the public. +\begin{center} +\vfill +\footnotesize THE END. +\vfill\vfill +\rule{1in}{0.5pt} \\[4pt] +\makebox[0pt][c]{\scriptsize THE WALTER SCOTT PUBLISHING CO., LIMITED, FELLING-ON-TYNE.} +\end{center} + +%%%%%%%%%%%%%%%%%%%%%%%%% GUTENBERG LICENSE %%%%%%%%%%%%%%%%%%%%%%%%%% +\PGLicense +\begin{PGtext} +End of Project Gutenberg's Science and hypothesis, by Henri Poincaré + +*** END OF THIS PROJECT GUTENBERG EBOOK SCIENCE AND HYPOTHESIS *** + +***** This file should be named 37157-t.tex or 37157-t.zip ***** +This and all associated files of various formats will be found in: + http://www.gutenberg.org/3/7/1/5/37157/ + +Produced by Andrew D. Hwang + +Updated editions will replace the previous one--the old editions +will be renamed. + +Creating the works from public domain print editions means that no +one owns a United States copyright in these works, so the Foundation +(and you!) can copy and distribute it in the United States without +permission and without paying copyright royalties. Special rules, +set forth in the General Terms of Use part of this license, apply to +copying and distributing Project Gutenberg-tm electronic works to +protect the PROJECT GUTENBERG-tm concept and trademark. Project +Gutenberg is a registered trademark, and may not be used if you +charge for the eBooks, unless you receive specific permission. If you +do not charge anything for copies of this eBook, complying with the +rules is very easy. You may use this eBook for nearly any purpose +such as creation of derivative works, reports, performances and +research. They may be modified and printed and given away--you may do +practically ANYTHING with public domain eBooks. Redistribution is +subject to the trademark license, especially commercial +redistribution. + + + +*** START: FULL LICENSE *** + +THE FULL PROJECT GUTENBERG LICENSE +PLEASE READ THIS BEFORE YOU DISTRIBUTE OR USE THIS WORK + +To protect the Project Gutenberg-tm mission of promoting the free +distribution of electronic works, by using or distributing this work +(or any other work associated in any way with the phrase "Project +Gutenberg"), you agree to comply with all the terms of the Full Project +Gutenberg-tm License (available with this file or online at +http://gutenberg.net/license). + + +Section 1. General Terms of Use and Redistributing Project Gutenberg-tm +electronic works + +1.A. By reading or using any part of this Project Gutenberg-tm +electronic work, you indicate that you have read, understand, agree to +and accept all the terms of this license and intellectual property +(trademark/copyright) agreement. If you do not agree to abide by all +the terms of this agreement, you must cease using and return or destroy +all copies of Project Gutenberg-tm electronic works in your possession. +If you paid a fee for obtaining a copy of or access to a Project +Gutenberg-tm electronic work and you do not agree to be bound by the +terms of this agreement, you may obtain a refund from the person or +entity to whom you paid the fee as set forth in paragraph 1.E.8. + +1.B. "Project Gutenberg" is a registered trademark. It may only be +used on or associated in any way with an electronic work by people who +agree to be bound by the terms of this agreement. There are a few +things that you can do with most Project Gutenberg-tm electronic works +even without complying with the full terms of this agreement. See +paragraph 1.C below. There are a lot of things you can do with Project +Gutenberg-tm electronic works if you follow the terms of this agreement +and help preserve free future access to Project Gutenberg-tm electronic +works. See paragraph 1.E below. + +1.C. The Project Gutenberg Literary Archive Foundation ("the Foundation" +or PGLAF), owns a compilation copyright in the collection of Project +Gutenberg-tm electronic works. Nearly all the individual works in the +collection are in the public domain in the United States. If an +individual work is in the public domain in the United States and you are +located in the United States, we do not claim a right to prevent you from +copying, distributing, performing, displaying or creating derivative +works based on the work as long as all references to Project Gutenberg +are removed. Of course, we hope that you will support the Project +Gutenberg-tm mission of promoting free access to electronic works by +freely sharing Project Gutenberg-tm works in compliance with the terms of +this agreement for keeping the Project Gutenberg-tm name associated with +the work. You can easily comply with the terms of this agreement by +keeping this work in the same format with its attached full Project +Gutenberg-tm License when you share it without charge with others. + +1.D. The copyright laws of the place where you are located also govern +what you can do with this work. Copyright laws in most countries are in +a constant state of change. If you are outside the United States, check +the laws of your country in addition to the terms of this agreement +before downloading, copying, displaying, performing, distributing or +creating derivative works based on this work or any other Project +Gutenberg-tm work. The Foundation makes no representations concerning +the copyright status of any work in any country outside the United +States. + +1.E. Unless you have removed all references to Project Gutenberg: + +1.E.1. The following sentence, with active links to, or other immediate +access to, the full Project Gutenberg-tm License must appear prominently +whenever any copy of a Project Gutenberg-tm work (any work on which the +phrase "Project Gutenberg" appears, or with which the phrase "Project +Gutenberg" is associated) is accessed, displayed, performed, viewed, +copied or distributed: + +This eBook is for the use of anyone anywhere at no cost and with +almost no restrictions whatsoever. You may copy it, give it away or +re-use it under the terms of the Project Gutenberg License included +with this eBook or online at www.gutenberg.net + +1.E.2. If an individual Project Gutenberg-tm electronic work is derived +from the public domain (does not contain a notice indicating that it is +posted with permission of the copyright holder), the work can be copied +and distributed to anyone in the United States without paying any fees +or charges. If you are redistributing or providing access to a work +with the phrase "Project Gutenberg" associated with or appearing on the +work, you must comply either with the requirements of paragraphs 1.E.1 +through 1.E.7 or obtain permission for the use of the work and the +Project Gutenberg-tm trademark as set forth in paragraphs 1.E.8 or +1.E.9. + +1.E.3. If an individual Project Gutenberg-tm electronic work is posted +with the permission of the copyright holder, your use and distribution +must comply with both paragraphs 1.E.1 through 1.E.7 and any additional +terms imposed by the copyright holder. Additional terms will be linked +to the Project Gutenberg-tm License for all works posted with the +permission of the copyright holder found at the beginning of this work. + +1.E.4. Do not unlink or detach or remove the full Project Gutenberg-tm +License terms from this work, or any files containing a part of this +work or any other work associated with Project Gutenberg-tm. + +1.E.5. Do not copy, display, perform, distribute or redistribute this +electronic work, or any part of this electronic work, without +prominently displaying the sentence set forth in paragraph 1.E.1 with +active links or immediate access to the full terms of the Project +Gutenberg-tm License. + +1.E.6. You may convert to and distribute this work in any binary, +compressed, marked up, nonproprietary or proprietary form, including any +word processing or hypertext form. However, if you provide access to or +distribute copies of a Project Gutenberg-tm work in a format other than +"Plain Vanilla ASCII" or other format used in the official version +posted on the official Project Gutenberg-tm web site (www.gutenberg.net), +you must, at no additional cost, fee or expense to the user, provide a +copy, a means of exporting a copy, or a means of obtaining a copy upon +request, of the work in its original "Plain Vanilla ASCII" or other +form. Any alternate format must include the full Project Gutenberg-tm +License as specified in paragraph 1.E.1. + +1.E.7. Do not charge a fee for access to, viewing, displaying, +performing, copying or distributing any Project Gutenberg-tm works +unless you comply with paragraph 1.E.8 or 1.E.9. + +1.E.8. You may charge a reasonable fee for copies of or providing +access to or distributing Project Gutenberg-tm electronic works provided +that + +- You pay a royalty fee of 20% of the gross profits you derive from + the use of Project Gutenberg-tm works calculated using the method + you already use to calculate your applicable taxes. The fee is + owed to the owner of the Project Gutenberg-tm trademark, but he + has agreed to donate royalties under this paragraph to the + Project Gutenberg Literary Archive Foundation. Royalty payments + must be paid within 60 days following each date on which you + prepare (or are legally required to prepare) your periodic tax + returns. Royalty payments should be clearly marked as such and + sent to the Project Gutenberg Literary Archive Foundation at the + address specified in Section 4, "Information about donations to + the Project Gutenberg Literary Archive Foundation." + +- You provide a full refund of any money paid by a user who notifies + you in writing (or by e-mail) within 30 days of receipt that s/he + does not agree to the terms of the full Project Gutenberg-tm + License. You must require such a user to return or + destroy all copies of the works possessed in a physical medium + and discontinue all use of and all access to other copies of + Project Gutenberg-tm works. + +- You provide, in accordance with paragraph 1.F.3, a full refund of any + money paid for a work or a replacement copy, if a defect in the + electronic work is discovered and reported to you within 90 days + of receipt of the work. + +- You comply with all other terms of this agreement for free + distribution of Project Gutenberg-tm works. + +1.E.9. If you wish to charge a fee or distribute a Project Gutenberg-tm +electronic work or group of works on different terms than are set +forth in this agreement, you must obtain permission in writing from +both the Project Gutenberg Literary Archive Foundation and Michael +Hart, the owner of the Project Gutenberg-tm trademark. Contact the +Foundation as set forth in Section 3 below. + +1.F. + +1.F.1. Project Gutenberg volunteers and employees expend considerable +effort to identify, do copyright research on, transcribe and proofread +public domain works in creating the Project Gutenberg-tm +collection. Despite these efforts, Project Gutenberg-tm electronic +works, and the medium on which they may be stored, may contain +"Defects," such as, but not limited to, incomplete, inaccurate or +corrupt data, transcription errors, a copyright or other intellectual +property infringement, a defective or damaged disk or other medium, a +computer virus, or computer codes that damage or cannot be read by +your equipment. + +1.F.2. LIMITED WARRANTY, DISCLAIMER OF DAMAGES - Except for the "Right +of Replacement or Refund" described in paragraph 1.F.3, the Project +Gutenberg Literary Archive Foundation, the owner of the Project +Gutenberg-tm trademark, and any other party distributing a Project +Gutenberg-tm electronic work under this agreement, disclaim all +liability to you for damages, costs and expenses, including legal +fees. YOU AGREE THAT YOU HAVE NO REMEDIES FOR NEGLIGENCE, STRICT +LIABILITY, BREACH OF WARRANTY OR BREACH OF CONTRACT EXCEPT THOSE +PROVIDED IN PARAGRAPH 1.F.3. YOU AGREE THAT THE FOUNDATION, THE +TRADEMARK OWNER, AND ANY DISTRIBUTOR UNDER THIS AGREEMENT WILL NOT BE +LIABLE TO YOU FOR ACTUAL, DIRECT, INDIRECT, CONSEQUENTIAL, PUNITIVE OR +INCIDENTAL DAMAGES EVEN IF YOU GIVE NOTICE OF THE POSSIBILITY OF SUCH +DAMAGE. + +1.F.3. LIMITED RIGHT OF REPLACEMENT OR REFUND - If you discover a +defect in this electronic work within 90 days of receiving it, you can +receive a refund of the money (if any) you paid for it by sending a +written explanation to the person you received the work from. If you +received the work on a physical medium, you must return the medium with +your written explanation. The person or entity that provided you with +the defective work may elect to provide a replacement copy in lieu of a +refund. If you received the work electronically, the person or entity +providing it to you may choose to give you a second opportunity to +receive the work electronically in lieu of a refund. If the second copy +is also defective, you may demand a refund in writing without further +opportunities to fix the problem. + +1.F.4. Except for the limited right of replacement or refund set forth +in paragraph 1.F.3, this work is provided to you 'AS-IS' WITH NO OTHER +WARRANTIES OF ANY KIND, EXPRESS OR IMPLIED, INCLUDING BUT NOT LIMITED TO +WARRANTIES OF MERCHANTIBILITY OR FITNESS FOR ANY PURPOSE. + +1.F.5. Some states do not allow disclaimers of certain implied +warranties or the exclusion or limitation of certain types of damages. +If any disclaimer or limitation set forth in this agreement violates the +law of the state applicable to this agreement, the agreement shall be +interpreted to make the maximum disclaimer or limitation permitted by +the applicable state law. The invalidity or unenforceability of any +provision of this agreement shall not void the remaining provisions. + +1.F.6. INDEMNITY - You agree to indemnify and hold the Foundation, the +trademark owner, any agent or employee of the Foundation, anyone +providing copies of Project Gutenberg-tm electronic works in accordance +with this agreement, and any volunteers associated with the production, +promotion and distribution of Project Gutenberg-tm electronic works, +harmless from all liability, costs and expenses, including legal fees, +that arise directly or indirectly from any of the following which you do +or cause to occur: (a) distribution of this or any Project Gutenberg-tm +work, (b) alteration, modification, or additions or deletions to any +Project Gutenberg-tm work, and (c) any Defect you cause. + + +Section 2. Information about the Mission of Project Gutenberg-tm + +Project Gutenberg-tm is synonymous with the free distribution of +electronic works in formats readable by the widest variety of computers +including obsolete, old, middle-aged and new computers. It exists +because of the efforts of hundreds of volunteers and donations from +people in all walks of life. + +Volunteers and financial support to provide volunteers with the +assistance they need are critical to reaching Project Gutenberg-tm's +goals and ensuring that the Project Gutenberg-tm collection will +remain freely available for generations to come. In 2001, the Project +Gutenberg Literary Archive Foundation was created to provide a secure +and permanent future for Project Gutenberg-tm and future generations. +To learn more about the Project Gutenberg Literary Archive Foundation +and how your efforts and donations can help, see Sections 3 and 4 +and the Foundation web page at http://www.pglaf.org. + + +Section 3. Information about the Project Gutenberg Literary Archive +Foundation + +The Project Gutenberg Literary Archive Foundation is a non profit +501(c)(3) educational corporation organized under the laws of the +state of Mississippi and granted tax exempt status by the Internal +Revenue Service. The Foundation's EIN or federal tax identification +number is 64-6221541. Its 501(c)(3) letter is posted at +http://pglaf.org/fundraising. Contributions to the Project Gutenberg +Literary Archive Foundation are tax deductible to the full extent +permitted by U.S. federal laws and your state's laws. + +The Foundation's principal office is located at 4557 Melan Dr. S. +Fairbanks, AK, 99712., but its volunteers and employees are scattered +throughout numerous locations. Its business office is located at +809 North 1500 West, Salt Lake City, UT 84116, (801) 596-1887, email +business@pglaf.org. Email contact links and up to date contact +information can be found at the Foundation's web site and official +page at http://pglaf.org + +For additional contact information: + Dr. Gregory B. Newby + Chief Executive and Director + gbnewby@pglaf.org + + +Section 4. Information about Donations to the Project Gutenberg +Literary Archive Foundation + +Project Gutenberg-tm depends upon and cannot survive without wide +spread public support and donations to carry out its mission of +increasing the number of public domain and licensed works that can be +freely distributed in machine readable form accessible by the widest +array of equipment including outdated equipment. Many small donations +($1 to $5,000) are particularly important to maintaining tax exempt +status with the IRS. + +The Foundation is committed to complying with the laws regulating +charities and charitable donations in all 50 states of the United +States. Compliance requirements are not uniform and it takes a +considerable effort, much paperwork and many fees to meet and keep up +with these requirements. We do not solicit donations in locations +where we have not received written confirmation of compliance. To +SEND DONATIONS or determine the status of compliance for any +particular state visit http://pglaf.org + +While we cannot and do not solicit contributions from states where we +have not met the solicitation requirements, we know of no prohibition +against accepting unsolicited donations from donors in such states who +approach us with offers to donate. + +International donations are gratefully accepted, but we cannot make +any statements concerning tax treatment of donations received from +outside the United States. U.S. laws alone swamp our small staff. + +Please check the Project Gutenberg Web pages for current donation +methods and addresses. Donations are accepted in a number of other +ways including including checks, online payments and credit card +donations. To donate, please visit: http://pglaf.org/donate + + +Section 5. General Information About Project Gutenberg-tm electronic +works. + +Professor Michael S. Hart is the originator of the Project Gutenberg-tm +concept of a library of electronic works that could be freely shared +with anyone. For thirty years, he produced and distributed Project +Gutenberg-tm eBooks with only a loose network of volunteer support. + + +Project Gutenberg-tm eBooks are often created from several printed +editions, all of which are confirmed as Public Domain in the U.S. +unless a copyright notice is included. Thus, we do not necessarily +keep eBooks in compliance with any particular paper edition. + + +Most people start at our Web site which has the main PG search facility: + + http://www.gutenberg.net + +This Web site includes information about Project Gutenberg-tm, +including how to make donations to the Project Gutenberg Literary +Archive Foundation, how to help produce our new eBooks, and how to +subscribe to our email newsletter to hear about new eBooks. +\end{PGtext} + +% %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% % +% % +% End of Project Gutenberg's Science and hypothesis, by Henri Poincaré % +% % +% *** END OF THIS PROJECT GUTENBERG EBOOK SCIENCE AND HYPOTHESIS *** % +% % +% ***** This file should be named 37157-t.tex or 37157-t.zip ***** % +% This and all associated files of various formats will be found in: % +% http://www.gutenberg.org/3/7/1/5/37157/ % +% % +% %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% % + +\end{document} +### +@ControlwordReplace = ( + ['\\ie', 'i.e.'], + ['\\QED', 'Q.E.D.'] + ); + +@ControlwordArguments = ( + ['\\Signature', 1, 1, '', ' ', 1, 1, '', ''], + ['\\BookMark', 1, 0, '', '', 1, 0, '', ''], + ['\\First', 1, 1, '', ''], + ['\\Part', 1, 1, 'Part ', ' ', 1, 1, '', ''], + ['\\OtherChapter', 1, 1, '', ''], + ['\\Chapter', 0, 0, '', '', 1, 1, 'Chapter ', ' ', 1, 1, '', ''], + ['\\ChapRef', 1, 1, 'Chapter ', ''], + ['\\hyperref', 0, 0, '', '', 1, 1, '', ''], + ['\\Section', 1, 1, '', ''], + ['\\Subsection', 1, 1, '', ''], + ['\\Par', 0, 1, '', '', 1, 1, '', ''], + ['\\Dict', 1, 1, '', ': ', 1, 1, '', ''], + ['\\Pagelabel', 1, 0, '', ''], + ['\\Pageref', 1, 1, 'p. ', ''], + ['\\Pagerefs', 1, 1, 'pp. ', ', ', 1, 1, '', ''], + ['\\Reword', 1, 0, '', '', 1, 1, '', ''], + ['\\Typo', 1, 0, '', '', 1, 1, '', ''], + ['\\Chg', 1, 0, '', '', 1, 1, '', ''], + ['\\Add', 1, 1, '', ''] + ); +$PageSeparator = qr/^\\PageSep/; +$CustomClean = 'print "\\nCustom cleaning in progress..."; +my $cline = 0; + while ($cline <= $#file) { + $file[$cline] =~ s/--------[^\n]*\n//; # strip page separators + $cline++ + } + print "done\\n";'; +### +This is pdfTeXk, Version 3.141592-1.40.3 (Web2C 7.5.6) (format=pdflatex 2010.5.6) 21 AUG 2011 16:35 +entering extended mode + %&-line parsing enabled. +**37157-t.tex +(./37157-t.tex +LaTeX2e <2005/12/01> +Babel <v3.8h> and hyphenation patterns for english, usenglishmax, dumylang, noh +yphenation, arabic, farsi, croatian, ukrainian, russian, bulgarian, czech, slov +ak, danish, dutch, finnish, basque, french, german, ngerman, ibycus, greek, mon +ogreek, ancientgreek, hungarian, italian, latin, mongolian, norsk, icelandic, i +nterlingua, turkish, coptic, romanian, welsh, serbian, slovenian, estonian, esp +eranto, uppersorbian, indonesian, polish, portuguese, spanish, catalan, galicia +n, swedish, ukenglish, pinyin, loaded. +(/usr/share/texmf-texlive/tex/latex/base/book.cls +Document Class: book 2005/09/16 v1.4f Standard LaTeX document class +(/usr/share/texmf-texlive/tex/latex/base/leqno.clo +File: leqno.clo 1998/08/17 v1.1c Standard LaTeX option (left equation numbers) +) (/usr/share/texmf-texlive/tex/latex/base/bk12.clo +File: bk12.clo 2005/09/16 v1.4f Standard LaTeX file (size option) +) +\c@part=\count79 +\c@chapter=\count80 +\c@section=\count81 +\c@subsection=\count82 +\c@subsubsection=\count83 +\c@paragraph=\count84 +\c@subparagraph=\count85 +\c@figure=\count86 +\c@table=\count87 +\abovecaptionskip=\skip41 +\belowcaptionskip=\skip42 +\bibindent=\dimen102 +) (/usr/share/texmf-texlive/tex/latex/base/inputenc.sty +Package: inputenc 2006/05/05 v1.1b Input encoding file +\inpenc@prehook=\toks14 +\inpenc@posthook=\toks15 +(/usr/share/texmf-texlive/tex/latex/base/latin1.def +File: latin1.def 2006/05/05 v1.1b Input encoding file +)) (/usr/share/texmf-texlive/tex/latex/base/fontenc.sty +Package: fontenc 2005/09/27 v1.99g Standard LaTeX package +(/usr/share/texmf-texlive/tex/latex/base/t1enc.def +File: t1enc.def 2005/09/27 v1.99g Standard LaTeX file +LaTeX Font Info: Redeclaring font encoding T1 on input line 43. +)) (/usr/share/texmf-texlive/tex/latex/base/ifthen.sty +Package: ifthen 2001/05/26 v1.1c Standard LaTeX ifthen package (DPC) +) (/usr/share/texmf-texlive/tex/latex/amsmath/amsmath.sty +Package: amsmath 2000/07/18 v2.13 AMS math features +\@mathmargin=\skip43 +For additional information on amsmath, use the `?' option. +(/usr/share/texmf-texlive/tex/latex/amsmath/amstext.sty +Package: amstext 2000/06/29 v2.01 +(/usr/share/texmf-texlive/tex/latex/amsmath/amsgen.sty +File: amsgen.sty 1999/11/30 v2.0 +\@emptytoks=\toks16 +\ex@=\dimen103 +)) (/usr/share/texmf-texlive/tex/latex/amsmath/amsbsy.sty +Package: amsbsy 1999/11/29 v1.2d +\pmbraise@=\dimen104 +) (/usr/share/texmf-texlive/tex/latex/amsmath/amsopn.sty +Package: amsopn 1999/12/14 v2.01 operator names +) +\inf@bad=\count88 +LaTeX Info: Redefining \frac on input line 211. +\uproot@=\count89 +\leftroot@=\count90 +LaTeX Info: Redefining \overline on input line 307. +\classnum@=\count91 +\DOTSCASE@=\count92 +LaTeX Info: Redefining \ldots on input line 379. +LaTeX Info: Redefining \dots on input line 382. +LaTeX Info: Redefining \cdots on input line 467. +\Mathstrutbox@=\box26 +\strutbox@=\box27 +\big@size=\dimen105 +LaTeX Font Info: Redeclaring font encoding OML on input line 567. +LaTeX Font Info: Redeclaring font encoding OMS on input line 568. +\macc@depth=\count93 +\c@MaxMatrixCols=\count94 +\dotsspace@=\muskip10 +\c@parentequation=\count95 +\dspbrk@lvl=\count96 +\tag@help=\toks17 +\row@=\count97 +\column@=\count98 +\maxfields@=\count99 +\andhelp@=\toks18 +\eqnshift@=\dimen106 +\alignsep@=\dimen107 +\tagshift@=\dimen108 +\tagwidth@=\dimen109 +\totwidth@=\dimen110 +\lineht@=\dimen111 +\@envbody=\toks19 +\multlinegap=\skip44 +\multlinetaggap=\skip45 +\mathdisplay@stack=\toks20 +LaTeX Info: Redefining \[ on input line 2666. +LaTeX Info: Redefining \] on input line 2667. +) (/usr/share/texmf-texlive/tex/latex/amsfonts/amssymb.sty +Package: amssymb 2002/01/22 v2.2d +(/usr/share/texmf-texlive/tex/latex/amsfonts/amsfonts.sty +Package: amsfonts 2001/10/25 v2.2f +\symAMSa=\mathgroup4 +\symAMSb=\mathgroup5 +LaTeX Font Info: Overwriting math alphabet `\mathfrak' in version `bold' +(Font) U/euf/m/n --> U/euf/b/n on input line 132. +)) (/usr/share/texmf-texlive/tex/latex/base/alltt.sty +Package: alltt 1997/06/16 v2.0g defines alltt environment +) (/usr/share/texmf-texlive/tex/latex/yfonts/yfonts.sty +Package: yfonts 2003/01/08 v1.3 (WaS) +) (/usr/share/texmf-texlive/tex/latex/footmisc/footmisc.sty +Package: footmisc 2005/03/17 v5.3d a miscellany of footnote facilities +\FN@temptoken=\toks21 +\footnotemargin=\dimen112 +\c@pp@next@reset=\count100 +\c@@fnserial=\count101 +Package footmisc Info: Declaring symbol style bringhurst on input line 817. +Package footmisc Info: Declaring symbol style chicago on input line 818. +Package footmisc Info: Declaring symbol style wiley on input line 819. +Package footmisc Info: Declaring symbol style lamport-robust on input line 823. + +Package footmisc Info: Declaring symbol style lamport* on input line 831. +Package footmisc Info: Declaring symbol style lamport*-robust on input line 840 +. +) (/usr/share/texmf-texlive/tex/latex/graphics/graphicx.sty +Package: graphicx 1999/02/16 v1.0f Enhanced LaTeX Graphics (DPC,SPQR) +(/usr/share/texmf-texlive/tex/latex/graphics/keyval.sty +Package: keyval 1999/03/16 v1.13 key=value parser (DPC) +\KV@toks@=\toks22 +) (/usr/share/texmf-texlive/tex/latex/graphics/graphics.sty +Package: graphics 2006/02/20 v1.0o Standard LaTeX Graphics (DPC,SPQR) +(/usr/share/texmf-texlive/tex/latex/graphics/trig.sty +Package: trig 1999/03/16 v1.09 sin cos tan (DPC) +) (/etc/texmf/tex/latex/config/graphics.cfg +File: graphics.cfg 2007/01/18 v1.5 graphics configuration of teTeX/TeXLive +) +Package graphics Info: Driver file: pdftex.def on input line 90. +(/usr/share/texmf-texlive/tex/latex/pdftex-def/pdftex.def +File: pdftex.def 2007/01/08 v0.04d Graphics/color for pdfTeX +\Gread@gobject=\count102 +)) +\Gin@req@height=\dimen113 +\Gin@req@width=\dimen114 +) (/usr/share/texmf-texlive/tex/latex/tools/calc.sty +Package: calc 2005/08/06 v4.2 Infix arithmetic (KKT,FJ) +\calc@Acount=\count103 +\calc@Bcount=\count104 +\calc@Adimen=\dimen115 +\calc@Bdimen=\dimen116 +\calc@Askip=\skip46 +\calc@Bskip=\skip47 +LaTeX Info: Redefining \setlength on input line 75. +LaTeX Info: Redefining \addtolength on input line 76. +\calc@Ccount=\count105 +\calc@Cskip=\skip48 +) (/usr/share/texmf-texlive/tex/latex/fancyhdr/fancyhdr.sty +\fancy@headwidth=\skip49 +\f@ncyO@elh=\skip50 +\f@ncyO@erh=\skip51 +\f@ncyO@olh=\skip52 +\f@ncyO@orh=\skip53 +\f@ncyO@elf=\skip54 +\f@ncyO@erf=\skip55 +\f@ncyO@olf=\skip56 +\f@ncyO@orf=\skip57 +) (/usr/share/texmf-texlive/tex/latex/geometry/geometry.sty +Package: geometry 2002/07/08 v3.2 Page Geometry +\Gm@cnth=\count106 +\Gm@cntv=\count107 +\c@Gm@tempcnt=\count108 +\Gm@bindingoffset=\dimen117 +\Gm@wd@mp=\dimen118 +\Gm@odd@mp=\dimen119 +\Gm@even@mp=\dimen120 +\Gm@dimlist=\toks23 +(/usr/share/texmf-texlive/tex/xelatex/xetexconfig/geometry.cfg) + +Package geometry Warning: `tmargin' and `bmargin' result in NEGATIVE (-0.44386p +t). + `height' should be shortened in length. + +) (/usr/share/texmf-texlive/tex/latex/hyperref/hyperref.sty +Package: hyperref 2007/02/07 v6.75r Hypertext links for LaTeX +\@linkdim=\dimen121 +\Hy@linkcounter=\count109 +\Hy@pagecounter=\count110 +(/usr/share/texmf-texlive/tex/latex/hyperref/pd1enc.def +File: pd1enc.def 2007/02/07 v6.75r Hyperref: PDFDocEncoding definition (HO) +) (/etc/texmf/tex/latex/config/hyperref.cfg +File: hyperref.cfg 2002/06/06 v1.2 hyperref configuration of TeXLive +) (/usr/share/texmf-texlive/tex/latex/oberdiek/kvoptions.sty +Package: kvoptions 2006/08/22 v2.4 Connects package keyval with LaTeX options ( +HO) +) +Package hyperref Info: Option `hyperfootnotes' set `false' on input line 2238. +Package hyperref Info: Option `bookmarks' set `true' on input line 2238. +Package hyperref Info: Option `linktocpage' set `false' on input line 2238. +Package hyperref Info: Option `pdfdisplaydoctitle' set `true' on input line 223 +8. +Package hyperref Info: Option `pdfpagelabels' set `true' on input line 2238. +Package hyperref Info: Option `bookmarksopen' set `true' on input line 2238. +Package hyperref Info: Option `colorlinks' set `true' on input line 2238. +Package hyperref Info: Hyper figures OFF on input line 2288. +Package hyperref Info: Link nesting OFF on input line 2293. +Package hyperref Info: Hyper index ON on input line 2296. +Package hyperref Info: Plain pages OFF on input line 2303. +Package hyperref Info: Backreferencing OFF on input line 2308. +Implicit mode ON; LaTeX internals redefined +Package hyperref Info: Bookmarks ON on input line 2444. +(/usr/share/texmf-texlive/tex/latex/ltxmisc/url.sty +\Urlmuskip=\muskip11 +Package: url 2005/06/27 ver 3.2 Verb mode for urls, etc. +) +LaTeX Info: Redefining \url on input line 2599. +\Fld@menulength=\count111 +\Field@Width=\dimen122 +\Fld@charsize=\dimen123 +\Choice@toks=\toks24 +\Field@toks=\toks25 +Package hyperref Info: Hyper figures OFF on input line 3102. +Package hyperref Info: Link nesting OFF on input line 3107. +Package hyperref Info: Hyper index ON on input line 3110. +Package hyperref Info: backreferencing OFF on input line 3117. +Package hyperref Info: Link coloring ON on input line 3120. +\Hy@abspage=\count112 +\c@Item=\count113 +) +*hyperref using driver hpdftex* +(/usr/share/texmf-texlive/tex/latex/hyperref/hpdftex.def +File: hpdftex.def 2007/02/07 v6.75r Hyperref driver for pdfTeX +\Fld@listcount=\count114 +) +\TmpLen=\skip58 +\c@ChapNo=\count115 +\c@ChapCount=\count116 +(./37157-t.aux) +\openout1 = `37157-t.aux'. + +LaTeX Font Info: Checking defaults for OML/cmm/m/it on input line 517. +LaTeX Font Info: ... okay on input line 517. +LaTeX Font Info: Checking defaults for T1/cmr/m/n on input line 517. +LaTeX Font Info: ... okay on input line 517. +LaTeX Font Info: Checking defaults for OT1/cmr/m/n on input line 517. +LaTeX Font Info: ... okay on input line 517. +LaTeX Font Info: Checking defaults for OMS/cmsy/m/n on input line 517. +LaTeX Font Info: ... okay on input line 517. +LaTeX Font Info: Checking defaults for OMX/cmex/m/n on input line 517. +LaTeX Font Info: ... okay on input line 517. +LaTeX Font Info: Checking defaults for U/cmr/m/n on input line 517. +LaTeX Font Info: ... okay on input line 517. +LaTeX Font Info: Checking defaults for LY/yfrak/m/n on input line 517. +LaTeX Font Info: ... okay on input line 517. +LaTeX Font Info: Checking defaults for LYG/ygoth/m/n on input line 517. +LaTeX Font Info: ... okay on input line 517. +LaTeX Font Info: Checking defaults for PD1/pdf/m/n on input line 517. +LaTeX Font Info: ... okay on input line 517. +(/usr/share/texmf/tex/context/base/supp-pdf.tex +[Loading MPS to PDF converter (version 2006.09.02).] +\scratchcounter=\count117 +\scratchdimen=\dimen124 +\scratchbox=\box28 +\nofMPsegments=\count118 +\nofMParguments=\count119 +\everyMPshowfont=\toks26 +\MPscratchCnt=\count120 +\MPscratchDim=\dimen125 +\MPnumerator=\count121 +\everyMPtoPDFconversion=\toks27 +) +-------------------- Geometry parameters +paper: class default +landscape: -- +twocolumn: -- +twoside: true +asymmetric: -- +h-parts: 9.03375pt, 289.07999pt, 9.03375pt +v-parts: -0.17752pt, 415.99635pt, -0.26634pt +hmarginratio: 1:1 +vmarginratio: 2:3 +lines: -- +heightrounded: -- +bindingoffset: 0.0pt +truedimen: -- +includehead: true +includefoot: true +includemp: -- +driver: pdftex +-------------------- Page layout dimensions and switches +\paperwidth 307.14749pt +\paperheight 415.55249pt +\textwidth 289.07999pt +\textheight 354.12256pt +\oddsidemargin -63.23624pt +\evensidemargin -63.23624pt +\topmargin -72.44751pt +\headheight 12.0pt +\headsep 19.8738pt +\footskip 30.0pt +\marginparwidth 98.0pt +\marginparsep 7.0pt +\columnsep 10.0pt +\skip\footins 10.8pt plus 4.0pt minus 2.0pt +\hoffset 0.0pt +\voffset 0.0pt +\mag 1000 +\@twosidetrue \@mparswitchtrue +(1in=72.27pt, 1cm=28.45pt) +----------------------- +(/usr/share/texmf-texlive/tex/latex/graphics/color.sty +Package: color 2005/11/14 v1.0j Standard LaTeX Color (DPC) +(/etc/texmf/tex/latex/config/color.cfg +File: color.cfg 2007/01/18 v1.5 color configuration of teTeX/TeXLive +) +Package color Info: Driver file: pdftex.def on input line 130. +) +Package hyperref Info: Link coloring ON on input line 517. +(/usr/share/texmf-texlive/tex/latex/hyperref/nameref.sty +Package: nameref 2006/12/27 v2.28 Cross-referencing by name of section +(/usr/share/texmf-texlive/tex/latex/oberdiek/refcount.sty +Package: refcount 2006/02/20 v3.0 Data extraction from references (HO) +) +\c@section@level=\count122 +) +LaTeX Info: Redefining \ref on input line 517. +LaTeX Info: Redefining \pageref on input line 517. +(./37157-t.out) (./37157-t.out) +\@outlinefile=\write3 +\openout3 = `37157-t.out'. + +LaTeX Font Info: Try loading font information for T1+cmtt on input line 523. + +(/usr/share/texmf-texlive/tex/latex/base/t1cmtt.fd +File: t1cmtt.fd 1999/05/25 v2.5h Standard LaTeX font definitions +) +LaTeX Font Info: Try loading font information for U+msa on input line 544. +(/usr/share/texmf-texlive/tex/latex/amsfonts/umsa.fd +File: umsa.fd 2002/01/19 v2.2g AMS font definitions +) +LaTeX Font Info: Try loading font information for U+msb on input line 544. +(/usr/share/texmf-texlive/tex/latex/amsfonts/umsb.fd +File: umsb.fd 2002/01/19 v2.2g AMS font definitions +) [1 + +{/var/lib/texmf/fonts/map/pdftex/updmap/pdftex.map}] [2] +LaTeX Font Info: Try loading font information for OML+cmr on input line 597. + +(/usr/share/texmf-texlive/tex/latex/base/omlcmr.fd +File: omlcmr.fd 1999/05/25 v2.5h Standard LaTeX font definitions +) +LaTeX Font Info: Font shape `OML/cmr/m/it' in size <12> not available +(Font) Font shape `OML/cmm/m/it' tried instead on input line 597. +[1 + + +] (./37157-t.toc [2 + + + +] [3]) +\tf@toc=\write4 +\openout4 = `37157-t.toc'. + +[4] <./images/tb.pdf, id=211, 469.755pt x 56.21pt> +File: ./images/tb.pdf Graphic file (type pdf) +<use ./images/tb.pdf> [5 + + + <./images/tb.pdf>] +File: ./images/tb.pdf Graphic file (type pdf) +<use ./images/tb.pdf> [6 + + +] [7] [8] [9] [10] [11] [12] [13] [14] +Underfull \hbox (badness 10000) in paragraph at lines 978--980 + + [] + +[15] +File: ./images/tb.pdf Graphic file (type pdf) +<use ./images/tb.pdf> [16 + + +] [17] [18] [19] [20] [21] [22] +File: ./images/tb.pdf Graphic file (type pdf) +<use ./images/tb.pdf> [1 + + + + + +] [2] [3] [4] [5] [6] [7] [8] [9] [10] [11] [12] [13] [14] [15] [16] [17] +Underfull \hbox (badness 1360) in paragraph at lines 1705--1710 +[]\T1/cmr/m/n/12 No doubt math-e-mat-i-cal re-cur-rent rea-son-ing and + [] + +[18] [19] [20] [21] [22 + + +] [23] [24] [25] [26] [27] [28] +Underfull \hbox (badness 1442) in paragraph at lines 2041--2059 +[]\T1/cmr/m/n/12 Nothing dis-tin-guishes a length di-rectly ob-served + [] + +[29] [30] [31] [32] [33] [34] [35] [36] [37] [38] [39] +Underfull \hbox (badness 1210) in paragraph at lines 2361--2368 +[]\T1/cmr/m/it/12 The Math-e-mat-i-cal Con-tin-uum of Sev-eral Di-men- + [] + +[40] [41] [42 + + +] [43] [44] [45] [46] [47] [48] [49] [50] [51] [52] [53] [54] [55] [56] [57] [5 +8] [59] [60 + + +] [61] [62] [63] [64] [65] [66] [67] [68] [69] [70] [71] [72] [73] [74] +Underfull \hbox (badness 1917) in paragraph at lines 3365--3383 +[]\T1/cmr/m/it/12 The Non-Euclidean World.\T1/cmr/m/n/12 ---If ge-o-met-ri-cal +space + [] + +[75] [76] [77] [78] [79] [80] [81] [82] [83 + + +] [84] [85] [86] [87] [88] [89] [90] [91] [92] [93] [94] [95] [96] [97] [98] [9 +9] [100] [101 + + +] [102] [103] [104] [105] [106] [107] [108] [109] [110] [111] [112] [113] [114] +[115] [116] [117] [118] [119] [120] [121] [122] [123] [124] [125 + + +] [126] [127] [128] [129] [130] [131] [132] [133] [134] [135] [136] [137] [138 + + +] [139] [140] [141] [142] [143] [144] [145] [146] [147] [148] [149] [150] [151] +[152] [153] [154] [155] [156 + + +] [157] [158] [159] [160] [161] [162] [163] [164] [165] [166] [167] [168] [169] +[170] [171] [172] [173] [174] [175] [176] [177] [178 + + +] [179] [180] [181] [182] [183] [184] +Underfull \hbox (badness 1442) in paragraph at lines 6638--6656 +[]\T1/cmr/m/it/12 Physics and Mech-a-nism.\T1/cmr/m/n/12 ---Most the-o-rists ha +ve a + [] + +[185] [186] [187] [188] [189] [190] [191] [192] [193] [194] [195] [196] [197] [ +198] [199] [200] [201] [202] [203] [204 + + +] [205] [206] [207] [208] [209] [210] [211] [212] [213] [214] [215] [216] [217] +[218] [219] [220] [221] [222] [223] [224] [225] [226] [227] [228] [229] [230] [ +231] [232] [233] [234] [235 + + +] [236] [237] [238] [239] [240] [241] [242] [243] [244] [245] [246] [247] [248] +[249] [250] +Underfull \hbox (badness 3250) in paragraph at lines 8568--8620 +[]\T1/cmr/m/n/12 I. \T1/cmr/m/it/12 Am-père's The-ory.\T1/cmr/m/n/12 ---In Am-p +ère's ex-per-i-men-tal + [] + +[251 + + +] [252] [253] [254] [255] [256] +Underfull \hbox (badness 2426) in paragraph at lines 8740--8770 +[]\T1/cmr/m/n/12 3. \T1/cmr/m/it/12 Con-tin-u-ous Ro-ta-tions.\T1/cmr/m/n/12 -- +-The most re-mark-able + [] + +[257] [258] [259] [260] [261] [262] [263] [264] +Overfull \hbox (0.82681pt too wide) in paragraph at lines 9008--9029 +[]\T1/cmr/m/n/12 III. \T1/cmr/m/it/12 Dif-fi-cul-ties raised by these The-o-rie +s.\T1/cmr/m/n/12 ---Helmholtz's + [] + +[265] [266] [267] [268] [269] [270] [271] [272] [1 + + +] [2] [3] [4] [5] [6] [7] [8] [9] [10] (./37157-t.aux) + + *File List* + book.cls 2005/09/16 v1.4f Standard LaTeX document class + leqno.clo 1998/08/17 v1.1c Standard LaTeX option (left equation numbers) + bk12.clo 2005/09/16 v1.4f Standard LaTeX file (size option) +inputenc.sty 2006/05/05 v1.1b Input encoding file + latin1.def 2006/05/05 v1.1b Input encoding file + fontenc.sty + t1enc.def 2005/09/27 v1.99g Standard LaTeX file + ifthen.sty 2001/05/26 v1.1c Standard LaTeX ifthen package (DPC) + amsmath.sty 2000/07/18 v2.13 AMS math features + amstext.sty 2000/06/29 v2.01 + amsgen.sty 1999/11/30 v2.0 + amsbsy.sty 1999/11/29 v1.2d + amsopn.sty 1999/12/14 v2.01 operator names + amssymb.sty 2002/01/22 v2.2d +amsfonts.sty 2001/10/25 v2.2f + alltt.sty 1997/06/16 v2.0g defines alltt environment + yfonts.sty 2003/01/08 v1.3 (WaS) +footmisc.sty 2005/03/17 v5.3d a miscellany of footnote facilities +graphicx.sty 1999/02/16 v1.0f Enhanced LaTeX Graphics (DPC,SPQR) + keyval.sty 1999/03/16 v1.13 key=value parser (DPC) +graphics.sty 2006/02/20 v1.0o Standard LaTeX Graphics (DPC,SPQR) + trig.sty 1999/03/16 v1.09 sin cos tan (DPC) +graphics.cfg 2007/01/18 v1.5 graphics configuration of teTeX/TeXLive + pdftex.def 2007/01/08 v0.04d Graphics/color for pdfTeX + calc.sty 2005/08/06 v4.2 Infix arithmetic (KKT,FJ) +fancyhdr.sty +geometry.sty 2002/07/08 v3.2 Page Geometry +geometry.cfg +hyperref.sty 2007/02/07 v6.75r Hypertext links for LaTeX + pd1enc.def 2007/02/07 v6.75r Hyperref: PDFDocEncoding definition (HO) +hyperref.cfg 2002/06/06 v1.2 hyperref configuration of TeXLive +kvoptions.sty 2006/08/22 v2.4 Connects package keyval with LaTeX options (HO +) + url.sty 2005/06/27 ver 3.2 Verb mode for urls, etc. + hpdftex.def 2007/02/07 v6.75r Hyperref driver for pdfTeX +supp-pdf.tex + color.sty 2005/11/14 v1.0j Standard LaTeX Color (DPC) + color.cfg 2007/01/18 v1.5 color configuration of teTeX/TeXLive + nameref.sty 2006/12/27 v2.28 Cross-referencing by name of section +refcount.sty 2006/02/20 v3.0 Data extraction from references (HO) + 37157-t.out + 37157-t.out + t1cmtt.fd 1999/05/25 v2.5h Standard LaTeX font definitions + umsa.fd 2002/01/19 v2.2g AMS font definitions + umsb.fd 2002/01/19 v2.2g AMS font definitions + omlcmr.fd 1999/05/25 v2.5h Standard LaTeX font definitions +./images/tb.pdf +./images/tb.pdf +./images/tb.pdf +./images/tb.pdf + *********** + + ) +Here is how much of TeX's memory you used: + 5416 strings out of 94074 + 70012 string characters out of 1165154 + 139676 words of memory out of 1500000 + 8147 multiletter control sequences out of 10000+50000 + 29817 words of font info for 77 fonts, out of 1200000 for 2000 + 646 hyphenation exceptions out of 8191 + 29i,12n,46p,258b,493s stack positions out of 5000i,500n,6000p,200000b,5000s +{/usr/share/texmf/fonts/enc/dvips/cm-super/cm-super-t1.enc}</usr/share/texmf- +texlive/fonts/type1/bluesky/cm/cmex10.pfb></usr/share/texmf-texlive/fonts/type1 +/bluesky/cm/cmmi10.pfb></usr/share/texmf-texlive/fonts/type1/bluesky/cm/cmmi12. +pfb></usr/share/texmf-texlive/fonts/type1/bluesky/cm/cmmi8.pfb></usr/share/texm +f-texlive/fonts/type1/bluesky/cm/cmr10.pfb></usr/share/texmf-texlive/fonts/type +1/bluesky/cm/cmr12.pfb></usr/share/texmf-texlive/fonts/type1/bluesky/cm/cmr8.pf +b></usr/share/texmf-texlive/fonts/type1/bluesky/cm/cmsy10.pfb></usr/share/texmf +-texlive/fonts/type1/bluesky/cm/cmsy8.pfb></usr/share/texmf/fonts/type1/public/ +cm-super/sfcc1000.pfb></usr/share/texmf/fonts/type1/public/cm-super/sfcc1095.pf +b></usr/share/texmf/fonts/type1/public/cm-super/sfcc1200.pfb></usr/share/texmf/ +fonts/type1/public/cm-super/sfrm0700.pfb></usr/share/texmf/fonts/type1/public/c +m-super/sfrm0800.pfb></usr/share/texmf/fonts/type1/public/cm-super/sfrm1000.pfb +></usr/share/texmf/fonts/type1/public/cm-super/sfrm1095.pfb></usr/share/texmf/f +onts/type1/public/cm-super/sfrm1200.pfb></usr/share/texmf/fonts/type1/public/cm +-super/sfrm1440.pfb></usr/share/texmf/fonts/type1/public/cm-super/sfrm1728.pfb> +</usr/share/texmf/fonts/type1/public/cm-super/sfrm2488.pfb></usr/share/texmf/fo +nts/type1/public/cm-super/sfti0800.pfb></usr/share/texmf/fonts/type1/public/cm- +super/sfti1000.pfb></usr/share/texmf/fonts/type1/public/cm-super/sfti1095.pfb>< +/usr/share/texmf/fonts/type1/public/cm-super/sfti1200.pfb></usr/share/texmf/fon +ts/type1/public/cm-super/sftt0800.pfb></usr/share/texmf/fonts/type1/public/cm-s +uper/sftt1095.pfb></usr/share/texmf-texlive/fonts/type1/public/gothic/yswab.pfb +> +Output written on 37157-t.pdf (306 pages, 994390 bytes). +PDF statistics: + 1752 PDF objects out of 2073 (max. 8388607) + 453 named destinations out of 1000 (max. 131072) + 230 words of extra memory for PDF output out of 10000 (max. 10000000) + diff --git a/37157-t/old/37157-t.zip b/37157-t/old/37157-t.zip Binary files differnew file mode 100644 index 0000000..554f9f9 --- /dev/null +++ b/37157-t/old/37157-t.zip |
