<?xml version="1.0"?>
<!DOCTYPE html    PUBLIC "-//W3C//DTD XHTML 1.1 plus MathML 2.0//EN"
           "http://www.w3.org/Math/DTD/mathml2/xhtml-math11-f.dtd">
<html xmlns="http://www.w3.org/1999/xhtml">
<head>
<title>H. Poincar&eacute; Correspondence</title>
<meta http-equiv="content-type" content="text/html; charset=utf-8"></meta>
<meta name="keywords" content="poincar&eacute;, letters, henri, correspondence, scientifique"></meta>
<style type="text/css">
 div.p { margin-top: 7pt; }
span.roman {font-family: serif; font-style: normal; font-weight: normal;}
</style>
</head>
<body>






 



<div class="p"><!----></div>


<div class="p"><!----></div>







 
<div class="p"><!----></div>
 




 


<div class="p"><!----></div>















    
  
  
   
<h2>Poincaré's <em>Thermodynamique,</em> by P.G. Tait</h2><a name="tait0">
</a>
<div class="p"><!----></div>

<div align="right">[14.01.1892]<a href="#tthFtNtAAB" name="tthFrefAAB">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>1</mn></mrow>
</msup>
</mrow></math></a>
</div>

<div class="p"><!----></div>

<div class="p"><!----></div>
The great expectations with which, on account of the well-won fame of
its Author, we took up this book have unfortunately not been
realized.The main reason is not far to seek, and requires 
no lengthened exposition. Its nature will be obvious from the 
following examples.

<div class="p"><!----></div>
The late Prof. W.H. Miller, as able a mathematician as he was a
trustworthy experimenter, regularly commenced his course of
Crystallography at Cambridge (after seizing the chalk and drawing a
diagram on the black board) with the words: "Gentlemen, let O
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>,
O
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>y</mi></mrow></math>, O
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>z</mi></mrow></math> be the coordinate axes."<a href="#tthFtNtAAC" name="tthFrefAAC">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></math></a> And, some forty years ago, in a certain mathematical
circle at Cambridge, men were wont to deplore the necessity of
introducing words <i>at all</i> in a physico-mathematical text-book:
the unattainable, though closely approachable, Ideal being regarded as
a work devoid of aught but formulæ!

<div class="p"><!----></div>
But one learns something in forty years, and accordingly the 
surviving members of that circle now take a very different view 
of the matter. They have been taught, alike by experience and 
by example, to regard mathematics, so far at least as physical 
inquiries are concerned, as a mere auxiliary to thought: of 
a vastly higher order of difficulty, no doubt, than ordinary 
numerical calculations, but still to be regarded as of essentially 
the same kind. This is one of the great truths which were enforced 
by Faraday's splendid career.

<div class="p"><!----></div>
And the consequence, in this country at least, has been that we 
find in the majority of the higher class of physical text-books 
few except the absolutely indispensable formulæ. Take, for 
instance, that profound yet homely and unpretentious work, Clerk-Maxwell's 
<i>Theory of Heat.</i> Even his great work, <i>Electricity</i>, though 
it seems to bristle with formulæ, contains but few which are 
altogether unnecessary. Compare it, in this respect, with the 
best of more recent works on the same advanced portions of the 
subject. 

<div class="p"><!----></div>
In M.&nbsp;Poincaré's work, however, all this is changed. Over and 
over again, in the frankest manner (see, for instance, pp.&nbsp;xvi, 
176), he confesses that he lays himself open to the charge of 
introducing unnecessary mathematics: and there are many other 
places where, probably thinking such a confession would be too 
palpably superfluous, he does not feel constrained to make it. 
This feature of his work, at least, is sure to render it acceptable 
to one limited but imposing body, the <i>Examiners for the Mathematical 
Tripos (Part II.).</i>

<div class="p"><!----></div>
M.&nbsp;Poincaré not only ranks very high indeed among pure mathematicians
but has done much excellent and singularly original work in applied
mathematics: all the more therefore should he be warned to bear in
mind the words of Shakespeare<a href="#tthFtNtAAD" name="tthFrefAAD">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>3</mn></mrow>
</msup>
</mrow></math></a>

<blockquote>
"Oh ! it is excellent <br />
To have a giant's strength; but it is tyrannous<br />
To use it like a giant."
</blockquote>
From the physical point of view, however, there is much more 
than this to be said. For mathematical analysis, like arithmetic, 
should never be appealed to in a physical inquiry till unaided 
thought has done its utmost. Then, and not till then, is the investigator 
in a position rightly to embody his difficulty in the language 
of symbols, with a clear understanding of what is demanded from 
their potent assistance. The violation of this rule is very frequent 
in M.&nbsp;Poincaré's work and is one main cause of its quite unnecessary 
bulk. Solutions of important problems, which are avowedly imperfect 
because based on untenable hypotheses (see, for instance, §§&nbsp;284-286),
are not useful to a student, even as a warning: they 
are much more likely to create confusion, especially when a complete 
solution, based upon full experimental data and careful thought, 
can be immediately afterwards placed before him. If something 
is really desired, in addition to the complete solution of any 
problem, the proper course is to prefix to the complete treatment 
one or more exact solutions of simple cases. This course is almost 
certain to be useful to the student. The whole of M.&nbsp;Poincaré's 
work savours of the consciousness of mathematical power: and 
exhibits a lavish, almost a reckless, use of it. Todhunter's 
favourite phrase, when one of his pupils happened to use processes 
more formidable than the subject required, was "Hm: breaking 
a fly on the wheel!" He would have had frequent occasion to use 
it during a perusal of this volume. An excellent instance of 
the dangerous results of this lavish display of mathematical 
skill occurs at pp.&nbsp;137-38, the greater part of which (<em>as printed</em>) 
consists of a mass of error of which no one, certainly, would 
accuse M.&nbsp;Poincaré. The cause must therefore be traced to the 
unnecessary display of dexterity with which, after obtaining 
the equation
<br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow>
<msub><mrow><mi>Q</mi></mrow><mrow><mn>2</mn></mrow>
</msub>
<mo stretchy="false">/</mo>
<msub><mrow><mi>Q</mi></mrow><mrow><mn>1</mn></mrow>
</msub>
<mo>=</mo><mn>1</mn><mo>-</mo><mi>Af</mi><mo stretchy="false">(</mo>
<msub><mrow><mi>T</mi></mrow><mrow><mn>1</mn></mrow>
</msub>
<mo>,</mo>
<msub><mrow><mi>T</mi></mrow><mrow><mn>2</mn></mrow>
</msub>
<mo stretchy="false">)</mo><mo>,</mo></mrow>
    </mstyle></math>
</td></tr></table>
<br />

where the <i>order</i> of the suffixes is evidently of paramount 
importance, M.&nbsp;Poincaré proceeded to say "Nous pouvons 
donc écrire
<br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow>
<msub><mrow><mi>Q</mi></mrow><mrow><mn>1</mn></mrow>
</msub>
<mo stretchy="false">/</mo>
<msub><mrow><mi>Q</mi></mrow><mrow><mn>2</mn></mrow>
</msub>
<mo>=</mo><mi>&Phi;</mi><mo stretchy="false">(</mo>
<msub><mrow><mi>T</mi></mrow><mrow><mn>1</mn></mrow>
</msub>
<mo>,</mo>
<msub><mrow><mi>T</mi></mrow><mrow><mn>2</mn></mrow>
</msub>
<mo stretchy="false">)</mo>
<mtext>."</mtext>
</mrow>
    </mstyle></math>
</td></tr></table>
<br />

But his unfortunate printer, not prepared for such a <i>tour de
  force</i>, very naturally repeated the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>Q</mi></mrow><mrow><mn>2</mn></mrow>
</msub>
<mo stretchy="false">/</mo>
<msub><mrow><mi>Q</mi></mrow><mrow><mn>1</mn></mrow>
</msub>
</mrow></math> of the first
equation, with the result of wholly falsifying all that follows. On
the other hand, we must fully recognize that, when more formidable
analysis is really required (as, for instance, in the treatment of v.&nbsp;Helmholtz's monocyclic and polycyclic systems), M.&nbsp;Poincaré seems to
feel so thoroughly at home as to criticize with
freedom.

<div class="p"><!----></div>
One test of the soundness of an author, writing on Thermodynamics, is
his treatment of temperature, and his introduction of absolute
temperature. M.&nbsp;Poincaré gets over this part of his work very
expeditiously. In §§&nbsp;15-17 temperature, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi></mrow></math>, is conventionally
defined as in the Centigrade thermometer by means of the volume of a
given quantity of mercury; or by any continous function of that volume
which increases along with it. Next (§&nbsp;22) absolute temperature, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>T</mi></mrow></math>,
is defined, provisionally and with a caution, as 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mn>273</mn><mo>+</mo><mi>t</mi></mrow></math>; from the
(so-called) laws of Mariotte and Gay-Lussac. Then, finally (§&nbsp;118),
absolute temperature is virtually defined afresh as the reciprocal of
Carnot's function. [We say <i>virtually</i>, as we use the term in
the sense defined by Thomson.  M.&nbsp;Poincaré's <i>fonction de
  Carnot</i> is a different thing.]  But there seems to be no hint given
as to the results of experiments made expressly to compare these two
definitions. Nothing, for instance, in this connection at all events,
is said about the long-continued early experimental work of Joule and
Thomson, which justified them in basing the measurement of absolute
temperature on Carnot's function.

<div class="p"><!----></div>
In saying this, however, we must most explicitly disclaim any 
intention of charging M.&nbsp;Poincaré with even a trace of that 
sometimes merely invidious, sometimes purely Chauvinistic, spirit 
which has done so much to embitter discussions of the history 
of the subject. On the contrary, we consider that he gives far 
too little prominence to the really extraordinary merits of his 
own countryman Sadi Carnot. He writes not as a partisan but rather 
as one to whom the history of the subject is a matter of all 
but complete indifference. So far, in fact, does he carry this 
that the name of Mayer, which frequently occurs, seems to be 
spelled incorrectly on by far the greater number of these occasions! 
He makes, however, one very striking historical statement (§&nbsp;95): 
"Clausius ... lui donna le nom de <i>Principe de Carnot</i>, bien 
qu'il l'eût énoncé sans avoir connaissance des travaux de 
Sadi Carnot."

<div class="p"><!----></div>
Still, one naturally expects to find, in a Treatise such as this, 
some little allusion at least to Thermodynamic Motivity; to its 
waste, the Dissipation of Energy; and to the rest of those important 
early results of Sir W. Thomson, which have had such immense 
influence on the development of the subject. We look in vain 
for any mention of Rankine or of his Thermodynamic Function; 
though we have enough, and to spare, of it under its later <i>alias</i> 
of Entropy. The word dissipation does indeed occur, for we are 
told in the Introduction that the <i>Principe de Carnot</i> is "<i>la 
dissipation de l'entropie</i>."<a href="#tthFtNtAAE" name="tthFrefAAE">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>4</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
We find Bunsen and Mousson cited, with regard to the effect of 
pressure upon melting points, almost before a word is said of 
James Thomson; and, when that word does come, it wholly fails 
to exhibit the real nature or value of the great advance he
made.<a href="#tthFtNtAAF" name="tthFrefAAF">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>5</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
Andrews again, <i>à propos</i> of the critical point, and his 
splendid work on the isothermals of carbonic acid, comes in for 
the barest mention only <i>after</i> a long discussion of those 
very curves, and of the equations suggested for them by Van der 
Waals, Clausius, and Sarrau: though his work was the acknowledged 
origin of their attempts.<a href="#tthFtNtAAG" name="tthFrefAAG">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>6</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
The reason for all this is, as before hinted, that M.&nbsp;Poincaré 
has, in this work, chosen to play almost exclusively the part 
of the pure technical analyst; instead of that of the profound 
thinker, though he is perfectly competent to do that also when 
he pleases. And, in his assumed capacity, he quite naturally 
looks with indifference, if not with absolute contempt, on the 
work of the lowly experimenter. Yet, in strange contradiction 
to this, and still more in contradiction to his ascription of 
the Conservation of Energy to Mayer, he says of that principle: 
"personne n'ignore que c'est un fait expérimental."

<div class="p"><!----></div>
Even the elaborate thermo-electric experiments of Sir W. Thomson, 
Magnus, &amp;c., are altogether ignored. What else can we gather 
from passages like the following?

<blockquote>
(§&nbsp;287) "Sir W. Thomson admet qu'il existe une force électromotrice 
au contact de deux portions d'un même conducteur à des températures 
différentes; il assimile donc ces deux portions à deux conducteurs 
de nature différente, assimilation qui paraît très vraisemblable."<br />
(§&nbsp;291) "... si l'effet Thomson a pu être mis en évidence 
par l'expérience, on n'a pu jusqu'ici constater l'existence 
des forces électromotrices qui lui donnent naissance."
</blockquote>

<div class="p"><!----></div>
Everyone who comes to this work of M.&nbsp;Poincaré fresh from the study of
Clerk-Maxwell's little treatise (or of the early papers of Thomson, to
which it owed much) will feel as if transferred to a totally new
world. Let him look, for instance, at Maxwell's treatment of the
Thermodynamic Relations, Intrinsic and Available Energy, &amp;c., and
then turn to pp.&nbsp;148-150 of M.&nbsp;Poincaré's work. There he will find at
least a large portion of these most important matters embodied in what
it seems we are now to call the <i>Fonctions caractéristiques de
  M.&nbsp;Massieu!</i><a href="#tthFtNtAAH" name="tthFrefAAH">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>7</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
But the most unsatisfactory part of the whole work is, it seems 
to us, the entire ignoration of the true (<i>i.e.</i> the statistical) 
basis of the second Law of Thermodynamics. According to Clerk-Maxwell 
(<em>Nature,</em> xvii.&nbsp;278)

<blockquote>
"The touch-stone of a treatise on Thermodynamics is what is called 
the second law."
</blockquote>

<div class="p"><!----></div>
We need not quote the very clear statement which follows this, 
as it is probably accessible to all our readers. It certainly 
has not much resemblance to what will be found on the point in 
M.&nbsp;Poincaré's work: so little, indeed, that if we were to 
judge by these two writings alone it would appear that, with 
the exception of the portion treated in the recent investigations 
of v. Helmholtz, the science had been retrograding, certainly 
not advancing, for the last twenty years.

<div class="p"><!----></div>
P. G. T.

<div class="p"><!----></div>
<br /><br /><font size="-1"><b>PD. 
  
  <a href="#TaiP1892a" name="CITETaiP1892a">Tait [1892</a>]
 .</b><font size="+0">

<div class="p"><!----></div>

<h2>R&#233;f&#233;rences</h2>

<dl compact="compact">
                                                                                                                                                                                                                                                                                          
<div class="p"><!----></div>

 <dt><a href="#CITEhp1892th" name="hp1892th">[Poincar&#233; 1892]</a></dt><dd>
Poincar&#233;, H.
 <em>Thermodynamique</em>.
   Publi&#233; par J.&nbsp;Blondin. Paris: Georges Carr&#233;, 1892.

<div class="p"><!----></div>
</dd>
 <dt><a href="#CITETaiP1892a" name="TaiP1892a">[Tait 1892]</a></dt><dd>
Tait, P.&nbsp;G.
 Poincar&#233;'s Thermodynamics.
 <em>Nature</em> 45 (1892): 245-246.</dd>
</dl>

Time-stamp: &lt;30.12.2011 00:42&#62;
</font></font><hr /><h3>Notes:</h3>

<div class="p"><!----></div>
<a name="tthFtNtAAB"></a><a href="#tthFrefAAB">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>1</mn></mrow>
</msup>
</mrow></math></a>Book review, published on 14.01.1892.
<div class="p"><!----></div>
<a name="tthFtNtAAC"></a><a href="#tthFrefAAC">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></math></a>William Hallowes Miller
  (1801-1880).
<div class="p"><!----></div>
<a name="tthFtNtAAD"></a><a href="#tthFrefAAD">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>3</mn></mrow>
</msup>
</mrow></math></a>Isabella to Angelo, in
  <em>Measure for Measure</em>, act 2, scene 2.
<div class="p"><!----></div>
<a name="tthFtNtAAE"></a><a href="#tthFrefAAE">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>4</mn></mrow>
</msup>
</mrow></math></a>
  
  <a href="#hp1892th" name="CITEhp1892th">Poincar&#233; [1892</a>,1]
 .
<div class="p"><!----></div>
<a name="tthFtNtAAF"></a><a href="#tthFrefAAF">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>5</mn></mrow>
</msup>
</mrow></math></a>Robert Bunsen, Albert Mousson (1805-1890).
<div class="p"><!----></div>
<a name="tthFtNtAAG"></a><a href="#tthFrefAAG">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>6</mn></mrow>
</msup>
</mrow></math></a>Thomas Andrews (1813-1885), J.D. van der Waals,
  Rudolf Clausius, Émile Sarrau.
<div class="p"><!----></div>
<a name="tthFtNtAAH"></a><a href="#tthFrefAAH">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>7</mn></mrow>
</msup>
</mrow></math></a>The functions to which Tait objects are those
  Jacques Massieu (1832-1896) presented in a series of notes on the
  "fonctions caractéristiques des divers fluides", in the
  <em>Comptes rendus</em> 69 (1869). For Poincaré
  
 

 

[<a href="#hp1892th" name="CITEhp1892th">&nbsp;Poincar&#233; 1892</a>,150]
  
, a "great simplification" may be
  realized in certain cases, as the equations of thermodynamics may be
  expressed in terms of Massieu's functions and their derivatives
  only.
<br /><br /><hr />
<a href="../index.html"><img src="../icons/contents_motif.gif" alt="contents_motif.gif" /></a>
&#x00A0;&#x00A0;&#x00A0;&#x00A0;&#x00A0;&#x00A0;
<a href="/poincare/chp/">Archives Henri Poincar&eacute;</a> (CNRS, UMR 7117)
</body>
</html>

