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<title>S. Walter: Minkowski, Mathematicians, and the Mathematical Theory of Relativity</title></head>
<body>

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


<a href="../index.html"><img src="../icons/contents_motif.gif" alt="../icons/contents_motif.gif" /></a>&#x00A0;&#x00A0;&#x00A0;&#x00A0;&#x00A0;&#x00A0;<font size="+2"><b><font color="#FFB528">Article</font></b></font>

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

<h1 align="center">Minkowski, Mathematicians and the Mathematical Theory of
Relativity </h1>

<h3 align="center">Scott Walter<br />
walter [at] univ-nancy2.fr </h3>

<h3 align="center">Preprint, published in H.&#x00A0;Goenner, J.&#x00A0;Renn, J.&#x00A0;Ritter, and T.&#x00A0;Sauer (eds.), <em>The
      Expanding Worlds of General Relativity</em>, Birkh&#228;user, 1999, 45-86. </h3>  




<h2>Introduction</h2>

<div class="p"><!----></div>
The importance of the theory of relativity for twentieth-century
physics, and the appearance of the G&#246;ttingen mathematician Hermann
Minkowski at a turning point in its history have both attracted
significant historical attention. The rapid growth in scientific and
philosophical interest in the principle of relativity has been linked
to the intervention of Minkowski by Tetu Hirosige, who identified
Minkowski's publications as the turning point for the theory of
relativity, and gave him credit for having clarified its fundamental
importance for all of physics (Hirosige 1968: 46; 1976: 78).  Lewis
Pyenson has placed Minkowski's work in the context of a mathematical
approach to physics popular in G&#246;ttingen, and attributed its success
to the prevalence of belief in a neo-Leibnizian notion of
pre-established harmony between pure mathematics and physics (Pyenson
1985, 1987: 95).  The novelty to physics of the aesthetic canon
embodied in Minkowski's theory was emphasized by Peter Galison (1979),
and several scholars have clarified technical and epistemological
aspects of Minkowski's theory.<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>
In particular, the introduction of sophisticated mathematical
techniques to theoretical physics by Minkowski and others is a theme
illustrated by Christa Jungnickel and Russell
McCormmach.<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>

<div class="p"><!----></div>
In what follows, we address another aspect of Minkowski's role in the
history of the theory of relativity: his disciplinary advocacy.
Minkowski's 1908 Cologne lecture "Raum und Zeit" (Minkowski
1909) may be understood as an effort to extend the disciplinary frontier
of mathematics to include the principle of relativity. We discuss the
tension created by a mathematician's intrusion into the specialized realm
of theoretical physics, and Minkowski's strategy to overcome disciplinary
obstacles to the acceptance of his work. The effectiveness of his approach
is evaluated with respect to a selection of responses, and related to
trends in bibliometric data on disciplinary contributions to
non-gravitational theories of relativity through 1915.

<div class="p"><!----></div>
 <h2><a name="tth_sEc1">
1</a>&#x00A0;&#x00A0;Minkowski's authority in mathematics and physics</h2>

<div class="p"><!----></div>
 At the time of the meeting of the German Association in late
September 1908, Minkowski was recognized as an authority on the theory
of relativity nowhere outside of the university town of G&#246;ttingen. The
structure and content of Minkowski's lecture, we will see later, was in
many ways a function of a perceived deficit of credibility. In order to
understand this aspect of Minkowski's lecture, we first examine how
Minkowski became acquainted with the electrodynamics of moving bodies.

<div class="p"><!----></div>
Around 1907, Minkowski's scientific reputation rested largely upon his
contribution to number theory.<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>
Yet Minkowski was also the author of an article on capillarity (1906) in
the authoritative <i>Encyklop&#228;die der mathematischen Wissenschaften</i>,
granting him a credential in the domain of mechanics and mathematical
physics. In addition, Minkowski had lectured on capillarity, potential
theory, and analytical mechanics, along with mathematical subjects such as
Analysis Situs and number theory at Zurich Polytechnic, where Einstein,
Marcel Grossmann and Walter Ritz counted among his students; he also
lectured on mechanics and electrodynamics (among other subjects) in
G&#246;ttingen, where he held the third chair in mathematics, created for him
at David Hilbert's request in 1902.<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>
In G&#246;ttingen, Minkowski took an interest in a subject strongly associated
with the work of many of his new colleagues: electron theory. An early
manifestation of this interest was Minkowski's co-direction of a seminar
on the subject with his friend Hilbert, plus Gustav Herglotz and Emil
Wiechert, which met during the summer semester of 1905.<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>
While Lorentz's 1904 paper (with a form of the transformations now bearing
his name) was not on the syllabus, and Einstein's 1905 paper had not yet
appeared, one of the students later recalled that Minkowski had hinted
that he was engaged with the Lorentz transformations.<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>
Minkowski was also busy with his article on capillarity, however, and for
the next two years there is no trace of his engagement with the theory of
relativity. In October 1907, Minkowski wrote to Einstein to request an
offprint of his <i>Annalen</i> article on the electrodynamics of moving
bodies, for use in his seminar on the partial differential equations of
physics, jointly conducted by Hilbert.<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>
During the following Easter vacation, he gave a short series of lectures
on "New Ideas on the Basic Laws of Mechanics" for the benefit of science 
teachers.<a href="#tthFtNtAAI" name="tthFrefAAI">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>8</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
In what seem to be notes to these holiday lectures, Einstein's knowledge
of mathematics was subject to criticism. Minkowski reminded his audience
that he was qualified to make this evaluation, since Einstein had him to
thank for his education in mathematics. From Zurich Polytechnic, Minkowski
added, a complete knowledge of mathematics could not be obtained.<a href="#tthFtNtAAJ" name="tthFrefAAJ">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>9</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
This frank assessment of Einstein's skills in mathematics, Minkowski
explained, was meant to establish his right to evaluate Einstein's work,
since he did not know how much his authority carried with respect to "the
validity of judgments in physical things," which he wanted "now to
submit." A pattern was established here, in which Minkowski would first
suggest that Einstein's work was mathematically incomplete, and then call
upon his authority in mathematics in order to validate his judgments in
theoretical physics. While Minkowski implicitly recognized Einstein's
competence in questions of physics, he did not yet appreciate how much
Europe's leading physicists admired the work of his former student.<a href="#tthFtNtABA" name="tthFrefABA">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>10</mn></mrow>
</msup>
</mrow></math></a>
Even in his fief of G&#246;ttingen, Minkowski knew he could not expect any
authority to be accorded to him in theoretical physics, yet this awareness
of his own lack of credentials in physics did not prevent him from
lecturing on the principle of relativity.

<div class="p"><!----></div>
While the scientific world had no real means of judging Minkowski's
competence in theoretical physics due to the paucity of relevant
publications, Minkowski himself did not consider his knowledge in physics
to be extensive. It is for this reason that he sought an assistant
capable of advising him on physical matters, and when Max Born-a former
student from the electron theory seminar-wrote him from Breslau (now
Wroc aw, Poland) for help with a technical problem, he found a suitable
candidate.

<div class="p"><!----></div>
Initially attracted to mathematics, Born heard lectures by Leo
K&#246;nigsberger in Heidelberg, and Adolf Hurwitz in Zürich, and later
considered Hurwitz's private lectures as the high point of his student
career. In G&#246;ttingen, Born obtained a coveted position as Hilbert's
private assistant, and began a doctoral dissertation on Bessel functions
under Hilbert's direction. When he abandoned the topic, as Born recalled
in old age, Hilbert laughed and consoled him, saying he was much better
in physics.<a href="#tthFtNtABB" name="tthFrefABB">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>11</mn></mrow>
</msup>
</mrow></math></a>
In the same year, Born attended Hilbert and Minkowski's electron theory
seminar, along with Max Laue and Jakob Laub, among others (Born 1959: 682;
Pyenson 1985: 102). Profoundly influenced by what he learned in this 
seminar, and deeply devoted to both Hilbert and Minkowski, Born was not
permitted to write a dissertation on electron theory, although the idea
appealed to him (Born 1959: 684). Felix Klein obliged him to write a
dissertation on elasticity theory, but in order to avoid having "the great
Felix" as an examiner, Born took up Karl Schwarzschild's suggestion to
prepare for the oral examination in astronomy (Born 1906, 1968: 20-21).
After defending his doctoral dissertation on 14 January 1907, Born spent six
months in Cambridge with Joseph Larmor and J.&#x00A0;J.&#x00A0;Thomson before returning to
Breslau, where the young theoretical physicists  Stanislaus Loria and Fritz
Reiche brought Einstein's 1905 <i>Annalen</i> paper on relativity to his
attention (Born 1959: 684).

<div class="p"><!----></div>
In studying relativity with Reiche, as Born recounted later, he
encountered some difficulties. He formulated these in a letter to
Minkowski, seeking his former teacher's advice. Minkowski's response
to Born's letter was a great surprise, for instead of the requested
technical assistance, Minkowski offered him the possibility of an
academic career. Minkowski wrote that he had been working on the same
problem as Born, and that he "would like to have a young collaborator
who knew something of physics, and of optics in particular" (Born
1978: 130).<a href="#tthFtNtABC" name="tthFrefABC">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>12</mn></mrow>
</msup>
</mrow></math></a>  Besides mathematics, Born had studied physics in
G&#246;ttingen, attending Voigt's "stimulating" lectures on optics and an
advanced course on optical experimentation (Born 1968: 21). It was
just this background in optics that Minkowski lacked, and he looked to
Born to guide him through unknown territory. In return, Minkowski
promised Born he would open the doors to an academic career. The
details were to be worked out when they met at the meeting of the
German Association of Scientists and Physicians, later that year in
Cologne (Born 1978: 130).<a href="#tthFtNtABD" name="tthFrefABD">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>13</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
In April 1908, Minkowski published a technically accomplished paper on
the electromagnetic processes in moving bodies ("Die Grundgleichungen
f&#252;r die electromagnetischen Vorg&#228;nge in bewegten K&#246;rpern," hereafter
<i>Grundgleichungen </i>). In this essay, Minkowski wrote the empty-space
field equations of relativistic electrodynamics in four-dimensional form,
using Arthur Cayley's matrix calculus. He also derived the equations of 
electrodynamics of moving media, and formulated the basis of a mechanics
appropriate to four-dimensional space with an indefinite squared
interval. Minkowski's study represented the first elaboration of the
principle of relativity by a mathematician in Germany.

<div class="p"><!----></div>
Soon after its publication, the <em>Grundgleichungen</em> sustained
restrained comment from Minkowski's former students Albert Einstein and
Jakob Laub (1908a, 1908b). These authors rejected out of hand the
four-dimensional apparatus of Minkowski's paper, the inclusion of which,
they wrote, would have placed "rather great demands" on their readers
(1908a: 532). No other reaction to Minkowski's work was published before
the Cologne meeting.

<div class="p"><!----></div>
By the fall of 1908, Minkowski had spoken publicly of his views on
relativity on several occasions, but never outside of G&#246;ttingen. The
annual meeting of the German Association was Minkowski's first
opportunity to speak on relativity before an elite international audience 
of physicists, mathematicians, astronomers, chemists and engineers. At no
other meeting could a scientist in Germany interact with other
professionals working in disciplines outside of his own.

<div class="p"><!----></div>
The organization of the various disciplinary sections of the annual
meeting of the German Association fell to the corresponding
professional societies (Forman 1967: 156). For example, the German
Physical Society organized the physics section, and the German Society
of Mathematicians managed the mathematics section. For the latter
section, the theme of discussion was announced in late April by the
society's president, Felix Klein. In a call for papers, Klein
encouraged authors to submit works especially in the area of
mechanics. Prior to the announcement, however, Klein must have already
arranged at least one contribution in mechanics, since he added a
teaser, promising an "expert aspect" of a recent investigation in
this area.<a href="#tthFtNtABE" name="tthFrefABE">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>14</mn></mrow>
</msup>
</mrow></math></a> It is tempting to identify this as a forward reference to
Minkowski's lecture, a draft of which predates Klein's communication
by a few days.  The lecture was to be the first talk out of seven in
the mathematics section, which doubled as a session of the German
Society of Mathematicians.<a href="#tthFtNtABF" name="tthFrefABF">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>15</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
 <h2><a name="tth_sEc2">
2</a>&#x00A0;&#x00A0;The Cologne lecture</h2>

<div class="p"><!----></div>
 The G&#246;ttingen archives contain four distinct manuscript drafts
of Minkowski's Cologne lecture, none of which corresponds precisely to
either of the two printed versions of the lecture in the original
German.<a href="#tthFtNtABG" name="tthFrefABG">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>16</mn></mrow>
</msup>
</mrow></math></a> Unless
stipulated otherwise, we refer here to the longer essay published
posthumously in both the <i>Physikalische Zeitschrift</i> and the <i>
  Jahresbericht der deutschen Mathematiker-Vereinigung</i> in early 1909.

<div class="p"><!----></div>
From the outset of his lecture, Minkowski announced that he would reveal
a radical change in the intuitions of space and time:

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

<blockquote>Gentlemen! The conceptions of space and time which I would like to
develop before you arise from the soil of experimental physics. Therein
lies their strength. Their tendency is radical. From this hour on, space
by itself and time by itself are to sink fully into the shadows and only a
kind of union of the two should yet preserve autonomy.

<div class="p"><!----></div>
First of all I would like to indicate how, [starting] from the mechanics
accepted at present, one could arrive through purely mathematical
considerations at changed ideas about space and time.<a href="#tthFtNtABH" name="tthFrefABH">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>17</mn></mrow>
</msup>
</mrow></math></a>
(Minkowski 1909: 75)
</blockquote>

<div class="p"><!----></div>
 The evocation of experimental physics was significant in the
first sentence of Minkowski's lecture, and it was deceptive. In what
followed, Minkowski would refer to experimental physics only once, to
invoke the null result of Albert A. Michelson's optical experiment to
detect motion with respect to the luminiferous ether. Otherwise,
Minkowski kept his promise of a "<i>rein mathematische</i>" expos&#233;,
devoid of experimental considerations. A purely theoretical presentation
enabled Minkowski to finesse the recent well-known experimental results
purporting to disconfirm relativity theory, obtained by Walter 
Kaufmann.<a href="#tthFtNtABI" name="tthFrefABI">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>18</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
Less illusory than the mention of experimental physics was Minkowski's
announcement of a radical change in conceptions of space and time. That
this revelation was local and immediate, is signaled by the phrase "from
this hour on" [<i>von Stund' an </i>]. Here it was announced that a union
of space and time was to be revealed, and for the first time. This was a
rhetorical gesture (all of the results presented in the Cologne lecture
had been published in the <i>Grundgleichungen </i>), but it was an
effective one, because the phrase in question became emblematic of the
theory of relativity in broader circles.

<div class="p"><!----></div>
It may be noted from the outset that the claims Minkowski made for his
theory fell into two categories. In one category were Minkowski's claims
for scientific priority, which concerned the physical, mathematical and
philosophical aspects of his theory of relativity. In what follows, we
will concentrate on the second category of claims, which were <i>
metatheoretical</i> in nature. The latter claims concerned the theory's
type, not its constituent elements. Claims of the second sort, all having
to do with the geometric nature of the theory, reinforced those of the
first sort. The opening remarks provide an example: the allusion to 
changed ideas about space and time belongs to the first sort, while the
claim of a purely mathematical development is of the second kind.

<div class="p"><!----></div>
In order to demonstrate the difference between the old view of space and
time and the new one, Minkowski distinguished two transformation groups
with respect to which the laws of classical mechanics were covariant.<a href="#tthFtNtABJ" name="tthFrefABJ">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>19</mn></mrow>
</msup>
</mrow></math></a>
Considering first the same zero point in time and space for two systems in
uniform translatory motion, he noted that the spatial axes 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>y</mi></mrow></math>, 

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>z</mi></mrow></math> could undergo an arbitrary rotation about the origin. This
corresponded to the invariance in classical mechanics of the sum of
squares 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow><mi>x</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>+</mo>
<msup><mrow><mi>y</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>+</mo>
<msup><mrow><mi>z</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></math>, and was a fundamental characteristic of
physical space, as Minkowski reminded his audience, that did not concern 
motion. Next, the second group was identified with the transformations: 
<br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow><mi>x</mi><mo>'</mo><mo>=</mo><mi>x</mi><mo>+</mo><mi>&alpha;</mi><mi>t</mi><mo>,</mo><mi>&#x2002;</mi><mi>y</mi><mo>'</mo><mo>=</mo><mi>y</mi><mo>+</mo><mi>&beta;</mi><mi>t</mi><mo>,</mo><mi>&#x2002;</mi><mi>z</mi><mo>'</mo><mo>=</mo><mi>z</mi><mo>+</mo><mi>&gamma;</mi><mi>t</mi><mo>,</mo><mi>&#x2002;</mi><mi>t</mi><mo>'</mo><mo>=</mo><mi>t</mi><mo>.</mo></mrow>
    </mstyle></math>
</td></tr></table>
<br />

Thus physical space, Minkowski pointed out, which one supposed to be at
rest, could in fact be in uniform translatory motion; from physical
phenomena no decision could be made concerning the state of rest (1909:
77).

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

<center><img src="born1920diagram.jpg" alt="born1920diagram.jpg" />

<div class="p"><!----></div>
<b>Figure 1.</b>
Classical displacement diagram.
</center>

<div class="p"><!----></div>
<br />After noting verbally the distinction between these two groups, Minkowski
turned to the blackboard for a graphical demonstration. He drew a diagram
to demonstrate that the above transformations allowed one to draw the
time axis in any direction in the half-space 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>&gt;</mo><mn>0</mn></mrow></math>. While no trace has
been found of Minkowski's drawing, it may have resembled the one 
published later by Max Born and other expositors of the theory of
relativity (see Figure&#x00A0;1).<a href="#tthFtNtACA" name="tthFrefACA">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>20</mn></mrow>
</msup>
</mrow></math></a>
This was the occasion for Minkowski to introduce a spate of neologisms 
(Minkowski 1909: 76-77): <i>Weltpunkt, Weltlinie</i> and <i>Weltachse</i>,
as well as new definitions of the terms <i>Substanz</i> [`something
perceptible'], and <i>Welt</i> [the manifold of all conceivable points 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>,

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>y</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>z</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi></mrow></math>].

<div class="p"><!----></div>
At this point, Minkowski raised the question of the relation between
these two groups, drawing special attention to the characteristics of
spatial orthogonality and an arbitrarily-directed temporal axis. In
response, he introduced the hyperbolic equation:
<br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow>
<msup><mrow><mi>c</mi></mrow><mrow><mn>2</mn></mrow>
</msup>

<msup><mrow><mi>t</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>-</mo>
<msup><mrow><mi>x</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>-</mo>
<msup><mrow><mi>y</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>-</mo>
<msup><mrow><mi>z</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>=</mo><mn>1</mn><mo>,</mo></mrow>
    </mstyle></math>
</td></tr></table>
<br />

where 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>c</mi></mrow></math> was an unspecified, positive-valued parameter (Minkowski
1909: 77). Suppressing two dimensions in 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>y</mi></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>z</mi></mrow></math>, he then showed how this
unit hypersurface might be used to construct a group of transformations

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
</mrow></math>, once the arbitrary displacements of the zero point were associated
with rotations about the origin. The figure obtained was introduced on a
transparent slide, showing two pairs of symmetric axes.<a href="#tthFtNtACB" name="tthFrefACB">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>21</mn></mrow>
</msup>
</mrow></math></a>

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

<center><img src="mmmfig2.jpg" alt="mmmfig2.jpg" />

<div class="p"><!----></div>
<b>Figure 2.</b>
Minkowski's space-time and length-contraction diagrams.
</center>

<div class="p"><!----></div>
<br />Minkowski constructed the figure using the upper branch of the
two-branched unit hyperbola 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow><mi>c</mi></mrow><mrow><mn>2</mn></mrow>
</msup>

<msup><mrow><mi>t</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>-</mo>
<msup><mrow><mi>x</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>=</mo><mn>1</mn></mrow></math> to determine the
parallelogram 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>OA</mi><mo>'</mo><mi>B</mi><mo>'</mo><mi>C</mi><mo>'</mo></mrow></math>, from which the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>'</mo></mrow></math> axes were
established (see Figure&#x00A0;2, left, and the Appendix). The relation between
this diagram and the one corresponding to classical mechanics he pointed
out directly: as the parameter 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>c</mi></mrow></math> approached infinity,

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

<blockquote> this special transformation becomes one in which the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>'</mo></mrow></math> axis can
have an arbitrary upward direction, and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo></mrow></math> approaches ever closer to

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>.<a href="#tthFtNtACC" name="tthFrefACC">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>22</mn></mrow>
</msup>
</mrow></math></a>
(Minkowski 1909: 78)
</blockquote>

<div class="p"><!----></div>
 In this way, the new space-time diagram collapsed into the old
one, in a lovely graphic recovery of classical kinematics.<a href="#tthFtNtACD" name="tthFrefACD">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>23</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
The limit-relation between the group 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
</mrow></math> and the group corresponding to
classical mechanics 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mo stretchy="false">(</mo>
<msub><mrow><mi>G</mi></mrow><mrow><mi>&infin;</mi></mrow>
</msub>
<mo stretchy="false">)</mo></mrow></math> called forth a comment on the history of
the principle of relativity. Minkowski observed that in light of this
limit-relation, and

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

<blockquote> since 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
</mrow></math> is mathematically more intelligible than 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>&infin;</mi></mrow>
</msub>
</mrow></math>,
a mathematician would well have been able, in free imagination, to arrive
at the idea that in the end, natural phenomena actually possess an
invariance not with respect to the group 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>&infin;</mi></mrow>
</msub>
</mrow></math>, but rather to a
group 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
</mrow></math>, with a certain finite, but in ordinary units of measurement
<i>extremely large</i> [value of] 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>c</mi></mrow></math>. Such a premonition would have
been an extraordinary triumph for pure mathematics.<a href="#tthFtNtACE" name="tthFrefACE">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>24</mn></mrow>
</msup>
</mrow></math></a>
(Minkowski 1909: 78)
</blockquote>

<div class="p"><!----></div>
 To paraphrase, it was no more than a fluke of history that a
nineteenth-century mathematician did not discover the role played by the
group 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
</mrow></math> in physics, given its greater mathematical intelligibility in
comparison to the group 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>&infin;</mi></mrow>
</msub>
</mrow></math>. In other words, the theory of
relativity was not a product of pure mathematics, although it could have
been. Minkowski openly recognized the role-albeit a heuristic one-of
experimental physics in the discovery of the principle of relativity. All
hope was not lost for pure mathematics, however, as Minkowski continued:

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

<blockquote>While mathematics displays only more staircase-wit here, it still
has the satisfaction of realizing straight away, thanks to fortunate
antecedents and the exercised acuity of its senses, the fundamental
consequences of such a reformulation of our conception of nature.<a href="#tthFtNtACF" name="tthFrefACF">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>25</mn></mrow>
</msup>
</mrow></math></a>
(Minkowski 1909: 78)
</blockquote>

<div class="p"><!----></div>
 Minkowski conceded that, in this instance, mathematics could
only display wisdom after the fact, instead of a creative power of
discovery. Again he stressed the mathematician's distinct advantage over
members of other scientific disciplines in seizing the deep consequences
of the new theoretical view.

<div class="p"><!----></div>
     <h3><a name="tth_sEc2.1">
2.1</a>&#x00A0;&#x00A0;Minkowski the mathematician</h3>

<div class="p"><!----></div>
 Minkowski's repetitive references to mathematicians and pure
mathematics demand an explanation. Minkowski was a mathematician by
training and profession. This fact is hardly obscure, but Minkowski's
reasons for stressing his point may not be immediately obvious. Two
suggestions may be made here.

<div class="p"><!----></div>
In the first place, we believe that Minkowski and his contemporaries saw
his work on relativity as an expansion of the disciplinary frontier of
mathematics. Furthermore, this expansion was naturally regarded by some
German physicists as imperialist, occurring at the expense of the 
nascent, growing sub-discipline of theoretical physics.<a href="#tthFtNtACG" name="tthFrefACG">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>26</mn></mrow>
</msup>
</mrow></math></a>
A desire to extend mathematical dominion over the newly-discovered region
of relativistic physics would explain why Minkowski chose neither to
describe his work as theoretical physics, nor to present himself as a
theoretical (or mathematical) physicist.

<div class="p"><!----></div>
Secondly, in relation to this, we want to suggest that Minkowski was
aware of the confusion that his ideas were likely to engender in the
minds of certain members of his audience. In effect, Minkowski's response
to this expected confusion was to reassure his audience, by constantly
reaffirming what they already knew to be true: he, Minkowski, was a 
mathematician.<a href="#tthFtNtACH" name="tthFrefACH">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>27</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
Minkowski's wide reputation and unquestioned authority in pure mathematics
created a tension, which is manifest throughout his writings on
relativity. As long as Minkowski signed his work as a mathematician, any
theory he produced lacked the "authenticity" of a theory advanced by a
theoretical physicist. No "guarantee" of physical relevance was attached
to his work-on the contrary. With very few exceptions (the article on
capillarity, for example), nothing Minkowski had published was relevant to
physics.

<div class="p"><!----></div>
Acutely aware of the cross-disciplinary tension created by his excursion 
into theoretical physics, Minkowski made two moves toward its
alleviation. The first of these was to assert, at the outset of the
lecture, that the basis of his theory was in experimental physics. The 
second was to display the physico-theoretical pedigree of the principle of
relativity, aspects of which had been developed by the paragon of
theoretical physicists, H.&#x00A0;A.&#x00A0;Lorentz, and by the lesser-known patent
clerk and newly-named lecturer in theoretical physics in Bern, Albert 
Einstein.

<div class="p"><!----></div>
Up to this point in his lecture, Minkowski had presented a new, real
geometric interpretation of a certain transformation in 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>y</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>z</mi></mrow></math> and

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi></mrow></math>, which formed a group denoted by 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
</mrow></math>. This group entertained a
limit relation with the group under which the laws of classical mechanics
were covariant. From this point on, until the end of the first section of
his lecture, Minkowski presented what he, and soon a great number of
scientists, considered to be <i>his</i> theory.<a href="#tthFtNtACI" name="tthFrefACI">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>28</mn></mrow>
</msup>
</mrow></math></a>
What was this new theory? Once a system of reference 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>y</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>z</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi></mrow></math>
was determined from observation, in which natural phenomena agreed with
definite laws, the system of reference could be changed arbitrarily
without altering the form of these laws, provided that the transformation
to the new system conformed to the group 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
</mrow></math>. As Minkowski put it:

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

<blockquote>The existence of the invariance of the laws of nature for the
group 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
</mrow></math> would now be understood as follows: from the entirety of
natural phenomena we can derive, through successively enhanced
approximations, an ever more precise frame of reference 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>y</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>z</mi></mrow></math> and

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi></mrow></math>, space and time, by means of which these phenomena can then be
represented according to definite laws. This frame of reference, however, 
is by no means uniquely determined by the phenomena. <i>We can still
arbitrarily change the frame of reference according to the
transformations of the group termed 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi fontstyle="normal">G</mi></mrow><mrow><mi fontstyle="normal">c</mi></mrow>
</msub>
</mrow></math> without changing the
expression of the laws of nature</i>.<a href="#tthFtNtACJ" name="tthFrefACJ">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>29</mn></mrow>
</msup>
</mrow></math></a>
(Minkowski 1909: 78-79)
</blockquote>

<div class="p"><!----></div>
 For anyone who might have objected that others had already
pointed this out, Minkowski offered an interpretation of his theory on
the space-time diagram.<a href="#tthFtNtADA" name="tthFrefADA">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>30</mn></mrow>
</msup>
</mrow></math></a>

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

<blockquote>We can, for example, also designate time [as] 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>'</mo></mrow></math>, according to
the figure described. However, in connection with this, space must then
necessarily be defined by the manifold of three parameters 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>y</mi></mrow></math>,

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>z</mi></mrow></math>, on which physical laws would now be expressed by means of 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>y</mi></mrow></math>,

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>z</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>'</mo></mrow></math> in exactly the same way as with 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>y</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>z</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi></mrow></math>. Then from
here on, we would no longer have <i>space</i> in the world, but endlessly
many spaces; analogously, endlessly many planes exist in
three-dimensional space. Three-dimensional geometry becomes a chapter of
four-dimensional physics. You realize why I said at the outset: space and
time are to sink into the shadows; only a world in and of itself endures.<a href="#tthFtNtADB" name="tthFrefADB">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>31</mn></mrow>
</msup>
</mrow></math></a>
(Minkowski 1909: 79)
</blockquote>

<div class="p"><!----></div>
 The emphasis on space was no accident, as Minkowski presented
the notion of "endlessly many spaces" as his personal contribution, in
analogy to Einstein's concept of relative time. The grandiose
announcement of the end of space and time served as a frame for the
enunciation of Minkowski's principle of relativity.<a href="#tthFtNtADC" name="tthFrefADC">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>32</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
Rhetorical gestures such as this directed attention to Minkowski's theory;
its acceptance by the scientific community, however, may be seen to
depend largely upon the presence of two elements: empirical adequacy,
claimed by Minkowski at the opening of the lecture, and the perception of
an advantage over existing theories. Minkowski went on to address in turn
the work of two of his predecessors, Lorentz and Einstein. Before
discussing Minkowski's expos&#233; of their work, however, we want to consider
briefly the work of a third precursor, whose name was not mentioned at
all in this lecture: Henri Poincar&#233;.

<div class="p"><!----></div>
     <h3><a name="tth_sEc2.2">
2.2</a>&#x00A0;&#x00A0;Why did Minkowski not mention Poincar&#233;?</h3>

<div class="p"><!----></div>
 Widely acknowledged at the turn of the century as the world's
foremost mathematician, Henri Poincar&#233; developed Lorentz's theory of
electrons to a state formally equivalent to the theory published at the
same time by Einstein.<a href="#tthFtNtADD" name="tthFrefADD">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>33</mn></mrow>
</msup>
</mrow></math></a>
Poincar&#233; and Einstein both recognized that the Lorentz transformations (so
named by Poincar&#233;) form a group; Poincar&#233; alone exploited this knowledge
in the search for invariants.<a href="#tthFtNtADE" name="tthFrefADE">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>34</mn></mrow>
</msup>
</mrow></math></a>
Among Poincar&#233;'s insights relating to his introduction of a fourth
imaginary coordinate in 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><msqrt><mrow><mo>-</mo><mn>1</mn></mrow></msqrt></mrow></math> (where 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>c</mi><mo>=</mo><mn>1</mn></mrow></math>), was the recognition of
a Lorentz transformation as a rotation about the origin in
four-dimensional space, and the invariance of the sum of squares in this 
space, which he described as a measure of distance (1906: 542). This
analysis then formed the basis of his evaluation of the possibility of a
Lorentz-covariant theory of gravitation.

<div class="p"><!----></div>
It is unlikely that the omission of Poincar&#233;'s name was a simple
oversight on Minkowski's part. The printed version of Minkowski's
lecture, the corrected proofs of which were mailed only days before a
fatal attack of appendicitis, was the result of careful attention in
the months following the Cologne meeting.<a href="#tthFtNtADF" name="tthFrefADF">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>35</mn></mrow>
</msup>
</mrow></math></a>
This suggests that both the structure of the paper and the decision to
include (or exclude) certain references were the result of deliberate 
choices on the part of the author.

<div class="p"><!----></div>
A great admirer of Poincar&#233;'s science, Minkowski was familiar with his
long paper on the dynamics of the electron, having previously cited it in
the <i>Grundgleichungen</i>, in the appendix on gravitation. In an
earlier, then-unpublished lecture to the G&#246;ttingen Mathematical Society
on the principle of relativity, delivered on 5 November 1907, Minkowski
went so far as to portray Poincar&#233; as one of the four principal authors of
the principle of relativity:

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

<blockquote>Concerning the credit to be accorded to individual authors,
stemming from the foundations of Lorentz's ideas, Einstein
developed the principle of relativity more distinctly [and] at the same
time applied it with particular success to the treatment of special
problems in the optics of moving media, [and] ultimately [was] also the
first to draw conclusions concerning the variability of mechanical mass in 
thermodynamic processes. A short while later, and no doubt independently
of Einstein, Poincar&#233; extended [the principle of relativity] in a more
mathematical study to Lorentz electrons and their status in gravitation.
Finally, Planck sought the basis of a dynamics grounded on the principle
of relativity.<a href="#tthFtNtADG" name="tthFrefADG">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>36</mn></mrow>
</msup>
</mrow></math></a>
(Minkowski 1907b: 16-17)
</blockquote>

<div class="p"><!----></div>
 Following their appearance in this short history of the
principle of relativity, the theoretical physicists Lorentz, Einstein and
Max Planck all made it into Minkowski's Cologne lecture, but the
more mathematical Poincar&#233; was left out.

<div class="p"><!----></div>
At least one theoretical physicist felt Minkowski's exclusion of Poincar&#233;
in "Raum und Zeit" was unfair: Arnold Sommerfeld. In the notes he
added to a 1913 reprint of this lecture, Sommerfeld attempted to right
the wrong by making it clear that a Lorentz-covariant law of gravitation
and the idea of a four-vector had both been proposed earlier by Poincar&#233;.

<div class="p"><!----></div>
Among the mathematicians following the developments of electron theory,
many considered Poincar&#233; as the founder of the new mechanics. For
instance, the editor of <i>Acta Mathematica</i>, Gustav Mittag-Leffler,
wrote to Poincar&#233; on 7 July  1909 of Stockholm mathematician Ivar
Fredholm's suggestion that Minkowski had given Poincar&#233;'s ideas a
different expression:

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

<blockquote>You undoubtedly know the pamphlet by Minkowski, "Raum und
Zeit," published after his death, as well as the ideas of Einstein and
Lorentz on the same question. Now, M.&#x00A0;Fredholm tells me that you have
touched upon similar ideas before the others, while expressing yourself
in a less philosophical, more mathematical manner.<a href="#tthFtNtADH" name="tthFrefADH">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>37</mn></mrow>
</msup>
</mrow></math></a>
(Mittag-Leffler 1909)
</blockquote>

<div class="p"><!----></div>
 It is unknown if Poincar&#233; ever received this letter. Like
Sommerfeld, Mittag-Leffler and Fredholm reacted to the omission of Poincar&#233;'s
name from Minkowski's lecture.

<div class="p"><!----></div>
The absence of Poincar&#233; from Minkowski's speech was remarked by leading
scientists, but what did Poincar&#233; think of this omission? His first
response, in any case, was silence. In the lecture Poincar&#233; delivered in
G&#246;ttingen on the new mechanics in April 1909, he did not see fit to
mention the names of Minkowski and Einstein (Poincar&#233; 1910a). Yet where
his own engagement with the principle of relativity was concerned,
Poincar&#233; became more expansive. In Berlin the following year, for
example, Poincar&#233; dramatically announced that already back in 1874 (or
1875), while a student at the &#201;cole polytechnique, he and a
friend had experimentally confirmed the principle of relativity for
optical phenomena (Poincar&#233; 1910b: 104).<a href="#tthFtNtADI" name="tthFrefADI">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>38</mn></mrow>
</msup>
</mrow></math></a>
Less than five years after its discovery, the theory of relativity's
prehistory was being revealed by Poincar&#233; in a way that underlined its
empirical foundations-in contradistinction to the Minkowskian version.
If Poincar&#233; expressed little enthusiasm for the new mechanics unleashed by
the principle of relativity, and had doubts concerning its experimental
underpinnings, he never disowned the principle.<a href="#tthFtNtADJ" name="tthFrefADJ">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>39</mn></mrow>
</msup>
</mrow></math></a>
In the spring of 1912, Poincar&#233; came to acknowledge the wide acceptance of
a formulation of physical laws in four-dimensional (Minkowski) space-time,
at the expense of the Lorentz-Poincar&#233; electron theory. His own
preference remained with the latter alternative, which did not require an
alteration of the concept of space (Poincar&#233; 1912: 170).

<div class="p"><!----></div>
In the absence of any clear indication why Minkowski left Poincar&#233; out of
his lecture, a speculation or two on his motivation may be entertained.
If Minkowski had chosen to include some mention of Poincar&#233;'s work, his
own contribution may have appeared derivative. Also, Poincar&#233;'s
modification of Lorentz's theory of electrons constituted yet another
example of the cooperative role played by the mathematician in the
elaboration of physical theory.<a href="#tthFtNtAEA" name="tthFrefAEA">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>40</mn></mrow>
</msup>
</mrow></math></a>
Poincar&#233;'s "more mathematical" study of Lorentz's electron theory
demonstrated the mathematician's dependence upon the insights of the
theoretical physicist, and as such, it did little to establish the
independence of the physical and mathematical paths to the Lorentz group.
The metatheoretical goal of establishing the essentially mathematical
nature of the principle of relativity was no doubt more easily attained by
neglecting Poincar&#233;'s elaboration of this principle.

<div class="p"><!----></div>
     <h3><a name="tth_sEc2.3">
2.3</a>&#x00A0;&#x00A0;Lorentz and Einstein</h3>

<div class="p"><!----></div>
 Turning first to the work of Lorentz, Minkowski made another
significant suppression. In the <i>Grundgleichungen</i>, Minkowski had
adopted Poincar&#233;'s suggestion to give Lorentz's name to a group of
transformations with respect to which Maxwell's equations were covariant
(p.&#x00A0;473), but in the Cologne lecture, this convention was dropped. Not
once did Minkowski mention the "Lorentz" transformations, he referred
instead to transformations of the group designated 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
</mrow></math>. The reason for
this suppression is unknown, but very probably is linked to Minkowski's
discovery of a precursor to Lorentz in the employment of the
transformations. In 1887, the G&#246;ttingen professor of mathematical
physics, Woldemar Voigt, published his proof that a certain transformation
in 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>y</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>z</mi></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi></mrow></math> (which was formally equivalent to the one used by
Lorentz) did not alter the fundamental differential equation for a light
wave propagating in the free ether with velocity 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>c</mi></mrow></math> (Voigt 1887). For
Minkowski, this was an essential application of the law's covariance with
respect to the group 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
</mrow></math>. Lorentz's insight he considered to be of a
more general nature: Lorentz would have attributed this covariance to all
of optics (Minkowski 1909; 80). By placing Voigt's transformations at the
origins of the principle of  relativity, Minkowski not only undercut
Poincar&#233;'s attribution to Lorentz, he also emulated Hertz's epigram
(Maxwell's theory is Maxwell's system of equations), whose underlying logic
could only reinforce his own metatheoretical claims. In addition, he showed
courtesy toward his colleague Voigt, who was not displeased by the gesture.<a href="#tthFtNtAEB" name="tthFrefAEB">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>41</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
Having dealt in this way with the origins of the group 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
</mrow></math>, Minkowski
went on to consider another Lorentzian insight: the contraction
hypothesis. Using the space-time diagram, Minkowski showed how to
interpret the hypothesis of longitudinal contraction of electrons in 
uniform translation (Figure&#x00A0;2, right). Reducing Lorentz's electron to one
spatial dimension, Minkowski showed two bars of unequal width,
corresponding to two electrons: one at rest with respect to an unprimed
system and one moving with relative velocity 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>v</mi></mrow></math>, but at rest with 
respect to the primed system. When the moving electron was viewed from the
unprimed system, it would appear shorter than an electron at rest in the
same system, by a factor 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><msqrt><mrow><mn>1</mn><mo>-</mo>
<msup><mrow><mi>v</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo stretchy="false">/</mo>
<msup><mrow><mi>c</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></msqrt></mrow></math>. Underlining the "fantastic"
nature of the contraction hypothesis, obtained "purely as a gift from
above," Minkowski asserted the complete equivalence between Lorentz's
hypothesis and his new conception of space and time, while strongly
suggesting that, by the latter, the former became "much more
intelligible." In sum, Minkowski held that his theory offered a better
understanding of the contraction hypothesis than did Lorentz's theory of
electrons (1909: 80).<a href="#tthFtNtAEC" name="tthFrefAEC">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>42</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
In his discussion of Lorentz's electron theory, Minkowski was led to bring
up the notion of local time, which was the occasion for him to mention
Einstein. To Einstein was due the credit

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

<blockquote> of first clearly recognizing that the time of one electron is just
as good as that of the other, that is to say, that 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>'</mo></mrow></math> are to be
treated identically.<a href="#tthFtNtAED" name="tthFrefAED">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>43</mn></mrow>
</msup>
</mrow></math></a>
(Minkowski 1909: 81)
</blockquote>

<div class="p"><!----></div>
 This interpretation of Einstein's notion of time with respect to
an electron was not one advanced by Einstein himself. We will return to
it shortly; for now we observe only that Minkowski seemed to lend some
importance to Einstein's contribution, because he went on to refer to him
as having deposed the concept of time as one proceeding unequivocally
from phenomena.<a href="#tthFtNtAEE" name="tthFrefAEE">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>44</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
     <h3><a name="tth_sEc2.4">
2.4</a>&#x00A0;&#x00A0;Minkowski's distortion of Einstein's kinematics</h3>

<div class="p"><!----></div>
 At this point in his lecture, after having briefly reviewed the
work of his forerunners, Minkowski was in a position to say just where
they went wrong. Underlining the difference between his view and that of
the theoretical physicists Lorentz and Einstein, Minkowski offered the
following observation:

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

<blockquote>Neither Einstein nor Lorentz rattled the concept of space,
perhaps because in the above-mentioned special transformation, where the
plane of 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo><mi>t</mi><mo>'</mo></mrow></math> coincides with the plane of 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>xt</mi></mrow></math>, an interpretation is
[made] possible by saying that the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>-axis of space maintains its
position.<a href="#tthFtNtAEF" name="tthFrefAEF">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>45</mn></mrow>
</msup>
</mrow></math></a>
(Minkowski 1909: 81-82)
</blockquote>

<div class="p"><!----></div>
 This was the only overt justification offered by Minkowski in
support of his claim to have surpassed the theories of Lorentz and
Einstein. His rather tentative terminology [<i>eine Deutung m&#246;glich
ist </i>] signaled uncertainty and perhaps discomfort in imputing such an
interpretation to this pair. Also, given the novelty of Minkowski's
geometric presentation of classical and relativistic kinematics, his
audience may not have seen just what difference Minkowski was pointing
to. Minkowski did not elaborate; but for those who doubted that a 
priority claim was in fact being made, he added immediately:

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

<blockquote>Proceeding beyond the concept of space in a corresponding way is
likely to be appraised as only another audacity of mathematical culture.
Even so, following this additional step, indispensable to the correct
understanding of the group 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
</mrow></math>, the term <i>relativity postulate</i>
for the requirement of invariance under the group 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
</mrow></math> seems very feeble
to me.<a href="#tthFtNtAEG" name="tthFrefAEG">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>46</mn></mrow>
</msup>
</mrow></math></a>
(Minkowski 1909: 82)
</blockquote>

<div class="p"><!----></div>
 Where Einstein had deposed the concept of time (and time alone,
by implication), Minkowski claimed in a like manner to have overthrown
the concept of space, as Galison has justly noted (1979: 113).
Furthermore, Minkowski went so far as to suggest that his "additional
step" was essential to a "correct understanding" of what he had presented
as the core of relativity: the group 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
</mrow></math>. He further implied that the
theoretical physicists Lorentz and Einstein, lacking a "mathematical
culture," were one step short of the correct interpretation of the
principle of relativity.

<div class="p"><!----></div>
Having disposed in this way of his precursors, Minkowski was authorized to invent a name for 
his contribution, which he called the postulate of the absolute world, or
world-postulate for short (1909: 82). It was on this note that Minkowski
closed his essay, trotting out the shadow metaphor one more time:

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

<blockquote>The validity without exception of the world postulate is, so I
would like to believe, the true core of an electromagnetic world picture;
met by Lorentz, further revealed by Einstein, [it is] brought fully to
light at last.<a href="#tthFtNtAEH" name="tthFrefAEH">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>47</mn></mrow>
</msup>
</mrow></math></a>
(Minkowski 1909: 88)
</blockquote>

<div class="p"><!----></div>
 According to Minkowski, Einstein clarified the physical
significance of Lorentz's theory, but did not grasp the true meaning and
full implication of the principle of relativity. Minkowski marked his
fidelity to the G&#246;ttingen electron-theoretical program, which was 
coextensive with the electromagnetic world picture. When Paul Ehrenfest
asked Minkowski for a copy of the paper going by the title "On
Einstein-Electrons," Minkowski replied that when used in reference to the
<i>Grundgleichungen</i>, this title was "somewhat freely chosen."
However, when applied to the planned sequels to the latter paper, he
explained, this name would be "more correct."<a href="#tthFtNtAEI" name="tthFrefAEI">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>48</mn></mrow>
</msup>
</mrow></math></a>
Ehrenfest's nickname for the <i>Grundgleichungen</i> no doubt reminded
Minkowski of a latent tendency among theoretical physicists to view his
theory as a prolongation of Einstein's work, and may have motivated him
to provide justification of his claim to have proceeded beyond the work of
Lorentz and Einstein.

<div class="p"><!----></div>
Did Minkowski offer a convincing argument for the superiority of his
theory? The argument itself requires some clarification. According to
Peter Galison's reconstruction (1979: 113), Minkowski "conjectures
[that a] relativistically correct solution can be obtained" in one 
(spatial) dimension by rotating the temporal axis through a certain angle,
leaving the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo></mrow></math>-axis superimposed on the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>-axis. Yet Minkowski did
<i>not</i> suggest that this operation was either correct or incorrect.
Rather, he claimed it was possible to interpret a previously-mentioned
transformation in a way which was at odds with his own geometric
interpretation. Proposed by Minkowski as Lorentz's and Einstein's view of
space and time, such a reading was at the same time possible, and
incompatible with Einstein's presentations of the principle of relativity.

<div class="p"><!----></div>
The claim referred back to Minkowski's expos&#233; of both classical and
relativistic kinematics by means of space-time diagrams. As mentioned
above, he had emphasized the fact that in classical mechanics the time
axis may be assigned any direction with respect to the fixed spatial axes

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>y</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>z</mi></mrow></math>, in the region 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>&gt;</mo><mn>0</mn></mrow></math>. Minkowski's specification of the
"special transformation" referred in all likelihood to the special
Lorentz transformations, in which case Minkowski's further requirement of
coincidence of the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>xt</mi></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo><mi>t</mi><mo>'</mo></mrow></math> planes was (trivially) satisfied; the
term is encountered nowhere else in the text. By singling out the
physicists' reliance on the special Lorentz transformation, Minkowski
underlined his introduction of the inhomogeneous transformations, which
accord no privilege to any single axis or origin.<a href="#tthFtNtAEJ" name="tthFrefAEJ">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>49</mn></mrow>
</msup>
</mrow></math></a>
He then proposed that Lorentz and Einstein <i>might</i> have interpreted
the special Lorentz transformation as a rotation of the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>'</mo></mrow></math>-axis alone,
the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo></mrow></math>-axis remaining fixed to the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>-axis. Since Minkowski presented
two geometric models of kinematics in his lecture, we will refer to them
in evaluating his view of Lorentz's and Einstein's kinematics.

<div class="p"><!----></div>
The first interpretation, and the most plausible one in the circumstances,
refers to the representation of Galilean kinematics (see Figure&#x00A0;1). On a
rectangular coordinate system in 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi></mrow></math>, a 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>'</mo></mrow></math>-axis is drawn at an
angle to the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi></mrow></math>-axis, and the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo></mrow></math>-axis lies on the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>-axis as required
by Minkowski. Lorentz's electron theory held that in inertial systems the 
laws of physics were covariant with respect to a Galilean transformation, 

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo><mo>=</mo><mi>x</mi><mo>-</mo><mi>vt</mi></mrow></math>.<a href="#tthFtNtAFA" name="tthFrefAFA">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>50</mn></mrow>
</msup>
</mrow></math></a>
In the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo><mi>t</mi><mo>'</mo></mrow></math>-system, the coordinates are oblique, and the relationship
between 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>'</mo></mrow></math> is fixed by Lorentz's requirement of absolute
simultaneity: 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>'</mo><mo>=</mo><mi>t</mi></mrow></math>. Where Poincar&#233; and Einstein wrote the Lorentz
transformation in one step, Lorentz used two, so that a Galilean
transformation was combined with a second transformation containing the
formula for local time.<a href="#tthFtNtAFB" name="tthFrefAFB">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>51</mn></mrow>
</msup>
</mrow></math></a>
The second transformation did not lend itself to graphical representation,
and had no physical meaning for Lorentz, who understood the transformed 
values as auxiliary quantities. The first stage of the two-dimensional
Lorentz transformation was identical to that of classical mechanics, and
may be represented in the same way, by rotating the time axis while
leaving the position of the space axis unchanged. When realized on a
Galilean space-time diagram, and in the context of Lorentz's electron
theory, Minkowski's description of the special Lorentz transformations
seems quite natural. On the other hand, as a description of Einstein's
kinematics it seems odd, because Einstein explicitly abandoned the use of
the Galilean transformations in favor of the Lorentz transformations.<a href="#tthFtNtAFC" name="tthFrefAFC">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>52</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
Lorentz's theory of electrons provided for a constant propagation velocity
of light <i>in vacuo</i>, when the velocity was measured in an inertial
frame. However, this propagation velocity was not considered to be a
universal invariant (as was maintained in the theories of both Einstein
and Minkowski). In Lorentz's theory of electrons, retention of classical 
kinematics (with the adjoining notion of absolute simultaneity) meant that
the velocity of light in a uniformly translating frame of reference would
in general depend on the frame's velocity with respect to the ether.
Measurements of light velocity performed by observers in these frames,
however, would always reveal the same value, due to compensating dilatory
effects of motion on the tools of measurement (Lorentz 1916: 224-225).

<div class="p"><!----></div>
The latter distinction enters into the second way by which Minkowski
might have measured Einstein's kinematics. Referring now to a Minkowski
diagram, two inertial systems 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>S</mi></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>S</mi><mo>'</mo></mrow></math> may be represented, as in the
left side of Figure&#x00A0;2. In system 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>S</mi></mrow></math>, points in time and space are
represented on general Cartesian axes, on which the units are chosen in
such a way that the velocity of light <i>in vacuo</i> is equal to 1.<a href="#tthFtNtAFD" name="tthFrefAFD">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>53</mn></mrow>
</msup>
</mrow></math></a>
For an observer at rest in 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>S</mi></mrow></math>, the system 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>S</mi><mo>'</mo></mrow></math> appears to be in uniform
motion in a direction parallel to the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>-axis with a sub-light velocity

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>v</mi></mrow></math>, and the temporal axis 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>ct</mi><mo>'</mo></mrow></math> for the system 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>S</mi><mo>'</mo></mrow></math> is drawn at an angle
to the axis 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>ct</mi></mrow></math>. Einstein postulated that the velocity of light <i>in
vacuo</i> was a universal constant, and asserted that units of length and
time could be defined in the same way for all inertial systems (this
definition will be discussed later, with respect to the concept of
simultaneity). He showed that from the light postulate and a constraint on
linearity, in accordance with his measurement conventions, it followed
that light propagated with the same velocity in both systems. From the
corresponding transformation equations, Einstein deduced the following
equations for the surface of a light wave emitted from the origin of the
space and time coordinates considered in the systems 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>S</mi></mrow></math> (with coordinates

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>,</mo><mi>y</mi><mo>,</mo><mi>z</mi><mo>,</mo><mi>t</mi></mrow></math>) and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>S</mi><mo>'</mo></mrow></math> (coordinates designated 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>&xi;</mi><mo>,</mo><mi>&eta;</mi><mo>,</mo><mi>&zeta;</mi><mo>,</mo><mi>&tau;</mi></mrow></math>):
<br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow>
<msup><mrow><mi>x</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>+</mo>
<msup><mrow><mi>y</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>+</mo>
<msup><mrow><mi>z</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>=</mo>
<msup><mrow><mi>c</mi></mrow><mrow><mn>2</mn></mrow>
</msup>

<msup><mrow><mi>t</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>,</mo><mi>&#x2003;&#x2003;&#x2003;&#x2003;&#x2003;&#x2003;</mi>
<msup><mrow><mi>&xi;</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>+</mo>
<msup><mrow><mi>&eta;</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>+</mo>
<msup><mrow><mi>&zeta;</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>=</mo>
<msup><mrow><mi>c</mi></mrow><mrow><mn>2</mn></mrow>
</msup>

<msup><mrow><mi>&tau;</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>.</mo></mrow>
    </mstyle></math>
</td></tr></table>
<br />

Einstein initially presented this equivalence as proof that his two
postulates were compatible; later he recognized that the Lorentz
transformations followed from this equivalence and a requirement of symmetry
(Einstein 1905: 901; 1907: 419). At the same time, he made no further
comment on the geometric significance of this invariance and maintained at
least a semantic distinction between kinematics and geometry.<a href="#tthFtNtAFE" name="tthFrefAFE">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>54</mn></mrow>
</msup>
</mrow></math></a>
Minkowski chose to fold one into the other, regarding 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow><mi>c</mi></mrow><mrow><mn>2</mn></mrow>
</msup>

<msup><mrow><mi>t</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>-</mo>
<msup><mrow><mi>x</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>-</mo>
<msup><mrow><mi>y</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>-</mo>
<msup><mrow><mi>z</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></math> as a <i>geometric</i> invariant. Since 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>y</mi></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>z</mi></mrow></math> do not change
in the case considered here, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow><mi>c</mi></mrow><mrow><mn>2</mn></mrow>
</msup>

<msup><mrow><mi>t</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>-</mo>
<msup><mrow><mi>x</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></math> is an invariant quantity when
measured in an inertial system. Minkowski's space-time diagram is a model
of the geometry based on this metric.

<div class="p"><!----></div>
Following Minkowski's interpretation of Einstein's kinematics, the

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo></mrow></math>-axis (that which records the spatial distribution of events
corresponding to 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>ct</mi><mo>'</mo><mo>=</mo><mn>0</mn></mrow></math>) coincides with the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>-axis. Recalling that the
units of length and time for inertial systems were defined by Einstein in
such a way that the quantity 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow><mi>c</mi></mrow><mrow><mn>2</mn></mrow>
</msup>

<msup><mrow><mi>t</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>-</mo>
<msup><mrow><mi>x</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></math> was invariant for any two points,
the position of the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo></mrow></math>-axis with respect to the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>-axis depended only upon
the relative velocity of 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>S</mi><mo>'</mo></mrow></math>, manifest in the tilt angle of the

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>ct</mi><mo>'</mo></mrow></math>-axis with respect to the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>ct</mi></mrow></math>-axis (and vice-versa). Consequently,
the requirement that the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo></mrow></math>-axis coincide with the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>-axis could not be
met here, either, at least not without: (1) sacrificing one of Einstein's
postulates, (2) abandoning Einstein's definition of time (and
simultaneity), or (3) arbitrarily introducing an additional 
transformation in order to recover the special Lorentz transformation
through composition. 

<div class="p"><!----></div>
Neither one of the first two options would have been considered natural
or plausible to one familiar with Einstein's publications. As for the
last option, since none of the properties of the Lorentz transformations
are reflected geometrically, the operation is far from
interpretative-it is pointless. It is also improbable that Minkowski
would have attributed, even implicitly, the use of his space-time diagram
to Lorentz or Einstein. For all these reasons, this reconstruction is far
less plausible than the one considered previously.

<div class="p"><!----></div>
If either of these two reconstructions reflects accurately what Minkowski
had in mind, the upshot is an assertion that Lorentz and Einstein
subscribed to a definition of space and time at variance with the one
proposed by Einstein in 1905. Ascribing the first (Galilean) 
interpretation to Lorentz was unlikely to raise any eyebrows. The second
interpretation is inconsistent with Einstein's presentation of
relativistic kinematics. Furthermore, Minkowski imputed <i>one</i>
interpretation [<i>eine Deutung </i>] to both Lorentz <i>and</i> Einstein.<a href="#tthFtNtAFF" name="tthFrefAFF">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>55</mn></mrow>
</msup>
</mrow></math></a>
Attentive to the distinction between Lorentz's theory of electrons and 
Einstein's theory of relativity, both Philipp Frank and Guido Castelnuovo
rectified what they perceived to be Minkowski's error, as we will see
later in detail for Castelnuovo.<a href="#tthFtNtAFG" name="tthFrefAFG">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>56</mn></mrow>
</msup>
</mrow></math></a>
On the other hand, Vito Volterra (1912: 23) and Lothar Heffter (1912: 4)
adopted Minkowski's view of Einstein's kinematics, so it appears that no
consensus was established on the cogency of Minkowski's argument in the
pre-war period.

<div class="p"><!----></div>
The confrontation of Einstein's articles of 1905 and 1907, both cited by
Minkowski, with the interpretation charged to Einstein (and Lorentz) by
Minkowski, offers matter for reflection. Indeed, the justification
offered by Minkowski for his claim would seem to support the view, held
by more than one historian, that Minkowski, to put it bluntly, did not
understand Einstein's theory of relativity.<a href="#tthFtNtAFH" name="tthFrefAFH">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>57</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
     <h3><a name="tth_sEc2.5">
2.5</a>&#x00A0;&#x00A0;Did Minkowski understand Einstein's concepts of
relative time and simultaneity?</h3>

<div class="p"><!----></div>
 A detailed comparison of the theories of Einstein and Minkowski
is called for, in order to evaluate Minkowski's understanding of
Einsteinian relativity; here we review only the way in which Einstein's
concepts of time and simultaneity were employed by both men up to 1908.
These concepts are chosen for their bearing upon Minkowski's unique
graphic representation of Lorentz's and Einstein's kinematics.

<div class="p"><!----></div>
The relativity of simultaneity and clock synchronization via optical
signals had been discussed by Poincar&#233; as early as 1898, and several
times thereafter (Poincar&#233; 1898, 1904: 311). As mentioned above,
Lorentz's theory of electrons did not admit the relativity of
simultaneity; Lorentz himself used this concept to distinguish his theory
from that of Einstein (Lorentz 1910: 1236).

<div class="p"><!----></div>
Along with the postulation of the invariance of the velocity of light
propagation in empty space and of the principle of relativity of the laws
of physics for inertial frames of reference, Einstein's 1905 <i>
Annalen</i> article began with a <i>definition</i> of simultaneity
(1905: 891-893). He outlined a method for clock synchronization involving
a pair of observers at rest, located at different points in space, denoted

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>A</mi></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>B</mi></mrow></math>, each with identical clocks. Noting that the time of an event
at 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>A</mi></mrow></math> may not be compared with the time of an event at 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>B</mi></mrow></math> without some
conventional definition of "time," Einstein proposed that time be defined
in such a way that the delay for light traveling from 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>A</mi></mrow></math> to 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>B</mi></mrow></math> has the
same duration as when light travels from 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>B</mi></mrow></math> to 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>A</mi></mrow></math>.

<div class="p"><!----></div>
Einstein supposed that a light signal was emitted from 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>A</mi></mrow></math> at time 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>t</mi></mrow><mrow><mi>A</mi></mrow>
</msub>
</mrow></math>, 
reflected at point 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>B</mi></mrow></math> at time 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>t</mi></mrow><mrow><mi>B</mi></mrow>
</msub>
</mrow></math>, and observed at point 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>A</mi></mrow></math> at time

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>t</mi></mrow><mrow><mi>A</mi></mrow>
</msub>
<mo>'</mo></mrow></math>. The clocks at 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>A</mi></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>B</mi></mrow></math> were then synchronous, again by
definition, if 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>t</mi></mrow><mrow><mi>B</mi></mrow>
</msub>
<mo>-</mo>
<msub><mrow><mi>t</mi></mrow><mrow><mi>A</mi></mrow>
</msub>
<mo>=</mo>
<msub><mrow><mi>t</mi></mrow><mrow><mi>A</mi></mrow>
</msub>
<mo>'</mo><mo>-</mo>
<msub><mrow><mi>t</mi></mrow><mrow><mi>B</mi></mrow>
</msub>
</mrow></math>. After defining time and
clock synchronicity, Einstein went on to postulate that the propagation
velocity of light in empty space is a universal constant (1905: 894),
such that
<br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow>
<mfrac><mrow><mn>2</mn><mi>&#x2002;</mi>
<mover><mrow><mi>AB</mi></mrow>
<mo stretchy="true">&OverBar;</mo></mover>
</mrow>
<mrow>
<msub><mrow><mi>t</mi></mrow><mrow><mi>A</mi></mrow>
</msub>
<mo>'</mo><mo>-</mo>
<msub><mrow><mi>t</mi></mrow><mrow><mi>A</mi></mrow>
</msub>
</mrow>
</mfrac>
<mo>=</mo><mi>c</mi><mo>.</mo></mrow>
    </mstyle></math>
</td></tr></table>
<br />

Essentially the same presentation of time and simultaneity was given by
Einstein in his 1908 review paper, except in this instance he chose to
refer to one-way light propagation (1907: 416).

<div class="p"><!----></div>
In summary, by the time of the Cologne lecture, Einstein had defined
clock synchronicity using both round-trip and one-way light travel
between points in an inertial frame. Furthermore, we know for certain that
Minkowski was familiar with both of Einstein's papers. The formal
equivalence of Einstein's theory with that of Minkowski is not an issue,
since Minkowski adopted unequivocally the validity of the Lorentz 
transformations, and stated just as clearly that the constant appearing
therein was the velocity of propagation of light in empty space. The
issue is Minkowski's own knowledge of this equivalence, in other words,
his recognition of either an intellectual debt to Einstein, or of the 
fact that he independently developed a partially or fully equivalent
theory of relativity. In what follows, we examine some old and new
evidence concerning Minkowski's grasp of Einstein's time concept.

<div class="p"><!----></div>
Insofar as meaning may be discerned from use, Minkowski's use of the
concepts of time and of simultaneity was equivalent to that of Einstein.
In the Cologne lecture, for example, Minkowski demonstrated the
relativity of simultaneity, employing for this purpose his space-time
diagram (1909: 83). A more detailed expos&#233; of the concept-without the
space-time diagram-had appeared in the <i>Grundgleichungen</i>. In the
earlier paper, Minkowski examined the conditions under which the notion
of simultaneity was well defined for a single frame of reference. His
reasoning naturally supposed that the one-way light delay between two
distinct points 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>A</mi></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>B</mi></mrow></math> was equal to the ordinary distance 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>AB</mi></mrow></math>
divided by the velocity of light, exactly as Einstein had supposed. To
conclude his discussion of the concept of time in the <i>
Grundgleichungen</i>, Minkowski remarked by way of acknowledgment that 
Einstein had addressed the need to bring the nature of the Lorentz
transformations physically closer (1908a: 487).

<div class="p"><!----></div>
Notwithstanding Minkowski's demonstrated mastery of Einstein's concepts of
time and of simultaneity, his understanding of Einstein's idea of time
has been questioned. In particular, a phrase cited above from the Cologne
lecture has attracted criticism, and is purported to be emblematic of
Minkowski's unsure grasp of the difference between Lorentz's theory and 
Einstein's (Miller 1981: 241). In explaining how Einstein's notion of
time was different from the "local time" employed by Lorentz in his
theory of electrons, Minkowski recognized the progress made by his former
student, for whom "the time of one electron is just as good as that of
the other." In his 1905 relativity paper, Einstein referred, not to the
time of one electron, but to the time associated with the origin of a
system of coordinates in uniform translation, instantaneously at rest
with respect to the velocity of an electron moving in an electromagnetic
field (1905: 917-918). Provided that such systems could be
determined for different electrons, the time coordinates established in
these systems would be related in Einstein's theory by a Lorentz
transformation. In this sense, Minkowski's electronic interpretation of
time was compatible with Einstein's application of his theory to electron 
dynamics.

<div class="p"><!----></div>
Minkowski's interpretation of Einstein's time also reflects the conceptual
change wrought in physics by his own notion of proper time (<i>
Eigenzeit </i>). Near the end of 1907, Minkowski became aware of the need
to introduce a coordinate-independent time parameter to his theory.<a href="#tthFtNtAFI" name="tthFrefAFI">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>58</mn></mrow>
</msup>
</mrow></math></a>
This recognition led him (in the appendix to the <i>Grundgleichungen </i>)
to introduce proper time, which he presented as a generalization of
Lorentz's local time (1908a: 515). From a formal perspective, proper
time was closely related to Einstein's formula for time dilation.<a href="#tthFtNtAFJ" name="tthFrefAFJ">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>59</mn></mrow>
</msup>
</mrow></math></a>
Minkowski may have simply conflated proper time with time dilation, since
the "time of one electron" that Minkowski found in Einstein's theory
naturally referred in his view to the <i>time parameter along the
world-line of an electron</i>, otherwise known as proper time. The
introduction of proper time enabled Minkowski to develop the space-time 
formalism for Lorentz-covariant mechanics, which formed the basis for
subsequent research in this area. In this way, proper time became firmly
embedded in the Minkowskian view of world-lines in space-time, which
Einstein also came to adopt several years later.<a href="#tthFtNtAGA" name="tthFrefAGA">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>60</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
While the electronic interpretation of time has a clear relation to both
Einstein's writings and Minkowski's proper time, the phrase "the time of
one electron is just as good as that of the other" appears to belong to
Lorentz. One of the drafts of the Cologne lecture features a discussion
of the physical meaning of Lorentz's local time, which was not retained in
the final version. Minkowski referred to a conversation with Lorentz
during the mathematicians' congress in Rome, in early April 1908:

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

<blockquote>For the uniformly moving electron, Lorentz had called the
combination 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>'</mo><mo>=</mo><mo stretchy="false">(</mo><mo>-</mo><mi>qx</mi><mo>+</mo><mi>t</mi><mo stretchy="false">)</mo><mo stretchy="false">/</mo><msqrt><mrow><mn>1</mn><mo>-</mo>
<msup><mrow><mi>q</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></msqrt></mrow></math> the local time of the
electron, and used this concept to understand the contraction hypothesis.
Lorentz himself told me conversationally in Rome that it was to Einstein's
credit to have recognized that <em>the time of one electron is just as
good as that of the other</em>, i.e., that 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>'</mo></mrow></math> are equivalent.
[Italics added]<a href="#tthFtNtAGB" name="tthFrefAGB">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>61</mn></mrow>
</msup>
</mrow></math></a>
</blockquote>

<div class="p"><!----></div>
 According to Minkowski's account, Lorentz employed the phrase
in question to characterize Einstein's new concept of time. In fact, what
Lorentz had called local time was not the above expression, but 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>'</mo><mo>=</mo><mi>t</mi><mo stretchy="false">/</mo><mi>&beta;</mi><mo>-</mo><mi>&beta;</mi><mi>vx</mi><mo stretchy="false">/</mo>
<msup><mrow><mi>c</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></math>. When combined with a Galilean transformation, the
latter expression is equivalent to the one Minkowski called Lorentz's local
time. Minkowski must have recognized his mistake, because in the final,
printed version of "<em>Raum und Zeit</em>" he rewrote his definition of local
time and suppressed the attribution of the italicized phrase to Lorentz.

<div class="p"><!----></div>
Based on the similarity of the treatment of simultaneity in the <i>
Grundgleichungen </i> with that of Einstein's writings, Minkowski's
acknowledgment of Einstein's contribution in this area, his extension via
proper time of Einstein's relative time to the parameterization of 
world-lines, and the change he made to the definition of local time given
in an earlier draft of the Cologne lecture, it appears that Minkowski
understood Einstein's concepts of time and simultaneity. This means, of
course, that Minkowski's graphic representation of Einstein's kinematics
was uncharitable at best. Minkowski may have perceived the success of his own
formulation of relativity to depend in some way upon a demonstration that his
theory was not just an elaboration of Einstein's work. Likewise, some
expedient was required in order for  Minkowski to achieve the metatheoretical
goal of demonstrating the superiority of pure mathematics over the intuitive
methods of physicists; he found one in a space-time diagram.

<div class="p"><!----></div>
 <h2><a name="tth_sEc3">
3</a>&#x00A0;&#x00A0;Responses to the Cologne lecture</h2>

<div class="p"><!----></div>
 The diffusion of Minkowski's lecture was exceptional. A few
months after the Cologne meeting, it appeared in three different
periodicals, and as a booklet. By the end of 1909, translations had
appeared in Italian and French, the latter with the help of Max Born 
(Minkowski 1909: 517, n.&#x00A0;1). The response to these publications was
phenomenal, and has yet to be adequately measured. In this direction, we
first present some bibliometric data on research in non-gravitational
relativity theory, then discuss a few individual responses to Minkowski's
work.

<div class="p"><!----></div>
In order to situate Minkowski's work in the publication history of the
theory of relativity, we refer to our bibliometric analysis (Walter
1996). The temporal evolution in the number of articles published on
non-gravitational relativity theory is shown in Figure&#x00A0;3, for West 
European-language journals worldwide from 1905 to 1915, along with the
relative contribution of mathematicians, theoretical physicists, and
non-theoretical physicists. These three groups accounted for nine out of
ten papers published in this time period.

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

<center><img src="mmmfig3.jpg" alt="mmmfig3.jpg" />

<div class="p"><!----></div>
<b>Figure 3.</b>
Papers on the non-gravitational theory of relativity.
</center>

<div class="p"><!----></div>
The plot is based on 610 articles out of a total of 674 for all
professions in the period from 1905 to 1915, inclusive. For details on
sources and selection criteria, see chapter&#x00A0;four of the author's
Ph.D.&#x00A0;dissertation (Walter 1996).


<div class="p"><!----></div>
<br /><br /> Starting in 1909, publication numbers increased rapidly until 1912,
when the attention of theoretical physicists shifted to quantum theory and
theories of gravitation. The annual publication total also declined then
for non-theoretical physicists, but remained stable for mathematicians
until the outbreak of war in 1914.

<div class="p"><!----></div>
A comparison of the relative strength of disciplinary involvement with
the theory of relativity can be made for a large group of contributors,
if we categorize individuals according to the discipline they professed
in the university. Factoring in the size of the teaching staff in German 
universities in 1911, and taking into consideration only research
published by certified teaching personnel (more than half of all authors
in 1911 Germany), we find the greatest penetration of relativity theory
among theoretical physicists, with one out of four contributing at least
one paper on this subject (Table 1, col.&#x00A0;5). Professors of mathematics and
of non-theoretical physics largely outnumbered professors of theoretical
physics in German universities, and consequently, the penetration of
relativity theory in the former fields was significantly lower than the
ratio for theoretical physics. The number of contributors for each of the
three groups was roughly equivalent, yet theoretical physicists wrote
three papers for every one published by their counterparts in mathematics
or non-theoretical physics (Table 1, col.&#x00A0;4).

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

<center>
<table border="1">
<tr><td align="left">Discipline </td><td align="center">Instructors </td><td align="center">Relativists </td><td align="center">Pubs. </td><td align="center">Rel./Instr.</td></tr>
<tr><td align="left">Theoretical Physics </td><td align="center">23 </td><td align="center">6 </td><td align="center">21 </td><td align="center">26% </td></tr>
<tr><td align="left">Non-Theoretical Physics </td><td align="center">100 </td><td align="center">6 </td><td align="center">8 </td><td align="center">6% </td></tr>
<tr><td align="left">Mathematics </td><td align="center">86 </td><td align="center">5 </td><td align="center">7 </td><td align="center">6% </td></tr></table>


<div class="p"><!----></div>
<b>Table 1.</b>
Disciplinary penetration of relativity <br />for university
instructors in 1911 Germany.
</center>

<div class="p"><!----></div>
The <i>relativist</i> category is
taken here to include critics of the special theory of relativity; <em>
physics</em> is taken to include applied physics. The number of teaching
positions is compiled from Auerbach &amp; Rothe 1911.


<div class="p"><!----></div>
     <h3><a name="tth_sEc3.1">
3.1</a>&#x00A0;&#x00A0;The physical reception of Minkowski's theory</h3>

<div class="p"><!----></div>
 The initial response by Einstein and Laub to the <i>
Grundgleichungen</i>, we mentioned earlier, dismissed the four-dimensional
approach, and criticized Minkowski's formula for ponderomotive force
density. Others were more appreciative of Minkowski's formalism,
including the co-editors of the <i>Annalen der Physik</i>, Max Planck and
Willy Wien. According to Planck and Wien, Minkowski had put Einstein's
theory in a very elegant mathematical form (Wien 1909a: 37; Planck
1910a: 110). In private, however, both men acknowledged a significant
physical content to Minkowski's work; in a letter to Hilbert, Wien 
expressed hope that these ideas would be "thoroughly worked out" (Wien
1909b; Planck 1909). While Wien and Planck applauded Minkowski's
mathematical reformulation of the theory of relativity, they clearly
rejected his metatheoretical views, and since their public evaluation came
to dominate physical opinion of Minkowski's theory, Minkowski's effort in
the Cologne lecture to disengage his work from that of Einstein must be
viewed as a failure, at least as far as most physicists were concerned.

<div class="p"><!----></div>
Not all physicists agreed with Planck and Wien, however. The respected
theorist Arnold Sommerfeld was the key exception to the rule of
recognizing only Minkowski's formal accomplishment. A former student of
Hurwitz and Hilbert, and an ex-prot&#233;g&#233; of Felix Klein, Sommerfeld taught
mathematics in G&#246;ttingen before being called to the Aachen chair in 
mechanics. In 1906, on the basis of his publications on diffraction and on
electron theory, and upon Lorentz's recommendation, he received a call to
the chair in theoretical physics in Munich, where he was also to head a
new institute.<a href="#tthFtNtAGC" name="tthFrefAGC">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>62</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
Sommerfeld was among the first to champion Minkowskian relativity for
both its physical and mathematical insights. The enthusiasm he showed
for Minkowski's theory contrasts with the skepticism with which he
initially viewed Einstein's theory. The latter held little appeal for
Sommerfeld, who preferred the G&#246;ttingen lecturer Max Abraham's
rigid-sphere electron theory for its promise of a purely
electromagnetic explanation of physical phenomena.<a href="#tthFtNtAGD" name="tthFrefAGD">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>63</mn></mrow>
</msup>
</mrow></math></a>
In Munich Sommerfeld's views began to change. The mathematical rigor
of his papers on the rigid electron was subjected to harsh criticism
by his former thesis advisor, now colleague, the professor of
mathematics Ferdinand Lindemann. Vexed by these attacks, Sommerfeld
finally suggested to Lindemann that the problems connected with time
in electron theory were due not to its mathematical elaboration, but
to its physical foundations (Sommerfeld 1907a: 281). Sommerfeld wrote
a paper defending Einstein's theory against an objection raised by
Wien (Sommerfeld 1907b), and in the summer of 1908, he exchanged
correspondence with Minkowski concerning Einstein's formula for
ponderomotive force, and Minkowski's description of the motion of a
uniformly-accelerating electron (Minkowski 1908b).<a href="#tthFtNtAGE" name="tthFrefAGE">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>64</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
The nature of Sommerfeld's immediate reaction to Minkowski's lecture is
unknown, although he was one of three members of the audience to respond
during the discussion period, and the only physicist.<a href="#tthFtNtAGF" name="tthFrefAGF">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>65</mn></mrow>
</msup>
</mrow></math></a>
After the meeting, he wrote to Lorentz to congratulate him on the 
success of his theory, for Alfred H. Bucherer had presented results of
Becquerel-ray deflection experiments that favored the "Lorentz-Einstein"
deformable-electron theory over the rigid-electron theory (Sommerfeld
1908). In another letter to Lorentz, a little over a year later,
Sommerfeld announced, "Now I, too, have adapted to the relative theory;
in particular, Minkowski's systematic form and view facilitated my
comprehension" (Sommerfeld 1910c).<a href="#tthFtNtAGG" name="tthFrefAGG">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>66</mn></mrow>
</msup>
</mrow></math></a>
Both Bucherer's experimental results and the Minkowskian theoretical view
contributed to Sommerfeld's adjustment to the theory of relativity, but
the latter was what he found most convincing.

<div class="p"><!----></div>
In Sommerfeld's first publications on Minkowski's theory, he
emphasized the geometric interpretation of the Lorentz transformations
as a rotation in space-time; this was an aspect that also featured in
lectures given in Munich during winter semester
1909/10.<a href="#tthFtNtAGH" name="tthFrefAGH">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>67</mn></mrow>
</msup>
</mrow></math></a>  He
further enhanced the geometric view of relativity by deriving the
velocity addition formula from spherical trigonometry with imaginary
sides-a method that pointed the way to a reformulation of the theory
of relativity in terms of hyperbolic trigonometry. Remarking that
Einstein's formula "loses all strangeness" in the Minkowskian
interpretation, Sommerfeld maintained that his only goal in presenting
this derivation was to show that the space-time view was a "useful
guide" in special questions, in addition to facilitating development
of the "relative theory" (Sommerfeld 1909a: 827, 829; Walter 1999).

<div class="p"><!----></div>
Sommerfeld naturally considered Minkowski's view to be more geometric
than Einstein's theory; he found also that Einstein and Minkowski
differed on what appeared to be substantial questions of physics. 
The prime example of this difference concerned the correct expression
for ponderomotive force density. The covariant expression employed by
Minkowski was presented by Sommerfeld as "closer to the principle of
relativity" than Einstein and Laub's formula (Sommerfeld 1909b: 815). Indeed,
the latter formula was not Lorentz-covariant, but it had been proposed solely
for a system at rest.<a href="#tthFtNtAGI" name="tthFrefAGI">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>68</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
Einstein appeared as a precursor to Minkowski in Sommerfeld's widely read
publication on the theory of relativity in the <i>Annalen der
Physik</i>. Offered in tribute to Minkowski, this work criticized "older
theories" that employed the concept of absolute space, in what appears to
be a response to Minkowski's self-presentation as genitor of a new notion
of space. In Sommerfeld's view, Einstein's theory represented an
intermediate step between Lorentz and Minkowski, who had rendered the
work of both Lorentz and Einstein "irrelevant":

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

<blockquote>The troublesome calculations through which Lorentz (1895 and 1904)
and Einstein (1905) prove their validity independent of the coordinate
system, and [for which they] had to establish the meaning of the
transformed field vectors, become irrelevant in the system of the
Minkowski "world."<a href="#tthFtNtAGJ" name="tthFrefAGJ">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>69</mn></mrow>
</msup>
</mrow></math></a>
(Sommerfeld 1910a: 224)
</blockquote>

<div class="p"><!----></div>
 Sommerfeld depicted the technical difficulty inherent to
Lorentz's and Einstein's theories as a thing of the past. Inasmuch as
Minkowski appealed to mathematicians to study the theory of relativity in
virtue of its essential mathematical nature, Sommerfeld encouraged 
physicists to take up Minkowski's theory in virtue of its new-found
technical simplicity. The pair of <i>Annalen</i> publications delivered
Minkowskian relativity in a form more palatable to physicists, by
replacing the unfamiliar matrix calculus with a four-dimensional vector 
notation. Similar vectorial reformulations of Minkowski's work were
published the same year by Max Abraham (1910) and Gilbert Newton Lewis
(1910a, 1910b).

<div class="p"><!----></div>
Apart from the change in notation, Sommerfeld's presentation was wholly
consonant with Minkowski's reinterpretation of electron-theoretical
results. He paraphrased, for example, Minkowski's remark to the effect
that, far from being rendered obsolete by his theory, the results for
retarded potentials from (pre-Einsteinian) electron-theoretical papers by
Li&#233;nard, Wiechert and Schwarzschild "first reveal their inner nature in
four dimensions, in full simplicity" (Sommerfeld 1909b: 813).<a href="#tthFtNtAHA" name="tthFrefAHA">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>70</mn></mrow>
</msup>
</mrow></math></a>
As mentioned above, Sommerfeld's reputation in theoretical physics had 
been established on the basis of his publications on the rigid-electron
theory, which for years had formed the basis of the electromagnetic world
picture. The rigid electron had now been repudiated empirically by
Bucherer's results, but Minkowski felt it was still possible to pursue 
the electromagnetic world picture with `Einstein-electrons,' as we saw
above.<a href="#tthFtNtAHB" name="tthFrefAHB">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>71</mn></mrow>
</msup>
</mrow></math></a>
Furthermore, this suggests that in supporting-unconditionally-Minkowski's
view of relativity, Sommerfeld did not "burn his boats," as once thought (Kuhn et al.&#x00A0;1967: 141). Instead, Sommerfeld's active promotion and extension of
Minkowski's theory is best understood as an <i>adaptation</i> of the framework
of the electromagnetic world picture to the principle of relativity.<a href="#tthFtNtAHC" name="tthFrefAHC">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>72</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
An example of this adaptation may be seen in Sommerfeld's redescription of
a primary feature of the electromagnetic world picture: the ether. For
those scientists still attached to the concept of ether (or absolute
space, in Sommerfeld's terminology), Sommerfeld proposed that they
substitute Minkowski's notion of the absolute world, in which the
"absolute substrate" of electrodynamics was now to be found (1910: 189).
In this way, Minkowski and Sommerfeld filled the conceptual void created
by Einstein's brusque elimination of the ether.

<div class="p"><!----></div>
Sommerfeld's mathematical background and close contacts with the
G&#246;ttingen faculty distinguished him from other theoretical physicists,
and enabled him to pass through the walls separating the mathematical and
physical communities. In the direction of mathematics, Sommerfeld was a
privileged interlocutor for G&#246;ttingen mathematicians. He shared their 
appreciation of the Lorentz transformation as a four-dimensional rotation;
his derivation of the velocity addition theorem via spherical
trigonometry stimulated dozens of publications by mathematicians in what
became a mathematical sub-specialty: the non-Euclidean interpretation of
relativity theory (Walter 1999). When David Hilbert needed an
assistant in physics, he trusted Sommerfeld to find someone with the
proper training.<a href="#tthFtNtAHD" name="tthFrefAHD">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>73</mn></mrow>
</msup>
</mrow></math></a>
Hilbert felt that Sommerfeld's view of theoretical physics could benefit
research in G&#246;ttingen (including his own), and after Poincar&#233; (1909),
Lorentz (1910), and Michelson (1911), Sommerfeld received an invitation
from the Wolfskehl Commission to give lectures on "recent questions in 
mathematical physics," in the summer of 1912.<a href="#tthFtNtAHE" name="tthFrefAHE">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>74</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
In the direction of physics, as we have mentioned, Sommerfeld rendered
Minkowskian relativity comprehensible to physicists by introducing it in
vector form. When chosen by the German Physical Society to deliver a
report on the theory of relativity for the Karlsruhe meeting of the
German Association in 1911, Sommerfeld announced that in the six years
since Einstein's publication, the theory had become the "secure property
of physics" (Sommerfeld 1911: 1057). His avowed enthusiasm for the theory,
made manifest in publications, lectures and personal contacts, was
essential in making this statement ring true.

<div class="p"><!----></div>
     <h3><a name="tth_sEc3.2">
3.2</a>&#x00A0;&#x00A0;Mathematicians and Minkowskian relativity</h3>

<div class="p"><!----></div>
 At the same time, there were many relativists who were
convinced that the theory of relativity belonged to mathematics.
Physicists typically rejected the Minkowskian view of the mathematical
essence of the principle of relativity, but the message was heard in
departments of mathematics around the world. Mathematicians were already
familiar with the concepts and techniques from matrix calculus,
hyperbolic geometry and group theory employed in Minkowski's theory, and
were usually able to grasp its unified structure with ease. As Hermann
Weyl recalled in retrospect, relativity theory seemed revolutionary to
physicists, but it had a pattern of ideas which made a perfect fit with
those already a part of mathematics (Weyl 1949: 541). Harry Bateman saw the
the principle of relativity as unifying disparate branches of mathematics
such as geometry, partial differential equations, generalized vector 
analysis, continuous groups of transformations, and differential and
integral invariants (Bateman et al. 1911: 500). Mathematicians, from
graduate students to full professors, some of whom had never made the
least foray into physics, answered the call to study and develop the
theory. According to our study (1996: chap.&#x00A0;4), between 1909 and 1915,
sixty-five mathematicians wrote 151 articles on non-gravitational relativity
theory, or one out of every four articles published in this domain. In 1913,
mathematicians publishing articles worldwide on the theory of relativity (22
individuals) outnumbered their counterparts in both theoretical (16) and
non-theoretical (15) physics.<a href="#tthFtNtAHF" name="tthFrefAHF">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>75</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
In addition to writing articles, some of these mathematicians introduced
the theory of relativity to their research seminars, and taught its
formal basis to an expanding student population eager to learn the
"radical" theory of space-time. In Germany, according to the listings in
the <i>Physikalische Zeitschrift</i>, out of thirty-nine regular course
offerings on the theory of relativity up to 1915, eight were taught by
mathematicians. This broad engagement with the theory of relativity
ensured the institutional integration and intellectual propagation
necessary to the survival of any research program.

<div class="p"><!----></div>
While the impetus for mathematical engagement with the theory of
relativity had several sources, the practical advantages offered by the
Minkowskian space-time formalism were probably decisive for many
`relativist' mathematicians, who almost invariably employed this 
formalism in their work. Minkowskian mathematicians made significant
contributions in relativistic kinematics and mechanics, although their
results were infrequently assimilated by physicists. A striking example
of this failure to communicate was pointed out by Stachel (1995: 278),
with respect to &#201;mile Borel's 1913 discovery of Thomas precession.

<div class="p"><!----></div>
Perhaps more significant to the history of relativity than any isolated
mathematical discovery was the introduction of a set of techniques and
ideas to the practice of relativity by Minkowskian mathematicians. In
favor of this standpoint we recall Stachel's view (1989: 55) of the
role of the rigidly-rotating disk problem in the history of general
relativity, and Pais's conjecture (1982: 216) that Born's definition of the
motion of a 'rigid' body pointed the way to Einstein's adoption (in 1912) of
a Riemannian metric in the <i>Entwurf</i> theory of gravitation and general
relativity. These are particular cases of a larger phenomenon; non-Euclidean
and nonstatic geometries were infused into the theory of relativity from late
1909 to early 1913, as a by-product of studies of accelerated motion in
space-time by the Minkowskians Max Born, Gustav Herglotz, Theodor Kaluza, 
&#201;mile Borel and others (Walter 1996: chap.&#x00A0;2).

<div class="p"><!----></div>
The clarion call to mathematicians did not come from Minkowski alone.
Felix Klein quickly recognized the great potential of Minkowski's
approach, integrating Minkowski's application of matrix calculus to the
equations of electrodynamics into his lectures on elementary mathematics
(1908: 165). The executive committee of the German Society of 
Mathematicians, of which Klein was a member, chose geometric kinematics as
one of the themes of the society's next annual meeting in Salzburg, but
Klein did not wait until the fall to give his own view of this subject.<a href="#tthFtNtAHG" name="tthFrefAHG">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>76</mn></mrow>
</msup>
</mrow></math></a>
Developing his ideas before G&#246;ttingen mathematicians in April 1909, Klein
pointed out that the new theory based on the Lorentz group (which he
preferred to call "<i>Invariantentheorie</i>") could have come from pure 
mathematics (1910: 19). He felt that the new theory was anticipated by
the ideas on geometry and groups that he had introduced in 1872,
otherwise known as the Erlangen program (see Gray 1989: 229). The
latter connection was not one made by Minkowski, yet it tended to anchor
the theory of relativity ever more solidly in the history of late
nineteenth century mathematics (for Klein's version see 1927: 28).

<div class="p"><!----></div>
The subdued response of the physics elite towards Minkowskian relativity
constrasts with the enthusiasm displayed by G&#246;ttingen mathematicians. Of
course, Minkowski's sudden death just months after the Cologne meeting
may have influenced early evaluations of his work. David Hilbert's 
appreciation of Minkowski's lecture, for example, was published as part of
an obituary. In Hilbert's account appeared nothing but full agreement
with the views expressed by Minkowski, including the assessment of the
contributions of Lorentz and Einstein. A few years later, Hilbert
portrayed Einstein's achievement as more fundamental than that of 
Minkowski, although this characterization appeared in a letter requesting
financial support for visiting lecturers in theoretical physicists.<a href="#tthFtNtAHH" name="tthFrefAHH">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>77</mn></mrow>
</msup>
</mrow></math></a>

<div class="p"><!----></div>
The axiomatic look of the theory presented by Minkowski in the <i>
Grundgleichungen</i> was perfectly in line with Hilbert's own aspirations
for the mathematization of physics, which he had announced as number six
in his famous list of worthy problems (Hilbert 1900; Rowe 1995; Corry
1996). In Hilbert's view, Minkowski's greatest positive result was not the
discovery of the world postulate, but its application to the derivation
of the basic electrodynamic equations for matter in motion (Minkowski <i>
GS</i>: I, xxv). Hilbert did not publish on the non-gravitational theory of
relativity, but like Einstein, he borrowed Minkowski's four-dimensional
formalism for his work on the general theory of relativity in 1915 (Hilbert
1916).

<div class="p"><!----></div>
In one sense, Minkowski's theory was the fruit of Hilbert's concerted
efforts, first in bringing Minkowski to G&#246;ttingen from Zürich, then in
creating jointly-led advanced seminars to enhance his friend's
considerable knowledge and skills in geometry and mechanics, and to 
direct these toward the development of an axiomatically-based physics. The
success of Minkowski's theory was also Hilbert's success and was, as
David Rowe has remarked, a major triumph for the G&#246;ttingen mathematical
community (Rowe 1995: 24). In 1909, on the occasion of Klein's sixtieth
birthday, and in the presence of Henri Poincar&#233;, David Hilbert offered
his thoughts on the outlook for mathematics:

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

<blockquote>What a joy to be a mathematician today, when mathematics is seen
sprouting up everywhere and blossoming, when it is shown ever more to
advantage in application in the natural sciences as well as in the
philosophical direction, and stands to reconquer its former central
position.<a href="#tthFtNtAHI" name="tthFrefAHI">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>78</mn></mrow>
</msup>
</mrow></math></a>
(Hilbert 1909b)
</blockquote>

<div class="p"><!----></div>
 Minkowski's theory of relativity was no doubt a prime example
for Hilbert of the reconquest of physics by mathematicians.

<div class="p"><!----></div>
So far we have encountered the responses to Minkowski's work by his
G&#246;ttingen colleagues, who of course had a privileged acquaintance with
his approach to electrodynamics. In this respect, most mathematicians
were in a position closer to that of our third and final illustration of
mathematical responses to the Cologne lecture, from Guido Castelnuovo.
This case, however, is chosen primarily for its bearing on Minkowski's
interpretation of Einsteinian kinematics, and should not be taken as
definitive of mathematical opinion of his work outside of G&#246;ttingen.

<div class="p"><!----></div>
Castelnuovo was a leading figure in algebraic geometry, a professor of
mathematics at the University of Rome and president of the Italian
Mathematical Society. In an article published in <i>Scientia</i>, he
reviewed the notions of space and time according to Minkowski, closely 
following the thematic progression of the Cologne lecture. With an
important difference, however: when Castelnuovo came to discuss the
difference between classical and relativistic space-time, he credited the
latter to Einstein instead of Minkowski. What is more, where Minkowski
maintained that Einstein did <i>not</i> modify the classical notion of
space, Castelnuovo insisted upon the contrary:

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

<blockquote>The statement that the velocity of light is always equal to 1 for
any observer is equivalent to the statement that a change in the temporal
axis also brings a change to the spatial axes.<a href="#tthFtNtAHJ" name="tthFrefAHJ">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>79</mn></mrow>
</msup>
</mrow></math></a>
(Castelnuovo 1911: 78)
</blockquote>

<div class="p"><!----></div>
 In light of our earlier reconstruction of Minkowski's argument,
it would seem that Castelnuovo denied the possibility of the
interpretation imputed to Einstein by Minkowski, in which a rotation of
the temporal axis left the spatial axis unchanged; in Castelnuovo's view, 
Einstein's theory required that the temporal and spatial axes rotate
together. From a disciplinary standpoint, it is remarkable that
Castelnuovo claimed to be giving an authentic account of <i>Minkowski's
view</i> of Einstein's kinematics.

<div class="p"><!----></div>
Since Castelnuovo apparently contested, and effectively silenced the
reasoning given by Minkowski to differentiate his theory from that of
Einstein, he might have gone on to assert the equivalence of the two
theories. Instead, he affirmed one of Minkowski's metatheoretical claims.
Following his expos&#233; of classical and Einsteinian kinematics, Castelnuovo
reiterated that in the latter, a rotation of the temporal axis is
necessarily accompanied by a rotation of the spatial axes. He continued:

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

<blockquote>In truth, this change could be perceived solely by [an observer
moving with the speed of light]. Yet if our senses were sufficiently
acute, certain differences in the details of the presentation of
phenomena would not escape us.<a href="#tthFtNtAIA" name="tthFrefAIA">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>80</mn></mrow>
</msup>
</mrow></math></a>
(Castelnuovo 1911: 78)
</blockquote>

<div class="p"><!----></div>
 Despite his destruction of the basis to Minkowski's priority claim,
Castelnuovo acknowledged the cogency of his geometric approach, while
recognizing the change in the concept of space brought about by
Einsteinian relativity. The perception of the aforementioned rotation of
the spatial axes concomitant with a rotation of the temporal axis 
required either the adoption of Minkowski's point of view, or the results
of experimental physics. Of course, this was a paraphrase of Minkowski;
we saw earlier how he conceded that the results of experimental physics
had led to the discovery of the principle of relativity, and argued that
pure mathematics could have done as well without Michelson's experiment.
For Castelnuovo, the acceptance of Minkowski's metatheoretical view of
the mathematical essence of the principle of relativity apparently did
not conflict with a rejection of his theoretical claim on a new view of
space.

<div class="p"><!----></div>
 <h2><a name="tth_sEc4">
4</a>&#x00A0;&#x00A0;Concluding remarks</h2>

<div class="p"><!----></div>
 Minkowski's semi-popular Cologne lecture was an audacious
attempt, seconded by G&#246;ttingen mathematicians and their allies, to change
the way scientists understood the principle of relativity. Henceforth,
this principle lent itself to a geometric conception, in terms of the
intersections of world-lines in space-time. Considered as a sales pitch
to mathematicians, Minkowski's speech appears to have been very 
effective, in light of the substantial post-1909 increase in mathematical
familiarity with the theory of relativity. Minkowski's lecture was also
instrumental in attracting the attention of physicists to the principle
of relativity. The G&#246;ttingen theorists Walter Ritz, Max Born and Max
Abraham were the first to adopt Minkowski's formalism, and following
Sommerfeld's intervention, the space-time theory seduced Max von Laue and
eventually even Paul Ehrenfest, both of whom had strong ties to G&#246;ttingen.

<div class="p"><!----></div>
For a mathematician of Minkowski's stature there was little glory to be
had in dotting the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>i</mi></mrow></math>'s on the theory discovered by a mathematically
unsophisticated, unknown, unchaired youngster. In choosing to publish his
space-time theory, Minkowski put his personal reputation at stake, along
with that of his university, whose identification with the effort to
develop the electromagnetic world picture was well established. As a
professor of mathematics in G&#246;ttingen, Minkowski engaged the reputation
of German mathematics, if not that of mathematics in general. From both a
personal and a disciplinary point of view, it was essential for Minkowski
to show his work to be different from that of Lorentz and Einstein. At
the same time, the continuity of his theory with those advanced by the
theoretical physicists was required in order to overcome his lack of
authority in physics. This tension led Minkowski to assimilate Einstein's
kinematics with those of Lorentz's electron theory, contrary to his 
understanding of the difference between these two theories. Minkowski was
ultimately unable to detach his theory from that of Einstein, because
even if he convinced some mathematicians that his work stood alone, the
space-time theory came to be understood by most German physicists as a
purely formal development of Einstein's theory.

<div class="p"><!----></div>
Einstein, too, seemed to share this view. It is well known that after
unifying geometry and physics on electrodynamic foundations, Minkowski's
theory of space-time was instrumental to the geometrization of the
gravitational field. In one of Einstein's first presentations of the 
general theory of relativity, he wrote with some understatement that his
discovery had been "greatly facilitated" by the form given to the
special theory of relativity by Minkowski (Einstein 1916: 769).

<div class="p"><!----></div>
The pronounced disciplinary character of this episode in the history of
relativity is undoubtedly linked to institutional changes in physics and
mathematics in the decades preceding the discovery of the theory of
relativity. For some mathematicians, the dawn of the twentieth century
was a time of conquest, or rather reconquest, of terrain occupied by
specialists in theoretical physics in the latter part of the nineteenth
century. In time, with the growing influence of this new sub-discipline,
candidates for mathematical chairs were evaluated by theoretical
physicists, and chairs of mathematics and mathematical physics were
converted to chairs in theoretical physics. After a decade of vacancy,
Minkowski's chair in Zürich, for example, was accorded to Einstein.<a href="#tthFtNtAIB" name="tthFrefAIB">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>81</mn></mrow>
</msup>
</mrow></math></a>
It seems that a critical shift took place in this period, as a new sense
emerged for the role of mathematics in the construction of physical 
theories, which was reinforced by Einstein's discovery of the field equations
of general relativity. Mathematicians followed this movement closely, as
Tullio Levi-Civita, Hermann Weyl, &#201;lie Cartan, Jan Schouten and
L.&#x00A0;P.&#x00A0;Eisenhart, among others, revived the tradition of seeking in the
theories of physics new directions for their research.

<div class="p"><!----></div>
 <h2><a name="tth_sEc5">
5</a>&#x00A0;&#x00A0;Appendix: Minkowski's space-time diagram and the Lorentz
transformations</h2>

<div class="p"><!----></div>
 The relation between the Minkowski space-time diagram and the
special Lorentz transformations is presented in many treatises on special
relativity. One way of recovering the transformations from the diagram,
recalling a method outlined by Max Laue (1911: 47), proceeds as follows.

<div class="p"><!----></div>
A two-dimensional Minkowski space-time diagram represents general
Cartesian systems with common origins, whereby we constrain the search to
linear, homogeneous transformations. For convenience, we let 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>&ell;</mi><mo>=</mo><mi>ct</mi></mrow></math>
and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>&beta;</mi><mo>=</mo><mi>v</mi><mo stretchy="false">/</mo><mi>c</mi></mrow></math>. These conditions determine the form of the desired
transformations:
<br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow><mi>x</mi><mo>=</mo><mi>&nu;</mi><mi>&ell;</mi><mo>'</mo><mo>+</mo><mi>&rho;</mi><mi>x</mi><mo>'</mo><mi>&#x2003;&#x2003;&#x2003;&#x2003;&#x2003;&#x2003;</mi>
<mtext>and</mtext>
<mi>&#x2003;&#x2003;&#x2003;&#x2003;&#x2003;&#x2003;</mi><mi>&ell;</mi><mo>=</mo><mi>&lambda;</mi><mi>&ell;</mi><mo>'</mo><mo>+</mo><mi>&mu;</mi><mi>x</mi><mo>'</mo><mo>.</mo></mrow>
    </mstyle></math>
</td></tr></table>
<br />


<div class="p"><!----></div>
On a Minkowski diagram (where the units are selected so that 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>c</mi><mo>=</mo><mn>1</mn></mrow></math>) we
draw the invariant curves 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow><mi>&ell;</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>-</mo>
<msup><mrow><mi>x</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>=</mo><mi>&ell;</mi><mo>'</mo>
<msup><mrow></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>-</mo><mi>x</mi><mo>'</mo>
<msup><mrow></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>=</mo><mo>&PlusMinus;</mo><mn>1</mn></mrow></math> (see
Figure&#x00A0;4).

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

<center><img src="mmmfig4.jpg" alt="mmmfig4.jpg" />

<div class="p"><!----></div>
<b>Figure 4.</b>
Minkowski diagram of systems 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>S</mi></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>S</mi><mo>'</mo></mrow></math>.
</center>

<div class="p"><!----></div>
<br />Next, we mark two points in the coordinate system 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>S</mi><mo stretchy="false">(</mo><mi>x</mi><mo>,</mo><mi>&ell;</mi><mo stretchy="false">)</mo></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>P</mi><mo>=</mo><mo stretchy="false">(</mo><mn>0</mn><mo>,</mo><mn>1</mn><mo stretchy="false">)</mo></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>Q</mi><mo>=</mo><mo stretchy="false">(</mo><mn>1</mn><mo>,</mo><mn>0</mn><mo stretchy="false">)</mo></mrow></math>, located at the intersections of the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>&ell;</mi></mrow></math>-axis
and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>-axis with these hyperbolae. Another system 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>S</mi><mo>'</mo></mrow></math> translates
uniformly at velocity 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>v</mi><mo>=</mo><mi>c</mi><mi>&beta;</mi></mrow></math> with respect to 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>S</mi></mrow></math>, such that the 
origin of 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>S</mi><mo>'</mo></mrow></math> appears to move according to the expression 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>=</mo><mi>&beta;</mi><mi>&ell;</mi></mrow></math>.
This line is taken to be the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>&ell;</mi><mo>'</mo></mrow></math>-axis. From the expression for the
hyperbolae, it is evident that the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo></mrow></math>-axis and the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>&ell;</mi><mo>'</mo></mrow></math>-axis are
mutually symmetric, and form the same angle 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow><mi>tan</mi></mrow><mrow><mo>-</mo><mn>1</mn></mrow>
</msup>
<mi>&beta;</mi></mrow></math> with the 

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>-axis and the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>&ell;</mi></mrow></math>-axis, respectively. The two points in 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>S</mi></mrow></math> are
denoted here as 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>P</mi><mo>'</mo><mo>=</mo><mo stretchy="false">(</mo><mn>0</mn><mo>,</mo><mn>1</mn><mo stretchy="false">)</mo></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>Q</mi><mo>'</mo><mo>=</mo><mo stretchy="false">(</mo><mn>1</mn><mo>,</mo><mn>0</mn><mo stretchy="false">)</mo></mrow></math> and marked accordingly,
at the intersections of the hyperbolae with the respective axes. The

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>&ell;</mi><mo>'</mo></mrow></math>-axis, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>=</mo><mi>&beta;</mi><mi>&ell;</mi></mrow></math>, intersects the hyperbola 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow><mi>&ell;</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>-</mo>
<msup><mrow><mi>x</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>=</mo><mn>1</mn></mrow></math> at 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>P</mi><mo>'</mo></mrow></math>. Using this data, we solve for the coefficients 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>&nu;</mi></mrow></math> and

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>&lambda;</mi></mrow></math>:

<div class="p"><!----></div>
<br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow><mi>&nu;</mi><mo>=</mo>
<mfrac><mrow><mi>&beta;</mi></mrow>
<mrow><msqrt><mrow><mn>1</mn><mo>-</mo>
<msup><mrow><mi>&beta;</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></msqrt></mrow>
</mfrac>
<mi>&#x2003;&#x2003;&#x2003;&#x2003;&#x2003;&#x2003;</mi>
<mtext>and</mtext>
<mi>&#x2003;&#x2003;&#x2003;&#x2003;&#x2003;&#x2003;</mi><mi>&lambda;</mi><mo>=</mo>
<mfrac><mrow><mn>1</mn></mrow>
<mrow><msqrt><mrow><mn>1</mn><mo>-</mo>
<msup><mrow><mi>&beta;</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></msqrt></mrow>
</mfrac>
<mo>.</mo></mrow>
    </mstyle></math>
</td></tr></table>
<br />


<div class="p"><!----></div>
Applying the same reasoning to the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo></mrow></math>-axis 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mo stretchy="false">(</mo><mi>x</mi><mo>=</mo><mi>&ell;</mi><mi>&#x2002;</mi><mi>&beta;</mi><mo stretchy="false">)</mo></mrow></math>, we solve
for the coefficients 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>&rho;</mi></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>&mu;</mi></mrow></math>, evaluating the expressions for 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>
and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>&ell;</mi></mrow></math> at the intersection of the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo></mrow></math>-axis with the hyperbola 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow><mi>&ell;</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>-</mo>
<msup><mrow><mi>x</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>=</mo><mo>-</mo><mn>1</mn></mrow></math>, at the point labeled 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>Q</mi><mo>'</mo></mrow></math>, and we find
<br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow><mi>&rho;</mi><mo>=</mo>
<mfrac><mrow><mn>1</mn></mrow>
<mrow><msqrt><mrow><mn>1</mn><mo>-</mo>
<msup><mrow><mi>&beta;</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></msqrt></mrow>
</mfrac>
<mi>&#x2003;&#x2003;&#x2003;&#x2003;&#x2003;&#x2003;</mi>
<mtext>and</mtext>
<mi>&#x2003;&#x2003;&#x2003;&#x2003;&#x2003;&#x2003;</mi><mi>&mu;</mi><mo>=</mo>
<mfrac><mrow><mi>&beta;</mi></mrow>
<mrow><msqrt><mrow><mn>1</mn><mo>-</mo>
<msup><mrow><mi>&beta;</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></msqrt></mrow>
</mfrac>
<mo>.</mo></mrow>
    </mstyle></math>
</td></tr></table>
<br />

Substituting these coefficients into the original expressions for 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math> and

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>&ell;</mi></mrow></math>, we obtain the following transformations:
<br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow><mi>x</mi><mo>=</mo>
<mfrac><mrow><mi>x</mi><mo>'</mo><mo>+</mo><mi>&beta;</mi><mi>&ell;</mi><mo>'</mo></mrow>
<mrow><msqrt><mrow><mn>1</mn><mo>-</mo>
<msup><mrow><mi>&beta;</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></msqrt></mrow>
</mfrac>
<mi>&#x2003;&#x2003;&#x2003;&#x2003;&#x2003;&#x2003;</mi>
<mtext>and</mtext>
<mi>&#x2003;&#x2003;&#x2003;&#x2003;&#x2003;&#x2003;</mi><mi>&ell;</mi><mo>=</mo>
<mfrac><mrow><mi>&ell;</mi><mo>'</mo><mo>+</mo><mi>&beta;</mi><mi>x</mi><mo>'</mo></mrow>
<mrow><msqrt><mrow><mn>1</mn><mo>-</mo>
<msup><mrow><mi>&beta;</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></msqrt></mrow>
</mfrac>
<mo>.</mo></mrow>
    </mstyle></math>
</td></tr></table>
<br />

The old form of the special Lorentz transformations is recovered by
substituting 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>&ell;</mi><mo>=</mo><mi>ct</mi></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>&beta;</mi><mo>=</mo><mi>v</mi><mo stretchy="false">/</mo><mi>c</mi></mrow></math>,
<br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow><mi>x</mi><mo>=</mo>
<mfrac><mrow><mi>x</mi><mo>'</mo><mo>+</mo><mi>vt</mi><mo>'</mo></mrow>
<mrow><msqrt><mrow><mn>1</mn><mo>-</mo>
<msup><mrow><mi>v</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo stretchy="false">/</mo>
<msup><mrow><mi>c</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></msqrt></mrow>
</mfrac>
<mi>&#x2003;&#x2003;&#x2003;&#x2003;&#x2003;&#x2003;</mi>
<mtext>and</mtext>
<mi>&#x2003;&#x2003;&#x2003;&#x2003;&#x2003;&#x2003;</mi><mi>t</mi><mo>=</mo>
<mfrac><mrow><mi>t</mi><mo>'</mo><mo>+</mo><mi>vx</mi><mo>'</mo><mo stretchy="false">/</mo>
<msup><mrow><mi>c</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow>
<mrow><msqrt><mrow><mn>1</mn><mo>-</mo>
<msup><mrow><mi>v</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo stretchy="false">/</mo>
<msup><mrow><mi>c</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></msqrt></mrow>
</mfrac>
<mo>.</mo></mrow>
    </mstyle></math>
</td></tr></table>
<br />


<div class="p"><!----></div>
Invoking the property of symmetry, the transformations for 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>'</mo></mrow></math>
may be calculated in the same fashion as above, by starting with 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>S</mi><mo>'</mo></mrow></math>
instead of 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>S</mi></mrow></math>.

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

<h2>Acknowledgments</h2>

<div class="p"><!----></div>
For their critiques of preliminary versions of this paper, my warmest
thanks go to Olivier Darrigol, Peter Galison, Christian Houzel, Arthur
Miller, Michel Paty, Jim Ritter and John Stachel. The themes of this
paper were presented in seminars at the University of Paris 7, at
University College London, and at the 1995 HGR congress; I am grateful to 
their participants and organizers for stimulating discussions. Financial
support was provided by a fellowship from the French Ministry of Research
and Higher Education, and archival research was made possible by travel
grants from the American Institute of Physics and the University of Paris
7.

<div class="p"><!----></div>
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--- (1915). "&#220;ber das Doppler'sche Prinzips." <i>Physikalische
Zeitschrift</i> <b>16</b>: 381-386.

<div class="p"><!----></div>
  V<font size="-2">OLKMANN</font>, Paul.
(1910). <i>Erkenntnistheoretische Grundz&#252;ge der 
Naturwissenschaften und ihre Beziehungen zum Geistesleben der Gegenwart.
Wissenschaft und Hypothese</i> <b>9</b>. Leipzig &amp; Berlin: Teubner.

<div class="p"><!----></div>
  V<font size="-2">OLTERRA</font>, Vito.
(1912). <i>Lectures Delivered at the Celebration of the 20th
Anniversary of the Foundation of Clark University</i>. Worcester: Clark
University.

<div class="p"><!----></div>
  W<font size="-2">ALTER</font>, Scott.
(1996). "Hermann Minkowski et la math&#233;matisation de la th&#233;orie de
la relativit&#233; restreinte, 1905-1915." Ph.D.&#x00A0;dissertation, University of
Paris 7.

<div class="p"><!----></div>
--- (1999). "The Non-Euclidean Style of Minkowskian Relativity." In <i>
The Symbolic Universe</i>. Jeremy J.&#x00A0;Gray, ed. 91-127. Oxford: Oxford University
Press.

<div class="p"><!----></div>
  W<font size="-2">EYL</font>, Hermann.
(1949). "Relativity Theory as a Stimulus in Mathematical
Research." <i>Proceedings of the American Philosophical Society</i> <b>
93</b>: 535-541.

<div class="p"><!----></div>
  W<font size="-2">IECHERT</font>, Emil.
(1915). "Die Mechanik im Rahmen der allgemeinen Physik." In
<i>Die Kultur der Gegenwart</i>. Teil 3, Abt.&#x00A0;3, Bd.&#x00A0;1: <i>Physik</i>.
Emil Warburg, ed. 1-78. Leipzig &amp; Berlin: Teubner.

<div class="p"><!----></div>
  W<font size="-2">IEN</font>, Wilhelm.
(1906). "&#220;ber die partiellen Differentialgleichungen der Physik."
<i>Jahresbericht der deutschen Mathematiker-Vereinigung</i> <b>15</b>:
42-51.

<div class="p"><!----></div>
--- (1909a). "&#220;ber die Wandlung des Raum- und Zeitbegriffs in der 
Physik." <i>Sitzungsberichte der physikalisch-medicinischen Gesellschaft
zu W&#252;rzburg</i>: 29-39.

<div class="p"><!----></div>
--- (1909b). Wilhelm Wien to David Hilbert. 15 April 1909. Hilbert
<i>Nachla&#223;</i> 436, Nieders&#228;chsische Staats- und Universit&#228;tsbibliothek.

<div class="p"><!----></div>
<hr /><h3>Footnotes:</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>On Minkowski's role in the
  history of relativity see also Illy 1981 and Pyenson 1987. Many
  references to the primary and secondary literature on the theory of
  relativity may be found in Miller 1981 and Paty 1993. Pauli 1958
  remains an excellent guide to the primary
literature.
<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>McCormmach 1976; Jungnickel &amp; McCormmach 1986:
  II, 334-347.
<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>Minkowski published his lectures on Diophantine analysis in
Minkowski 1907a.
<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>Copies of Minkowski's manuscript notes of these lectures are in the
Niels Bohr Library, Minkowski Papers, Boxes 7, 8 and 9.
<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>On the G&#246;ttingen electron theory seminar, see Pyenson 1985: 102.
<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>Undated manuscript, Nieders&#228;chsische Staats- und 
Universit&#228;tsbibliothek, Hilbert <i>Nachla&#223;</i> 570/9; Born 1959: 682.
<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>Minkowski to Einstein, 9 October 1907 (Einstein <i>CP5</i>: doc.&#x00A0;62);
course listing in <i>Physikalische Zeitschrift</i> <b>8</b> (1907): 712.
Fragmentary notes by Hermann Mierendorff from this seminar show a
discussion of Lorentz's electrodynamics of moving media, see
Nieders&#228;chsische Staats- und Universit&#228;tsbibliothek, Hilbert <i>Nachla&#223;</i>
570/5; Pyenson 1985: 83. During the same semester, Minkowski introduced
the principle of relativity into his lectures on the theory of functions
("Funktionentheorie." Minkowski Papers: Box 9, Niels Bohr Library).
<div class="p"><!----></div>
<a name="tthFtNtAAI"></a><a href="#tthFrefAAI">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>8</mn></mrow>
</msup>
</mrow></math></a>"Neuere Ideen &#252;ber die Grundgesetze der Mechanik," held in 
G&#246;ttingen from 21 April to 2 May, see <i>L'Enseignement Math&#233;matique</i>
<b>10</b> (1908): 179.
<div class="p"><!----></div>
<a name="tthFtNtAAJ"></a><a href="#tthFrefAAJ">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>9</mn></mrow>
</msup>
</mrow></math></a>Undated manuscript, Nieders&#228;chsische Staats- und 
Universit&#228;tsbibliothek, Math.&#x00A0;Archiv 60: 4, 52. Minkowski's uncharitable
assessment of mathematics at Zurich Polytechnic belied the presence on the
faculty of his friend Adolf Hurwitz, a member of the mathematical elite,
and a lecturer of great repute. Graduates included Marcel Grossmann,
L.-Gustave du Pasquier and Minkowski's doctoral student Louis Kollros, all
of whom were called upon to teach university mathematics upon completion
of their studies. In recollections of his years as Einstein's classmate,
Kollros wrote that there was "almost too much mathematics" at Zürich
Polytechnic (Kollros 1956: 273). Minkowski's remark that Einstein's
mathematical knowledge was incomplete may have been based on the fact
that, unlike his classmates, Einstein did not elect to pursue graduate
studies in mathematics, after obtaining the diploma from Polytechnic.
<div class="p"><!----></div>
<a name="tthFtNtABA"></a><a href="#tthFrefABA">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>10</mn></mrow>
</msup>
</mrow></math></a>In a letter of 18 October 1908, Minkowski wrote to Robert Gnehm of 
his satisfaction in learning-during the Cologne meeting of scientists
and physicians-how much Einstein's work was admired by the likes of
Walther Nernst, Max Planck and H.&#x00A0;A.&#x00A0;Lorentz (Seelig 1956: 131-132).
<div class="p"><!----></div>
<a name="tthFtNtABB"></a><a href="#tthFrefABB">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>11</mn></mrow>
</msup>
</mrow></math></a>Transcript of an oral interview with Thomas S.&#x00A0;Kuhn, 18 October 1962,
Archives for History of Quantum Physics, p.&#x00A0;5.
<div class="p"><!----></div>
<a name="tthFtNtABC"></a><a href="#tthFrefABC">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>12</mn></mrow>
</msup>
</mrow></math></a>According to another version, the manuscript sent
  to Minkowski showed a new way of calculating the electromagnetic
  mass of the electron, described by Born as a combination of
  "Einstein's ideas with Minkowski's mathematical methods" (Born
  1968: 25).
<div class="p"><!----></div>
<a name="tthFtNtABD"></a><a href="#tthFrefABD">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>13</mn></mrow>
</msup>
</mrow></math></a>Minkowski's premature death
  prevented him from personally fulfilling his obligation to Born, but
  his G&#246;ttingen colleagues accorded Born the venia legendi in
  theoretical physics, on Voigt's recommendation (Born 1978: 136).
<div class="p"><!----></div>
<a name="tthFtNtABE"></a><a href="#tthFrefABE">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>14</mn></mrow>
</msup>
</mrow></math></a><i>Jahresbericht der deutschen
    Mathematiker-Vereinigung</i> <b>17</b> (1908): 61, dated 26 April
  1908.
<div class="p"><!----></div>
<a name="tthFtNtABF"></a><a href="#tthFrefABF">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>15</mn></mrow>
</msup>
</mrow></math></a>Most of the lectures in the first
  section were published in volume 18 of the <i>Jahresbericht der
    deutschen Mathematiker-Vereinigung</i>.  Shortly after the end of the
  First World War, the German Physical Society also held session at
  meetings of the German Association (see Forman 1967: 156).
<div class="p"><!----></div>
<a name="tthFtNtABG"></a><a href="#tthFrefABG">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>16</mn></mrow>
</msup>
</mrow></math></a>Nieders&#228;chsische Staats- und Universit&#228;tsbibliothek,
  Math.&#x00A0;Arch. 60: 2 and 60: 4. An early draft is dated 24 April 1908
  (60: 4, folder 1, p.&#x00A0;66.); the other drafts are undated.
<div class="p"><!----></div>
<a name="tthFtNtABH"></a><a href="#tthFrefABH">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>17</mn></mrow>
</msup>
</mrow></math></a>"M. H.! Die Anschauungen &#252;ber Raum und Zeit, die ich Ihnen 
entwickeln m&#246;chte, sind auf experimentell-physikalischem Boden erwachsen.
Darin liegt ihre St&#228;rke. Ihre Tendenz ist eine radikale. Von Stund' an
sollen Raum f&#252;r sich und Zeit f&#252;r sich v&#246;llig zu Schatten herabsinken und
nur noch eine Art Union der beiden soll Selbst&#228;ndigkeit bewahren. Ich
m&#246;chte zun&#228;chst ausf&#252;hren, wie man von der gegenw&#228;rtig angenommen
Mechanik wohl durch eine rein mathematische &#220;berlegung zu ver&#228;nderten
Ideen &#252;ber Raum und Zeit kommen k&#246;nnte."
<div class="p"><!----></div>
<a name="tthFtNtABI"></a><a href="#tthFrefABI">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>18</mn></mrow>
</msup>
</mrow></math></a>The empirical adequacy of the "Lorentz-Einstein" theory had been 
challenged by Walter Kaufmann in 1905, on the basis of his measurements of
the magnetic deflection of cathode rays (see Miller 1981 and Hon 1995).
Two days after Minkowski's lecture, Alfred Bucherer announced to the
physical section the results of his deflection experiments, which
contradicted those of Kaufmann and confirmed the expectations of the
Lorentz-Einstein theory (Bucherer 1908). In the discussion of this
lecture, Minkowski expressed joy in seeing the "monstrous" rigid electron
hypothesis experimentally defeated in favor of the deformable electron of
Lorentz's theory (see Bucherer 1908: 762).
<div class="p"><!----></div>
<a name="tthFtNtABJ"></a><a href="#tthFrefABJ">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>19</mn></mrow>
</msup>
</mrow></math></a>Minkowski introduced the use of <i>covariance</i> with respect to
the Lorentz transformations in Minkowski 1908a: 473. In the Cologne
lecture, the term <i>invariant</i> was employed in reference to both
covariant and invariant expressions.
<div class="p"><!----></div>
<a name="tthFtNtACA"></a><a href="#tthFrefACA">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>20</mn></mrow>
</msup>
</mrow></math></a>Born 1920. A similar diagram appeared earlier in a work by Vito
Volterra, who attributed it to a lecture given in Rome by Guido
Castelnuovo (Volterra 1912: 22, fig.&#x00A0;5).
<div class="p"><!----></div>
<a name="tthFtNtACB"></a><a href="#tthFrefACB">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>21</mn></mrow>
</msup>
</mrow></math></a>Nieders&#228;chsische Staats- und Universit&#228;tsbibliothek, Math.&#x00A0;Archiv
60: 2, courtesy of the Handschriftenabteilung. Minkowski's
hand-colored, transparent slide (
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mn>10</mn><mo>&times;</mo><mn>15</mn></mrow></math> cm) is reproduced here as
Figure&#x00A0;2. Similar figures appear in Minkowski 1909: 77.
<div class="p"><!----></div>
<a name="tthFtNtACC"></a><a href="#tthFrefACC">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>22</mn></mrow>
</msup>
</mrow></math></a>"jene spezielle Transformation in der Grenze sich in eine
solche verwandelt, wobei die 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>'</mo></mrow></math>-Achse eine beliebige Richtung nach oben
haben kann und 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo></mrow></math> immer genauer sich an 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math> ann&#228;hert."
<div class="p"><!----></div>
<a name="tthFtNtACD"></a><a href="#tthFrefACD">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>23</mn></mrow>
</msup>
</mrow></math></a>The elegance of Minkowski's presentation of relativistic kinematics
with respect to classical kinematics was admired and appreciated by many,
including Max Planck, who may have been in the audience. See Planck 1910b:
42.
<div class="p"><!----></div>
<a name="tthFtNtACE"></a><a href="#tthFrefACE">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>24</mn></mrow>
</msup>
</mrow></math></a>"Bei dieser Sachlage, und da 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
</mrow></math> mathematisch verst&#228;ndlicher ist 
als 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>&infin;</mi></mrow>
</msub>
</mrow></math>, h&#228;tte wohl ein Mathematiker in freier Phantasie auf den
Gedanken verfallen k&#246;nnen, da&#223; am Ende die Naturerscheinungen
tats&#228;chlich eine Invarianz nicht bei der Gruppe 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>&infin;</mi></mrow>
</msub>
</mrow></math>, sondern
vielmehr bei einer Gruppe 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
</mrow></math> mit bestimmtem endlichen, nur in den
gew&#246;hnlichen Ma&#223;einheiten <i>&#228;us&#223;erst gro&#223;en</i> 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>c</mi></mrow></math> besitzen.
Eine solche Ahnung w&#228;re ein au&#223;erordentlicher Triumph der reinen
Mathematik gewesen."
<div class="p"><!----></div>
<a name="tthFtNtACF"></a><a href="#tthFrefACF">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>25</mn></mrow>
</msup>
</mrow></math></a>"Nun, da die Mathematik hier nur mehr Treppenwitz bekundet, bleibt
ihr doch die Genugtuung, da&#223; sie dank ihren gl&#252;cklichen Antezedenzien
mit ihren in freier Fernsicht gesch&#228;rften Sinnen die tiefgreifenden
Konsequenzen einer solcher Ummodelung unserer Naturauffassung auf der
Stelle zu erfassen vermag." We translate "Treppenwitz" literally as
"staircase-wit," although the term was taken by Giuseppe Gianfranceschi
and Guido Castelnuovo to mean that mathematics had not accomplished the first
step: "Qui veramente la matematica non ha compiuro il primo passo ... " (see
Minkowski 1909: 338).
<div class="p"><!----></div>
<a name="tthFtNtACG"></a><a href="#tthFrefACG">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>26</mn></mrow>
</msup>
</mrow></math></a>The entry of mathematicians into the field of relativity was
described by Einstein as an invasion, as Sommerfeld later recalled (1949:
102). To counterbalance what he found "extraordinarily compelling" [<i>
ungemein Zwingendes </i>] in Minkowski's theory, Wien stressed the
importance to the physicist of experimental results, in contrast to the
"aesthetic factors" that guided the mathematician (1909a: 39). On the
emergence of theoretical physics in Germany, see Stichweh 1984;
Jungnickel &amp; McCormmach 1986; Olesko 1991. The term "disciplinary
frontier" is borrowed from Rudolf Stichweh's writings.
<div class="p"><!----></div>
<a name="tthFtNtACH"></a><a href="#tthFrefACH">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>27</mn></mrow>
</msup>
</mrow></math></a>This is further suggested by the sociologist Erving Goffman's
analysis of the presentation of self. Goffman noted that individuals
present a different "face" to different audiences. The audience reserves
the right to take the individual at his occupational face value, seeing in
this a way to save time and emotional energy. According to Goffman, even
if an individual were to try to break out of his occupational role,
audiences would often prevent such action (see Goffman 1959: 57).
<div class="p"><!----></div>
<a name="tthFtNtACI"></a><a href="#tthFrefACI">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>28</mn></mrow>
</msup>
</mrow></math></a>Examples of the identification of this passage as Minkowski's
principle of relativity are found in several reports, such as Volkmann
1910: 148, and Wiechert 1915: 55.
<div class="p"><!----></div>
<a name="tthFtNtACJ"></a><a href="#tthFrefACJ">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>29</mn></mrow>
</msup>
</mrow></math></a>"Das Bestehen der Invarianz der Naturgesetze f&#252;r die bez&#252;gliche 
Gruppe 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
</mrow></math> w&#252;rde nun so zu fassen sein: Man kann aus der Gesamtheit der 
Naturerscheinungen durch sukzessiv gesteigerte Approximationen immer
genauer ein Bezugsystem 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>,</mo><mi>y</mi><mo>,</mo><mi>z</mi></mrow></math> und 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi></mrow></math>, Raum und Zeit, ableiten,
mittels dessen diese Erscheinungen sich dann nach bestimmten Gesetzen
darstellen. Dieses Bezugsystem ist dabei aber durch die Erscheinungen
keineswegs eindeutig festgelegt. <i>Man kann das Bezugsystem noch
entsprechend den Transformationen der genannten Gruppe 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi fontstyle="normal">G</mi></mrow><mrow><mi fontstyle="normal">c</mi></mrow>
</msub>
</mrow></math> beliebig
ver&#228;ndern, ohne da&#223; der Ausdruck der Naturgesetze sich dabei
ver&#228;ndert</i>."
<div class="p"><!----></div>
<a name="tthFtNtADA"></a><a href="#tthFrefADA">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>30</mn></mrow>
</msup>
</mrow></math></a>Neither Einstein, nor Lorentz, nor Poincar&#233; attended the Cologne
meeting, although in late February Einstein wrote to Johannes Stark of
his intention to do so (Einstein <i>CP5</i>: doc. 88).
<div class="p"><!----></div>
<a name="tthFtNtADB"></a><a href="#tthFrefADB">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>31</mn></mrow>
</msup>
</mrow></math></a>"Z. B. kann man der beschriebenen Figur entsprechend auch 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>'</mo></mrow></math> Zeit 
benennen, mu&#223; dann aber im Zusammenhange damit notwendig den Raum
durch die Mannigfaltigkeit der drei Parameter 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>y</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>z</mi></mrow></math> definieren,
wobei nun die physikalischen Gesetze mittels 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>y</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>z</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>'</mo></mrow></math> sich
genau ebenso ausdr&#252;cken w&#252;rden, wie mittels 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>y</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>z</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi></mrow></math>. Hiernach
w&#252;rden wir dann in der Welt nicht mehr <i>den</i> Raum, sondern 
unendlich viele R&#228;ume haben, analog wie es im dreidimensionalen Raume
unendlich viele Ebenen gibt. Die dreidimensionale Geometrie wird ein
Kapitel der vierdimensionalen Physik. Sie erkennen, weshalb ich am
Eingange sagte, Raum und Zeit sollen zu Schatten herabsinken und nur eine
Welt an sich bestehen."
<div class="p"><!----></div>
<a name="tthFtNtADC"></a><a href="#tthFrefADC">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>32</mn></mrow>
</msup>
</mrow></math></a>In G&#246;ttingen, Minkowski's lofty assertions were the target of
student humor, as witnessed by a student parody of the course guide, see
Galison 1979: 111, n. 69. Minkowski, whose lectures were said by
Born (1959: 682) to be punctuated by witty remarks, undoubtedly found
this amusing. His sharp sense of humor is also evident in the
correspondence with Hilbert (see R&#252;denberg &amp; Zassenhaus 1973).
<div class="p"><!----></div>
<a name="tthFtNtADD"></a><a href="#tthFrefADD">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>33</mn></mrow>
</msup>
</mrow></math></a>One sign of Poincar&#233;'s mathematical preeminence was the B&#243;lyai
Prize, awarded him by a unanimous jury in 1905. For studies of Poincar&#233;'s
mathematical contributions to relativity theory see Cuvaj 1968 and
Miller 1973. Poincar&#233;'s critique of fin-de-si&#232;cle electrodynamics is
discussed in Darrigol 1995.
<div class="p"><!----></div>
<a name="tthFtNtADE"></a><a href="#tthFrefADE">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>34</mn></mrow>
</msup>
</mrow></math></a>Poincar&#233; proved that the Lorentz transformations form a group in a 
letter to Lorentz (reproduced in Miller 1980), and later pointed out to
students the group nature of the parallel velocity transformations (see
the notes by Henri Vergne of Poincar&#233;'s 1906/7 lectures, Poincar&#233;
1906/7: 222).
<div class="p"><!----></div>
<a name="tthFtNtADF"></a><a href="#tthFrefADF">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>35</mn></mrow>
</msup>
</mrow></math></a>On Minkowski's labors see Hilbert 1909a: xxix.
<div class="p"><!----></div>
<a name="tthFtNtADG"></a><a href="#tthFrefADG">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>36</mn></mrow>
</msup>
</mrow></math></a>"Was das Verdienst der einzelnen Autoren angeht, so r&#252;hren die 
Grundlagen der Ideen von Lorentz her, Einstein hat das
Prinzip der Relativit&#228;t reinlicher herauspr&#228;pariert, zugleich es mit
besonderem Erfolge zur Behandlung spezieller Probleme der Optik bewegter
Medien angewandt, endlich auch zuerst die Folgerungen &#252;ber 
Ver&#228;nderlichkeit der mechanischen Masse bei thermodynamischen Vorg&#228;ngen
gezogen. Kurz danach und wohl unabh&#228;ngig von Einstein hat Poincar&#233; sich
in mehr mathematischer Untersuchung &#252;ber die Lorentzschen Elektronen und
die Stellung der Gravitation zu ihnen verbreitet, endlich hat Planck
einen Ansatz zu einer Dynamik auf Grund des Relativit&#228;tsprinzipes
versucht."
<div class="p"><!----></div>
<a name="tthFtNtADH"></a><a href="#tthFrefADH">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>37</mn></mrow>
</msup>
</mrow></math></a>"Vous connaissez sans doute l'opuscule de Minkowski "Raum und
Zeit," publi&#233; apr&#232;s sa mort ainsi que les id&#233;es de Einstein et Lorentz
sur la m&#234;me question. Maintenant M.&#x00A0;Fredholm me dit que vous avez touch&#233; &#224;
des id&#233;es semblables avant les autres, mais en vous exprimant d'une
mani&#232;re moins philosophique et plus math&#233;matique." It is a pleasure to
acknowledge the assistance of Dr.&#x00A0;K.&#x00A0;Broms in providing me with a copy of
this letter.
<div class="p"><!----></div>
<a name="tthFtNtADI"></a><a href="#tthFrefADI">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>38</mn></mrow>
</msup>
</mrow></math></a>The experiment was designed to test the validity of the principle
of relativity for the phenomenon of double refraction. The telling of 
this school anecdote may also be connected to Mittag-Leffler's campaign
to nominate Poincar&#233; for the 1910 Nobel Prize for physics. Poincar&#233; never
mentioned the names of Einstein or Minkowski in print in relation to the
theory of relativity, but during the course of this lecture, according to
one witness, he mentioned Einstein's work in this area (see Moszkowski
1920: 15).
<div class="p"><!----></div>
<a name="tthFtNtADJ"></a><a href="#tthFrefADJ">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>39</mn></mrow>
</msup>
</mrow></math></a>In a lecture to the Saint Louis Congress in September 1904,
Poincar&#233; interpreted the "principe de relativit&#233;" with respect to
Lorentz's theory of electrons, distinguishing this extended relativity
principle from the one employed in classical mechanics (1904: 314).
<div class="p"><!----></div>
<a name="tthFtNtAEA"></a><a href="#tthFrefAEA">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>40</mn></mrow>
</msup>
</mrow></math></a>Willy Wien spelled out this role at the 1905 meeting of the German 
Society of Mathematicians in Meran. Wien suggested that "physics itself"
required "more comprehensive cooperation" from mathematicians in order
to solve its current problems, including those encountered in the theory
of electrons (Wien 1906: 42; McCormmach 1976: xxix). While
Poincar&#233;'s work in optics and electricity was well received, and his
approach emulated by some German physicists (see Darrigol 1993: 223),
mathematicians generally considered him their representative.
<div class="p"><!----></div>
<a name="tthFtNtAEB"></a><a href="#tthFrefAEB">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>41</mn></mrow>
</msup>
</mrow></math></a>In response to Minkowski's attribution of the transformations to
his 1887 paper, Voigt gently protested that he was concerned at that time
with the elastic-solid ether theory of light, not the electromagnetic
theory. At the same time, Voigt acknowledged that his paper contained
some of the results later obtained from electromagnetic-field theory (see
the discussion following Bucherer 1908: 762). In honor of the tenth
anniversary of the principle of relativity, the editors of <i>
Physikalische Zeitschrift</i>, Voigt's colleagues Peter Debye and Hermann
Simon, decided to re-edit the 1887 paper, with additional notes by the 
author (Voigt 1915). Shortly afterwards, Lorentz generously conceded
that the idea for the transformations might have come from Voigt (Lorentz
1916: 198, n. 1).
<div class="p"><!----></div>
<a name="tthFtNtAEC"></a><a href="#tthFrefAEC">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>42</mn></mrow>
</msup>
</mrow></math></a>Lorentz's theory did not purport to explain the hypothetical
contraction. Although he made no mention of this in the Cologne lecture,
Minkowski pointed out in the <i>Grundgleichungen</i> that the
(macroscopic) equations for moving dielectrics obtained from Lorentz's
electron theory did not respect the principle of relativity (1908: 493).
<div class="p"><!----></div>
<a name="tthFtNtAED"></a><a href="#tthFrefAED">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>43</mn></mrow>
</msup>
</mrow></math></a>"Jedoch scharf erkannt zu haben, da&#223; die Zeit des einen Elektrons
ebenso gut wie die des anderen ist, d.h.&#x00A0;da&#223; 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi></mrow></math> und 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>'</mo></mrow></math> gleich zu
behandeln sind, ist erst das Verdienst von A.&#x00A0;Einstein."
<div class="p"><!----></div>
<a name="tthFtNtAEE"></a><a href="#tthFrefAEE">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>44</mn></mrow>
</msup>
</mrow></math></a>"Damit war nun zun&#228;chst die Zeit als ein durch die Erscheinungen 
eindeutig festgelegter Begriff abgesetzt" (Minkowski 1909: 81).
<div class="p"><!----></div>
<a name="tthFtNtAEF"></a><a href="#tthFrefAEF">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>45</mn></mrow>
</msup>
</mrow></math></a>"An dem Begriffe des Raumes r&#252;ttelten weder Einstein noch Lorentz, 
vielleicht deshalb nicht, weil bei der genannten speziellen
Transformation, wo die 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo><mo>,</mo><mi>t</mi><mo>'</mo></mrow></math>-Ebene sich mit der 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>,</mo><mi>t</mi></mrow></math>-Ebene deckt,
eine Deutung m&#246;glich ist, als sei die 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi></mrow></math>-Achse des Raumes in ihrer Lage
erhalten geblieben."
<div class="p"><!----></div>
<a name="tthFtNtAEG"></a><a href="#tthFrefAEG">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>46</mn></mrow>
</msup>
</mrow></math></a>"&#220;ber den Begriff des Raumes in entsprechender Weise 
hinwegzuschreiten, ist auch wohl nur als Verwegenheit mathematischer
Kultur einzutaxieren. Nach diesem zum wahren Verst&#228;ndnis der Gruppe 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
</mrow></math>
jedoch unerl&#228;&#223;lichen weiteren Schritt aber scheint mir das Wort <i>
Relativit&#228;tspostulat</i> f&#252;r die Forderung einer Invarianz bei der Gruppe

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>G</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
</mrow></math> sehr matt."
<div class="p"><!----></div>
<a name="tthFtNtAEH"></a><a href="#tthFrefAEH">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>47</mn></mrow>
</msup>
</mrow></math></a>"Die ausnahmslose G&#252;ltigkeit des Weltpostulates ist, so m&#246;chte ich 
glauben, der wahre Kern eines elektromagnetischen Weltbildes, der von
Lorentz getroffen, von Einstein weiter herausgesch&#228;lt, nachgerade
vollends am Tage liegt."
<div class="p"><!----></div>
<a name="tthFtNtAEI"></a><a href="#tthFrefAEI">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>48</mn></mrow>
</msup>
</mrow></math></a>Minkowski to Paul Ehrenfest, 22 October 1908, Ehrenfest Papers, 
Museum Boerhaave, Leiden. Judging from the manuscripts in Minkowski's 
<i>Nachla&#223;</i> (Nieders&#228;chsische Staats- und Universit&#228;tsbibliothek,
Math.&#x00A0;Archiv 60: 1), he had made little progress on Einstein-electrons
before an attack of appendicitis put an end to his life in January 1909,
only ten weeks after writing to Ehrenfest. An electron-theoretical
derivation of the basic electromagnetic equations for moving media
appeared under Minkowski's name in 1910, but was actually written by Max
Born (cf. Minkowski &amp; Born 1910: 527).
<div class="p"><!----></div>
<a name="tthFtNtAEJ"></a><a href="#tthFrefAEJ">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>49</mn></mrow>
</msup>
</mrow></math></a>See Minkowski 1908a: &#167;  5; 1909: 78.
<div class="p"><!----></div>
<a name="tthFtNtAFA"></a><a href="#tthFrefAFA">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>50</mn></mrow>
</msup>
</mrow></math></a>The terminology of <i>Galilean transformations</i> was introduced
by Philipp Frank (1908: 898) in his analysis of the <i>
Grundgleichungen</i>.
<div class="p"><!----></div>
<a name="tthFtNtAFB"></a><a href="#tthFrefAFB">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>51</mn></mrow>
</msup>
</mrow></math></a>Lorentz (1904) used the Galilean transformations separately from,
and in conjunction with the following transformations (the notation is
modified): 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>x</mi><mo>'</mo><mo>=</mo><mi>&beta;</mi><mi>x</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>y</mi><mo>'</mo><mo>=</mo><mi>y</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>z</mi><mo>'</mo><mo>=</mo><mi>z</mi></mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>=</mo><mi>t</mi><mo stretchy="false">/</mo><mi>&beta;</mi><mo>-</mo><mi>&beta;</mi><mi>vx</mi><mo stretchy="false">/</mo>
<msup><mrow><mi>c</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></math>,
where 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>&beta;</mi><mo>=</mo><mn>1</mn><mo stretchy="false">/</mo><msqrt><mrow><mn>1</mn><mo>-</mo>
<msup><mrow><mi>v</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo stretchy="false">/</mo>
<msup><mrow><mi>c</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></msqrt></mrow></math>.
<div class="p"><!----></div>
<a name="tthFtNtAFC"></a><a href="#tthFrefAFC">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>52</mn></mrow>
</msup>
</mrow></math></a>To suppose 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi></mrow></math> equal to 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>'</mo></mrow></math>, Einstein commented later, was to make
an "arbitrary hypothesis" (1910: 26).
<div class="p"><!----></div>
<a name="tthFtNtAFD"></a><a href="#tthFrefAFD">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>53</mn></mrow>
</msup>
</mrow></math></a>This value of 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>c</mi></mrow></math> itself implies the orthogonality of temporal and
spatial axes in every inertial system, a feature which is not apparent on
a Minkowski diagram. For his part, Einstein defined the units of length
and time (ideal rods and clocks) in a coordinate-free manner.
<div class="p"><!----></div>
<a name="tthFtNtAFE"></a><a href="#tthFrefAFE">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>54</mn></mrow>
</msup>
</mrow></math></a>On Einstein's reluctance to confound kinematics with geometry see 
his introduction of the terms "geometric shape" and "kinematic shape"
to distinguish the forms of rigid bodies in a rest frame from those of
rigid bodies in frames in uniform relative motion (Einstein 1907: 417,
1910: 28; Paty 1993: 170). At the same time, Einstein's recognition
of the fundamental nature of the invariance of the quantity 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow><mi>c</mi></mrow><mrow><mn>2</mn></mrow>
</msup>

<msup><mrow><mi>t</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>-</mo>
<msup><mrow><mi>x</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>-</mo>
<msup><mrow><mi>y</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>-</mo>
<msup><mrow><mi>z</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></math> can not be doubted; in 1907, for example, he used this
invariance to simplify his derivation of the special Lorentz
transformations (1907: 419).
<div class="p"><!----></div>
<a name="tthFtNtAFF"></a><a href="#tthFrefAFF">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>55</mn></mrow>
</msup>
</mrow></math></a>A basis for this conflation was provided by Einstein in 1906, when
he referred to the "<i>Theorie von Lorentz und Einstein</i>" (see the
editorial note in Einstein <i>CP2</i>: 372).
<div class="p"><!----></div>
<a name="tthFtNtAFG"></a><a href="#tthFrefAFG">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>56</mn></mrow>
</msup>
</mrow></math></a>Frank 1910: 494; Castelnuovo 1911: 78. For later examples
see Silberstein 1914: 134 and Born 1920: 170. Extreme discretion was
exercised here, as none of these writers taxed Minkowski with error.
<div class="p"><!----></div>
<a name="tthFtNtAFH"></a><a href="#tthFrefAFH">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>57</mn></mrow>
</msup>
</mrow></math></a>Many historians have suggested that Minkowski never fully
understood Einstein's theory of relativity, for example, Miller
(1981: 241), Goldberg (1984: 193); Pyenson (1985: 130).
<div class="p"><!----></div>
<a name="tthFtNtAFI"></a><a href="#tthFrefAFI">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>58</mn></mrow>
</msup>
</mrow></math></a> On Minkowski's discovery of proper time, see Walter 1996: 101.
<div class="p"><!----></div>
<a name="tthFtNtAFJ"></a><a href="#tthFrefAFJ">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>59</mn></mrow>
</msup>
</mrow></math></a>Minkowski's expression for proper time, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mo>&int;</mo><mi>d</mi><mi>&tau;</mi><mo>=</mo><mo>&int;</mo><mi>dt</mi><msqrt><mrow><mn>1</mn><mo>-</mo>
<msup><mrow><mi>v</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo stretchy="false">/</mo>
<msup><mrow><mi>c</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></msqrt></mrow></math>, may be compared with Einstein's expression for
time dilation, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>&tau;</mi><mo>=</mo><mi>t</mi><msqrt><mrow><mn>1</mn><mo>-</mo>
<msup><mrow><mi>v</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo stretchy="false">/</mo>
<msup><mrow><mi>c</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></msqrt></mrow></math>, although the contexts in which
these formulae appeared were quite dissimilar (Einstein 1905: 904; Miller
1981: 271-272). The notation has been changed for ease of comparison.
<div class="p"><!----></div>
<a name="tthFtNtAGA"></a><a href="#tthFrefAGA">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>60</mn></mrow>
</msup>
</mrow></math></a>Einstein's research notes indicate that he adopted a Riemannian
space-time metric as the basis of his theory of gravitation in the summer
of 1912; see the transcriptions and editorial notes in Einstein <i>CP4</i>.
<div class="p"><!----></div>
<a name="tthFtNtAGB"></a><a href="#tthFrefAGB">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>61</mn></mrow>
</msup>
</mrow></math></a>"Lorentz hatte f&#252;r das gleichf&#246;rmig bewegte Elektron die Verbindung 

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>'</mo><mo>=</mo><mo stretchy="false">(</mo><mo>-</mo><mi>qx</mi><mo>+</mo><mi>t</mi><mo stretchy="false">)</mo><mo stretchy="false">/</mo><msqrt><mrow><mn>1</mn><mo>-</mo>
<msup><mrow><mi>q</mi></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></msqrt></mrow></math> Ortszeit des Elektrons genannt, und
zum Verst&#228;ndnis der Kontraktionshypothese diesen Begriff verwandt.
Lorentz selbst sagte mir gespr&#228;chsweise in Rom, dass die Zeit des einen
Elektrons ebensogut wie die des anderen ist, d.h. die Gleichwertigkeit zu

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi></mrow></math> und 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>t</mi><mo>'</mo></mrow></math> erkannt zu haben, das Verdienst von Einstein ist." (Undated manuscript, Nieders&#228;chsische Staats- und Universit&#228;tsbibliothek,
Math. Archiv 60:4, 11) Minkowski's story was corroborated in part by his student Louis Kollros,
who recalled overhearing Lorentz and Minkowski's conversation on
relativity during a Sunday visit to the gardens of the Villa d'Este in
Tivoli (Kollros 1956: 276).
<div class="p"><!----></div>
<a name="tthFtNtAGC"></a><a href="#tthFrefAGC">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>62</mn></mrow>
</msup>
</mrow></math></a>See Eckert &amp; Pricha 1984; Jungnickel &amp; McCormmach 1986: vol.&#x00A0;2,
274.
<div class="p"><!----></div>
<a name="tthFtNtAGD"></a><a href="#tthFrefAGD">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>63</mn></mrow>
</msup>
</mrow></math></a>See the
  remarks made by Sommerfeld after a lecture by Planck (1906: 761).
<div class="p"><!----></div>
<a name="tthFtNtAGE"></a><a href="#tthFrefAGE">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>64</mn></mrow>
</msup>
</mrow></math></a>In this
  letter, Minkowski extended an invitation to Sommerfeld to
  participate in a debate on electron theory to be held at the meeting
  of the Mathematical Society in G&#246;ttingen on the eighth of August.
<div class="p"><!----></div>
<a name="tthFtNtAGF"></a><a href="#tthFrefAGF">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>65</mn></mrow>
</msup>
</mrow></math></a>Along with the mathematicians Eduard Study and Friedrich Engel.
Only Study's remarks were recorded; see <i>Verhandlungen der
Gesellschaft Deutscher Naturforscher und &#196;rzte</i> <b>80</b> (1909): vol.&#x00A0;2,
9.
<div class="p"><!----></div>
<a name="tthFtNtAGG"></a><a href="#tthFrefAGG">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>66</mn></mrow>
</msup>
</mrow></math></a>"Ich bin jetzt auch zur Relativtheorie bekehrt; besonders die
systematische Form und Auffassung Minkowski's hat mir das Verst&#228;ndnis
erleichtert."
<div class="p"><!----></div>
<a name="tthFtNtAGH"></a><a href="#tthFrefAGH">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>67</mn></mrow>
</msup>
</mrow></math></a>Sommerfeld (1909a); (1909b); lecture notes entitled
  "<em>Elektronentheorie</em>," Deutsches Museum, Sommerfeld <em>
    Nachla&#223;</em>; Archives for History of Quantum Physics, reel 22.
<div class="p"><!----></div>
<a name="tthFtNtAGI"></a><a href="#tthFrefAGI">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>68</mn></mrow>
</msup>
</mrow></math></a>Einstein later wrote to Laub that he had persuaded Sommerfeld of the
correctness of their formula (27 August 1910; Einstein <i>CP5</i>: doc.&#x00A0;224).
For a description of the physics involved, see the editorial note in
Einstein <i>CP2</i>: 503. Debate on this question continued for several
years, but by 1918, as Einstein candidly acknowledged to Walter
D&#228;llenbach, it had been known for a while that the formula he derived
with Laub was wrong (F&#246;lsing 1993: 276).
<div class="p"><!----></div>
<a name="tthFtNtAGJ"></a><a href="#tthFrefAGJ">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>69</mn></mrow>
</msup>
</mrow></math></a>"Die umst&#228;ndlichen Rechnungen, durch die Lorentz (1895 und 1904)
und Einstein (1905) ihre vom Koordinatensystem unabh&#228;ngige G&#252;ltigkeit
erweisen und die Bedeutung der transformierten Feldvektoren feststellen
mu&#223;ten, werden also im System der Minkowskischen `Welt' gegenstandslos."
<div class="p"><!----></div>
<a name="tthFtNtAHA"></a><a href="#tthFrefAHA">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>70</mn></mrow>
</msup>
</mrow></math></a>"Enth&#252;llen erst in vier Dimensionen ihr inneres Wesen voller
Einfachheit" in a paraphrase of Minkowski 1909: 88. On this theme see also
Sommerfeld 1910b: 249-250.
<div class="p"><!----></div>
<a name="tthFtNtAHB"></a><a href="#tthFrefAHB">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>71</mn></mrow>
</msup>
</mrow></math></a>Poincar&#233; had shown that the stability of Lorentz's deformable
electron required the introduction of a compensatory non-electromagnetic
potential, producing what was later dubbed <i>Poincar&#233; pressure</i>; for
details, see Cuvaj 1968 and Miller 1973:&#x00A0;300.
<div class="p"><!----></div>
<a name="tthFtNtAHC"></a><a href="#tthFrefAHC">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>72</mn></mrow>
</msup>
</mrow></math></a>For an example of Sommerfeld's later fascination with the
electromagnetic world picture, see Sommerfeld 1922: chap.&#x00A0;1, &#167;  2.
<div class="p"><!----></div>
<a name="tthFtNtAHD"></a><a href="#tthFrefAHD">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>73</mn></mrow>
</msup>
</mrow></math></a>According to Reid 1970: 129, Sommerfeld sent his student
P.&#x00A0;P.&#x00A0;Ewald to Hilbert in 1912.
<div class="p"><!----></div>
<a name="tthFtNtAHE"></a><a href="#tthFrefAHE">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>74</mn></mrow>
</msup>
</mrow></math></a><i>Nachrichten von der K&#246;niglichen Gesellschaft der
Wissenschaften zu G&#246;ttingen, gesch&#228;ftliche Mitteilungen</i> (1910): 13,
117; (1913): 18; Born 1978: 147.
<div class="p"><!----></div>
<a name="tthFtNtAHF"></a><a href="#tthFrefAHF">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>75</mn></mrow>
</msup>
</mrow></math></a>These figures are based on primary articles only, excluding book
reviews and abstracts; for details, see the author's Ph.D.&#x00A0;dissertation
(Walter 1996: chap.&#x00A0;4).
<div class="p"><!----></div>
<a name="tthFtNtAHG"></a><a href="#tthFrefAHG">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>76</mn></mrow>
</msup>
</mrow></math></a>On the research themes chosen by the German Society of
Mathematicians and Klein's role in promoting applied mathematics, see
Tobies 1989: 229.
<div class="p"><!----></div>
<a name="tthFtNtAHH"></a><a href="#tthFrefAHH">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>77</mn></mrow>
</msup>
</mrow></math></a>Hilbert to Professor H.&#x00A0;A.&#x00A0;Kr&#252;ss, undated typescript,
Nieders&#228;chsische Staats- und Universit&#228;tsbibliothek, Hilbert <i>Nachla&#223;</i>
494. Hilbert gave Einstein credit for having drawn the "full
logical consequence" of the Einstein addition theorem, while the
"definitive mathematical expression of Einstein's idea" was left to
Minkowski. See also Pyenson 1985: 192.
<div class="p"><!----></div>
<a name="tthFtNtAHI"></a><a href="#tthFrefAHI">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>78</mn></mrow>
</msup>
</mrow></math></a>"Lust ist er heute, Mathematiker zu sein, wo allerwegen die Math.
emporspriesst und die emporgesprossene erblickt, wo in ihrer Anwendung
auf Naturwissenschaft wie andererseits in der Richtung nach der
Philosophie hin die Math. immer mehr zur Geltung kommt und ihre ehemalige
zentrale Stellung zur&#252;ckzuerobern ein Begriff steht." For a
full translation of Hilbert's address, differing slightly from my own,
see Rowe 1986: 76.
<div class="p"><!----></div>
<a name="tthFtNtAHJ"></a><a href="#tthFrefAHJ">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>79</mn></mrow>
</msup>
</mrow></math></a>"Affermare che la velocit&#224; della luce vale sempre 1, qualunque sia
l'osservatore, equivale ad asserire che il cambiamento nell'asse del
tempo porta pure un cambiamento nell'asse dello spazio."
<div class="p"><!----></div>
<a name="tthFtNtAIA"></a><a href="#tthFrefAIA">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>80</mn></mrow>
</msup>
</mrow></math></a>"Il cambiamento a dir vero sarebbe solo percepito dal demone di
Minkowski. Ma di qualche differenza nelle particolarit&#224; dei fenomeni
dovremmo accorgerci noi pure, quando i nostri sensi fossero abbastanza
delicati." The artifice of a demon-recalling Maxwell's demon-was
attributed to Minkowski by Castelnuovo earlier in his article, and
connected to H.&#x00A0;G.&#x00A0;Wells' writings. According to Castelnuovo, Minkowski
"immagina uno spirito superiore al nostro, il quale concepisca il tempo
come une quarta dimensione dello spazio, e possa seguire l'eroe di un noto
romanzo di Wells nel suo viaggio meraviglioso attraverso ai secoli"
(Castelnuovo 1911: 76).
<div class="p"><!----></div>
<a name="tthFtNtAIB"></a><a href="#tthFrefAIB">
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mn>81</mn></mrow>
</msup>
</mrow></math></a>Robert Gnehm to Einstein, 8 December 1911 (Einstein <i>CP5</i>: doc.
317).</body></html>
