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	<id>https://invarians.org/index.php?action=history&amp;feed=atom&amp;title=Noether%27s_theorems%2FHistory%2FThe_recovery_in_field_theory</id>
	<title>Noether&#039;s theorems/History/The recovery in field theory - Revision history</title>
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	<updated>2026-10-21T07:34:18Z</updated>
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		<id>https://invarians.org/index.php?title=Noether%27s_theorems/History/The_recovery_in_field_theory&amp;diff=549&amp;oldid=prev</id>
		<title>BFP Rauch: 1 revision imported</title>
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		<updated>2026-09-10T13:29:56Z</updated>

		<summary type="html">&lt;p&gt;1 revision imported&lt;/p&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 13:29, 10 September 2026&lt;/td&gt;
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		<author><name>BFP Rauch</name></author>
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	<entry>
		<id>https://invarians.org/index.php?title=Noether%27s_theorems/History/The_recovery_in_field_theory&amp;diff=548&amp;oldid=prev</id>
		<title>NT&gt;NoetherVolumeBuild: Noether theorems volume, initial import (H-08)</title>
		<link rel="alternate" type="text/html" href="https://invarians.org/index.php?title=Noether%27s_theorems/History/The_recovery_in_field_theory&amp;diff=548&amp;oldid=prev"/>
		<updated>2026-09-10T00:00:00Z</updated>

		<summary type="html">&lt;p&gt;Noether theorems volume, initial import (H-08)&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{DISPLAYTITLE:The recovery in field theory}}&lt;br /&gt;
&lt;br /&gt;
By the 1970s &amp;quot;Noether&amp;#039;s theorem&amp;quot; was standard in every graduate course in field&lt;br /&gt;
theory. This page traces how it got there, and notes what the route cost.&lt;br /&gt;
&lt;br /&gt;
== The waypoints ==&lt;br /&gt;
&lt;br /&gt;
The recovery was not a single event and no one paper did it. The following are&lt;br /&gt;
the points usually named, and they are named here as the commonly cited route,&lt;br /&gt;
not as a verified account.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Belinfante and Rosenfeld, 1939 and 1940.&amp;#039;&amp;#039;&amp;#039; The stress-energy tensor that the&lt;br /&gt;
first theorem produces is the canonical one, which is neither unique nor&lt;br /&gt;
generally symmetric. Their improvement adds a divergence term that symmetrises&lt;br /&gt;
it without changing the conserved charges. This put the theorem&amp;#039;s output into&lt;br /&gt;
the form general relativity needs, and made the non-uniqueness a subject rather&lt;br /&gt;
than an embarrassment.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Bergmann and the constrained-Hamiltonian programme, from 1949.&amp;#039;&amp;#039;&amp;#039; Work on the&lt;br /&gt;
Hamiltonian formulation of general relativity ran directly into the fact that&lt;br /&gt;
the second theorem describes: a theory with local symmetry has fewer independent&lt;br /&gt;
equations than fields, and its Hamiltonian formulation therefore carries&lt;br /&gt;
constraints. This is the second theorem rediscovered from the inside, by people&lt;br /&gt;
solving a concrete problem.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Hill, 1951.&amp;#039;&amp;#039;&amp;#039; A review article in &amp;#039;&amp;#039;Reviews of Modern Physics&amp;#039;&amp;#039; on&lt;br /&gt;
Hamilton&amp;#039;s principle and the conservation theorems. This is the paper most often&lt;br /&gt;
credited with putting the theorem in front of physicists in a form they could&lt;br /&gt;
use, and it is also, on the usual account, where the restriction to the first&lt;br /&gt;
theorem in its field-theory special case became the standard presentation.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Yang and Mills, 1954, and the gauge theories that followed.&amp;#039;&amp;#039;&amp;#039; Utiyama in&lt;br /&gt;
1956 and Kibble in 1961 extended the gauge idea to gravitation. Once physics had&lt;br /&gt;
several theories with local symmetry rather than one, the second theorem stopped&lt;br /&gt;
being a remark about general relativity and became the general structural fact&lt;br /&gt;
about gauge theories.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Trautman, from 1962.&amp;#039;&amp;#039;&amp;#039; Conservation laws in general relativity, treated&lt;br /&gt;
properly as an instance of the theorem rather than as a special problem.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Ward and Takahashi, 1950 and 1957.&amp;#039;&amp;#039;&amp;#039; The quantum statement. A symmetry of&lt;br /&gt;
the action constrains the correlation functions of the quantised theory, and the&lt;br /&gt;
Ward-Takahashi identity is what survives of the classical conservation law. This&lt;br /&gt;
is also where the boundary appears: a classical symmetry can fail to survive&lt;br /&gt;
quantisation, and the anomaly is the failure.&lt;br /&gt;
&lt;br /&gt;
== What the route cost ==&lt;br /&gt;
&lt;br /&gt;
The theorem physics recovered is not the theorem Noether proved, and the&lt;br /&gt;
differences are traceable to the route.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;One theorem, not two.&amp;#039;&amp;#039;&amp;#039; What entered the textbooks was the first theorem.&lt;br /&gt;
The second entered separately and under other names — constraints, Noether&lt;br /&gt;
identities, Bianchi identities — and its connection to the same 1918 paper was&lt;br /&gt;
often not made.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;One direction, not two.&amp;#039;&amp;#039;&amp;#039; The converses were dropped almost everywhere. A&lt;br /&gt;
textbook statement of the theorem usually proves that a symmetry gives a&lt;br /&gt;
conservation law and stops.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;A special case, not the general statement.&amp;#039;&amp;#039;&amp;#039; Physics needed one independent&lt;br /&gt;
variable or four, first derivatives, and transformations that do not mix the&lt;br /&gt;
dependent and independent variables. That is what got stated. Noether&amp;#039;s actual&lt;br /&gt;
statement allows arbitrary derivative order and full mixing.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;An addition credited backwards.&amp;#039;&amp;#039;&amp;#039; Divergence invariance is&lt;br /&gt;
[[Noether&amp;#039;s theorems/History/Bessel-Hagen and the first uses|Bessel-Hagen&amp;#039;s]],&lt;br /&gt;
and is now routinely presented as part of Noether&amp;#039;s theorem.&lt;br /&gt;
&lt;br /&gt;
None of these losses is a mistake in the physics. A special case correctly&lt;br /&gt;
stated is still correct. They are losses in what the theorem is understood to&lt;br /&gt;
say, and they are why&lt;br /&gt;
[[Noether&amp;#039;s theorems/History/What Noether&amp;#039;s theorem now means|the name now means&lt;br /&gt;
different things]] in different rooms.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;Provenance: this page contains no verbatim quotation and no page reference was&lt;br /&gt;
verified against the papers named. The route above is the one the secondary&lt;br /&gt;
literature commonly gives; the attributions are standard but were not checked&lt;br /&gt;
against the primary papers. See [[Noether&amp;#039;s theorems/Sources|Sources]].&amp;#039;&amp;#039;&lt;br /&gt;
&lt;/div&gt;</summary>
		<author><name>NT&gt;NoetherVolumeBuild</name></author>
	</entry>
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