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	<id>https://invarians.org/index.php?action=history&amp;feed=atom&amp;title=Noether%27s_theorems%2FApplications%2FGeneral_relativity_and_the_Bianchi_identity</id>
	<title>Noether&#039;s theorems/Applications/General relativity and the Bianchi identity - Revision history</title>
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	<updated>2026-10-21T16:04:03Z</updated>
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	<entry>
		<id>https://invarians.org/index.php?title=Noether%27s_theorems/Applications/General_relativity_and_the_Bianchi_identity&amp;diff=417&amp;oldid=prev</id>
		<title>BFP Rauch: 1 revision imported</title>
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		<updated>2026-09-10T13:29:54Z</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>
	</entry>
	<entry>
		<id>https://invarians.org/index.php?title=Noether%27s_theorems/Applications/General_relativity_and_the_Bianchi_identity&amp;diff=416&amp;oldid=prev</id>
		<title>NT&gt;NoetherVolumeBuild: Noether theorems volume, initial import (A-06)</title>
		<link rel="alternate" type="text/html" href="https://invarians.org/index.php?title=Noether%27s_theorems/Applications/General_relativity_and_the_Bianchi_identity&amp;diff=416&amp;oldid=prev"/>
		<updated>2026-09-10T00:00:00Z</updated>

		<summary type="html">&lt;p&gt;Noether theorems volume, initial import (A-06)&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{DISPLAYTITLE:General relativity and the Bianchi identity}}&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;Plain-language counterpart: [[Noether&amp;#039;s theorems/Explainers/An identity hiding inside Einstein&amp;#039;s equations|An identity hiding inside Einstein&amp;#039;s equations]].&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
[[File:NT-F-13.png|thumb|right|360px|alt=Two groups of five bars representing field equations. On the left, without a local symmetry, all five are independent. On the right, one free function makes the fifth follow from the other four, shown by a curved arrow. A caption states the counting: one arbitrary function gives one identity and one equation that was never independent.|Identities among the field equations from a local symmetry]]&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;This page derives the count and does not derive the identity.&amp;#039;&amp;#039;&amp;#039; The&lt;br /&gt;
distinction is the whole content.&lt;br /&gt;
&lt;br /&gt;
== The count, derived ==&lt;br /&gt;
&lt;br /&gt;
General relativity&amp;#039;s local symmetry is the freedom to relabel the points of&lt;br /&gt;
spacetime. In &amp;lt;math&amp;gt;n&amp;lt;/math&amp;gt; dimensions that is &amp;lt;math&amp;gt;n&amp;lt;/math&amp;gt; arbitrary&lt;br /&gt;
functions, entering the transformation of the metric through their first&lt;br /&gt;
derivatives, so &amp;lt;math&amp;gt;\varrho=n&amp;lt;/math&amp;gt; and &amp;lt;math&amp;gt;\sigma=1&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
[[Noether&amp;#039;s theorems/Second theorem/The second theorem stated and proved|The&lt;br /&gt;
second theorem]] then returns, with no further input, exactly &amp;lt;math&amp;gt;n&amp;lt;/math&amp;gt;&lt;br /&gt;
identities among the Lagrange expressions of the gravitational action and their&lt;br /&gt;
first derivatives. In four dimensions, four.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;That number is a theorem, not an observation.&amp;#039;&amp;#039;&amp;#039; It was fixed the moment the&lt;br /&gt;
symmetry was named, before anything was computed about curvature.&lt;br /&gt;
&lt;br /&gt;
Noether states this case herself, in her first section, as one of two examples&lt;br /&gt;
given before any proof — the metric and a linear form subjected to the induced&lt;br /&gt;
transformations, and the known &amp;lt;math&amp;gt;n&amp;lt;/math&amp;gt; dependencies following.&lt;br /&gt;
&lt;br /&gt;
== The identity, not derived ==&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;UNVERIFIED.&amp;#039;&amp;#039;&amp;#039; The identities are stated in the literature to be the contracted&lt;br /&gt;
Bianchi identities: the divergence of the Einstein tensor vanishes identically,&lt;br /&gt;
which in index form is one relation for each free index, four in four dimensions.&lt;br /&gt;
Deriving that requires the Riemann tensor&amp;#039;s symmetries, which this volume does not&lt;br /&gt;
set up.&lt;br /&gt;
&lt;br /&gt;
== What the count buys without the identity ==&lt;br /&gt;
&lt;br /&gt;
Three consequences follow from the count alone.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Four of the ten field equations are not independent.&amp;#039;&amp;#039;&amp;#039; The count says so&lt;br /&gt;
directly, and this is the fact underlying the whole discussion on&lt;br /&gt;
[[Noether&amp;#039;s theorems/Second theorem/Fewer independent field equations than fields|the&lt;br /&gt;
counting page]].&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;The source must be divergence-free.&amp;#039;&amp;#039;&amp;#039; The field equations set a&lt;br /&gt;
divergence-free object equal to the matter&amp;#039;s energy and momentum, so the matter&amp;#039;s&lt;br /&gt;
energy and momentum must be divergence-free too, on pain of inconsistency. This is&lt;br /&gt;
the same structure as&lt;br /&gt;
[[Noether&amp;#039;s theorems/Applications/Electromagnetism and charge conservation|the&lt;br /&gt;
electromagnetic case]] and it is not a coincidence: both are the second theorem&amp;#039;s&lt;br /&gt;
identity forcing a conservation law on whatever is coupled.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Initial data does not determine the future.&amp;#039;&amp;#039;&amp;#039; Four functions&amp;#039; worth of any&lt;br /&gt;
solution is a choice of labels. That is what Hilbert had spelled out in 1916, and&lt;br /&gt;
[[Noether&amp;#039;s theorems/History/Hilbert and Klein|the history track]] gives the&lt;br /&gt;
sequence.&lt;br /&gt;
&lt;br /&gt;
== Who had it first ==&lt;br /&gt;
&lt;br /&gt;
Klein derived these identities in general form before Noether&amp;#039;s paper, by the&lt;br /&gt;
method of infinitesimal transformations. Hilbert had asserted them for a&lt;br /&gt;
particular case. Hilbert&amp;#039;s own 1924 reprint credits Klein with the general form&lt;br /&gt;
and Noether with the general proof of the theorem that has them as an instance.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;The four identities are not Noether&amp;#039;s discovery. The theorem is.&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;Provenance: the count is derived above from the second theorem. The&lt;br /&gt;
identification with the contracted Bianchi identities is flagged UNVERIFIED. The&lt;br /&gt;
priority account rests on Hilbert&amp;#039;s 1924 reprint, summarised from the secondary&lt;br /&gt;
literature and not reached in full text. Noether&amp;#039;s own example is read from the&lt;br /&gt;
public-domain German original. 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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