<?xml version="1.0"?>
<feed xmlns="http://www.w3.org/2005/Atom" xml:lang="en">
	<id>https://invarians.org/index.php?action=history&amp;feed=atom&amp;title=Noether%27s_theorems%2FSecond_theorem%2FProper_and_improper_conservation_laws</id>
	<title>Noether&#039;s theorems/Second theorem/Proper and improper conservation laws - Revision history</title>
	<link rel="self" type="application/atom+xml" href="https://invarians.org/index.php?action=history&amp;feed=atom&amp;title=Noether%27s_theorems%2FSecond_theorem%2FProper_and_improper_conservation_laws"/>
	<link rel="alternate" type="text/html" href="https://invarians.org/index.php?title=Noether%27s_theorems/Second_theorem/Proper_and_improper_conservation_laws&amp;action=history"/>
	<updated>2026-10-21T12:59:56Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
	<generator>MediaWiki 1.46.2</generator>
	<entry>
		<id>https://invarians.org/index.php?title=Noether%27s_theorems/Second_theorem/Proper_and_improper_conservation_laws&amp;diff=577&amp;oldid=prev</id>
		<title>BFP Rauch: 1 revision imported</title>
		<link rel="alternate" type="text/html" href="https://invarians.org/index.php?title=Noether%27s_theorems/Second_theorem/Proper_and_improper_conservation_laws&amp;diff=577&amp;oldid=prev"/>
		<updated>2026-09-10T13:29:56Z</updated>

		<summary type="html">&lt;p&gt;1 revision imported&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw-interface=&quot;&quot;&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;1&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;1&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 13:29, 10 September 2026&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-notice&quot; lang=&quot;en&quot;&gt;&lt;div class=&quot;mw-diff-empty&quot;&gt;(No difference)&lt;/div&gt;
&lt;/td&gt;&lt;/tr&gt;&lt;/table&gt;</summary>
		<author><name>BFP Rauch</name></author>
	</entry>
	<entry>
		<id>https://invarians.org/index.php?title=Noether%27s_theorems/Second_theorem/Proper_and_improper_conservation_laws&amp;diff=576&amp;oldid=prev</id>
		<title>NT&gt;NoetherVolumeBuild: Noether theorems volume, initial import (S-04)</title>
		<link rel="alternate" type="text/html" href="https://invarians.org/index.php?title=Noether%27s_theorems/Second_theorem/Proper_and_improper_conservation_laws&amp;diff=576&amp;oldid=prev"/>
		<updated>2026-09-10T00:00:00Z</updated>

		<summary type="html">&lt;p&gt;Noether theorems volume, initial import (S-04)&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{DISPLAYTITLE:Proper and improper conservation laws}}&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;Plain-language counterpart: [[Noether&amp;#039;s theorems/Explainers/A conservation law that is only wearing the costume|A conservation law that is only wearing the costume]].&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
This is her sixth section and the reason the paper was written. It answers a&lt;br /&gt;
claim of Hilbert&amp;#039;s, and it answers it with a biconditional.&lt;br /&gt;
&lt;br /&gt;
== The definition ==&lt;br /&gt;
&lt;br /&gt;
Let &amp;lt;math&amp;gt;I&amp;lt;/math&amp;gt; admit a &amp;lt;math&amp;gt;\mathfrak{G}_{\infty\varrho}&amp;lt;/math&amp;gt;, and let&lt;br /&gt;
&amp;lt;math&amp;gt;\mathfrak{G}_{\sigma}&amp;lt;/math&amp;gt; be any finite group arising by specialising&lt;br /&gt;
the arbitrary functions — a subgroup of the infinite one. The infinite group&lt;br /&gt;
gives dependencies (N16); the finite subgroup gives divergence relations (N13).&lt;br /&gt;
&lt;br /&gt;
The dependencies can be written&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\sum\psi_{i}a_{i}^{(\lambda)}=\mathrm{Div}\,\chi^{(\lambda)}\qquad\qquad\mathrm{(1)}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where the &amp;lt;math&amp;gt;\chi^{(\lambda)}&amp;lt;/math&amp;gt; are linear combinations of the Lagrange&lt;br /&gt;
expressions and their derivatives. Because the &amp;lt;math&amp;gt;\psi&amp;lt;/math&amp;gt; enter linearly&lt;br /&gt;
in both (N13) and (N16), the divergence relations must be linear combinations of&lt;br /&gt;
the dependencies, so&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\mathrm{Div}\,B^{(\lambda)}=\mathrm{Div}\left(\sum\alpha\cdot\chi^{(\lambda)}\right)\qquad\qquad\mathrm{(2)}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
and the &amp;lt;math&amp;gt;B^{(\lambda)}&amp;lt;/math&amp;gt; themselves compose linearly out of the&lt;br /&gt;
Lagrange expressions and their derivatives, together with functions whose&lt;br /&gt;
divergence vanishes identically — such as the &amp;lt;math&amp;gt;B-\Gamma&amp;lt;/math&amp;gt; obtained at&lt;br /&gt;
the end of the previous proof.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Divergence relations whose &amp;lt;math&amp;gt;B^{(\lambda)}&amp;lt;/math&amp;gt; can be composed in that&lt;br /&gt;
way Noether calls &amp;#039;&amp;#039;uneigentlich&amp;#039;&amp;#039;, improper. All others are &amp;#039;&amp;#039;eigentlich&amp;#039;&amp;#039;,&lt;br /&gt;
proper.&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
An improper conservation law is an identity wearing the costume of a&lt;br /&gt;
conservation law. Its conserved quantity is built from the field equations&lt;br /&gt;
themselves, so the statement that it is conserved carries no information the&lt;br /&gt;
field equations did not already carry.&lt;br /&gt;
&lt;br /&gt;
== The criterion, which is a biconditional ==&lt;br /&gt;
&lt;br /&gt;
Conversely, if the divergence relations are linear combinations of the&lt;br /&gt;
dependencies — that is, improper — then invariance under&lt;br /&gt;
&amp;lt;math&amp;gt;\mathfrak{G}_{\sigma}&amp;lt;/math&amp;gt; follows from invariance under&lt;br /&gt;
&amp;lt;math&amp;gt;\mathfrak{G}_{\infty\varrho}&amp;lt;/math&amp;gt;, and &amp;lt;math&amp;gt;\mathfrak{G}&amp;lt;/math&amp;gt; becomes&lt;br /&gt;
a subgroup of &amp;lt;math&amp;gt;\mathfrak{G}_{\infty\varrho}&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
Hence: &amp;#039;&amp;#039;&amp;#039;the divergence relations belonging to a finite group&lt;br /&gt;
&amp;lt;math&amp;gt;\mathfrak{G}_{\sigma}&amp;lt;/math&amp;gt; are improper if and only if&lt;br /&gt;
&amp;lt;math&amp;gt;\mathfrak{G}_{\sigma}&amp;lt;/math&amp;gt; is a subgroup of an infinite group with&lt;br /&gt;
respect to which &amp;lt;math&amp;gt;I&amp;lt;/math&amp;gt; is invariant.&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
The &amp;quot;if and only if&amp;quot; is Noether&amp;#039;s and it is the whole content. A one-directional&lt;br /&gt;
statement of this criterion is not a weaker version of it; it is a different and&lt;br /&gt;
much less useful claim.&lt;br /&gt;
&lt;br /&gt;
== Specialising to translations ==&lt;br /&gt;
&lt;br /&gt;
Let the translation group be&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;y_{i}=x_{i}+\varepsilon_{i};\qquad v_{i}(y)=u_{i}(x)\qquad\qquad\mathrm{(3)}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
so that&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\Delta x_{i}=\varepsilon_{i},\qquad\Delta u_{i}=0,\qquad\bar{\delta}u_{i}=-\sum_{\lambda}\frac{\partial u_{i}}{\partial x_{\lambda}}\varepsilon_{\lambda}\qquad\qquad\mathrm{(4)}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Invariance under this group says that the &amp;lt;math&amp;gt;x&amp;lt;/math&amp;gt; do not occur explicitly&lt;br /&gt;
in &amp;lt;math&amp;gt;f&amp;lt;/math&amp;gt;. The corresponding &amp;lt;math&amp;gt;n&amp;lt;/math&amp;gt; divergence relations&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\sum\psi_{i}\frac{\partial u_{i}}{\partial x_{\lambda}}=\mathrm{Div}\,B^{(\lambda)}\qquad(\lambda=1,2,\dots n)\qquad\qquad\mathrm{(5)}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Noether calls the &amp;#039;&amp;#039;&amp;#039;energy relations&amp;#039;&amp;#039;&amp;#039;, since the conservation laws&lt;br /&gt;
&amp;lt;math&amp;gt;\mathrm{Div}\,B^{(\lambda)}=0&amp;lt;/math&amp;gt; belonging to the variational problem&lt;br /&gt;
correspond to the energy theorems and the &amp;lt;math&amp;gt;B^{(\lambda)}&amp;lt;/math&amp;gt; to the&lt;br /&gt;
energy components.&lt;br /&gt;
&lt;br /&gt;
The criterion then reads: &amp;#039;&amp;#039;&amp;#039;if &amp;lt;math&amp;gt;I&amp;lt;/math&amp;gt; admits the translation group, the&lt;br /&gt;
energy relations are improper if and only if &amp;lt;math&amp;gt;I&amp;lt;/math&amp;gt; is invariant under an&lt;br /&gt;
infinite group containing the translation group as a subgroup.&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
Noether adds, in a footnote, that the energy theorems of classical mechanics and&lt;br /&gt;
of the old relativity theory are proper, since no infinite groups occur there.&lt;br /&gt;
That footnote is what makes the criterion a criterion rather than an observation:&lt;br /&gt;
it exhibits the other side of the biconditional.&lt;br /&gt;
&lt;br /&gt;
== Her worked example ==&lt;br /&gt;
&lt;br /&gt;
Not general relativity — a group she constructs precisely because it cannot be a&lt;br /&gt;
coefficient transformation, the logarithm seeing to that:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;y=x+p(x);\qquad v_{i}=u_{i}+\lg\left(1+p&amp;#039;(x)\right)=u_{i}+\lg\frac{dy}{dx}\qquad\qquad\mathrm{(6)}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\Delta x=p(x);\qquad\Delta u_{i}=p&amp;#039;(x);\qquad\bar{\delta}u_{i}=p&amp;#039;(x)-u&amp;#039;_{i}p(x)\qquad\qquad\mathrm{(7)}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The dependencies (N16) here become&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\sum_{i}\left(\psi_{i}u_{i}&amp;#039;+\frac{d\psi_{i}}{dx}\right)=0\qquad\qquad\mathrm{(8)}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
and the improper energy relations&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\sum\left(\psi_{i}u_{i}&amp;#039;+\frac{d\left(\psi_{i}+\mathrm{const.}\right)}{dx}\right)=0\qquad\qquad\mathrm{(9)}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
A simplest invariant integral of the group is&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;I=\int\frac{e^{-2u_{1}}}{u&amp;#039;_{1}-u&amp;#039;_{2}}dx\qquad\qquad\mathrm{(10)}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Why she chose this example rather than gravity.&amp;#039;&amp;#039;&amp;#039; It shows the phenomenon in&lt;br /&gt;
a case with nothing physical attached, which is exactly her point about what the&lt;br /&gt;
phenomenon depends on.&lt;br /&gt;
&lt;br /&gt;
== The remark that governs how the whole subject is read ==&lt;br /&gt;
&lt;br /&gt;
Noether closes by observing that for Hilbert&amp;#039;s assertion to hold literally, the&lt;br /&gt;
designation &amp;quot;general relativity&amp;quot; must be taken more broadly than usual, extended&lt;br /&gt;
to the groups depending on &amp;lt;math&amp;gt;n&amp;lt;/math&amp;gt; arbitrary functions treated above. And&lt;br /&gt;
she endorses Klein&amp;#039;s suggestion that the physicists&amp;#039; term &amp;#039;&amp;#039;Relativität&amp;#039;&amp;#039; would&lt;br /&gt;
be better replaced by invariance with respect to a group.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;The property is group-theoretic. General relativity is one theory that has it.&lt;br /&gt;
It is not the reason.&amp;#039;&amp;#039;&amp;#039; The consequences for gravitational energy are on&lt;br /&gt;
[[Noether&amp;#039;s theorems/Applications/General relativity and the energy question|their&lt;br /&gt;
own page]], which is downstream of this one and not the other way round.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;Provenance: the definitions, the criterion, the translation specialisation, the&lt;br /&gt;
footnote on classical mechanics, the worked example and the closing remark are&lt;br /&gt;
all Noether&amp;#039;s sixth section. Displays (1) to (10) are hers, set as running text in&lt;br /&gt;
the original and numbered here. Reproduced in her notation from the&lt;br /&gt;
public-domain German original; her prose is paraphrased. See&lt;br /&gt;
[[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>
</feed>