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	<entry>
		<id>https://en.formulasearchengine.com/index.php?title=Perturbative_QCD&amp;diff=9909</id>
		<title>Perturbative QCD</title>
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		<updated>2013-11-12T13:37:21Z</updated>

		<summary type="html">&lt;p&gt;87.167.229.70: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;A &#039;&#039;&#039;homothetic vector field&#039;&#039;&#039; (sometimes &#039;&#039;&#039;homothetic collineation&#039;&#039;&#039; or &#039;&#039;&#039;homothety&#039;&#039;&#039;) is a [[projective vector field]] which satisfies the condition:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\mathcal{L}_X g_{ab}=2c g_{ab}&amp;lt;/math&amp;gt; &lt;br /&gt;
&lt;br /&gt;
where c is a real constant. Homothetic vector fields find application in the study of [[gravitational singularity|singularities]] in general relativity, also it can be used to generate new solutions for Einstein equations by similarity reduction.&amp;lt;ref&amp;gt;{{cite book|title=Exact Solutions of Einstein’s Field Equations|publisher=Cambridge  University  Press|isbn=978-0-521-46136-8|pages=163}}&amp;lt;/ref&amp;gt; &lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
&lt;br /&gt;
* [[Affine vector field]]&lt;br /&gt;
* [[Curvature collineation]]&lt;br /&gt;
* [[Killing vector field]]&lt;br /&gt;
* [[Matter collineation]]&lt;br /&gt;
* [[Spacetime symmetries]]&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
&lt;br /&gt;
{{relativity-stub}}&lt;br /&gt;
[[Category:Mathematical methods in general relativity]]&lt;/div&gt;</summary>
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