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		<summary type="html">&lt;p&gt;&lt;a href=&quot;/index.php?title=En:WP:CLEANER&amp;amp;action=edit&amp;amp;redlink=1&quot; class=&quot;new&quot; title=&quot;En:WP:CLEANER (page does not exist)&quot;&gt;WPCleaner&lt;/a&gt; v1.14 - fix link&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;In the theory of [[smooth manifold]]s, a &amp;#039;&amp;#039;&amp;#039;congruence&amp;#039;&amp;#039;&amp;#039; is the set of [[integral curve]]s defined by a nonvanishing [[vector field]] defined on the manifold.  &lt;br /&gt;
&lt;br /&gt;
Congruences are an important concept in [[general relativity]], and are also important in parts of [[Riemannian geometry]].&lt;br /&gt;
&lt;br /&gt;
==A motivational example==&lt;br /&gt;
&lt;br /&gt;
The idea of a congruence is probably better explained by giving an example than by a definition.  Consider the smooth manifold &amp;#039;&amp;#039;&amp;#039;R&amp;#039;&amp;#039;&amp;#039;².  Vector fields can be specified as &amp;#039;&amp;#039;first order linear partial differential operators&amp;#039;&amp;#039;, such as &lt;br /&gt;
:&amp;lt;math&amp;gt;\vec{X} = ( x^2 - y^2 ) \, \partial_x + 2 \, x y \, \partial_y&amp;lt;/math&amp;gt;&lt;br /&gt;
These correspond to a system of &amp;#039;&amp;#039;first order linear ordinary differential equations&amp;#039;&amp;#039;, in this case&lt;br /&gt;
:&amp;lt;math&amp;gt;\dot{x} = x^2 - y^2,\; \dot{y} = 2 \, x y&amp;lt;/math&amp;gt;&lt;br /&gt;
where dot denotes a derivative with respect to some (dummy) parameter.  The solutions of such systems are &amp;#039;&amp;#039;families of parameterized curves&amp;#039;&amp;#039;, in this case&lt;br /&gt;
:&amp;lt;math&amp;gt; x(\lambda) = \frac{x_0 - (x_0^2+y_0^2) \, \lambda}{1 - 2 \, x_0 \, \lambda + (x_0^2 + y_0^2) \, \lambda^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
:&amp;lt;math&amp;gt; y(\lambda) = \frac{y_0}{1 - 2 \, x_0 \, \lambda + (x_0^2 + y_0^2) \, \lambda^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
This family is what is often called a &amp;#039;&amp;#039;congruence of curves&amp;#039;&amp;#039;, or just &amp;#039;&amp;#039;congruence&amp;#039;&amp;#039; for short.&lt;br /&gt;
&lt;br /&gt;
This particular example happens to have two &amp;#039;&amp;#039;singularities&amp;#039;&amp;#039;, where the vector field vanishes.  These are [[Fixed point (mathematics)|fixed point]]s of the &amp;#039;&amp;#039;flow&amp;#039;&amp;#039;. (A flow is a one dimensional group of [[diffeomorphism]]s; a flow defines an [[group action|action]] by the one dimensional [[Lie group]] &amp;#039;&amp;#039;&amp;#039;R&amp;#039;&amp;#039;&amp;#039;, having locally nice geometric properties.)  These two singularities correspond to two &amp;#039;&amp;#039;points&amp;#039;&amp;#039;, rather than two curves.  In this example, the other integral curves are all [[simple closed curve]]s.  Many flows are considerably more complicated than this.  To avoid complications arising from the presence of singularities, usually one requires the vector field to be &amp;#039;&amp;#039;nonvanishing&amp;#039;&amp;#039;.&lt;br /&gt;
&lt;br /&gt;
If we add more mathematical structure, our congruence may acquire new significance.&lt;br /&gt;
&lt;br /&gt;
==Congruences in Riemannian manifolds==&lt;br /&gt;
&lt;br /&gt;
For example, if we make our &amp;#039;&amp;#039;smooth manifold&amp;#039;&amp;#039; into a &amp;#039;&amp;#039;Riemannian manifold&amp;#039;&amp;#039; by adding a Riemannian [[metric tensor]], say the one defined by the line element&lt;br /&gt;
:&amp;lt;math&amp;gt;ds^2 = \left( \frac{2}{1 + x^2 + y^2} \right)^2 \, \left( dx^2 + dy^2 \right) &amp;lt;/math&amp;gt;&lt;br /&gt;
our congruence might become a &amp;#039;&amp;#039;geodesic congruence&amp;#039;&amp;#039;.  Indeed, in the example from the preceding section, our curves become [[geodesic]]s on an ordinary round sphere (with the North pole excised).  If we had added the standard Euclidean metric &amp;lt;math&amp;gt;ds^2 = dx^2 + dy^2&amp;lt;/math&amp;gt; instead, our curves would have become [[circle]]s, but not geodesics.&lt;br /&gt;
&lt;br /&gt;
An interesting example of a Riemannian geodesic congruence, related to our first example, is the [[Clifford congruence]] on P³, which is also known at the [[Hop pi bundle]] or &amp;#039;&amp;#039;Hop pi fibration&amp;#039;&amp;#039;.  The integral curves or fibers respectively are certain &amp;#039;&amp;#039;pairwise linked&amp;#039;&amp;#039; great circles, the [[orbit]]s in the space of unit norm [[quaternion]]s under left multiplication by a given unit quaternion of unit norm.&lt;br /&gt;
&lt;br /&gt;
==Congruences in Lorentzian manifolds==&lt;br /&gt;
&lt;br /&gt;
In a [[Lorentzian manifold]], such as a [[spacetime]] model in general relativity (which will usually be an [[exact solutions in general relativity|exact]] or approximate solution to the [[Einstein field equation]]), congruences are called &amp;#039;&amp;#039;timelike&amp;#039;&amp;#039;, &amp;#039;&amp;#039;null&amp;#039;&amp;#039;, or &amp;#039;&amp;#039;spacelike&amp;#039;&amp;#039; if the tangent vectors are everywhere timelike, null, or spacelike respectively.  A congruence is called a &amp;#039;&amp;#039;geodesic congruence&amp;#039;&amp;#039; if the tangent vector field &amp;lt;math&amp;gt;\vec{X}&amp;lt;/math&amp;gt; has vanishing [[covariant derivative]], &amp;lt;math&amp;gt;\nabla_{\vec{X}} \vec{X} = 0&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
&lt;br /&gt;
*[[congruence (general relativity)]]&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
&lt;br /&gt;
*{{cite book | author=Lee, John M. | title=Introduction to smooth manifolds | location=New York | publisher=Springer | year=2003 | isbn=0-387-95448-1}}  A textbook on manifold theory.  See also the same author&amp;#039;s textbooks on topological manifolds (a lower level of structure) and Riemannian geometry (a higher level of structure).&lt;br /&gt;
&lt;br /&gt;
[[Category:Differential topology]]&lt;/div&gt;</summary>
		<author><name>en&gt;Niceguyedc</name></author>
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