Spherically symmetric spacetime: Difference between revisions

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:<math>\dim K(M) = 3</math>.
:<math>\dim K(M) = 3</math>.


It is known (see [[Birkhoff's theorem (relativity)|Birkhoff's theorem]]) that any spherically symmetric solution of the [[vacuum field equations]] is necessarily isometric to a subset of the maximally extended [[Schwarzschild solution]]. This means that the exterior region around a spherically symmetric gravitating object must be [[static]] and [[asymptotically flat]].
It is known (see [[Birkhoff's theorem (relativity)|Birkhoff's theorem]]) that any spherically symmetric solution of the [[vacuum field equations]] is necessarily isometric to a subset of the maximally extended [[Schwarzschild solution]]. This means that the exterior region around a spherically symmetric gravitating object must be [[static spacetime|static]] and [[asymptotically flat]].


== See also ==
== See also ==
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[[pt:Espaço-tempo esfericamente simétrico]]

Latest revision as of 11:27, 23 March 2013

A spherically symmetric spacetime is a spacetime whose isometry group contains a subgroup which is isomorphic to the (rotation) group and the orbits of this group are 2-dimensional spheres (2-spheres). The isometries are then interpreted as rotations and a spherically symmetric spacetime is often described as one whose metric is "invariant under rotations". The spacetime metric induces a metric on each orbit 2-sphere (and this induced metric must be a multiple of the metric of a 2-sphere).

Spherical symmetry is a characteristic feature of many solutions of Einstein's field equations of general relativity, especially the Schwarzschild solution. A spherically symmetric spacetime can be characterised in another way, namely, by using the notion of Killing vector fields, which, in a very precise sense, preserve the metric. The isometries referred to above are actually local flow diffeomorphisms of Killing vector fields and thus generate these vector fields. For a spherically symmetric spacetime , there are precisely 3 rotational Killing vector fields. Stated in another way, the dimension of the Killing algebra is 3

.

It is known (see Birkhoff's theorem) that any spherically symmetric solution of the vacuum field equations is necessarily isometric to a subset of the maximally extended Schwarzschild solution. This means that the exterior region around a spherically symmetric gravitating object must be static and asymptotically flat.

See also

References

  • {{#invoke:citation/CS1|citation

|CitationClass=book }} See Section 6.1 for a discussion of spherical symmetry.

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