Topology of Event Horizons and Topological Censorship
arXiv:gr-qc/9410023 · doi:10.1088/0264-9381/12/4/012
Abstract
We prove that, under certain conditions, the topology of the event horizon of a four dimensional asymptotically flat black hole spacetime must be a 2-sphere. No stationarity assumption is made. However, in order for the theorem to apply, the horizon topology must be unchanging for long enough to admit a certain kind of cross section. We expect this condition is generically satisfied if the topology is unchanging for much longer than the light-crossing time of the black hole. More precisely, let be a four dimensional asymptotically flat spacetime satisfying the averaged null energy condition, and suppose that the domain of outer communication $\C_K$ to the future of a cut of $\Sm$ is globally hyperbolic. Suppose further that a Cauchy surface for $\C_K$ is a topological 3-manifold with compact boundary in , and is a compact submanifold of $\bS$ with spherical boundary in (and possibly other boundary components in ). Then we prove that the homology group must be finite. This implies that either consists of a disjoint union of 2-spheres, or is nonorientable and contains a projective plane. Further, $\partial§=\partial\Ip[K]\cap\partial\Im[\Sp]$, and will be a cross section of the horizon as long as no generator of $\partial\Ip[K]$ becomes a generator of $\partial\Im[\Sp]$. In this case, if is orientable, the horizon cross section must consist of a disjoint union of 2-spheres.}
11 pages, plain latex (minor revision: replaced by its closure in various places.)
References in corpus (2)
Cited by in corpus (57)
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