Formation of Topological Black holes from Gravitational Collapse

Details Formation of Topological Black holes from Gravitational Collapse Formation of Topological Black holes from Gravitational Collapse

1997-03-04

arxiv.org/abs/gr-qc/9703007v2

Phys.Rev.D56:4942-4947,1997

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

latex, 16 pages, four postscript figures

Scientific paper

10.1103/PhysRevD.56.4942

We consider the gravitational collapse of a dust cloud in an asymptotically anti de Sitter spacetime in which points connected by a discrete subgroup of an isometry subgroup of anti de Sitter spacetime are identified. We find that black holes with event horizons of any topology can form from the collapse of such a cloud. The quasilocal mass parameter of such black holes is proportional to the initial density, which can be arbitrarily small.

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