Formation of Topological Black holes from Gravitational Collapse

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dc.creatorSmith, W. L.
dc.creatorMann, R. B.
dc.date1997-03-04
dc.date1997-03-06
dc.date.accessioned2026-07-07T10:31:57Z
dc.date.available2026-07-07T10:31:57Z
dc.descriptionWe 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.
dc.descriptionlatex, 16 pages, four postscript figures
dc.identifierhttps://arxiv.org/abs/gr-qc/9703007
dc.identifierhttp://arxiv.org/abs/gr-qc/9703007
dc.identifierPhys.Rev.D56:4942-4947,1997
dc.identifierdoi:10.1103/PhysRevD.56.4942
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/178595
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleFormation of Topological Black holes from Gravitational Collapse
dc.typetext

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