Anti-de Sitter Quotients, Bubbles of Nothing, and Black Holes

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dc.creatorAman, Jan E.
dc.creatorAminneborg, Stefan
dc.creatorBengtsson, Ingemar
dc.creatorPidokrajt, Narit
dc.date2008-01-28
dc.date2008-02-20
dc.date.accessioned2026-07-07T12:14:10Z
dc.date.available2026-07-07T12:14:10Z
dc.descriptionIn 3+1 dimensions there are anti-de quotients which are black holes with toroidal event horizons. By analytic continuation of the Schwarzschild-anti-de Sitter solution (and appropriate identifications) one finds two one parameter families of spacetimes that contain these quotient black holes. One of these families consists of B-metrics ("bubbles of nothing"), the other of black hole spacetimes. All of them have vanishing conserved charges.
dc.description14 pages, 3 figures. References added, one explanation improved
dc.identifierhttps://arxiv.org/abs/0801.4214
dc.identifierhttp://arxiv.org/abs/0801.4214
dc.identifierGen.Rel.Grav.40:2557-2567,2008
dc.identifierdoi:10.1007/s10714-008-0639-z
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/211098
dc.subjectHigh Energy Physics - Theory
dc.titleAnti-de Sitter Quotients, Bubbles of Nothing, and Black Holes
dc.typetext

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