Rotating Black Holes in Higher Dimensions

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dc.creatorKleihaus, Burkhard
dc.creatorKunz, Jutta
dc.creatorNavarro-Lerida, Francisco
dc.date2007-10-11
dc.date2007-11-07
dc.date.accessioned2026-07-07T11:12:09Z
dc.date.available2026-07-07T11:12:09Z
dc.descriptionThe properties of higher-dimensional black holes can differ significantly from those of black holes in four dimensions, since neither the uniqueness theorem, nor the staticity theorem or the topological censorship theorem generalize to higher dimensions. We first discuss black holes of Einstein-Maxwell theory and Einstein-Maxwell-Chern-Simons theory with spherical horizon topology. Here new types of stationary black holes are encountered. We then discuss nonuniform black strings and present evidence for a horizon topology changing transition.
dc.descriptionSmall errors corrected
dc.identifierhttps://arxiv.org/abs/0710.2291
dc.identifierhttp://arxiv.org/abs/0710.2291
dc.identifierAIPConf.Proc.977:94-115,2008
dc.identifierdoi:10.1063/1.2902801
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191287
dc.subjectHigh Energy Physics - Theory
dc.titleRotating Black Holes in Higher Dimensions
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