Mechanics of higher-dimensional black holes in asymptotically anti-de Sitter space-times

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dc.creatorAshtekar, Abhay
dc.creatorPawlowski, Tomasz
dc.creatorBroeck, Chris Van Den
dc.date2006-11-07
dc.date2006-12-19
dc.date.accessioned2026-07-07T10:21:59Z
dc.date.available2026-07-07T10:21:59Z
dc.descriptionWe construct a covariant phase space for Einstein gravity in dimensions d>=4 with negative cosmological constant, describing black holes in local equilibrium. Thus, space-times under consideration are asymptotically anti-de Sitter and admit an inner boundary representing an isolated horizon. This allows us to derive a first law of black hole mechanics that involves only quantities defined quasi-locally at the horizon, without having to assume that the bulk space-time is stationary. The first law proposed by Gibbons et al. for the Kerr-AdS family follows from a special case of this much more general first law.
dc.descriptionRevtex4, 23 pages. Minor typos corrected and one reference added
dc.identifierhttps://arxiv.org/abs/gr-qc/0611049
dc.identifierhttp://arxiv.org/abs/gr-qc/0611049
dc.identifierClass.Quant.Grav.24:625-644,2007
dc.identifierdoi:10.1088/0264-9381/24/3/007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/175362
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleMechanics of higher-dimensional black holes in asymptotically anti-de Sitter space-times
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