Topological deformation of isolated horizons

dc.creatorLiko, Tomas
dc.date2007-05-10
dc.date2008-03-05
dc.date.accessioned2026-07-07T11:41:06Z
dc.date.available2026-07-07T11:41:06Z
dc.descriptionWe show that the Gauss-Bonnet term can have physical effects in four dimensions. Specifically, the entropy of a black hole acquires a correction that is proportional to the Euler characteristic of the cross sections of the horizon. While this term is constant for a single black hole, it will be a non-trivial function for a system with dynamical topologies such as black-hole mergers: it is shown that for certain values of the GB parameter, the second law of black-hole mechanics can be violated.
dc.description8 pages; 1 figure; v2: 9 pages; some comments added at the end; 3 references added; v3: minor corrections; v4: some corrections; discussion added on black-hole mergers and violations of the second law; 2 references added; v5: minor corrections; v6: final corrections to match PRD version
dc.identifierhttps://arxiv.org/abs/0705.1518
dc.identifierhttp://arxiv.org/abs/0705.1518
dc.identifierPhys.Rev.D77:064004,2008
dc.identifierdoi:10.1103/PhysRevD.77.064004
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/200421
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleTopological deformation of isolated horizons
dc.typetext

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