Supersymmetric isolated horizons in ADS spacetime

dc.creatorBooth, Ivan
dc.creatorLiko, Tomas
dc.date2008-08-06
dc.date2008-10-13
dc.date.accessioned2026-07-07T12:15:11Z
dc.date.available2026-07-07T12:15:11Z
dc.descriptionWe discuss various physical aspects of nonextremal, extremal and supersymmetric black holes in asymptotically anti-de Sitter (ADS) spacetimes. Specifically, we discuss how the isolated horizon (IH) framework leads to an ambiguity-free description of rotating black holes in these spacetimes. We then apply this framework to investigate the properties of supersymmetric isolated horizons (SIHs) in four-dimensional N = 2 gauged supergravity. Among other results we find that they are necessarily extremal, that rotating SIHs must have non-trivial electromagnetic fields, and that non-rotating SIHs necessarily have constant curvature horizon cross sections and a magnetic (though not electric) charge.
dc.description15 pages, 1 figure; v2: two references added; minor corrections; to appear in Physics Letters B
dc.identifierhttps://arxiv.org/abs/0808.0905
dc.identifierhttp://arxiv.org/abs/0808.0905
dc.identifierPhys.Lett.B670:61-66,2008
dc.identifierdoi:10.1016/j.physletb.2008.10.020
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/211429
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleSupersymmetric isolated horizons in ADS spacetime
dc.typetext

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