Supersymmetry of Anti-de Sitter Black Holes

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dc.creatorCaldarelli, Marco M.
dc.creatorKlemm, Dietmar
dc.date1998-08-17
dc.date1999-01-18
dc.date.accessioned2026-07-07T11:36:16Z
dc.date.available2026-07-07T11:36:16Z
dc.descriptionWe examine supersymmetry of four-dimensional asymptotically anti-de Sitter (AdS) dyonic black holes in the context of gauged N=2 supergravity. Our calculations concentrate on black holes with unusual topology and their rotating generalizations, but we also reconsider the spherical rotating dyonic Kerr-Newman-AdS black hole, whose supersymmetry properties have previously been investigated by Kostelecký and Perry within another approach. We find that in the case of spherical, toroidal or cylindrical event horizon topology, the black holes must rotate in order to preserve some supersymmetry; the non-rotating supersymmetric configurations representing naked singularities. However, we show that this is no more true for black holes whose event horizons are Riemann surfaces of genus $g>1$, where we find a nonrotating extremal solitonic black hole carrying magnetic charge and permitting one Killing spinor. For the nonrotating supersymmetric configurations of various topologies, all Killing spinors are explicitly constructed.
dc.description27 pages, revtex, no figures. Minor errors corrected. Final version to appear in Nucl. Phys. B
dc.identifierhttps://arxiv.org/abs/hep-th/9808097
dc.identifierhttp://arxiv.org/abs/hep-th/9808097
dc.identifierNucl.Phys.B545:434-460,1999
dc.identifierdoi:10.1016/S0550-3213(98)00846-3
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/198862
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSupersymmetry of Anti-de Sitter Black Holes
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