Kerr-Gauss-Bonnet Black Holes: An Analytical Approximation

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dc.creatorAlexeyev, S.
dc.creatorPopov, N.
dc.creatorStartseva, M.
dc.creatorBarrau, A.
dc.creatorGrain, J.
dc.date2007-12-20
dc.date2008-04-17
dc.date.accessioned2026-07-07T11:39:36Z
dc.date.available2026-07-07T11:39:36Z
dc.descriptionGauss-Bonnet gravity provides one of the most promising frameworks to study curvature corrections to the Einstein action in supersymmetric string theories, while avoiding ghosts and keeping second order field equations. Although Schwarzschild-type solutions for Gauss-Bonnet black holes have been known for long, the Kerr-Gauss-Bonnet metric is missing. In this paper, a five dimensional Gauss-Bonnet approximation is analytically derived for spinning black holes and the related thermodynamical properties are briefly outlined.
dc.description5 pages, 1 figure
dc.identifierhttps://arxiv.org/abs/0712.3546
dc.identifierhttp://arxiv.org/abs/0712.3546
dc.identifierJ.Exp.Theor.Phys.106:709-713,2008
dc.identifierdoi:10.1134/S1063776108040092
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/199975
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleKerr-Gauss-Bonnet Black Holes: An Analytical Approximation
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