Quasinormal Modes of Kerr Black Holes in Four and Higher Dimensions

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dc.creatorKao, Hsien-chung
dc.creatorTomino, Dan
dc.date2008-01-28
dc.date.accessioned2026-07-07T11:40:00Z
dc.date.available2026-07-07T11:40:00Z
dc.descriptionWe analytically calculate to leading order the asymptotic form of quasinormal frequencies of Kerr black holes in four, five and seven dimensions. All the relevant quantities can be explicitly expressed in terms of elliptical integrals. In four dimensions, we confirm the results obtained by Keshest and Hod by comparing the analytic results to the numerical ones.
dc.description14 pages, 7 figures
dc.identifierhttps://arxiv.org/abs/0801.4195
dc.identifierhttp://arxiv.org/abs/0801.4195
dc.identifierPhys.Rev.D77:127503,2008
dc.identifierdoi:10.1103/PhysRevD.77.127503
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/200124
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleQuasinormal Modes of Kerr Black Holes in Four and Higher Dimensions
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