Exact Gravitational Quasinormal Frequencies of Topological Black Holes

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dc.creatorBirmingham, Danny
dc.creatorMokhtari, Susan
dc.date2006-09-04
dc.date2006-09-18
dc.date.accessioned2026-07-07T10:26:03Z
dc.date.available2026-07-07T10:26:03Z
dc.descriptionWe compute the exact gravitational quasinormal frequencies for massless topological black holes in d-dimensional anti-de Sitter space. Using the gauge invariant formalism for gravitational perturbations derived by Kodama and Ishibashi, we show that in all cases the scalar, vector, and tensor modes can be reduced to a simple scalar field equation. This equation is exactly solvable in terms of hypergeometric functions, thus allowing an exact analytic determination of the gravitational quasinormal frequencies.
dc.description14 pages, Latex; v2 additional references
dc.identifierhttps://arxiv.org/abs/hep-th/0609028
dc.identifierhttp://arxiv.org/abs/hep-th/0609028
dc.identifierPhys.Rev.D74:084026,2006
dc.identifierdoi:10.1103/PhysRevD.74.084026
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/176748
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleExact Gravitational Quasinormal Frequencies of Topological Black Holes
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