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Quasi-normal modes of toroidal, cylindrical and planar black holes in anti-de Sitter spacetimes: scalar, electromagnetic and gravitational perturbations

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arxiv gr-qc/0107098 v2 pith:QBL42CQX submitted 2001-07-30 gr-qc hep-th

Quasi-normal modes of toroidal, cylindrical and planar black holes in anti-de Sitter spacetimes: scalar, electromagnetic and gravitational perturbations

Vitor Cardoso , Jose' P. S. Lemos This is my paper
classification gr-qc hep-th
keywords blackanti-decorrespondingcylindricalelectromagneticfieldgravitationalholes
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We study the quasi-normal modes (QNM) of scalar, electromagnetic and gravitational perturbations of black holes in general relativity whose horizons have toroidal, cylindrical or planar topology in an asymptotically anti-de Sitter (AdS) spacetime. The associated quasinormal frequencies describe the decay in time of the corresponding test field in the vicinities of the black hole. In terms of the AdS/CFT conjecture, the inverse of the frequency is a measure of the dynamical timescale of approach to thermal equilibrium of the corresponding conformal field theory.

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Cited by 6 Pith papers

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