Quasi-normal Modes of Toroidal, Cylindrical and Planar Black Holes in Anti-de Sitter Spacetimes: Scalar, Electromagnetic and Gravitational Perturbations
نویسندگان
چکیده
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 QNM 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.
منابع مشابه
Quasi-normal Modes of Toroidal, Cylindrical and Planar Black Holes in Anti-de Sitter Spacetimes
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 th...
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تاریخ انتشار 2008