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

被引：88

作者：

Cardoso, V ^{[1
]}

Lemos, JPS ^{[1
]}

机构：

[1] Univ Tecn Lisboa, Dept Fis, CENTRA, Inst Super Tecn, P-1096 Lisbon, Portugal

来源：

CLASSICAL AND QUANTUM GRAVITY | 2001年 / 18卷 / 23期

关键词：

D O I：

10.1088/0264-9381/18/23/319

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页码：5257 / 5267

页数：11

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