Quasinormal modes of Reissner-Nordstrom Anti-de Sitter black holes

被引：158
|
作者：
Wang, B
Lin, CY
Abdalla, E
机构：
[1] Univ Sao Paulo, Inst Fis, BR-05315970 Sao Paulo, Brazil
[2] Shandong Teachers Univ, Dept Phys, Shanghai, Peoples R China
来源：
PHYSICS LETTERS B | 2000年 / 481卷 / 01期
基金：
巴西圣保罗研究基金会;
关键词：
D O I：
10.1016/S0370-2693(00)00409-3
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Complex frequencies associated with quasinormal modes for large Reissner-Nordstrom Anti-de Sitter black holes have been computed. These frequencies have close relation to the black hole charge and do not linearly scale with the black hole temperature as in Schwarzschild Anti-de Sitter case. In terms of AdS/CFT correspondence, we found that the bigger the black hole charge is, the quicker for the approach to thermal equilibrium in the CFT. The properties of quasinormal modes for l > 0 have also been studied. (C) 2000 Elsevier Science B.V. All rights reserved.
引用
收藏
页码：79 / 88
页数：10
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