Black hole quasinormal modes using the asymptotic iteration method

被引：100
作者：
Cho, H. T. [1 ]
Cornell, A. S. [2 ]
Doukas, Jason [3 ]
Naylor, Wade [4 ,5 ]
机构：
[1] Tamkang Univ, Dept Phys, Taipei, Taiwan
[2] Univ Witwatersrand, Sch Phys, Natl Inst Theoret Phys, ZA-2050 Wits, South Africa
[3] Kyoto Univ, Yukawa Inst Theoret Phys, Kyoto 6068502, Japan
[4] Doshisha Univ, Dept Elect Engn, Kyoto 5103210, Japan
[5] Osaka Univ, Dept Phys, Osaka 5600043, Japan
来源：
CLASSICAL AND QUANTUM GRAVITY | 2010年 / 27卷 / 15期
基金：
日本学术振兴会;
关键词：
GENERIC SINGULARITIES;
D O I：
10.1088/0264-9381/27/15/155004
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In this paper we show that the asymptotic iteration method (AIM) allows one to numerically find the quasinormal modes of Schwarzschild and Schwarzschild de Sitter black holes. An added benefit of the method is that it can also be used to calculate the Schwarzschild anti-de Sitter quasinormal modes for the case of spin-zero perturbations. We also discuss an improved version of the AIM, more suitable for numerical implementation.
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页数：12
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