Semi-analytic expressions for quasinormal modes of slowly rotating Kerr black holes

被引:16
作者
Hatsuda, Yasuyuki [1 ]
Kimura, Masashi [1 ]
机构
[1] Rikkyo Univ, Dept Phys, Tokyo 1718501, Japan
来源
PHYSICAL REVIEW D | 2020年 / 102卷 / 04期
关键词
GRAVITATIONAL-RADIATION; EQUATIONS; PERTURBATIONS;
D O I
10.1103/PhysRevD.102.044032
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We provide semi-analytic expressions for quasinormal mode frequencies of slowly rotating Kerr black holes to the quadratic order in the rotation parameter. We apply the parametrized black hole quasinormal mode ringdown formalism to the Chandrasekhar-Detweiler equation and the Sasaki-Nakamura equation instead of the Teukolsky equation, and compare our result with the previous numerical calculations.
引用
收藏
页数:11
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