Quasinormal modes of Kerr black holes using a spectral decomposition of the metric perturbations

被引：11

作者：

Blazquez-Salcedo, Jose Luis ^{[1
,2
]}

Khoo, Fech Scen ^{[3
]}

Kunz, Jutta ^{[3
]}

Gonzalez-Romero, Luis Manuel ^{[1
,2
]}

机构：

[1] Univ Complutense Madrid, Fac Ciencias Fis, Dept Fis Teor, Madrid 28040, Spain

[2] Univ Complutense Madrid, Fac Ciencias Fis, IPARCOS, Madrid 28040, Spain

[3] Carl von Ossietzky Univ Oldenburg, Inst Phys, Postfach 2503, D-26111 Oldenburg, Germany

来源：

PHYSICAL REVIEW D | 2024年 / 109卷 / 06期

关键词：

FIELD;

D O I：

10.1103/PhysRevD.109.064028

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We report a new method to calculate the quasinormal modes of rotating black holes, using a spectral decomposition to solve the partial differential equations that result from introducing linear metric perturbations to a rotating background. Our approach allows us to calculate a large sector of the quasinormal mode spectrum. In particular, we study the accuracy of the method for the (l = 2)-led and (l = 3)-led modes for different values of the M(z )azimuthal number, considering the fundamental modes as well as the first two excitations. We show that our method reproduces the Kerr fundamental modes with an accuracy of 10(-6) or better for a/M < 0.8, while it stays below 0.1% for a/M < 0.98.

引用

页数：13

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