Scalar perturbation of the higher-dimensional rotating black holes

被引：45

作者：

Ida, D ^{[1
]}

Uchida, Y

Morisawa, Y

机构：

[1] Tokyo Inst Technol, Dept Phys, Tokyo 1528550, Japan

[2] Osaka City Univ, Dept Phys, Osaka 5588585, Japan

来源：

PHYSICAL REVIEW D | 2003年 / 67卷 / 08期

关键词：

D O I：

10.1103/PhysRevD.67.084019

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The massless scalar field in the higher-dimensional Kerr black hole (Myers-Perry solution with a single rotation axis) has been investigated. It was shown that the field equation is separable in arbitrary dimensions. The quasinormal modes of the scalar field were searched in five dimensions using the continued fraction method. The numerical result shows evidence for the stability of the scalar perturbation of five-dimensional Kerr black holes. The time scale of the resonant oscillation in a rapidly rotating black hole, in which case the horizon radius becomes small, is characterized by (black hole mass)(1/2)(Planck mass)(-3/2) rather than the light-crossing time of the horizon.

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