Stability of Reissner-Nordstrom black hole in de Sitter background under charged scalar perturbation

被引：72

作者：

Zhu, Zhiying ^{[1
,2
]}

Zhang, Shao-Jun ^{[1
]}

Pellicer, C. E. ^{[3
]}

Wang, Bin ^{[1
]}

Abdalla, Elcio ^{[4
]}

机构：

[1] Shanghai Jiao Tong Univ, Dept Phys & Astron, Shanghai 200240, Peoples R China

[2] Changsha Univ Sci & Technol, Dept Phys & Elect Sci, Changsha 410076, Hunan, Peoples R China

[3] Univ Fed Rio Grande do Norte, Escola Ciencias & Tecnol, BR-59072970 Natal, RN, Brazil

[4] Univ Sao Paulo, Inst Fis, BR-05315970 Sao Paulo, Brazil

来源：

PHYSICAL REVIEW D | 2014年 / 90卷 / 04期

基金：

中国博士后科学基金; 巴西圣保罗研究基金会; 中国国家自然科学基金;

关键词：

QUASI-NORMAL MODES; P-BRANES; ASTROPHYSICS; STRINGS; SPACE;

D O I：

10.1103/PhysRevD.90.044042

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We find a new instability in the four-dimensional Reissner-Nordstrom-de Sitter black holes against charged scalar perturbations with vanishing angular momentum, l = 0. We show that such an instability is caused by superradiance. The instability does not occur for a larger angular index, as explicitly proved for l = 1. Our results are obtained from a numerical investigation of the time-domain profiles of the perturbations.

引用

页数：9

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