Instability of the de Sitter Reissner-Nordstrom black hole in the 1/D expansion

被引:27
|
作者
Tanabe, Kentaro [1 ]
机构
[1] KEK, Inst Particles & Nucl Studies, Ctr Theory, Tsukuba, Ibaraki 3050801, Japan
关键词
classical gravity; black hole physics; perturbation analysis;
D O I
10.1088/0264-9381/33/12/125016
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the large D effective theory for D dimensional charged (Anti) de Sitter black holes. Then we show that the de Sitter Reissner-Nordstrom black hole becomes unstable against gravitational perturbations at larger charge than a critical charge in a higher dimension. Furthermore, we find that there is a nontrivial zero-mode static perturbation at the critical charge. The existence of static perturbations suggests the appearance of non-spherical symmetric solution branches of static charged de Sitter black holes. This expectation is confirmed by constructing the non-spherical symmetric static solutions of large D effective equations.
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收藏
页数:9
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