Horizon instability of massless scalar perturbations of an extreme Reissner-Nordstrom-AdS black hole

被引：12
|
作者：
Zhang, Shao-Jun [1 ]
Pan, Qiyuan [2 ,3 ]
Wang, Bin [1 ]
Abdalla, Elcio [4 ]
机构：
[1] Shanghai Jiao Tong Univ, Dept Phys & Astron, Shanghai 200240, Peoples R China
[2] Hunan Normal Univ, Inst Phys, Changsha 410081, Hunan, Peoples R China
[3] Hunan Normal Univ, Dept Phys, Changsha 410081, Hunan, Peoples R China
[4] Univ Sao Paulo, Inst Fis, BR-05315970 Sao Paulo, Brazil
来源：
JOURNAL OF HIGH ENERGY PHYSICS | 2013年 / 09期
基金：
中国国家自然科学基金; 巴西圣保罗研究基金会;
关键词：
Black Holes; Classical Theories of Gravity; LATE-TIME BEHAVIOR; QUASI-NORMAL MODES; STELLAR COLLAPSE; EXPLOSIONS; EVOLUTION;
D O I：
10.1007/JHEP09(2013)101
中图分类号：
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号：
摘要：
We study the stability of extreme Reissner-Nordstrom-AdS black hole under massless scalar perturbations. We show that the perturbation on the horizon of the extreme Reissner-Nordstrom-AdS black hole experiences a power-law decay, instead of an exponential decay as observed in the nonextreme AdS black hole. On the horizon of the extreme Reissner-Nordstrom-AdS black hole, the blow up happens at lower order derivative of the scalar field compared with that of the extreme Reissner-Nordstrom black hole, which shows that extreme AdS black holes tend to instability in comparison to black holes in asymptotic flat space-times.
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收藏
页数：18
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