Quasi-Normal Modes of Gravitational Perturbation around a Reissner-Nordstrom Black Hole Surrounded by Quintessence

被引：13
|
作者：
Saleh, Mahamat [1 ]
Thomas, Bouetou Bouetou [1 ,2 ,3 ]
Kofane, Timoleon Crepin [1 ,3 ]
机构：
[1] Univ Yaounde I, Fac Sci, Dept Phys, Yaounde, Cameroon
[2] Univ Yaounde I, Ecole Natl Super Polytech, Yaounde, Cameroon
[3] Abdus Salam Int Ctr Theoret Phys, II-34014 Trieste, Italy
来源：
CHINESE PHYSICS LETTERS | 2009年 / 26卷 / 10期
关键词：
WKB APPROACH;
D O I：
10.1088/0256-307X/26/10/109802
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
We investigate quasi-normal (QN) modes of gravitational perturbation around a Reissner-Nordstrom black hole surrounded by quintessence. The third-order Wentzel-Kramers-Brillouin approximation is used to evaluate QN frequencies. The behavior of the gravitational perturbation is plotted for some frequencies. Due to the presence of quintessence, QN modes of the Reissner-Nordstrom black hole damp at a slower rate.
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页数：4
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