Quasinormal modes and Hawking radiation of a Reissner-Nordstrom black hole surrounded by quintessence

被引：34

作者：

Saleh, Mahamat ^{[1
,3
]}

Bouetou, Bouetou Thomas ^{[2
,3
]}

Kofane, Timoleon Crepin ^{[3
]}

机构：

[1] Univ Maroua, Dept Phys, Higher Teachers Training Coll, Maroua, Cameroon

[2] Univ Yaounde I, Ecole Natl Super Polytech, Yaounde, Cameroon

[3] Univ Yaounde I, Dept Phys, Fac Sci, Yaounde, Cameroon

来源：

ASTROPHYSICS AND SPACE SCIENCE | 2011年 / 333卷 / 02期

关键词：

Quasinormal modes; Hawking radiation; WKB approximation; WKB APPROACH; CHARGED-PARTICLES;

D O I：

10.1007/s10509-011-0643-8

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We investigate quasinormal modes (QNMs) and Hawking radiation of a Reissner-Nordstrom black hole surrounded by quintessence. The Wentzel-Kramers-Brillouin (WKB) method is used to evaluate the QNMs and the rate of radiation. The results show that due to the interaction of the quintessence with the background metric, the QNMs of the black hole damp more slowly when increasing the density of quintessence and the black hole radiates at slower rate.

引用

页码：449 / 455

页数：7

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