Quasinormal modes of a Schwarzschild black hole surrounded by free static spherically symmetric quintessence: electromagnetic perturbations

被引：68
|
作者：
Zhang, Yu [1 ]
Gui, Yuanxing
Yu, Fei
Li, FengLin
机构：
[1] Dalian Univ Technol, Sch Phys & Optoelect Technol, Dalian 116024, Peoples R China
[2] Chungnam Natl Univ, Dept Mat Sci & Engn, Taejon 305764, South Korea
来源：
GENERAL RELATIVITY AND GRAVITATION | 2007年 / 39卷 / 07期
基金：
中国国家自然科学基金;
关键词：
quasinormal modes; electromagnetic perturbation; WKB approximation;
D O I：
10.1007/s10714-007-0434-2
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In this paper, we evaluated the quasinormal modes of electromagnetic perturbation in a Schwarzschild black hole surrounded by the static spherically symmetric quintessence by using the third-order WKB approximation when the quintessential state parameter w(q) in the range of -1/3 < w(q) < 0. Due to the presence of quintessence, Maxwell field damps more slowly. And when at -1 < w(q) < -1/3, it is similar to the black hole solution in the ds/Ads spacetime. The appropriate boundary conditions need to be modified.
引用
收藏
页码：1003 / 1010
页数：8
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