Quasinormal Modes of Massless Scalar Field Perturbation in Reissner-Nordström-de Sitter Quintessence Spacetime

被引：0
|
作者：
Zhong-Wen Feng
Guo-Ping Li
Xiao-Tao Zu
机构：
[1] University of Electronic Science and Technology of China,School of Physical Electronics
来源：
International Journal of Theoretical Physics | 2016年 / 55卷
关键词：
Quasinormal modes; RN-dSQ black hole; Scalar field perturbation; WKB approximation;
D O I：
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学科分类号：
摘要：
Using the WKB approximation method, the massless scalar quasinormal modes are studied in Reissner-Nordström-de Sitter quintessence spacetime. We analyze the effective potential and QNMs frequencies by varying angular harmonic index l, mass M, charge Q, quintessence energy b and cosmological constant L2. The results show the effective potential and QNMs frequency are related to l, M, Q, b and L2. Moreover, the b and L2 can make the effective potential and QNMs frequency reduces.
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页码：367 / 379
页数：12
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