Quasinormal modes and hidden conformal symmetry in the Reissner-Nordstrom black hole

被引：16
|
作者：
Kim, Yong-Wan [1 ]
Myung, Yun Soo [2 ,3 ]
Park, Young-Jai [1 ,4 ,5 ]
机构：
[1] Sogang Univ, Ctr Quantum Spacetime, Seoul 121742, South Korea
[2] Inje Univ, Inst Basic Sci, Gimhae 621749, South Korea
[3] Inje Univ, Sch Comp Aided Sci, Gimhae 621749, South Korea
[4] Sogang Univ, Dept Phys, Seoul 121742, South Korea
[5] Sogang Univ, Dept Global Serv Management, Seoul 121742, South Korea
来源：
EUROPEAN PHYSICAL JOURNAL C | 2013年 / 73卷 / 05期
基金：
新加坡国家研究基金会;
关键词：
Black Hole; Event Horizon; Gordon Equation; Quasinormal Mode; Scalar Perturbation;
D O I：
10.1140/epjc/s10052-013-2440-8
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：
It is shown that the scalar wave equation in the near-horizon limit respects a hidden SL(2, R) invariance in the Reissner-Nordstrom (RN) black hole spacetimes. We use the SL(2, R) symmetry to determine algebraically the purely imaginary quasinormal frequencies of the RN black hole. We confirm that these are exactly quasinormal modes of scalar perturbation around the near-horizon region of a near-extremal black hole.
引用
收藏
页码：1 / 7
页数：7
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