Quasinormal modes of the (2+1)-dimensional Chern-Simons black hole via symmetry

被引：0

作者：

Avramov, V. ^{[1
]}

Rashkov, R. C. ^{[1
,2
]}

Vetsov, T. ^{[1
]}

机构：

[1] Sofia Univ, Dept Phys, 5 J Bourchier Blvd, Sofia 1164, Bulgaria

[2] Vienna Univ Technol, Inst Theoret Phys, Wiedner Hauptstr 8-10, A-1040 Vienna, Austria

来源：

INTERNATIONAL JOURNAL OF MODERN PHYSICS A | 2023年 / 38卷 / 32期

关键词：

Three-dimensional gravity models; black holes; quasinormal modes; lie algebra;

D O I：

10.1142/S0217751X23430091

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

In this study, we adopt an algebraic method to find the spectrum of quasinormal modes for the three-dimensional regular rotating Chern-Simons black hole solution. The latter is a solution to topologically massive gravitoelectrodynamics (TMGE). Due to the fact that the Chern-Simons black hole metric admits four local Killing vectors generating the sl(2, R) x R Lie algebra, the solutions to the equations of motion for the fields can be classified by the representations of this algebra. Subsequently, the quasinormal spectrum can be extracted as the infinite tower of descendants of the highest weight mode of sl(2, R).

引用

页数：9

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