Quasinormal modes for the Vaidya metric in asymptotically anti-de Sitter spacetime

被引：17
作者：
Lin, Kai [1 ,2 ]
Liu, Yunqi [3 ]
Qian, Wei-Liang [2 ,3 ,4 ]
Wang, Bin [3 ,5 ]
Abdalla, Elcio [6 ]
机构：
[1] China Univ Geosci, Inst Geophys & Geomat, Hubei Subsurface Multiscale Imaging Key Lab, Wuhan 430074, Hubei, Peoples R China
[2] Univ Sao Paulo, Escola Engn Lorena, BR-12602810 Lorena, SP, Brazil
[3] Yangzhou Univ, Sch Phys Sci & Technol, Ctr Gravitat & Cosmol, Yangzhou 225002, Jiangsu, Peoples R China
[4] Univ Estadual Paulista, Fac Engn Guaratingueta, BR-12516410 Guaratingueta, SP, Brazil
[5] Shanghai Jiao Tong Univ, Sch Aeronaut & Astronaut, Shanghai 200240, Peoples R China
[6] Univ Sao Paulo, Inst Fis, BR-05315970 Sao Paulo, SP, Brazil
来源：
PHYSICAL REVIEW D | 2019年 / 100卷 / 06期
基金：
巴西圣保罗研究基金会; 中国国家自然科学基金;
关键词：
LATE-TIME BEHAVIOR; HOLE NORMAL-MODES; BLACK-HOLES; STELLAR COLLAPSE; EXPLOSIONS;
D O I：
10.1103/PhysRevD.100.065018
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In this work, we present a numerical scheme to study the quasinormal modes of the time-dependent Vaidya black hole metric in asymptotically anti-de Sitter spacetime. The proposed algorithm is primarily based on a generalized matrix method for quasinormal modes. The main feature of the present approach is that the quasinormal frequency, as a function of time, is obtained by a generalized secular equation and therefore a satisfactory degree of precision is achieved. The implications of the results are discussed.
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页数：9
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