Quasinormal modes of a massless Dirac field in de Rham-Gabadadze-Tolley massive gravity

被引：10
作者：
Wongjun, Pitayuth [1 ,2 ]
Chen, Chun-Hung [1 ]
Nakarachinda, Ratchaphat [1 ,2 ]
机构：
[1] Naresuan Univ, Inst Fundamental Study, Phitsanulok 65000, Thailand
[2] Minist Higher Educ Sci Res & Innovat, Thailand Ctr Excellence Phys, 328 Si Ayutthaya Rd, Bangkok 10400, Thailand
来源：
PHYSICAL REVIEW D | 2020年 / 101卷 / 12期
关键词：
TIME-PERIODIC SOLUTIONS; HOLE NORMAL-MODES; BLACK-HOLES; STELLAR COLLAPSE; NONEXISTENCE; EQUATION; PERTURBATIONS; EXPLOSIONS; STABILITY; BEHAVIOR;
D O I：
10.1103/PhysRevD.101.124033
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The quasinormal modes of a massless Dirac field in the de Rham-Gabadadze-Tolley (dRGT) massive gravity theory with asymptotically de Sitter spacetime are investigated using the Wentzel-Kramers-Brillouin approximation. The effective potential for the massless Dirac field due to the dRGT black hole is derived. It is found that the shape of the potential depends crucially on the structure of the graviton mass and the behavior of the quasinormal modes is controlled by the graviton mass parameters. Higher potentials give stronger damping of the quasinormal modes. We compare our results to the Schwarzschild-de Sitter case. Our numerical calculations are checked using Pade approximation and found that the quasinormal mode frequencies converge to ones with reasonable accuracy.
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页数：18
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