Quasinormal modes of quantum corrected black hole in the non-Ricci-flat spacetime perturbation

被引:1
|
作者
Zhang, C. [1 ]
Guo, W. [1 ]
Yan, Z. [2 ,3 ]
Zhang, X. [1 ]
机构
[1] Univ Shanghai Sci & Technol, Coll Sci, Shanghai 200093, Peoples R China
[2] Fudan Univ, Dept Phys, Shanghai 200433, Peoples R China
[3] Fudan Univ, Ctr Field Theory & Particle Phys, Shanghai 200433, Peoples R China
基金
中国国家自然科学基金;
关键词
Quasinormal modes; Quantum corrected black hole; Non-Ricci-flat spacetime; SCALAR FIELD; MATTER;
D O I
10.1007/s12648-022-02389-x
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We investigate the quasinormal modes (QNMs) of non-Ricci-flat quantum corrected black hole spacetime. We calculated the case of higher multipole l compared to Konoplya's work (Phys Lett B 804:135363, 2020). Because it is very difficult for Wentzel-Kramers-Brillouin method to calculate, we use Mashhoon (Poschl-Teller) method and asymptotic iteration method (AIM) to calculate the QNMs of quantum corrected black hole, and obtain the numerical results. We conclude that AIM takes less time to calculate and can ensure accuracy. In addition, we supplement the time-domain profiles that is not shown in Konoplya's work.
引用
收藏
页码:623 / 629
页数:7
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