Shadow, quasinormal modes, and quasiperiodic oscillations of rotating Kaluza-Klein black holes

被引：64
|
作者：
Ghasemi-Nodehi, M. [1 ]
Azreg-Ainou, Mustapha [2 ]
Jusufi, Kimet [3 ,4 ]
Jamil, Mubasher [5 ,6 ,7 ]
机构：
[1] Inst Res Fundamental Sci IPM, Sch Astron, POB 19395-5531, Tehran, Iran
[2] Baskent Univ, Engn Fac, Baglica Campus, TR-06790 Ankara, Turkey
[3] State Univ Tetovo, Phys Dept, Ilinden St Nn, Tetovo 1200, North Macedonia
[4] Ss Cyril & Methodius Univ, Fac Nat Sci & Math, Inst Phys, Arhimedova 3, Skopje 1000, North Macedonia
[5] Zheijiang Univ Technol, Inst Theoret Phys & Cosmol, Hangzhou 310023, Peoples R China
[6] Natl Univ Sci & Technol NUST, Dept Math, Sch Nat Sci SNS, H-12, Islamabad 44000, Pakistan
[7] Canadian Quantum Res Ctr, 204-3002 32 Ave, Vernon, BC V1T 2L7, Canada
来源：
PHYSICAL REVIEW D | 2020年 / 102卷 / 10期
关键词：
GEODESIC MOTION; RESONANCE; STABILITY;
D O I：
10.1103/PhysRevD.102.104032
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In this paper we study the shadow of rotating Kaluza-Klein (KK) black holes and the connection between the shadow radius and the real part of quasinormal modes (QNMs) in the eiokonal limit. In addition we have explored the quasiperiodic oscillations (QPOs) in the rotating KK black hole.
引用
收藏
页数：16
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