Quasinormal modes of the Kerr-Newman black hole: GW150914 and fundamental physics implications

被引：8
|
作者：
Wang, Hai-Tian [1 ,2 ,3 ,4 ]
Tang, Shao-Peng [1 ,2 ]
Li, Peng-Cheng [5 ,6 ,7 ,8 ]
Fan, Yi-Zhong [1 ,2 ]
机构：
[1] Chinese Acad Sci, Purple Mt Observ, Nanjing 210023, Peoples R China
[2] Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Anhui, Peoples R China
[3] Sun Yat Sen Univ, TianQin Res Ctr Gravitat Phys, Zhuhai Campus, Zhuhai 519082, Peoples R China
[4] Sun Yat Sen Univ, Sch Phys & Astron, Zhuhai Campus, Zhuhai 519082, Peoples R China
[5] Peking Univ, Ctr High Energy Phys, 5 Yiheyuan Rd, Beijing 100871, Peoples R China
[6] Peking Univ, Dept Phys, 5 Yiheyuan Rd, Beijing 100871, Peoples R China
[7] Peking Univ, State Key Lab Nucl Phys & Technol, 5 Yiheyuan Rd, Beijing 100871, Peoples R China
[8] South China Univ Technol, Sch Phys & Optoelect, Guangzhou 510641, Peoples R China
来源：
PHYSICAL REVIEW D | 2021年 / 104卷 / 10期
基金：
中国博士后科学基金;
关键词：
GRAVITATIONAL-WAVES; EXTRACTION;
D O I：
10.1103/PhysRevD.104.104063
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We develop an analytical ringdown waveform model, including both the fundamental and the overtone quasinormal modes, for charged black holes and show that it is precise enough to analyze current gravitational wave data. Applying this waveform model to GW150914, the charge to mass ratio of the remnant black hole (lambda(f)) has been constrained with the sole ringdown gravitational wave data for the first time and the 90% upper limit is lambda(f) <= 0.38. Correspondingly, the deviation parameter of the scalar-tensor vector gravity (alpha(s)) is limited to be alpha(s) <= 0.17. Our approach can be directly applied to other binary black hole mergers with loud ringdown radiation.
引用
收藏
页数：7
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