Dynamics of null particles and shadow for general rotating black hole

被引:5
|
作者
Meng, Kun [1 ]
Fan, Xi-Long [2 ]
Li, Song [3 ,4 ]
Han, Wen-Biao [3 ,4 ,5 ,6 ]
Zhang, Hongsheng [7 ]
机构
[1] Weifang Univ, Sch Phys & Elect Informat, Weifang 261061, Peoples R China
[2] Wuhan Univ, Sch Phys & Technol, Wuhan 430072, Hubei, Peoples R China
[3] Shanghai Astron Observ, Shanghai 200030, Peoples R China
[4] Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China
[5] UCAS, Hangzhou Inst Adv Study, Sch Fundamental Phys & Math Sci, Hangzhou 310024, Peoples R China
[6] Int Ctr Theoret Phys Asia Pacific Beijing, Hangzhou, Peoples R China
[7] Univ Jinan, Sch Phys & Technol, Jinan, Peoples R China
基金
国家重点研发计划; 中国国家自然科学基金;
关键词
Black Holes; Classical Theories of Gravity; ACCRETION;
D O I
10.1007/JHEP11(2023)141
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
The Johannsen black hole (BH) is a generic rotating BH admitting three constants of motions (energy, angular momentum, and Carter constant) and is characterized by four deviation parameters besides mass and spin, which could be a model-independent probe of the no-hair theorem. We systematically study the dynamics of null particles around Johannsen BH, revealing the effects of the deviation parameters on the BH shadow as well as the effects of spin. By using the shadow boundaries of M87* and SgrA*, for the first time, the deviation parameters of those BHs are constrained. The detailed results depend on the spin a and inclination angle theta(0). Assuming a = 0.2 and theta(0) = 15 degrees, the deviation parameter alpha(13) are constained within similar to [-3.5, 6] for M87* observation and [-3, 0.5] for SgrA* observation. We also show the images of a Johannsen BH surrounded by a Page-Thorne thin accretion disk observed by a remote observer with a ray-tracing method and discuss the effects of the deviation parameters on deforming the accretion disk image, which could be tested by observations with higher sensitivities in the future.
引用
收藏
页数:28
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