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
相关论文
共 50 条
  • [21] Black hole shadow in a general rotating spacetime obtained through Newman-Janis algorithm
    Shaikh, Rajibul
    PHYSICAL REVIEW D, 2019, 100 (02)
  • [22] A GENERAL RELATIVISTIC NULL HYPOTHESIS TEST WITH EVENT HORIZON TELESCOPE OBSERVATIONS OF THE BLACK HOLE SHADOW IN Sgr A*
    Psaltis, Dimitrios
    Oezel, Feryal
    Chan, Chi-Kwan
    Marrone, Daniel P.
    ASTROPHYSICAL JOURNAL, 2015, 814 (02):
  • [23] Black hole shadow of a rotating polytropic black hole by the Newman–Janis algorithm without complexification
    Ernesto Contreras
    J. M. Ramirez–Velasquez
    Ángel Rincón
    Grigoris Panotopoulos
    Pedro Bargueño
    The European Physical Journal C, 2019, 79
  • [24] Influence of an anisotropic matter field on the shadow of a rotating black hole
    Badia, Javier
    Eiroa, Ernesto F.
    PHYSICAL REVIEW D, 2020, 102 (02)
  • [25] Shadow and quasinormal modes of a rotating loop quantum black hole
    Liu, Cheng
    Zhu, Tao
    Wu, Qiang
    Jusufi, Kimet
    Jamil, Mubasher
    Azreg-Aïnou, Mustapha
    Wang, Anzhong
    arXiv, 2020,
  • [26] Shadow and quasinormal modes of a rotating loop quantum black hole
    Liu, Cheng
    Zhu, Tao
    Wu, Qiang
    Jusufi, Kimet
    Jamil, Mubasher
    Azreg-Ainou, Mustapha
    Wang, Anzhong
    PHYSICAL REVIEW D, 2020, 101 (08)
  • [27] Shadow of rotating Hořava-Lifshitz black hole
    Farruh Atamurotov
    Ahmadjon Abdujabbarov
    Bobomurat Ahmedov
    Astrophysics and Space Science, 2013, 348 : 179 - 188
  • [28] Shadow of a rotating squashed Kaluza-Klein black hole
    Fen Long
    Jieci Wang
    Songbai Chen
    Jiliang Jing
    Journal of High Energy Physics, 2019
  • [29] Shadow of a charged rotating black hole in f(R) gravity
    Sara Dastan
    Reza Saffari
    Saheb Soroushfar
    The European Physical Journal Plus, 137
  • [30] Shadow of a rotating squashed Kaluza-Klein black hole
    Long, Fen
    Wang, Jieci
    Chen, Songbai
    Jing, Jiliang
    JOURNAL OF HIGH ENERGY PHYSICS, 2019, 2019 (10)