Shadow of the 5D Reissner-Nordstrom AdS black hole

被引:15
|
作者
Mandal, Surajit [1 ]
Upadhyay, Sudhaker [2 ,3 ,6 ]
Myrzakulov, Yerlan [4 ,5 ]
Yergaliyeva, Gulmira [4 ,5 ]
机构
[1] Jadavpur Univ, Dept Phys, Kolkata 700032, W Bengal, India
[2] Magadh Univ, KLS Coll, Dept Phys, Nawada 805110, Bihar, India
[3] Damghan Univ, Sch Phys, Damghan 3671641167, Iran
[4] LN Gumilyov Eurasian Natl Univ, Dept Gen & Theoret Phys, Astana 010008, Kazakhstan
[5] Ratbay Myrzakulov Eurasian Int Ctr Theoret Phys, Astana 010009, Kazakhstan
[6] IUCAA Pune, Pune 411007, Maharashtra, India
来源
关键词
Black hole shadow; RN AdS(5) black hole; plasma medium; energy emission rate; FIELD; CAST;
D O I
10.1142/S0217751X23500471
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
In this paper, we discuss the shadow cast by the charged Reissner-Nordstrom (RN) anti-de Sitter (AdS) black hole. With the help of the Killing equation and Hamilton-Jacobi equation, we calculate the geodesic equations for null particles. With the help of geodesics of null particle, we then determine the celestial coordinates (alpha, beta) and the shadow radius of the RN AdS black hole. We present a graphical analysis of the black hole shadow and find that shadow is a perfectly dark circle. The impacts of charge and cosmological constant of the RN AdS black hole on the radius of shadow are also presented. In this connection, the radius of the shadow is a decreasing function of the charge. Furthermore, we study the effects of plasma medium on the RN AdS black hole shadow. Here, we find that radius of circular shadow increases with increasing plasma parameter. We study the shadow radius for the constrained values of charge and cosmological constant from the M87(star) and Sgr A(star) black holes. In addition, we also discuss the energy emission the rate of RN black hole. The effects of parameters like charge, cosmological constant and plasma parameter on energy emission rate are analyzed graphically.
引用
收藏
页数:26
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