Shadow cast and deflection of light by charged rotating regular black holes

被引:132
作者
Kumar, Rahul [1 ]
Ghosh, Sushant G. [1 ,2 ]
Wang, Anzhong [3 ,4 ]
机构
[1] Jamia Millia Islamia, Ctr Theoret Phys, New Delhi 110025, India
[2] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, Private Bag 54001, ZA-4000 Durban, South Africa
[3] Baylor Univ, Dept Phys, GCAP CASPER, Waco, TX 76798 USA
[4] Zhejiang Univ Technol, Inst Theoret Phys & Cosmol, Hangzhou 310032, Zhejiang, Peoples R China
基金
中国国家自然科学基金;
关键词
GRAVITATIONAL COLLAPSE; SINGULARITIES; FIELD; MASS;
D O I
10.1103/PhysRevD.100.124024
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss the horizon properties, shadow cast, and the weak gravitational lensing of charged rotating regular black holes, which in addition to mass (M) and rotation parameter (a) have an electric charge (Q) and magnetic charge (g). The considered regular black holes are the generalization of the Kerr (Q = g = 0) and Kerr-Newman (g 1/4 0) black holes. Interestingly, for a given parameter set, the apparent size of the shadow monotonically decreases and the shadow gets more distorted with increasing charge parameter Q. We put constraints on the black hole parameters with the aid of recent M87* shadow observation. The conserved quantities associated with the rotating regular black holes are calculated and also a brief description of the weak gravitational lensing using the Gauss-Bonnet theorem is presented. Interestingly, the deflection angle decreases with the charge of the black hole. Our results vis-a-vis go over to the Kerr and Kerr-Newman black holes in the appropriate limits.
引用
收藏
页数:18
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