Revisiting the shadow of a black hole in the presence of a plasma

被引:57
作者
Huang, Yang
Dong, Yi-Ping
Liu, Dao-Jun [1 ]
机构
[1] Shanghai Normal Univ, Ctr Astrophys, 100 Guilin Rd, Shanghai 200234, Peoples R China
来源
INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 2018年 / 27卷 / 12期
关键词
Shadow of black hole; plasma; ray-tracing; GALACTIC-CENTER; ACCRETION;
D O I
10.1142/S0218271818501146
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the photon's motion around a black hole in the presence of a plasma whose density is a function of the radius coordinate by a renewed ray-tracing algorithm and investigate the influence of the plasma on the shadow of the black hole. The presence of plasma affects not only the size but also the shape of the black hole shadow. Furthermore, the influence of plasma on trajectories of photons depends on the frequency of the photons. For the high-frequency photons, the influence is negligible, on the contrary, the trajectories of low-frequency photons are affected significantly by the plasma. Interestingly, it is also found that the black hole image would take on a multi-ring structure due to the presence of plasma.
引用
收藏
页数:15
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