Optical properties of black holes in the presence of a plasma: The shadow

被引:175
作者
Atamurotov, Farruh [1 ,2 ]
Ahmedov, Bobomurat [1 ,3 ,4 ]
Abdujabbarov, Ahmadjon [1 ,3 ,4 ]
机构
[1] Inst Nucl Phys, Tashkent 100214, Uzbekistan
[2] Inha Univ Tashkent, Tashkent 100170, Uzbekistan
[3] Ulugh Beg Astron Inst, Tashkent 100052, Uzbekistan
[4] Natl Univ Uzbekistan, Tashkent 100174, Uzbekistan
来源
PHYSICAL REVIEW D | 2015年 / 92卷 / 08期
关键词
GALACTIC-CENTER; FIELD;
D O I
10.1103/PhysRevD.92.084005
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have studied photon motion around axially symmetric rotating Kerr black holes in the presence of a plasma with radial power-law density. It is shown that in the presence of a plasma, the observed shape and size of the shadow changes depending on the (i) plasma parameters, (ii) black hole spin, and (iii) inclination angle between the observer plane and the axis of rotation of the black hole. In order to extract the pure effect of the plasma influence on the black hole image, the particular case of the Schwarzschild black hole has also been investigated and it has been shown that the photon sphere around the spherically symmetric black hole is left unchanged under the plasma influence; however, the Schwarzschild black hole shadow size in the plasma is reduced due to the refraction of the electromagnetic radiation in the plasma environment of the black hole. The study of the energy emission from the black hole in plasma environment shows that in the presence of the plasma the maximal energy emission rate from the black hole decreases.
引用
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页数:7
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