Polarization distribution in the image of a synchrotron emitting ring around a regular black hole

被引:20
作者
Liu, Xueyao [1 ]
Chen, Songbai [1 ,2 ]
Jing, Jiliang [1 ,2 ]
机构
[1] Hunan Normal Univ, Synerget Innovat Ctr Quantum Effects & Applicat, Dept Phys,Minist Educ, Key Lab Low Dimens Quantum Struct & Quantum Contr, Changsha 410081, Peoples R China
[2] Yangzhou Univ, Coll Phys Sci & Technol, Ctr Gravitat & Cosmol, Yangzhou 225009, Jiangsu, Peoples R China
来源
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY | 2022年 / 65卷 / 12期
基金
中国国家自然科学基金;
关键词
black hole image; regular black hole; polarization distribution; synchrotron emitting ring; EVENT HORIZON;
D O I
10.1007/s11433-022-1946-2
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The polarized images of a synchrotron emitting ring are studied in the regular Hayward and Bardeen black hole spacetimes. These regular black holes carry a magnetic field in terms of gravity coupled to nonlinear electrodynamics. Results show that the main features of the polarization images of the emitting rings are similar in these two regular black hole spacetimes. As the magnetic charge parameter increases, the polarization intensity and the electric vector position angle in the image plane increase in Hayward and Bardeen black hole spacetimes. Moreover, the polarization intensity and electric vector position angle in the image of the emitting ring in the Hayward black hole spacetime are closer to those in the Schwarzschild case. The effects of the magnetic charge parameter on the Strokes Q-U loops are also slightly smaller in the Hayward black hole spacetime. This information stored in the polarization images around Hayward and Bardeen black holes could help understand regular black holes and the gravity coupled to nonlinear electrodynamics.
引用
收藏
页数:12
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