Surface geometry and shadow of a Schwarzschild black hole with a halo

被引:2
|
作者
Wang, Mingzhi [1 ]
Guo, Guanghai [1 ]
Chen, Songbai [2 ,3 ,4 ]
Jing, Jiliang [2 ,3 ,4 ]
机构
[1] Qingdao Univ Sci & Technol, Sch Math & Phys, Qingdao 266061, Peoples R China
[2] Hunan Normal Univ, Inst Phys, Changsha 410081, Peoples R China
[3] Hunan Normal Univ, Synerget Innovat Ctr Quantum Effects & Applicat, Dept Phys, Key Lab Low Dimens Quantum Struct & Quantum Contro, Changsha 410081, Peoples R China
[4] Yangzhou Univ, Coll Phys Sci & Technol, Ctr Gravitat & Cosmol, Yangzhou 225009, Peoples R China
基金
中国国家自然科学基金;
关键词
cluster radioactivity; cluster-formation model (CFM); half-lives; preformation probability; TELESCOPE RESULTS. VI;
D O I
10.1088/1674-1137/ac94bc
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
We studied the surface geometry and shadows of a Schwarzschild black hole with a halo containing quadrupolar and octopolar terms. It was found that the quadrupole term causes a Schwarzschild black hole to be prolate at the quadrupole strength Q < 0 and oblateQ at > 0 , and the octopole term causes to the shadow stretch upward at the octopolar strength ngth O < 0 and downward at O > 0 . The shadow of a Schwarzschild black hole with a halo stretches and squeezes along the horizontal directionQ at < 0 and Q > 0 , respectively. Meanwhile, the black hole shadow shifts upwardO at < 0 and downwardO at > 0 . We present the light rays that form the shadow boundary to explain the emergence of the extraordinary patterns of the black hole shadow with quadrupole and octopole terms. From the observable width W, height H, oblateness K, and distortion parameter of the black hole shadow, ?c we can determine the quadrupole and octopolar strengths of a Schwarzschild black hole with a halo. Our results show that the quadrupolar and octopolar terms yield a series of interesting patterns for the shadow of a Schwarzschild black hole with a halo.
引用
收藏
页数:12
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