Rotating black hole mimicker surrounded by the string cloud

被引:8
|
作者
Yang, Yi [1 ]
Liu, Dong [2 ]
Ovgun, Ali [3 ]
Lambiase, Gaetano [4 ,5 ]
Long, Zheng-Wen [2 ]
机构
[1] Guizhou Univ Finance & Econ, Sch Math & Stat, Guiyang 550025, Peoples R China
[2] Guizhou Univ, Coll Phys, Guiyang 550025, Peoples R China
[3] Eastern Mediterranean Univ, Phys Dept, North Cyprus via Mersin 10, TR-99628 Famagusta, Turkiye
[4] Univ Salerno, Dipartimento Fis ER Caianiello, Via Giovanni Paolo II,132, I-84084 Fisciano, Italy
[5] Ist Nazl Fis Nucl, Sez Napoli, Grp Collegato Salerno, Via Giovanni Paolo II,132, I-84084 Fisciano, SA, Italy
基金
中国国家自然科学基金;
关键词
DARK-MATTER; FIELD; MASS;
D O I
10.1103/PhysRevD.109.024002
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Traversable wormholes and regular black holes usually represent completely different scenarios. But in the black bounce spacetime they can be described by a same line element, which is very attractive. Furthermore, the black hole photos taken by EHT show that black holes have spin, so spin is an indispensable intrinsic property of black holes in the actual Universe. In this work, we derive a rotating black hole mimicker surrounded by the string cloud (SC), which can be interpolated to represent regular black hole spacetime and traversable wormhole spacetime. We investigate the effect of the spin a and SC parameter L on the observables (shadow radius Rs and distortion delta s) and energy emission rate of the black hole mimicker surrounded by the SC. We find that shadow for this spacetime is very sensitive to the L, i.e., the SC parameter can significantly increase the boundary of the shadow.
引用
收藏
页数:13
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