1. Shadow cast by a rotating and nonlinear magnetic-charged black hole in perfect fluid dark matter
- Author
-
Peng-Zhang He, Hao-Ran Zhang, Jian-Bo Deng, Tian-Chi Ma, He-Xu Zhang, and Yuan Chen
- Subjects
Physics ,Nuclear and High Energy Physics ,010308 nuclear & particles physics ,Astrophysics::High Energy Astrophysical Phenomena ,Dark matter ,Astrophysics::Instrumentation and Methods for Astrophysics ,General Physics and Astronomy ,FOS: Physical sciences ,Computer Science::Computation and Language (Computational Linguistics and Natural Language and Speech Processing) ,Astronomy and Astrophysics ,Perfect fluid ,General Relativity and Quantum Cosmology (gr-qc) ,Charged black hole ,01 natural sciences ,General Relativity and Quantum Cosmology ,Black hole ,Nonlinear system ,Exact solutions in general relativity ,Quantum electrodynamics ,0103 physical sciences ,Shadow ,Computer Science::General Literature ,010306 general physics - Abstract
In this paper, we derived an exact solution of the spherically symmetric Hayward black hole surrounded by perfect fluid dark matter (PFDM). By applying the Newman–Janis algorithm, we generalized it to the corresponding rotating black hole. Then, we studied the shadows of rotating Hayward black hole in PFDM. The apparent shape of the shadow depends upon the black hole spin [Formula: see text], the magnetic charge [Formula: see text] and the PFDM intensity parameter [Formula: see text]. The shadow is a perfect circle in the non-rotating case [Formula: see text] and a deformed one in the rotating case [Formula: see text]. For a fixed value of [Formula: see text], the size of the shadow increases with the increasing [Formula: see text], but decreases with the increasing [Formula: see text]. We further investigated the black hole emission rate. We found that the emission rate decreases with the increasing [Formula: see text] (or [Formula: see text]) and the peak of the emission shifts to lower frequency. Finally, we discussed the observational prospects corresponding to the supermassive black hole Sgr A[Formula: see text] at the center of the Milky Way.
- Published
- 2020