Influence of an anisotropic matter field on the shadow of a rotating black hole
classification
🌀 gr-qc
keywords
anisotropicblackcorrespondingfieldmatterrotatingshadowapparent
read the original abstract
In this paper, we study the shadow produced by rotating black holes with charge in the presence of an anisotropic matter field. We obtain the apparent shape and the corresponding observables characterizing the size, oblateness, and deviation of the center, for different values of the parameters of the model. We compare the new results with those corresponding to the Kerr-Newmann spacetime and we also discuss the observational prospects in this case.
This paper has not been read by Pith yet.
Forward citations
Cited by 1 Pith paper
-
Anisotropic matter and nonlinear electromagnetics black holes
Establishes a parameter mapping from anisotropic matter black holes to nonlinear electrodynamics black holes, recovering known solutions like dark matter and scalar hair cases and extending to rotating extremal limits.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.