Shadow cast and deflection angle of Kerr-Newman-Kasuya spacetime
By A. Ovgun, I. Sakalli, J. Saavedra. Journal of Cosmology and Astroparticle Physics, 2018
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We study the shadow cast or silhouette generated by a Kerr-Newman-Kasuya (KNK) spacetime (rotating dyon black hole). It is shown that in addition to the angular momentum of the black hole, the dyon charge also affects the shadow image of the KNK black hole. Moreover, we analyze the weak gravitational lensing by the KNK black hole by using the Gauss-Bonnet theorem. Finally, we find that extra dyon charge decreases both the deflection angle and shadow of the KNK black hole.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/9d07d25904eb788c677038e8bfd72ab4b86d4ddc
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Citations in the corpus
- Shadows and deflection angle of charged and slowly rotating black holes in Einstein-Æther theory (2019, background): “Some notable results of black hole shadows are already discussed in the literature, to list a few: Schwarzschild black hole surrounded by a Bach-Weyl ring [7]; Einstein-dilaton-Gauss-Bonnet black hole [8]; Konoplya-Zhidenko or more general parameterized black holes [9, 10]; Einstein-Maxwell-ChernSim”