Preserved in Portico This version is not peer-reviewed
Weak Gravitational Lensing by Einstein-Non-Linear-Maxwell-Yukawa Black Hole
: Received: 12 January 2020 / Approved: 12 January 2020 / Online: 12 January 2020 (17:40:26 CET)
A peer-reviewed article of this Preprint also exists.
Journal reference: International Journal of Geometric Methods in Modern Physics 2020, 17, 2050182
In this article, we analyze the weak gravitational lensing in the context of Einstein-non-linear Maxwell-Yukawa black hole. To this desire, we derive the deflection angle of light by Einstein-non-linear Maxwell-Yukawa black hole using the Gibbons and Werner method. For this purpose, we obtain the Gaussian optical curvature and implement the Gauss-Bonnet theorem to investigate the deflection angle of Einstein-non-linear Maxwell-Yukawa black hole. Moreover, we derive the deflection angle of light in the presence of plasma medium. We also analyze the graphical behavior of deflection angle by Einstein-non-linear Maxwell-Yukawa black hole in the presence of plasma as well as non-plasma medium.
Weak gravitational lensing; Einstein-non-linear Maxwell-Yukawa black holes; Deflection angle; Gauss-Bonnet theorem
PHYSICAL SCIENCES, General & Theoretical Physics
This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
We encourage comments and feedback from a broad range of readers. See criteria for comments and our diversity statement.