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Weak Gravitational Lensing by Einstein-Non-Linear-Maxwell-Yukawa Black Hole
Wajiha Javed
Ali Övgün
Version 1
: Received: 12 January 2020 / Approved: 12 January 2020 / Online: 12 January 2020 (17:40:26 CET)
How to cite: Javed, W.; Khadim, M.B.; Övgün, A. Weak Gravitational Lensing by Einstein-Non-Linear-Maxwell-Yukawa Black Hole. Preprints 2020, 2020010136 (doi: 10.20944/preprints202001.0136.v1). Javed, W.; Khadim, M.B.; Övgün, A. Weak Gravitational Lensing by Einstein-Non-Linear-Maxwell-Yukawa Black Hole. Preprints 2020, 2020010136 (doi: 10.20944/preprints202001.0136.v1).
Abstract
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.
Subject Areas
Weak gravitational lensing; Einstein-non-linear Maxwell-Yukawa black holes; Deflection angle; Gauss-Bonnet theorem
Copyright: 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.
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