Weak Gravitational Lensing by Einstein-Non-Linear-Maxwell-Yukawa Black Hole

Wajiha Javed; Muhammad Bilal Khadim; Ali Övgün

doi:10.20944/preprints202001.0136.v1

Preprint Article Version 1 Preserved in Portico This version is not peer-reviewed

Version 1 : Received: 12 January 2020 / Approved: 12 January 2020 / Online: 12 January 2020 (17:40:26 CET)

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

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Weak Gravitational Lensing by Einstein-Non-Linear-Maxwell-Yukawa Black Hole

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