Study of bending angle and shadow in a new Schwarzschild-like black hole affected by plasma and non-plasma medium

R. Ali, Xia Tie Cheng, Muhammad Awais, R. Babar
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Abstract

In this study, we analyze the models of the deflection angle of a new Schwarzschild-like black hole and employ the optical metric of the black hole. To do so, we use the Gaussian curvature of the optical metric and the Gauss-Bonnet theorem, known as the Gibbons-Werner technique, to determine the deflection angle. Furthermore, we examine the deflection angle in the presence of the plasma medium and how the plasma medium affects the deflection angle. The deflection angle of the BH solution in the gauged super-gravity is computed using the Keeton-Petters approach. By utilizing the ray-tracing technique, we investigate the shadow of corresponding black hole and analyze the plots of the deflection angle as well as shadow to check the influence of the plasma and the algebraic thermodynamic parameters on the deflection angle and the shadow.
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受等离子体和非等离子体介质影响的新型类施瓦茨黑洞的弯曲角和阴影研究
在这项研究中,我们分析了新的类施瓦兹丘尔德黑洞的偏转角模型,并采用了黑洞的光学度量。为此,我们利用光学度量的高斯曲率和高斯-波内定理(即吉本斯-沃纳技术)来确定偏转角。此外,我们还研究了等离子体介质存在时的偏转角,以及等离子体介质如何影响偏转角。利用基顿-彼得斯方法计算了测量超引力中 BH 解决方案的偏转角。利用射线追踪技术,我们研究了相应黑洞的阴影,并分析了偏转角和阴影的曲线图,以检验等离子体和代数热力学参数对偏转角和阴影的影响。
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