https://doi.org/10.1140/epjc/s10052-020-8346-3
Regular Article - Theoretical Physics
Optical properties of Kerr–Newman spacetime in the presence of plasma
1
School of Natural Sciences, National University of Sciences and Technology, Sector H-12, Islamabad, Pakistan
2
Department of Electrical Engineering, Air University, Islamabad, Pakistan
3
Inha University in Tashkent, Ziyolilar 9, Tashkent, 100170, Uzbekistan
4
Ulugh Beg Astronomical Institute, Astronomy St. 33, Tashkent, 100052, Uzbekistan
* e-mail: atamurotov@yahoo.com
** e-mail: fatamurotov@gmail.com
Received:
16
July
2020
Accepted:
12
August
2020
Published online:
20
August
2020
We have studied the null geodesics in the background of the Kerr–Newman black hole veiled by a plasma medium using the Hamilton–Jacobi method. The influence of black hole’s charge and plasma parameters on the effective potential and the generic photon orbits has been investigated. Furthermore, our discussion embodies the effects of black hole’s charge, plasma and the inclination angle on the shadow cast by the gravity with and without the spin parameter. We examined the energy released from the black hole as a result of the thermal radiations, which exclusively depends on the size of the shadow. The angle of deflection of the massless particles is also explored considering a weak-field approximation. We present our results in juxtaposition to the analogous black holes in General Relativity, particularly the Schwarzschild and Kerr black hole.
© The Author(s), 2020
