Non-Equatorial Deflection of Light due to Kerr-Newman Black Hole: A Material Medium Approach
Saswati Roy, Shubham Kala, Prasanjit Ghosh, Hemwati Nandan, and Asoke K. Sen

TL;DR
This paper analytically investigates how charge and rotation of Kerr-Newman black holes influence the deflection of light rays in non-equatorial planes using a material medium approach, revealing complex frame-dragging effects.
Contribution
It provides a novel analytical expression for light deflection in Kerr-Newman space-time on non-equatorial planes, incorporating charge, rotation, and frame-dragging effects.
Findings
Deflection angle decreases with increasing charge at constant rotation.
Deflection angle increases with rotation for prograde and decreases for retrograde trajectories.
Frame dragging effects vary with latitude, affecting light velocity and refractive index.
Abstract
We explored the effect of space-time geometry on the trajectory of light rays in the context of a charged, rotating black hole. We derived an analytical expression for the deflection of light rays in Kerr-Newman space-time geometry, using a material medium approach, on non-equatorial plane. From this deflection angle expression it is evident that the charge and rotation of the black hole can affect the light rays' paths. Additionally, we calculated the refractive index of light rays by treating space-time as a medium. We demonstrated how the rotation parameter and charge influence the refractive index and hence the deflection angle of light rays. For Kerr-Newman geometry, the deflection angle decreases with increasing charge when the rotation parameter is held constant. Conversely, for a constant charge, the deflection angle increases with the rotation parameter for prograde and…
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Taxonomy
TopicsAdaptive optics and wavefront sensing
