A uniform magnetic field around a rotating black hole enhances light deflection and monotonically decreases entropy while increasing Hawking temperature.
Null geodesics, thermodynamics, weak gravitational lensing, and black hole shadow characteristics of a Frolov regular black hole with constraints from EHT observa- tions,
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Light bending around the Kerr-Bertotti-Robinson black hole using material medium approach
A uniform magnetic field around a rotating black hole enhances light deflection and monotonically decreases entropy while increasing Hawking temperature.