A uniform magnetic field around a rotating black hole enhances light deflection and monotonically decreases entropy while increasing Hawking temperature.
Shadow and weak gravitational lensing of a rotating regular black hole in a non-minimally coupled Einstein-Yang-Mills theory in the presence of plasma,
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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.