A uniform magnetic field around a rotating black hole enhances light deflection and monotonically decreases entropy while increasing Hawking temperature.
Topological classes of ther- modynamics of black holes in perfect fluid dark matter background,
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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.