A uniform magnetic field around a rotating black hole enhances light deflection and monotonically decreases entropy while increasing Hawking temperature.
Magnetohydrody- namics Simulations of Active Galactic Nucleus Disks and Jets,
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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.