For a pair of accelerating rotating charged NUT black holes, the GUP-corrected Hawking temperature is T'_H = T_H (1 - beta Xi), where beta is the quantum gravity parameter and Xi involves the emitted particle's mass and angular momentum.
Thermodynamics of accelerating and rotating black holes
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abstract
Thermodynamics of a large family of black holes from electrovacuum solutions of Einstein's equations is studied. This family includes rotating and non-accelerating black holes with NUT charge, and rotating and accelerating black holes. The surface gravity, Hawking temperature and the area laws for these black holes are presented. The first law of thermodynamics is also given. An interesting outcome of our analysis is the restriction obtained on the magnitude of acceleration for these black holes.
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Tunneling of Massive Vector Particles under the Influence of Quantum Gravity
For a pair of accelerating rotating charged NUT black holes, the GUP-corrected Hawking temperature is T'_H = T_H (1 - beta Xi), where beta is the quantum gravity parameter and Xi involves the emitted particle's mass and angular momentum.