Quantum-corrected black hole thermodynamics to all orders in the Planck length

Understand

We investigate the effects to all orders in the Planck length from a generalized un- certainty principle (GUP) on black holes thermodynamics.

• We calculate the corrected Hawking temperature, entropy, and examine in details the Hawking evaporation process.
• As a result, the evaporation process is accelerated and the evaporation end-point is a zero entropy, zero heat capacity and finite non zero temperature black hole remnant (BHR).
• In particular we obtain a drastic reduction of the decay time, in comparison with the results obtained in the Hawking semi classical picture and with the GUP to leading order in the Planck length.