Quantum corrections to Schwarzschild black hole evaporation produce a maximum temperature, radiation cessation, an extremal remnant, and logarithmic entropy correction.
Nicolini,Noncommutative black holes, the final appeal to quantum gravity: a review, International Journal of Modern Physics A24(2009), no
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Hawking radiation from a semi-classical Schwarzschild black hole
Quantum corrections to Schwarzschild black hole evaporation produce a maximum temperature, radiation cessation, an extremal remnant, and logarithmic entropy correction.