Quantum corrections to Schwarzschild black hole evaporation produce a maximum temperature, radiation cessation, an extremal remnant, and logarithmic entropy correction.
Sen,Logarithmic corrections to rotating extremal black hole entropy in four and five dimensions,General Relativity and Gravitation44(2012), 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.