We study the effects of the generalized uncertainty
principle in the tunneling formalism for Hawking radiation
to evaluate the quantum-corrected Hawking temperature
and entropy for a Kerr black hole. By assumption
of a spatially flat universe accompanied with expansion of
metric, the modified area and entropy of Kerr black hole
are calculated and we could obtain an expression for entropy
of black hole that is changing with respect to time and
Bekenstein-Hawking temperature.
کلید واژگان :
Kerr black hole · Hawking temperature · B-H entropy · Tunneling probability
