It is shown that the Bekenstein-Hawking entropy
of black holes can accept a correction that effects on the radiation
tunneling probability. By assumption of a spatially flat
universe accompanied with expansion of metric, we could
obtain an expression for entropy of black hole that is changing
with respect to time and Bekenstein-Hawking temperature.
کلید واژگان :
Hawking temperature · Tunneling probability · Generalized uncertainty principle · Plank length
