Entropy of Vaidya Black Hole on Apparent Horizon with Minimal length Revisited

Abstract

By considering the generalized uncertainty principle, the degrees of freedom near the apparent horizon of Vaidya black hole are calculated with thin film model. The result shows that a cut-off can be introduced naturally rather than taking by hand. Furthermore, if the minimal length is chosen to be a specific value, the statistical entropy will satisfy the conventional area law at the horizon, which might reveal some deep things of the minimal length.

arXiv comment8pages, 0 figures, Int J Theor Phys(2018)

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Cited by in corpus (1)

• Evaporation of dynamical horizon with the Hawking temparature in the {\bf K-}essence emergent Vaidya spacetime