Simple regular black hole with logarithmic entropy correction

Abstract

A simple regular black hole solution satisfying the weak energy condition is obtained within Einstein--non--linear electrodynamics theory. We have computed the thermodynamic properties of this black hole by a careful analysis of the horizons and we have found that the usual Bekenstein--Hawking entropy gets corrected by a logarithmic term. Therefore, in this sense our model realizes some quantum gravity predictions which add this kind of correction to the black hole entropy. In particular, we have established some similitudes between our model and a quadratic generalized uncertainty principle. This similitude has been confirmed by the existence of a remnant, which prevents complete evaporation, in agreement with the quadratic generalized uncertainty principle case.

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• Quantum corrections to a finite temperature BIon
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• The phase transition and holographic in modified Horava -Lifshitz black hole
• New models of d-dimensional black holes without inner horizon and with an integrable singularity
• Regularized Black Hole Solution from a New String Cloud Source