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Black hole thermodynamics with generalized uncertainty principle

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arxiv gr-qc/0609031 v2 pith:C57H424O submitted 2006-09-08 gr-qc hep-th

classification gr-qchep-th
keywords blackholetransitiongeneralizedlargephaseprincipleremnant
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We apply the generalized uncertainty principle to the thermodynamics of a small black hole. Here we have a black hole system with the UV cutoff. It is shown that the minimal length induced by the GUP interrupts the Gross-Perry-Yaffe phase transition for a small black hole. In order to see whether the black hole remnant takes place a transition to a large black hole, we introduce a black hole in a cavity (IR system). However, we fail to show the phase transition of the remnant to the large black hole.

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  1. Holographic explorations of regular black holes in pure gravity

    hep-th 2025-05 conditional novelty 6.0 of 10

    Regular, asymptotically AdS black holes are shown to exist in pure quasi-topological gravity, and their thermodynamics, quasinormal modes, Wilson loops, and a Type IIB field redefinition map are worked out.

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