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Thermodynamic Instability of $\mathrm{{3D}}$ Einstein-Born-Infeld AdS Black Holes

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arxiv 2012.14206 v3 pith:5IC4NQEW submitted 2020-12-28 gr-qc

classification gr-qc
keywords blackholesconjectureinstabilityelectrodynamicsnonlinearconstanteffects
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abstract

Super-entropic black holes possess finite-area but noncompact event horizons and violate the reverse isoperimetric inequality. It has been conjectured that such black holes always have negative specific heat at constant volume $C_{V}$ or negative specific heat at constant pressure $C_{P}$ whenever $C_{V}>0$, making them unstable in extended thermodynamics. In this paper, we test this instability conjecture on a family of nonlinear electrodynamics black holes, namely $3$D Einstein-Born-Infeld (EBI) AdS black holes. Our results show that when nonlinear electrodynamics effects are weak, the instability conjecture is valid. However, the conjecture can be violated in some parameter region when nonlinear electrodynamics effects are strong enough. This observation thus provides a counter example to the instability conjecture, which suggests that super-entropic black holes could be thermodynamically stable.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Specific Heats for Rotating Quantum BTZ Black Holes in Extended Thermodynamics

    hep-th 2025-02 conditional novelty 5.0 of 10

    For the rotating quantum BTZ black hole, the paper derives path-dependent heat capacities at constant pressure and volume with multiple positive and negative branches.

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