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Thermodynamics of Higher Order Entropy Corrected Schwarzschild-Beltrami-de Sitter Black Hole

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arxiv 1701.08650 v4 pith:7VHVVWIJ submitted 2017-01-24 physics.gen-ph

classification physics.gen-ph
keywords orderblackentropyhigherholecorrectedcorrectionsfirst
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In this paper, we consider higher order correction of the entropy and study the thermodynamical properties of recently proposed Schwarzschild-Beltrami-de Sitter black hole, which is indeed an exact solution of Einstein equation with a positive cosmological constant. By using the corrected entropy and Hawking temperature we extract some thermodynamical quantities like Gibbs and Helmholtz free energies and heat capacity. We also investigate the first and second laws of thermodynamics. We find that presence of higher order corrections, which come from thermal fluctuations, may remove some instabilities of the black hole. Also unstable to stable phase transition is possible in presence of the first and second order corrections.

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  1. Quantum-Corrected Thermodynamics and Phase Structure of AdS Euler-Heisenberg Black Hole

    gr-qc 2026-08 conditional novelty 4.0 of 10

    Thermal fluctuation corrections to entropy change the stability and phase structure of an AdS Euler-Heisenberg black hole, producing multiple specific-heat divergences and a stable small-hole phase.

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