Quasi-local restricted phase space for RN black holes adds pressure and area variables, producing isocharge temperature-entropy transitions and neutral Hawking-Page-like transitions absent in the asymptotic description.
Extended quasilocal Thermodynamics of Schwarzchild–anti de Sitter black holes
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Applies Parikh-Wilczek tunneling with backreaction to evaporating AdS black holes, finding luminosity deviates from blackbody scaling for small masses due to rapid mass loss, and computes renormalized energy-momentum tensor in Vaidya-AdS.
Quantum-statistical constraints restrict the infinite family of KadS thermodynamic descriptions to a subclass that reduces to Schwarzschild-AdS and Kerr cases in appropriate limits, with uniqueness for co-rotating and volume-coincident descriptions.
citing papers explorer
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Black holes at a finite distance: Quasi-local restricted phase space formalism
Quasi-local restricted phase space for RN black holes adds pressure and area variables, producing isocharge temperature-entropy transitions and neutral Hawking-Page-like transitions absent in the asymptotic description.
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Hawking atmosphere of anti-de Sitter black holes
Applies Parikh-Wilczek tunneling with backreaction to evaporating AdS black holes, finding luminosity deviates from blackbody scaling for small masses due to rapid mass loss, and computes renormalized energy-momentum tensor in Vaidya-AdS.
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Quantum-statistical constraints on Kerr-anti-de Sitter thermodynamics
Quantum-statistical constraints restrict the infinite family of KadS thermodynamic descriptions to a subclass that reduces to Schwarzschild-AdS and Kerr cases in appropriate limits, with uniqueness for co-rotating and volume-coincident descriptions.