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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Analyses of three gas systems show effective temperature rises with velocity, supporting Ott-Eddington interpretation and linking temperature to the inverse-temperature four-vector beta.
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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Relativistic transformation of temperature revisited
Analyses of three gas systems show effective temperature rises with velocity, supporting Ott-Eddington interpretation and linking temperature to the inverse-temperature four-vector beta.