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.
The Four laws of black hole mechanics,
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A new gauge-invariant effective action computes black hole Love numbers without Regge-Wheeler methods, and these numbers determine leading thermodynamic corrections under external perturbations.
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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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Tidal Response and Thermodynamics of Black Holes
A new gauge-invariant effective action computes black hole Love numbers without Regge-Wheeler methods, and these numbers determine leading thermodynamic corrections under external perturbations.