A quasi-stationary non-equilibrium partition functional unifies entropy principles, pole-based temperature, and horizon topology to extend black hole thermodynamics to dynamically driven cases, applied to Kerr-Newman black holes in f(R) gravity.
Padmanabhan,Thermodynamical aspects of gravity: New insights, Rep
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Non-Equilibrium Physics of Thermodynamicized Black Holes
A quasi-stationary non-equilibrium partition functional unifies entropy principles, pole-based temperature, and horizon topology to extend black hole thermodynamics to dynamically driven cases, applied to Kerr-Newman black holes in f(R) gravity.