A new variation scheme using dS multipliers on horizon field equations yields the first law of black hole thermodynamics for general unconstrained changes in M, J, Q.
Area spectra versus entropy spectra in black holes in topologically massive gravity.Class
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A Constraint-Free Formulation of Black Hole Thermodynamics from the Field Equations
A new variation scheme using dS multipliers on horizon field equations yields the first law of black hole thermodynamics for general unconstrained changes in M, J, Q.