Generalized mass-to-horizon entropy with index n is reconstructed from f(R) gravity Lagrangian L proportional to R^{1+epsilon} where epsilon equals (n-1)/2 using Iyer-Wald on constant-curvature spherically symmetric solutions.
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Gravity theory of the generalized mass to horizon entropy The Iyer Wald approach
Generalized mass-to-horizon entropy with index n is reconstructed from f(R) gravity Lagrangian L proportional to R^{1+epsilon} where epsilon equals (n-1)/2 using Iyer-Wald on constant-curvature spherically symmetric solutions.
- Model-independent reconstruction of cosmic thermodynamics and dark energy dynamics