Model-independent Gaussian Process reconstruction from CC+DESI+supernova data shows positive entropy production and approach to thermodynamic equilibrium, with dark energy equation of state consistent with a cosmological constant.
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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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Model-independent reconstruction of cosmic thermodynamics and dark energy dynamics
Model-independent Gaussian Process reconstruction from CC+DESI+supernova data shows positive entropy production and approach to thermodynamic equilibrium, with dark energy equation of state consistent with a cosmological constant.
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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.