Beyond the Einstein Equation of State: Wald Entropy and Thermodynamical Gravity
Maulik K. Parikh, Sudipta Sarkar

TL;DR
This paper demonstrates that classical gravity equations can be derived from thermodynamic principles using Wald entropy, indicating gravity's potential thermodynamic origin across all diffeomorphism-invariant theories.
Contribution
It establishes a general derivation of gravity equations from thermodynamics using Wald entropy for any diffeomorphism-invariant theory.
Findings
Gravity equations follow from thermodynamic relation dQ = T dS
Wald entropy applies to local Rindler horizons
Supports gravity's thermodynamic origin
Abstract
We show that the classical equations of gravity follow from a thermodynamic relation, dQ = T dS, where S is taken to be the Wald entropy, applied to a local Rindler horizon at any point in spacetime. Our approach works for all diffeomorphism-invariant theories of gravity. This suggests that classical gravity may be thermodynamic in origin.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Quantum Electrodynamics and Casimir Effect
