paper

Thermodynamics of scalar-tensor gravity

arXiv:2103.05389 · doi:10.1103/PhysRevD.103.L121501

Abstract

Previously, the Einstein equation has been described as an equation of state, general relativity as the equilibrium state of gravity, and gravity as a non-equilibrium one. We apply Eckart's first order thermodynamics to the effective dissipative fluid describing scalar-tensor gravity. Surprisingly, we obtain simple expressions for the effective heat flux, "temperature of gravity", shear and bulk viscosity, and entropy density, plus a generalized Fourier law in a consistent Eckart thermodynamical picture. Well-defined notions of temperature and approach to equilibrium, missing in the current thermodynamics of spacetime scenarios, naturally emerge.

arXiv comment5 pages. Corrected Eq. (26) describing the approach to equilibrium and one typographical error. Matches Letter to appear in Physical Review D

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