Thermodynamics of scalar-tensor gravity

Abstract

Previously, the Einstein equation has been described as an equation of state, general relativity as the equilibrium state of gravity, and $f(\mathcal{R})$ 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.

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