Gravitational Entropy and the Second Law of Thermodynamics
J. W. Moffat

TL;DR
This paper proposes that spontaneous Lorentz symmetry breaking near the big bang reduces gravitational entropy, establishing an arrow of time consistent with the second law of thermodynamics through a phase transition.
Contribution
It introduces a model linking gravitational entropy, symmetry breaking, and phase transitions to explain the arrow of time in cosmology.
Findings
Spontaneous Lorentz symmetry breaking occurs at a critical temperature.
The ordered phase has vanishingly small entropy, while the disordered phase has large entropy.
A phase transition explains the increase in entropy as the universe expands.
Abstract
The spontaneous violation of Lorentz and diffeomorphism invariance in a phase near the big bang lowers the entropy, allowing for an arrow of time and the second law of thermodynamics. The spontaneous symmetry breaking leads to , where is the rotational symmetry of the Friedmann-Lema\^{i}tre-Robertson-Walker spacetime. The Weyl curvature tensor vanishes in the FLRW spacetime satisfying the Penrose zero Weyl curvature conjecture. The requirement of a measure of gravitational entropy is discussed. The vacuum expectation value for a vector field acts as an order parameter and at the critical temperature a phase transition occurs breaking the Lorentz symmetry spontaneously. During the ordered symmetry phase the entropy is vanishingly small and for as…
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