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Gravitational Entropy and the Second Law of Thermodynamics

机译:引力熵和热力学第二定律

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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 O ( 3 , 1 ) → O ( 3 ) × R , where O ( 3 ) is the rotational symmetry of the Friedmann–Lemaître–Robertson–Walker spacetime. The Weyl curvature tensor C μ ν ρ σ 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 〈 0 | ψ μ | 0 〉 ≠ 0 for a vector field ψ μ acts as an order parameter and at the critical temperature T c a phase transition occurs breaking the Lorentz symmetry spontaneously. During the ordered O ( 3 ) symmetry phase the entropy is vanishingly small and for T T c as the universe expands the anti-restored O ( 3 , 1 ) Lorentz symmetry leads to a disordered phase and a large increase in entropy creating the arrow of time.
机译:在大爆炸附近的相中自发地违反了洛伦兹和微分不变性,从而降低了熵,从而有了时间箭和热力学第二定律。自发的对称破坏导致O(3,1)→O(3)×R,其中O(3)是Friedmann–Lemaître–Robertson–Walker时空的旋转对称。满足Penrose零Weyl曲率猜想的FLRW时空,Weyl曲率张量Cμνρσ消失。讨论了测量重力熵的要求。真空期望值<0 | ψμ|对于矢量场ψμ,0〉≠0充当阶数参数,并且在临界温度T c处发生相变,自然地打破了洛伦兹对称性。在有序的O(3)对称阶段,熵逐渐消失,对于T

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