封闭振荡宇宙的统计力学理论
Statistical Mechanical Theory of a Closed Oscillating Universe
摘要：
基于牛顿定律在哈密顿动力学中的重新表述，结合统计力学，我们建立了一个支持闭合振荡宇宙假设的统计力学理论.我们发现，宇宙作为一个整体的行为可以表示为一个自由熵振荡器的寿命是非均匀的，从而意味着时间是短或长根据宇宙本身的状态通过其熵。我们的结论是，时间减少到宇宙的熵产生，而非零熵产生意味着局部波动可能存在，从而引起质量的出现和空间的曲率。
英文摘要：
Based on Newton's laws reformulated in the Hamiltonian dynamics combined with statistical mechanics, we formulate a statistical mechanical theory supporting the hypothesis of a closed oscillating universe. We find that the behaviour of the universe as a whole can be represented by a free entropic oscillator whose lifespan is nonhomogeneous, thus implying that time is shorter or longer according to the state of the universe itself given through its entropy. We conclude that time reduces to the entropy production of the universe and that a nonzero entropy production means that local fluctuations could exist giving rise to the appearance of masses and to the curvature of the space.
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