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arXiv 0712.0993gr-qc
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具有动力学混沌的de Sitter空间的Poincaré回归时

The Poincaré recurrence time for the de Sitter space with dynamical chaos

K. Ropotenko

摘要:

对于一个普通的系统,庞加莱递归时间是指数大的玻尔兹曼熵的系统。事实证明,对于具有动态混沌的系统,它由Kolmogorov-Sinai熵确定,并且可以相当短。本文指出,对于具有强混合性质的德西特空间,平均重现时间等于逆哈勃常数。这意味着我们的宇宙可以有一个有限的寿命,由宇宙的当前年龄限制。在这段时间之后,宇宙应该自我循环,这个过程既没有开始也没有结束。

英文摘要:

For an ordinary thermodynamical system the Poincaré recurrence time is exponentially large in the Boltzmann entropy of the system. It turns out, that for a system with dynamical chaos it is determined by the Kolmogorov-Sinai entropy and can be considerably shorter. It is shown in this note that for the de Sitter space with strong mixing properties the mean recurrence time is equal to the inverse Hubble constant. This means that our universe can have a finite lifetime bounded by the current age of the universe. After this time, the universe should recycle itself and this process has neither a beginning nor an end.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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