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arXiv 1003.5495nlin.CD
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Fermi-Pasta-Ulam $β$系统$π$模解附近的热统计:从弱混沌到强混沌

Thermostatistics in the neighborhood of the $π$-mode solution for the Fermi-Pasta-Ulam $β$ system: from weak to strong chaos

M. Leo, R. A. Leo, P. Tempesta

摘要:

我们考虑Fermi-Pasta-Ulam $β$系统的$π$模解.通过扰动它,我们研究了系统作为能量密度的函数从一个区域的解是稳定的,到一个区域,在那里是不稳定的,首先弱,然后强混沌。我们介绍,作为随机性的指标,比率$ρ$(定义时)之间的第二和第一时刻的一个给定的概率分布。我们将用数值方法证明弱混沌和强混沌之间的过渡可以解释为一组合适的动力学变量的对称破缺。此外,我们表明,在该地区的弱混沌有数值证据表明,由Tsallis分布的热统计。

英文摘要:

We consider a $π$-mode solution of the Fermi-Pasta-Ulam $β$ system. By perturbing it, we study the system as a function of the energy density from a regime where the solution is stable to a regime, where is unstable, first weakly and then strongly chaotic. We introduce, as indicator of stochasticity, the ratio $ρ$ (when is defined) between the second and the first moment of a given probability distribution. We will show numerically that the transition between weak and strong chaos can be interpreted as the symmetry breaking of a set of suitable dynamical variables. Moreover, we show that in the region of weak chaos there is numerical evidence that the thermostatistic is governed by the Tsallis distribution.

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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