Lozej Črt
Center for Applied Mathematics and Theoretical Physics, University of Maribor, Mladinska 3, Maribor, Slovenia.
Phys Rev E. 2020 May;101(5-1):052204. doi: 10.1103/PhysRevE.101.052204.
We analyze the structure and stickiness in the chaotic components of generic Hamiltonian systems with divided phase space. Following the method proposed recently in Lozej and Robnik [Phys. Rev. E 98, 022220 (2018)2470-004510.1103/PhysRevE.98.022220], the sticky regions are identified using the statistics of recurrence times of a single chaotic orbit into cells dividing the phase space into a grid. We perform extensive numerical studies of three example systems: the Chirikov standard map, the family of Robnik billiards, and the family of lemon billiards. The filling of the cells is compared to the random model of chaotic diffusion, introduced in Robnik et al. [J. Phys. A: Math. Gen. 30, L803 (1997)JPHAC50305-447010.1088/0305-4470/30/23/003] for the description of transport in the phase spaces of ergodic systems. The model is based on the assumption of completely uncorrelated cell visits because of the strongly chaotic dynamics of the orbit and the distribution of recurrence times is exponential. In generic systems the stickiness induces correlations in the cell visits. The distribution of recurrence times exhibits a separation of timescales because of the dynamical trapping. We model the recurrence time distributions to cells inside sticky areas as a mixture of exponential distributions with different decay times. We introduce the variable S, which is the ratio between the standard deviation and the mean of the recurrence times as a measure of stickiness. We use S to globally assess the distributions of recurrence times. We find that in the bulk of the chaotic sea S=1, while S>1 in areas of stickiness. We present the results in the form of animated grayscale plots of the variable S in the largest chaotic component for the three example systems, included as supplemental material to this paper.
我们分析了具有相空间划分的一般哈密顿系统混沌分量中的结构和粘性。遵循最近在洛泽伊和罗布尼克 [《物理评论E》98, 022220 (2018)2470 - 004510.1103/PhysRevE.98.022220] 中提出的方法,通过单个混沌轨道进入将相空间划分为网格的单元格的回归时间统计来识别粘性区域。我们对三个示例系统进行了广泛的数值研究:奇里科夫标准映射、罗布尼克台球族和柠檬台球族。将单元格的填充情况与罗布尼克等人 [《物理学杂志A:数学一般》30, L803 (1997)JPHAC50305 - 447010.1088/0305 - 4470/30/23/003] 中引入的用于描述遍历系统相空间中输运的混沌扩散随机模型进行比较。该模型基于由于轨道的强混沌动力学导致单元格访问完全不相关的假设,并且回归时间的分布是指数分布。在一般系统中,粘性会在单元格访问中引起相关性。由于动态捕获,回归时间的分布呈现出时间尺度的分离。我们将粘性区域内单元格的回归时间分布建模为具有不同衰减时间的指数分布的混合。我们引入变量S,它是回归时间的标准差与均值之比,作为粘性的一种度量。我们使用S来全局评估回归时间的分布。我们发现,在混沌海的大部分区域S = 1,而在粘性区域S > 1。我们以三个示例系统最大混沌分量中变量S的动画灰度图形式呈现结果,作为本文的补充材料包含在内。