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受参数漂移影响的哈密顿系统中的混沌。

Chaos in Hamiltonian systems subjected to parameter drift.

机构信息

Institute for Theoretical Physics, Eötvös Loránd University, Pázmány Péter Sétány 1/A, H-1117 Budapest, Hungary.

出版信息

Chaos. 2019 Dec;29(12):121105. doi: 10.1063/1.5139717.

DOI:10.1063/1.5139717
PMID:31893674
Abstract

Based on the example of a paradigmatic low-dimensional Hamiltonian system subjected to different scenarios of parameter drifts of non-negligible rates, we show that the dynamics of such systems can best be understood by following ensembles of initial conditions corresponding to tori of the initial system. When such ensembles are followed, toruslike objects called snapshot tori are obtained, which change their location and shape. In their center, one finds a time-dependent, snapshot elliptic orbit. After some time, many of the tori break up and spread over large regions of the phase space; however, one may find some smaller tori, which remain as closed curves throughout the whole scenario. We also show that the cause of torus breakup is the collision with a snapshot hyperbolic orbit and the surrounding chaotic sea, which forces the ensemble to adopt chaotic properties. Within this chaotic sea, we demonstrate the existence of a snapshot horseshoe structure and a snapshot saddle. An easily visualizable condition for torus breakup is found in relation to a specific snapshot stable manifold. The average distance of nearby pairs of points initiated on an original torus at first hardly changes in time but crosses over into an exponential growth when the snapshot torus breaks up. This new phase can be characterized by a novel type of a finite-time Lyapunov exponent, which depends both on the torus and on the scenario followed. Tori not broken up are shown to be the analogs of coherent vortices in fluid flows of arbitrary time dependence, and the condition for breakup can also be demonstrated by the so-called polar rotation angle method.

摘要

基于一个受显著非零速率参数漂移影响的典范低维哈密顿系统的示例,我们表明,通过遵循对应于初始系统环面的初始条件集合,可以最好地理解此类系统的动力学。当遵循这些集合时,会得到称为快照环面的类环面物体,它们会改变位置和形状。在它们的中心,会找到一个时变的、快照椭圆轨道。一段时间后,许多环面会分裂并散布在相空间的大片区域中;然而,可能会发现一些较小的环面,它们在整个场景中保持为封闭曲线。我们还表明,环面分裂的原因是与快照双曲轨道和周围的混沌海的碰撞,这迫使集合采用混沌特性。在这个混沌海中,我们证明了快照马蹄铁结构和快照鞍点的存在。在与特定快照稳定流形相关的关系中,找到了环面分裂的一个易于可视化的条件。最初在原始环面上启动的邻近点对的平均距离在时间上几乎没有变化,但当快照环面分裂时会跨越到指数增长。这个新的阶段可以用一种新的有限时间李雅普诺夫指数来描述,它既取决于环面,也取决于所遵循的场景。未分裂的环面被证明是任意时变流场中相干涡旋的类似物,并且可以通过所谓的极坐标旋转角方法来证明分裂的条件。

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