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混沌层的宽度:由边缘共振引起的最大值。

Width of the chaotic layer: maxima due to marginal resonances.

作者信息

Shevchenko Ivan I

机构信息

Pulkovo Observatory of the Russian Academy of Sciences, Pulkovskoje Ave. 65, St. Petersburg 196140, Russia.

出版信息

Phys Rev E Stat Nonlin Soft Matter Phys. 2012 Jun;85(6 Pt 2):066202. doi: 10.1103/PhysRevE.85.066202. Epub 2012 Jun 4.

Abstract

Modern theoretical methods for estimating the width of the chaotic layer in the presence of prominent marginal resonances are considered in the perturbed pendulum model of nonlinear resonance. The fields of applicability of these methods are explicitly and precisely formulated. The comparative accuracy is investigated in massive and long-run numerical experiments. It is shown that the methods are naturally subdivided in classes applicable for adiabatic and nonadiabatic cases of perturbation. It is explicitly shown that the pendulum approximation of marginal resonance works well in the nonadiabatic case. In this case, the role of marginal resonances in determining the total layer width is demonstrated to diminish with increasing main parameter λ (equal to the ratio of the perturbation frequency to the frequency of small-amplitude phase oscillations on the resonance). Solely the "bending effect" is important in determining the total amplitude of the energy deviations of the near-separatrix motion at λ≳7. In the adiabatic case, it is demonstrated that the geometrical form of the separatrix cell can be described analytically quite easily by means of using a specific representation of the separatrix map. It is shown that the nonadiabatic (and, to some extent, intermediary) case is most actual, in comparison with the adiabatic one, for the physical or technical applications that concern the energy jumps in the near-separatrix chaotic motion.

摘要

在非线性共振的受扰摆模型中,考虑了用于估计存在显著边缘共振时混沌层宽度的现代理论方法。明确且精确地阐述了这些方法的适用范围。在大量长期的数值实验中研究了比较精度。结果表明,这些方法自然地细分为适用于绝热和非绝热扰动情况的类别。明确表明,边缘共振的摆近似在非绝热情况下效果良好。在这种情况下,随着主参数λ(等于扰动频率与共振时小振幅相位振荡频率之比)的增加,边缘共振在确定总层宽度中的作用被证明会减小。仅在λ≳7时,“弯曲效应”在确定近分离线运动能量偏差的总幅度方面才重要。在绝热情况下,证明了通过使用分离线映射的特定表示,可以很容易地解析描述分离线单元的几何形式。结果表明,与绝热情况相比,非绝热(在某种程度上还有中间)情况对于涉及近分离线混沌运动中能量跳跃的物理或技术应用最为实际。

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