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arXiv 1502.02510nlin.CD
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经典Henon-Heiles Hamilton系统的轨道分类

Classifying orbits in the classical Henon-Heiles Hamiltonian system

Euaggelos E. Zotos

摘要:

Hénon-Heiles势无疑是最简单、最经典、最有特色的哈密顿系统之一。本文的目的是通过观测混沌轨道的百分比以及组成主要规则轨道族的轨道的百分比随能量变化的情况,揭示作为系统唯一参数的总轨道能量的值对不同轨道族的影响。特别是,我们进行了彻底的数值调查区分有序和混沌轨道,只考虑有界运动的几个能级。通过将运动方程和变分方程数值积分到广泛的轨道样本中来计算较小的对准指数(SALI),以便安全地区分有序和混沌运动。此外,一种方法的基础上的概念的频谱动力学,利用傅立叶变换的时间序列的每个坐标被用来识别各种家庭的定期轨道,也认识到二次共振,从他们分叉。我们的探索发生在物理$(x,y)$和相位$(y,\dot{y})$空间更好地了解系统的轨道特性。结果发现,对于低能级的运动是完全有规律的盒子轨道人口最多的家庭,而随着能量的值增加混乱和几个共振家庭出现。我们还观察到,绝大多数共振轨道实际上属于主要1:1共振家族的分叉家族。我们还将我们的结果与以前使用不同的混沌指标获得的类似结果进行了比较。

英文摘要:

The Hénon-Heiles potential is undoubtedly one of the most simple, classical and characteristic Hamiltonian systems. The aim of this work is to reveal the influence of the value of the total orbital energy, which is the only parameter of the system, on the different families of orbits, by monitoring how the percentage of chaotic orbits, as well as the percentages of orbits composing the main regular families evolve when energy varies. In particular, we conduct a thorough numerical investigation distinguishing between ordered and chaotic orbits, considering only bounded motion for several energy levels. The smaller alignment index (SALI) was computed by numerically integrating the equations of motion as well as the variational equations to extensive samples of orbits in order to distinguish safely between ordered and chaotic motion. In addition, a method based on the concept of spectral dynamics that utilizes the Fourier transform of the time series of each coordinate is used to identify the various families of regular orbits and also to recognize the secondary resonances that bifurcate from them. Our exploration takes place both in the physical $(x,y)$ and the phase $(y,\dot{y})$ space for a better understanding of the orbital properties of the system. It was found, that for low energy levels the motion is entirely regular being the box orbits the most populated family, while as the value of the energy increases chaos and several resonant families appear. We also observed, that the vast majority of the resonant orbits belong in fact in bifurcated families of the main 1:1 resonant family. We have also compared our results with previous similar outcomes obtained using different chaos indicators.

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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