Graphical Evolution of the Arnold Web: From Order to Chaos

Author:

Froeschlé Claude1,Guzzo Massimiliano1,Lega Elena1

Affiliation:

1. Observatoire de Nice, Boulevard de l'Observatoire, Boı̂te Postale 4229, 06304 Nice Cedex 4, France.

Abstract

We represent graphically the evolution of the set of resonances of a quasi-integrable dynamical system, the so-called Arnold web, whose structure is crucial for the stability properties of the system. The basis of our representation is the use of an original numerical method, whose definition is directly related to the dynamics of orbits, and the careful choice of a model system. We also show the transition from the Nekhoroshev stability regime to the Chirikov diffusive one, which is a generic nontrivial phenomenon occurring in many physical processes, such as slow chaotic transport in the asteroid belt and beam-beam interaction.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference30 articles.

1. Kolmogorov A. N., Dokl. Akad. Nauk SSSR 98, 527 (1954).

2. Moser J., Comm. Pure Appl. Math. 11, 81 (1958).

3. Arnold V. I., Russ. Math. Surv. 18, 9 (1963);

4. . The nondegeneracy condition requires that the set of invariant tori can be locally labeled by means of the frequencies on each torus. Another possible condition independent from the previous one is the so-called isoenergetic nondegeneracy condition which considers the restriction of the Hamiltonian on the surface of constant energy. Very often realistic models of physical systems are perturbations of integrable systems that are degenerate and also isoenergetically degenerate (such as the Euler-Poinsot rigid body the Kepler problem and the stability of elliptic equilibria). However many efforts have made perturbation theory results suitable to such systems (7–9).

5. Analyticity is sufficient.

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