z-logo
open-access-imgOpen Access
Periodic orbits and stability islands in chaotic seas created by separatrix crossings in slow-fast systems
Author(s) -
A. A. Vasiliev,
Dmitry Treschev,
Carles Simö,
А. И. Нейштадт
Publication year - 2008
Publication title -
discrete and continuous dynamical systems - b
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.864
H-Index - 53
eISSN - 1553-524X
pISSN - 1531-3492
DOI - 10.3934/dcdsb.2008.10.621
Subject(s) - kinetic energy , phase space , separatrix , physics , hamiltonian system , chaotic , measure (data warehouse) , hamiltonian (control theory) , phase plane , domain (mathematical analysis) , stability (learning theory) , plane (geometry) , classical mechanics , mathematical physics , mathematics , mathematical analysis , magnetic field , geometry , quantum mechanics , nonlinear system , computer science , mathematical optimization , database , artificial intelligence , machine learning
We consider a 2 d.o.f. natural Hamiltonian system with one degree of freedom corresponding to fast motion and the other one corresponding to slow motion. The Hamiltonian function is the sum of potential and kinetic energies, the kinetic energy being a weighted sum of squared momenta. The ratio of time derivatives of slow and fast variables is of order \epsilon « 1. At frozen values of the slow variables there is a separatrix on the phase plane of the fast variables and there is a region in the phase space (the domain of separatrix crossings) where the projections of phase points onto the plane of the fast variables repeatedly cross the separatrix in the process of evolution of the slow variables. Under a certain symmetry condition we prove the existence of many, of order 1/\epsilon, stable periodic trajectories in the domain of the separatrix crossings. Each of these trajectories is surrounded by a stability island whose measure is estimated from below by a value of order \epsilon. Thus, the total measure of the stability islands is estimated from below by a value independent of \epsilon. We find the location of stable periodic trajectories and an asymptotic formula for the number of these trajectories. As an example, we consider the problem of motion of a charged particle in the parabolic model of magnetic field in the Earth magnetotail

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom