We consider the existence and effective computation of low-dimensional (less independent frequencies than degrees of freedom) invariant tori of a near-integrable system. Lindstedt method is a systematic procedure to compute formal power series expansions of quasi-periodic solutions. This procedure is very suitable for numerical computations. Under some non-degeneracy assumptions it is possible to show that a finite number of this low dimensional tori persist in the sense of formal power series expansions of the perturbation parameter ($\varepsilon$). Contrary to the series for full dimensional tori, whose convergence is established by KAM theory, the convergence of the expansions for low-dimensional tori is not settled -- even if its reason...
Perturbation theory is introduced by means of models borrowed from Celestial Mechanics, namely the t...
Perturbation theory is introduced by means of models borrowed from Celestial Mechanics, namely the t...
Perturbation theory is introduced by means of models borrowed from Celestial Mechanics, namely the t...
We consider the existence and effective computation of low-dimensional (less independent frequencies...
Introduction One of the first methods to compute quasi-periodic orbits (i. e. invariant tori with l...
Quasi-periodic motions on invariant tori of an integrable system of dimension smaller than half the ...
Quasi-periodic motions on invariant tori of an integrable system of dimension smaller than half the...
The parametric equations of the surfaces on which highly resonant quasiperiodic motions develop lowe...
The parametric equations of the surfaces on which highly resonant quasiperiodic motions develop lowe...
We consider a class of a priori stable quasi-integrable analytic Hamiltonian systems and study the r...
The parametric equations of the surfaces on which highly resonant quasi-periodic motions ...
We study elliptic lower dimensional invariant tori of Hamiltonian systems via parameterizations. The...
Perturbation theory is introduced by means of models borrowed from Celestial Mechanics, namely the t...
We study elliptic lower dimensional invariant tori of Hamiltonian systems via parameterizations. Th...
Perturbation theory is introduced by means of models borrowed from Celestial Mechanics, namely the t...
Perturbation theory is introduced by means of models borrowed from Celestial Mechanics, namely the t...
Perturbation theory is introduced by means of models borrowed from Celestial Mechanics, namely the t...
Perturbation theory is introduced by means of models borrowed from Celestial Mechanics, namely the t...
We consider the existence and effective computation of low-dimensional (less independent frequencies...
Introduction One of the first methods to compute quasi-periodic orbits (i. e. invariant tori with l...
Quasi-periodic motions on invariant tori of an integrable system of dimension smaller than half the ...
Quasi-periodic motions on invariant tori of an integrable system of dimension smaller than half the...
The parametric equations of the surfaces on which highly resonant quasiperiodic motions develop lowe...
The parametric equations of the surfaces on which highly resonant quasiperiodic motions develop lowe...
We consider a class of a priori stable quasi-integrable analytic Hamiltonian systems and study the r...
The parametric equations of the surfaces on which highly resonant quasi-periodic motions ...
We study elliptic lower dimensional invariant tori of Hamiltonian systems via parameterizations. The...
Perturbation theory is introduced by means of models borrowed from Celestial Mechanics, namely the t...
We study elliptic lower dimensional invariant tori of Hamiltonian systems via parameterizations. Th...
Perturbation theory is introduced by means of models borrowed from Celestial Mechanics, namely the t...
Perturbation theory is introduced by means of models borrowed from Celestial Mechanics, namely the t...
Perturbation theory is introduced by means of models borrowed from Celestial Mechanics, namely the t...
Perturbation theory is introduced by means of models borrowed from Celestial Mechanics, namely the t...