Pseudo-synchronous solutions for dissipative non-autonomous systems

TL;DR

This paper proves the existence of pseudo-synchronous quasi-periodic solutions in dissipative, non-autonomous systems with finite-order non-resonance conditions, extending KAM theory to systems with small dissipation and polynomial perturbations.

Contribution

It introduces a new approach to establish quasi-periodic solutions under finite-order non-resonance conditions without requiring parameter tuning.

Findings

Existence of quasi-periodic solutions with slightly perturbed frequencies.

Applicable to spin-orbit models with dissipation via MacDonald torque.

No uniform perturbation size limit; allows finitely many frequencies.

Abstract

In the framework of KAM theory, the persistence of invariant tori in quasi-integrable systems is proved by assuming a non-resonance condition on the frequencies, such as the standard Diophantine condition or the milder Bryuno condition. In the presence of dissipation, most of the quasi-periodic solutions disappear and one expects, at most, only a few of them to survive together with the periodic attractors. However, to prove that a quasi-periodic solution really exists, usually one assumes that the frequencies still satisfy a Diophantine condition and, furthermore, that some external parameters of the system are suitably tuned with them. In this paper we consider a class of systems on the one-dimensional torus, subject to a periodic perturbation and in the presence of dissipation, and show that, however small the dissipation, if the perturbation is a trigonometric polynomial in the angles and the unperturbed frequencies satisfy a non-resonance condition of finite order, depending on the size of the dissipation, then a quasi-periodic solution exists with slightly perturbed frequencies provided the size of the perturbation is small enough. If on the one hand the maximal size of the perturbation is not uniform in the degree of the trigonometric polynomial, on the other hand all but finitely many frequencies are allowed and there is no restriction arising from the tuning of the external parameters. A physically relevant case, where the result applies, is the spin-orbit model, which describes the rotation of a satellite around its own axis, while revolving on a Keplerian orbit around a planet, in the case in which the dissipation is taken into account through the MacDonald torque.