A remark on omega limit sets for non-expansive dynamics

Fuente: arXiv
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Main Authors: Duvall, Alon, Sontag, Eduardo D.
Format: Preprint
Published: 2024
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author Duvall, Alon
Sontag, Eduardo D.
author_facet Duvall, Alon
Sontag, Eduardo D.
contents In this paper, we study systems of time-invariant ordinary differential equations whose flows are non-expansive with respect to a norm, meaning that the distance between solutions may not increase. Since non-expansiveness (and contractivity) are norm-dependent notions, the topology of $ω$-limit sets of solutions may depend on the norm. For example, and at least for systems defined by real-analytic vector fields, the only possible $ω$-limit sets of systems that are non-expansive with respect to polyhedral norms (such as $\ell^p$ norms with $p =1$ or $p=\infty$) are equilibria. In contrast, for non-expansive systems with respect to Euclidean ($\ell^2$) norm, other limit sets may arise (such as multi-dimensional tori): for example linear harmonic oscillators are non-expansive (and even isometric) flows, yet have periodic orbits as $ω$-limit sets. This paper shows that the Euclidean linear case is what can be expected in general: for flows that are contractive with respect to any strictly convex norm (such as $\ell^p$ for any $p\not=1,\infty$), and if there is at least one bounded solution, then the $ω$-limit set of every trajectory is also an omega limit set of a linear time-invariant system.
format Preprint
id arxiv_https___arxiv_org_abs_2404_02352
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle A remark on omega limit sets for non-expansive dynamics
Duvall, Alon
Sontag, Eduardo D.
Dynamical Systems
In this paper, we study systems of time-invariant ordinary differential equations whose flows are non-expansive with respect to a norm, meaning that the distance between solutions may not increase. Since non-expansiveness (and contractivity) are norm-dependent notions, the topology of $ω$-limit sets of solutions may depend on the norm. For example, and at least for systems defined by real-analytic vector fields, the only possible $ω$-limit sets of systems that are non-expansive with respect to polyhedral norms (such as $\ell^p$ norms with $p =1$ or $p=\infty$) are equilibria. In contrast, for non-expansive systems with respect to Euclidean ($\ell^2$) norm, other limit sets may arise (such as multi-dimensional tori): for example linear harmonic oscillators are non-expansive (and even isometric) flows, yet have periodic orbits as $ω$-limit sets. This paper shows that the Euclidean linear case is what can be expected in general: for flows that are contractive with respect to any strictly convex norm (such as $\ell^p$ for any $p\not=1,\infty$), and if there is at least one bounded solution, then the $ω$-limit set of every trajectory is also an omega limit set of a linear time-invariant system.
title A remark on omega limit sets for non-expansive dynamics
topic Dynamical Systems
url https://arxiv.org/abs/2404.02352