On the Stability of the Set of Hyperbolic Closed Orbits of a Hamiltonian

TL;DR

This paper proves that in four-dimensional Hamiltonian systems, the set of hyperbolic closed orbits remains stable under small perturbations, with the dynamics being Anosov if the energy surface has no critical points.

Contribution

It establishes the stability of hyperbolic closed orbits in four-dimensional Hamiltonian systems and characterizes when the energy surface exhibits Anosov dynamics.

Findings

Hamiltonian star levels with no critical points are Anosov.

Existence of nearby energy levels with Anosov flow when critical points are present.

Stability of hyperbolic closed orbits under $C^2$ perturbations.

Abstract

A Hamiltonian level, say a pair $(H,e)$ of a Hamiltonian $H$ and an energy $e \in \mathbb{R}$, is said to be Anosov if there exists a connected component $\mathcal{E}_{H,e}$ of $H^{-1}({e})$ which is uniformly hyperbolic for the Hamiltonian flow $X_H^t$. The pair $(H,e)$ is said to be a Hamiltonian star system if there exists a connected component $\mathcal{E}^\star_{H,e}$ of the energy level $H^{-1}({{e}})$ such that all the closed orbits and all the critical points of $\mathcal{E}^\star_{H,e}$ are hyperbolic, and the same holds for a connected component of the energy level $\tilde{H}^{-1}({\tilde{e}})$, close to $\mathcal{E}^\star_{H,e}$, for any Hamiltonian $\tilde{H}$, in some $C^2$-neighbourhood of $H$, and $\tilde{e}$ in some neighbourhood of $e$. In this article we prove that for any four-dimensional Hamiltonian star level $(H,e)$ if the surface $\mathcal{E}^\star_{H,e}$ does not contain critical points, then $X_H^t|_{\mathcal{E}^\star_{H,e}}$ is Anosov; if $\mathcal{E}^\star_{H,e}$ has critical points, then there exists $\tilde{e}$, arbitrarily close to $e$, such that $X_H^t|_{\mathcal{E}^\star_{H,\tilde{e}}}$ is Anosov.