Geodesics with Unbounded Speed on Fluctuating Surfaces
Andrew Clarke Universitat Politècnica de Catalunya, Escola d’Enginyeria de Barcelona Est,
Campus Diagonal Besòs, Edifici A (EEBE) Av. Eduard Maristany,
16, 08019 Barcelona, Spain
Аннотация:
We construct
$C^{\infty}$ time-periodic fluctuating surfaces in
$\mathbb R^3$ such that the corresponding non-autonomous geodesic flow has orbits along which the energy, and thus the speed goes to infinity. We begin with a static surface
$M$ in
$\mathbb R^3$ on which the geodesic flow (with respect to the induced metric from
$\mathbb R^3$) has a hyperbolic periodic orbit with a transverse homoclinic orbit. Taking this hyperbolic periodic orbit in an interval of energy levels gives us a normally hyperbolic invariant manifold
$\Lambda$, the stable and unstable manifolds of which have a transverse homoclinic intersection. The surface
$M$ is embedded into
$\mathbb R^3$ via a near-identity time-periodic embedding
$G: M \to \mathbb R^3$. Then the pullback under
$G$ of the induced metric on
$G(M)$ is a time-periodic metric on
$M$, and the corresponding geodesic flow has a normally hyperbolic invariant manifold close to
$\Lambda$, with stable and unstable manifolds intersecting transversely along a homoclinic channel. Perturbative techniques are used to calculate the scattering map and construct pseudo-orbits that move up along the cylinder. The energy tends to infinity along such pseudo-orbits. Finally, existing shadowing methods are applied to establish the existence of actual orbits of the non-autonomous geodesic flow shadowing these pseudo-orbits. In the same way we prove the existence of oscillatory trajectories, along which the limit inferior of the energy is finite, but the limit superior is infinite.
Ключевые слова:
Hamiltonian dynamics, geodesic flow, non-autonomous perturbation, Arnold diffusion, Fermi acceleration
MSC: 37J40 Поступила в редакцию: 01.12.2023
Принята в печать: 13.05.2024
Язык публикации: английский
DOI:
10.1134/S1560354724030018