The Hopf--Rinow Theorem and Mañé's Critical Value for Magnetic Geodesics on Half Lie-Groups
Levin Maier, Francesco Ruscelli
TL;DR
The work extends the Hopf–Rinow theorem to magnetic geodesic flows on infinite-dimensional half-Lie groups with right-invariant metrics and closed 2-forms. It introduces Mañé's critical value on the universal cover and shows that above this energy threshold the lifted flow becomes a Randers-type Finsler geodesic flow, yielding a complete metric structure and global magnetic exponential. The authors prove magnetically geodesic completeness and the existence of energy-preserving, action-minimizing magnetic geodesics between any pair of points, with these results persisting for $G^{\ell}$ and accommodating Sobolev-diffeomorphism groups as key examples. The framework recovers known finite-dimensional results in the $\sigma=0$ case and provides a robust infinite-dimensional analogue via variational methods and a careful treatment of regularity and invariance properties. These results have implications for geometric hydrodynamics and the study of magnetic Euler–Arnold equations on diffeomorphism groups.
Abstract
In this article, we investigate \emph{right-invariant magnetic systems} on half-Lie groups, which consist of a strong right-invariant Riemannian metric and a right-invariant closed two-form. The main examples are groups of $H^s$ or $C^k$ diffeomorphisms of compact manifolds. In this setting, we define \emph{Mañé's critical value} on the universal cover for weakly exact right-invariant magnetic fields. First, we prove that the lift of the magnetic flow to the universal cover coincides with a Finsler geodesic flow for energies above this threshold. Finally, we show that for energies above Mañé's critical value, the full Hopf--Rinow theorem holds for such magnetic systems, thereby generalizing the work of Contreras and Merry from closed finite-dimensional manifolds to this infinite-dimensional context. Our work extends the recent results of Bauer, Harms, and Michor from geodesic flows to magnetic geodesic flows.
