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On geometric hydrodynamics and infinite-dimensional magnetic systems

Levin Maier

Abstract

In this article, we combine V. Arnold's celebrated approach via the Euler-Arnold equation -- describing the geodesic flow on a Lie group equipped with a right-invariant metric \cite{Arnold66} -- with his formulation of the motion of a charged particle in a magnetic field \cite{ar61}. We introduce the \emph{magnetic Euler-Arnold equation}, which is the Eulerian form of the magnetic geodesic flow for an infinite-dimensional magnetic system on a Lie group endowed with a right-invariant metric and a right-invariant closed two-form serving as the magnetic field. As an illustration, we demonstrate that the Korteweg-de Vries equation, the generalized Camassa-Holm equation, the infinite conductivity equation, and the global quasi-geostrophic equations can all be interpreted as magnetic Euler-Arnold equations. In particular, we obtain both local and global well-posedness results for the magnetic Euler-Arnold equation associated with the global quasi-geostrophic equations.

On geometric hydrodynamics and infinite-dimensional magnetic systems

Abstract

In this article, we combine V. Arnold's celebrated approach via the Euler-Arnold equation -- describing the geodesic flow on a Lie group equipped with a right-invariant metric \cite{Arnold66} -- with his formulation of the motion of a charged particle in a magnetic field \cite{ar61}. We introduce the \emph{magnetic Euler-Arnold equation}, which is the Eulerian form of the magnetic geodesic flow for an infinite-dimensional magnetic system on a Lie group endowed with a right-invariant metric and a right-invariant closed two-form serving as the magnetic field. As an illustration, we demonstrate that the Korteweg-de Vries equation, the generalized Camassa-Holm equation, the infinite conductivity equation, and the global quasi-geostrophic equations can all be interpreted as magnetic Euler-Arnold equations. In particular, we obtain both local and global well-posedness results for the magnetic Euler-Arnold equation associated with the global quasi-geostrophic equations.

Paper Structure

This paper contains 18 sections, 15 theorems, 81 equations, 1 table.

Key Result

Lemma 2.3

The magnetic geodesic flow $\varPhi^t_{g,\sigma}$ of $(M,g,\sigma)$ is the Hamiltonian flow induced by the kinetic energy $E\colon TM\to\mathbb{R}$ and the twisted symplectic form where $\lambda$ is the metric pullback of the canonical Liouville $1$-form from $T^*M$ to $TM$, and $\pi_{TM}\colon TM\to M$ is the canonical projection.

Theorems & Definitions (45)

  • Definition 2.1
  • Remark 2.2
  • Lemma 2.3: Gin
  • Definition 2.4
  • Remark 2.5
  • Proposition 2.6
  • Remark 2.7
  • proof
  • Corollary 2.8
  • Theorem 2.9: The magnetic Euler--Arnold equation
  • ...and 35 more