Remark on the Stability of Energy Maximizers for the 2D Euler equation on $\mathbb{T}^2$

TL;DR

This paper provides a simple, quantitative proof of the $L^2$ stability of energy maximizers for the 2D Euler equation on the torus, highlighting cases of potentially reduced stability.

Contribution

It introduces a new, straightforward method leveraging Casimir conservation to prove stability of single modes, extending classical results.

Findings

Lyapunov stability of energy shells on $ abla^2$

Quantitative estimates for stability bounds

Potential reduced stability in extremal cases

Abstract

It is well-known that the first energy shell, \[\mathcal{S}_1^{c_0}:=\{\alpha \cos(x+\mu)+\beta\cos(y+\lambda): \alpha^2+\beta^2=c_0\,\, \&\,\, (\mu,\lambda)\in\mathbb{R}^2\}\] of solutions to the 2d Euler equation is Lyapunov stable on $\mathbb{T}^2$. This is simply a consequence of the conservation of energy and enstrophy. Using the idea of Wirosoetisno and Shepherd \cite{WS}, which is to take advantage of conservation of a properly chosen Casimir, we give a simple and quantitative proof of the $L^2$ stability of single modes up to translation. In other words, each \[\mathcal{S}_1^{\alpha,\beta}:=\{\alpha \cos(x+\mu)+\beta\cos(y+\lambda): (\mu,\lambda)\in\mathbb{R}^2\}\] is Lyapunov stable. Interestingly, our estimates indicate that the extremal cases $\alpha=0,$ $\beta=0$, and $\alpha=\pm\beta$ may be markedly less stable than the others.