Characterization of three-dimensional Euler flows supported on finitely many Fourier modes

TL;DR

This paper classifies all three-dimensional Euler flows with finitely many Fourier modes, showing they are limited to stationary 2D-like flows and Beltrami flows, extending previous 2D results and exploring effects of viscosity and Coriolis force.

Contribution

It provides a complete classification of 3D Euler solutions with finitely many Fourier modes, revealing their limited types and extending 2D classifications to 3D.

Findings

No non-trivial 3D Euler flows with finitely many Fourier modes exist beyond stationary 2D-like and Beltrami flows.

The classification extends the 2D result by Elgindi-Hu-vere1k (2017) to 3D.

Discussion includes effects of viscosity and Coriolis force on such flows.

Abstract

Recently, the Nash-style convex integration has been becoming the main scheme for the mathematical study of turbulence, and the main building block of it has been either Beltrami flow (finite mode) or Mikado flow (compactly supported in the physical side). On the other hand, in physics, it is observed that turbulence is composed of a hierarchy of scale-by-scale vortex stretching. Thus our mathematical motivation in this study is to find another type of building blocks accompanied by vortex stretching and scale locality (possibly finitely many Fourier modes). In this paper, we give a complete list of solutions to the 3D Euler equations with finitely many Fourier modes, which is an extension of the corresponding 2D result by Elgindi-Hu-\v{S}ver\'ak (2017). In particular, we show that there is no 3D Euler flows with finitely many Fourier modes, except for stationary 2D-like flows and Beltrami flows. We also discuss the case when viscosity and Coriolis effect are present.