An Eulerian-Lagrangian Form for the Euler Equations in Sobolev Spaces

preprint2016arXivOpen access

Abstract

In 2000 Constantin showed that the incompressible Euler equations can be written in an "Eulerian-Lagrangian" form which involves the back-to-labels map (the inverse of the trajectory map for each fixed time). In the same paper a local existence result is proved in certain Hölder spaces C1,μC^{1,μ}. We review the Eulerian-Lagrangian formulation of the equations and prove that given initial data in HsH^s for n≥2n\geq2 and s>n2+1s>\frac{n}{2}+1, a unique local-in-time solution exists on the nn-torus that is continuous into HsH^s and C1C^1 into Hs−1H^{s-1}. These solutions automatically have C1C^1 trajectories. The proof here is direct and does not appeal to results already known about the classical formulation. Moreover, these solutions are regular enough that the classical and Eulerian-Lagrangian formulations are equivalent, therefore what we present amounts to an alternative approach to some of the standard theory.

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