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Magnetically Induced Rotating Rayleigh-Taylor Instability
Published on: March 3, 2017
Isolated steady solutions of the 3D Euler equations
Alberto Enciso1, Willi Kepplinger2, Daniel Peralta-Salas1
1Instituto de Ciencias Matemáticas, Consejo Superior de Investigaciones Cientí ficas, Madrid 28049, Spain.
Abstract:
We show that there exist closed three-dimensional Riemannian manifolds where the incompressible Euler equations exhibit smooth steady solutions that are isolated in the C1-topology. The proof of this fact combines ideas from dynamical systems, which appear naturally because these isolated states have strongly chaotic dynamics, with techniques from spectral geometry and contact topology, which can be effectively used to analyze the steady Euler equations on carefully chosen Riemannian manifolds. Interestingly, much of this strategy carries over to the Euler equations in Euclidean space, leading to the weaker result that there exist analytic steady solutions on [Formula: see text] such that the only analytic steady Euler flows in a C1-neighborhood must belong to a certain linear space of dimension six. For comparison, note that in any C-neighborhood of a shear flow, there are infinitely many linearly independent analytic shears.
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