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Vorticity blowup in compressible Euler equations in $\mathbb{R}^d, d \geq 3$

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arxiv 2408.04319 v1 pith:BRPUJYAO submitted 2024-08-08 math.AP physics.flu-dyn

classification math.APphysics.flu-dyn
keywords blowupmathbbvorticitycompressibleequationseulerimplosionnon-radial
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abstract

We prove finite-time vorticity blowup in the compressible Euler equations in $\mathbb{R}^d$ for any $d \geq 3$, starting from smooth, localized, and non-vacuous initial data. This is achieved by lifting the vorticity blowup result from [CCSV24] in $\mathbb{R}^2$ to $\mathbb{R}^d$ and utilizing the axisymmetry in $\mathbb{R}^d$. At the time of the first singularity, both vorticity blowup and implosion occur on a sphere $S^{d-2}$. Additionally, the solution exhibits a non-radial implosion, accompanied by a stable swirl velocity that is sufficiently strong to initially dominate the non-radial components and to generate the vorticity blowup.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Blow-up of the 3-D compressible Navier-Stokes equations for monatomic gases

    math.AP 2025-01 conditional novelty 8.0 of 10

    For gamma = 5/3, corresponding to a monatomic gas, there exist smooth initial data for which the 3-D compressible Navier-Stokes equations blow up in finite time in a self-similar implosion.

  2. Gradient catastrophes and an infinite hierarchy of H\"older cusp-singularities for 1D Euler

    math.AP 2024-12 conditional novelty 8.0 of 10

    For every integer n>=1, smooth 1D Euler data can form a pre-shock cusp with Holder exponent 1/(2n+1), and the set of such data is a codimension-(2n-2) Banach manifold in W^{2n+2,infinity}.

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