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From Instability to Singularity Formation in Incompressible Fluids
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abstract
We establish finite-time singularity formation for $C^{1,\alpha}$ solutions to the Boussinesq system that are compactly supported on $\mathbb{R}^2$ and infinitely smooth except in the radial direction at the origin. The solutions are smooth in the angular variable at the blow-up point, which was a fundamental obstruction in previous works. This is done by exploiting a second-order effect, related to the classical Rayleigh--B\'enard instability, that overcomes the regularizing effect of transport. A similar result is established for the 3d Euler system based on the Taylor--Couette instability.
Forward citations
Cited by 4 Pith papers
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Instabilities of internal gravity waves in the two-dimensional Boussinesq system
Small-amplitude plane internal waves in the 2D inviscid Boussinesq system are proven to be spectrally unstable via a rigorous Floquet-Bloch analysis.
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There exist compactly supported, smooth-before-blow-up solutions of the forced 2D Boussinesq equation that blow up in finite time with a uniformly C^{1,alpha} cap L^2 force for every alpha < sqrt(4/3)-1.
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On putative self-similarity for incompressible 3D Euler
Self-similar blow-up exponents for 3D Euler are shown to satisfy γ≥2/5 for finite-energy solutions and γ≥1/2 for globally self-similar profiles with outgoing or axisymmetric nodal conditions.
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Analytic finite-rank corrections for singularly weighted estimates in a computer-assisted proof of 3D Euler singularity
Analytic low-rank corrections convert numerically determined global basis functions into exactly vanishing local modes, enforcing |x|^3 vanishing conditions needed for singular weighted stability estimates in computer...
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