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On the implosion of a three dimensional compressible fluid

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arxiv 1912.11009 v2 pith:SWQI6QQO submitted 2019-12-23 math.AP

classification math.AP
keywords compressibleequationsassociateddimensionaleulerself-similarsmoothsolutions
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abstract

We consider the compressible three dimensional Navier Stokes and Euler equations. In a suitable regime of barotropic laws, we construct a set of finite energy smooth initial data for which the corresponding solutions to both equations implode (with infinite density) at a later time at a point, and completely describe the associated formation of singularity. Two essential steps of the analysis are the existence of $\mathcal C^\infty$ smooth self-similar solutions to the compressible Euler equations for quantized values of the speed and the derivation of spectral gap estimates for the associated linearized flow which are addressed in the companion papers \cite{MRRSprofile, MRRSdefoc}. All blow up dynamics obtained for the Navier-Stokes problem are of type II (non self-similar).

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Cited by 2 Pith papers

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  1. Magnetic Stabilization of Compressible Flows: Global Existence in 3D Inviscid Non-Isentropic MHD Equations

    math.AP 2025-07 conditional novelty 6.0 of 10

    Near a generic background magnetic field, small perturbations of the 3D inviscid non-isentropic compressible MHD system on the torus exist globally and decay, unlike the compressible Euler case.

  2. Global solutions to 3D compressible MHD equations with partial magnetic diffusion

    math.AP 2025-05 conditional novelty 6.0 of 10

    For small H3 initial data in R3, the 3D compressible viscous MHD equations with horizontal magnetic diffusion have unique global strong solutions.

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