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Sharp norm inflation for 3D Navier-Stokes equations in supercritical spaces

Xiaoyutao Luo

TL;DR

This work establishes norm inflation and strong ill-posedness for the 3D Navier–Stokes equations in almost all supercritical Besov spaces near the scaling-critical line $s=-1+\tfrac{3}{p}$ (except at $s=0$). The authors build an axisymmetric approximate solution by reducing the dynamics to a stationary radial vortex in the $rz$-plane and a transported swirl component, then induce inflation via two distinct mechanisms: $s>0$ uses mixing to drive a forward energy cascade, while $s<0$ leverages un-mixing to trigger growth in negative regularity norms. A careful stability analysis shows the approximate solution reflects in the full NS flow on a short time window $[0,t^{*}]$, yielding explicit lower bounds on Besov norms and, in particular, arbitrarily large finite-time growth of the vorticity. Together, these results imply strong ill-posedness in broad supercritical regimes and provide a rigorous link between norm inflation, small-scale formation, and rapid vorticity amplification, while highlighting open questions about sustained growth and potential blow-up.

Abstract

We prove that the incompressible Navier-Stokes equations exhibit norm inflation in $\dot B^{s}_{p,q}(\mathbb{R}^3)$ with smooth, compactly supported initial data. Such norm inflation is shown in all supercritical $\dot B^{s}_{p,q} $ near the scaling-critical line $s = -1+ \frac{3}{p}$ except at $s=0$. The growth mechanism differs depending on the sign of the regularity index $s$: forward energy cascade driven by mixing for $s>0$ and backward energy cascade caused by un-mixing for $s<0$. The construction also demonstrates arbitrarily large, finite-time growth of the vorticity, the first of such examples for the Navier-Stokes equations.

Sharp norm inflation for 3D Navier-Stokes equations in supercritical spaces

TL;DR

This work establishes norm inflation and strong ill-posedness for the 3D Navier–Stokes equations in almost all supercritical Besov spaces near the scaling-critical line (except at ). The authors build an axisymmetric approximate solution by reducing the dynamics to a stationary radial vortex in the -plane and a transported swirl component, then induce inflation via two distinct mechanisms: uses mixing to drive a forward energy cascade, while leverages un-mixing to trigger growth in negative regularity norms. A careful stability analysis shows the approximate solution reflects in the full NS flow on a short time window , yielding explicit lower bounds on Besov norms and, in particular, arbitrarily large finite-time growth of the vorticity. Together, these results imply strong ill-posedness in broad supercritical regimes and provide a rigorous link between norm inflation, small-scale formation, and rapid vorticity amplification, while highlighting open questions about sustained growth and potential blow-up.

Abstract

We prove that the incompressible Navier-Stokes equations exhibit norm inflation in with smooth, compactly supported initial data. Such norm inflation is shown in all supercritical near the scaling-critical line except at . The growth mechanism differs depending on the sign of the regularity index : forward energy cascade driven by mixing for and backward energy cascade caused by un-mixing for . The construction also demonstrates arbitrarily large, finite-time growth of the vorticity, the first of such examples for the Navier-Stokes equations.

Paper Structure

This paper contains 30 sections, 17 theorems, 187 equations, 2 figures.

Key Result

Theorem 1.1

For any $s \neq 0$ and $1\leq p,q \leq \infty$ such that $-3 < s - \frac{3}{p} < -1$, the 3D Navier-Stokes equations eq:NS are strongly ill-posed in $\dot B^{s}_{p,q} (\mathbb{R}^3)$ in the following sense. For any $\epsilon>0$, there exists a time $0< t^* \leq \epsilon$ and a solution $u$ of eq:

Figures (2)

  • Figure 1: Left: Supercritical region in light blue. Right: Ill-posedness region of Theorem \ref{['thm:Besov']} in pink
  • Figure 2: Anisotropic setup in $rz$-plane with $\mu^{-1} \ll \nu^{-1}$.

Theorems & Definitions (32)

  • Theorem 1.1
  • Remark 1.2
  • Theorem 1.3
  • Lemma 1.4
  • Proposition 1.5
  • Proposition 2.1
  • Lemma 2.2
  • proof
  • Lemma 2.3
  • proof
  • ...and 22 more