English

Growth estimates for axisymmetric Euler equations without swirl

Analysis of PDEs 2025-12-16 v1

Abstract

We consider the axisymmetric Euler equations in R3\mathbb{R}^3 without swirl, and establish several upper and lower bounds for the growth of solutions. On the one hand, we obtain an upper bound t2t^2 for the radial moment R3rωθdx\int_{\mathbb{R}^3} r\omega^\theta dx, which is the conjectured optimal rate by Childress (Phys. D 237(14-17):1921-1925, 2008). On the other hand, for all initial data satisfying certain symmetry and sign conditions, we prove that the radial moment grows at least like t/logtt/\log t as time goes to infinity, and ω(,t)Lp(R3)\|\omega(\cdot,t)\|_{L^p(\mathbb{R}^3)} exhibits at least t1/4t^{1/4} growth in the limsup sense for all 1p1\leq p\leq \infty. To the best of our knowledge, this is the first result to establish power-law LpL^p-norm growth for smooth, compactly supported initial vorticity in R3\mathbb{R}^3. For these initial data, we also show that nearly all vorticity must eventually escape to rr\to\infty in the time-integral sense.

Cite

@article{arxiv.2512.13456,
  title  = {Growth estimates for axisymmetric Euler equations without swirl},
  author = {Khakim Egamberganov and Yao Yao},
  journal= {arXiv preprint arXiv:2512.13456},
  year   = {2025}
}

Comments

22 pages, 1 figure

R2 v1 2026-07-01T08:25:30.585Z