2021
DOI: 10.48550/arxiv.2107.06035
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Filamentation near Hill's vortex

Abstract: For the axisymmetric incompressible Euler equations, we prove linear in time filamentation near Hill's vortex: there exists an arbitrary small outward perturbation growing linearly for all times. This is based on combining recent nonlinear orbital stability statement with a dynamical bootstrapping scheme for particle trajectories. These results rigorously confirm numerical simulations by Pozrikidis [45] in 1986.

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Cited by 5 publications
(7 citation statements)
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References 53 publications
(62 reference statements)
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“…Even in the case of T 3 , we are not aware of any results giving infinite vorticity growth for smooth vorticity, not relying on the 2+ 1 2 dimensional geometry (however see [42]). In our previous work, we obtained arbitrarily large but finite growth of ω(t, •) L ∞ in R 3 using perturbations of the Hill's vortex [9]. Very recent numerical computations by Hou suggests finite time singularity for axisymmetric Euler with swirl in the interior of the domain [25].…”
Section: Discussionmentioning
confidence: 94%
See 1 more Smart Citation
“…Even in the case of T 3 , we are not aware of any results giving infinite vorticity growth for smooth vorticity, not relying on the 2+ 1 2 dimensional geometry (however see [42]). In our previous work, we obtained arbitrarily large but finite growth of ω(t, •) L ∞ in R 3 using perturbations of the Hill's vortex [9]. Very recent numerical computations by Hou suggests finite time singularity for axisymmetric Euler with swirl in the interior of the domain [25].…”
Section: Discussionmentioning
confidence: 94%
“…(for solvability, e.g. see Section 2.4 of [9]). Then, along the flow, we have the important Cauchy formula…”
Section: Axisymmetric Flows Without Swirlmentioning
confidence: 99%
“…We remark that the improved stability statements, Theorem 1.2 and Corollary 1.3, are essential in the proof of above instability result. For other works on perimeter growth of perturbations, we refer to [16] for a disk patch, [17] for the Lamb dipole, [15] for the Hill's spherical vortex.…”
Section: Resultsmentioning
confidence: 99%
“…see [35]), there are only a few results on the norm growth for smooth solutions; see references in [9,17]. In our companion work [9] (based on orbital stability [7]), we consider perturbations of the Hill's vortex, which is a traveling-wave solution to the axisymmetric Euler equation supported on the unit ball in R 3 . The Hill's vortex could be seen as the 3D analogue of the Lamb dipole.…”
Section: Previous Workmentioning
confidence: 99%
“…The Hill's vortex could be seen as the 3D analogue of the Lamb dipole. In [9], stability and instability of the Hill's vortex is established using a largely parallel argument as in this work. However, let us point out the main differences: the gradient growth in the current paper is strictly harder to achieve since we face the restriction that the vorticity must vanish on the symmetry axis {x 2 = 0}, for the vorticity to be smooth.…”
Section: Previous Workmentioning
confidence: 99%