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Radial symmetry of stationary and uniformly-rotating solutions to the 2D Euler equation in a disc
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abstract
We study the radial symmetry properties of stationary and uniformly rotating solutions of the 2D Euler equation in the unit disc, both in the smooth setting and the patch setting. In the patch setting, we prove that every uniformly rotating patch with angular velocity $\Omega\le 0$ or $\Omega \ge 1/2$ must be radial, where both bounds are sharp. The conclusion holds under the assumption that the rotating patch considered is disconnected, with its boundaries consisting of several Jordan curves. We also show that every uniformly rotating smooth solution $\omega_0$ must be radially symmetric if its angular velocity $\Omega\le \inf \omega_0/2$ or $\Omega\ge \sup \omega_0/2$. The proof is based on the symmetry properties of non-negative solutions to elliptic problems. A newly tailored approach is developed to address the symmetries of non-negative solutions to piecewise coupled semi-linear elliptic equations.
Forward citations
Cited by 2 Pith papers
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On stationary Quasi-Geostrophic Shallow-Water flows
Non-trivial m-fold doubly-connected stationary vortex patches are proven to exist for the quasi-geostrophic shallow-water equations via bifurcation from annuli.
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Remarks on radial symmetry of stationary and uniformly-rotating solutions for the 2D Euler equation
Uniformly rotating 2D Euler solutions with compactly supported vorticity are forced to be radially symmetric whenever the angular velocity lies outside half the range of the vorticity, including irregular vortex patches.
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