Abstract
We address the local existence and uniqueness of solutions for the 3D Euler equations with a free interface. We prove the local well-posedness in the rotational case when the initial datum \(u_0\) satisfies \(u_0\in H^{2.5+\delta }\) and , where \(\delta >0\) is arbitrarily small, under the Taylor condition on the pressure.
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Acknowledgments
I.K. was supported in part by the NSF Grant DMS-1311943, while V.V. was supported in part by the A.P. Sloan fellowship and the NSF Grants DMS-1348193 and DMS-1514771.
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Appendix
Appendix
For convenience, we provide here two proofs of the Cauchy invariance identity
The first proof, which establishes also the Weber formula, is from [10, 19, 51], however rewritten in the coordinate notation used in the present paper. The second proof, which we believe is new, is shorter and bypasses the Weber formula.
Proof 1 We start with the Weber formula [12, 44]
which is proven as follows. The left side equals
where we used
Applying the curl operator to the identity (6.2), rewritten as
we get
Note that
since
using \(\partial _{jk}=\partial _{kj}\) in the first equality and \(\epsilon _{ijk}=-\epsilon _{ikj}\) in the second. By (6.6) and (6.7), we obtain
The expression in parentheses at \(t=0\) equals
and thus (6.1) follows.
Proof 2 Taking the time derivative, we obtain
where we replaced \(v^{m}_{t}\) by \(-a^{l}_{m}\partial _{l} q\) using the Euler equation. Now, by \(\partial _{j} a^{l}_{m} = a^{l}_{s} \partial _{jr}\eta ^{s} a^{r}_{m} \), which follows by differentiating \(a:\nabla \eta =I\), we get
where we used in the second equality \(a:\nabla \eta =I\). Hence,
and the proof of (6.1) is concluded.
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Kukavica, I., Tuffaha, A. & Vicol, V. On the Local Existence and Uniqueness for the 3D Euler Equation with a Free Interface. Appl Math Optim 76, 535–563 (2017). https://doi.org/10.1007/s00245-016-9360-6
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DOI: https://doi.org/10.1007/s00245-016-9360-6