Benjamin-Feir instability of Stokes waves in finite depth
| Autor: | Berti, Massimiliano, Maspero, Alberto, Ventura, Paolo |
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| Rok vydání: | 2022 |
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| Druh dokumentu: | Working Paper |
| Popis: | Whitham and Benjamin predicted in 1967 that small-amplitude periodic traveling Stokes waves of the 2d-gravity water waves equations are linearly unstable with respect to long-wave perturbations, if the depth $\mathtt h$ is larger than a critical threshold $\mathtt h_{WB} \approx 1.363$. In this paper we completely describe, for any value of $\mathtt h > 0$, the four eigenvalues close to zero of the linearized equations at the Stokes wave, as the Floquet exponent $\mu$ is turned on. We prove in particular the existence of a unique depth $\mathtt h_{WB}$, which coincides with the one predicted by Whitham and Benjamin, such that, for any $0 < \mathtt h < \mathtt h_{WB}$, the eigenvalues close to zero remain purely imaginary and, for any $\mathtt h > \mathtt h_{WB}$, a pair of non-purely imaginary eigenvalues depicts a closed figure "8", parameterized by the Floquet exponent. As $\mathtt h \to \mathtt h_{WB}^+$ this figure "8" collapses to the origin of the complex plane. The proof combines a symplectic version of Kato's perturbative theory to compute the eigenvalues of a $4 \times 4$ Hamiltonian and reversible matrix, and KAM inspired transformations to block-diagonalize it. The four eigenvalues have all the same size $O(\mu)$ - unlike the infinitely deep water case in [6]- and the correct Benjamin-Feir phenomenon appears only after one non-perturbative block-diagonalization step. In addition one has to track, along the whole proof, the explicit dependence of the entries of the $4 \times 4$ reduced matrix with respect to the depth $\mathtt h$. Comment: 47 pages, 5 figures, revised introduction. arXiv admin note: substantial text overlap with arXiv:2109.11852 |
| Databáze: | arXiv |
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