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Stability of Solitary Capillary-Gravity Water Waves in Three Dimensions

Changfeng Gui, Shanfa Lai, Yong Liu, Juncheng Wei, Wen Yang

TL;DR

The paper tackles the conditional orbital stability of fully localized three-dimensional capillary-gravity solitary waves in finite depth, constructed non-variationally via a Lyapunov–Schmidt reduction. By marrying Grillakis–Shatah–Strauss with Mielke's conditional stability framework and exploiting the Hamiltonian structure given by the Dirichlet-to-Neumann operator, it derives a reduced augmented potential and a mixed local–nonlocal linearized operator whose spectral properties drive the stability analysis. In the small-amplitude, high-surface-tension KP-I regime, the authors perform a precise spectral analysis: the rescaled operator converges to a KP-I–type limit with a single negative eigenvalue and a two-dimensional neutral spectrum from translations, while the remainder is positive; they then establish convexity $d''(c)>0$ and construct modulation to obtain conditional orbital stability of the solitary waves, up to horizontal translations. This work extends stability theory to non-variational 3D capillary-gravity waves, linking KP-I lump dynamics with finite-depth water waves and offering a rigorous stability framework for reduction-based solitary waves.

Abstract

This paper establishes the conditional orbital stability of fully localized solitary waves for the three-dimensional capillary-gravity water wave problem in finite depth under strong surface tension. The waves, constructed via a non-variational Lyapunov-Schmidt reduction in [26], are not energy minimizers and thus require a direct stability analysis. We adapt the Grillakis-Shatah-Strauss framework within Mielke's approach to handle the mismatch between well-posedness and energy spaces. The proof relies on spectral analysis of the linearized dynamics and careful treatment of the Hamiltonian structure defined by the energy and momentum functionals.

Stability of Solitary Capillary-Gravity Water Waves in Three Dimensions

TL;DR

The paper tackles the conditional orbital stability of fully localized three-dimensional capillary-gravity solitary waves in finite depth, constructed non-variationally via a Lyapunov–Schmidt reduction. By marrying Grillakis–Shatah–Strauss with Mielke's conditional stability framework and exploiting the Hamiltonian structure given by the Dirichlet-to-Neumann operator, it derives a reduced augmented potential and a mixed local–nonlocal linearized operator whose spectral properties drive the stability analysis. In the small-amplitude, high-surface-tension KP-I regime, the authors perform a precise spectral analysis: the rescaled operator converges to a KP-I–type limit with a single negative eigenvalue and a two-dimensional neutral spectrum from translations, while the remainder is positive; they then establish convexity and construct modulation to obtain conditional orbital stability of the solitary waves, up to horizontal translations. This work extends stability theory to non-variational 3D capillary-gravity waves, linking KP-I lump dynamics with finite-depth water waves and offering a rigorous stability framework for reduction-based solitary waves.

Abstract

This paper establishes the conditional orbital stability of fully localized solitary waves for the three-dimensional capillary-gravity water wave problem in finite depth under strong surface tension. The waves, constructed via a non-variational Lyapunov-Schmidt reduction in [26], are not energy minimizers and thus require a direct stability analysis. We adapt the Grillakis-Shatah-Strauss framework within Mielke's approach to handle the mismatch between well-posedness and energy spaces. The proof relies on spectral analysis of the linearized dynamics and careful treatment of the Hamiltonian structure defined by the energy and momentum functionals.

Paper Structure

This paper contains 6 sections, 16 theorems, 263 equations.

Key Result

Theorem 1.1

Every solitary capillary-gravity water wave $\bar{u}(c)=(\bar{\eta}(c), \bar{\xi}(c))$ with wave speed $c = \frac{1}{\sqrt{1+\varepsilon^2}}$ for $\varepsilon \in (0,\varepsilon_0)$ is conditionally orbitally stable in the following sense: For every $R > 0$ and $\rho > 0$, there exists $\rho_0 > 0$ then for all $t \in [0,T)$,

Theorems & Definitions (33)

  • Theorem 1.1
  • Lemma 2.1
  • proof
  • Lemma 2.2
  • proof
  • Theorem 2.1
  • proof
  • Theorem 2.2
  • proof
  • Proposition 3.1
  • ...and 23 more