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Sharp local well-posedness for KP-I equations in the semilinear regime

Published online by Cambridge University Press:  03 March 2026

Shinya Kinoshita
Affiliation:
Graduate School of Mathematics, Nagoya University , Furo-cho, Chikusa-ku, Nagoya, 464-8602, Japan; E-mail: kinoshita@math.nagoya-u.ac.jp
Akansha Sanwal
Affiliation:
Institut für Mathematik, Universität Innsbruck , Technikerstraße 13, 6020 Innsbruck, Austria; E-mail: akansha.sanwal@uibk.ac.at
Robert Schippa*
Affiliation:
Department of Mathematics, UC Berkeley , Evans Hall, Berkeley, CA 94720-3840, USA
*
E-mail: rschippa@berkeley.edu (Corresponding author)

Abstract

We show sharp well-posedness with analytic data-to-solution mapping in the semilinear regime for dispersion-generalized KP-I equations on $\mathbb {R}^2$ and $\mathbb {R} \times \mathbb {T}$. On $\mathbb {R}^2$ we cover the full subcritical range, whereas on $\mathbb {R} \times \mathbb {T}$ the sharp well-posedness is strictly subcritical. We rely on linear and bilinear Strichartz estimates which are proved using decoupling techniques and square function estimates. Nonlinear Loomis-Whitney inequalities are a further ingredient. These are presently proved for Borel measures with growth condition reflecting the different geometries of the plane $\mathbb {R}^2$, the cylinder $\mathbb {R} \times \mathbb {T}$, and the torus $\mathbb {T}^2$. Finally, we point out that on tori $\mathbb {T}^2_\gamma $, KP-I equations are never semilinear.

Information

Type
Analysis
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© The Author(s), 2026. Published by Cambridge University Press

1 Introduction

1.1 Dispersion-generalized KP-I equations

In this article, we show new low regularity well-posedness for the dispersion-generalized Kadomtsev Petviashvili-I (KP-I) equations:

(1.1) $$ \begin{align} \left\{ \begin{array}{@{}cl} \partial_t u - \partial_x D_x^\alpha u - \partial_{x}^{-1} \partial_{y}^2 u &= u \partial_x u, \quad (t,x,y) \in \mathbb{R} \times \mathbb{D}, \\ u(0) &= u_0, \end{array} \right. \end{align} $$

where $\mathbb {D} = \mathbb {R} \times \mathbb {K}$ , $\mathbb {K} \in \{ \mathbb {R} , \mathbb {T} = \mathbb {R} /(2 \pi \mathbb {Z}) \}$ , and $\alpha \geqslant 2$ . The dual variables of $(t,x,y)$ are denoted by $(\tau ,\xi ,\eta )$ . We define $\partial _x^{-1}$ and $D_x^\alpha $ on $\mathbb {D}$ as Fourier multipliers

$$ \begin{align*} \widehat{(\partial_x^{-1} f)} (\xi,\eta) = (i \xi)^{-1} \hat{f}(\xi,\eta), \quad \widehat{(D_x^{\alpha} f)} (\xi,\eta)= |\xi|^{\alpha} \hat{f}(\xi,\eta). \end{align*} $$

By local well-posedness, we refer to the existence, uniqueness, and continuity of the data-to-solution mapping assigning initial data from suitable Sobolev spaces to continuous curves on time intervals

$$ \begin{align*} S_T : H^{s,0}(\mathbb{D}) \to X_T \hookrightarrow C([0,T], H^{s,0}(\mathbb{D})), \quad u_0 \mapsto u \end{align*} $$

with $T=T(\| u_0 \|_{H^{s,0}})$ depending lower semicontinuously on the norm of the initial data and $T(u) \gtrsim 1$ for $u \downarrow 0$ . In this article, we are concerned with semilinear well-posedness when the solution mapping is real-analytic. This is the case upon constructing the solution mapping via Picard iteration as a consequence of the real analyticity of the nonlinearity. The evolution is referred to as quasilinear if the data-to-solution mapping fails to be real analytic.

1.2 Derivation and applications

For $\alpha = 2$ , (1.1) becomes the original KP-I equation. The KP equations were introduced by Kadomtsev and Petviashvili to model two-dimensional water waves (see [Reference Borisovich Kadomtsev and Petviashvili24] and [Reference Ablowitz and Segur1]) with an emphasis on the transverse stability of solitons of the Korteweg-de Vries (KdV) equation:

$$ \begin{align*} \partial_t u + \partial_{x}^3 u = u \partial_x u. \end{align*} $$

The KdV equation is a one-dimensional model of traveling waves in shallow water. Adding the weakly transverse approximation of the wave dispersion relation

$$ \begin{align*} \omega_{\Box}(\xi,\eta) = \pm (\xi^2 + \eta^2)^{\frac{1}{2}} = \pm \xi \Big(1 + \frac{\eta^2}{ 2 \xi^2}\Big) + \mathcal{O}\Big(\frac{\eta^4}{\xi^3}\Big), \quad \xi> 0 \end{align*} $$

to the KdV equation results in the KP evolution after changing the system of rest and mild dilation:

(1.2) $$ \begin{align} \partial_t u + \partial_x^3 u + \kappa \partial_{x}^{-1} \partial_{y}^2 u = u \partial_x u, \quad \kappa \in \{1; - 1 \}. \end{align} $$

For $\kappa = -1$ the equation is known as KP-I equation, and for $\kappa =1$ the equation is referred to as KP-II. The former corresponds to strong surface tension and the latter models the weak surface tension case. Similarly, starting from dispersion-generalized versions of the KdV equation:

$$ \begin{align*} \partial_t u + \partial_x D_x^\alpha u = u \partial_x u, \quad \alpha \geqslant 2, \end{align*} $$

and adding the weakly transverse perturbation leads to the dispersion-generalized KP equations:

$$ \begin{align*} \partial_t u + \partial_x D_x^\alpha u + \kappa \partial_x^{-1} \partial_y^2 u = u \partial_x u. \end{align*} $$

For instance, for higher dispersion, the Kawahara equation [Reference Kawahara25, Reference Sprenger, Bridges and Shearer45]

$$ \begin{align*} \partial_t u + u\partial_x u + \alpha \partial_x^3 u + \partial_x^5 u=0 \end{align*} $$

is a model for shallow water waves when the surface tension and gravity effects are comparable (controlled by the parameter $\alpha $ ). Adding a weakly transverse perturbation leads to the fifth-order KP equations. For further reading, we refer to the recent monograph by Klein–Saut [Reference Klein and Saut31, Chapter 5].

In this paper, we are only concerned with the analysis of the dispersion-generalized KP-I equations. The dispersion relation in this case is given by

$$ \begin{align*} \omega_\alpha(\xi,\eta) = \xi |\xi|^\alpha + \frac{\eta^2}{\xi}. \end{align*} $$

The behavior of solutions to KP-II equations deviates significantly due to a nonlinear defocusing effect absent in the KP-I case, see below. We note that both KP equations (1.2) are known to be completely integrable as proved in [Reference Dryuma12].

Furthermore, it is known that the KdV soliton:

$$ \begin{align*} S_c(t,x) = cQ(\sqrt{c}(x-ct)), c>0, \quad Q(x) = 3 \, \mathrm{sech}^2 \big( {\frac{x}{2}} \big). \end{align*} $$

is known to be orbitally unstable as a solution to the KP-I equation for $c>\frac {4}{\sqrt {3}}$ but is stable in the case $c<\frac {4}{\sqrt {3}}$ as shown in [Reference Rousset and Tzvetkov39, Reference Rousset and Tzvetkov40]. We hope that with the semilinear analysis completed in the present paper stability of line solitons for dispersion-generalized KP-I equations can be analyzed in the future.

Lastly, we remark on the higher dimensional variants of the KP equations, namely with $\partial _x^{-1}\partial _y^2$ replaced by $\partial _x^{-1}\Delta _y$ . The connection with the Gross–Pitaevskii equation

$$ \begin{align*} i\partial_t \psi + \Delta \psi + \psi(1-|\psi|^2) = 0 \end{align*} $$

in the long wave transonic limit has been pointed out in [Reference Béthuel, Gravejat and Saut7]. The second and third author obtained jointly with S. Herr well-posedness results for the three-dimensional KP equations on different domains in [Reference Herr, Sanwal and Schippa20].

1.3 Known results

Owing to their physical relevance, the KP equations have been extensively studied. In the following, we recall some results for the well-posedness of the KP-I equations. Using standard energy methods, in [Reference Ukai47, Reference jun and Nunes23], it is proved that the KP equations are well-posed in Sobolev spaces of high regularity. In [Reference Molinet, Saut and Tzvetkov35], Molinet–Saut–Tzvetkov prove local well-posedness for the KP-I equations in $L^2$ -based Sobolev spaces $H^s(\mathbb {R}^2)$ for $s>2$ . The same authors in [Reference Molinet, Saut and Tzvetkov35] prove global well-posedness for the KP-I equation for initial data related to the “second energy” for the KP-I equation. In a seminal contribution Ionescu–Kenig–Tataru [Reference Ionescu, Kenig and Tataru22] showed global well-posedness for the KP-I equation in the first energy space using short-time Fourier restriction. Local well-posedness in larger spaces of initial data was proved in [Reference Guo, Peng and Wang17, Reference Guo and Molinet15, Reference Guo14]; see also our companion paper [Reference Kinoshita, Sanwal and Schippa29]. For results on the dispersion-generalized equations we refer to our paper [Reference Sanwal and Schippa41] and references therein.

For the KP-I equation posed on the cylinder T. Robert [Reference Robert38] showed global well-posedness in the energy space. On the torus Zhang [Reference Zhang48] showed local well-posedness in the Besov-energy space. Both results are based on short-time Fourier restriction.

1.4 More about KP equations

On $\mathbb {R}^2$ we observe that for any solution u to (1.1) with initial data $\phi $ the rescalings

$$ \begin{align*} u_\lambda(t,x,y) = \lambda^{-\alpha} u(\lambda^{-(\alpha+1)}t, \lambda^{-1} x, \lambda^{-\frac{\alpha+2}{2}} y) \end{align*} $$

solve (1.1) with initial data

$$ \begin{align*} \phi_\lambda(x,y)= \lambda^{-\alpha} \phi(\lambda^{-1} x, \lambda^{-\frac{\alpha+2}{2}} y). \end{align*} $$

Let $\dot {H}^{s_1,s_2}(\mathbb {R}^2)$ denote the anisotropic homogeneous Sobolev space with norm

$$ \begin{align*} \| f \|^2_{\dot{H}^{s_1,s_2}(\mathbb{R}^2)} = \int_{\mathbb{R}^2} |\xi|^{2s_1} |\eta|^{2s_2} |\hat{f}(\xi,\eta)|^2 d\xi d\eta. \end{align*} $$

We compute

$$ \begin{align*} \| \phi_\lambda \|_{\dot{H}^{s_1,s_2}(\mathbb{R}^2)} = \lambda^{-\frac{3 \alpha}{4} + 1 - s_1 - \big( \frac{\alpha}{2}+ 1 \big) s_2 } \| \phi \|_{\dot{H}^{s_1,s_2}(\mathbb{R}^2)}. \end{align*} $$

In the scale of the anisotropic Sobolev spaces with $s_2 = 0$ , this distinguishes $\dot {H}^{s_c,0}$ with $s_c = 1 - \frac {3 \alpha }{4}$ as scaling critical space. Moreover, $s_2 = 0$ is distinguished as this is the lowest regularity in the y-variable, which still respects the Galilean invariance:

$$ \begin{align*} \eta \to \eta + A \xi. \end{align*} $$

For $\alpha \in \mathbb {R}$ , we have the following conserved quantities for real-valued solutions:

(1.3) $$ \begin{align} M(u)(t) &= \int_{\mathbb{D}} u^2(x,y) dx dy, \end{align} $$
(1.4) $$ \begin{align} E_\alpha(u)(t) &= \int_{\mathbb{D}} \big( \frac{1}{2} |D_x^{\frac{\alpha}{2}} u|^2 + \frac{1}{2} |\partial_{x}^{-1} \partial_y u|^2 + \frac{1}{6} u^3 \big) dx dy. \end{align} $$

The energy space is given by

$$ \begin{align*} E^{\frac{\alpha}{2}}(\mathbb{D}) = \Big\{ \phi \in L^2(\mathbb{D}) : \Big\| \big(1+|\xi|^{\frac{\alpha}{2}} + \frac{|\eta|}{|\xi|} \big) \hat{\phi}(\xi,\eta)\Big \|_{L^2} < \infty \Big\}. \end{align*} $$

Since the energy spaces are smaller spaces than the anisotropic Sobolev spaces, we opt to work in the anisotropic Sobolev spaces $H^{s,0}$ , which are defined by

$$ \begin{align*} H^{s,0}(\mathbb{D}) = \{ f \in L^2(\mathbb{D}) : \| \langle \xi \rangle^{s}\hat{f}(\xi,\eta) \|_{L^2_{\xi,\eta}} < \infty \}. \end{align*} $$

1.5 Nonlinear evolution: Resonance and transversality considerations

We shall construct solutions in Fourier restriction spaces [Reference Bourgain8, Reference Bourgain9] with norms given by:

$$ \begin{align*} \| u \|^2_{X^{s,b}} = \int_{\mathbb{R} \times \mathbb{D}^*} \langle \xi \rangle^{2s} \langle \tau - \omega_\alpha(\xi,\eta) \rangle^{2b} |\mathcal{F}_{t,x,y} u(\tau,\xi,\eta) |^2 d \tau d \xi d\eta. \end{align*} $$

The weight in Fourier space $\langle \tau - \omega _\alpha (\xi ,\eta ) \rangle ^b$ penalizes the deviation from free solutions and becomes effective for $b> \frac {1}{2}$ . The resonance function quantifies how plane wave solutions can superimpose to another plane wave solution and is given by

$$ \begin{align*} \begin{aligned} \Omega_\alpha(\xi_1,\eta_1,\xi_2,\eta_2) &= \omega_\alpha(\xi_1+\xi_2,\eta_1+\eta_2) - \omega_\alpha(\xi_1,\eta_1) - \omega_\alpha(\xi_2,\eta_2) \\ &= \underbrace{(\xi_1+\xi_2) |\xi_1+\xi_2|^\alpha - \xi_1 |\xi_1|^\alpha - \xi_2 |\xi_2|^\alpha}_{\Omega_{\alpha,1}(\xi_1,\xi_2)} - \frac{(\eta_1 \xi_2 - \eta_2 \xi_1)^2}{\xi_1 \xi_2 (\xi_1+\xi_2)}. \end{aligned} \end{align*} $$

Estimates in Fourier restriction norms allow us to recover $|\Omega _{\alpha }|^{-\frac {1}{2}}$ in the borderline case $b=\frac {1}{2}$ . For KP-I equations we need to consider the possibility

(1.5) $$ \begin{align} |\Omega_\alpha(\xi_1,\eta_1,\xi_2,\eta_2)| \ll |\Omega_{\alpha,1}(\xi_1,\xi_2)|, \end{align} $$

and consequently, for $\alpha =2$ we cannot recover the derivative loss in a High $\times $ Low-interaction (with regard to the x-frequencies) through the resonance. Indeed, Molinet–Saut–Tzvetkov [Reference Molinet, Saut and Tzvetkov36] showed that the data-to-solution mapping of the KP-I equation on $\mathbb {R}^2$ is not in $C^2$ in any anisotropic Sobolev space.

We shall see that in case (1.5) holds, we have

$$ \begin{align*} \Big| \frac{(\eta_1 \xi_2 - \eta_2 \xi_1)^2}{\xi_1 \xi_2 (\xi_1+\xi_2)} \Big| \sim \big| \Omega_{\alpha,1}(\xi_1,\xi_2) \big|, \end{align*} $$

and we obtain favorable bounds for the full transversality. This allows us to obtain trilinear smoothing estimates as a consequence of nonlinear Loomis–Whitney inequalities, on which we elaborate in Section 1.6. The trilinear smoothing estimate for the KP-I equation was a key ingredient to show global well-posedness of the KP-I equation in the energy space [Reference Ionescu, Kenig and Tataru22]. The analysis in [Reference Ionescu, Kenig and Tataru22] combined Fourier restriction arguments with frequency-dependent time localization and energy methods.

Further tools to control the nonlinear evolution are linear and bilinear Strichartz estimates. The basic bilinear Strichartz estimates follow from transversality arguments (see Proposition 4.1, Lemma 4.3). We shall see that in case of small transversality, we can use a variant of the Córdoba–Fefferman square function estimate, which leads to refined bilinear Strichartz estimates (see Lemma 4.4).

Sharp linear Strichartz estimates on $\mathbb {R}^2$ are well-known ([Reference Hadac18]). On $\mathbb {R} \times \mathbb {T}$ we show linear Strichartz estimates using $\ell ^2$ -decoupling for elliptic hypersurfaces due to Bourgain–Demeter [Reference Bourgain and Demeter10]. Increasing the dispersion parameter $\alpha $ on $\mathbb {R} \times \mathbb {T}$ , we point out how $\ell ^2$ -decoupling captures a smoothing effect, which is not observed in the fully periodic case. Increasing $\alpha $ the resonance relation and the nonlinear Loomis–Whitney inequality become likewise more favorable and on $\mathbb {R}^2$ and $\mathbb {R} \times \mathbb {T}$ , the evolution becomes semilinear for large $\alpha $ . This is described in Subsection 1.7.

We remark that the preceding description to control the nonlinear evolution does not depend on the underlying geometry $\mathbb {R}^2$ or $\mathbb {R} \times \mathbb {T}$ . It is one purpose of the present work to emphasize robust perturbative methods to control nonlinear interactions and to compare the influence of the different geometries on the (multi)linear Strichartz estimates, which are presently described in a unified way.

1.6 Nonlinear Loomis–Whitney inequalities with general measure

The nonlinear Loomis-Whitney inequalities are convolution inequalities for functions supported on the Pontryagin dual

$$ \begin{align*} \mathbb{R} \times \mathbb{D}^* = (\mathbb{R} \times \mathbb{K}_1 \times \mathbb{K}_2)^* \text{ with } \mathbb{R}^* = \mathbb{R} \text{ and } \mathbb{T}^* = \mathbb{Z}. \end{align*} $$

The literature on Loomis–Whitney inequalities and the related Brascamp–Lieb inequalities is vast, and the following list of references is by no means exhaustive. We refer the interested reader to the references therein ([Reference Bennett, Carbery and Wright6, Reference Bejenaru, Herr and Tataru2, Reference Bennett and Bez4, Reference Kinoshita and Schippa30]) for further reading and to the recent overview by Bennett–Bez [Reference Bennett and Bez5]. However, we remark that most statements in the literature are local and not immediately suitable for application to PDE since the “small” support assumptions on the involved functions are not quantified. We shall be brief here and refer to Subsection 4.2 for precise notions.

Let $(S_i)_{i=1}^3 \subseteq \mathbb {R}^3$ denote $C^{1,\beta }$ -hypersurfaces, $\beta>0$ , which allow for a global graph parametrization. For $x_i \in S_i$ we denote with $\mathfrak {n}_i(x_i)$ the outer unit normal. We suppose that there is $A \geqslant 1$ such that for any $x_i \in S_i$ :

(1.6) $$ \begin{align} A^{-1} \leqslant |\mathfrak{n}_1(x_1) \wedge \mathfrak{n}_2(x_2) \wedge \mathfrak{n}_3(x_3) | \leqslant 1. \end{align} $$

For the (classical) nonlinear Loomis–Whitney inequality we endow $S_i$ with the surface measure. Let $f_i : S_i \to \mathbb {R}$ , $i=1,2,3$ with $S_i \subseteq \mathbb {R}^3$ like above. $S_i$ carries the surface measure $\sigma _i$ , and the global convolution estimate proved in [Reference Kinoshita and Schippa30] reads as follows:

$$ \begin{align*} \int_{S_3} (f_1 * f_2) f_3 d\sigma_3 \lesssim A^{\frac{1}{2}} \prod_{i=1}^3 \| f_i \|_{L^2(S_i)}. \end{align*} $$

For our purposes when applying the convolution estimates, we shall thicken the hypersurfaces and consider functions $f_i \in L^2(S_i(\varepsilon ),d\nu _\gamma )$ , which are supported on the $\varepsilon $ -neighbourhood $S_i(\varepsilon )$ of $S_i$ , where $\nu _\gamma $ is a Borel measure on $\mathbb {R}^3$ , which satisfies for any $r>0$ and $x \in \mathbb {R}^3$ the estimate:

(1.7) $$ \begin{align} \nu_\gamma(B(x,r)) \leqslant C_{\nu} r^\gamma \text{ for } 0 < r \leqslant \varepsilon. \end{align} $$

We formulate the following version of global nonlinear Loomis-Whitney inequalities, which is related to convolution estimates for functions on product spaces.

Theorem 1.1 (Nonlinear Loomis-Whitney inequalities with general measure)

Let $\varepsilon>0$ , $(S_i)_{i=1,2,3}$ be a collection of hypersurfaces, which satisfy Assumption 4.7, $\nu _{\gamma }$ be a Borel measure, which satisfies (1.7), and $f_i \in L^2(S_i(\varepsilon ),d\nu _\gamma )$ , $i=1,2$ . Then the following estimate holds:

(1.8) $$ \begin{align} \| f_1 * f_2 \|_{L^2(S_3(\varepsilon),d\nu_\gamma)} \lesssim A^{\frac{1}{2}} \varepsilon^{\frac{\gamma}{2}} \prod_{i=1}^2 \| f_i \|_{L^2(S_i(\varepsilon),d\nu_\gamma)}. \end{align} $$

Its proof uses almost orthogonal decompositions like in [Reference Kinoshita and Schippa30]. Interestingly, the constant in the estimate (1.8) does not depend on the regularity parameters b, $\beta $ of $(S_i)_{i=1,2,3}$ from Assumption 4.7, but it depends only on the constant $C_\nu $ from (1.7).

1.7 Sharp local well-posedness results

Here we state the new results concerning the well-posedness of KP-I equations. We emphasize that the arguments described above per se do not depend on the geometry, but the constants in the linear and multilinear estimates depend on the geometry.

1.7.1 Euclidean geometry

The second and third author considered KP-I equations (1.1) on $\mathbb {R}^2$ for $2<\alpha <4$ in [Reference Sanwal and Schippa41]. The analysis combined the nonlinear Loomis-Whitney inequality, bilinear Strichartz estimates, and frequency-dependent time localization in the quasilinear regime. In the present work we improve the estimate in the resonant case by using bilinear Strichartz estimates, which allows us to cover the full subcritical range.

We summarize our results improving on [Reference Sanwal and Schippa41]. More detailed statements are provided in Theorems 5.2 and 6.1.

Theorem 1.2. Let $\alpha \geqslant \frac {5}{2}$ , $\mathbb {D} = \mathbb {R}^2$ , and $s^*(\alpha ) = 1- \frac {3\alpha }{4}$ . (1.1) is locally well-posed for complex-valued initial data in $H^{s,0}(\mathbb {D})$ for $s> s^*(\alpha )$ . For real-valued initial data (1.1) is globally well-posed in $L^2(\mathbb {D})$ . For $\alpha < \frac {5}{2}$ the data-to-solution mapping for (1.1), if it exists, fails to be $C^2$ from $H^{s_1,s_2}(\mathbb {R}^2)$ to $H^{s_1,s_2}(\mathbb {R}^2)$ , $(s_1,s_2)\in \mathbb {R}^2$ .

1.7.2 Partially periodic geometry

Secondly, we consider (1.1) posed on the cylinder $\mathbb {D} = \mathbb {R} \times \mathbb {T}$ . Special attention in the derivation of KP-equations [Reference Borisovich Kadomtsev and Petviashvili24] was paid to stability of the line soliton, which makes the domain $\mathbb {D} = \mathbb {R} \times \mathbb {T}$ interesting.

The dispersive effects on $\mathbb {D} = \mathbb {R} \times \mathbb {T}$ are decreased compared to the Euclidean case. We obtain a critical dispersion parameter for semilinear well-posedness $\alpha _c = 5$ , which is proved in Theorem 5.3.

By combining Strichartz estimates with nonlinear Loomis-Whitney inequalities with general measure, we obtain local well-posedness sharp up to the endpoints as shown in Theorem 6.3. Notably, the sharp regularity for local well-posedness is strictly above the scaling critical regularity, as proved in Theorem 5.4. The following summarizes Theorems 5.3, 5.4, and 6.3:

Theorem 1.3. Let $\alpha \geqslant 5$ , $\mathbb {D} = \mathbb {R} \times \mathbb {T}$ , and $s^*(\alpha ) = \frac {1-\alpha }{4}$ . (1.1) is locally well-posed for complex-valued initial data in $H^{s,0}(\mathbb {D})$ for $s> s^*(\alpha )$ . For real-valued initial data (1.1) is globally well-posed in $L^2(\mathbb {D})$ . Moreover, (1.1) is ill-posed in $H^{s,0}(\mathbb {R} \times \mathbb {T})$ for $s<s^*(\alpha )$ in the sense that the data-to-solution mapping, if it exists, fails to be continuous. For $\alpha < 5$ , the data-to-solution mapping for (1.1), if it exists, fails to be $C^2$ from $H^{s_1,s_2}(\mathbb {R}\times \mathbb {T})$ to $H^{s_1,s_2}(\mathbb {R}\times \mathbb {T})$ , $(s_1,s_2)\in \mathbb {R}^2$ .

1.8 Further remarks

The presently proved multilinear estimates yield new well-posedness results for the dispersion-generalized KP-I equations exhibiting quasilinear behavior with dispersion parameter $\alpha \geqslant 2$ . Via frequency-dependent time localization as introduced by Ionescu–Kenig–Tataru [Reference Ionescu, Kenig and Tataru22] the second and third author showed improved local well-posedness on $\mathbb {R}^2$ in [Reference Sanwal and Schippa41]. In the companion paper [Reference Kinoshita, Sanwal and Schippa29], we improve the results on $\mathbb {R}^2$ and show new results on $\mathbb {R} \times \mathbb {T}$ .

Lastly, we remark that the methods of the paper yield the corresponding linear and multilinear estimates (see Sections 3.3, 4.2) as well on tori $\mathbb {T}^2_\gamma $ . However, we point out in Theorem 5.5 that KP-I equations are never semilinear on $\mathbb {T}^2_\gamma $ , regardless of the dispersion parameter.

Outline of the paper. In Section 2 we introduce more notations. In Section 3 we show linear Strichartz estimates using $\ell ^2$ -decoupling, and in Section 4 we analyze the interplay between resonance and transversality. In the resonant case we show bilinear Strichartz estimates and show a trilinear estimate based on the nonlinear Loomis–Whitney inequality. Here we moreover compare the nonlinear Loomis–Whitney inequalities on product spaces obtained for dispersion-generalized KP-I equations. In Section 5 we show that the data-to-solution mapping for (1.1) on $\mathbb {R}^2$ cannot be $C^2$ for $\alpha < \frac {5}{2}$ . On $\mathbb {R} \times \mathbb {T}$ the mapping cannot be $C^2$ for $\alpha < 5$ and on $\mathbb {T}^2$ , it cannot be expected to be $C^2$ for any $\alpha $ . Sharp well-posedness results for the semilinear KP-I equations on $\mathbb {R}^2$ and $\mathbb {R} \times \mathbb {T}$ are proved in Section 6.

2 Notations

2.1 Basic conventions

Time and space variables are denoted by $(t,x,y) \in \mathbb {R} \times \mathbb {D}$ , $\mathbb {D} \in \{ \mathbb {R}^2, \mathbb {R} \times \mathbb {T}, \mathbb {T}^2 \}$ . The dual variables are denoted by $(\tau ,\xi ,\eta ) \in \mathbb {R} \times \mathbb {D}^*$ . Capital letters $M,N,L,\ldots $ denote dyadic numbers in $2^{\mathbb {Z}} := \{ \ldots ,1/4,1/2,1,2,4,8,\ldots \}$ . We write $N_+ = \max (1,N)$ . We also denote $a \vee b:=\max (a,b)$ and $a \wedge b:=\min (a,b)$ for $a,b\in \mathbb {R}$ .

2.2 Fourier transform preliminaries

The (spatial) Fourier transform of $f: \mathbb {D} \to \mathbb {C}$ is denoted by

$$ \begin{align*} \hat{f}(\xi,\eta) = (\mathcal{F}_{x,y} f)(\xi,\eta) = \frac{1}{(2\pi)^2} \int_{\mathbb{D}} e^{-i (\xi,\eta)\cdot (x,y)} f(x,y) dx dy. \end{align*} $$

The inverse Fourier transform of $g: \mathbb {D}^* \to \mathbb {C}$ is given by

$$ \begin{align*} f(x,y) = (\mathcal{F}^{-1}_{x,y} g)(x,y) = \frac{1}{(2\pi)^2} \int_{\mathbb{D}^*} e^{i (\xi,\eta)\cdot (x,y)} g(\xi,\eta) d\xi d\eta. \end{align*} $$

The space-time Fourier transform of $u:\mathbb {R} \times \mathbb {D} \to \mathbb {C}$ is obtained from extending the definition to $\mathbb {R} \times \mathbb {D}$ . We abuse notation and denote it as well as $\hat {u}$ . In case $\mathbb {D}^* = \mathbb {R} \times \mathbb {Z}$ we indicate the counting measure by writing $(d \eta )_1$ . When scaling the domain, we also normalize the measure to retain Plancherel’s theorem, namely, we denote the counting measure for $\gamma \in (1/2,\infty )$ by

$$ \begin{align*} \int_{\mathbb{Z}/\gamma} f(\eta)(d\eta)_{\gamma} = \frac{1}{\gamma}\sum_{\eta \in \mathbb{Z}/\gamma} f(\eta). \end{align*} $$

2.3 Littlewood-Paley decompositions

Next, we introduce notations and function spaces for the nonlinear analysis to solve (1.1). Recall that the dispersion relation is given by $\omega _{\alpha }(\xi ,\eta ) = \xi |\xi |^\alpha + \frac {\eta ^2}{\xi }$ . Let $\zeta : \mathbb {R} \to \mathbb {R}$ denote a smooth cutoff, which is radially decreasing and satisfies $\zeta (\tau ) = 1$ for $0\leqslant |\tau | \leqslant 1$ , and $\zeta (\tau ) = 0$ for $|\tau | \geqslant 2$ . We denote $\zeta _{1} = \zeta $ and for $L \in 2^{\mathbb {Z}}$ let $\zeta _L(\tau ) = \zeta (\tau / L) - \zeta (\tau /(L/2))$ . For $N \in 2^{\mathbb {Z}}$ let $A_N = \{ \xi \in \mathbb {R} : N/4 \leqslant |\xi | \leqslant 4N \}$ denote the N-annulus on the real line. We let $A_{\leqslant 1}= \{ \xi \in \mathbb {R} : |\xi | \leqslant 2 \}$ . We shall write $\tilde {A}_N = \mathbb {R} \times A_N \times \mathbb {K}^* \subseteq \mathbb {R}^3$ and similarly for $\tilde {A}_{\leqslant 1}$ . For $f\in \mathcal {S}'(\mathbb {D}), N \in 2^{\mathbb {N}_0}$ , the Littlewood–Paley projections $P_N$ are defined as follows:

$$ \begin{align*} \widehat{P_N f}(\xi,\eta) = \zeta_N(\xi)\hat{f}(\xi,\eta). \end{align*} $$

We define

$$ \begin{align*} D_{\alpha, N, L}:= \{ (\tau,\xi,\eta) \in \mathbb{R} \times \mathbb{D}^* : \xi \in A_N, \; |\tau-\omega_{\alpha}(\xi,\eta)| \leqslant L\}. \end{align*} $$

We shall often omit the subscript $\alpha $ to lighten the notation.

The dispersion relation of the (1.2) is given by

$$ \begin{align*} \omega_{\alpha}(\xi,\eta) = |\xi|^{\alpha}\xi + \frac{\eta^2}{\xi}, \quad (\xi,\eta)\in \mathbb{D}^*, \end{align*} $$

and we define the linear propagator $S_{\alpha }(t)$ as a Fourier multiplier:

$$ \begin{align*} \widehat{S_{\alpha}(t)f}(\xi,\eta) = e^{it\omega_{\alpha}(\xi,\eta)}\hat{f}(\xi,\eta). \end{align*} $$

3 Linear Strichartz estimates

3.1 Linear Strichartz estimates on Euclidean space

Hadac [Reference Hadac18] proved linear Strichartz estimates for generalized KP-II equations in [Reference Hadac18, Theorem 3.1]. The proof extends to KP-I equations, which leads to the following:

Proposition 3.1. Let $\alpha \geqslant 2$ , $2<q \leqslant \infty $ , $\frac {1}{r}+\frac {1}{q}= \frac {1}{2}$ , and $s = (1-\frac {2}{r})(\frac {1}{2}-\frac {\alpha }{4})$ . Then we have

$$ \begin{align*} \| S_\alpha(t) u_0 \|_{L_t^q(\mathbb{R};L_{xy}^r(\mathbb{R}^2))} \lesssim \| u_0 \|_{\dot{H}^{s,0}(\mathbb{R}^2)}. \end{align*} $$

For $q=r=4$ we obtain the estimate

$$ \begin{align*} \| S_\alpha(t) u_0 \|_{L_t^4(\mathbb{R};L_{xy}^4(\mathbb{R}^2))} \lesssim \| u_0 \|_{\dot{H}^{\gamma,0}(\mathbb{R}^2)} \end{align*} $$

with $\gamma = \frac {2-\alpha }{8}$ .

3.2 Linear Strichartz estimates on cylinders

In the following we use $\ell ^2$ -decoupling due to Bourgain–Demeter [Reference Bourgain and Demeter10] for elliptic hypersurfaces to show linear Strichartz estimates on cylinders. We state the special case of decoupling in $2+1$ -dimensions for convenience:

Theorem 3.2 ( $\ell ^2$ -decoupling for elliptic hypersurfaces)

Let $\Lambda> 0$ , $A \subseteq \mathbb {R}^2$ be compact, and $\varphi : A \to \mathbb {R}$ be a $C^2$ -function such that

$$ \begin{align*} S = \{(\xi,\varphi(\xi)) : \, \xi \in A \} \end{align*} $$

has principal curvatures in $[\Lambda ^{-1},\Lambda ]$ . Define the Fourier extension operator adapted to S by

$$ \begin{align*} \mathcal{E}_S f(x) = \int_A e^{i (x',x_3) \cdot (\xi, \varphi(\xi))} f(\xi) d\xi, \quad x = (x',x_3) \in \mathbb{R}^2 \times \mathbb{R}. \end{align*} $$

Let $R \geqslant 1$ . The following estimate holds:

(3.1) $$ \begin{align} \| \mathcal{E}_S f \|_{L^4_x(B(0,R))} \lesssim_\varepsilon R^\varepsilon \big( \sum_{\theta: R^{-\frac{1}{2}}-\text{ball}} \| \mathcal{E}_S f_\theta \|_{L^4(w_{B(0,R)})}^2 \big)^{\frac{1}{2}}, \end{align} $$

where the sum ranges over a finitely overlapping collection of balls $\theta $ of radius $R^{-\frac {1}{2}}$ covering A. The implicit constant in (3.1) depends on S, $\Lambda $ , but not on R.

We now formulate its consequence for generalized KP-I equations:

Proposition 3.3. Let $N \in 2^{\mathbb {N}_0}$ , $A \in \mathbb {R}$ , and $u_0: \mathbb {R} \times \mathbb {T} \to \mathbb {C}$ with $\text {supp}( \hat {u}_0) \subseteq \{(\xi ,\eta ) \in \mathbb {R}^2 : |\xi | \sim N, \; \big | \frac {\eta }{\xi } - A \big | \lesssim N^{\frac {\alpha }{2}} \}.$ Then the following estimate holds:

$$ \begin{align*} \| P_N S_\alpha(t) u_0 \|_{L_t^4([0,1],L^4_{xy}(\mathbb{R} \times \mathbb{T}))} \lesssim_\varepsilon N^{\frac{2-\alpha}{8}+\varepsilon} \| u_0 \|_{L^2(\mathbb{R} \times \mathbb{T})}. \end{align*} $$

Proof. First, we consider the case $|A| \lesssim N^{\frac {\alpha }{2}}$ , in which case we find $|\eta | \lesssim N^{\frac {\alpha }{2}+1}$ . Let $Z=[0,1] \times \mathbb {R} \times \mathbb {T}$ . We carry out the change of variables

(3.2) $$ \begin{align} x' = Nx, \; y' = N^{\frac{\alpha}{2}+1} y, \; t' = N^{\alpha+1} t, \; \xi' = N^{-1} \xi, \; \eta' = N^{-(\frac{\alpha}{2}+1)} \eta, \end{align} $$

and noting that $\omega _{\alpha }(N\xi ',N^{\frac {\alpha }{2}+1} \eta ') = N^{\alpha +1} \omega _\alpha (\xi ',\eta ')$ , to find with $Z'=[0,N^{\alpha +1}] \times \mathbb {R} \times 2 \pi N^{\frac {\alpha }{2}+1}$

$$ \begin{align*} \begin{aligned} &\, \| P_N S_\alpha(t) u_0 \|^4_{L^4_{t,x,y}([0,1], \mathbb{R} \times \mathbb{T}))} = \big\| \int_{\mathbb{R} \times \mathbb{Z}} e^{i(x \cdot \xi + y \cdot \eta + t \omega_\alpha(\xi,\eta))} \hat{u}_0(\xi,\eta) d\xi (d\eta)_1 \big\|^4_{L^4_{t,x,y}(Z)} \\ &= N^{-(\alpha+1)} N^{4(1-\frac{1}{4})} N^{-(\frac{\alpha}{2}+1)} N^{4 (\frac{\alpha}{2}+1)} \\ &\quad \times\big\| \int_{\mathbb{R}} N^{-(\frac{\alpha}{2}+1)} \sum_{\eta' \in \mathbb{Z} / N^{\frac{\alpha}{2}+1}} e^{i(x' \cdot \xi' + y' \eta' + t' \omega_\alpha(\xi',\eta'))} \hat{u}_0(N \xi' , N^{\frac{\alpha}{2}+1} \eta') d\xi' \big\|^4_{L^4_{t',x',y'}(Z')}. \end{aligned} \end{align*} $$

Note that by the support properties of $\hat {u}_0$ we can suppose that $|\xi '| \sim 1$ and $|\eta '| \lesssim 1$ . Note that $\eta ' \in \mathbb {Z}/N^{\frac {\alpha }{2}+1}$ .

Now we enlarge the y-domain of integration $\mathbb {R} / (2 \pi N^{\frac {\alpha }{2}+1} \mathbb {Z})$ perceived as an interval in $\mathbb {R}$ to an interval of size $N^{\alpha +1}$ by periodicity. To ease notation, we denote the integral over $\xi '$ and the summation over $\eta ' \in \mathbb {Z}/N^{\frac {\alpha }{2}+1}$ as integral $\int _*$ with measure given as product of Lebesgue and normalized counting measure $(d \eta ')_{N^{-(\frac {\alpha }{2}+1})}$ .

By spatial periodicity this amounts to a factor of $(N^{\alpha +1} / N^{\frac {\alpha }{2}+1} )^{-1} = N^{- \alpha /2}$ , and we continue the above, letting $Z = [0,N^{\alpha +1}] \times \mathbb {R} \times [0,N^{\alpha +1}]$ as

(3.3) $$ \begin{align} \begin{aligned} &= N^{-(\alpha+1)} N^{3} N^{-\big( \frac{\alpha}{2}+1 \big)} N^{4 (\frac{\alpha}{2}+1)} N^{- \frac{\alpha}{2}} \\ &\times \Big\| \int_* e^{i(x' \xi'+ y' \eta' + t'(|\xi'|^\alpha \xi' + (\eta')^2/\xi'))} \hat{u}_0(N \xi', N^{\frac{\alpha}{2}+1} \eta') d\xi' (d\eta')_{N^{-\frac{\alpha}{2}-1}} \Big\|^4_{L^4_{t',x',y'}(Z)}. \end{aligned} \end{align} $$

We invoke $\ell ^2$ -decoupling for elliptic surfaces in two dimensions. Here we note that the Hessian is for $\xi ' \neq 0$ given by

$$ \begin{align*} \partial^2 \omega_\alpha(\xi',\eta') = \begin{pmatrix} \alpha (\alpha + 1) \text{sgn}(\xi') |\xi'|^{\alpha-1} + 2 \frac{(\eta')^2}{(\xi')^3} & - \frac{2 \eta'}{(\xi')^2} \\ - \frac{2 \eta'}{(\xi')^2} & \frac{2}{\xi'} \end{pmatrix}. \end{align*} $$

$\partial ^2 \omega _\alpha $ is uniformly elliptic for $|\xi '| \sim 1$ and $|\eta '| \lesssim 1$ . Indeed, we compute

$$ \begin{align*} \det \partial^2 \omega_\alpha(\xi',\eta') = \alpha (\alpha-1) |\xi'|^{\alpha-2}, \quad |\text{tr} (\partial^2 \omega_\alpha)| \sim 1. \end{align*} $$

We infer for $\xi ' \sim 1$ the existence of two positive eigenvalues of size comparable to $1$ , and for $\xi ' \sim -1$ two negative eigenvalues of size comparable to $-1$ . The latter case can be reduced to the elliptic case by time reversal.

A few remarks about decoupling are in order: To apply decoupling as formulated in Theorem 3.2, we break up the domain of integration $[0,N^{\alpha +1}] \times \mathbb {R} \times [0,N^{\alpha +1}]$ into finitely overlapping balls of size $N^{\alpha +1}$ . The shift in x is admissible by translation invariance. Secondly, decoupling requires a continuous approximation, that is, approximating the exponential sum with a Fourier extension operator by mollifying the Dirac comb.

We give the details: For brevity let $\varphi (x',y',t',\xi ',\eta ') = x' \xi ' + y' \eta ' + t' \omega _\alpha (\xi ',\eta ')$ . Firstly, we break the x-integration into balls of size $N^{\alpha +1}$ .

$$ \begin{align*} \begin{aligned} &\quad \big\| \int e^{i \varphi(x',y',t',\xi',\eta')} \hat{u}_0(N \xi', N^{\frac{\alpha}{2}+1} \eta') d\xi' (d \eta')_{N^{-\frac{\alpha}{2}-1}} \big\|_{L^4_{t',x',y'}([0,N^{\alpha+1}] \times \mathbb{R} \times [0,N^{\alpha+1}])}^4 \\ &\lesssim \sum_{B_{N^{\alpha+1}}} \big\| \int e^{i\varphi(x',y',t',\xi',\eta')} \hat{u}_{0N} d\xi' (d \eta')_{N^{-\frac{\alpha}{2}-1}} \big\|_{L^4_{t',x',y'}([0,N^{\alpha+1}] \times B_{N^{\alpha+1}} \times [0,N^{\alpha+1}])}^4. \end{aligned} \end{align*} $$

Next, by a linear change of variables $x' \to x' + c(B_{N^{\frac {\alpha }{2}+1}})$ with $c(B)$ denoting the center of the ball, we can suppose that the ball is centered at the origin. The phase factor is absorbed into $\hat {u}_{0N}$ .

For the continuous approximation, we consider a sequence of smooth functions $\hat {f}_\lambda $ such that for $|x'|,|t'|,|y'| \lesssim N^{\alpha +1}$ we have

$$ \begin{align*} \int e^{i(x' \xi' + y' \eta' + t' \omega_\alpha(\xi',\eta'))} \hat{f}_\lambda(\xi',\eta') d\xi' d\eta' \to \int e^{i(x' \xi' + y' \eta' + t' \omega_\alpha(\xi',\eta'))} \hat{u}_{0N} d\xi' (d\eta')_{N^{-(\frac{\alpha}{2}+1)}}. \end{align*} $$

More specifically, we can choose $\text {supp}(\hat {f}_\lambda ) \subseteq \mathcal {N}_{\lambda ^{-1}}(\text {supp}(\hat {u}_{0N}))$ in a $\lambda ^{-1}$ -neighbourhood. Then, choosing $\lambda $ large enough, we can estimate by the theorem of dominated convergence:

$$ \begin{align*} \begin{aligned} &\quad \big\| \int e^{i\varphi(x',y',t',\xi',\eta')} \hat{u}_{0N} d\xi' (d \eta')_{N^{-\frac{\alpha}{2}-1}} \big\|_{L^4_{t',x',y'}([0,N^{\alpha+1}] \times B_{N^{\alpha+1}} \times N^{\alpha+1} \mathbb{T})} \\ &\lesssim \big\| \int e^{i\varphi(x',y',t',\xi',\eta')} \hat{f}_\lambda(\xi',\eta') d\xi' d\eta' \big\|_{L^4_{t',x',y'}(B_{N^{\alpha+1}})}. \end{aligned} \end{align*} $$

The final expression is amenable to decoupling as recorded and after reversing the continuous approximation by letting $\lambda \to \infty $ , we obtain an $\ell ^2$ -sum into balls on the frequency side of size $N^{- \frac {\alpha +1}{2}}$ . On this scale the phase function can be trivialized by Taylor expansion and we obtain from integration in time after reversing the continuous approximation:

$$ \begin{align*} \begin{aligned} &\quad \big\| \int_* e^{i\varphi(x',y',t',\xi',\eta')} \hat{u}_{0 \theta}(N \xi', N^{\frac{\alpha}{2}+1} \eta') d\xi' (d \eta')_{N^{-\frac{\alpha}{2}-1}} \big\|^2_{L_{t'}^4([0,N^{\alpha+1}],L^4_{x' y'}(B_{N^{\alpha+1}})} \\ &\lesssim N^{\frac{\alpha+1}{2}} \big\| \int_* e^{i(x' \xi' + y' \eta')} \hat{u}_{0 \theta}(N \xi', N^{\frac{\alpha}{2}+1} \eta') d\xi' (d \eta')_{N^{-\frac{\alpha}{2}-1}} \big\|^2_{L^4_{x' y'}(B_{{N^{\alpha+1}}})}. \end{aligned} \end{align*} $$

Now we reverse the scaling in x and y, which compensates the scaling factors $N^{3}$ and $N^{-(\frac {\alpha }{2}+1)} N^{4(\frac {\alpha }{2}+1)}$ in (3.3).

It remains to estimate

$$ \begin{align*} \big\| \int_* e^{i(x \xi + y \eta)} \hat{u}_{0 \theta}(\xi,\eta) d\xi d\eta \big\|^2_{L^4_{xy}} \end{align*} $$

with $\theta $ denoting a rectangle of size $N^{\frac {1-\alpha }{2}} \times N^{\frac {1}{2}}$ . We can use Bernstein’s inequality to find

(3.4) $$ \begin{align} \big\| \int_{\mathbb{R} \times \mathbb{Z}} e^{i(x \xi + y \eta)} \hat{u}_{0 \theta}(\xi,\eta) d\xi (d\eta)_1 \big\|_{L^4_{xy}} \lesssim N^{\frac{1-\alpha}{8}} N^{\frac{1}{8}} \| u_{0 \theta} \|_{L^2_{xy}}. \end{align} $$

We summarize the estimates as follows: Scaling to unit frequencies and enlarging the spatial domain to $N^{\alpha +1}$ incurs a factor of

$$ \begin{align*} N^{-(\alpha+1)} N^{3} N^{-(\frac{\alpha}{2} + 1)} N^{4(\frac{\alpha}{2}+1)} N^{- \frac{\alpha}{2}}. \end{align*} $$

Invoking $\ell ^2$ -decoupling incurs a factor of $N^\varepsilon $ and decouples the integral into balls of size $N^{-\frac {\alpha +1}{2}}$ . Carrying out the time integral yields a factor $N^{\alpha +1}$ and reversing the scaling in x and $\xi $ , and y and $\eta $ gives factors $N^3$ and $N^{\frac {\alpha }{2}+1}$ , respectively. Moreover, we use periodicity to decrease the spatial domain to $\mathbb {T}$ again after inverting the scaling. This incurs a factor $N^{\frac {\alpha }{2}}$ .

We have proved so far

(3.5) $$ \begin{align} \| P_N S_\alpha(t) u_0 \|^4_{L_{t,x,y}^4([0,1], \mathbb{R} \times \mathbb{T})} \lesssim_\varepsilon N^{\varepsilon} \big( \sum_{\theta} \| u_{0 \theta} \|^2_{L^4_{xy}} \big)^{2} \end{align} $$

with the sum over $\theta $ being over essentially disjoint rectangles of size $N^{\frac {1-\alpha }{2}} \times N^{\frac {1}{2}}$ . Plugging (3.4) into (3.5) yields

$$ \begin{align*} \| P_N S_\alpha(t) u_0 \|^4_{L^4_{t,x,y}} \lesssim_\varepsilon N^{\varepsilon + \frac{2-\alpha}{2}} \| u_0 \|_{L^2_{xy}}^4, \end{align*} $$

which completes the proof in case $|A| \lesssim N^{\frac {\alpha }{2}}$ .

Now we turn to the case $|A| \gg N^{\frac {\alpha }{2}}$ : In the first step we apply the scaling (3.2), which maps the Fourier support to the set

$$ \begin{align*} |\xi'| \sim 1, \quad \big| \frac{\eta'}{\xi'} - A' \big| \lesssim 1 \end{align*} $$

for $A' = A/N^{\frac {\alpha }{2}}$ . Like above, by periodic extension in $y'$ , we reduce to estimate the expression up to scaling factors

$$ \begin{align*} \big\| \int e^{i(x'\xi' + y' \eta' + t' \omega_{\alpha}(\xi',\eta'))} \hat{u}_0(N \xi', N^{\frac{\alpha}{2}+1} \eta') d\xi' (d\eta')_{N^{-\frac{\alpha}{2}-1}} \big\|_{L^4_{t'}([0,N^{\alpha+1}], L^4_{x' y'}(\mathbb{R} \times B_{N^{\alpha+1}}))}. \end{align*} $$

We can apply the Galilean invariance

$$ \begin{align*} (\xi",\eta") = F'(\xi',\eta') = (\xi',\eta' - A' \xi') \end{align*} $$

to obtain

$$ \begin{align*} |\xi"| \sim 1, \quad \big| \frac{\eta"}{\xi"} \big| \lesssim 1. \end{align*} $$

Note that this does not change the domain of integration $\mathbb {R} \times B_{N^{\alpha +1}}$ , but it is important to note that in general $(\xi ",\eta ") \notin \mathbb {R} \times \mathbb {Z}$ . Now we again break the domain of integration $[0,N^{\alpha +1}] \times \mathbb {R} \times B_{N^{\alpha +1}}$ into balls of size $B_{N^{\alpha +1}}$ and use translation invariance.

We have by continuous approximation

$$ \begin{align*} \begin{aligned} &\quad \big\| \int d \xi" \sum_{\eta" \in \mathbb{Z} - A' \xi"} e^{i(x' \xi"+y' \eta" + t' \omega_\alpha(\xi",\eta"))} \hat{u}_{0N}(\xi",\eta"+ A' \xi') \big\|_{L^4_{t'}([0,N^{\alpha+1}], L^4_{x' y'}(B_{N^{\alpha+1}}))} \\ &\lesssim \big\| \int_{|\xi"| \sim 1, \, |\eta"| \lesssim 1} e^{i(x' \xi" + y' \eta" + t' \omega_\alpha(\xi",\eta"))} \hat{f}_\lambda(\xi",\eta") d\xi" d\eta" \big\|_{L^4_{t',x',y'}(B_{N^{\alpha+1}})}. \end{aligned} \end{align*} $$

Now we can apply $\ell ^2$ -decoupling and reverse the continuous approximation, which gives the estimate

$$ \begin{align*} \begin{aligned} &\quad \big\| \int d \xi" \sum_{\eta" \in \mathbb{Z} - A' \xi"} e^{i(x' \xi" + y' \eta" + t' \omega_\alpha(\xi",\eta")} \hat{u}_{0,N}(\xi",\eta" + A' \xi") \big\|_{L^4_{t',x',y'}(B_{N^{\alpha+1}})} \\ &\lesssim_\varepsilon N^{\varepsilon} \big( \sum_{\theta \in \mathcal{B}_{N^{-\frac{\alpha+1}{2}}}} \big\| \int d\xi" \sum_{\eta" \in \mathbb{Z} - A' \xi"} e^{i(x' \xi" + y' \eta" + t' \omega_\alpha(\xi",\eta"))}\\ &\quad \quad \times \chi_{\theta}(\xi",\eta") \hat{u}_{0N}(\xi",\eta"+A'\xi") \big\|_{L^4_{t',x',y'}(w_{B_{N^{\alpha+1}}})}^2 \big)^{\frac{1}{2}}. \end{aligned} \end{align*} $$

The sum over $\theta $ is over essentially disjoint $N^{-\frac {\alpha +1}{2}}$ -balls, which cover the set $\{|\xi "| \sim 1, |\eta "| \lesssim 1 \}$ .

Summing over the $B_{N^{\alpha +1}}$ -balls in the x-coordinate and reversing all linear transformations and the scalings, we arrive at the expression

$$ \begin{align*} \begin{aligned} &\quad \big\| \int d\xi \sum_{\eta \in \mathbb{Z}} e^{i(x\xi + y \eta + t \omega_\alpha(\xi,\eta))} \hat{u}_0(\xi,\eta) \big\|_{L_t^4([0,1], L^4_{xy}(\mathbb{R} \times \mathbb{T}))} \\ &\lesssim_\varepsilon N^\varepsilon \big( \sum_{\theta \in \mathcal{B}_{N^{-\frac{\alpha+1}{2}}}} \big\| \int d\xi \sum_{\eta \in \mathbb{Z}} e^{i(x \xi + y \eta + t \omega_\alpha(\xi,\eta))} \\ &\quad \quad \quad \times \chi_{\theta}(N^{-1} \xi, N^{-(\frac{\alpha}{2}+1)}(\eta - A \xi)) \hat{u}_0(\xi,\eta) \big\|^2_{L_t^4(w_1,L^4_{xy}(\mathbb{R} \times \mathbb{T}))}. \end{aligned} \end{align*} $$

Since there are no oscillations of $\omega _\alpha (\xi ,\eta )$ for $(N^{-1} \xi , N^{-(\frac {\alpha }{2}+1)}(\eta -A\xi ))$ contained in $\theta $ , we can carry out the integration in time without loss.

Let $\bar {\theta } = I_{N^{\frac {1-\alpha }{2}}} \times I_{N^{\frac {1}{2}}}$ be the anisotropic dilation of $\theta $ . Let

$$ \begin{align*} (\bar{\xi},\bar{\eta}) = F(\xi,\eta) = (\xi,\eta - A \xi) \end{align*} $$

denote the Galilean transform without anisotropic dilation.

To conclude the argument, we apply Bernstein’s inequality for which we need to understand $F^{-1}(\bar {\theta })$ . Since $\xi \in I_{N^{\frac {1-\alpha }{2}}}$ the condition $\eta - A \xi \in I_{N^{\frac {1}{2}}}$ yields the bound

$$ \begin{align*} \# \{ \eta \in \mathbb{Z} \; | \; \exists \xi \in I_{N^{\frac{1}{2}}}: \eta - A \xi \in I_{N^{\frac{1}{2}}} \} \lesssim N^{\frac{1}{2}} + A N^{\frac{1-\alpha}{2}} \sim A N^{\frac{1-\alpha}{2}}. \end{align*} $$

The final estimate is due to the size assumption on A. For fixed $\eta $ , we estimate the measure of $\xi $ such that $F(\xi ,\eta ) \in \bar {\theta }$ as

$$ \begin{align*} \text{meas}( \{ \xi \in \mathbb{R} : F(\xi,\eta) \in \bar{\theta} \}) \lesssim N^{\frac{1}{2}} / A. \end{align*} $$

Then it is a consequence of Bernstein’s inequality that

$$ \begin{align*} \begin{aligned} &\quad \big\| \int_{F(\xi,\eta) \in \bar{\theta}} e^{i(x \xi + y \eta)} \hat{f}(\xi,\eta) d\xi d\eta \big\|_{L^4_{xy}(\mathbb{R} \times \mathbb{T})} \\ &\lesssim (A N^{\frac{1-\alpha}{2}})^{\frac{1}{4}} (N^{\frac{1}{2}} / A)^{\frac{1}{4}} \| \int_{(\xi,\eta) \in F^{-1}(\bar{\theta})} e^{i(x\xi + y \eta)} \hat{u}_0(\xi,\eta) \|_{L^2_{xy}} \\ &\lesssim N^{\frac{2-\alpha}{8}} \| \int_{(\xi,\eta) \in F^{-1}(\bar{\theta})} e^{i(x\xi + y \eta)} \hat{u}_0(\xi,\eta) \|_{L^2_{xy}}. \end{aligned} \end{align*} $$

The proof is then concluded by the essential disjointness of $F^{-1}(\bar {\theta })$ .

Remark 3.4. We remark that the argument does not yield an improved estimate when considering frequency-dependent time intervals $T=T(N)=N^{-\kappa }$ . Moreover, a comparison of the estimate on cylinders with the Strichartz estimates on Euclidean space indicates sharpness of the derivative loss up to the endpoint.

3.3 Linear Strichartz estimates on tori

The above arguments yield the following result on tori:

Proposition 3.5. Let $N \in 2^{\mathbb {N}_0}$ , $\alpha \geqslant 2$ , and $\text {supp}(\hat {u}_0) \subseteq \{(\xi ,\eta ) \in \mathbb {R}^2 : |\xi | \sim N, \quad |\eta | \lesssim N^{\frac {\alpha }{2}+1} \} = A_{N,N^{\frac {\alpha }{2}+1}}$ . Then the following estimate holds:

(3.6) $$ \begin{align} \| S_\alpha(t) u_0 \|_{L_t^4([0,1],L^4_{xy}(\mathbb{T}^2_{\gamma}))} \lesssim_\varepsilon N^{\frac{1}{8}+\varepsilon} \| u_0 \|_{L^2_{xy}(\mathbb{T}^2_\gamma)}. \end{align} $$

Proof. We can follow along the arguments of the proof of Proposition 3.1, that is, employ the anisotropic scaling (3.2), use a continuous approximation to invoke $\ell ^2$ -decoupling, and finally reverse the continuous approximation and scaling. After carrying out the integration in time, we arrive at the expression:

$$ \begin{align*} \| S_\alpha(t) u_0 \|_{L_t^4([0,1],L^4_{xy}(\mathbb{T}^2_\gamma))} \lesssim_\varepsilon N^\varepsilon \big( \sum_{\theta \in \mathcal{R}_{N^{\frac{1-\alpha}{2}} \times N^{\frac{1}{2}}}} \| u_{0 \theta} \|^2_{L^4_{xy}(\mathbb{T}^2_\gamma)} \big)^{\frac{1}{2}}, \end{align*} $$

where the sum is carried out over essentially disjoint rectangles $\theta $ of size $N^{\frac {1-\alpha }{2}} \times N^{\frac {1}{2}}$ , which cover $A_{N,N^{\frac {\alpha }{2}+1}}$ . An application of Bernstein’s inequality yields

$$ \begin{align*} \| u_{0 \theta} \|_{L^4_{xy}(\mathbb{T}^2_\gamma)} \lesssim N^{\frac{1}{8}} \| u_{0 \theta} \|_{L^2 (\mathbb{T}^2_\gamma)}, \end{align*} $$

since presently the estimate is carried out with counting measure compared to the previous section. The proof is concluded by essential disjointness of $\theta $ .

Remark 3.6 (Sharpness of the Strichartz estimate)

The Strichartz estimate is sharp, which can be seen from considering the initial data

$$ \begin{align*} \hat{u}_0(\xi,\eta) = \delta_{N}(\xi) 1_{[1,N^{\frac{1}{2}}]}(\eta). \end{align*} $$

In this case, there are no oscillations, for which reason

$$ \begin{align*} \| S_\alpha(t) u_0 \|_{L_t^4([0,1],L^4_{xy}(\mathbb{T}^2_{\gamma}))} \sim \| u_0 \|_{L^4_{xy}(\mathbb{T}^2_\gamma)}. \end{align*} $$

Next, we observe by $u_0(0) = N^{\frac {1}{2}}$ and the uncertainty principle that

$$ \begin{align*} \| u_0 \|_{L^4_{xy}(\mathbb{T}^2_\gamma)} \gtrsim N^{\frac{1}{2}} (N^{-\frac{1}{2}})^{\frac{1}{4}} \sim N^{\frac{3}{8}}. \end{align*} $$

Since $\| u_0 \|_{L^2_{xy}} \sim N^{\frac {1}{4}}$ , this example exhausts (3.6) up to the endpoint.

This points out that for the KP-I dispersion relation the Strichartz estimates on tori deviate significantly from the Strichartz estimates on Euclidean space, which is not the case for the Schrödinger equation. For the Schrödinger evolution, $\ell ^2$ -decoupling recovers Euclidean Strichartz estimates on finite times up to arbitrarily small derivative loss (see [Reference Bourgain and Demeter10]).

4 Resonance, Transversality, and multilinear estimates

In this section we show bilinear Strichartz estimates and trilinear convolution estimates for approximate solutions to dispersion-generalized KP-I equations.

4.1 Resonance and bilinear Strichartz estimates

We recall resonance and transversality identities from [Reference Sanwal and Schippa41]. The resonance function is given by

$$ \begin{align*} \begin{aligned} \Omega_{\alpha}(\xi_1,\xi_2,\eta_1,\eta_2) &= \omega_\alpha(\xi_1+\xi_2,\eta_1+\eta_2) - \omega_\alpha(\xi_1,\eta_1) - \omega_\alpha(\xi_2,\eta_2) \\ &= \underbrace{|\xi_1+\xi_2|^\alpha (\xi_1+\xi_2) - |\xi_1|^\alpha \xi_1 - |\xi_2|^\alpha \xi_2}_{\Omega_{\alpha,1}} - \frac{(\eta_1 \xi_2 - \eta_2 \xi_1)^2}{\xi_1 \xi_2 (\xi_1+\xi_2)}. \end{aligned} \end{align*} $$

We say that we are in the resonant case, if

(4.1) $$ \begin{align} |\Omega_\alpha| \ll \big| \Omega_{\alpha,1} \big|. \end{align} $$

Suppose that $|\xi _1+\xi _2| \sim |\xi _1| \sim N_{\max } \gtrsim N_{\min } \sim |\xi _2|$ : Applying the mean-value theorem gives

$$ \begin{align*} |\Omega_{\alpha,1}| \sim N_{\max}^\alpha N_{\min}. \end{align*} $$

We see that in the nonresonant case the derivative loss is readily recovered, for example, using standard Fourier restriction spaces (cf. [Reference Bourgain8, Reference Bourgain9]) because $|\Omega _{\alpha ,1}|^{\frac {1}{2}} \gtrsim N^{\frac {\alpha }{2}}_{\max } N_{\min }^{\frac {1}{2}}$ .

We focus on the resonant case. Here we obtain a bound for the transversality quantified by the difference of the group velocity:

$$ \begin{align*} \nabla \omega_{\alpha}(\xi,\eta) = ( (\alpha+1) |\xi|^\alpha - \frac{\eta^2}{\xi^2}, \frac{2 \eta}{\xi} ). \end{align*} $$

It follows

(4.2) $$ \begin{align} |\partial_\eta \omega_{\alpha}(\xi_1,\eta_1) - \partial_\eta \omega_\alpha(\xi_2,\eta_2) | \gtrsim \big| \frac{\eta_1}{\xi_1} - \frac{\eta_2}{\xi_2} \big| \sim N_{\max}^{\frac{\alpha}{2}}. \end{align} $$

This is a key ingredient for the bilinear Strichartz estimates in the resonant case. Define

(4.3) $$ \begin{align} C_{1,\mathbb{D}}(L,N) = \begin{cases} (L / N^{\frac{\alpha}{2}} )^{\frac{1}{2}}, \; &\mathbb{D} = \mathbb{R}^2, \\ \langle L / N^{\frac{\alpha}{2}} \rangle^{\frac{1}{2}}, \; &\mathbb{D} = \mathbb{R} \times \mathbb{T}. \end{cases} \end{align} $$

For later use we show the following bilinear Strichartz estimate depending on transversality:

Proposition 4.1. Let $\mathbb {D} \in \{ \mathbb {R}^2, \mathbb {R} \times \mathbb {T} \}$ . Let $f_i: \mathbb {R} \times \mathbb {D}^* \to \mathbb {C}$ , $i=1,2$ satisfy the support conditions $\pi _{\xi } (\text {supp}(f_j)) \subseteq I_j$ with $|I_j| \lesssim N_{\min }$ and

(4.4) $$ \begin{align} |\partial_{\eta} \omega_\alpha(\xi_1,\eta_1) - \partial_\eta \omega_\alpha(\xi - \xi_1, \eta - \eta_1)| \gtrsim N_{\max}^{\frac{\alpha}{2}} \end{align} $$

for $(\xi _1,\eta _1) \in \pi _{\xi ,\eta }(\text {supp}(f_1))$ , $(\xi -\xi _1,\eta -\eta _1) \in \pi _{\xi ,\eta }(\text {supp}(f_2))$ , and $|\tau _i - \omega _\alpha (\xi _i,\eta _i) | \lesssim L_i$ for $(\tau _i,\xi _i,\eta _i) \in \text {supp}(f_i)$ . Then the following estimate holds:

(4.5) $$ \begin{align} \| f_{1,N_1,L_1} * f_{2,N_2,L_2} \|_{L^2_{\tau,\xi,\eta}} \lesssim N_{\min}^{\frac{1}{2}} L_{\min}^{\frac{1}{2}} C_{1,\mathbb{D}}(L_{\max},N_{\max}) \prod_{i=1}^2 \| f_{i,N_i,L_i} \|_{L^2_{\tau,\xi,\eta}}. \end{align} $$

Proof. Suppose that $L_1 = \min (L_1,L_2)$ and $L_2 = \max (L_1,L_2)$ by symmetry. We obtain by the Cauchy-Schwarz inequality:

$$ \begin{align*} \begin{aligned} &\quad \| (f_{1,N_1,L_1} * f_{2,N_2,L_2}) \|_{L^2_{\tau,\xi,\eta}} \\ &\leqslant \sup_{(\tau,\xi,\eta) \in \mathbb{R}^3} \text{meas}( S= \{ (\tau_1,\xi_1,\eta_1) \in \text{supp}(f_{1,N_1,L_1}), \; \xi_1 \in I_1 : \\ &\quad \quad (\tau-\tau_1,\xi-\xi_1,\eta-\eta_1) \in \text{supp}(f_{2,N_2,L_2}), \; \xi - \xi_1 \in I_2 \} )^{\frac{1}{2}} \prod_{i=1}^2 \|f_{i,N_i,L_i} \|_{L_{\tau,\xi,\eta}^2}. \end{aligned} \end{align*} $$

The assumption (4.4) yields

$$ \begin{align*} \big| \frac{\eta_1}{\xi_1} - \frac{\eta - \eta_1}{\xi - \xi_1} \big| \gtrsim N_{\max}^{\frac{\alpha}{2}}. \end{align*} $$

Note moreover that

(4.6) $$ \begin{align} \big| \big( \tau_1 - \omega_\alpha(\xi_1,\eta_1) \big) + \big( (\tau - \tau_1) - \omega_\alpha(\xi - \xi_1,\eta- \eta_1) \big) \big| \lesssim L_2. \end{align} $$

We estimate the measure of S by fixing $\xi _1$ , which amounts to a factor $|I_1|$ , and counting $\tau _1$ and $\eta _1$ . From (4.4) and (4.6) follows that for fixed $\tau $ , $\xi _1$ , $\xi $ , $\eta $ that on $\mathbb {R}^2$ the measure of $\eta _1$ is estimated by $\big ( \frac {L_2}{ N_{\max }^{\frac {\alpha }{2}}} \big )^{\frac {1}{2}}$ . On $\mathbb {R} \times \mathbb {T}$ there are at most $\langle \frac {L_2}{ N_{\max }^{\frac {\alpha }{2}}} \rangle ^{\frac {1}{2}}$ values of $\eta _1$ such that $(\xi _1,\eta _1,\tau _1) \in S$ . This is a consequence of the mean-value theorem. Finally, with $(\xi _1,\eta _1)$ fixed, we trivially estimate

$$ \begin{align*} \text{meas} ( \{ \tau_1 : |\tau_1 - \omega_\alpha(\xi_1,\eta_1)| \leqslant L_1 \} ) \leqslant L_1. \end{align*} $$

In conclusion we obtain

$$ \begin{align*} \begin{aligned} \text{meas} (S) &\leqslant |I_1| \cdot \# \{ \eta_1 : (4.4) \text{ and } (4.6) \text{ holds } \} \cdot \big| \{ \tau_1 : |\tau_1 - \omega_\alpha(\xi_1,\eta_1) \big| \leqslant L_1 \} \big| \\ &\lesssim N_{\min} \cdot C_{1,\mathbb{D}}(L_2,N_{\max}) \cdot L_1. \end{aligned} \end{align*} $$

with $C_{1,\mathbb {D}}$ defined in (4.3). This finishes the proof.

We shall see that the support assumptions are satisfied in the resonant case, which implies:

Corollary 4.2. Let $\mathbb {D} \in \{ \mathbb {R}^2, \mathbb {R} \times \mathbb {T} \}$ , $N_3 \sim N_1 \gtrsim N_2$ and for $i=1,2$ suppose that $\text {supp}(f_{i,N_i,L_i}) \subseteq D_{N_i,L_i}$ with $L_i \ll N_1^\alpha N_2$ for $i=1,2,3$ . Then the following estimate holds with $C_{1,\mathbb {D}}$ defined in (4.3):

(4.7) $$ \begin{align} \begin{aligned} &\quad \| 1_{D_{\alpha,N_3,L_3}} ( f_{1,N_1,L_1} * f_{2,N_2,L_2} ) \|_{L^2_{\tau,\xi,\eta}(\mathbb{R} \times \mathbb{D}^*)} \\ &\lesssim (L_1 \wedge L_2)^{\frac{1}{2}} N_{\min}^{\frac{1}{2}} C_{1,\mathbb{D}}(L_1 \vee L_2, N_{\max}) \prod_{i=1}^2 \| f_{i,N_i,L_i} \|_{L^2_{\tau,\xi,\eta}(\mathbb{R} \times \mathbb{D}^*)}. \end{aligned} \end{align} $$

Proof. Since

$$ \begin{align*} \begin{aligned} &\quad |\Omega_\alpha(\xi_1,\eta_1,\xi-\xi_1,\eta-\eta_1)| \\ &= |\tau - \omega_\alpha(\xi,\eta) - (\tau_1 - \omega_\alpha(\xi_1,\eta_1)) - ((\tau-\tau_1) - \omega_\alpha(\xi-\xi_1,\eta-\eta_1)) | \\ &\ll N_{\max}^\alpha N_{\min}, \end{aligned} \end{align*} $$

we are in the resonant case (4.1) and we have by (4.2)

(4.8) $$ \begin{align} \big| \frac{\eta_1}{\xi_1} - \frac{\eta - \eta_1}{\xi - \xi_1} \big| \sim N_{\max}^{\frac{\alpha}{2}}. \end{align} $$

The assumptions of Proposition 4.1 are satisfied, which yields the claim.

We have the following alternative bilinear Strichartz estimate, which is based on the second order transversality:

$$ \begin{align*} |\partial^2_{\eta} ( \omega_\alpha(\xi_1,\eta_1) + \omega_\alpha(\xi - \xi_1,\eta- \eta_1) | = 2 \Big| \frac{1}{\xi_1} + \frac{1}{\xi - \xi_1} \Big|. \end{align*} $$

The estimate was observed by Bourgain [Reference Bourgain9] in the context of the KP-II equation. This will serve to estimate several boundary cases, in case the low frequency is very small or the resonance is very large. Define

(4.9) $$ \begin{align} C_{2,\mathbb{D}}(L,N) = \begin{cases} (L N)^{\frac{1}{4}}, \quad &\mathbb{D} = \mathbb{R}^2, \\ \langle L N \rangle^{\frac{1}{4}}, \quad &\mathbb{D} = \mathbb{R} \times \mathbb{T}. \end{cases} \end{align} $$

Lemma 4.3 [Reference Bourgain9]

Let $\mathbb {D} \in \{ \mathbb {R}^2, \mathbb {R} \times \mathbb {T} \}$ , and $f_{i,N_i,L_i} : \mathbb {R} \times \mathbb {D}^* \to \mathbb {R}_{\geqslant 0}$ with $\text {supp}(f_{i,N_i,L_i}) \subseteq D_{N_i,L_i}$ and $\pi _{\xi }(\text {supp}(f_{i,N_i,L_i})) \subseteq I_i$ with $|I_i| \leqslant K$ . Then the following estimate holds:

(4.10) $$ \begin{align} \| f_{1,N_1,L_1} * f_{2,N_2,L_2} \|_{L^2_{\tau,\xi,\eta}} \lesssim K^{\frac{1}{2}} (L_1 \wedge L_2)^{\frac{1}{2}} C_{2,\mathbb{D}}(L_1 \vee L_2, N_{\min}) \prod_{i=1}^2 \| f_{i,N_i,L_i} \|_{L^2}. \end{align} $$

Next, we obtain refined bilinear Strichartz estimates employing the Córdoba–Fefferman square function estimate. We point out that the following estimate is less restrictive than Proposition 4.1 or Corollary 4.2 in the sense that we do not require condition (4.4) to hold or that $L_i, i=1,2$ to be bounded above by $N_{\max }^{\alpha }N_{\min }$ . Consequently, when estimating a trilinear expression with $L_i\geqslant N_{\max }^{\alpha }N_{\min }$ for exactly one i, we can gain from the high modulation ( $L_i$ ), and from the following estimate simultaneously. We contend that the estimates are of independent interest, also for future work.

Lemma 4.4. Let $\alpha \geqslant 1$ , $N_1 \in 2^{\mathbb {N}_0}$ , $N_2 \in 2^{\mathbb {Z}}$ , $N_1 \gg N_2$ , $L_1, L_2 \in 2^{\mathbb {N}_0}$ . For $i=1,2$ , let $f_{i,N_i,L_i} : \mathbb {R} \times \mathbb {R}^2 \to \mathbb {R}_{\geqslant 0}$ with $\text {supp}(f_{i,N_i,L_i}) \subseteq D_{N_i,L_i}$ .

Then the following estimate holds:

$$ \begin{align*} \| f_{1,N_1,L_1} * f_{2,N_2,L_2} \|_{L^2_{\tau,\xi,\eta}} \lesssim \frac{N_2^{\frac{1}{2}}}{N_1^{\frac{\alpha}{4}}} \prod_{i=1}^2 L_i^{\frac{1}{2}} \| f_{i,N_i,L_i} \|_{L^2}. \end{align*} $$

Proof. If $L_{\max } = \max (L_1,L_2) \gtrsim N_1^\alpha N_2$ , this is a consequence of Lemma 4.3:

$$ \begin{align*} \begin{aligned} \| f_{1,N_1,L_1} * f_{2,N_2,L_2} \|_{L^2_{\tau,\xi,\eta}} &\lesssim N_2^{\frac{3}{4}} L_{\min}^{\frac{1}{2}} L_{\max}^{\frac{1}{4}} \prod_{i=1}^2 \| f_{i,N_i,L_i} \|_2 \\ &\lesssim \frac{N_2^{\frac{1}{2}}}{N_1^{\frac{\alpha}{4}}} \prod_{i=1}^2 L_i^{\frac{1}{2}} \| f_{i,N_i,L_i} \|_2. \end{aligned} \end{align*} $$

In the following we suppose that $L_{\max } \ll N_1^\alpha N_2$ . We carry out a dyadic decomposition (Whitney) in the transversality parameter:

$$ \begin{align*} D \sim \big| \frac{\eta_1}{\xi_1} - \frac{\eta_2}{\xi_2} \big| \end{align*} $$

with the range $D \in [\big ( \frac {L_{\max }}{N_2} \big )^{\frac {1}{2}}, \infty )$ :

$$ \begin{align*} \| f_{1,N_1,L_1} * f_{2,N_2,L_2} \|_{L^2_{\tau,\xi,\eta}} \leqslant \sum_{D \geqslant \big( \frac{L_{\max}}{N_2} \big)^{\frac{1}{2}}} \sum_{I_1^D \sim I_2^D} \| f_{1,N_1,L_1}^{I_1^D} * f_{2,N_2,L_2}^{I_2^D} \|_{L^2_{\tau,\xi,\eta}}. \end{align*} $$

Here we have broken the support of $f_{i,N_i,L_i}$ into intervals $I_i^D$ of $(\eta _i/\xi _i)$ of length $\sim D$ with

$$ \begin{align*} \big| \frac{\eta_1}{\xi_1} - \frac{\eta_2}{\xi_2} \big| \sim D \text{ for } \frac{\eta_i}{\xi_i} \in I_i^D. \end{align*} $$

The contribution of $D \gtrsim N_1^{\frac {\alpha }{2}}$ is handled by Proposition 4.1:

$$ \begin{align*} \begin{aligned} \sum_{D \gtrsim N_1^{\frac{\alpha}{2}}} \sum_{I_1^D \sim I_2^D} \| f_{1,N_1,L_1}^{I_1^D} * f_{2,N_2,L_2}^{I_2^D} \|_{L^2_{\tau,\xi,\eta}} &\lesssim \sum_{D \gtrsim N_1^{\frac{\alpha}{2}}} \sum_{I_1^D \sim I_2^D} \frac{N_2^{\frac{1}{2}}}{D^{\frac{1}{2}}} \prod_{i=1}^2 L_i^{\frac{1}{2}} \| f_{i,N_i,L_i}^{I_i^D} \|_{L^2_{\tau,\xi,\eta}} \\ &\lesssim \frac{N_2^{\frac{1}{2}}}{N_1^{\frac{\alpha}{4}}} \prod_{i=1}^2 L_i^{\frac{1}{2}} \| f_{i,N_i,L_i} \|_{L^2_{\tau,\xi,\eta}}. \end{aligned} \end{align*} $$

For $D \ll N_1^{\frac {\alpha }{2}}$ we can use an almost orthogonal decomposition to effectively reduce the $\xi $ -support of $f_{i,N_i,L_i}$ . Without loss of generality we can suppose that $\pi _{\xi }(f_{i,N_i,L_i}) \subseteq \mathbb {R}_{>0}$ by complex conjugation and symmetry of the dispersion relation.

The convolution constraint reads

$$ \begin{align*} \left\{ \begin{array}{cl} \xi_1 + \xi_2 &= \xi_3 + \xi_4, \\ \eta_1 + \eta_2 &= \eta_3 + \eta_4, \\ \xi_1^{\alpha+1} + \frac{\eta_1^2}{\xi_1} + \xi_2^{\alpha+1} + \frac{\eta_2^2}{\xi_2} &= \xi_3^{\alpha+1} + \frac{\eta_3^2}{\xi_3} + \xi_4^{\alpha+1} + \frac{\eta_4^2}{\xi_4} + \mathcal{O}(L_{\max}). \end{array} \right. \end{align*} $$

We rescale to unit $\xi $ -frequencies by $\xi \to \frac {\xi }{N_1}$ , $\eta \to \frac {\eta }{N_1^{\frac {\alpha }{2} + 1}}$ to find the following for the renormalized frequencies:

$$ \begin{align*} \left\{ \begin{array}{cl} \xi^{\prime}_1 + \xi^{\prime}_2 &= \xi^{\prime}_3 + \xi^{\prime}_4, \\ \eta^{\prime}_1 + \eta^{\prime}_2 &= \eta^{\prime}_3 + \eta^{\prime}_4, \\ (\xi^{\prime}_1)^{\alpha+1} + \frac{(\eta^{\prime}_1)^2}{\xi^{\prime}_1} + (\xi^{\prime}_2)^{\alpha+1} + \frac{(\eta^{\prime}_2)^2}{\xi^{\prime}_2} &= (\xi^{\prime}_3)^{\alpha+1} + \frac{(\eta^{\prime}_3)^2}{\xi^{\prime}_3} \\ &\quad +\ (\xi^{\prime}_4)^{\alpha+1} + \frac{(\eta^{\prime}_4)^2}{\xi^{\prime}_4} + \mathcal{O}(L_{\max}/N_1^{\alpha+1}). \end{array} \right. \end{align*} $$

We subtract

$$ \begin{align*} \frac{(\eta_1' + \eta_2')^2}{\xi_1'+\xi_2'} = \frac{(\eta_3'+\eta_4')^2}{\xi_3'+\xi_4'} \end{align*} $$

from the third equation to find

$$ \begin{align*} \left\{ \begin{array}{cl} \xi_1' + \xi_2' &= \xi_3' + \xi_4', \\ (\xi_1')^{\alpha+1} + (\xi_2')^{\alpha+1}- \frac{(\eta_1' \xi_2' - \eta_2' \xi_1')^2}{\xi_1' \xi_2' (\xi_1'+\xi_2')} &= (\xi_3')^{\alpha+1} + (\xi_4')^{\alpha+1} \\ &\quad \quad - \frac{(\eta_3' \xi_4' - \eta_4' \xi_3')^2}{\xi_3' \xi_4' (\xi_3'+\xi_4')} + \mathcal{O}(L_{\max}/N_1^{\alpha+1}). \end{array} \right. \end{align*} $$

This yields

$$ \begin{align*} \left\{ \begin{array}{cl} \xi_1' + \xi_2' &= \xi_3' + \xi_4', \\ (\xi_1')^{\alpha+1} + (\xi_2')^{\alpha+1} &= (\xi_3')^{\alpha+1} + (\xi_4')^{\alpha+1} + \mathcal{O}(\frac{D^2 N_2}{N_1^{\alpha+1}} + \frac{L_{\max}}{N_1^{\alpha+1}}). \end{array} \right. \end{align*} $$

Note that for our Whitney decomposition we always have $D^2 N_2 \gtrsim L_{\max }$ . Note that the curve $\xi ' \mapsto (\xi ')^{\alpha +1}$ degenerates at the origin for $\alpha> -1$ . To still find an almost orthogonality resembling the Córdoba–Fefferman square function estimate, we rewrite the second line as

$$ \begin{align*} f'(\xi_{1*}) (\xi_1' - \xi_3') + f'(\xi_{2*})(\xi_2'-\xi_4') = \mathcal{O}\big( \frac{D^2 N_2}{N_1^\alpha N_1} \big). \end{align*} $$

We have $f'(\xi _{2*}) = f'(\xi _{1*}) + \Delta $ with $|\Delta | \gtrsim 1$ , for which reason

$$ \begin{align*} f'(\xi_{1*}) (\xi_1' - \xi_3' + \xi_2' - \xi_4') + \Delta (\xi_2'-\xi_4') = \mathcal{O}\big( \frac{D^2 N_2}{N_1^\alpha N_1} \big). \end{align*} $$

Consequently, $\xi _i' = \xi _{i+2}' + \mathcal {O}\big ( \frac {D^2 N_2}{N_1^\alpha N_1} \big )$ for $i \in \{1,2\}$ , and we obtain an almost orthogonal decomposition of

$$ \begin{align*} \| f^{\prime}_{1,N_1,L_1} * f^{\prime}_{2,N_2,L_2} \|^2_{L^2_{\tau,\xi,\eta}} \lesssim \sum_{I_1', I^{\prime}_2} \| f^{\prime}_{1,N_1,L_1,I^{\prime}_1} * f^{\prime}_{2,N_2,L_2,I^{\prime}_2} \|^2_{L^2} \end{align*} $$

with $\xi '$ -intervals of length $\mathcal {O}(\frac {D^2 N_2}{N_1^\alpha N_1})$ . After rescaling we obtain a decomposition into intervals of length $D^2 N_2 / N_1^\alpha $ .

First we handle the contribution $D \gg L_{\max }/N_2$ . Applying the bilinear Strichartz estimate Proposition 4.1 gives

$$ \begin{align*} \| f^{I_1}_{1,N_1,L_1} * f^{I_2}_{2,N_2,L_2} \|_{L^2_{\tau,\xi,\eta}} \lesssim \frac{D N_2^{\frac{1}{2}}}{N_1^{\frac{\alpha}{2}}} D^{-\frac{1}{2}} \prod_{i=1}^2 L_i^{\frac{1}{2}} \| f^{I_i}_{i,N_i,L_i} \|_2. \end{align*} $$

Summation in the intervals can be carried out by almost orthogonality. Summation in $L_{\max } / N_2 \ll D \lesssim N_1^{\alpha /2}$ gives

$$ \begin{align*} \sum_{L_{\max} / N_2 \ll D \lesssim N_1^{\alpha/2}} \frac{D^{\frac{1}{2}} N_2^{\frac{1}{2}}}{N_1^{\frac{\alpha}{2}}} \lesssim \frac{N_2^{\frac{1}{2}}}{N_1^{\frac{\alpha}{4}}}. \end{align*} $$

For the contribution $D \sim \big ( \frac {L_{\max }}{N_2} \big )^{\frac {1}{2}}$ we use Lemma 4.3 after almost orthgonal decomposition into intervals of length $\big ( \frac {L_{\max }}{N_1^{\alpha }} \big )^{\frac {1}{2}}$ :

$$ \begin{align*} \| f_{1,N_1,L_1}^{I_1} * f^{I_2}_{2,N_2,L_2} \|_{L^2_{\tau,\xi,\eta}} \lesssim L_{\min}^{\frac{1}{2}} \big( \frac{L_{\max}}{N_1^\alpha} \big)^{\frac{1}{2}} N_2^{\frac{1}{4}} L_{\max}^{\frac{1}{4}} \prod_{i=1}^2 \| f_{i,N_i,L_i}^{I_i} \|_2. \end{align*} $$

By the upper bound for $L_{\max }$ this gives

$$ \begin{align*} \| f_{1,N_1,L_1}^{I_1} * f^{I_2}_{2,N_2,L_2} \|_{L^2_{\tau,\xi,\eta}} \lesssim \frac{N_2^{\frac{1}{2}}}{N_1^{\frac{\alpha}{4}}} \prod_{i=1}^2 \| f_{i,N_i,L_i}^{I_i} \|_2. \end{align*} $$

This handles all possible transversalities $D \in [\big ( \frac {L_{\max }}{N_2} \big )^{\frac {1}{2}}, N_1^\alpha ]$ . The proof is complete.

We have the following analog on $\mathbb {R} \times \mathbb {T}$ :

Lemma 4.5. Let $N_i \in 2^{\mathbb {Z}}$ , $N_2 \ll N_1$ , $N_1 \gtrsim 1$ , $L_i \in 2^{\mathbb {N}_0}$ , $i=1,2$ , $D^* \in 2^{\mathbb {N}}$ . Let $\text {supp}(f_{i,N_i,L_i}) \subseteq D_{N_i,L_i}$ , $i=1,2$ with

$$ \begin{align*} \big| \frac{\eta_1}{\xi_1} - \frac{\eta_2}{\xi_2} \big| \lesssim D^* \end{align*} $$

for $(\xi _i,\eta _i) \in \pi _{\xi ,\eta }(\text {supp}(f_{i,N_i,L_i}))$ . Then the following estimate holds:

(4.11) $$ \begin{align} \| f_{1,N_1,L_1} * f_{2,N_2,L_2} \|_{L^2_{\tau,\xi,\eta}} \lesssim \log(D^*) N_2^{\frac{1}{2}} L_{\min}^{\frac{1}{2}} \langle L_{\max} / N_1^{\frac{\alpha}{2}} \rangle^{\frac{1}{2}} \prod_{i=1}^2 \| f_{i,N_i,L_i} \|_2. \end{align} $$

Proof. First, we suppose that $L_{\max } \gtrsim N_1^\alpha N_2$ . In this case we apply Lemma 4.3 to find

$$ \begin{align*} \| f_{1,N_1,L_1} * f_{2,N_2,L_2} \|_{L^2} \lesssim N_2^{\frac{1}{2}} L_{\min}^{\frac{1}{2}} \langle L_{\max} N_2 \rangle^{\frac{1}{4}} \prod_{i=1}^2 \| f_{i,N_i,L_i} \|_2, \end{align*} $$

which implies (4.11).

Next, suppose that $L_{\max } \ll N_1^\alpha N_2$ . We carry out a Whitney decomposition in the transversality parameter

$$ \begin{align*} D \sim \big| \frac{\eta_1}{\xi_1} - \frac{\eta_2}{\xi_2} \big| \end{align*} $$

in the range $D \in [ \big ( \frac {L_{\max }}{N_2} \big )^{\frac {1}{2}}, D^*]$ :

$$ \begin{align*} \| f_{1,N_1,L_1} * f_{2,N_2,L_2} \|_{L^2_{\tau,\xi,\eta}} \leqslant \sum_{D \in \big[ \big( \frac{L_{\max}}{N_2}\big)^{\frac{1}{2}}, D^* ]} \sum_{I_1^D \sim I_2^D} \| f_{1,N_1,L_1}^{I_{1}^D} * f_{2,N_2,L_2}^{I_{2}^D} \|_{L^2_{\tau,\xi,\eta}}. \end{align*} $$

By the argument from the proof of Lemma 4.4 we can effectively localize the $\xi $ -support to intervals of length $\mathcal {O}(\frac {D^2 N_2}{N_1^\alpha } \big )$ . We obtain for $D= \big ( L_{\max } / N_2 \big )^{\frac {1}{2}}$ by applying Lemma 4.3

(4.12) $$ \begin{align} \| f^{I_{1}^D}_{1,N_1,L_1} * f^{I_{2}^D}_{2,N_2,L_2} \|_{L^2_{\tau,\xi,\eta}} \lesssim L_{\min}^{\frac{1}{2}} \frac{L_{\max}^{\frac{1}{2}}}{N_1^{\frac{\alpha}{2}}} \langle L_{\max} N_2 \rangle^{\frac{1}{4}} \prod_{i=1}^2 \| f_{i,N_i,L_i}^{I_{i}^D} \|_{L^2}. \end{align} $$

This is sufficient for $L_{\max } \ll N_1^\alpha N_2$ .

Next, we handle the contribution $D \in \big ( \big ( \frac {L_{\max }}{N_2} \big )^{\frac {1}{2}}, N_1^{\alpha /2} \big ]$ . After localizing the $\xi $ -support to intervals of length $\mathcal {O}\big ( D^2 N_2 / N_1^\alpha \big )$ by almost orthogonality, we can apply Proposition 4.1 to find

(4.13) $$ \begin{align} \begin{aligned} &\quad \sum_{D \in \big( \big( \frac{L_{\max}}{N_2}\big)^{\frac{1}{2}}, N_1^{\frac{\alpha}{2}} \big) ]} \sum_{I_1^D \sim I_2^D} \| f_{1,N_1,L_1}^{I_{1}^D} * f_{2,N_2,L_2}^{I_{2}^D} \|_{L^2_{\tau,\xi,\eta}} \\ &\lesssim L_{\min}^{\frac{1}{2}} \sum_{D \in \big( \big( \frac{L_{\max}}{N_2}\big)^{\frac{1}{2}}, N_1^{\frac{\alpha}{2}} \big) ]} \frac{D N_2^{\frac{1}{2}}}{N_1^{\frac{\alpha}{2}}} \langle L_{\max} / D \rangle^{\frac{1}{2}} \prod_{i=1}^2 \| f_{i,N_i,L_i} \|_2 \\ &\lesssim L_{\min}^{\frac{1}{2}} N_2^{\frac{1}{2}} \langle L_{\max} / N_1^{\alpha/2} \rangle^{\frac{1}{2}} \prod_{i=1}^2 \| f_{i,N_i,L_i} \|_2. \end{aligned} \end{align} $$

Finally, we turn to the contribution with large transversality. Here we apply Proposition 4.1 directly to find

(4.14) $$ \begin{align} \begin{aligned} &\quad \sum_{D \in [ N_1^{\frac{\alpha}{2}} , D^* ]} \sum_{I_1^D \sim I_2^D} \| f_{1,N_1,L_1}^{I_{1}^D} * f_{2,N_2,L_2}^{I_{2}^D} \|_{L^2_{\tau,\xi,\eta}} \\ &\lesssim N_2^{\frac{1}{2}} L_{\min}^{\frac{1}{2}} \sum_{D \in [ N_1^{\frac{\alpha}{2}} , D^* ]} \langle L_{\max} / D \rangle^{\frac{1}{2}} \prod_{i=1}^2 \| f_{i,N_i,L_i} \|_2 \\ &\lesssim \log(D^*) N_2^{\frac{1}{2}} \langle L_{\max} / N_1^{\alpha/2} \rangle^{\frac{1}{2}} \prod_{i=1}^2 \| f_{i,N_i,L_i} \|_2. \end{aligned} \end{align} $$

Collecting contributions (4.12)-(4.14) the proof is complete.

We record the following simple estimate, which is a consequence of the Cauchy-Schwarz inequality. This will serve as substitute when (4.8) fails:

Lemma 4.6. Let $f_{i,N_i,L_i} : \mathbb {R} \times \mathbb {D}^* \to \mathbb {C}$ satisfy support properties $\pi _{\xi } \text {supp}(f_i) \subseteq I_i$ , $i=1,2$ with $|I_i| \sim N_i$ and $\pi _{\eta } \text {supp}(f_i) \subseteq J_i$ with $|J_i| \lesssim M_i$ and $|\tau _i - \omega _\alpha (\xi _i,\eta _i)| \lesssim L_i$ for $(\tau _i,\xi _i,\eta _i) \in \text {supp}(f_{i,N_i,L_i})$ and $i=1,2$ . The following estimate holds:

$$ \begin{align*} \| f_{1,N_1,L_1} * f_{2,N_2,L_2} \|_{L^2_{\tau,\xi,\eta}} \lesssim (N_{\min} M_{\min} L_{\min})^{\frac{1}{2}} \prod_{i=1}^2 \| f_{i,N_i,L_i} \|_{L^2}. \end{align*} $$

4.2 Nonlinear Loomis-Whitney inequalities with measure

In preparation for the proof of trilinear convolution estimates for approximate solutions to dispersion-generalized KP-I equations, we prove Theorem 1.1. We impose the following assumptions on the hypersurfaces $(S_i)_{i=1,2,3}$ following [Reference Kinoshita and Schippa30, Reference Koch and Steinerberger33]:

Assumption 4.7. For $i=1,2,3$ there exist $0 < \beta \leqslant 1$ , $b>0$ , $A \geqslant 1$ , $F_i \in C^{1,\beta }(\mathcal {U}_i)$ , where the $\mathcal {U}_i$ denote open and convex sets in $\mathbb {R}^2$ and $G_i \in O(3)$ such that

  1. (i) the oriented surfaces $S_i$ are given by

    $$ \begin{align*} S_i = G_i \text{gr}(F_i), \quad \text{gr}(F_i) = \{ (x,y,z) \in \mathbb{R}^3 : z = F_i(x,y), \; (x,y) \in \mathcal{U}_i \}; \end{align*} $$
  2. (ii) the vector field $\mathfrak {n}_i : S_i \to \mathbb {S}^2$ of outward unit normals on $S_i$ satisfies the Hölder condition:

    $$ \begin{align*} \sup_{\sigma,\tilde{\sigma}} \frac{|\mathfrak{n}_i(\sigma) - \mathfrak{n}_i(\tilde{\sigma})|}{|\sigma - \tilde{\sigma}|^\beta} + \frac{|\mathfrak{n}_i(\sigma).(\sigma - \tilde{\sigma})|}{|\sigma - \tilde{\sigma}|^{1+\beta}} \leqslant b; \end{align*} $$
  3. (iii) there is $A \geqslant 1$ such that for all $\sigma _i \in S_i$ , $i=1,2,3$ the following estimate holds:

    $$ \begin{align*} A^{-1} \leqslant |\mathfrak{n}_1(\sigma_1) \wedge \mathfrak{n}_2(\sigma_2) \wedge \mathfrak{n}_3(\sigma_3) | \leqslant 1. \end{align*} $$

For convenience, we recall the statement of Theorem 1.1:

Theorem 4.8 (Nonlinear Loomis–Whitney inequalities with general measure)

Let $\varepsilon>0$ , $(S_i)_{i=1,2,3}$ be a collection of hypersurfaces, which satisfy Assumption 4.7, $\nu _{\gamma }$ be a Borel measure, which satisfies (1.7), and $f_i \in L^2(S_i(\varepsilon ),d\nu _\gamma )$ , $i=1,2$ . Then the following estimate holds:

$$ \begin{align*} \| f_1 * f_2 \|_{L^2(S_3(\varepsilon),d\nu_\gamma)} \lesssim A^{\frac{1}{2}} \varepsilon^{\frac{\gamma}{2}} \prod_{i=1}^2 \| f_i \|_{L^2(S_i(\varepsilon),d\nu_\gamma)}. \end{align*} $$

We emphasize that the almost-orthogonal decompositions used in [Reference Kinoshita and Schippa30] do not depend on the underlying measure. This fact makes the strategy applicable to periodic or cylindrical domains as well.

Proof. We follow the argument in [Reference Kinoshita and Schippa30]. By duality it suffices to show the trilinear expression

$$ \begin{align*} \int_{S_3(\varepsilon)} (f_1 * f_2) f_3 d \nu_\gamma \lesssim A^{\frac{1}{2}} \varepsilon^{\frac{\gamma}{2}} \prod_{i=1}^3 \| f_i \|_{L^2(S_i(\varepsilon),d \nu_\gamma)}. \end{align*} $$

To this end, let $(B_{\varepsilon ,j})_{j \in \mathbb {N}}$ be an essentially disjoint cover of $\mathbb {R}^3$ with balls of size $\varepsilon $ . Set

$$ \begin{align*} J_{3,\varepsilon} = \{ j \in \mathbb{N} : B_{\varepsilon,j} \cap S_3(\varepsilon) \neq \emptyset \} \text{ and } S_{3,j}(\varepsilon) = B_{\varepsilon,j} \cap S_3(\varepsilon). \end{align*} $$

By Minkowski’s inequality we find

$$ \begin{align*} \big| \int_{\mathbb{R}^3} (f_1 * f_2)(\lambda) f_3(\lambda) d\nu_\gamma(\lambda) \big| \leqslant \sum_{j \in J_{3,\varepsilon}} \big| \int_{\mathbb{R}^3} (f_1 * f_2)(\lambda) f_3 \big\vert_{S_{3,j}(\varepsilon)}(\lambda) d\nu_\gamma(\lambda) \big|. \end{align*} $$

By Hölder’s inequality and (1.7), we find

$$ \begin{align*} \big| \int_{\mathbb{R}^3} (f_1 * f_2)(\lambda) f_3 \big\vert_{S_{3,j_3}(\varepsilon)}(\lambda) d\nu_\gamma (\lambda) \big| \lesssim \varepsilon^{\frac{\gamma}{2}} \prod_{i=1}^3 \| f_i \|_{L^2(S_{i,j,\varepsilon})}. \end{align*} $$

Above we denote

$$ \begin{align*} S_{1,j,\varepsilon} &= \{ \lambda_1 \in S_1(\varepsilon) : \exists \lambda' \in B_{\varepsilon,j} : \lambda' - \lambda_1 \in S_2(\varepsilon) \}, \\ S_{2,j,\varepsilon} &= \{ \lambda_2 \in S_2(\varepsilon) : \exists \lambda' \in B_{\varepsilon,j} : \lambda' - \lambda_2 \in S_1(\varepsilon)\}. \end{align*} $$

The following estimate was proved in [Reference Kinoshita and Schippa30, Eq. (16), p. 13]:

(4.15) $$ \begin{align} \sum_{j \in J_{3,\varepsilon}} \chi_{S_{1,j,\varepsilon} \times S_{2,j,\varepsilon}}(\lambda_1,\lambda_2) \lesssim A. \end{align} $$

With this at hand, we can conclude as follows:

$$ \begin{align*} \begin{aligned} &\quad \sum_{j \in J_{3,\varepsilon}} \big| \int_{\mathbb{R}^3} (f_1 * f_2)(\lambda) f_3 \big\vert_{S_{3,j}(\varepsilon)}(\lambda) d \nu_\gamma(\lambda) \big| \\ &\lesssim \varepsilon^{\frac{\gamma}{2}} \sum_{j \in J_{3,\varepsilon}} \| f_1 \|_{L^2(S_{1,j,\varepsilon}, d\nu_\gamma)} \| f_2 \|_{L^2(S_{2,j,\varepsilon},d \nu_\gamma)} \| f_3\|_{L^2(S_{3,j}(\varepsilon),d\nu_\gamma)} \\ &\lesssim \varepsilon^{\frac{\gamma}{2}} \big( \sum_{ j \in J_{3,\varepsilon}} \| f_3 \|_{L^2(S_{3,j}(\varepsilon),d\nu_\gamma)}^2 \big)^{\frac{1}{2}} \big( \sum_{j \in J_{3,\varepsilon}} \| f_1 \|^2_{L^2(S_{1,j,\varepsilon}, d\nu_\gamma)} \| f_2 \|_{L^2(S_{2,j,\varepsilon},d\nu_\gamma)}^2 \big)^{\frac{1}{2}} \\ &\lesssim \varepsilon^{\frac{\gamma}{2}} \| f_3 \|_{L^2(S_3(\varepsilon),d\nu_\gamma)} \big( \int_{\mathbb{R}^3 \times \mathbb{R}^3} \sum_{j \in J_{3,\varepsilon}} \chi_{S_{1,j,\varepsilon} \times S_{2,j,\varepsilon}}(\lambda_1,\lambda_2) \\ &\quad \qquad \quad \times |f_1(\lambda_1)|^2 |f_2(\lambda_2)|^2 d\nu_\gamma(\lambda_1) d\nu_\gamma(\lambda_2) \big)^{\frac{1}{2}} \\ &\lesssim \varepsilon^{\frac{\gamma}{2}} A^{\frac{1}{2}} \prod_{i=1}^3 \| f_i \|_{L^2(S_i(\varepsilon)}. \end{aligned}\\[-46pt] \end{align*} $$

4.3 Resonance and the nonlinear Loomis–Whitney inequality

In addition to the lower bound for the difference in group velocity in the resonant case, we shall see that we can compute the full transversality. To show a trilinear estimate in the resonant case, consider

$$ \begin{align*} \int (f_{1,N_1,L_1} * f_{2,N_2,L_2} ) f_{3,N_3,L_3} d \tau d \xi d \eta \end{align*} $$

with $\text {supp}(f_{i,N_i,L_i}) \subseteq D_{N_i, \leqslant L_i}$ with $L_i \ll N_1^\alpha N_2$ . Let $N = \max (N_i)$ . We suppose that $N_1 = N$ and $N_3 \sim N_1 \gtrsim N_2$ . We use the scaling

(4.16) $$ \begin{align} \tau \to \frac{\tau}{ N^{\alpha+1}}, \; \xi \to \frac{\xi}{N}, \; \eta \to \frac{\eta}{ N^{\frac{\alpha}{2}+1}} \end{align} $$

to reduce to $1 \sim |\xi _1'| \sim |\xi _3'| \gtrsim |\xi _2'| \sim \frac {N_2}{N_1}$ . The smallness of $|\xi _2'|$ allows us to localize $\xi _i'$ to intervals of length $\frac {N_2}{N_1}$ using almost orthogonality.

In the resonant case, it holds, moreover

$$ \begin{align*} \big| \frac{\eta_1'}{\xi_1'} - \frac{\eta_2'}{\xi_2'} \big| \sim 1. \end{align*} $$

This induces an almost orthogonal decomposition in $\eta _i'/\xi _i'$ (cf. [Reference Ionescu, Kenig and Tataru22]), by which we can suppose that $\eta _i'/\xi _i'$ is localized to intervals of size $\sim 1$ . Now we use a Galilean invariance:

$$ \begin{align*} \frac{\eta_i'}{\xi_i'} \to \frac{\eta_i'}{\xi_i'} - A. \end{align*} $$

This localizes $|\frac {\eta _i'}{\xi _i'}| \lesssim 1$ . Considering $i=2$ , we can suppose that $|\eta _2'| \lesssim N_2/N_1$ . This induces an almost orthogonal decomposition in $\eta _i'$ , by which we can suppose that $(\xi _i',\eta _i')$ are localized to balls of size $c(N_2/N_1)$ for some $c \ll 1$ to be chosen later. We stress that like in the proof of Proposition 3.3 for $(\xi ',\eta ') \in \mathbb {R} \times \mathbb {Z}/(N_1^{\frac {\alpha }{2}+1})$ , we have in general for the transformed variables $(\xi ',\eta ' - A \xi ') \notin \mathbb {R} \times \mathbb {Z}/(N_1^{\frac {\alpha }{2}+1})$ and some care is required on the cylinder when estimating the measure.

To compute the full transversality, we need to consider the wedge product of normals

$$ \begin{align*} |\mathfrak{n}(\xi_1,\eta_1) \wedge \mathfrak{n}(\xi_2,\eta_2) \wedge \mathfrak{n}(\xi_3,\eta_3) |. \end{align*} $$

We compute

$$ \begin{align*} \mathfrak{n}(\xi',\eta') = \begin{pmatrix} -(\alpha+1) |\xi'|^{\alpha} + (\eta')^2 / (\xi')^2 \\ -2 \eta' / \xi' \\ 1 \end{pmatrix}. \end{align*} $$

The normals have modulus $\sim 1$ after rescaling and supposing that $|\eta '| \lesssim 1$ . This is clear for $\mathfrak {n}(\xi _i',\eta _i')$ for $i=1,3$ since $|\xi _i'|\sim 1$ . In the resonant case it holds moreover

$$ \begin{align*} \big| \frac{\eta_1'}{\xi_1'} - \frac{\eta_2'}{\xi_2'} \big| \sim 1, \end{align*} $$

for which reason we have $|\mathfrak {n}(\xi _2',\eta _2')| \sim 1$ .

Let $C_\alpha = \alpha +1$ . We find under the convolution constraint:

$$ \begin{align*} \begin{aligned} &\quad \det(\mathfrak{n}(\xi_1,\eta_1), \mathfrak{n}(\xi_2,\eta_2), \mathfrak{n}(\xi_1+\xi_2,\eta_1+\eta_2)) \\ &= \begin{vmatrix} -C_\alpha |\xi_1|^{\alpha} + \frac{\eta_1^2}{\xi_1^2} & -C_\alpha |\xi_2|^\alpha + \frac{\eta_2^2}{\xi_2^2} & -C_\alpha |\xi_1+\xi_2|^\alpha + \frac{(\eta_1+\eta_2)^2}{(\xi_1+\xi_2)^2} \\ - \frac{2 \eta_1}{\xi_1} & - \frac{2 \eta_2}{\xi_2} & - \frac{2(\eta_1+\eta_2)}{\xi_1+\xi_2} \\ 1 & 1 & 1 \end{vmatrix} \\ &= \frac{-2}{\Omega_{KdV}} \begin{vmatrix} -C_\alpha \xi_1 |\xi_1|^\alpha + \frac{\eta_1^2}{\xi_1} & -C_\alpha \xi_2 |\xi_2|^\alpha + \frac{\eta_2^2}{\xi_2} & - C_\alpha |\xi_1+\xi_2|^\alpha (\xi_1+\xi_2) + \frac{(\eta_1+\eta_2)^2}{\xi_1 + \xi_2} \\ \eta_1 & \eta_2 & \eta_1 + \eta_2 \\ \xi_1 & \xi_2 & \xi_1 + \xi_2 \end{vmatrix}. \end{aligned} \end{align*} $$

where $\Omega _{KdV} = \xi _1\xi _2(\xi _1+\xi _2)$ . Now we subtract the first column and the second column from the third column to find

$$ \begin{align*} \begin{aligned} &\quad \begin{vmatrix} -C_\alpha \xi_1 |\xi_1|^\alpha + \frac{\eta_1^2}{\xi_1} & -C_\alpha \xi_2 |\xi_2|^\alpha + \frac{\eta_2^2}{\xi_2} & - C_\alpha |\xi_1+\xi_2|^\alpha (\xi_1+\xi_2) + \frac{(\eta_1+\eta_2)^2}{\xi_1 + \xi_2} \\ \eta_1 & \eta_2 & \eta_1 + \eta_2 \\ \xi_1 & \xi_2 & \xi_1 + \xi_2 \end{vmatrix} \\ &= \begin{vmatrix} -C_\alpha \xi_1 |\xi_1|^\alpha + \frac{\eta_1^2}{\xi_1} & -C_\alpha \xi_2 |\xi_2|^\alpha + \frac{\eta_2^2}{\xi_2} & - C_\alpha \Omega_{\alpha,1} + \frac{(\eta_1+\eta_2)^2}{\xi_1 + \xi_2} - \frac{\eta_1^2}{\xi_1} - \frac{\eta_2^2}{\xi_2} \\ \eta_1 & \eta_2 & 0 \\ \xi_1 & \xi_2 & 0 \end{vmatrix} \\ &= (\eta_1 \xi_2 - \eta_2 \xi_1) (- C_\alpha \Omega_{\alpha,1} + \frac{(\eta_1+\eta_2)^2}{\xi_1 + \xi_2} - \frac{\eta_1^2}{\xi_1} - \frac{\eta_2^2}{\xi_2}) \\ &= -(\eta_1 \xi_2 - \eta_2 \xi_1) \big( C_\alpha \Omega_{\alpha,1} + \frac{(\eta_1 \xi_2 - \eta_2 \xi_1)^2}{(\xi_1+\xi_2) \xi_1 \xi_2} \big). \end{aligned} \end{align*} $$

This can be summarized as:

$$ \begin{align*} \begin{aligned} &\quad |\mathfrak{n}(\xi_1',\eta_1') \wedge \mathfrak{n}(\xi_2',\eta_2') \wedge \mathfrak{n}(\xi_1'+\xi_2',\eta^{\prime}_1+\eta_2') | \\ &= \frac{2 |\eta_1' \xi_2' - \eta_2' \xi_1'|}{|\xi_1' \xi_2' (\xi_1' + \xi_2')|} \big| C_\alpha \Omega_{\alpha,1} (\xi') + \frac{(\eta_1' \xi_2' - \eta_2' \xi_1')^2}{\xi_1' \xi_2' (\xi_1'+\xi_2')} \big|. \end{aligned} \end{align*} $$

Note that $\Omega _{\alpha ,1}$ and $\frac {(\eta _1' \xi _2' - \eta _2' \xi _1')^2}{\xi _1' \xi _2' (\xi _1' + \xi _2')}$ have the same sign and by the resonance condition a comparable modulus:

$$ \begin{align*} |\mathfrak{n}(\xi_1',\eta_1') \wedge \mathfrak{n}(\xi_2',\eta_2') \wedge \mathfrak{n}(\xi_1'+\xi_2',\eta_1'+\eta_2')| \sim \frac{|\eta_1' \xi_2' - \eta_2' \xi_1'|}{|\xi_1' \xi_2' (\xi_1'+\xi_2')|} \cdot \frac{N_2}{N_1} \sim \frac{N_2}{N_1}. \end{align*} $$

The extension off the convolution constraint for perturbations of size $c(N_2/N_1)$ is carried out by checking $|\partial _{\xi '} \mathfrak {n}(\xi _3',\eta _3')| + |\partial _{\eta '} \mathfrak {n}(\xi _3',\eta _3')| \lesssim 1$ . This is immediate from $|\xi _3'| \sim 1$ and $|\eta _3'| \lesssim 1$ .

From $\mathfrak {n} \in C^2(\mathbb {R}^2 \backslash (\{0\} \times \mathbb {R}))$ the Hölder regularity Assumption 4.7 (ii) with $\beta =1$ follows. We can allow for crude estimates since the constant in the nonlinear Loomis-Whitney estimate does not depend on b and $\beta $ .

Now we can formulate the trilinear estimate in the resonant case on different domains:

Proposition 4.9. Let $2^{\mathbb {N}_0} \ni N_1 \sim N_3 \gtrsim N_2 \in 2^{\mathbb {Z}}$ , $L_i \in 2^{\mathbb {N}_0}$ , and $f_{i,N_i,L_i} \in L^2(\mathbb {R}^3)$ with $\text {supp}(f_{i,N_i,L_i}) \subseteq D_{\alpha ,N_i,\leqslant L_i}$ , $i=1,2,3$ . Suppose that $L_{\max } \ll N_1^\alpha N_2$ . Then the following estimate holds:

(4.17) $$ \begin{align} \big| \int_{\mathbb{R}^3} (f_{1,N_1,L_1} * f_{2,N_2,L_2} ) f_{3,N_3,L_3} d \xi d\eta d\tau \big| \lesssim N_1^{\frac{1}{2}-\frac{3 \alpha}{4}} N_2^{-\frac{1}{2}} \prod_{i=1}^3 L_i^{\frac{1}{2}} \| f_{i,N_i,L_i} \|_{L^2_{\tau,\xi,\eta}(\mathbb{R}^3)}. \end{align} $$

Under the above assumptions, if $f_{i,N_i,L_i} \in L^2(\mathbb {R} \times \mathbb {R} \times \mathbb {Z}/\gamma )$ for some $\gamma \in (1/2,1]$ , then the following estimate holds:

(4.18) $$ \begin{align} \big| \int \big( f_{1,N_1,L_1} * f_{2,N_2,L_2} \big) f_{3,N_3,L_3} d \xi (d \eta)_\gamma d \tau \big| \lesssim C(\underline{N},\underline{L})\prod_{i=1}^3 \| f_{i,N_i,L_i} \|_{L^2_{\tau, \xi, \eta}(\mathbb{R} \times \mathbb{R} \times \mathbb{Z}/\gamma)} \end{align} $$

with

$$ \begin{align*} C(\underline{N},\underline{L}) = \big( \frac{N_1}{N_2} \big)^{\frac{1}{2}} (L_{\min} / N_1^{\alpha/2})^{\frac{1}{2}} \langle L_{\text{med}} / N_1^{\alpha/2} \rangle^{\frac{1}{2}} (L_{\max} / N_1^{\alpha/2} )^{\frac{1}{2}}. \end{align*} $$

Remark 4.10. The estimate (4.17) recovers [Reference Sanwal and Schippa41, Lemma 4.2]. We shall be brief in the proof. For $\alpha = 2$ , (4.18) recovers Robert’s estimate [Reference Robert38, Proposition 5.7].

Proof. We start with the proof of the estimate in Euclidean space. To ease notation, let $N = N_1$ . Firstly, we decompose $f_{i,j_i,k_i} = \sum _c f^c_{i,j_i,k_i}$ into $\sim \langle L_i \rangle $ functions, which are in the $1$ -neighbourhood of a translation of the characteristic surface. Write below $g_{i,N_i,L_i} = f^c_{i,N_i,L_i}$ to ease notation. We use the anisotropic rescaling to find

$$ \begin{align*} \begin{aligned} &\quad \int (g_{1,N_1,L_1} * g_{2,N_2,L_2} ) g_{3,N_3,L_3} d \tau d \xi d \eta \\ &= N^{2(\alpha+1)} N^2 N^{\alpha + 2} \int (g^{\prime}_{1,N_1,L_1} * g^{\prime}_{2,N_2,L_2} ) g^{\prime}_{3,N_3,L_3} d \tau' d \xi' d \eta'. \end{aligned} \end{align*} $$

This makes the rescaled functions $f^c_{i,N_i,L_i}$ (or a translate thereof) supported in the $N^{-(\alpha +1)}$ -neighbourhood of the characteristic surface. After the almost orthogonal decomposition from above, we can suppose that $|\eta _i'| \lesssim 1$ . We have computed for the transversality:

$$ \begin{align*} |\mathfrak{n}(\xi_1',\eta_1') \wedge \mathfrak{n}(\xi_2',\eta_2') \wedge \mathfrak{n}(\xi_3',\eta_3') | \sim \frac{N_2}{N_1}. \end{align*} $$

In the above $(\xi _i',\eta _i')$ are contained in balls of size $c(N_2 / N_1)$ , which constitute an almost orthogonal decomposition of the spatial frequency support.

Hence, we can apply Theorem 1.1 with Lebesgue measure and $\varepsilon = N^{-(\alpha +1)}$ to find

$$ \begin{align*} | \int (g^{\prime}_{1,N_1,L_1} * g^{\prime}_{2,N_2,L_2} ) g^{\prime}_{3,N_3,L_3} d \tau' d \xi' d \eta' | \lesssim \big( \frac{N_1}{N_2} \big)^{\frac{1}{2}} N^{-\frac{3(\alpha+1)}{2}} \prod_{i=1}^3 \| g^{\prime}_{i,N_i,L_i} \|_{L^2}. \end{align*} $$

The claim follows from reversing the scaling (4.16), which yields a factor of $N^{-\frac {3(\alpha +1)}{2}} N^{-\frac {3}{2}} N^{-\frac {3(\alpha +2)}{4}}$ , and summing over $c_i$ with $\# c_i \sim L_i$ with Cauchy-Schwarz. This finishes the proof in the Euclidean case.

We turn to the cylinder case. First we suppose that $L_{\text {med}} \ll N_1^{\alpha /2}$ . If $L_{\max } \leqslant N_1^{\alpha /2}$ , we do not decompose. If $L_{\max } \geqslant N_1^{\alpha /2}$ , we decompose $f_{i,N_i,L_i}$ with $L_i = L_{\max }$ into layers having modulation size $N_1^{\alpha /2}$ such that in the following we suppose $L_{\max } \lesssim N_1^{\alpha /2}$ . We use the anisotropic scaling

$$ \begin{align*} \tau \to \tau' = \frac{\tau}{N_1^{\alpha+1}}, \quad \xi \to \xi' = \frac{\xi}{ N}, \quad \eta \to \eta'=\frac{\eta}{N_1^{\frac{\alpha}{2}+1}}, \end{align*} $$

which leads to

$$ \begin{align*} \begin{aligned} &\quad \big| \int_{\mathbb{R} \times \mathbb{R} \times \mathbb{Z}/\gamma} (f_{1,N_1,L_1} * f_{2,N_2,L_2} ) f_{3,N_3,L_3} d \xi (d \eta)_\gamma d\tau \big| = N_1^2 N_1^{2(\alpha+1)} \\ &\times (\gamma N_1^{\frac{\alpha}{2}+1}) \big| \int_{\mathbb{R} \times \mathbb{R} \times \mathbb{Z}/(\gamma N_1^{\frac{\alpha}{2}+1})} (f^{\prime}_{1,N_1,L_1} * f^{\prime}_{2,N_2,L_2} ) f_{3,N_3,L_3}' d\xi' (d\eta')_{\gamma N_1^{\frac{\alpha}{2}+1}} d\tau' \big|. \end{aligned} \end{align*} $$

Write $L_i' = L_i / N_1^{\alpha +1}$ . We carry out the Galilean transform

$$ \begin{align*} (\xi",\eta") = (\xi',\eta' - A' \xi') \end{align*} $$

with $A' = N_1^{-\frac {\alpha }{2}} A$ such that given $\xi "$ we have $\eta " + A' \xi " \in \mathbb {Z} / N_1^{\frac {\alpha }{2}+1}$ . Moreover, we have $|\eta "| \lesssim 1$ and we can carry out like above an almost orthogonal decomposition of $(\xi ",\eta ")$ into balls of size $c(N_2/N_1)$ .

Next, we decompose the supports of $f^{\prime }_{i,N_i,L_i}$ into balls $\theta _i$ of size $L_{\max }' = \frac {L_{\max }}{N_1^{\alpha +1}} \lesssim N_1^{-\frac {\alpha }{2} - 1}$ . Then, we obtain

(4.19) $$ \begin{align} \begin{aligned} &\quad \sum_{\theta_3} \big| \int \sum_{\theta_1 \sim_{\theta_3} \theta_2} \big( f^{\prime}_{1,\theta_1} * f^{\prime}_{2,\theta_2} \big) f^{\prime}_{3,\theta_3} \big| \\ &\leqslant \sum_{\theta_3} \sum_{\theta_1 \sim_{\theta_3} \theta_2} \| f^{\prime}_{1,\theta_1} * f^{\prime}_{2,\theta_2} \|_{L^2_{(\tau,\xi,\eta)'}} \| f^{\prime}_{3,\theta_3} \|_{L^2_{(\tau,\xi,\eta)'}}. \end{aligned} \end{align} $$

By symmetry we can suppose that $L_1' = L_{\min }'$ . We estimate the convolution with the Cauchy-Schwarz inequality. Let $I_{L_{\max }'}$ denote the interval of length $L^{\prime }_{\max } = L_{\max }/(N_1^{\alpha +1})$ , which contains $\pi _{\eta "}(\text {supp}(f^{\prime }_{1,\theta _1}))$ . We let $J_{L_{\max }'}$ denote the interval which contains $\pi _{\xi "}(\text {supp}(f^{\prime }_{1,\theta _1})$ . We count the number of $\eta '$ such that $\eta ' - A' \xi ' \in I_{L_{\max }'}$ for $\xi " \in I^{\prime }_{L_{\max }'}$ . This is similar to the proof of Proposition 3.3:

$$ \begin{align*} \# \{ \eta' \in \mathbb{Z}/(N_1^{\frac{\alpha}{2}+1}) : (\xi",\eta") \in I_{L_{\max}'} \times I^{\prime}_{L_{\max}'} \} \lesssim \langle A' \cdot L^{\prime}_{\max} \cdot N_1^{\frac{\alpha}{2}+1} \rangle \sim \langle A' \cdot \frac{L_{\max}}{N_1^{\frac{\alpha}{2}}} \rangle. \end{align*} $$

Now, for fixed $\eta '$ from the above set, we estimate

$$ \begin{align*} \text{meas}( \{ \xi" \in I_{L_{\max}'} : (\xi",\eta") \in I^{\prime}_{L^{\prime}_{\max}} \times I_{L_{\max}} \} \lesssim \frac{L^{\prime}_{\max}}{A'}. \end{align*} $$

Given $(\xi ",\eta ")$ from above, we finally have

$$ \begin{align*} \text{meas} ( \{ \tau' \in \mathbb{R} : (\tau',\xi",\eta") \in \theta_1 \} ) \lesssim L^{\prime}_{\min}. \end{align*} $$

For this reason we find

$$ \begin{align*} \| f^{\prime}_{1,\theta_1} * f^{\prime}_{2,\theta_2} \|_{L^2_{\tau',\xi',\eta'}} \lesssim (L_{\min}' (L^{\prime}_{\max}/A') \langle A' \cdot \frac{L_{\max}}{N_1^{\frac{\alpha}{2}}} \rangle)^{\frac{1}{2}} \| f^{\prime}_{1,\theta_1} \|_{L^2_{\tau',\xi',\eta'}} \| f^{\prime}_{2,\theta_2} \|_{L^2_{\tau',\xi',\eta'}}. \end{align*} $$

By two more applications of the Cauchy-Schwarz inequality to carry out the summation over $\theta _i$ , we incur a factor of $A^{\frac {1}{2}} \sim \Big (\frac {N_1}{N_2}\Big )^{\frac {1}{2}}$ and obtain

$$ \begin{align*} \begin{aligned} &\quad \sum_{\theta_3} \sum_{\theta_1 \sim_{\theta_3} \theta_2} \| f^{\prime}_{1,\theta_1} * f^{\prime}_{2,\theta_2} \|_{L^2_{\tau',\xi',\eta'}} \| f^{\prime}_{3,\theta_3} \|_{L^2_{\tau',\xi',\eta'}} \\ &\lesssim (L^{\prime}_{\min} L^{\prime}_{\max})^{\frac{1}{2}} \sum_{\theta_3} \sum_{\theta_1 \sim_{\theta_3} \theta_2} \| f^{\prime}_{1,\theta_1} \|_{L^2_{\tau',\xi',\eta'}} \| f^{\prime}_{2,\theta_2} \|_{L^2_{\tau',\xi',\eta'}} \| f^{\prime}_{3,\theta_3} \|_{L^2_{\tau',\xi',\eta'}} \\ &\lesssim (L^{\prime}_{\min} L_{\max}')^{\frac{1}{2}} (N_1 /N_2)^{\frac{1}{2}} \prod_{i=1}^3 \| f^{\prime}_{i,N_i,L_i} \|_{L^2_{\tau',\xi',\eta'}}. \end{aligned} \end{align*} $$

Now we reverse the scaling which yields a factor $N_1^{-\frac {3}{2}} N_1^{-\frac {3}{2}(\alpha +1)}$ . Taking into account the scaling factor from above gives

$$ \begin{align*} N_1^2 N_1^{2(\alpha+1)} \big( \frac{N_1}{N_2} \big)^{\frac{1}{2}} N_1^{-\frac{3}{2}} N_1^{-\frac{3}{2}(\alpha+1)} N_1^{-(\alpha+1)} (L_{\min} L_{\max})^{\frac{1}{2}} = N_1^{\frac{1}{2}-\frac{\alpha}{2}} N_2^{-\frac{1}{2}} (L_{\min} L_{\max})^{\frac{1}{2}}. \end{align*} $$

This proves (4.18) in case $L_{\text {med}} \ll N_1^{\alpha /2}$ .

We turn to the case $L_{\text {med}} \gtrsim N_1^{\alpha /2}$ and suppose that $L_{\min } \ll N_1^{\alpha /2}$ . We decompose the modulation of $f_{i_j}$ with $L_{i_1} = L_{\text {med}}$ and $L_{i_2} = L_{\text {max}}$ into layers of thickness $N_1^{\frac {\alpha }{2}}$ , such that we can apply the previous result with $L_{\text {med}} \sim L_{\max } \sim N_1^{\alpha /2}$ . The claim follows then from the Cauchy-Schwarz inequality which incurs factors

$$ \begin{align*} (L_{\text{med}} / N_1^{\alpha/2})^{\frac{1}{2}} (L_{\text{max}} / N_1^{\alpha/2})^{\frac{1}{2}}. \end{align*} $$

Finally, we turn to the case $L_{\min } \gtrsim N_1^{\alpha /2}$ . In this case we decompose all functions into layers of modulation with size $N_1^{\alpha /2}$ . Then we can apply the previous arguments and finally, we can apply the Cauchy-Schwarz inequality, which incurs a factor of

$$ \begin{align*} \big( \prod_{i=1}^3 L_i \big)^{\frac{1}{2}} / N_1^{\frac{3 \alpha}{2}}. \end{align*} $$

This completes the proof of the Loomis-Whitney inequality on the cylinder.

5 Ill-posedness results for KP-I equations

In this section, we show that (1.1) posed on $\mathbb {D} \in \{ \mathbb {R}^2, \mathbb {R} \times \mathbb {T}, \mathbb {T}^2 \}$ is $C^2$ ill-posed for different choices of $\alpha $ , namely one cannot use Picard iteration (the fixed point argument) to solve the problem. On $\mathbb {R}^2$ we prove the following optimal result, which improves on the argument from [Reference Sanwal and Schippa41]. Moreover, we show that on $\mathbb {R} \times \mathbb {T}$ for semilinear KP-I equations, the regularity for local well-posedness is strictly subcritical.

5.1 Sharp $C^2$ -ill-posedness for KP-I equations on $\mathbb {R}^2$

We prove that

(5.1) $$ \begin{align} \left\{ \begin{array}{cl} \partial_t u - \partial_x D_x^\alpha u - \partial_{x}^{-1} \partial_{y}^2 u &= u \partial_x u, \quad (t,x,y) \in \mathbb{R} \times \mathbb{D}, \\ u(0) &= u_0, \end{array} \right. \end{align} $$

is not analytically well-posed in $H^{s_1,s_2}$ for $\alpha <\frac {5}{2}$ .

First, we state a preliminary result:

Lemma 5.1. The spatial Fourier transform of

$$ \begin{align*} v(t) = \int_0^t U_\alpha(t-s) \partial_x (U_\alpha(s) \phi_1 U_\alpha(s) \phi_2)ds \end{align*} $$

is given by

(5.2) $$ \begin{align} \begin{aligned} \hat{v}(t,\xi,\eta) = \xi e^{it\omega_{\alpha}(\xi,\eta)} \int_{*} \frac{1-e^{-it\Omega_{\alpha}(\xi_1,\xi_2,\eta_1,\eta_2)}}{\Omega_{\alpha}(\xi_1,\xi_2,\eta_1,\eta_2)}\hat{\phi}_1(\xi_1,\eta_1)\hat{\phi}_2(\xi_2,\eta_2)d\xi_1 d\eta_1, \end{aligned} \end{align} $$

where $*$ denotes the convolution constraint $(\xi ,\eta ) = (\xi _1,\eta _1) + (\xi _2,\eta _2)$ with $(\xi _i,\eta _i) \in D_i$ .

Proof. With $(\xi ,\eta ) = (\xi _1,\eta _1) + (\xi _2,\eta _2)$ , we have

$$ \begin{align*} \begin{aligned} &\mathcal{F}_{x,y}\Big(U_{\alpha}(t-s)\partial_x\big(U_{\alpha}(s)\phi_1 U_{\alpha}(s)\phi_2\big)\Big) (t,\xi,\eta)\\ &~~=e^{i(t-s)\Omega_{\alpha}(\xi,\eta)}(i\xi)\mathcal{F}_{x,y}\big(U_{\alpha}(s)\phi_1U_{\alpha}(s)\phi_2\big)(t,\xi,\eta)\\ &~~=e^{i(t-s)\Omega_{\alpha}(\xi,\eta)}(i\xi) \int_{*} e^{is\omega_{\alpha}(\xi_1,\eta_1)}\hat{\phi}(\xi_1,\eta_1) e^{is\omega_{\alpha}(\xi_2,\eta_2)} \hat{\phi}_2(\xi_2,\eta_2)d\xi_1d\eta_1\\ &~~=e^{it\Omega_{\alpha}(\xi,\eta)} (i\xi)\int_{*} e^{is(\omega_{\alpha}(\xi_1,\eta_1)+\omega_{\alpha}(\xi_2,\eta_2)-\omega_{\alpha}(\xi,\eta))} \hat{\phi}_1(\xi_1,\eta_1)\hat{\phi}_2(\xi_2,\eta_2)d\xi_1d\eta_1\\ &~~=i\xi e^{it\Omega_{\alpha}(\xi,\eta)} \int_{*} e^{-is\Omega_{\alpha}(\xi_1,\xi_2,\eta_1,\eta_2)}\hat{\phi}_1(\xi_1,\eta_1)\hat{\phi}_2(\xi_2,\eta_2)d\xi_1d\eta_1. \end{aligned} \end{align*} $$

This implies after integrating in time

$$ \begin{align*} \begin{aligned} \hat{v}(t,\xi,\eta) &= i\xi e^{it\Omega_{\alpha}(\xi,\eta)} \int_0^t \int_{*} e^{-is\Omega_{\alpha}(\xi_1,\xi_2,\eta_1,\eta_2)}\hat{\phi}_1(\xi_1,\eta_1)\hat{\phi}_2(\xi_2,\eta_2)d\xi_1d\eta_1 ds\\ &=\xi e^{it\Omega_{\alpha}(\xi,\eta)} \int_{*} \frac{1-e^{-it\Omega_{\alpha}(\xi_1,\xi_2,\eta_1,\eta_2)}}{\Omega_{\alpha}(\xi_1,\xi_2,\eta_1,\eta_2)} \hat{\phi}_1(\xi_1,\eta_1)\hat{\phi}_2(\xi_2,\eta_2)d\xi_1d\eta_1. \end{aligned}\\[-40pt] \end{align*} $$

Theorem 5.2. Let $1 \leqslant \alpha < \frac {5}{2}$ , $(s_1,s_2)\in \mathbb {R}^2$ . Then, there does not exist a $T>0$ such that there is a function space $X_T \hookrightarrow C([-T,T];H^{s_1,s_2}(\mathbb {R}^2;\mathbb {R}))$ in which (1.1) admits a local solution with a $C^2$ -differentiable flow-map $\Gamma _t$ :

$$ \begin{align*} \Gamma_t:H^{s_1,s_2}(\mathbb{R}^2;\mathbb{R}) \to H^{s_1,s_2}(\mathbb{R}^2;\mathbb{R}), \quad u_0 \mapsto u(t), ~~t \in [-T,T]. \end{align*} $$

Proof. We recall that the resonance function is given by

$$ \begin{align*} \Omega_{\alpha}(\xi_1,\xi_2,\eta_1,\eta_2) = \Omega_{\alpha}^1(\xi_1,\xi_2) - \Omega_{\alpha}^2(\xi_1,\xi_2,\eta_1,\eta_2), \end{align*} $$

where

$$ \begin{align*} \begin{aligned} \Omega_{\alpha}^1(\xi_1,\xi_2) &= |\xi_1+\xi_2|^{\alpha}(\xi_1+\xi_2) - |\xi_1|^{\alpha}\xi_1 - |\xi_2|^{\alpha}\xi_2,\\ \Omega_{\alpha}^2(\xi_1,\xi_2,\eta_1,\eta_2) &= \frac{(\eta_1\xi_2-\eta_2\xi_1)^2}{\xi_1\xi_2( \xi_1+\xi_2)}. \end{aligned} \end{align*} $$

We define functions via their Fourier transforms as follows:

(5.3) $$ \begin{align} \begin{aligned} \hat{\phi}_1(\xi_1,\eta_1) &= \frac{1_{D_1}(\xi_1,\eta_1)}{N^{-\frac{\alpha}{2}+\frac{1}{4}}}, \quad D_1 = [N^{-\frac{\alpha-1}{2}}, 2N^{-\frac{\alpha-1}{2}}] \times [-N^{-\frac{\alpha}{2}}, N^{-\frac{\alpha}{2}}],\\ \hat{\phi}_2(\xi_2,\eta_2) &= \frac{1_{D_2}(\xi_2,\eta_2)}{N^{s_1 +(1+\frac{\alpha}{2})s_2}N^{-\frac{\alpha}{2}+\frac{1}{4}}}, \\ D_2 &= [N,N+ N^{-\frac{\alpha-1}{2}}] \times [\sqrt{1+\alpha}N^{\frac{\alpha}{2}+1}, \sqrt{1+\alpha}N^{\frac{\alpha}{2}+1} +N^{-\frac{\alpha}{2}}]. \end{aligned} \end{align} $$

From [Reference Sanwal and Schippa41, Lemma 3.1], we estimate the size of the resonance function by

$$ \begin{align*} |\Omega_{\alpha}| \sim 1. \end{align*} $$

In Lemma 5.1 we computed

$$ \begin{align*} |\hat{v}(t,\xi,\eta)| \sim t \frac{N}{N^{s_1} N^{(1+\frac{\alpha}{2})s_2}} \end{align*} $$

for a significant measure of $(\xi ,\eta ) = (\xi _1,\eta _1) + (\xi _2,\eta _2)$ with $(\xi _i,\eta _i) \in D_i$ . For $0<t\leqslant c \ll 1$ , the Sobolev norm of $v(t)$ is given by

$$ \begin{align*} \|v(t)\|_{H^{s_1,s_2}(\mathbb{R}^2)} \sim tN^{\frac{5}{4}-\frac{\alpha}{2}}. \end{align*} $$

For $\Gamma _t$ to be $C^2$ -differentiable, it needs to hold

$$ \begin{align*} 1 \sim \|\phi_1\|_{H^{s_1,s_2}(\mathbb{R}^2)} \|\phi_2\|_{H^{s_1,s_2}(\mathbb{R}^2)} \gtrsim t N^{\frac{5}{4}-\frac{\alpha}{2}}, \end{align*} $$

which requires $\alpha \geqslant \frac {5}{2}$ for $N\gg 1$ . Clearly, $\phi _i$ are not real-valued, but letting $u^*_0 = \phi _1 + \phi _2$ and symmetrizing the Fourier transform we find real-valued initial data $u_0$ with comparable Sobolev norm. The above estimates remain unchanged, which completes the proof.

5.2 $C^2$ -ill-posedness for KP-I equations on $\mathbb {R} \times \mathbb {T}$

Next, we treat the case of the cylinder $\mathbb {R} \times \mathbb {T}$ .

Theorem 5.3. Let $\alpha <5$ , $(s_1,s_2) \in \mathbb {R}^2$ . Then there does not exist any time $T>0$ such that there is a function space $X_T \hookrightarrow C([-T,T];H^{s_1,s_2}(\mathbb {R} \times \mathbb {T}))$ in which (1.1) has a unique local solution with a $C^2$ -differentiable flow map $\Gamma _t$ :

$$ \begin{align*} \Gamma_t:H^{s_1,s_2}(\mathbb{R} \times \mathbb{T}) \to H^{s_1,s_2}(\mathbb{R} \times \mathbb{T}), \quad u_0 \mapsto u(t), ~~t \in [-T,T]. \end{align*} $$

We remark that the cases $\alpha \leqslant 1$ can be readily seen to be $C^2$ -illposed by comparison with the dispersion-generalized Benjamin-Ono equation:

$$ \begin{align*} \left\{ \begin{array}{cl} \partial_t u + \partial_x D_x^\alpha u &= u \partial_x u, \quad (t,x) \in \mathbb{R} \times \mathbb{R}, \\ u(0) &= u_0 \in H^{s}(\mathbb{R}). \end{array} \right. \end{align*} $$

This evolution is recovered by considering initial data to KP-equations on $\mathbb {R} \times \mathbb {T}$ , which do not depend on the periodic coordinate.

In the following we suppose that $\alpha \geqslant 1$ . As an ansatz to prove Theorem 5.3, we consider the following functions with parameters $\gamma $ and $\beta (N)$ to be determined:

(5.4) $$ \begin{align} \begin{aligned} \hat{\phi}(\xi_1,\eta_1) &= \gamma^{-\frac{1}{2}} 1_{D_1}(\xi_1,\eta_1), ~~D_1 = [\gamma, 2\gamma] \times \{0\},\\ \hat{\phi}_2(\xi_2,\eta_2) &= \gamma^{-\frac{1}{2}} N^{-s_1}(\beta(N))^{-s_2} 1_{D_2}(\xi_2,\eta_2), ~~D_2 = [N-\gamma, N]\times \{\beta(N)\}, \end{aligned} \end{align} $$

where $N \gg 1$ , $\beta (N)\sim N^{\frac {\alpha }{2}+1}$ , and $\gamma = \gamma (N) \ll 1$ will be chosen later. We find an upper bound for the size of the resonance function. With $\xi _1, \xi _2>0$ , we can compute $\Omega _{\alpha }^1$ invoking the mean value theorem:

$$ \begin{align*} \Omega_{\alpha}^1(\xi_1,\xi_2) = (\xi_1+\xi_2)^{\alpha+1} - \xi_2^{\alpha+1}-\xi_1^{\alpha+1}= (\alpha + 1)\xi_1\xi_*^{\alpha} - \xi_1^{\alpha+1}, \end{align*} $$

for $\xi _* \in (\xi _2,\xi _2+\xi _1)$ . For $\eta _1=0$ which is relevant for our setting, we have

$$ \begin{align*} \Omega_{\alpha}^2(\xi_1,\xi_2,\eta_1,\eta_2) = \frac{\eta_2^2\xi_1}{\xi_2(\xi_1+\xi_2)}=:f(\xi_1). \end{align*} $$

Using Taylor’s theorem, we have

(5.5) $$ \begin{align} f(\xi_1) = f(\xi_1^*) + f'(\xi_1^*)(\xi_1-\xi_1^*)+R, \end{align} $$

where R includes all the lower order terms. This gives

$$ \begin{align*} f(\xi_1) = f(\xi_1^*) + \frac{\eta_2^2}{\xi_2(\xi_1^*+\xi_2)}(\xi_1-\xi_1^*) -\frac{\eta_2^2(\xi_1^*)}{\xi_2(\xi_1^*+\xi_2)^2}(\xi_1 - \xi_1^*) + R. \end{align*} $$

From the definition of $D_1$ and $D_2$ in (5.4), we have that the first two terms on the right-hand side above have similar size while the remainder term is smaller in size than the first two terms. Now we choose $\xi _1^*, \xi _1, \xi _2,\xi ^*,\eta _2 \in \mathbb {R}$ such that the leading order terms in $\Omega _1^{\alpha }$ and $\Omega _2^{\alpha }$ cancel, namely

$$ \begin{align*} \begin{aligned} (\alpha+1)\xi_1\xi_*^{\alpha} - \xi_1^{\alpha+1} = f(\xi_1^*) + \frac{\eta_2^2(\xi_1-\xi_1^*)}{\xi_2(\xi_1^* + \xi_2)} = \frac{\eta_2^2\xi_1}{\xi_2(\xi_1^* + \xi_2)}, \end{aligned} \end{align*} $$

which gives

$$ \begin{align*} \eta_2^2 = \big((\alpha+1)\xi_*^{\alpha} - \xi_1^{\alpha}\big) \xi_2(\xi_1^* + \xi_2). \end{align*} $$

With this choice, for the size of the resonance function, we conclude

$$ \begin{align*} |\Omega_{\alpha}| \sim \Big| \frac{\eta_2^2 \xi_1^*(\xi_1-\xi_1^*)}{\xi_2(\xi_1^*+\xi_2)^2}\Big| \sim N^{\alpha-1}\gamma^2. \end{align*} $$

However, with the choice

$$ \begin{align*} \eta_2 =:\beta(N,\gamma) = \Big(\big((\alpha+1)\xi_*^{\alpha} - \xi_1^{\alpha}\big) \xi_2(\xi_1^* + \xi_2) \Big)^{\frac{1}{2}}, \end{align*} $$

we cannot ascertain that $\beta (N,\gamma ) \in \mathbb {N}$ . To this end, we find a rational approximation of $\eta _2$ . Using Dirichlet’s approximation theorem, we have for $\beta (N, \gamma ) \in \mathbb {R}$ , the existence of infinitely many rational numbers $\frac {p}{q}$ such that

(5.6) $$ \begin{align} | \beta(N, \gamma)-\frac{p}{q}| <\frac{1}{q^2}. \end{align} $$

The above implies that

(5.7) $$ \begin{align} |q\beta(N,\gamma) - p| <\frac{1}{q}. \end{align} $$

Since we have a natural number ( $q\beta (N,\gamma )>0$ ) approximation for $q\beta (N,\gamma )$ (and not $\beta (N,\gamma )$ ), we make use of the anisotropic scaling (4.16) for (1.1): for any $\lambda \in \mathbb {R}$

$$ \begin{align*} \tau \to \lambda^{\alpha}\tau, \quad \xi \to \lambda \xi, \quad \eta \to \lambda^{\frac{\alpha}{2}+1}\eta. \end{align*} $$

With this, for $q \in \mathbb {N}$ , we introduce the following scaling

(5.8) $$ \begin{align} \tau \to\tau':= q^{2\frac{\alpha+1}{\alpha+2}} \tau, \quad \xi \to \xi':=q^{\frac{2}{\alpha+2}}\xi, \quad \eta \to \eta':=q\eta. \end{align} $$

It is easy to check that with the scaling (5.8), the resonance function scales as

$$ \begin{align*} \Omega_{\alpha} \to \Omega^{\prime}_{\alpha} = q^{2\frac{\alpha+1}{\alpha+2}} \Omega_{\alpha}. \end{align*} $$

Now we work with the scaled variables ( $\xi ^{\prime }_i, \eta ^{\prime }_i)$ , $i=1,2$ and ensure that the natural number approximation (5.7) of $q\beta (N,\gamma )$ does not affect the size of the resonance function. Consider the difference

$$ \begin{align*} \begin{aligned} |\Omega^{\prime}_{\alpha}(\xi^{\prime}_1, \xi^{\prime}_2, 0, q\beta(N,\gamma)) - \Omega^{\prime}_{\alpha}(\xi^{\prime}_1,\xi_2',0,p)|&= q^{2\frac{\alpha+1}{\alpha+2}} | \Omega_{\alpha}(\xi_1,\xi_2,0,\beta) - \Omega_{\alpha}(\xi_1,\xi_2,0,\frac{p}{q})|\\ &=q^{2\frac{\alpha+1}{\alpha+2}}\frac{\xi_1}{\xi_2(\xi_1+\xi_2)}\Big|\beta^2 - \frac{p^2}{q^2}\Big|\\ &\lesssim q^{2\frac{\alpha+1}{\alpha+2}}\frac{\gamma}{N^2} \Big| \beta-\frac{p}{q}\Big| \Big|\beta +\frac{p}{q}\Big|\\ &\lesssim q^{2\frac{\alpha+1}{\alpha+2}} \frac{\gamma}{N^2} \frac{N^{\frac{\alpha}{2}+1}}{q^2}. \end{aligned} \end{align*} $$

We require the size of the above expression to be negligible compared to

$|\Omega ^{\prime }_{\alpha }(\xi ^{\prime }_1,\xi _2',0, q\beta (N,\gamma ))|$ , that is,

$$ \begin{align*} q^{2\frac{\alpha+1}{\alpha+2}} \frac{\gamma}{N^2} \frac{N^{\frac{\alpha}{2}+1}}{q^2} \ll q^{2\frac{\alpha+1}{\alpha+2}} N^{\alpha-1}\gamma^2 \end{align*} $$

which requires

(5.9) $$ \begin{align} q \gg N^{-\frac{\alpha}{4}} \gamma^{-\frac{1}{2}}. \end{align} $$

Furthermore, we choose $\gamma = \gamma (N)$ such that the size of the new resonance function $\Omega ^{\prime }_{\alpha }$ is small, namely

$$ \begin{align*} q^{2\frac{\alpha+1}{\alpha+2}} N^{\alpha-1}\gamma^2 \sim 1, \end{align*} $$

which gives

(5.10) $$ \begin{align} \gamma \sim N^{\frac{1}{2}-\frac{\alpha}{2}} q^{-\frac{\alpha+1}{\alpha+2}}. \end{align} $$

We remark that this is consistent with (5.9) since taking the two conditions together

$$ \begin{align*} q^{\frac{\alpha+3}{2(\alpha+2)}} \gg N^{-\frac{1}{4}}. \end{align*} $$

This is automatically satisfied for $\alpha \geqslant 1$ , $N \in 2^{\mathbb {N}_0}$ , and $q \in \mathbb {N}$ .

With the choice of q and $\gamma $ made above, we are set to prove Theorem 5.3.

Proof of Theorem 5.3

We define the input functions $\phi _1$ and $\phi _2$ via their spatial Fourier transforms as follows:

$$ \begin{align*} \begin{aligned} \hat{\phi}_1(\xi_1,\eta_1) &= q^{-\frac{1}{\alpha+2}} \gamma^{-\frac{1}{2}} 1_{D_1}(\xi_1,\eta_1), \text{ where } D_1 = [q^{\frac{2}{\alpha+2}}\gamma, 2q^{\frac{2}{\alpha+2}}\gamma] \times \{0\},\\ \hat{\phi}_2(\xi_2,\eta_2) &= q^{-\frac{1}{\alpha+2}} \gamma^{-\frac{1}{2}} (q^{\frac{2}{\alpha+2}}N)^{-s_1} p^{-s_2}1_{D_2}(\xi_2,\eta_2), \\ &\quad \text{ where } D_2 = [q^{\frac{2}{\alpha+2}} (N-\gamma), q^{\frac{2}{\alpha+2}}N] \times \{p\}. \end{aligned} \end{align*} $$

In the above definition we choose q such that $[q^{\frac {2}{\alpha +2}}\gamma , 2q^{\frac {2}{\alpha +2}}\gamma ] \subseteq [0,1]$ , that is, $ q^{\frac {2}{\alpha +2}} \gamma \lesssim 1$ which follows from (5.10) and $\alpha \geqslant 1$ .

It is straight-forward to check that $\|\phi _i\|_{H^{s_1,s_2}} \sim 1$ for $i=1,2$ . We consider the contribution to the second Picard iterate given by the Duhamel integral:

$$ \begin{align*} v(t) = \int_0^t S_{\alpha}(t-s)\partial_x\big(S_{\alpha}(s)\phi_1 S_{\alpha}(s)\phi_2\big)ds. \end{align*} $$

To show that the flow map $\Gamma _t$ is not $C^2$ differentiable at the origin, we show that

$$ \begin{align*} \|v(t)\|_{H^{s_1,s_2}} \to \infty \text{ as } N \to \infty. \end{align*} $$

From Lemma 5.1, we have

$$ \begin{align*} \hat{v}(t,\xi,\eta) = \xi e^{it\omega_{\alpha}(\xi,\eta)} \int_{*} \frac{1-e^{-it\Omega_{\alpha}(\xi_1,\xi_2,\eta_1,\eta_2)}}{\Omega_{\alpha}(\xi_1,\xi_2,\eta_1,\eta_2)} \hat{\phi}_1(\xi_1,\eta_1)\hat{\phi}_2(\xi_2,\eta_2) d\xi_1d\eta_1, \end{align*} $$

where $*$ denotes the convolution constraint and we have the counting measure in the $\eta $ variable. To compute the $H^{s_1,s_2}$ norm of v, we estimate the size of $\hat {v}$ for $0<t\leqslant c \ll 1$ :

$$ \begin{align*} |\hat{v}(t,\xi,\eta)| \sim t \frac{q^{\frac{2}{\alpha+2}}N}{(q^{\frac{2}{\alpha+2}}N)^{s_1}p^{s_2}}. \end{align*} $$

Thus,

$$ \begin{align*} \|v(t)\|_{H^{s_1,s_2}}^2 \sim \int \langle \xi\rangle^{2s_1}\langle \eta \rangle^{2s_2}|\hat{v}(t,\xi,\eta)|^2d\xi d\eta \sim t^2 q^{\frac{4}{\alpha+2}} N^2 q^{\frac{2}{\alpha+2}}\gamma. \end{align*} $$

For the flow map $\Gamma _t$ to be $C^2$ , we require

$$ \begin{align*} 1\sim \|\phi_1\|_{H^{s_1,s_2}} \|\phi_2\|_{H^{s_1,s_2}} \gtrsim \|v(t)\|_{H^{s_1,s_2}} \sim t q^{\frac{3}{\alpha+2}}N\gamma^{\frac{1}{2}} \sim t N^{-\frac{1}{4} \frac{5-\alpha}{\alpha+3}} N^{\frac{5-\alpha}{4}}, \end{align*} $$

where we used (5.9) and (5.10) to obtain the last term in the above display. Hence, we conclude that $\Gamma _t$ can be $C^2$ -differentiable only for $\alpha \geqslant 5$ .

5.3 Subcritical ill-posedness for semilinear KP-I equations on $\mathbb {R} \times \mathbb {T}$

We supplement the analytic well-posedness result proved in Theorem 6.3:

Theorem 5.4. Let $\alpha \geqslant 5$ , and $s<\frac {1-\alpha }{4}$ . Then, for initial data in $H^{s,0}(\mathbb {R} \times \mathbb {T},\mathbb {R})$ , (1.1) is ill-posed on $\mathbb {R}\times \mathbb {T}$ , that is, the data-to-solution map

$$ \begin{align*} u_0 \mapsto u(t) \end{align*} $$

fails to be continuous.

Proof. The proof relies on [Reference Bejenaru and Tao3, Proposition 1]. The starting point is an analytic data-to-solution mapping assigning more regular initial data from a ball in $H^{\bar {s},0}$ , $\bar {s} \in (\frac {1-\alpha }{4},0)$ to solutions of higher regularity:

$$ \begin{align*} (B_{R,\bar{s}}, \| \cdot \|_{H^{\bar{s},0}}) \to (B_{R}, X_{\bar{s}}), \quad u_0 \mapsto u. \end{align*} $$

This is provided by Theorem 6.3.

[Reference Bejenaru and Tao3, Proposition 1] now states that a possible well-posedness for $s'<\frac {1-\alpha }{4}$ implies continuity of

$$ \begin{align*} \begin{aligned} (B_{R,\bar{s}}, \| \cdot \|_{H^{s',0}}) \to C_T H^{s',0}, \quad u_0 &\mapsto \int_0^t S_\alpha(t-s) (\partial_x(S_\alpha(s) u_0 S_\alpha(s) u_0)) ds. \end{aligned} \end{align*} $$

The above display is the second Picard iterate, and we furnish initial data for which the estimate

(5.11) $$ \begin{align} \Big \| \int_0^t S_\alpha(t-s) (\partial_x(S_\alpha(s) u_0 S_\alpha(s) u_0)) ds \Big\|_{H^{s,0}(\mathbb{R} \times \mathbb{T})} \lesssim \|u_0\|_{H^{s,0}(\mathbb{R} \times \mathbb{T})}^2 \end{align} $$

holds only for $s\geqslant \frac {1-\alpha }{4}$ . We rely on a High $\times $ High $\to $ Low resonant interaction, which is crucial to apply [Reference Bejenaru and Tao3, Proposition 1] because the sequence of initial data must be contained in $(B_{R,\bar {s}}, \| \cdot \|_{H^{\bar {s},0}})$ . Define

$$ \begin{align*} \hat{u}_0(\xi,\eta) = 1_{[A,A+A^{1-\alpha}]}(\xi) \cdot \delta_0(\eta) + 1_{[1-A,1-A+A^{1-\alpha}]}(\xi) \cdot \delta_m(\eta), \end{align*} $$

where $m \in \mathbb {N}$ and $1\ll A \in \mathbb {R}_{>0}$ is such that for some output frequencies $\xi $ , we have $\xi \sim 1$ . It is straightforward to check that

$$ \begin{align*} \|u_0\|_{H^{s,0}} \sim A^s A^{\frac{1-\alpha}{2}}. \end{align*} $$

Again we remark that $u_0$ is not real-valued, which can be accomplished by symmetrization of the Fourier transform like in previous sections.

Furthermore, choosing $m \sim A^{\frac {\alpha }{2}}$ and A suitably, we have

$$ \begin{align*} |\Omega_\alpha(\xi_1,\xi-\xi_1,\eta_1,\eta-\eta_1)| \sim 1. \end{align*} $$

Indeed, it suffices to check this for one specific $\xi _1 \in A$ and $\xi \sim 1$ . The estimate follows then from simple derivative estimates.

By Lemma 5.1 and that $|\xi |\sim 1$ we have

$$ \begin{align*} \Big \| \int_0^t S_\alpha(t-s) (\partial_x(S_\alpha(s) u_0 S_\alpha(s) u_0)) ds \Big\|_{H^{s,0}} \sim N^{\frac{3-3\alpha}{2}}. \end{align*} $$

For (5.11) to hold, we require

$$ \begin{align*} N^{\frac{3-3\alpha}{2}} \lesssim N^{2s} N^{1-\alpha}, \end{align*} $$

which is true only for $s\geqslant \frac {1-\alpha }{4}$ . This completes the proof.

5.4 Ill-posedness on tori

Finally, we prove the following result on $\mathbb {T} \times \mathbb {T}_\gamma $ .

Theorem 5.5. Let $\alpha \in \mathbb {R}_{>0}$ , $(s_1,s_2) \in \mathbb {R}^2$ . Then, there is $\gamma = \gamma (\alpha ) \in (1/2,1]$ such that there does not exist any time $T>0$ , for which there is a function space $X_T \hookrightarrow C([-T,T];H^{s_1,s_2}(\mathbb {T} \times \mathbb {T}_\gamma ))$ in which (1.1) has a unique local solution with a $C^2$ -differentiable flow map $\Gamma _t$ :

$$ \begin{align*} \Gamma_t:H^{s_1,s_2}(\mathbb{T} \times \mathbb{T}_\gamma) \to H^{s_1,s_2}(\mathbb{T} \times \mathbb{T}_\gamma), \quad u_0 \mapsto u(t), ~~t \in [-T,T]. \end{align*} $$

Proof. Considering initial data, which do not depend on the second variable, the evolution becomes

$$ \begin{align*} \partial_t u + \partial_x D_x^\alpha u = u \partial_x u. \end{align*} $$

For this equation it is easy to see, choosing initial data

$$ \begin{align*} \hat{u}_0(\xi) = \delta_1(\xi) + \delta_N(\xi) \end{align*} $$

for $N \gg 1$ , the data-to-solution mapping fails to be $C^2$ for $\alpha < 1$ .

In the following we suppose that $\alpha \geqslant 1$ and consider the following functions:

(5.12) $$ \begin{align} \begin{aligned} \hat{\phi}_1(\xi_1,\eta_1) &= 1_{D_1}(\xi_1,\eta_1), \quad D_1 = \{ 1 \} \times \{ 0 \},\\ \hat{\phi}_2(\xi_2,\eta_2) &= N^{-s_1} p^{-s_2} 1_{D_2}(\xi_2,\eta_2), \quad D_2 = \{ N \} \times \{ p \}. \end{aligned} \end{align} $$

We choose p such that

$$ \begin{align*} \Omega_\alpha(1,0,N,p) = (N+1)^{\alpha+1} - 1 - N^{\alpha+1} - \frac{p^2}{(N+1)N} = 0. \end{align*} $$

Note that this requires a choice of $\gamma \in (\frac {1}{2},1]$ such that $p \in \gamma ^{-1} \mathbb {Z}$ , that is, fixing the ratio of the periods.

Clearly, for the Fourier transform of the Duhamel integral

$$ \begin{align*} |\hat{v}(t,\xi,\eta)| \sim \frac{N t}{N^{s_1} p^{s_2}}, \quad \xi = N+1, \; \eta = p. \end{align*} $$

Hence,

$$ \begin{align*} \| v(t) \|_{H^{s_1,s_2}} \gtrsim N t. \end{align*} $$

This implies that for $\alpha \geqslant 1$ , the data-to-solution mapping of (1.1) fails to be $C^2$ for some $\gamma = \gamma (\alpha )$ .

6 Semilinear well-posedness

In this section, we show the sharp semilinear local well-posedness for KP-I equations posed on the Euclidean plane and on the cylinder. The results are proved by invoking the contraction mapping principle in Fourier restriction spaces.

6.1 $\mathbb {R}^2$ case

We state the following theorem which is an improvement of [Reference Sanwal and Schippa41, Theorem 6.1] and proves well-posedness in the full subcritical range.

Let $s,b \in \mathbb {R}$ , recall $\omega _\alpha (\xi ,\eta ) = \xi |\xi |^\alpha + \frac {\eta ^2}{\xi }$ , and we define the space $X^{s,b}$ as closure of Schwartz functions with respect to the norm:

$$ \begin{align*} \| u \|_{X^{s,b}} = \| \langle \xi \rangle^s \langle \tau - \omega_\alpha(\xi,\eta) \rangle^b \mathcal{F}_{t,x,y}(u) \|_{L^2_{\tau,\xi,\eta}}. \end{align*} $$

We define for measurable $u:[0,T] \times \mathbb {R}^2 \to \mathbb {C}$ :

$$ \begin{align*} \| u \|_{X^{s,b}_T} = \inf_{\substack{\tilde{u} \in X^{s,b}, \\ u = \tilde{u} \vert_{[0,T]} } } \| \tilde{u} \|_{X^{s,b}}. \end{align*} $$

Theorem 6.1. Let $\alpha \geqslant \frac {5}{2}$ and $s>1-\frac {3\alpha }{4}$ . Then, there is some $b>\frac {1}{2}$ such that for $T=T(\|u_0\|_{H^{s,0}})$ , (5.1) is analytically locally well-posed in $H^{s,0}$ with the solution lying in $X^{s,b}_T \hookrightarrow C([0,T];H^{s,0})$ .

We shall be brief here and refer the reader to [Reference Sanwal and Schippa41, Section 6] for the properties of the auxiliary spaces $X^{s,b}_T$ . The proof of the theorem is concluded in Subsection 6.3. The following estimate is crucial:

Proposition 6.2. Let $\alpha \geqslant \frac {5}{2}$ and $s>1-\frac {3\alpha }{4}$ . Then there is some $b>\frac {1}{2}$ such that the following estimate is true:

(6.1) $$ \begin{align} \| \partial_x(uv)\|_{X^{s,b-1}} \lesssim \|u\|_{X^{s,b}} \|v\|_{X^{s,b}}. \end{align} $$

Proof. By duality and Plancherel’s theorem, we can reduce the above to proving

(6.2) $$ \begin{align} \int_{\mathbb{R}^3} \xi~ \widehat{uv}\cdot \overline{\widehat{w}} d\tau d\xi d\eta \lesssim \|u\|_{X^{s,b}} \|v\|_{X^{s,b}} \|w\|_{X^{-s,1-b}}. \end{align} $$

After a dyadic decomposition, for $N_i \in 2^{\mathbb {Z}}, L_i\in 2^{\mathbb {N}_0}$ , we prove the following estimate

(6.3) $$ \begin{align} \Big| \int_{\mathbb{R}^3}(f_{N_1,L_1}\ast g_{N_2,L_2})h_{N,L}d\tau d\xi d\eta\Big| \lesssim C(N_1,N_2,N) L_1^{\frac{1}{2}} L_2^{\frac{1}{2}} L^{\frac{1}{2}-} \mathcal{A} \end{align} $$

with $\mathcal {A} = \|f_{N_1,L_1}\|_{L^2} \|g_{N_2,L_2}\|_{L^2} \|h_{N,L} \|_{L^2}$ for a suitable constant $C(N_1,N_2,N)$ which also incorporates the derivative loss from the nonlinearity. To avoid writing the integral on the left-hand side in the above display repetitively, we denote:

$$ \begin{align*} I:= \Big| \int_{\mathbb{R}^3}(f_{N_1,L_1}\ast g_{N_2,L_2})h_{N,L}d\tau d\xi d\eta\Big|. \end{align*} $$

In the following we do a case-by-case analysis depending on the size of the x-frequencies. In cases (i) and (ii) we suppose that $N_{\max } \gtrsim 1$ .

(i) High $\boldsymbol {\times }$ Low $\boldsymbol {\rightarrow }$ High ( $N_2 \lesssim N_1\sim N$ ): We consider two more cases:

  • $\underline {L_{\max }\ll N_1^{\alpha }N_2}$ : In case $N_1^{-\frac {\alpha }{2}+\frac {1}{2}} L_3^{\varepsilon } \lesssim N_2 \lesssim 1$ , using the nonlinear Loomis–Whitney estimate (4.17), we obtain

    $$ \begin{align*} \begin{aligned} \sum_{N_1^{-\frac{\alpha}{2}+\frac{1}{2}} L_3^{\varepsilon} \lesssim N_2 \lesssim 1} I &\lesssim \sum_{N_1^{-\frac{\alpha}{2}+\frac{1}{2}} L_3^{\varepsilon} \lesssim N_2 \lesssim 1} N_1^{-\frac{3\alpha}{4} +\frac{1}{2}} N_2^{-\frac{1}{2}} (L_1 L_2 L )^{\frac{1}{2}} \mathcal{A} \\ & \lesssim N_1^{-\frac{\alpha}{2}+\frac{1}{4}} (L_1L_2)^{\frac{1}{2}} L_3^{\frac{1}{2}-\frac{\varepsilon}{2}} \|f_{N_1,L_1}\|_{L^2} \|g_{\lesssim 1,L_2}\|_{L^2} \|h_{N,L}\|_{L^2}. \end{aligned} \end{align*} $$

    In the other case where $N_2 \lesssim N_1^{-\frac {\alpha }{2} +\frac {1}{2}} L^{\varepsilon }$ , using the bilinear Strichartz estimate (4.7), we have

    $$ \begin{align*} \begin{aligned} \sum_{ N_2 \lesssim N_1^{-\frac{\alpha}{2}+\frac{1}{2}} L^{\varepsilon}} I &\lesssim \sum_{ N_2 \lesssim N_1^{-\frac{\alpha}{2}+\frac{1}{2}} L_3^{\varepsilon}} N_1^{-\frac{\alpha}{4}} N_2^{\frac{1}{2}} (L_1L_2)^{\frac{1}{2}} \mathcal{A}\\ &\lesssim N_1^{-\frac{\alpha}{2}+\frac{1}{4}} (L_1L_2)^{\frac{1}{2}} L^{\frac{\varepsilon}{2}} \mathcal{A}. \end{aligned} \end{align*} $$
    In both cases, after considering the derivative loss and summing up, the estimate leads to (6.3). In the case $N_2 \gtrsim 1$ , we use the nonlinear Loomis–Whitney estimate (4.17) to obtain
    $$ \begin{align*} \begin{aligned} \sum_{1\lesssim N_2\lesssim N_1} I &\lesssim \sum_{1 \lesssim N_2\lesssim N_1} N_1^{-\frac{1}{2}-\frac{3\alpha}{4}}N_2^{-\frac{1}{2}} (L_1L_2L)^{\frac{1}{2}} \mathcal{A}\\ &\lesssim N_1^{1-\frac{3\alpha}{4}-s+(\alpha+1)\varepsilon} \sum_{1\lesssim N_2 \lesssim N_1} \Big(\frac{N_2}{N_1}\Big)^{-\frac{1}{2}-s+\varepsilon} (L_1L_2)^{\frac{1}{2}}L^{\frac{1}{2}-\varepsilon} N_2^s N^{-1} \mathcal{A}. \end{aligned} \end{align*} $$
  • $\underline {L_{\max }\gtrsim N_1^{\alpha }N_2}$ : Using [Reference Sanwal and Schippa41, Lemma 4.6], we have

    $$ \begin{align*} \begin{aligned} I &\lesssim \frac{(L_1L_2L)^{\frac{1}{2}}}{L_{\max}^{\frac{1}{4}}} N_1^{-\frac{\alpha}{2}} N_2^{\frac{1}{4}} \mathcal{A} \\ &\lesssim (L_1L_2)^{\frac{1}{2}} L_{\max}^{\frac{1}{2}-\varepsilon} N_1^{-\frac{3\alpha}{4}+\alpha \varepsilon} N_2^{\varepsilon} \mathcal{A} \\ &\lesssim N_1^{-1} (L_1L_2)^{\frac{1}{2}} L_{\max}^{\frac{1}{2}-\varepsilon} N_1^{1-\frac{3\alpha}{4}+\alpha\varepsilon} N_2^{-1+\frac{3\alpha}{4} -\alpha\varepsilon} N_2^{1-\frac{3\alpha}{4}+\alpha\varepsilon+\varepsilon} \mathcal{A} \\ &\lesssim N_1^{-1} (L_1L_2)^{\frac{1}{2}} L_{\max}^{\frac{1}{2}-\varepsilon} \Big(\frac{N_1}{N_2}\Big)^{1-\frac{3\alpha}{4}+\alpha \varepsilon} N_2^{1-\frac{3\alpha}{4} +(\alpha+1)\varepsilon} \mathcal{A}, \end{aligned} \end{align*} $$
    which is summable since $\alpha \geqslant \frac {5}{2}$ .

(ii) High $\boldsymbol {\times }$ High $\boldsymbol {\rightarrow }$ Low ( $N \lesssim N_1 \sim N_2$ ): The two cases are

  • $\underline {L_{\max }\ll N_1^{\alpha }N_2}$ : In case $N\gtrsim 1$ , using the nonlinear Loomis–Whitney estimate (4.17), we obtain

    $$ \begin{align*} \begin{aligned} \sum_{N\ll N_1\sim N_2} I &\lesssim \sum_{N \ll N_1\sim N_2} N^{-\frac{1}{2}+\varepsilon} N_1^{\frac{1}{2}-\frac{3\alpha}{4}+\alpha\varepsilon} N N_1^{-2s} N^s (L_1L_2)^{\frac{1}{2}} L^{\frac{1}{2}-\varepsilon}\\ &\qquad N^{-1}N_1^s N_2^s N^{-s} \mathcal{A} \\ &=\sum_{N\ll N_1\sim N_2} N^{\frac{1}{2}+s+\epsilon} N_1^{\frac{1}{2}-\frac{3\alpha}{4}-2s+\alpha\varepsilon} N^{-1}N_1^s N_2^s N^{-s} \mathcal{A} \\ &\lesssim \sum_{N_1\sim N_2 \gtrsim 1} N_1^{1-\frac{3\alpha}{4}-s+\alpha\varepsilon +\varepsilon} N^{-1}N_1^s N_2^s N^{-s} \mathcal{A}. \end{aligned} \end{align*} $$
    The above can be summed up for $s>1-\frac {3\alpha }{4}$ .
  • $\underline {L_{\max }\gtrsim N_1^{\alpha }N_2}$ : This case can be handled in the same way as the analogous subcase in High $\times $ Low $\rightarrow $ High interaction.

(iii) Very low frequencies ( $N , N_1 , N_2 \lesssim 1$ ): Using the bilinear Strichartz estimate from Lemma 4.3, we have

$$ \begin{align*} \begin{aligned} \sum_{N, N_1, N_2 \lesssim 1} N \cdot I &\lesssim \sum_{N\sim N_1\sim N_2 \lesssim 1} \|f_{N_1,L_1} * g_{N_2,L_2} \|_{L^2} N \|h_{N,L}\|_{L^2}\\ &\lesssim \sum_{N, N_1, N_2 \lesssim 1} (L_1 L_2)^{\frac{1}{2}} (N_1 \wedge N_2)^{\frac{1}{2}} (N_1 \vee N_2)^{\frac{1}{4}} L^{\frac{1}{2}-}\\ &\qquad \times \|f_{N_1,L_1}\|_{L^2} \|g_{N_2,L_2}\|_{L^2} N \|h_{N,L}\|_{L^2} \end{aligned} \end{align*} $$

with straight-forward summation.

6.2 $\mathbb {R} \times \mathbb {T}$ case

We prove the following result:

Theorem 6.3. Let $\alpha \geqslant 5$ and $s>\frac {1}{4}-\frac {\alpha }{4}$ . Then, there is some $b>\frac {1}{2}$ such that for $T=T(\|u_0\|_{H^{s,0}})$ , (1.1) is analytically locally well-posed in $H^{s,0}$ with the solution lying in $X^{s,b}_T \hookrightarrow C([0,T];H^{s,0})$ .

As in the $\mathbb {R}^2$ case, the claim is implied by the bilinear estimate:

Proposition 6.4. Let $\alpha \geqslant 5$ and $s>\frac {1}{4}-\frac {\alpha }{4}$ . Then there is some $b>\frac {1}{2}$ such that the following estimate is true:

(6.4) $$ \begin{align} \| \partial_x(uv)\|_{X^{s,b-1}} \lesssim \|u\|_{X^{s,b}} \|v\|_{X^{s,b}}. \end{align} $$

We prove Proposition 6.4 in a series of lemmata. After dyadic decomposition in the x-frequencies, we aim to prove an estimate similar to (6.3) with a suitable, but different summability constant, say $\tilde {C}(N,N_1,N_2)$ . We first observe that for $L_{med} \gtrsim N_{\max }^{\frac {\alpha }{2}}$ , the nonlinear Loomis–Whitney estimate and the bilinear Strichartz estimates are the same as in the $\mathbb {R}^2$ case. The boundary cases $N_{\max } \lesssim 1$ and $N_{\min } \lesssim N_{\max }^{-\frac {\alpha }{2}}$ are treated in Lemma 6.8.

Hence, it remains to consider the following cases:

  • $L_{\max } \lesssim N_{\max }^{\frac {\alpha }{2}}$ ,

  • $L_{med} \lesssim N_{\max }^{\frac {\alpha }{2}} \lesssim L_{\max } \lesssim N_{\max }^\alpha N_{\min }$ ,

  • $L_{\max } \gtrsim N_{\max }^{\alpha }N_{\min }$ .

The first two cases are sub-cases of the resonant case, while the last case is the nonresonant case. In the following, we assume that

(6.5) $$ \begin{align} N_{\max} \gtrsim 1, \text{ and } N_{\min} \gtrsim N_{\max}^{-\frac{\alpha}{2}}. \end{align} $$

We handle the first case in the following:

Lemma 6.5. Let $\alpha \geqslant 5$ , $s>\frac {1-\alpha }{4}$ and $N, N_i \in 2^{\mathbb {Z}}$ , $L_i \in 2^{\mathbb {N}_0}$ , and suppose that (6.5). Let $f_{N_1,L_1}, g_{N_2,L_2}, h_{N,L}:\mathbb {R} \times \mathbb {R} \times \mathbb {Z}\to \mathbb {R}_{+}$ and $supp(f_{N_1,L_1}) \subseteq D_{N_1,L_1}$ , $supp(g_{N_2,L_2}) \subseteq D_{N_2,L_2}$ , and $supp(h_{N,L}) \subseteq D_{N,L}$ with $L_{\max } \lesssim \max (N, N_1,N_2)^{\frac {\alpha }{2}}$ . Then, the estimate (6.4) holds.

Proof. Let $\mathcal {A} = \|f_{N_1,L_1}\|_{L^2} \|g_{N_2,L_2}\|_{L^2} \|h_{N,L} \|_{L^2}$ . To prove the result, we consider the following cases:

(i) Low $\boldsymbol {\times }$ High $\boldsymbol {\rightarrow }$ High ( $N_2 \lesssim N_1\sim N$ ): If the size of the low frequency, viz. $N_2\lesssim 1$ , we consider two cases: In case $N_1^{-\frac {\alpha }{2}+\frac {1}{2}} L_{\max }^{\frac {1}{2}} \lesssim N_2 \lesssim 1$ , we use the Loomis–Whitney estimate (4.18), (note: $L_{\max } \ll N_1^\alpha N_2$ ) to obtain

$$ \begin{align*} \begin{aligned} \sum_{N_1^{-\frac{\alpha}{2}+\frac{1}{2}}L_{\max}^{\frac{1}{2}} \lesssim N_2 \lesssim 1} I &\lesssim \sum_{N_1^{-\frac{\alpha}{2}+\frac{1}{2}} L_{\max}^{\frac{1}{2}} \lesssim N_2 \lesssim 1} N_1^{\frac{1}{2}-\frac{\alpha}{2}} N_2^{-\frac{1}{2}} (L_{\max}L_{\min})^{\frac{1}{2}} \mathcal{A} \\ &\lesssim N_1^{\frac{5}{4}-\frac{\alpha}{4}}N_1^{-1} L_{\max}^{\frac{1}{4}} L_{\min}^{\frac{1}{2}} \mathcal{A}. \end{aligned} \end{align*} $$

Summing up the above in the spatial frequencies gives the required estimate. In case $N_2 \lesssim N_1^{-\frac {\alpha }{2}+\frac {1}{2}}L_{\max }^{\frac {1}{2}}$ , we use the bilinear Strichartz estimate (4.7) to obtain

$$ \begin{align*} \begin{aligned} \sum_{N_2 \lesssim N_1^{-\frac{\alpha}{2}+\frac{1}{2}}L_{\max}^{\frac{1}{2}}} I &\lesssim \sum_{N_2 \lesssim N_1^{-\frac{\alpha}{2}+\frac{1}{2}}L_{\max}^{\frac{1}{2}}} N_2^{\frac{1}{2}} L_{\min}^{\frac{1}{2}} \mathcal{A} \\ &\lesssim N_1^{\frac{5}{4}-\frac{\alpha}{4}} N_1^{-1} L_{\min}^{\frac{1}{2}} L_{\max}^{\frac{1}{4}} \mathcal{A}. \end{aligned} \end{align*} $$

In the case $N_2\gtrsim 1$ , the nonlinear Loomis–Whitney estimate (4.18) gives

$$ \begin{align*} \begin{aligned} \sum_{1 \lesssim N_2\lesssim N_1} I &\lesssim \sum_{1 \lesssim N_2 \lesssim N_1} N_2^{-\frac{1}{2}} N_1^{-\frac{\alpha}{2}+\frac{1}{2}} (L_{\min}L_{\max})^{\frac{1}{2}} \mathcal{A} \\ &\lesssim \sum_{1\lesssim N_2 \lesssim N_1} N_2^{-\frac{1}{2}-s} N_1^{\frac{3}{2}-\frac{\alpha}{2}+\varepsilon'} L_{\min}^{\frac{1}{2}} L_{\max}^{\frac{1}{2}-\varepsilon} N_2^s \mathcal{A}. \end{aligned} \end{align*} $$

We observe that in case $s>-\frac {1}{2}$ , it is straightforward to sum the above expression in $N_1$ and $N_2$ . In case $-\frac {1}{2}-s \geq 0$ , we obtain for the above expression that it is bounded by

$$ \begin{align*} \sum_{1 \lesssim N_2 \lesssim N_1} \Big(\frac{N_2}{N_1}\Big)^{-\frac{1}{2}-s} N_1^{1-\frac{\alpha}{2}-s+\varepsilon} N^{-1} L_{\min}^{\frac{1}{2}} L_{\max}^{\frac{1}{2}-\varepsilon'} \|f_{N_1,L_1}\|_{L^2} \|h_{N,L}\|_{L^2} N_2^s\|g_{N_2,L_2}\|_{L^2}. \end{align*} $$

It is easy to observe that the above is summable for $s>1-\frac {\alpha }{2}$ .

(ii) High $\boldsymbol {\times }$ High $\boldsymbol {\rightarrow }$ Low ( $N_1 \sim N_2 \gtrsim N$ ): We first consider the case $N\lesssim 1$ where the derivative in the nonlinearity is smoothing. Using the nonlinear Loomis–Whitney estimate (4.18), we have

$$ \begin{align*} \begin{aligned} \sum_{N\lesssim 1\lesssim N_1\sim N_2} I &\lesssim \sum_{N\lesssim 1\lesssim N_1\sim N_2}N^{-\frac{1}{2}} N_1^{\frac{1}{2}-\frac{\alpha}{2}} (L_{\min}L_{\max})^{\frac{1}{2}} \mathcal{A} \\ &\lesssim \sum_{N\lesssim 1\lesssim N_1\sim N_2} N^{\frac{1}{2}} N_1^{\frac{1}{2}-\frac{\alpha}{2}-2s+\varepsilon} L_{\min}^{\frac{1}{2}} L_{\max}^{\frac{1}{2}-\varepsilon'} N^{-1}N_1^s \|f_{N_1,L_1}\|_{L^2} \\ &\quad \quad \times N_2^s\|g_{N_2,L_2}\|_{L^2} \|h_{N,L}\|_{L^2}. \end{aligned} \end{align*} $$

We observe that the above is summable for $s>\frac {1}{4}-\frac {\alpha }{2}$ .

For $N \gtrsim 1$ , the same estimate yields

$$ \begin{align*} \begin{aligned} \sum_{1 \lesssim N \lesssim N_1\sim N_2}I &\lesssim \sum_{1 \lesssim N \lesssim N_1\sim N_2} N^{\frac{1}{2}+s} N_1^{\frac{1}{2}-\frac{\alpha}{2}-2s+\varepsilon'}L_{\min}^{\frac{1}{2}} L_{\max}^{\frac{1}{2}-\varepsilon'}N^{-1} N_1^s\|f_{N_1,L_1}\|_{L^2} \\ &\quad \qquad \qquad \times N_2^s\|g_{N_2,L_2}\|_{L^2} N^{-s}\|h_{N,L}\|_{L^2}. \end{aligned} \end{align*} $$

The above is summable for $s>\frac {1}{4}-\frac {\alpha }{4}$ . We observe that this is the case which determines the regularity threshold for local well-posedness.

Next, we have the following result to deal with the intermediate case $L_{med} \lesssim N_{\max }^{\frac {\alpha }{2}} \lesssim L_{\max } \lesssim N_{\max }^{\alpha } N_{\min }$ :

Lemma 6.6. Let $\alpha \geqslant 5$ , $s>\frac {1-\alpha }{4}$ , and $N, N_i \in 2^{\mathbb {Z}}$ , $L_i,L \in 2^{\mathbb {N}}$ , and suppose that (6.5). Let $f_{N_1,L_1}, g_{N_2,L_2}, h_{N,L}:\mathbb {R} \times \mathbb {R} \times \mathbb {Z}\to \mathbb {R}_{+}$ and $supp(f_{N_1,L_1}) \subseteq D_{N_1,L_1}$ , $\text {supp}(g_{N_2,L_2}) \subseteq D_{N_2,L_2}$ , $\text {supp}(h_{N,L}) \subseteq D_{N,L}$ such that $L_{med} \lesssim N_{\max }^{\frac {\alpha }{2}} \lesssim L_{\max } \lesssim N_{\max }^{\alpha } N_{\min }$ . Then, the estimate (6.4) holds.

Proof. Note that in this case the Loomis–Whitney estimate remains the same, but the bilinear Strichartz estimate gains $N_1^{-\frac {\alpha }{4}}$ at the cost of $L_{\max }^{\frac {1}{2}}$ .

(i) Low $\boldsymbol {\times }$ High $\boldsymbol {\rightarrow }$ High ( $N_2 \lesssim N_1\sim N$ ): In the case $N_2 \lesssim 1$ , we consider two subcases. For $N_1^{\frac {1}{2}-\frac {\alpha }{4}} \lesssim N_2$ , we use the Loomis-Whitney estimate (4.18) to obtain

$$ \begin{align*} \begin{aligned} \sum_{N_1^{\frac{1}{2}-\frac{\alpha}{4}} \lesssim N_2}I &\lesssim \sum_{N_1^{\frac{1}{2}-\frac{\alpha}{4}} \lesssim N_2} N^{\frac{3}{2}-\frac{\alpha}{2}+\varepsilon} N_2^{-\frac{1}{2}} (L_1L_2)^{\frac{1}{2}}L^{\frac{1}{2}-\varepsilon'}N^{-1} \mathcal{A} \\ &\lesssim N_1^{\frac{5}{4}-\frac{3\alpha}{8}+\varepsilon} \sum_{N_1^{\frac{1}{2}-\frac{\alpha}{4}} \lesssim N_2} (L_1L_2)^{\frac{1}{2}}L^{\frac{1}{2}-\varepsilon'}N^{-1} \mathcal{A}. \end{aligned} \end{align*} $$

In the complementary case viz. $N_2\lesssim N_1^{\frac {1}{2}-\frac {\alpha }{4}}$ , using the bilinear Strichartz estimate (4.7), we have

$$ \begin{align*} \begin{aligned} \sum_{N_2\lesssim N_1^{\frac{1}{2}-\frac{\alpha}{4}}} I &\lesssim \sum_{N_2\lesssim N_1^{\frac{1}{2}-\frac{\alpha}{4}}} N_2^{\frac{1}{2}} N_1^{-\frac{\alpha}{4}} (L_{\min}L_{\max})^{\frac{1}{2}} \mathcal{A} \\ &\lesssim N_1^{\frac{5}{4}-\frac{3\alpha}{8}+\varepsilon}\sum_{N_2\lesssim N_1^{\frac{1}{2}-\frac{\alpha}{4}}} (L_1L_2)^{\frac{1}{2}}L^{\frac{1}{2}-\varepsilon'}N^{-1} \mathcal{A}. \end{aligned} \end{align*} $$

For $N_2\gtrsim 1$ , the same estimate as the case $L_{\max } \lesssim N_1^{\frac {\alpha }{2}}$ suffices.

(ii) High $\boldsymbol {\times }$ High $\boldsymbol {\rightarrow }$ Low ( $N_1\sim N_2 \gtrsim N$ ): This case can be dealt with in the same way as the corresponding case in $L_{\max } \lesssim N_1^{\frac {\alpha }{2}}$ since we employ the Loomis–Whitney estimate which is the same for both the cases.

The case $L_{\max }\gtrsim N_{\max }^{\alpha }N_{\min }$ is dealt with in the following:

Lemma 6.7. Let $\alpha \geqslant 5$ , $s>\frac {1-\alpha }{4}$ and $N,N_i \in 2^{\mathbb {Z}}$ , $L_i,L \in 2^{\mathbb {N}_0}$ , and suppose that (6.5). Let $f_{N_1,L_1}, g_{N_2,L_2}, h_{N,L}:\mathbb {R} \times \mathbb {R} \times \mathbb {Z}\to \mathbb {R}_{+}$ and $supp(f_{N_1,L_1}) \subseteq D_{N_1,L_1}$ , $\text {supp}(g_{N_2,L_2}) \subseteq D_{N_2,L_2}$ , $\text {supp}(h_{N,L}) \subseteq D_{N,L}$ such that $L_{\max }\gtrsim N_{\max }^{\alpha }N_{\min }$ . Then, the estimate (6.4) holds.

Proof. (i) Low $\boldsymbol {\times }$ High $\boldsymbol {\rightarrow }$ High ( $N_2 \lesssim N_1\sim N$ ): In case $L_{\max } = L_2$ , using Lemma 4.3, we have

$$ \begin{align*} \begin{aligned} I &\lesssim \|f_{N_1,L_1} \ast h_{N,L}\|_{L^2} \|g_{N_2,L_2} \|_{L^2}\\ &\lesssim N_2^{\frac{1}{2}} (L \wedge L_1)^{\frac{1}{2}} \langle (L \vee L_1) N_1\rangle^{\frac{1}{4}} \mathcal{A}\\ &\lesssim N_1^{-\frac{\alpha}{2}+\frac{5}{4}} (L\wedge L_1)^{\frac{1}{2}} (L \vee L_1)^{\frac{1}{4}}L_2^{\frac{1}{2}} N^{-1} \mathcal{A}. \end{aligned} \end{align*} $$

If $N_2 \lesssim 1$ , the above is summable for any s. For $N_2 \gtrsim 1$ , the above expression is dominated by

$$ \begin{align*} N_1^{-\frac{\alpha}{2} +\frac{5}{4}} N_2^{-s}(L\wedge L_1)^{\frac{1}{2}} (L \vee L_1)^{\frac{1}{4}}L_2^{\frac{1}{2}} N^{-1}\|f_{N_1,L_1}\|_{L^2} N_2^s\|g_{N_2,L_2}\|_{L^2} \|h_{N,L}\|_{L^2}. \end{align*} $$

If $s\geqslant 0$ , the expression is summable in the spatial frequencies. For $s<0$ , the above is dominated by

$$ \begin{align*} \Big(\frac{N_1}{N_2}\Big)^{-\frac{\alpha}{2}+\frac{5}{4}}N_2^{-s-\frac{\alpha}{2}+\frac{5}{4}} (L\wedge L_1)^{\frac{1}{2}} (L \vee L_1)^{\frac{1}{4}}L_2^{\frac{1}{2}} N^{-1}\|f_{N_1,L_1}\|_{L^2} N_2^s\|g_{N_2,L_2}\|_{L^2} \|h_{N,L}\|_{L^2} \end{align*} $$

which is summable for $s>\frac {5-\alpha }{4}$ .

If $L_{\max } = L$ , we use Lemma 4.3 as follows:

$$ \begin{align*} \begin{aligned} I &\lesssim \|f_{N_1,L_1}\ast g_{N_2,L_2}\|_{L^2} \|h_{N,L}\|_{L^2}\\ &\lesssim N_2^{\frac{1}{2}} (L_1 \wedge L_2)^{\frac{1}{2}} \langle (L_1 \vee L_2)N_2 \rangle^{\frac{1}{4}} \mathcal{A} \\ &\lesssim N_2^{\frac{1}{4}+\varepsilon} N_1^{1-\frac{\alpha}{2}+\varepsilon} (L_1 \wedge L_2)^{\frac{1}{2}} (L_1 \vee L_2)^{\frac{1}{4}} L^{\frac{1}{2}-\varepsilon'} N^{-1} \mathcal{A}. \end{aligned} \end{align*} $$

For $N_2\lesssim 1$ , summability follows since $\alpha \geqslant 5$ . For $N_2 \gtrsim 1$ , the above expression is bounded by

$$ \begin{align*} N_2^{\frac{1}{4}-s+\varepsilon} N_1^{1-\frac{\alpha}{2}+\varepsilon} (L_1 \wedge L_2)^{\frac{1}{2}} (L_1 \vee L_2)^{\frac{1}{4}} L^{\frac{1}{2}-\varepsilon'} N^{-1} N_2^s \mathcal{A}, \end{align*} $$

which can be summed up for $s>\frac {5}{4}-\frac {\alpha }{2}$ .

(ii) High $\boldsymbol {\times }$ High $\boldsymbol {\rightarrow }$ Low ( $N\lesssim N_1\sim N_2$ ): We first consider the case $L_{\max } = L$ . If $N\lesssim 1$ , the derivative in the nonlinearity is smoothing and using the bilinear Strichartz estimate from Lemma 4.3 for the high frequencies, we obtain

$$ \begin{align*} \begin{aligned} I &\lesssim \| f_{1,N_1,L_1} * g_{2,N_2,L_2} \|_{L^2} \|h_{N,L}\|_{L^2} \\ &\lesssim (N_1^\alpha N)^{-\frac{1}{2}+\varepsilon} N^{\frac{1}{2}} N_1^{\frac{1}{4}} (L_1 L_2)^{\frac{1}{2}} L^{\frac{1}{2}-\varepsilon} \mathcal{A}\\ &\lesssim N_1^{\frac{1}{4}- \frac{\alpha}{2}+\alpha \varepsilon - 2s} (L_1L_2)^{\frac{1}{2}} L^{\frac{1}{2}-\varepsilon} N_1^s \|f_{N_1,L_1}\|_{L^2} N_2^s \|g_{N_2,L_2}\|_{L^2} N^{\varepsilon} \|h_{N,L}\|_{L^2}. \end{aligned} \end{align*} $$

The above is summable for $s>\frac {1}{8}-\frac {\alpha }{4}$ .

For $N\gtrsim 1$ , the above estimate is still sufficient and is summable for $s>\frac {1}{8}-\frac {\alpha }{4}$ .

If $L_{\max } = L_1$ , we have using Lemma 4.3,

$$ \begin{align*} \begin{aligned} I &\lesssim \|g_{N_2,L_2}\ast h_{N,L}\|_{L^2} \|f_{N_1,L_1} \|_2 \\ &\lesssim N^{\frac{1}{2}} (L_2 \wedge L)^{\frac{1}{2}} \langle (L_2 \vee L) N\rangle^{\frac{1}{4}} \mathcal{A}\\ &\lesssim NN_1^{-\frac{\alpha}{2}} (L_2 \wedge L)^{\frac{1}{2}} \langle (L_2 \vee L) N\rangle^{\frac{1}{4}}L_1^{\frac{1}{2}} N^{-1} \mathcal{A} \\ &\lesssim NN_1^{-\frac{\alpha}{2}-2s} (L_2 \wedge L)^{\frac{1}{2}} \langle (L_2 \vee L) N\rangle^{\frac{1}{4}}L_1^{\frac{1}{2}} N^{-1} N_1^s\|f_{N_1,L_1}\|_{L^2} N_2^s \|g_{N_2,L_2}\|_{L^2} \|h_{N,L}\|_{L^2} \end{aligned} \end{align*} $$

If $N \lesssim 1$ , we require $s>-\frac {\alpha }{4}$ for summability in spatial frequencies. If $N \gtrsim 1$ , the following bound

$$ \begin{align*} \begin{aligned} &\lesssim N^{\frac{5}{4}+s} N_1^{-\frac{\alpha}{2}-2s} (L_2 \wedge L)^{\frac{1}{2}} \langle (L_2 \vee L) N\rangle^{\frac{1}{4}}L_1^{\frac{1}{2}} N^{-1} N_1^s\|f_{N_1,L_1}\|_{L^2} N_2^s \|g_{N_2,L_2}\|_{L^2} \\ &\quad \quad \times N^{-s}\|h_{N,L}\|_{L^2} \end{aligned} \end{align*} $$

implies that we require $s>\frac {-\alpha }{4}$ to be able to sum up the above estimate.

The very small frequencies can be handled as follows:

Lemma 6.8. Let $\alpha \geqslant 5$ , $s>\frac {1-\alpha }{4}$ and $N, N_i \in 2^{\mathbb {Z}}$ such that $N_{\max } \lesssim 1$ or $N_{\min } \lesssim N_{\max }^{-\frac {\alpha }{2}}$ . Let $f_{N_1,L_1}, g_{N_2,L_2}, h_{N,L}:\mathbb {R} \times \mathbb {R} \times \mathbb {Z}\to \mathbb {R}_{+}$ and $supp(f_{N_1,L_1}) \subseteq D_{N_1,L_1}$ , $\text {supp}(g_{N_2,L_2}) \subseteq D_{N_2,L_2}$ , $\text {supp}(h_{N,L}) \subseteq D_{N,L}$ . Then, the estimate (6.4) holds.

Proof. In this case, we do not distinguish between the resonant and the nonresonant case. Using Lemma 4.3, we have

$$ \begin{align*} \begin{aligned} I &\lesssim \|f_{N_1,L_1} \ast g_{N_2,L_2}\|_{L^2}\|h_{N,L}\|_{L^2}\\ &\lesssim N_{\min}^{\frac{1}{2}} (L_1\wedge L_2)^{\frac{1}{2}} \langle (L_1 \vee L_2) N_{\max} \rangle^{\frac{1}{4}} \mathcal{A}, \end{aligned} \end{align*} $$

which is sufficient.

6.3 Conclusion of the theorems on semilinear local well-posedness

Proof of Theorem 6.1

The proof follows along the same lines as for [Reference Sanwal and Schippa41, Theorem 6.1], and we shall be brief. We use $X^{s,b}$ spaces as the auxiliary spaces to run a fixed point argument for the operator given by:

$$ \begin{align*} \Gamma(u)(t):= \eta(t) S_{\alpha}(t)u_0 + \eta(t) \int_0^t S_{\alpha}(t-s)(u \partial_x u)(s)ds. \end{align*} $$

Here, $\eta $ is a smooth compactly supported time cut-off. Using the linear estimate, the energy estimate for $X^{s,b}$ spaces [Reference Tao46, Section 2.6] and Proposition 6.2, we obtain

$$ \begin{align*} \|\Gamma(u)\|_{X^{s,b}_1} \leqslant C (\|u(0)\|_{H^{s,0}} + \|u\|_{X^{s,b}_1}^2). \end{align*} $$

Similarly,

$$ \begin{align*} \| \Gamma(u_1) -\Gamma(u_2)\|_{X^{s,b}_1} \leqslant 2\tilde{C}(\|u_0\|_{H^{s,0}}) \|u_1-u_2\|_{X^{s,b}_1}. \end{align*} $$

For small initial data (attributed in the constants $C,\tilde {C}$ ), we can prove local well-posedness for (5.1) on $X^{s,b}_1$ . Using scaling and subcriticality of the regularity, any large data can be scaled to be small and one obtains well-posedness on a time interval $[0,T]$ , with T depending on the size of the initial data.

In preparation of the proof, we recall the following lemma to trade regularity in modulation to powers of time:

Lemma 6.9. Let $\eta \in \mathbb {R}$ , $-\frac {1}{2}<b' \leq b < \frac {1}{2}$ , then for any $0<T<1$ and $s \in \mathbb {R}$ , it holds

$$ \begin{align*} \| \eta(t/T) u \|_{X^{s,b'}} \lesssim_{\eta,b,b'} T^{b-b'} \| u \|_{X^{s,b}}. \end{align*} $$

Proof of Theorem 6.3

For small initial data and a fixed time interval $[0,1]$ , the proof of local well-posedness is the same as in the $\mathbb {R}^2$ case. In the large data case, we use the leeway in the modulation regularity in the proof of Proposition 6.4 to apply Lemma 6.9. This yields a modified bilinear estimate

$$ \begin{align*} \| \partial_x(u v) \|_{X^{s,b-1}_T} \lesssim T^{\delta} \| u \|_{X^{s,b}} \| v \|_{X^{s,b}}. \end{align*} $$

Thus, we see that the time of existence of the solution will depend on the size of the initial data and the well-posedness result follows similarly as in the $\mathbb {R}^2$ case.

Acknowledgments

Robert Schippa would like to thank the Department of Mathematics at the Tokyo Institute of Technology for kind hospitality in December 2023.

Competing interest

The authors have no competing interest to declare.

Funding statement

Shinya Kinoshita was supported by JSPS KAKENHI Grant number JP24K16945. Robert Schippa conducted initial work on this project at the Korea Institute for Advanced Study, whose financial support through the grant No. MG093901 is gratefully acknowledged. Further financial support from the Humboldt Foundation (Feodor-Lynen fellowship) and partial support by the NSF grant DMS-2054975 is gratefully acknowledged.

Data availability statement

Data sharing not applicable to this article as no datasets were generated or analyzed during the current study.

Ethical standards

The research meets all ethical guidelines, including adherence to the legal requirements of the study country.

Author contributions

R.S. conceptualized and drafted the study; the details were worked out by all authors together. All authors approved the final version of the manuscript.

References

Ablowitz, M. J. and Segur, H., ‘On the evolution of packets of water waves’, J. Fluid Mech. 92(4) (1979), 691715.10.1017/S0022112079000835CrossRefGoogle Scholar
Bejenaru, I., Herr, S. and Tataru, D., ‘A convolution estimate for two-dimensional hypersurfaces’, Rev. Mat. Iberoam. 26(2) (2010), 707728.10.4171/rmi/615CrossRefGoogle Scholar
Bejenaru, I. and Tao, T., ‘Sharp well-posedness and ill-posedness results for a quadratic non-linear Schrödinger equation’, J. Funct. Anal. 233(1) (2006), 228259.10.1016/j.jfa.2005.08.004CrossRefGoogle Scholar
Bennett, J. and Bez, N., ‘Some nonlinear Brascamp-Lieb inequalities and applications to harmonic analysis’, J. Funct. Anal. 259(10) (2010), 25202556.10.1016/j.jfa.2010.07.015CrossRefGoogle Scholar
Bennett, J. and Bez, N., ‘Higher order transversality in harmonic analysis’, in Harmonic Analysis and Nonlinear Partial Differential Equations, RIMS Kôkyûroku Bessatsu, B88 (Res. Inst. Math. Sci. (RIMS), Kyoto, 2021), 75103.Google Scholar
Bennett, J., Carbery, A. and Wright, J., ‘A non-linear generalisation of the Loomis-Whitney inequality and applications’, Math. Res. Lett. 12(4) (2005), 443457.10.4310/MRL.2005.v12.n4.a1CrossRefGoogle Scholar
Béthuel, F., Gravejat, P. and Saut, J.-C., ‘On the KPI transonic limit of two-dimensional Gross-Pitaevskii travelling waves’, Dyn. Partial Differ. Equ. 5(3) (2008), 241280.10.4310/DPDE.2008.v5.n3.a3CrossRefGoogle Scholar
Bourgain, J., ‘Fourier transform restriction phenomena for certain lattice subsets and applications to nonlinear evolution equations. II. The KdV-equation’, Geom. Funct. Anal. 3(3) (1993), 209262.10.1007/BF01895688CrossRefGoogle Scholar
Bourgain, J., ‘On the Cauchy problem for the Kadomtsev-Petviashvili equation’, Geom. Funct. Anal. 3(4) (1993), 315341.10.1007/BF01896259CrossRefGoogle Scholar
Bourgain, J. and Demeter, C., ‘The proof of the ${l}^2$ decoupling conjecture’, Ann. Math. (2) 182(1) (2015), 351389.10.4007/annals.2015.182.1.9CrossRefGoogle Scholar
Córdoba, A., ‘A note on Bochner-Riesz operators’, Duke Math. J. 46(3) (1979), 505511.10.1215/S0012-7094-79-04625-8CrossRefGoogle Scholar
Dryuma, V. S., ‘Analytic solution of the two-dimensional Korteweg-de Vries (KdV) equation’, Soviet Journal of Experimental and Theoretical Physics Letters 19 (June 1974), 387.Google Scholar
Fefferman, C., ‘A note on spherical summation multipliers’, Israel J. Math. 15 (1973), 4452.10.1007/BF02771772CrossRefGoogle Scholar
Guo, Z., ‘Remark on the low regularity well-posedness of the KP-I equation’, August 2024, arXiv e-prints, page arXiv:2408.14932.Google Scholar
Guo, Z. and Molinet, L., ‘On the well-posedness of the KP-I equation’, April 2024, arXiv e-prints, page arXiv:2404.12364.Google Scholar
Guo, Z. and Oh, T., ‘Non-existence of solutions for the periodic cubic NLS below ${L}^2$ ’, Int. Math. Res. Not. IMRN 6 (2018), 16561729.Google Scholar
Guo, Z., Peng, L. and Wang, B., ‘On the local regularity of the KP-I equation in anisotropic Sobolev space’, J. Math. Pures Appl. (9) 94(4) (2010), 414432.10.1016/j.matpur.2010.03.012CrossRefGoogle Scholar
Hadac, M., ‘Well-posedness for the Kadomtsev-Petviashvili II equation and generalisations’, Trans. Am. Math. Soc. 360(12) (2008), 65556572.10.1090/S0002-9947-08-04515-7CrossRefGoogle Scholar
Hadac, M., Herr, S. and Koch, H., ‘Well-posedness and scattering for the KP-II equation in a critical space’, Ann. Inst. Henri Poincaré, Anal. Non Linéaire 26(3) (2009), 917941.10.1016/j.anihpc.2008.04.002CrossRefGoogle Scholar
Herr, S., Sanwal, A. and Schippa, R., ‘Low regularity well-posedness of KP-I equations: The three-dimensional case’, J. Funct. Anal. 286(4) (2024), Paper No. 110292.10.1016/j.jfa.2023.110292CrossRefGoogle Scholar
Herr, S., Schippa, R. and Tzvetkov, N., ‘The Cauchy problem for the periodic Kadomtsev–Petviashvili–II equation below ${L}^2$ ’, July 2024, arXiv e-prints, page arXiv:2407.12222.Google Scholar
Ionescu, A. D., Kenig, C. E. and Tataru, D., ‘Global well-posedness of the KP-I initial-value problem in the energy space’, Invent. Math. 173(2) (2008), 265304.10.1007/s00222-008-0115-0CrossRefGoogle Scholar
jun, R. J. Iório and Nunes, W. V. L., ‘On equations of KP-type’, Proc. R. Soc. Edinb. Sect. A Math. 128(4) (1998), 725743.Google Scholar
Borisovich Kadomtsev, B. and Petviashvili, V. I., ‘On the stability of solitary waves in weakly dispersing media’, Sov. Phys. Dokl. 15 (1970), 539541.Google Scholar
Kawahara, T., ‘Oscillatory solitary waves in dispersive media’, J. Phys. Soc. Jpn. 33(1) (1972), 260264.10.1143/JPSJ.33.260CrossRefGoogle Scholar
Kenig, C. E., ‘On the local and global well-posedness theory for the KP-I equation’, Ann. Inst. H. Poincaré C Anal. Non Linéaire 21(6) (2004), 827838.10.1016/j.anihpc.2003.12.002CrossRefGoogle Scholar
Killip, R. and Vişan, M., ‘KdV is well-posed in ${H}^{-1}$ ’, Ann. Math. (2) 190(1) (2019), 249305.10.4007/annals.2019.190.1.4CrossRefGoogle Scholar
Killip, R., Vişan, M. and Zhang, X., ‘Low regularity conservation laws for integrable PDE’, Geom. Funct. Anal. 28(4) (2018), 10621090.10.1007/s00039-018-0444-0CrossRefGoogle Scholar
Kinoshita, S., Sanwal, A. and Schippa, R., ‘Improved well-posedness results for KP-I equations in the quasilinear regime’, accepted to Discrete Cont. Dyn. Syst.Google Scholar
Kinoshita, S. and Schippa, R., ‘Loomis-Whitney-type inequalities and low regularity well-posedness of the periodic Zakharov-Kuznetsov equation’, J. Funct. Anal. 280(6) (2021), Paper No. 108904, 53.10.1016/j.jfa.2020.108904CrossRefGoogle Scholar
Klein, C. and Saut, J.-C., ‘Nonlinear dispersive equations—inverse scattering and PDE methods’, volume 209 of Applied Mathematical Sciences. Springer, Cham, 2021.10.1007/978-3-030-91427-1CrossRefGoogle Scholar
Koch, H. and Tzvetkov, N., ‘On the local well-posedness of the Benjamin-Ono equation in ${H}^s\left(\mathbb{R}\right)$ ’, Int. Math. Res. Not. 2003(26) (2003), 14491464.10.1155/S1073792803211260CrossRefGoogle Scholar
Koch, H. and Steinerberger, S., ‘Convolution estimates for singular measures and some global nonlinear Brascamp-Lieb inequalities’, Proc. Roy. Soc. Edinburgh Sect. A 145(6) (2015), 12231237.10.1017/S0308210515000323CrossRefGoogle Scholar
Koch, H. and Tataru, D., ‘Conserved energies for the cubic nonlinear Schrödinger equation in one dimension’, Duke Math. J. 167(17) (2018), 32073313.10.1215/00127094-2018-0033CrossRefGoogle Scholar
Molinet, L., Saut, J. C. and Tzvetkov, N., ‘Global well-posedness for the KP-I equation’, Math. Ann. 324(2) (2002), 255275.10.1007/s00208-002-0338-0CrossRefGoogle Scholar
Molinet, L., Saut, J.-C. and Tzvetkov, N., ‘Well-posedness and ill-posedness results for the Kadomtsev-Petviashvili-I equation’, Duke Math. J. 115(2) (2002), 353384.10.1215/S0012-7094-02-11525-7CrossRefGoogle Scholar
Molinet, L., Saut, J. C. and Tzvetkov, N., ‘Global well-posedness for the KP-I equation on the background of a non-localized solution’, Commun. Math. Phys. 272(3) (2007), 775810.10.1007/s00220-007-0243-1CrossRefGoogle Scholar
Robert, T., ‘Global well-posedness of partially periodic KP-I equation in the energy space and application’, Ann. Inst. H. Poincaré C Anal. Non Linéaire 35(7) (2018), 17731826.10.1016/j.anihpc.2018.03.002CrossRefGoogle Scholar
Rousset, F. and Tzvetkov, N., ‘Stability and instability of the KdV solitary wave under the KP-I flow’, Commun. Math. Phys. 313(1) (2012), 155173.10.1007/s00220-012-1495-yCrossRefGoogle Scholar
Rousset, F. and Tzvetkov, N., ‘Transverse nonlinear instability for two-dimensional dispersive models’, Ann. Inst. Henri Poincaré, Anal. Non Linéaire 26(2) (2009), 477496.10.1016/j.anihpc.2007.09.006CrossRefGoogle Scholar
Sanwal, A. and Schippa, R., ‘Low regularity well-posedness for KP-I equations: the dispersion-generalized case’, Nonlinearity 36(8) (2023), 43424383.10.1088/1361-6544/ace1ccCrossRefGoogle Scholar
Saut, J.-C. and Tzvetkov, N., ‘The Cauchy problem for higher-order KP equations’, J. Differ. Equations 153(1) (1999), 196222.10.1006/jdeq.1998.3534CrossRefGoogle Scholar
Saut, J.-C. and Tzvetkov, N., ‘The Cauchy problem for the fifth order KP equations’, J. Math. Pures Appl. (9) 79(4) (2000), 307338.10.1016/S0021-7824(00)00156-2CrossRefGoogle Scholar
Schippa, R., ‘Short-time Fourier transform restriction phenomena and applications to nonlinear dispersive equations’, PhD thesis, Bielefeld University, 2019.Google Scholar
Sprenger, P., Bridges, T. J. and Shearer, M., ‘Traveling wave solutions of the Kawahara equation joining distinct periodic waves’, J. Nonlinear Sci. 33(5) (2023), 79.10.1007/s00332-023-09922-0CrossRefGoogle Scholar
Tao, T., Nonlinear dispersive equations: local and global analysis. CBMS Regional Conference Series in Mathematics, 106 American Mathematical Society (AMS), Providence, RI, 2006, 373 p.10.1090/cbms/106CrossRefGoogle Scholar
Ukai, S., ‘On the Cauchy problem for the KP equation’, Recent Topics in Nonlinear PDE, IV, Proc. 5th Meet., Kyoto/Jap. 1988, North-Holland Math. Stud. 160 (1989), 179194.10.1016/S0304-0208(08)70512-7CrossRefGoogle Scholar
Zhang, Y., ‘Local well-posedness of KP-I initial value problem on torus in the Besov space’, Comm. Partial Differential Equations 41(2) (2016), 256281.10.1080/03605302.2015.1126733CrossRefGoogle Scholar