Abstract
This paper is devoted to studying the Cauchy problem for the generalized Ostrovsky equation
with \(\beta \gamma <0,\gamma >0\). Firstly, we prove that the Cauchy problem for the generalized Ostrovsky equation is locally well-posed in \(H^{s}(\mathbf{R})\left( s>\frac{1}{2}-\frac{2}{k}\right) \). Then, we prove that the Cauchy problem for the generalized Ostrovsky equation is locally well-posed in \(X_{s}(\mathbf{R}): =\Vert f\Vert _{H^{s}}+\left\| {\mathscr {F}}_{x}^{-1}\left( \frac{{\mathscr {F}}_{x} f(\xi )}{\xi }\right) \right\| _{H^{s}}\left( s>\frac{1}{2}-\frac{2}{k}\right) .\) Finally, we show that the solution to the Cauchy problem for generalized Ostrovsky equation converges to the solution to the generalized KdV equation as the rotation parameter \(\gamma \) tends to zero for data belonging to \(X_{s}(\mathbf{R})(s>\frac{3}{2})\). The main difficulty is that the phase function of Ostrovsky equation with negative dispersive \(\beta \xi ^{3}+\frac{\gamma }{\xi }\) possesses the zero singular point.
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1 Introduction
In this paper, we consider the Cauchy problem for the generalized Ostrovsky equation
Here \(\partial _{x}^{-1}\) is defined by
This equation was introduced by Levandosky and Liu in [28]. When \(k=2\), (1.1) was Ostrovsky equation with negative dispersion, which was introduced by Ostrovsky in [33] as a model for weakly nonlinear long waves, by taking into account of the Coriolis force, to describe the propagation of surface waves in the ocean in a rotating frame of reference [1, 11, 12]. The Ostrovsky equation with negative dispersion has been investigated by some authors [15,16,17,18,19,20, 29, 31, 36]. In the absence of rotation (that is, \(\gamma =0\)), it becomes the generalized Korteweg–de Vries equation, which has been investigated by some authors [5,6,7,8,9,10, 22, 23]. Kenig et al. [23] established the small data global theory of generalized Korteweg–de Vries equation in the critical Sobolev space \({\dot{H}}^{s_{k}}(\mathbf{R})\) with \(s_{k}=\frac{1}{2}-\frac{2}{k}.\) Farah and Pastor [7] presented an alternative proof of the result of Kenig, Ponce and Vega [23].
To the best of our knowledge, the optimal regularity problem of the Cauchy problem for (1.1) in inhomogeneous Sobolev spaces has not been investigated. In this paper, we investigate the Cauchy problem for (1.1) in inhomogeneous Sobolev spaces. By using the Fourier restriction norm method introduced in [2, 3] and developed in [24,25,26], firstly we establish three multilinear estimates. Then, by exploiting the multilinear estimates and the fixed point theorem, we prove that the Cauchy problem for the generalized Ostrovsky equation is locally well-posed in \(H^{s}(\mathbf{R})\left( s>\frac{1}{2}-\frac{2}{k}\right) \) and in \(X_{s}(\mathbf{R}): =\Vert f\Vert _{H^{s}}+\left\| {\mathscr {F}}_{x}^{-1}\left( \frac{{\mathscr {F}}_{x}f(\xi )}{\xi }\right) \right\| _{H^{s}}\left( s>\frac{1}{2}-\frac{2}{k}\right) .\) Finally, we show that the solution to the Cauchy problem for generalized Ostrovsky equation converges to the solution to the generalized KdV equation as the rotation parameter \(\gamma \) tends to zero for data belonging to \(X_{s}(\mathbf{R})(s>\frac{3}{2})\).
We give some notations before presenting the main results. \(\chi _{A}(x)=1\) if \(x\in A\), otherwise \(\chi _{A}(x)=0\). \(a\sim b\) means that there exists two positive constants \(C_{1},C_{2}\) which may depend on \(\beta ,\gamma \) such that \(C_{1}|a|\le |b|\le C_{2}|a|.\) \(a\gg b\) means that there exists positive constant C which may depend on \(\beta ,\gamma \) such that \(|a|\ge C |b|.\) We define \(A:= \max \left\{ 1,\left| \frac{6\gamma }{7\beta }\right| ^{\frac{1}{4}}, \left| \frac{\gamma }{3\beta }\right| ^{\frac{1}{2}},\left| \frac{\gamma }{\beta }\right| ,100|\beta |, 100|\gamma |\right\} ,a:=2^{[A]}\), where [A] denotes the largest integer which is smaller than A. We define \(\langle \cdot \rangle =1+|\cdot |.\) Let \(\psi \) be a smooth jump function, satisfying \(0\le \psi \le 1\), \(\psi (t)=1\) for \(|t|\le 1\), \(supp\psi \in [-2,2]\) and \(\psi (t)=0\) for \(|t|>2.\) For \(\delta >0\) define \(\psi _{\delta }(t)=\psi (\frac{t}{\delta })\).
\(H^{s}(\mathbf{R})=\left\{ f\in {\mathscr {S}}^{\prime }(\mathbf{R}):\Vert f \Vert _{H^{s}(\mathbf{R})}= \Vert \langle \xi \rangle ^{s}{\mathscr {F}}_{x}{f}\Vert _{L_{\xi }^{2}(\mathbf{R})}<\infty \right\} \). The space \(X_{s,b}(\mathbf{R}^{2})\) is defined as follows:
Here, \(\langle \sigma \rangle =1+|\tau +\phi (\xi )|.\) The space \(X_{s}(\mathbf{R})\) is defined \(X_{s}(\mathbf{R})=\{f\in H^{s}(\mathbf{R}):{\mathscr {F}}_{x}^{-1} (\frac{{\mathscr {F}}_{x}f(\xi )}{\xi })\in H^{s}(R)\}\) with the norm \(\Vert f\Vert _{X_{s}(\mathbf{R})}=\Vert f\Vert _{H^{s}}+\left\| {\mathscr {F}}_{x}^{-1} \left( \frac{{\mathscr {F}}_{x}f(\xi )}{\xi }\right) \right\| _{H^{s}}\). The space \({\tilde{X}}_{s,b}\) is defined as follows
The main result of this paper are as follows:
Theorem 1.1
(1.1). is locally well-posed for the initial data \(u_{0}\) in \(H^{s}(\mathbf{R})\) with \(s>\frac{1}{2}-\frac{2}{k},k\ge 5\) and \(\beta <0,\gamma >0\) .
Remark 1
Theorem 1.1 is obtained by combining the multilinear estimate proved in Lemma 3.1, the linear estimate of Lemma 2.1, and a fixed point argument. Thus, Lemma 3.1 plays the crucial role in establishing Theorem 1.1. The structure of (1.1) is more complicated than that of the generalized KdV equation. More precisely, the phase function of (1.1) \(\beta \xi ^{3} +\frac{\gamma }{\xi }\) possesses the zero singular point. For the generalized KdV equation, the following two important facts are valid.
and
where \(0<M\le 1.\) For the proof of (1.3) and (1.4), we refer the readers to [14, 24].
The two main ingredients in the proof of the multilinear estimate are as follows:
and
for \(0<M\le 1,s_{1}>\frac{1}{4}.\) For the proof of (1.5) and (1.6), we refer the readers to the proof of Lemmas 2.2, 2.4, respectively.
For (1.5), only when
then we have
When
in most cases, we consider
Moreover, the maximal function estimate (2.46) plays the important role in dealing with \((\xi _{1},\xi _{2},\ldots ,\xi _{k},\xi ,\tau _{1},\tau _{2}, \ldots ,\tau _{k},\tau )\in \Omega _{5}\).
Remark 2
From [31], we know that when \(u_{0}\in H^{1}(\mathbf{R}),\) we cannot obtain the upper bound of \(\Vert u\Vert _{H^{1}(\mathbf{R})}\); thus, we cannot obtain the global well-posedness of (1.1).
Remark 3
From [23] and [7], we know that \(s=\frac{1}{2}-\frac{2}{k}\) is the critical regularity index in Sobolev spaces for (1.1) with \(\gamma =0\), which is just the generalized KdV equation.
Theorem 1.2
(1.1). is locally well-posed for the initial data \(u_{0}\) in \(X_{s}(\mathbf{R})\) with \(s>\frac{1}{2}-\frac{2}{k},k\ge 5\) and \(\beta <0,\gamma >0\).
Theorem 1.3
Let \(u^{\gamma }\) be the solution to (1.1) in \(X_{s}(\mathbf{R})\) with \(s>\frac{3}{2},k\ge 5\) and \(\beta <0,\gamma >0\). Then, \(u^{\gamma }\) converges in \(H^{s}(\mathbf{R})\) with \(s>\frac{3}{2},k\ge 5\) to the solution to generalized KdV equation as \(\gamma \rightarrow 0\) and \(u_{0}\) tends to the initial data of the generalized KdV in \(L^{2}(\mathbf{R})\). More precisely,
Here, T is the time lifespan of the solution to (1.1) for data in \(X_{s}(\mathbf{R})\) guaranteed by Theorem 1.2 and u is the solution to (1.1)–(1.2) and v is the solution to the Cauchy problem for the generalized KdV equation
The rest of the paper is arranged as follows. In Sect. 2, we give some preliminaries. In Sect. 3, we show some multilinear estimates. In Sect. 4, we prove Theorem 1.1. In Sect. 5, we prove Theorem 1.2. In Sect. 6, we prove Theorem 1.3.
2 Preliminaries
Lemma 2.1
Let \(\delta \in (0,1)\) and \(s\in \mathbf{R}\) and \(-\frac{1}{2}<b^{\prime } \le 0\le b\le b^{\prime }+1\). Then, for \(h\in X_{s,b^{\prime }},\) we have
For the proof of Lemma 2.1, we refer the readers to [2, 3, 14].
Lemma 2.2
Let \(q\ge 8, 0<M\le 1\) and \(s=\frac{1}{8}-\frac{1}{q}\), \(s_{1}=\frac{1}{4}+\epsilon \) and \(b=\frac{1}{2}+\frac{\epsilon }{24}\) and \(0\le \epsilon \le 10^{-3}\). Then, we have
Proof
For (2.3), we refer the readers to Lemma 2.1 of [37]. By using the Sobolev embeddings theorem and (2.3), we derive
By changing variable \(\tau =\lambda -\phi (\xi )\), we derive
By using (2.12), (2.13) and Minkowski’s inequality, for \(b>\frac{1}{2},\) we derive
Thus, we obtain (2.4).
can be seen in (2.3) of Lemma 2.1 of [15]. By using (2.15) and a proof similar to (2.4), we obtain (2.5). By using (2.3) and a proof similar to (2.4), we obtain (2.6). Interpolating (2.6) with
yields (2.7).
can be seen in (2.1) of Lemma 2.1 of [15]. By using (2.17) and a proof similar to (2.4), we obtain (2.8). From (31) of Lemma 3.4 of [31], for \(s_{1}=\frac{1}{4}+\epsilon , s_{2}>\frac{3}{4},0<M\le 1\), we know that
By using (2.18) and a proof similar to (2.4), we obtain (2.9). Interpolating (2.8) with (2.16) leads to (2.10). Interpolating (2.5) with (2.16) leads to (2.11).
We have completed the proof of Lemma 2.2.
Lemma 2.3
We assume that \(\phi \in C^{\infty }(\mathbf{R})\) and \(x_{i}(1\le i\le n)\) are only simple zeros of \(\phi (x)\) which means \(\phi (x_{i})=0\) and \(\phi ^{\prime }(x_{i})\ne 0\). Then, we have
where \(\delta \) is Dirac delta function.
Proof
For \(f\in C_{0}(\mathbf{R})\) as a test function for the distribution. Since \(f\in C_{0}(\mathbf{R})\) and \(\phi \in C^{\infty }(\mathbf{R})\) and \(\phi ^{\prime }(x_{i})\ne 0\), \(\forall \epsilon >0(<\frac{|\phi ^{\prime }(x_{i})|}{2}),\) there exists \(\delta _{1} >0\) such that when \(|x-x_{i}|<\delta _{1}\), we have
From (2.21), we know that \(|\phi ^{\prime }(x)|\ge |\phi ^{\prime }(x_{i})|-\epsilon \ge \frac{|\phi ^{\prime }(x_{i})|}{2}.\) Thus, when \(x\in (x_{i}-\delta _{1},x_{i}+\delta _{1})\), we have
We define
We claim
By a change of the variable \(u=\phi (x)\), \(\mathrm{d}u=\phi ^{\prime }(x)\mathrm{d}x\). Then, by using (2.24) and \(\int _{\phi (x_{i}-\delta _{1})}^{\phi (x_{i}+\delta _{1})}\delta (u)\mathrm{d}u=1\), we have
Since \(\epsilon >0\) is arbitrary small, from (2.25), we know that (2.24) is valid. Using (2.24), we have
Thus, since \(f\in C_{0}(\mathbf{R}),\) we obtain
We have completed the proof of Lemma 2.3.
Remark 3
In page 184 of [11], Gel’fand and Shilov [11] presented the conclusion of Lemma 2.3, however, they did not give the strict proof.
Lemma 2.4
Let \(b>\frac{1}{2}\). Then, we have
Here
In particular, for \(b>\frac{1}{2},\) we have
Here
Proof
Following the idea of [13, 14], we present the proof of Lemma 2.4. By using the Plancherel identity with respect to the space variable and
we derive
From Lemma 2.3, we have \(\delta [g(x)]=\sum \limits _{i=1}^{n} \frac{\delta (x-x_{i})}{|g^{\prime }(x_{i})|}\), where
and Lemma 2.3 is going to be applied with the variable \(x=\eta _{1}\). Since \(g^{\prime \prime }\ne 0\), then g has only two simple zeros, \(x_{1}=\xi _{1}\) and \(x_{2}=\xi -\xi _{1}\).
Hence, \(g^{\prime }(x_{1})=\phi ^{\prime }(\xi _{2})-\phi ^{\prime }(\xi _{1})\) and \(g^{\prime }(x_{2})=\phi ^{\prime }(\xi _{1})-\phi ^{\prime }(\xi _{2})\). Thus, (2.31) can be rewritten as
We define \({\mathscr {F}}v_{j\lambda }(\xi )={\mathscr {F}}u_{j}(\xi ,\lambda -\phi (\xi ))(j=1,2),\) and
Thus, by using (2.34), we have
By using a direct computation, we have
By using the Minkowski’s inequality, the Plancherel identity, (2.28), (2.35) and (2.36), we have
We have completed the proof of Lemma 2.4.
Lemma 2.5
We assume that \(b>\frac{1}{2}\), \(0\le s\le \frac{1}{2}.\) Then, we have
Lemma 2.5 can be proved similarly to Corollary 3.2 of [13] and Lemma 2.2 of [30] with the aid of Lemma 2.4.
Lemma 2.6
Let \(\phi _{j}(j=1,2)\in C^{\infty }(\mathbf{R})\) and \({\text {supp}}\phi _{2}\subset (a,b)\). If \(\phi _{1}^{\prime }(\xi )\ne 0\) for all \(\xi \in [a,b]\), then
for all \(k\ge 0\), where the constant C depends on \(\phi _{1},\phi _{2}\) and k.
Lemma 2.6 can be seen in [35].
Lemma 2.7
Let \(\phi _{4}(\xi )\in C^{\infty }(\mathbf{R})\) and \(\phi _{3}(\xi )\in C^{3}(\mathbf{R})\) and \({\text {supp}}\phi _{3}(\xi )\subset (a,b)\) and \(\left| \phi _{3}^{(3)}(\xi )\right| \ge 1\) uniformly with respect to \(\xi \). Then, we have
Lemma 2.7 can be seen in [35].
Lemma 2.8
Let
Here, \(N\in 2^{Z},N\ge a\). For \(\gamma \ge 7\), we obtain
Proof
We define
Obviously, \(\mathbf{R}_{x}\times \mathbf{R}_{t}=\bigcup \nolimits _{j=1}^{3}\Omega _{j}\). We define \(\Omega _{x,i}:=\left\{ t\in \mathbf{R}|(x,t)\in \Omega _{i}\right\} \) for a fixed \(x\in \mathbf{R}\). Without loss of generality, we assume that \(N\le \xi \le 4N.\) Assume that \(\eta =\frac{\xi }{N}\), then we have
By using a direct computation and from the definition \(\Omega _{x1}\), we have
By using a direct computation, we have \(-it\phi (\xi )+ix\xi =-i\beta N^{3}\eta ^{3}t-\frac{i\gamma t}{N\eta }+ixN\eta =ixN(\eta -\frac{\beta N^{2}\eta ^{3}t}{x}-\frac{\gamma t}{N^{2}x\eta }):= ixN\phi _{5}(\eta ),\) where \(\phi _{5}(\eta )=\eta -\frac{\beta N^{2}\eta ^{3}t}{x} -\frac{\gamma t}{N^{2}x\eta }\). Obviously,
for any \((x,t)\in \Omega _{2}\). Therefore, \(\phi _{5}^{\prime }\ne 0\) in this region. From Lemma 2.6, we know that \(|K(x,t)|\le C N(N|x|)^{-2}=N^{-1}x^{-2}\). Thus, we derive
We define \(-i\beta N^{3}\eta ^{3}t+ixN\eta -\frac{i\gamma t}{N\eta }=-it\beta N^{3}(\eta ^{3}+\frac{\gamma }{\beta \eta N^{4}}-\frac{x\eta }{\beta N^{2}t}): =itN^{3}\beta \phi _{6}(\eta )\).Obviously, we have \(|\phi _{6}^{(3)}(\eta )|\ge 1\). By using Lemma 2.7, we have
Thus, by using (2.41), for \(\gamma \ge 7,\) we have
Putting together (2.39), (2.40) with (2.42), we derive
We have completed the proof of Lemma 2.8.
Remark 3
Inspired by the idea of Proposition 2.5 of [34], we show Lemma 2.8.
Lemma 2.9
We assume that \(\gamma \ge 4\) and \(supp({\mathscr {F}}_{x}{f}) \subseteq \{\xi |N\le |\xi |\le 4N\}\), where \(N\in 2^{Z}\), \(N\ge a\). For \(f\in L_{x}^{2}(\mathbf{R})\), we have
Here
We assume that \(b>\frac{1}{2},\) \(\gamma \ge 4\) and \(supp({\mathscr {F}}_{x}{u}) \subseteq \{\xi |N\le |\xi |\le 4N\}\), where \(N\in 2^{Z}\), \(N\ge a.\) Then, we derive
We assume that \(b>\frac{1}{2},\) \(\gamma \ge 4\) and \(supp({\mathscr {F}}_{x}{u}) \subseteq \{\xi |a\le |\xi |<\infty \}\) for any t. Then, we have
Here, \(s=\frac{1}{2}-\frac{1}{\gamma }+\epsilon .\)
Proof
From (2.1) of [15], we have
We firstly show that (2.43) is valid for \(\gamma \ge 7.\) We define \(Tf:=U^{\gamma ,\beta }(t)f\), where \(T:L_{x}^{2}\rightarrow L_{x}^{\gamma }L_{t}^{\infty }\). Obviously, we have \(T^{*}F=\int _{\mathbf{R}}e^{t(\beta \partial _{x}^{3}+\gamma \partial _{x}^{-1})}F \mathrm{d}t\). By Using the \(TT^{*}\) idea, we know that that (2.43) is equivalent to
Here, \(F\in L_{x}^{2}L_{t}^{1}(\mathbf{R}\times \mathbf{R})\) possesses the same frequency support as u. Thus, to obtain (2.43), it suffices to prove (2.48). By using a direct computation, we have
Thus, the term on the left hand side of (2.48) can be rewritten as
Here, \(*\) denotes the convolution with respect to variables x, t and
From Young inequality and Lemma 2.8, we derive
Consequently, when \(\gamma \ge 7,\) we derive
Interpolating (2.47) with (2.50) leads to
By changing variable \(\tau =\lambda -\phi (\xi )\), we derive
By using (2.51), (2.52) and Minkowski’s inequality and the change of variable \(\lambda =\tau +\phi ,\) for \(b>\frac{1}{2}\), we have
Since
thus, by using the Minkowski equality and Cauchy–Schwarz inequality, we have
where \(s=\frac{1}{2}-\frac{1}{\gamma }+\epsilon .\) By using (2.55) and a proof similar to (2.45), we obtain that (2.46) is valid.
We have completed the proof of Lemma 2.9.
Lemma 2.10
We assume that \(\gamma \ge 4\) and \(supp({\mathscr {F}}_{x}{u})\subseteq \{\xi |N\le |\xi |\le 4N\}\), \(N\in 2^{Z}\). For \(b>\frac{1}{2}\) and \(f\in L_{x}^{2}(\mathbf{R})\), we have
For \(b>\frac{1}{2},\) and \(supp({\mathscr {F}}_{x}{u}) \subseteq \{\xi |0<|\xi |\le a\}\) for any t, we have
Here, \(s=\frac{1}{4}-\epsilon .\) For \(b>\frac{1}{2},\) and \(supp({\mathscr {F}}_{x}{u}) \subseteq \{\xi |0<|\xi |\le a\}\) for any t, we have
Proof
Without loss of generality, we can assume that \(supp({\mathscr {F}}_{x}{u})\subseteq [N,4N]\). By using the Cauchy–Schwarz inequality and the Minkowski’s inequality, we have
Thus, by using the Minkowski’s inequality, from (2.59) and (2.9), we have
By using (2.60) and a proof similar to (2.46), we obtain that (2.57) is valid. Interpolating (2.9) with (2.57) yields (2.58).
This completes the proof of Lemma 2.10.
Lemma 2.11
For \(b>\frac{1}{2}\), we have
Proof
Using the Sobolev embeddings theorem and (2.3),we have
By using (2.62) and a proof similar to (2.4), we obtain that (2.61) is valid.
This completes the proof of Lemma 2.11.
Lemma 2.12
Let \(s>0\), \(1<p<\infty \). Then, we have
For the proof of Lemma 2.12, we refer the readers to Lemma XI of [21].
3 Multilinear estimates
In this section, we present some crucial multilinear estimates which play an important role in establishing Theorems 1.1 and 1.2.
Lemma 3.1
Let \(s\ge \frac{1}{2}-\frac{2}{k}+2\epsilon ,k\ge 5\) and \(b=\frac{1}{2}+\frac{\epsilon }{24}\) and \(g_{j}=\psi (t)u_{j}.\) Then, we have
Proof
To prove (3.1), by duality, it suffices to prove
We define
By using the Plancherel identity, to prove (3.2), it suffices to prove
where \(\mathrm{d}\delta =\mathrm{d}\xi _{1}\mathrm{d}\xi _{2}\cdot \cdot \cdot \mathrm{d}\xi _{k} \mathrm{d}\xi \mathrm{d}\tau _{1}\mathrm{d}\tau _{2}\cdot \cdot \cdot \mathrm{d}\tau _{k}\mathrm{d}\tau .\)
We define
Without loss of generality, we can assume that \(|\xi _{1}|\ge |\xi _{2}|\ge \cdot \cdot \cdot \ge |\xi _{k+1}|.\)
Obviously,
Here,
(1) Case \((\xi _{1},\xi _{2},\ldots ,\xi _{k},\xi ,\tau _{1},\tau _{2},\ldots , \tau _{k},\tau )\in \Omega _{0}\), by using the Plancherel identity, the Hölder inequality and (2.4), we have
(2) Case \((\xi _{1},\xi _{2},\ldots ,\xi _{k},\xi ,\tau _{1},\tau _{2},\ldots ,\tau _{k},\tau )\in \Omega _{1}\), we have \(|\xi |\sim |\xi _{1}|\), then we consider
When (3.5) is valid, we have
Thus,
By using (3.7), the Plancherel identity, the Hölder inequality, Lemma 2.5, (2.4) and (2.7), we have
When (3.6) is valid, we have \(|\xi _{1}|\sim |\xi _{2}|^{-1}\). In this case, we consider
respectively.
When (3.8) is valid, since \(|\xi |\sim |\xi _{1}|\sim |\xi _{2}|^{-1}, s\ge \frac{1}{2}-\frac{2}{k}+2\epsilon \), we have
By using (3.10), the Plancherel identity, the Hölder inequality, Lemma 2.5, (2.8), (2.9) and (2.57), we have
When (3.9) is valid, we have that \(|\xi _{2}|^{-1}\sim |\xi _{1}|\sim |\xi |\sim |\xi _{k+1}|^{-1}\), since \(s\ge \frac{1}{2}-\frac{2}{k}+2\epsilon \), we have
By using (3.11), the Plancherel identity, the Hölder inequality, (2.8)–(2.10), (2.57), (2.58), we have
(3) Case \((\xi _{1},\xi _{2},\ldots ,\xi _{k},\xi ,\tau _{1},\tau _{2}, \ldots ,\tau _{k},\tau )\in \Omega _{2}\), we have \(|\xi _{1}|\sim |\xi _{2}|\ge 80ka|\xi _{3}|\), and then we consider
When (3.12) is valid, since \(s\ge \frac{1}{2}-\frac{2}{k}+2\epsilon \), \(|\xi _{1}|\sim |\xi _{2}|\), \(|\xi |\le C|\xi _{1}|\), we have
By using (3.14), the Plancherel identity, the Hölder inequality, Lemma 2.5, (2.4), (2.5), (2.7), we have
When (3.13) is valid, we have \(|\xi _{1}|\sim |\xi _{2}|\sim |\xi _{3}|^{-1}\), and we consider \(|\xi |\le a,|\xi |\ge a\), respectively.
When \(|\xi |\le a,\) we have
By using (3.15), the Plancherel identity, the Hölder inequality, (2.4) and (2.57), we have
When \(|\xi |\ge a,\) we consider (3.8), (3.9), respectively.
When (3.8) is valid, since \(|\xi _{1}|\sim |\xi _{2}|\sim |\xi _{3}|^{-1}, s\ge \frac{1}{2}-\frac{2}{k}+2\epsilon \), we have
By using (3.16), the Plancherel identity, the Hölder inequality, Lemmas 2.5, 2.11, (2.8), (2.9) and (2.57), we have
When (3.9) is valid, since \(|\xi |\sim |\xi _{k+1}|^{-1}\), \(|\xi _{1}|\sim |\xi _{2}|\sim |\xi _{3}|^{-1}\), \(s\ge \frac{1}{2}-\frac{2}{k}+2\epsilon \); thus, we have
By using (3.17), the Plancherel identity, the Hölder inequality, Lemma 2.11, (2.8)–(2.10), (2.57), (2.58), we have
(4) When \((\xi _{1},\xi _{2},\ldots ,\xi _{k},\xi ,\tau _{1},\tau _{2}, \ldots ,\tau _{k},\tau )\in \Omega _{3}\), we have \(|\xi _{1}|\sim |\xi _{3}|\), then we consider
respectively.
When (3.18) is valid, since \(|\xi _{1}|\sim |\xi _{3}|, |\xi |\le C|\xi _{1}|\), we have
By using (3.20), the Plancherel identity, the Hölder inequality and (2.4), (2.6), (2.7) as well as Lemma 2.5, we have
When (3.19) is valid, we have \(|\xi _{1}|\sim |\xi _{3}|\sim |\xi _{4}|^{-1}\).
We consider \(|\xi |\le a,|\xi |\ge a,\) respectively.
When \(|\xi |\le a,\) we have
By using (3.21), the Plancherel identity, the Hölder inequality, (2.4) and (2.57), we have
When \(|\xi |\ge a,\) we consider
respectively.
When (3.22) is valid, this case can be proved similarly to (3.18).
When (3.23) is valid, we have that \(|\xi _{1}|\sim |\xi _{3}|\sim |\xi _{4}|^{-1}\sim |\xi _{5}|^{-1},\) we consider (3.8), (3.9), respectively.
When (3.8) is valid, since \(|\xi _{1}|\sim |\xi _{3}|\sim |\xi _{4}|^{-1}\sim |\xi _{5}|^{-1}, s\ge \frac{1}{2}-\frac{2}{k}+2\epsilon \), we have
By using (3.24), the Plancherel identity, the Hölder inequality, Lemmas 2.5, 2.11, (2.8) and (2.9), (2.57), we have
When (3.9) is valid, since \(|\xi |\sim |\xi _{k+1}|^{-1}\), \(|\xi _{1}|\sim |\xi _{3}|\sim |\xi _{4}|^{-1}\sim |\xi _{5}|^{-1},\) \(s\ge \frac{1}{2}-\frac{2}{k}+2\epsilon \), we have
By using (3.25), the Plancherel identity, the Hölder inequality, (2.5) and (2.10), (2.58), we have
(5) Case \((\xi _{1},\xi _{2},\ldots ,\xi _{k},\xi ,\tau _{1},\tau _{2}, \ldots ,\tau _{k},\tau )\in \Omega _{4}\), this case can be proved similarly to Case (4).
(6) Case \((\xi _{1},\xi _{2},\ldots ,\xi _{k},\xi ,\tau _{1},\tau _{2}, \ldots ,\tau _{k},\tau )\in \Omega _{5}\), we have \(|\xi _{1}|\sim |\xi _{5}|\), then we consider
respectively.
When (3.26) is valid, we consider \(k=5\), \(k\ge 6,\) respectively.
When \(k=5,\) since \(|\xi _{1}|\sim |\xi _{5}|\), \(s\ge \frac{1}{2}-\frac{2}{k}+2\epsilon \), we have
By using (3.28), the Plancherel identity, the Hölder inequality and (2.4), (2.5) and (2.7), we have
When \(k\ge 6,\) since \(|\xi _{1}|\sim |\xi _{5}|\), \(s\ge \frac{1}{2}-\frac{2}{k}+2\epsilon \), we have
By using (3.29), the Plancherel identity, the Hölder inequality and (2.4), (2.7), Lemma 2.5, we have
When (3.27) is valid, we have \(|\xi _{1}|\sim |\xi _{5}|\sim |\xi _{6}|^{-1}\). If there exists some \(k\in N,7\le k\le k+1\) such that
we can use a proof similar to (3.26) to derive the result, otherwise we have that \(|\xi _{1}|\sim |\xi _{5}|\sim |\xi _{6}|^{-1}\sim |\xi _{k+1}|^{-1}\).
In this case, since \(|\xi _{1}|\sim |\xi _{5}|\sim |\xi _{6}|^{-1}\sim |\xi _{k+1}|^{-1}\), \(s\ge \frac{1}{2}-\frac{2}{k}+2\epsilon \), we have
By using (3.30), the Plancherel identity, the Hölder inequality, (2.8), (2.10), (2.46) and (2.57), we have
(7) Case \((\xi _{1},\xi _{2},\ldots ,\xi _{k},\xi ,\tau _{1}, \tau _{2},\ldots ,\tau _{k},\tau )\in \Omega _{6}\), this case can be proved similarly to \((\xi _{1},\xi _{2},\ldots ,\xi _{k},\xi ,\tau _{1},\tau _{2}, \ldots ,\tau _{k},\tau )\in \Omega _{5}\).
(8) Case \((\xi _{1},\xi _{2},\ldots ,\xi _{k},\xi ,\tau _{1}, \tau _{2},\ldots ,\tau _{k},\tau )\in \Omega _{7}\), we have \(|\xi _{1}|\sim |\xi _{k+1}|\), and then we consider \(|\xi |\le a,|\xi |\ge a\), respectively.
When \(|\xi |\le a,\) we consider (3.8), (3.9), respectively.
When (3.8) is valid, we have
By using (3.31), the Plancherel identity, the Hölder inequality and (2.4), Lemma 2.5, we have
When (3.9) is valid, we have \(|\xi |\sim |\xi _{k+1}|^{-1}\) we consider \(|\sigma |\ge |\xi _{1}|, |\sigma |\le |\xi _{1}|,\) respectively.
When \(|\sigma |\ge |\xi _{1}|,\) we have
By using (3.32), the Plancherel identity, the Hölder inequality and (2.4), we have
When \(|\sigma |\le |\xi _{1}|,\) since \(|\xi _{1}|\sim |\xi _{k+1}|\ge 80ka\), \(|\xi |\sim |\xi _{k+1}|^{-1}, |\xi |\le a\), we have
By using (3.33), the Plancherel identity, the Hölder inequality and (2.4), (2.10), (2.58), we have
When \(|\xi |\ge a,\) since \(|\xi _{1}|\sim |\xi _{k+1}|\ge 80ka\), we have
By using (3.34), the Plancherel identity, the Hölder inequality and (2.4), (2.5), (2.11), we have
We have completed the proof of Lemma 3.1.
Lemma 3.2
Let \(s\ge \frac{1}{2}-\frac{2}{k}+2\epsilon ,k\ge 5\), \(b=\frac{1}{2}+\frac{\epsilon }{24}\) and \(b^{\prime }=-\frac{1}{2}+\frac{\epsilon }{12}\) and \(g=\psi (t)u\). Then, we have
Lemma 3.2 can be proved similarly to Lemma 3.1.
Lemma 3.3
Let \(s\ge \frac{1}{2}-\frac{2}{k}+2\epsilon ,k\ge 5\), \(b=\frac{1}{2}+\frac{\epsilon }{24}\) and \(b^{\prime }=-\frac{1}{2}+\frac{\epsilon }{12}\) and \(g=\psi (t)u\). Then, we have
Proof
Since \(\Vert g\Vert _{{\tilde{X}}_{s,b}}= \Vert g\Vert _{X_{s,b}}+\Vert \partial _{x}^{-1}g\Vert _{X_{s,b}}\), we have
using Lemmas 3.1 and 3.2, we have
We have completed the proof of Lemma 3.3.
4 Proof of Theorem 1.1
Proof
Obviously, (1.1)–(1.2) are equivalent to
For \(u_{0}\in H^{s}(\mathbf{R})\) and \(\delta \in (0,1]\), we define
We define \(B(0,r)=\{u\in X_{s,b}\cap C([-\delta ,\delta ],H^{s}(\mathbf{R})),\Vert u\Vert _{X_{s,b}}\le r:=2C\Vert u_{0}\Vert _{H^{s}(\mathbf{R})}\}\). By using Lemmas 2.1, 3.1 and choosing sufficiently small \(\delta >0\) such that
we have
By a similar calculation, we have
Thus, \(\Gamma \) is a contraction mapping from the closed ball
into itself. From the fixed point theorem and (4.3), we have \(\Gamma (v)=v\). The uniqueness of solution to (4.1) is easily derived from (4.3).
The rest of the local well-posedness results of Theorem 1.1 follow from a standard argument, for instance, see [24].
This completes the proof of Theorem 1.1.
6 Proof of Theorem 1.3
Proof
In this section, inspired by [4, 27, 32, 36], we study the relationship between the solution to (1.1)–(1.2) and the solution to
as \(\gamma \rightarrow 0\).
From (1.1), we have
Multiplying by \(J_{x}^{s}u\) on both sides of (6.3) and integration by parts with respect to x on \(\mathbf{R}\) as well as \(H^{s-1}(\mathbf{R})\hookrightarrow L^{\infty }\) with \(s>\frac{3}{2},\) by using Lemma 2.12, we obtain
Here, \(C_{0}\) is a constant independent of \(\gamma \). Similarly, we obtain
Then, using (6.4) and (6.5), we have
from (6.6), we have
When \(t<\min \left\{ T,\frac{1}{Ck\Vert u_{0}\Vert _{X_{s}}^{k}}\right\} \), where T is the time lifespan of the solution to (1.1)–(1.2) for data in \(X_{s}(\mathbf{R})\) with \(s>\frac{3}{2}\) in Theorem 1.2, by using (6.7), we have
Let \(u:=u^{\gamma }\) and the solution to (1.1). Therefore, \(w:=u-v\) satisfies the equation
Multiplying by w on both sides of (6.9) and integrating by parts with respect to x on \(\mathbf{R}\), we obtain
From (6.10), we have
By using the Gronwall’s inequality and (6.12), we can get
Thus, when \(\gamma \rightarrow 0\) and \(\Vert u_{0}-v_{0}\Vert _{L^{2}}\rightarrow 0\), we have \(\Vert w\Vert _{L^{2}}=\Vert u-v\Vert _{L^{2}}\rightarrow 0.\)
This completes the proof of Theorem 1.3.
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This work is supported by the Young core Teachers program of Henan province under Grant Number 2017GGJS044.
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Yan, X., Yan, W. The Cauchy problem for the generalized Ostrovsky equation with negative dispersion. J. Evol. Equ. 22, 40 (2022). https://doi.org/10.1007/s00028-022-00802-w
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DOI: https://doi.org/10.1007/s00028-022-00802-w