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A new type of solutions for a nonlinear Schrödinger system with \(\chi ^{(2)}\) nonlinearities
Boundary Value Problems volume 2022, Article number: 54 (2022)
Abstract
We are concerned with the question of constructing a new type of solution to the problem with \(\chi ^{(2)}\) nonlinearities
where \(P(x)=P(|x|)\) and \(Q(x)=Q(|x|)\) are positive bounded radial potentials, \(3\leq N<6\), \(\alpha >0\) and \(\alpha >\beta \). Assuming that the potentials \(P(x)\) and \(Q(x)\) satisfy certain conditions, the existence of a new type of solutions is proved.
1 Introduction
This paper deals with the questions of the existence of a new type of solution of the following systems of coupled elliptic equations with \(\chi ^{(2)}\) nonlinearities
where \(P(x)=P(|x|)\) and \(Q(x)=Q(|x|)\) are positive bounded radial potentials, \(3\leq N<6\), \(\alpha >0\) and \(\alpha >\beta \).
The system (1.1) has strongly attracted researchers’ attention and has been extensively studied because it arises from nonlinear optical theory. In the nonlinear optical theory, the following cubic nonlinear Schrödinger equation
is the basic equation that can be used to describe the formation and propagation of optical solutions in Kerr-type materials [6, 15]. Here, the slowly varying envelope of electric field ϕ represents the relative strength, the real-valued parameter r is concerned with the sign of dispersion/diffraction, and χ represents the nonlinearity. z describes the propagation distance coordinate. The Laplacian operator \(\nabla ^{2}\) can either be \(\frac{\partial ^{2}}{\partial \tau ^{2}}\) for temporal solitons, where τ is the normalized retarded time, or \(\nabla ^{2}=\sum_{i=1}^{N}\frac{\partial ^{2}}{\partial x_{i}^{2}}\), where \(x=(x_{1},\ldots ,x_{N})\) is in the direction orthogonal to z. Solitary wave solutions to (1.2) and its generations have been proved in [2, 14].
As the optical material has a \(\chi ^{(2)}\) (i.e., quadratic) nonlinear response instead of a conventional \(\chi ^{(3)}\) material for which the problem (1.2) is based on (see [3, 4]), the nonlinear optical effects such as Second Harmonic Generation were discovered. As is known, the \(\chi ^{(3)}\) nonlinear Schrödinger system is well studied and has been explored by many authors in recent years, one can refer to [1, 7, 9, 10, 12, 13, 18] and the references therein. For the \(\chi ^{(2)}\) nonlinear Schrödinger system, in the case \(\alpha =1\), \(\beta =0\), \(N=1\), Zhao, Zhao and Shi in [22] proved the existence of a ground-state solution for (1.1). Very recently, using the finitely dimensional reduction method, Wang and Zhou in [17] studied the existence of infinitely many nonradial positive synchronized solutions of the system (1.1) under radial potentials satisfying some algebraic decay. Using the same method in [19], Yang and Zhou proved the existence of a single peak solution for (1.1). For more results, we refer the readers to [16, 20, 21] and the references therein.
In this paper, we construct a new type of solutions for the \(\chi ^{(2)}\) nonlinear Schrödinger system (1.1). The new type of solutions that were first introduced by Duan and Musso recently in [8] have polygonal symmetry in the \((x_{1}, x_{2})\)-plane, even symmetry in the \(x_{3}\) direction, and radial symmetry in other variables. Due to the \(\chi ^{(2)}\) nonlinearity that appears in our paper, we need to improve some estimates and give precise computing techniques. To the best of our knowledge, there is no result on such a question in the current the literature.
First, we will give some notations.
Let
and
where k is an integer and 0 is the zero vector in , \(r\in [r_{1} m\ln m,r_{2} m\ln m]\) for some \(r_{2}>r_{1}>0\), \(h\in [h_{1}\frac{1}{m},h_{2}\frac{1}{m}]\) for some \(h_{2}>h_{1}>0\).
It is well known that the following equation
has a unique positive ground state W that satisfies:
By direct computation, we know that \((U,V)=(\mu W,\gamma W)\) solves the following limit system for (1.1):
where \(\mu =\frac{1}{\alpha}\sqrt{\frac{2(\alpha -\beta )}{\alpha}}\), \(\gamma = \frac{1}{\alpha}\).
Remark 1.1
If \((U,V)\) is a solution of the system (1.3), so is \((-U,V)\).
Remark 1.2
From the proposition 2.2 in [17], \((U,V)\) is nondegenerate for system (1.3), which is important in the proof of our result.
For any function \(P(x)>0\), we define the norm of as follows
with the inner product
We define the product space that is denoted by H with the norm
Set
where \(j=1,2,\ldots ,m\) and denote the dot product in .
We see that can be divided into k parts: \(\Omega _{1},\ldots ,\Omega _{k}\). For \(\Omega _{j}\), we divided it into two parts:
We know the interior of \(\Omega _{j}\cap \Omega _{i}\), \(\Omega _{j}^{+}\cap \Omega _{j}^{-} \) are empty sets for \(i\neq j\).
Define
where \(\theta =\arctan \frac{x_{2}}{x_{1}}\).
We define \(H_{Q,s}\) similarly.
Denote
where
In what follows, we make some assumptions:
\((P)\) There exist constants \(a>0\), \(s>1\) and \(\theta >0\), such that as \(r\rightarrow +\infty \),
\((Q)\) There exist constants \(b>0\), \(t>1\) and \(\varepsilon >0\), such that as \(r\rightarrow +\infty \),
In this paper, we always assume
for some \(\alpha ,\beta >0\) small.
Our main result can be stated as follows:
Theorem 1.3
Suppose that \(P(x)\) and \(Q(x)\) satisfy \((P)\) and \((Q)\), \(3\leq N<6\), \(\alpha >0\) and \(\alpha >\beta \), the parameters \((r,h)\) satisfy (1.5). Then, there is an integer \(m_{0}\), such that for any integer \(m\geq m_{0}\), (1.1) has a solution \((u_{m},v_{m})\) of the form
where , \((r_{m},h_{m})\in \Lambda _{m}\) and as \(m\rightarrow +\infty \), \(\|(\varphi _{m},\psi _{m})\|\rightarrow 0\).
Remark 1.4
The results in [22] show that \(N=6\) is a critical dimension, that is to say, the positive solutions do not exist when \(N \geq 6\). At the same time, by the structure of the new type of solution in our paper, the dimension N must be greater than or equal to 3.
Remark 1.5
The solutions of the system (1.1) has a large number of bumps near infinity, which causes the energy to become very large.
2 Finite-dimensional reduction
Define
Set
and
It is standard to see that .
We expand the functional \(K(\varphi ,\psi )\) as follows
where
and
Here, L is a linear operator from to , that satisfies
\(l(\varphi ,\psi )\) is a bounded linear operator defined on , thus there exists such that \(l(\varphi ,\psi )=\langle l_{m},(\varphi ,\psi )\rangle \).
We have the following important results that have been proved in [8].
Lemma 2.1
(Lemma 3.1, [8])
For r, h as parameters in \(\Lambda _{m}\) and any \(\eta \in (0,1]\), there is a constant \(C>0\), such that
and
By the same argument as that of Lemma 2.2 in [8], we can prove:
Lemma 2.2
There exists a constant \(C>0\), independent of m, such that for any \((r,h)\in \Lambda _{m}\),
The following important Proposition can be found in [17], we only need to use the contraction theorem to prove it. Meanwhile, the new type of solution is not weighing on the proof of this Proposition. Hence, we omit it for conciseness.
Proposition 2.3
There exists an integer \(m_{0}>0\), such that for any \(m\geq m_{0}\), there is a unique \(C^{1}\) map: and
Moreover, there is a positive constant C, such that
where \(\tau >0\) is small enough.
Next, we will give the estimate for \(l_{m}\).
Lemma 2.4
There exist constants \(C>0\) independent of m and \(\tau >0\) sufficiently small such that
provided \(m\geq m_{0}\) for some integer \(m_{0}>0\).
Proof
Recall that
By symmetry, we have
Similarly, we can obtain
By using the estimates (3.14) and (3.15) in [8], we obtain
where \(\tau >0\) is sufficiently small.
Similarly, we have
where \(\tau >0\) is sufficiently small.
Since \(U=\frac{\mu}{\gamma} V\), we can estimate
Hence,
□
Lemma 2.5
There holds,
where , , and \(B_{1}>0\) is defined in [8], \(\delta >0\) is sufficiently small.
Proof
Here, we calculate \(I(U_{r,h},V_{r,h})\):
By symmetry and Lemma 3.1 in [8], we have
Analogously,
Using symmetry, we obtain
Also, we have
Inserting (2.12)–(2.15) into (2.11) and by Lemma 3.2 in [8], we have
where , , and \(B_{1}>0\) is defined in [8], \(\delta >0\) is sufficiently small. □
Proof of Theorem 1.3
Let \((\varphi ,\psi )=(\varphi (r,h),\psi (r,h))\) be the map obtained in Proposition 2.3. Define
With a similar argument as used in [5, 11], we can prove that for m large, if \((r,h)\) is a critical point of \(F(r,h)\), then \((U_{r,h}+\varphi ,V_{r,h}+\psi )\) is a critical point of I. Next, we will prove that the function \(F(r,h)\) has a critical point that is an interior point of \(\Lambda _{m}\). It follows from Proposition 2.3, and Lemmas 2.4 and 2.5 that
where \(D=2\gamma (\beta \gamma ^{2}+\frac{3}{2}\alpha \mu ^{2}) B_{1}\), \(E=\gamma (\beta \gamma ^{2}+\frac{3}{2}\alpha \mu ^{2})B_{1}\).
We only prove the Theorem 1.3 for the case \(s< t\), since the other case is similar.
If \(s< t\), then
In [8], we know that the same function \(F(r,h)\) has a maximum point \((r_{m},h_{m})\), which is an interior point of \(\Lambda _{m}\). □
Availability of data and materials
No data were used to support this study.
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The authors would like to thank the referees for their comments that improved the manuscript.
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The authors are partially supported by the Scientific Research and Innovation Team of Hubei Normal University (2019CZ010).
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The idea of this research was introduced by Weiming Liu. All authors contributed to the main results. All authors read and approved the final manuscript.
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Xiong, M., Liu, W. A new type of solutions for a nonlinear Schrödinger system with \(\chi ^{(2)}\) nonlinearities. Bound Value Probl 2022, 54 (2022). https://doi.org/10.1186/s13661-022-01635-9
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DOI: https://doi.org/10.1186/s13661-022-01635-9