Abstract
We consider the following quasilinear Schrödinger equations of the form
where \(N\ge 3,\) \(p>\frac{N+2}{N-2},\) \(\varepsilon >0\) and V(x) is a positive function. By imposing appropriate conditions on V(x), we prove that, for \(\varepsilon =1,\) the existence of infinity many positive solutions with slow decaying \(O(|x|^{-\frac{2}{p-1}})\) at infinity if \(p>\frac{N+2}{N-2}\) and, for \(\varepsilon \) sufficiently small, a positive solution with fast decaying \(O(|x|^{2-N})\) if \(\frac{N+2}{N-2}<p<\frac{3N+2}{N-2}.\) The proofs are based on perturbative approach. To this aim, we also analyze the structure of positive solutions for the zero mass problem.
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1 Introduction
The nonlinear Schrödinger equation
where \(W:\mathbb {R}^{N}\rightarrow \mathbb {R}\) is a given potential, has been introduced in [1,2,3] to study a model of a self-trapped electrons in quadratic or hexagonal lattices (see also [4]). In those references numerical and analytical results have been given.
Here of particular interest is in the existence of standing wave solutions, that is, solutions of type \(z(x,t)=\exp (-iE t)u(x),\) where \(E\in \mathbb {R}.\) Assuming that the amplitude u(x) is positive and vanishing at infinity, it is well known that z satisfies (1.1) if and only if the function u solves the following equation of quasilinear elliptic type
where \(V(x)=W(x)-E\) is the new potential function. In the rest of this paper we will assume that V(x) is a bound and positive function.
Because of the presence of the quasilinear term \(u\triangle u^2,\) we can see that \(p=\frac{3N+2}{N-2}\) is the critical exponent for the existence of solutions from the view of variational methods. For the subcritical case, that is, \(1<p<\frac{3N+2}{N-2},\) construction of solutions to this problem by variational methods has been a hot topic during the last decade. A typical result for the Eq. (1.2) is, up to our knowledge, due to Liu et al. [5]. The idea in [5] is to make a change of variable and reduce the quasilinear problem (1.2) to a semilinear one and the Orlicz space framework is used to prove the existence of positive solutions via the mountain pass theorem. Subsequently, the same method of changing of variable is also used in Colin and Jeanjean [6], but the usual Sobolev space \(H^{1}(\mathbb {R}^{N})\) is used as the working space. Recently, Shen and Wang [7] study the following generalized quasilinear Schrödinger equation:
where \(g^{2}(s)=1+\frac{1}{2}(l(s^2)')^{2}.\) By introducing the variable replacement
and imposing some conditions on V(x), the authors obtain the positive solution for (1.3) with a general function l(s) when h(s) is superlinear and subcritical. But under the condition
the solvability of the Eq. (1.2) with \(1<p<\frac{3N+2}{N-2}\) still remains open.
Subcriticality is a rather essential constraint in the use of many variational methods devised in the literature and many papers [8,9,10,11,12] focused on the subcritical case. Very little is known in the supercritical case since a major technical obstacle in understanding such problems stems from the lack of Sobolev embeddings suitably fit to a weak formulation of this problem. Direct tools of the calculus of variation, very useful in subcritical, and even critical cases, are not appropriate in the supercritical. In the critical case, Liu et al. [5] asked the following open question: are there solutions for (1.2) in the case of \(p=\frac{3N+2}{N-2}?\) However, generally speaking, except some results relate to the critical exponent, see, for instance, [13,14,15,16,17,18,19,20], there are still no conclusive results about the existence of positive solutions for the problem (1.2) with \(p=\frac{3N+2}{N-2}\) or \( p>\frac{3N+2}{N-2}\).
In all the papers mentioned above variational methods are used. In this paper, we shall explore the distinctive nature of this problem for having two critical exponents, one being \(p=\frac{3N+2}{N-2}\) (from the quasilinear term \(u \Delta u^2\)) and the other being \(p=\frac{N+2}{N-2}\) which is \(H^1\)-critical (from the term \(\Delta u\)). We shall concentrate in the problem (1.2) when the exponent p is \(H^{1}\)-supercritical, that is, \(p>\frac{N+2}{N-2},\) (which includes \(p=\frac{3N+2}{N-2}\)), and we establish a new phenomenon from the viewpoint of singular perturbations. Noticing that (1.2) is a quasilinear problem, we adopt the change of variables which enable us to convert the original quasilinear problem (1.2) into a semilinear problem
where \(f(v)=\frac{G^{-1}(v)^{p}}{g(G^{-1}(v))}\) and \(g(s)=\sqrt{1+2s^{2}}.\) Thus, if v is a solution of (1.6), we have \(u=G^{-1}(v)\) is a solution of (1.2).
A solution v to (1.6) is called fast decaying if \( v = O(|x|^{2-N})\) at infinity and slow decaying if \( v>> O(|x|^{2-N})\). Then, to describe our result about the fast and slow decaying solutions, our starting point is the zero mass problem
Applying the change of variables (1.4) again, the quasilinear problem (1.7) can be reduced to the equations of the form
Our first result concerns with the structure of positive radial solutions of the zero mass problem (1.7).
Theorem 1.1
Suppose that \(p>1.\) Then
-
(1)
there exist no fast decaying solutions to the problem (1.7) if \(p\ge \frac{3N+2}{N-2}\) or \(1<p\le \frac{N+2}{N-2};\)
-
(2)
there exist a unique fast decaying radial solution to the problem (1.7) if \(\frac{N+2}{N-2}<p<\frac{3N+2}{N-2};\)
-
(3)
there exist a one-parameter family of slow decaying radial solutions to the problem (1.7) if \(p>\frac{N+2}{N-2}.\)
Remark 1.1
Some cases of the results of Theorem 1.1 are contained in [21, 22]. More specifically, similarly to the standard Liouville theorem, if \(1<p<\frac{N+2}{N-2},\) the authors proved the nonexistence results of fast decaying solutions to (1.7) (see [21]). In [22], the authors showed the existence of a unique fast decaying solution and a one-parameter family of slow decaying solutions to (1.7) if \(\frac{N+2}{N-2}<p<\frac{3N+2}{N-2}\) via the results introduced in [23]. Moreover, the authors in [22] also pointed out that they did not know whether there are solutions for the Eq. (1.7) with \(p=\frac{N+2}{N-2}.\) Particularly, in Theorem 1.1, we draw the definite conclusion about this case by using the Pohozeav identity.
Theorem 1.1 shows that the structure of solutions changes along with the variations of the power p and we remark that the solvability of the Eq. (1.7) heavily depends on the power p. Let us explain the main reason for such a rich phenomenon. On one hand, \(f(v)\rightarrow v^{p}\) as \(v\rightarrow 0.\) On the other hand, \(f(v)\rightarrow 2^{\frac{p-3}{4}}v^{\frac{p-1}{2}}\) as \(v\rightarrow +\infty .\) That is, the nonlinearity f is not a pure power of v but f has both \(H^{1}\)-subcritical and \(H^{1}\)-supercritical growth in \(v>0.\) In [24], the authors consider a similar model
where \(1<p<\frac{N+2}{N-2}<q\) and give an almost complete description for the structure of positive radial solutions by a shooting argument.
The following result is about the fast decaying solutions of the Eq. (1.2).
Theorem 1.2
Assume that
hold. Then for \(\varepsilon \) sufficiently small the problem (1.2) has a positive fast decaying solution if \(\frac{N+2}{N-2}<p<\frac{3N+2}{N-2}.\)
Compared with Theorem 1.1, it is natural to ask whether the nonexistence of a fast decaying solution remains true for (1.2) when \(p\ge \frac{3N+2}{N-2}.\) This may be in general a difficult question to answer if no other conditions imposed on V(x). For the special case \(x\cdot \nabla V(x)+2V(x)\ge 0,\) the authors in [25] show the nonexistence results of fast decaying solutions by a Pohozeav identity for the Eq. (1.2) in the case \(p\ge \frac{3N+2}{N-2}\) and \(\varepsilon =1.\)
Our final result concerns the existence of slow decaying solutions.
Theorem 1.3
Assume that \(\varepsilon =1.\) Then the problem (1.2) has a continuum of solutions \(u_{\lambda }(x)\) such that \(\underset{\lambda \rightarrow 0}{\lim }u_{\lambda }(x)=0\) uniformly in \(\mathbb {R}^{N}\) provided that either \(N\ge 4,\) \(p>\frac{N+1}{N-3}\) and the condition (1.9) holds or \(N\ge 3,\) \(\frac{N+2}{N-2}<p< \frac{N+1}{N-3}\) and there exist \(C>0,\) \(\mu >N\) such that
Remark 1.2
In this theorem, we answer the question raised in [5] for \(p=\frac{3N+2}{N-2}.\)
The proofs of Theorems 1.2 and 1.3 are based on perturbative approach, introduced by Dávila et al. [26,27,28,29] in the study of fast and slow decaying solutions for second order or nonlinear Schrödinger equations and exterior domain problems. Some of our ideas are motivated from these papers.
In the fast-decaying case, we consider the problem (1.6) as small perturbation of the problem (1.8) when \(\varepsilon >0\) is sufficiently small. For a point \(\xi \in \mathbb {R}^{N}\) used as the reference origin, the function \(v_{f}(x+\xi )\) is considered as an initial approximation, where \(v_{f}\) is a solution of (1.8). This function will constitute a good approximation for small \(\varepsilon .\) By adjusting \(\xi ,\) we prove that the solutions we want can be achieved.
As for the slow decaying solution of the Eq. (1.2), we set \(\varepsilon =1\) and consider the equation with a parameter \(\lambda \) by means of replacing the variable v in the Eq. (1.6) by \(\lambda ^{\frac{2}{p-1}}v(\lambda x+\xi )\)
where \(\lambda >0,\) \(\xi \in \mathbb {R}^{N}\) and \(V_{\lambda }(x)=\lambda ^{-2}V(\frac{x-\xi }{\lambda }).\) We observe that \(\lambda ^{-\frac{2}{p-1}}\frac{G^{-1}(\lambda ^{\frac{2}{p-1}}v)}{g(G^{-1}(\lambda ^{\frac{2}{p-1}}v))}\rightarrow v\) and \(\lambda ^{-\frac{2p}{p-1}}f(\lambda ^{\frac{2}{p-1}}v)\rightarrow v^{p}\) as \(\lambda \rightarrow 0.\) Thus the problem may be regarded as small perturbation of the problem
when \(\lambda >0\) is sufficiently small. Consequently, infinitely many positive solutions with slow decaying \(O(|x|^{-\frac{2}{p-1}})\) at infinity can be constructed similar to the perturbative procedure introduced by Dávila et al. [26].
In this paper, we make use of the following notations: the symbol C denotes a positive constant (possibly different) independent with \(\lambda .\) \(A\sim B\) if and only if there exist two positive constants a, b such that \(aA\le B\le bA.\) \( v_f\) denotes the unique fast decaying solution of (1.8).
2 Proof of Theorem 1.1
In this section, we analyze the structure of positive decaying solutions of (1.7). We first prove the nonexistence of fast-decaying solutions for \(p\le \frac{N+2}{N-2}\) or \(p\ge \frac{3N+2}{N-2}\) by using the Pohozaev identity. Then we show the existence of the fast decaying solution for (1.7) by using the classical Berestycki–Lions condition in [30] for \(\frac{N+2}{N-2}<p<\frac{3N+2}{N-2}.\) Finally we use a perturbative approach to prove the existence of a family of slow-decaying solutions for \(p>\frac{N+2}{N-2}.\)
To prove the nonexistence results for the Eq. (1.8), we recall the following Pohozaev identity.
Lemma 2.1
(Pohozaev identity) Suppose \(F(x,u,r)\in C^{1}(\mathbb {R}^{N}\times \mathbb {R}\times \mathbb {R}^{N})\) satisfies
where
and
Then, if \(F(x,u,\nabla u), x\cdot F_{x}(x,u,\nabla u)\) and \(F_{r}(x,u,\nabla u)\cdot \nabla u\in L^{1}(\mathbb {R}^{N}),\) there holds the following identity
We omit the proof of this lemma, since it can be mainly found in [31].
To present the Pohozaev identity associated to (1.7), we rewrite the Eq. (1.7) as
Thus, the integrands in (2.2) can be expressed as
and
Consequently, we achieve the following lemma based on Lemma 2.1 under the conditions \(|\nabla u|^2,\) \(u^2|\nabla u|^2\) and \(u^{p+1}\in L^{1}(\mathbb {R}^{N}).\)
Lemma 2.2
Suppose that \(u\in C^{2}(\mathbb {R}^{N})\) is a solution of (1.7). Then
if \(|\nabla u|^2,\) \(u^2|\nabla u|^2\) and \(u^{p+1}\in L^{1}(\mathbb {R}^{N}).\)
Equation (1.7) can be rewritten as
where \(g^2(u)=1+2u^2.\) By Lemma 2.2, the Pohozaev identity associated to (2.5) is
On the other hand, the classical solution \(u\in D^{1,2}(\mathbb {R}^{N})\) of (2.5) satisfies
By taking \(\phi =u,\) we achieve
Consequently, combining (2.6) and (2.7), we have
If \(p\ge \frac{3N+2}{N-2},\) then \((N-2)-\frac{4N}{p+1}\ge 0\) and \(\frac{N-2}{2}-\frac{N}{p+1}>0.\) Therefore, (2.8) implies that \(u=0\) under this situation. Similarly, if \(p\le \frac{N+2}{N-2},\) it follows that \((N-2)-\frac{4N}{p+1}< 0\) and \(\frac{N-2}{2}-\frac{N}{p+1}\le 0.\) Thus, (2.8) also shows that \(u=0.\) So there are no nonzero solutions for (1.7) if \(p\le \frac{N+2}{N-2}\) or \(p\ge \frac{3N+2}{N-2}.\)
This proves (1) of Theorem 1.1.
Next we prove the existence of fast decaying solutions to (1.7). By the change of variable \(u=G^{-1}(v)\) we only need to consider (1.8). To this end we recall the following classical proposition by Berestycki and Lions [30].
Proposition 2.1
Suppose that the following assumptions hold:
-
(F-1)
\(f(0)=0\) and \( \underset{s\rightarrow 0^{+}}{{\overline{\lim }}}\frac{f(s)}{s^{l}}\le 0,\) where \(l=\frac{N+2}{N-2};\)
-
(F-2)
There exists \(\zeta >0\) such that \(F(\zeta )>0,\) where \(F(\zeta )=\int _{0}^{\zeta }f(s)\text{ d }s;\)
-
(F-3)
Let \(\zeta _{0}=\inf \left\{ \zeta : \zeta>0,\ F(\zeta )>0\right\} .\) If \(f(s)>0\) for all \(s>\zeta _{0},\) then \(\underset{s\rightarrow +\infty }{\lim }\frac{f(s)}{s^{l}}=0.\)
Then the problem (1.8) has a positive, spherically symmetric and decreasing (with r) solution v such that \(v\in D^{1,2}(\mathbb {R}^{N})\cap C^{2}(\mathbb {R}^{N}).\)
We now show that f(s) satisfies the conditions (F-1)–(F-3) in Proposition 2.1.
By the definition of f(s), we know that (F-2) is trivial. Noticing that \(\underset{s\rightarrow 0}{\lim }\frac{G^{-1}(s)}{s}=1,\) we have
which shows that f(s) satisfies the condition (F-1).
To verify the condition (F-3), it suffices to show that
since \(\zeta _{0}=0\) and \(f(s)>0\) for all \(s>0.\) Combining the fact \(\underset{s\rightarrow +\infty }{\lim }\frac{G^{-1}(s)}{\sqrt{s}}=2^{\frac{1}{4}},\) we deduce that
This proves (2) of Theorem 1.1.
Finally we prove (3) of Theorem 1.1. To prove the existence of slow decaying solutions, since we are considering the autonomous case, that is, \(V(x)\equiv 0,\) we can restrict to the radially symmetric case. For this reason, we take \(v(x)=v(r),\) where \(r=|x|.\)
We first consider the problem in the entire space
It is well known that this problem possesses a unique positive symmetric solution w(|x|) whenever \(p>\frac{N+2}{N-2}.\) Then all radial solutions to this problem defined in \(\mathbb {R}^{N}\) can be expressed as
and, at a main order, one has
which implies that this behavior is actually common to all solutions \(w_{\lambda }(r).\)
Since the problem (1.8) does not carry any parameter explicitly, for \(\lambda >0,\) we can make parameters appear by means of replacing the variable v in the equation by \(\lambda ^{\frac{2}{p-1}}v(\lambda |x|),\) in such a way the problem (1.8) becomes
Then, jointly with the properties of \(G^{-1}(v)=v+o(1)\) and \(g(G^{-1}(v))=1+o(1)\) as \(v\rightarrow 0,\) if v is uniformly bounded, we observe that \(\lambda ^{-\frac{2p}{p-1}}f(\lambda ^{\frac{2}{p-1}}v)\rightarrow v^{p}\) as \(\lambda \rightarrow 0.\) Thus the problem may be regarded as small perturbation of the problem
when \(\lambda >0\) is sufficiently small. Consequently, a positive solution with slow decaying \(O(|x|^{-\frac{2}{p-1}})\) at infinity can be constructed by asymptotic analysis and Liapunov-Schmidt reduction method. To be more specific, the idea of the proof of Theorem 1.1-(3) is, for \(\lambda \) small, to consider the function \(\lambda ^{\frac{2}{p-1}}w(\lambda |x|)\) as an initial approximation. This scaling will constitute a good approximation under our situations for \(\lambda \) sufficiently small. Then, by a classical fixed point argument for contraction mappings, we prove that (2.9) possesses solutions as desired. Similar idea has been used in [26, 28].
Under appropriate norms
and
where \(\sigma >0,\) we first consider the solvability of the linear problem
and thus we need the following lemma which is Lemma A. 1 proved by Dávila et al. [26].
Lemma 2.3
Assume \(0<\sigma <N-2\) and \(p> \frac{N+2}{N-2}.\) Then there exists a constant \(C>0\) such that for any h satisfying \(\Vert h\Vert _{**}<+\infty ,\) Eq. (2.12) has a solution \(\phi =\mathcal {T}(h)\) such that \(\mathcal {T}\) define a linear map and
Let us look for a solution to (2.9) of the form \(v=w+\phi ,\) which yields the following equation for \(\phi =\phi (r)\)
where
and
We first estimate the error \(\Vert S(w)\Vert _{**}\) of the approximate solution. The fact
and the properties of the change of variables (1.4) show that, for \(C_{p}>0,\)
Thus, it follows that
We then conclude
On the other hand, recalling that \(w(x)\le C (1+ |x|)^{-\frac{2}{p-1}}\ \text{ for }\ x\in \mathbb {R}^{N},\) we obtain
From (2.14) and (2.15), we have
In what follows, the proof relies on the contraction mapping theorem. We observe that \(\phi \) solves (2.13) if and only if \(\phi \) is a fixed point for the operator
where \(\mathcal {T}\) is introduced in Lemma 2.3. That is to say, \(\phi \) solves (2.13) if and only if \(\phi \) is a fixed point for the operator
We define
and we will prove that \(\mathcal {A}\) has a fixed point in \(\Sigma .\)
For any \(\phi \in \Sigma \) and \(\sigma \in \left( 0,\min \left\{ 2,\frac{2}{p-1}\right\} \right) ,\) according to the arguments given in [26], we have
since
Therefore, combining (2.16), (2.17) and Lemma 2.3, it follows that
which implies that \(\mathcal {A}(\Sigma )\subset \Sigma .\)
We still have to prove that \(\mathcal {A}\) is a contraction mapping in \(\Sigma .\) Let us take \(\phi _{1},\phi _{2}\in \Sigma .\) Then we have
Moreover, noting that
we have the estimate
for suitable small \(\lambda .\) This means that \(\mathcal {A}\) is a contraction mapping from \(\Sigma \) into itself, and hence a fixed point \(\phi \) in this region indeed exists. So the function \(v_{\lambda }(|x|):=\lambda ^{\frac{2}{p-1}}(w(\lambda |x|)+\phi (\lambda |x|))\) is a continuum solutions of (2.13) satisfying \(\underset{\lambda \rightarrow 0}{\lim } v_{\lambda }(|x|)=0\) uniformly in \(\mathbb {R}^{N}\) and \(u_{\lambda }(|x|)=G^{-1}(v_{\lambda }(|x|))\) is our desired solution. This complete the proof of Theorem 1.1.
3 Proof of Theorem 1.2
In this section, we will construct a fast decaying solution to the problem (1.2) when \(\frac{N+2}{N-2}<p<\frac{3N+2}{N-2}\) by the reduction method. The idea of the proof of Theorem 1.2 is, for \(\xi \in \mathbb {R}^{N}\) and \(\varepsilon \) small, to consider the function \(v_{f}(x+\xi )\) as an initial approximation, where \(v_{f}(x)\) is the unique positive radial solution of the zero mass problem (1.7) stated in Theorem 1.1. These functions will constitute good approximations under our situations for suitable \(\xi \in \mathbb {R}^{N}\) and \(\varepsilon \) sufficiently small. Then, by adjusting \(\xi ,\) we prove that (1.2) possesses a solution as desired.
At the beginning, we state some notations which will be used in the following. We consider the initial value problem
where \(f(s)=\frac{G^{-1}(s)^{p}}{g(G^{-1}(s))}.\) By Theorem 1.1, there exists a unique \(d^{*}>0\) such that the corresponding solution \(v_{f}(r;d^{*})\) is the unique positive fast decaying solution. Moreover, \(z_{0}(r):=\frac{\partial v_{f}}{\partial d}(r;d^{*}) \) satisfies the following initial value problem
Then by Lemma 4.4 in [22], we have that \(v_{f}\) is non-degenerate in \(D_r^{1,2}(\mathbb {R}^{N})\)–radial functions in \( D^{1,2}\). Our next lemma shows that it is nondegenerate in the class of bounded functions. Let \(Z_{i}=\frac{\partial v_{f}}{\partial x_{i}}\) for \(1\le i\le N.\) Then we have the following result.
Lemma 3.1
If \(\phi \) satisfies \(|\phi |\le C\) and
then \(\phi \in W=\text{ Span }\left\{ Z_{1},Z_{2},\ldots ,Z_{n}\right\} .\)
Proof
If \(\phi \) is bounded and satisfies (3.3), by bootstrapping, we achieve \(\phi (x)=O(|x|^{2-N})\) as \(|x|\rightarrow +\infty .\) Expanding \(\phi \) as
we see that \(\phi _{k}\) is a solution of
For mode 0, noticing that \(\lambda _{0}=0,\) we know \(\phi _{0}(r)\) is a solution of (3.4) and, by Lemma 4.2 in [22], \(\phi _{0}(r)\) satisfies
where \(\lambda ^*={\left\{ \begin{array}{ll}\frac{N-1}{2}\ \text{ if }\ N\ge 4;\\ \frac{1}{2}\ \ \ \ \ \text{ if }\ N=3.\end{array}\right. }\) Thus, if \(\phi _{0}(r)\in D^{1,2}_{r} (\mathbb {R}^{N})\), we conclude that
which is a contradiction. For mode k with \(k>1,\) according to Lemma A. 3 in [26], we conclude that the solution \(\phi _{k}\) to (3.4) is zero by the maximum principle. Consequently, jointly with the nondegeneracy in radial class, we have
\(\square \)
We introduce appropriate norms
and
where \(<\cdot >:=\left( 1+|\cdot |^{2}\right) ^{\frac{1}{2}}\) and \(0<\sigma < N-2.\) We first solve the linear problem
Lemma 3.2
Let \(\Lambda >0\) and \(|\xi |\le \Lambda .\) Assume \(\frac{N+2}{N-2}<p<\frac{3N+2}{N-2}\) and \(\sigma <N-2.\) Then there is a linear map \((\phi ,c_{1},\ldots ,c_{N})=\mathcal {T}(h)\) defined whenever \(\Vert h\Vert _{**,\xi }<\infty \) such that \((\phi ,c_{1},\ldots ,c_{N})\) satisfies (3.7) and
Moreover, \(c_{i}=0\) for all \(1 \le i\le N\) if and only if
Proof
We will divide the proof into two steps.
Step 1. A priori estimate
By taking \(h=h^{(1)}+h^{(2)}\) in (3.7), where \(h^{(1)}\in W_{1}=\left\{ f'(v_{f})Z_{1},f'(v_{f})Z_{2},\ldots , f'(v_{f})Z_{N}\right\} \) and \(h^{(2)}\in W_{1}^{\bot },\) we have
If we take \(h^{(1)}=-\sum _{i=1}^{N}c_{i}f'(v_{f})Z_{i},\) that is,
it follows from (3.10) that
and \(c_{i}=0\) for all \(1\le i\le N\) if and only if
So, in what follows, we consider
We first prove the priori estimates (3.8) by using the contradiction argument. Suppose that there exist \(\phi _{n},\) \(h^{(2)}_{n}\) such that \(\Vert \phi _{n}\Vert _{*,\xi }=1\) and \(\Vert h^{(2)}_{n}\Vert _{**,\xi }=o(1)\) as \(n\rightarrow +\infty .\) By the definition of \(\Vert \phi _{n}\Vert _{*,\xi },\) we can take \(x_{n}\in \mathbb {R}^{N}\) with the property
Then, we again have to distinguish two possibilities. Along a subsequence, it follows that \(x_{n}\rightarrow x_{0}\in \mathbb {R}^{N}\) or \(|x_{n}|\rightarrow +\infty .\)
If \(x_{n}\rightarrow x_{0},\) standard elliptic estimates show that \(\phi _{n}\rightarrow \phi \) uniformly on compact sets of \(\mathbb {R}^{N}.\) Moreover, \(\phi \) is a solution to (3.13) with \(h^{(2)}=0\) satisfying
and \(|\phi (x)|<+\infty .\) Thus Lemma 3.1 shows that
Then the facts \(\int _{\mathbb {R}^{N}}\nabla \phi \cdot \nabla Z_{i}=0\) for \(i=1,2,\ldots ,N\) show that \(\nabla \phi =0.\) We achieve a contradiction to (3.15) since \(\underset{|x|\rightarrow +\infty }{\lim }\phi (x)=0.\)
If \(x_{n}\rightarrow +\infty ,\) We consider \({\tilde{\phi }}_{n}(y)=|x_{n}|^{\sigma }\phi _{n}(|x_{n}|y+x_{n}+\xi )\) and observe that \({\tilde{\phi }}_{n}\) satisfies
where \(v_{f,n}(y)=v_{f}(|x_{n}|y+x_{n}+\xi )\) and \({\tilde{h}}^{(2)}_{n}(y)=|x_{n}|^{2+\sigma }h_{n}^{(2)}(|x_{n}|y+x_{n}+\xi ).\) Noticing that \(\Vert \phi _{n}\Vert _{*,\xi }=1,\) we have
where \({\hat{x}}_{n}:=\frac{x_{n}}{|x_{n}|}.\) So \(\tilde{\phi }_{n}\) is uniformly bounded on compact sets of \(\mathbb {R}^{N}{\setminus } \left\{ -{\hat{x}}_{n}\right\} .\) Similarly, considering that
we obtain \({\tilde{h}}^{(2)}_{n}\rightarrow 0\) uniformly on compact sets of \(\mathbb {R}^{N}{\setminus } \left\{ -{\hat{x}}_{n}\right\} \) as \(n\rightarrow +\infty .\) Thus, by elliptic estimates, we have \(\tilde{\phi }_{n}\rightarrow \tilde{\phi }\) uniformly on compact sets of \(\mathbb {R}^{N}{\setminus } \left\{ {\hat{e}}\right\} \) and \(\tilde{\phi }\) satisfies
where \(\hat{e}=-\underset{n\rightarrow +\infty }{\lim }\frac{x_{n}}{|x_{n}|}.\) By the maximum principle, we conclude that \(\tilde{\phi }=0\) which is impossible since \(\tilde{\phi }\left( -\hat{e}\right) \ne 0.\)
Step 2. Existence
We first want to solve (3.7) on a bounded domain \(B_{R}(\xi ).\) Let us consider the subspace
Then, according the arguments in [32], finding solution to (3.7) in this case is equivalent to finding \(\phi \in X\) such that
Now, for h satisfying \(\Vert h\Vert _{**,\xi }<+\infty ,\) let us denote by \(\phi =A(h)\) the unique solution of the problem
Thus, (3.17) can be written as
and, by the compactness of Sobolev’s embedding, the map \(\phi \rightarrow f'(v_{f})\phi \) is compact.
Hence, we conclude the existence of the solution by the Fredholm alternative since the priori estimate (3.8) implies that the only solution of this equation is \(\phi =0\) when \(h=0.\) Finally, thanks to the priori estimate again, we can let \(R\rightarrow +\infty \) and obtain the existence in the whole space. \(\square \)
Now we begin to prove Theorem 1.2. We look for a solution of the form \(v=v_{f}+\phi \) to the Eq. (1.6) and thus acieve the following equation for \(\phi \)
where
and
However, the problem (3.18) may not be solvable under our situation unless \(\xi \) can be chosen in a very special way. So instead of solving (3.18), we consider the following projected problem
where \(c_{i}\) are constants.
For \(\frac{2}{p-1}<\sigma <N-2,\) we first estimate the error \(\Vert E(v_{f})\Vert _{**,\xi }\) of the approximate solution \(v_{f}.\) Considering that
and
we have
In what follows, by applying the Banach fixed point theorem, we can prove that (3.19) is indeed solvable and achieve a solution \((\phi _{\varepsilon },c_{1}, \ldots ,c_{N}).\) We then obtain a solution of the problem (3.18) if \(c_{i}=0\) for all \(i=1,2,\ldots ,N.\)
Based on the description of Lemma 3.2, solving (3.19) reduces now to a fixed point problem. Namely, we need to find a fixed point for the map
Here, we will restrict \(\phi \) to be small enough such that the function \(v_{f}+\phi \) is always positive and we define the set
We now prove that \(\mathcal {A}\) has a fixed point in \(\Theta .\)
For any \((\phi ,c_{1},c_{2},\ldots ,c_{N} )\in \Theta ,\) we first estimate \(M(\phi ).\) Note that
We have
and then
To estimate \(F(\phi ),\) we need the following fact: if \(1<p<2,\) then
Indeed, since
we have
Then, noticing that \(|s_{1}-s_{2}|\le 1,\) we have
since
where \(s_{12}\) belongs to the segment jointing \(s_{1}\) and \(s_{2}.\) On the other hand, by a similar strategy as the proof of the inequality (3.23), we conclude that
and thus show the inequality (3.21).
Since \(\phi \) is small, based on the fact (3.21), we observe that
where \(v_{1}\) lies in the segment jointing \(v_{f},\) \(v_{f}+\phi \) and \(v_{2}=tv_{f}+(1-t)v_{1}\) with \(t\in [0,1].\) Thus, jointly with the fact \(|v_{2}|\le C (1+|x|)^{-\sigma }\) for all \(x\in \mathbb {R}^{N},\) we have
where \(\gamma =\min \left\{ 2,p\right\} .\)
Therefore, by (3.20) and (3.25), jointly with Lemma 3.2, it follows that
which shows \(\mathcal {A}(\Theta )\subset \Theta .\)
We still have to prove that \(\mathcal {A}\) is a contraction mapping in \(\Theta .\) If we take
then we have
To estimate \(\Vert M(\phi _{1})-M(\phi _{2})\Vert _{**,\xi },\) we note that
where \({\bar{\phi }}\) lies in the segment joining \(\phi _{1}\) and \(\phi _{2}.\) Moreover, a direct calculation shows
Then,
Thus, we have
Now we estimate \(\Vert F(\phi _{1})-F(\phi _{2})\Vert _{**,\xi }.\) We note that
where \({\bar{\phi }}\) lies in the segment joining \(\phi _{1}\) and \(\phi _{2}.\) Moreover,
where \(v_{1}=tv_{f}+(1-t)(v_{f}+\phi )\) with \(t\in [0,1].\) Then, similarly as the proof of (3.25), we have
Thus, under our situation, combining (3.27), (3.31) and (3.34), we have that \(\mathcal {A}\) is a contraction mapping in \(\Theta \) and hence there indeed exists a fixed point \((\phi _{\varepsilon },c_{1},c_{2},\ldots ,c_{N}).\)
In what follows of this section, we will complete the proof of Theorem 1.2.
We have found a solution \((\phi _{\varepsilon },c_{1},c_{2},\ldots ,c_{N})\) to (3.19) satisfying
To prove the result contained in Theorem 1.2, it suffices to show that the point \(\xi \) can be adjust so that the constants \(c_{1},c_{2},\ldots ,c_{N}\) are all contemporarily equal to zero. Combining Lemma 3.2, we only need to show
We first define
The subordinate terms in (3.36) are \(\int _{\mathbb {R}^{N}}F(\phi _{\varepsilon })\frac{\partial v_{f}}{\partial y_{j}} \) and \(\int _{\mathbb {R}^{N}}M(\phi _{\varepsilon })\frac{\partial v_{f}}{\partial y_{j}} .\) Indeed, we have the following estimates
and
Noticing that there exist \(k_{0}\in (0,1)\) and \(k_{1}>1\) such that \(k_{0}v_{f}\le \frac{G^{-1}(v_{f})}{g(G^{-1}(v_{f}))}\le k_{1}v_{f},\) the dominant term in (3.36) satisfies
Combining (3.37)–(3.39), we achieve
Thus, if we set \(G(\xi )=\int _{\mathbb {R}^{N}}v_{f}^2V(y-\xi ),\) then \(G(0)>0\) and \(\underset{|x|\rightarrow +\infty }{\lim }G(\xi )=0.\) This implies that G attains a global maximum point \(\xi _{0}\in B_{M}(0)\) for some \(M>0.\) By the definition of stable critical point [33], G has a stable critical point in \(B_{M}(0)\) and as a result, we deduce that, for \(\varepsilon \) small, \(F(\varepsilon ,\xi )=(F_{1}(\varepsilon ,\xi ),F_{2}(\varepsilon ,\xi ),\ldots , F_{N}(\varepsilon ,\xi ))\) has a zero point in \(B_{M}(0).\) Consequently, \(c_{j}=0\) for \(j=1,2,\ldots ,N.\)
4 Proof of Theorem 1.3
In this section, we will construct slow decaying solutions to the problem (1.2) with \(\varepsilon =1.\) The results of Theorem 1.3 are based on a suitable linear theory devised for the linearized operator associated to the Eq. (1.2) at \(u=w\) in the entire space \(\mathbb {R}^{N}\) and in the application of perturbation arguments. We consider w as an approximation for a solution of (1.2), provided that \(\lambda >0\) is chosen small enough. To this aim, we need to know the solvability of the operator \(\triangle -V_{\lambda }+pw^{p-1}\) in suitable weighted \(L^{\infty }\) space.
Let
where \(\eta \in C_{0}^{\infty }(\mathbb {R}^{N})\) satisfies \(0\le \eta \le 1.\) Moreover, \(\eta (x)=1\) if \(|x|\le R_{0}\) and \(\eta (x)=0\) if \(|x|\ge R_{0}+1\) for a fixed number \(R_{0}>0\) large enough.
Under appropriate norms
and
where \(\sigma >0\) and \(\xi \in \mathbb {R}^{N},\) we first consider the solvability of the linear problem
and thus we need the following lemma which is proved by Dávila et al. [26].
Lemma 4.1
Let \(|\xi |\le \Lambda .\) Suppose V satisfies (1.9) and \(\Vert h\Vert _{**,\xi }<\infty .\) Then, for \(\lambda >0\) sufficiently small,
-
(1)
if \(N\ge 4,\) \(p>\frac{N+1}{N-3},\) Eq. (4.3) with \(c_{i}=0\) for \(1\le i\le N\) and \(\xi =0\) has a solution \(\phi =\mathcal {T}_{\lambda }(h)\) which depends linearly on h and there exist a constant C independent with \(\lambda \) such that
$$\begin{aligned} \Vert \mathcal {T}_{\lambda }(h)\Vert _{*,0}\le C\Vert h\Vert _{**,0}; \end{aligned}$$ -
(2)
if \(N\ge 3,\) \(\frac{N+2}{N-2}<p< \frac{N+1}{N-3}\) and V also satisfies (1.10), Eq. (4.3) has a solution \((\phi ,c_{1},c_{2},\ldots ,c_{N})=\mathcal {T}_{\lambda }(h)\) which depends linearly on h and there exist a constant C independent with \(\lambda \) such that
$$\begin{aligned} \Vert \phi \Vert _{*,\xi }+\underset{1\le i\le N}{\max }|c_{i}|\le C\Vert h\Vert _{**,\xi }. \end{aligned}$$Moreover, \(c_{i}=0\) for all \(1\le i\le N\) if and only if
$$\begin{aligned} \int _{\mathbb {R}^{N}}h\frac{\partial w}{\partial x_{i}}=0\ \text{ for }\ 1\le N\le N. \end{aligned}$$(4.4)
Based on Lemma 4.1, we can prove Theorem 1.3. We look for a solution of the form \(v=w+\phi \) to the Eq. (1.11) and, for S(w), \(N(\phi )\) defined in Sect. 2 and \(l(s):=\frac{G^{-1}(s)}{g(G^{-1}(s))}\), we achieve the following equation
where
and
The case \(p>\frac{N+1}{N-3}\)
In this case, we rescale v(x) as \(\lambda ^{\frac{2}{p-1}}v(\lambda x),\) that is, \(\xi =0\) in the previous paragraph. Computations show that
According to the arguments in [26], we know
Thus, for \(\sigma \in \left( 0,\min \left\{ 2,\frac{2}{p-1}\right\} \right) ,\) the error of the approximate solution in the norm (4.2) is
where \(\rho (\lambda ):=\lambda ^{\frac{4}{p-1}}+\delta (\lambda ).\) Consequently, for the operator \(\mathcal {A}_{\lambda }(\phi ):=\mathcal {T}_{\lambda }(S_{1}(w)+N(\phi )+P(\phi )),\) where \(\mathcal {T}_{\lambda }\) is given in Lemma 4.1-(1), we can use the contraction mapping theorem on
and we will prove that \(\mathcal {A}_{\lambda }\) has a fixed point in \(\Sigma _{\lambda }.\)
For any \(\phi \in \Sigma _{\lambda },\) we first give the estimate of \(\Vert P(\phi )\Vert _{**,0}.\) We observe that, for a number \(C_{3}>0,\)
Thus, we have
On the other hand, combining
and
we have
Consequently, combining (4.8) and (4.11), we have
Thus, jointly with the estimate of \(\Vert N(\phi )\Vert _{**,0}\) in Sect. 2, we conclude
That is, \(\mathcal {A}_{\lambda }(\Sigma _{\lambda })\subset \Sigma _{\lambda }.\)
For any \(\phi _{1},\phi _{2}\in \Sigma _{\lambda },\) we want to estimate \(\Vert P(\phi _{1})-P(\phi _{2})\Vert _{**,0}.\) We note that
where \({\bar{\phi }}\) lies in the segment joining \(\phi _{1}\) and \(\phi _{2}.\) Then, it follows that
and
Thus, we have
Moreover, a direct calculation shows
To go a step further, based on the arguments in the previous paragraph, we conclude that
Consequently, combining (4.14) and (4.16), it follows that
for \(\lambda \) sufficiently small.
It is straightforward to show that
since we can achieve that
according to Sect. 2 for \(\lambda \) sufficiently small. This means that \(\mathcal {A}_{\lambda }\) is a contraction mapping from \(\Sigma _{\lambda }\) into itself and hence a fixed point \(\phi _{\lambda }\) indeed exists. So the function \(v_{\lambda }(x):=\lambda ^{\frac{2}{p-1}}(w(\lambda x)+\phi _{\lambda }(\lambda x))\) is a continuum solutions of (1.11) satisfying \(\lim \nolimits _{\lambda \rightarrow 0} v_{\lambda }(x)=0\) uniformly in \(\mathbb {R}^{N}\) and \(u_{\lambda }(x)=G^{-1}(v_{\lambda }(x))\) is our desired solution to (1.2).
The case \(\frac{N+2}{N-2}<p<\frac{N+1}{N-3}\)
In this case, the problem (4.5) may not be solvable under our situation unless \(\xi \) is chosen in a very special way. So, instead of solving (4.5), we consider the following projected problem
where \(c_{i}\) are constants. Moreover, we will slightly change the previous definition of the norms as
and
Just as the case \(p>\frac{N+1}{N-3},\) we can prove that (4.19) is indeed solvable and achieve a solution \((\phi (\lambda ,\xi ),c_{1}(\lambda ,\xi ),c_{2}(\lambda ,\xi ),\ldots ,c_{N}(\lambda ,\xi )).\) We then obtain a solution of the problem (4.5) if \(c_{i}(\lambda ,\xi )=0\) for all \(i=1,2,\ldots ,N.\)
Here, we also fix \(\sigma \in \left( 0,\min \left\{ 2,\frac{2}{p-1}\right\} \right) \) and find the error of the approximate solution is
where \(\rho (\lambda )=o(1)\) as \(\lambda \rightarrow 0.\) So we can define
Similarly, as the proof of the previous case, jointly with Lemma 4.1-(2), we conclude that the operator \((\phi , c_{1},c_{2},\ldots ,c_{N})=\mathcal {A}_{\lambda }(\phi , c_{1},c_{2},\ldots ,c_{N}):=\mathcal {T}_{\lambda }(S_{1}(w)+N(\phi )+P(\phi ))\) is a contraction mapping in \(\Sigma _{\lambda ,\sigma }\) and hence achieve a fixed point
which satisfies the Eq. (4.19). Moreover, under the condition (1.10), we observe that \(\rho (\lambda )\) can be taken as \(\lambda ^{\theta }\) in (4.20) for any \(\theta \in \left( 0,\frac{4}{p-1} \right) .\) That is,
and
Thus, to complete our proof, by Lemma 4.1-(2) we need to find \(\xi =\xi _{\lambda }\) such that
Combining the arguments in [26] and noticing that \(\frac{4}{p-1}<N-2\), we know
and
Moreover, noticing that
we have
Now, we claim that the dominant term in (4.24) is
Note that
We have
If we define
and \(F_{\lambda }(\xi )=(F_{\lambda }^{(1)}(\xi ),F_{\lambda }^{(2)}(\xi ), \ldots ,F_{\lambda }^{(N)}(\xi )).\) Then, by (4.25)–(4.27) and (4.29), we achieve that
and so we can show the existence of a solution \(\xi _{\lambda }\) to (4.24) since 0 is a critical point of w. Thus, we conclude that
where \(\delta \) is a fixed small constant. Using this fact and degree theory we obtain the existence of \(\xi _{\lambda }\) such that \(F_{\lambda }(\xi _{\lambda })=0\) in \(B_{\delta }.\) This complete the proof of Theorem 1.3.
References
Brizhik, L., Eremko, A., Piette, B., Zakrzewski, W.J.: Electron self-trapping in a discrete two-dimensional lattice. Physica D 159, 71–90 (2001)
Brizhik, L., Eremko, A., Piette, B., Zakrzewski, W.J.: Static solutions of a D-dimensional modified nonlinear Schrödinger equation. Nonlinearity 16, 1481–1497 (2003)
Hartmann, H., Zakrzewski, W.J.: Electrons on hexaonal lattices and applications to nanotubes. Phys. Rev. B 68, 184–302 (2003)
Brihaye, Y., Hartmann, B., Zakrzewski, W.J.: Spinning solitons of a modified nonlinear Schrödinger equation. Phys. Rev. D 69, 087701 (2004)
Liu, J.Q., Wang, Y.Q., Wang, Z.Q.: Soliton solutions for quasilinear Schrödinger equations II. J. Differ. Equ. 187, 473–493 (2003)
Colin, M., Jeanjean, L.: Solutions for quasilinear Schrödinger equations: a dual approach. Nonlinear Anal. TMA 56, 213–226 (2004)
Shen, Y.T., Wang, Y.J.: Soliton solutions for generalized quasilinear Schrödinger equations. Nonlinear Anal. TMA 80, 194–201 (2013)
Poppenberg, M., Schmitt, K., Wang, Z.Q.: On the existence of soliton solutions to quasilinear Schrödinger equation. Calc. Var. Partial Differ. Equ. 14, 329–344 (2002)
Liu, J.Q., Wang, Z.Q.: Soliton solutions for quasilinear Schrödinger equations. Proc. Am. Math. Soc. 131, 441–448 (2002)
Liu, J.Q., Wang, Y., Wang, Z.Q.: Solutions to quasilinear Schrödinger equations via the Nehari method. Commun. Partial Differ. Equ. 29, 879–901 (2004)
Moameni, A.: Existence of soliton solutions for a quasilinear Schrödinger equation involving critical exponent in \(\mathbb{R}^{N}\). J. Differ. Equ. 229, 570–587 (2006)
Moameni, A.: On the existence of standing wave solutions to a quasilinear Schrödinger equations. Nonlinearity 19, 937–957 (2006)
do Ó, J.M., Miyagaki, U., Soares, S.: Soliton solutions for quasilinear equations with critical growth. J. Differ. Equ. 248, 722–744 (2010)
Liu, X.Q., Liu, J.Q., Wang, Z.Q.: Ground states for quasilinear Schrödinger equations with critical growth. Calc. Var. Partial Differ. Equ. 46, 641–669 (2013)
Liu, X.Q., Liu, J.Q., Wang, Z.Q.: Quasilinear elliptic equations with critical growth via perturbation method. J. Differ. Equ. 254, 102–124 (2013)
He, X., Qian, A., Zou, W.: Existence and concentration of positive solutions for quasilinear equations with critical growth. Nonlinearity 26, 3137–3168 (2013)
Ye, H., Li, G.: Concentrating soliton solutions for quasilinear equations involving critical Sobolev exponents. Discrete Contin. Dyn. Syst. A 36, 731–762 (2016)
Silva, E.A.B., Vieira, G.F.: Quasilinear asymptotically periodic Schrödinger equations with critical growth. Calc. Var. Partial Differ. Equ. 39, 1–33 (2010)
Deng, Y.B., Peng, S.J., Yan, S.S.: Critical exponents and solitary wave solutions for generalized quasilinear Schrödinger equations. J. Differ. Equ. 260, 1228–1262 (2016)
Shen, Y.T., Wang, Y.J.: A class of generalized quasilinear Schrödinger equations. Commun. Pure Appl. Anal. 15, 853–870 (2016)
Adachi, S., Watanabe, T.: Asymptotic properties of ground states for a class of quasilinear Schrödinger equations with \(H^{1}\)-subcritical exponent. Adv. Nonlinear Stud. 12, 255–279 (2012)
Adachi, S., Watanabe, T.: Asymptotic uniqueness of ground states for a class of quasilinear Schrödinger equations with \(H^{1}\)-supercritical exponent. J. Differ. Equ. 260, 3086–3118 (2016)
Tang, M.: Uniqueness and global structure of positive radial solutions for quasilinear elliptic equations. Commun. Partial Differ. Equ. 26, 909–938 (2001)
Erbe, L., Tang, M.: Structure of positive radial solutions of semilinear elliptic equations. J. Differ. Equ. 133, 179–202 (1997)
Severo, U.B., Gloss, E., da Silva, E.G.: On a class of quasilinear Schrödinger equations with superlinear or asymptotically linear terms. J. Differ. Equ. 263, 3550–3580 (2017)
Dávila, J., del Pino, M., Musso, M., Wei, J.: Standing waves for supercritical nonlinear Schrödinger equations. J. Differ. Equ. 236, 164–198 (2007)
del Pino, M.: Supercritical elliptic problems from a perturbation viewpoint. Discrete Contin. Dyn. Syst. 21, 69–89 (2008)
Dávila, J., del Pino, M., Musso, M., Wei, J.: Fast and slow decay solutions for supercritical elliptic problem in exterior domains. Calc. Var. Partial Differ. Equ. 32, 453–480 (2008)
Wang, L., Wei, J.: Infinite multiplicity for an inhomogeneous supercritical problem in entire space. Commun. Pure Appl. Anal. 12, 1243–1257 (2013)
Berestycki, H., Lions, P.L.: Nonlinear scalar fields equations, I. Existence of a ground state. Arch. Ration. Mech. Anal. 82, 313–345 (1983)
Pucci, P., Serrin, J.: A general variational identity. Indiana Univ. Math. J. 35(3), 681–703 (1986)
del Pino, M., Wei, J.: An introduction to the finite and infinite dimensional reduction method. In: Xu, X., Han, F., Zhang, W. (eds.) Geometric Analysis Around Scalar Curratures, pp. 35–118. World Scientific, Singapore (2016)
Musso, M., Pistoia, A.: Multispike solutions for a nonlinear elliptic problem involving the critical Sobolev exponent. Indiana Univ. Math. J. 51(3), 541–579 (2002)
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Cheng, Y., Wei, J. Fast and slow decaying solutions for \(H^{1}\)-supercritical quasilinear Schrödinger equations. Calc. Var. 58, 144 (2019). https://doi.org/10.1007/s00526-019-1594-0
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DOI: https://doi.org/10.1007/s00526-019-1594-0