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Existence and concentration behavior of positive solutions to Schrödinger-Poisson-Slater equations

  • Yiqing Li , Binlin Zhang EMAIL logo and Xiumei Han
Published/Copyright: February 25, 2023

Abstract

This article is directed to the study of the following Schrödinger-Poisson-Slater type equation:

ε 2 Δ u + V ( x ) u + ε α ( I α u 2 ) u = λ u p 1 u in R N ,

where ε , λ > 0 are parameters, N 2 , ( α + 6 ) / ( α + 2 ) < p < 2 1 , I α is the Riesz potential with 0 < α < N , and V C ( R N , R ) . By using variational methods, we prove that there is a positive ground state solution for the aforementioned equation concentrating at a global minimum of V in the semi-classical limit, and then we found that this solution satisfies the property of exponential decay. Finally, the multiplicity and concentration behavior of positive solutions for the aforementioned problem is investigated by the Ljusternik-Schnirelmann theory. Our article improves and extends some existing results in several directions.

MSC 2010: 35B33; 35J20; 35J61

1 Introduction and main results

In this article, we investigate some qualitative properties of the Schrödinger-Poisson-Slater problem:

(1.1) ε 2 Δ ψ + V ( x ) ψ + ε α ( I α ψ 2 ) ψ = λ ψ p 1 ψ in R N , ψ H 1 ( R N ) ,

where ε , λ > 0 is a parameter, V : R N R are continuous functions, ( α + 6 ) / ( α + 2 ) < p < 2 1 , and here, 2 = 2 N / ( N 2 ) when N 3 and 2 = when N = 2 , I α is the Riesz potential, 0 < α < N , defined by

(1.2) I α ( x ) = A α x N α , A α = Γ N α 2 π N 2 2 α Γ α 2 .

Let ϕ I α ψ 2 , λ = 1 , one can deduce that problem (1.1) is equivalent to the following system:

(1.3) ε 2 Δ ψ + V ( x ) ψ + ϕ ψ = ψ p 1 ψ in R N , ε α ( Δ ) α 2 ϕ = ψ 2 in R N .

When ε = 1 , N = 3 , and α = 2 , the aforementioned system without critical nonlinearity expresses as a Schrödinger-Poisson system, which has extensive applications with the presence of Hamiltonian structure, see [9]. More physical backgrounds are directed to [8,10,11,14,31]. In particular, in addition that p = 5 / 3 , it is well known that problem (1.1) appeared as a simple approximation for the exchange term of the Hartree-Fork model of a quantum many-body system of electrons, in which V ( x ) is the external potential, u p 1 u is the Slater correction that was introduced by Slater in 1951 as a local approximation of the exchange potential, and λ is named Slater constant, see, e.g., [16,30,38]. It is worth mentioning that Bao et al. [3] proposed the multidimensional version of Schrödinger-Poisson-Slater, where p = 2 + 2 / n , and see also [19] for the relation with Thomas-Fermi-Dirac-von Weizsäcker models of the density functional theory. There are considerable analytical results about the Schrödinger-Poisson-Slater equation, such as [2,12,18,2630,3537,40,42] and the references therein.

Now we revisit some intrinsically relevant results in recent years. In [34], Ruiz sought positive radial solutions to the following Schrödinger-Poisson equation:

(1.4) Δ ψ + ψ + λ ϕ ψ = ψ p in R 3 , Δ ϕ = ψ 2 , lim x ϕ ( x ) = 0 ,

where ϕ and ψ are positive radial functions, 1 < p < 5 . In particular, he pointed out that there is only trivial solution for (1.4) as p ( 1 , 2 ] and λ 1 / 4 . Later, the author [35] continued to investigate the behavior of minimizers for the following version of the Schrödinger-Poisson-Slater problem:

(1.5) Δ ψ + ψ + λ 1 x ψ 2 ψ = ψ p 1 ψ in R 3 , ψ H 1 ( R 3 ) ,

where λ > 0 , 1 < p < 2 . By making the change of variables, (1.5) can be reduced to the study of the limit problem as the zero mass Schrödinger-Poisson-Slater equation:

(1.6) Δ u + 1 4 π 1 x u 2 u = μ u p 1 u , u H 1 ( R 3 ) ,

which was discussed by Ianni and Ruiz [18] in the case of μ > 0 and 2 < p < 5 . Through monotonicity trick and concentration compactness lemma, they proved the existence of ground state solutions. Moreover, by comparison arguments, they also obtained the exponential decay estimate of solutions. Mercuri et al. [30] investigated the nonlocal Schrödinger-Poisson-Slater equation as follows:

Δ ψ + ( I α ψ p ) ψ p 2 ψ = ψ q 2 ψ , ψ H 1 ( R N ) ,

where N N , p , q > 1 . They worked in the Coulommb-Sobolev space and proved a family of optimal interpolation inequalities. For the parameters in a defined range, the authors established the existence of radial solutions and some qualitative properties. In [5,6], the following minimization problem

(1.7) inf ψ 0 ψ 2 p ( N + α ) 4 N 4 + α N [ L ( ψ ) ] 2 N p ( N 2 ) 2 ( 4 + α N ) ψ p p , where L ( ψ ) = R N R N ψ ( x ) 2 ψ ( y ) 2 x y N α d x d y ,

is achieved, where

(1.8) p 2 ( 4 + α ) 2 + α , , N = 2 ; p 2 ( 4 + α ) 2 + α , 2 N N 2 , 3 N < 4 + α ; p 2 N N 2 , 2 ( 4 + α ) 2 + α , N > 4 + α .

While the Euler-Lagrange equation of problem (1.7) is exactly equation (1.1) with V ( x ) = 0 and ε = 1 . Very recently, Lei and Lei in [23] considered the higher-dimensional version of problem (1.1) with V ( x ) = 0 and ε = 1 , and detected a Nehari-Pohozaev type ground state solution under the hypothesis that p belongs to the intervals in (1.8).

In those articles we refereed earlier, the authors usually dealt with the convolution term by Hardy-Littlewood-Sobolev inequality, so we expound this inequality here.

Lemma 1.1

(Hardy-Littlewood-Sobolev inequality [24]) Let α ( 0 , N ) and s ( 1 , N / α ) . Then for any Ψ L s ( R N ) , I α Ψ L N s N α s ( R N ) , and

R N I α Ψ N s N α s d x C ( α , s ) R N Ψ s d x N N α s .

Remark 1.1

In this article, we use the Hardy-Littlewood-Sobolev inequality with the form

R N ( I α Ψ 2 ) u 2 d x = R N I α 2 Ψ 2 2 d x C R N Ψ 4 N N + α d x N + α N .

In fact, the following property of I α ensures that the aforementioned special form is true:

I s + t = I s I t ,

where s , t ( 0 , N ) , s + t < N , see [32].

To continue the following statements, we point out that as N = 3 , V ( x ) = 0 , and α = 2 , the case p = 2 in (1.1) is critical in a certain sense. In fact, this is due to the appearance of scaling invariance, that is to say, if u is a solution of (1.1), then for some parameter μ R , μ 2 u ( μ x ) is a solution of (1.1).

In the following, we present some existence results of the Schrödinger-Poisson-Slater equations involving a critical nonlinearity. Yang and Liu [40] consider the following critical Schrödinger-Poisson-Slater equation:

Δ ψ + ψ 2 1 4 π x ψ = μ λ ( x ) ψ p 1 ψ + ψ 4 ψ , ψ R 3 ,

where μ > 0 , 2 < p < 3 , λ ( x ) L 6 / ( 5 p ) ( R 3 ) . Applying truncation technique and Krasnoselskii genus theory, the authors proved that there exist infinitely many solutions with μ ( 0 , μ ) . Liu et al. [28] investigated the same problem as [40] with λ ( x ) = 1 , by combining perturbation approach with Mountain-Pass lemma, the authors achieved the existence of positive ground state solutions as p ( 11 / 7 , 5 ) . And for μ in the defined range, by using constrained minimization approach, they proved the nonexistence of nontrivial solutions in the critical case p = 2 . Moreover, they illustrated the existence of radial symmetrical solutions by combining concentration-compactness principle and truncation technique.

Recently, some existence and multiplicity results concerning the Schrödinger-Poisson-Slater equations have been involved a prescribed L 2 -norm. Luo [29] studied the stationary Schrödinger-Poisson-Slater problem as follows:

Δ ψ λ ψ + ( x 1 * ψ 2 ) ψ = ψ p 1 ψ , ψ R 3 ,

where λ R , 7 / 3 < p < 5 . Motivated by the work of Bartsch and De Valeriola [4], they proved the existence and multiplicity of couple solutions with the prescribed L 2 -norm. Siciliano [37] investigated the following system:

Δ ψ + ψ + λ ϕ ψ = ψ p 2 ψ in Ω , Δ ϕ = ψ 2 in Ω , ψ = ϕ = 0 on Ω ,

where Ω is a bounded domain in R 3 , λ > 0 , p [ 4 , 2 ) . By employing some appropriate variational methods, the author obtained that the number of positive solutions is more than the Ljusternik-Schnirelmann category when p near 2 .

As far as we know, there is only one result concerned with the concentration behavior of Schrödinger-Poisson-Slater problem, we briefly introduce this result as follows. Ruiz and Vaira [36] concerned the Schrödinger-Poisson-Slater problem as follows in R 3 :

(1.9) ε 2 Δ ψ + V ( x ) ψ + ϕ ( x ) ψ = ψ p , Δ ϕ = ψ 2 ,

where 1 < p < 5 . They considered the problem (1.9) under the following assumption:

( V 1 ) There is a bounded open set Ω 0 satisfying P 0 Ω 0 and

V ( P 0 ) = min x Ω ¯ 0 V ( x ) < V ( P ) , P Ω 0 \ { P 0 } ;

( V 2 ) for any x Ω 0 , β 0 > 2 , V ( x ) = 1 + g ( x ) β 0 , where g : Ω 0 R is a C 2 , 1 function.

Via a singular perturbation arguments and Lyapunov-Schmidt reduction, the authors established that there exist multi-bump solutions concentrating at a local minimum of V . Inspired by this work, a natural question arises: Whether the concentration behavior occurs for ground state solutions? One will find an answer in the present article.

Motivated by the aforementioned works, we consider the existence, multiplicity, and concentration behavior of positive ground state solutions for the Schrödinger-Poisson-Slater problem (1.1) with the assumption on V ( x ) :

( V ) V C ( R N , R ) and 0 < V 0 inf R N V ( x ) < V = lim x V ( x ) .

Note that the aforementioned hypothesis ( V ) was first introduced by Rabinowitz [33] to the research of Schrödinger equation. By contracting the transformation u ( x ) = ψ ( ε x ) in (1.1), we can deduce the following problem

(1.10) Δ u + V ( ε x ) u + ( I α u 2 ) u = λ u p 1 u in R N .

It is evident to obtain that the solution of (1.10) corresponds to the critical point of energy functional given by

(1.11) I ε ( u ) = 1 2 R N u 2 d x + 1 2 R N V ( ε x ) u 2 d x + 1 4 R N ( I α u 2 ) u 2 d x λ 1 + p R N u 1 + p d x .

Let H 1 ( R N ) be the Sobolev space endowed with the standard norm

u R N ( u 2 + u 2 ) d x 1 2 .

For any ε > 0 , let H ε ( R N ) { u H 1 ( R N ) : R N V ( ε x ) u 2 d x < } denote the Sobolev space endowed with the norm

u ε R N ( u 2 + V ( ε x ) u 2 ) d x 1 2 .

Also, denote

u V 0 R N ( u 2 + V 0 u 2 ) d x 1 2 , u V R N ( u 2 + V u 2 ) d x 1 2 .

It is standard to verify that I ε C 1 ( H ε ( R N ) , R ) .

The purpose of this article contains two folds. The first one consider the existence and concentration behavior of positive groundstates for (1.10) under the assumption ( V ) . Here is the first main result.

Theorem 1.1

Suppose that V satisfies ( V ) . Then, for ε > 0 , problem (1.1) has at least a positive ground state solution ψ ε ( ε x ) in H ε ( R N ) under one of the following cases:

  1. 3 p < 2 1 , for any λ > 0 ;

  2. α + 6 α + 2 < p < 3 , for λ > 0 small.

Moreover, the following statements hold:
  1. Let η ε R N be a global maximum point of this positive ground state solution ψ ε ( ε x ) to (1.1), then

    lim ε 0 V ( η ε ) = V 0 .

    Meanwhile, for all ε n 0 , ψ ε n ( ε n x + η ε n ) converges to a positive ground state solution of the following equation:

    (1.12) Δ u + V 0 u + ( I α u 2 ) u = λ u p 1 u , i n R N , u H 1 ( R N ) .

  2. There exist C , κ > 0 independent of η ε satisfying

    ψ ε ( x ) C e κ ε x η ε , x R N .

In the second part, we concern the multiplicity and concentration behavior of positive ground state solutions for (1.1) under the assumption ( V ) . To illustrate the relationship between the number of solutions and the topology of the set of minima of the potential V , we set

Θ { x R N : V ( x ) = V 0 }

and

Θ δ { x R N : dist ( x , Θ ) δ } for δ > 0 .

From ( V ) , it is easy to obtain that the set Θ is compact. Furthermore, we demonstrate that let be the closed subset of a topological space A , cat A ( ) is the Ljusternik-Schnirelmann category, namely, the number of closed and contractible set in A , which cover . There is the second main result.

Theorem 1.2

Suppose that 3 p < 2 1 , λ > 0 , and V satisfies ( V ) . Then for any δ > 0 , there exists ε δ > 0 such that problem (1.1) has at least cat Θ δ ( Θ ) positive solutions in H ε ( R N ) for all ε ( 0 , ε δ ) . Also, the statements ( c ) and ( d ) of Theorem 1.1hold true for these positive solutions.

Finally, we sketch technical approaches used along this article to obtain the main results. We study the existence and concentration behavior of positive ground state solutions by virtue of variational methods. Moreover, we obtain the multiplicity of positive solutions by the Ljusternik-Schnirelmann theory. More specifically, we first study the existence of ground state solution for the limit problem V V 0 , and then, compared with the limit problem, we obtain the existence of positive groundstates of (1.1) by exploiting variational approaches. Consequently, we prove the concentration behavior and exponential of the positive groundstate by Moser’s iteration technique and maximum principle. It is worth mentioning that we need to distinguish two cases of V in the course of the proof, for example, the convergence of (PS) sequence. In the meantime, we provide a direct proof to compare the mountain pass value of (1.1) with the limit problem. Furthermore, the multiplicity of positive solutions is demonstrated by the Ljusternik-Schnirelmann theory. Also, by the analogous arguments of proving concentration behavior and exponential decay of positive groundstate, the same properties of multiple positive solutions are confirmed. It is interesting that the existence and concentration results of this article are valid for the critical case p = 2 as λ is small according to a general lower bound of p .

Remark 1.2

If V ( x ) V 0 , then it is not difficult to deduce the following Pohozaev identity:

(1.13) N 2 2 R N u 2 d x + N 2 R N V 0 u 2 d x + N + α 4 R N ( I α u 2 ) u 2 d x λ N p + 1 R N u p + 1 d x = 0 ,

see, e.g., [30]. From (1.13), it follows that there is only trivial solution for problem (1.1) with ε = 1 , N < 4 + α and p = 2 1 . As for some recent results involving semiclassical ground state solutions in the critical case, for example, we refer to [13,25] and the references therein.

Remark 1.3

In [21], we obtained the existence, multiplicity, and concentration behavior of positive solutions for the following Schrödinger-Poisson problem in R 2 :

ε 2 Δ ψ + V ( x ) ψ + ε α ( I α ψ q ) ψ q 2 ψ = f ( ψ ) ,

where f C ( R , R ) satisfies critical exponential growth and V < . Compared with the work in [21], we consider (1.1) in dimension R N ( N 2 ) , and we introduce some new techniques and subtle analyses in the present article. For detailed description, we consider: (i) the case V = , this shows that we cannot obtain the positive solution of (1.1) by maximum principle; hence, the Harnack’s inequality enters into our consideration; (ii) for the Schrödinger-Poisson-Slater problem (1.1), we need a new method to prove that the solution of (1.1) is nonnegative; and (iii) we find a more straightforward approach to certify the existence of ground state solutions for the limit equation.

This article is planned as follows. Section 2 gives some preliminaries. Sections 3 and 4 show the proof of Theorem 1.1, and in particular, Section 3 illustrates the existence of groundstates for the limit problem (1.10). Section 4 explains the concentration behavior and exponential decay of the groundstate for problem (1.1). Furthermore, the proof of Theorem 1.2 is demonstrated in Section 5.

Here, we state some notations used in this article:

  • Let Ω be an open subset of R N , L s ( Ω ) denotes the Lebesgue space equipped with the norm u s ( Ω ) = Ω u s d x 1 / s , 2 s < + ;

  • B R ( y ) denotes the open ball centered at y with radius R > 0 ;

  • C , C ¯ , and C ˜ denote different positive constants in different places.

2 The limit equation

This section is devoted to investigating the limit equation when V ( x ) V 0 , that is,

(2.1) Δ u + V 0 u + ( I α u 2 ) u = λ u p 1 u in R N .

It is evident that the corresponding functional of aforementioned equation is

I V 0 ( u ) = 1 2 R N u 2 d x + 1 2 R N V 0 u 2 d x + 1 4 R N ( I α u 2 ) u 2 d x λ 1 + p R N u 1 + p d x .

There are some lemmas which will be used later.

Lemma 2.1

The following statements hold:

  1. There exists ρ > 0 such that I V 0 S ρ ( u ) > 0 , u S ρ = { u H ε ( R N ) : u V 0 = ρ } .

  2. There is e H ε ( R N ) with e V 0 > ρ such that I V 0 ( e ) < 0 .

Proof

(i) By Sobolev’s embedding inequality, one has

I V 0 ( u ) = 1 2 R N u 2 d x + 1 2 R N V 0 u 2 d x + 1 4 R N ( I α u 2 ) u 2 d x λ 1 + p R N u 1 + p d x 1 2 u V 0 2 λ 1 + p u 1 + p 1 + p 1 2 u V 0 2 C λ u V 0 1 + p ,

where C > 0 is a constant. Note that 1 + p > 2 , we choose 0 < ρ < ( 2 C λ ) 1 1 p such that u V 0 = ρ , then, ( i ) holds.

(ii) Let u t t a u ( t b x ) here and in the sequel, where a = α + 2 2 b > 0 . Then

I V 0 ( u t ) = t 2 a + 2 b N b 2 R N u 2 d x + t 2 a N b 2 R N V 0 u 2 d x + t 4 a α b N b 4 R N ( I α u 2 ) u 2 d x λ t ( 1 + p ) a N b 1 + p R N u 1 + p d x .

Note that p > ( α + 6 ) / ( α + 2 ) , we have ( 1 + p ) a > 2 a + 2 b = 4 a α b , and it follows that lim t I V 0 ( u t ) = . Hence, we can choose t ¯ > 0 such that e = u t ¯ { u H ε ( R N ) : u V 0 > ρ } and I V 0 ( e ) < 0 .□

By using Lemma 2.1, one can obtain that there is a Palais-Smale sequence { u n } H ε ( R N ) such that

I V 0 ( u n ) c V 0 , I V 0 ( u n ) 0 ,

where c V 0 is characterized by

(2.2) 0 < c V 0 inf γ Γ max t [ 0 , 1 ] I V 0 ( γ ( t ) )

with

Γ { γ C 1 ( [ 0 , 1 ] , H ε ( R N ) ) : γ ( 0 ) = 0 , I V 0 ( γ ( 1 ) ) < 0 } .

Now we give the proof of the existence of weak solution to (2.1).

Lemma 2.2

Let { u n } H ε ( R N ) be a (PS) sequence for I V 0 , that is,

I V 0 ( u n ) c V 0 , I V 0 ( u n ) 0 i n ( H ε ( R N ) ) , a s n .

Then, going to a subsequence, there is u H ε ( R N ) such that u n u in H ε ( R N ) , and u is a weak solution of (2.1).

Proof

Note that { u n } is a (PS) sequence for I V 0 , then

(2.3) 1 2 u n V 0 2 + 1 4 R N ( I α u n 2 ) u n 2 d x λ 1 + p R N u n 1 + p d x c V 0 ,

(2.4) u n V 0 2 + R N ( I α u n 2 ) u n 2 d x λ R N u n 1 + p d x 0 .

Now we prove the boundedness of { u n } in H ε ( R N ) . Observe that

(2.5) c V 0 + o ( 1 ) = I V 0 ( u n ) 1 4 I V 0 ( u n ) , u n = 1 4 u n V 0 2 + λ 1 4 1 1 + p R N u n 1 + p d x .

Now we distinguish two cases. When p 3 , we have

c V 0 + o ( 1 ) 1 4 u n V 0 2 ,

which means the boundedness of u n V 0 . When α + 6 α + 2 < p < 3 , it follows from Sobolev’s embedding inequality that

c V 0 + o ( 1 ) 1 4 u n V 0 2 C λ u n V 0 1 + p .

Choosing 0 < λ ( 8 C u n V 0 p 1 ) 1 such that λ ( 0 , λ ] , we can found that u n V 0 is bounded. Thus,

(2.6) u n u in H ε ( R N ) , u n u in L loc s ( R N ) , 2 s < 2 .

Since for any ϕ C 0 ( R N ) ,

R N ( u n ϕ + V 0 u n ϕ ) d x + R N ( I α u n 2 ) u n ϕ d x λ R N u n p ϕ d x 0 , as n .

From (2.6), we obtain

R N ( u ϕ + V 0 u ϕ ) d x + R N ( I α u 2 ) u ϕ d x λ R N u p ϕ d x = 0 , as n ,

for any ϕ C 0 ( R N ) . Thus, u is a weak solution of (2.1).□

Lemma 2.3

Problem (2.1) has a ground state solution in H ε ( R N ) .

Proof

From Lemmas 2.1 and 2.2, we obtain that there exists a (PS) sequence { u n } weakly converging to the weak solution of (2.1), and then it remains only to prove that the weak solution u is nontrivial. With the reduction to absurdity, we suppose that u 0 . Since { u n } is bounded, there are two cases need to be distinguished: { u n } is vanishing or nonvanishing.

Case (i): { u n } is vanishing. By Lion’s concentration compactness lemma (see [41, Lemma 1.21]), for any 2 s < 2 , one has

(2.7) u n 0 in L s ( R N ) , as n .

Noticing that { u n } is a ( PS ) c V 0 sequence, applying Lemma 2.2, we have

lim n 1 2 u n V 0 2 + 1 4 R N ( I α u n 2 ) u n 2 d x = c V 0 .

Since u n 0 in H ε ( R N ) , then I V 0 ( u n ) 0 , that is, c V 0 = 0 . Impossible.

Case (ii): { u n } is nonvanishing. Thus, there exist δ , r > 0 and a sequence { y n } Z N such that

lim n B r ( y n ) u n 2 d x δ .

Let v n u n ( x y n ) , we obtain

(2.8) B r ( 0 ) v n 2 d x δ .

By using the fact that I V 0 and I V 0 are invariant by Z N translations, one has that { v n } is also a (PS) sequence. Hence, v n v in H ε ( R N ) . From (2.8) and v n v in L loc 2 ( R N ) , one has v 0 . Then, v is a nontrivial critical point of I V 0 .□

3 Existence of positive groundstates

Now, we consider problem (1.1). Define the Nehari manifold associated to I ε as follows:

N ε = { u H ε ( R N ) : u 0 , I ε ( u ) , u = 0 } .

First, we investigate some technical lemmas that will be used later.

Lemma 3.1

There exists α 1 > 0 independent of ε , such that

u ε α 1 , u N ε .

Proof

Since u N ε ,

u ε 2 + R N ( I α u 2 ) u 2 d x = λ R N u 1 + p d x ,

it follows from Sobolev’s embedding inequality that

(3.1) u ε 2 λ u 1 + p 1 + p C u ε 1 + p .

Then, u ε is bounded from below.□

In terms of Lemma 2.1, the functional I ε satisfies the mountain pass geometry. Thus, there is a sequence { u n } H ε ( R N ) satisfying

I ε ( u n ) c ε , I ε ( u n ) 0 ,

where

(3.2) c ε inf u H ε ( R N ) \ { 0 } max t 0 I ε ( u t ) ,

and 0 < C < c ε . In addition, for all u H ε ( R N ) \ { 0 } , by a direct calculation, it is easy to obtain that there exists a unique positive number t = t ( u ) such that

I ε ( u t ( u ) ) = max s 0 I ε ( u s ( u ) ) , u t ( u ) N ε .

Hence, by standard argument as in [41, Theorem 4.2], one has

c ε = inf u N ε I ε ( u ) .

Lemma 3.2

Assume that ( V ) holds. Then

lim ε 0 c ε = c V 0 < c V ,

where c V is defined as (2.2).

Proof

Applying Lemma 2.3, we know that there exists a ground state solution w H ε ( R N ) , that is,

(3.3) w V 0 2 + R N ( I α w 2 ) w 2 d x = λ R N w 1 + p d x .

For any δ > 0 , let w δ C 0 ( R N ) , such that

w δ N V 0 , w δ w in H ε ( R N ) , I V 0 ( w δ ) < c V 0 + δ .

Fix η C 0 ( R N , [ 0 , 1 ] ) such that η = 1 on B 1 ( 0 ) and η = 0 on R N \ B 2 ( 0 ) . Define v n ( x ) = η ( ε n x ) w δ ( x ) with ε n 0 , one has

v n w δ in H ε ( R N ) , as n .

By the definition of N ε , there exists a unique t n such that ( v n ) t n N ε n , note that ( v n ) t n = t n a v n ( t n b x ) . Thus,

c ε n I ε n ( ( v n ) t n ) = t n 2 a + 2 b N b 2 R N v n 2 d x + t n 2 a N b 2 R N V ( t n b ε n x ) v n 2 d x + t n 4 a α b N b 4 R N ( I α v n 2 ) v n 2 d x λ t n ( 1 + p ) a N b 1 + p R N v n 1 + p d x .

Since I ε n ( ( v n ) t n ) , ( v n ) t n = 0 , we obtain

(3.4) t n 2 a + 2 b N b R N v n 2 d x + t n 2 a N b R N V ( t n b ε n x ) v n 2 d x + t n 4 a α b N b R N ( I α v n 2 ) v n 2 d x = λ t n ( 1 + p ) a N b R N v n 1 + p d x .

It follows from Hardy-Littlewood-Sobolev inequality (see Remark 1.1) that

(3.5) λ t n ( 1 + p ) a R N v n 1 + p d x t n 2 a + 2 b R N v n 2 d x + t n 2 a R N V ( t n b ε n x ) v n 2 d x + C t n 4 a α b v n 4 n n + α 4 ,

then { t n } is bounded. Going to a subsequence if necessary, we assume that t n t 0 0 . Note that c ε n > C > 0 , one has t 0 > 0 . Let n in (3.4), one has

(3.6) t 0 2 a + 2 b N b R N w δ 2 d x + t 0 2 a N b R N V 0 w δ 2 d x + t 0 4 a α b N b R N ( I α w δ 2 ) w δ 2 d x = λ t 0 ( 1 + p ) a N b R N w δ 1 + p d x .

Thus, by (3.3) and (3.6), let n , we know

( t 0 2 b 1 ) R N V 0 w 2 d x = [ t 0 ( p 1 ) a 2 b 1 ] λ w 1 + p 1 + p .

Note that ( p 1 ) a 2 b > 0 , if t 0 > 1 , the right-hand side of the aforementioned equality is more than zero, while the left side is less than zero, impossible. If t 0 < 1 , we obtain a contradiction analogously. Consequently, t 0 = 1 .

Furthermore, since

R N ( V ( t n b ε n x ) V 0 ) v n 2 d x 0 , I V 0 ( ( v n ) t n ) I V 0 ( w δ ) ,

and

c ε n I ε n ( ( v n ) t n ) = I V 0 ( ( v n ) t n ) + t n 2 a n b 2 R N ( V ( t n b ε n x ) V 0 ) v n 2 d x ,

one has

limsup n c ε n I V 0 ( w δ ) c V 0 + δ .

Due to the arbitrariness of δ and ε n , we have

(3.7) limsup ε 0 c ε c V 0 .

Note that

c ε c V 0 , ε > 0 ,

which means

(3.8) liminf ε 0 c ε c V 0 .

Combining (3.7) with (3.8), we deduce that

lim ε 0 c ε = c V 0 .

From (V), c V 0 < c V , we complete the proof.□

Here, we clarify that I ε satisfies ( PS ) c ε condition for ε [ 0 , ε 0 ) .

Lemma 3.3

Assume that ( V ) holds. For any ε [ 0 , ε 0 ) , let { u n } be a ( PS ) c ε sequence and u n u ε , then u n u ε in H ε ( R N ) .

Proof

Analogous to (2.5) and Lemma 3.1, one has

(3.9) C ¯ < u n ε < C ˜ ,

where C ¯ , C ˜ > 0 .

First, we consider the case V = . Then, one can easily obtain that V is coercive and the continuous embedding H ε ( R N ) L s ( R N ) is compact, and here, 2 s < 2 . Thus, going to a subsequence if necessary, u n u ε in L s ( R N ) . Let w ¯ n = u n u ε , using the well-known Brezis-Lieb lemma, one has

w ¯ n ε 2 + R N ( I α w ¯ n 2 ) w ¯ n 2 d x = λ R N w ¯ n 1 + p d x + o ( 1 ) = o ( 1 ) ,

which leads to w ¯ n 0 in H ε , that is, u n u ε in H ε .

Now we consider V < . We prove that u ε 0 in the sequel. Arguing by contradiction, we suppose u ε = 0 . Now, we claim that there exist δ ˜ , R > 0 and { y n } R N such that

B R ( y n ) u n 2 d x δ ˜ ,

otherwise, by Lion’s concentration compactness lemma, we have

u n 0 in L s ( R N ) , s 2 .

By using the similar arguments of Lemma 2.3, we obtain the claim.

Let t n > 0 such that ( u n ) t n N V . From line by line to Lemma 3.2, we deduce that { t n } is bounded, and one can obtain that

lim n t n = t 0 > 0 .

We divide three steps in the following proof.

Step 1: t 0 1 . Arguing by contradiction, we suppose that there exist δ > 0 and a subsequence, for convenience, denoted by { t n } also, satisfying

t n 1 + δ , n N .

Since I ε ( u n ) , u n = o n ( 1 ) and { ( u n ) t n } N V , we have

(3.10) R N u n 2 d x + R N V ( ε x ) u n 2 d x + R N ( I α u n 2 ) u n 2 d x = λ R N u n 1 + p d x + o n ( 1 )

and

(3.11) t n 2 a + 2 b N b R N u n 2 d x + t n 2 a N b R N V u n 2 d x + t n 4 a α b N b R N ( I α u n 2 ) u n 2 d x = λ t n ( 1 + p ) a N b R N u n 1 + p d x .

Thus,

R N ( t n 2 b V V ( ε x ) ) u n 2 d x + o n ( 1 ) = R N ( t n ( p 1 ) a 2 b 1 ) λ u n 1 + p d x .

Let ζ > 0 , it follows from ( V ) that there exists R ( ζ ) > 0 satisfying

(3.12) V ( ε x ) V ζ > t n 2 b V ζ , x R .

It follows from u n 0 in L 2 ( B R ( 0 ) ) that

R N ( t n ( p 1 ) a 2 b 1 ) λ u n 1 + p d x ζ C ˜ 1 + o n ( 1 ) ,

where C ˜ 1 sup n N u n 2 2 . Let v n = u n ( x + y n ) , up to a subsequence, we suppose that v n v in H ε . By u n 0 , there exist C > 0 and Ω R N with positive measure, such that, for any x Ω , v ( x ) > C . Then

0 < Ω [ ( 1 + δ ) ( p 1 ) a 2 b 1 ] λ v n 1 + p d x ζ C ˜ 1 + o n ( 1 ) .

Let n , we have

0 < Ω [ ( 1 + δ ) ( p 1 ) a 2 b 1 ] λ v 1 + p d x ζ C ˜ 1 ,

since ζ is arbitrary, we obtain a contradiction.

Step 2: t 0 = 1 . From I V ( ( u n ) t n ) c V , we have

(3.13) c ε + o n ( 1 ) = I ε ( u n ) I ε ( u n ) + c V I V ( ( u n ) t n ) .

Note that

(3.14) I ε ( u n ) I V ( ( u n ) t n ) = 1 2 R N u n 2 d x t n 2 a + 2 b N b 2 R N u n 2 d x + 1 2 R N V ( ε x ) u n 2 d x t n 2 a N b 2 R N V u n 2 d x + 1 4 t n 4 a α b N b 4 R N ( I α u n 2 ) u n 2 d x + t n ( 1 + p ) a N b 1 + p 1 1 + p λ u n 1 + p 1 + p .

By u n 0 , { u n } is bounded in H ε ( R N ) . Then, it follows from (3.12)–(3.14) that

c ε + o n ( 1 ) c V ζ C + o n ( 1 ) .

Since ζ is arbitrary, one has

limsup ε 0 c ε c V ,

which contradicts to Lemma 3.2.

Step 3: t 0 < 1 . We may suppose that t n < 1 for n N . From (3.10) and (3.11), we have

R N ( t n 2 b V V ( ε x ) ) u n 2 d x + o n ( 1 ) = R N ( t n ( p 1 ) a 2 b 1 ) λ u n 1 + p d x .

From ( V ) , there exists R large enough such that

t n 2 b V V ( ε x ) > V V ( ε x ) > 0 , x R .

Then, by u n 0 in L 2 ( B R ( 0 ) ) , one has

R N ( t n ( p 1 ) a 2 b 1 ) λ u n 1 + p d x > o n ( 1 ) .

As the arguments of Step 1, note that t n < 1 , we can conclude that

o n ( 1 ) < Ω ( t n ( p 1 ) a 2 b 1 ) λ v n 1 + p d x < 0 ,

which is absurd as n . Consequently, u ε 0 . Now we prove that u n u ε in H ε ( R N ) , when p 3 , by using Fatou’s lemma directly, we have

(3.15) c ε I ε ( u ε ) 1 4 I ε ( u ε ) , u ε = 1 4 u ε ε 2 + 1 4 1 1 + p λ u ε 1 + p 1 + p = liminf n 1 4 u n ε 2 + 1 4 1 1 + p λ u n 1 + p 1 + p = liminf n I ε ( u n ) 1 4 I ε ( u n ) , u n limsup n I ε ( u n ) 1 4 I ε ( u n ) , u n = c ε .

Also, in the case of ( 6 + α ) / ( 2 + α ) < p < 3 , from line by line of Lemma 2.2, one can choosing a λ > 0 such that (3.15) holds for any λ ( 0 , λ ] . Consequently, I ε ( u ε ) = c ε and I ε ( u ε ) , u ε = 0 . So, u n u ε in H ε ( R N ) , we complete the proof.□

Lemma 3.4

Assume that ( V ) holds. Let u be the solution of (1.10), then u > 0 for all x R N .

Proof

First, we prove that u does not change sign. For any t > 0 , we define the following functions:

f ( t ) = I ε ( u t ) = t 2 a + 2 b N b 2 R N u 2 d x + t 2 a N b 2 R N V 0 u 2 d x + t 4 a α b N b 4 R N ( I α u 2 ) u 2 d x t ( 1 + p ) a N b 1 + p λ R N u 1 + p d x , g ( t ) = I ε ( u t + ) = t 2 a + 2 b N b 2 R N ( u + ) 2 d x + t 2 a N b 2 R N V ( ε x ) ( u + ) 2 d x + t 4 a α b N b 4 R N ( I α u + 2 ) u + 2 d x t ( 1 + p ) a N b 1 + p λ R N u + 1 + p d x , h ( t ) = I ε ( u t ) = t 2 a + 2 b N b 2 R N ( u ) 2 d x + t 2 a N b 2 R N V ( ε x ) ( u ) 2 d x + t 4 a α b N b 4 R N ( I α u 2 ) u 2 d x t ( 1 + p ) a N b 1 + p λ R N u 1 + p d x ,

where u + = max { 0 , u } and u = min { 0 , u } . Due to the existence of nonlocal term, one can easily obtain that g ( t ) + h ( t ) f ( t ) . By using the arguments of Lemma 3.2, we can deduce that

max t > 0 f ( t ) = f ( 1 ) = I ε ( u ) = c ε .

Let t 1 and t 2 denote the maxima point of the functions g and h respectively. Then, we may assume that t 1 t 2 , which means that h ( t 1 ) 0 . Consequently,

max t > 0 g = g ( t 1 ) g ( t 1 ) + h ( t 1 ) f ( t 1 ) max t > 0 f = c ε .

It follows from the definition of c ε that

max t > 0 g = g ( t 1 ) = g ( t 1 ) + h ( t 1 ) .

Then, h ( t 1 ) = 0 . And so, u = 0 . In the case of t 1 > t 2 , using the similar argument, one can conclude that u + = 0 . Therefore, regarding to the change of sign, we may assume that u 0 .

Applying the standard arguments as in [15,20], we can conclude that u L ( R N ) and u C loc 1 , α 0 ( R N ) , where 0 < α 0 < 1 . Furthermore, from Harnack’s inequality in [39], one has u > 0 for all x R N .□

Combining Lemma 3.3 with Lemma 3.4, we obtain the corollary as follows.

Corollary 3.1

Assume that ( V ) holds. Then for ε > 0 small enough, c ε is achieved, and problem (1.10) has a positive ground state solution.

4 Concentration and decay of groundstate

We study the concentration behavior of ground state solution of problem (1.10) in this section.

Lemma 4.1

Assume that ( V ) holds. Let ε n 0 and { u n } N ε n be such that I ε n ( u n ) c V 0 . Then, there is a sequence { y n } R N such that v n = u n ( x + y n ) has a convergent subsequence in H ε ( R N ) . Moreover, up to a subsequence, y n y Θ { x R N : V ( x ) = V 0 } .

Proof

Analogous to [1, Proposition 4.2], we can prove that Lemma 4.1 holds, and for reader’s convenience, we sketch the proof here. Let { u n } be the solutions obtained in Corollary 3.1, and it is obvious that

c ε n = I ε n ( u n ) c V 0 , 0 < c V 0 = limsup n c ε n ,

and { u n } is bounded in H ε ( R N ) . Repeating the same arguments used in Lemma 2.3, it is easy to see that there exist δ , r > 0 and { y n ˜ } R N satisfying

liminf n B r ( y n ˜ ) u n 2 d x δ .

Letting v n ( x ) = u n ( x + y n ˜ ) , going to a subsequence if necessary, one can suppose that v n v 0 in H ε ( R N ) .

Now we prove that v n v in H ε ( R N ) . Fix t n > 0 satisfying v n ˜ = ( u n ) t n N V 0 . Hence,

c V 0 I V 0 ( v n ˜ ) = I V 0 ( ( u n ) t n ) I ε ( ( u n ) t n ) I ε ( u n ) c V 0 ,

then

I V 0 ( v n ˜ ) c V 0 , { v n ˜ } N V 0 .

Thus, { v n ˜ } is a minimizing sequence. By using Ekeland’s variational principle [17], { v n ˜ } is a bounded ( PS ) c V 0 sequence. And so, v n ˜ v ˜ weakly in H ε ( R N ) , and here, v ˜ 0 , I V 0 ( v ˜ ) = 0 . By applying the arguments from the proof of Lemma 3.3, one can obtain that v n ˜ v ˜ in H ε ( R N ) . Noticing that { t n } is bounded, then we suppose that t n t 0 = 1 ; thus, v n v in H ε ( R N ) .

We clarify that { y n } = { ε n y n ˜ } has a subsequence such that y n y Θ as follows. First, we claim that { y n } is bounded in R N . Arguing by contradiction, if { y n } is unbounded, then there is a subsequence, we denote by { y n } also, satisfying y n . Now we distinguish two cases:

When V = , since

R N V ( ε n x + y n ) v n 2 d x R N v n 2 d x + R N V ( ε n x + y n ) v n 2 d x + R N ( I α v n 2 ) v n 2 d x = R N v n 1 + p d x ,

by Fatou’s lemma, we have

liminf n R N v n 1 + p d x = ,

which contradicts to the boundedness of { v n } in L 1 + p ( R N ) .

When V < , it follows from v n ˜ v ˜ and V 0 < V that

c V 0 = 1 2 v ˜ V 0 2 + 1 4 R N ( I α v ˜ 2 ) v ˜ 2 d x λ 1 + p R N v ˜ 1 + p d x < 1 2 v ˜ V 2 + 1 4 R N ( I α v ˜ 2 ) v ˜ 2 d x λ 1 + p R N v ˜ 1 + p d x liminf n 1 2 R N v n ˜ 2 d x + 1 2 R N V ( ε n x + y n ) v n ˜ 2 d x + 1 4 R N ( I α v n ˜ 2 ) v n ˜ 2 d x λ 1 + p R N v n ˜ 1 + p d x = liminf n t n 2 a + 2 b n b 2 R N u n 2 d x + t n 2 a n b 2 R N V 0 u n 2 d x + t n 4 a α b n b 4 R N ( I α u n 2 ) u n 2 d x λ t n ( 1 + p ) a n b 1 + p R N u n 1 + p d x = liminf n I ε n ( ( u n ) t n ) liminf n I ε n ( u n ) = c V 0 ,

which yields a contradiction. Consequently, the claim holds. Up to a subsequence, y n y in R N . Repeating the aforementioned arguments, one can conclude that y Θ .□

Let ε n 0 as n and u n be the ground state solution of (1.10). From Lemma 3.2, one has

I ε n ( u n ) c V 0 .

Consequently, there exists { y ˜ n } R N satisfying v n = u n ( x + y ˜ n ) be a solution of the equation:

(4.1) Δ v n + V ( ε n x + ε n y ˜ n ) v n + ( I α v n 2 ) v n = λ v n p 1 v n , in R N .

In addition, { v n } has a convergent subsequence in H ε ( R N ) , and y n y Θ .

Lemma 4.2

Assume that ( V ) holds. Then for any n N , there exist C > 0 and δ ¯ > 0 such that δ ¯ v n L ( R N ) C . Moreover,

lim x v n ( x ) = 0 uniformly i n n N .

Proof

For any R > 0 , 0 < r R / 2 , let η C ( R N ) , 0 η 1 with η ( x ) = 1 if x R and η ( x ) = 0 if x R r and η 2 / r . Set

v L , n = v n ( x ) , v n ( x ) L , L , v n ( x ) > L ,

and

z L , n = η 2 v L , n 2 ( γ 1 ) v n , w L , n = η v n v L , n γ 1 ,

where L > 0 , γ > 1 to be determined later. Letting z L , n as a test function, that is, I ε ( u n ) , z L , n = 0 , then

(4.2) R N η 2 v L , n 2 ( γ 1 ) v n 2 d x + R N V ( ε x ) v n 2 η 2 v L , n 2 ( γ 1 ) d x + R N ( I α v n 2 ) η 2 v n 2 v L , n 2 ( γ 1 ) d x = λ R N v n 1 + p η 2 v L , n 2 ( γ 1 ) d x 2 ( γ 1 ) R N v n v L , n 2 γ 3 η 2 v n v L , n d x 2 R N η v L , n 2 ( γ 1 ) v n v n η d x .

By (4.2) and Young’s inequality, for any θ > 0 , one has

R N η 2 v L , n 2 ( γ 1 ) v n 2 d x + R N V 0 v n 2 η 2 v L , n 2 ( γ 1 ) d x λ R N v n 1 + p η 2 v L , n 2 ( γ 1 ) d x + 2 R N η v L , n 2 ( γ 1 ) v n v n η d x λ R N v n 1 + p η 2 v L , n 2 ( γ 1 ) d x + 2 C θ R N v n 2 v L , n 2 ( γ 1 ) η 2 d x + 2 θ R N η 2 v L , n 2 ( γ 1 ) v n 2 d x .

Fix θ = 1 4 , we obtain

(4.3) R N η 2 v L , n 2 ( γ 1 ) v n 2 d x 2 λ R N v n 1 + p η 2 v L , n 2 ( γ 1 ) d x + C R N v n 2 v L , n 2 ( γ 1 ) η 2 d x .

Moreover, it follows from Sobolev’s embedding inequality that

(4.4) w L , n 1 + p 2 C γ 2 R N v n 2 v L , n 2 ( γ 1 ) η 2 d x + R N η 2 v L , n 2 ( γ 1 ) v n 2 d x .

By using (4.3) and (4.4), one has

(4.5) w L , n 1 + p 2 C γ 2 R N v n 2 v L , n 2 ( γ 1 ) η 2 d x + λ R N v n 1 + p η 2 v L , n 2 ( γ 1 ) d x C γ 2 R x R r v n 2 v L , n 2 ( γ 1 ) d x + λ x R r v n 1 + p v L , n 2 ( γ 1 ) d x .

Consequently, from the Hölder inequality, we deduce that

(4.6) w L , n 1 + p 2 C γ 2 R x R r v n 2 γ d x + x R r v n 2 γ + p 1 d x C γ 2 R x R r v n 2 γ t t 1 d x t 1 t R x R r 1 d x 1 t + x R r v n ( p 1 ) t d x 1 t x R r v n 2 γ t t 1 d x t 1 t ,

where t > 1 to be determined later. Furthermore, let γ = ( 1 + p ) / 2 > 1 , by Hölder’s inequality and (4.5), we have

R N ( η v n v L , n 1 + p 2 1 ) 1 + p d x 2 1 + p C γ 2 R N v n 2 v L , n 2 1 + p 2 1 η 2 d x + λ x R 2 v n 1 + p η 2 v L , n 2 1 + p 2 1 d x C γ 2 R N v n 2 v L , n 2 1 + p 2 1 η 2 d x + C γ 2 λ x R 2 v n 1 + p d x p 1 1 + p R N η 1 + p v n 1 + p v L , n ( 1 + p ) 1 + p 2 1 d x 2 1 + p .

Note that v n v in H ε ( R N ) , let 0 < τ ( 2 C ¯ γ 2 ) 1 , for R sufficiently large, one has

x R 2 v n 1 + p d x τ uniformly in n .

Hence, from the definition of w L , n , we obtain

x R ( v n v L , n 1 + p 2 1 ) 1 + p d x 2 1 + p C γ 2 R N v n 2 v L , n 2 1 + p 2 1 η 2 d x C γ 2 R N v n 1 + p d x C .

By Fatou’s lemma, let L , one has

x R v n ( 1 + p ) 2 2 d x < ,

which means v n L ( 1 + p ) 2 2 ( x R ) .

Using (4.6) and Hölder’s inequality, fix γ = p 2 + 3 4 , t = ( 1 + p ) 2 2 ( p 1 ) , then γ > 1 , 2 t t 1 < ( 1 + p ) 2 2 and v n L 2 γ t t 1 ( x R r ) , we have

w L , n 1 + p 2 C γ 2 x R r v n 2 γ t t 1 d x t 1 t .

Hence,

v L , n ( 1 + p ) γ ( x R ) 2 γ x R r v L , n ( 1 + p ) γ d x 2 1 + p R N η 1 + p v n 1 + p v L , n ( 1 + p ) ( γ 1 ) d x 2 1 + p = w L , n 1 + p 2 C γ 2 x R r v n 2 γ t t 1 d x t 1 t = C γ 2 v n 2 γ t t 1 ( x R r ) 2 γ .

By applying Fatou’s lemma, one has

v n ( 1 + p ) γ ( x R ) 2 γ C γ 2 v n 2 γ t t 1 ( x R r ) 2 γ .

By the same arguments used in the proof of [22, Lemma 4.5], set χ = ( 1 + p ) ( t 1 ) 2 t , s = 2 t t 1 , and we conclude that

v n χ m + 1 s ( x R ) C i = 1 m χ i χ i = 1 m i χ i v n 1 + p ( x R r ) ,

which means

(4.7) v n L ( x R ) C v n 1 + p ( x R r ) .

For any x ¯ B R , repeating the aforementioned argument, set η C ( R N ) , 0 η 1 with η ( x ) = 1 if x x ¯ R ¯ and η ( x ) = 0 if x x ¯ > 2 R ¯ and η 2 / R ¯ , we conclude that

(4.8) v n L ( x x ¯ R ¯ ) C v n 1 + p ( x x ¯ 2 R ¯ ) .

Together (4.7) with (4.8), by a standard covering argument, one has

v n L ( R N ) < C .

Furthermore, since v n v in H ε ( R N ) and (4.7), there exist R > 0 and δ > 0 such that v n L ( x R ) < δ . Then,

lim x v n ( x ) = 0 uniformly in n N .

On the other hand, by the same arguments of [1, Lemma 4.4], we have

δ ¯ v n L ( R N ) .

We completes the proof.□

Proof of Theorem 1.1

By Corollary 3.1, we know that there exists a positive ground state solution to problem (1.10). The proof of statements as follows.

We now consider item ( c ) . Let b n be the maximum of v n , then, we obtain the global maximum of u ε n , we denoted it by z n = b n + y ¯ n and ε n z n = ε n b n + ε n y ¯ n = ε n b n + y n . Note that { b n } is bounded, we have

lim n z n = y

and

lim n V ( ε n z n ) = V 0 .

Let u ε be the ground state solution of (1.10), and so w ε ( x ) = u ε ( x ε ) is a ground state solution of (1.1). Then, the maxima points of w ε and u ε , denoted by η ε and ς ε , respectively, satisfy η ε = ε ς ε and

lim ε 0 V ( η ε ) = V 0 .

Consequently, it follows from (4.1) that item ( c ) holds.

For the statement ( d ) , since u ε is the ground state solution of (1.10), we denoted it by u for convenience and fixed ς ε be the maxima point of u , and one has u ( ς ε ) = max x R N u ( x ) . Note that ς ε is bounded, by using Lemma 4.2, we have

u ( x ) 0 as x ς ε .

By the boundedness of u in H ε ( R N ) , we obtain

Δ u = u Δ u u = V ( ε x ) u 2 + ( I α u 2 ) u 2 λ u p u u ( V 0 C ) u ϱ u .

Set w ˜ = u ( x ) C e ϱ ( x ς ε R ¯ ) , here C is given by Lemma 4.2. Hence,

Δ w ˜ ϱ w ˜ , x ς ε R ¯ .

By using the weak maximum principle, one has

w ˜ 0 , x ς ε R ¯ ,

i.e.,

u ( x ) C e ϱ ( x ς ε R ¯ ) , x ς ε R ¯ ,

and thus, item ( d ) holds.□

5 Qualitative behaviors of multiple positive solutions

In this section, we focus on the multiplicity of positive solutions to problem (1.1). Let w be the ground state solution of problem (2.1), φ C ( R + , [ 0 , 1 ] ) be a smooth nonincreasing function satisfy φ ( t ) = 1 on 0 , 1 2 , and φ ( t ) = 0 on [ 1 , ) . For any y Θ , define

Ψ ε , y ( x ) φ ( ε x y ) w ε x y ε

and t ε > 0 such that

I ε ( ( Ψ ε , y ) t ε ) = max t 0 I ε ( ( Ψ ε , y ) t ) .

Meanwhile, we define

Φ ε : Θ N ε , Φ ε ( y ) = ( Ψ ε , y ) t ε .

Lemma 5.1

Assume that ( V ) holds. Then,

lim ε 0 I ε ( Φ ε ( y ) ) = c V 0 uniformly i n y Θ .

Proof

With the reduction to absurdity, we suppose that there exist δ 0 , { y n } Θ and ε n 0 satisfying

(5.1) I ε n ( Φ ε n ( y n ) ) c V 0 δ 0 .

Now we prove lim n t ε n = 1 . In fact, by Lemma 3.1 and the definition of t ε n , we have

α 1 t ε n 2 a + 2 b N b R N Ψ ε n , y n 2 d x + t ε n 2 a N b R N V ( t ε n b ε n x ) ( Ψ ε n , y n ) 2 d x + t ε n 4 a α b N b R N ( I α Ψ ε n , y n 2 ) Ψ ε n , y n 2 d x = λ t ε n ( 1 + p ) a N b R N Ψ ε n , y n 1 + p d x .

Then, t ε n > 0 . If t ε n , it follows from the boundedness of Ψ ε n , y n that

R N Ψ ε n , y n 2 d x + t ε n 2 b R N V ( t ε n b ε n x ) ( Ψ ε n , y n ) 2 d x + R N ( I α Ψ ε n , y n 2 ) Ψ ε n , y n 2 d x = t ε n ( p 1 ) a 2 b λ R N Ψ ε n , y n 1 + p d x > t ε n ( p 1 ) a 2 b λ B 1 2 ( 0 ) φ ( ε n z ) w ( z ) 1 + p d z = t ε n ( p 1 ) a 2 b λ B 1 2 ( 0 ) w 1 + p d x t ε n ( p 1 ) a 2 b λ B 1 2 ( 0 ) w ¯ 1 + p d x ,

where w ¯ = inf x B 1 2 ( 0 ) w ( x ) . Due to t ε n as ε n 0 , the left side of aforementioned inequality tends to R N w 2 d x + λ R N ( I α w 2 ) w 2 d x , which yields a contradiction, and we obtain t ε n C . We may suppose that t ε n t ¯ 0 . By using the similar arguments of Lemma 3.2, we conclude that t ¯ 0 = 1 .

On the other hand,

I ε n ( Φ ε n ( y n ) ) = t ε n 2 a + 2 b N b 2 R N ( φ ( ε n z ) w ) 2 d z + t ε n 2 a N b 2 R N V ( t ε n b ε n z + y n ) φ ( ε n z ) w 2 d z + t ε n 4 a α b N b 4 R N ( I α φ ( ε n z ) w 2 ) φ ( ε n z ) w 2 d z λ t ε n ( 1 + p ) a N b 1 + p R N φ ( ε n z ) w 1 + p d z .

Then lim n I ε n ( Φ ε n ( y n ) ) = c V 0 , which contradicts (5.1). This ends the proof.□

For any δ > 0 , set ρ = ρ ( δ ) > 0 such that Θ δ B ρ ( 0 ) . Now, define ψ : R N R N be such that ψ ( x ) = x for x ρ and ψ ( x ) = ρ x / x for x ρ . Then, we consider the map β ε : N ε R N as follows:

β ε ( u ) = R N ψ ( ε x ) u 4 d x R N u 4 d x .

From Θ B ρ ( 0 ) and the Lebesgue’s theorem, we have

lim ε 0 β ε ( Φ ε ( y ) ) = y uniformly in y Θ .

Lemma 5.2

Assume that ( V ) holds. Then, for any δ > 0 ,

lim ε 0 sup u N ε ˜ dist ( β ε ( u ) , Θ δ ) = 0 ,

where N ε ˜ { u N ε : I ε ( u ) c V 0 + a ( ε ) } , a : R + R + is a positive function such that a ( ε ) 0 as ε 0 .

Proof

Let { ε n } R + such that ε n 0 . By definition, one can see that there exists { u n } N ε n ˜ satisfying

dist ( β ε n ( u n ) , Θ δ ) = sup u N ε n ˜ dist ( β ε n ( u ) , Θ δ ) + o ( 1 ) .

Then, it suffices to verify that there exists a sequence { y n } Θ δ such that

(5.2) β ε n ( u n ) y n = o ( 1 ) .

Since

{ u n } N ε n ˜ N ε n ,

we obtain

c V 0 c ε n I ε n ( u n ) c V 0 + a ( ε n ) .

Thus, I ε n ( u n ) c V 0 . We can invoke Lemma 4.1 to obtain that there is a sequence { y ˜ n } R N verifying y n = ε n y ˜ n Θ δ , for n large enough. Consequently,

β ε n ( u n ) = y n + R N ( ψ ( ε n z + y n ) y n ) u n 4 ( z + y ˜ n ) d z R N u 4 ( z + y ˜ n ) d z .

Note that ε n z + y n y Θ δ , we have β ε n ( u n ) = y n + o ( 1 ) . This completes the proof.□

Lemma 5.3

Assume that ( V ) holds. Let { u n } be the ( PS ) c ε sequence for I ε in N ε . Then { u n } possesses a convergent subsequence in H ε ( R N ) .

Proof

Since { u n } N ε satisfying

I ε ( u n ) c ε , I ε ( u n ) ( H ε ) = o ( 1 ) .

Then, there is { μ n } R such that

(5.3) I ε ( u n ) = μ n J ε ( u n ) + o ( 1 ) ,

where

J ε ( u ) = R N ( u 2 + V ( ε x ) u 2 ) d x + R N ( I α u 2 ) u 2 d x λ R N u 1 + p d x .

Consequently, for 3 p < 2 1 ,

J ε ( u n ) , u n = 2 R N ( u n 2 + V ( ε x ) u n 2 ) d x + 4 R N ( I α u n 2 ) u n 2 d x ( 1 + p ) λ R N u n 1 + p d x [ 4 λ ( 1 + p ) λ ] R N u n 1 + p d x 0 .

We may suppose that J ε ( u n ) , u n l 0 . Now we prove that l 0 . If l = 0 , from the aforementioned inequality, one has u n 0 in L 1 + p ( R N ) , then u n 0 in H ε ( R N ) , which contradicts to Lemma 3.1. Thus, l 0 , and it follows that μ n = o n ( 1 ) . By applying (5.3), we have I ε ( u n ) = o ( 1 ) . Hence, { u n } is a ( PS ) c ε sequence in H ε ( R N ) . By Lemma 3.3, { u n } has a convergent subsequence in H ε ( R N ) . The proof is completed.□

By the similar arguments explored in aforementioned lemmas, we are able to obtain the following result.

Corollary 5.1

Assume that ( V ) holds. Then the critical points of I ε on N ε are critical points of I ε in H ε ( R N ) .

Proof of Theorem 1.2

By Lemmas 5.15.2, one can obtain that β ε Φ ε is homotopically equivalent to the embedding map ι : Θ Θ δ . Then, by using the analogous arguments of the proof of Lemma 4.3 in [7], we have

cat N ε ˜ ( N ε ˜ ) cat Θ δ ( Θ ) .

Since I ε satisfies the ( PS ) c condition for c ( c V 0 , c V 0 + a ( ε ) ) , invoking the Ljusternik-Schnirelmann theory [41], I ε has at least cat Θ δ ( Θ ) critical points in N ε . Thus, by Corollary 5.1, I ε possesses at least cat Θ δ ( Θ ) critical points in H ε ( R N ) . Furthermore, by repeating the proof of Theorem 1.1, we obtain that the positive solutions satisfy concentration behavior and exponential decay.□

Acknowledgments

All authors would like to express their sincere gratitude to the anonymous reviewers for their helpful suggestions and comments.

  1. Funding information: The research of Binlin Zhang was supported by National Natural Science Foundation of China (Nos. 11871199 and 12171152) and Cultivation Project of Young and Innovative Talents in Universities of Shandong Province.

  2. Conflict of interest: The authors declare that this work does not have any conflict of interest.

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Received: 2022-11-06
Revised: 2022-12-31
Accepted: 2023-01-24
Published Online: 2023-02-25

© 2023 the author(s), published by De Gruyter

This work is licensed under the Creative Commons Attribution 4.0 International License.

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