Startseite Multiplicity and concentration behavior of solutions for the generalized quasilinear Schrödinger equation with critical growth
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Multiplicity and concentration behavior of solutions for the generalized quasilinear Schrödinger equation with critical growth

  • Yongpeng Chen und Zhipeng Yang EMAIL logo
Veröffentlicht/Copyright: 8. Oktober 2025
Veröffentlichen auch Sie bei De Gruyter Brill

Abstract

In this study, we are interested in multiplicity results for positive solutions of the generalized quasilinear Schrödinger equations with critical growth

div ( g 2 ( u ) u ) + g ( u ) g ( u ) u 2 + V ( ε x ) u = u α p 2 u + Q ( ε x ) u α 2 * 2 u , x R N ,

where g C 1 ( R , R + ) , α [ 1 , 2 ] , 2 < p < 2 * , and ε > 0 is a parameter. Under suitable assumptions on g , V , and Q , we obtain the concentration behavior of positive solutions for ε > 0 small and establish the relationship between the number of positive solutions and the profiles of potentials V and Q using variational methods.

MSC 2020: 35J62; 35J50; 35B65

1 Introduction and main results

The multiple solutions to the following generalized quasilinear Schrödinger equation in R N are the focus of this work:

(1.1) div ( g 2 ( u ) u ) + g ( u ) g ( u ) u 2 + V ( ε x ) u = u α p 2 u + Q ( ε x ) u α 2 * 2 u , x R N ,

where g C 1 ( R , R + ) , α [ 1 , 2 ] , 2 < p < 2 * , and ε > 0 is a parameter.

Equation (1.1) is closely related to the existence of standing wave solutions to the quasilinear Schrödinger equation of the form

(1.2) i t z = Δ z + W ( x ) z h ( x , z ) z κ Δ ( l ( z 2 ) ) l ( z 2 ) z ,

where κ R + , z : R × R N C , W : R N R is a given potential and l , h are real functions in R + . Let z ( t , x ) = exp ( i E t ) u ( x ) , where E R and u is a real function. Then, we can obtain an equation of the form

(1.3) Δ u κ Δ l ( u 2 ) l ( u 2 ) u + V ( x ) u = f ( x , u ) , x R N

for some functions V : R N R and f : R N × R R . Several physical phenomena that correlate with various types of l ( s ) can be modeled using equation (1.3). Specifically, if l ( s ) = s , then equation (1.3) becomes

(1.4) Δ u κ Δ ( u 2 ) u + V ( x ) u = f ( x , u ) , x R N ,

which is called the superfluid film equation in plasma physics [1,2]. If l ( s ) = 1 + s , problem (1.3) turns into

(1.5) Δ u κ [ Δ ( 1 + u 2 ) ] u 2 1 + u 2 + V ( x ) u = f ( x , u ) , x R N ,

which describes the self-channeling of a high power ultrashort laser in matter [3,4]. For the further physical background, we refer the readers to [58] and references therein.

It is important to note that dealing with the quasilinear Schrödinger equations (1.4) in R N presents a number of challenges, including lack of compactness and the existence of the term Δ ( u 2 ) u that inhibits us from working directly in a classical working space. In light of this, challenging tasks, tricky to be managed, appear. To the best of our knowledge, a constrained minimization technique was used by Poppenberg et al. [8] to obtain the existence results for quasilinear equations of the type similar to (1.4). Using a change in variables, Liu et al. [9] investigated (1.4), which transformed into semilinear. The existence of a positive solution has been shown using the mountain pass theorem in an Orlicz space. Additionally, they discovered that 2 2 * behaves similar to a critical exponent. Later, Colin and Jeanjean [10] introduced a dual technique, which allows problems of the kind (1.4) to be solved in H 1 ( R N ) rather than the Orlicz space.

The technique of changing variables proposed in [9] and [10] works incredibly well for solving the problem (1.4). For instance, do Ó et al. [11] took into consideration the critical growth problem (1.4). A positive solution was obtained by applying the concentration-compactness principle and the mountain pass theory. He et al. [12] analyzed the quasilinear issues’ semiclassical states. The authors established ground state existence, multiplicity, and concentration behavior using variational methods and Lusternik-Schnirelmann theory.

Concerning the quasilinear Schrödinger equation with steep potential well, Guo and Tang [13] participated in it. They established the existence of a ground state solution that localizes close to the bottom of the potential well for sufficiently large parameters by applying the variational approach and the concentration compactness method in Orlicz space. In R N , quasilinear Schrödinger equations with an indefinite potential were studied by Liu and Zhou [14]. Using Morse theory and a local linking argument, they were able to obtain a nontrivial solution for this problem. For more results about problems (1.4) and (1.5), refer [1522] and references therein.

In particular, equation (1.3) is a special case of the following generalized quasilinear elliptic equations:

(1.6) div ( g 2 ( u ) u ) + g ( u ) g ( u ) u 2 + V ( x ) u = f ( x , u ) , x R N ,

if one takes

g 2 ( u ) = 1 + ( [ l ( u 2 ) ] ) 2 2 κ .

For the generalized quasilinear equation (1.6), by introducing a new variable replacement v = G ( u ) = 0 u g ( s ) d s , Shen and Wang [23] reduced (1.6) to a semilinear elliptic equation

Δ v + V ( x ) G 1 ( v ) g ( G 1 ( v ) ) = f ( x , G 1 ( v ) ) g ( G 1 ( v ) ) .

Positive solutions were obtained when the nonlinearity is subcritical, as a result of the use of the mountain pass theorem. Deng et al. [24] subsequently studied the generalized quasilinear Schrödinger equations (1.6) including critical growth by using the same change in variable. Through the addition of a suitable condition, they proved that, for some α 1 , α 2 * is the critical exponent for problem (1.6) if lim s + g ( s ) s α 1 β > 0 . Fang and Liu [25] developed multiple localized solutions of higher topological type centered around the set of critical points of the potential function by employing a form of the penalization argument. Chen et al. [26] investigated the generalized quasilinear Schrödinger equation with critical growth and found the existence and concentration behavior of ground state solutions via the Nehari manifold approach. Moreover, it was demonstrated that there are multiple solutions by Lusternik-Schnirelmann theory. After studying the generalized quasilinear Schrödinger equations that include several competing potentials and critical growth, Li et al. [27] were able to establish the existence and concentration of positive solutions. Please refer [2831] for additional results about (1.6).

Motivated by the aforementioned results, the main purpose of this study is to prove the existence of multiple positive solutions and their concentration behavior to problem (1.1). The current study draws motivation from several ideas presented by Cao and Noussair [32], Meng and He [33], and Zhang and Zou [34]. By using variational methods, they have showed how the profiles of potentials affect the number of positive solutions. However, since we are working with a large class of quasilinear operators, some estimates which hold for (1.4) are not immediate for the general equation (1.1), and so, we must be careful to obtain some of them.

To obtain the main results, we give some assumptions about g , V , and Q .

  1. V ( x ) is locally Hölder continuous, inf x R N V ( x ) = V 0 > 0 , and lim x V ( x ) = V < + .

  2. There exists x i R N satisfying V ( x i ) = V 0 , and it is a strict global minima of V ( x ) , where i = 1 , 2 , , k .

  3. Q ( x ) is locally Hölder continuous, 0 Q ( x ) Q 0 , lim x Q ( x ) = Q > 0 and Q ( x i ) = Q 0 , i = 1 , 2 , , k .

  4. g C 1 ( R , R + ) is an even function, g ( 0 ) = 1 , g ( s ) 0 for all s 0 , g ( s ) = β s α 1 + O ( s γ 1 ) as s for some constants α [ 1 , 2 ] , β > 0 , γ < α , and ( α 1 ) g ( s ) g ( s ) s for all s 0 ,

Now, we can state our main results as follows.

Theorem 1.1

Let N 2 + 4 α α γ + ( γ + = max { γ , 0 } ) , and assume that ( g ) , ( V 1 ) , ( V 2 ) , and ( Q ) hold. Then, there is ε * > 0 such that problem (1.1) has at least k positive solutions u ε i , i = 1 , 2 , , k , for 0 < ε < ε * , and each u ε i possesses a maximum point y ε i R N satisfying V ( ε y ε i ) V 0 and Q ( ε y ε i ) Q 0 as ε 0 . Moreover, there exist constants C i , c i > 0 such that

u ε i ( x ) C i exp ( c i x y ε i )

for ε ( 0 , ε * ) and x R N .

This study is organized as follows. In Section 2, we give preliminary Lemmas, which will be used later. In Section 3, we prove the existence of k positive solutions associated with (1.1). In Section 4, we establish the concentration behavior of these solutions.

Notation. In this study, we make use of the following notations.

  • B R ( x ) denotes the open ball of radius R centered at x , where R > 0 and x R N , and B R ( x ) denotes the boundary of B R ( x ) .

  • The letters C and C i , i N + stand for any positive constants.

  • ” and “ ” represent strong convergence and weak convergence, respectively.

  • o n ( 1 ) is a quantity tending to 0 as n , and o ε ( 1 ) is a quantity tending to 0 as ε 0 .

  • m ( Ω ) is the Lebesgue measure of Ω R N .

  • S = inf u D 1 , 2 ( R N ) \ { 0 } R N u 2 d x R N u 2 * d x 2 2 * denotes the best Sobolev constant, where 2 * = 2 N N 2 .

2 Preliminaries

In what follows, we will use the working space E H 1 ( R N ) endowed with the standard norm

v = R N v 2 + v 2 1 2 .

Since V is bounded and inf x R N V ( x ) > 0 , for any ε > 0 ,

v ε = R N v 2 + V ( ε x ) v 2 1 2

is equivalent to the standard norm in E . Particularly, for any d > 0 ,

v d = R N v 2 + d v 2 1 2

is also an equivalent norm in E . First, the associated energy functional with equation (1.1) is

I ε ( u ) = 1 2 R N ( g 2 ( u ) u 2 + V ( ε x ) u 2 ) 1 α p R N u α p 1 α 2 * R N Q ( ε x ) u α 2 * .

However, I ε is not well defined in E because of the term R N g 2 ( u ) u 2 . In terms of the change in variable in [23]

v G ( u ) 0 u g ( t ) d t ,

we can obtain

(2.1) J ε ( v ) = 1 2 R N ( v 2 + V ( ε x ) G 1 ( v ) 2 ) 1 α p R N G 1 ( v ) α p 1 α 2 * R N Q ( ε x ) G 1 ( v ) α 2 * .

Then, Lemma 2.2, ensures that the functional J ε is well defined in E . If u is a critical point of (2.1), we have

J ε ( v ) , ψ = R N v ψ + V ( ε x ) G 1 ( v ) g ( G 1 ( v ) ) ψ G 1 ( v ) α p 2 G 1 ( v ) g ( G 1 ( v ) ) ψ Q ( ε x ) G 1 ( v ) α 2 * 2 G 1 ( v ) g ( G 1 ( v ) ) ψ = 0

for all ψ C 0 ( R N ) . Therefore, in order to find the solutions of (1.1), it suffices to study the solutions of the equation

(2.2) Δ v + V ( ε x ) G 1 ( v ) g ( G 1 ( v ) ) G 1 ( v ) α p 2 G 1 ( v ) g ( G 1 ( v ) ) Q ( ε x ) G 1 ( v ) α 2 * 2 G 1 ( v ) g ( G 1 ( v ) ) = 0 , x R N .

Remark 2.1

Since we shall find the positive solutions to problem (1.1), we can rewrite the functional J ε in (2.1) as follows:

J ε ( v ) = 1 2 R N v 2 + V ( ε x ) G 1 ( v ) 2 1 α p R N G 1 ( v + ) α p 1 α 2 * R N Q ( ε x ) G 1 ( v + ) α 2 * ,

where v + max { v , 0 } . If v E is a nontrivial critical point of J ε and let v = min { v , 0 } , then we can obtain

0 = J ε ( v ) , v = R N v v + V ( ε x ) G 1 ( v ) g ( G 1 ( v ) ) v G 1 ( v + ) α p 2 G 1 ( v + ) g ( G 1 ( v + ) ) v Q ( ε x ) G 1 ( v + ) α 2 * 2 G 1 ( v + ) g ( G 1 ( v + ) ) v = R N v 2 + G 1 ( v ) g ( G 1 ( v ) ) v ,

which implies that v = 0 . From the theory of elliptic regularity, we see that v C 2 ( R N ) . Then, by using strong maximum principle, we obtain v > 0 in R N .

Lemma 2.2

The functions g , G , and G 1 have the following properties:

  1. G ( ) and G 1 ( ) are strictly increasing and odd;

  2. G ( s ) g ( s ) s α G ( s ) for all s 0 ; α G ( s ) g ( s ) s G ( s ) for all s 0 ;

  3. g ( G 1 ( s ) ) g ( 0 ) = 1 for all s R ;

  4. G 1 ( s ) s is decreasing on ( 0 , + ) and increasing on ( , 0 ) ;

  5. G 1 ( s ) 1 g ( 0 ) s = s for all s R ;

  6. G 1 ( s ) g ( G 1 ( s ) ) 1 g 2 ( 0 ) s = s for all s R ;

  7. G 1 ( s ) s g ( G 1 ( s ) ) G 1 ( s ) 2 α G 1 ( s ) s g ( G 1 ( s ) ) for all s R ;

  8. lim s 0 G 1 ( s ) s = 1 g ( 0 ) = 1 and

    lim s G 1 ( s ) s = 1 g ( ) , if g is b o u n d e d , 0 , if g is u n b o u n d e d ;

  9. s α α β G ( s ) for all s R ;

  10. ( G 1 ( s ) ) q s g ( G 1 ( s ) ) is increasing on ( 0 , + ) for q > 2 α 1 ;

  11. lim s + G ( s ) s α = β α .

Proof

For the proof of (1)–(9), we refer to [35] and [27]. For (10), let l ( s ) = ( G 1 ( s ) ) q s g ( G 1 ( s ) ) , s > 0 . Using ( α 1 ) g ( s ) g ( s ) s and (2), we have

l ( s ) = ( G 1 ( s ) ) q 1 s q g ( G 1 ( s ) ) G 1 ( s ) s g ( G 1 ( s ) ) G 1 ( s ) g ( G 1 ( s ) ) s 2 g 2 ( G 1 ( s ) ) ( G 1 ( s ) ) q 1 [ s q g ( G 1 ( s ) ) G 1 ( s ) ( α 1 ) s ] s 2 g 2 ( G 1 ( s ) ) ( G 1 ( s ) ) q 1 [ s q α s ( α 1 ) s ] s 2 g 2 ( G 1 ( s ) ) = ( G 1 ( s ) ) q 1 ( q + 1 2 α ) s g 2 ( G 1 ( s ) ) > 0 .

As for ( 11 ) , noting γ < α ,

lim s + G ( s ) s α = lim s + g ( s ) α s α 1 = lim s + β s α 1 + O ( s γ 1 ) α s α 1 = β α .

From Lemma 2.2, J ε is well defined in E and J ε C 1 ( E , R ) . Define the Nehari manifold

N ε = { v E \ { 0 } J ε ( v ) , v = 0 }

and

c ε = inf v N ε J ε ( v ) .

Set

k 1 , ε ( x , s ) V ( ε x ) s G 1 ( s ) g ( G 1 ( s ) )

and

k 2 , ε ( x , s ) G 1 ( s ) α p 2 G 1 ( s ) g ( G 1 ( s ) ) + Q ( ε x ) G 1 ( s ) α 2 * 2 G 1 ( s ) g ( G 1 ( s ) ) α 2 * 1 β 2 * s 2 * 2 s .

Then,

K 1 , ε ( x , s ) 0 s k 1 , ε ( x , τ ) d τ = 1 2 V ( ε x ) [ s 2 G 1 ( s ) 2 ]

and

K 2 , ε ( x , s ) 0 s k 2 , ε ( x , τ ) d τ = 1 α p G 1 ( s ) α p + 1 α 2 * Q ( ε x ) G 1 ( s ) α 2 * α 2 * 1 2 * β 2 * Q ( ε x ) s 2 * .

Thus,

J ε ( v ) = 1 2 R N ( v 2 + V ( ε x ) v 2 ) R N K 1 , ε ( x , v ) R N K 2 , ε ( x , v + ) α 2 * 1 2 * β 2 * R N Q ( ε x ) v + 2 * = 1 2 v ε R N K 1 , ε ( x , v ) R N K 2 , ε ( x , v + ) α 2 * 1 2 * β 2 * R N Q ( ε x ) v + 2 * .

Lemma 2.3

The functions k i , ε ( x , s ) and K i , ε ( x , s ) , i = 1 , 2 , have the following properties:

  1. lim s 0 k i , ε ( x , s ) s = 0 and lim s 0 K i , ε ( x , s ) s 2 = 0 uniformly in x R N .

  2. lim s k i , ε ( x , s ) s 2 * 1 = 0 and lim s K i , ε ( x , s ) s 2 * = 0 uniformly in x R N .

Proof

Similar to the proof of Lemma 2.2 in [24], we can obtain the results.□

Lemma 2.4

Given v E with v + 0 , there exists a unique t v > 0 such that t v v N ε . Moreover, J ε ( t v v ) = max t 0 J ε ( t v ) .

Proof

Using Lemma 2.3, for any δ > 0 , there exists C δ > 0 such that

K 1 , ε ( x , s ) + K 2 , ε ( x , s ) δ s 2 + C δ s 2 * .

Therefore, for t > 0 ,

h ( t ) J ε ( t v ) = t 2 2 v ε 2 R N K 1 , ε ( x , t v ) R N K 2 , ε ( x , t v + ) α 2 * 1 t 2 * β 2 * 2 * R N Q ( ε x ) v + 2 * t 2 2 v ε 2 δ t 2 R N v 2 C δ + α 2 * 1 β 2 * 2 * t 2 * Q 0 R N v 2 * t 2 2 v ε 2 δ C t 2 v ε 2 C t 2 * v ε 2 * .

When δ is small enough, we can obtain h ( t ) > 0 for small t . On the other hand, since v + 0 , there exists γ > 0 such that m ( Ω ) > 0 , where Ω { x R N : v + ( x ) γ } . Using (5) and ( 11 ) of Lemma 2.2, for t large enough, one has

h ( t ) = 1 2 R N ( t v ) 2 + V ( ε x ) G 1 ( t v ) 2 1 α p R N G 1 ( t v + ) α p 1 α 2 * R N Q ( ε x ) G 1 ( t v + ) α 2 * 1 2 t 2 v ε 2 1 α p Ω G 1 ( t v + ) α p 1 2 t 2 v ε 2 C t p Ω v + p .

It follows that h ( t ) as t + .

Therefore, there exists a t v > 0 such that h ( t v ) = 0 , that is, t v v N ε . Furthermore, h ( t v ) = max t 0 h ( t ) . From h ( t ) = 0 , we have

R N v 2 = R N V ( ε x ) G 1 ( t v ) t g ( G 1 ( t v ) ) v + R N G 1 ( t v + ) α p 2 G 1 ( t v + ) t g ( G 1 ( t v + ) ) v + + R N Q ( ε x ) G 1 ( t v + ) α 2 * 2 G 1 ( t v + ) t g ( G 1 ( t v + ) ) v + = R N V ( ε x ) G 1 ( t v ) t v g ( G 1 ( t v ) ) v 2 + R N G 1 ( t v + ) α p 1 t v + g ( G 1 ( t v + ) ) ( v + ) 2 + R N Q ( ε x ) G 1 ( t v + ) α 2 * 1 t v + g ( G 1 ( t v + ) ) ( v + ) 2 .

In terms of (1), (4), and (10) of Lemma 2.2, we know that

V ( ε x ) G 1 ( s ) s g ( G 1 ( s ) ) , G 1 ( s ) α p 1 s g ( G 1 ( s ) ) , and Q ( ε x ) G 1 ( s ) α 2 * 1 s g ( G 1 ( s ) )

are increasing with respect to s ( 0 , + ) . Then, the uniqueness of t v can be obtained.□

Lemma 2.5

There is a positive constant θ independent of ε , such that v ε θ , v N ε .

Proof

By Lemma 2.3, for any δ > 0 , there exists C δ > 0 such that

k 1 , ε ( x , s ) s + k 2 , ε ( x , s ) s δ s 2 + C δ s 2 * .

For v N ε , one has

v ε 2 = R N k 1 , ε ( x , v ) v + R N k 2 , ε ( x , v + ) v + + α 2 * 1 β 2 * R N Q ( ε x ) v + 2 * δ R N v 2 + C δ + α 2 * 1 β 2 * C R N v 2 * .

Then, we have

( 1 C δ ) v ε 2 C v ε 2 * .

Therefore, there exists θ > 0 such that

v ε θ .

On the other hand, for v N ε , by (7) of Lemma 2.2,

J ε ( v ) 1 2 R N ( v 2 + V ( ε x ) G 1 ( v ) 2 ) 1 p R N G 1 ( v + ) α p 2 G 1 ( v + ) g ( G 1 ( v + ) ) v + 1 2 * R N Q ( ε x ) G 1 ( v + ) α 2 * 2 G 1 ( v + ) g ( G 1 ( v + ) ) v + 1 2 R N ( v 2 + V ( ε x ) G 1 ( v ) 2 ) 1 p R N v 2 + V ( ε x ) G 1 ( v ) g ( G 1 ( v ) ) v 1 2 R N ( v 2 + V ( ε x ) G 1 ( v ) 2 ) 1 p R N ( v 2 + V ( ε x ) G 1 ( v ) 2 ) = 1 2 1 p R N ( v 2 + V ( ε x ) G 1 ( v ) 2 ) .

Lemma 2.6

Suppose that { v n } is a ( PS ) c sequence for J ε . Then, { v n } is bounded in E.

Proof

Let ω n = g ( G 1 ( v n ) ) G 1 ( v n ) . Then,

ω n 2 = 1 + g ( G 1 ( v n ) ) G 1 ( v n ) g ( G 1 ( v n ) ) 2 v n 2 α 2 v n 2

and

ω n 2 = ( g ( G 1 ( v n ) ) G 1 ( v n ) ) 2 α 2 v n 2 ,

which imply that

ω n ε α v n ε .

Therefore,

J ε ( v n ) , ω n = o n ( 1 ) ,

and then

J ε ( v n ) 1 α p J ε ( v n ) , ω n = R N 1 2 1 α p 1 + g ( G 1 ( v n ) ) G 1 ( v n ) g ( G 1 ( v n ) ) v n 2 + 1 2 1 α p R N V ( ε x ) G 1 ( v n ) 2 + 1 α p 1 α 2 * R N Q ( ε x ) G 1 ( v n ) α 2 * = c + o n ( 1 ) + o n ( 1 ) v n ε .

It follows from ( α 1 ) g ( s ) g ( s ) s that

(2.3) limsup n R N ( v n 2 + V ( ε x ) G 1 ( v n ) 2 ) 2 p c p 2 .

Next we prove that { v n } is bounded in E . We just need to show that { v n } is bounded in L 2 ( R N ) . In fact, by (4) in Lemma 2.2 and the definition of S , one has

{ x R N : v n > 1 } v n 2 { x R N : v n > 1 } v n 2 * R N v n 2 * 1 S R N v n 2 2 * 2

and

{ x R N : v n 1 } v n 2 1 G 1 ( 1 ) 2 { x R N : v n 1 } G 1 ( v n ) 2 1 G 1 ( 1 ) 2 R N G 1 ( v n ) 2

It follows from (2.3) that { v n } is bounded in E .□

Remark 2.7

From the proof of Lemma 2.6, we can obtain that there exist C > 0 , such that, for any v E ,

v ε 2 C max R N v 2 + V ( ε x ) G 1 ( v ) 2 , R N v 2 + V ( ε x ) G 1 ( v ) 2 N N 2 ,

and, by (5) of Lemma 2.2,

R N v 2 + V ( ε x ) G 1 ( v ) 2 v ε 2 .

Lemma 2.8

For u N ε , we have L ε ( u ) , u < 0 , where L ε ( u ) = J ε ( u ) , u .

Proof

For u 0 and u E \ { 0 } , define H t ( u ) = R N ( G 1 ( u ) ) t 1 u g ( G 1 ( u ) ) , where t > 2 . Then, using (2) and (7) of Lemma 2.2 and ( α 1 ) g ( s ) g ( s ) s for all s 0 ,

(2.4) H t ( u ) , u = R N ( t 1 ) ( G 1 ( u ) ) t 2 u 2 g 2 ( G 1 ( u ) ) + ( G 1 ( u ) ) t 1 u g ( G 1 ( u ) ) ( G 1 ( u ) ) t 1 u 2 g ( G 1 ( u ) ) g 3 ( G 1 ( u ) ) R N ( t 1 ) ( G 1 ( u ) ) t 2 u 2 g 2 ( G 1 ( u ) ) + ( G 1 ( u ) ) t 1 u g ( G 1 ( u ) ) ( α 1 ) ( G 1 ( u ) ) t 2 u 2 g 2 ( G 1 ( u ) ) = R N ( t α ) ( G 1 ( u ) ) t 2 u 2 g 2 ( G 1 ( u ) ) + ( G 1 ( u ) ) t 1 u g ( G 1 ( u ) ) R N ( t α ) ( G 1 ( u ) ) t 1 u α g ( G 1 ( u ) ) + ( G 1 ( u ) ) t 1 u g ( G 1 ( u ) ) = t α R N ( G 1 ( u ) ) t 1 u g ( G 1 ( u ) ) .

For u E \ { 0 } , define H 2 ( u ) = R N V ( ε x ) G 1 ( u ) u g ( G 1 ( u ) ) . In terms of (2) of Lemma 2.2, we have

(2.5) H 2 ( u ) , u = R N V ( ε x ) u 2 g 2 ( G 1 ( u ) ) + G 1 ( u ) u g ( G 1 ( u ) ) G 1 ( u ) u 2 g ( G 1 ( u ) ) g 3 ( G 1 ( u ) ) R N V ( ε x ) u 2 g 2 ( G 1 ( u ) ) + G 1 ( u ) u g ( G 1 ( u ) ) R N V ( ε x ) G 1 ( u ) u g ( G 1 ( u ) ) + G 1 ( u ) u g ( G 1 ( u ) ) = 2 R N V ( ε x ) G 1 ( u ) u g ( G 1 ( u ) ) .

Then, for u N ε , by (2.4) and (2.5), we have

(2.6) L ε ( u ) , u = 2 R N u 2 + H ( u ) , u H ( u + ) , u H ˜ ( u ) , u 2 R N u 2 + 2 R N V ( ε x ) G 1 ( u ) u g ( G 1 ( u ) ) α p α R N ( G 1 ( u + ) ) α p 1 u + g ( G 1 ( u + ) ) α 2 * α R N Q ( ε x ) ( G 1 ( u + ) ) α 2 * 1 u + g ( G 1 ( u + ) ) 2 R N u 2 + 2 R N V ( ε x ) G 1 ( u ) u g ( G 1 ( u ) ) p R N u 2 + R N V ( ε x ) G 1 ( u ) u g ( G 1 ( u ) ) = ( 2 p ) R N u 2 + R N V ( ε x ) G 1 ( u ) u g ( G 1 ( u ) ) < 0 ,

where H ˜ α 2 * ( u ) = R N Q ( ε x ) ( G 1 ( u + ) ) α p 1 u + g ( G 1 ( u + ) ) .□

For any a , b > 0 , we consider the following constant coefficient equation

(2.7) Δ v + a G 1 ( v ) g ( G 1 ( v ) ) G 1 ( v ) α p 2 G 1 ( v ) g ( G 1 ( v ) ) b G 1 ( v ) α 2 * 2 G 1 ( v ) g ( G 1 ( v ) ) = 0 , x R N .

Define the energy functional

J a , b ( v ) 1 2 R N ( v 2 + a G 1 ( v ) 2 ) 1 α p R N G 1 ( v + ) α p b α 2 * R N G 1 ( v + ) α 2 * .

The associated Nehari manifold can be defined as

a , b = { v E \ { 0 } J a , b ( v ) , v = 0 } .

Set

m a , b = inf v a , b J a , b ( v ) .

For simplicity, when a = V 0 and b = Q 0 , we shall use J 0 , 0 , and m 0 to represent J a , b , a , b , and m a , b , respectively. Similarly, for a = V and b = Q , we are going to use J , , and m .

Remark 2.9

J a , b , a , b , and m a , b have similar properties from Lemmas 2.4 to 2.8.

Lemma 2.10

Let a , b > 0 , then

m a , b < β N N α N + 2 2 b N 2 2 S N 2 ,

and equation (2.7) possesses a positive ground state solution.

Proof

Since N 2 + 4 α α γ + and 2 < p < 2 * , from Lemma 2.5 in [36], the first part can be obtained. We can choose a sequence { u n } a , b such that J a , b ( u n ) m a , b . It follows from Ekeland’s variational principle that there exist { θ n } R and { v n } a , b such that

v n u n = o n ( 1 ) , J a , b ( v n ) = θ n L a , b ( v n ) + o n ( 1 ) , J a , b ( v n ) = m a , b + o n ( 1 ) ,

where L d ( v ) = J d ( v ) , v . It follows from v n d and Lemma 2.8 that

L a , b ( v n ) , v n < 0 .

If L a , b ( v n ) , v n 0 , by (2.6) and Remark 2.7, we have

v n 0 ,

which contradicts Lemma 2.5. Consequently, from 0 = J a , b ( v n ) , v n , we have θ n = o n ( 1 ) . Therefore, J a , b ( v n ) = o n ( 1 ) . Thus, by Lemma 2.6, we see that { v n } is bounded in E and there exists v E such that v n v in E , v n v almost everywhere in R N and J a , b ( v ) = 0 . We next distinguish the following two cases:

Case 1. v 0 . Noting J a , b ( v ) = 0 , we have v a , b . Then,

m a , b J a , b ( v ) 1 α p J a , b ( v ) , g ( G 1 ( v ) ) G 1 ( v ) = R N 1 2 1 α p 1 + g ( G 1 ( v ) ) G 1 ( v ) g ( G 1 ( v ) ) v 2 + 1 2 1 α p R N a G 1 ( v ) 2 + 1 α p 1 α 2 * R N b G 1 ( v ) α 2 * liminf n R N 1 2 1 α p 1 + g ( G 1 ( v n ) ) G 1 ( v n ) g ( G 1 ( v n ) ) v n 2 + 1 2 1 α p R N a G 1 ( v n ) 2 + 1 α p 1 α 2 * R N b G 1 ( v n ) α 2 * = lim n J a , b ( v n ) 1 α p J a , b ( v n ) , g ( G 1 ( v n ) ) G 1 ( v n ) = m a , b ,

which means that

J a , b ( v ) = m a , b .

Let ω n = v n v . It follows from Lemma 2.5 of [24] that

J a , b ( ω n ) 0 and J a , b ( ω n ) 0 .

Thus,

o n ( 1 ) = J a , b ( ω n ) 1 α p J a , b ( ω n ) , g ( G 1 ( ω n ) ) G 1 ( ω n ) = R N 1 2 1 α p 1 + g ( G 1 ( ω n ) ) G 1 ( ω n ) g ( G 1 ( ω n ) ) ω n 2 + 1 2 1 α p R N a G 1 ( ω n ) 2 + 1 α p 1 α 2 * R N b G 1 ( w n ) α 2 * .

This, combining with ( α 1 ) g ( s ) g ( s ) s for all s 0 , leads to

lim n R N ω n 2 + G 1 ( ω n ) 2 = 0 .

From Remark 2.7, we deduce that

v n v in E .

Case 2. v = 0 . In this case, we claim that there exist R , η > 0 , and { y n } R N such that

limsup n B R ( y n ) v n 2 d x η > 0 .

Otherwise, we have

limsup n B R ( y n ) v n 2 d x = 0 .

Using Lions lemma, we have

v n 0 in L t ( R N ) for t ( 2 , 2 * ) .

For simplicity, let V ( ε x ) = a and Q ( ε x ) = b . By Lemma 2.3, for any δ > 0 , there exists C δ > 0 such that

K 1 , ε ( x , v n ) + K 2 , ε ( x , v n + ) δ ( v n 2 * + v n 2 ) + C δ v n p , k 1 , ε ( x , v n ) v n + k 2 , ε ( x , v n + ) v n δ ( v n 2 * + v n 2 ) + C δ v n p .

Thus, one has

R N K 1 , ε ( x , v n ) + K 2 , ε ( x , v n + ) = o n ( 1 ) , R N k 1 , ε ( x , v n ) v n + k 2 , ε ( x , v n + ) v n = o n ( 1 ) .

Then,

J a , b ( v n ) = 1 2 v a 2 α 2 * 1 β 2 * 2 * R N b v n + 2 * + o n ( 1 )

and

J a , b ( v n ) , v n = v a 2 α 2 * 1 β 2 * R N b v n + 2 * + o n ( 1 ) .

Assume that v a 2 l and α 2 * 1 β 2 * R N b v n + 2 * l . It follows from the definition of S that

S R N v n + 2 * 2 2 * R N v n 2 v a 2 .

Letting n ,

S β 2 * b α 2 * 1 l 2 2 * l

Thus, l = 0 or l β N α N + 2 2 b N 2 2 S N 2 . If l = 0 , we can deduce a contradiction with m a , b > 0 . Therefore, l β N α N + 2 2 b N 2 2 S N 2 . Then, we can deduce that

m a , b 1 2 1 2 * l 1 N β N α N + 2 2 b N 2 2 S N 2 ,

which is a contradiction.

Letting w n ( x ) = v n ( x + y n ) , we can obtain J a , b ( w n ) m a , b and J a , b ( w n ) 0 . Then, { w n } is bounded in E and there exists w E with w 0 such that w n w in E , w n w almost everywhere in R N and J a , b ( w ) = 0 . Then,

w n w , in E ,

follows from the same arguments used in Case 1. Moreover, y n . Suppose by contradiction that { y n } is a bounded, passing to a subsequence if necessary, then there exists R > 0 such that B R ( y n ) B R ( 0 ) . Therefore, for n N , we have

B R ( 0 ) v n 2 d x η > 0 .

It follows from v n 0 in E that v n 0 in L 2 ( B R ( 0 ) ) , which contradicts the above inequality.□

Lemma 2.11

If min { a 2 a 1 , b 1 b 2 } 0 , then m a 1 , b 1 m a 2 , b 2 . Moreover, if additionally max { a 2 a 1 , b 1 b 2 } > 0 , then m a 1 , b 1 < m a 2 , b 2 .

Proof

We refer to the proof of Lemma 2.12 in [27].□

Lemma 2.12

c ε m 0 .

Proof

From the definition of c ε , for any η > 0 , there exists v η N ε such that c ε > J ε ( v η ) η . It follows from Lemma 2.4 that there exists a unique t η > 0 satisfying t η v η 0 . Noting V ( ε x ) V 0 and Q ( ε x ) Q 0 , we can deduce that

c ε + η > J ε ( v η ) = sup t 0 J ε ( t v η ) J ε ( t η v η ) J 0 ( t η v η ) m 0 .

Sending η 0 in the above inequality, we can complete the proof.□

3 Existence of multiple solutions

By conditions ( V 1 ) and ( V 2 ) , we can choose r 0 > 0 such that B r 0 ( x i ) ¯ B r 0 ( x j ) ¯ = for i j , i , j { 1 , , k } , and V ( x ) > V ( x i ) for x B r 0 ( x i ) ¯ \ { x i } . Define β ε : E \ { 0 } R N by

β ε ( v ) = R N χ ( ε x ) v 2 d x R N v 2 d x ,

where χ : R N R N is given by

χ ( x ) = x , if x r , r x x , if x > r ,

where r > max { x 1 + r 0 , x 2 + r 0 , , x k + r 0 } . Then, β ε is continuous in E \ { 0 } . Set

N ε i = { v N ε : β ε ( v ) x i < r 0 } , α ε i = inf v N ε i J ε ( v ) , N ε i = { v N ε : β ε ( v ) x i = r 0 } and α ˜ ε i = inf v N ε i J ε ( v ) ,

where i = 1 , 2 , , k .

Lemma 3.1

For i = 1 , 2 , , k , given η ( 0 , m 0 ) , there exists ε η > 0 such that

c ε α ε i < m 0 + η ,

whenever ε ( 0 , ε η ) .

Proof

By the definitions of c ε and α ε i , we have α ε i c ε . Set ε ( 0 , 1 ) . Choose a function ϕ ε C 0 ( R N ) satisfying ϕ ε ( x ) = 1 for x < 1 ε 1 , ϕ ε = 0 for x > 1 ε , 0 < ϕ ε ( x ) < 1 , and ϕ ε 2 . By Lemma 2.10, there exists v that is a positive ground state solution of equation (2.7) with a = V 0 and b = Q 0 . By direct computation, we can obtain

(3.1) lim ε 0 v ϕ ε v = 0 .

Define v ε i ( x ) = v x x i ε ϕ ε x x i ε . By Lemma 2.4, there exists t ε i > 0 such that J ε ( t ε i v ε i ) = sup t 0 J ε ( t v ε i ) and t ε i v ε i N ε . Using (3.1), r > x i + r 0 and the Lebesgue dominated convergence theorem, we can obtain

lim ε 0 β ε ( t ε i v ε i ) = lim ε 0 β ε ( v ε i ) = lim ε 0 R N χ ( ε x + x i ) v ϕ ε 2 d x R N v ϕ ε 2 d x = lim ε 0 R N χ ( x i ) v 2 d x R N v 2 d x = x i .

Thus, t ε i v ε i N ε i for ε > 0 small. It follows that α ε i J ε ( t ε i v ε i ) . Then, to obtain this lemma, we only need to show J ε ( t ε i v ε i ) < m 0 + η for ε > 0 small. Applying Lemma 2.5 to t ε i v ε i , we can obtain t ε i v ε i ε θ . Then, noting V 0 > 0 , we have t ε i v ϕ ε C . Using (3.1), we can derive that t ε i C , for ε small enough. On the other hand,

(3.2) R N ( t ε i v ε i ) 2 + V ( ε x ) G 1 ( t ε i v ε i ) g ( G 1 ( t ε i v ε i ) ) t ε i v ε i = R N G 1 ( t ε i v ε i ) α p 1 g ( G 1 ( t ε i v ε i ) ) t ε i v ε i + R N Q ( ε x ) G 1 ( t ε i v ε i ) α 2 * 1 g ( G 1 ( t ε i v ε i ) ) t ε i v ε i .

Then, by (5) and (7) of Lemma 2.2, the boundness of V ( x ) and the definition of v ε i , we can obtain

(3.3) R N ( t ε i v ϕ ε ) 2 + ( t ε i v ϕ ε ) 2 C R N G 1 ( t ε i v ϕ ε ) α p .

Since v > 0 , there exists δ > 0 and R > 0 such that m ( Ω ) > 0 , where Ω { x B R ( 0 ) : v δ } . By the Egoroff theorem, there exists Ω 0 Ω such that m ( Ω \ Ω 0 ) > 0 and v ϕ ε v uniformly in Ω \ Ω 0 . If t ε i is unbounded, using ( 11 ) of Lemma 2.2, (3.1) and (3.3), we have

C ( t ε i ) 2 Ω \ Ω 0 G 1 ( t ε i v ϕ ε ) α p C Ω \ Ω 0 t ε i v ϕ ε p C ( t ε i ) p ,

which is impossible due to 2 < p < 2 * . Therefore, t ε i t i > 0 , as ε 0 . Then, by (3.1) and (3.2), we have

R N ( t i v ) 2 + V 0 G 1 ( t i v ) g ( G 1 ( t i v ) ) t i v = R N G 1 ( t i v ) α p 1 g ( G 1 ( t i v ) ) t i w + R N Q 0 G 1 ( t i v ) α 2 * 1 g ( G 1 ( t i v ) ) t i v ,

that is, t i v 0 . From Lemma 2.4 and v 0 , we obtain t i = 1 . Therefore, by (3.1) and t ε i 1 , as ε 0 , one has

R N ( t ε i v ε i ) 2 = R N ( t ε i v ϕ ε ) 2 R N v 2 , R N V ( ε x ) G 1 ( t ε i v ε i ) 2 = R N V ( ε x + x i ) G 1 ( t ε i v ϕ ε ) 2 R N V 0 G 1 ( v ) 2 , R N G 1 ( t ε i v ε i ) α p = R N G 1 ( t ε i v ϕ ε ) α p R N G 1 ( v ) α p

and

R N Q ( ε x ) G 1 ( t ε i v ε i ) α 2 * = R N Q ( ε x + x i ) G 1 ( t ε i v ϕ ε ) α 2 * R N Q 0 G 1 ( v ) α 2 * .

Thus, we have

J ε ( t ε i v ε i ) = J 0 ( v ) + o ε ( 1 ) = m 0 + o ε ( 1 ) ,

which implies that the lemma holds.□

Lemma 3.2

For i = 1 , 2 , , k , given μ > 0 , there exists ε μ > 0 such that

α ˜ ε i > m 0 + μ

whenever ε ( 0 , ε μ ) .

Proof

Otherwise, we can obtain a sequence ε n 0 such that α ˜ ε n i b m 0 . By the definition of α ˜ ε n i , we have { v n } N ε n i satisfying J ε n ( v n ) b . In terms of Lemma 2.4, J ε n ( v n ) = sup t 0 J ε n ( t v n ) , and there exists a unique t n > 0 such that t n v n 0 . Noting V ( ε n x ) V 0 and Q ( ε n x ) Q 0 ,

m 0 + o n ( 1 ) J ε n ( v n ) = sup t 0 J ε n ( t v n ) J ε n ( t n v n ) J 0 ( t n v n ) m 0 ,

which means that

(3.4) R N V ( ε n x ) G 1 ( t n v n ) 2 = R N V 0 G 1 ( t n v n ) 2 + o n ( 1 ) .

and

J 0 ( t n v n ) = m 0 + o n ( 1 ) .

For u E , define L 0 ( u ) = J 0 ( u ) , u . By the Ekeland’s variational principle, there exist { w n } 0 such that

w n t n v n = o n ( 1 ) , J 0 ( w n ) = m 0 + o n ( 1 ) , and J 0 ( w n ) μ n L 0 ( w n ) = o n ( 1 ) .

From w n 0 , we have μ n L 0 ( w n ) , w n = o n ( 1 ) . It follows from Lemma 2.8 that lim n L 0 ( w n ) , w n 0 . If lim n L 0 ( w n ) , w n = 0 , by (2.6), we see that w n 0 , which is a contradiction with J 0 ( w n ) m 0 > 0 . Therefore,

lim n L 0 ( w n ) , w n < 0 .

Thus, μ n = o n ( 1 ) . Then, J 0 ( w n ) = o n ( 1 ) . Thus, { w n } is a ( PS ) m 0 sequence for J 0 . By Lemma 2.6, w n is bounded. Then, there exists w E such that w n w in E . We have two cases.

Case 1. w = 0 . It follows from the proof of case 2 in Lemma 2.10 that there exists { y n } R N with y n such that e n w n ( + y n ) e 0 in E . From v n N ε n i , we can obtain β ε n ( t n v n ) = β ε n ( v n ) B r 0 ( x i ) . Noting w n t n v n 0 , we can assume that β ε n ( w n ) x 0 B r 0 ( x i ) , and hence

x 0 = lim n R N χ ( ε n x ) w n 2 d x R N w n 2 d x = lim n R N χ ( ε n x + ε n y n ) e n ( x ) 2 d x R N e n ( x ) 2 d x .

Then, there exists y 0 R N with y 0 < r such that ε n y n y 0 . Otherwise, we have ε n y n , or ε n y n y 0 with y 0 r . From e n e in E , the definition of χ and the above limit, we can deduce that x 0 = r , which violates x 0 B r 0 ( x i ) and r > x i + r 0 . Then, we can obtain y 0 = x 0 B r 0 ( x i ) , and hence V ( y 0 ) > V 0 . From w n t n v n 0 and e n e in E , we have t n v n ( + y n ) e in E . Therefore,

lim n R N V ( ε n x ) G 1 ( t n v n ) 2 = lim n R N V ( ε n x + ε n y n ) G 1 ( t n v n ( x + y n ) ) 2 = R N V ( y 0 ) G 1 ( e ) 2 ,

which, together with (3.4), implies R N V ( y 0 ) G 1 ( e ) 2 = R N V 0 G 1 ( e ) 2 , and this violates V ( y 0 ) > V 0 .

Case 2. w 0 . It follows from the proof of case 1 in Lemma 2.10 that w n w in E . v n N ε n i means β ε n ( t n v n ) = β ε n ( v n ) B r 0 ( x i ) . By w n t n v n 0 , we can assume that β ε n ( w n ) x 0 B r 0 ( x i ) , and hence

x 0 = lim n R N χ ( ε n x ) w n 2 d x R N w n 2 d x = 0 .

Thus, we have 0 = x 0 B r 0 ( x i ) . Then, V ( 0 ) > V 0 . From w n t n v n 0 and w n w in E , we can obtain t n v n w in E . Then,

lim n R N V ( ε n x ) G 1 ( t n v n ) 2 = R N V ( 0 ) G 1 ( w ) 2 ,

which, together with (3.4), implies R N V ( 0 ) G 1 ( w ) 2 = R N V 0 G 1 ( w ) 2 , and this violates V ( 0 ) > V 0 .□

Following the idea of [32], we have the following two lemmas.

Lemma 3.3

For u N ε i , there exist k i > 0 and a differentiable functional l : B ( 0 ; k i ) E R + such that l ( 0 ) = 1 , l ( v ) ( u v ) N ε i for any v B ( 0 ; k i ) and

l ( 0 ) , ϕ = L ε ( u ) , ϕ L ε ( u ) , u for any ϕ C 0 ( R N ) ,

where B ( 0 ; k i ) = { u E : u ε < k i } .

Proof

For each u N ε i , we define a function F u : R × E R by

F u ( t , v ) = J ε ( t ( u v ) ) , t ( u v ) = t 2 R N ( u v ) 2 + H 2 ( t ( u v ) ) H α p [ ( t ( u v ) ) + ] H ˜ α 2 * ( t ( u v ) ) ,

where H 2 , H α p , and H ˜ α 2 * are defined in Lemma 2.8. Then, F u ( 1,0 ) = J ε ( u ) , u = 0 and

d d t F u ( 1,0 ) = 2 R N u 2 + H ( u ) , u H ( u + ) , u H ˜ ( u ) , u = L ( u ) , u < 0 ,

where we have used Lemma 2.8. From the implicit function theorem, there exist k i > 0 and a differentiable function l : B ( 0 ; k i ) E R + such that l ( 0 ) = 1 , for any ϕ C 0 ( R N ) ,

l ( 0 ) , ϕ = 2 R N u ϕ + H ( u ) , ϕ H ( u + ) , ϕ H ˜ ( u ) , ϕ 2 R N u 2 + H ( u ) , u H ( u + ) , u H ˜ ( u ) , u = L ε ( u ) , ϕ L ε ( u ) , u ,

and

F u ( l ( v ) , v ) = 0 , v B ( 0 ; k i ) ,

which means that

J ε ( l ( v ) ( u v ) ) , l ( v ) ( u v ) = 0 , v B ( 0 ; k i ) .

Therefore, l ( v ) ( u v ) N ε . By continuity of β ε and l , taking k i > 0 small enough if necessary, one has β ε ( l ( v ) ( u v ) ) B r 0 ( x i ) . Then, l ( v ) ( u v ) N ε i . This completes the proof of this lemma.□

Lemma 3.4

For i = 1 , 2 , , k , J ε has a ( PS ) α ε i sequence { v n i } N ε i .

Proof

By Lemmas 3.1 and 3.2, we obtain that α ε i < α ˜ ε i . Then,

α ε i = inf v N ε i N ε i J ε ( v ) .

Let { v n i } N ε i N ε i be a minimizing sequence for α μ i . Now, we prove that { v n i } is a ( P S ) α ε i sequence for J ε . Applying Ekeland’s variational principle, there exists a subsequence { v n i } (still denoted by { v n i } ) such that

  1. J ε ( v n i ) < α ε i + 1 n .

  2. J ε ( v ) J ε ( v n i ) 1 n v v n i , v N ε i .

Thus, we only need to prove that J ε ( v n i ) 0 in E 1 as n . By Lemma 3.3, there exist k n i > 0 and a differentiable functional l n i : B ( 0 ; k n i ) E R + such that l n i ( 0 ) = 1 , l n i ( v ) ( v n i v ) N ε i for any v B ( 0 ; k n i ) . Let ϕ E with ϕ = 1 and 0 < s < k n i , and choosing v = s ϕ . Then, v = s ϕ B ( 0 ; k n i ) and l n i ( s v ) ( v n i s v ) N ε i . From ( i i ) and the mean value theorem, one has

l n i ( s ϕ ) ( v n i s ϕ ) v n i n J ε ( v n i ) J ε [ l n i ( s ϕ ) ( v n i s ϕ ) ] = J ε ( t 0 v n i + ( 1 t 0 ) l n i ( s ϕ ) ( v n i s ϕ ) ) , v n i l n i ( s ϕ ) ( v n i s ϕ ) = J ε ( v n i ) , v n i l n i ( s ϕ ) ( v n i s ϕ ) + o s ( 1 ) v n i l n i ( s ϕ ) ( v n i s ϕ ) = s l n i ( s ϕ ) J ε ( v n i ) , ϕ + ( 1 l n i ( s ϕ ) ) J ε ( v n i ) , v n i + o s ( 1 ) v n i l n i ( s ϕ ) ( v n i s ϕ ) = s l n i ( s ϕ ) J ε ( v n i ) , ϕ + o s ( 1 ) v n i l n i ( s ϕ ) ( v n i s ϕ ) ,

where 0 < t 0 < 1 and o s ( 1 ) is a quantity tending to 0 as s 0 . Therefore, noting l n i ( 0 ) = 1 , for s small,

J ε ( v n i ) , ϕ v n i l n i ( s ϕ ) ( v n i s ϕ ) s l n i ( s ϕ ) 1 n + o s ( 1 ) v n i ( l n i ( s ϕ ) l n i ( 0 ) ) s l n i ( s ϕ ) ϕ s l n i ( s ϕ ) 1 n + o s ( 1 ) v n i l n i ( s ϕ ) l n i ( 0 ) + s l n i ( s ϕ ) ϕ s l n i ( s ϕ ) 1 n + o s ( 1 ) C 1 + v n i l n i ( s ϕ ) l n i ( 0 ) s 1 n + o s ( 1 ) .

Sending s 0 + , and noting the arbitrariness of ϕ , we obtain

J ε ( v n i ) , ϕ C 1 n ( 1 + v n i ( l n i ) ( 0 ) ) .

By Lemma 3.3 and (2.6), we can obtain the boundedness of ( l n i ) ( 0 ) , and the boundedness of { v n i } follows from Lemma 2.6. Then, J ε ( v n i ) 0 in E 1 as n .□

Lemma 3.5

For i = 1 , 2 , , k , there exists ε ˜ > 0 , and when ε ( 0 , ε ˜ ) , if { u n } N ε i is a ( PS ) α ε i sequence for J ε , then { u n } converges strongly in E up to a subsequence.

Proof

By Lemma 2.6, u n ε is bounded. Then, there exists u E such that u n u in E after selecting a subsequence. We have two cases.

Case 1. u = 0 . It follows from Lions lemma that R N u n t d x 0 for any t ( 2 , 2 * ) , or there exists y n R N with y n such that v n = u n ( + y n t ) v 0 in E . Define a functional on E by

L ε ( w ) = 1 2 R N w 2 + V G 1 ( w ) 2 1 α p R N G 1 ( w + ) α p 1 α 2 * R N Q ( ε x ) G 1 ( w + ) α 2 * .

In view of lim x V ( x ) = V , u n 0 in E , J ε ( u n ) α ε i , and J ε ( u n ) 0 , we know that

(3.5) L ε ( u n ) α ε i and L ε ( u n ) 0 .

By Lemma 2.3, for any δ > 0 , there exists C δ > 0 such that

K 1 , ε ( x , u n ) + K 2 , ε ( x , u n + ) δ ( u n 2 * + u n 2 ) + C δ u n p , k 1 , ε ( x , u n ) u n + k 2 , ε ( x , u n + ) u n δ ( u n 2 * + u n 2 ) + C δ u n p .

If u n 0 in L t ( R N ) with t ( 2 , 2 * ) , one has

R N K 1 , ε ( x , u n ) + K 2 , ε ( x , u n + ) = o n ( 1 ) , R N k 1 , ε ( x , u n ) u n + k 2 , ε ( x , u n + ) u n = o n ( 1 ) .

Then,

L ε ( u n ) = 1 2 u n V 2 α 2 * 1 β 2 * 2 * R N Q ( ε x ) u n + 2 * + o n ( 1 )

and

L ε ( u n ) , u n = u n V 2 α 2 * 1 β 2 * R N Q ( ε x ) u n + 2 * + o n ( 1 ) .

Assume that u n V 2 l and α 2 * 1 β 2 * R N Q ( ε x ) u n + 2 * l . It follows from the definition of S and Q ( x ) Q 0 that

S R N Q ( ε x ) u n + 2 * 2 2 * S Q 0 R N u n + 2 * 2 2 * ( Q 0 ) 2 2 * R N u n 2 ( Q 0 ) 2 2 * u n V 2 .

Letting n ,

S β 2 * α 2 * 1 l 2 2 * ( Q 0 ) 2 2 * l .

Thus, l = 0 or l β N α N + 2 2 ( Q 0 ) N 2 2 S N 2 . If l = 0 , we can deduce a contradiction with α ε i > 0 . Therefore, l β N α N + 2 2 ( Q 0 ) N 2 2 S N 2 . Then, we can deduce that

α ε i 1 2 1 2 * l 1 N β N α N + 2 2 ( Q 0 ) N 2 2 S N 2 ,

which violates Lemmas 2.10 and 3.1 for small ε . Therefore, there exists y n R N with y n such that v n = u n ( + y n ) v 0 in E . By L ε ( u n ) = o n ( 1 ) and lim x Q ( x ) = Q , we have J ( v ) = 0 . For w E , define

L n ( w ) = 1 2 R N w 2 + V G 1 ( w ) 2 1 α p R N G 1 ( w + ) α p 1 α 2 * R N Q ( ε x + ε y n ) G 1 ( w + ) α 2 * .

Since lim x Q ( x ) = Q , we have

L n ( w ) = J ( w ) + o n ( 1 ) , L n ( w ) = J ( w ) + o n ( 1 ) .

Let w n v n v . By Lemma 2.5 of [24], we have

L n ( w n ) = L n ( v n ) L n ( v ) + o n ( 1 ) = α ε i L n ( v ) + o n ( 1 )

and

L n ( w n ) = L n ( v n ) L n ( v ) + o n ( 1 ) = L n ( v ) + o n ( 1 ) .

Then, we can obtain

L n ( w n ) = α ε i J ( v ) + o n ( 1 )

and

L n ( w n ) = J ( v ) + o n ( 1 ) = o n ( 1 ) .

If w n 0 in E , then by y n , we have

β ε ( u n ) = R N χ ( ε x ) u n 2 d x R N u n 2 d x = R N χ ( ε x + ε y n ) v n 2 d x R N v n 2 d x r ,

which violates β ε ( u n ) B r 0 ( x i ) and r > x i + r 0 , and hence w n converges weakly and not strongly to 0 in E . Noting L n ( w n ) = o n ( 1 ) , similar to the proof of Lemma 2.5, we derive that there exists 0 < δ 0 < 1 such that w n δ 0 . From J ( v ) = 0 , Lemma 2.11, and the definition of m , we can obtain J ( v ) m m 0 . Thus, by Remark 2.7, we have

(3.6) α ε i = L n ( w n ) 1 α p L n ( w n ) , g ( G 1 ( w n ) ) G 1 ( w n ) + J ( v ) + o n ( 1 ) = R N 1 2 1 α p 1 + g ( G 1 ( w n ) ) G 1 ( w n ) g ( G 1 ( w n ) ) w n 2 + 1 2 1 α p R N V G 1 ( w n ) 2 + 1 α p 1 α 2 * R N Q ( ε x + ε y n ) G 1 ( w n ) α 2 * + J ( v ) + o n ( 1 ) C R N ( w n 2 + G 1 ( w n ) 2 ) + m 0 + o n ( 1 ) C δ 0 + m 0 + o n ( 1 ) ,

which violates Lemma 3.1.

Case 2. u 0 . It is easy to see that J ε ( u ) = 0 . Define u ^ n = u n u . It follows from Lemma 2.5 of [24] that

α ε i = J ε ( u n ) + o n ( 1 ) = J ε ( u ^ n ) + J ε ( u ) + o n ( 1 )

and

J ε ( u ^ n ) = o n ( 1 ) .

Then, u ^ n 0 in E . Otherwise, u ^ n converges weakly and not strongly to 0 in E . Similar to the proof of Lemma 2.5, there exists 0 < δ 0 < 1 such that u ^ n δ 0 . Noting lim x V ( x ) = V , we have

α ε i = L ε ( u ^ n ) + J ε ( u ) + o n ( 1 ) , L ε ( u ^ n ) = o n ( 1 ) .

From J ε ( u ) = 0 , Lemma 2.11, and the definition of c ε , we can deduce that J ε ( u ) c ε m 0 . Therefore,

(3.7) α ε i = L ε ( u ^ n ) 1 α p L ε ( u ^ n ) , g ( G 1 ( u ^ n ) ) G 1 ( u ^ n ) + J ε ( u ) + o n ( 1 ) = R N 1 2 1 α p 1 + g ( G 1 ( u ^ n ) ) G 1 ( u ^ n ) g ( G 1 ( u ^ n ) ) u ^ n 2 + 1 2 1 α p R N V G 1 ( u ^ n ) 2 + 1 α p 1 α 2 * R N Q ( ε x ) G 1 ( u ^ n ) α 2 * + J ε ( u ) + o n ( 1 ) C R N ( u ^ n 2 + G 1 ( u ^ n ) 2 ) + m 0 + o n ( 1 ) C δ 0 + m 0 + o n ( 1 ) ,

which violates Lemma 3.1, and hence u ^ n 0 in E .□

Lemma 3.6

Let ε ( 0 , ε ˜ ) . Problem (2.2) has at least k different positive solutions v ε i , i = 1 , 2 , , k .

Proof

It follows from Lemma 3.4 that there exists { v n i } N ε i such that J ε ( v n i ) α ε i and J ε ( v n i ) 0 . By Lemma 3.5, v n i v ε i in E . Thus, v ε i N ε i ¯ , J ε ( v ε i ) = α ε i , and J ε ( v ε i ) = 0 . Because of α ε i < α ˜ ε i , we conclude v ε i N ε i and β ε ( v ε i ) B r 0 ( x i ) . Recalling B r 0 ( x i ) , i = 1 , 2 , , k are disjoint, it follows that v ε i , i = 1 , 2 , , k are different positive solutions for problem (2.2).□

4 Concentration of solutions of (1.1)

Lemma 4.1

For i = 1 , 2 , , k , we have ε * ( 0 , ε ˜ ) , { x ε i } R N , R 0 , γ 0 > 0 satisfying

B R 0 ( x ε i ) v ε i 2 d x γ 0 ,

whenever ε ( 0 , ε * ) .

Proof

Otherwise, we can obtain a sequence ε n 0 such that

lim n sup x R N B R ( x ) v ε n i 2 d x = 0

for any R > 0 . It follows from Lions lemma that R N v ε n t d x 0 for any t ( 2 , 2 * ) . From Lemmas 2.12, 3.1 and 3.6, we can obtain J ε n ( v ε n i ) = α ε n i m 0 and J ε n ( v ε n i ) = 0 . Then, similar to the proof of Case 1 in Lemma 3.5, we deduce that m 0 1 N β N α N + 2 2 ( Q 0 ) N 2 2 S N 2 , which violates Lemma 2.10.□

Lemma 4.2

For i = 1 , 2 , , k , lim ε 0 ε x ε i = x i .

Proof

We claim that { ε x ε i } is bounded in R N . Otherwise, we can obtain ε n 0 such that ε n x ε n i . It follows from J ε n ( v ε n i ) = α ε n i m 0 and J ε n ( v ε n i ) = 0 that v ε n i ε n is bounded. Then, { v ε n i } is bounded in E . Define w ε n i = v ε n i ( + x ε n i ) . From Lemma 4.1, we know that B R 0 ( 0 ) w ε n i 2 d x γ 0 for some R 0 , γ 0 > 0 , and hence w ε n i w i 0 in E . Define a functional on E by

H ε i ( u ) 1 2 R N ( u 2 + V ( ε x + ε x ε i ) G 1 ( u ) 2 ) 1 α p R N G 1 ( u ) α p 1 α 2 * R N Q ( ε x + ε x ε i ) G 1 ( u ) α 2 * .

It is easy to see that H ε n i ( w ε n i ) m 0 and ( H ε n i ) ( w ε n i ) = 0 . Therefore,

R N w ε n i w i + V ( ε n x + ε n x ε n i ) G 1 ( w ε n i ) g ( G 1 ( w ε n i ) ) w i = R N Q ( ε n x + ε n x ε n i ) ( G 1 ( w ε n i ) ) α 2 * 1 g ( G 1 ( w ε n i ) ) w i + R N ( G 1 ( w ε n i ) ) α p 1 g ( G 1 ( w ε n i ) ) w i .

From ε n x ε n i and w ε n i w i in E , we can obtain

R N w i 2 + V G 1 ( w i ) g ( G 1 ( w i ) ) w i = R N Q ( G 1 ( w i ) ) α 2 * 1 g ( G 1 ( w i ) ) w i + R N ( G 1 ( w i ) ) α p 1 g ( G 1 ( w i ) ) w i ,

which means that w i . From H ε n i ( w ε n i ) m 0 and ( H ε n i ) ( w ε n i ) = 0 ,

m 0 = H ε n i ( w ε n i ) 1 α p ( H ε n i ) ( w ε n i ) , g ( G 1 ( w ε n i ) ) G 1 ( w ε n i ) + o n ( 1 ) = R N 1 2 1 α p 1 + g ( G 1 ( w ε n i ) ) G 1 ( w ε n i ) g ( G 1 ( w ε n i ) ) w ε n i 2 + 1 2 1 α p R N V ( ε x ) G 1 ( w ε n i ) 2 + 1 α p 1 α 2 * R N Q ( ε x ) G 1 ( w ε n i ) α 2 * + o n ( 1 ) .

Applying Fatou’s lemma to the above expression and using Lemma 2.11, we can deduce that

m 0 R N 1 2 1 α p 1 + g ( G 1 ( w i ) ) G 1 ( w i ) g ( G 1 ( w i ) ) w i 2 + 1 2 1 α p R N V G 1 ( w i ) 2 + 1 α p 1 α 2 * R N Q G 1 ( w i ) α 2 * = J ( w i ) 1 α p J ( w i ) , g ( G 1 ( w i ) ) G 1 ( w i ) = J ( w i ) m m 0 ,

and hence w ε n i w i in E . Note that

β ε n ( v ε n i ) = R N χ ( ε n x ) v ε n i 2 d x R N v ε n i 2 d x = R N χ ( ε n x + ε n x ε n i ) w ε n i 2 d x R N w ε n i 2 d x .

In terms of w ε n i w i in E and ε n x ε n i , we can obtain r = lim n β ε n ( v ε n i ) , which violates β ε n ( v ε n i ) B r 0 ( x i ) and r > x i + r 0 .

We now show ε x ε i x i as ε 0 . Due to the boundness of ε x ε i , we can assume ε x ε i x 0 i as ε 0 . Define w ε i = v ε i ( + x ε i ) . Lemma 4.1 guarantees w ε i w i 0 in E . For u E , define

H i ( u ) 1 2 R N ( u 2 + V ( x 0 i ) G 1 ( u ) 2 ) 1 α p R N G 1 ( u ) α p 1 α 2 * R N Q ( x 0 i ) G 1 ( u ) α 2 * .

It follows from J ε ( v ε i ) = 0 that ( H i ) ( w i ) = 0 . J ε ( v ε i ) = α ε i m 0 and J ε ( v ε i ) = 0 imply that

m 0 = J ε ( v ε i ) 1 α p J ε ( v ε i ) , g ( G 1 ( v ε i ) ) G 1 ( v ε i ) + o ε ( 1 ) = R N 1 2 1 α p 1 + g ( G 1 ( w ε i ) ) G 1 ( w ε i ) g ( G 1 ( w ε i ) ) w ε i 2 + 1 2 1 α p R N V ( ε x + ε x ε i ) G 1 ( w ε i ) 2 + 1 α p 1 α 2 * R N Q ( ε x + ε x ε i ) G 1 ( w ε i ) α 2 * + o ε ( 1 ) .

Applying Fatou’s lemma to the above expression, and using Lemma 2.11, we can deduce that

m 0 R N 1 2 1 α p 1 + g ( G 1 ( w i ) ) G 1 ( w i ) g ( G 1 ( w i ) ) w i 2 + 1 2 1 α p R N V ( x 0 i ) G 1 ( w i ) 2 + 1 α p 1 α 2 * R N Q ( x 0 i ) G 1 ( w i ) α 2 * = H i ( w i ) 1 α p H i ( w i ) , g ( G 1 ( w i ) ) G 1 ( w i ) = H i ( w i ) m 0 ,

and hence w ε i w i in E and V ( x 0 i ) = V 0 . Note that

β ε ( v ε i ) = R N χ ( ε x ) v ε i 2 d x R N v ε i 2 d x = R N χ ( ε x + ε x ε i ) w ε i 2 d x R N w ε i 2 d x .

If x 0 i r , then lim n β ε ( v ε i ) = r , which violates β ε ( v ε i ) B r 0 ( x i ) and r > x i + r 0 . Thus, x 0 i < r . Then, lim n β ε ( v ε i ) = x 0 i B r 0 ( x i ) ¯ . This, together with V ( x 0 i ) = V 0 , guarantees x 0 i = x i . Therefore, we complete the proof.□

Lemma 4.3

For i = 1 , 2 , , k , v ε i possesses a maximum y ε i R N satisfying V ( ε y ε i ) V ( x i ) and Q ( ε y ε i ) Q ( x i ) as ε 0 . Moreover, there exist C i , c i > 0 such that

v ε i ( x ) C i exp ( c i x y ε i )

for ε ( 0 , ε * ) and x R N .

Proof

From the proof of Lemma 4.2, we know that w ε i is a solution of

(4.1) Δ w ε i + V ( ε x + ε x ε i ) G 1 ( w ε i ) g ( G 1 ( w ε i ) ) = G 1 ( w ε i ) α p 2 G 1 ( w ε i ) g ( G 1 ( w ε i ) ) + Q ( ε x + ε x ε i ) G 1 ( w ε i ) α 2 * 2 G 1 ( w ε i ) g ( G 1 ( w ε i ) ) .

and w ε i w i 0 in E as ε 0 . Then, { w ε i 2 * } uniformly integrable near infinity, it follows from Theorem 1.1 of [37] that

(4.2) lim x w ε i ( x ) = 0 uniformly for ε .

If z ε i is a maximum point w ε i , then Δ w ε i ( z ε i ) 0 . This and (4.1) imply that

V ( ε x + ε x ε i ) G 1 ( w ε i ( z ε i ) ) g ( G 1 ( w ε i ( z ε i ) ) ) G 1 ( w ε i ( z ε i ) ) α p 2 G 1 ( w ε i ( z ε i ) ) g ( G 1 ( w ε i ( z ε i ) ) ) + Q ( ε x + ε x ε i ) G 1 ( w ε i ( z ε i ) ) α 2 * 2 G 1 ( w ε i ( z ε i ) ) g ( G 1 ( w ε i ( z ε i ) ) ) .

Thus,

V 0 G 1 ( w ε i ( z ε i ) ) α p 2 + Q 0 G 1 ( w ε i ( z ε i ) ) α 2 * 2 .

By (5) of Lemma 2.2, one has

C w ε i ( z ε i ) α p 2 + w ε i ( z ε i ) α 2 * 2 ,

which yields

w ε i ( z ε i ) C > 0 .

Then, (4.2) implies z ε i is bounded. Thus, there exists C i > 0 independent of ε such that z ε i C i . It follows from z ε i is a maximum point of w ε i = v ε i ( + x ε i ) that x ε i + z ε i is a maximum point of v ε i . Set y ε i = x ε i + z ε i . In terms of Lemma 4.2 and the boundness of z ε i , we have ε y ε i x i , and hence V ( ε y ε i ) V ( x i ) = V 0 and Q ( ε y ε i ) Q ( x i ) = Q 0 as ε 0 . Moreover, by standard argument, there exists C 0 i , c i > 0 such that w ε i ( x ) C 0 i exp ( c i x ) , refer [38] and [26] for example. Noting z ε i C i , we can obtain

v ε i ( x ) = w ε i ( x x ε i ) C ̀ 0 i exp ( c i x x ε i ) = C 0 i ̀ exp ( c i x y ε i + z ε i ) C i exp ( c i x y ε i ) .

Proof of Theorem 1.1

By Lemma 3.6, we know (2.2) admits at least k different positive solutions v ε i , i = 1 , 2 , , k . Then, u ε i G 1 ( v ε i ) , i = 1 , 2 , , k are k different positive solutions for (1.1). By Lemma 4.3, u ε i possesses a maximum y ε i R N satisfying V ( ε y ε i ) V ( x i ) and Q ( ε y ε i ) Q ( x i ) as ε 0 . Besides, noting (5) of Lemma 2.2, there exist C i , c i > 0 such that

u ε i = G 1 ( v ε i ) v ε i ( x ) C i exp ( c i x y ε i )

for ε ( 0 , ε * ) and x R N .□

Acknowledgments

We would like to express our sincere gratitude to the anonymous referee for their meticulous review of our manuscript and for providing valuable suggestions that have greatly contributed to its improvement.

  1. Funding information: Y. Chen received support from the National Natural Science Foundation of China (12161007) and Guangxi Natural Science Foundation Project (2023GXNSFAA026190). Z. Yang was supported by the National Natural Science Foundation of China (12301145, 12261107), Yunnan Fundamental Research Projects (202201AU070031, 202401AU070123).

  2. Author contributions: Both authors have accepted responsibility for the entire content of this manuscript and consented to its submission to the journal, reviewed all the results, and approved the final version of the manuscript.

  3. Conflict of interest: The authors declare that there is no conflict of interest.

  4. Data availability statement: Data sharing is not applicable to this article as no new data were created or analyzed in this study.

References

[1] S. Kurihara, Exact soliton solution for superfluid film dynamics, J. Phys. Soc. Japan 50 (1981), no. 11, 3801–3805. 10.1143/JPSJ.50.3801Suche in Google Scholar

[2] E. W. Laedke, K. H. Spatschek, and L. Stenflo, Evolution theorem for a class of perturbed envelope soliton solutions, J. Math. Phys. 24 (1983), no. 12, 2764–2769. 10.1063/1.525675Suche in Google Scholar

[3] A. de Bouard, N. Hayashi, P. I. Naumkin, and J. Saut, Scattering problem and asymptotics for a relativistic nonlinear Schrödinger equation, Nonlinearity 12 (1999), no. 5, 1415–1425. 10.1088/0951-7715/12/5/313Suche in Google Scholar

[4] A. de Bouard, N. Hayashi, and J. Saut, Global existence of small solutions to a relativistic nonlinear Schrödinger equation, Comm. Math. Phys. 189 (1997), no. 1, 73–105. 10.1007/s002200050191Suche in Google Scholar

[5] L. Brüll and H. Lange, Solitary waves for quasilinear Schrödinger equations, Expo. Math. 4 (1986), no. 3, 279–288. Suche in Google Scholar

[6] R. W. Hasse, A general method for the solution of nonlinear soliton and kink Schrödinger equations, Z. Physik B 37 (1980), no. 1, 83–87. 10.1007/BF01325508Suche in Google Scholar

[7] H. Lange, M. Poppenberg, and H. Teismann, Nash-Moser methods for the solution of quasilinear Schrödinger equations, Comm. Partial Differential Equations 24 (1999), no. 7–8, 1399–1418. 10.1080/03605309908821469Suche in Google Scholar

[8] M. Poppenberg, K. Schmitt, and Z. Wang, On the existence of soliton solutions to quasilinear Schrödinger equations, Calc. Var. Partial Differential Equations 14 (2002), no. 3, 329–344. 10.1007/s005260100105Suche in Google Scholar

[9] J. Liu, Y. Wang, and Z. Wang, Soliton solutions for quasilinear Schrödinger equations. II, J. Differential Equations 187 (2003), no. 2, 473–493. 10.1016/S0022-0396(02)00064-5Suche in Google Scholar

[10] M. Colin and L. Jeanjean, Solutions for a quasilinear Schrödinger equation: a dual approach, Nonlinear Anal. 56 (2004), no. 2, 213–226. 10.1016/j.na.2003.09.008Suche in Google Scholar

[11] J. M. B. do Ó, O. H. Miyagaki, and S. H. M. Soares, Soliton solutions for quasilinear Schrödinger equations with critical growth, J. Differential Equations 248 (2010), no. 4, 722–744. 10.1016/j.jde.2009.11.030Suche in Google Scholar

[12] X. He, A. Qian, and W. Zou, Existence and concentration of positive solutions for quasilinear Schrödinger equations with critical growth, Nonlinearity 26 (2013), no. 12, 3137–3168. 10.1088/0951-7715/26/12/3137Suche in Google Scholar

[13] Y. Guo and Z. Tang, Ground state solutions for the quasilinear Schrödinger equation, Nonlinear Anal. 75 (2012), no. 6, 3235–3248. 10.1016/j.na.2011.12.024Suche in Google Scholar

[14] S. Liu and J. Zhou, Standing waves for quasilinear Schrödinger equations with indefinite potentials, J. Differential Equations 265 (2018), no. 9, 3970–3987. 10.1016/j.jde.2018.05.024Suche in Google Scholar

[15] C. Xiang, Remarks on nondegeneracy of ground states for quasilinear Schrödinger equations, Discrete Contin. Dyn. Syst. 36 (2016), no. 10, 5789–5800. 10.3934/dcds.2016054Suche in Google Scholar

[16] C. O. Alves, Y. Wang, and Y. Shen, Soliton solutions for a class of quasilinear Schrödinger equations with a parameter, J. Differential Equations 259 (2015), no. 1, 318–343. 10.1016/j.jde.2015.02.030Suche in Google Scholar

[17] G. M. de Carvalho, R. G. Clemente, and J. de Albuquerque, Quasilinear Schrödinger equations with unbounded or decaying potentials in dimension 2, Math. Nachr. 296 (2023), no. 9, 4357–4373. 10.1002/mana.202100324Suche in Google Scholar

[18] H. Li and W. Zou, Quasilinear Schrödinger equations: ground state and infinitely many normalized solutions, Pacific J. Math. 322 (2023), no. 1, 99–138. 10.2140/pjm.2023.322.99Suche in Google Scholar

[19] S. Liu and L. Yin, Quasilinear Schrödinger equations with concave and convex nonlinearities, Calc. Var. Partial Differential Equations 62 (2023), no. 3, Paper No. 100, 14. 10.1007/s00526-023-02434-5Suche in Google Scholar

[20] M. Yang, C. A. Santos, P. Ubilla, and J. Zhou, On a defocusing quasilinear Schrödinger equation with singular term, Discrete Contin. Dyn. Syst. 43 (2023), no. 1, 507–536. 10.3934/dcds.2022158Suche in Google Scholar

[21] Y. Cheng and J. Wei, Fast and slow decaying solutions for H1-supercritical quasilinear Schrödinger equations, Calc. Var. Partial Differential Equations 58 (2019), no. 4, 144, 24. 10.1007/s00526-019-1594-0Suche in Google Scholar

[22] U. B. Severo, E. Gloss, and E. D. da Silva, On a class of quasilinear Schrödinger equations with superlinear or asymptotically linear terms, J. Differential Equations 263 (2017), no. 6, 3550–3580. 10.1016/j.jde.2017.04.040Suche in Google Scholar

[23] Y. Shen and Y. Wang, Soliton solutions for generalized quasilinear Schrödinger equations, Nonlinear Anal. 80 (2013), 194–201. 10.1016/j.na.2012.10.005Suche in Google Scholar

[24] Y. Deng, S. Peng, and S. Yan, Critical exponents and solitary wave solutions for generalized quasilinear Schrödinger equations, J. Differential Equations 260 (2016), no. 2, 1228–1262. 10.1016/j.jde.2015.09.021Suche in Google Scholar

[25] X. Fang and M. Liu, Localized solutions of higher topological type for semiclassical generalized quasilinear Schrödinger equations, Z. Angew. Math. Phys. 74 (2023), no. 2, 81, 22. 10.1007/s00033-023-01971-5Suche in Google Scholar

[26] J. Chen, X. Huang, D. Qin, and B. Cheng, Existence and asymptotic behavior of standing wave solutions for a class of generalized quasilinear Schrödinger equations with critical Sobolev exponents, Asymptot. Anal. 120 (2020), no. 3–4, 199–248. 10.3233/ASY-191586Suche in Google Scholar

[27] Q. Li, J. Zhang, J. Nie, and W. Wang, Semiclassical solutions of generalized quasilinear Schrödinger equations with competing potentials, Complex Var. Elliptic Equ. 68 (2023), no. 7, 1045–1076. 10.1080/17476933.2022.2034153Suche in Google Scholar

[28] X. Meng and S. Ji, Positive ground state solutions for generalized quasilinear Schrödinger equations with critical growth, J. Geom. Anal. 33 (2023), no. 12, 372, 20. 10.1007/s12220-023-01429-0Suche in Google Scholar

[29] Y. Jing, Z. Liu, and Z. Wang, Parameter-dependent multiplicity results of sign-changing solutions for quasilinear elliptic equations, Commun. Contemp. Math. 25 (2023), no. 9, 2250039, 37. 10.1142/S0219199722500390Suche in Google Scholar

[30] A. Mennuni, F.and Salvatore, Generalized quasilinear elliptic equations in RN, Mediterr. J. Math. 20 (2023), no. 4, 205, 27. 10.1007/s00009-023-02393-3Suche in Google Scholar

[31] A. Candela, A. Salvatore, and C. Sportelli, Bounded solutions for quasilinear modified Schrödinger equations, Calc. Var. Partial Differential Equations 61 (2022), no. 6, 220, 28. 10.1007/s00526-022-02328-ySuche in Google Scholar

[32] D. Cao and E. S. Noussair, Multiplicity of positive and nodal solutions for nonlinear elliptic problems in RN, Ann. Inst. H. Poincaré C Anal. Non Linéaire 13 (1996), no. 5, 567–588. 10.1016/s0294-1449(16)30115-9Suche in Google Scholar

[33] Y. Meng and X. He, Multiplicity of concentrating solutions for Choquard equation with critical growth, J. Geom. Anal. 33 (2023), no. 3, 78, 29. 10.1007/s12220-022-01129-1Suche in Google Scholar

[34] J. Zhang and W. Zou, Multiplicity and concentration behavior of solutions to the critical Kirchhoff-type problem, Z. Angew. Math. Phys. 68 (2017), no. 3, 57, 27. 10.1007/s00033-017-0803-ySuche in Google Scholar

[35] Q. Li and X. Wu, Existence, multiplicity, and concentration of solutions for generalized quasilinear Schrödinger equations with critical growth, J. Math. Phys. 58 (2017), no. 4, 041501, 30. 10.1063/1.4982035Suche in Google Scholar

[36] Q. Li, J. Zhang, and J. Nie, Ground state solutions for generalized quasilinear Schrödinger equations with critical growth, Qual. Theory. Dyn. Syst. 21 (2022), no. 4, 137, 33. 10.1007/s12346-022-00667-xSuche in Google Scholar

[37] G. Li, Some properties of weak solutions of nonlinear scalar field equations, Ann. Acad. Sci. Fenn. Ser. A I Math. 15 (1990), no. 1, 27–36. 10.5186/aasfm.1990.1521Suche in Google Scholar

[38] Y. Wang and W. Zou, Bound states to critical quasilinear Schrödinger equations, NoDEA Nonlinear Differential Equations Appl. 19 (2012), no. 1, 19–47. 10.1007/s00030-011-0116-3Suche in Google Scholar

Received: 2024-11-26
Revised: 2025-02-23
Accepted: 2025-06-20
Published Online: 2025-10-08

© 2025 the author(s), published by De Gruyter

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

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Heruntergeladen am 17.10.2025 von https://www.degruyterbrill.com/document/doi/10.1515/dema-2025-0164/html?lang=de
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