Startseite On singularly perturbed (p, N)-Laplace Schrödinger equation with logarithmic nonlinearity
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On singularly perturbed (p, N)-Laplace Schrödinger equation with logarithmic nonlinearity

  • Deepak Kumar Mahanta , Tuhina Mukherjee und Patrick Winkert EMAIL logo
Veröffentlicht/Copyright: 7. Oktober 2025
Advanced Nonlinear Studies
Aus der Zeitschrift Advanced Nonlinear Studies

Abstract

This article focuses on the study of the existence, multiplicity and concentration behavior of ground states as well as the qualitative aspects of positive solutions for a (p, N)-Laplace Schrödinger equation with logarithmic nonlinearity and critical exponential nonlinearity in the sense of Trudinger-Moser in the whole Euclidean space R N . Through the use of smooth variational methods, penalization techniques, and the application of the Lusternik–Schnirelmann category theory, we establish a connection between the number of positive solutions and the topological properties of a set in which the potential function achieves its minimum values.

2020 Mathematics Subject Classification: 35A15; 35D30; 35J10; 35J60; 35J92

1 Introduction

In this article, we deal with the following singularly perturbed (p, N)-Laplace Schrödinger equation

L p ε ( u ) + L N ε ( u ) = | u | N 2 u log | u | N + f ( u ) in  R N , R N V ( x ) | u | p + | u | N d x < + , u W 1 , p ( R N ) W 1 , N ( R N ) , ( P ε )

where

L t ε ( u ) = ε t Δ t u + V ( x ) | u | t 2 u for  t { p , N }

with N ≥ 2. Further, we assume that 1 < p < N and ɛ is a very small positive parameter. The operator Δ t u = div(|∇u| t−2u) with t ∈ {p, N} is the standard t-Laplace operator and the scalar potential V : R N R is a continuous function. The nonlinearity f : R R has critical exponential growth at infinity, i.e., it behaves like exp ( α | u | N N 1 ) when |u| → for some α > 0, which means that there exists a positive constant α 0 such that the following condition holds:

lim | u | | f ( u ) | exp α | u | N N 1 = 0 if  α > α 0 , + if  α < α 0 .

Throughout the paper, we suppose the following assumptions on the scalar potential V : R N R :

  1. V C ( R N ; R ) and there exists a constant V 0 > 0 such that inf x R N V ( x ) V 0 .

  2. There exists an open and bounded set Λ R N such that

    V 0 = inf x Λ V ( x ) < min Λ V ( x ) .

We define

M = { x Λ : V ( x ) = V 0 } and M δ = { x R N : dist ( x , M ) δ }

for δ > 0 small enough such that M δ ⊂ Λ. Moreover, the nonlinearity f : R R is supposed to satisfy the following conditions:

  1. Let f C 1 ( R , R ) be an odd function such that f(0) = 0, f(s) < 0 for all s < 0 and f(s) > 0 for all s > 0. Further, there exists a constant α 0 ∈ (0, α) with the property that for all τ > 0, there exists κ τ > 0 such that for all s R , we have

    | f ( s ) | τ | s | N 1 + κ τ Φ α 0 | s | N with  Φ ( t ) = exp ( t ) j = 0 N 2 t j j ! and N = N N 1 .

  2. There exists μ > N such that

    s f ( s ) μ F ( s ) 0 for all  s R ,  where F ( s ) = 0 s f ( t ) d t for all  s R .

  3. The mapping s f ( s ) | s | N 2 s is increasing for all s > 0 and decreasing for all s < 0.

  4. There exists a constant γ > 0 such that f(s) ≥ γs μ−1 for all s ≥ 0.

Remark 1.1.

A typical example of a function that satisfies (f1)–(f4) can be considered as

f ( s ) = | s | N 2 s Φ ( | s | N ) for all  s R ,

with α 0 > 1, where N ≥ 2, N = N N 1 and Φ is defined as in (f1).

In order to familiarize the reader with the special behaviors of the classical Sobolev spaces, it is worth pointing out that the space W 1 , p ( R N ) can be distinguished in three different ways, namely:

( a )  the Sobolev case:  p < N , ( b )  the Sobolev limiting case:  p = N , ( c )  the Morrey case:  p > N .

The Sobolev embedding theorem says that for p < N, there holds W 1 , p ( R N ) L q ( R N ) for any q ∈ [p, p*], where p * = N p N p is the critical Sobolev exponent to p. In this scenario, to study variational problems, the nonlinearity cannot exceed the polynomial of degree p*. In contrast to this, for the Sobolev limiting case commonly known as the Trudinger-Moser case, one can notice that p* converges to as p converges to N and thus, we might except that W 1 , N ( R N ) is continuously embedded in L ( R N ) . This is, however, wrong for N > 1. In order to see this, let φ C c ( R N , [ 0,1 ] ) be such that φ ≡ 1 in B 1(0) and φ ≡ 0 in B 2 c ( 0 ) , then the function u ( x ) = φ ( x ) log log 1 + 1 | x | belongs to W 1 , N ( R N ) but not to L ( R N ) . Moreover, in this situation, every polynomial growth is allowed. To fill this gap, it is fairly natural to look for the maximal growth of a function g : R R + such that

sup u W 1 , N ( R N ) u W 1 , N 1 R N g ( u ) | x | β d x < + for all  0 β < N ,

where u W 1 , N = u N N + u N N 1 N and ‖ ⋅ ‖ N is the usual norm of the Lebesgue space L N ( R N ) . It is noteworthy that many authors have independently proved that the maximum growth of such a function g is of exponential type. In that context, we mention the works of Adimurthi-Yang [1] and Li-Ruf [2]. In recent years, the existence and multiplicity of solutions to elliptic equations involving the N-Laplace operator with subcritical and critical growth in the sense of Trudinger-Moser inequality have been extensively studied, motivated by their applicability in many fields of modern mathematics. For a detailed study, we refer to Beckner [3], Chang-Yang [4], Chen-Lu-Zhu [5], Lam-Lu [6], Zhang-Zhu [7] and the references therein.

It should be pointed out here that the Trudinger-Moser type inequalities and the Adams type inequalities have been widely studied by many authors across diverse domains such as Euclidean spaces, Heisenberg groups, Riemannian manifolds, and so on. In this context, we recommend that readers take a look at some works by Chen-Wang-Zhu [8], Cohn-Lu [9], do Ó-Lu-Ponciano [10], Duy-Phi [11], Jiang-Xu-Zhang-Zhu [12], Lam-Lu [13], [14], Li-Lu-Zhu [15], Wang [16], Xue-Zhang-Zhu [17] and the references cited therein.

In the last decade, great attention has been focused on the study of (p, q)-Laplace equations as well as double phase problems in the whole Euclidean space R N due to the broad applications in biophysics, plasma physics, solid state physics, and chemical reaction design, see, for example, the books of Aris [18], Fife [19] and Murray [20] as well as the papers of Myers-Beaghton-Vvedensky [21] and Wilhelmsson [22] and the references therein. On the other hand, concerning the Sobolev limiting case, that is, p < q and q = N, such types of problems are often comparatively less looked upon. This is one of the main motivations for the study in this article. More details on (p, N)-Laplace equations can be found in the papers of Carvalho-Figueiredo-Furtado-Medeiros [23], Chen-Fiscella-Pucci-Tang [24], Fiscella-Pucci [25], Mahanta-Mukherjee-Sarkar [26] and Mahanta-Winkert [27], as well as the references therein.

Moreover, we make a note that one of the hypotheses on the potential function V that appears in (V1) says that the corresponding first-order weighted Sobolev spaces make sense and are well-behaved; see, for instance, Lemma 2.2 and Lemma 2.3, respectively. To address the challenge posed by the lack of compactness, Bartsch-Wang [28] were the first to place assumptions on the potential function V. Further, as an application, they studied the existence and multiplicity of solutions for a superlinear Schrödinger type equation in R N . Afterwards, reducing the conditions on the potential and the nonlinearity, Tang [29] achieved some more general results. Later on, Chen-Lu-Zhu [5], [30], [31], [32] developed and introduced some more generalized form of assumptions on the potential function V, called degenerated and trapping types of potentials, to establish the Trudinger-Moser type inequalities as well as the consequences of the Adams type inequalities, and by employing such inequalities, they studied elliptic and subelliptic PDEs. In addition, we also mention here that Chen-Lu-Zhu [33] showed the existence of extremals for Trudinger-Moser inequalities in R 2 in the presence of trapping potential.

Nowadays, there is a great interest in the study of the time-dependent nonlinear logarithmic Schrödinger equation of the form

(NLS) i ε t Ψ = ε 2 Δ Ψ + ( V ( x ) + E ) Ψ Ψ log | Ψ | 2 for all  ( x , t ) R N × [ 0 , + ) ,

where Ψ : R N × [ 0 , + ) C , N ≥ 2, E R , ɛ is a positive parameter and V is a continuous function satisfying certain hypotheses. It is worth noting that the standing wave solution of (NLS) is of the form Ψ(x, t) = exp(−iEt/ɛ)u(x), where u is a solution of the equation

(1.1) ε 2 Δ u + V ( x ) u = u log u 2 in  R N , u H 1 ( R N ) .

From the point of view of the application, such equations are the main tools for studying quantum physics, quantum optics, effective quantum gravity, nuclear physics, transport and diffusion phenomena, theory of superfluidity and Bose–Einstein condensation. For more information in this direction, we refer to Białynicki-Birula-Mycielski [34], Carles-Gallagher [35], Cazenave [36], Cazenave-Lions [37], Zloshchastiev [38] and the references therein. In addition, in order to study (1.1), there have been several technical difficulties due to the presence of logarithmic nonlinearity. For example, let u be a smooth function satisfying

u ( x ) = | x | N 2 log | x | 1 if  | x | 3 , 0 if  | x | 2 .

By direct computation, one has u H 1 ( R N ) but R N u 2 log u 2 d x = . So, the Euler–Lagrange functional associated to (1.1) is not finite and is no longer C 1 on H 1 ( R N ) . As a result, we cannot directly use the classical critical point theory to study the behavior of solutions of (1.1). To overcome these difficulties, several approaches have been developed in the mathematical literature so far. We will discuss some of them below.

Initially, Cazenave [36] studied the following time-dependent logarithmic Schrödinger equation

(1.2) i u t + Δ u + u log u 2 = 0 in  R × R N

by considering the N-function A and the function space W defined as

A ( s ) = 1 2 s 2 log s 2 if  0 s e 3 , 3 s 2 + 4 e 3 s e 6 if  s e 3 , and W = u H 1 ( R N ) : R N | u 2 log u 2 | d x < + ,

endowed with the Luxemburg norm  W = H 1 ( R N ) + A , where

u A = inf   λ > 0 : R N A ( λ 1 | u | ) d x 1 .

The author defined the associated functional L : W R given by

L ( u ) = 1 2 R N | u | 2 d x 1 2 R N u 2 log u 2 d x for all  u W

and proved the existence of infinitely many critical points of L on the set u W : R N | u | 2 d x = 1 . As a result, he also provided a lot of information about the behavior of the solutions of equation (1.2).

Later, Squassina-Szulkin [39], [40] investigated the following logarithmic Schrödinger equation

(1.3) Δ u + V ( x ) u = Q ( x ) u log u 2 in  R N , u H 1 ( R N ) ,

where V , Q C ( R N , R ) are 1-periodic functions of the variables x 1, x 2, …, x N satisfying the hypotheses

min x R N Q ( x ) > 0 and min x R N ( V + Q ) ( x ) > 0 .

Employing the standard nonsmooth critical point theory of lower semicontinuous functionals, which was developed by Szulkin [41], the authors showed first the existence of positive ground state solutions by adopting the deformation lemma. Then, by using the genus theory, they proved the existence of infinitely many high-energy solutions, which are geometrically distinct under Z N -action. Moreover, several authors used nonsmooth variational techniques to study the logarithmic Schrödinger equations, such as Alves-Ambrosio [42], Alves-de Morais Filho [43], Alves-Ji [44], [45], d’Avenia-Montefusco-Squassina [46], Deng-He-Pan-Zhong [47], Ji-Szulkin [48], Li-Peng-Shuai [49] and Liu-Peng-Zou [50]. In contrast to this, Tanaka-Zhang [51] have also studied (1.3) by considering V, Q as spatially 1-periodic functions of class C 1. The authors showed the existence of infinitely many multi-bump solutions for (1.3), which are distinct under Z N -action, by taking an approach using spatially 2L-periodic problems with L ≫ 1.

During the last decade, Wang-Zhang [52] introduced an advanced way of studying logarithmic equations, which is known as the power approximation method. First, they considered the following semiclassical scalar field equation with power-law nonlinearity

(1.4) Δ u + λ u = | u | p 2 u in  R N , lim | x | u ( x ) = 0 ,

where p ∈ (2, 2*) with 2 * = 2 N N 2 if N ≥ 3 and 2* = + if N ≤ 2. The authors showed that when p ↘ 2, then the ground state solutions of (1.4) either blow up or vanish, and converge to the ground state solutions of the logarithmic-scalar field equation

Δ u = λ u log | u | in  R N , lim | x | u ( x ) = 0 .

In addition, they also proved that the same result holds for bound-state solutions. Later, the authors studied the concentration behavior of nodal solutions of (1.1) in [53] by employing the same idea discussed above.

On the other hand, concerning the penalization method and the Lusternik–Schnirelmann category theory, which are generally used to study the multiplicity of the positive solutions of nonlinear PDEs and their concentration phenomena, we recommend the readers to study the papers of Alves-Figueiredo [54], Ambrosio-Repovš [55], Thin [56] and Zhang-Sun-Liang-Thin [57], see also the references therein. The most important features and novelties of our problem are listed below:

  1. The appearance of the (p, N)-Laplace operator in our problem is nonhomogeneous, and thus, the calculations are more complicated.

  2. Due to the lack of compactness caused by the unboundedness of the domain, the Palais-Smale sequences do not have the compactness property.

  3. The reaction combines the multiple effects generated by the logarithmic term and a term with critical growth with respect to the exponential nonlinearity, making our study more delicate and challenging.

  4. The concentration phenomena create a bridge between the global maximum point of the solution and the global minimum of the potential function.

  5. The proofs combine refined techniques, including variational and topological tools.

To the best of our knowledge, this is the first time in the literature, in which two penalized functions are used simultaneously, one corresponds to the logarithmic nonlinearity and the other one corresponds to the exponential growth. Motivated by all the cited works, especially by the papers of Alves-da Silva [58], Alves-Ji [44] and Squassina-Szulkin [39], we study the existence, multiplicity and concentration phenomena of solutions for problem ( P ε ).

Note that, by the change of variable xɛx, we can see that ( P ε ) is equivalent to the problem

L ̃ p ε ( u ) + L ̃ N ε ( u ) = | u | N 2 u log | u | N + f ( u ) in  R N , R N V ( ε x ) | u | p + | u | N d x < + , u W 1 , p ( R N ) W 1 , N ( R N ) , ( S ε )

where

L ̃ t ε ( u ) = Δ t u + V ( ε x ) | u | t 2 u for  t { p , N } .

Definition 1.2.

We say uX ɛ (see (2.1) for its definition) is a (weak) solution of ( S ε ), if

| u | N 2 u ψ log | u | N L 1 ( R N )

and

u , ψ p , V ε + u , ψ N , V ε = R N | u | N 2 u ψ log | u | N d x + R N f ( u ) ψ d x

is satisfied for all ψX ɛ , where , t , V ε for t ∈ {p, N} is defined as

u , ψ t , V ε = R N | u | t 2 u ψ d x + R N V ( ε x ) | u | t 2 u ψ d x for all  u , ψ X ε .

Now, we state the main results of this article.

Theorem 1.3

(Concentration phenomena). Let hypotheses (V1)–(V2) and (f1)–(f4) be satisfied. Then there exists ɛ 0 > 0 such that for any ɛ ∈ (0, ɛ 0), problem ( P ε ) has a positive solution v ɛ . Further, if η ɛ is the global maximum point of v ɛ , then it holds

lim ε 0 V ( η ε ) = V 0 .

Theorem 1.4

(Multiplicity of positive solutions). Let hypotheses (V1)–(V2) and (f1)–(f4) be satisfied and let δ > 0 be sufficiently small. Then there exists ɛ 1 > 0 such that for ɛ ∈ (0, ɛ 1), the following hold:

  1. problem ( P ε ) has at least cat M δ ( M ) 2 positive solutions, whenever cat M δ ( M ) is an even number;

  2. problem ( P ε ) has at least cat M δ ( M ) + 1 2 positive solutions, whenever cat M δ ( M ) is an odd number.

The paper is organized as follows. In Section 2, we introduce the underlying function spaces, the main tools of the variational framework and some preliminary results. Section 3 is devoted to the study of the penalized problem by using the mountain pass geometry and some topological tools. In Section 4, the properties of the Nehari manifold associated with the penalized problem and the concentration behavior of the positive solutions for ( P ε ) are studied. Finally, in Section 5, we prove Theorem 1.4 by invoking the Lusternik–Schnirelmann category theory.

2 Some preliminary results

This section is devoted to some basic results on Sobolev spaces, Orlicz spaces and related lemmas that will be used to establish the main results of this article. To this end, for t ∈ (1, + ), L t ( R N ) denotes the standard Lebesgue space with the norm ‖ ⋅ ‖ t . Further, if Ω R N , then we define the norm of L t (Ω) by L t ( Ω ) . For nonnegative measurable functions V : R N R , the space L V ε t ( R N ) consists of all real-valued measurable functions such that V ( ε x ) | u | t L 1 ( R N ) and is equipped with the seminorm

u t , V ε = R N V ( ε x ) | u | t d x 1 t for all  u L V ε t ( R N ) ,

which turns into a norm due to hypothesis (V1). The space L V ε t ( R N ) , t , V ε is a separable and uniform convex Banach space (see Pucci-Xiang-Zhang [59]). Note that under the assumption (V1), the embedding L V ε t ( R N ) L t ( R N ) is continuous.

Next, we define

W 1 , t ( R N ) = u L t ( R N ) : | u | L t ( R N ) ,

endowed with the norm

u W 1 , t = u t t + u t t 1 t .

It is well-known that the space W 1 , t ( R N ) , W 1 , t is a separable and uniformly convex Banach space. Note that C c ( R N ) is a dense subset of W 1 , t ( R N ) . Moreover, the critical Sobolev exponent of t is defined by t * = N t N t if t < N and t* = + otherwise. Further, we set

X = W 1 , p ( R N ) W 1 , N ( R N )

and endow it with the norm

u X = u W 1 , p + u W 1 , N .

Then, the space (X, ‖ ⋅‖ X ) is a reflexive and separable Banach space.

The weighted Sobolev space W V ε 1 , t ( R N ) is defined by

W V ε 1 , t ( R N ) = u W 1 , t ( R N ) : R N V ( ε x ) | u | t d x < + ,

equipped with the norm

u W V ε 1 , t = u t t + u t , V ε t 1 t .

The space W V ε 1 , t ( R N ) , W V ε 1 , t is a separable and uniformly convex Banach space, see Proposition 2.1 in Bartolo-Candela-Salvatore [60], thanks to (V1). Moreover, C c ( R N ) is a dense subset of W V ε 1 , t ( R N ) , see Bartolo-Candela-Salvatore [60] and Chen-Chen [61]. From now on, our function space is given by

(2.1) X ε = W V ε 1 , p ( R N ) W V ε 1 , N ( R N ) ,

which is endowed with the norm

u X ε = u W V ε 1 , p + u W V ε 1 , N for all  u X ε .

Because of assumptions (V1) and Proposition 2.1 in Bartolo-Candela-Salvatore [60], it is easy to see that ( X ε , X ε ) is a reflexive and separable Banach space. In the entire paper, C, C 1, C 2, C 3, … denote some fixed positive constants possibly different at different places. Moreover, for any Banach space (X, ‖ ⋅‖ X ), we denote its continuous dual by X * , X * and o n (1) denotes the real sequence such that o n (1) → 0 as n. By ⇀ we mean the weak convergence and → means the strong convergence, while u ± = max {±u, 0} stand for the positive and negative part of a function u, respectively. Furthermore, B r (x 0) is an open ball centered at x 0 R N with radius r > 0 and B r = B r (0). Finally, for any set S R N , we denote its Lebesgue measure by |S| and its complement by S c .

Now, we shall discuss some basic properties of Orlicz spaces.

Definition 2.1.

We say that a continuous function F : R [ 0 , + ) is a N-function if there hold

  1. F is an even function.

  2. F ( s ) = 0 if and only if s = 0 and F is convex.

  3. lim s 0 F ( s ) s = 0 and lim s F ( s ) s = .

Further, we say that a N-function F satisfies the Δ2-condition, which is denoted by F Δ 2 , if there exists a constant c > 0 such that

F ( 2 s ) c F ( s ) for all  s 0 .

The conjugate of the N-function F is denoted by F ̃ and defined as

F ̃ = max s 0 { t s F ( s ) } for all  t 0 .

Note that F ̃ is always an N-function and F ̃ ̃ = F , i.e., F and F ̃ are complementary to each other. Now, we define the Orlicz space associated with the N-function F by

L F ( R N ) = u L loc 1 ( R N ) : R N F | u | λ d x < +  for some  λ > 0 ,

endowed with the Luxemburg norm

u F = inf   λ > 0 : R N F | u | λ d x 1 .

Clearly, the space L F ( R N ) , F is a Banach space. Consequently, the Young’s type and Hölder’s type inequalities in Orlicz spaces are given by

s t F ( s ) + F ̃ ( t ) for all  s , t 0

and

R N u v d x 2 u F v F ̃ for all  u L F ( R N ) , v L F ̃ ( R N ) .

Moreover, if F , F ̃ Δ 2 , then the space L F ( R N ) is reflexive and separable. Again, the Δ2-condition implies at once that

L F ( R N ) = u L loc 1 ( R N ) : R N F ( | u | ) d x < +

and

(2.2) u n u in  L F ( R N ) if and only if R N F ( | u n u | ) d x 0 as  n .

Now, we shall characterize an important property of the N-function. It states that if F is an N-function of class C 1 and F ̃ be its conjugate such that the following condition holds

(2.3) 1 < l F ( s ) s F ( s ) m < + for all s 0 ,

then F , F ̃ Δ 2 .

Due to some mathematical difficulties in ( S ε ), we cannot directly apply smooth variational techniques to study the problem ( S ε ). Indeed, if we set the energy functional I ɛ associated with ( S ε ), which is defined on the space X ɛ as

(2.4) I ε ( u ) = 1 p u W V ε 1 , p p + 1 N u W V ε 1 , N N R N H ( u ) d x R N F ( u ) d x for all  u X ε ,

where

H ( s ) = 1 N | s | N log | s | N 1 N | s | N ,

then the energy functional I ɛ is not well-defined on X ɛ , since it may happen that there exists uX ɛ satisfying R N | u | N log | u | N d x = and hence, I ɛ (u) = +. Inspired by the works of [39], [43], [44], we can avoid this difficulty by choosing

H 2 ( s ) H 1 ( s ) = 1 N | s | N log | s | N for all  s R ,

where H 1 is a nonnegative C 1-function, which is also convex and H 2 is also a nonnegative C 1-function satisfying some growth condition. Hence, one can easily obtain from (2.4) that

I ε ( u ) = 1 p u W V ε 1 , p p + 1 N u W V ε 1 , N N + 1 N u N N + R N H 1 ( u ) d x R N H 2 ( u ) d x R N F ( u ) d x .

This technique guarantees that I ɛ may be expressed as the combination of a C 1-functional with a convex and lower semicontinuous functional. Therefore, the critical point theory for lower semicontinuous functionals, as established by Szulkin [41], can be used to examine solutions of ( P ε ).

Another feature and novelty of ( S ε ) is the fact that the corresponding energy functional defined in (2.4) is not a C 1-functional and hence, we shall not be able to find the multiplicity of solutions of ( S ε ) by using smooth variational methods together with the Lusternik–Schnirelmann category theory. To overcome this difficulty, we shall work with a newly constructed Banach space, where the functional I ɛ is C 1. Inspired by the work of Shen-Squassina [62], we fix δ > 0 sufficiently small and define H 1 and H 2 by

H 1 ( s ) =     0 if  s = 0 , 1 N | s | N log | s | N if  0 < | s | < ( N 1 ) δ , 1 N | s | N log ( N 1 ) δ N + N + 1 + N δ | s | N 1 ( N 1 ) δ N N ( N 1 ) if  | s | ( N 1 ) δ ,

and

H 2 ( s ) =     0 if  | s | ( N 1 ) δ , 1 N | s | N log | s | N ( N 1 ) δ N + N δ | s | N 1 N + 1 N | s | N ( N 1 ) δ N N ( N 1 ) if  | s | ( N 1 ) δ ,

so that

(2.5) H 2 ( s ) H 1 ( s ) = 1 N | s | N log | s | N for all  s R .

The functions H 1 and H 2 have the following properties, respectively.

  • ( H 1 )

    1. For δ > 0 small enough, H 1 is convex, even and of class C 1 ( R , R ) .

    2. H 1 ( s ) 0 and H 1 ( s ) s 0 for all s R .

    3. For any q > N, there exists constants C 1, C 2 > 0 such that

      | H 1 ( s ) | C 1 | s | q 1 + C 2 for all  s R .

    4. There exists constants C 1, C 2 > 0 such that

      | H 1 ( s ) | C 1 | s | N + C 2 for all  s R .

  • ( H 2 )

    1. There hold H 2 ( s ) 0 for all s > 0 and H 2 ( s ) > 0 for all s > (N − 1)δ.

    2. H 2 C 2 ( R , R ) and for any q > N, there exists a constant C = C q > 0 such that

      | H 2 ( s ) | C | s | q 1 and | H 2 ( s ) | C | s | q for all  s R .

    3. The map s H 2 ( s ) s N 1 is nondecreasing for s > 0 and strictly increasing for s > (N − 1)δ.

    4. H 2 is an odd function and there holds lim s H 2 ( s ) s N 1 = .

The following lemmas can be directly obtained from the classical Sobolev embedding theorem.

Lemma 2.2.

Let (V1) be satisfied. If q ∈ [p, p*], then the following embeddings are continuous

W V ε 1 , p ( R N ) W 1 , p ( R N ) L q ( R N )

with min { 1 , V 0 } u W 1 , p p u W V ε 1 , p p for all u W V ε 1 , p ( R N ) . Furthermore, the embedding W V ε 1 , p ( R N ) L loc q ( R N ) is compact for any q ∈ [1, p*).

Lemma 2.3.

Let (V1) be satisfied. If s ∈ [N, + ), then the following embeddings are continuous

W V ε 1 , N ( R N ) W 1 , N ( R N ) L s ( R N )

with min { 1 , V 0 } u W 1 , N N u W V ε 1 , N N for all u W V ε 1 , N ( R N ) . Furthermore, the embedding W V ε 1 , N ( R N ) L loc s ( R N ) is compact for any s ∈ [1, + ).

Corollary 2.4.

Let (V1) be satisfied. Then, in view of Lemma 2.2 and Lemma 2.3, the embeddings

X ε W 1 , p ( R N ) W 1 , N ( R N ) L ϑ ( R N )

are continuous for any ϑ ∈ [p, p*] ∪ [N, + ). Also, the embedding X ε L loc ϑ ( R N ) is compact for any ϑ ∈ [1, + ).

Remark 2.5.

Let (V1) be satisfied. Then, the following continuous embeddings hold:

X ε W V ε 1 , t ( R N ) W 1 , t ( R N ) for  t { p , N } .

The next two results can be found in Shen-Squassina [62].

Lemma 2.6.

The function H 1 is an N-function and there holds H 1 , H ̃ 1 Δ 2 . In particular, the Orlicz space L H 1 ( R N ) is a reflexive and separable Banach space, where

L H 1 ( R N ) = u L loc 1 ( R N ) : R N H 1 | u | d x < + ,

equipped with the Luxemburg norm

u H 1 = inf   λ > 0 : R N H 1 | u | λ d x 1 .

Corollary 2.7.

The functional Θ : L H 1 ( R N ) R given by u R N H 1 ( u ) d x is of class C 1 L H 1 ( R N ) , R with

Θ ( u ) , v = R N H 1 ( u ) v d x for all  u , v L H 1 ( R N ) .

Remark 2.8.

Note that the condition (2.3) is satisfied by the N-function H 1 with l ∈ (1, N) and m = N.

We define now the spaces

Y = X L H 1 ( R N ) and Y ε = X ε L H 1 ( R N )

endowed with the norms

u Y = u X + u H 1 for all  u Y and u Y ε = u X ε + u H 1 for all  u Y ε .

Thanks to Lemma 2.6, the spaces (Y, ‖ ⋅‖ Y ) and ( Y ε , Y ε ) are reflexive and separable Banach spaces. Moreover, we have the continuous embeddings

Y ε X ε and Y ε L H 1 ( R N ) .

Similarly, these continuous embeddings are also true, if we replace Y ɛ by Y and X ɛ by X, respectively. Next, we denote by S r (or by S r ) the best constant in the embedding from Y ɛ (or Y) into some Lebesgue space L r ( R N ) .

Lemma 2.9.

The embedding Y L θ ( R N ) is continuous for any θ ∈ [p, p*] ∪ [N, + ). Consequently, the embedding Y L loc θ ( R N ) is compact for any θ ∈ [1, + ). Moreover, under (V1), these embeddings also hold true if we replace Y by Y ɛ .

Now, we recall the following version of Lions’ compactness lemma, see Alves-Figueiredo [[54], Proposition 4].

Lemma 2.10.

Let { u n } n N Y ε be a bounded sequence in Y ɛ and there holds

lim inf n sup y R N B R ( y ) | u n | N d x = 0

for some R > 0, then we have u n → 0 in L υ ( R N ) as n for any υ ∈ (N, + ).

The next lemma can be found in Alves-da Silva [58].

Lemma 2.11.

In view of Remark 2.8, we have for any u L H 1 ( R N ) that

min u H 1 l , u H 1 N R N H 1 ( | u | ) d x max u H 1 l , u H 1 N .

From Yang [63], we have the following result.

Corollary 2.12.

The function Φ ( t ) = exp ( t ) j = 0 N 2 t j j ! is increasing and convex in [0, + ). Moreover, for any ≥ 1, t ≥ 0 real numbers and N ≥ 2, it holds that

exp ( t ) j = 0 N 2 t j j ! exp ( t ) j = 0 N 2 ( t ) j j ! .

The inequality in the following lemma is known as the Trudinger-Moser inequality, which was first studied by Adimurthi-Yang [1].

Lemma 2.13.

For all α > 0, 0 ≤ β < N and u W 1 , N ( R N ) with N ≥ 2, we have Φ α | u | N | x | β L 1 ( R N ) . Furthermore, we have for all α 1 β N α N and γ > 0

sup u W γ 1 , N 1 R N Φ α | u | N | x | β d x < + , where u W γ 1 , N = u N N + γ u N N 1 N ,

Φ is defined as in (f1) and α N = N ω N 1 1 N 1 , with ω N−1 being the volume of the unit sphere S N−1. Also, the above inequality is sharp for α > 1 β N α N , i.e., the supremum is infinity.

Remark 2.14.

To study problem ( P ε ), we are going to use Lemma 2.13 with β = 0 and γ = 1.

3 Existence of solution for the penalized problem

In this section, we shall establish the existence of a solution for the penalized problem ( S ̃ ε ) by using the mountain pass theorem stated in Pucci-Serrin [[64], p. 142].

Note that for the well-definedness of the functional I ɛ defined in Section 2, we shall restrict I ɛ to the space Y ɛ , which will be denoted by E ɛ (u) = I ɛ (u) for all uY ɛ . Hence, in view of the conditions on H 1 , V and Lemma 2.13, the functional I ɛ is a C 1-functional on the space Y ɛ and its Gâteaux derivative is given by

E ε ( u ) , ψ = u , ψ p , V ε + u , ψ N , V ε + R N | u | N 2 u ψ d x + R N H 1 ( u ) ψ d x R N H 2 ( u ) ψ d x R N f ( u ) ψ d x

for all ψY ɛ , where ⟨⋅, ⋅⟩ is the duality pairing between Y ε * and Y ɛ .

Let , ′ > 0 be small enough such that V 0 + 1 ≥ 2( + ′) and take a > (N − 1)δ such that H 2 ( a ) a N 1 = . Then, we define

H ̂ 2 ( s ) =     H 2 ( s ) if  0 s a , s N 1 if  s a .

Further, let t 1 > (N − 1)δ be such that a ∈ (t 1, t 2) and h C 1 [ t 1 , t 2 ] satisfying the following properties:

  1. h ( s ) H ̂ 2 ( s ) for all s ∈ [t 1, t 2].

  2. h ( t i ) = H ̂ 2 ( t i ) and h ( t i ) = H ̂ 2 ( t i ) for i ∈ {1, 2}.

  3. The map s h ( s ) s N 1 is nondecreasing on [t 1, t 2].

Define another function

H ̃ 2 ( s ) =     H ̂ 2 ( s ) if  s [ t 1 , t 2 ] , h ( s ) if  s [ t 1 , t 2 ] .

If χ Λ denotes the characteristic function corresponding to the set Λ, then we introduce the first penalized nonlinearity G 2 : R N × [ 0 , + ) R , which is defined by

G 2 ( x , s ) = χ Λ ( x ) H 2 ( s ) + ( 1 χ Λ ( x ) ) H ̃ 2 ( s ) for all  ( x , s ) R N × [ 0 , + ) .

Note that H 2 is an odd function and hence, we can extend the definition of G 2 to R N × R by setting

G 2 ( x , s ) = G 2 ( x , s ) for all  ( x , s ) R N × ( , 0 ] .

The following properties can be proved by using the definition of G 2 :

  • ( A )

    1. There exists a constant C = C q > 0 and q > N such that

      | G 2 ( x , s ) | | s | N 1 + C | s | q 1 for all  ( x , s ) R N × R .

    2. | G 2 ( x , s ) | | H 2 ( s ) | for all ( x , s ) R N × R . Consequently, in view of ( H 2 ) (b), we have

      | G 2 ( x , s ) | C | s | q for all  ( x , s ) R N × R .

    3. | G 2 ( x , s ) | | s | N 1 for all ( x , s ) Λ c × R .

    4. 1 N | s | N + H 2 ( s ) 1 N H 2 ( s ) s + 1 N G 2 ( x , s ) s G 2 ( x , s ) 0 for all ( x , s ) R N × R .

    5. The map s G 2 ( x , s ) s N 1 is nondecreasing for all ( x , s ) R N × ( 0 , + ) .

On the other hand, we set f ( a ) a N 1 = and define

f ̂ ( s ) =     f ( s )   if  0 s a , s N 1  if  s a .

Now, we consider the function η such that η C 1 [ t 1 , t 2 ] satisfying the following properties:

  • (η1)   η ( s ) f ̂ ( s ) for all s ∈ [t 1, t 2].

  • (η2)   η ( t i ) = f ̂ ( t i ) and η ( t i ) = f ̂ ( t i ) for i ∈ {1, 2}.

  • (η3)  The map s η ( s ) s N 1 is nondecreasing on [t 1, t 2].

Further, we define another function

f ̃ ( s ) =     f ̂ ( s ) if  s [ t 1 , t 2 ] , η ( s ) if  s [ t 1 , t 2 ] .

Next, we introduce the second penalized nonlinearity g : R N × [ 0 , + ) R , which is defined by

g ( x , s ) = χ Λ ( x ) f ( s ) + ( 1 χ Λ ( x ) ) f ̃ ( s ) for all  ( x , s ) R N × [ 0 , + ) .

Observe that f is an odd function, therefore we can extend the definition of g to R N × R by setting

g ( x , s ) = g ( x , s ) for all  ( x , s ) R N × ( , 0 ] .

Moreover, we also define

Λ ε = { x R N : ε x Λ } , G 2 ( x , s ) = 0 s G 2 ( x , t ) d t for all  ( x , s ) R N × R , G ( x , s ) = 0 s g ( x , t ) d t for all  ( x , s ) R N × R .

By using the definition of g, one can prove the following properties:

  • ( B )

    1. g(x, s) ≤ 0 for all ( x , s ) R N × ( , 0 ] and g(x, s) ≥ 0 for all ( x , s ) R N × [ 0 , + ) .

    2. |g(x, s)| ≤ |f(s)| for all ( x , s ) R N × R .

    3. μ G ( x , s ) s g ( x , s ) for all ( x , s ) Λ × R .

    4. N G ( x , s ) s g ( x , s ) | s | N for all ( x , s ) Λ c × R .

    5. The map s g ( x , s ) | s | N 2 s is nondecreasing for all ( x , s ) R N × R \ { 0 } .

Since our goal is to study the positive solutions of ( P ε ), we deal with the following penalized problem:

L ̃ p ε ( u ) + L ̃ N ε ( u ) + | u | N 2 u = G 2 ( ε x , u ) H 1 ( u ) + g ( ε x , u ) in  R N , R N V ( ε x ) | u | p + | u | N d x < + , u Y ε . ( S ̃ ε )

Note that if u ɛ is a positive solution of ( S ̃ ε ) with 0 < u ɛ (x) < t 1 for all x R N \ Λ ε , then G 2 ( ε x , u ε ) = H 2 ( u ε ) and g(ɛx, u ɛ ) = f(u ɛ ). Due to this fact, we conclude that v ε ( x ) = u ε ( x ε ) is a positive solution of ( P ε ). Now, we define the functional J ε : Y ε R associated with ( S ̃ ε ) by

(3.1) J ε ( u ) = 1 p u W V ε 1 , p p + 1 N u W V ε 1 , N N + u N N + R N H 1 ( u ) d x R N G 2 ( ε x , u ) d x R N G ( ε x , u ) d x for all  u Y ε .

Clearly, J ɛ is well-defined, of class C 1 ( Y ε , R ) and the critical points of J ɛ are weak solutions of ( S ̃ ε ). Note that, from the assumptions (f1), (f2) and Corollary 2.12, one can easily verify that for any τ > 0, ϑ > N, there exists a constant κ ̃ τ > 0 and 0 < α 0 < α such that for all s R , we have

(3.2) | f ( s ) | τ | s | N 1 + κ ̃ τ | s | ϑ 1 Φ ( α | s | N ) , | F ( s ) | τ | s | N + κ ̃ τ | s | ϑ Φ ( α | s | N ) .

The following two lemmas show that the functional J ɛ satisfies the mountain pass geometry.

Lemma 3.1

(Mountain Pass Geometry-I). There exist ρ ∈ (0, 1] very small enough and ȷ > 0 such that J ɛ (u) ≥ ȷ for all uY ɛ with u Y ε = ρ .

Proof.

From ( B ) (b) and (3.2), we have

(3.3) | G ( x , s ) | τ | s | N + κ ̃ τ | s | ϑ Φ ( α | s | N ) for all  ( x , s ) R N × R .

Let σ ∈ (0, 1] be sufficiently small such that 0 < u Y ε σ . Further, we choose r, r′ > 1 satisfying 1 r + 1 r = 1 , then, by using Hölder’s inequality, Corollary 2.12 and Lemma 2.9, we obtain from (3.3) that

(3.4) R N | G ( x , u ) | d x τ S N N u Y ε N + κ ̃ τ S ϑ r ϑ u Y ε ϑ   R N Φ r α u Y ε N | u ̃ | N d x 1 r ,

where u ̃ = u / u Y ε . Since u Y ε is very small, we can choose r′ > 1 close to 1 and α > α 0 close to α 0 such that r α u Y ε N α N holds. Take γ > 0 with γV 0, then we have u ̃ W γ 1 , N u ̃ W V ε 1 , N u ̃ Y ε = 1 . Consequently, by using (3.4) and Lemma 2.13, there exists a constant C ̃ > 0 such that

(3.5) R N | G ( x , u ) | d x τ S N N u Y ε N + κ ̃ τ C ̃ S ϑ r ϑ u Y ε ϑ .

Note that u Y ε 1 , therefore it follows from ( A ) (b) and Lemma 2.9 that

(3.6) R N | G 2 ( x , u ) | d x C S q q u Y ε q C S q q u Y ε N .

Hence, in view of Lemma 2.11, we obtain from (3.1), (3.5) and (3.6) that

J ε ( u ) 1 N u W V ε 1 , p N + u W V ε 1 , N N + u H 1 N C S q q u Y ε N τ S N N u Y ε N κ ̃ τ C ̃ S ϑ r ϑ u Y ε ϑ 3 1 N N C S q q + τ S N N u Y ε N C ϑ u Y ε ϑ ,

for all uY ɛ satisfying u Y ε σ , where C ϑ = κ ̃ τ C ̃ S ϑ r ϑ . Choose C S q q + τ S N N = 2 3 N N and define the function

ψ ( t ) = 1 3 N + 1 N t N C ϑ t ϑ for all  t [ 0 , σ ] .

By using elementary calculus, we infer that ψ admits a positive maximum ȷ in [0, σ] at a point ρ ∈ (0, σ]. Moreover, for all uY ɛ satisfying u Y ε = ρ , we obtain

J ε ( u ) 1 3 N N ρ N C ϑ ρ ϑ ψ ( ρ ) = ȷ > 0 .

This completes the proof. □

Lemma 3.2

(Mountain Pass Geometry-II). Let ρ ∈ (0, 1] be as in Lemma 3.1, then there exists a nonnegative function eY ɛ with e Y ε > ρ satisfying J ɛ (e) < 0.

Proof.

Define

O ε = u Y ε : | supp ( | u | ) Λ ε | > 0

and let u O ε \ { 0 } be such that u(x) ≥ 0 a.e. in R N . Define

Ψ ( t ) = t μ G ( x , t u ) G ( x , u ) for all  x Λ and t 1 .

From ( B ) (c), we have

Ψ ( t ) = t μ 1 g ( x , t u ) t u μ G ( x , t u ) 0 for all  x Λ  and for all  t 1 .

It follows that Ψ is an increasing function on [1, + ). Hence, we obtain G(x, tu) ≥ t μ G(x, u) for all x ∈ Λ and t ≥ 1. Further, since μ > N and u(x) ≥ 0 a.e. in R N , we infer that G(x, tu) ≥ t N G(x, u) for all x ∈ Λ and t ≥ 1. Similarly, by using ( B ) (d), we can prove that G(x, tu) ≥ t N G(x, u) for all x ∈ Λ c and t ≥ 1. Consequently, we obtain

(3.7) G ( x , t u ) t N G ( x , u ) for all  x R N  and for all  t 1 .

Notice that for each x R N and t > 0, we can write

H 1 ( t u ) = χ Λ ε ( x ) H 1 ( t u ) + ( 1 χ Λ ε ( x ) ) H 1 ( t u ) .

Now, by using the definition of G 2 and (2.5), it follows that

(3.8) R N H 1 ( t u ) G 2 ( ε x , t u ) d x = 1 N R N χ Λ ε | t u | N log | t u | N d x 1 N { t u t 1 } ( 1 χ Λ ε ) | t u | N log | t u | N d x + { t u > t 1 } ( 1 χ Λ ε ) H 1 ( t u ) H ̃ 2 ( t u ) d x .

By the definition of H ̃ 2 and ( H 1 ) (d), we have

H ̃ 2 ( s ) 0 and 0 H 1 ( s ) C 1 s N + C 2 for all  s 0 .

In addition, it follows from uY ɛ that

{ t u > t 1 } | t u | N d x K t N and | { t u > t 1 } | K 1 t N ,

where K = u N N and K 1 = K t 1 N . Consequently, from the above information, we can deduce that

(3.9) { t u > t 1 } ( 1 χ Λ ε ) H 1 ( t u ) H ̃ 2 ( t u ) d x C t N ,

where C = C 1 K + C 2 K 1 > 0. Let t ≥ 1 be large enough, then by using (3.7), (3.8) and (3.9), we obtain from (3.1) that

(3.10) J ε ( t u ) t N 1 p   u W V ε 1 , p N + u W V ε 1 , N N + u N N p R N G ( ε x , u ) d x 1 N R N χ Λ ε | u | N log | u | N d x log t   R N χ Λ ε | u | N d x + { t u t 1 } ( 1 χ Λ ε ) | u | N d x 1 N { t u t 1 } ( 1 χ Λ ε ) | u | N log | u | N d x + C .

Due to the application of Lebesgue’s dominated convergence theorem, we obtain

(3.11) { t u t 1 } ( 1 χ Λ ε ) | u | N d x 0 as  t .

Now, by using (2.5), ( H 2 ) (b), Lemma 2.9 and the fact that u L H 1 ( R N ) , we have

(3.12) 1 N { t u t 1 } ( 1 χ Λ ε ) | u | N log | u | N d x R N | H 1 ( u ) | d x + R N | H 2 ( u ) | d x < + .

Sending t in (3.10) and using (3.11) as well as (3.12), we deduce that J ɛ (tu) → − as t. Taking e = tu with t sufficiently large shows that assertion of the lemma. □

To use the mountain pass theorem, it is necessary to verify the Palais-Smale compactness condition at a suitable level c. We say that a sequence { u n } n N Y ε is a (PS) c sequence for J ɛ at any suitable level c R if

(3.13) J ε ( u n ) c and sup φ Y ε = 1 | J ε ( u n ) , φ | 0 as n .

If this sequence has a convergent subsequence in Y ɛ , we say that J ɛ satisfies (PS) c condition at any suitable level c R .

Note that the following logarithmic inequality is useful to prove the boundedness of (PS) c sequences for J ɛ .

Lemma 3.3.

Let N ≥ 2 with N < s and uL N ɛ ) ∩ L s ɛ ). Then, we have

Λ ε | u | N log | u | u L N ( Λ ε ) d x s s N u L N ( Λ ε ) log u L s ( Λ ε ) u L N ( Λ ε ) .

Proof.

By using the logarithmic interpolation inequality in Del Pino-Dolbeault [[65], p. 153] and applying a similar procedure as in Alves-Ambrosio [[42], Lemma 3.2], the lemma can be proved. □

Remark 3.4.

To study quasilinear elliptic problems involving N-Laplace operator, generally one requires the following condition

(3.14) lim sup n u n W 1 , N N < α N α 0

to handle terms containing critical exponential growth. Such type of inequality originates by default from the well-known Palais-Smale condition or Cerami condition at a suitable level c.

Whereas, in this article, due to the presence of logarithmic nonlinearity, by using the (PS) c condition it is difficult to directly prove the boundedness of the corresponding Palais-Smale sequence as well as we can not obtain inequality of type (3.14). To show the boundedness of such type of sequence, we need the inequality (3.14) along with some extra computational work. Moreover, one can see that the inequality (3.14) can be assumed because of Lemma 2.3 due to the fact that the bounedness of u n W 1 , N does not imply the boundedness of u n W V ε 1 , N in general.

Lemma 3.5.

Let { u n } n N Y ε be a (PS) c sequence for J ɛ satisfying lim sup n u n W 1 , N N < α N α 0 . Then, the sequence { u n } n N is bounded in Y ɛ .

Proof.

Let { u n } n N Y ε be a (PS) c sequence for J ɛ and let lim sup n u n W 1 , N N < α N α 0 be satisfied. Now, by using (3.13) and the properties of ( B ) , there exists d > 0 such that, as n, we have

(3.15) c + d u n Y ε + o n ( 1 ) J ε ( u n ) 1 N J ε ( u n ) , u n 1 p 1 N u n W V ε 1 , p p + R N H 1 ( u n ) 1 N H 1 ( u n ) u n + 1 N G 2 ( ε x , u n ) u n G 2 ( ε x , u n ) d x 1 N R N | u n | N d x + R N H 2 ( u n ) 1 N H 2 ( u n ) u n + 1 N G 2 ( ε x , u n ) u n G 2 ( ε x , u n ) d x T ( u n ) ,

where we have used

R N H 1 ( u n ) 1 N H 1 ( u n ) u n + 1 N H 2 ( u n ) u n H 2 ( u n ) d x = 1 N R N | u n | N d x .

Observe that

R N = Λ ε { | u n | t 1 } Λ ε c { | u n | > t 1 } .

Consequently, by using ( A ) (d), one can easily deduce that

(3.16) T ( u n ) 1 N Λ ε | u n | N d x + Λ ε c { | u n | > t 1 } 1 N | u n | N + H 2 ( u n ) 1 N H 2 ( u n ) u n + 1 N G 2 ( ε x , u n ) u n G 2 ( ε x , u n ) d x 1 N Λ ε | u n | N d x .

Combining (3.15) and (3.16), we obtain

(3.17) 1 N Λ ε | u n | N d x c + d u n Y ε + o n ( 1 ) as  n .

By using ( H 1 ) (d) and (3.17), we can find constants c ̃ , d ̃ > 0 such that

(3.18) Λ ε H 1 ( u n ) d x c ̃ + d ̃ u n Y ε + o n ( 1 ) as  n .

On the other hand, by using Lemma 3.3 with D = s s N and Lemma 2.9, we have

(3.19) Λ ε | u n | N log | u n | N d x N u n L N ( Λ ε ) N D N u n L N ( Λ ε ) log u n L N ( Λ ε ) + D N u n L N ( Λ ε ) log u n L s ( Λ ε ) N u n L N ( Λ ε ) N + D N u n L N ( Λ ε ) log u n L N ( Λ ε ) + D ̃ u n Y ε log D ̃ u n Y ε ,

where the constant D ̃ > 0 is independent of ɛ. Recall that in view of Lemma 4.2 of Alves-da Silva [58], there exists ξ ∈ (0, 1) and a constant A > 0 such that

(3.20) | t log t | A ( 1 + t 1 + ξ ) for all  t 0 .

Due to the above inequality and (3.17), we obtain

(3.21) u n L N ( Λ ε ) N log u n L N ( Λ ε ) A N 1 + u n L N ( Λ ε ) N 1 + ξ A ̃ 1 1 + u n Y ε 1 + ξ + o n ( 1 )

as n. Likewise, by using (3.20) and Lemma 2.9, we have

(3.22) u n L N ( Λ ε ) log u n L N ( Λ ε ) A 1 + u n L N ( Λ ε ) 1 + ξ A ̃ 2 1 + u n Y ε 1 + ξ , D ̃ u n Y ε log D ̃ u n Y ε A 1 + D ̃ u n Y ε 1 + ξ ) A ̃ 3 1 + u n Y ε 1 + ξ ,

where in the above estimates A ̃ i with i = 1, 2, 3 are positive constants. Now, by using (3.21) and (3.22) in (3.19), we deduce that there exists a constant A ̃ > 0 such that

(3.23) Λ ε | u n | N log | u n | N d x A ̃ 1 + u n Y ε 1 + ξ + o n ( 1 ) as  n .

In virtue of ( B ) (b), (f1) and Corollary 2.12, we can deduce that

(3.24) | G ( x , s ) | τ | s | N + κ τ | s | Φ ( α | s | N ) for all  ( x , s ) R N × R .

From the assumption, it follows that there exists m 0 > 0 and n 0 N sufficiently large such that

u n W 1 , N N < m 0 < α N α 0 for all  n n 0 .

Take rN with r = r r 1 > 1 and satisfying 1 r + 1 r = 1 . Let r′ close to 1 and α > α 0 close to α 0 such that we still have r α u n W 1 , N N < m 0 < α N for all nn 0. Consequently, by applying Hölder’s inequality, Corollary 2.12 and Lemma 2.9, we obtain from (3.24) that

(3.25) R N | G ( ε x , u n ) | d x τ u n N N + κ τ u n r   R N Φ r α u n W 1 , N N | u ̃ n | N d x 1 r τ u n N N + κ τ C S r 1 u n Y ε

for n large enough, where u ̃ n = u n u n W 1 , N . Moreover, due to Lemma 2.13, we have

C = sup n n 0 R N Φ r α u n W 1 , N N | u ̃ n | N d x 1 r < + .

By using (2.5)(3.18)(3.23) and the growth |G 2(ɛx, s)| ≤ |s| N for all ( x , s ) Λ ε c × R , we have, as n, that

(3.26) R N H 1 ( u n ) G 2 ( ε x , u n ) d x Λ ε c H 1 ( u n ) d x u n N N 1 N Λ ε | u n | N log | u n | N d x R N H 1 ( u n ) d x ( c ̃ + d ̃ u n Y ε ) A ̃ N 1 + u n Y ε 1 + ξ u n N N + o n ( 1 ) .

In view of (3.25)(3.26) and the fact that { u n } n N is a (PS) c sequence for J ɛ , we obtain, as n, that

(3.27) c + o n ( 1 ) = J ε ( u n ) 1 p u n W V ε 1 , p p + 1 N u n W V ε 1 , N N + 1 N τ u n N N κ τ C S r 1 u n Y ε + R N H 1 ( u n ) d x ( c ̃ + d ̃ u n Y ε ) A ̃ N 1 + u n Y ε 1 + ξ .

Since τ > 0 is arbitrary and > 0 is small enough, we can choose τ small enough such that τ + 2 1 N . Consequently, by using (3.27) and Lemma 2.11, there exists constants C 1, C 2, C 3 > 0 such that, as n, we have

(3.28) C 1 + C 2 u n Y ε + C 3 u n Y ε 1 + ξ + o n ( 1 ) 1 N u n W V ε 1 , p p + u n W V ε 1 , N N + min u n H 1 l , u n H 1 N ,

where 1 < l < N. For the rest of the proof, we fix ξ ∈ (0, 1) such that 1 + ξ < p < l. If possible, let u n H 1 1 , then we obtain from (3.28) that

(3.29) C 1 + C 2 u n Y ε + C 3 u n Y ε 1 + ξ + o n ( 1 ) 1 N u n W V ε 1 , p p + u n W V ε 1 , N N + u n H 1 N as  n .

In this case, we have three possibilities as follows:

Case-1: Let u n W V ε 1 , p and u n W V ε 1 , N as n. It follows that u n W V ε 1 , N N u n W V ε 1 , N p > 1 for n large enough. Consequently, we obtain from (3.29) that

C 1 + C 2 u n Y ε + C 3 u n Y ε 1 + ξ + o n ( 1 ) 2 1 p N u n X ε p + u n H 1 N as  n .

Dividing u n X ε p on both sides and letting n, we get 0 2 1 p N > 0 , which is a contradiction.

Case-2: Let u n W V ε 1 , p as n and u n W V ε 1 , N is bounded. Dividing u n W V ε 1 , p on both the sides of (3.29) and letting n, we get 0 1 N > 0 , which is again a contradiction.

Case-3: Let u n W V ε 1 , N as n and u n W V ε 1 , p is bounded. Similar to Case-2, we get a contradiction.

Suppose that u n H 1 as n, then we can assume that u n H 1 > 1 for n large enough and hence, we obtain from (3.28) that

(3.30) C 1 + C 2 u n Y ε + C 3 u n Y ε 1 + ξ + o n ( 1 ) 1 N u n W V ε 1 , p p + u n W V ε 1 , N N + u n H 1 l as  n .

In this case, we have four possibilities as follows:

Case-1: If u n W V ε 1 , p and u n W V ε 1 , p are bounded, then dividing u n H 1 l on both sides of (3.30) and letting n, we get 0 ≥ 1 > 0, which is a contradiction.

Case-2: Let u n W V ε 1 , p and u n W V ε 1 , N as n. It follows that u n W V ε 1 , N N u n W V ε 1 , N p > 1 and u n H 1 l u n H 1 p > 1 for n large enough. Hence, we obtain from (3.30) that

C 1 + C 2 u n Y ε + C 3 u n Y ε 1 + ξ + o n ( 1 ) 3 1 p N u n Y ε p as  n .

Dividing u n Y ε p on both sides and letting n, we get 0 3 1 p N > 0 , which is again contradiction.

Case-3: Let u n W V ε 1 , p as n and u n W V ε 1 , N is bounded. It follows that u n H 1 l u n H 1 p > 1 for n large enough. Consequently, from (3.30), we have

C 1 + C 2 u n Y ε + C 3 u n Y ε 1 + ξ + o n ( 1 ) 2 1 p N u n W V ε 1 , p + u n H 1 p as  n .

Dividing u n W V ε 1 , p + u n H 1 p on both sides and letting n, we get 0 2 1 p N > 0 , which is a contradiction.

Case-4: Let u n W V ε 1 , N as n and u n W V ε 1 , p is bounded. Similar to Case-3, we get a contradiction.

Hence, we conclude from the above seven cases that { u n } n N Y ε must be bounded. This finishes the proof. □

The following lemma is devoted to the tightness of the Palais-Smale sequences for J ɛ .

Lemma 3.6.

Let { u n } n N Y ε be a (PS) c sequence for J ɛ as stated in Lemma 3.5. Then, for all ξ > 0, there exists R = R(ξ) > 0 such that

lim sup n B R c | u n | p + V ( ε x ) | u n | p + | u n | N + ( V ( ε x ) + 1 ) | u n | N d x < ξ .

Proof.

For R > 0, let ψ R C ( R N ) be a such that 0 ψ R 1 in R N , ψ R 0 in B R 2 , ψ R 1 in B R c and | ψ R | C R , where C > 0 is a constant independent of R. Further, we choose R > 0 in such a way that Λ ε B R 2 . Due to Lemma 3.5, we infer that the sequence { u n ψ R } n N is bounded in Y ɛ and there holds J ε ( u n ) , u n ψ R 0 as n. Consequently, by using ( H 1 ) (b), ( A ) (c) and ( B ) (d), we obtain

(3.31) R N | u n | p + V ( ε x ) | u n | p + | u n | N + ( V ( ε x ) + 1 ) | u n | N ψ R d x I 1 + I 2 + o n ( 1 ) as  n ,

where

I 1 = ( + ) R N | u n | N ψ R d x and I 2 = R N u n | u n | p 2 + | u n | N 2 u n ψ R d x .

In view of (V1) and the fact that V 0 + 1 ≥ 2( + ′), we get

(3.32)   I 1 V 0 + 1 2 R N | u n | N ψ R d x 1 2 R N ( V ( ε x ) + 1 ) | u n | N ψ R d x                                                         1 2 R N | u n | p + V ( ε x ) | u n | p + | u n | N + ( V ( ε x ) + 1 ) | u n | N ψ R d x .

Moreover, due to the boundedness of { u n } n N in Y ɛ and Hölder’s inequality, we have

(3.33) I 2 C R u n p u n p p 1 + u n N u n N N 1 C R S p 1 u n Y ε p + S N 1 u n Y ε N C ̃ R ,

where C ̃ > 0 is a constant. Now, it follows from (3.31), (3.32) and (3.33) that

R N | u n | p + V ( ε x ) | u n | p + | u n | N + ( V ( ε x ) + 1 ) | u n | N ψ R d x 2 C ̃ R + o n ( 1 ) as  n .

Fix ξ > 0 and take R > 0 sufficiently large such that 2 C ̃ R < ξ . Passing to n in the above inequality, we obtain

lim sup n B R c | u n | p + V ( ε x ) | u n | p + | u n | N + ( V ( ε x ) + 1 ) | u n | N d x 2 C ̃ R < ξ .

This finishes the proof. □

Lemma 3.7.

Let uY ɛ and { u n } n N be a (PS) c sequence for J ɛ satisfying lim sup n u n W 1 , N N < α N α 0 . If u n u in Y ɛ as n, then we have ∇u n → ∇u a.e. in R N as n. Consequently, we deduce that u is a critical point for J ɛ , that is, J ε ( u ) = 0 .

Proof.

Note that by Lemma 3.5, we conclude that the sequence { u n } n N is bounded in Y ɛ . By the hypothesis, we have u n u in Y ɛ as n. Due to Remark 2.5 and Lemma 2.9, we infer that

(3.34) u n u in  W V ε 1 , t ( R N )  for  t { p , N } , u n u in  L θ ( B R ) , u n u a.e. in  R N as  n

for any R > 0 and θ ∈ [1, + ). Consequently, there exists g R L (B R ) with N such that |u n | ≤ g R a.e. in B R . Fix R > 0 and ψ C c ( R N ) such that 0 ≤ ψ ≤ 1 in R N , ψ ≡ 1 in B R , ψ ≡ 0 in B 2 R c and ‖∇ψ C for some constant C > 0 independent of R. Note that J ε C 1 ( Y ε , R ) , u n u in Y ɛ , and J ε ( u n ) 0 in Y ε * as n, thus we obtain

(3.35) J ε ( u n ) J ε ( u ) , ( u n u ) ψ = o n ( 1 ) as  n .

For any n N and t ∈ {p, N}, we define

D n t = | u n | t 2 u n | u | t 2 u u n u + V ( ε x ) | u n | t 2 u n | u | t 2 u ( u n u ) .

Moreover, by convexity and (V1), we can see that

| u n | t 2 u n | u | t 2 u u n u 0 a.e. in  R N , V ( ε x ) | u n | t 2 u n | u | t 2 u ( u n u ) 0 a.e. in  R N

for any n N and t ∈ {p, N}. Due to Simon’s inequality (see [66]) with N ≥ 2 and (3.35), there exists c N > 0 such that as n, we have

(3.36) c N 1 B R | u n u | N d x c N 1 B R | u n u | N d x + B R V ( ε x ) | u n u | N d x B R D n N d x t { p , N } B R D n t d x t { p , N } R N D n t ψ d x = o n ( 1 ) t { p , N } R N | u n | t 2 u n | u | t 2 u ψ ( u n u ) d x R N | u n | N 2 u n | u | N 2 u ( u n u ) ψ d x R N H 1 ( u n ) H 1 ( u ) ( u n u ) ψ d x + R N G 2 ( ε x , u n ) G 2 ( ε x , u ) ( u n u ) ψ d x + R N g ( ε x , u n ) g ( ε x , u ) ( u n u ) ψ d x .

Using Hölder’s inequality and (3.34), for t ∈ {p, N}, we get

R N | u n | t 2 u n | u | t 2 u ψ ( u n u ) d x ψ u n t t 1 + u t t 1 B 2 R | u n u | t d x 1 t 0 as  n .

It follows that for t ∈ {p, N}, we have

(3.37) lim n R N | u n | t 2 u n | u | t 2 u ψ ( u n u ) d x = 0 .

Likewise, we can also prove that

(3.38) lim n R N | u n | N 2 u n | u | N 2 u ( u n u ) ψ d x = 0 .

In view of Hölder’s inequality, ( H 1 ) (c) and (3.34), we obtain

R N H 1 ( u n ) H 1 ( u ) ( u n u ) ψ d x C 1 u n q q 1 + u q q 1 B 2 R | u n u | q d x 1 q + 2 C 2 B 2 R | u n u | d x 0 as  n .

This yields

(3.39) lim n R N H 1 ( u n ) H 1 ( u ) ( u n u ) ψ d x = 0 .

Similarly, by using Hölder’s inequality, ( A ) (a) and (3.34), we have

R N G 2 ( ε x , u n ) G 2 ( ε x , u ) ( u n u ) ψ d x u n N N 1 + u N N 1 B 2 R | u n u | N d x 1 N + C u n q q 1 + u q q 1 B 2 R | u n u | q d x 1 q 0 as  n .

It follows that

(3.40) lim n R N G 2 ( ε x , u n ) G 2 ( ε x , u ) ( u n u ) ψ d x = 0 .

Due to Hölder’s inequality and (3.34), we have

J 1 = τ B 2 R | u n | N 1 + | u | N 1 | u n u | d x τ u n N N 1 + u N N 1 B 2 R | u n u | N d x 1 N 0

as n. From the hypothesis, it follows that there exists m 1 > 0 and n 0 N sufficiently large such that u n W 1 , N N < m 1 < α N α 0 for all nn 0. Take r > 1 with r = r r 1 > 1 and satisfying 1 r + 1 r = 1 . Let r′ close to 1 and α > α 0 close to α 0 such that we still have r α u n W 1 , N N < m 1 < α N for all nn 0 and u ̃ n = u n u n W 1 , N . By using Hölder’s inequality, Corollary 2.12 and (3.34), we obtain

J 2 = κ τ B 2 R Φ α 0 | u n | N + Φ α 0 | u | N | u n u | d x κ τ Φ α 0 | u n | N r + Φ α 0 | u | N r B 2 R | u n u | r d x 1 r κ τ   R N Φ r α u n W 1 , N N | u ̃ n | N d x 1 r + R N Φ r α 0 | u | N d x 1 r   B 2 R | u n u | r d x 1 r C   ̂ B 2 R | u n u | r d x 1 r 0 as  n ,

where

C ̂ = κ τ   sup n n 0 R N Φ r α u n W 1 , N N | u ̃ n | N d x 1 r + R N Φ r α 0 | u | N d x 1 r < + ,

thanks Lemma 2.13. Consequently, by using ( B ) (b) and (f1), we obtain

R N g ( ε x , u n ) g ( ε x , u ) ( u n u ) ψ d x B 2 R | f ( u n ) | + | f ( u ) | | u n u | d x J 1 + J 2 0

as n. This shows that

(3.41) lim n R N g ( ε x , u n ) g ( ε x , u ) ( u n u ) ψ d x = 0 .

Passing n in (3.36) and using (3.37), (3.38), (3.39), (3.40) and (3.41), we get ∇u n → ∇u in L N ( B R ) N as n for all R > 0. Hence, up to a subsequence, still denoted by itself, ∇u n → ∇u a.e. in R N as n.

Now, fix v C c ( R N ) and let R > 0 be large enough such that supp(v) ⊂ B R . Using the boundedness of { u n } n N in Y ɛ , we deduce that | u n | t 2 u n n N and V ( ε x ) t 1 t | u n | t 2 u n n N are bounded in [ L t t 1 ( R N ) ] N and L t t 1 ( R N ) , respectively, for t ∈ {p, N}. Note that for t ∈ {p, N}, we have

| u n | t 2 u n | u | t 2 u and V ( ε x ) t 1 t | u n | t 2 u n V ( ε x ) t 1 t | u | t 2 u a.e. in  R N as  n .

Consequently, for t ∈ {p, N}, we have

| u n | t 2 u n | u | t 2 u in  L t t 1 ( R N ) N , V ( ε x ) t 1 t | u n | t 2 u n V ( ε x ) t 1 t | u | t 2 u in  L t t 1 ( R N )

as n. Exploiting the density of C c ( R N ) in W V ε 1 , t ( R N ) for t ∈ {p, N}, we obtain for t ∈ {p, N} that

(3.42) R N | u n | t 2 u n v d x R N | u | t 2 u v d x as  n

and

(3.43) R N V ( ε x ) | u n | t 2 u n v d x R N V ( ε x ) | u | t 2 u v d x as  n .

Similarly, we can also prove that

(3.44) R N | u n | N 2 u n v d x R N | u | N 2 u v d x as  n .

On the other hand, by using Hölder’s inequality, ( H 1 ) (c), ( A ) (a) and (3.34), we get

| H 1 ( u n ) v | C 1 | u n | q 1 + C 2 | v | C 1 g R q 1 + C 2 | v | L 1 ( B R )

and

| G 2 ( ε x , u n ) v | | u n | N 1 + C | u n | q 1 | v | g R N 1 + C g R q 1 | v | L 1 ( B R ) .

Due to Lebesgue’s dominated convergence theorem, we conclude that

(3.45) R N H 1 ( u n ) v d x R N H 1 ( u ) v d x as  n

and

(3.46) R N G 2 ( ε x , u n ) v d x R N G 2 ( ε x , u ) v d x as  n .

Taking into account the notations used on the previous page to handle the exponential nonlinearity, we obtain by using ( B ) (b), (f1), Hölder’s inequality, Corollary 2.12 and Lemma 2.9 that for all nn 0

(3.47) R N g ( ε x , u n ) v d x C   R N | v | N d x 1 N + R N | v | r d x 1 r < + ,

where

C = τ S N ( N 1 ) sup n N u n Y ε N 1 + κ τ   sup n n 0 R N Φ r α u n W 1 , N N | u ̃ n | N d x 1 r ,

which is finite because of Lemma 2.13 and the fact that { u n } n N is uniformly bounded in Y ɛ . It follows from (3.47) that { g ( ε x , u n ) v } n n 0 is bounded L 1 ( R N ) . Consequently, it is not difficult to verify that { g ( ε x , u n ) v } n n 0 is uniformly absolutely integrable and tight over R N . Since u n u a.e. in R N as n, therefore we have g(ɛx, u n )vg(ɛx, u)v a.e. in R N as n. Now, by applying Vitali’s convergence theorem, we obtain

(3.48) R N g ( ε x , u n ) v d x R N g ( ε x , u ) v d x as  n .

Observe that J ε ( u n ) , v = o n ( 1 ) as n, therefore using (3.42), (3.43), (3.44), (3.45), (3.46), (3.47) and (3.48), we infer that J ε ( u ) , v = 0 for all v C c ( R N ) . Exploiting the density of C c ( R N ) in Y ɛ , we deduce that u is a critical point for J ɛ , that is, J ε ( u ) = 0 . This completes the proof. □

Lemma 3.8.

Under the assumptions of Lemma 3.5, Lemma 3.6 and Lemma 3.7, the functional J ɛ satisfies the (PS) c condition at any level c R .

Proof.

Let c R and { u n } n N Y ε be a (PS) c sequence for J ɛ at level c R . By Lemma 3.5, the sequence { u n } n N is bounded in Y ɛ . Then, without loss of generality, up to a subsequence, we have u n u in Y ɛ as n for some uY ɛ . By using Lemma 3.7, we have J ε ( u ) , v = 0 for all vY ɛ . In particular, we have J ε ( u ) , u = 0 , that is,

(3.49) u W V ε 1 , p p + u W V ε 1 , N N + R N H 1 ( u ) u d x = R N G 2 ( ε x , u ) u d x + R N g ( ε x , u ) u d x R N | u | N d x .

Note that (3.34) holds. In view of (V1) and Lemma 3.6, we obtain

lim sup n B R c | u n | p d x < ξ V 0 and lim sup n B R c | u n | N d x < ξ V 0 + 1 .

It follows from u L t ( R N ) for t ∈ {p, N} that there exists R > 0 large enough such that B R c | u | t d x < ξ . Now, using all these information and (3.34), we get

lim sup n u n u p p = lim sup n u n u L p ( B R ) p + u n u L p B R c p = lim n u n u L p ( B R ) p + lim sup n u n u L p B R c p = lim sup n u n u L p B R c p 2 p 1 lim sup n u n L p B R c p + u L p B R c p < 2 p 1 ξ V 0 + ξ = C ̃ 1 ξ with   C ̃ 1 > 0 .

Similarly, we can also prove that

lim sup n u n u N N < 2 N 1 ξ V 0 + 1 + ξ = C ̃ 2 ξ with  C ̃ 2 > 0 .

Due to the arbitrariness of ξ > 0, it follows that u n u in L t ( R N ) for t ∈ {p, N} as n. Applying the boundedness of { u n } n N in Y ɛ , we obtain by using Lemma 2.9 and the interpolation inequality that

(3.50) u n u in  L θ ( R N ) for  θ [ p , p * ) [ N , + ) as  n .

By using (3.34)(3.50) and Lebesgue’s dominated convergence theorem, it follows that

lim R lim sup n u n L θ B R c θ = 0 for any  θ [ p , p * ) [ N , + ) .

This implies that for all ξ > 0, there exists R = R(ξ) large enough such that

(3.51) lim sup n B R c | u n | θ d x < ξ for any  θ [ p , p * ) [ N , + ) .

In view of (3.51) and ( A ) (a), we have

lim sup n B R c G 2 ( ε x , u n ) u n d x lim sup n B R c | u n | N + C | u n | q d x < ( + C ) ξ = C ̃ 3 ξ

with C ̃ 3 > 0 . Note that G 2 ( ε x , u ) u L 1 ( R N ) , therefore choosing R > 0 large enough, we may assume that B R c G 2 ( ε x , u ) u d x < ξ . Gathering all these information, we have

lim sup n B R c G 2 ( ε x , u n ) u n d x B R c G 2 ( ε x , u ) u d x < C ̃ ξ ,

for all ξ > 0 and some suitable constant C ̃ > 0 . By the arbitrariness of ξ > 0, we conclude that

(3.52) B R c G 2 ( ε x , u n ) u n d x B R c G 2 ( ε x , u ) u d x as  n .

On the other hand, from ( A ) (a) and (3.34), we get

| G 2 ( ε x , u n ) u n | | u n | N + C | u n | q g R N + C g R q L 1 ( B R ) .

Consequently, by (3.34) and Lebesgue’s dominated convergent theorem, it follows that

(3.53) B R G 2 ( ε x , u n ) u n d x B R G 2 ( ε x , u ) u d x as  n .

Combining (3.52) and (3.53) together, we obtain

(3.54) R N G 2 ( ε x , u n ) u n d x R N G 2 ( ε x , u ) u d x as  n .

From the hypothesis, there exists m 2 > 0 and n 0 N sufficiently large such that u n W 1 , N N < m 2 < α N α 0 for all nn 0. Choose r > 1 with r = r r 1 > 1 and satisfying 1 r + 1 r = 1 . Let r′ close to 1 and α > α 0 close to α 0 such that we still have r α u n W 1 , N N < m 2 < α N for all nn 0 and u ̃ n = u n u n W 1 , N . It follows from ( B ) (b), (3.2), Hölder’s inequality, Corollary 2.12 and (3.34) that for all nn 0, we have

(3.55) B R g ( ε x , u n ) u n d x C   B R g R N d x + B R g R r ϑ d x 1 r < + ,

where

C = max   τ , κ ̃ τ   sup n n 0 R N Φ r α u n W 1 , N N | u ̃ n | N d x 1 r < + ,

due to Lemma 2.13. Then, from (3.55), we get that { g ( ε x , u n ) u n } n n 0 is bounded L 1(B R ). Consequently, it is not difficult to verify that { g ( ε x , u n ) u n } n n 0 is uniformly absolutely integrable and tight over B R . In virtue of (3.34), we have u n u a.e. in B R as n and hence, g(ɛx, u n )u n g(ɛx, u)u a.e. in B R as n. Now, by applying Vitali’s convergence theorem, we obtain

(3.56) B R g ( ε x , u n ) u n d x B R g ( ε x , u ) u d x as  n .

Similarly, by using ( B ) (b), (3.2), Hölder’s inequality, Corollary 2.12 and (3.51), we have for all nn 0

B R c g ( ε x , u n ) u n d x C   B R c | u n | N d x + B R c | u n | r ϑ d x 1 r < C ξ + ξ 1 r ,

where C is defined below (3.55). It follows that

lim sup n B R c g ( ε x , u n ) u n d x C ξ + ξ 1 r .

One can observe that g ( ε x , u ) u L 1 ( R N ) . So, there exists R > 0 large enough such that B R c g ( ε x , u ) u d x < ξ . Consequently, we deduce that

lim sup n B R c g ( ε x , u n ) u n d x B R c g ( ε x , u ) u d x < C ̂ ξ + ξ 1 r ,

for some suitable constant C ̂ > 0 . Now, letting ξ → 0+ in the above inequality, we obtain

(3.57) B R c g ( ε x , u n ) u n d x B R c g ( ε x , u ) u d x as  n .

Combining (3.56) and (3.57) together, we get

(3.58) R N g ( ε x , u n ) u n d x R N g ( ε x , u ) u d x as  n .

Using the fact that J ε ( u n ) , u n = o n ( 1 ) as n, we have as n

(3.59) u n W V ε 1 , p p + u n W V ε 1 , N N + R N H 1 ( u n ) u n d x = R N G 2 ( ε x , u n ) u n d x + R N g ( ε x , u n ) u n d x R N | u n | N d x + o n ( 1 ) .

Therefore, by using (3.50), (3.54) and (3.58), we obtain from (3.49) and (3.59) that

u n W V ε 1 , p p + u n W V ε 1 , N N + R N H 1 ( u n ) u n d x = u W V ε 1 , p p + u W V ε 1 , N N + R N H 1 ( u ) u d x + o n ( 1 )

as n. From this, one has

(3.60) u n W V ε 1 , t t u W V ε 1 , t t for  t { p , N } and R N H 1 ( u n ) u n d x R N H 1 ( u ) u d x as  n .

Consequently, by using (3.34) and Corollary A.2 of Autuori-Pucci [67], we obtain from (3.60) that u n u in W V ε 1 , t ( R N ) as n for t ∈ {p, N}. By Remark 2.8 and (2.3), one can notice that 0 H 1 ( s ) H 1 ( s ) s for all s R . Using this fact together with the generalized dominated convergence theorem of Lebesgue, see Royden [[68], Theorem 19] and (3.60), we conclude that

R N H 1 ( u n ) d x R N H 1 ( u ) d x as  n .

Recall that H 1 is a N-function, which satisfies the Δ2-condition. Hence, by using a Brézis-Lieb type result found in Alves-da Silva [[69], Proposition 2.2], we can prove that

R N H 1 ( u n u ) d x 0 as  n .

This shows that u n u in L H 1 ( R N ) as n and hence, u n u in Y ɛ as n. This finishes the proof. □

Now, we can give the main result in this section.

Theorem 3.9.

For each ɛ > 0, the functional J ɛ has a nontrivial critical point u ɛ Y ɛ such that J ɛ (u ɛ ) = c ɛ , where c ɛ denotes the mountain pass level associated with J ɛ . Consequently, we deduce that u ɛ is a solution of ( S ̃ ε ).

Proof.

Due to Lemmas 3.1, 3.2 and 3.8, the functional J ɛ fulfills the geometry of the mountain pass theorem, see [[64], p. 142]. Consequently, for each ɛ > 0, there exists a nontrivial critical point u ɛ Y ɛ of J ɛ such that J ɛ (u ɛ ) = c ɛ , where the mountain pass level c ɛ is characterized as

c ε = inf γ Γ ε max t [ 0,1 ] J ε ( γ ( t ) )

with

Γ ε = γ C [ 0,1 ] , Y ε : γ ( 0 ) = 0 and J ε ( γ ( 1 ) ) < 0 .

The proof is now complete. □

4 Existence of positive solution to the main problem via Nehari manifold method

This section is devoted to the study of the existence of a positive solution of ( P ε ) by using the Nehari manifold technique and the characterization of the mountain pass levels c ɛ as ɛ → 0+. To this end, we define the Nehari manifold associated with the functional J ɛ , which is defined by

N ε = u Y ε \ { 0 } : J ε ( u ) , u = 0 .

A very nice introduction to this method has been done by Szulkin-Weth [70]. It is obvious that N ε contains all nontrivial critical points of J ɛ . Define

c ε = inf u N ε J ε ( u ) .

Note that, if c ɛ is achieved by some v ε N ε , then we say that v ɛ is a critical point of J ɛ . In addition, since c ɛ is the lowest level for J ɛ , therefore, v ɛ is said to be a ground state solution of ( S ̃ ε ). Furthermore, we define

(4.1) Ψ ε ( u ) = 1 N J ε ( u ) , u = J ε ( u ) 1 p 1 N u W V ε 1 , p p 1 N u N N R N 1 N g ( ε x , u ) u G ( ε x , u ) d x   R N H 2 ( u ) 1 N H 2 ( u ) u + 1 N G 2 ( ε x , u ) u G 2 ( ε x , u ) d x .

It follows that

N ε = Ψ ε 1 ( { 0 } ) .

Now, we prove some properties of N ε , which will be used in the sequel of this paper.

Proposition 4.1.

The set N ε is bounded away from the origin, that is, there exists a constant β > 0 such that u Y ε β > 0 for all u N ε and for all ɛ > 0.

Proof.

By Lemma 2.3, one can easily see that

(4.2) u W 1 , N min { 1 , V 0 } 1 N u W V ε 1 , N min { 1 , V 0 } 1 N u Y ε .

If u Y ε min { 1 , V 0 } 1 N , the conclusion is obvious. If u Y ε < min { 1 , V 0 } 1 N , then one has u W 1 , N < 1 , thanks to (4.2). Choose r, r′ > 1 satisfying 1 r + 1 r = 1 . Further, suppose α > α 0 close to α 0 and r′ > 1 close to 1 such that rαα N holds. Now, by using ( B ) (b), (3.2), Hölder’s inequality, Corollary 2.12 and Lemma 2.9, we can deduce that

(4.3) R N | g ( ε x , u ) u | d x τ S N N u Y ε N + κ ̃ τ S ϑ r ϑ D u Y ε ϑ ,

where, due to Lemma 2.13, we have

D = sup u Y ε R N Φ ( r α | u | N ) d x : u Y ε < min { 1 , V 0 } 1 N 1 r < + ,

for ϑ > N and for all u N ε with u Y ε small enough. Suppose by contradiction that { u n } n N N ε is a sequence such that u n Y ε 0 as n. Consequently, we can see that (4.3) holds whenever u is replaced by u n for n large enough. From the definition of N ε , we have J ε ( u n ) , u n = 0 for each n N . It follows at once that

(4.4) u n W V ε 1 , p p + u n W V ε 1 , N N + u n N N + R N H 1 ( u n ) u n d x = R N G 2 ( ε x , u n ) u n d x + R N g ( ε x , u n ) u n d x .

Note that u n W V ε 1 , p and u n H 1 are small enough for sufficiently large n. Consequently, by using the fact that 0 H 1 ( s ) H 1 ( s ) s for all s R and Lemma 2.11, we obtain for n large enough that

(4.5) u n W V ε 1 , p p u n W V ε 1 , p N and R N H 1 ( u n ) u n d x u n H 1 N .

It follows from ( A ) (a) and Lemma 2.9 that

(4.6) R N | G 2 ( ε x , u n ) u n | d x S N N u n Y ε N + C S q q u n Y ε q .

In view of (4.2), (4.3), (4.4), (4.5) and (4.6), we get for n large enough that

( τ + ) S N N u n Y ε N + C S q q u n Y ε q + κ ̃ τ S ϑ r ϑ D u n Y ε ϑ 3 1 N u n Y ε N .

Due to the arbitrariness of τ and the fact that is very small, we deduce from the above inequality that there exist constants C 1, C 2, C 3 > 0 such that for n large enough there holds

C 1 u n Y ε q + C 2 u n Y ε ϑ C 3 u n Y ε N .

Dividing u n Y ε N on both sides of the above inequality and letting n, we get 0 ≥ C 3 > 0, which is a contradiction. It follows that there exists β > 0 such that u Y ε β > 0 for all u N ε and for all ɛ > 0. □

Lemma 4.2.

For each u O ε = { u Y ε : | supp ( | u | ) Λ ε | > 0 } \ { 0 } , there exists a unique t u > 0 such that t u u N ε . In particular, for u N ε O ε , we have J ɛ (u) = max t≥0 J ɛ (tu). Consequently, if u N ε , then u O ε .

Proof.

We define the function h(t) = J ɛ (tu) for t > 0 and u O ε \ { 0 } . From Lemmas 3.1 and 3.2, we have h(0) = 0, h(t) > 0 for t > 0 sufficiently small and h(t) < 0 for t > 0 sufficiently large. It follows that max t>0 h(t) is achieved at some point t = t u such that h′(t u ) = 0 and t u u N ε . Next, we claim that t u is the unique critical point of h. Assume by contradiction that there exist t 1 and t 2 with 0 < t 1 < t 2 such that h′(t 1) = h′(t 2) = 0. Consequently, we obtain for i = 1, 2 that

1 t i N p u W V ε 1 , p p + u W V ε 1 , N N + u N N + R N H 1 ( t i u ) u t i N 1 d x R N G 2 ( ε x , t i u ) u t i N 1 d x R N g ( ε x , t i u ) u t i N 1 d x = 0 .

Subtracting the equalities above gives

1 t 1 N p 1 t 2 N p u W V ε 1 , p p + R N G 2 ( ε x , t 2 u ) u t 2 N 1 G 2 ( ε x , t 1 u ) u t 1 N 1 d x + R N g ( ε x , t 2 u ) u t 2 N 1 g ( ε x , t 1 u ) u t 1 N 1 d x = R N H 1 ( t 2 u ) u t 2 N 1 H 1 ( t 1 u ) u t 1 N 1 d x J .

Now, it follows from the definitions of G 2 and g together with ( A ) (e) as well as ( B ) (e) that the right-hand side of the above equality is positive. On the other hand, we have

J = x R N : | u | < ( N 1 ) δ t 2 H 1 ( t 2 u ) u t 2 N 1 H 1 ( t 1 u ) u t 1 N 1 d x + x R N : ( N 1 ) δ t 2 < | u | < ( N 1 ) δ t 1 H 1 ( t 2 u ) u t 2 N 1 H 1 ( t 1 u ) u t 1 N 1 d x + x R N : | u | > ( N 1 ) δ t 1 H 1 ( t 2 u ) u t 2 N 1 H 1 ( t 1 u ) u t 1 N 1 d x = x R N : | u | < ( N 1 ) δ t 2 | u | N log t 1 t 2 N d x + x R N : | u | > ( N 1 ) δ t 1 N ( N 1 ) δ | u | N 1 1 t 2 1 t 1 d x + x R N : ( N 1 ) δ t 2 < | u | < ( N 1 ) δ t 1 | u | N log | t 1 u | ( N 1 ) δ N + N | u | N 1 ( N 1 ) δ t 2 | u | d x < 0 ,

which is a contradiction and thus, t u must be unique. Next, we have to prove that if u N ε , then u O ε . Indeed, if not, then for |supp(|u|) ∩Λ ɛ | = 0 and u N ε , we obtain by using (V1), V 0 + 1 ≥ 2( + ′), H 1 ( u ) H 1 ( u ) u , ( A ) (c), ( B ) (d), and Lemma 2.11 that

u W V ε 1 , p p + u W V ε 1 , N N + u N N + min u H 1 l , u H 1 N ( + ) R N | u | N d x 1 2 R N V ( ε x ) + 1 | u | N d x 1 2 u W V ε 1 , p p + u W V ε 1 , N N + u N N .

This shows that

0 < 1 2 u W V ε 1 , p p + u W V ε 1 , N N + u N N + min u H 1 l , u H 1 N 0 .

The above inequality implies u = 0 in Y ɛ , which is a contradiction because u N ε . This finishes the proof. □

Proposition 4.3.

The set N ε is a C 1-manifold for each ɛ > 0. Moreover, the critical points of J ε N ε are critical points of J ɛ in Y ɛ .

Proof.

To prove that N ε is a C 1-manifold, it is sufficient to show that Ψ ε ( u ) , u 0 for all u N ε . Now, arguing by contradiction, we assume that there exists some u N ε such that Ψ ε ( u ) , u = 0 . Consequently, by using J ε ( u ) , u = 0 , we obtain from (4.1) that

0 = p 1 p 1 N u W V ε 1 , p p R N | u | N d x R N 1 N g ( ε x , u ) u 2 N 1 N g ( ε x , u ) u d x R N N 1 N H 2 ( u ) u 1 N H 2 ( u ) u 2 d x R N 1 N G 2 ( ε x , u ) u 2 N 1 N G 2 ( ε x , u ) u d x .

Observe that g(ɛx, u) = f(u) and G 2 ( ε x , u ) = H 2 ( u ) for all x Λ ε . Now, simplifying the above equality, we obtain

(4.7) Λ ε | u | N d x < Λ ε c | u | N + N 1 N H 2 ( u ) u 1 N H 2 ( u ) u 2 d x Λ ε c 1 N G 2 ( ε x , u ) u 2 N 1 N G 2 ( ε x , u ) u d x Λ ε 1 N f ( u ) u 2 N 1 N f ( u ) u d x Λ ε c 1 N g ( ε x , u ) u 2 N 1 N g ( ε x , u ) u d x .

By the definition of H 2 and using the assumption (f3), one can easily obtain

| u | N + N 1 N H 2 ( u ) u 1 N H 2 ( u ) u 2 0 for a.a.  x Λ ε c

and

1 N f ( u ) u 2 N 1 N f ( u ) u 0 for a.a.  x Λ ε c .

Note that

Λ ε c { u > 0 } = Λ ε c { 0 < u < t 1 } Λ ε c { t 1 u t 2 } Λ ε c { u > t 2 } .

Due to ( H 2 ) (c) and (f3), one has

1 N G 2 ( ε x , u ) u 2 N 1 N G 2 ( ε x , u ) u = 1 N H 2 ( u ) u 2 ( N 1 ) H 2 ( u ) u 0

for a.a. x Λ ε c { 0 < u < t 1 } and

1 N g ( ε x , u ) u 2 N 1 N g ( ε x , u ) u = 1 N f ( u ) u 2 ( N 1 ) f ( u ) u 0

for a.a. x Λ ε c { 0 < u < t 1 } . Moreover, because of (h3) and (η3), we infer that

1 N G 2 ( ε x , u ) u 2 N 1 N G 2 ( ε x , u ) u = 1 N h ( u ) u 2 ( N 1 ) h ( u ) u 0

for a.a. x Λ ε c { t 1 u t 2 } and

1 N g ( ε x , u ) u 2 N 1 N g ( ε x , u ) u = 1 N η ( u ) u 2 ( N 1 ) η ( u ) u 0

for a.a. x Λ ε c { t 1 u t 2 } .

By using the definitions of H ̂ 2 and f ̂ , we have

1 N G 2 ( ε x , u ) u 2 N 1 N G 2 ( ε x , u ) u = 1 N g ( ε x , u ) u 2 N 1 N g ( ε x , u ) u = 0

for a.a. x Λ ε c { u > t 2 } . Consequently, we deduce that

(4.8) Λ ε c { u > 0 } 1 N G 2 ( ε x , u ) u 2 N 1 N G 2 ( ε x , u ) u d x 0

and

(4.9) Λ ε c { u > 0 } 1 N g ( ε x , u ) u 2 N 1 N g ( ε x , u ) u d x 0 .

From the definitions of G 2 and (4.8), we have

Λ ε c { u < 0 } 1 N G 2 ( ε x , u ) u 2 N 1 N G 2 ( ε x , u ) u d x = Λ ε c { u > 0 } 1 N G 2 ( ε x , u ) ( u ) 2 N 1 N G 2 ( ε x , u ) ( u ) d x 0 .

Similarly, from the definition of g and (4.9), we have

Λ ε c { u < 0 } 1 N g ( ε x , u ) u 2 N 1 N g ( ε x , u ) u d x = Λ ε c { u > 0 } 1 N g ( ε x , u ) ( u ) 2 N 1 N g ( ε x , u ) ( u ) d x 0 .

Combining all these facts, we obtain from (4.7) that 0 < Λ ε | u | N d x < 0 . This yields that u = 0 a.e. in Λ ɛ . Moreover, since J ε ( u ) , u = 0 , arguing similarly as in Lemma 4.2, we can obtain

0 < 1 2 u W V ε 1 , p p + u W V ε 1 , N N + u N N + min u H 1 l , u H 1 N 0 .

This ensures that u = 0 in Y ɛ , which is a contradiction because u N ε . It follows that Ψ ε ( u ) , u 0 for all u N ε .

Now, let u N ε be a critical point of J ɛ constrained to N ε . Due to the application of Lagrange’s multiplier rule, we infer that

J ε ( u ) = λ Ψ ε ( u ) in  Y ε *  for some  λ R .

Because of u N ε , we obtain from the above relation that

0 = J ε ( u ) , u = λ Ψ ε ( u ) , u .

It follows that λ = 0 and J ε ( u ) = 0  in Y ε * , that is, u is a critical point of J ɛ on Y ɛ . This completes the proof. □

The last proposition implies at once that a critical point of J ε N ε is a point uY ɛ such that

(4.10) J ε ( u ) Y ε * = min   λ R J ε ( u ) λ Ψ ε ( u ) = 0 ,

thanks to Proposition 5.12 of Willem [71]. Now, we recall that a (PS) c sequence for J ε N ε is a sequence { u n } n N in N ε such that

(4.11) J ε ( u n ) c and J ε ( u n ) Y ε * 0 as  n .

We say that J ε N ε satisfies the (PS) condition when each (PS) c sequence for J ε N ε has a convergent subsequence for any c R .

Proposition 4.4.

If { u n } n N N ε is a (PS) c sequence for J ɛ satisfying lim sup n u n W 1 , N N < α N α 0 , then J ε N ε satisfies the (PS) condition.

Proof.

Let { u n } n N N ε be a (PS) c sequence for J ɛ satisfying lim sup n u n W 1 , N N < α N α 0 . Therefore, we infer that (4.11) is satisfied. Further, in view of (4.10), there exists a real sequence { λ n } n N R such that

J ε ( u n ) = λ n Ψ ε ( u n ) + o n ( 1 ) as  n .

Since u n N ε for each n N , we have J ɛ (u n ) → c as n and J ε ( u n ) , u n = 0 . Repeating the same arguments as in Lemma 3.5, one can see that { u n } n N is a bounded sequence. In addition to this, due to Lemma 3.8, we only have proved that { u n } n N is a (PS) c sequence for J ɛ . To finish the proof, it is sufficient to show that λ n → 0 as n. It is obvious that the sequence { u n } n N satisfies the following relation:

(4.12) 0 = J ε ( u n ) , u n = λ n Ψ ε ( u n ) , u n + o n ( 1 ) as  n .

Due to Proposition 4.3, if Ψ ε ( u n ) , u n = o n ( 1 ) as n, then one has u n → 0 in L N ɛ ) as n. From the boundedness of { u n } n N in Y ɛ , we deduce from Lemma 2.9 and the interpolation inequality that

(4.13) u n 0 in  L θ ( Λ ε )  for  θ [ N , + ) as  n .

From the hypothesis, it follows that there exist m > 0 and n 0 N large enough such that u n W 1 , N N < m < α N α 0 for all nn 0. Take r > 1 with r = r r 1 > 1 and satisfying 1 r + 1 r = 1 . Let r′ be close to 1 and α > α 0 close to α 0 such that we still have r α u n W 1 , N N < m < α N for all nn 0 and u ̃ n = u n u n W 1 , N . It follows from ( B ) (b), (3.2), Hölder’s inequality, Corollary 2.12 and (4.13) that

Λ ε g ( ε x , u n ) u n d x τ Λ ε | u n | N d x + C   Λ ε | u n | ϑ r d x 1 r 0 as  n ,

where

C = κ ̃ τ   sup n n 0 R N Φ r α u n W 1 , N N | u ̃ n | N d x 1 r < + ,

due to Lemma 2.13. Consequently, we get

(4.14) lim n Λ ε g ( ε x , u n ) u n d x = 0 .

Following similar arguments as in Lemma 4.2 and using the facts in ( A ) (a), (c) and ( B ) (d) as well as (4.12), (4.13) and (4.14), one can easily obtain

0 < 1 2 u n W V ε 1 , p p + u n W V ε 1 , N N + u n N N + min u n H 1 l , u n H 1 N o n ( 1 ) as  n .

It follows that u n → 0 in Y ɛ as n, which contradicts Proposition 4.3 (or Proposition 4.1). Hence, we must have λ n → 0 as n. This finishes the proof. □

4.1 Existence and concentration phenomena of positive ground state solutions

In this part, we first introduce the autonomous problem related to ( S ε ) as follows:

L p ( u ) + L N ( u ) = | u | N 2 u log | u | N + f ( u ) in R N , u Y = W 1 , p ( R N ) W 1 , N ( R N ) L H 1 ( R N ) , ( P 0 )

where

L t ( u ) = Δ t u + V 0 | u | t 2 u for  t { p , N } .

The corresponding energy functional associated to ( P 0 ) will be denoted by J 0 : Y R and is defined by

J 0 ( u ) = 1 p u W V 0 1 , p p + 1 N u W V 0 1 , N N + u N N + R N H 1 ( u ) d x R N H 2 ( u ) d x R N F ( u ) d x

for all uY. By adopting a similar strategy as in [39], [40], [42], [43], [44], [48], one sees that ( P 0 ) has a ground state solution u 0 which fulfills

J 0 ( u 0 ) = c 0 = inf u N 0 J 0 ( u ) = inf u Y \ { 0 } max t 0 J 0 ( t u ) ,

where N 0 is the Nehari set associated with J 0 and defined by

N 0 = u Y \ { 0 } : J 0 ( u ) , u = 0 .

Recall that W V 0 1 , t and W 1 , t are two equivalent norms on the Banach space W 1 , t ( R N ) for any t ∈ {p, N}.

In the next lemma, we demonstrate that the mountain pass level c ɛ is the ground state level of J ɛ , and we establish an important relation between the two levels c ɛ and c 0.

Lemma 4.5.

The following properties hold:

  1. c ɛ β > 0 for all ɛ > 0,

  2. c ε = inf u N ε J ε ( u ) for all ɛ > 0,

  3. lim sup ɛ→0 c ɛ c 0.

Proof.

The assertion in (a) follows directly from the definition of c ɛ (see Theorem 3.9) and Lemma 3.1. Now, we prove (b). For this, observe that by Lemma 4.2, we have u O ε for each u N ε . Further, by Lemma 3.2, there exists t 0 > 0 such that J ɛ (t 0 u) < 0. Define the map γ ɛ : [0, 1] → Y ɛ such that γ ɛ (t) = t(t 0 u) for all t ∈ [0, 1]. It is easy to see that γ ɛ ∈ Γ ɛ . Consequently, from the definition of c ɛ , we have

c ε max   t [ 0,1 ] J ε ( γ ε ( t ) ) max   t 0 J ε ( t u ) = J ε ( u ) .

Due to the arbitrariness of u N ε and from the definition of the infimum, we obtain from the above inequality that

(4.15) c ε inf u N ε J ε ( u ) .

By Theorem 3.9, we have u ɛ Y ɛ  \{0}, J ɛ (u ɛ ) = c ɛ and J ε ( u ε ) = 0 . It follows that u ε N ε and hence, we have

(4.16) inf u N ε J ε ( u ) J ε ( u ε ) = c ε .

Combining (4.15) and (4.16), we get c ε = inf u N ε J ε ( u ) = J ε ( u ε ) . This completes the proof of (b).

Next, we aim to prove (c). To prove this, we assume that u 0 N 0 is a positive ground state solution of ( P 0 ), that is, there hold

c 0 = J 0 ( u 0 ) = inf u N 0 J 0 ( u ) and J 0 ( u 0 ) = 0 .

Choose ϕ C c ( R N ) be such that 0 ≤ ϕ ≤ 1, ϕ ≡ 1 in B 1, and ϕ ≡ 0 in B 2 c . For each R > 0, let B 2R ⊂ Λ ɛ and define ϕ R ( ) = ϕ ( R ) . Next, we set u R ( ) = u ( R ) and u R (x) = ϕ R (x)u 0(x). It follows that 0 ≤ u R u 0, u R u 0 in B R , and u R ≡ 0 in B 2 R c . Note that supp(u R ) ⊂ B 2R ⊂ Λ ɛ and hence, u R O ε . By applying Lebesgue’s dominated convergence theorem, we can easily deduce that

(4.17) u R u 0 in  W 1 , t ( R N ) as  R  for  t { p , N } .

It follows that u R u 0 a.e. in R N as R. Observe that H 1 is nondecreasing for all t ≥ 0. This implies at once that H 1 ( u R ) H 1 ( u 0 ) L 1 ( R N ) . Further, due to the continuity of H 1 , we infer that H 1 ( u R ) H 1 ( u 0 ) a.e. R N as R. Consequently, by Lebesgue’s dominated convergence theorem, we have

R N H 1 ( u R ) d x R N H 1 ( u 0 ) d x as  R .

Employing similar ideas as in Lemma 3.8, we can deduce that u R u 0 in L H 1 ( R N ) as R. Consequently, we obtain u R u in Y as R.

Using the fact that u R O ε , we obtain from Lemma 4.2 that there exists t ɛ > 0 such that t ε u R N ε . Now, arguing similarly as in (b), we have

c ε max   t 0 J ε ( t u ) = J ε ( t ε u R ) .

Next, we claim that for some ɛ 0 > 0, the family { t ε } 0 < ε < ε 0 is bounded. Indeed, if not, assume that t ɛ as ɛ → 0. Now, using the fact that t ε u R N ε , we have

(4.18) 1 t ε N p u R W V ε 1 , p p + u R W V ε 1 , N N + u R N N = Λ ε H 2 ( t ε u R ) u R t ε N 1 d x + Λ ε c H ̃ 2 ( t ε u R ) u R t ε N 1 d x R N H 1 ( t ε u R ) u R t ε N 1 d x + Λ ε f ( t ε u R ) u R t ε N 1 d x + Λ ε c f ̃ ( t ε u R ) u R t ε N 1 d x .

Without loss of generality, we can choose V(0) = V 0. Note that u R has compact support and V(ɛx) → V 0 as ɛ → 0. Also observe that Λ ε R N as ɛ → 0, see Alves-Ji [[44], Lemma 3.7]. This yields that | Λ ε c | 0 as ɛ → 0. Consequently, due to Lebesgue’s dominated convergence theorem, we have for each R > 0

R N | u R | t + V ( ε x ) | u R | t d x R N | u R | t + V 0 | u R | t d x as  ε 0  and  t { p , N } .

Using again Lebesgue’s dominated convergence theorem leads to

Λ ε c H ̃ 2 ( t ε u R ) u R t ε N 1 d x 0 and Λ ε c f ̃ ( t ε u R ) u R t ε N 1 d x 0 as  ε 0 .

Define

T ε = Λ ε f ( t ε u R ) u R t ε N 1 d x + Λ ε H 2 ( t ε u R ) u R t ε N 1 d x R N H 1 ( t ε u R ) u R t ε N 1 d x .

In view of (f4) and (2.5), we have

T ε γ t ε μ N Λ ε | u R | μ d x + log ( t ε ) N R N | u R | N d x Λ ε c H 2 ( t ε u R ) u R t ε N 1 d x + A ,

where A = R N | u R | N 1 + log | u R | N d x . From the definition of H 2 , we have the estimate

H 2 ( t ε u R ) u R t ε N 1 = | u R | N log | t ε u R | N log ( ( N 1 ) δ ) N + N | u R | N + N ( N 1 ) δ t ε | u R | N 1 .

This yields

Λ ε c H 2 ( t ε u R ) u R t ε N 1 d x Λ ε c | u R | N log | t ε u R | N d x + N ( N 1 ) δ t ε R N | u R | N 1 d x + B ,

where B = log ( ( N 1 ) δ ) N + N R N | u R | N d x . Gathering all these information and the fact that t ɛ as ɛ → 0, we obtain by setting C = AB that

T ε γ t ε μ N Λ ε | u R | μ d x + log ( t ε ) N Λ ε | u R | N d x Λ ε c | u R | N log | u R | N d x + C + o ε ( 1 ) as  ε 0 .

It follows that T ε as ɛ → 0. Letting ɛ → 0 in (4.18) and using the above estimates, we get a contradiction. Hence, we conclude that { t ε } 0 < ε < ε 0 is bounded. Choose t R > 0 such that J 0(t R u R ) = max t≥0 J 0(tu R ). It follows that t R u R N 0 .

Now, we claim that t R is bounded for R > 0 large enough. Indeed, if not, let t R as R. In virtue of J 0 ( t R u R ) , t R u R = 0 , we have

(4.19) 1 t R N p u R W V 0 1 , p p + u R W V 0 1 , N N + u R N N = R N f ( t R u R ) u R t R N 1 d x + R N H 2 ( t R u R ) u R t R N 1 d x R N H 1 ( t R u R ) u R t R N 1 d x .

Due to (4.17), one sees that

t R p N u R W V 0 1 , p p + u R W V 0 1 , N N + u R N N u 0 W V 0 1 , N N + u 0 N N as  R .

Moreover, using (f4), (2.5) and (4.17), one has

R N f ( t R u R ) u R t R N 1 d x + R N H 2 ( t R u R ) u R t R N 1 d x R N H 1 ( t R u R ) u R t R N 1 d x γ t R μ N R N | u R | μ d x + log ( t R ) N + 1 R N | u R | N d x + R N | u R | N log | u R | N d x as  R .

It follows that

R N f ( t R u R ) u R t R N 1 d x + R N H 2 ( t R u R ) u R t R N 1 d x R N H 1 ( t R u R ) u R t R N 1 d x as  R .

We get a contradiction by using all of the above information and letting R in (4.19). This shows the claim. Hence, up to a subsequence still denoted by the same symbol, t R t 1 (≥ 0) as R. Employing the same ideas as in Proposition 4.1, one can prove that N 0 is bounded away from the origin. This together with t R u R N 0 implies that there exists some β > 0 such that ‖t R u R Y β > 0. Now, sending R and using u R u 0 in Y as R, we can see that t 1u 0 Y β > 0. From this, we conclude that t 1 ≠ 0. A direct computation implies that

J ε ( t ε u R ) J 0 ( t ε u R ) = t ε p p R N V ( ε x ) V 0 | u R | p d x + t ε N N R N V ( ε x ) V 0 | u R | N d x + Λ ε c H 2 ( t ε u R ) H ̃ 2 ( t ε u R ) d x + Λ ε c F ( t ε u R ) F ̃ ( t ε u R ) d x .

Using the fact that { t ε } 0 < ε < ε 0 is bounded, u R has compact support, V(ɛx) → V 0 as ɛ → 0 and 0 ≤ u R u 0, we obtain from Lebesgue’s dominated convergence theorem that

t ε R N V ( ε x ) V 0 | u R | d x 0 as  ε 0  for  { p , N } .

In virtue of | Λ ε c | 0 as ɛ → 0, by using ( H 2 ) (b), (3.2) and Lemma 2.13, we obtain from Lebesgue’s dominated convergence theorem that

Λ ε c H 2 ( t ε u R ) H ̃ 2 ( t ε u R ) d x 0 and Λ ε c F ( t ε u R ) F ̃ ( t ε u R ) d x 0 as  ε 0 .

Gathering all of the above information, we deduce that

J ε ( t ε u R ) J 0 ( t ε u R ) = o ε ( 1 ) as  ε 0 .

Consequently, we have

(4.20) lim sup   ε 0 c ε lim sup   ε 0 J ε ( t ε u R ) J 0 ( t R u R ) .

Notice that H 1 ( t R u R ) H 1 ( t 1 u 0 ) and H 1 ( t R u R ) t R u R H 1 ( t 1 u 0 ) t 1 u 0 a.e. in R N as R. Now, using the fact that { t R } R > 0 is bounded for large R, 0 ≤ u R u 0 and H 1 is nondecreasing for t ≥ 0, we infer that there exists K > 0 such that t R K and satisfying H 1 ( t R u R ) H 1 ( K u 0 ) L 1 ( R N ) , thanks to u 0 N 0 . Further, in light of Remark 2.8 and u 0 N 0 , we also have H 1 ( t R u R ) t R u R N H 1 ( t R u R ) N H 1 ( K u 0 ) L 1 ( R N ) . Consequently, due to Lebesgue’s dominated convergence theorem, we obtain

R N H 1 ( t R u R ) d x R N H 1 ( t 1 u 0 ) d x and R N H 1 ( t R u R ) t R u R d x R N H 1 ( t 1 u 0 ) t 1 u 0 d x as  R .

By using ( H 2 ) (b), (3.2) and Lemma 2.13, we obtain from Lebesgue’s dominated convergence theorem that

R N H 2 ( t R u R ) d x R N H 2 ( t 1 u 0 ) d x , R N H 2 ( t R u R ) t R u R d x R N H 2 ( t 1 u 0 ) t 1 u 0 d x ,

R N F ( t R u R ) d x R N F ( t 1 u 0 ) d x and R N f ( t R u R ) t R u R d x R N f ( t 1 u 0 ) t 1 u 0 d x as  R .

Combining the above information, we deduce that J 0(t R u R ) → J 0(t 1 u 0) and 0 = J 0 ( t R u R ) , t R u R J 0 ( t 1 u 0 ) , t 1 u 0 as R. Next, we claim that t 1 = 1. Indeed, if not, then either t 1 > 1 or t 1 < 1. To prove the claim, we first observe that J 0 ( t 1 u 0 ) , t 1 u 0 = 0 and hence, we have

(4.21) 1 t 1 N p u 0 W V 0 1 , p p + u 0 W V 0 1 , N N + u 0 N N + R N H 1 ( t 1 u 0 ) u 0 t 1 N 1 d x = R N H 2 ( t 1 u 0 ) u 0 t 1 N 1 d x + R N f ( t 1 u 0 ) u 0 t 1 N 1 d x .

On the other hand, since u 0 N 0 , we have

(4.22) u 0 W V 0 1 , p p + u 0 W V 0 1 , N N + u 0 N N + R N H 1 ( u 0 ) u 0 d x = R N H 2 ( u 0 ) u 0 d x + R N f ( u 0 ) u 0 d x .

Subtracting (4.22) from (4.21), we get

(4.23) 1 t 1 N p 1 u 0 W V 0 1 , p p + R N H 1 ( t 1 u 0 ) t 1 N 1 H 1 ( u 0 ) u 0 d x = R N H 2 ( t 1 u 0 ) t 1 N 1 H 2 ( u 0 ) u 0 d x + R N f ( t 1 u 0 ) t 1 N 1 f ( u 0 ) u 0 d x .

Now, we consider the case when t 1 > 1. Recall that by Lemma 4.2, for any 0 < t 1 < t 2, we have

R N H 1 ( t 2 u ) u t 2 N 1 H 1 ( t 1 u ) u t 1 N 1 d x < 0 .

Replacing t 1 = 1, t 2 = t 1 and u = u 0, respectively in the above inequality, we infer that the left-hand side of (4.23) is negative. On the other hand, by using ( H 2 ) (c) and (f3), one sees that the right-hand side of (4.23) is nonnegative. This shows at once that t 1 > 1 is impossible. Similarly, when t 1 < 1, we can easily arrive at a contradiction. It follows that t 1 = 1 and hence, we obtain J 0(t R u R ) → J 0(u 0) as R. Consequently, we deduce from (4.20) that

lim sup   ε 0 c ε lim R J 0 ( t R u R ) = J 0 ( u 0 ) = c 0 .

The proof is now complete. □

Finally, we shall be able to prove the following result.

Proposition 4.6.

The problem ( S ̃ ε ) has a positive ground state solution.

Proof.

Let u ɛ be a solution to ( S ̃ ε ) as in Theorem 3.9 and hence, J ɛ (u ɛ ) = c ɛ and J ε ( u ε ) = 0 . Set u ε = u ε + u ε . It follows that J ε ( u ε ) = J ε u ε + + J ε u ε . Moreover, we claim that either u ε + = 0 or u ε = 0 . Indeed, if not, then 0 = J ε ( u ε ) , u ε + = J ε u ε + , u ε + . It follows that u ε + N ε . Similarly, we can also prove that u ε N ε . Because of Lemma 4.5(b), one sees that c ε = J ε ( u ε ) = J ε u ε + + J ε u ε 2 c ε , which is a contradiction. Using that G 2 and g are odd functions, we can assume that u ɛ is a nonnegative solution of ( S ̃ ε ). Employing a slight variant of a Moser iteration argument explored in Lemma 4.10, it follows that u ε L ( R N ) C loc 0 , α ( R N ) for some 0 < α < 1, and therefore, from Harnack’s inequality (see Trudinger [72]), we obtain u ɛ (x) > 0 for a.e. x R N . This finishes the proof. □

Hereafter, unless otherwise noted, the solution of ( S ̃ ε ) provided in the previous proposition is denoted by the notation u ɛ . The following corollary is a consequence of the Lions’ compactness result that appears in Lemma 2.10.

Corollary 4.7.

Let { u n } n N Y ε be a bounded sequence in Y ɛ verifying lim sup n u n W 1 , N N < α N α 0 . If there exists R > 0 such that

(4.24) lim inf n sup y R N B R ( y ) | u n | N d x = 0 ,

then the following holds:

  1. R N g ( ε x , u n ) u n d x 0 and R N G ( ε x , u n ) d x 0 as n;

  2. R N G 2 ( ε x , u n ) u n d x 0 and R N G 2 ( ε x , u n ) d x 0 as n.

Proof.

Given { u n } n N Y ε to be bounded in Y ɛ and lim sup n u n W 1 , N N < α N α 0 . It follows from (4.24) and Lemma 2.10 that u n → 0 in L υ ( R N ) as n for any υ ∈ (N, + ).

Now, by the hypothesis, there exist m > 0 and n 0 N large enough such that u n W 1 , N N < m < α N α 0 for all nn 0. Take r > 1 with r = r r 1 > 1 and satisfying 1 r + 1 r = 1 . Let r′ close to 1 and α > α 0 close to α 0 such that we still have r α u n W 1 , N N < m < α N for all nn 0 and u ̃ n = u n u n W 1 , N . It follows from ( B ) (b), (3.2), Hölder’s inequality, Corollary 2.12 and Lemma 2.9 that for n large enough, we have

R N g ( ε x , u n ) u n d x τ S N N u n Y ε N + C u n ϑ r ϑ ,

where

C = κ ̃ τ   sup n n 0 R N Φ r α u n W 1 , N N | u ̃ n | N d x 1 r < + ,

thanks to Lemma 2.13. Consequently, due to the boundedness of the sequence { u n } n N in Y ɛ and u n → 0 in L ϑ r ( R N ) as n, there exists a constant C 1 > 0 such that

lim sup n R N g ( ε x , u n ) u n d x τ S N N C 1 .

Letting τ → 0, we obtain from the above inequality that

R N g ( ε x , u n ) u n d x 0 as  n .

Further, by using (3.3) and employing similar arguments explored as above, one has

R N G ( ε x , u n ) d x 0 as  n .

On the other hand, by using ( H ) (b), ( A ) (b) and the fact that u n → 0 in L υ ( R N ) as n for any υ ∈ (N, + ), we can easily deduce that (b) holds. This completes the proof. □

Now, we are ready to prove the following important compactness result.

Lemma 4.8.

Let ɛ n → 0 as n and { u n } n N = { u ε n } n N Y ε n be a nonnegative sequence such that J ε n ( u n ) = c ε n , J ε n ( u n ) = 0 and satisfying lim sup n u n W 1 , N N < α N α 0 . Then, there exists a sequence { y ̃ n } n N R N such that the translated sequence

w n ( x ) = u ̃ n ( x ) = u n ( x + y ̃ n )

has a convergent subsequence in Y. Furthermore, up to a subsequence, y n = ε n y ̃ n y 0 as n for some y 0 ∈ Λ and V(y 0) = V 0.

Proof.

Following the ideas in the proof of Lemma 3.5, one sees that { u n } n N is bounded in Y ε n . Consequently, due to (V1), we conclude that { u n } n N is bounded in Y. Now, we claim that there exist R > 0, α > 0 and a sequence { y ̃ n } n N R N such that there holds

(4.25) lim inf n B R ( y ̃ n ) | u n | N d x α > 0 .

Indeed, if (4.25) does not hold, it means that (4.24) holds. In virtue of Lemma 2.10, we obtain that u n → 0 in L υ ( R N ) as n for any υ ∈ (N, + ). In addition, one can notice that the results of Corollary 4.7 also hold whenever ɛ is replaced by ɛ n . By the hypothesis, we have J ε n ( u n ) , u n = 0 . This fact together with Corollary 4.7 implies that

u n W V ε n 1 , p p + u n W V ε n 1 , N N + u n N N + R N H 1 ( u n ) u n d x = o n ( 1 ) as  n .

Now, employing similar arguments explored in Lemma 4.2, one has

0 u n W V ε n 1 , p p + u n W V ε n 1 , N N + u n N N + min u n H 1 l , u n H 1 N o n ( 1 ) as  n .

It follows at once that u n → 0 in Y ε n as n. Consequently, due to (2.2) and Corollary 4.7, we infer that J ε n ( u n ) = c ε n 0 as n, which is a contradiction because of Lemma 4.5(a). This shows that (4.25) holds. Set w n ( x ) = u ̃ n ( x ) = u n ( x + y ̃ n ) , then using the fact that ‖ ⋅‖ Y is invariant under translation, we deduce that { w n } n N is bounded in Y. Thus, up to a subsequence not relabeled, we may assume that there exists wY such that

(4.26) w n w in  Y , w n w in  L s ( B R ) and  w n w a.e. in  R N as  n ,

and also there exists gL s (B R ) such that |w n | ≤ g a.e. in R N for s ∈ [1, + ) and for all R > 0, thanks to Lemma 2.9. In view of (4.26), we obtain from (4.25) that

B R ( 0 ) | w | N d x α > 0 .

This infers that w ≠ 0. Define y n = ε n y ̃ n . Now, our aim is to show that { y n } n N is a bounded sequence in R N . For this, we prove the following claim.

Claim I: There holds lim n dist ( y n , Λ ̄ ) = 0 .

If the claim does not hold, then there exists δ > 0 and a subsequence of { y n } n N , not relabeled, such that

dist ( y n , Λ ̄ ) δ for all  n N .

It follows that there exists some r > 0 such that B r (y n ) ⊂ Λ c for all n N . Next, let ϕ C c ( R N ) be such that 0 ≤ ϕ ≤ 1, ϕ ≡ 1 in B 1, and ϕ ≡ 0 in B 2 c . For each j N , define ϕ j ( ) = ϕ ( j ) . Further, set ψ j ( ) = ψ ( j ) and ψ j (x) = ϕ j (x)w(x). It follows that 0 ≤ ψ j w, ψ j w in B j , and ψ j ≡ 0 in B 2 j c . Observe that supp(ψ j ) ⊂ B 2j . By using similar arguments explored in Lemma 4.5, we can obtain

(4.27) ψ j w in  Y  as  j .

Now, by fixing j > 0 and using ψ j as a test function along with the change of variable z x + y ̃ n and the invariance by translation, we can see that

(4.28)   t { p , N }   R N | w n | t 2 w n ψ j + V ( ε n x + y n ) w n t 1 ψ j d x + R N w n N 1 ψ j d x + R N H 1 ( w n ) ψ j d x = R N G 2 ( ε n x + y n , w n ) ψ j d x + R N g ( ε n x + y n , w n ) ψ j d x .

From the definitions of G 2 together with ( A ) (c), we can see that

R N G 2 ( ε n x + y n , w n ) ψ j d x = B r ε n G 2 ( ε n x + y n , w n ) ψ j d x + B r ε n c G 2 ( ε n x + y n , w n ) ψ j d x B r ε n w n N 1 ψ j d x + B r ε n c H 2 ( w n ) ψ j d x R N w n N 1 ψ j d x + B r ε n c H 2 ( w n ) ψ j d x .

Similarly, by using the definition of g and ( B ) (d), one has

R N g ( ε n x + y n , w n ) ψ j d x R N w n N 1 ψ j d x + B r ε n c f ( w n ) ψ j d x .

Observe that lim sup n w n W 1 , N N < α N α 0 holds. In virtue of B r ε n c ( 0 ) 0 as n, ( H 2 ) (b), (f1) and Lemma 2.13, we obtain from Lebesgue’s dominated convergence theorem or Vitali’s theorem that

B r ε n c H 2 ( w n ) ψ j d x 0 and B r ε n c f ( w n ) ψ j d x 0 as  n .

Using that ψ j has compact support, (4.26) and ( H 1 ) (c), due to Lebesgue’s dominated convergence theorem, we have

(4.29) R N H 1 ( w n ) ψ j d x R N H 1 ( w ) ψ j d x as  n .

Note that { w n } n N is bounded in Y. Now, arguing similarly as in Lemma 3.7, we can easily prove that ∇w n → ∇w a.e. in R N as n and for any t ∈ {p, N} there hold

(4.30) R N | w n | t 2 w n ψ j R N | w | t 2 w ψ j d x as  n , R N w n t 1 ψ j d x R N w t 1 ψ j d x as  n .

Combining all the above information with (V1) and V 0 + 1 ≥ 2( + ′), we obtain by sending n in (4.28) that

(4.31) R N | w | p 2 w ψ j + V 0 w p 1 ψ j d x + R N | w | N 2 w ψ j + η w N 1 ψ j d x + R N H 1 ( w ) ψ j d x 0 ,

where η = V 0 + 1 2 . It follows immediately from (4.27) that ψ j w in L t ( R N ) and ∇ψ j ⇀ ∇w in [ L t ( R N ) ] N as j for t ∈ {p, N}. Moreover, one has | w | t 2 w [ L t t 1 ( R N ) ] N and w t 1 L t t 1 ( R N ) for t ∈ {p, N}. This shows that

R N | w | t 2 w ψ j R N | w | t d x and R N w t 1 ψ j d x R N w t d x as  j .

Due to Lebesgue’s dominated convergence theorem, we also have

R N H 1 ( w ) ψ j d x R N H 1 ( w ) w d x as  j .

Letting j in (4.31) and gathering all these information, we get

0 R N | w | p + V 0 w p d x + R N | w | N + η w N d x + R N H 1 ( w ) w d x 0 .

Following similar ideas explored in Lemma 4.2, we deduce from the above inequality that

0 w W V 0 1 , p p + w W η 1 , N N + min w H 1 l , w H 1 N 0 .

It follows that w = 0 in Y is a contradiction. This completes the proof of the claim. Hence, up to a subsequence, still denoted by itself, we have y n y 0 Λ ̄ as n.

Claim II: y 0 ∈ Λ.

Choose θ ∈ [N, + ) and R > 0, then the sequence χ n (x) = χ Λ(ɛ n x + y n ) is bounded in L θ (B R ). Due to the reflexivity of the space L θ (B R ), there exists χ R L θ (B R ) such that χ n χ R in L θ (B R ) as n. Suppose 0 < R 1 < R 2, then the functions χ R 1 and χ R 2 are obtained in the same way of χ R satisfying χ R 1 = χ R 2 | B R 1 . Hence, we conclude there exists a measurable function χ L loc θ ( R N ) with 0 ≤ χ ≤ 1 such that we have

(4.32) χ n χ in  L θ ( B R ) as  n  for all  θ [ N , + )  and for all  R > 0 .

Fix ψ C c ( R N ) and R > 0 large enough with supp(ψ) ⊂ B R . Following similar arguments as in Claim I, we can see that when ψ j is replaced by ψ in (4.28), then (4.28) is also true for any ψ C c ( R N ) . Similarly, we can also see that (4.29) and (4.30) also hold by replacing ψ j by ψ. Further, since ψ has compact support and V C ( R N , R ) , therefore by (4.26) and Lebesgue’s dominated convergence theorem, one has

R N V ( ε n x + y n ) w n t 1 ψ d x R N V ( y 0 ) w t 1 ψ d x as  n  for  t { p , N } .

Note that C c ( R N ) is a dense subset of L ( R N ) for any ∈ [1, + ). Therefore, by using (4.26) and the growth assumptions on H 2 and H ̃ 2 , we obtain from Lebesgue’s dominated convergence theorem that

H 2 ( w n ) ψ H 2 ( w ) ψ and H ̃ 2 ( w n ) ψ H ̃ 2 ( w ) ψ in  L q q 1 ( B R ) as  n  for all  q > N .

This together with (4.32) implies that

R N G 2 ( ε n x + y n , w n ) ψ d x R N G ̃ 2 ( x , w ) ψ d x as  n ,

where

G ̃ 2 ( x , s ) = χ ( x ) H 2 ( s ) + ( 1 χ ( x ) ) H ̃ 2 ( s ) for all  ( x , s ) R N × [ 0 , + ) , G ̃ 2 ( x , s ) = G ̃ 2 ( x , s ) for all  ( x , s ) R N × ( , 0 ] .

Recall that lim sup n w n W 1 , N N < α N α 0 holds. Now, by using (4.26), the growth assumptions on f and f ̃ as well as Lemma 2.13, we obtain from Vitali’s convergence theorem that

f ( w n ) ψ f ( w ) ψ and f ̃ ( w n ) ψ f ̃ ( w ) ψ in  L q q 1 ( B R ) as  n  for all  q > N .

Consequently, from (4.32), we infer that

R N g ( ε n x + y n , w n ) ψ d x R N g ̃ ( x , w ) ψ d x as  n ,

where

g ̃ ( x , s ) = χ ( x ) f ( s ) + ( 1 χ ( x ) ) f ̃ ( s ) for all  ( x , s ) R N × [ 0 , + ) , g ̃ ( x , s ) = g ̃ ( x , s ) for all  ( x , s ) R N × ( , 0 ] .

Now, replacing ψ in place of ψ j in (4.28) and using the above convergence results, we obtain by letting n in (4.28) that

(4.33) R N | w | p 2 w ψ + V ( y 0 ) w p 1 ψ d x + R N | w | N 2 w ψ + V ( y 0 ) + 1 w N 1 ψ d x + R N H 1 ( w ) ψ d x = R N G ̃ 2 ( x , w ) ψ d x + R N g ̃ ( x , w ) ψ d x .

Note that for q > N, we have

| G ̃ 2 ( x , s ) | | s | N 1 + C | s | q 1 and | g ̃ ( x , s ) | | f ( s ) | for all  ( x , s ) R N × R .

In addition, the maps t G ̃ 2 ( x , s ) s N 1 and t g ̃ ( x , s ) s N 1 are nondecreasing on (0, + ). Applying the density of C c ( R N ) in Y, we infer from (4.33) that w is a critical point for J ̃ , that is, J ̃ ( w ) = 0 , where J ̃ : Y R is defined by

J ̃ ( u ) = 1 p u W V ( y 0 ) 1 , p p + 1 N u W V ( y 0 ) 1 , N N + u N N + R N H 1 ( u ) d x R N G ̃ 2 ( x , u ) d x R N G ̃ ( x , u ) d x for all  u Y ,

where

G ̃ 2 ( x , s ) = 0 s G ̃ 2 ( x , t ) d t and G ̃ ( x , s ) = 0 s g ̃ ( x , t ) d t for all  ( x , s ) R N × R .

We define J V ( y 0 ) : Y R by

J V ( y 0 ) ( u ) = 1 p u W V ( y 0 ) 1 , p p + 1 N u W V ( y 0 ) 1 , N N + u N N + R N H 1 ( u ) d x R N H 2 ( u ) d x R N F ( u ) d x for all  u Y .

Further, let

N V ( y 0 ) = u Y \ { 0 } : J V ( y 0 ) ( u ) , u = 0 , c V ( y 0 ) = inf u N V ( y 0 ) J V ( y 0 ) ( u ) = inf u Y \ { 0 } max   t 0 J V ( y 0 ) ( t u ) .

Denote O 0 = { u Y ε : | supp ( | u | ) supp χ | > 0 } . Now, using the growth assumptions on G ̃ 2 and g ̃ and employing similar arguments explored in Lemma 3.2, we can deduce that for fixed u O 0 \ { 0 } with u ≥ 0 a.e. in R N , J ̃ ( t u ) as t. In virtue of w ≠ 0 and J ̃ ( w ) = 0 , it follows that w O 0 . Consequently, we have

J ̃ ( w ) = max   t 0 J ̃ ( t w ) max t 0   J V ( y 0 ) ( t w ) c V ( y 0 ) .

Following similarly ideas as in Lemma 3.5 and using the change of variable z x + y ̃ n together with ( A ) (d) and N G ( x , s ) s g ( x , s ) for all ( x , s ) R N × [ 0 , + ) , we get

c ε n = J ε n ( u n ) 1 N J ε n ( u n ) , u n = 1 p 1 N R N | w n | p + V ( ε n x + y n ) | w n | p d x + R N 1 N g ( ε n x + y n , w n ) w n G ( ε n x + y n , w n ) d x + R N 1 N | w n | N + H 2 ( w n ) 1 N H 2 ( w n ) w n + 1 N G 2 ( ε n x + y n , w n ) w n G 2 ( ε n x + y n , w n ) d x 1 p 1 N B R | w n | p + V ( ε n x + y n ) | w n | p d x + B R 1 N g ( ε n x + y n , w n ) w n G ( ε n x + y n , w n ) d x + B R 1 N | w n | N + H 2 ( w n ) 1 N H 2 ( w n ) w n + 1 N G 2 ( ε n x + y n , w n ) w n G 2 ( ε n x + y n , w n ) d x

for all R > 0. Now, from (4.26) and the growth assumptions on H 2 and H ̃ 2 together with Lebesgue’s dominated convergence implies that

H 2 ( w n ) w n H 2 ( w ) w and H ̃ 2 ( w n ) w n H ̃ 2 ( w ) w in  L q + 1 q ( B R ) as  n  for all  q > N .

The above result together with (4.32) gives

B R G 2 ( ε n x + y n , w n ) w n d x B R G ̃ 2 ( x , w ) w d x as  n .

Likewise, we can prove that

B R G 2 ( ε n x + y n , w n ) d x B R G ̃ 2 ( x , w ) d x as  n .

Further, using lim sup n w n W 1 , N N < α N α 0 , (4.26), the growth assumptions on f and f ̃ , and Lemma 2.13, we deduce from Vitali’s convergence theorem that

f ( w n ) w n f ( w ) w and f ̃ ( w n ) w n f ̃ ( w ) w in  L q + 1 q ( B R ) as  n  for all  q > N .

Now, it follows from (4.32) that

B R g ( ε n x + y n , w n ) w d x B R g ̃ ( x , w ) w d x as  n .

Similarly, we can prove that

B R G ( ε n x + y n , w n ) d x B R G ̃ ( x , w ) d x as  n .

In a similar fashion, we obtain from Lebesgue’s dominated convergence theorem that

B R H 2 ( w n ) d x B R H 2 ( w ) d x and B R H 2 ( w n ) w n d x B R H 2 ( w ) w d x as  n .

Gathering all the above information, we obtain by using Fatou’s lemma and Lemma 4.5(c) that

c 0 1 p 1 N B R | w | p + V ( y 0 ) | w | p d x + B R 1 N g ̃ ( x , w ) w G ̃ ( x , w ) d x + B R 1 N | w | N + H 2 ( w ) 1 N H 2 ( w ) w + 1 N G ̃ 2 ( x , w ) w G ̃ 2 ( x , w ) d x .

Letting R in the above inequality, we get

c 0 1 p 1 N R N | w | p + V ( y 0 ) | w | p d x + R N 1 N g ̃ ( x , w ) w G ̃ ( x , w ) d x + R N 1 N | w | N + H 2 ( w ) 1 N H 2 ( w ) w + 1 N G ̃ 2 ( x , w ) w G ̃ 2 ( x , w ) d x = J ̃ ( w ) 1 N J ̃ ( w ) , w = J ̃ ( w ) c V ( y 0 ) .

It follows from the above inequality and the definitions of c 0 and c V ( y 0 ) that V ( y 0 ) V 0 = inf x Λ V ( x ) . Consequently, by (V2), we have V(y 0) = V 0 and y 0 ∈ Λ. This finishes the proof of the claim.

To finish the proof, we only have to prove w n w in Y as n. For this, we have the following claim.

Claim III: w n w in Y as n.

Notice that

R N = Λ n { w n t 1 } Λ n c { w n > t 1 } ,

where Λ n = Λ y n ε n . From the definitions of G 2 and H 2 along with ( B ) (d), one has

1 N G 2 ( ε n x + y n , w n ) w n G 2 ( ε n x + y n , w n ) 0 on  Λ n c { w n > t 1 } , 1 N g ( ε n x + y n , w n ) w n G ( ε n x + y n , w n ) 0 on  Λ n c { w n > t 1 } ,

and

1 N | w n | N + H 2 ( w n ) 1 N H 2 ( w n ) w n > ( N 1 ) δ N N > 0 for w n > t 1 .

It follows from w n w a.e. in R N , ∇w n → ∇w a.e. in R N , y n y 0 and χ Λ n 1 a.e. in R N as n that

  1. | w n | p + V ( ε n x + y n ) | w n | p χ Λ n c { w n > t 1 } 0 a.e. in R N as n,

  2. 1 N G 2 ( ε n x + y n , w n ) w n G 2 ( ε n x + y n , w n ) χ Λ n c { w n > t 1 } 0 a.e. in R N as n,

  3. 1 N | w n | N + H 2 ( w n ) 1 N H 2 ( w n ) w n χ Λ n c { w n > t 1 } 0 a.e. in R N as n,

  4. 1 N g ( ε n x + y n , w n ) w n G ( ε n x + y n , w n ) χ Λ n c { w n > t 1 } 0 a.e. in R N as n.

In virtue of G ̃ 2 ( x , s ) H ( s ) , g ̃ 2 ( x , s ) f ( s ) for all ( x , s ) R N × [ 0 , + ) and V(y 0) = V 0, we obtain from J ̃ ( w ) , w = 0 that J 0 ( w ) , w 0 . Define ξ : ( 0 , + ) R by ξ ( t ) = J 0 ( t w ) , t w . It follows immediately that ξ(1) ≤ 0. Choose 0 < t < 1, then by using ( H 1 ) (b), ( H 2 ) (b), (3.2) with ϑ = q > N and Corollary 2.12, we get

ξ ( t ) t N w W V 0 1 , p p + w W V 0 1 , N N + ( 1 τ ) w N N t q   C w q q + κ ̃ τ R N | w | q Φ ( α | w | N ) d x .

Due to the arbitrariness of τ > 0, we can choose τ > 0 small enough such that V 0 + 1 − τσ > 0. Consequently, we have

ξ ( t ) t N w W V 0 1 , p p + w W σ 1 , N N t q   C w q q + κ ̃ τ R N | w | q Φ ( α | w | N ) d x .

This shows that there exist constants C 1, C 2 > 0 such that

ξ ( t ) C 1 t N C 2 t q > 0 for  t ( 0,1 )  sufficiently small .

Due to the continuity of ξ, we infer that there exists t 0 ∈ (0, 1] such that ξ(t 0) = 0, that is, t 0 w N 0 . Now, combining all the above information, we obtain from the change of variable, Lemma 4.5(c), Fatou’s Lemma and (f3) that

(4.34) c 0 lim sup   n c ε n = lim sup   n J ε n ( u n ) = lim sup   n J ε n ( u n ) 1 N J ε n ( u n ) , u n = lim sup   n 1 p 1 N R N | w n | p + V ( ε n x + y n ) | w n | p d x + R N 1 N | w n | N + H 2 ( w n ) 1 N H 2 ( w n ) w n d x + R N 1 N g ( ε n x + y n , w n ) w n G ( ε n x + y n , w n ) d x + R N 1 N G 2 ( ε n x + y n , w n ) w n G 2 ( ε n x + y n , w n ) d x lim inf   n 1 p 1 N R N | w n | p + V ( ε n x + y n ) | w n | p χ Λ n d x + R N 1 N f ( w n ) w n F ( w n ) χ Λ n d x + R N 1 N | w n | N χ Λ n d x + 1 p 1 N R N | w n | p + V ( ε n x + y n ) | w n | p χ Λ n c { w n > t 1 } d x + R N 1 N | w n | N + H 2 ( w n ) 1 N H 2 ( w n ) w n χ Λ n c { w n > t 1 } d x + R N 1 N G 2 ( ε n x + y n , w n ) w n G 2 ( ε n x + y n , w n ) χ Λ n c { w n > t 1 } d x + R N 1 N g ( ε n x + y n , w n ) w n G ( ε n x + y n , w n ) χ Λ n c { w n > t 1 } d x

1 p 1 N R N | w | p + V 0 | w | p d x + 1 N R N | w | N d x + R N 1 N f ( w ) w F ( w ) d x 1 p 1 N t 0 p R N | w | p + V 0 | w | p d x + t 0 N N R N | w | N d x + R N 1 N f ( t 0 w ) t 0 w F ( t 0 w ) d x = J 0 ( t 0 w ) 1 N J 0 ( t 0 w , t 0 w = J 0 ( t 0 w ) c 0 .

It follows that t 0 = 1. Moreover, due to the simple change of variable, we obtain the following convergences

R N | w n | t + V ( ε n x + y n ) | w n | t d x R N | w | t + V 0 | w | t d x as  n  for  t { p , N }

and

R N H 1 ( w n ) w n d x R N H 1 ( w ) w d x as  n .

Consequently, it is not difficult to show that

R N | w n | t d x R N | w | t d x as  n  for  t { p , N } .

This implies that w n W V 0 1 , t w W V 0 1 , t as n for t ∈ {p, N}. Now, arguing similarly as in Lemma 3.8, we can deduce that w n w in Y as n. This completes the proof. □

Remark 4.9.

In view of (4.34), we deduce that there holds lim ɛ→0 c ɛ = c 0.

To study the behavior of the maximum points of the solutions, the following lemma is quite important. The proof relies on the appropriate Moser iteration argument found in Moser [73] and the notions discussed in Ambrosio [74].

Lemma 4.10.

Let { w n } n N be a sequence that appears in Lemma 4.8. Then, { w n } n N L ( R N ) and there is a constant K > 0 such that

w n L ( R N ) K for all  n N .

In addition, we have

(4.35) lim | x | sup n N | w n ( x ) | = 0 .

Proof.

For all L > 0 and β > 1, we define γ ( w n ) = w n w n , L N ( β 1 ) and u n , L = w n w n , L β 1 , where w n,L = min{w n , L}. Note that the function γ is an increasing function, so we have (ab)(γ(a) − γ(b)) ≥ 0 for all a , b R . Define

Λ ( t ) = | t | N N and Γ ( t ) = 0 t ( γ ( s ) ) 1 N d s .

Invoking Lemma 29 of Zhang-Sun-Liang-Thin [57], one sees that

Λ ( a b ) ( γ ( a ) γ ( b ) ) | Γ ( a ) Γ ( b ) | N for all  a , b R .

Consequently, there holds

1 β w n w n , L β 1 Γ ( w n ) w n w n , L β 1 .

Let η > 0 be specified later and S be the best Sobolev constant of the embedding W 1 , N ( R N ) L N * ( R N ) for any N* > N. Using the fact that W η 1 , N is an equivalent norm for W 1 , N ( R N ) , the last inequality yields

(4.36) w n w n , L β 1 N * N C 1 β N   R N w n , L N ( β 1 ) | w n | N d x + η R N w n N w n , L N ( β 1 ) d x ,

where C 1 = C 1(N, β, S) > 0 is a constant. Due to w n,L L, we have H 1 ( w n ) γ ( w n ) L N ( β 1 ) H 1 ( w n ) w n L 1 ( R N ) . By direct calculation, one has

R N | w n | p 2 w n ( γ ( w n ) ) d x = R N w n , L N ( β 1 ) | w n | p d x + N ( β 1 ) { w n L } w n , L N ( β 1 ) | w n | p d x 0 ,

R N | w n | N 2 w n ( γ ( w n ) ) d x = R N w n , L N ( β 1 ) | w n | N d x + N ( β 1 ) { w n L } w n , L N ( β 1 ) | w n | N d x R N w n , L N ( β 1 ) | w n | N d x ,

and

R N V ( ε n x + y n ) ( w n p 1 + w n N 1 ) γ ( w n ) d x V 0 R N w n p w n , L N ( β 1 ) d x + V 0 R N w n N w n , L N ( β 1 ) d x V 0 R N w n N w n , L N ( β 1 ) d x .

Combining all the above information and using ( H 1 ) (b), ( A ) (a), ( B ) (b) and (3.2), we obtain by taking γ(w n ) as test function in the weak formulation of the problem solved by w n that

(4.37) R N w n , L N ( β 1 ) | w n | N d x + η R N w n N w n , L N ( β 1 ) d x C q R N w n q w n , L N ( β 1 ) d x + κ ̃ τ R N w n ϑ w n , L N ( β 1 ) Φ α w n N d x ,

where we have used that τ ∈ (0, ′] to be small enough and η = V 0 + 1 − ( + ′) > 0, thanks to V 0 + 1 ≥ 2( + ′). Consequently, we obtain from (4.36) and (4.37) that

(4.38) w n w n , L β 1 N * N C 1 β N   C q R N w n q w n , L N ( β 1 ) d x + κ ̃ τ R N w n ϑ w n , L N ( β 1 ) Φ α w n N d x .

By the hypothesis, we have lim sup n w n W 1 , N N < α N α 0 . Following similar arguments as in Fiscella-Pucci [[25], Theorem 1.1], up to a subsequence, not relabeled, we may suppose that

(4.39) sup n N w n W 1 , N N < α N α 0 .

Set min{ϑ, q}≥ 2N and take μ, μ′, σ > 1 such that 1 μ + 1 μ = 1 . It is easy to see that μ′(qN) ≥ N and σ(ϑN) ≥ N. Further, we select t > 1 such that 1 t + 1 σ + 1 μ = 1 . In view of (4.39), we can find m > 0 such that w n W 1 , N N < m < α N α 0 for all n N . Let t > 1 be close to 1 and α > α 0 be close to α 0 such that we still have α t w n W 1 , N N < m < α N for all n N and w ̃ n = w n w n W 1 , N . Using that { w n } n N is bounded in Y, it follows from the generalized Hölder inequality, Corollary 2.12 and Lemma 2.9 that

(4.40) C q R N w n q w n , L N ( β 1 ) d x + κ ̃ τ R N w n ϑ w n , L N ( β 1 ) Φ α w n N d x = C q R N w n q N u n , L N d x + κ ̃ τ R N w n ϑ N u n , L N Φ α w n N d x C q w n μ ( q N ) q N + κ ̃ τ w n σ ( ϑ N ) ϑ N R N Φ α t w n W 1 , N N | w ̃ n | N d x 1 t u n , L N μ N C ̃ u n , L N μ N = C ̃ w n w n , L β 1 N μ N C ̃ w n N β μ N β ,

where the last inequality is obtained by using w n,L w n and C ̃ is defined as

C ̃ = C q sup n N w n μ ( q N ) q N + κ ̃ τ sup n N w n σ ( ϑ N ) ϑ N sup n N R N Φ α t w n W 1 , N N | w ̃ n | N d x 1 t < + ,

thanks to Lemma 2.13. In virtue of (4.38) and (4.40), we deduce that there exists a constant C > 0 such that

w n w n , L β 1 N * N C β N w n N β μ N β .

By applying Fatou’s lemma as L, we obtain from the above inequality by setting = N** < N* that

(4.41) w n N * β C 1 N β β 1 β w n N * * β .

Define β = N * N * * > 1 , then one has N**β 2 = N*β. Replacing β with β 2 in (4.41), we get

w n N * β 2 C 1 N β 2 β 2 β 2 w n N * * β 2 = C 1 N β 2 β 2 β 2 w n N * β C 1 N 1 β + 1 β 2 β 1 β + 2 β 2 w n N * β .

Using the fact that w n N * β C 2 for all n N , where C 2 > 0 is a constant and iterating the formula (4.41), we get

w n N * β m C Σ i = 1 m 1 N β i β Σ i = 1 m i β i w n N * β C 2 C Σ i = 1 m 1 N β i β Σ i = 1 m i β i for all n , m N .

By d’Alembert’s ratio test, the series Σ i = 1 N 1 β i and Σ i = 1 i β i are convergent. Therefore, by letting m in the above inequality, we obtain

(4.42) w n L ( R N ) K for all n N

for some constant K > 0. Now, employing the standard regularity theory for quasilinear elliptic equations (see the works in [75], [76], [77], [78], [79], [80]), we conclude that w n C loc 0 , α ( R N ) for some 0 < α < 1 and for each n N . Moreover, due to the embedding YX, Corollary 2.4 and (4.42), we deduce that { w n } n N is bounded in X, ‖w n θ C for all n N and θ ∈ [p, p*] ∪ [N, + ]. Moreover, w n w in L θ ( R N ) , w n w a.e. in R N as n and there exists g L θ ( R N ) such that |w n | ≤ g a.e. in R N for all θ ∈ [p, p*] ∪ [N, + ). It is easy to see that w n solves (in a weak sense)

(4.43) Δ p w n + V 0 w n p 1 + Δ N w n + η w n N 1 C q w n q 1 + κ ̃ τ w n ϑ 1 Φ α w n N in  R N .

Define the operator T : XX* by

T ( u ) , v = R N | u | p 2 u v + V 0 | u | p 2 u v d x + R N | u | N 2 u v + η | u | N 2 u v d x

for all u, vX. By direct computation, we can deduce that T is coercive. Further, employing a slight variant argument explored by Liu-Zheng [[81], Lemmas 3.1 and 3.2], it follows that T is monotone. Next, we prove that T is hemicontinuous, that is, the function [0, 1] ∋ t↦⟨T(u + tv), w⟩ is continuous for all u, v, wX. For this purpose, let { t n } n N [ 0,1 ] be such that t n t as n. By the discrete Hölder inequality, for any α ∈ (0, 1) and a, b, c, d ≥ 0, there holds

a α c 1 α + b α d 1 α ( a + b ) α ( c + d ) 1 α .

This together with Hölder’s inequality implies that for any ψ ∈ {u, v} and k > 0, we have

(4.44) R N | ψ | t 1 | w | + k | ψ | t 1 | w | d x max { 1 , k } ψ W 1 , t t 1 w W 1 , t < + ,

where t ∈ {p, N}. In virtue of (4.44), for any t ∈ {p, N} and k > 0, we have

| ( u + t n v ) | t 2 ( u + t n v ) w + k | u + t n v | t 2 ( u + t n v ) w C | u | t 1 | w | + k | u | t 1 | w | + | v | t 1 | w | + k | v | t 1 | w | L 1 ( R N )

for some constant C > 0. Hence, by Lebesgue’s dominated convergence theorem, we ensure that

T ( u + t n v ) , w T ( u + t v ) , w as  n .

It follows that T is hemicontinuous. Consequently, by the Browder-Minty theorem (see, for example, Zeidler [[82], Theorem 26.A]), the operator T is surjective, that is, for all vX*, there exists uX such that T(u) = v.

Note that ( r 1 ) N > N ( N 1 ) for any r ∈ {q, ϑ}. Therefore, by using Hölder’s inequality, (4.39), Corollary 2.12 and Lemma 2.13, one has C q w n q 1 + κ ̃ τ w n ϑ 1 Φ α w n N L N N 1 ( R N ) X * , thanks to the boundedness of { w n } n N in X. Consequently, there exists v n X such that it solves (in a weak sense)

(4.45) Δ p v n + V 0 | v n | p 2 v n + Δ N v n + η | v n | N 2 v n = C q w n q 1 + κ ̃ τ w n ϑ 1 Φ α w n N in  R N .

Putting v n = v n + v n and testing (4.45) by v n , we obtain by using w n ≥ 0 that

v n W V 0 1 , p p v n W η 1 , N N = R N | v n | p 2 v n v n + V 0 | v n | p 2 v n v n + | v n | N 2 v n v n + η | v n | N 2 v n v n d x = { v n 0 } C q w n q 1 + κ ̃ τ w n ϑ 1 Φ α w n N v n d x 0 .

This shows that v n W V 0 1 , p = v n W η 1 , N = 0 , that is , v n X = 0 . It follows that v n = 0 a.e. in R N , that is, v n ≥ 0 a.e. in R N . Inspired by the comparison principle as used in Brasco-Prinari-Zagati [[83], Theorem 4.1] and in Corrêa-Corrêa-Figueiredo [[84], Lemma 2.2], we get from (4.43) and (4.45) that 0 ≤ w n v n a.e. in R N . Once more, by testing (4.45) with v n , we have

(4.46) v n W V 0 1 , p p + v n W η 1 , N N = R N C q w n q 1 + κ ̃ τ w n ϑ 1 Φ α w n N v n d x .

Due to the Young’s inequality with ζ ( 0 , η C q + κ ̃ τ ) , that is, a b ζ a N + C ζ b N N 1 for all a, b ≥ 0, we obtain from (4.46), Corollary 2.12 and by setting ξ = η ζ ( C q + κ ̃ τ ) > 0 that

v n W V 0 1 , p p + v n W ξ 1 , N N C q C ζ R N | w n | ( q 1 ) N N 1 d x + κ ̃ τ C ζ R N w n ( ϑ 1 ) N N 1 Φ N α w n N d x C ̃

for some constant C ̃ > 0 , thanks to Hölder’s inequality, (4.39), Corollary 2.12, Lemma 2.13 and the boundedness of { w n } n N in X. This shows that there exists a constant C > 0 such that ‖v n X C for all n N . It follows, up to subsequence not relabeled, that there exists vX such that we obtain from Corollary 2.4 that

v n v in  X and v n v in  L ϑ ( R N )  for all  ϑ [ p , p * ] [ N , + ) as  n .

Observe that v solves (in a weak sense)

Δ p v + V 0 | v | p 2 v + Δ N v + η | v | N 2 v = C q w q 1 + κ ̃ τ w ϑ 1 Φ ( α w N ) in  R N .

In particular, we have

(4.47) v W V 0 1 , p p + v W η 1 , N N = R N C q w q 1 + κ ̃ τ w ϑ 1 Φ ( α w N ) v d x .

Claim I: R N w n q 1 v n d x R N w q 1 v d x as  n .

By using the fact that w q 1 L N N 1 ( R N ) and v n v in L N ( R N ) as n, we have

R N w q 1 ( v n v ) d x 0 as  n .

On the other hand, we have

| w n q 1 w q 1 | N 2 N 1 g ( q 1 ) N + | w | ( q 1 ) N L 1 ( R N ) .

In virtue of Lebesgue’s dominated convergence theorem, we have

R N | w n q 1 w q 1 | N d x 0 as  n .

Using this and Hölder’s inequality gives

R N w n q 1 w q 1 v n d x v n N   R N | w n q 1 w q 1 | N d x 1 N 0 as  n .

It follows that

R N w n q 1 w q 1 v n d x 0 as  n .

The proof of Claim I now follows directly from the above convergences.

Claim II: R N w n ϑ 1 Φ α w n N v n R N w ϑ 1 Φ ( α w N ) v d x as  n .

Due to Lemma 2.13, one has w ϑ 1 Φ ( α w N ) L N N 1 ( R N ) . Now, it follows from v n v in L N ( R N ) as n that

R N ( v n v ) w ϑ 1 Φ ( α w N ) d x 0 as  n .

Further, by Hölder’s inequality, (4.39), Corollary 2.12 and Lemma 2.13, it is not difficult to see that

w n ϑ 1 Φ α w n N w ϑ 1 Φ ( α w N ) N 2 N 1 g ( ϑ 1 ) N Φ N α w n N + | w | ( ϑ 1 ) N Φ ( N α w N ) L 1 ( R N ) .

Invoking Lebesgue’s dominated convergence theorem, we get

R N w n ϑ 1 Φ α w n N w ϑ 1 Φ ( α w N ) N d x 0 as  n .

Consequently, by Hölder’s inequality, we infer that for n, there holds

R N w n ϑ 1 Φ α w n N w ϑ 1 Φ ( α w N ) v n d x v n N   R N w n ϑ 1 Φ α w n N w ϑ 1 Φ ( α w N ) N d x 1 N 0 .

This yields

R N w n ϑ 1 Φ α w n N w ϑ 1 Φ ( α w N ) v n d x 0 as  n .

Now, the proof of Claim II follows immediately by using these convergences.

In view of Claim I and Claim II, we obtain from (4.46) and (4.47) that

v n W V 0 1 , p p + v n W η 1 , N N = v W V 0 1 , p p + v W η 1 , N N + o n ( 1 ) as  n .

This shows that

v n W V 0 1 , p p v W V 0 1 , p p and v n W η 1 , N N v W η 1 , N N as  n .

Repeating the same procedure as in Lemma 3.8, we get v n v in X as n and hence, v n v in L θ ( R N ) as n for all θ ∈ [p, p*] ∪ [N, + ). This shows that the first assumption of Lemma 2.1 in Ambrosio [74] is satisfied.

On the other hand, by using the fact that C q w n q 1 + κ ̃ τ w n ϑ 1 Φ α w n N C q v n q 1 + κ ̃ τ v n ϑ 1 Φ α w n N and testing (4.45) by v n v n , L N ( β 1 ) , we obtain by performing a similar Moser iteration as before that

(4.48) v n L ( R N ) K for all n N .

This together with the interior regularity result for quasilinear elliptic equations mentioned above implies the existence of a fixed x 0 R N such that { v n } n N C 0 , α ( B 1 2 ( x 0 ) ) for some α ∈ (0, 1) depending on p, N and independent on n N and x 0. Further, there also holds

(4.49) [ v n ] C 0 , α B 1 2 ( x 0 ) = sup x , y B 1 2 ( x 0 ) , x y | v n ( x ) v n ( y ) | | x y | α C ,

where the constant C = C(p, N) > 0 is independent on x 0. Now, we claim that [ v n ] C 0 , α ( R N ) C ̃ , where C ̃ > 0 is a constant. For this, we first fix x , y R N . Note that when |xy|≥ 1, then using (4.48), one has

| v n ( x ) v n ( y ) | 2 v n L ( R N ) 2 K 2 K | x y | α .

Conversely, when |xy| < 1, then one sees that x x + y 2 = y x + y 2 = | x y | 2 < 1 2 . Hence, by using (4.49), we obtain

| v n ( x ) v n ( y ) | v n ( x ) v n x + y 2 + v n ( y ) v n x + y 2 C ̂ | x y | α

for some constant C ̂ > 0 . This proves the claim. Consequently, we deduce that

v n C 0 , α ( R N ) = v n L ( R N ) + [ v n ] C 0 , α ( R N ) C 1 for all n N

for some constant C 1 > 0. Take ɛ > 0 and choose δ = ε 2 C 1 α , then for all x , y R N with |xy| < δ implies that

| v n ( x ) v n ( y ) | C 1 | x y | α < ε for all  n N .

It follows that { v n } n N is uniformly equicontinuous in R N . Therefore, by applying Lemma 2.1 of Ambrosio [74], we get

lim | x | sup n N | v n ( x ) | = 0 .

Due to 0 ≤ w n v n in R N for all n N , it follows that (4.35) holds. This finishes the proof. □

Finally, we end this section by proving the concentration phenomena of positive solutions of ( P ε ).

Proof of Theorem 1.3.

Let ɛ 0 be small enough. Note that if u ɛ is a positive solution of ( S ̃ ε ), which is obtained by Proposition 4.6, then there must hold

(4.50) u ε ( x ) < t 1 for all  x R N \ Λ ε  and  ε ( 0 , ε 0 ) .

In fact, if (4.50) does not hold, let { ε n } n N and a solution u n = u ε n of ( S ̃ ε ) such that ɛ n → 0 as n and there hold J ε n ( u n ) = c ε n , J ε n ( u n ) = 0 and

(4.51) u n ( x ) t 1 for all  x R N \ Λ ε n .

In view of Lemma 4.8, we can find a sequence { y ̃ n } n N R N such that w n ( ) = u n ( + y ̃ n ) w in Y and ε n y ̃ n y 0 as n for some y 0 ∈ Λ and V(y 0) = V 0. Using that y 0 ∈ Λ, there exists some r > 0 such that B r ( ε n y ̃ n ) Λ , that is, B r ε n ( y ̃ n ) Λ ε n for all n sufficiently large. Consequently, we obtain for these values of n that

(4.52) R N \ Λ ε n B r ε n c ( y ̃ n ) .

Further, since w n w in Y as n, by invoking Lemma 4.10, one sees that (4.35) holds. Hence, we can find R > 0 such that

w n ( x ) < t 1 for all  | x | R  and  n N .

In particular, the last inequality together with a simple change of variable yields

u n ( x ) < t 1 for all  x B R c ( y ̃ n ) and n N .

Consequently, there exists n 0 N such that for any nn 0 and r ε n > R , we deduce from (4.52) that

R N \ Λ ε n B r ε n c ( y ̃ n ) B R c ( y ̃ n ) for all  n n 0 .

It follows immediately that u n (x) < t 1 for all x R N \ Λ ε n and nn 0, which contradicts (4.51) and thus, (4.50) holds. Now, by setting v ε ( x ) = u ε ( x ε ) , we can conclude that v ɛ is a positive solution of ( P ε ).

Finally, we study the behavior of maximum points of v ɛ (x) as ɛ → 0. For this, we assume that ɛ n → 0 as n and { u n } n N = { u ε n } n N Y ε n is a nonnegative sequence of solution for ( S ̃ ε ). In virtue of the definition of G 2 and g, we can find ρ ∈ (0, t 1) such that

(4.53) G 2 ( ε x , s ) s s N and g ( ε x , s ) s s N for all  ( x , s ) R N × [ 0 , ρ ] .

Employing a similar argument as done above, we can find R > 0 such that

(4.54) u n L ( B R c ( y ̃ n ) ) < t 1 for all  n N .

Note that, up to a subsequence not relabeled, we can assume that

(4.55) u n L ( B R ( y ̃ n ) ) t 1 for all  n N .

In fact, if (4.55) does not hold, then we have u n L ( R N ) < t 1 for all n N . Consequently, by using (4.53), J ε n ( u n ) = 0 , and arguing similarly as in Lemma 4.2, we deduce that

0 u n W V ε n 1 , p p + u n W V ε n 1 , N N + u n N N + min u n H 1 l , u n H 1 N 0 .

Letting n in the above inequality, we ensure that u n → 0 in Y ε n as n. Hence, we get J ε n ( u n ) = c ε n 0 as n, which is a contradiction because of Lemma 4.5(a). It follows that (4.55) holds.

Taking (4.54) and (4.55) into account, we conclude that the global maximum points p n R N of u n belong to B R ( y ̃ n ) . It follows that p n = r n + y ̃ n , where r n B R . Note that the solution of ( P ε ) is of the type v n ( x ) = u n ( x ε n ) and thus, a maximum point η ε n of v n (x) is of the form η ε n = ε n r n + ε n y ̃ n . By using r n B R , ε n y ̃ n y 0 and V(y 0) = V 0, we deduce from the continuity of V that

lim n V ( η ε n ) = V ( y 0 ) = V 0 .

Hence, the proof is completed. □

5 Mutiplicity of solutions to the main problem via category theory

This section is focused on the study of the multiplicity of positive solutions to ( P ε ) using the Lusternik–Schnirelmann category theory. This theory is a variational technique which helps us to find critical points of a functional on a manifold, in connection with the topological properties of that manifold. For more details on this theory, we refer to the papers of Benci-Cerami [85], [86], Benci-Cerami-Passaseo [87], Cingolani-Lazzo [88] and the monograph of Willem [71].

Now, we recall some basic definitions that will be needed in the sequel.

Definition 5.1.

A closed subset A is contractible in a topological space X, if there exists a homotopy H C [ 0,1 ] × A , X such that for any u, vA, there holds H(0, u) = u and H(1, u) = H(1, v).

Definition 5.2.

Let A be a closed subset of a topological space X. Then, the Lusternik–Schnirelmann category of A in X is denoted by cat X (A), which is the least number of closed and contractible sets in X that cover A.

Let X be a Banach space and Ψ : X R be of class C 1 ( X , R ) . We define a C 1-manifold V of the form V = Ψ 1 ( { 0 } ) , where 0 is the regular value of Ψ. Now, for any functional I : X R , we define the following level set

I d = { u V : I ( u ) d } .

Recall the following result for critical points involving the Lusternik–Schnirelmann category, see Theorem 5.20 by Willem [71].

Corollary 5.3.

Suppose I : X R is of class C 1 ( X , R ) . Further, if I V is bounded from below and I satisfies the (PS) c condition for c [ inf I V , d ] , then I V has at least cat I d ( I d ) critical points in I d .

To implement Corollary 5.3, the following corollary, found in Cingolani-Lazzo [[88], Lemma 2.2], plays a significant role in relating the topology of some sublevel of a functional to the topology of some subset of the space R N .

Corollary 5.4.

Let Ω, Ω1 and Ω2 be closed sets with Ω1 ⊂ Ω2, and let β: Ω → Ω2, ψ: Ω1 → Ω be continuous maps such that βψ is homotopically equivalent to the embedding j : Ω1 → Ω2. Then, there holds cat Ω ( Ω ) cat Ω 2 ( Ω 1 ) .

Let δ > 0 be fixed and u 0 be a positive ground state solution of ( P 0 ), that is, J 0(u 0) = c 0 and J 0 ( u 0 ) = 0 . Next, we consider a nondecreasing function ηC ([0, + ), [0, 1]) satisfying η ≡ 1 in [ 0 , δ 2 ] , η 0 in [δ, + ) and |η′| ≤ C for some C > 0. For any yM, we define

ξ ε , y ( x ) = η | ε x y | u 0 ε x y ε .

Moreover, let t ɛ be the unique positive number such that t ε ξ ε , y N ε . Note that, if |supp(|ξ ɛ,y) |)∩Λ ɛ | > 0, then t ɛ satisfies

J ε ( t ε ξ ε , y ) = max t 0 J ε ( t ξ ε , y ) .

We define Φ ε : M N ε by Φ ɛ (y) = t ɛ ξ ɛ,y . By the above construction, we see that Φ ɛ has compact support for any yM.

Inspired by Ambrosio-Repovš [[55], Lemma 6.1] and by Thin [[56], Lemma 13], we have the following lemma.

Lemma 5.5.

There holds

lim   ε 0 J ε ( Φ ε ( y ) ) = c 0 uniformly in  y M .

Proof.

Let us assume by contradiction, there exist δ 0 > 0, { y n } n N M and ɛ n → 0 as n such that

(5.1) J ε n ( Φ ε n ( y n ) ) c 0 δ 0 .

Invoking Lebesgue’s dominated convergence theorem, we have

(5.2) ξ ε n , y n W V ε n 1 , t t u 0 W V 0 1 , t t and ξ ε n , y n t t u 0 t t as  n  for  t { p , N } .

Setting t n = t ε n > 0 and using that J ε n ( t n ξ ε n , y n ) , t n ξ ε n , y n = 0 , we obtain by that change of variable z = ε n x y n ε n that

(5.3) t n p ξ ε n , y n W V ε n 1 , p p + t n N ξ ε n , y n W V ε n + 1 1 , N N = R N G 2 ( ε n x , t n ξ ε n , y n ) H 1 ( t n ξ ε n , y n ) + g ( ε n x , t n ξ ε n , y n ) t n ξ ε n , y n d x = R N G 2 ( ε n z + y n , t n η ( | ε n z | ) u 0 ( z ) ) H 1 ( t n η ( | ε n z | ) u 0 ( z ) ) + g ( ε n z + y n , t n η ( | ε n z | ) u 0 ( z ) ) t n η ( | ε n z | ) u 0 ( z ) d z ,

where we have used W V ε n + 1 1 , N N = W V ε n 1 , N N + N N . Now, we claim that { t n } n N is bounded. Indeed, if not, let t n as n. Take z B δ ε n , then ɛ n z + y n B δ (y n ) ⊂ M δ ⊂ Λ. By using G 2 H 2 and gf on Λ together with (2.5) and (f4), we obtain from (5.3) that

(5.4) 1 t n N p ξ ε n , y n W V ε n 1 , p p + ξ ε n , y n W V ε n + 1 1 , N N = log t n N B δ ε n | η ( | ε n z | ) u 0 ( z ) | N d z + B δ ε n f ( t n η ( | ε n z | ) u 0 ( z ) ) η ( | ε n z | ) u 0 ( z ) t n N 1 d z + B δ ε n | η ( | ε n z | ) u 0 ( z ) | N log | η ( | ε n z | ) u 0 ( z ) | N + 1 d z log t n N B δ 2 ε n | u 0 ( z ) | N d z + γ t n μ N B δ 2 ε n | u 0 ( z ) | μ d z + D n ,

where

D n = B δ ε n | η ( | ε n z | ) u 0 ( z ) | N log | η ( | ε n z | ) u 0 ( z ) | N + 1 d z .

Using the fact that u 0Y is a positive solution of ( P 0 ), χ B δ ε n 1 and χ B δ 2 ε n 1 a.e. in R N as n, we obtain by using Lemma 2.9 and Lebesgue’s dominated convergence theorem that

(5.5) B δ 2 ε n | u 0 ( z ) | r d z R N | u 0 ( z ) | r d z and D n R N | u 0 ( z ) | N log ( | u 0 ( z ) | N ) + 1 d z ( < + )

as n, where we have used r ∈ {μ, N} and | s | N [ log ( | s | N ) + 1 ] = H 2 ( s ) s H 1 ( s ) s . In view of (5.2) and (5.5), we have a contradiction by letting n in (5.4). This shows that { t n } n N is bounded and thus, up to a subsequence, we can assume that t n t 0 ≥ 0 as n. Now, we prove that t 0 ≠ 0. In fact, if not, suppose t 0 = 0, that is, t n → 0 as n. Since { t n } n N is bounded, we can find C > 0 such that |t n | ≤ C. Moreover, by using Corollary 2.12 and (3.2), one sees that

| f ( t n η ( | ε n z | ) u 0 ( z ) ) t n η ( | ε n z | ) u 0 ( z ) | τ t n N | η ( | ε n z | ) u 0 ( z ) | N + κ ̃ τ t n ϑ | η ( | ε n z | ) u 0 ( z ) | ϑ Φ ( C N α | η ( | ε n z | ) u 0 ( z ) | N ) .

It follows immediately from the above inequality and (5.4) that

ξ ε n , y n W V ε n 1 , p p + t n N p ξ ε n , y n W V ε n + 1 1 , N N t n N p   log t n N + τ B δ ε n | η ( | ε n z | ) u 0 ( z ) | N d z + D n + κ ̃ τ t n ϑ p B δ ε n | η ( | ε n z | ) u 0 ( z ) | ϑ Φ ( C N α | η ( | ε n z | ) u 0 ( z ) | N ) d z .

Again by Lebesgue’s dominated convergence theorem together with Hölder’s inequality, Corollary 2.12 and Lemma 2.13, we get

B δ ε n | η ( | ε n z | ) u 0 ( z ) | N d z R N | u 0 ( z ) | N d z

and

B δ ε n | η ( | ε n z | ) u 0 ( z ) | ϑ Φ ( C N α | η ( | ε n z | ) u 0 ( z ) | N ) d z R N | u 0 ( z ) | ϑ Φ ( C N α | u 0 ( z ) | N ) d z < +

as n. Letting n in the above inequality and using the above convergences together with (5.2) and (5.5), we get u 0 W V 0 1 , p p = 0 , that is, u 0 = 0 a.e. in R N , which is a contradiction. This shows that t 0 ≠ 0. Repeating the same arguments used in Lemma 4.5(c) with simple modifications and using that { t n } n N is bounded, we can deduce from Lebesgue’s dominated convergence theorem that

B δ ε n H 1 ( t n η ( | ε n z | ) u 0 ( z ) ) d z R N H 1 ( t 0 u 0 ( z ) ) d z , B δ ε n H 2 ( t n η ( | ε n z | ) u 0 ( z ) ) d z R N H 2 ( t 0 u 0 ( z ) ) d z , B δ ε n F ( t n η ( | ε n z | ) u 0 ( z ) ) d z R N F ( t 0 u 0 ( z ) ) d z as  n .

Similarly, we also have

B δ ε n H 1 ( t n η ( | ε n z | ) u 0 ( z ) ) t n η ( | ε n z | ) u 0 ( z ) d z R N H 1 ( t 0 u 0 ( z ) ) t 0 u 0 ( z ) d z , B δ ε n H 2 ( t n η ( | ε n z | ) u 0 ( z ) ) t n η ( | ε n z | ) u 0 ( z ) d z R N H 2 ( t 0 u 0 ( z ) ) t 0 u 0 ( z ) d z , B δ ε n f ( t n η ( | ε n z | ) u 0 ( z ) ) t n η ( | ε n z | ) u 0 ( z ) d z R N f ( t 0 u 0 ( z ) ) t 0 u 0 ( z ) d z as  n .

Combining all the above information and sending n in (5.3), we get

1 t 0 N p u 0 W V 0 1 , p p + u 0 W V 0 1 , N N + u 0 N N + R N H 1 ( t 0 u 0 ) u 0 t 1 N 1 d x = R N H 2 ( t 0 u 0 ) u 0 t 0 N 1 d x + R N f ( t 0 u 0 ) u 0 t 0 N 1 d x .

But u 0 N 0 , therefore we get

u 0 W V 0 1 , p p + u 0 W V 0 1 , N N + u 0 N N + R N H 1 ( u 0 ) u 0 d x = R N H 2 ( u 0 ) u 0 d x + R N f ( u 0 ) u 0 d x .

Subtracting these equalities, we have

1 t 0 N p 1 u 0 W V 0 1 , p p + R N H 1 ( t 0 u 0 ) t 0 N 1 H 1 ( u 0 ) u 0 d x = R N H 2 ( t 0 u 0 ) t 0 N 1 H 2 ( u 0 ) u 0 d x + R N f ( t 0 u 0 ) t 0 N 1 f ( u 0 ) u 0 d x .

Employing similar arguments as done before in Lemma 4.5(c), from the above equation, we conclude that t 0 = 1. Consequently, we obtain from the above convergences that

lim n J ε n ( Φ ε n ( y n ) ) = J 0 ( u 0 ) = c 0 ,

which contradicts (5.1). This finishes the proof. □

We define by N ̃ ε a subset of N ε given by

N ̃ ε = { u N ε : J ε ( u ) c 0 + h ( ε ) } ,

where h : R + R + is defined by h(ɛ) = sup yM |J ɛ (u) − c 0|. From the above lemma, we have h(ɛ) → 0 as ɛ → 0. Moreover, we know that Φ ε ( y ) N ̃ ε for all yM and ɛ > 0. It follows that N ̃ ε . Let for any δ > 0 with ρ = ρ(δ) > 0 be such that M δ B ρ . Let χ : R N R N be defined by

χ ( x ) =     x if  | x | < ρ , ρ x | x | if  | x | ρ .

Now, we define the barycenter map β ε : N ε R N by

β ε ( u ) = R N χ ( ε x ) ( | u | p + | u | N ) d x R N ( | u | p + | u | N ) d x .

Lemma 5.6.

There holds

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

Proof.

Let us assume by contradiction there exist δ 0 > 0, { y n } n N M and ɛ n → 0 as n such that

(5.6) β ε n ( Φ ε n ( y n ) ) y n δ 0 .

Note that for z B δ ε n , one has ɛ n z + y n B δ (y n ) ⊂ M δ B ρ . Therefore, from the definitions of Φ ε n , β ε n and η as well as the change of variable z = ε n x y n ε n , we have

β ε n ( Φ ε n ( y n ) ) = y n + R N ε n z | η ( | ε n z | ) u 0 ( z ) | p + | η ( | ε n z | ) u 0 ( z ) | N d z R N | η ( | ε n z | ) u 0 ( z ) | p + | η ( | ε n z | ) u 0 ( z ) | N d z .

This together with Lebesgue’s dominated convergence theorem implies that

β ε n ( Φ ε n ( y n ) ) y n = o n ( 1 ) as  n ,

which contradicts (5.6). This completes the proof. □

The following compactness principle is crucial in order to find multiplicity of solutions for our problem.

Lemma 5.7.

Let ɛ n → 0 as n and { u n } n N N ε n be a sequence such that J ε n ( u n ) c 0 as n and satisfying (3.14). Then, there exists a sequence { y ̃ n } n N R N such that w n ( x ) = u n ( x + y ̃ n ) has a convergent subsequence in Y. Moreover, there holds y n = ε n y ̃ n y 0 as n for some y 0M.

Proof.

By applying the same idea as in Alves-da Silva [[58], Lemma 6.5], the lemma can be proved. □

Now, we shall discuss the multiplicity of solutions to ( S ̃ ε ) by using the Lusternik–Schnirelmann category theory.

Proposition 5.8.

Assume that (V1)–(V2) hold and let δ > 0 be small enough. Then, the problem ( S ̃ ε ) has at least cat M δ ( M ) solutions for ɛ small enough such that ε ( 0 , ε ̃ 1 ) for some ε ̃ 1 > 0 .

Proof.

Choose ε ̃ 1 > 0 be sufficiently small and fix ε ( 0 , ε ̃ 1 ) . Let us set I = J ε , V = N ε , d = c 0 + h(ɛ) and I d = J ε d = N ̃ ε . In view of Proposition 4.4, one sees that J ε N ε satisfies the (PS) condition and thus, by Corollary 5.3, it implies that J ε N ε has at least cat N ̃ ε ( N ̃ ε ) critical points in N ̃ ε . Consequently, by Proposition 4.3, we deduce that J ɛ has at least cat N ̃ ε ( N ̃ ε ) critical points. This shows that ( S ̃ ε ) has at least cat N ̃ ε ( N ̃ ε ) critical points. To complete the proof, we only have to show that cat N ̃ ε ( N ̃ ε ) cat M δ ( M ) . One can notice that Φ ε ( M ) N ̃ ε for ɛ small enough, thanks to Lemma 5.5. Moreover, the following diagram

M Φ ε N ̃ ε β ε M δ

is well-defined for ɛ small enough. It follows that the map β ɛ ◦Φ ɛ : MM δ is well-defined for ɛ small enough. Define the map H : [0, 1] × MM δ by H(t, y) = (1 − t)y + ɛ ɛ (y)) for all (t, y) ∈ [0, 1] × M. This shows that H(0, y) = y and H(1, y) = β ɛ ɛ (y)). Therefore, we infer that the map β ɛ ◦Φ ɛ is homotopically equivalent to the embedding j : MM δ and thus, by Corollary 5.4 implies that cat N ̃ ε ( N ̃ ε ) cat M δ ( M ) . □

Proposition 5.9.

Let V satisfies (V1)–(V2) and let δ > 0 sufficiently small, then there exists ε ̃ 2 > 0 such that for ε ( 0 , ε ̃ 2 ) , we have the following assertions:

  1. problem ( S ̃ ε ) has at least cat M δ ( M ) 2 positive solutions, whenever cat M δ ( M ) is an even number;

  2. problem ( S ̃ ε ) has at least cat M δ ( M ) + 1 2 positive solutions, whenever cat M δ ( M ) is an odd number.

Proof.

Let ε ̃ 2 > 0 be small enough and fix ε ( 0 , ε ̃ 2 ) . Further, assume that w ɛ is a critical point of J ɛ and J ɛ (w ɛ ) ≤ c 0 + h(ɛ) holds. Then either w ε + = 0 or w ε = 0 . Indeed, if not, then repeating a similar procedure as in Proposition 4.6, one has w ε + , w ε N ε . Consequently, we deduce that

c 0 + h ( ε ) J ε ( w ε ) = J ε w ε + + J ε w ε 2 c ε .

Letting ɛ → 0 in the above inequality and using Remark 4.9, we get a contradiction. Once more by similar arguments as in Proposition 4.6, we infer that either w ɛ > 0 or w ɛ < 0. Denote ϱ = cat M δ ( M ) . Let ϱ be an even number and w 1, …, w ϱ be the solutions of ( S ̃ ε ) as in Proposition 5.8. If at least ϱ 2 of the solutions w 1, …, w ϱ are positive, then (a) is proved. In fact, if not, suppose that at least ϱ 2 of the solutions w 1, …, w ϱ are negative and denote these negative solutions by v 1 , , v ϱ 2 . Observe that G 2 ( x , ) + g ( x , ) H 1 ( ) is an odd function, therefore v 1 , , v ϱ 2 are positive solutions of ( S ̃ ε ). The assertion in (a) follows. In a similar way, one can prove the statement (b). □

Now, we shall be able to prove Theorem 1.4.

Proof of Theorem 1.4.

Suppose w ɛ is a critical point of J ɛ satisfying J ɛ (w ɛ ) ≤ c 0 + h(ɛ). In order to complete the proof, it is sufficient to show that there exists ɛ 1 > 0 small enough with ɛ ∈ (0, ɛ 1) such that

(5.7) 0 < w ε ( x ) < t 1 for all  x R N \ Λ ε

holds, where each solution w ɛ of ( S ̃ ε ) is given in (a) and (b) of Proposition 5.9. Let us assume by contradiction that there exists a sequence { ε n } n N such that ɛ n → 0 as n, { w n } n N = { w ε n } n N be a sequence of solution for ( S ̃ ε n ) and (3.14) holds but (5.7) is not satisfied. It is easy to see that { w n } n N satisfies the assumptions of Lemma 5.7 and thus, (4.35) holds. Now, using a similar procedure as in the proof of Theorem 1.3, we get a contradiction. It follows that (5.7) holds true. Consequently, we deduce that ( S ε ) satisfies (a) and (b) of Theorem 1.4. Hence, the result follows immediately by using a simple change of variable. This completes the proof. □


Corresponding author: Patrick Winkert, Technische Universität Berlin, Institut für Mathematik, Straße des 17. Juni 136, 10623 Berlin, Germany, E-mail:

Acknowledgements

The authors would like to thank the anonymous referees for their careful reading and valuable comments and suggestions that improved the quality of the article. We acknowledge support by the Open Access Publication Fund of TU Berlin.

  1. Research ethics: Not applicable.

  2. Informed consent: Not applicable.

  3. Author contributions: The authors have all agreed to submit this article to the journal, taken full responsibility for its content, examined all of the results, and approved the final version of the manuscript.

  4. Use of Large Language Models, AI and Machine Learning Tools: None declared.

  5. Conflict of interest: The authors state no conflict of interest.

  6. Research funding: Deepak Kumar Mahanta wishes to convey his sincere appreciation for the DST INSPIRE Fellowship with reference number DST/INSPIRE/03/2019/000265 funded by the Government of India. Tuhina Mukherjee thanks the CSIR-HRDG grant; sanction number 25/0324/23/EMR-II.

  7. Data availability: Not applicable.

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Received: 2025-02-13
Accepted: 2025-08-28
Published Online: 2025-10-07

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