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Nodal Solutions for a Quasilinear Elliptic Equation Involving the p-Laplacian and Critical Exponents

  • Yinbin Deng EMAIL logo , Shuangjie Peng and Jixiu Wang
Published/Copyright: June 21, 2017

Abstract

This paper is concerned with the following type of quasilinear elliptic equations in N involving the p-Laplacian and critical growth:

- Δ p u + V ( | x | ) | u | p - 2 u - Δ p ( | u | 2 ) u = λ | u | q - 2 u + | u | 2 p * - 2 u ,

which arises as a model in mathematical physics, where 2<p<N, p*=NpN-p. For any given integer k0, by using change of variables and minimization arguments, we obtain, under some additional assumptions on p and q, a radial sign-changing nodal solution with k+1 nodal domains. Since the critical exponent appears and the lower order term (obtained by a transformation) may change sign, we shall use delicate arguments.

MSC 2010: 35J20; 35J62; 35J92

1 Introduction and Main Results

This paper is concerned with the following quasilinear elliptic equation:

(1.1) { - Δ p u + V ( x ) | u | p - 2 u - Δ p ( | u | 2 ) u = k ( u ) , x N , u 0 as  | x | ,

where Δp=div(||p-2) is the p-Laplacian operator with 2<p<N.

Such types of equations have been derived as models of several physical phenomena and have been the subject of extensive study in recent years. For example, solutions to (1.1) for p=2 are related to the solitary wave solutions for quasilinear Schrödinger equations of the form

(1.2) i t z = - Δ z + W ( x ) z - f ( | z | 2 ) z - κ Δ h ( | z | 2 ) h ( | z | 2 ) z ,

where z:×N, W:N is a given potential, κ is a real constant and f,h:+ are suitable functions. The quasilinear equation (1.2) appears more naturally in mathematical physics and has been derived as a model for several physical phenomena corresponding to various types of h(s). For instance, the case h(s)=s models the time evolution of the condensate wave function in super-fluid film [17, 18], and are called the superfluid film equation in fluid mechanics by Kurihara [17]. We can refer to [3, 7, 16, 30, 31] and references therein for more physical motivations and applications.

Considering the case h(s)=s, κ>0, and taking z(t,x)=exp(-iEt)u(x) in (1.2), we find that u(x) solves the following elliptic equation:

(1.3) { - Δ u + V ( x ) u - κ Δ ( u 2 ) u = f ( u 2 ) u , x N , u 0 as  | x | ,

where V(x)=W(x)-E is a new potential.

Our paper was motivated by the quasilinear Schrödinger equation (1.3), on which much concentration has been focused in the past several years. The case f(s2)s=|s|q-2s (4q<22*, 2*=2NN-2, N3) is called subcritical growth in the spirit of [22], and this case was studied extensively recently; we can refer to the references [10, 13, 23, 24, 21, 22, 30, 29, 19], where positive or sign-changing solutions were obtained by using a constrained minimization argument, or a Nehari method, or a technique of changing variables. We remark that among the above three methods, the last one, which was first proposed in [22], is most effective for the power nonlinearity case, since this argument can transform the quasilinear problem to a semilinear one, and hence an Orlitz space framework can be used. The case q=22* corresponds to a critical growth for (1.3), since it was shown in [22] that (1.3) has no positive solutions in H1(N) with u2|u|2L1(N) if f(u2)u=|u|p-2u, p22*, and V satisfies V(x)x0 in N. Concerning this case, very few results can be found. Positive solutions were obtained in [4] via the mountain pass lemma, and nonnegative nontrivial solutions were given by Moameni in [27]. By a constructing argument, the authors considered problem (1.3) with f(u2)u=|u|22*-2u+λ|u|q-2u, and infinitely many node solutions were given in [14].

It should be mentioned that Liu et al. recently considered the existence of positive solutions and sign-changing solutions for general quasilinear elliptic equations like (1.3), which cannot be transformed into a semilinear form by a perturbation method. Particularly, some interesting results when the nonlinearity f(u2)u has critical growth were obtained in [20] and [25].

Here, our main purpose is to construct infinitely many nodal solutions for (1.1) with the following assumptions:

  1. k(u)=λ|u|q-2u+|u|2p*-2u, λ>0, N>p>2, 2p<q<2p*, where p*=pNN-p is the Sobolev critical exponent,

  2. VC1(N,)L(N), V(0)>0 and V(x)=V(r), V(r)0 for all r=|x|(0,).

A function u:N is called a weak solution of (1.1) if uW1,p(N)Lloc(N), and for all φC0(N), we have

N ( 1 + 2 p - 1 | u | p ) | u | p - 2 u φ d x + 2 p - 1 N | u | p | u | p - 2 u φ d x = N ( k ( u ) - V ( x ) | u | p - 2 u ) φ d x .

We point out that we can not apply directly variational methods here because the natural functional corresponding to (1.1), given by

I ( u ) = 1 p N ( 1 + 2 p - 1 | u | p ) | u | p 𝑑 x + 1 p N V | u | p 𝑑 x - N K ( u ) 𝑑 x ,

where

K ( s ) = λ q | s | q + 1 2 p * | s | 2 p * ,

satisfying K(s)=k(s), is not well defined in W1,p(N), since for uW1,p(N)L(N), it may hold that N|u|p|u|p=+.

To overcome this difficulty, we generalize an argument developed in [22] for p=2 (see also [32]). We make the change of variables v=f-1(u), where f is defined by

f ( t ) = 1 ( 1 + 2 p - 1 | f ( t ) | p ) 1 p on  [ 0 , + ) ,
f ( - t ) = - f ( t ) on  ( - , 0 ] .

After the change of variables, I(u) can be reduced to the following functional:

J ( v ) = 1 p N [ | v | p + V ( x ) | f ( v ) | p ] 𝑑 x - N K ( f ( v ) ) 𝑑 x ,

which is C1 on the usual Sobolev space W1,p(N) under suitable assumptions on the potential V(x) and the nonlinearity K(s). Moreover, critical points of the functional J correspond to weak solutions of the following equation:

(1.4) - Δ p v = f ( v ) [ k ( f ( v ) ) - V ( x ) | f ( v ) | p - 2 f ( v ) ] in  N .

For convenience, we rewrite equation (1.4) in the following form:

(1.5) { - Δ p v + V ( x ) | v | p - 2 v = g ( x , v ) + 2 p N - p | v | p * - 2 v , v 0 as  | x | ,

and the related variational functional is

J ( v ) = 1 p N [ | v | p + V ( x ) | v | p ] d x - 2 p N - p p * N | v | p * d x - N G ( x , v ) d x , v W 1 , p ( N ) ,

where

g ( x , v ) = f ( v ) [ k ( f ( v ) ) - V ( x ) | f ( v ) | p - 2 f ( v ) ] + V ( x ) | v | p - 2 v - 2 p N - p | v | p * - 2 v

and

G ( x , v ) = 0 v g ( x , s ) 𝑑 s = K ( f ( v ) ) + 1 p V ( x ) | v | p - 1 p V ( x ) | f ( v ) | p - 2 p N - p p * | v | p * .

For any k{0,1,2,}, u± is said to be a pair of k-node solution if u± is a radial solution with the following properties:

  1. u-(0)<0<u+(0),

  2. u± possess exactly k nodes ri with 0<r1<r2<<rk<+, and u±(ri)=0, i=1,2,,k.

The following theorems are our main results.

Theorem 1.1.

Assume (A) and (V1). Then problem (1.1) has a positive radial solution if λ, q and p satisfy one of the following three conditions:

  1. Np2+p, 2p<q<2p* and λ>0,

  2. p<N<p2+p, 2(p*-1)<q<2p* and λ>0,

  3. p<N<p2+p, 2p<q2(p*-1) and λ sufficiently large.

Theorem 1.2.

Assume (A) and (V1). Then problem (1.1) has at least one pair of k-node solutions for any kN if λ, q and p satisfy one of the following three conditions:

  1. Np(p2-p+1), 2p<q<2p* and λ>0,

  2. p<N<p(p2-p+1), 2(p*-1p-1)<q<2p* and λ>0,

  3. p<N<p(p2-p+1), 2p<q2(p*-1p-1) and λ sufficiently large.

To find nontrivial critical points of J, we face two main difficulties: firstly, since the domain is unbounded and the Sobolev critical exponent p* appears, the related Palais–Smale condition may not be satisfied. To regain the compactness of functional J, we should work out a threshold value of energy under which a Palais–Smale sequence is pre-compact. To this end, we need to make a precise estimate on the nonlinearity g(x,v) in (1.5). The second difficulty lies in a new phenomenon in which the nonlinear term g(x,s) satisfies

lim s g ( x , s ) | s | p * - 1 = 0 ,

instead of the usual subcritical condition g(x,s)=o(|s|t) (p<t<p*) at infinity. Furthermore, as we will see later, the functions G(x,v), g(x,v)v and 12g(x,v)v-G(x,v) may change sign. These two new phenomena cause two more obstacles. On the one hand, the usual Ambrosetti–Rabinowitz condition is not satisfied. On the other hand, the usual argument to verify that the functional J satisfies the (PS) condition (see [9, 8]) cannot be employed directly. Hence, we need to analyze the exact asymptotic behavior of g(x,s) and should apply more delicate analysis to the functional J.

To construct nodal solutions for (1.1), we will look for a minimizer for a constrained minimization problem in a special space in which each function changes sign k (k{0,1,2,}) times and then verify that the minimizer is smooth and indeed a solution to (1.1) by analyzing the least energy related to the minimizer. We mention here that the main method to prove our theorem was essentially introduced by Bartsch and Willem in [2], and Cao and Zhu in [8], independently. However, as we have pointed out, the lower order term g(x,s) may cause more difficulties. This argument was also used by the authors in [14] to construct infinitely many nodal solutions for (1.1) with p=2. But, for the case p2, the operator Δp is quasilinear, which makes the problem more complicated.

The paper is organized as follows. In Section 2, besides providing some useful lemmas, we will give an exact analysis to the asymptotic behavior of g(x,s). Theorems 1.1 and 1.2 are proved in Section 3 and 4, respectively.

In what follows, if uW1,p(N), we shall denote as usual by u+ and u- the functions defined by u+(x)=max{u(x),0} and u-(x)=max{-u(x), 0}.

2 Some Preliminary Lemmas

In this section, we give some lemmas. The proof of some of those lemmas can be found in the corresponding references. For any given set KN, we define

| u | s , K := ( K | u ( x ) | s d x ) 1 s .

In the sequel, for a radial domain Ω, we set

W r 1 , p ( N ) = { u W 1 , p ( N ) : u ( x ) = u ( | x | ) } ,
W r 1 , p ( Ω ) = { u W 0 1 , p ( Ω ) : u ( x ) = u ( | x | ) }

and

u = ( N ( | u | p + V | u | p ) 𝑑 x ) 1 p ,

which is equivalent to the usual norm in W1,p(N).

Let f, g and G be as defined in the introduction, we will summarize here some properties of them for completeness.

Lemma 2.1 ([32]).

The function f(t) enjoys the following properties:

  1. f is uniquely defined C 2 function and invertible.

  2. |f(t)|1 for all t.

  3. f(t)|t| for all t.

  4. f(t)t1 as t0.

  5. f(t)t212p as t+.

  6. f(t)2tf(t)f(t) for all t0.

  7. |f(t)|212p|t|12 for all t.

  8. There exists a positive constant C such that

    | f ( t ) | { C | t | , | t | 1 , C | t | 1 2 , | t | 1 .

  9. |f(t)f(t)|2-p-1p for all t.

Lemma 2.2.

G ( x , s ) and g(x,s) satisfy the following properties:

  1. lims0G(x,s)sp=0,

  2. limsG(x,s)sp*=0,

  3. lims0g(x,s)sp-1=0,

  4. limsg(x,s)sp*-1=0.

Moreover, for all ϵ>0, there exists a positive constant Cϵ such that

G ( x , v ) ϵ ( v p + v p * ) + C ϵ v q 2 , g ( x , v ) v ϵ ( v p + v p * ) + C ϵ v q 2 ,

where 2p<q<2p*.

Proof.

We must analyze the terms

(2.1) f ( s ) q s p = ( f ( s ) s ) p f ( s ) q - p and f ( s ) 2 p * s p = ( f ( s ) s ) p f ( s ) 2 p * - p .

Since N,q>p, from Lemma 2.1 (3)–(4), the two terms in (2.1) converge to zero as s0. Thus, (A1) holds. Similarly, we can prove property (A3). Now, by q<2p* and Lemma 2.1 (5), we have

(2.2) f ( s ) q s p * = ( f ( s ) s ) q s q 2 - p * 0 as  s .

Also, from Lemma 2.1 (3), we have

0 1 p V ( x ) ( | s | p | s | p * - | f ( s ) | p | s | p * ) 1 p V ( x ) | s | p | s | p * ,

thus

(2.3) 1 p V ( x ) ( | s | p | s | p * - | f ( s ) | p | s | p * ) 0 as  s .

On the other hand, from Lemma 2.1 (5), we have

(2.4) f ( s ) 2 p * s p * = ( f ( s ) s ) 2 p * 2 N N - p as  s .

Combining (2.2)–(2.4) yields (A2). Also,

f ( s ) | f ( s ) | 2 p * - 2 f ( s ) s p * - 1 = f ( s ) f ( s ) ( | f ( s ) | s ) 2 p * - 2 = f ( s ) ( 1 + 2 p - 1 f ( s ) p ) 1 p ( | f ( s ) | s ) 2 p * - 2 2 p N - p as  s ,

thus (A4) holds. ∎

Lemma 2.1 (7) suggests that the functions G(x,v), g(x,v)v and 12g(x,v)v-G(x,v) may change sign, which will add new obstacles when one tries to obtain nontrivial solutions. Hence, we need to analyze the properties of f(t).

Lemma 2.3.

For p>2, there exists a positive constant A such that

( f ( t ) t ) 2 p 2 - A t - 1 for large  t > 0 .

Proof.

By the definition of f(t), we see that f(t)1+2p-1|f(t)|pp=1 and

t = 0 t f ( s ) ( 1 + 2 p - 1 | f ( s ) | p ) 1 p 𝑑 s = 0 f ( t ) ( 1 + 2 p - 1 s p ) 1 p 𝑑 s = f ( t ) 2 ( 1 + 2 p - 1 | f ( t ) | p ) 1 p + 1 2 0 f ( t ) d s ( 1 + 2 p - 1 s p ) 1 - 1 p .

Using Lemma 2.1 (5) and p>2, we deduce that

1 = f ( t ) 2 t ( 2 p - 1 ( f ( t ) t ) p + t - p 2 ) 1 p + O ( t - 1 ) as  t .

Again from Lemma 2.1 (5), we have

1 = 2 - p ( f ( t ) t ) p [ 2 p - 1 ( f ( t ) t ) p + t - p 2 ] + O ( t - 1 ) as  t .

Setting w=(f(t)t)p, we obtain that

2 p - 1 w 2 + t - p 2 w - 2 p + O ( t - 1 ) = 0 as  t ,

which gives

w = - t - p 2 + t - p + 2 p + 1 ( 2 p - O ( t - 1 ) ) 2 p as  t .

Thus,

w 2 = 2 - 2 - 2 p + 1 t - p 2 t - p + 2 2 p + 1 - O ( t - 1 ) + 2 - 2 p + 1 t - p - O ( t - 1 ) 2 - A t - 1 for large  t > 0 ,

i.e.,

( f ( t ) t ) 2 p 2 - A t - 1 for large  t > 0 .

Remark 2.4.

Using Lemma 2.3, we can prove that

1 2 ( f ( t ) t ) 2 p * 2 p N - p - B t - 1

for a positive constant B, if t is large enough. In fact, by Lemma 2.1, and noting that (a-b)αaα-αaα-1b for all 0ba and α1, we have

1 2 ( f ( t ) t ) 2 p * = 1 2 [ ( f ( t ) t ) 2 p ] p * p 1 2 ( 2 - A t - 1 ) p * p 1 2 ( 2 p * p - p * p A 2 p * p - 1 t - 1 ) = 2 p N - p - B t - 1

for large t.

3 The Existence of Positive Solutions

In this section, we prove the existence of positive solutions for problem (1.5) by using the mountain pass lemma [1]. Using the lemmas in Section 2 and proceeding as done in [4], we can verify that the functional J exhibits the mountain pass geometry.

Lemma 3.1.

The functional J has the following properties:

  1. There exist α,ρ0 such that J(v)α, v=ρ.

  2. There exists vW1,p(N) such that v>ρ and J(v)<0.

As a consequence of Lemma 3.1 and the mountain pass lemma, for the constant

c = inf γ Γ sup t [ 0 , 1 ] J ( γ ( t ) ) > 0 ,

where

Γ = { γ C ( [ 0 , 1 ] , W 1 , p ( N ) ) : γ ( 0 ) = 0 , γ ( 1 ) 0 , J ( γ ( 1 ) ) < 0 } ,

there exists a (PS)c sequence {vn} in W1,p(N) at the level c, that is,

J ( v n ) c and J ( v n ) 0 as  n .

We will verify that the level value c is in an interval where the (PS)c condition holds. To this end, we introduce a well-known fact that the minimization problem S=inf{|u|pp:uW1,p(N),|u|p*=1} has a solution given by

w ϵ = A ϵ N - p p 2 - p ( ϵ p p - 1 + | x | p p - 1 ) p - N p .

We can choose A>0 so that wϵ satisfies |wϵ|pp=|wϵ|p*p*. Thus,

| w ϵ | p p = | w ϵ | p * p * = S N p .

Let φC0(N,[0,1]) be a radial cut-off function such that φ(|x|)=1 for |x|ρϵ, φ(|x|)(0,1) for ρϵ<|x|<2ρϵ, and φ(|x|)=0 for |x|2ρϵ, where ρϵ=ϵτ, τ(1p,1). Set ψϵ(x)=φ(x)wϵ(x). We have the following estimations (see [12]).

Lemma 3.2.

We have

| ψ ϵ | p p = { C ϵ p + O ( ϵ N - p p - 1 ) if  N > p 2 , C ϵ p | ln ϵ | + O ( ϵ N - p p - 1 ) if  N = p 2 , O ( ϵ N - p p - 1 ) if  N < p 2 ,
| ψ ϵ | p p = S N p + O ( ϵ N - p p - 1 ) , | ψ ϵ | p * p * = S N p + O ( ϵ N p - 1 ) , | ψ ϵ | 1 = O ( ϵ N - p p 2 - p ) , | ψ ϵ | p - 1 p - 1 = O ( ϵ N - p p ) , | ψ ϵ | p * - 1 p * - 1 = C ϵ N - p p + O ( ϵ N p + 1 p - 1 ) , | ψ ϵ | 1 O ( ϵ N - p p 2 - p ) .

Lemma 3.3.

The functional J satisfies the (PS)c condition if c<12NSNp .

Proof.

Let {vn(x)} be a (PS)c sequence. As done in [4], we can verify that {vn} is bounded in Wr1,p(N). Therefore, up to a subsequence,

(3.1) { v n v weakly in  W r 1 , p ( N ) , v n v strongly in  L s ( N ) , p < s < p * , v n v a.e. in  N ,
(3.2) { v n v a.e. in  N , | v n | p - 2 v n x i | v | p - 2 v x i in  ( L p ( N ) ) ,  1 i N ,

where (Lp(N)) stands for the dual space of Lp(N).

By 2p<q<2p*, we have from Lemma 2.2 and (3.1) that

(3.3) lim n N G ( x , v n ) = N G ( x , v ) , lim n N g ( x , v n ) v n = N g ( x , v ) v .

From (3.1), (3.2) and (3.3), it follows that

(3.4) N [ | v | p + V ( x ) | v | p ] - 2 p N - p N | v | p * - N g ( x , v ) v = 0 .

Set vn=vn-v. By the Brezis–Lieb lemma [6] and (3.1)–(3.4), we see that

(3.5) J ( v ) + 1 p N [ | v n | p + V ( x ) | v n | p ] - 2 p N - p p * N | v n | p * = c + o ( 1 )

and

N [ | v n | p + V ( x ) | v n | p ] - 2 p N - p N | v n | p * = o ( 1 ) .

Suppose that N|vn|p*=l. Then

N ( | v n | p + V ( x ) | v n | p ) = 2 p N - p l .

By the Sobolev inequality,

S ( N | v n | p * ) p p * N | v n | p d x N [ | v n | p + V ( x ) | v n | p ] .

If l>0, we get

l 2 - N N - p S N p .

By (3.5) we get that

(3.6) J ( v ) = c - 1 N 2 p N - p l c - 1 2 N S N p < 0 .

On the other hand,

g ( x , v ) v = f ( v ) v [ k ( f ( v ) ) - V ( x ) | f ( v ) | p - 2 f ( v ) ] + V ( x ) | v | p - 2 p N - p | v | p *
λ 2 | f ( v ) | q + 1 2 | f ( v ) | 2 p * - V ( x ) | f ( v ) | p + V ( x ) | v | p - 2 p N - p | v | p * ,

thus

(3.7) 1 p g ( x , v ) v - G ( x , v ) ( λ 2 p - λ q ) | f ( v ) | q + ( 1 2 p - 1 2 p * ) | f ( v ) | 2 p * - ( 1 p - 1 p * ) 2 p N - p | v | p * .

Now combining (3.4) and (3.7), we find that

J ( v ) = ( 1 p - 1 p * ) N 2 p N - p | v | p * + N ( 1 p g ( x , v ) v - G ( x , v ) )
( λ 2 p - λ q ) N | f ( v ) | q + ( 1 2 p - 1 2 p * ) N | f ( v ) | 2 p *
0 for  2 p < q < 2 p * ,

which contradicts (3.6), hence l=0 and J satisfies the (PS) condition. This completes the proof. ∎

By Lemmas 3.1 and 3.3, and the mountain pass lemma, we can easily verify the following lemma.

Lemma 3.4.

Suppose that there exists v0Wr1,p(RN), v00, such that

(3.8) sup t 0 J ( t v 0 ) < 1 2 N S N p .

Then problem (1.5) (and hence (1.1)) possesses at least one positive weak solution.

Lemma 3.5.

There exists v0Wr1,p(RN) such that (3.8) holds naturally if λ, q and p satisfy one of assumptions (A1), (A2) or (A3).

Proof.

From Lemma 3.3, we need to verify that condition (3.8) holds naturally.

First we claim that for ϵ>0 small enough, there exists a constant tϵ>0 such that

J ( t ϵ ψ ϵ ) = max t 0 J ( t ψ ϵ )

and

(3.9) 0 < A 1 < t ϵ < A 2 < + for all  ϵ > 0  small enough ,

where A1 and A2 are positive constants independent of ϵ.

In fact, since

J ( 0 ) = 0 and lim t J ( t ψ ϵ ) = - ,

there exists tϵ>0 such that

J ( t ϵ ψ ϵ ) = max t 0 J ( t ψ ϵ ) and d J ( t ψ ϵ ) d t | t = t ϵ = 0 .

Thus, we have

(3.10) ψ ϵ p | ψ ϵ | p * p * - 2 p N - p t ϵ p * - p - N g ( t ϵ ψ ϵ ) ψ ϵ t ϵ p - 1 | ψ ϵ | p * p * = 0 .

By Lemmas 3.2 and 2.2, for any μ>0, there exists a constant C>0 such that

N g ( t ϵ ψ ϵ ) ψ ϵ t ϵ p - 1 | ψ ϵ | p * p * N μ t ϵ p * ψ ϵ p * + C t ϵ p ψ ϵ p t ϵ p | ψ ϵ | p * p *
= μ t ϵ p * - p + C | ψ ϵ | p p | ψ ϵ | p * p *
= μ t ϵ p * - p + C ( S N p + O ( ϵ N p - 1 ) ) - 1 | ψ ϵ | p p
μ t ϵ p * - p + C S - N p { O ( ϵ p ) for  N > p 2 , O ( ϵ p | ln ϵ | ) for  N = p 2 , O ( ϵ N - p p - 1 ) for  N < p 2
= μ t ϵ p * - p + o ( 1 ) as  ϵ 0 ,

which implies that

1 - 2 p N - p t ϵ p * - p - μ t ϵ p * - p + o ( 1 ) 0 as  ϵ 0 .

Thus,

t ϵ ( 2 ( 2 p N - p + μ ) ) - 1 p * - p A 1 > 0 if  ϵ  small enough.

On the other hand, from (3.10) we have

2 p N - p t ϵ p * - p ψ ϵ p | ψ ϵ | p * p * + N | g ( t ϵ ψ ϵ ) | ψ ϵ t ϵ p - 1 | ψ ϵ | p * p * 1 + μ t ϵ p * - p + o ( 1 ) as  ϵ 0 ,

for μ>0 small enough. Thus,

t ϵ ( 1 2 p N - p - μ + o ( 1 ) ) 1 p * - p < A 2 < + if  ϵ  small enough.

Next, we are going to estimate J(tϵψϵ). From Lemma 3.2 and (3.9), we have

J ( t ϵ ψ ϵ ) t ϵ p p N ( | ψ ϵ | p + V ( x ) ψ ϵ p ) - 2 p N - p t ϵ p * p * N | ψ ϵ | p * - N G ( x , t ϵ ψ ϵ )
( t ϵ p p - 2 p N - p t ϵ p * p * ) S N p + O ( ϵ N - p p - 1 ) + t ϵ p p N V ( x ) | ψ ϵ | p - N G ( x , t ϵ ψ ϵ ) .

Since Q(t)=tpp-2pN-ptp*p* has only maximum at t=2-1p, we have

J ( t ϵ ψ ϵ ) 1 2 N S N p + O ( ϵ N - p p - 1 ) + C B 2 ρ ϵ | ψ ϵ | p - ( B ρ ϵ + B 2 ρ ϵ B ρ ϵ ) G ( x , t ϵ ψ ϵ ) .

In the following, we estimate

B ρ ϵ G ( x , t ϵ ψ ϵ ) and B 2 ρ ϵ B ρ ϵ G ( x , t ϵ ψ ϵ ) .

By Lemma 2.1 (3) and Remark 2.4, for ϵ small, we have that

B ρ ϵ G ( x , t ϵ ψ ϵ ) = B ρ ϵ [ λ q | f ( t ϵ w ϵ ) | q + 1 2 p * | f ( t ϵ w ϵ ) | 2 p * + 1 p V ( x ) ( | t ϵ w ϵ | p - | f ( t ϵ w ϵ ) | p ) - 2 p N - p p * | t ϵ w ϵ | p * ]
B ρ ϵ [ λ q | f ( t ϵ w ϵ ) t ϵ w ϵ | q ( t ϵ w ϵ ) q 2 + 1 p * ( 1 2 | f ( t ϵ w ϵ ) t ϵ w ϵ | 2 p * - 2 p N - p ) ( t ϵ w ϵ ) p * ]
B ρ ϵ [ C λ ( t ϵ w ϵ ) q 2 - C ( t ϵ w ϵ ) p * - 1 ] .

Thus,

(3.11) B ρ ϵ G ( x , t ϵ ψ ϵ ) B ρ ϵ [ C λ ( w ϵ ) q 2 - C ( w ϵ ) p * - 1 ] for  ϵ > 0  small.

On the other hand, set ω=B2ρϵρϵ. Using Lemma 2.1 (3), we get

ω G ( x , t ϵ ψ ϵ ) ω [ λ q | f ( t ϵ φ w ϵ ) | q + 1 2 p * | f ( t ϵ φ w ϵ ) | 2 p * - 2 p N - p p * | t ϵ φ w ϵ | p * ]
= ϵ τ 2 ϵ τ [ λ q | f ( t ϵ φ ( r ) w ϵ ( r ) ) | q + 1 2 p * | f ( t ϵ φ ( r ) w ϵ ( r ) ) | 2 p * - 2 p N - p p * | t ϵ φ ( r ) w ϵ ( r ) | p * ] r N - 1 𝑑 r .

From the integral mean value theorem, it follows that there exists θ(0,1) such that

ω G ( x , t ϵ ψ ϵ ) [ λ q | f ( t ϵ φ ( ( 1 + θ ) ϵ τ ) w ϵ ( ( 1 + θ ) ϵ τ ) ) | q + 1 2 p * | f ( t ϵ φ ( ( 1 + θ ) ϵ τ ) w ϵ ( ( 1 + θ ) ϵ τ ) ) | 2 p *
(3.12) - 2 p N - p p * | t ϵ φ ( ( 1 + θ ) ϵ τ ) w ϵ ( ( 1 + θ ) ϵ τ ) | p * ] ϵ τ 2 ϵ τ r N - 1 d r .

Noting ρϵ=ϵτ, τ(1p,1), we deduce

(3.13) C ϵ N - p p 2 - p - τ N - p p - 1 w ϵ ( ( 1 + θ ) ϵ τ ) C ϵ - N - p p .

Hence, wϵ((1+θ)ϵτ)+ and φ((1+θ)ϵτ)1 as ϵ0. Now, using Remark 2.4, we have that

| f ( t ϵ φ ( ( 1 + θ ) ϵ τ ) w ϵ ( ( 1 + θ ) ϵ τ ) ) | q = | f ( t ϵ φ ( ( 1 + θ ) ϵ τ ) w ϵ ( ( 1 + θ ) ϵ τ ) ) t ϵ φ ( ( 1 + θ ) ϵ τ ) w ϵ ( ( 1 + θ ) ϵ τ ) | q [ t ϵ φ ( ( 1 + θ ) ϵ τ ) w ϵ ( ( 1 + θ ) ϵ τ ) ] q 2
(3.14) C [ w ϵ ( ( 1 + θ ) ϵ τ ) ] q 2

and

1 2 p * | f ( t ϵ φ ( ( 1 + θ ) ϵ τ ) w ϵ ( ( 1 + θ ) ϵ τ ) ) | 2 p * - 2 p N - p p * | t ϵ φ ( ( 1 + θ ) ϵ τ ) w ϵ ( ( 1 + θ ) ϵ τ ) | p *
- C [ t ϵ φ ( ( 1 + θ ) ϵ τ ) w ϵ ( ( 1 + θ ) ϵ τ ) ] p * - 1
(3.15) - C [ w ϵ ( ( 1 + θ ) ϵ τ ) ] p * - 1 .

It follows from (3.12)–(3.15) that

ω G ( x , t ϵ ψ ϵ ) { C λ [ w ϵ ( ( 1 + θ ) ϵ τ ) ] q 2 - C [ w ϵ ( ( 1 + θ ) ϵ τ ) ] p * - 1 } ϵ τ N
C ϵ τ N - N + δ [ λ ϵ ( N - p p 2 - p - τ N - p p - 1 ) × q 2 + N - δ - C ] , δ = N - p p .

If (A1) or (A2) holds, we can take τ(1p+2(Np-N+p)(p-1)(N-p)pq,1)(1p,1), so that

( N - p p 2 - p - τ N - p p - 1 ) × q 2 + N - δ < 0 ,

which gives

(3.16) B 2 ρ ϵ B ρ ϵ G ( x , t ϵ ψ ϵ ) 0

for all λ>0 and small ϵ>0.

If (A3) holds, we can take λ=ϵ1-p2p, τ(1p+2(N-p)(p-1)2+2p-2(N-p)pq,1)(1p,1) so that

( N - p p 2 - p - τ N - p p - 1 ) × q 2 + N - δ - p + 1 p < 0 ,

which again gives (3.16) for small ϵ>0 and large λ.

From (3.11), (3.16) and Lemma 3.2, we have

J ( t ϵ ψ ϵ ) 1 2 N S N p + C B 2 ρ ϵ | ψ ϵ | p - B ρ ϵ [ C λ ( w ϵ ) q 2 - C ( w ϵ ) p * - 1 ]
1 2 N S N p + C ϵ δ + C B 2 ρ ϵ | ψ ϵ | p - C λ B ρ ϵ w ϵ q 2
(3.17) 1 2 N S N p + C ϵ δ + C B 2 ρ ϵ | ψ ϵ | p - C λ B ρ ϵ w ϵ q 2 .

Noting that

B ρ ϵ w ϵ q 2 = C ϵ N - δ 2 q 0 ρ ϵ ϵ s N - 1 d s ( 1 + s p p - 1 ) δ 2 q

and

0 s N - 1 d s ( 1 + s p p - 1 ) δ 2 q C > 0 for all  N > p  and  q > 2 p ,

we have that

(3.18) J ( t ϵ ψ ϵ ) 1 2 N S N p + C ϵ δ - C λ ϵ N - δ 2 q + C { O ( ϵ p ) for  N > p 2 , O ( ϵ p | ln ϵ | ) for  N = p 2 , O ( ϵ N - p p - 1 ) for  N < p 2 .

From (3.17) and (3.18), we only need to prove J(tϵψϵ)<12NSNp for small ϵ.

If assumption (A1) or (A2) holds, we can verify that both δ and p are larger than N-δ2q, which gives J(tϵψϵ)<12NSNp for ϵ sufficiently small.

If assumption (A3) holds, we take λ=ϵ1-p2p, then we have that δ<p and N-δ2q+1-p2p<δ. Hence, J(tϵψϵ)<12NSNp for ϵ sufficiently small.

Thus, (3.8) holds naturally. ∎

Proof of Theorem 1.1.

Using Lemmas 3.4 and 3.5, there exists vW1,p(N){0} such that v is a weak solution of problem (1.1). By Lp-regularity theory (see [15]), vW1,p(N)Cloc1,α(N). Using the strong maximum principle (see also [15]), we see v>0. ∎

Remark 3.6.

By the same argument, we can consider a similar problem on a bounded domain ΩN:

(3.19) - Δ p u + V ( x ) | u | p - 2 u - Δ p ( | u | 2 ) u = λ | u | q - 2 u + | u | 2 p * - 2 u , x Ω , u | Ω = 0 .

and prove the following corollary.

Corollary 3.7.

Problem (3.19) has a positive solution if λ, q and p satisfy one of assumptions (A1), (A2) or (A3).

4 The Existence of Sign-Changing Solutions

Let Ω be one of the following three types of domains:

(4.1) { x N : | x | < R 1 } , { x N : 0 < R 2 | x | < R 3 < + } , { x N : | x | R 4 > 0 } .

Define

J Ω ( v ) = 1 p Ω [ | v | p + V ( x ) | v | p ] - 2 p N - p p * Ω | v | p * - Ω G ( x , v ) ,
γ Ω ( v ) = J Ω ( v ) , v = Ω [ | v | p + V ( x ) | v | p - 2 p N - p | v | p * - g ( x , v ) v ]

and

M ( Ω ) = { v W r 1 , p ( Ω ) : v 0 , v | Ω = 0 , γ Ω ( v ) = 0 } .

Then we have the following lemmas.

Lemma 4.1.

Let Ω be of one of the forms given by (4.1) and c¯=infvM(Ω)JΩ(v). Then c¯=infvM(Ω)supt>0JΩ(tv).

Proof.

We know that for all vM(Ω), there exists t*>0, satisfying

J Ω ( t * v ) = sup t > 0 J Ω ( t v ) and d J Ω ( t v ) d t | t = t * = 0 .

Direct calculation gives

d J Ω ( t v ) d t = t p - 1 Ω | v | p + Ω [ V ( x ) | f ( t v ) | p - 2 - λ | f ( t v ) | q - 2 - | f ( t v ) | 2 p * - 2 ] f ( t v ) f ( t v ) v
= t p - 1 Ω ( | v | p + [ V ( x ) | f ( t v ) | p - 2 - λ | f ( t v ) | q - 2 - | f ( t v ) | 2 p * - 2 ] f ( t v ) f ( t v ) v t p - 1 )
=: t p - 1 f ~ ( t ) .

Then

f ~ ( t ) t p = Ω [ ( p - 1 ) f 2 ( t v ) t v 2 + f ( t v ) f ′′ ( t v ) t v 2 - ( p - 1 ) f ( t v ) f ( t v ) v ] V ( x ) | f ( t v ) | p - 2
+ λ Ω [ - ( q - 1 ) f 2 ( t v ) t v 2 - f ( t v ) f ′′ ( t v ) t v 2 + ( p - 1 ) f ( t v ) f ( t v ) v ] | f ( t v ) | q - 2
+ Ω [ - ( 2 p * - 1 ) f 2 ( t v ) t v 2 - f ( t v ) f ′′ ( t v ) t v 2 + ( p - 1 ) f ( t v ) f ( t v ) v ] | f ( t v ) | 2 p * - 2
=: I + II + III .

Since f′′(tv)=-2p-1f(tv)p+2|f(tv)|p-2f(tv), from Lemma 2.1 (6), we find that

I = Ω [ ( p - 1 ) f 2 ( t v ) t v 2 - 2 p - 1 | f ( t v ) | p | f ( t v ) | p + 2 t v 2 - ( p - 1 ) f ( t v ) f ( t v ) v ] V ( x ) | f | p - 2
Ω [ ( p - 1 ) f ( t v ) f ( t v ) v - 2 p - 1 | f ( t v ) | p | f ( t v ) | p + 2 t v 2 - ( p - 1 ) f ( t v ) f ( t v ) v ] V ( x ) | f | p - 2
= - 2 p - 1 Ω V ( x ) | f ( t v ) | 2 p - 2 | f ( t v ) | p + 2 t v 2
< 0

and

II = λ Ω [ - ( q - 1 ) f 2 ( t v ) t v 2 + 2 p - 1 | f ( t v ) | p | f ( t v ) | p + 2 t v 2 + ( p - 1 ) f ( t v ) f ( t v ) v ] | f | q - 2
λ Ω [ ( - q + 2 ) f 2 ( t v ) t v 2 + ( p - 1 ) f ( t v ) f ( t v ) v ] | f | q - 2
λ Ω [ - q + 2 2 f ( t v ) f ( t v ) v + ( p - 1 ) f ( t v ) f ( t v ) v ] | f ( t v ) | q - 2
- q + 2 p 2 λ Ω | f ( t v ) | q - 2 f ( t v ) f ( t v ) v
< 0 .

Similarly, we can obtain

III = Ω [ - ( 2 p * - 1 ) f 2 ( t v ) t v 2 + 2 p - 1 | f ( t v ) | p | f ( t v ) | p + 2 t v 2 + ( p - 1 ) f ( t v ) f ( t v ) v ] | f | 2 p * - 2
- 2 p * + 2 p 2 Ω | f ( t v ) | 2 p * - 2 f ( t v ) f ( t v ) v
< 0 .

Thus, f~(t)<0 for t>0, and f~(t) has at most one zero in (0,+). Since vM(Ω),

d J Ω ( t v ) d t | t = 1 = 0 and d J Ω ( t v ) d t | t = t * = 0 ,

we can conclude that t*=1, which implies that

c ¯ = inf v M ( Ω ) J Ω ( v ) = inf v M ( Ω ) sup t > 0 J Ω ( t v ) .

The proof is complete. ∎

By a standard method, we can obtain the following compact lemma (see [5]).

Lemma 4.2.

Let Ω={xRN:0<R1|x|R2+}, then JΩ(v) satisfies the (PS) condition if 2p<q<2p*.

Lemma 4.3.

Let Ω be of one of the forms given by (4.1). Then c¯=infvM(Ω)JΩ(v) can be achieved by a positive function w* which is a positive solution of the following problem:

(4.2) - Δ p v + V ( x ) | v | p - 2 v = g ( x , v ) + 2 p N - p | v | p * - 2 v , x Ω , v | Ω = 0 ,

under the assumption of Theorem 1.1.

Proof.

Firstly, we prove c¯ can be attained. Using Lemmas 2.12.2 and the same argument as in [4], we can verify that the functional JΩ exhibits the mountain pass geometry. By Lemma 4.1, we deduce that for any vM(Ω),

(4.3) c ¯ = inf v M ( Ω ) J Ω ( v ) = inf v M ( Ω ) sup t > 0 J Ω ( t v ) inf γ Γ sup t [ 0 , 1 ] J Ω ( γ ( t ) ) = : c * ,

where

Γ = { γ C ( [ 0 , 1 ] , W 1 , p ( N ) ) : γ ( 0 ) = 0 , γ ( 1 ) = w , J Ω ( γ ( 1 ) ) < 0 } .

Now we show that c¯ is attained by v which is the solution of (4.2). We distinguish two cases. Case 1: Ω=BR, 0<R+. As done in the proof of Lemma 3.5, we can prove that c* is a critical value by the mountain pass lemma, under the assumptions of Theorem 1.1. Thus, there exists w*Wr1,p(Ω) such that JΩ(w*)=c* and JΩ(w*)=0. Hence,

c ¯ = inf v M ( Ω ) J Ω ( v ) J Ω ( w * ) = c * .

Considering (4.3), we find that JΩ(w*)=c¯ and JΩ(w*)=0, and that w* is the weak solution of (4.2). Case 2: Ω={xRN:0<R1|x|R2+}. By Lemma 4.2 and the mountain pass lemma, we can deduce that c* is the critical value of JΩ. Repeating the argument of case 1, we can conclude that c¯ can be attained by w* and w* is a week solution of (4.2).

Next, we prove w*>0. By Lp-regularity theory [15], we have w*Wr1,p(Ω)C1,α(Ω). If the attained function w* changes sign in Ω, then

J Ω ( ( w * ) + ) < J Ω ( w * ) = inf M ( Ω ) J Ω ( v ) J Ω ( ( w * ) + ) ,

which is a contradiction. Therefore, either w*0 or w*0. Without loss of generality, we can assume w*0. If there exists x0 such that w*(x0)=0, then (w*)(x0)=0. By the strong maximum principle (see, e.g., [15]), w*=0 near x0 and w* will vanish identically, which is impossible since w*M(Ω). Hence, w*>0 and we complete the proof. ∎

In the following, we will consider the existence of the nodal solutions for (1.1). For any given k+2 numbers rj (j=0,1,,k+1) such that 0=r0<r1<r2<<rk<rk+1=+, denote

Ω 1 = { x N : | x | < r 1 } , Ω j = { x N : r j - 1 < | x | < r j } , j = 2 , 3 , , k + 1 .

We will always extend vjWr1,p(Ωj) to Wr1,p(N) by setting v0 for xNΩj for every vj, j=1,2,,k+1. In this sense, we use J(vj) to replace JΩj(vj), and γ(vj) to replace γΩj(vj) in the sequel.

Define

Y k ± ( r 1 , r 2 , , r k + 1 ) = { v W r 1 , p ( N ) : v = ± j = 1 k + 1 ( - 1 ) j - 1 v j , v j 0 , v j 0 , v j W r 1 , p ( Ω j ) , j = 1 , 2 , , k + 1 }

and

M k ± = { v W r 1 , p ( N ) : there exist  0 < r 1 < r 2 < < r k < r k + 1 = +  such that
v Y k ± ( r 1 , r 2 , , r k + 1 )  and  v j M ( Ω j ) , j = 1 , 2 , , k + 1 } .

Note that Mk±, k=1,2,. In the following, we will drop the superscript “+” from Mk+ for simplicity. For Mk-, everything could be done exactly in the same way. By using arguments of the standard Nehari method [28], it is easy to verify that

v = j = 1 k + 1 ( - 1 ) j - 1 v j M k J ( v ) = max α j > 0 1 j k + 1 J ( j = 1 k + 1 α j v ~ j ) ,

where v~j=(-1)j-1vj.

Set

c k = inf M k J ( v ) , k = 1 , 2 , .

For vW1,p(N), define

h ( v ) = { 2 p N - p N | v | p * N [ | v | p + V ( x ) | v | p - g ( x , v ) v ] if  v 0 , 0 if  v = 0 .

Lemma 4.4.

Suppose λ, q and p satisfy one of assumptions (A1*)’, (A2*)’ or (A3*)’, and that ck can be attained. Then

c k + 1 < c k + 1 2 N S N p .

Proof.

A similar statement is proved, for instance, in [9]. For sake of completeness, we give here the proof.

Let ck be attained by v and r1 be the first node of v. Set

v 0 = { v , x B r 1 , 0 , otherwise .

First we define P={vWr1,p(N):v0}. Let Σ be the set of maps such that:

  1. σC(D,Wr1,p(N)),

  2. σ(s,0)=0, σ(0,t)P, σ(1,t)-P,

  3. (Jσ)(s,1)0, (hσ)(s,1)2,

where D=[0,1]×[0,1], s[0,1]. We claim that Σ. Indeed, the map

σ = σ ( s , t ) = ρ t ( ( 1 - s ) v 0 - s ψ ϵ )

is in Σ for large ρ and small ϵ.

For any σΣ,

h ( σ + ( x ) ) - h ( σ - ( x ) ) 0 for  x { ( 0 , t ) : t [ 0 , 1 ] } ,
h ( σ + ( x ) ) - h ( σ - ( x ) ) 0 for  x { ( 1 , t ) : t [ 0 , 1 ] } ,
h ( σ + ( x ) ) + h ( σ - ( x ) ) - 2 0 for  x { ( s , 1 ) : s [ 0 , 1 ] } ,
h ( σ + ( x ) ) + h ( σ - ( x ) ) - 2 0 for  x { ( s , 0 ) : s [ 0 , 1 ] } .

We deduce (by Miranda’s theorem [26]) that there exists x¯D such that

h ( σ + ( x ¯ ) ) - h ( σ - ( x ¯ ) ) = h ( σ + ( x ¯ ) ) + h ( σ - ( x ¯ ) ) - 2

and

(4.4) h ( σ + ( x ¯ ) ) = h ( σ - ( x ¯ ) ) = 1 .

Define w*=σ(x¯)=α*v0+β*ψϵ, where α*=ρt¯(1-s¯), β*=-ρt¯s¯,x¯D.

In the following, we will prove that w* has only one zero point r¯(0,r1). Indeed, by a standard ODE technique, we can deduce that v0(r)<0 for 0<r<r1, since V(r)0. Thus, α*v0 is monotonically decreasing because α*>0. By the definition of ψϵ and the fact that β*<0, we can conclude that β*ψϵ is monotonically increasing. This implies that w* has only one zero point if ϵ small enough. By (4.4), we get that (w*)+M(Ω+), (w*)-M(Ω-). Define

w ( x ) = { - ( w * ) - ( x ) , x B r ¯ , - ( w * ) + ( x ) , x B r 1 B r ¯ , - v ( x ) , x N B r 1 .

Clearly, w(x)Mk+1, thus we have that

c k + 1 J ( w ( x ) ) sup α , β J ( α v 0 + β ψ ϵ ) + J ( v * )
= sup { J ( α v 0 + β ψ ϵ ) + J ( v * ) : α , β , J ( α v 0 + β ψ ϵ ) 0 } ,

where

v * = { 0 , x B r 1 , v , x N B r 1 .

In order to prove Lemma 4.4, we only need to verify the following inequality:

sup α , β J ( α v 0 + β ψ ϵ ) + J ( v * ) < c k + 1 2 N S N p .

Now we claim that if

( α , β ) { ( α , β ) 2 : J ( α v 0 + β ψ ϵ ) 0 } ,

then α and β are bounded, provided 2p<q<2p*.

Indeed, from Lemma 2.1 (8), there exist a,b>0 such that

a f 2 ( t ) + b f ( t ) - t 0 for all  t 0 ,

i.e.,

f ( t ) - b + b 2 + 4 a t 2 a for all  t 0 .

Thus,

f 2 ( t ) 1 4 a 2 [ 2 b 2 + 4 a t - 2 b b 2 + 4 a t ]
1 4 a 2 [ 2 b 2 + 4 a t - 1 2 ( ( 2 b ) 2 + b 2 + 4 a t ) ]
= t 2 a - b 2 8 a 2 ,

i.e.,

( t 2 a ) p * ( f 2 ( t ) + b 2 8 a 2 ) p * C 1 ( f 2 ( t ) ) p * + C 2 ( b 2 8 a 2 ) p * C 1 f 2 p * ( t ) + C 3 ,

which gives

(4.5) f 2 p * ( t ) C 4 t p * - C 5 for all  t 0 .

Thus, using Lemma 2.1 (3), (4.5) and the inequality

| c + d | m | c | m + | d | m - C ( | c | m - 1 | d | + | c | | d | m - 1 ) for all  c , d , m 1

(see [11]), we see that

0 J ( α v 0 + β ψ ϵ )
= 1 p N ( | ( α v 0 + β ψ ϵ ) | p + V ( x ) | f ( α v 0 + β ψ ϵ ) | p ) - N K ( f ( α v 0 + β ψ ϵ ) )
1 p N ( | ( α v 0 + β ψ ϵ ) | p + V ( x ) | α v 0 + β ψ ϵ | p ) - 1 2 p * N | f ( α v 0 + β ψ ϵ ) | 2 p *
C N ( | ( α v 0 + β ψ ϵ ) | p + | α v 0 + β ψ ϵ | p ) - C 6 N | α v 0 + β ψ ϵ | p * + C 7
C N ( | ( α v 0 + β ψ ϵ ) | p + | α v 0 + β ψ ϵ | p ) - C N ( | α v 0 | p * + | β ψ ϵ | p * )
+ C N ( | α | p * - 1 | β | | v 0 | p * - 1 | ψ ϵ | + | α | | β | p * - 1 | v 0 | | ψ ϵ | p * - 1 ) + C 7
C ( | α | p + | β | p ) - C ( | α | p * + | β | p * ) + C 7 + C N ( | α | p * - 1 | β | | ψ ϵ | + | α | | β | p * - 1 | ψ ϵ | p * - 1 ) .

Using the estimations in Lemma 3.2 and Young’s inequality, we have

0 C ( | α | p + | β | p ) - C ( | α | p * + | β | p * ) + C ϵ N - p p 2 - p ( | α | p * + | β | p * ) + C 7 .

By taking ϵ small enough so that C¯=C-CϵN-pp2-p>0 as N>p, we get that

0 C ( | α | p + | β | p ) - C ¯ ( | α | p * + | β | p * ) + C 7 ,

which immediately implies that α and β are bounded.

On the other hand, by Lemma 2.1 (3), (8), (9) and the mean value theorem, we have

| 1 q N [ | f ( α v 0 + β ψ ϵ ) | q - | f ( α v 0 ) | q - | f ( β ψ ϵ ) | q ] |
= | 0 1 N [ | f ( s α v 0 + β ψ ϵ ) | q - 2 f ( s α v 0 + β ψ ϵ ) f ( s α v 0 + β ψ ϵ ) - | f ( s α v 0 ) | q - 2 f ( s α v 0 ) f ( s α v 0 ) ] α v 0 𝑑 s |
| 0 1 N [ | f ( s α v 0 + β ψ ϵ ) | q - 2 f ( s α v 0 + β ψ ϵ ) - | f ( s α v 0 ) | q - 2 f ( s α v 0 ) ] f ( s α v 0 + β ψ ϵ ) α v 0 𝑑 s |
    + | 0 1 N | f ( s α v 0 ) | q - 2 f ( s α v 0 ) [ f ( s α v 0 + β ψ ϵ ) - f ( s α v 0 ) ] α v 0 d s |
C 0 1 N | f ( s α v 0 + θ 1 β ψ ϵ ) | q - 2 | f ( s α v 0 + θ 1 β ψ ϵ ) | | f ( s α v 0 + β ψ ϵ ) | | α v 0 | | β ψ ϵ | d s
    + C 0 1 N | f ( s α v 0 ) | q - 1 | f ′′ ( s α v 0 + θ 2 β ψ ϵ ) | | α v 0 | | β ψ ϵ | d s ,

where θ1,θ2(0,1). Since |f′′(t)|=2p-1|f(t)f(t)|p-1|f(t)|3C|f(t)|3 and |f(t)|C, we have

| N [ | f ( α v 0 + β ψ ϵ ) | q - | f ( α v 0 ) | q - | f ( β ψ ϵ ) | q ] | C 0 1 N | f ( s α v 0 + θ 1 β ψ ϵ ) | q - 3 | f ( s α v 0 + β ψ ϵ ) | | α v 0 | | β ψ ϵ | d s + C N | ψ ϵ |
C 0 1 N | s α v 0 + θ 1 β ψ ϵ | q - 3 2 | s α v 0 + β ψ ϵ | 1 2 | α v 0 | | β ψ ϵ | d s + C N | ψ ϵ |
C 0 1 N | s α v 0 + C β ψ ϵ | q 2 - 2 | α v 0 | | β ψ ϵ | d s + C N | ψ ϵ |
C N ( | ψ ϵ | + | ψ ϵ | q 2 - 1 )
C N ( | ψ ϵ | + | ψ ϵ | p - 1 + | ψ ϵ | p * - 1 ) .

Similarly, we verify that

| N [ | f ( α v 0 + β ψ ϵ ) | 2 p * - | f ( α v 0 ) | 2 p * - | f ( β ψ ϵ ) | 2 p * ] | C N ( | ψ ϵ | + | ψ ϵ | p * - 1 ) .

It follows that

J ( α v 0 + β ψ ϵ ) = 1 p N ( | ( α v 0 + β ψ ϵ ) | p + V ( x ) | f ( α v 0 + β ψ ϵ ) | p ) - N K ( f ( α v 0 + β ψ ϵ ) )
J ( α v 0 ) + J ( β ψ ϵ ) + C N ( | ψ ϵ | + | ψ ϵ | p - 1 + | ψ ϵ | + | ψ ϵ | p - 1 + | ψ ϵ | p * - 1 ) .

Thus, from Lemma 3.4, (3.17) and the above inequality, we have

J ( α v 0 + β ψ ϵ ) + J ( v * ) c k + J ( β ψ ϵ ) + O ( ϵ N - p p 2 - p )
c k + 1 2 N S N p + O ( ϵ N - p p 2 - p ) + C ϵ δ - C λ ϵ N - δ 2 q + C { O ( ϵ p ) for  N > p 2 , O ( ϵ p | ln ϵ | ) for  N = p 2 , O ( ϵ N - p p - 1 ) for  N < p 2 ,

where δ=N-pp. Next, repeating the last part in the proof of Lemma 3.5, we find that if (A1*)’ or (A2*)’ holds, then ck+1<ck+12NSNp for ϵ sufficiently small.

On the other hand, if (A3*)’ holds, we take λ=ϵ-p. Then N-pp2-p<p and N-δ2q+1-p2p<N-pp2-p, which again gives that ck+1<ck+12NSNp for ϵ sufficiently small.

Thus, we have

J ( α v 0 + β ψ ϵ ) + J ( v * ) < c k + 1 2 N S N p .

Lemma 4.5.

Suppose λ, q and p satisfy one of assumptions (A1*)’, (A2*)’ or (A3*)’. Then ck can be attained, where k=0,1,.

Proof.

We intend to prove by induction that for each k there exists vkMk such that J(vk)=ck.

The case that k=0 can be deduced by setting Ω=N in Lemma 4.3. We discuss the case k1. Suppose the claim is true for k-1 and let {vj} be a minimizing sequence of ck in Mk. Then

lim j J ( v j ) = c k ,

where vj corresponds to k nodes, rj1,rj2,,rjk, with 0<rj1<rj2<<rjk<+. Set

Ω j i = { x N : r j i - 1 < | x | < r j i } ,

and define

v j i = { v j , x Ω j i , 0 , x Ω j i .

By selecting a subsequence, we may assume that limjrji=ri. Clearly, 0r1r2rk+. Step 1: rk<+. If rk=+, then limjrjk=+. By Strauss’ lemma,

v j ( x ) 0 as  | x |  uniformly,  j = 1 , 2 , .

Taking g~(x,v)=g(x,v)+2pN-p|v|p*-2v, by Lemma 2.2, we can obtain g~(x,s)sp-1|s=0=0. Thus, for fixed ϵ,0<ϵ<1, there exists J0 such that if jJ0, then by vjkM(Ωjk),

| x | > r j k ( | v j k | p + V ( x ) | v j k | p ) = | x | > r j k g ~ ( x , v j k ) v j k
C sup | x | > r j k | g ~ ( x , v j k ) | | v j k | p - 1 | x | > r j k | v j k | p
ϵ | x | > r j k ( | v j k | p + V ( x ) | v j k | p ) ,

hence ϵ1, and we get contradiction. Step 2: riri-1, i=1,2,,k. Here we set r0=0.

If there exists some i{1,2,,k} such that ri=ri-1, then limjrji=limjrji-1. We denote the measure of Ωji by |Ωji|. Then |Ωji|0 as j. By Hölder’s inequality, we have that

(4.6) | v j i | s s | v j i | p * s | Ω j i | 1 - s p * 0 as  j ,  if  p s < p * .

On the other hand, by Lemma 2.2, for any ϵ1>0, there exists C(ϵ1)>0 such that

g ( x , v j i ) v j i ϵ 1 | v j i | p + C ( ϵ 1 ) | v j i | p * .

Since vjiM(Ωji), we have

2 p N - p | v j i | p * p * v j i p - ϵ 1 | v j i | p p - C ( ϵ 1 ) | v j i | p * p * .

Thus,

| v j i | p * p * C v j i p C S | v j i | p * p ,

which implies that

(4.7) | v j i | p * p * - p C S > 0 .

Combining (4.6) and (4.7), we have

(4.8) lim j Ω j i | v j i | s 0 and lim j Ω j i | v j i | p * a > 0 , p s < p * .

Using Lemma 2.2, for any ϵ2>0, there exists C(ϵ2)>0 such that

g ( x , v j i ) v j i C ( ϵ 2 ) | v j i | p + ϵ 2 | v j i | p * .

From (4.6)–(4.7), the fact that vjiM(Ωji) and the Sobolev inequality, we have

( 2 p N - p + ϵ 2 ) | v j i | p * p * - p S + o ( 1 ) ,

which implies that

(4.9) 2 p N - p lim j | v j i | p * p * - p S .

From (3.7) and Remark 2.4, for t large, we get that

1 p g ( x , t ) t - G ( x , t ) ( λ 2 p - λ q ) | f ( t ) | q + 1 N [ 1 2 ( f ( t ) t ) 2 p * - 2 p N - p ] t p * - C t p * - 1 .

Choosing M>0 such that

(4.10) 1 p g ( x , t ) t - G ( x , t ) - C t p * - 1 if  t M ,

and using the fact that vjiM(Ωji), we have

L := lim j J ( v j i ) = lim j { 1 p Ω j i [ | v j i | p + V ( x ) | v j i | p ] - 2 p N - p p * Ω j i | v j i | p * - Ω j i G ( x , v j i ) }
= 1 N lim j 2 p N - p | v j i | p * p * + ( { | v j i | M } Ω j i + { | v j i | M } Ω j i ) ( 1 p g ( x , v j i ) v j i - G ( x , v j i ) )
=: I 2 + I 3 + I 4 .

By (4.8), (4.10) and Hölder’s inequality, we find that

I 3 - C lim j { | v j i | M } Ω j i | v j i | p * - 1 - C lim j Ω j i | v j i | p * - 1 - C lim j ( Ω j i | v j i | p * ) p * - 1 p * lim j | Ω j i | 1 p * = 0

and

I 4 - lim j { | v j i | M } Ω j i | 1 p g ( x , v j i ) v j i - G ( x , v j i ) | - C lim j { | v j i | M } Ω j i d x - C lim j | Ω j i | = 0 .

Thus, by (4.9),

L 1 N lim j 2 p N - p | v j i | p * p * 1 2 N S N p .

By the inductive assumption and Lemma 4.4, we deduce that L>ck-ck-1. Now we fix ϵ=L-(ck-ck-1)2>0 and choose M>0 so that

| J ( v j i ) - L | < ϵ , | J ( v j ) - c k | < ϵ for  j M .

Then we may define v^(x)Mk-1 by

v ^ ( x ) = { v j l ( x ) , x Ω j l ,  for  l < i , 0 , x Ω j i , - v j l ( x ) , x Ω j l ,  for  l > i .

Hence,

J ( v ^ ) = J ( v j ) - J ( v j i ) < c k - L + 2 ϵ = c k - 1 for  j M ,

which contradicts the fact that ck-1=infMk-1J(v). Thus, riri-1, i=1,2,,k. Step 3: ck is attained.

We can find a subsequence (still denoted by {vj}) such that

v j v weakly in  W r 1 , p ( N ) ,
v j v strongly in  L s ( N ) , p < s < p * .

Set Ωi={xN:ri-1<|x|<ri} for all i=1,2,,k+1, r0=0 and rk+1=+. Set vi=v in Ωi and vi=0 in NΩi. Lemma 4.3 implies that c¯=infM(Ωi)J(v) is attained by some positive function v^i satisfying the following problem:

{ - Δ p v + V ( x ) | v | p - 2 v = g ( x , v ) + 2 p N - p | v | p * - 2 v , x Ω i , v | Ω i = 0 , v > 0  in  Ω i .

Define vk=i=1k+1(-1)i-1v^i(x) (v^i(x)=0, xΩi). Then, vkMk.

Consider the coordinate transformations Φj:NN, j=1,2,, defined by

Φ j ( x ) = φ j ( | x | ) x | x | , x N , where  φ j ( r ) = ( r i - r i - 1 ) ( r - r j i - 1 ) r j i - r j i - 1 + r i - 1 .

For any r, clearly, Φj(Ωji)=Ωi.

Let y=Φj(x)Ωi for xΩji. Then

(4.11) | v ( y ) | = ( R j i ) - 1 | v ( x ) | ,
(4.12) d y = | J j i | d x

and

(4.13) a j i ( Φ j ( r ) r ) N - 1 A j i ,

where

R j i = r i - r i - 1 r j i - r j i - 1 , J j i = [ φ j ( | x | ) ] N - 1 ( φ j ( | x | ) ) | x | 1 - N , a j i = ( min { r i r j i , r i - 1 r j i - 1 } ) N - 1 , A j i = ( max { r i r j i , r i - 1 r j i - 1 } ) N - 1 .

Clearly,

(4.14) a j i R j i | J j i | A j i R j i

and

(4.15) R j i 1 , a j i 1 , A j i 1 , J j i 1 as  j .

Let

f i ( t ) = t p Ω i ( | ( v j i ) | p + V | v j i | p ) d y - 2 p N - p t p * Ω i | v j i | p * d y - Ω i g ( y , t v j i ) t v j i d y .

Using Lemma 2.2, we can find tji>0 satisfying fi(tji)=0. Thus, tjivjiM(Ωi).

Now, we claim that

(4.16) t j i 1 as  j , i = 1 , 2 , , k .

Indeed, since fi(tji)=0, we have

(4.17) Ω i ( | ( v j i ) | p + V ( y ) | v j i | p ) d y - 2 p N - p ( t j i ) p * - p Ω i | v j i | p * d y - Ω i g ( y , t j i v j i ) ( t j i ) 1 - p v j i d y = 0 .

It is easy to verify that there exists a constant M>0 such that

0 < t j i M < .

Selecting a subsequence, we assume limjtji=ti. Using (4.11)–(4.15), we find

(4.18) lim j Ω i | v j i ( y ) | p d y = lim j Ω j i | v j i ( x ) | p d x ,
(4.19) lim j Ω i V ( y ) | v j i ( y ) | p 𝑑 y = lim j Ω j i V ( x ) | v j i ( x ) | p 𝑑 x ,
(4.20) lim j Ω i | v j i ( y ) | p * d y = lim j Ω j i | v j i ( x ) | p * d x .

By Lemma 2.2, Strauss’ lemma and the fact vji(y)=0, yΩi, we have that

(4.21) lim j Ω i g ( y , t j i v j i ) t j i v j i 𝑑 y = N g ( x , t i v i ) t i v i 𝑑 x .

Substituting (4.18)–(4.21) into (4.17), we find that

(4.22) lim j [ Ω j i ( | ( v j i ) | p + V ( x ) | v j i | p ) d x - 2 p N - p ( t i ) p * - p Ω j i | v j i | p * d x ] - N g ( x , t i v i ) ( t i ) 1 - p v i d x = 0 .

Proceeding as in step 2, we conclude that

2 p N - p lim j Ω j i | v j i | p * = 2 p N - p N | v i | p * := l .

From (4.22), using the Brezis–Lieb lemma [6] and vjiM(Ωji), we have that

(4.23) ( 1 - ( t i ) p * - p ) l + N g ( x , v i ) v i 𝑑 x - N g ( x , t i v i ) ( t i ) 1 - p v i 𝑑 x = 0 .

Set

(4.24) P ( s ) = ( 1 - s p * - p ) l + N g ( x , v i ) v i 𝑑 x - N g ( x , s v i ) s 1 - p v i 𝑑 x .

Lemma 4.6 below implies that P(s) has only one zero point in (0,+). On account of (4.23), we have ti>0 and hence ti=1, which implies (4.16). Moreover, by (4.16)–(4.21), we deduce that

lim j J ( t j i v j i ( y ) ) = lim j J ( v j i ( x ) ) .

On the other hand, since J(v^i)=infM(Ωi)J(v) and tjivji(y)M(Ωi), we get J(v^i)J(tjivji(y)), and hence

lim j J ( v j i ( x ) ) J ( v ^ i ) , i = 1 , 2 , , k + 1 .

As a result,

c k = lim j J ( v j ) = lim j i = 1 k + 1 J ( v j i ) i = 1 k + 1 J ( v ^ i ) = J ( v k ) .

Since vkMk, we have that ck=J(vk), which means that ck is attained. ∎

Lemma 4.6.

Let P(s) be defined by (4.24). Then P(s)<0, s(0,+).

Proof.

Noticing

g ( x , s ) = f ( s ) [ λ | f ( s ) | q - 2 f ( s ) + | f ( s ) | 2 p * - 2 f ( s ) - V ( x ) | f ( s ) | p - 2 f ( s ) ] + V ( x ) | s | p - 2 s - 2 p N - p | s | p * - 2 s ,

we see

g ( x , s ) s = f ′′ ( s ) f ( s ) [ λ | f ( s ) | q - 2 + | f ( s ) | 2 p * - 2 - V ( x ) | f ( s ) | p - 2 ] + ( p - 1 ) V ( x ) | s | p - 2 - ( p * - 1 ) 2 p N - p | s | p * - 2
+ f 2 ( s ) [ ( q - 1 ) λ | f ( s ) | q - 2 + ( 2 p * - 1 ) | f ( s ) | 2 p * - 2 - ( p - 1 ) V ( x ) | f ( s ) | p - 2 ] .

Hence,

g ( x , s v i ) s ( s v i ) 2 - ( p - 1 ) g ( x , s v i ) s v i
= [ f ′′ ( s v i ) f ( s v i ) ( s v i ) 2 + ( q - 1 ) f 2 ( s v i ) ( s v i ) 2 - ( p - 1 ) f ( s v i ) f ( s v i ) s v i ] λ | f ( s v i ) | q - 2
    + [ f ′′ ( s v i ) f ( s v i ) ( s v i ) 2 + ( 2 p * - 1 ) f 2 ( s v i ) ( s v i ) 2 - ( p - 1 ) f ( s v i ) f ( s v i ) s v i ] | f ( s v i ) | 2 p * - 2
    + [ - f ′′ ( s v i ) f ( s v i ) ( s v i ) 2 - ( p - 1 ) f 2 ( s v i ) ( s v i ) 2 + ( p - 1 ) f ( s v i ) f ( s v i ) s v i ] V ( x ) | f ( s v i ) | p - 2
    - ( p * - p ) 2 p N - p | s v i | p *
=: I 5 + I 6 + I 7 - ( p * - p ) 2 p N - p | s v i | p * .

Considering f′′=-2p-1(f)p+2|f|p-2f and Lemma 2.1, we find

I 5 = λ [ ( q - 1 ) f 2 ( s v i ) ( s v i ) 2 - 2 p - 1 | f ( s v i ) | p | f ( s v i ) | p + 2 ( s v i ) 2 - ( p - 1 ) f ( s v i ) f ( s v i ) s v i ] | f ( s v i ) | q - 2
λ [ ( q - 2 ) f 2 ( s v i ) ( s v i ) 2 - ( p - 1 ) f ( s v i ) f ( s v i ) v i ] | f ( s v i ) | q - 2
( q - 2 p ) λ | f ( s v i ) | q - 2 f 2 ( s v i ) ( s v i ) 2 > 0 for  q > 2 p .

Similarly, we have

I 6 ( 2 p * - 2 p ) | f ( s v i ) | 2 p * - 2 f 2 ( s v i ) ( s v i ) 2 > 0 .

On the other hand, from Lemma 2.1, it follows that

I 7 [ 2 p - 1 | f ( s v i ) | p | f ( s v i ) | p + 2 ( s v i ) 2 - ( p - 1 ) f ( s v i ) f ( s v i ) s v i + ( p - 1 ) f ( s v i ) f ( s v i ) s v i ] V ( x ) | f | p - 2
= 2 p - 1 V ( x ) | f ( s v i ) | 2 p - 2 | f ( s v i ) | p + 2 ( s v i ) 2 > 0 .

Hence,

P ( s ) = - ( p * - p ) s p * - p - 1 l - N g ( x , s v i ) s ( s v i ) 2 - ( p - 1 ) g ( x , s v i ) s v i s p + 1
= - ( p * - p ) s p * - p - 1 l - N I 5 + I 6 + I 7 s p + 1 + ( p * - p ) s p * - p - 1 N 2 p N - p | v i | p *
= - N I 5 + I 6 + I 7 s p + 1 < 0 .

Consequently, the proof is completed. ∎

Now, we are ready to prove the main result.

Proof of Theorem 1.2.

The main argument is essentially the same as in the proof of [13, Theorem 1.1], and we only give a sketch.

By Lemma 4.3, we can find vkMk which attains ck. Now we need to prove that vk solves (1.1). For convenience, we define v:=vk and suppose that 0<r1<r2<<rk<+ are k nodes of vk. We rewrite (1.4) as

- ( r N - 1 | v | p - 2 v ) = r N - 1 ( h ( r , v ) - V | v | p - 2 v ) ,

where

h ( r , v ) = f ( v ) [ λ | f ( v ) | q - 2 f ( v ) + | f ( v ) | 2 p * - 2 f ( v ) - V ( r ) | f ( v ) | p - 2 f ( v ) ] + V ( r ) | v | p - 2 v

and H(r,v)=0vh(r,s)𝑑s. Obviously v is of class C1 on

E = { r ( 0 , + ) : r r j , j = 1 , 2 , , k } .

To complete the proof, we only need to show

v + = lim r r j v ( r ) = lim r r j v ( r ) = v - , j = 1 , 2 , , k .

To this end, we use an indirect argument. Assume that v+v- and set ρ=rj-1, σ=rj, τ=rj+1. We may assume that v0 on [ρ,σ], and v0 on [σ,τ]. Now fix ν>0 (ν<min{σ-ρ,τ-σ}) and define v~:[ρ,τ] by

v ~ ( r ) = { v ( r ) if  | r - σ | ν , v ( σ - ν ) + ( r - σ + ν ) [ v ( σ + ν ) - v ( σ - ν ) ] 2 ν if  | r - σ | < ν .

Let σ0=σ0(ν)(σ-ν,σ+ν) be defined by v~(σ0)=0. There exist α=α(ν)>0 and β=β(ν)>0 such that

ρ σ 0 ( | α v ~ | p + V ( y ) | α v ~ | p - h ( r , α v ~ ) α v ~ ) r N - 1 𝑑 r = 0 , σ 0 τ ( | β v ~ | p + V ( y ) | β v ~ | p - h ( r , β v ~ ) β v ~ ) r N - 1 𝑑 r = 0 .

Next we define w:[ρ,τ]N by setting

w ( r ) = { α v ~ ( r ) , ρ r σ 0 , β v ~ ( r ) , σ 0 r τ .

Obviously, ψ(v)ψ(w), where

ψ ( s ) = ρ τ ( 1 p ( | s | p + V | s | p ) - H ( r , s ) ) r N - 1 𝑑 r .

Now, we estimate ψ(w) exactly as done in the proof of [12, Theorem 1.1] and can deduce that ψ(w)<ψ(v) for ν>0 small enough, which contradicts the fact that ψ(v)ψ(w). ∎


Communicated by Yinbin Deng


Award Identifier / Grant number: 11371160

Award Identifier / Grant number: 11629101

Funding statement: The research was supported by the Natural Science Foundation of China (11371160, 11629101).

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Received: 2016-09-13
Accepted: 2017-05-16
Published Online: 2017-06-21
Published in Print: 2018-02-01

© 2018 Walter de Gruyter GmbH, Berlin/Boston

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

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