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Existence and multiplicity of positive solutions to a perturbed singular elliptic system deriving from a strongly coupled critical potential

Tsing-San Hsu

Author Affiliations

Department of Natural Sciences in the Center for General Education, Chang Gung University, Kwei-San, Tao-Yuan, 333, Taiwan, ROC

Boundary Value Problems 2012, 2012:116  doi:10.1186/1687-2770-2012-116

The electronic version of this article is the complete one and can be found online at: http://www.boundaryvalueproblems.com/content/2012/1/116


Received:12 March 2012
Accepted:3 October 2012
Published:17 October 2012

© 2012 Hsu; licensee Springer

This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/2.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

Abstract

In this paper, we consider singular elliptic systems involving a strongly coupled critical potential and concave nonlinearities. By using variational methods and analytical techniques, the existence and multiplicity of positive solutions to the system are established.

MSC: 35J60, 35B33.

Keywords:
Palais-Smale condition; Nehari manifold; strongly coupled; elliptic system; critical potential

1 Introduction and main results

In this paper, we consider the following elliptic system:

{ L u = η 1 α 1 2 | u | α 1 2 | v | β 1 u + η 2 α 2 2 | u | α 2 2 | v | β 2 u + σ 1 | u | q 2 u , L v = η 1 β 1 2 | u | α 1 | v | β 1 2 v + η 2 β 2 2 | u | α 2 | v | β 2 2 v + σ 2 | v | q 2 v , u , v H 0 1 ( Ω ) , (1.1)

where Ω R N is a smooth bounded domain such that 0 Ω , L : = ( Δ μ | x | 2 ) , 2 : = 2 N N 2 is the critical Sobolev exponent, μ ¯ : = ( N 2 2 ) 2 is the best Hardy constant and H : = H 0 1 ( Ω ) denotes the completion of C 0 ( Ω ) with respect to the norm u 0 = ( Ω | u | 2 d x ) 1 2 and H μ = H μ ( Ω ) is defined as the completion of the C 0 ( Ω ) with respect to the norm defined by u μ = ( Ω ( | u | 2 μ u 2 | x | 2 ) d x ) 1 2 for μ < μ ¯ .

Definitions of strongly and weakly coupled terms are as follows.

The terms | u | α and | v | β ( α , β > 0 ) are weakly coupled, | L u | α | K v | β ( α , β > 0 ) is strongly coupled when L or K is a derivative operator. Thus, η 1 | u | α 1 | v | β 1 + η 2 | u | α 2 | v | β 2 is strongly coupled when η 1 and η 2 are positive.

The parameters in (1.1) satisfy the following assumption.

(ℋ) N 3 , 0 μ < μ ¯ , 1 < q < 2 , η 1 + η 2 > 0 , 0 η i < + , σ i > 0 , α i , β i > 1 , α i + β i = 2 , i = 1 , 2 .

The corresponding energy functional of (1.1) is defined in H × H by

J ( u , v ) : = 1 2 Ω ( | u | 2 + | v | 2 μ | u | 2 + | v | 2 | x | 2 ) d x 1 2 Q ( u , v ) 1 q K ( u , v ) ,

where Q ( u , v ) : = Ω ( η 1 | u | α 1 | v | β 1 + η 2 | u | α 2 | v | β 2 ) d x and K ( u , v ) : = Ω ( σ 1 | u | q + σ 2 | v | q ) d x . Then J C 1 ( H × H , R ) and the duality product between H × H and its dual space ( H × H ) 1 is defined as

J ( u , v ) , ( ϕ 1 , ϕ 2 ) : = Ω ( u ϕ 1 + v ϕ 2 μ u ϕ 1 + v ϕ 2 | x | 2 ) d x Ω ( η 1 α 1 2 | u | α 1 2 | v | β 1 u ϕ 1 + η 2 α 2 2 | u | α 2 2 | v | β 2 u ϕ 1 ) d x Ω ( η 1 β 1 2 | u | α 1 | v | β 1 2 v ϕ 2 + η 2 β 2 2 | u | α 2 | v | β 2 2 v ϕ 2 ) d x Ω ( σ 1 | u | q 2 u ϕ 1 + σ 2 | v | q 2 v ϕ 2 ) d x ,

where u , v , ϕ 1 , ϕ 2 H and J ( u , v ) denotes the Fréchet derivative of J at ( u , v ) . A pair of functions ( u , v ) H × H is said to be a weak solution of (1.1) if

( u , v ) ( 0 , 0 ) , J ( u , v ) , ( ϕ 1 , ϕ 2 ) = 0 , ( ϕ 1 , ϕ 2 ) H × H .

Therefore, a weak solution of (1.1) is equivalent to a nonzero critical point of J ( u , v ) [1].

Problem (1.1) is related to the well-known Hardy inequality [2]

R N | u | 2 | x | 2 d x 1 μ ¯ R N | u | 2 d x , u C 0 ( R N ) . (1.2)

If μ < μ ¯ , by (1.2), Ω ( | u | 2 μ u 2 | x | 2 ) d x is an equivalent norm of H, the operator L is positive and the first eigenvalue Λ 1 ( μ ) of L and the following best constant are well defined:

S ( μ ) : = inf u D 1 , 2 ( R N ) { 0 } R N ( | u | 2 μ u 2 | x | 2 ) d x ( R N | u | 2 d x ) 2 2 , μ ( , μ ¯ ) , (1.3)

where D 1 , 2 ( R N ) is the completion of C 0 ( R N ) with respect to ( R N | u | 2 d x ) 1 2 . Note that S ( 0 ) is the well-known best Sobolev constant. For 0 μ < μ ¯ , the constant S ( μ ) is achieved by the following extremal functions [3]:

V μ , ε ( x ) : = ε 2 N 2 U μ ( ε 1 x ) , ε > 0 , (1.4)

where U μ ( x ) = U μ ( | x | ) is a radially symmetric function

U μ ( x ) = ( 2 N ( μ ¯ μ ) μ ¯ ) μ ¯ 2 ( | x | μ ¯ μ ¯ μ μ ¯ + | x | μ ¯ + μ ¯ μ μ ¯ ) μ ¯ .

On the other hand, for any μ < μ ¯ , η 1 + η 2 > 0 , 0 η i < , α i , β i > 1 and α i + β i = 2 , i = 1 , 2 , by the Young and Sobolev inequalities, the following best constants are well defined on the space D = ( D 1 , 2 ( R N ) { 0 } ) 2 :

S η , β ( μ ) : = inf ( u , v ) D R N ( | u | 2 + | v | 2 μ | u | 2 + | v | 2 | x | 2 ) d x ( R N ( η 1 | u | α 1 | v | β 1 + η 2 | u | α 2 | v | β 2 ) d x ) 2 2 . (1.5)

We define

f ( τ ) : = 1 + τ 2 ( η 1 τ β 1 + η 2 τ β 2 ) 2 2 , τ > 0 . (1.6)

Since f is a continuous function on ( 0 , ) such that lim τ 0 + f ( τ ) = lim τ + f ( τ ) = + . Then there exists τ 0 > 0 such that

f ( τ 0 ) : = min τ > 0 f ( τ ) > 0 . (1.7)

Set α 1 = β 1 , α 2 = β 2 , σ 1 = σ 2 and u = v . Then (1.1) reduces to the semilinear scalar problems that have been extensively investigated by many authors. See [4-6] and the references therein.

Regular semilinear elliptic systems have been studied extensively and many conclusions have been established. For example, Alves et al. studied in [7] an elliptic system and some important conclusions had been obtained. However, the elliptic systems involving the Hardy inequality have seldom been studied and we only find some results in [8-16]. Thus it is necessary for us to investigate the related singular systems deeply. Among the references above, the elliptic systems involving the Hardy inequality and concave-convex nonlinearities had been studied only in [12]. In this paper, only the case 1 < q < 2 of (1.1) involving multiple strongly-coupled critical terms is considered.

Let | Ω | be the Lebesgue measure of Ω. We define the following constant:

ϒ 1 : = ( 2 q 2 2 Λ 1 q 2 | Ω | 1 q 2 ) 1 ( 2 q 2 q ( S η , β ( μ ) ) 2 2 ) 2 q 2 2 . (1.8)

Then the main results of this paper can be concluded in the following theorems and the conclusions are new to the best of our knowledge. It can be verified that the intervals in Theorems 1.1 and 1.2 for the parameters σ 1 , σ 2 , μ and q are allowable.

Theorem 1.1Suppose that (ℋ) holds and σ 1 + σ 2 < ϒ 1 . Then problem (1.1) has at least one positive solution.

Theorem 1.2Suppose that (ℋ) holds, N > 4 , μ < μ ¯ ( N q μ ¯ ) 2 and N N 2 < q < 2 . Then there exists ϒ 2 > 0 such that problem (1.1) has at least two positive solutions for all σ 1 and σ 2 satisfying σ 1 + σ 2 < ϒ 2 .

This paper is organized as follows. Some preliminary results and properties of the Nehari manifold are established in Sections 2 and 3, and Theorems 1.1 and 1.2 are proved in Section 4.

2 The local Palais-Smale condition

Throughout this paper, we always assume that the assumption (ℋ) holds, u H : = u μ = ( Ω ( | u | 2 μ | u | 2 | x | 2 ) d x ) 1 / 2 denotes the norm of the space H, by the Hardy inequality μ is equivalent to 0 , i.e.,

( 1 1 μ ¯ max ( μ , 0 ) ) 1 / 2 u 0 u μ ( 1 1 μ ¯ min ( μ , 0 ) ) 1 / 2 u 0 , u H .

Λ 1 denotes the first eigenvalue of the operator L, z = z H × H = ( u , v ) H × H = ( u H 2 + v H 2 ) 1 / 2 means the norm of the space E : = H 0 1 ( Ω ) × H 0 1 ( Ω ) , E 1 is the dual space of E. t z = t ( u , v ) = ( t u , t v ) for all z E and t R . z = ( u , v ) is said to be nonnegative in Ω if u 0 and v 0 in Ω. z = ( u , v ) is said to be positive in Ω if u > 0 and v > 0 in Ω. B r ( 0 ) = { x R N | x | < r } is a ball in R N . O ( ε t ) denotes a quantity satisfying | O ( ε t ) | / ε t C , o ( ε t ) means | o ( ε t ) | / ε t 0 as ε 0 and o ( 1 ) is a generic infinitesimal value. In particular, the quantity O 1 ( ε t ) means that there exist the constants C 1 , C 2 > 0 such that C 1 ε t O 1 ( ε t ) C 2 ε t as ε is small. We always denote positive constants as C and omit dx in integrals for convenience.

Lemma 2.1If { z n } E is a (PS)c-sequence ofJwith z n z inE, then J ( z ) = 0 and J ( z ) F ( τ 0 ( 1 ) , τ 0 ( 2 ) ) , where

Proof Let z n = ( u n , v n ) and z = ( u , v ) . Since { z n } is a (PS)c-sequence of J with z n z in E, we can deduce that J ( z ) = 0 , and therefore J ( z ) , z = 0 , that is,

Q ( z ) = z 2 K ( z ) .

Consequently,

J ( z ) = ( 1 2 1 2 ) z 2 ( 1 q 1 2 ) K ( z ) .

From the Hölder inequality it follows that

J ( z ) ( 1 2 1 2 ) z 2 ( 1 q 1 2 ) | Ω | 1 q 2 ( σ 1 ( Ω | u | 2 ) q 2 + σ 2 ( Ω | u | 2 ) q 2 ) 1 N z 2 2 q 2 q Λ 1 q 2 | Ω | 1 q 2 ( σ 1 u H q + σ 2 v H q ) F ( τ 0 ( 1 ) , τ 0 ( 2 ) ) .

Thus, the proof is complete. □

Lemma 2.2If { z n } E is a (PS)c-sequence of the functionalJ, then { z n } is bounded inE.

Proof See Hsu [[12], Lemma 2.2]. □

Lemma 2.3Suppose that (ℋ) holds. ThenJsatisfies the (PS)ccondition for all c < c , where

c = 1 N ( S η , β ( μ ) ) N 2 + F ( τ 0 ( 1 ) , τ 0 ( 2 ) ) . (2.1)

Proof We follow the argument in [15]. Let { z n } E be a (PS)c-sequence of J with c < c . Write z n = ( u n , v n ) . We know from Lemma 2.2 that { z n } is bounded in E, and then z n z = ( u , v ) up to a subsequence, z is a critical point of J. Furthermore, we may assume that u n u , v n v weakly in H and u n u , v n v strongly in L s ( Ω ) for all 1 s < 2 and u n u , v n v a.e. in Ω. Hence, we have that

J ( z ) = 0 and K ( z n ) = K ( z ) + o ( 1 ) . (2.2)

Set u ˜ n = u n u , v ˜ n = v n v and z ˜ n = ( u ˜ n , v ˜ n ) . From the Brézis-Lieb lemma [17] it follows that

z ˜ n 2 = z n 2 z 2 + o ( 1 ) , (2.3)

and by Lemma 2.1 in [18] we have

Ω | u ˜ n | α i | v ˜ n | β i = Ω | u n | α i | v n | β i Ω | u | α i | v | β i + o ( 1 ) , i = 1 , 2 . (2.4)

Since J ( z n ) = c + o ( 1 ) , J ( z n ) = o ( 1 ) and by (2.2) to (2.4), we can deduce that

1 2 z ˜ n 2 1 2 Q ( z ˜ n ) = c J ( z ) + o ( 1 ) (2.5)

and

z ˜ n 2 Q ( z ˜ n ) = o ( 1 ) .

Hence, we may assume that

lim n z ˜ n 2 = lim n Q ( z ˜ n ) = l . (2.6)

If l = 0 , the proof is complete. Assume l > 0 ; then from (2.6) and the definition of S η , β ( μ ) it follows that

S η , β ( μ ) l 2 2 = lim n S η , β ( μ ) ( Q ( z ˜ n ) ) 2 2 lim n z ˜ n 2 = l ,

which implies that

l ( S η , β ( μ ) ) N 2 . (2.7)

In addition, from (2.5) to (2.7) and Lemma 2.1, we get

c = ( 1 2 1 2 ) l + J ( z ) 1 N ( S η , β ( μ ) ) N 2 + F ( τ 0 ( 1 ) , τ 0 ( 2 ) ) = c ,

which is a contradiction. Therefore, the proof of Lemma 2.3 is complete. □

3 Nehari manifold

Since J is unbounded below on E, we need to consider J on the Nehari manifold

M σ = { z E { 0 } : J ( z ) , z = 0 } .

Thus, z M σ if and only if

J ( z ) , z = z 2 Q ( z ) K ( z ) = 0 . (3.1)

By the Hölder inequality and the definition of Λ 1 it follows that

K ( z ) ( σ 1 ( Ω | u | 2 ) q 2 + σ 2 ( Ω | v | 2 ) q 2 ) | Ω | 1 q 2 ( σ 1 ( u H ) q + σ 2 ( v H ) q ) Λ 1 q 2 | Ω | 1 q 2 ( σ 1 + σ 2 ) Λ 1 q 2 | Ω | 1 q 2 z q . (3.2)

Lemma 3.1The functionalJis coercive and bounded below on M σ .

Proof Suppose that z = ( u , v ) M σ . From (3.1) and (3.2) we get

J ( z ) = ( 1 2 1 2 ) z 2 ( 1 q 1 2 ) K ( z ) (3.3)

1 N z 2 ( 2 q 2 q ) ( σ 1 + σ 2 ) Λ 1 q 2 | Ω | 1 q 2 z q . (3.4)

Thus, J is coercive and bounded below on M σ . □

Define Φ ( z ) = J ( z ) , z . Then for all z = ( u , v ) M σ we have

Φ ( z ) , z = 2 z 2 2 Q ( z ) q K ( z ) = ( 2 q ) z 2 ( 2 q ) Q ( z ) (3.5)

= ( 2 2 ) z 2 + ( 2 q ) K ( z ) . (3.6)

We split M σ into three parts:

Lemma 3.2Suppose that z E is a local minimizer ofJon M σ and z M σ 0 . Then J ( z ) = 0 in E 1 .

Proof The proof is similar to that of [19] and the details are omitted. □

Lemma 3.3 M σ 0 = for all σ 1 + σ 2 ( 0 , ϒ 1 ) .

Proof We argue by contradiction. Suppose that there exist σ 1 , σ 2 > 0 such that 0 < σ 1 + σ 2 < ϒ 1 and M σ 0 . Then the fact z = ( u , v ) M σ 0 together with (3.5) and (3.6) imply that

z 2 = 2 q 2 q Q ( z ) , (3.7)

and

z 2 = 2 q 2 2 K ( z ) . (3.8)

By (1.5) and (3.7) we have

z 2 2 q 2 q ( S η , β ( μ ) ) 2 2 z 2 ,

which implies that

z ( 2 q 2 q ( S η , β ( μ ) ) 2 2 ) 1 2 2 . (3.9)

By (3.2) and (3.8) we have

z ( 2 q 2 2 Λ 1 q 2 | Ω | 1 q 2 ) 1 2 q ( σ 1 + σ 2 ) 1 2 q . (3.10)

From (3.9) and (3.10) it follows that

σ 1 + σ 2 ( 2 q 2 2 Λ 1 q 2 | Ω | 1 q 2 ) 1 ( 2 q 2 q ( S η , β ( μ ) ) 2 2 ) 2 q 2 2 = ϒ 1 ,

which is a contradiction. □

By Lemma 3.3, we write M σ = M σ + M σ and define

α σ = inf z M σ J ( z ) ; α σ ± = inf z M σ ± J ( z ) .

Lemma 3.4

(i) α σ α σ + < 0 for all σ 1 + σ 2 ( 0 , ϒ 1 ) .

(ii) There exists a positive constant d 0 depending on σ 1 , σ 2 , q, N, S η , β ( μ ) , Λ 1 and | Ω | such that α σ > d 0 for all σ 1 + σ 2 ( 0 , q 2 ϒ 1 ) .

Proof (i) Let z = ( u , v ) M σ + . By (3.1) and (3.6) it follows that

2 q 2 q z 2 > Q ( z ) . (3.11)

According to (3.1) and (3.11), we have that

J ( z ) = ( 1 2 1 q ) z 2 + ( 1 q 1 2 ) Q ( z ) < [ ( 1 2 1 q ) + ( 1 q 1 2 ) 2 q 2 q ] z 2 = 2 q q N z 2 < 0 ,

which implies that α σ α σ + < 0 .

(ii) Suppose that σ 1 + σ 2 ( 0 , q 2 ϒ 1 ) and z = ( u , v ) M σ . By (1.7), (3.1) and (3.5) we have that

2 q 2 q z < Q ( z ) ( S η , β ( μ ) ) 2 2 z 2 ,

which implies that

z > ( 2 q 2 q ) 1 2 2 ( S η , β ( μ ) ) 2 2 ( 2 2 ) . (3.12)

From (3.4) and (3.12) it follows that

J ( z ) z q ( 1 N z 2 q ( 2 q 2 q ) Λ 1 q 2 | Ω | 1 q 2 ( σ 1 + σ 2 ) ) d 0 ,

where d 0 = d 0 ( σ 1 , σ 2 , q , N , Λ 1 , S η , β ( μ ) , | Ω | ) is a positive constant. □

Lemma 3.5Suppose that σ 1 + σ 2 ( 0 , ϒ 1 ) and z E with Q ( z ) > 0 . Then there exist unique t + , t > 0 such that t + z M σ + and t z M σ . In particular, we have

t > t max : = ( ( 2 q ) z 2 ( 2 q ) Q ( z ) ) 1 2 2 > t + ,

J ( t + z ) = min 0 t t max J ( t z ) and J ( t z ) = max t t max J ( t z ) .

Proof The proof is similar to that of [20] and is omitted. □

For each z E with K ( z ) > 0 , we write

t ¯ max = ( ( 2 q ) K ( z ) ( 2 2 ) z 2 ) 1 2 q > 0 .

Then we have the following lemma.

Lemma 3.6Suppose that σ 1 + σ 2 ( 0 , ϒ 1 ) and z E { ( 0 , 0 ) } with K ( z ) > 0 . Then there exist unique 0 < t + < t ¯ max < t such that t + z M σ + , t z M σ and

J ( t + z ) = inf 0 t t ¯ max J ( t z ) ; J ( t z ) = sup t 0 J ( t z ) .

Proof The proof is almost the same as that in [[20], Lemma 2.7] and is omitted here. □

4 Proof of Theorems 1.1 and 1.2

Lemma 4.1

(i) If σ 1 + σ 2 ( 0 , ϒ 1 ) , then the functionalJhas a (PS)-sequence { z n } M σ .

(ii) If σ 1 + σ 2 ( 0 , q 2 ϒ 1 ) , then the functionalJhas a ( PS ) α σ -sequence { z n } M σ .

Proof The proof is similar to that of [21] and is omitted. □

Lemma 4.2Suppose that σ 1 + σ 2 ( 0 , ϒ 1 ) . ThenJhas a minimizer z ( 1 ) M σ + such that z ( 1 ) is a positive solution of (1.1) and J ( z ( 1 ) ) = α σ = α σ + < 0 .

Proof By Lemma 4.1(i), there exists a (PS)-sequence { z n } M σ of J such that

J ( z n ) = α σ + o ( 1 ) and J ( z n ) = o ( 1 ) in  E 1 . (4.1)

Since J is coercive on M σ (see Lemma 3.1), we get that { z n } is bounded in E. Passing to a subsequence (still denoted by { z n } ), we can assume that there exists z ( 1 ) = ( u ( 1 ) , v ( 1 ) ) E such that

{ u n u ( 1 ) , v n v ( 1 ) weakly in  H , u n u ( 1 ) , v n v ( 1 ) a.e. in  Ω , u n u ( 1 ) , v n v ( 1 ) strongly in  L s ( Ω )  for all  1 s < 2 , (4.2)

which implies that

K ( z n ) = K ( z ( 1 ) ) + o ( 1 ) as  n . (4.3)

First, we claim that z ( 1 ) is a solution of (1.1). By (4.1) and (4.2), it is easy to see that z ( 1 ) is a solution of (1.1). Furthermore, from { z n } M σ and (3.3), we deduce that

K ( z n ) = q ( 2 2 ) 2 ( 2 q ) z n 2 2 q 2 q J ( z n ) . (4.4)

Taking n in (4.4), by (4.1), (4.2) and the fact α σ < 0 , we get

K ( z ( 1 ) ) 2 q 2 q α σ > 0 .

Therefore, z ( 1 ) M σ is a nontrivial solution of (1.1).

Next, we prove that z n z ( 1 ) strongly in E and J ( z ( 1 ) ) = α σ . Noting z ( 1 ) M σ and applying the Fatou lemma, we have

α σ J ( z ( 1 ) ) = 1 N z ( 1 ) 2 2 q 2 q K ( z ( 1 ) ) lim inf n ( 1 N z n 2 2 q 2 q K ( z n ) ) = lim inf n J ( z n ) = α σ .

Therefore, J ( z ( 1 ) ) = α σ and lim n z n 2 = z ( 1 ) 2 . Set z ˜ n = z n z ( 1 ) . By the Brézis-Lieb lemma [17], we get

z ˜ n 2 = z n 2 z ( 1 ) 2 + o ( 1 ) .

Then standard argument shows that z n z ( 1 ) strongly in E. Moreover, we have z ( 1 ) M σ + . Otherwise, if z ( 1 ) M σ , then by Lemma 3.5 there exist unique t 0 ± such that t 0 ± z ( 1 ) M σ ± and t 0 + < t 0 = 1 . Since

d d t J ( t 0 + z ( 1 ) ) = 0 and d 2 d t 2 J ( t 0 + z ( 1 ) ) > 0 ,

there exists t ¯ ( t 0 + , t 0 ) such that J ( t 0 + z ( 1 ) ) < J ( t ¯ z ( 1 ) ) . By Lemma 3.5 we get that

J ( t 0 + z ( 1 ) ) < J ( t ¯ z ( 1 ) ) J ( t 0 z ( 1 ) ) = J ( z ( 1 ) ) ,

which is a contradiction. Since J ( z ( 1 ) ) = J ( | z ( 1 ) | ) and | z ( 1 ) | M σ + , by Lemma 3.2 we may assume that z ( 1 ) is a nontrivial nonnegative solution of (1.1).

In particular u ( 1 ) 0 , v ( 1 ) 0 . Indeed, without loss of generality, we may assume that v ( 1 ) 0 . Then as u ( 1 ) is a nontrivial nonnegative solution of

{ Δ u μ u | x | 2 = σ 1 | u | q 2 u in  Ω , u = 0 on  Ω ,

by the standard regularity theory, we have u ( 1 ) > 0 in Ω and

( u ( 1 ) , 0 ) 2 = K ( u ( 1 ) , 0 ) > 0 .

Moreover, we may choose w H 0 1 ( Ω ) { 0 } such that

( 0 , w ) 2 = K ( 0 , w ) > 0 .

Now,

K ( u ( 1 ) , w ) = K ( u ( 1 ) , 0 ) + K ( 0 , w ) > 0

and so by Lemma 3.6 there is unique 0 < t + < t ¯ max such that ( t + u ( 1 ) , t + w ) M σ + . Moreover,

t ¯ max = ( ( 2 q ) K ( u ( 1 ) , w ) ( 2 2 ) ( u ( 1 ) , w ) 2 ) = ( 2 q 2 2 ) 1 / ( 2 q ) > 1

and

J ( t + u ( 1 ) , t + w ) = inf 0 t t ¯ max J ( t u ( 1 ) , t w ) .

This implies

α σ + J ( t + u ( 1 ) , t + w ) J ( u ( 1 ) , w ) < J ( u ( 1 ) , 0 ) = α σ +

which is a contradiction.

Finally, from the maximum principle [22] we deduce that z ( 1 ) > 0 in Ω and z ( 1 ) is thus a positive solution of (1.1). □

Let V μ , ε ( x ) be defined as in (1.4) and set u ε ( x ) = ψ ( x ) V μ , ε ( x ) , where ψ ( x ) is a cut-off function:

ψ ( x ) D ( Ω ) : = { ψ C 0 ( Ω ) : ψ ( x ) 1  in a neighborhood of  x = 0 } .

The following results are already known.

Lemma 4.3[4]

As ε 0 we have the following estimates:

(4.5)

(4.6)

(4.7)

Lemma 4.4[11]

Suppose that (ℋ) holds, f ( τ ) is defined as in (1.6) and V μ , ε ( x ) are the minimizers of S ( μ ) defined as in (1.4). Then S η , β ( μ ) = f ( τ 0 ) S ( μ ) and has the minimizers ( V μ , ε ( x ) , τ 0 V μ , ε ( x ) ) , where f ( τ 0 ) : = min τ 0 f ( τ ) > 0 .

Lemma 4.5Under the assumptions of Theorem 1.2, there exist z ˜ E { 0 } and Λ > 0 such that for all σ 1 + σ 2 < Λ there holds

sup t 0 J ( t z ˜ ) < c = 1 N ( S η , β ( μ ) ) N 2 + F ( τ 0 ( 1 ) , τ 0 ( 2 ) ) . (4.8)

In particular, α σ < c for all σ 1 + σ 2 < Λ .

Proof For all t 0 , define the functions g 1 ( t ) : = J ( t u ε , t τ 0 u ε ) and

g 2 ( t ) : = t 2 2 ( 1 + ( τ 0 ) 2 ) u ε H 2 t 2 2 ( η 1 ( τ 0 ) β 1 + η 2 ( τ 0 ) β 2 ) Ω | u ε | 2 .

Note that lim t + g 2 ( t ) = and g 2 ( t ) > 0 as t is closed to 0. Thus, sup t 0 g 2 ( t ) is attained at some finite t ε > 0 with g 2 ( t ε ) = 0 . Furthermore, C < t ε < C , where C and C are the positive constants independent of ε.

Choose δ 1 > 0 small enough such that c > 0 for all σ 1 + σ 2 < δ 1 . Set z ε = ( u ε , τ 0 u ε ) . Then J ( t z ε ) t 2 2 z ε 2 for all t 0 and σ 1 , σ 2 > 0 , which implies that there exists t 0 ( 0 , 1 ) satisfying sup 0 t t 0 J ( t z ε ) < c , for all σ 1 + σ 2 < δ 1 . Note that

max t 0 ( t 2 2 B 1 t 2 2 B 2 ) = 1 N ( B 1 B 2 2 2 ) N 2 , B 1 , B 2 > 0 . (4.9)

From (4.9) and Lemmas 4.3, 4.4 it follows that

g 2 ( t ε ) 1 N ( ( 1 + ( τ 0 ) 2 ) u ε H 2 ( ( η 1 ( τ 0 ) β 1 + η 2 ( τ 0 ) β 2 ) Ω | u ε | 2 ) 2 2 ) N 2 1 N ( f ( τ 0 ) S ( μ ) N 2 + O ( ε 2 μ ¯ μ ) ( S ( μ ) N 2 + O ( ε 2 μ ¯ μ ) ) 2 2 ) N 2 1 N ( f ( τ 0 ) S ( μ ) ) N 2 + O ( ε 2 μ ¯ μ ) = 1 N ( S η , β ( μ ) ) N 2 + O ( ε 2 μ ¯ μ ) .

Consequently,

sup t t 0 g 1 ( t ) < sup t t 0 ( g 2 ( t ) t q q K ( z ε ) ) 1 N ( S η , β ( μ ) ) N 2 + O ( ε 2 μ ¯ μ ) t 0 q q ( σ 1 + ( τ 0 ) q σ 2 ) Ω | u ε | q 1 N ( S η , β ( μ ) ) N 2 + O ( ε 2 μ ¯ μ ) C ( σ 1 + σ 2 ) Ω | u ε | q 1 N ( S η , β ( μ ) ) N 2 + O ( ε 2 μ ¯ μ ) ( σ 1 + σ 2 ) O 1 ( ε N q μ ¯ )

and

( N q μ ¯ ) 2 q q < 2 μ ¯ μ ( N q μ ¯ ) ,

where we have used the assumption μ < μ ¯ ( N q μ ¯ ) 2 .

Therefore we can choose σ 1 = O 1 ( ε r 1 ) , σ 2 = O 1 ( ε r 2 ) such that

The definition of F ( τ 0 ( 1 ) , τ 0 ( 2 ) ) in Lemma 2.1 implies that

F ( τ 0 ( 1 ) , τ 0 ( 2 ) ) = O 1 ( ε 2 2 q min ( r 1 , r 2 ) ) .

Note that

Taking ε small enough, there exists δ 2 > 0 such that for all 0 < σ 1 + σ 2 < δ 2 ,

O ( ε 2 μ ¯ μ ) ( σ 1 + σ 2 ) O 1 ( ε N q μ ¯ ) < F ( τ 0 ( 1 ) , τ 0 ( 2 ) ) . (4.10)

Choose Λ = min { δ 1 , δ 2 } > 0 . Then for all σ 1 + σ 2 ( 0 , Λ ) there holds

sup t 0 J ( t z ε ) < c . (4.11)

Finally, we prove that α σ < c for all σ 1 + σ 2 < Λ . Recall that z ε = ( u ε , τ 0 u ε ) . By Lemma 3.5, the definition of α σ and (4.11), we can deduce that there exists t ˜ 0 > 0 such that t ˜ 0 z ε M σ and

α σ J ( t ˜ 0 z ε ) sup t 0 J ( t ˜ 0 z ε ) < c .

The proof is thus complete by taking z ˜ = z ε . □

Lemma 4.6Set ϒ 2 : = min { Λ , q 2 ϒ 1 } . Then for all σ 1 + σ 2 ( 0 , ϒ 2 ) , problem (1.1) has a positive solution z ( 2 ) such that z ( 2 ) M σ and J ( z ( 2 ) ) = α σ .

Proof By Lemma 4.1, there exists a (PS) α σ -sequence { z n } M σ of J for all σ 1 + σ 2 < q 2 ϒ 1 . From Lemmas 2.3, 3.4 and 4.5, it follows that α σ > 0 and J satisfies the (PS) α σ condition for all σ 1 + σ 2 < ϒ 2 . Since J is coercive on M σ , we get that { z n } is bounded in E. Therefore, there exist a subsequence (still denoted by { z n } ) and z ( 2 ) = ( u ( 2 ) , v ( 2 ) ) M σ such that z n z ( 2 ) strongly in E and J ( z ( 2 ) ) = α σ > 0 for all σ 1 + σ 2 < ϒ 2 . Since J ( z ( 2 ) ) = J ( | z ( 2 ) | ) and | z ( 2 ) | M σ , by Lemma 3.2 we may assume that z ( 2 ) is a nontrivial nonnegative solution of (1.1). Moreover, by (3.7) and z ( 2 ) = ( u ( 2 ) , v ( 2 ) ) M σ , we get

Q ( z ( 2 ) ) = 2 q 2 q z ( 2 ) 2 > 0 .

This implies that u ( 2 ) 0 and v ( 2 ) 0 . From the strong maximum principle [22] it follows that z ( 2 ) is a positive solution of (1.1). □

Proof of Theorems 1.1 and 1.2. By Lemma 4.2, we obtain that (1.1) has a positive solution z ( 1 ) M σ + for all σ 1 + σ 2 < ϒ 1 . On the other hand, from Lemma 4.6, we can get the second positive solution z ( 2 ) M σ for all σ 1 + σ 2 < ϒ 2 < ϒ 1 . Since M σ + M σ = , this implies that z ( 1 ) and z ( 2 ) are distinct. □

Competing interests

The author declares that he has no competing interests.

Acknowledgements

The author was grateful for the referee’s helpful suggestions and comments.

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