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Bubbles clustered inside for almost-critical problems

  • Mohamed Ben Ayed and Khalil El Mehdi EMAIL logo
Published/Copyright: June 5, 2025

Abstract

We investigate the existence of blowing-up solutions of the following almost-critical problem:

Δ u + V ( x ) u = u p ε , u > 0 in Ω , u = 0 on Ω ,

where Ω is a bounded regular domain in R n , n 4 , ε is a small positive parameter, p + 1 = ( 2 n ) ( n 2 ) is the critical Soblolev exponent, and the potential V is a smooth positive function. We find solutions that exhibit bubbles clustered inside as ε goes to zero. To the best of our knowledge, this is the first existence result for interior non-simple blowing-up positive solutions to Dirichlet problems in general domains. Our results are proven through delicate asymptotic estimates of the gradient of the associated Euler-Lagrange functional.

MSC 2010: 35A15; 35J20; 35J25

1 Introduction and main results

In this article, we study the following almost-critical problem:

(1) ( P V , ε ) : Δ u + V u = u p ε , in Ω , u > 0 , in Ω , u = 0 , on Ω ,

where Ω is a bounded regular domain in R n , n 4 , p + 1 = ( 2 n ) ( n 2 ) is the critical Sobolev exponent for the embedding H 0 1 ( Ω ) L q ( Ω ) , the potential V is a C 3 positive function on Ω ¯ , and ε is a small positive parameter.

The problem in the form of ( P V , ε ) arises in various physical models, such as quantum transport and non-relativistic Newtonian gravity, as detailed in [13] and their associated references. It is also connected to the Yamabe problem in differential geometry, as discussed, for example, in [4] and references therein.

In the critical case, where ε = 0 , it is well established that the existence of solutions to problem ( P V , ε ) is influenced by the geometry of the domain, the characteristics of the potential V , and the dimension n . For instance, when V is constant and the domain is star-shaped, there are no solutions to the given problem. Due to the vast amount of research on this subject, we will only mention the seminal works by Brezis and Nirenberg [5] and Bahri and Coron [6].

In the subcritical case where ε > 0 , proving the existence of a solution to the problem ( P V , ε ) is relatively simple. This can be shown by observing that the infimum

inf Ω ( u 2 + V u 2 ) : u H 0 1 ( Ω ) and Ω u p + 1 ε = 1

is achieved, thanks to the compactness of the embedding H 0 1 ( Ω ) L p + 1 ε ( Ω ) .

In [7], solutions of ( P V , ε ) were constructed that concentrate, as ε 0 , at interior blow-up points, forming isolated bubbles. By bubble here, we refer to the functions defined by

δ a , λ ( x ) c 0 λ ( n 2 ) 2 ( 1 + λ 2 x a 2 ) ( n 2 ) 2 , with c 0 [ n ( n 2 ) ] n 2 4 , a R n , λ > 0 ,

which are the only solutions to equation [8]

Δ u = u p , u > 0 in R n .

In this article, we focus on the construction of interior bubbling solutions of ( P V , ε ) with clustered bubbles at critical points of V . These solutions reveal a new phenomenon for positive solutions, namely, the existence of non-simple blow-up points in the interior for the subcritical problem with Dirichlet boundary conditions in general domains. This phenomenon has been observed for sign-changing solutions on certain symmetric domains [9], as well as for positive solutions on the ball [10]. It has also been noted in the setting of non-locally conformally compact Riemannian manifolds [11,12]. To the best of our knowledge, this is the first existence result for interior non-simple blowing-up positive solutions to Dirichlet problems in general domains.

In order to formulate our results, we need to introduce some notation. Let b be a non-degenerate critical point of V and N N , we define the following function:

(2) b , N ( z 1 , , z N ) i = 1 N D 2 V ( b ) ( z i , z i ) 1 j i N 1 z j z i n 2 .

The aim of our first result is to construct interior bubbling solutions with clustered bubbles at a critical point of V , Namely, we have

Theorem 1.1

Let n 4 , N 2 , and b Ω be a non-degenerate critical point of V. Assume that the function b , N has a non-degenerate critical point ( z ¯ 1 , , z ¯ N ) . Then, there exists a small positive real ε 0 such that for any ε ( 0 , ε 0 ] , problem ( P V , ε ) has a solution u ε , b with the following property:

u ε , b = i = 1 N α i , ε δ a i , ε , λ i , ε + v ε ,

with

(3) v ε < c ε ,

(4) α i , ε 1 ε ln 2 ε 1 i N ,

(5) 1 c ln σ n λ i , ε ε λ i , ε 2 c 1 i N ,

(6) a i , ε b + η ( ε ) σ z ¯ i η ( ε ) η 0 1 i N ,

where η 0 is a small positive constant, σ 4 = 1 , σ n = 0 for n 5 , c is a positive constant, η ( ε ) and σ are defined in (54).

In addition, if for each N, b , N has a non-degenerate critical point, then, problem ( P V , ε ) has an arbitrary number of non-constant distinct solutions, provided that ε is small.

Remark 1.2

  1. Note that for N = 1 , the existence of solution blowing up at a critical point of V with only one bubble has already been proved in [7].

  2. One can readily construct examples of potentials V for which the function b , N , defined in (2), possesses a non-degenerate critical point. For instance, let us fix a point b Ω , denote R = diam ( Ω ) , and choose a constant γ > 0 such that 2 n 1 γ n = n 2 . Define the points z ¯ 1 = ( γ , 0 ) R × R n 1 and z ¯ 2 = z ¯ 1 , and consider the potential function

    V ( x ) = R 2 1 2 ( x 1 b 1 ) 2 + 1 2 i = 2 n ( x i b i ) 2 .

    Then, the associated functional b , 2 , defined for z 1 = ( z 11 , z 12 ) , z 2 = ( z 21 , z 22 ) R × R n 1 , takes the form

    b , 2 ( z 1 , z 2 ) = z 11 2 z 21 2 + z 12 2 + z 22 2 2 ( ( z 11 z 21 ) 2 + z 12 z 22 2 ) n 2 2 .

    A straightforward computation shows that the point z ¯ = ( z ¯ 1 , z ¯ 2 ) is a non-degenerate critical point of b , 2 .

Our second result addresses the case of multiple interior blow-up points with clustered bubbles. More precisely, we prove:

Theorem 1.3

Let n 4 , b 1 , , b k Ω be non-degenerate critical points of V and N 1 , , N k be non-zero natural integers. For each i { 1 , , k } such that N i 2 , assume that the function b i , N i has a non-degenerate critical point ( z ¯ 1 i , , z ¯ N i i ) . Then, there exists a small positive real ε 0 such that for any ε ( 0 , ε 0 ] , problem ( P V , ε ) has a solution u ε , b 1 , , b k satisfying

u ε , b 1 , , b k = i = 1 N 1 α 1 , i , ε δ a 1 , i , ε , λ 1 , i , ε + + i = 1 N k α k , i , ε δ a k , i , ε , λ k , i , ε + v ε ,

with v ε c ε and for each l k the coefficients α l , i , ε , the speeds λ l , i , ε , and the points a l , i , ε satisfy the properties (4), (5), and (6), respectively.

The proof of our results relies on refined asymptotic estimates of the gradient of the associated Euler-Lagrange functional in the neighborhood of bubbles. The goal is to determine the equilibrium conditions satisfied by the concentration parameters. These balancing conditions are derived by testing the equation with vector fields that represent the dominant terms of the gradient relative to the concentration parameters. Analyzing these conditions provides all the necessary information to establish our results.

The rest of this article is organized as follows: in Section 2, we introduce the parameterization of the neighborhood of bubbles, provide a precise estimate of the infinite-dimensional part, and carry out a delicate asymptotic expansion of the gradient of the associated Euler-Lagrange functional. Section 3 is dedicated to proving our results. Finally, in Section 4, we present several estimates that are referenced throughout this article.

2 Analytical framework

Problem ( P V , ε ) has a variational structure, and its Euler-Lagrange functional is defined on H 0 1 ( Ω ) by

(7) I V , ε ( u ) 1 2 Ω u 2 + 1 2 Ω V u 2 1 p + 1 ε Ω u p + 1 ε with p n + 2 n 2 .

In the sequel, we will use the following scalar product and its corresponding norm defined by

(8) v , w Ω v w + Ω V v w ; w 2 Ω w 2 + Ω V w 2 .

Note that, since V is a C 0 -positive function on Ω ¯ , we deduce that this norm is equivalent to the two norms 0 and 1 of H 0 1 ( Ω ) and H 1 ( Ω ) , respectively.

We start by giving some estimates concerning the approximate solutions for ( P V , ε ) . For a Ω and λ > 0 , let π δ a , λ the projection defined by

Δ π δ a , λ + V π δ a , λ = δ a , λ n + 2 n 2 , in Ω , π δ a , λ = 0 , on Ω ,

and

θ a , λ δ a , λ π δ a , λ .

These functions are introduced in [7], and they satisfy, for n 4 ,

(9) 0 π δ a , λ δ a , λ ; λ π δ a , λ λ n + 2 2 π δ a , λ ; 1 λ π δ a , λ a j n + 2 2 π δ a , λ , in Ω ,

(10) 0 θ a , λ δ a , λ ; λ θ a , λ λ n 2 2 θ a , λ ; 1 λ θ a , λ a j n 2 2 θ a , λ , in Ω ,

(11) θ a , λ c R a , λ 1 δ a , λ ; 1 λ θ a , λ a j c R a , λ 2 δ a , λ , in Ω 0 { x Ω : d ( x , Ω ) d 0 } ,

(12) with R a , λ 1 ( x ) ln σ n ( λ ) λ 2 + x a 2 ln x a σ n ; R a , λ 2 ( x ) λ 2 + λ 1 x a ,

where d 0 is any fixed small positive constant, σ 4 1 , σ n 0 for n 5 , and a j is the j th-component of a .

For the proof of these facts, the interested reader is referred to [7].

Now, we introduce the parameterization of the neighborhood of bubbles. Let N N and μ > 0 be a small real. We define the following set:

(13) O ( N , μ ) { ( α , a , λ ) ( 0 , ) N × Ω N × ( μ 1 , ) N : α i 1 < μ ; d ( a i , Ω ) > 2 d 0 ; ε ln λ i < μ ; i and ε i j < μ i j } ,

where ε i j is defined by

(14) ε i j λ i λ j + λ j λ i + λ i λ j a i a j 2 ( 2 n ) 2 .

Observe that, since Ω is bounded, for each b Ω and λ > 0 satisfying ε ln λ is small, it follows that

(15) δ b , λ ε = c 0 ε λ ε ( n 2 ) 2 1 + n 2 2 ε ln ( 1 + λ 2 x b 2 ) + O ( ε 2 ln 2 ( 1 + λ 2 x b 2 ) ) = 1 + o ( 1 ) .

For each ( α , a , λ ) O ( N , μ ) and v E a , λ , we associate a function

(16) u i = 1 N α i ( π δ a i , λ i ) + v u ̲ + v , where

(17) E a , λ span π δ a i , λ i , ( π δ a i , λ i ) λ i , ( π δ a i , λ i ) a i , j , i { 1 , , N } , j { 1 , , n } .

We note that the orthogonality is taken with respect to the scalar product defined in (8).

In the sequel, we need to study the functional I V , ε and to find some positive critical points u having form (16). We start by studying the v -part of u .

2.1 Estimate of the infinite-dimensional part

Let ( α , a , λ ) O ( N , μ ) , v E a , λ and u be defined in (16). In this section, we are going to study the v -part of u . To this aim, we need to expand I V , ε with respect to v .

Observe that, for b 1 , b 2 R , and γ > 2 , it holds

(18) b 1 + b 2 γ b 1 γ γ b 1 γ 2 b 1 b 2 1 2 γ ( γ 1 ) b 1 γ 2 b 2 2 c b 1 γ 3 b 2 3 + c b 2 γ , if γ > 3 , c b 2 γ , if γ 3 .

Thus, using the fact that v , u ̲ = 0 , we obtain

(19) I V , ε ( u ) = I V , ε ( u ̲ ) f ε ( v ) + 1 2 Q ε ( v ) + o ( v 2 ) , where

(20) f ε ( v ) Ω ( u ̲ ) p ε v and Q ε ( v ) v 2 ( p ε ) Ω ( u ̲ ) p ε 1 v 2 .

Note that Q ε is a positive definite quadratic form (see Proposition 3.1 of [7]) and the linear form f ε satisfies:

Lemma 2.1

Let ( α , a , λ ) O ( N , μ ) . Then, for each v E a , λ , we have

f ε ( v ) c v ε + 1 i N T 2 ( λ i ) + i j T 3 ( ε i j ) , w h e r e T 2 ( λ ) ( λ 2 i f n 5 ; λ 2 ln λ i f n = 4 ; λ 1 i f n = 3 ) , T 3 ( t ) ( t ( n + 2 ) ( 2 ( n 2 ) ) ( ln t 1 ) ( n + 2 ) 2 n if n 6 , t if n 5 ) .

Proof

First, observe that, for β i > 0 and γ > 1 , it holds

(21) i = 1 N β i γ i = 1 N β i γ c i j ( β i β j ) γ 2 , if γ 2 , c i j β i γ 1 β j , if γ > 2 .

Thus, we obtain

(22) f ε ( v ) = i = 1 N α i p ε Ω ( π δ a i , λ i ) p ε v + i j O Ω [ ( π δ a i , λ i ) ( π δ a j , λ j ) ] p ε 2 v , if n 6 , O Ω ( π δ a i , λ i ) p ε 1 ( π δ a j , λ j ) v , if n 5 .

Observe that, using (9) and (15), we obtain

(23) Ω [ ( π δ a i , λ i ) ( π δ a j , λ j ) ] p ε 2 v Ω ( δ a i , λ i δ a j , λ j ) p 2 v Ω ( δ a i , λ i δ a j , λ j ) n n 2 ( n + 2 ) 2 n Ω v 2 n n 2 ( n 2 ) ( 2 n ) .

Note that estimate (E2) of [13] gives us

(24) R n ( δ a i , λ i δ a j , λ j ) n ( n 2 ) c ε i j n n 2 ln ( ε i j 1 ) ,

and using the embedding theorem of H 0 1 ( Ω ) L 2 n n 2 ( Ω ) , we derive that

(25) Ω [ ( π δ a i , λ i ) ( π δ a j , λ j ) ] p ε 2 v c ε i j n + 2 2 ( n 2 ) ( ln ε i j 1 ) n + 2 2 n v .

In the same way, for n 5 (which implies p 1 4 n 2 > 1 ), using Lemma 2.2 of [14], we have

(26) Ω ( π δ a i , λ i ) p ε 1 ( π δ a j , λ j ) v Ω δ a i , λ i p 1 δ a j , λ j v c v Ω δ a i , λ i ( p 1 ) 2 n n + 2 δ a j , λ j 2 n n + 2 n + 2 2 n c v ε i j .

It remains to estimate the first integral in (22). Observe that, for 0 < b 2 < b 1 and γ > 1 , it holds

(27) ( b 1 b 2 ) γ = b 1 γ + O ( b 1 γ 1 b 2 ) .

Thus, we obtain

Ω ( π δ a i , λ i ) p ε v = Ω ( δ a i , λ i θ a i , λ i ) p ε v = Ω δ a i , λ i p ε v + O Ω δ a i , λ i 4 n 2 ε θ a i , λ i v .

The last integral can be deduced following the proof of Lemma 6.5 of [7] by using (15) and we obtain

(28) Ω δ a , λ 4 n 2 ε θ a , λ v c Ω δ a , λ 4 ( n 2 ) θ a , λ v c v T 2 ( λ ) .

For the other one, using (15), and the fact that v π δ a i , λ i , we obtain

(29) Ω δ a i , λ i p ε v = c 0 ε λ i ε n 2 2 Ω δ a i , λ i p v + O ε Ω δ a i , λ i p ln ( 1 + λ i 2 x a i 2 ) v = O ε v Ω δ a i , λ i 2 n n 2 ln 2 n n + 2 ( 1 + λ i 2 x a i 2 ) n + 2 2 n = O ( ε v ) .

Thus, (28) and (29) imply that

(30) Ω ( π δ a i , λ i ) p ε v = O ( ε v + v T 2 ( λ i ) ) .

Substituting (30), (26), and (25) into (22), the result follows.□

Combining (19), Lemma 2.1, and the fact that Q ε is a positive definite quadratic form, we deduce that

Proposition 2.2

Let ( α , a , λ ) O ( N , μ ) and u ̲ i = 1 N α i π δ a i , λ i . Then, for ε small, there exists a unique v ¯ E a , λ satisfying:

(31) I V , ε ( u ̲ + v ¯ ) , h = 0 h E a , λ .

Moreover, v ¯ satisfies

v ¯ c R v ( a , λ ) , w i t h R v ( a , λ ) ε + i j T 3 ( ε i j ) + 1 i N T 2 ( λ i ) ,

where T 2 and T 3 are defined in Lemma 2.1.

2.2 Expansion of the gradient of the associated functional

In this section, we will provide asymptotic expansions of the gradient of functional I V , ε . We begin with the expansion with respect to the gluing parameter α s , specifically proving:

Proposition 2.3

Let ( α , a , λ ) O ( N , μ ) , v E a , λ , and u = i = 1 N α i π δ a i , λ i + v . Then, for ε small and i { 1 , , N } , we have:

I V , ε ( u ) , π δ a i , λ i = α i S n ( 1 α i p 1 ε λ i ε ( n 2 ) 2 ) + O ( R α i ) ,

where

S n R n δ 0,1 2 n ( n 2 ) , R α i ε + T 2 ( λ i ) + v 2 + i j ε i j

and T 2 is defined in Lemma 2.1.

Proof

Observe that, since v E a , λ , it holds

(32) I V , ε , π δ a i , λ i = j = 1 N α j π δ a j , λ j , π δ a i , λ i Ω u p 1 ε u π δ a i , λ i .

First, for j i , we have

(33) π δ a j , λ j , π δ a i , λ i = Ω ( π δ a j , λ j ) ( π δ a i , λ i ) + Ω V ( π δ a j , λ j ) ( π δ a i , λ i ) = Ω ( Δ + V ) ( π δ a j , λ j ) ( π δ a i , λ i ) Ω δ a j , λ j n + 2 n 2 δ a i , λ i c ε i j ,

using Estimate (E1) of [13]. Second, for j = i , as in the previous computation, we have

π δ a i , λ i 2 = Ω δ a i , λ i n + 2 n 2 ( π δ a i , λ i ) = Ω δ a i , λ i 2 n n 2 Ω δ a i , λ i n + 2 n 2 θ a i , λ i .

The estimate of the first integral is well known and we have

Ω δ a i , λ i 2 n n 2 = S n + O 1 λ i n .

For the second integral, let B i B ( a i , d 0 ) , using (10) and (11), easy computations imply that

(34) Ω δ a i , λ i n + 2 n 2 θ a i , λ i c B i R 1 ( x , a i , λ i ) δ a i , λ i 2 n n 2 + Ω \ B i δ a i , λ i 2 n n 2 c T 2 ( λ i ) + c λ i n c T 2 ( λ i ) .

Thus, we deduce that

(35) π δ a i , λ i 2 = S n + O ( λ 2 , if n 5 ; λ 2 ln λ , if n = 4 ; λ 1 , if n = 3 ) .

Now, we focus on the last term in (32). Observe that, for b 1 , b 2 , z R such that z β b 1 for some positive constant β and γ > 0 , it holds

(36) b 1 + b 2 γ 1 ( b 1 + b 2 ) z = b 1 γ 1 b 1 z + γ b 1 γ 1 b 2 z + O ( b 1 γ 1 b 2 2 + b 2 γ + 1 ) ,

(37) b 1 + b 2 γ = b 1 γ + O ( b 1 γ 1 b 2 + b 2 γ ) .

Thus, let u ̲ j = 1 N α j ( π δ a j , λ j ) ; using (36), we obtain

(38) Ω u p ε 1 u ( π δ a i , λ i ) = Ω ( u ̲ ) p ε ( π δ a i , λ i ) + ( p ε ) Ω ( u ̲ ) p ε 1 v ( π δ a i , λ i ) + O ( v 2 ) .

The first integral in the right-hand side of (38) can be written as (using (37), (27), and (9))

Ω ( u ̲ ) p ε ( π δ a i , λ i ) = α i p ε Ω ( π δ a i , λ i ) p + 1 ε + j i O Ω δ a i , λ i p ε δ a j , λ j + Ω δ a j , λ j p ε δ a i , λ i = α i p ε Ω δ a i , λ i p + 1 ε + O Ω δ a i , λ i p ε θ a i , λ i + j i Ω δ a i , λ i p δ a j , λ j + Ω δ a j , λ j p δ a i , λ i = α i p ε c 0 ε λ i ε ( n 2 ) 2 S n + O ε + 1 λ i n + T 2 ( λ i ) + i j ε i j ,

where we have used ( 64 ) of [15], (34), and the last inequality in (33). Concerning the second integral in (38), it is computed in Lemma A.2.

Combining the previous estimates, the proof follows.□

We will now present a balancing formula that involves the rate of concentration λ i and the self-interaction of the bubbles ε i j . Specifically, we prove:

Proposition 2.4

Let n 4 , ( α , a , λ ) O ( N , μ ) , v E a , λ , and u = j = 1 N α j π δ a j , λ j + v . For ε small and i { 1 , , N } , we have

I V , ε ( u ) , λ i ( π δ a i , λ i ) λ i = j i α j c ¯ 2 λ i ε i j λ i ( 1 α i p 1 ε λ i ε ( n 2 ) 2 α j p 1 ε λ j ε ( n 2 ) 2 ) + c 0 ε λ i ε n 2 2 c 2 α i p ε ε c ( n ) α i ln σ n ( λ i ) λ i 2 V ( a i ) 2 α i p ε 1 c 0 ε λ i ε n 2 2 1 + O ( R λ i ) ,

where

c ( 4 ) c 0 2 mes ( S 3 ) , c ( n ) n 2 2 c 0 2 R n x 2 1 ( 1 + x 2 ) n 1 d x > 0 i f n 5 , c 2 n 2 2 2 c 0 2 n n 2 R n ( x 2 1 ) ( 1 + x 2 ) n + 1 ln ( 1 + x 2 ) d x > 0 , c ¯ 2 c 0 2 n n 2 R n 1 ( 1 + x 2 ) ( n + 2 ) 2 d x , R λ i ε 2 + v 2 + 1 λ i n 2 + 1 λ i 4 + ( i f n = 6 ) ln λ i λ i 4 + k j ε k j n n 2 ln ( ε k j 1 ) + j i 1 ( λ j λ i ) ( n 2 ) 2 + ε i j Ξ i j + 1 λ j 3 2 + 1 λ i 3 2

and where Ξ i j is defined in Lemma A.3.

Proof

We will follow the proof of Proposition 2.3, and we need to be more precise in some integrals. Since v E a , λ , we have

u , λ i ( π δ a i , λ i ) λ i = α j π δ a j , λ j , λ i ( π δ a i , λ i ) λ i .

First, for j = i , using Lemma 6.3 of [7], we obtain

(39) π δ a i , λ i , λ i ( π δ a i , λ i ) λ i = Ω δ a i , λ i n + 2 n 2 λ i δ a i , λ i λ i λ i θ a i , λ i λ i = c ( n ) ln σ n λ i λ i 2 V ( a i ) + O 1 λ i n 2 + 1 λ i 4 + ( if n = 6 ) ln λ i λ i 4 .

Second, for j i , we have

(40) π δ a j , λ j , λ i ( π δ a i , λ i ) λ i = Ω δ a j , λ j n + 2 n 2 λ i δ a i , λ i λ i λ i θ a i , λ i λ i .

Observe that, using Estimate F16 of [13] and the fact that d ( a k , Ω ) c > 0 for k { i , j } , we deduce that

Ω δ a j , λ j n + 2 n 2 λ i δ a i , λ i λ i = c ¯ 2 λ i ε i j λ i + O ε i j n n 2 ln ( ε i j 1 ) + 1 λ j ( n + 2 ) 2 λ i ( n 2 ) 2 .

Furthermore, using Lemma A.3, equation (40) becomes

(41) π δ a j , λ j , λ i ( π δ a i , λ i ) λ i = c ¯ 2 λ i ε i j λ i + O ε i j n n 2 ln ( ε i j 1 ) + 1 ( λ j λ i ) ( n 2 ) 2 + Ξ i j ε i j .

Thus, we derive that

(42) u , λ i ( π δ a i , λ i ) λ i = α i c ( n ) ln σ n λ i λ i 2 V ( a i ) + c ¯ 2 j i α j λ i ε i j λ i + O 1 λ i n 2 + 1 λ i 4 + ( if n = 6 ) ln λ i λ i 4 + j i O ε i j n n 2 ln ( ε i j 1 ) + 1 ( λ j λ i ) ( n 2 ) 2 + ε i j Ξ i j .

Now, using (36), we obtain

(43) Ω u p ε 1 u λ i ( π δ a i , λ i ) λ i = Ω ( u ̲ ) p ε λ i ( π δ a i , λ i ) λ i + ( p ε ) Ω ( u ̲ ) p ε 1 v λ i ( π δ a i , λ i ) λ i + O ( v 2 ) .

The last integral is computed in Lemma A.2. For the first one, we need the following formula. Let 1 < γ 3 , b j > 0 for j { 1 , , N } , and s be such that s c b i for some index i . Then, it holds

(44) j = 1 N b j γ s = j = 1 N b j γ s + γ b i γ 1 j i b j s + k j O ( ( b k b j ) ( γ + 1 ) 2 ) .

Thus, we obtain

(45) Ω ( u ̲ ) p ε λ i ( π δ a i , λ i ) λ i = 1 j N α j p ε Ω ( π δ a j , λ j ) p ε λ i ( π δ a i , λ i ) λ i + ( p ε ) j i Ω ( α i π δ a i , λ i ) p ε 1 ( α j π δ a j , λ j ) λ i ( π δ a i , λ i ) λ i + j k O Ω ( δ a j , λ j δ a k , λ k ) n n 2 .

First, we remark that the remainder term is computed in (24). Second, the first integral, with j = i , is computed in [7] (see equation (45)) and we have

(46) Ω ( π δ a i , λ i ) p ε λ i ( π δ a i , λ i ) λ i = c 0 ε λ i ε n 2 2 c 2 ε + 2 c ( n ) ln σ n λ i λ i 2 + O ε 2 + 1 λ i n 2 + 1 λ i 4 + ( if n = 6 ) ln λ i λ i 4 .

Third, we focus on estimating the first integral of (45) with j i . Using (27), (9), and (15), we deduce that

Ω ( π δ a j , λ j ) p ε λ i ( π δ a i , λ i ) λ i = Ω ( δ a j , λ j p ε + O ( δ a j , λ j p 1 θ a j , λ j ) ) λ i π δ a i , λ i λ i = c 0 ε λ j ε ( n 2 ) 2 Ω δ a j , λ j p λ i π δ a i , λ i λ i + O Ω θ a j , λ j δ a j , λ j p 1 δ a i , λ i + ε Ω δ a j , λ j p ln ( 1 + λ j 2 x a j 2 ) δ a i , λ i .

Observe that, let B j B ( a j , d 0 ) , we have

(47) Ω δ a j , λ j p 1 θ a j , λ j δ a i , λ i c B j R 1 ( x , a j , λ j ) δ a j , λ j p δ a i , λ i + c λ j ( n + 2 ) 2 δ a i , λ i c ln σ n λ j λ j 2 B j δ a j , λ j p δ a i , λ i + B j x a j 2 ln x a j σ n δ a j , λ j p δ a i , λ i + c λ j ( n + 2 ) 2 δ a i , λ i .

Using Holder’s inequality and Lemma 2.2 of [14], we deduce that

B j x a j 2 ln σ n x a j δ a j , λ j p δ a i , λ i c λ j 3 2 B j ln x a j σ n x a j δ a j , λ j n 1 n 2 δ a i , λ i c λ j 3 2 B j ln x a j ( n 1 ) σ n x a j n 1 1 ( n 1 ) B j δ a j , λ j n 1 n 2 2 δ a i , λ i n 1 n 2 ( n 2 ) ( n 1 ) c λ j 3 2 ε i j .

Thus, (47) becomes

(48) Ω δ a j , λ j p 1 θ a j , λ j δ a i , λ i c λ j 3 2 ε i j + c λ i ( n 2 ) 2 λ j ( n + 2 ) 2 .

Hence, we obtain

Ω ( π δ a j , λ j ) p ε λ i ( π δ a i , λ i ) λ i = c 0 ε λ j ε n 2 2 π δ a j , λ j , λ i ( π δ a i , λ i ) λ i + O 1 λ i ( n 2 ) 2 λ j ( n + 2 ) 2 + ε i j ε + 1 λ j 3 2 .

In the same way, we deduce the estimate of the second integral of (45), and we obtain

p Ω ( π δ a i , λ i ) p ε 1 λ i ( π δ a i , λ i ) λ i π δ a j , λ j = c 0 ε λ i ε n 2 2 π δ a j , λ j , λ i ( π δ a i , λ i ) λ i + O 1 λ j ( n 2 ) 2 λ i ( n + 2 ) 2 + ε i j ε + 1 λ i 3 2 .

Finally, combining (42), (43), (45), (41), (46), and Lemma A.2, the result follows.□

Next, we present a balancing condition that involves the concentration points.

Proposition 2.5

Let n 4 , ( α , a , λ ) O ( N , μ ) , v E a , λ , and u = j = 1 N α j ( π δ a j , λ j ) + v . For ε small and i { 1 , , N } , we have

I V , ε ( u ) , 1 λ i ( π δ a i , λ i ) a i = c 2 ( n ) α i ln σ n ( λ i ) λ i 3 V ( a i ) 2 α i p ε 1 c 0 ε λ i ε n 2 2 1 + c ¯ 2 j i α j 1 λ i ε i j a i 1 c 0 ε λ i ε n 2 2 α i p ε 1 c 0 ε λ i ε n 2 2 α j p ε 1 + O ( R a i ) ,

with

R a i j i λ j a i a j ε i j n + 1 n 2 + v 2 + 1 λ i 4 + ( i f n = 5 ) ln λ i λ i 4 + 1 λ k n 1 + k j ε k j n ( n 2 ) ln ε k j 1 + ε i j ε + 1 λ i + 1 λ j 3 2 + ε ln σ n λ i λ i 2 ,

where

c 2 ( 4 ) 1 2 c 0 2 meas ( S 3 ) a n d c 2 ( n ) n 2 n c 0 2 R n x 2 ( 1 + x 2 ) n 1 , i f n 5 .

Proof

We will follow the proof of Proposition 2.4. Since v E a , λ , we have

u , 1 λ i ( π δ a i , λ i ) a i = α j π δ a j , λ j , 1 λ i ( π δ a i , λ i ) a i .

First, the scalar product, with j = i , is computed in [7] and we have

(49) π δ a i , λ i , 1 λ i ( π δ a i , λ i ) a i = c 2 ( n ) ln σ n λ i λ i 3 V ( a i ) + O 1 λ i n 1 + 1 λ i 4 + ( if n = 5 ) ln λ i λ i 4 .

Second, for j i , using (11) and (12), the last inequality in (33) and (F11) of [13], we obtain

(50) π δ a j , λ j , 1 λ i ( π δ a i , λ i ) a i = Ω δ a j , λ j n + 2 n 2 1 λ i δ a i , λ i a i 1 λ i θ a i , λ i a i = R n δ a j , λ j n + 2 n 2 1 λ i δ a i , λ i a i + O 1 λ j ( n + 2 ) 2 λ i n 2 + 1 λ i Ω δ a j , λ j n + 2 n 2 δ a i , λ i = c ¯ 2 1 λ i ε i j a i + O λ j a i a j ε i j n + 1 n 2 + 1 λ i ε i j + 1 λ i n 2 λ j ( n + 2 ) 2 .

Thus, we derive that

(51) u , 1 λ i ( π δ a i , λ i ) a i = α i c 2 ( n ) ln σ n λ i λ i 3 V ( a i ) + c ¯ 2 α j 1 λ i ε i j a i + O j i λ j a i a j ε i j n + 1 n 2 + 1 λ i ε i j + 1 λ i n 2 λ j ( n + 2 ) 2 + 1 λ i n 1 + 1 λ i 4 + ( if n = 5 ) ln λ i λ i 4 .

Now, note that (43) and (45) hold true with λ i 1 ( π δ a i , λ i ) a i instead of λ i ( π δ a i , λ i ) λ i . Furthermore, equation (53) of [7] implies that

(52) Ω ( π δ a i , λ i ) p ε 1 λ i ( π δ a i , λ i ) a i = 2 c 2 ( n ) c 0 ε λ i ε n 2 2 ln σ n λ i λ i 3 V ( a i ) + O 1 λ i n 1 + 1 λ i 4 + ( if n = 5 ) ln λ i λ i 4 + ε ln σ n λ i λ i 2 .

In addition, for j i , using (27), (9), (48), and (15), we deduce that

Ω ( π δ a j , λ j ) p ε 1 λ i ( π δ a i , λ i ) a i = Ω ( δ a j , λ j p ε + O ( δ a j , λ j p 1 θ a j , λ j ) ) 1 λ i π δ a i , λ i a i = c 0 ε λ j ε n 2 2 Ω δ a j , λ j p 1 λ i π δ a i , λ i a i + O Ω θ a j , λ j δ a j , λ j p 1 δ a i , λ i + ε Ω δ a j , λ j p ln ( 1 + λ j 2 x a j 2 ) δ a i , λ i = c 0 ε λ j ε n 2 2 π δ a j , λ j , 1 λ i ( π δ a i , λ i ) a i + O 1 λ i ( n 2 ) 2 λ j ( n + 2 ) 2 + ε i j ε + 1 λ j 3 2 .

In the same way, we obtain

p Ω ( π δ a i , λ i ) p ε 1 1 λ i ( π δ a i , λ i ) a i π δ a j , λ j = c 0 ε λ i ε n 2 2 π δ a j , λ j , 1 λ i ( π δ a i , λ i ) a i + O 1 λ j ( n 2 ) 2 λ i ( n + 2 ) 2 + ε i j ε + 1 λ i 3 2 .

Combining the previous estimates, the result follows.□

3 Interior blowing-up solutions with clustered bubbles

This section is devoted to the proof of Theorems 1.1 and 1.3. We start by proving Theorem 1.1. The proof structure adopts a method comparable to the one presented in [1517]. Let n 4 , b Ω be a non-degenerate critical point of V and ( z ¯ 1 , , z ¯ N ) be a non-degenerate critical point of F b , N , where F b , N is defined by (2). We start by introducing a parameterization of the neighborhood of the desired constructed solutions. Let

(53) O 1 ( N , b , ε ) = { ( α , λ , a , v ) ( R + ) N × ( R + ) N × Ω N × H 1 ( Ω ) : v E a , λ , v < ε , α i 1 < ε ln 2 ε , 1 c < ln σ n ( λ i ) λ i 2 ε < c , a i b η ( ε ) σ z ¯ i η ( ε ) η 0 1 i N ,

where η 0 is a small constant, σ 4 = 1 , σ n = 0 for n 5 , E a , λ is defined by (17),

(54) η ( ε ) ε γ if n 5 ln ε 1 4 if n = 4 , γ = n 4 2 n and σ = c ¯ 2 c 2 ( n ) 1 n c 2 c ( n ) V ( b ) γ

with c 2 , c ¯ 2 , c 2 ( n ) , and c ( n ) are the constants defined in Propositions 2.4 and 2.5.

In addition, we consider the following function:

ψ ε : O 1 ( N , b , ε ) R , ( α , λ , a , v ) ψ ε ( α , λ , a , v ) = I V , ε i = 1 N α i π δ a i , λ i + v .

We note that ( α , λ , a , v ) is a critical point of ψ ε if and only if u = i = 1 N α i π δ a i , λ i + v is a critical point of I V , ε . Thus, we need to look for critical points of ψ ε . Since the variable v belongs to E a , λ , the Lagrange multiplier theorem allows us to obtain the following proposition.

Proposition 3.1

( α , λ , a , v ) O 1 ( N , b , ε ) is a critical point of ψ ε if and only if there exists ( A , B , C ) R N × R N × ( R n ) N such that the following holds:

(55) ψ ε α i ( α , λ , a , v ) = 0 i { 1 , , N } ,

(56) ψ ε λ i ( α , λ , a , v ) = B i v , λ i 2 ( π δ a i , λ i ) λ i 2 + j = 1 n C i j v , 1 λ i 2 ( π δ a i , λ i ) λ i a i j i { 1 , , N } ,

(57) ψ ε a i ( α , λ , a , v ) = B i v , λ i 2 ( π δ a i , λ i ) λ i a i + j = 1 n C i j v , 1 λ i 2 ( π δ a i , λ i ) a i j a i i { 1 , , N } ,

(58) ψ ε v ( α , λ , a , v ) = k = 1 N A k π δ a k , λ k + B k λ k ( π δ a k , λ k ) λ k + j = 1 n C k j 1 λ k ( π δ a k , λ k ) a k j .

To prove Theorem 1.1, we will make a careful study of the previous equations. Note that

(59) ψ ε α i ( α , λ , a , v ) = I V , ε i = 1 N α i π δ a i , λ i + v , π δ a i , λ i ,

(60) ψ ε λ i ( α , λ , a , v ) = I V , ε i = 1 N α i π δ a i , λ i + v , α i ( π δ a i , λ i ) λ i ,

(61) ψ ε a i ( α , λ , a , v ) = I V , ε i = 1 N α i π δ a i , λ i + v , α i ( π δ a i , λ i ) a i ,

(62) ψ ε v ( α , λ , a , v ) = I V , ε i = 1 N α i π δ a i , λ i + v .

Let ( α , λ , a , 0 ) O 1 ( N , b , ε ) , which is defined by (53). We are going to solve the system defined by equations (55)–(58). The strategy of the proof of Theorem 1.1 is to reduce the problem to a finite-dimensional system. Proposition 2.2 allows us to obtain such a reduction by finding v ¯ verifying equation (58). Combining equations (55), …, (62), we see that u = i = 1 N α i π δ a i , λ i + v ¯ is a critical point of I V , ε if and only if ( α , λ , a ) solves the following system: for each 1 i N ,

(63) ( E α i ) I V , ε ( u ) , π δ a i , λ i = 0 ,

(64) ( E λ i ) I V , ε ( u ) , α i ( π δ a i , λ i ) λ i = B i v ¯ , λ i 2 ( π δ a i , λ i ) λ i 2 + j = 1 n C i j v ¯ , 1 λ i 2 ( π δ a i , λ i ) λ i a i j ,

(65) ( E a i ) I V , ε ( u ) , α i ( π δ a i , λ i ) a i = B i v ¯ , λ i 2 ( π δ a i , λ i ) λ i a i + j = 1 n C i j v ¯ , 1 λ i 2 ( π δ a i , λ i ) a i j a i .

We are looking for ( α , λ , a ) O 2 ( N , b , ε ) solution of the system defined by equations (63), (64), and (65), where O 2 ( N , b , ε ) is defined by

(66) O 2 ( N , b , ε ) = { ( α , λ , a ) ( R + ) N × ( R + ) N × Ω N : ( α , λ , a , 0 ) O 1 ( N , b , ε ) } .

In order to work with a simpler system, we make the following change of variables, for 1 i N ,

(67) β i = 1 α i p 1 , ( a i b ) = η ( ε ) σ ( ζ i + z ¯ i ) , 1 λ i 2 = c 2 c ( n ) 1 V ( b ) ε ( ln ε 2 ) σ n ( 1 + i ) .

Using these changes of variables, it is easy to see that

(68) c λ i a i a j ε 2 n ln ε σ n 4 c ,

(69) ε i j = 1 ( λ i λ j a i a j 2 ) n 2 2 1 + O 1 λ i 2 a i a j 2 + 1 λ j 2 a i a j 2 = 1 ( λ i λ j a i a j 2 ) n 2 2 ( 1 + O ( ε 4 n ln ε σ n 2 ) ) = O ( ε 2 γ + 1 ln ε σ n 2 ) ,

(70) ε i j a i = ( n 2 ) λ i λ j ( a j a i ) ε i j n ( n 2 ) = ( n 2 ) ( a j a i ) ( λ i λ j ) ( n 2 ) 2 a i a j n ( 1 + O ( ε 4 n ln ε σ n 2 ) ) = ( n 2 ) ( ε ln ε σ n ) ( n 2 ) 2 σ n 1 η ( ε ) n 1 c 2 c ( n ) V ( b ) n 2 2 ( ζ j + z ¯ j ζ i z ¯ i ) ζ i + z ¯ i ζ j z ¯ j n × ( 1 + R ( i , j ) ) ( 1 + O ( ε 4 n ln ε σ n 2 ) )

(71) = O ( ε γ + 1 ln ε σ n 4 ) ,

where

(72) R ( i , j ) = n 2 4 i + n 2 4 j + O ( i 2 ) + O ( j 2 ) .

Next, using Propositions 2.12.5, we deduce that the following estimates hold:

Lemma 3.2

For ε small, the following statements hold:

v ¯ c ε , R α i c ε , R λ i c ε 2 γ + 1 ln ε σ n 2 , R a i c ε 2 ln ε + ε ( 5 2 ) ( 4 n ) , i f n 5 , ε 3 2 ln ε 1 , i f n = 4 .

where R α i , R λ i , and R a i are defined in Propositions 2.32.5, respectively.

Now, arguing as in the proof of Lemma 4.2 of [7] and using Lemma A.4, we derive that the constants A i ’s, B i ’s and C i j ’s which appear in equations ( E v ) , ( E λ i ) , and ( E a i ) satisfy the following estimates:

Lemma 3.3

Let ( α , λ , a ) O 2 ( N , b , ε ) . Then, for ε small, the following statements hold:

A i = O ( ε ln 2 ε ) , B i = O ( ε ) a n d C i j c ε γ + 3 2 , i f n 5 , ε 3 2 ln ε 3 4 , i f n = 4 , i N , j n .

Next, our aim is to rewrite equations ( E α i ) , ( E λ i ) , and ( E a i ) in a simple form.

Lemma 3.4

For ε small, equations ( E α i ) , ( E λ i ) , and ( E a i ) are equivalent to the following system:

( S ) β i = O ( ε ln ε ) 1 i N , ( F α i ) i = O ( β i + ε 2 γ ln ε σ n 2 ) 1 i N , ( F λ i ) D 2 V ( b ) ( ζ i , ) ( n 2 ) j i ζ j ζ i z ¯ j z ¯ i n + n ( n 2 ) j i z ¯ j z ¯ i z ¯ j z ¯ i 2 , ζ j ζ i z ¯ j z ¯ i z ¯ j z ¯ i n ( n 2 ) j i z ¯ j z ¯ i z ¯ j z ¯ i n n 6 4 i + n 2 4 j = O ( R S ) 1 i N , ( F a i )

where

R S = j = 1 N j 2 + j = 1 N ζ j 2 + η ( ε ) + ε 1 2 γ ln ε .

Proof

First, using Proposition 2.3, Lemma 3.2, and the fact that ( α , λ , a ) O 2 ( N , b , ε ) , we see that ( E α i ) is equivalent to the equation ( F α i ) . Second, using Lemmas 3.3 and A.4, we write

I ε ( u ) , λ i π δ a i , λ i λ i = O B i v λ i 2 2 π δ a i , λ i λ i 2 + j = 1 N C i j v 2 π δ a i , λ i λ i a i j = O ( ε v ) .

Using Proposition 2.4, Lemma 3.2 and (69), we obtain

c 2 ε c ( n ) ln σ n λ i λ i 2 V ( a i ) = O ( ε β i + ε 2 γ + 1 ln ε σ n 2 ) .

But we have

V ( a i ) = V ( b ) + O ( a i b 2 ) = V ( b ) + O ( η ( ε ) 2 ) .

This implies that ( E λ i ) is equivalent to the equation ( F λ i ) .

To deal with the third equation ( E a i ) , using Lemma A.4, we write

(73) I ε ( u ) , 1 λ i π δ a i , λ i a i = O B i v 2 π δ a i , λ i λ i a i + j = 1 N C i j v 1 λ i 2 2 π δ a i , λ i a i a i j = O ( ε v ) .

But, combining (70), Proposition 2.5 and Lemma 3.2, (73) becomes

(74) c 2 ( n ) ln σ n λ i λ i 3 V ( a i ) ( n 2 ) c ¯ 10 ε η ( ε ) λ i j i ( ζ j + z ¯ j ζ i z ¯ i ) ζ j + z ¯ j ζ i z ¯ i n 1 + n 2 4 i + n 2 4 j = O ε 2 ln ε σ n 2 + R a i + η ( ε ) ε 3 2 ln ε σ n 2 ( β j + j 2 ) ,

where

c ¯ 10 = c ¯ 2 σ n 1 c 2 c ( n ) V ( b ) ( n 2 ) 2 .

Observe that

(75) V ( a i ) = D 2 V ( b ) ( a i b , ) + O ( a i b 2 ) = η ( ε ) σ D 2 V ( b ) ( ζ i + z ¯ i , ) + O ( η ( ε ) 2 ) .

Combining (74), (75), and (54), we obtain

(76) D 2 V ( b ) ( ζ i + z ¯ i , ) ( n 2 ) j i ( ζ j + z ¯ j ζ i z ¯ i ) ζ j + z ¯ j ζ i z ¯ i n 1 + n 6 4 i + n 2 4 j = O η ( ε ) + ε 1 2 γ ln ε + ( β j + j 2 ) .

But we have

(77) D 2 V ( b ) ( ζ i + z ¯ i , ) = D 2 V ( b ) ( ζ i , ) + D 2 V ( b ) ( z ¯ i , )

and

(78) ( ζ j + z ¯ j ζ i z ¯ i ) ζ j + z ¯ j ζ i z ¯ i n = ( z ¯ j z ¯ i ) z ¯ j z ¯ i n + ( ζ j ζ i ) z ¯ j z ¯ i n 1 n ( z ¯ j z ¯ i ) z ¯ j z ¯ i 2 , ζ j ζ i + O ( ζ i 2 + ζ j 2 ) = ( z ¯ j z ¯ i ) z ¯ j z ¯ i n n ( z ¯ j z ¯ i ) z ¯ j z ¯ i 2 , ζ j ζ i ( z ¯ j z ¯ i ) z ¯ j z ¯ i n + ( ζ j ζ i ) z ¯ j z ¯ i n + O ( ζ i 2 + ζ j 2 ) .

Combining (76)–(78) and the fact that ( z ¯ 1 , , z ¯ N ) is a critical point of F N , b , we see that equation ( E a i ) is equivalent to the equation ( F a i ) , which completes the proof of Lemma 3.4.□

Now, we are ready to prove our results related to the construction of clustered bubbling solutions.

Proof of Theorem 1.1

Note that the system ( F a 1 ) , , ( F a N ) is equivalent to

1 2 D 2 F N , b ( z ¯ 1 , , z ¯ N ) ( ζ 1 , , ζ N ) ( n 2 ) ( Γ 1 , , Γ N ) = O j = 1 N ( j 2 + ζ j 2 ) + η ( ε ) + ε 1 2 γ ln ε ,

where

Γ i j i z ¯ j z ¯ i z ¯ j z ¯ i n n 6 4 i + n 2 4 j , 1 i N .

As in the proof of Theorem 1 of [15], we define a linear map by taking the left-hand side of the system defined by ( F α i ) , ( F λ i ) , and ( F a i ) . Since ( z ¯ 1 , , z ¯ N ) is a non-degenerate critical point of F N , b , we deduce that such a linear map is invertible and arguing as in the proof of Theorem 1 of [15], we derive that the system ( S ) has a solution ( β ε , ε , ζ ε ) for ε small. This implies that ( P V , ε ) admits a solution u ε , b = i = 1 N α i , ε π δ a i , ε , λ i , ε + v ε and, by construction, properties (3)–(6) are satisfied. The proof of Theorem 1.1 is thereby complete.□

Proof of Theorem 1.3

Let b 1 and b 2 be two non-degenerate critical points of V . First, we observe that in the equation ( E λ i ) , the interaction between the bubbles of two different blocks is of the order of ε ( n 2 ) 2 , which is negligible in front of the main term whose order is ε . This implies that terms of this type will fit into the rest. Second, we note that in the equation ( E a i ) , the interaction between the bubbles of two distinct blocks is of order ( ε ( n 1 ) 2 if n 5 ; ( ε ln ε ) 3 2 if n = 4 ), which is negligible compared to the main term of order ( ε 2 2 n if n 5 ; ln ε 3 4 ε 3 2 if n = 4 ). Consequently, terms of this form can be incorporated into the remaining terms. Hence, arguing as in the proof of Theorem 1.1 and taking a new system ( ( S 1 ) , , ( S m ) ) with each ( S i ) representing the system studied in the proof of Theorem 1.1, the proof of the theorem follows.□

4 Conclusion

In this article, we have investigated the existence of solutions to a nonlinear elliptic problem with Dirichlet boundary conditions, involving a slightly subcritical exponent for Sobolev embedding H 0 1 ( Ω ) L q ( Ω ) . Through a careful asymptotic analysis of the gradient of the associated Euler-Lagrange functional near the “bubbles,” we successfully constructed solutions that exhibit bubble formation clustered at interior points. The methodology adopted is tailored to variational problems. While our work demonstrates the existence of solutions with clustered bubbles for the given problem, several promising avenues for further research and open questions remain:

  1. Location of the concentration points: this article focuses on the construction of interior bubbling solutions with clustered bubbles. A natural extension of this work would be to investigate the existence of solutions that concentrate at non-isolated interior points that approach the boundary in the limit.

  2. Impact of the nature of critical points: the solutions constructed in this article are based on the assumption that the chosen critical point b of the potential V is non-degenerate, and that the corresponding function b , N has a non-degenerate critical point, where b , N is defined by (2) with N denoting the number of bubbles clustered at point b. A natural question arises: what occurs if b is degenerate, or if b , N lacks non-degenerate critical points?

  3. Impact of subcritical exponent: the present work addresses a slightly subcritical exponent for Sobolev embedding. Future investigations could extend the analysis to exponents that are slightly supercritical, i.e., when ε < 0 but close to zero.

Acknowledgment

The researchers would like to thank the Deanship of Graduate Studies and Scientific Research at Qassim University for financial support (QU-APC-2025).

  1. Funding information: The Article Processing Charge of this article was supported by the Deanship of Graduate Studies and Scientific Research at Qassim University.

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

  3. Conflict of interest: The authors state no conflict of interest.

  4. Data availability statement: All data generated or analyzed during this study are included in this published article.

Appendix

In this appendix, we compile several estimates necessary for the analysis presented in this article. We begin with the following result, which is taken from [14] (see Lemma 2.2).

Lemma A.1

Let a i , a j , λ i , and λ j be such that ε i j is small. For α and β satisfying α + β = 2 n ( n 2 ) and α β , it holds

Ω δ i α δ j β c ε i j min ( α , β ) .

We now prove some estimations involving bubbles and the approximate solutions.

Lemma A.2

For i { 1 , , N } and j { 1 , , n } , let

φ i π δ a i , λ i , λ i ( π δ a i , λ i ) λ i , 1 λ i ( π δ a i , λ i ) ( a i ) j .

Let u ̲ i = 1 N α i π δ a i , λ i and v E a , λ , it holds

Ω ( u ̲ ) p ε 1 v φ i c v ε + T 2 ( λ i ) + j i T 3 ( ε i j ) ,

where T 2 ( λ ) and T 3 ( ε i j ) are defined in Lemma 2.1.

Proof

Observe that, from (9), we deduce that φ i c π δ a i , λ i . Thus, using the fact that: for b 1 , b 2 , z R such that z c b 1 ,

(A1) b 1 + b 2 γ z b 1 γ z c b 1 b 2 ( γ + 1 ) 2 , if γ 1 , b 1 γ b 2 + b 2 γ b 1 , if γ > 1 ,

it follows that

Ω ( u ̲ ) p ε 1 v φ i = α i p ε 1 Ω ( π δ a i , λ i ) p ε 1 v φ i + j i O Ω ( δ a i , λ i δ a j , λ j ) p 2 v , if n 6 , O Ω δ a i , λ i p 1 δ a j , λ j v + Ω δ a i , λ i δ a j , λ j p 1 v , if n 5 .

Note that, for n 5 (which implies that p 1 > 1 ), for each k and , it holds

Ω δ a k , λ k p 1 δ a , λ v c v Ω ( δ a k , λ k p 1 δ a , λ ) 2 n n + 2 n + 2 2 n c v ε k ,

using Lemma A.1. However, using (24), we derive that

Ω ( δ a i , λ i δ a j , λ j ) p 2 v c v Ω ( δ a i , λ i δ a j , λ j ) n n 2 n + 2 2 n c v ε i j n + 2 2 ( n 2 ) ( ln ε i j 1 ) n + 2 2 n .

For the other integral, following the end of the proof of Lemma 6.6 of [7], we deduce that

Ω ( π δ a i , λ i ) p ε 1 v φ i c v ( ε + T 2 ( λ i ) ) .

Hence, the proof of lemma is complete.□

Lemma A.3

Let a 1 , a 2 Ω be such that d ( a i , Ω ) c > and λ 1 , λ 2 be large reals such that ε 12 is small. Let ψ 1 { θ a 1 , λ 1 , λ 1 θ a 1 , λ 1 λ 1 } . It holds that

Ω δ a 2 , λ 2 n + 2 n 2 ψ 1 c ( λ 1 λ 2 ) ( n 2 ) 2 + c ε 12 1 λ 1 , i f n = 3 , ln λ 1 λ 1 2 + a 1 a 2 2 ln a 1 a 2 + 1 λ 2 3 2 , i f n = 4 , 1 λ 1 2 + a 1 a 2 2 + 1 λ 2 3 2 , i f n 5 . Ξ 12

Proof

First, we remark that we can modify the proof to improve the power of λ 2 . It can be β with β < 2 .

Let B 1 B ( a 1 , r 1 ) , where r 1 ( 1 2 ) min ( d a 1 , e 4 ) ; using (10) and (11), we obtain

Ω δ a 2 , λ 2 n + 2 n 2 ψ 1 c B 1 R a 1 , λ 1 1 ( x ) δ a 2 , λ 2 n + 2 n 2 δ a 1 , λ 1 + Ω \ B 1 δ a 2 , λ 2 n + 2 n 2 δ a 1 , λ 1 ,

where R a 1 , λ 1 1 is defined in (12). For the last integral, it is easy to obtain

Ω \ B 1 δ a 2 , λ 2 n + 2 n 2 δ a 1 , λ 1 c λ 1 ( n 2 ) 2 R n δ a 2 , λ 2 n + 2 n 2 c λ 1 ( n 2 ) 2 λ 2 ( n 2 ) 2 .

Concerning the other one, using the formula of R a 1 , λ 1 1 , we have to distinguish three cases.

  • For n = 3 , we remark that, in this case, x a δ a , λ c λ . Thus, it holds

    B 1 R a 1 , λ 1 1 ( x ) δ a 2 , λ 2 n + 2 n 2 δ a 1 , λ 1 c λ 1 R n δ a 2 , λ 2 n + 2 n 2 δ a 1 , λ 1 + B 1 x a 1 δ a 2 , λ 2 n + 2 n 2 δ a 1 , λ 1 c λ 1 ε 12 + c λ 1 R n δ a 2 , λ 2 n + 2 n 2 c λ 1 ε 12 + c λ 1 λ 2 .

  • For n 5 , it holds that

    B 1 R a 1 , λ 1 1 ( x ) δ a 2 , λ 2 n + 2 n 2 δ a 1 , λ 1 c λ 1 2 R n δ a 2 , λ 2 n + 2 n 2 δ a 1 , λ 1 + c B 1 x a 1 2 δ a 2 , λ 2 n + 2 n 2 δ a 1 , λ 1 c ε 12 λ 1 2 + c a 1 a 2 2 R n δ a 2 , λ 2 n + 2 n 2 δ a 1 , λ 1 + c Ω x a 2 2 δ a 2 , λ 2 n + 2 n 2 δ a 1 , λ 1 .

    Note that

    (A2) Ω x a 2 2 δ a 2 , λ 2 n + 2 n 2 δ a 1 , λ 1 = Ω c λ 2 3 2 x a 2 δ a 2 , λ 2 n 1 n 2 δ a 1 , λ 1 c λ 2 3 2 Ω 1 x a 2 2 n 3 3 ( 2 n ) Ω δ a 2 , λ 2 n 1 n 2 δ a 1 , λ 1 2 n 2 n 3 ( 2 n 3 ) ( 2 n ) c λ 2 3 2 ε 12 .

  • For n = 4 ,

    B 1 R a 1 , λ 1 1 ( x ) δ a 2 , λ 2 n + 2 n 2 δ a 1 , λ 1 c ln λ 1 λ 1 2 R n δ a 2 , λ 2 n + 2 n 2 δ a 1 , λ 1 + B 1 x a 1 2 ln x a 1 δ a 2 , λ 2 n + 2 n 2 δ a 1 , λ 1 .

    Concerning the second integral, observe that, if a 1 a 2 e 4 , it follows that x a 2 e 4 2 for each x B 1 , and therefore,

    B 1 x a 1 2 ln x a 1 δ a 2 , λ 2 3 δ a 1 , λ 1 c λ 2 3 B 1 x a 1 2 ln x a 1 δ a 1 , λ 1 .

    In the other case, i.e., a 1 a 2 e 4 , it follows that x a 2 ( 3 2 ) e 4 , and therefore, since the function : t t 2 ln t is increasing and convex on the set ( 0 , e 4 ) , we deduce that

    x a 1 2 ln x a 1 c x a 2 2 ln x a 2 + c a 2 a 1 2 ln a 2 a 1 .

    Thus, the integral becomes

    B 1 x a 1 2 ln x a 1 δ a 2 , λ 2 3 δ a 1 , λ 1 c B 1 x a 2 2 ln x a 2 δ a 2 , λ 2 3 δ a 1 , λ 1 + c a 2 a 1 2 ln a 2 a 1 B 1 δ a 2 , λ 2 3 δ a 1 , λ 1 Ω c ln x a 2 λ 2 3 2 x a 2 ( δ a 2 , λ 2 3 2 δ a 1 , λ 1 ) + c a 2 a 1 2 ln a 2 a 1 ε 12 c λ 2 3 2 ε 12 + c a 2 a 1 2 ln a 2 a 1 ε 12 ,

    where we have used the same computations done in (A2).

This completes the proof of the lemma.□

Lemma A.4

Let n 4 .

(1) Let d 0 be a fixed small positive constant, a Ω 0 { x Ω : d ( x , Ω ) d 0 } , and λ be large. Then, we have

(A3) π δ a , λ 2 = S n + O ln σ n λ λ 2 , π δ a , λ , φ = O ln σ n λ λ m , w i t h m = 2 , i f φ = λ ( π δ a , λ ) λ , m = 3 , i f φ = λ 1 ( π δ a , λ ) a ,

(A4) λ π δ a , λ λ 2 = c + O ln σ n λ λ 2 , λ π δ a , λ λ , 1 λ π δ a , λ a = O ln σ n λ λ 3 ,

(A5) 1 λ π δ a , λ a j 2 = c + O ln σ n λ λ 3 , 1 λ δ a , λ a j , 1 λ δ a , λ a = O ln σ n λ λ 3 j .

(2) Let a 1 , a 2 Ω 0 , and λ 1 , λ 2 be large so that ε 12 , defined in (14), is small. Then, we have

(A6) φ 1 , φ 2 = O ( ε 12 ) φ i π δ a i , λ i , λ i π δ a i , λ i λ i , 1 λ i π δ a i , λ i a i j , f o r i { 1 , 2 } a n d j { 1 , , n } .

Proof

Note that the first assertion is proved in (35), (39), and (49), respectively. Concerning Claim (A4), using (9) and (10), we obtain

λ π δ a , λ λ 2 = Ω ( Δ + V ) λ π δ a , λ λ λ π δ a , λ λ = n + 2 n 2 Ω δ a , λ 4 ( n 2 ) λ δ a , λ λ λ δ a , λ λ λ θ a , λ λ = n + 2 n 2 R n δ a , λ 4 ( n 2 ) λ δ a , λ λ 2 + O R n \ Ω δ a , λ 2 n ( n 2 ) + Ω δ a , λ ( n + 2 ) ( n 2 ) θ a , λ .

Thus, (34) and easy computations imply the proof of the first equality in (A4). For the other equality, observe that

λ π δ a , λ λ , 1 λ π δ a , λ a = Ω ( Δ + V ) λ π δ a , λ λ 1 λ π δ a , λ a = n + 2 n 2 Ω δ a , λ 4 n 2 λ δ a , λ λ 1 λ δ a , λ a 1 λ θ a , λ a .

Let B B ( a , d 0 ) , by oddness, it holds that

Ω δ a , λ 4 n 2 λ δ a , λ λ 1 λ δ a , λ a = Ω \ B δ a , λ 4 n 2 λ δ a , λ λ 1 λ δ a , λ a = O 1 λ n + 1 .

For the other integral, since a Ω 0 , we obtain

n + 2 n 2 Ω δ a , λ 4 n 2 λ δ a , λ λ 1 λ θ a , λ a = Ω ( Δ + V ) λ π δ a , λ λ 1 λ θ a , λ a = Ω λ π δ a , λ λ ( Δ + V ) 1 λ θ a , λ a Ω ν λ π δ a , λ λ 1 λ θ a , λ a = Ω λ π δ a , λ λ V 1 λ δ a , λ a + O 1 λ n 1 .

To complete the proof, using (9)–(11) and the fact that δ a , λ a c δ a , λ x a , we obtain

Ω \ B λ π δ a , λ λ V 1 λ δ a , λ a c Ω \ B δ a , λ 1 λ δ a , λ a c λ n 1 , B λ π δ a , λ λ V 1 λ δ a , λ a = V ( a ) B ( a , d 0 ) δ a , λ λ δ a , λ a + O B 1 λ δ a , λ 2 + B R a , λ 1 ( x ) δ a , λ 2 λ x a c ln σ n λ λ 3 .

This completes the proof of assertion (A4).

The proof of (A5) can be done in the same way than the proof of (A4). Thus, we will omit it here.

Concerning assertion (A6), note that (9) and easy computations imply that

( Δ + V ) φ i c δ a i , λ i ( n + 2 ) ( n 2 ) and φ i c δ a i , λ i , for i { 1 , 2 } .

Thus, using the last inequality of (33), we deduce that

φ 1 , φ 2 = Ω ( ( Δ + V ) φ 1 ) φ 2 c Ω δ a 1 , λ 1 ( n + 2 ) ( n 2 ) δ a 2 , λ 2 c ε 12 .

This completes the proof of assertion (A6).□

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Received: 2025-01-16
Revised: 2025-04-27
Accepted: 2025-05-06
Published Online: 2025-06-05

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

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

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