Startseite Nontrivial solution for Klein-Gordon equation coupled with Born-Infeld theory with critical growth
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Nontrivial solution for Klein-Gordon equation coupled with Born-Infeld theory with critical growth

  • Chuan-Min He , Lin Li EMAIL logo und Shang-Jie Chen
Veröffentlicht/Copyright: 3. März 2023

Abstract

In this article, we study the following system:

Δ u + V ( x ) u ( 2 ω + ϕ ) ϕ u = λ f ( u ) + u 4 u , in R 3 , Δ ϕ + β Δ 4 ϕ = 4 π ( ω + ϕ ) u 2 , in R 3 ,

where f ( u ) is without any growth and Ambrosetti-Rabinowitz condition. We use a cut-off function and Moser iteration to obtain the existence of nontrivial solution. Finally, as a by-product of our approaches, we obtain the same result for the Klein-Gordon-Maxwell system.

MSC 2010: 35A15; 35B33; 35J60

1 Introduction

This article studies the Klein-Gordon equation coupled with the Born-Infeld (BI) theory with critical growth

(1.1) Δ u + V ( x ) u ( 2 ω + ϕ ) ϕ u = λ f ( u ) + u 4 u , in R 3 , Δ ϕ + β Δ 4 ϕ = 4 π ( ω + ϕ ) u 2 , in R 3 ,

where ω > 0 is a constant and λ > 0 is a positive parameter. The Klein-Gordon equation can be used to develop the theory of electrically charged fields [14] and study the interaction with an assigned electromagnetic field [12]. The BI electromagnetic theory [2,3] was originally proposed as a nonlinear correction of the Maxwell theory in order to overcome the problem of infiniteness in the classical electrodynamics of point particles (see [15]). The Klein-Gordon equation coupled with BI theory system has attracted many theoretic physicists. For more physical applications, please refer to references [20,30] and the references therein.

In the past decades, many people have studied this system by using variational methods and have also obtained the existence of nontrivial solution under different assumptions. Let us recall some previous results.

The first result is due to d’Avenia and Pisani, in which the existence of infinitely many radially symmetric solutions for the following form:

(1.2) Δ u + [ m 2 ( ω + ϕ ) 2 ] u = u p 2 u , in R 3 , Δ ϕ + β Δ 4 ϕ = 4 π ( ω + ϕ ) u 2 , in R 3 ,

where 4 < p < 6 and ω < m 0 in [13]. Mugnai [20] obtained the same result when 2 < p 4 and 0 < ω < 1 2 p 1 m . Afterward, Wang [26] used Pohožaev identity to improve [13,20] and obtained the solitary wave solution when one of the following conditions is satisfied,

  1. 3 < p < 6 and m > ω > 0 ,

  2. 2 < p 3 and ( p 2 ) ( 4 p ) m 2 > ω 2 > 0 .

Yu [30] obtain the existence of the least-action solitary wave. Moreover, replacing u p 2 u by u p 2 u + h ( x ) , Chen and Li in [8] obtain the existence of multiple solution if one of the following conditions holds
  1. 4 < p < 6 and m > ω ,

  2. 2 < p 4 and 1 2 p 1 m > ω .

Later, Chen and Song [9] studied the following Klein-Gordon equation with concave and convex nonlinearities coupled with BI theory:

(1.3) Δ u + V ( x ) u ( 2 ω + ϕ ) ϕ u = λ k ( x ) u q 2 u + g ( x ) u p 2 u , in R 3 , Δ ϕ + β Δ 4 ϕ = 4 π ( ω + ϕ ) u 2 , in R 3 .

Under some appropriate assumptions on V ( x ) , λ , k ( x ) , and g ( x ) , they obtained the existence of multiple nontrivial solutions when 1 < q < 2 < p < 6 . Recently, for general potential V ( x ) and u p 2 u by a continuous nonlinearity f ( x , u ) with polynomial growth, Wen et al. [27] obtained infinitely many solutions and least energy solution. Che and Chen [7] used the genus theory to obtain the nontrivial solution.

We know that many papers about the nonlinearity are on subcritical growth. When the nonlinearity term is accompanied by critical growth, it is one of the most dramatic cases of loss compactness. To our best knowledge, there are only two works about the Klein-Gordon-Born-Infeld system with critical growth. Teng and Zhang [24] investigated the following system:

(1.4) Δ u + [ m 2 ( ω + ϕ ) 2 ] u = u p 2 u + u 2 2 u , in R 3 , Δ ϕ + β Δ 4 ϕ = 4 π ( ω + ϕ ) u 2 , in R 3 .

They obtained (1.4) has at least a nontrivial solution when 4 < p < 6 and m < ω . Later, the authors of [16] proved that there is a ground state solution for 2 < p < 4 . For some other equations where nonlinearity is critical growth, such as Choquard-Kirchhoff equation, Schrödinger equation, Schrödinger-Poisson system, and Schrödinger-Choquard-Kirchhoff equation, there are many mathematicians have obtained many interesting results. We just list a few, for example, see [10,18,19,21] and the references therein.

Motivated by the aforementioned works, in this article, we will use some new tricks to generalize [16,24] under the following conditions:

  1. V C 1 ( R 3 , R ) and there is a V 0 > 0 such that V ( x ) V 0 for all x R 3 .

  2. V ( x ) as x .

  3. f C ( R ) , lim u 0 f ( u ) u = 0 .

  4. lim u f ( u ) u = + .

Our first result is as follows.

Theorem 1.1

Assume that ( V 1 )–( V 2 ) and ( f 1 )–( f 2 ) hold. Then there exists a constant λ 1 0 such that, for any λ ( 0 , λ 1 ) , system (1.1) has a nontrivial solution.

Remark 1.2

We all know that if the nonlinear term of (1.1) is u 4 u , we can use the Pohožaev identity and the classical variational method to know whether the system has nontrivial solution. When the nonlinearity term like f(u) in problem (1.1) are on critical growth case, it is usually to add a high energy lower-order perturbation term like [5,24,25]. By comparing with the aforementioned articles, in this paper, λ is small enough, that is, the lower-order perturbation is a lower energy perturbation.

Remark 1.3

  1. The condition ( V 2 ) was first introduced by Rabinowitz in [22] to overcome the lack of compactness.

  2. It is worth noting that in this article we did not require any growth conditions and the Ambrosetti-Rabinowitz condition, and the function f can also be sign-changing.

  3. There are many functions to satisfy the condition ( f 1 )–( f 2 ), and the most typical example is f ( t ) = t p 2 t , p > 6 . Moreover, our result is valid for general supercritical nonlinearity.

To prove the existence of the nontrivial solution, we adapt a similar argument as in [17,29]. Here, we briefly explain the process. First, we make a suitable cut-off function to replace f ( u ) in problem (1.1), so we can obtain a new system. Second, we prove the new system have a nontrivial solution. Finally, we use the Moser iteration to obtain the existence of a nontrivial solution to the original Klein-Gordon equation coupled with BI theory.

In the second part of this article, when β = 0 , problem (1.1) will become a Klein-Gordon-Maxwell system with critical growth, namely:

(1.5) Δ u + V ( x ) u ( 2 ω + ϕ ) ϕ u = λ f ( u ) + u 4 u , in R 3 , Δ ϕ = ( ω + ϕ ) u 2 , in R 3 .

This system has been extensively studied by many authors. A pioneering work is due to Cassani [6]. He considered the following Klein-Gordon-Maxwell critical system:

Δ u + [ m 2 ( ω + ϕ 2 ) ] u = λ u p 2 u + u 4 u , in R N , Δ ϕ = ( ω + ϕ ) u 2 , in R N ,

where λ > 0 , 2 < p < 6 , and 0 < ω < m . When N = 3 , he obtained the existence of a radially symmetric solution for any λ > 0 if p ( 4 , 6 ) and for λ is sufficiently large if p = 4 . Afterward Carrião et al. [5] complement the result of [6] and extend it in higher dimensions. They obtained the existence nontrivial solution of the previous equation provided one of those conditions satisfies

  1. N = 4 and N 6 for 2 < p < 2 and m > ω if λ > 0 ;

  2. N = 5 and either 2 < p < 8 3 if λ > 0 or 8 3 p < 2 if λ is sufficiently large;

  3. N = 3 and either 4 < p < 2 if λ > 0 or 2 < p 4 if λ is sufficiently large.

Later, when N = 3 , Wang [25] improved as the result of [5,6] when one of the following holds:
  1. 4 < p < 6 , 0 < ω < m and λ > 0 ;

  2. 3 < p 4 , 0 < ω < m and λ is sufficiently large;

  3. 2 < p 3 , 0 < ω < ( p 2 ) ( 4 p ) m and λ is sufficiently large.

In a recent article [11], Chen et al. use some analytical skills and variational method, which is different from [25] to obtain the same result. The authors of [5] have also studied that for problem (1.5), N = 3 , V ( x ) is a periodic function and f ( u ) = u p 2 u in [4]. They use the minimization of the corresponding Euler-Lagrange functional on the Nehari manifold and the Brézis and Nirenberg technique to obtain a positive ground state solution for each λ > 0 if p ( 4 , 6 ) and for λ sufficiently large if p ( 2 , 4 ] . Moreover, the following problem

(1.6) Δ u + μ V ( x ) u ( 2 ω + ϕ ) ϕ u = λ f ( x , u ) + u 4 u , in R 3 , Δ ϕ = ( ω + ϕ ) u 2 , in R 3 ,

admits that a nontrivial solution has been proved by Zhang [31]. Instead of the expression “ λ sufficiently large” in the aforementioned existing works, Tang et al. [23] give a certain range λ λ 0 , which admits a ground state solution when V is positive and periodic.

Similar to the method of Theorem 1.1, we can also obtain a nontrivial solution. Compared with the hypothesis of subcritical perturbation in the aforementioned article, in this article, the perturbation term f ( u ) can be not only a subcritical perturbation but also a supercritical perturbation. What’s more the restriction on λ is no longer sufficiently larger or greater than a certain number, we can only require λ ( 0 , λ 2 ) , where λ 2 0 . Our second result is as follows.

Theorem 1.4

Assume that ( V 1 )–( V 2 ) and ( f 1 )–( f 2 ) hold. Then there exists a constant λ 2 0 such that, for any λ ( 0 , λ 2 ) , system (1.5) has a nontrivial solution.

Remark 1.5

We notice that the existence of nontrivial solution for problem (1.5) has been proved by aforementioned articles with a different approach in this article. However, it is interesting that we do not need λ is sufficiently larger or greater than a certain number.

This article is organized as follows. In Section 2, we present some preliminary lemmas. In Section 3, we prove Theorems 1.1. In Section 4, we prove Theorem 1.4.

2 Preliminaries

In this section, we explain the notations and some auxiliary lemmas, which are useful later.

H 1 ( R 3 ) denotes the usual Sobolev space equipped with the standard norm.

L ( R 3 ) , [ 1 , + ) denotes the Lebesgue space with the norm u = R 3 u d x 1 .

Under ( V 1 ) and ( V 2 ) , we define the Hilbert space

E = u H 1 ( R 3 ) : R 3 V ( x ) u 2 d x < ,

with respect to the norm

u = R 3 ( u 2 + V ( x ) u 2 ) d x 1 2 .

Then, the embedding E H 1 ( R 3 ) is continuous. The embedding from E into L q ( R 3 ) is compact for q [ 2 , 6 ) , and its detailed proof process can be seen in Lemma 3.4 in [33].

We denote by D ( R 3 ) the completion of C 0 ( R 3 ) with respect to the norm

ϕ D ( R 3 ) = R 3 ϕ 2 d x 1 2 + R 3 ϕ 4 d x 1 4 .

It is easy to know that D ( R 3 ) is continuously embedded in D 1 , 2 ( R 3 ) , where D 1 , 2 ( R 3 ) is the completion of C 0 ( R 3 ) with respect to the norm ϕ D 1 , 2 ( R 3 ) = R 3 ϕ 2 d x 1 2 . Moreover, D 1 , 2 ( R 3 ) is continuously embedded in L 6 ( R 3 ) by Sobolev inequality and D ( R 3 ) is continuously embedded in L ( R 3 ) .

C 1 , C 2 , denote positive constant possibly different in different places.

Indeed, solutions of (1.1) are critical points of functional G λ : E ( R 3 ) × D ( R 3 ) R , defined by

(2.1) G λ ( u , ϕ ) = 1 2 R 3 ( u 2 + V ( x ) u 2 ( 2 ω + ϕ ) ϕ u 2 ) d x 1 8 π R 3 ϕ 2 d x β 16 π R 3 ϕ 4 d x R 3 λ F ( u ) + 1 6 u 6 d x .

Due to the strong indefiniteness of functional (2.1), we use the reduction method that can reduce the study of G λ ( u , ϕ ) to study a new functional I λ ( u ) as in [1].

We state some properties of the second equation of problem (1.1).

Lemma 2.1

For any u H 1 ( R 3 ) , we have:

  1. there exists a unique ϕ u D ( R 3 ) , which solves the second equation of problem (1.1);

  2. in the set { X : u ( x ) 0 } , we have ω ϕ u 0 ;

  3. ϕ u D C u 2 and R 3 ϕ u u 2 d x C u 12 5 4 .

Proof

(i) is proved in Lemma 3 of [13] and (ii) can be found in Lemma 2.3 of [20].

(2.2) R 3 ϕ u 2 d x + β R 3 ϕ u 4 d x = R 3 4 π ω ϕ u u 2 d x R 3 4 π ϕ u 2 u 2 d x 4 π ω R 3 ϕ u u 2 d x 4 π ω ϕ u D u 12 5 2 .

We can obtain ϕ u D C u 2 and R 3 ϕ u u 2 d x C u 12 5 4 .□

From the second equation in (1.1) and Lemma 2.1, we obtain

(2.3) 1 4 π R 3 ϕ u 2 d x + β 4 π R 3 ϕ u 4 d x = R 3 ( ω ϕ u + ϕ u 2 ) u 2 d x .

Consider the functional I λ ( u ) : E R defined by I λ ( u ) = G λ ( u , ϕ u ) , and by combining with (2.3), we obtain

(2.4) I λ ( u ) = 1 2 R 3 ( u 2 + V ( x ) u 2 ( 2 ω + ϕ u ) ϕ u u 2 ) d x 1 8 π R 3 ϕ u 2 d x β 16 π R 3 ϕ u 4 d x R 3 λ F ( u ) + 1 6 u 6 d x = 1 2 R 3 ( u 2 + V ( x ) u 2 ) d x 3 4 R 3 ω ϕ u u 2 d x 1 4 R 3 ϕ u 2 u 2 d x 1 16 π R 3 ϕ u 2 d x R 3 λ F ( u ) + 1 6 u 6 d x = 1 2 R 3 ( u 2 + V ( x ) u 2 ) d x 1 2 R 3 ω ϕ u u 2 d x + β 16 π R 3 ϕ u 4 d x R 3 λ F ( u ) + 1 6 u 6 d x .

Of course I λ ( u ) C 1 ( E , R ) and for any u , v E , we have

(2.5) I λ ( u ) , v = R 3 { u v + V ( x ) u v ( 2 ω + ϕ u ) ϕ u u v λ f ( u ) v u 4 u v } d x .

Lemma 2.2

[20] The following statements are equivalent:

  1. ( u , ϕ ) E ( R 3 ) × D ( R 3 ) is a critical point of G λ , i.e., ( u , ϕ ) is a solution of problem (1.1);

  2. u is a critical point of I λ and ϕ = ϕ u .

From ( f 2 ) , there exist T > 0 large enough such that f ( T ) > 0 . Let

(2.6) h T ( t ) = f ( t ) , 0 < t T , C T t p 1 , t > T , 0 , t 0 ,

where f satisfies ( f 1 ) , ( f 2 ) , and C T = f ( T ) T p 1 ( 4 < p < 6 ) . h T is a continuous function and satisfies the following properties:

  1. lim t 0 + h T ( t ) t = 0 .

  2. lim t + H T ( t ) t 4 = + , where H T ( t ) = 0 t h T ( s ) d s .

  3. h T ( t ) C T t + C T t p 1 , where C T = max t [ 0 , T ] f ( t ) t .

  4. There exists μ = μ ( T ) > 0 such that t h T ( t ) 4 H T ( t ) μ t 2 for all t 0 .

Next, we will use the cut-off function h to replace f in problem (1.1). Now, we face a new problem, namely,

(2.7) Δ u + V ( x ) u ( 2 ω + ϕ u ) ϕ u u = λ h T ( u ) + u 4 u , x R 3 , u ( x ) > 0 , u E .

We will study the critical points for the functional

(2.8) J λ , T ( u ) = 1 2 R 3 ( u 2 + V ( x ) u 2 ( 2 ω + ϕ u ) ϕ u u 2 ) d x 1 8 π R 3 ϕ u 2 d x β 16 π R 3 ϕ u 4 d x R 3 λ H T ( u ) + 1 6 u 6 d x = 1 2 R 3 ( u 2 + V ( x ) u 2 ) d x 3 4 R 3 ω ϕ u u 2 d x 1 4 R 3 ϕ u 2 u 2 d x 1 16 π R 3 ϕ u 2 d x R 3 λ H T ( u ) + 1 6 u 6 d x = 1 2 R 3 ( u 2 + V ( x ) u 2 ) d x 1 2 R 3 ω ϕ u u 2 d x + β 16 π R 3 ϕ u 4 d x R 3 λ H T ( u ) + 1 6 u 6 d x .

From direct calculation, we know that the function h T is continuous, and we have J λ , T C 1 ( E , R ) , and for any u , v E ,

(2.9) J λ , T ( u ) , v = R 3 { u v + V ( x ) u v ( 2 ω + ϕ u ) ϕ u u v λ h T ( u ) v u 4 u v } d x .

The next lemma shows that functional J λ , T ( u ) satisfies the mountain pass geometry.

Lemma 2.3

The functional J λ , T ( u ) satisfies the following conditions:

  1. there exists α , ρ > 0 such that J λ , T ( u ) α when u = ρ ;

  2. there exists e E such that e > ρ and J λ , T ( e ) < 0 .

Proof

From ( h 1 ) and ( h 3 ) , there exists ε > 0 such that

h T ( t ) ε t + C ε t 5 ,

and

(2.10) H T ( t ) ε 2 t 2 + C ε 6 t 6 .

Then from Lemma 2.1, (2.8), (2.10) and Sobolev embedding theorem, for every u E { 0 } , we can deduce

(2.11) J λ , T ( u ) = 1 2 R 3 ( u 2 + V ( x ) u 2 ) d x 1 2 R 3 ω ϕ u u 2 d x + β 16 π R 3 ϕ u 4 d x R 3 λ H T ( u ) + 1 6 u 6 d x 1 2 R 3 ( u 2 + V ( x ) u 2 ) d x R 3 λ H T ( u ) + 1 6 u 6 d x 1 2 u 2 R 3 λ ε 2 u 2 + λ C ε 6 u 6 + 1 6 u 6 d x 1 2 u 2 C ε u 2 C u 6 .

Since ε is arbitrarily small, there exists ρ > 0 and α > 0 such that J λ . T ( u ) α > 0 for u = ρ . Hence, J λ . T ( u ) satisfied (i).

From ( h 1 ) , ( h 2 ) , and ( h 3 ) , for any M > 0 , there exists a positive constant C M > 0 such that

(2.12) H T ( u ) M t 4 C M t 2 , t > 0 .

So, fix u E { 0 } and t > 0 . From (2.8) and (2.12), we obtain

(2.13) J λ , T ( t u ) = t 2 2 R 3 ( u 2 + V ( x ) u 2 ) d x t 2 R 3 ω ϕ t u u 2 d x t 2 2 R 3 ϕ t u 2 u 2 1 8 π R 3 ϕ t u 2 d x β 16 π R 3 ϕ t u 4 d x R 3 λ H T ( t u ) + t 6 6 u 6 d x t 2 2 R 3 ( u 2 + V ( x ) u 2 ) d x t 2 R 3 ω ϕ t u u 2 d x + λ C M t 2 R 3 u 2 d x λ M t 4 R 3 u 4 d x t 6 6 R 3 u 6 d x .

Now J λ , T ( t u ) for t + . The step (ii) is proved by taking e = t 0 u with t 0 > 0 large enough.□

From Lemma 2.3, we can obtain a ( P S ) sequence, namely, there exists a sequence { u n } E satisfying

(2.14) J λ , T ( u n ) c λ , T , J λ , T ( u n ) 0 ,

where

c λ , T inf γ Γ max 0 t 1 J λ , T ( γ ( t ) ) , Γ { γ C ( [ 0 , 1 ] , H 1 ( R 3 ) ) : γ ( 0 ) = 0 , γ ( 1 ) = e } .

Lemma 2.4

The sequence { u n } defined by (2.14) is bounded in E.

Proof

From (2.8), (2.9), (2.14), and ( h 4 ) , we obtain that

(2.15) c λ , T + o n ( 1 ) u n J λ , T ( u n ) 1 4 J λ , T ( u n ) = 1 4 R 3 ( u n 2 + V ( x ) u n 2 ) d x + β 16 π R 3 ϕ u n 4 d x + 1 4 R 3 ϕ u n 2 u n 2 d x + λ 4 R 3 ( h T ( u n ) u n 4 H T ( u n ) ) d x + 1 12 R 3 u n 6 d x 1 4 R 3 ( u n 2 + V ( x ) u n 2 ) d x + λ 4 R 3 ( h T ( u n ) u n 4 H T ( u n ) ) d x 1 4 u n 2 λ μ 4 R 3 u n + 2 d x ,

where u n ( x ) = u n + ( x ) + u n ( x ) , u n + ( x ) = max { u n ( x ) , 0 } , u n ( x ) = min { u n ( x ) , 0 } . Assume u n + as n . Let v n = u n u n , n 1 , which is bounded, then up to a subsequence, v n v in E and from Sobolev embedding

(2.16) v n v in E v n v , in L q ( R 3 ) , 2 q < 6 , v n v , a.e. in R 3 .

What’s more, we deduce

(2.17) v n + v + , in E , v n + v + , in L q ( R 3 ) , 2 q < 6 , v n + v + , a.e. in R 3 .

By dividing both sides of (2.15) by u n 2 , we obtain

(2.18) o n ( 1 ) 1 4 λ μ 4 R 3 v n + 2 d x = 1 4 λ μ 4 R 3 v + 2 d x + o ( 1 ) .

We can deduce v + 0 . Due to u n + = v n + u n + , (2.9), (2.14), and Lemma 2.1, we obtain

(2.19) J λ , T ( u n ) u n u n 4 = u n 2 u n 4 R 3 2 ω ϕ u n u n 2 d x u n 4 R 3 ϕ u n 2 u n 2 d x u n 4 R 3 λ h T ( u n ) u n d x u n 4 R 3 u n 6 d x u n 4 o n ( 1 ) + R 3 2 ω ϕ u n u n 2 d x u n 4 R 3 λ h T ( u n + ) u n + ( v n + ) 4 ( u n + ) 4 d x .

From Lemma 2.1(iii), (2.17), and ( h 2 ) , we know that R 3 2 ω ϕ u n u n 2 d x u n 4 2 ω and R 3 λ h T ( u n + ) u n + ( v n + ) 4 ( u n + ) 4 d x + . Taking the limit of (2.19), we obtain 0 which has a contradiction. Therefore, { u n } is bounded in E .□

Lemma 2.5

If { u n } is bounded in E, then, up to a subsequence, ϕ u n ϕ u in D .

Proof

Due to { u n } is bounded in E , we know

(2.20) u n u weakly in E u n u in L q ( R 3 ) , 2 q < 6 .

From (2.2), we can easily know { ϕ u n } is bounded in D ( R 3 ) . So, there exists a ϕ 0 D such that ϕ u n ϕ 0 in D , as a consequence,

(2.21) ϕ u n ϕ 0 weakly in L 6 ( R 3 ) , ϕ u n ϕ 0 in L loc q ( R 3 ) , 1 q < 6 .

Next we will show ϕ u = ϕ 0 . By Lemma (2.1), it suffices to show that

Δ ϕ 0 + β Δ 4 ϕ 0 = 4 π ( ω + ϕ 0 ) u 2 .

Let φ C 0 ( R 3 ) be a test function. Since Δ ϕ u n + β Δ 4 ϕ u n = 4 π ( ω + ϕ u n ) u 2 , we obtain

R 3 ϕ u n , φ d x β R 3 ϕ u n 2 ϕ u n , φ d x = R 3 4 π ω u n 2 φ d x + R 3 4 π ϕ u n u n 2 φ d x .

From (2.20), (2.21), and the boundedness of { ϕ u n } in D , the following formulas are all true, namely,

R 3 ϕ u n , φ d x n R 3 ϕ 0 , φ d x , R 3 ϕ u n 2 ϕ u n , φ d x n R 3 ϕ 0 2 ϕ 0 , φ d x , R 3 u n 2 φ d x n R 3 u 2 φ d x , R 3 4 π ϕ u n u n 2 φ d x n R 3 4 π ϕ 0 u 2 φ d x .

This proves that ϕ u = ϕ 0 .

Since ϕ u n and ϕ u satisfy the second equation in problem (1.1), let us take the difference between them, and we obtain

(2.22) R 3 { ( ϕ u n ϕ u ) v + β ( ϕ u n 2 ϕ u n ϕ u 2 ϕ u ) v } d x = 4 π R 3 { ω ( u n 2 u 2 ) v + ( ϕ u n u n 2 ϕ u u 2 ) v } d x ,

for any v D . Let v = ϕ u n ϕ u , and using the inequality,

( x p 2 x y p 2 y ) ( x y ) c p x y p , for any x , y R N , p 2 ,

we obtain

(2.23) C ( ϕ u n ϕ u 2 2 + ϕ u n ϕ u 4 4 ) 4 π R 3 ( ω u n 2 u 2 ϕ u n ϕ u + ϕ u n ϕ u n ϕ u u n 2 + ϕ u ϕ u n ϕ u u 2 ) d x .

By the Hölder inequality, the Sobolev inequality and (2.20), we complete the statement.□

Lemma 2.6

J λ , T satisfies the ( PS ) c condition at any level c 0 , 1 3 S 3 2 , where S is the best constant of the Sobolev embedding H 1 ( R 3 ) L 6 ( R 3 ) , i.e.,

S = inf u D 1 , 2 ( R 3 ) R 3 u 2 d x R 3 u 6 d x 1 3 .

Proof

Let { u n } be a ( P S ) sequence satisfying (2.14). Form Lemma 2.4, we know that { u n } is bounded in E , then up to a subsequence, we obtain

(2.24) u n u , in E , u n u , in L q ( R 3 ) , 2 q < 6 , u n u , a.e. in R 3 .

Assume ν n = u n u , from the Brezis-Lieb lemma in [28], we obtain

(2.25) R 3 u n 2 d x = R 3 u 2 d x + R 3 ν n 2 d x + o ( 1 ) , R 3 u n 2 d x = R 3 u 2 d x + R 3 ν n 2 d x + o ( 1 ) , R 3 u n 6 d x = R 3 u 6 d x + R 3 ν n 6 d x + o ( 1 ) .

Due to [28, Theorem A.1], for any φ C 0 E , we deduce

R 3 h T ( u n ) φ d x R 3 h T ( u ) φ d x .

It is easy to know that

(2.26) R 3 ( h T ( u n ) u n h T ( u ) u ) d x = R 3 ( h T ( u n ) h T ( u ) ) u n d x + R 3 h T ( u ) ( u n u ) d x R 3 ( h T ( u n ) h T ( u ) ) u n d x + R 3 ( h T ( u ) ) 2 d x 1 2 u n u L 2 .

From the Hölder inequality, one has

(2.27) R 3 ( ϕ u n u n 2 ϕ u u 2 ) d x R 3 ϕ u n u n + u u n u d x + R 3 ϕ u n ϕ u u 2 d x ϕ u n L 6 ( R 3 ) u n + u L 2 ( R 3 ) u n u L 3 ( R 3 ) + ϕ u n ϕ u L 6 ( R 3 ) u L 12 5 ( R 3 ) 2

and

(2.28) R 3 ( ϕ u n 2 u n 2 ϕ u 2 u 2 ) d x R 3 ϕ u n 2 u n + u u n u d x + R 3 ϕ u n + ϕ u ϕ u n ϕ n u 2 d x ϕ u n L 6 ( R 3 ) 2 u n + u L 3 ( R 3 ) u n u L 3 ( R 3 ) + ϕ u n ϕ u L 6 ( R 3 ) ϕ u n + ϕ u L 6 ( R 3 ) u L 3 ( R 3 ) 2 .

By combining (2.24)–(2.28) with Lemma (2.5), up to a subsequence, we obtain

(2.29) J λ , T ( u n ) , u n J λ , T ( u ) , u = R 3 ( u n 2 u 2 ) d x + R 3 V ( x ) ( u n 2 u 2 ) d x R 3 2 ω ( ϕ u n u n 2 ϕ u u 2 ) d x R 3 ( ϕ u n 2 u n 2 ϕ u 2 u 2 ) d x R 3 λ ( h T ( u n ) u n h T ( u ) u ) d x R 3 ( u n 6 u 6 ) d x = R 3 ν n 2 d x + V ( x ) R 3 ν n 2 d x R 3 ν n 6 d x + o ( 1 ) , as n .

It is easy to know that J λ , T ( u n ) , u n J λ , T ( u ) , u = 0 , we assume that

R 3 ν n 2 d x + V ( x ) R 3 ν n 2 d x b , R 3 ν n 6 d x b ,

where b is a nonnegative constant.

We assert that b = 0 . If b 0 , under the definition of S , we obtain

R 3 ν n 2 d x S R 3 ν n 2 d x 1 3 .

Then

R 3 ν n 2 d x + V ( x ) R 3 ν n 2 d x S R 3 ν n 2 d x 1 3 ,

which means b S b 1 3 . Thus, b S 3 2 .

From ϕ u 0 and b S 3 2 , we know

c = lim n J λ , T ( u n ) lim n 1 2 R 3 ( ν n 2 + V ( x ) ν n 2 ) d x 1 6 R 3 ν n 6 d x = 1 3 b 1 3 S 3 2 ,

which is a contradiction. Hence, b = 0 . Thus,

0 ν n = R 3 ( ν n 2 + V ( x ) ν n 2 ) d x 1 2 0 .

Lemma 2.7

c λ , T < 1 3 S 3 2 , where c λ , T and S are defined in (2.14) and Lemma 2.6, respectively.

Proof

Let φ C 0 is a cut-off function, that is, there exists R > 0 such that φ B R = 1 , 0 φ 1 in B 2 R and supp φ B 2 R . Let ε > 0 and define u ε w ε φ where w ε D 1 , 2 ( R 3 ) is the Talenti function w ε ( x ) = ( 3 ε 2 ) 1 4 ( ε 2 + x 2 ) 1 2 . From estimates obtained in [28], we obtain if ε is small enough,

(2.30) R 3 u ε 2 d x = S 3 2 + O ( ε ) ,

(2.31) R 3 u ε 6 d x = S 3 2 + O ( ε 3 ) ,

(2.32) R 3 u ε q d x = O ( ε q 2 ) , q [ 2 , 3 ) , O ( ε q 2 ln ε ) , q = 3 , O ( ε 6 q 2 ) , q ( 3 , 6 ) .

Since for any ε > 0 , lim t J λ , T ( t u ε ) = . We can assume there exists t ε 0 such that sup t 0 J λ , T ( t u ε ) = J λ , T ( t ε u ε ) , and without loss of generality, let t ε C 0 > 0 . In fact, suppose there exists a sequence ε n R + such that lim n t ε n = 0 and J λ , T ( t ε n u ε n ) = sup t 0 J λ , T ( t u ε ) . We can deduce 0 < α < c λ , T lim n J λ , T ( t ε n u ε n ) = 0 , which is a contradiction.

Moreover, we claim that { t ε } ε > 0 is bounded from above. Otherwise, there exists a subsequence t ε n such that lim n t ε n = + . From (2.8), (2.12), (2.30)–(2.32), and Lemma (2.1), we obtain

0 < c λ , T J λ , T ( t ε n u ε n ) t ε n 2 2 R 3 ( u ε n 2 + V ( x ) u ε n 2 ) d x t ε n 2 R 3 ω ϕ t ε n u ε n 2 d x R 3 λ H T ( t ε n u ε n ) d x t ε n 6 6 R 3 u ε n 6 d x t ε n 2 2 R 3 ( u ε n 2 + V ( x ) u ε n 2 ) d x t ε n 2 R 3 ω ϕ t ε n u ε n 2 d x + t ε n 2 R 3 C M u ε n 2 d x t ε n 4 R 3 λ M u ε n 4 d x t ε n 6 6 R 3 u ε n 6 d x C 1 t ε n 2 C 2 t ε n 4 C 3 t ε n 6 , as n .

Therefore, 0 < is a contradiction.

Let

ϱ ( t ) = t 2 2 R 3 u ε 2 d x t 6 6 R 3 u ε 6 d x .

It is easy to know that

(2.33) sup t 0 ϱ ( t ) = 1 3 S 3 2 + O ( ε ) .

According to assumption ( V 2 ) , for x < r , there exists ξ > 0 such that

(2.34) V ( x ) ξ .

Form (2.12) and (2.30)–(2.34), we obtain

J λ , T ( t ε u ε ) = t ε 2 2 R 3 u ε 2 d x + t ε 2 2 R 3 V ( x ) u ε 2 d x 3 t ε 2 4 R 3 ω ϕ t ε u ε u ε 2 d x t ε 2 4 R 3 ϕ t ε u ε 2 u ε 2 d x 1 16 π R 3 ϕ t ε u ε 2 d x R 3 λ H T ( t ε u ε ) d x t ε 6 6 R 3 u ε 6 d x t ε 2 2 R 3 u ε 2 d x + t ε 2 2 R 3 V ( x ) u ε 2 d x 3 t ε 2 4 R 3 ω ϕ t ε u ε u ε 2 d x λ M t ε 4 R 3 u ε 4 d x + λ C M t ε 2 R 3 u ε 2 d x t ε 6 6 R 3 u ε 6 d x sup t 0 ϱ ( t ) + t ε 2 2 ξ R 3 u ε 2 d x 3 t ε 2 4 R 3 ω ϕ t ε u ε u ε 2 d x λ M t ε 4 R 3 u ε 4 d x + λ C M t ε 2 R 3 u ε 2 d x sup t 0 ϱ ( t ) + C u ε 2 2 + C u ε 12 5 2 λ M C u ε 4 4 1 3 S 3 2 + C O ( ε ) λ M C O ( ε ) .

When M large enough, we know C O ( ε ) λ M C O ( ε ) for small enough ε > 0 .

Theorem 2.8

Assume λ > 0 and T > 0 , problem (2.7) has a nontrivial solution u λ , T with J λ , T ( u λ , T ) = c λ , T .

Proof

First, we know that the function J λ , T satisfies Lemma 2.3, that is, the geometric structure of the Mountain Pass Theorem, so we can obtain a ( P S ) sequence. Second, because of Lemma 2.6, functional J λ , T satisfies the ( P S ) condition. According to the Mountain Pass Theorem, there exists a critical point u λ , T E . Moreover, J λ , T = c λ , T α > 0 = J ( 0 ) , so u λ , T is a nontrivial solution.□

3 Proof of the Theorem 1.1

In this section, we will prove Theorem 1.1. First, we prove that the solution of problem (2.7) satisfied u λ , T T , which means that the solution at this time is the solution of problem (1.1). The method is similar to [17,29] by using the Nash-Moser method.

Lemma 3.1

If u is a critical point of J λ , T , then u L ( R 3 ) and

u C 0 1 2 ( ζ 1 ) ζ ζ ( ζ 1 ) 2 [ ( λ C T + α ( ε , u ) ) ( 1 + u 2 ) 2 + λ C T u 6 p 2 ] 1 2 ( ζ 1 ) u 6 κ ,

where C 0 > 0 and κ 1 are constants independent of λ and T , ζ = 8 p 2 .

Proof

Assume A k = { x R 3 : u s 1 k } , B k = R 3 A k , where s > 1 , k > 0 . Let

(3.1) u k = u u 2 ( s 1 ) , x A k , k 2 u , x B k

and

(3.2) χ k = u u s 1 , x A k , k u , x B k .

It is easy to know that u k u 2 s 1 if u k , χ k E , and χ k 2 = u u k u 2 s . Through direct calculation, the following formulas can be obtained:

(3.3) u k = ( 2 s 1 ) u 2 s 2 u , x A k , k 2 u , x B k ,

(3.4) χ k = s u s 1 u , x A k , k u , x B k ,

and

(3.5) R 3 ( χ k 2 u u k ) d x = ( s 1 ) 2 A k u 2 ( s 1 ) u 2 d x .

Due to its definition, we obtain

(3.6) R 3 u u k d x = ( 2 s 1 ) A k u 2 ( s 1 ) u 2 d x + k 2 B k u 2 d x ( 2 s 1 ) A k u 2 ( s 1 ) u 2 d x .

From (3.5) and (3.6), we obtain R 3 u u k d x 0 and

(3.7) R 3 χ k 2 d x s 2 R 3 u u k d x .

Since u is the critical point, let u k be a test function defined in (2.9), we can deduce

(3.8) R 3 ( u u k + V ( x ) u u k 2 ω ϕ u u u k ϕ u 2 u u k ) d x = R 3 λ h T ( u ) u k d x + R 3 u 4 u u k d x .

By combining (3.7) with Lemma 2.1, it is easy to obtain

R 3 χ k 2 d x s 2 R 3 λ h T ( u ) u k d x + R 3 u 4 u u k d x .

By a version of the Brezis-Kato lemma as done in [32, Lemma 2.5], for any ε > 0 , we can find α ( ε , u ) such that

R 3 u 4 χ k 2 d x ε R 3 χ k 2 d x + α ( ε , u ) R 3 χ k 2 d x .

Let ε = 1 2 s 2 , from χ k 2 = u u k and ( h 3 ) , we deduce

(3.9) R 3 χ k 2 d x 2 s 2 R 3 λ h T ( u ) u k d x + α ( ε , u ) R 3 χ k 2 d x ,

and

(3.10) h T ( u ) u k C T χ k 2 + C T u p 2 χ k 2 .

From the Sobolev embedding theorem, the Hölder inequality, and (3.9)–(3.10), we obtain

(3.11) A k χ k 6 d x 1 3 S 1 R 3 χ k 2 d x S 1 2 s 2 R 3 λ ( C T χ k 2 + C T u p 2 χ k 2 ) d x + α ( ε , u ) R 3 χ k 2 d x S 1 2 s 2 [ ( λ C T + α ( ε , u ) ) χ k 2 2 + λ C T u 6 p 2 χ k 2 q 2 ] ,

where q = 6 8 p 3 2 , 3 and S defined in Lemma 2.6. Due to χ k u s and χ k = u s for x A k , together with (3.11), we can obtain

(3.12) A k u 6 s d x 1 3 S 1 2 s 2 [ ( λ C T + α ( ε , u ) ) u 2 s 2 s + λ C T u 6 p 2 u 2 s q 2 s ] .

Through the interpolation inequality, we know u 2 s u 2 1 σ u 2 q s σ , where σ ( 0 , 1 ) and 1 2 s = 1 σ 2 + σ 2 s q , so σ = q ( s 1 ) q s 1 . Moreover, since 2 s ( 1 σ ) = 2 + 2 ( 1 s ) q s 1 < 2 , we know

(3.13) u 2 s 2 s u 2 2 s ( 1 σ ) u 2 s q 2 s σ ( 1 + u 2 ) 2 u 2 s q 2 s σ .

When k , together with (3.12)and (3.13), we deduce

(3.14) u 6 s ( S 1 2 s 2 ) 1 2 s [ ( λ C T + α ( ε , u ) ) ( 1 + u 2 ) 2 u 2 s q 2 s σ + λ C T u 6 p 2 u 2 s q 2 s ] 1 2 s C 0 1 2 s s 1 s [ ( λ C T + α ( ε , u ) ) ( 1 + u 2 ) 2 + λ C T u 6 p 2 ] 1 2 s u 2 s q κ ,

where κ { σ , 1 } and C 0 = max { 2 S 1 , 1 } . Let ζ = 6 2 q , then ζ ( 1 , 2 ) . Now we use j iterations by letting s j = ζ j in (3.14), and then we obtain

(3.15) u 6 ζ j C 0 1 2 j = 1 1 ζ j ζ j = 1 j ζ j [ ( λ C T + α ) ( 1 + u 2 ) 2 + λ C T u 6 p 2 ] 1 2 j = 1 1 ζ j u 6 κ 1 κ j ,

where σ j = q ( ζ j 1 ) q ζ j 1 < 1 , κ j { σ j , 1 } 1 . From a direct calculation, we obtain

j = 1 1 ζ j = 1 ζ 1 , j = 1 j ζ j = ζ ( ζ 1 ) 2 .

The estimates of u will be divided into two cases.

  1. When u 6 1 , then u 6 κ 1 κ j u 6 . If j in equation (3.15), we can obtain

    (3.16) u C 0 1 2 ( ζ 1 ) ζ ζ ( ζ 1 ) 2 [ ( λ C T + α ( ε , u ) ) ( 1 + u 2 ) 2 + λ C T u 6 p 2 ] 1 2 ( ζ 1 ) u 6 .

  2. When u 6 < 1 , by σ j = q ( ζ j 1 ) q ζ j 1 1 1 ζ j and κ j { σ j , 1 } , for any j N , we deduce

    0 < σ 1 σ 2 σ j κ 1 κ 2 κ j .

    For s ( 0 , 1 ) , we know that ln ( 1 s ) s s 2 2 ( 1 s ) 2 . Then we can easily obtain

    i = 1 j ln κ i i = 1 j ln σ i i = 1 j 1 ζ i 1 2 i = 1 j 1 ( ζ i 1 ) 2 .

    From a direct calculation, we obtain

    i = 1 j 1 ( ζ i 1 ) 2 ζ 2 ( ζ 2 1 ) ( ζ 1 ) 2 .

    So

    i = 1 ln κ i 1 ζ 1 ζ 2 2 ( ζ 2 1 ) ( ζ 1 ) 2 θ .

    Therefore, κ 1 κ 2 κ j e θ for any j N . Due to u 6 < 1 , then u 6 κ 1 κ 2 κ j u 6 e θ . If j in equation (3.15), we can obtain

    (3.17) u C 0 1 2 ( ζ 1 ) ζ ζ ( ζ 1 ) 2 [ ( λ C T + α ( ε , u ) ) ( 1 + u 2 ) 2 + λ C T u 6 p 2 ] 1 2 ( ζ 1 ) u 6 e θ .

By combining with the two cases, we know that the proof is complete if κ = 1 or κ = e θ 1 .□

Proof of Theorem 1.1

Let u C 0 ( R 3 ) and u ( x ) 0 , then from the definition of h T ( t ) in (2.6), we know that H T ( t u ) = 0 for any t > 0 . Hence,

(3.18) J λ , T ( t u ) = t 2 2 R 3 ( u 2 + V ( x ) u 2 ) d x t 2 R 3 ω ϕ t u u 2 d x t 2 2 R 3 ϕ t u 2 u 2 1 8 π R 3 ϕ t u 2 d x β 16 π R 3 ϕ t u 4 d x t 6 6 R 3 u 6 d x .

It shows that J λ , T ( t u ) for t + . Then we can find a t 0 > 0 such that J λ , T ( t 0 u ) < 0 . we can assume γ ( ) = t t 0 u , t [ 0 , 1 ] , so γ ( t ) Γ . Because H T ( u ) = 0 , as t [ 0 , 1 ] , we obtain

(3.19) c λ , T max t [ 0 , 1 ] J λ , T ( γ ( t ) ) max t 0 t 2 2 R 3 ( u 2 + V ( x ) u 2 ) d x t 2 R 3 ω ϕ t u u 2 d x t 6 6 R 3 u 6 d x . D > 0 ,

where D is constant independent of λ and T . From Theorem 2.8, ( h 4 ) and ( V 1 )–( V 2 ), we know

(3.20) 4 D 4 c λ , T 4 J λ , T J λ , T ( u λ , T ) , u λ , T = R 3 u λ , T 2 + V ( x ) u λ , T 2 d x + β 4 π R 3 ϕ u λ , T 4 d x + R 3 ϕ u λ , T 2 u λ , T 2 d x + R 3 λ ( h T ( u λ , T ) u λ , T 4 H T ( u λ , T ) ) d x + 1 3 R 3 u λ , T 6 d x R 3 u λ , T 2 + V ( x ) u λ , T 2 d x λ μ R 3 u λ , T 2 d x 1 2 u λ , T 2 + V 0 2 λ μ u λ , T 2 2 .

We can find a λ 0 such that V 0 2 λ 0 μ > 0 . Then from (3.20), u λ , T 8 D . Hence, we deduce

u λ , T 2 C 5 , u λ , T 6 2 C 6 ,

where C 5 , C 6 > 0 independent of λ , T .

From Lemma (3.1), we obtain

u λ , T C 0 1 2 ( ζ 1 ) ζ ζ ( ζ 1 ) 2 [ ( λ C T + α ( ε , u ) ) ( 1 + C 5 ) 2 + λ C T C 6 p 2 ] 1 2 ( ζ 1 ) C 6 κ .

So, we can choose T > 0 large enough such that

C 0 1 2 ( ζ 1 ) ζ ζ ( ζ 1 ) 2 [ α ( ε , u ) ( 1 + C 5 ) 2 ] 1 2 ( ζ 1 ) C 6 κ T 2 .

Since C T and C T are fixed constants for the aforementioned T , we can choose λ 1 < λ 0 such that

u λ , T C 0 1 2 ( ζ 1 ) ζ ζ ( ζ 1 ) 2 [ ( λ 1 C T + α ( ε , u ) ) ( 1 + C 5 ) 2 + λ 1 C T C 6 p 2 ] 1 2 ( ζ 1 ) C 6 κ T .

Then, for λ ( 0 , λ 1 ) , we can obtain u λ , T T , u λ , T is also a solution for problem (1.1).□

4 Proof of the Theorem 1.4

Proof

When β = 0 , the proof of Theorem 1.4 is similar with the proof of Theorem 1.1 step by step, we omit the details.□



Acknowledgments

We are very grateful to the anonymous referees for their knowledgeable reports, which helped us to improve our manuscript.

  1. Funding information: C. M. He was supported by the Innovative Project of Chongqing Technology and Business University (CYS22697), L. Li was supported by the Research Fund of National Natural Science Foundation of China (No. 11861046), the Chongqing Municipal Education Commission (No. KJQN20190081), and the Chongqing Technology and Business University (No. CTBUZDPTTD201909).

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

  3. Data availability statement: Data sharing not applicable to this article as no data sets were generated or analyzed during the current study.

References

[1] V. Benci, D. Fortunato, A. Masiello, and L. Pisani, Solitons and the electromagnetic field, Math. Z. 232 (1999), no. 1, 73–102. 10.1007/PL00004759Suche in Google Scholar

[2] M. Born, On the quantum theory of the electromagnetic field, Proc. R. Soc. Lond. Ser. 143 (1934), no. 849, 410–437. 10.1098/rspa.1934.0010Suche in Google Scholar

[3] M. Born and L. Infeld, Foundations of the new field theory, Proc. R. Soc. Lond. Ser. A Math. Phys. Eng. Sci. 144 (1934), no. 852, 425–451. 10.1038/1321004b0Suche in Google Scholar

[4] P. C. Carriaaao, P. L. Cunha, and O. H. Miyagaki, Positive ground state solutions for the critical Klein-Gordon-Maxwell system with potentials, Nonlinear Anal. 75 (2012), no. 10, 4068–4078. 10.1016/j.na.2012.02.023Suche in Google Scholar

[5] P. C. Carrião, P. L. Cunha, and O. H. Miyagaki, Existence results for the Klein-Gordon-Maxwell equations in higher dimensions with critical exponents, Commun. Pure Appl. Anal. 10 (2011), no. 2, 709–718. 10.3934/cpaa.2011.10.709Suche in Google Scholar

[6] D. Cassani, Existence and non-existence of solitary waves for the critical Klein-Gordon equation coupled with Maxwellas equations, Nonlinear Anal. 58 (2004), no. 7–8, 733–747. 10.1016/j.na.2003.05.001Suche in Google Scholar

[7] G. F. Che and H. B. Chen, Infinitely many solutions for the Klein-Gordon equation with sublinear nonlinearity coupled with Born-Infeld theory, Bull. Iranian Math. Soc. 46 (2020), no. 4, 1083–1100. 10.1007/s41980-019-00314-3Suche in Google Scholar

[8] S. J. Chen and L. Li, Multiple solutions for the nonhomogeneous Klein-Gordon equation coupled with Born-Infeld theory on R3, J. Math. Anal. Appl. 400 (2013), no. 2, 517–524. 10.1016/j.jmaa.2012.10.057Suche in Google Scholar

[9] S. J. Chen and S. Z. Song, The existence of multiple solutions for the Klein-Gordon equation with concave and convex nonlinearities coupled with Born-Infeld theory on R3, Nonlinear Anal. Real World Appl. 38 (2017), 78–95. 10.1016/j.nonrwa.2017.04.008Suche in Google Scholar

[10] S. T. Chen, A. Fiscella, P. Pucci, and X. H. Tang, Semiclassical ground state solutions for critical Schrödinger-Poisson systems with lower perturbations, J. Differential Equations, 268 (2020), no. 6, 2672–2716. 10.1016/j.jde.2019.09.041Suche in Google Scholar

[11] Z. Chen, X. H. Tang, L. Qin, and D. D. Qin, Improved results for Klein-Gorden-Maxwell systems with critical growth, Appl. Math. Lett. 91 (2019), 158–164. 10.1016/j.aml.2018.12.015Suche in Google Scholar

[12] J. M. Combes, R. Schrader, and R. Seiler, Classical bounds and limits for energy distributions of Hamilton operators in electromagnetic fields, Ann Phys. 111 (1978), no. 1, 1–18. 10.1016/0003-4916(78)90221-XSuche in Google Scholar

[13] P. d’Avenia and L. Pisani, Nonlinear Klein-Gordon equations coupled with Born-Infeld type equations, Electron. J. Differential Equations 26 (2002), 13. Suche in Google Scholar

[14] B. Felsager and B. R. Holstenim Geometry, Particles and Fields, J. Amer. J. Phys. 52 (1997), 573.10.1007/978-1-4612-0631-6Suche in Google Scholar

[15] D. Fortunato, L. Orsina, and L. Pisani, Born-Infeld type equations for electrostatic fields, J. Math. Phys. 43 (2002), no. 11, 5698–5706. 10.1063/1.1508433Suche in Google Scholar

[16] C. M. He, L. Li, S. J. Chen, and D. O’Regan, Ground state solution for the nonlinear Klein-Gordon equation coupled with Born-Infeld theory with critical exponents, Anal. Math. Phys. 12 (2022), no. 2, Paper No. 48, 17. 10.1007/s13324-022-00661-1Suche in Google Scholar

[17] Y. H. Li and Q. Geng, The existence of nontrivial solution to a class of nonlinear Kirchhoff equations without any growth and Ambrosetti-Rabinowitz conditions, Appl. Math. Lett. 96 (2019), 153–158. 10.1016/j.aml.2019.04.027Suche in Google Scholar

[18] S. H. Liang, P. Pucci, and B. L. Zhang, Multiple solutions for critical Choquard-Kirchhoff type equations, Adv. Nonlinear Anal. 10 (2021), no. 1, 400–419. 10.1515/anona-2020-0119Suche in Google Scholar

[19] J. J. Liu and C. Ji, Concentration results for a magnetic Schrödinger-Poisson system with critical growth, Adv. Nonlinear Anal. 10 (2021), no. 1, 775–798. 10.1515/anona-2020-0159Suche in Google Scholar

[20] D. Mugnai, Coupled Klein-Gordon and Born-Infeld-type equations: looking for solitary waves, Proc. R. Soc. Lond. Ser. A Math. Phys. Eng. Sci. 460 (2004), no. 2045, 1519–1527. 10.1098/rspa.2003.1267Suche in Google Scholar

[21] P. Pucci, M. Q. Xiang, and B. L. Zhang, Existence results for Schrödinger-Choquard-Kirchhoff equations involving the fractional p-Laplacian, Adv. Calc. Var. 12 (2019), no. 3, 253–275. 10.1515/acv-2016-0049Suche in Google Scholar

[22] P. H. Rabinowitz, On a class of nonlinear Schrödinger equations, Z. Angew. Math. Phys. 43 (1992), no. 2, 270–291. 10.1007/BF00946631Suche in Google Scholar

[23] X. H. Tang, L. X. Wen, and S. T. Chen, On critical Klein-Gordon-Maxwell systems with super-linear nonlinearities, Nonlinear Anal. 196 (2020), no. 21, 111771. 10.1016/j.na.2020.111771Suche in Google Scholar

[24] K. M. Teng and K. J. Zhang, Existence of solitary wave solutions for the nonlinear Klein-Gordon equation coupled with Born-Infeld theory with critical Sobolev exponent, Nonlinear Anal. 74 (2011), no. 12, 4241–4251. 10.1016/j.na.2011.04.002Suche in Google Scholar

[25] F. Z. Wang, Solitary waves for the Klein-Gordon-Maxwell system with critical exponent, Nonlinear Anal. 74 (2011), no. 3, 827–835. 10.1016/j.na.2010.09.033Suche in Google Scholar

[26] F. Z. Wang, Solitary waves for the coupled nonlinear Klein-Gordon and Born-Infeld type equations, Electron. J. Differential Equations 12 (2012), 82. Suche in Google Scholar

[27] L. X. Wen, X. H. Tang, and S. T. Chen, Infinitely many solutions and least energy solutions for Klein-Gordon equation coupled with Born-Infeld theory, Complex Var. Elliptic Equ. 64 (2019), no. 12, 2077–2090. 10.1080/17476933.2019.1572124Suche in Google Scholar

[28] M. Willem, Minimax Theorems, Birkhäuser Boston, Inc., Boston, MA, 1996. 10.1007/978-1-4612-4146-1Suche in Google Scholar

[29] J. Yang, H. B. Chen, and S. L. Liu, The existence of nontrivial solution of a class of Schrödinger-Bopp-Podolsky system with critical growth, Bound. Value Probl. 2020 (2020), Paper No. 144, 16. 10.1186/s13661-020-01442-0Suche in Google Scholar

[30] Y. Yu, Solitary waves for nonlinear Klein-Gordon equations coupled with Born-Infeld theory, Ann. Inst. H. Poincaré Anal. Non Linéaire, 27 (2010), no. 1, 351–376. 10.1016/j.anihpc.2009.11.001Suche in Google Scholar

[31] J. Zhang, Solutions to the critical Klein-Gordon-Maxwell system with external potential, J. Math. Anal. Appl. 455 (2017), no. 2, 1152–1177. 10.1016/j.jmaa.2017.06.028Suche in Google Scholar

[32] J. J. Zhang, D. G. Costa, and J. M. do Ó, Semiclassical states of p-Laplacian equations with a general nonlinearity in critical case, J. Math. Phys. 57 (2016), no. 7, 071504, 12. 10.1063/1.4959220Suche in Google Scholar

[33] W. M. Zou and M. Schechter, Critical Point Theory and Its Applications, Springer, New York, 2006. Suche in Google Scholar

Received: 2022-01-26
Revised: 2022-09-25
Accepted: 2023-01-01
Published Online: 2023-03-03

© 2023 the author(s), published by De Gruyter

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

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  53. Existence and concentration of solutions to Kirchhoff-type equations in ℝ2 with steep potential well vanishing at infinity and exponential critical nonlinearities
  54. Multiplicity results for fractional Schrödinger-Kirchhoff systems involving critical nonlinearities
  55. On double phase Kirchhoff problems with singular nonlinearity
  56. Estimates for eigenvalues of the Neumann and Steklov problems
  57. Nodal solutions with a prescribed number of nodes for the Kirchhoff-type problem with an asymptotically cubic term
  58. Dirichlet problems involving the Hardy-Leray operators with multiple polars
  59. Incompressible limit for compressible viscoelastic flows with large velocity
  60. Characterizations for the genuine Calderón-Zygmund operators and commutators on generalized Orlicz-Morrey spaces
  61. Non-local gradients in bounded domains motivated by continuum mechanics: Fundamental theorem of calculus and embeddings
  62. Noncoercive parabolic obstacle problems
  63. Touchdown solutions in general MEMS models
  64. Existence and nonexistence of nontrivial solutions for the Schrödinger-Poisson system with zero mass potential
  65. Short-time existence of a quasi-stationary fluid–structure interaction problem for plaque growth
  66. Fine bounds for best constants of fractional subcritical Sobolev embeddings and applications to nonlocal PDEs
  67. Symmetries of Ricci flows
  68. Asymptotic behavior of solutions of a second-order nonlinear discrete equation of Emden-Fowler type
  69. On the topological gradient method for an inverse problem resolution
  70. Supersolutions to nonautonomous Choquard equations in general domains
  71. Uniform complex time heat Kernel estimates without Gaussian bounds
  72. Global existence for time-dependent damped wave equations with nonlinear memory
  73. Normalized solutions for a critical fractional Choquard equation with a nonlocal perturbation
  74. Reversed Hardy-Littlewood-Sobolev inequalities with weights on the Heisenberg group
  75. Lamé system with weak damping and nonlinear time-varying delay
  76. Global well posedness for the semilinear edge-degenerate parabolic equations on singular manifolds
  77. Blowup in L1(Ω)-norm and global existence for time-fractional diffusion equations with polynomial semilinear terms
  78. Boundary regularity results for minimisers of convex functionals with (p, q)-growth
  79. Parametric singular double phase Dirichlet problems
  80. Special Issue on Nonlinear analysis: Perspectives and synergies
  81. Editorial to Special issue “Nonlinear analysis: Perspectives and synergies”
  82. Identification of discontinuous parameters in double phase obstacle problems
  83. Global boundedness to a 3D chemotaxis-Stokes system with porous medium cell diffusion and general sensitivity
  84. On regular solutions to compressible radiation hydrodynamic equations with far field vacuum
  85. On Cauchy problem for fractional parabolic-elliptic Keller-Segel model
  86. The evolution of immersed locally convex plane curves driven by anisotropic curvature flow
  87. Stability of combination of rarefaction waves with viscous contact wave for compressible Navier-Stokes equations with temperature-dependent transport coefficients and large data
  88. On concave perturbations of a periodic elliptic problem in R2 involving critical exponential growth
  89. Existence of solutions for a double-phase variable exponent equation without the Ambrosetti-Rabinowitz condition
Heruntergeladen am 16.9.2025 von https://www.degruyterbrill.com/document/doi/10.1515/anona-2022-0282/html
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