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Article

Infinitely Many Solutions for Fractional p-Laplacian Schrödinger–Kirchhoff Type Equations with Symmetric Variable-Order

1
College of Science, Hohai University, Nanjing 210098, China
2
College of Science, Zhongyuan University of Technology, Zhengzhou 450007, China
3
Center for Mathematics, Computing and Cognition, Federal University of ABC, Avenida dos Estados, 5001, Bairro Bangu, Santo André 09210-580, SP, Brazil
*
Author to whom correspondence should be addressed.
Symmetry 2021, 13(8), 1393; https://doi.org/10.3390/sym13081393
Submission received: 26 April 2021 / Revised: 25 July 2021 / Accepted: 28 July 2021 / Published: 31 July 2021

Abstract

:
In this article, we first obtain an embedding result for the Sobolev spaces with variable-order, and then we consider the following Schrödinger–Kirchhoff type equations a + b Ω × Ω | ξ ( x ) ξ ( y ) | p | x y | N + p s ( x , y ) d x d y p 1 ( Δ ) p s ( · ) ξ + λ V ( x ) | ξ | p 2 ξ = f ( x , ξ ) , x Ω , ξ = 0 , x Ω , where Ω is a bounded Lipschitz domain in R N , 1 < p < + , a , b > 0 are constants, s ( · ) : R N × R N ( 0 , 1 ) is a continuous and symmetric function with N > s ( x , y ) p for all ( x , y ) Ω × Ω , λ > 0 is a parameter, ( Δ ) p s ( · ) is a fractional p-Laplace operator with variable-order, V ( x ) : Ω R + is a potential function, and f ( x , ξ ) : Ω × R N R is a continuous nonlinearity function. Assuming that V and f satisfy some reasonable hypotheses, we obtain the existence of infinitely many solutions for the above problem by using the fountain theorem and symmetric mountain pass theorem without the Ambrosetti–Rabinowitz ((AR) for short) condition.

1. Introduction and the Main Results

In this article, we investigate the following Schrödinger–Kirchhoff type equations
( P v ) : a + b Ω × Ω | ξ ( x ) ξ ( y ) | p | x y | N + p s ( x , y ) d x d y p 1 ( Δ ) p s ( · ) ξ + λ V ( x ) | ξ | p 2 ξ = f ( x , ξ ) , x Ω , ξ = 0 , x Ω ,
where Ω is a bounded Lipschitz domain in R N and 1 < p < + , s ( · ) : R N × R N ( 0 , 1 ) is a continuous symmetric function with N > s ( x , y ) p for all ( x , y ) Ω × Ω , ( Δ ) p s ( · ) is the fractional p-Laplace operator with variable-order, defined as
( Δ ) p s ( · ) ξ ( x ) : = P . V . Ω | ξ ( x ) ξ ( y ) | p 2 ( ξ ( x ) ξ ( y ) ) | x y | N + p s ( x , y ) d y , x Ω ,
where ξ C 0 ( Ω ) , and P . V . stands for the Cauchy principal value. Since s ( · ) is a continuous function, ( Δ ) p s ( · ) is called fractional Laplace operator with variable-order. The usual fractional p-Laplace operator has been studied extensively by many scholars, see [1,2,3,4,5,6].
For the variable-order fractional and some important results, we refer to [7,8,9,10,11,12]. The fractional derivatives of variable-order were introduced by Lorenzo et al. in [7]. Subsequently, Samko et al. generalized the Riemann–Liouville fractional integration and differentiation to the fractional operator with variable-order, see [9,10] for more details with respect to this topic.
When p = 2 , the fractional Laplace operator with variable-order was studied by Xiang et al. in [11], they investigated the following Laplacian equations
( ) s ( · ) ξ + λ V ( x ) ξ = α | ξ | p ( x ) 2 ξ + β | ξ | q ( x ) 2 ξ , x Ω , ξ = 0 , x R \ Ω ,
where ( Δ ) s ( · ) is the fractional Laplacian operator. First of all, they proved the embedding theorem of variable-order fractional Sobolev space, and then they obtained a multiplicity result for a Schrödinger equation via variational methods.
Note that we also mention the work by Wang et al. in [12]; they also studied the fractional Laplace operator with variable-order, as follows
M ( [ ξ ] s ( · ) 2 ) ( ) s ( · ) ξ + V ( x ) ξ = λ | ξ | p ( x ) 2 ξ + μ | ξ | q ( x ) 2 ξ , x Ω , ξ = 0 , x R \ Ω ,
where M is a model of Kirchhoff coefficient, and infinitely many solutions were obtained by using four different critical point theorems. The main feature for this kind of Kirchhoff-type problem is that M could be zero at zero.
In recent decades, many scholars have extensively studied the existence of results for classical Schrödinger equations and fractional Schrödinger equations under reasonable assumptions of V and f. We refer the reader to [13,14,15,16,17]. Nyamoradi et al. in [15] studied the Schrödinger–Kirchhoff type equations by variational methods. Note that Teng in [16] established the existence of high or small energy solutions by applying a variant fountain theorem. Especially, in [17] César E. Torres Ledesma studied the existence of multiple solutions for Schrödinger–Kirchhoff type involving the non-homogeneous fractional p-Laplacian, which V and f are under some weaker assumptions.
On the other hand, the Kirchhoff equation was introduced by Kirchhoff in [18]. Kirchhoff proposed the following model
ρ 2 ξ t 2 p 0 h + E 2 L 0 L ξ t 2 d x 2 ξ x 2 = 0 ,
where ρ , p 0 , h , E , L are constants with respect to some physical meanings, respectively. We call ( P v ) a problem of Kirchhoff type because there is the Kirchhoff term
a + b Ω × Ω | ξ ( x ) ξ ( y ) | p | x y | N + p s ( x , y ) d x d y ,
which not only makes the study of ( P v ) interesting but also becomes more delicate and causes some mathematical difficulties. The literature on Kirchhoff type problems about the existence and multiplicity of solutions is quite large; here we just list a few, for example, [4,6,17,19,20,21,22,23,24] for further details. It is worth pointing out that if a > 0 , b 0 , M ( t ) = a + b t m is non-degenerate Kirchhoff type equations, for example, see [23,24]; if a = 0 , b > 0 , M ( t ) = a + b t m is degenerate Kirchhoff type equations, such as, see [6,20]. The fractional Kirchhoff type equation regarding non-local integro-differential operator was first introduced in [19] by Fiscella et al., and they studied the non-negative solutions for this kind of equation as follows
M ( [ ξ ] s 2 ) = f ( x , ξ ) , in Ω , ξ = 0 , in R N \ Ω ,
where Ω is a bounded Lipschitz domain of R N . Moreover, in [20], Molica et al. investigated a kind of nonlocal fractional Kirchhoff type equations, and three solutions were obtained by applying the critical points theorem.
Indeed, the works of literature on Kirchhoff equations, Schrödinger equations, and their applications are quite large. Kirchhoff equations model several physical and biological systems, for example, population density, see [25,26,27] for some related works. On the other hand, many scholars are interested in Schrödinger equations, which describe the dynamic behavior of particles in quantum mechanics, see [28], and the standing wave solutions, see [29]. Moreover, fractional Schrödinger–Kirchhoff type equations involving an external magnetic potential were studied in [30].
As is known, the (AR) condition plays a crucial role to guarantee that the Palais–Smale sequences are bounded. In the famous paper [31], Ambrosetti and Rabinowitz introduced the well-known (AR) condition, that is, there exist constants p 0 2 < μ 0 and 0 < M 0 such that
0 < μ 0 F ( x , ξ ) f ( x , ξ ) ξ , for x R N , | ξ | M 0 ,
where F ( x , ξ ) = 0 ξ f ( x , t ) d t . In [32], Servadei et al. obtained the existence and multiplicity of nontrivial solutions and showed that the verification of the Palais–Smale compactness condition depends on the (AR) condition. However, there are a lot of functions where the (AR) condition is not satisfied, an example of such function is
f ( x , ξ ) = | ξ | p 2 ξ log ( 1 + | ξ | ) .
For this kind of problem, many people have attached much importance to finding new, reasonable conditions instead of the (AR) condition, see, for instance, [5,6,33,34].
Motivated by the above cited works, we find that there are some papers on Kirchhoff equations or Schrödinger equations involving the fractional p-Laplace operator; however, there are no results for Schrödinger–Kirchhoff type equations driven by the fractional p-Laplace operator with variable-order. Thus, we are devoted to investigating the existence of infinitely many solutions for Schrödinger–Kirchhoff type equations involving a variable-order fractional p-Laplace operator by applying the fountain theorem and symmetric mountain pass theorem, respectively.
Our work is different from the previous articles. To the best of our knowledge, this article is the first to discuss the existence of infinitely many solutions for the fractional p-Laplacian Schrödinger–Kirchhoff type equations without the (AR) condition. Under the reasonable hypothesis, we first establish an embedding theorem for the variable-order fractional Sobolev spaces. Second, compared with [15], we deal with the problem ( P v ) generalized from fractional framework to variable-order fractional framework, and our results generalize Theorem 1 and Theorem 2 of [15] in some directions. Finally, relative to paper [11], for the case p = 2 , we can deal with a general Kirchhoff–Schrödinger type equations and the nonlinearity with variable coefficients.
Throughout this paper, for simplicity, C i and K i , i = 1 , 2 , . . . , N are used in various places to denote distinct constants, and we will specify them whenever it is necessary. Define the function space C + ( Ω ¯ )
C + ( Ω ¯ ) : = H ( x ) C ( Ω ¯ , R ) , 1 < H H ( x ) H + < + ,
where H : = min H ( x ) and H + : = max H ( x ) for all x Ω ¯ .
s ( · ) : R N × R N ( 0 , 1 ) is a continuous function, satisfying:
(S1):
s ( · ) is symmetric function, that is, s ( x , y ) = s ( y , x ) for all ( x , y ) R n × R n .
(S2):
0 < s : = min ( x , y ) R n × R n s ( x , y ) < s ( x , y ) < s + : = max ( x , y ) R n × R n s ( x , y ) < 1 for all ( x , y ) R n × R n .
Regarding the potential function V ( x ) : Ω R , we assume the following hypothesis:
(V1):
V ( x ) is the continuous function, satisfying inf x Ω V ( x ) > V 0 , where V 0 is a positive constant. Moreover, there is d > 0 such that the set { x Ω : V ( x ) d } is nonempty and meas ( { x Ω : V ( x ) d } ) < + .
(V2):
There exists positive constant h such that
lim | y | m e a s { x B h ( y ) : V ( x ) κ 0 } = 0 f o r a n y κ 0 > 0 ,
where B R 0 ( x ) denotes the open ball of Ω centered at x and of radius R 0 > 0 .
Furthermore, the nonlinearity f ( x , t ) : Ω × R R is a continuous Carathéodory function, satisfying:
(F1):
There exist positive constants C 1 and C 2 such that
| f ( x , t ) | C 1 | t | p 1 + C 2 | t | ϑ ( x ) 1 f o r a l l ( x , t ) Ω × R ,
where ϑ ( x ) C + ( Ω ¯ ) and 1 < p < ϑ ( x ) < p s ( · ) * = ( p N ) / ( N p s ( x , x ) ) .
(F2):
lim | t | 0 f ( x , t ) | t | p 1 = 0 for x Ω uniformly.
(F3):
There exist positive constants p 2 < μ < p s ( · ) * and r such that
F ( x , t ) 1 μ f ( x , t ) t + C 3 | t | p f o r a l l ( x , t ) Ω × R ,
where 0 < C 3 < β ( μ p ) r p and inf x Ω , | t | = r F ( x , t ) : = β > 0 .
(F4):
f ( x , t ) = f ( x , t ) f o r a l l ( x , t ) Ω × R .
Remark 1.
It is obvious that the condition (F3) is weaker than the well-known (AR) condition.
Before stating our main results, we need to present the corresponding variational framework and definition, which plays an important role to solve problem ( P v ) .
Definition 1.
We say that ξ X 0 is a (weak) solution of Schrödinger–Kirchhoff type equations ( P v ) , if
a + b Ω × Ω | ξ ( x ) ξ ( y ) | p | x y | N + p s ( x , y ) d x d y p 1 × Ω × Ω | ξ ( x ) ξ ( y ) | p 2 ( ξ ( x ) ξ ( y ) ) ( φ ( x ) φ ( y ) ) | x y | N + p s ( x , y ) d x d y = Ω λ V ( x ) | ξ | p 2 ξ φ d x + Ω f ( x , ξ ) φ d x
for any φ X 0 , where X 0 will be introduction in Section 2.
The functional I : X 0 R , which is defined as
I ( ξ ) : = 1 b p 2 a + b Ω × Ω | ξ ( x ) ξ ( y ) | p | x y | N + p s ( x , y ) d x d y p + 1 p Ω λ V ( x ) | ξ | p d x Ω F ( x , ξ ) d x
for all ξ X 0 , where F ( x , ξ ) = 0 ξ f ( x , s ) d s . Moreover, if (F1) and ( V 1 ) hold, then I : X 0 R is of class C 1 ( X 0 , R ) and
I ( ξ ) , φ : = a + b Ω × Ω | ξ ( x ) ξ ( y ) | p | x y | N + p s ( x , y ) d x d y p 1 × Ω × Ω | ξ ( x ) ξ ( y ) | p 2 ( ξ ( x ) ξ ( y ) ) ( φ ( x ) φ ( y ) ) | x y | N + p s ( x , y ) d x d y + Ω λ V ( x ) | ξ | p 2 ξ φ d x Ω f ( x , ξ ) φ d x
for any ξ , φ X 0 . Under our reasonable assumptions, the functional I is well defined. Hence, ξ X 0 is a (weak) solution of Schrödinger–Kirchhoff type equations ( P v ) if and only if ξ X 0 is a critical point of the functional I.
Theorem 1.
Let (S1)–(S2), (V1)–(V2), (F1)–(F4) hold, then the problem ( P v ) has infinitely many nontrivial weak solutions in X 0 , whenever λ > 0 is sufficiently large.
The remainder of this paper is organized as follows. Some basic knowledge about the Lebesgue spaces with variable exponent and fractional Sobolev spaces with variable exponents and variable-order are given in Section 2. The functional I satisfying ( P S ) condition is proved in Section 3. In Section 4, by using the fountain theorem, we prove Theorem 1. Finally, in Section 5, we prove Theorem 1 by applying the symmetric mountain pass theorem.

2. Preliminary Results

2.1. Variable Exponent Lebesgue Spaces

In this subsection, we recall some preliminary knowledge of generalized Lebesgue spaces with variable exponent. The readers are invited to consult [35,36,37,38,39,40] for a detailed description.
Let Ω be a nonempty Lipschitz domain in R N , a measurable function ϑ ( x ) C + ( Ω ¯ ) , and u be a measurable real-valued function. We introduce the Lebesgue spaces with variable exponent
L ϑ ( x ) ( Ω ) : = ξ : ξ is a measurable and Ω | ξ | ϑ ( x ) d x <
with the norm
ξ L ϑ ( x ) ( Ω ) : = inf χ > 0 : Ω ξ χ ϑ ( x ) d x 1 ,
then ( L ϑ ( x ) ( Ω ) , · L ϑ ( x ) ( Ω ) ) is a Banach space (see [38]), called generalized Lebesgue space.
Lemma 1 (See [40]). 
The space ( L ϑ ( x ) ( Ω ) , · L ϑ ( x ) ( Ω ) ) is separable, uniformly convex, reflexive, and its conjugate space is ( L ϑ ( x ) ( Ω ) , · L ϑ ( x ) ( Ω ) ) , where ϑ ( x ) is the conjugate function of ϑ ( x ) i.e.,
1 ϑ ( x ) + 1 ϑ ( x ) = 1 , f o r a l l x Ω .
For all ξ L ϑ ( x ) ( Ω ) , v L ϑ ( x ) ( Ω ) , the Hölder type inequality
Ω ξ v d x 1 ϑ + 1 ( ϑ ) ξ L ϑ ( x ) ( Ω ) v L ϑ ( x ) ( Ω ) 2 ξ L ϑ ( x ) ( Ω ) v L ϑ ( x ) ( Ω )
holds.
The mapping ρ ϑ ( x ) : L ϑ ( x ) ( Ω ) R is defined:
ρ ϑ ( x ) ( ξ ) : = Ω | ξ | ϑ ( x ) d x .
The relation between modular and Luxemburg norm is clarified by the following properties.
Lemma 2 (See [36]). 
Suppose that ξ n , ξ L ϑ ( x ) ( Ω ) , then the following properties hold
(i) ξ L ϑ ( x ) ( Ω ) > 1 ξ L ϑ ( x ) ( Ω ) ϑ ρ ϑ ( x ) ( ξ ) ξ L ϑ ( x ) ( Ω ) ϑ + ;
(ii) ξ L ϑ ( x ) ( Ω ) < 1 ξ L ϑ ( x ) ( Ω ) ϑ + ρ ϑ ( x ) ( ξ ) ξ L ϑ ( x ) ( Ω ) ϑ ;
(iii) ξ L ϑ ( x ) ( Ω ) < 1 ( r e s p e c t i v e l y , = 1 , > 1 ) ρ ϑ ( x ) ( ξ ) < 1 ( r e s p e c t i v e l y , = 1 , > 1 ) ) ;
(iv) ξ n L ϑ ( x ) ( Ω ) 0 ( r e s p e c t i v e l y , ) ρ ϑ ( x ) ( ξ n ) 0 ( r e s p e c t i v e l y , ) ;
(v) lim n | ξ n ξ | ϑ ( x ) = 0 lim n ρ ϑ ( x ) ( ξ n ξ ) = 0 .
Remark 2.
Note that for any function ϑ 1 ( x ) , ϑ 2 ( x ) C + ( Ω ¯ ) and ϑ 1 ( x ) < ϑ 2 ( x ) , there exists a continuous embedding L ϑ 2 ( x ) ( Ω ) L ϑ 1 ( x ) ( Ω ) for any x Ω ¯ . Especially, when ϑ ( x ) constant, the results of Lemmas 1 and 2 still hold.

2.2. Variable-Order Fractional Sobolev Spaces

Let 1 < p < + , s ( · ) is a continuous symmetric function, and let the Gagliardo seminorm with variable-order be denoted as
[ ξ ] s ( · ) , p p : = Ω × Ω | ξ ( x ) ξ ( y ) | p | x y | N + p s ( x , y ) d x d y ,
where ξ : Ω R is a measurable function. Now, we define the fractional Sobolev spaces with variable-order by
W = W s ( · ) , p ( Ω ) : = ξ L p ( Ω ) : ξ is a measurable and [ ξ ] s ( · ) , p p < ,
then ( W , · W ) is a reparable, reflexive Banach space and assume that it is endowed with the norm
ξ W : = ξ L p ( Ω ) p + a p 1 [ ξ ] s ( · ) , p p 1 / p .
The variable-order fractional critical exponent is defined by
p s ( · ) * = N p N p s ( x , y ) if p s ( x , y ) < N , if p s ( x , y ) N .
We denote by W 0 the closure of C 0 ( Ω ) in W and with the norm
ξ W 0 : = [ ξ ] s ( · ) , p p ,
then, the ( W 0 , · W 0 ) is also a reparable, reflexive Banach space. W 0 * denotes the dual space of W 0 .
Now let us give a very crucial lemma, which the proof process is similar to the one of Lemma 2.1 of [11].
Lemma 3.
Let 0 < s 0 < s ( · ) < s 1 < 1 < p < + and W 0 s j ( j = 0 , 1 ) in W 0 with s ( x , y ) = s j , the embeddings W 0 s 1 W 0 W 0 s 0 are continuous. Moreover, if N > p s 0 , for any constant exponent p [ 1 , N p / ( N p s 0 ) ] , W 0 can be continuously embedded into L p ( Ω ) .
Proof. 
First, for any ξ W 0 , we obtain
Ω Ω | x y | 1 | ξ | p | x y | N + p s ( x , y ) d x d y Ω | z | 1 1 | z | N + p s ( x , y ) d z | ξ | p d x C ( N , s ( · ) , p ) ξ L p ( Ω ) p ,
where we used the fact that the kernel 1 / | z | N + p s ( x , y ) is integrable since N + p s ( x , y ) > N . Taking into account the above estimate, it follows
Ω Ω | x y | 1 | ξ ( x ) ξ ( y ) | p | x y | N + p s ( x , y ) d x d y 2 p 1 Ω Ω | x y | 1 | ξ ( x ) | p + | ξ ( y ) | p | x y | N + p s ( x , y ) d x d y 2 p C ( N , s ( · ) , p ) ξ L p ( Ω ) p ,
hence, for any ξ W 0 s 1 and s 0 < s ( · ) , we have
Ω Ω | x y | 1 | ξ | p | x y | N + p s ( x , y ) d x d y Ω Ω | x y | 1 | ξ | p | x y | N + s 0 p d x d y Ω | z | 1 1 | z | n + s 0 p d z | ξ | p d x C ( N , s 0 , p ) ξ L p ( Ω ) p .
On the other hand
Ω Ω | x y | 1 | ξ ( x ) ξ ( y ) | p | x y | N + p s ( x , y ) d x d y Ω Ω | x y | 1 | ξ ( x ) ξ ( y ) | p | x y | N + p s 1 d x d y Ω Ω | ξ ( x ) ξ ( y ) | p | x y | N + p s 1 d x d y .
Thus, combining with (3)–(5), we get
Ω Ω a p 1 | ξ ( x ) ξ ( y ) | p | x y | N + p s ( x , y ) d x d y Ω Ω | x y | 1 a p 1 | ξ ( x ) ξ ( y ) | p | x y | N + p s ( x , y ) d x d y + Ω Ω | x y | 1 a p 1 | ξ ( x ) ξ ( y ) | p | x y | N + p s ( x , y ) d x d y ( 2 p C ( N , s 0 , p ) + 1 ) ξ L p ( Ω ) p + Ω Ω a p 1 | ξ ( x ) ξ ( y ) | p | x y | N + p s 1 d x d y C ( N , s 0 , p ) ξ L p ( Ω ) p + Ω Ω a p 1 | ξ ( x ) ξ ( y ) | p | x y | N + p s 1 d x d y ,
which gives the desired estimate, up to relabeling the constant C ( N , s 0 , p ) . From this inequality, we can obtain the following continuous embedding
W 0 s 1 W 0 .
Similarly, we can also deduce the following continuous embedding
W 0 W 0 s 0 .
Finally, by Theorem 6.7 and Theorem 6.9 of [41], we know that for any constant exponent p ( 1 , N p / ( N p s 0 ) ) , the following continuous embedding holds
W 0 s 0 L p ( Ω ) .
Therefore, the embedding W 0 L p ( Ω ) is continuous. □
Theorem 2.
Let Ω R N be a smooth bounded domain, 1 < p < + and s ( · ) : R N × R N ( 0 , 1 ) is a continuous function satisfying (S1) with N > p s ( x , y ) for all ( x , y ) Ω × Ω . Assume that ϑ ( x ) C + ( Ω ¯ ) such that ϑ ( x ) < p s ( · ) * for all x Ω ¯ . Then, there exists C ϑ = C ϑ ( N , p , s , ϑ , Ω ) such that for any ξ W , it holds that
ξ L ϑ ( x ) ( Ω ) C ϑ ξ W .
That is, the space W is continuously embedded in L ϑ ( x ) ( Ω ) . Furthermore, this embedding is compact. If ξ W 0 , then there exists a constant C ϑ = C ϑ ( N , p , s , ϑ , Ω ) such that
ξ L ϑ ( x ) ( Ω ) C ϑ [ ξ ] s ( · ) , p .
Proof. 
Here the process of proof is similar to [39]. Since 1 < p < + , ϑ ( x ) C + ( Ω ¯ ) , s ( x , y ) are continuous symmetric functions, there is a constant k 1 > 0 such that
inf x Ω ¯ N p N p s ( x , x ) ϑ ( x ) = k 1 > 0 for all x Ω ¯ .
Hence, we find a positive constant ϵ and K numbers of disjoint hypercubes Ω i such that Ω = i = 1 K Ω i and diam ( Ω i ) < ϵ , that verify that
N p N p s ( z , y ) ϑ ( x ) = k 1 2 > 0
for all ( z , y ) Ω i × Ω i and x Ω i , i = 1 , 2 , . . . , K . Let s i = inf ( z , y ) Ω i × Ω i s ( z , y ) and the fractional Sobolev critical exponent p s i * = N p N s i p . Then
p s i * = N p N p s i k 1 2 + ϑ ( x )
for all x Ω i and N > s i p . According to the Sobolev embedding theorem (Theorem 6.7 and Theorem 6.9 of [41]), there exists a positive constant k 2 such that
ξ L p s i * ( Ω i ) k 2 ξ L p ( Ω i ) + Ω i × Ω i a p 1 | ξ ( x ) ξ ( y ) | p | x y | n + p s i d x d y .
In addition, from Lemma 3, we obtain
ξ L p s i * ( Ω i ) k 3 ξ L p ( Ω i ) + Ω i × Ω i a p 1 | ξ ( x ) ξ ( y ) | p | x y | n + p s ( x , y ) d x d y .
Since | ξ | = i = 1 K | ξ | χ Ω i , from (6), we get ϑ ( x ) < p s i * . There exist a i ( x ) C + ( Ω ) such that 1 / ϑ ( x ) = 1 / p s i * + 1 / a i ( x ) . By utilizing the Hölder’s inequality, we have
ξ L ϑ ( x ) ( Ω i ) k 4 ξ L p s i * ( Ω i ) ξ L a i ( x ) ( Ω i ) k 5 ξ L p s i * ( Ω i ) .
Note that
ξ L ϑ ( x ) ( Ω ) k 6 i = 1 K ξ L ϑ ( x ) ( Ω i ) ,
by (7)–(9), we have
ξ L ϑ ( x ) ( Ω ) k 7 i = 1 K ξ L p ( Ω i ) + Ω i × Ω i a p 1 | ξ ( x ) ξ ( y ) | p | x y | n + p s ( x , y ) d x d y C ϑ ξ W ,
where the constants C ϑ = C ϑ ( N , p , s , ϑ , Ω ) > 0 .
Finally, we recall that the previous embedding is compact since in the constant s i case we have that for subcritical exponents the embedding is compact. This completes the proof. □
Moreover, in order to investigate the Schrödinger–Kirchhoff type equations ( P v ) , we consider the variable-order fractional Sobolev linear subspace X 0 with potential function, which is defined as follows
X 0 = ξ : ξ W 0 , Ω V ( x ) | ξ | p d x < +
with the norm
ξ X 0 : = Ω V ( x ) | ξ | p d x + Ω × Ω a p 1 | ξ ( x ) ξ ( y ) | p | x y | N + p s ( x , y ) d x d y 1 / p .
The mapping ρ : X 0 R is defined:
ρ X 0 ( ξ ) : = Ω V ( x ) | ξ | p d x + Ω × Ω a p 1 | ξ ( x ) ξ ( y ) | p | x y | N + p s ( x , y ) d x d y .
Lemma 4.
Let ( V 1 ) holds. If ϑ ( x ) [ p , p s ( · ) * ] , then the embeddings
X 0 W 0 L ϑ ( x ) ( Ω )
are continuous with min { 1 , V 0 } ξ W 0 p ξ X 0 p for all ξ X 0 . In particular, there exists a constant C ϑ 0 such that
ξ L ϑ ( x ) ( Ω ) C ϑ 0 ξ X 0
for all ξ X 0 . If ϑ ( x ) [ p , p s ( · ) * ] , then the embedding X 0 L ϑ ( x ) ( B R 1 ) is compact for any R 1 > 0 .
Proof. 
From the definition of ξ X 0 and ( V 1 ) , we can get the following inequality
min { 1 , V 0 } ξ W 0 p ξ X 0 p
for any ξ > 0 . Combined with Lemma 3, we have X 0 W 0 L ϑ ( x ) ( Ω ) . The embeddings are obviously continuous, so
ξ L ϑ ( x ) ( Ω ) C ϑ 0 ξ X 0 .
Fix R 1 > 0 and note that
ξ L p ( B R 1 ) p + B R 1 × B R 1 a p 1 | ξ ( x ) ξ ( y ) | p | x y | n + s ( x , y ) p d x d y 1 / p
is an equivalent norm on W 0 and the embedding X 0 W 0 is continuous. According to Corollary 7.2 of [41], the embedding
W 0 L ϑ ( x ) ( Ω )
is compact. Therefore, also the embedding X 0 L ϑ ( x ) ( Ω ) is compact by the first part of the lemma.
Lemma 5.
Assume that Ω R N is a bounded open domain, then ( X 0 , · X 0 ) is a separable and reflexive Banach space.
Proof. 
First, we prove that ( X 0 , ξ X 0 ) is a Banach space. Set ( V 1 ) holds, { ξ n } n N be a Cauchy sequence in X 0 , for all ς > 0 , there is a natural number N such that if n , k N
V 0 ξ n ξ k L p ( Ω ) < ξ n ξ k X 0 < ς .
Since ξ X 0 ξ W 0 and ( W 0 , ξ W 0 ) is a Banach space, there is ξ W 0 such that ξ n ξ strongly in W 0 . Therefore, there is a subsequence ξ n j such that ξ n j ( x ) ξ ( x ) a . e . x Ω . From Fatou’s lemma with ς = 1 , we have
Ω V ( x ) | ξ | p d x lim inf n Ω V ( x ) | ξ n | p d x lim inf n Ω V ( x ) | ξ n ξ N 0 + ξ N 0 | p d x 2 p lim inf n Ω V ( x ) | ξ n ξ N 0 | p d x + Ω V ( x ) | ξ N 0 | p d x 2 p lim inf n 1 + Ω V ( x ) | ξ N 0 | p d x < ,
and then ξ X 0 . Combining Fatou’s lemma and (10), we deduce for all n , n j N
ρ X 0 ( ξ n ξ ) lim inf j ρ X 0 ( ξ n ξ n j ) < ς ,
this implies that ξ n ξ strongly in X 0 as n . Hence, ( X 0 , · X 0 ) is a Banach space.
Next, we show that ( X 0 , · X 0 ) is a separable and reflexive space. We define the operator G : W s ( · ) , p ( Ω ) L p ( Ω ) × L p ( Ω × Ω ) by
G ( ξ ) = V 1 / p ξ ( x ) , a p 1 | ξ ( x ) ξ ( y ) | | x y | N p + s ( x , y ) ,
clearly G ( ξ ) is an isometry, the rest of the proof is similar to Theorem 8.1 of [42]. Thus, we get ( X 0 , · X 0 ) is reflexive space (see [42], Proposition 3.20), and we get ( X 0 , · X 0 ) is separable space (see [42], Proposition 3.25). □
Lemma 6.
Let (V1)-(V2) hold. Let ϑ ( x ) [ p , p s ( · ) * ) and { ξ n } n N be a bounded sequence in X 0 . Then there exists u X 0 L ϑ ( x ) ( Ω ) such that up to a subsequence
ξ n ξ s t r o n g l y i n L ϑ ( x ) ( Ω ) as n .
Proof. 
The proof of ξ n ξ strongly in L p ( Ω ) is similar to the process of proof Theorem 2.1 in [4], so it is omitted. For p < ϑ ( x ) < p s ( · ) * , there exists ϱ ( 0 , 1 ) such that 1 ϑ ( x ) = ϱ p + 1 ϱ p s ( · ) * and
ξ n ξ L ϑ ( x ) ( Ω ) ξ n ξ L p ( Ω ) ϱ ξ n ξ L p s ( · ) * ( Ω ) 1 ϱ 0 , as n .
Since { ξ n } n N is bounded sequence in L p s ( · ) * ( Ω ) , ξ n ξ strongly in L ϑ ( x ) ( Ω ) as n .
Let { e j } X 0 , { e j * } X 0 * such that X 0 = span { e j : j = 1 , 2 , . . . } ¯ , X 0 * = span { e j * : j = 1 , 2 , . . . } ¯ and
e j * , e i = 1 , i j ; 0 , i = j .
Set X i = span { e j : j = 1 , 2 , . . . } , and define A k = i = 1 k X i , B k = i = k X i ¯ .
To prove our results, we need the following fountain theorem and symmetric mountain pass theorem.
Theorem 3 (Fountain Theorem, see [43]). 
Let X 0 be a real Banach space and an even functional I C 1 ( X 0 , R ) satisfies the Palais–Smale ( ( P S ) for short) condition, for every c > 0 , and that there is k 0 > 0 , such that for every k k 0 there exists ρ k > r k > 0 , so that the following properties hold:
(i) a k = m a x { I ( ξ ) : ξ A k , ξ = ρ k } 0 ;
(ii) b k = i n f { I ( ξ ) : ξ B k , ξ = r k } + a s k .
Then I has a sequence of critical points ξ k such that I ( ξ k ) + .
Theorem 4 (Symmetric Mountain Pass Theorem, see [44]). 
Let X 0 be an infinite dimensional Banach space and let I C 1 ( X 0 , R ) be even, satisfy ( P S ) condition, and I ( 0 ) = 0 . If X 0 = A k B k , where A k is finite dimensional and I satisfies:
(i) there exist constants ρ , α > 0 such that I | B ρ B k α ;
(ii) for any finite dimensional subspace X ˜ X 0 , there is R = R ( X ˜ ) > 0 such that I ( ξ ) 0 on X ˜ \ B R , then I possesses an unbounded sequence of critical values.

3. Palais–Smale Condition

In what follows, we need the following definition and prove a lemma which will play a critical role.
Definition 2.
Let X 0 be a Banach space, I C 1 ( X 0 , R ) . We say that I satisfies the ( P S ) condition, if any ( P S ) c sequence { ξ n } n N X 0 with
I ( ξ n ) c , I ( ξ n ) 0 , as n ,
possesses a convergent subsequence in X 0 .
Suppose that { ξ n } n N is a bounded sequence in X 0 . Combining Theorem 2 with Lemma 6, there exists ξ X 0 such that
ξ n ξ in X 0 , ξ n ξ a . e . in Ω , ξ n ξ in L ϑ ( x ) ( Ω ) .
Lemma 7.
Let the conditions of Theorem 1 hold, then I satisfies the ( P S ) condition for large λ > 0 .
Proof. 
Step 1. We show that { ξ n } n N is bounded in X 0 . Assume that { ξ n } n N X 0 is a sequence, from Definition 2, there exists a positive constant C such that
| I ( ξ n ) | C and I ( ξ n ) X 0 * C
for every n N .
We prove this by contrary arguments. Supposing { ξ n } n N is unbounded in X 0 , that is
ξ n X 0 , as n .
Let ω n : = ξ n ξ n X 0 , then ω n X 0 with ω n X 0 = 1 , ω n s C s ω n X 0 = C s for s [ p , p s ( · ) * ] . Set
G ( t ) = F ( x , t 1 z ) t μ for all ( x , z ) Ω × R and for all t > 1 .
For | z | r and t [ 1 , | z | r ] , by (F3), we obtain
G ( t ) = z t 2 f ( x , t 1 z ) t μ + F ( x , t 1 z ) t μ 1 μ = t μ 1 [ μ F ( x , t 1 z ) t 1 z f ( x , t 1 z ) ] C 3 t μ p 1 | z | p .
Then
G ( | z | r ) G ( 1 ) = 1 | z | / r G ( t ) d t 1 | z | / r C 3 t μ p 1 | z | p d t = C 3 | z | μ ( μ p ) r ( μ p ) C 3 | z | μ ( μ p ) .
when t = 1 , we have
F ( x , z ) = G ( 1 ) G ( | z | r ) C 3 | z | μ ( μ p ) r ( μ p ) β r μ C 3 ( μ p ) r ( μ p ) | z | μ .
Noting that 0 < C 3 < β ( μ p ) r p , we have β r μ C 3 ( μ p ) r ( μ p ) | z | μ > 0 . Since μ > p 2 , there is a constant p 2 < θ < p s ( · ) * so that θ < μ , and
lim | ξ | F ( x , ξ ) | ξ | θ = + .
In particular, we have
lim | ξ | F ( x , ξ ) | ξ | p 2 = + .
By (F1) and (F2), we get
| F ( x , ξ ) | C 4 | ξ | p + C 5 | ξ | ϑ ( x ) .
Combining (16) and (18), for any M 1 > 0 , there is a positive constant C ( M 1 ) so that
| F ( x , ξ ) | M 1 | ξ | θ C M 1 | ξ | p , for all ( x , ξ ) Ω × R .
Moreover, we have
I ( ξ n ) ξ n X 0 θ = 1 ξ n X 0 θ 1 b p 2 a + b Ω × Ω | ξ n ( x ) ξ n ( y ) | p | x y | N + p s ( x , y ) d x d y p + 1 ξ n X 0 θ 1 p Ω λ V ( x ) | ξ n | p d x Ω F ( x , ξ n ) ξ n X 0 θ d x .
Since p 2 < θ , we deduce that
lim n + Ω F ( x , ξ n ) ξ n X 0 θ d x = 0 .
Since ω n X 0 = 1 , up to subsequences, there exists ω X 0 such that ω n ω in X 0 , ω n ω   a . e . in Ω , ω n ω in L ϑ ( x ) ( Ω ) . In the case of ω 0 , setting Ω 0 : = { x Ω : ω 0 } . If m e a s ( Ω ) > 0 , then Ω ω θ d x > 0 . By (19), we have
Ω F ( x , ξ n ) ξ n X 0 θ d x > M 1 ω n L θ ( Ω ) θ C ( M 1 ) ω n L p ( Ω ) p ξ n X 0 θ p .
Therefore
0 = lim inf n Ω F ( x , ξ n ) ξ n X 0 θ d x + C ( M 1 ) ω n L p ( Ω ) p ξ n X 0 θ p > lim inf n M 1 ω n L θ ( Ω ) θ > Ω ω θ d x > 0 .
This is a contradiction. Hence m e a s ( Ω ) = 0 and as a result ω = 0 a.e. in R N . Thus, according to (V1), we obtain
ω n L p ( Ω ) p = V ( x ) d | ω n | p d x + V ( x ) < d | ω n | p d x 1 λ d ω n X 0 p + o ( 1 ) 2 λ d
for large n. Combining (F1) and (F3), there exists a positive constant C 6 such that
μ F ( x , ξ ) f ( x , ξ ) ξ C 6 | ξ | p , for all ( x , ξ ) Ω × X 0 .
Consequently, we have
0 1 ξ n X 0 p μ I ( ξ n ) I ( ξ n ) , ξ n = 1 ξ n X 0 p μ b p 2 a + b [ ξ n ] s ( · ) , p p p + μ p Ω λ V ( x ) | ξ n | p d x μ Ω F ( x , ξ n ) d x a + b [ ξ n ] s ( · ) , p p p 1 × [ ξ n ] s ( · ) , p p Ω λ V ( x ) | ξ n | p d x + Ω f ( x , ξ n ) ξ n d x , = 1 ξ n X 0 p a μ b p 2 a + b [ ξ n ] s ( · ) , p p p 1 + μ p 2 p 2 a + b [ ξ n ] s ( · ) , p p p 1 × [ ξ n ] s ( · ) , p p + μ p p Ω λ V ( x ) | ξ n | p d x + Ω ( f ( x , ξ n ) ξ n μ F ( x , ξ n ) ) d x 1 ξ n X 0 p μ p 2 p 2 a p 1 [ ξ n ] s ( · ) , p p + μ p p Ω λ V ( x ) | ξ n | p d x C 6 Ω | ξ n | p d x 1 ξ n X 0 p μ p 2 p 2 ξ n X 0 p C 6 Ω | ξ n | p d x μ p 2 p 2 C 6 λ d .
Since μ > p 2 , letting λ > 0 be so large that the term μ p 2 p 2 C 6 λ d is positive, we get a contradiction. Therefore, the sequence { ξ n } n N is bounded in X 0 .
Step 2. To show that { ξ n } n N has a convergent subsequence in X 0 . Then, the sequence { ξ n } n N has a subsequence, still denoted by { ξ n } n N , and there exists ξ X 0 such that
ξ n ξ , weakly in X 0 ,
this implies
I ( ξ n ) I ( ξ ) , ξ n ξ 0 , as n .
Moreover, combining with (F1) and the Hölder inequality, we obtain
Ω ( f ( x , ξ n ) f ( x , ξ ) ) ( ξ n ξ ) d x Ω | C 1 ( | ξ n | p 1 + | ξ | p 1 ) + C 2 ( | ξ n | ϑ ( x ) 1 + | ξ | ϑ ( x ) 1 ) | ( ξ n ξ ) d x C 1 ξ n L p ( Ω ) p 1 + ξ L p ( Ω ) p 1 ( ξ n ξ ) L p ( Ω ) + C 2 ξ n L ϑ ( x ) ( Ω ) ϑ ( x ) 1 + ξ L ϑ ( x ) ( Ω ) ϑ ( x ) 1 ( ξ n ξ ) L ϑ ( x ) ( Ω ) ,
hence, by (13) implies that
lim n Ω ( f ( x , ξ n ) f ( x , ξ ) ) ( ξ n ξ ) d x = 0 .
For convenience, fix ψ X 0 and the linear functional Γ ψ is defined as
Γ ψ ( ν ) = Ω × Ω | ψ ( x ) ψ ( y ) | p 2 ( ψ ( x ) ψ ( y ) ) ( ν ( x ) ν ( y ) ) | x y | N + s ( x , y ) p d x d y
for all ν X 0 . According to the Hölder inequality, Γ ψ ( ν ) is continuous and we obtain
| Γ ψ ( ν ) | ψ X 0 ν X 0 , for all ν X 0 .
Obviously, Γ ψ ( ν ) is bounded. Therefore, (13) gives that
lim n Γ ψ ( ν n ν ) = 0 and lim n [ ξ n ] s ( · ) , p p [ ξ ] s ( · ) , p p Γ ψ ( ν n ν ) = 0 .
Since { [ ξ n ] s ( x , y ) , p [ ξ ] s ( x , y ) , p } n is bounded in R . Hence, combining (13) and (21)–(23), we obtain
o ( 1 ) = I ( ξ n ) I ( ξ ) , ξ n ξ = a + b [ ξ n ] s ( · ) , p p p 1 × Ω × Ω | ξ n ( x ) ξ n ( y ) | p 2 ( ξ n ( x ) ξ n ( y ) ) ( ξ n ( x ) ξ n ( y ) ξ ( x ) + ξ ( y ) ) | x y | N + s ( x , y ) p d x d y a + b [ ξ ] s ( · ) , p p p 1 × Ω × Ω | ξ ( x ) ξ ( y ) | p 2 ( ξ ( x ) ξ ( y ) ) ( ξ n ( x ) ξ n ( y ) ξ ( x ) + ξ ( y ) ) | x y | N + s ( x , y ) p d x d y Ω λ V ( x ) ( | ξ n | p 2 ξ n | ξ | p 2 ξ ) ( ξ n ξ ) d x Ω ( f ( x , ξ n ) f ( x , ξ ) ) ( ξ n ξ ) d x
= a + b [ ξ n ] s ( · ) , p p p 1 × Ω × Ω | ξ n ( x ) ξ n ( y ) | p 2 ( ξ n ( x ) ξ n ( y ) ) ( ξ n ( x ) ξ n ( y ) ξ ( x ) + ξ ( y ) ) | x y | N + s ( x , y ) p d x d y a + b [ ξ n ] s ( · ) , p p p 1 × Ω × Ω | ξ ( x ) ξ ( y ) | p 2 ( ξ ( x ) ξ ( y ) ) ( ξ n ( x ) ξ n ( y ) ξ ( x ) + ξ ( y ) ) | x y | N + s ( x , y ) p d x d y + a + b [ ξ n ] s ( · ) , p p p 1 × Ω × Ω | ξ ( x ) ξ ( y ) | p 2 ( ξ ( x ) ξ ( y ) ) ( ξ n ( x ) ξ n ( y ) ξ ( x ) + ξ ( y ) ) | x y | N + s ( x , y ) p d x d y a + b [ ξ ] s ( · ) , p p p 1 × Ω × Ω | ξ ( x ) ξ ( y ) | p 2 ( ξ ( x ) ξ ( y ) ) ( ξ n ( x ) ξ n ( y ) ξ ( x ) + ξ ( y ) ) | x y | N + s ( x , y ) p d x d y Ω λ V ( x ) ( | ξ n | p 2 ξ n | ξ | p 2 ξ ) ( ξ n ξ ) d x Ω ( f ( x , ξ n ) f ( x , ξ ) ) ( ξ n ξ ) d x = a + b [ ξ n ] s ( · ) , p p p 1 × Γ ξ n ( ξ n ξ ) Γ u ( ξ n ξ ) + b [ ξ n ] s ( x , y ) , p p [ ξ ] s ( x , y ) , p p × Γ ξ ( ξ n ξ ) Ω λ V ( x ) ( | ξ n | p 2 ξ n | ξ | p 2 ξ ) ( ξ n ξ ) d x Ω ( f ( x , ξ n ) f ( x , ξ ) ) ( ξ n ξ ) d x = a + b [ ξ n ] s ( · ) , p p p 1 × Γ ξ n ( ξ n ξ ) Γ ξ ( ξ n ξ ) Ω λ V ( x ) ( | ξ n | p 2 ξ n | ξ | p 2 ξ ) ( ξ n ξ ) d x + o ( 1 ) .
That is
lim n ( a + b [ ξ n ] s ( · ) , p p ) p 1 × ( Γ ξ n ( ξ n ξ ) Γ ξ ( ξ n ξ ) ) Ω λ V ( x ) ( | ξ n | p 2 ξ n | ξ | p 2 ξ ) ( ξ n ξ ) d x = 0 .
Note that
( a + b [ ξ n ] s ( · ) , p p ) p 1 × Γ ξ n ( ξ n ξ ) Γ ξ ( ξ n ξ ) 0 and Ω λ V ( x ) ( | ξ n | p 2 ξ n | ξ | p 2 ξ ) ( ξ n ξ ) d x 0
for any n N . Considering a , b > 0 and (V1), we have
lim n ( a + b [ ξ n ] s ( · ) , p p ) p 1 × Γ ξ n ( ξ n ξ ) Γ ξ ( ξ n ξ ) = 0 and
lim n Ω λ V ( x ) ( | ξ n | p 2 ξ n | ξ | p 2 ξ ) ( ξ n ξ ) d x = 0 .
Now, we describe the Simon inequalities, that is
| η 1 η 2 | p c p [ ( | η 1 | p 2 η 1 | η 2 | p 2 η 2 ) ( η 1 η 2 ) ] p 2 ( | η 1 | p | η 2 | p ) 2 p p , 1 < p < 2 , c ˜ p ( | η 1 | p 2 η 1 | η 2 | p 2 η 2 ) ( η 1 η 2 ) , p 2 ,
for all η 1 , η 2 R N , where c p > 0 and c ˜ p > 0 are constants which depend on p. We also need the following elementary inequalities, that is to say
( ϱ 1 + ϱ 2 ) p ( 2 p ) 2 ϱ 1 p ( 2 p ) 2 + ϱ 2 p ( 2 p ) 2 , for all ϱ 1 ϱ 2 0 and 1 < p < 2 .
when p 2 , by the well-know Simon inequalities (24) and (26) as n , we have
[ ξ n ξ ] s ( · ) , p p Ω × Ω | ( ξ n ( x ) ξ n ( y ) ξ ( x ) + ξ ( y ) | p | x y | N + s ( x , y ) p d x d y = c p Γ ξ n ( ξ n ξ ) Γ ξ ( ξ n ξ ) = o ( 1 ) .
Similarly, combining with (V1) and (24) as n , we obtain
ξ n ξ p c p Ω V ( x ) ( | ξ n | p 2 ξ n | ξ | p 2 ξ ) ( ξ n ξ ) d x = o ( 1 ) .
Hence, ξ n ξ X 0 0 as n , as required.
When 1 < p < 2 . Since ξ n ξ weakly in X 0 , there exists a positive constant κ 1 such that [ ξ ] s ( x , y ) , p κ 1 for all n N . Combining with the Simon inequality (26), Hölder inequality and (24) as n , we get
[ ξ n ξ ] s ( · ) , p p c ˜ p [ Γ ξ n ( ξ n ξ ) Γ ξ ( ξ n ξ ) ] p 2 [ ( a + b [ ξ n ] s ( x , y ) , p p ) p + ( a + b [ ξ n ] s ( x , y ) , p p ) p ] 2 p 2 c ˜ p [ Γ ξ n ( ξ n ξ ) Γ ξ ( ξ n ξ ) ] p 2 [ ( a + b [ ξ n ] s ( x , y ) , p p ) p ( 2 p ) 2 + ( a + b [ ξ n ] s ( x , y ) , p p ) p ( 2 p ) 2 ] 2 c ˜ p ( a + b κ 1 ) p ( 2 p ) 2 [ Γ u n ( ξ n ξ ) Γ ξ ( ξ n ξ ) ] p 2 = o ( 1 ) .
Similarly, since ξ n ξ weakly in X 0 , there exists a positive constant ϱ 0 such that ξ n p ϱ 0 for all n N . Moreover, combining with the elementary inequality (27), Hölder inequality and (24) as n , we obtain
ξ n ξ p 2 c ˜ p ϱ 0 p ( 2 p ) 2 Ω V ( x ) ( | ξ n | p 2 ξ n | ξ | p 2 ξ ) ( ξ n ξ ) d x p 2 = o ( 1 ) .
Therefore, ξ n ξ X 0 0 as n . Thus, the functional I satisfies the ( P S ) condition.

4. Proof of Theorem 1 by Using the Fountain Theorem

Lemma 8 (see [21]). 
Assume that ζ ( x ) C + ( Ω ¯ ) , ζ ( x ) < p * ( x ) , for any x Ω ¯ and denote
β k = s u p ξ B k , ξ X 0 = 1 | ξ | ζ ( x ) ,
then lim k β k = 0 .
To prove Theorem 1 by using the fountain theorem, we first prove the following two lemmas.
Lemma 9.
Let the conditions of Theorem 1 hold, then there exist constants ρ k > 0 such that
max ξ A k , ξ = ρ k I ( ξ ) 0 .
Proof. 
By (17), there exist C 7 > b p 1 C A k p 2 a p ( p 1 ) , C 8 > 0 such that
| F ( x , ξ ) | C 7 | ξ | p 2 C 8 for all x Ω and ξ X 0 .
Since all norms are equivalent on the finite dimensional Banach space A k , there exists a positive constant C A k such that ξ L p 2 ( Ω ) C A k ξ X 0 . Then for ξ X 0 = ρ k 1 , from (28), we have
I ( ξ ) : = 1 b p 2 a + b [ ξ ] s ( · ) , p p p + 1 p Ω λ V ( x ) | ξ | p d x Ω F ( x , ξ ) d x 1 b p 2 a + b [ ξ ] s ( · ) , p p p + 1 p Ω λ V ( x ) | ξ | p d x + C 8 Ω d x C 7 Ω | ξ | p 2 d x 1 b p 2 a + b a p 1 ξ X 0 p p + 1 p ξ X 0 p + C 8 | Ω | C 7 ξ L P 2 ( Ω ) p 2 1 b p 2 a + b a p 1 ξ X 0 p p + 1 p ξ X 0 p + C 8 | Ω | C 7 C A k ξ X 0 p 2 1 b p 2 a + b a p 1 ρ k p p + 1 p ρ k p + C 8 | Ω | C 7 C A k ρ k p 2 .
Therefore, for p 2 > p > 1 , there exists ρ k > 1 large enough such that
a k = max ξ A k , ξ = ρ k I ( ξ ) 0 .
This completes the proof. □
Lemma 10.
Let the conditions of Theorem 1 hold, then there exist constants r k such that
inf ξ B k , ξ = r k I ( ξ ) > + .
Proof. 
Note that by Young’s inequality, we have
a + b [ ξ ] s ( · ) , p p = a p 1 p p p 1 + b [ ξ ] s ( · ) , p p 1 p p = p p 1 1 p p 1 p p 1 × a p 1 p p p 1 + 1 p p b [ ξ ] s ( · ) , p p 1 p p p p 1 p p 1 × a p 1 p p b [ ξ ] s ( · ) , p p 1 p a p 1 p p b [ ξ ] s ( · ) , p p 1 p ,
hence, we get the following conclusion from the above derivation
a + b [ ξ ] s ( · ) , p p p p b a p 1 [ ξ ] s ( · ) , p p .
For ξ B k , according to (F1) and (29), we obtain that
I ( u ) : = 1 b p 2 a + b [ ξ ] s ( · ) , p p p + 1 p Ω λ V ( x ) | ξ | p d x Ω F ( x , ξ ) d x a p 1 p [ ξ ] s ( · ) , p p + 1 p Ω λ V ( x ) | ξ | p d x Ω F ( x , ξ ) d x a p 1 p [ ξ ] s ( · ) , p p + 1 p Ω λ V ( x ) | ξ | p d x C 1 p Ω | ξ | p d x C 2 ϑ Ω | ξ | ϑ ( x ) d x 1 p ξ X 0 p C 1 p C p p ξ X 0 p C 2 ϑ C ϑ + ϑ + β k ϑ + ξ X 0 ϑ + = ξ X 0 p 1 p C 1 p C p p C 2 ϑ C ϑ + ϑ + β k ϑ + ξ X 0 ϑ + p ,
where β k is defined as in Lemma 8 and 1 C 1 C p p > 0 , choosing
r k = ( 1 C 1 C p p ) ϑ 1 ϑ + p ( 2 p C 2 C ϑ + ϑ + β k ϑ + ) 1 ϑ + p .
Thus, we obtain r k + as k + , thanks to Lemma 8 and the fact that 1 < p < ϑ + . By the choice of r k B k with ξ X 0 = r k such that ρ k > r k > 0 , we get
b k = inf ξ B k , ξ = r k I ( ξ ) 1 C 1 C p p 2 p r k p + ,
as k + . This completes the proof. □
Proof of Theorem 1. 
Let X 0 be a Banach space and the conditions of Theorem 1 hold. First, from Lemma 7 that I satisfies the (PS) condition. Moreover, according to the condition (F4) that I ( 0 ) = 0 and I is an even function. Finally, by Lemmas 9 and 10, we deduce that I satisfies the conditions (i) and (ii) of Theorem 3. Therefore, I satisfies all the conditions of Theorem 3, we obtain that problem ( P v ) has a sequence of solutions ξ k as k . In conclusion, by Theorem 3, the problem ( P v ) has infinitely many nontrivial weak solutions. This completes the proof. □

5. Proof of Theorem 1 by Applying the Symmetric Mountain Pass Theorem

In order to prove Theorem 1 by applying the symmetric mountain pass theorem, we first prove the following results.
Lemma 11.
Let the conditions of Theorem 1 hold, then there exist constants ρ , α > 0 such that
I | B ρ B k α
Proof. 
From (F2) that for any ε > 0 there exists a positive δ = δ ε such that
| f ( x , ξ ) | ε p | ξ | p 1 , for all x Ω and | ξ | δ ,
by (F1), we obtain
| f ( x , ξ ) | C 2 + C 1 δ p ϑ ( x ) | ξ | ϑ ( x ) 1 , for all x Ω and | ξ | δ ,
combining with the above two inequalities, we have
| f ( x , ξ ) | ε p | ξ | p 1 + C 2 + C 1 δ p ϑ ( x ) | ξ | ϑ ( x ) 1 , for all x Ω and ξ X 0 .
Therefore, we get
| F ( x , ξ ) | ε p | ξ | p + C ε ϑ | ξ | ϑ ( x ) , for all x Ω and ξ X 0 ,
where C ε = C 2 + C 1 δ p ϑ ( x ) . Thus, using Lemma 4, (29) and (30), we obtain
I ( ξ ) : = 1 b p 2 a + b [ ξ ] s ( · ) , p p p + 1 p Ω λ V ( x ) | ξ | p d x Ω F ( x , ξ ) d x a p 1 p [ ξ ] s ( · ) , p p + 1 p Ω λ V ( x ) | ξ | p d x Ω F ( x , ξ ) d x a p 1 p [ ξ ] s ( · ) , p p + 1 p Ω λ V ( x ) | ξ | p d x ε p Ω | ξ | p d x C ε ϑ Ω | ξ | ϑ ( x ) d x 1 p ξ X 0 p ε p C p p ξ X 0 p C ε ϑ C ϑ ϑ ξ X 0 ϑ ξ X 0 1 p ε p C p p ξ X 0 p 1 C ε ϑ C ϑ ϑ ξ X 0 ϑ 1 .
Taking ε = 1 2 C p p and setting
η ( t ) = 1 2 p t p 1 C ε ϑ C ϑ ϑ t ϑ 1 for all t R 0 + ,
there exists a positive ρ such that max t R 0 + η ( t ) = η ( ρ ) , since ϑ > p > 1 , we deduce that
I ( ξ ) α = ρ η ( ρ ) 2 > 0
for all ξ X 0 with ξ X 0 = ρ . □
Lemma 12.
Let the conditions of Theorem 1 hold, then for any finite dimensional subspace X ˜ X 0 , there is R = R ( X ˜ ) > 0 such that
I ( ξ ) 0
on X ˜ \ B R .
Proof. 
We show that for any finite dimensional subspace X ˜ of X 0 , there exists R 0 = R 0 ( X ˜ ) such that I ( ξ ) < 0 for all ξ X 0 \ B R 0 ( X ˜ ) , where B R 0 ( X ˜ ) = { ξ X 0 : ξ < R 0 } . By (F1) and (17), for any M > b p 1 p 2 a p ( p 1 ) C ( p 2 ) , there exists a positive constant C ( M ) such that
| F ( x , ξ ) | M | ξ | p 2 C ( M ) | ξ | p for all x Ω and ξ X 0 .
For any finite dimensional subspace X ˜ X 0 , by the equivalence of norms in the finite dimensional space, there exists a positive constant C ( p 2 ) such that
ξ L p 2 ( Ω ) C ( p 2 ) ξ X 0 , for all ξ X ˜ ,
therefore, we get that for all t 1 sufficiently large,
I ( t ξ ) : = 1 b p 2 a + b [ t ξ ] s ( · ) , p p p + 1 p Ω λ V ( x ) | t ξ | p d x Ω F ( x , t ξ ) d x 1 b p 2 a + b [ t ξ ] s ( · ) , p p p + 1 p Ω λ V ( x ) | t ξ | p d x Ω M | t ξ | p 2 C ( M ) | t ξ | p d x t p 2 b p 2 a + b [ ξ ] s ( · ) , p p p + t p p Ω λ V ( x ) | ξ | p d x + C ( M ) t p Ω | ξ | p d x M t p 2 Ω | ξ | p 2 d x t p 2 b p 2 a + b a p 1 t p 2 ξ X 0 p p + t p p ξ X 0 p + C ( M ) C p p t p ξ X 0 p M C ( p 2 ) t p 2 ξ X 0 p 2 ,
when M is sufficiently large, we get
I ( t ξ ) = t p 2 b p 2 a + b a p 1 t p 2 ξ X 0 p p + t p p ξ X 0 p + C ( M ) C p p t p ξ X 0 p M C ( p 2 ) t p 2 ξ X 0 p 2 as t
for all ξ X 0 . Consequently, there exists a positive constant R 0 such that I ( ξ ) 0 with ξ = R and R R 0 . □
Proof of Theorem 1. 
Let X 0 be a Banach space and the conditions of Theorem 1 hold. First, from Lemma 7 that I satisfies the (PS) condition. Moreover, according to the condition (F4) that I ( 0 ) = 0 and I is an even function. Finally, by Lemmas 11 and 12, we deduce that I satisfies the conditions (i) and (ii) of Theorem 4. Therefore, I satisfies all the conditions of Theorem 4, we obtain that problem ( P v ) has a sequence of solutions ξ k as k . In conclusion, by Theorem 4, the problem ( P v ) has infinitely many nontrivial weak solutions. This completes the proof. □

6. Conclusions

In this article, we obtain an embedding result for the variable-order fractional Sobolev spaces, and then we investigate the following Schrödinger–Kirchhoff type equations. The existence of infinitely many solutions is obtained by utilizing the fountain theorem and symmetric mountain pass theorem respectively, and the Ambrosetti–Rabinowitz condition is not required.

Author Contributions

Writing original draft, W.B.; Writing review and editing, T.A., J.V.d.C.S. and Y.Y. All authors have read and agreed to the published version of the manuscript.

Funding

This work is supported by the Natural Science Foundation of Jiangsu Province (BK20180500), the National Key Research and Development Program of China (2018YFC1508100) and the Natural Science Foundation of China (11701595).

Institutional Review Board Statement

Not applicable.

Informed Consent Statement

Each of the authors contributed to each part of this study equally, and all authors read and approved the final manuscript.

Data Availability Statement

No data and materials were used to support this study.

Conflicts of Interest

The authors declare that they have no competing interests.

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Bu, W.; An, T.; Sousa, J.V.d.C.; Yun, Y. Infinitely Many Solutions for Fractional p-Laplacian Schrödinger–Kirchhoff Type Equations with Symmetric Variable-Order. Symmetry 2021, 13, 1393. https://doi.org/10.3390/sym13081393

AMA Style

Bu W, An T, Sousa JVdC, Yun Y. Infinitely Many Solutions for Fractional p-Laplacian Schrödinger–Kirchhoff Type Equations with Symmetric Variable-Order. Symmetry. 2021; 13(8):1393. https://doi.org/10.3390/sym13081393

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Bu, Weichun, Tianqing An, José Vanteler da C. Sousa, and Yongzhen Yun. 2021. "Infinitely Many Solutions for Fractional p-Laplacian Schrödinger–Kirchhoff Type Equations with Symmetric Variable-Order" Symmetry 13, no. 8: 1393. https://doi.org/10.3390/sym13081393

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