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Article

Multiple Normalized Solutions to a Choquard Equation Involving Fractional p-Laplacian in ℝN

College of Mathematics, Changchun Normal University, Changchun 130032, China
*
Author to whom correspondence should be addressed.
Fractal Fract. 2024, 8(6), 310; https://doi.org/10.3390/fractalfract8060310
Submission received: 9 April 2024 / Revised: 19 May 2024 / Accepted: 21 May 2024 / Published: 23 May 2024
(This article belongs to the Special Issue Variational Problems and Fractional Differential Equations)

Abstract

:
In this paper, we study the existence of multiple normalized solutions for a Choquard equation involving fractional p-Laplacian in R N . With the help of variational methods, minimization techniques, and the Lusternik–Schnirelmann category, the existence of multiple normalized solutions is obtained for the above problem.

1. Introduction

This work concerns the existence of multiple normalized solutions for the following Choquard equation involving fractional p-Laplacian in R N of the form:
( Δ ) p s u + B ( ϖ x ) | u | p 2 u = λ | u | p 2 u + 1 | x | N α G ( u ) g ( u ) in R N , R N | u | p d x = a p ,
where ϖ > 0 ,   a > 0 , α ( 0 , N ) ,   λ R is a Lagrange multiplier, g is a continuous differentiable function with L p -subcritical growth, and B : R N [ 0 , ) is a continuous function satisfying some appropriate conditions. B ε ( x ) is a sphere with the center x and radius ε , and the fractional p-Laplace operator ( Δ ) p s is defined by
( Δ ) p s u ( x ) = 2 lim ε 0 R N B ε ( x ) | u ( x ) u ( y ) | p 2 ( u ( x ) u ( y ) ) | x y | N + p s d y ( x R N ) .
Our research on problem (1) is based on theoretical and practical application research. First, the equations with p-Laplacian occur in fluid dynamics, nonlinear elasticity, glaciology, and so on; please refer to [1,2]. When p = 2 , problem (1) comes from the research of solitary waves for the following fractional Schrödinger equation
i 𝜕 ψ 𝜕 t = ( Δ ) s ψ + B ( x ) ψ G ( ψ ) ψ ( I α g ( ψ ) ) in R N ,
where 0 < s < 1 , ( Δ ) s is the fractional Laplacian, i denotes the imaginary unit and ψ ( x , t ) is a complex wave. The standing wave is a solution of the form ψ ( t , x ) = e i λ t B ( x ) , where λ R and u : R N R is a time-independent function that satisfies the following equation:
( Δ ) s u + B ( x ) u = λ u + 1 | x | N α G ( u ) g ( u ) i n R N .
Fix λ , the energy functional E λ : H 1 ( R N ) R corresponding to problem (3) is defined by
E λ ( u ) = 1 2 R N | u | 2 + ( B ( x ) λ ) | u | 2 d x 1 2 R N 1 | x | N α G ( u ) G ( u ) d x .
In recent years, many papers have been published concerning the existence and multiplicity of solutions for this case. For instance, Ambrosio [3] studied the following equation with the potential function of the form:
ϵ 2 s ( Δ ) s u + B ( x ) u = ϵ μ N 1 | x | μ G ( u ) g ( u ) ,
where 0 < s < 1 and g have subcritical growth. They obtained the concentration and multiplicity of positive solutions to (4) using the Ljusternik–Schnirelmann theory and the penalization method. Moreover, Ambrosio [4] investigated the following fractional Choquard equation involving the fractional p-Laplacian operator:
ϵ s p ( Δ ) p s u + B ( x ) | u | p 2 u = ϵ μ N 1 | x | μ G ( u ) g ( u ) in R N , u W s , p ( R N ) , u > 0 in R N .
Under the suitable assumptions, they can also obtain the multiplicity and concentration of positive solutions to problem (5). For critical growth cases, please see [5,6,7]. For the supercritical growth case, Li and Wang [8] obtained the existence of a nontrivial solution to p-Laplacian equations in R N using the Moser iteration and perturbation arguments. For more interesting results, see [9,10,11,12] and their references.
For another, from a physical point of view, some authors are interested in finding solutions to problem (1) with prescribed mass
R N | u | p d x = a p for a > 0 .
Under this circumstance, the parameter λ R is the Lagrange multiplier, which relies on the solution and is not a priori given. In our study, we intend to establish the existence of multiple weak solutions to problem (1). Here and after, by a solution, we always mean a couple ( u , λ ) , which satisfies problem (1). We refer to this type of solution as a normalized solution since condition (6) imposes a normalization on the L p -norm of u.
In the local case, i.e., s = 1 , the fractional Laplace ( Δ ) s reduces to the local differential operator Δ . In recent years, for some special forms of problem (1), many authors have obtained the existence, multiplicity, and asymptotic properties of normalized solutions under different conditions by various methods. For example, when p = 2 ,   B ( x ) = 0 and s = 1 , some authors have studied the following nonlinear elliptic problems:
Δ u = λ u + g ( u ) in R N , R N | u | 2 d x = a 2 .
Jeanjean [13] used mountain-pass geometry to study the existence of normalized solutions in purely L 2 -supercritical. Cazenave and Lions [14] showed the orbital stability of some standing waves in nonlinear Schrödinger equations when g ( u ) = | u | p 1 u for three cases. For the general case of g ( u ) , with a scaling argument, Shibata [15] studied (7). If g ( u ) = μ | u | q 2 u + | u | p 2 u , Soave [16] studied the existence and properties of solutions to the problem with prescribed mass for the L 2 -supercritical case with subcritical Sobolev growth. Moreover, they also gave the new criteria for global existence and finite-time blow-up in the associated dispersive equation. For the critical case, Jeanjean and Le [17] considered a class of Sobolev critical Schrödinger equation, and they proved the existence of standing waves that are not ground states while located at a mountain-pass level of the energy functional. Furthermore, when time is finite, these solutions are not stable because of blow-up.
For s 1 and B = 0 , Yu et al. [18] considered the following mass subcritical fractional Schrödinger equations:
( Δ ) s u = λ u + | u | p 2 u in Ω , u = 0 in 𝜕 Ω , Ω | u | 2 d x = a 2 ,
where s ( 0 , 1 ) , 2 < p < 2 + N 4 , Ω R N is an exterior domain with smooth boundary satisfying R N Ω contained in a small ball. For any a > 0 , they not only used barycentric functions to show the existence of a positive normalized solution but also used the minimax method and Brouwer degree theory. Moreover, if Ω is the complement of the unit ball in R N , for any a > 0 , they established the existence and multiplicity of radial normalized solutions according to genus theory. If we consider the case of whole space, Luo and Zhang [19] studied the fractional nonlinear Schrödinger equations with combined nonlinearities under different assumptions on parameters, and they proved some existence and nonexistence results about the normalized solutions.
Then, for p = 2 ,   B ( x ) 0 , there is some literature devoted to these problems:
( Δ ) s u + B ( x ) u = λ u + g ( x , u ) in R N , R N | u | 2 d x = a 2 .
If B and g satisfy some suitable assumptions, Ikoma and Miyamoto [20] proved the L 2 -constraint minimization exists and a minimizer to problem (9) does not exist. If g ( x , u ) = h ( ε x ) f ( u ) in problem (9), Zhang et al. [21] showed the existence of normalized solutions depends on the global maximum points of h when ε is small enough. For g ( x , u ) = | u | p 2 u , Peng and Xia [22] used a new min–max argument and splitting lemma for the nonlocal version to overcome the lack of compactness and proved that there exists at least one L 2 -normalized solution ( u , ω ) H s ( R N ) × R + of problem (9).
However, for the case p 2 , as far as we know, the results about the normalized solution of the p-Laplacian equation are relatively few. Wang et al. [23] considered the following p-Laplacian equation:
Δ p u + λ | u | p 2 u = μ u + | u | s 2 u in R N , R N | u | 2 d x = ρ 2 ,
where Δ p u = div ( | u | p 2 u ) , 1 < p < N , μ R , s ( N + 2 N p , p ) , p = N p N p is the critical Sobolev exponent. They proved that problem (10) has a normalized solution with constrained variational methods. Zhang and Zhang [24] is the first paper to study the following p-Laplacian equation:
Δ p u = λ | u | p 2 v + μ | u | q 2 u + g ( u ) in R N , R N | u | p d x = ρ p ,
where N 2 , ρ > 0 , 1 < p < q p ¯ : = p + p 2 N , μ R , g C ( R , R ) and λ R is a Lagrange multiplier. They used the Schwarz rearrangement and Ekeland variational principle to prove the existence of positive radial ground states for suitable μ . Recently, Wang and Sun [25] considered the following p-Laplacian equation with a trapping potential B ( x ) of the form:
Δ p u + B ( x ) | u | p 2 u = λ | u | r 2 u + | u | q 2 u in R N , R N | u | r d x = c ,
where 1 < p < N , ρ > 0 , r = p or 2, p < q < p and λ R is a Lagrange multiplier. The trapping potential B is a continuous function with B C ( R N , R ) L ( R N ) ,   B ( 0 ) = 0 satisfying
( A ) 0 = inf x R N B ( x ) < lim inf | x | + B ( x ) = B .
When r = p , they showed that problem (12) has a ground-state solution with positive energy for c small enough. When r = 2 , the authors also showed that problem (12) has at least two solutions, both with positive energy, where one is a ground state and the other is a high-energy solution.
Thin and Rădulescu [26] first considered the following fractional p-Laplace problem:
( Δ ) p s u + B ( ϖ x ) | u | p 2 u = λ | u | p 2 u + g ( u ) in R N , R N | u | p d x = a p ,
where ( Δ ) p s is the fractional p-Laplace operator, p 2 , a > 0 ,   ϖ > 0 ,   λ R is an uncharted Lagrange multiplier, the potential function B verifies condition ( B ) , and g is a continuous function with L p -subcritical growth. They proved the existence of multiple normalized solutions using the Lusternik–Schnirelmann category.
Inspired by the above literature, in this paper, we intend to prove the existence of multiple normalized solutions for a Choquard equation involving fractional p-Laplacian and potential functions. As far as we know, there are no results about the existence of multiple normalized solutions to problem (1). In order to give our main results, let us fix some notations and also assume that the nonlinearity g is a continuous differentiable function and satisfies the following growth conditions:
( g 1 )
g is an odd and continuous function, for q ( p ( N + α ) 2 N , p ( N + α ) + p 2 s 2 N ) ,   α ( 0 , + ) such that lim t 0 | g ( t ) | | t | q 1 = α .
( g 2 )
There are two positive constants c 1 ,   c 2 > 0 and p ( p ( N + α ) 2 N , p ( N + α ) + p 2 s 2 N ) ,   t R such that
| g ( t ) | c 1 + c 2 | t | p 1 .
( g 3 )
There is q 1 > p 2 such that g ( t ) t q 1 1 > 0 for all t ( 0 , + ) .
( g 4 )
There exists θ > 2 p such that 2 g ( t ) t θ G ( t ) > 0 for all t > 0 , where G ( t ) = 0 t g ( τ ) d τ .
In the present paper, we intend to prove the existence of multiple normalized solutions for problem (1) involving the nonautonomous case, i.e., the case B 0 , with the Lusternik–Schnirelmann category of the sets M and M δ given by
M = { x R N : B ( x ) = 0 }
and
M δ = { x R N : d i s t ( x , M ) δ } .
Here, we mention that if Y is a closed subset of a topological space X , and the Lusternik–Schnirelmann category c a t X ( Y ) is the least number of closed and contractible sets in X that cover Y. If X = Y , we use c a t ( X ) instead of c a t ( Y ) . For more details, see Willem [27].
Now, we are ready to state our main results in this paper.
Theorem 1.
Let g satisfy conditions ( g 1 ) ( g 4 ) and B satisfy condition ( B ) . Then for each δ > 0 , there exists ϖ 0 > 0 and B > 0 such that problem (1) admits at least c a t M δ ( M ) couples ( u j , λ j ) W s , p ( R N ) × R of weak solutions for 0 < ϖ < ϖ 0 and | B | < B while R N | u j | p d x = a p ,   λ j < 0 and J ϖ ( u j ) < 0 . Additionally, when u ϖ is one of these solutions, ζ ϖ is the global maximum of | u ϖ | , satisfies
lim ϖ 0 B ( ϖ ζ ϖ ) = 0 .
Remark 1.
Compared with the previous literature, our paper has the following characteristics:
( 1 )
When p 2 , the operator Δ p is no longer linear, which leads to some quite different properties from the classical Laplacian operator Δ . For example, for the case p = 2 , the equation
Δ p u + | u | p 2 u = | u | q 2 u i n R N
has a unique positive radially symmetric solution (see [28,29]), but in general cases, we know that this fact holds only for 1 < p < 2 (see [30,31]), and it is still unknown for 2 < p < N . Moreover, because of the nonlinear character of Δ p , the approach in Moroz and Van Schaftingen [32] becomes not simple for p-Laplacian operator Δ p with p 2 .
( 2 )
Unlike Li and Ye [33], we do not consider Hilbert space, and we cannot use some properties. For example, Wang et al. [23] use the workspace W 1 , p ( R N ) L 2 ( R N ) which is a Hilbert space. The workspace is Hilbert space and very important for Wang et al. [23] because they need the direct-sum decomposition.
( 3 )
Due to p 2 , it is difficult to prove that x · u W s , p ( R N ) for the nonlinearity of the operator ( Δ ) p s and its nonlocal character. Meanwhile, it is also hard to deal with an integration by parts formula for ( Δ ) p s . Moreover, we cannot directly adopt these methods in [24,25,26] due to nonlocal term [ 1 | x | N α G ( u ) ] g ( u ) . Therefore, we need to develop new techniques to overcome this difficulty and the loss of compactness due to the unbounded regions.
( 4 )
The nonlinearity g has L p -subcritical growth, so we need to estimate the mountain-pass level situated in a suitable interval when ( P S ) condition holds. To use the Ljusternik–Schnirelmann category theory, we establish some lemmas and technical results. Compared to the work by the authors in [26], the difficulties raise the Choquard term. We overcome this using the Hardy–Littlewood–Sobolev inequality and some new technique analysis steps.
Remark 2.
Our work is independent from [34]. Indeed, Chen and Wang studied problem (1) as ϖ = 1 and g has exponential growth in the Trudinger–Moser sense, and they did not study the multiple solutions. In our work, we study the nonautonomous problem and g has subcritical growth. We mainly use the Lusternik–Schnirelmann category to obtain multiple solutions. We also do not use the genus method as in He et al. [35] to obtain multiple solutions.
Remark 3.
In different research fields, we have different definitions of fractional operators and different applications. Here, we give some examples. In physics, Maheswari and Bakshi [36] mentioned a general time-fractional differential equation defined by ( 𝜕 α v / 𝜕 t α ) = F [ x , v , v x , v x x , v x x x ] , by using the invariant subspace method. For different equations with different operators of F, they obtain various solutions. In quantum mechanics, by using a method with the parameters of the system and Riemann–Liouville definition of the fractional derivatives, Al-Raeei [37] considered the Schrödinger equation for the electrical screening potential and obtained the amplitude of the wave functions for multiple values of the spatial fractional parameter. In kernel dynamics, Al Baidani et al. [38] considered magneto-acoustic waves in plasma. In a manner of Caputo derivatives, they studied the Caputo–Fabrizio and the Atangana–Baleanu derivatives. Finally, they obtained the solution calculated as a convergent series, and it was demonstrated that the NTDM solutions converge to the exact solutions. There are many applications of fractional order operators, and we will not give any examples here.
The paper is organized as follows: in Section 2, we consider the autonomous case associated with problem (1). In Section 3, we consider the nonautonomous case and give the corresponding energy functional. Moreover, to obtain the multiplicity consequence, we verify the Palais–Smale condition and establish some tools and lemmas. Finally, in Section 4, we give the proof of Theorem 1.

2. The Autonomous Case

In this section, we consider the autonomous case corresponding to problem (1). First, we list some notations for readers to study.
It is also known that the fractional Sobolev space W s , p ( R N ) is a uniformly convex Banach space equipped with the norm
u p : = u L p ( R N ) p + [ u ] s , p p ,
where
[ u ] s , p p = R 2 N | u ( x ) u ( y ) | p | x y | N + s p d x d y
and
u L p ( R N ) p = R N | u | p d x .
Then we give a statement of Lions’s theorem:
Lemma 1
(Ambrosio [39]). Let N > s p and r [ p , p s ) . If ( u n ) is a bounded sequence in W s , p ( R N ) and let
lim n sup y R N B R ( y ) | u n | r d x = 0
for some R > 0 . Then, u n 0 in L q ( R N ) for all q ( p , p s ) .
Lemma 2
(Lieb and Loss [40]). For r , t > 1 ,   0 < μ < N be such that 1 r + μ N + 1 t = 2 . For g L r ( R N ) and h L t ( R N ) . We have a constant C ( r , N , μ , t ) > 0 which does not depend on g and h such that
R N R N g ( x ) h ( y ) | x y | μ d x d y C ( r , N , μ , t ) g L r ( R N ) h L t ( R N ) .
If r = t = 2 N 2 N μ , for G ( u ) = | u | q , we can see
R N [ 1 | x | μ G ( u ) ] g ( u ) d x
is well defined on L t ( R N ) for t = 2 N 2 N μ .
Now, we consider the autonomous case corresponding to problem (1), i.e.,
( Δ ) p s u + μ | u | p 2 u = λ | u | p 2 u + 1 | x | N α G ( u ) g ( u ) in R N , R N | u | p d x = a p
where μ > 0 ,   a > 0 , α ( 0 , N ) , and λ is a Lagrange multiplier, which is an unknown parameter.
We denote the energy functional associated with problem (15) as follows:
I μ ( u ) = 1 p R 2 N | u ( x ) u ( y ) | p | x y | N + s p d x d y + μ R N | u | p d x 1 2 R N [ 1 | x | N α G ( u ) ] G ( u ) d x
restricted to the sphere S ( a ) and
S ( a ) = { u W s , p ( R N ) : u L p ( R N ) = a } .
Lemma 3.
The energy functional I μ is bounded and coercive on S ( a ) .
Proof. 
According to ( g 1 ) ( g 3 ) , there exist C 1 , C 2 > 0 such that
| G ( t ) | C 1 | t | q + C 2 | t | p , t R .
Then by the Hardy–Littlewood–Sobolev inequality in Lemma 2, we have
R N 1 | x | N α G ( u ) G ( u ) d x C N , α R N | G ( u ) | 2 N N + α d x N + α N .
Thus, there exists a suitable constant C > 0 such that
R N 1 | x | N α G ( u ) G ( u ) d x C R N | u | 2 N q N + α d x N + α N + R N | u | 2 N p N + α d x N + α N .
Because C 0 ( R N ) is density in W s , p ( R N ) for all u W s , p ( R N ) , the fractional Gagliardo–Nirenberg inequality (Nguyen and Squassina [41], Lemma 2.1) gives us
u L τ ( R N ) τ C u L p ( R N ) τ ( 1 a ) [ u ] s , p τ a ,
where τ > 0 ,   0 a 1 ,   C = C ( s , N , τ ) 1 and
1 τ = a ( 1 p s N ) + 1 a p .
Then, τ = p N N a p s [ p , p s ] and we deduce
u L τ ( R N ) τ N + α N C N + α N u L p ( R N ) τ ( 1 a ) N + α N [ u ] s , p τ a N + α N ,
where τ a N + α N = p , then a = p τ N N + α so τ = p + p 2 s N + α .
We can apply (16) for τ = 2 N q N + α , thus
R N | u | 2 N q N + α d x N + α N C 1 [ u ] s , p 2 N q a N
on S ( a ) = { u W s , p ( R N ) : u L p ( R N ) = a } , where C 1 > 0 is a suitable constant depending on a . Since q p ( N + α ) 2 N , p ( N + α ) + p 2 s 2 N , then 2 N q a N < p , where a = N s 1 p N + α 2 N q . Similarly, there exists C 2 > 0 such that
R N | u | 2 N p N + α d x N + α N C 2 [ u ] s , p 2 N p a N .
Hence, we have
I μ ( u ) = 1 p [ u ] s , p p + μ R N | u | p d x 1 2 R N 1 | x | N α G ( u ) G ( u ) d x 1 p [ u ] s , p p + μ R N | u | p d x 1 2 C R N | u | 2 N q N + α d x N + α N + R N | u | 2 N p N + α d x N + α N 1 p [ u ] s , p p + μ R N | u | p d x 1 2 C C 1 [ u ] s , p 2 N q a N 1 2 C C 2 [ u ] s , p 2 N p a N 1 p [ u ] s , p p C 3 [ u ] s , p 2 N q a N C 4 [ u ] s , p 2 N p a N .
Since q , p p ( N + α ) 2 N , p ( N + α ) + p 2 s 2 N , then 0 < 2 N t 1 a N < p , for t 1 { p , q } . Above all, we prove the coercivity and boundedness of I μ on S ( a ) . □
Thus, we obtain the existence of
I μ , a = inf u S ( a ) I μ ( u ) .
Then, we show some properties of I μ in relation to the parameter μ 0 .
Lemma 4.
There is a constant B > 0 such that I μ , a ( u ) < 0 when 0 μ < B .
Proof. 
Fix a function u 0 L ( R N ) S ( a ) ,   u 0 > 0 and let
H ( u 0 , t ) ( x ) = e N t p u 0 ( e t x ) for   all x R N and   all t R .
Obviously, we have
R N | H ( u 0 , t ) ( x ) | p d x = a p .
For any fixed t 0 , let
L ( m ) : = R N R N 1 | x | N α G ( m u 0 ) G ( m u 0 ) d x for   any m > 0 .
By using ( g 4 ) , for any m > 0 , we have
d L d m = R N 1 | x | N α G ( m u 0 ) G ( m u 0 ) d x = 2 m R N 1 | x | N α G ( m u 0 ) g ( m u 0 ) m u 0 d x > θ m L ( m ) .
Thus, integrating this on [ 1 , e N t p ] , we have
L ( e N t p ) L ( 1 ) ( e N t p ) θ
which yields
R N 1 | x | N α G ( e N t p u 0 ) G ( e N t p u 0 ) d x e N t θ p R N 1 | x | N α G ( u 0 ) G ( u 0 ) d x .
Note that
R 2 N | H ( u 0 , t ) ( x ) H ( u 0 , t ) ( y ) | p | x y | N + s p d x d y = e p s t R 2 N | u 0 ( x ) u 0 ( y ) | p | x y | N + s p d x d y
and so,
I μ ( H ( u 0 , t ) ) e N t p [ u 0 ] s , p p + μ a p p e N t θ p 2 R N 1 | x | N α G ( u 0 ) G ( u 0 ) d x .
Since θ > 2 p , we have N t θ p > 2 N t > N t , so increasing | t | if necessary, we deduce that
e N t p [ u 0 ] s , p p e N t θ p 2 R N 1 | x | N α G ( u 0 ) G ( u 0 ) d x = Q t < 0 .
Thus,
I μ ( H ( u 0 , t ) ) Q t + μ a p p .
Then, take B > 0 such that
Q t + B a p p < 0 .
Therefore, if μ < B , then we derive that for any μ [ 0 , B ) ,
I μ ( H ( u 0 , t ) ) < 0 ,
so I μ , a < 0 .  □
Lemma 5.
There exists a constant C > 0 and n 0 N such that
R N R N G ( u n ( y ) ) G ( u n ( x ) ) | x y | N α d x d y C f o r a l l n n 0 .
Proof. 
If we assume that there exists a subsequence ( u n ) , still denoted by itself such that
R N R N G ( u n ( y ) ) G ( u n ( x ) ) | x y | N α d x d y 0 as n + .
Then, we have
0 > I μ , a + o n ( 1 ) = I μ ( u n ) R N R N G ( u n ( y ) ) G ( u n ( x ) ) | x y | N α d x d y .
This is a contradiction. Therefore, we obtain the proof of Lemma 4. □
Lemma 6.
Let μ [ 0 , B ) and 0 < a 1 < a 2 . Then, a 1 p a 2 p I μ , a 2 < I μ , a 1 < 0 .
Proof. 
Since | | u ( x ) | | u ( y ) | | | u ( x ) u ( y ) | for all u W s , p ( R N ) , we obtain
R 2 N | | u ( x ) | | u ( y ) | | p | x y | N + s p d x d y R 2 N | u ( x ) u ( y ) | p | x y | N + s p d x d y .
Therefore, I μ ( u ) I μ ( | u | ) .
Fixing ϑ > 1 such that a 2 = ϑ a 1 and ( u n ) S ( a 1 ) be a nonnegative minimizing sequence with respect to the I μ , a 1 , which exists because I μ ( u ) I μ ( | u | ) for all u W s , p ( R N ) , i.e., when n + ,
I μ ( u n ) I μ , a 1 .
Letting u n = ϑ u n , then u n S ( a 2 ) . From ( g 3 ) , when t 1 and l > 0 , we obtain
G ( t l ) t q 1 G ( l ) .
Therefore,
I μ , a 2 I μ ( u n ) = I μ ( ϑ u n ) = 1 p R 2 N | ϑ u n ( x ) ϑ u n ( y ) | p | x y | N + s p d x d y + μ R N | ϑ u n | p d x 1 2 R N 1 | x | N α G ( ϑ u n ) G ( ϑ u n ) d x = ϑ p I μ ( u n ) + 1 2 ϑ p R N R N G ( u n ( y ) ) G ( u n ( x ) ) | x y | N α d x d y 1 2 R N R N G ( ϑ u n ( y ) ) G ( ϑ u n ( x ) ) | x y | N α d x d y ϑ p I μ ( u n ) + 1 2 ( ϑ p ϑ 2 q 1 ) R N R N G ( u n ( y ) ) G ( u n ( x ) ) | x y | N α d x d y .
When ϑ > 1 ,   2 q 1 > p , we obtain
ϑ p ϑ 2 q 1 < 0 .
By Lemma 5, fix n N large enough, we have
I μ , a 2 ϑ p I μ ( u n ) + 1 2 ( ϑ p ϑ 2 q 1 ) C .
Let n + , it is easy to obtain
I μ , a 2 ϑ p I μ , a 1 + ( ϑ p ϑ 2 q 1 ) C < ϑ p I μ , a 1 .
Then
a 1 p a 2 p I μ , a 2 < I μ , a 1 .
This completes the proof of Lemma 6. □
To overcome the loss of compactness, on S ( a ) , we establish the next theorem that will be used in the autonomous case and the nonautonomous case.
Lemma 7.
We fix μ [ 0 , B ) and ( u n ) S ( a ) To be a minimizing sequence with respect to I μ . Hereafter, either
( i )
( u n ) is a strongly convergent sequence,
or
( i i )
for ( y n ) R N and | y n | + , the sequence u n ( x ) = u n ( x + y n ) is strongly convergent to the function u S ( a ) and I μ ( u ) = I μ , a .
Proof. 
Let us prove it by contradiction. According to Lemma 3, for some subsequence in W s , p ( R N ) we have u n u . If u L p ( R N ) = b a and u 0 then b ( 0 , a ) and we use the Brézis-Lieb lemma [27],
u n L p ( R N ) p = u n u L p ( R N ) p + u L p ( R N ) p + o n ( 1 ) .
Moreover, as the same argument in Chen et al. [42], we have
R N R N G ( u n ( y ) ) G ( u n ( x ) ) | x y | N α d x d y = R N R N G ( ( u n u ) ( y ) ) G ( ( u n u ) ( x ) ) | x y | N α d x d y + R N R N G ( u ( y ) ) G ( u ( x ) ) | x y | N α d x d y + o n ( 1 ) .
Setting u n = u n u ,   d n = u n L p ( R N ) and supposing that u n L p ( R N ) d for n large enough, we have a p = b p + d p and d n ( 0 , a ) . Thus,
I μ , a + o n ( 1 ) = I μ ( u n ) = I μ ( u n ) + I μ ( u ) + o n ( 1 ) I μ , d n + I μ , b + o n ( 1 )
while combining Lemma 6, we deduce
I μ , a + o n ( 1 ) d n p a p I μ , a + I μ , b + o n ( 1 ) .
Fixing n , we have
I μ , a d p a p I μ , a + I μ , b .
Because b ( 0 , a ) , together with (22), Lemma 6, one has
I μ , a > d p a p I μ , a + b p a p I μ , a = I μ , a
which is absurd. Therefore, u L p ( R N ) = a , that is u S ( a ) .
Since u n u ,   u n L p ( R N ) = u L p ( R N ) = a in L p ( R N ) while L p ( R N ) is reflexive, so
u n u in L p ( R N ) .
Then make use of the interpolation theorem in the Lebesgue spaces, ( g 1 ) ( g 2 ) leads to
R N R N G ( u n ( y ) ) G ( u n ( x ) ) | x y | N α d x d y R N R N G ( u ( y ) ) G ( u ( x ) ) | x y | N α d x d y .
From I μ , a = lim n + I μ ( u n ) , we have
I μ , a I μ ( u ) .
Because u S ( a ) , it is easy to obtain that I μ , a = I μ ( u ) , and
lim n + I μ ( u n ) = I μ ( u ) = I μ , a ,
then utilize (23) with (24), we have
u n p u p ,
where · denotes the usual norm in W s , p ( R N ) . Therefore, in W s , p ( R N ) ,   u n u .
On the other hand, we suppose that u n 0 in W s , p ( R N ) . With Lemma 5, we know that there exists C > 0 such that for n N large
R N R N G ( u n ( y ) ) G ( u n ( x ) ) | x y | N α d x d y C .
According to Lemma 1, for y n R N , we have R ,   β > 0 and such that
B R ( y n ) | u n | p d x β , n R N .
Otherwise, by Ambrosio and Isernia [43]’s Lemma 2.1, it is easy to show that for all t ( p , p s ) ,   u n 0 in L t ( R N ) . It implies
G ( u n ( y ) ) G ( u n ( x ) ) | x y | N α 0
which contradicts (25). For u = 0 , with the inequality (26) and the fractional Sobolev embedding, we understand that ( y n ) is unbounded. From this, considering u ˜ n ( x ) = u ( x + y n ) , obviously ( u ˜ n ) S ( a ) , and it is also a minimizing sequence for I μ , a . Thus,
u ˜ n u ˜ in W s , p ( R N ) and u ˜ n ( x ) u ˜ ( x ) a . e . in R N
for u ˜ W s , p ( R N ) { 0 } . Above all, u ˜ n u ˜ in W s , p ( R N ) . This proves Lemma 7. □
Next, we state the main result of this section.
Theorem 2.
When g meets the conditions ( g 1 ) ( g 3 ) , there is B > 0 such that for 0 μ < B , problem (15) has a coupled ( u , λ ) solution and here, u is nonnegative while λ satisfies λ < 0 .
Proof. 
First, we prove λ < 0 . With Lemma 3, we have I μ ( u n ) = I μ , a . Then, using Theorem 7, we have I μ ( u ) = I μ , a . Thus, for λ a R and by the Lagrange multiplier, we have
I μ ( u ) = λ a Ψ μ ( u ) in ( W s , p ( R N ) ) ,
where u W s , p ( R N ) and Ψ : W s , p ( R N ) R is given by
Ψ ( u ) = R N | u | p d x .
Therefore, using (27) in R N , it is obvious to obtain that
( Δ ) p s u + μ | u | p 2 u = λ a | u | p 2 u + 1 | x | N α G ( u ) g ( u ) .
Since I μ ( u ) = I μ , a < 0 , we obtain λ a < 0 .
Next, we are going to prove that u is nonnegative. With the definition of the functional I μ , i.e., I μ ( u ) I μ ( | u | ) . Moreover, with u S ( a ) , then | u | S ( a ) , and
I μ , a = I μ ( u ) I μ ( | u | ) I μ , a
which implies that I μ , a = I μ ( | u | ) ; hence, we can replace u by | u | . Moreover, we denote u by Schwarz’s symmetrization of u (Almgren and Lieb [44], Section 9.2) that we have
R 2 N | u ( x ) u ( y ) | p | x y | N + s p d x d y R 2 N | u ( x ) u ( y ) | p | x y | N + s p d x d y , R N | u | p d x = R N | u | p d x
and
R N 1 | x | N α G ( u ) G ( u ) d x = R N 1 | x | N α G ( u ) G ( u ) d x ,
then u S ( a ) with I μ ( u ) = I μ , a . Therefore, we can replace u by u . For some α ( 0 , 1 ) by Iannizzotto et al. [45]’s Corollary 5.5, we have that u C α ( R N ) . This completes the proof of Theorem 2. □
According to Theorem 2, we deduce the next corollary:
Corollary 1.
Let a > 0 ,   0 μ 1 < μ 2 B . Then, I μ 1 , a < I μ 2 , a < 0 .
Proof. 
Fix μ 2 , a S ( a ) and I μ 2 ( u μ 2 , a ) = I μ 2 , a . Afterwards,
I μ 1 , a I μ 1 ( u μ 2 , a ) < I μ 2 ( u μ 2 , a ) = I μ 2 , a < 0 .
This completes the proof of Corollary 1. □

3. The Nonautonomous Case

In this section, we will study the nonautonomous case. The energy function J ϖ : W s , p ( R N ) R given by
J ϖ ( u ) = 1 p [ u ] s , p p + R N B ( ϖ x ) | u | p d x 1 2 R N 1 | x | N α G ( u ) G ( u ) d x ,
is restricted to the sphere
S ( a ) = { u W s , p ( R N ) : u L p ( R N ) = a } .
It and it is easy to prove that J ϖ ( u ) C 1 . Moreover
J ϖ ( u ) φ = R 2 N | u ( x ) u ( y ) | p 2 ( u ( x ) u ( y ) ) φ ( x ) φ ( y ) | x y | N + s p d x d y + B ( ϖ x ) R N | u | p 2 u φ d x R 2 N G ( u ( y ) ) g ( u ( x ) ) φ ( x ) | x y | N α d x d y .
Here, B is given in Section 3. We suppose that B L ( R N ) < B .
Then, we give some notations that will be used in the following. Let J 0 , J : W s , p ( R N ) R as
J 0 ( u ) = 1 p R 2 N | u ( x ) u ( y ) | p | x y | N + s p d x d y 1 2 R N 1 | x | N α G ( u ) G ( u ) d x
and
J ( u ) = 1 p R 2 N | u ( x ) u ( y ) | p | x y | N + s p d x d y + R N B | u | p d x 1 2 R N 1 | x | N α G ( u ) G ( u ) d x .
Additionally, we note Φ ϖ , a ,   Φ 0 , a and Φ , a by
Φ ϖ , a = inf u S ( a ) J ϖ ( u ) , Φ 0 , a = inf u S ( a ) J 0 ( u ) , Φ , a = inf u S ( a ) J ( u ) .
With 0 < B < + and Corollary 1, we have
Φ 0 , a < Φ , a < 0 .
Above all, we can fix 0 < ρ 1 = 1 2 ( Φ , a Φ 0 , a ) .
Then, we give a lemma to show the relationship among Φ ϖ , a ,   Φ 0 , a and Φ , a .
Lemma 8.
lim sup ϖ 0 + Φ ϖ , a Φ 0 , a and there is ϖ 0 > 0 satisfying Φ ϖ , a < Φ , a for all ϖ ( 0 , ϖ 0 ) .
Proof. 
Note u 0 S ( a ) and J 0 ( u 0 ) = Φ 0 , a . Then
Φ ϖ , a J ϖ ( u 0 ) = 1 p R 2 N | u 0 ( x ) u 0 ( y ) | p | x y | N + s p d x d y + R N B ( ϖ x ) | u 0 | p d x 1 2 R N 1 | x | N α G ( u 0 ) G ( u 0 ) d x .
Fixing ϖ 0 + , then
lim sup ϖ 0 + Φ ϖ , a lim ϖ 0 + J ϖ ( u 0 ) = J 0 ( u 0 ) = Φ 0 , a .
Combining (28) and (29), when ϖ is small enough, we obtain Φ ϖ , a < Φ , a .  □
Lemma 9.
Let ( u n ) S ( a ) , ϖ ( 0 , ϖ 0 ) such that J ϖ ( u n ) c and c < Φ 0 , a + ρ 1 < 0 . For u n u in W s , p ( R N ) , we have u 0 .
Proof. 
When u = 0 , it is easy to deduce that
Φ 0 , a + ρ 1 + o n ( 1 ) > J ϖ ( u n ) = J ( u n ) + 1 p R N B ( ϖ x ) B | u n | p d x .
By condition of ( B ) for ζ 1 > 0 , there exists R > 0 such that
B ( x ) B ζ 1 , | x | R .
Therefore,
Φ 0 , a + ρ 1 + o n ( 1 ) > J ϖ ( u n ) J ( u n ) + 1 p B R ϖ ( 0 ) B ( ϖ x ) B | u n | p d x ζ 1 p B R ϖ c ( 0 ) | u n | p d x .
Since ( u n ) is bounded in W s , p ( R N ) while for all γ [ 1 , p s ) ,   u n 0 in L γ ( B R ϖ ( 0 ) ) for some K > 0 , we have
Φ 0 , a + ρ 1 + o n ( 1 ) J ( u n ) ζ 1 K Φ , a ζ 1 K .
Because ζ 1 > 0 is arbitrary, we have
Φ 0 , a + ρ 1 Φ , a
which is a contradiction with the definition of ρ 1 = 1 2 ( Φ , a Φ 0 , a ) . Therefore, we obtain u 0 .  □
Lemma 10.
Assume that g satisfies condition ( g 1 ) ( g 3 ) and ( u n ) is a bounded sequence in W s , p ( R N ) . Hereafter, there exists C 0 > 0 such that
| 1 | x | μ G ( u n ) | C 0 f o r a l l n .
Proof. 
According to condition ( g 1 ) , for all t R , we have
| G ( t ) | C ( | t | q + | t | p ) .
Thus, with the boundedness of ( u n ) and Lemma 2, we have
| 1 | x | N α G ( u n ) | | | x y | 1 G ( u n ( y ) ) | x y | N α d y | + | | x y | 1 G ( u n ( y ) ) | x y | N α d y |
C | x y | 1 | u n | q + | u n | p | x y | N α d y + R N ( | u n | q + | u n | p ) d y
C | x y | 1 | u n | q + | u n | p | x y | N α d y + C .
By using the Hölder inequality for max { 1 , p p } < t < p s p , we obtain
| x y | 1 | u n | p | x y | N α d y | x y | 1 | u n | p t 1 t | x y | 1 1 | x y | t ( N α ) t 1 d y t 1 t C < 0 1 ρ N 1 t ( N α ) t 1 d ρ t 1 t < + ,
because of N 1 t ( N α ) t 1 > 1 . Similarly, for max { 1 , p q } < r < p s q , we obtain
| x y | 1 | u n | q | x y | N α d y | x y | 1 | u n | q r 1 r | x y | 1 1 | x y | r ( N α ) r 1 d y r 1 r C < 0 1 ρ N 1 r ( N α ) r 1 d ρ r 1 r < + ,
due to N 1 r ( N α ) r 1 > 1 . Combining (33) and (34), we prove that
| x y | 1 | u n | q + | u n | p | x y | N α d y C for all x R N
which in view of (31) yields
| 1 | x | μ G ( u n ) | C 0 for all n .
Above all, we end the proof. □
Lemma 11.
Note that ( u n ) S ( a ) is a ( P S ) c sequence for J ϖ constrained to S ( a ) satisfying c < Φ 0 , a + ρ 1 < 0 and u n u ϖ in W s , p ( R N ) , when n ,
J ϖ ( u n ) c a n d J ϖ | S ( a ) ( u n ) 0 .
For u n = u n u ϖ 0 in W s , p ( R N ) , we understand that β > 0 does not depend on ϖ ( 0 , ϖ 0 ) and
lim inf n + u n u ϖ L p ( R N ) p β .
Proof. 
Note Ψ : W s , p ( R N ) R is given by
Ψ ( u ) = 1 p R N | u | p d x , u W s , p ( R N ) ,
we find that S ( a ) = Ψ 1 ( { a p / p } ) . Hereafter, according to Willem [27]’s Proposition 5.12, it is easy to obtain a sequence ( λ n ) R satisfying
J ϖ ( u n ) λ n Ψ ( u n ) ( W s , p ( R N ) ) 0 a s n + .
Because ( u n ) is bounded in W s , p ( R N ) and ( λ n ) is also a bounded sequence, so up to a subsequence, when n + , we can assume that λ n λ ϖ . Therefore
J ϖ ( u n ) λ ϖ Ψ ( u ϖ ) = 0 in ( W s , p ( R N ) ) .
In order to prove (35), the following claims need to be proved.
Claim 1.
For all φ W s , p ( R N )
R N R N G ( u n ( y ) ) g ( u n ( x ) ) φ ( x ) | x y | N α d x d y R N R N G ( u ϖ ( y ) ) g ( u ϖ ( x ) ) φ ( x ) | x y | N α d x d y
Since u n is bounded in W s , p ( R N ) , by Lemma 10, there exists C 0 > 0 such that
| 1 | x | N α G ( u n ) | C 0 for all n .
Thus, combining the Vitali’s Convergence Theorem and φ W s , p ( R N ) , it is easy to deduce that
| R N 1 | x | N α G ( u n ) ( g ( u n ) g ( u ϖ ) ) φ d x | C 0 | R N ( g ( u n ) g ( u ϖ ) ) φ d x | 0 .
By the growth conditions on g and the boundedness of ( u n ) in W s , p ( R N ) imply that G ( u n ) is bounded in L 2 N N + α ( R N ) . Observe that u n u ϖ in L 2 N N + α ( R N ) . Then, we may assume G ( u n ) G ( u ϖ ) in L 2 N N + α ( R N ) . It is easy to see that g ( u ϖ ) φ L 2 N N + α ( R N ) , so 1 | x | N α ( g ( u n ) φ ) L 2 N N α ( R N ) . Therefore,
| R N 1 | x | N α ( G ( u n ) G ( u ϖ ) ) g ( u ϖ ) φ d x | = | R N ( G ( u n ) G ( u ϖ ) ) 1 | x | N α ( g ( u ϖ ) φ ) d x | 0
for any φ W s , p ( R N ) . In view of (37) and (38), we infer
| R N R N G ( u n ( y ) ) g ( u n ( x ) ) φ ( x ) | x y | N α d x d y R N R N G ( u ϖ ( y ) ) g ( u ϖ ( x ) ) φ ( x ) | x y | N α d x d y | | R N 1 | x | N α G ( u n ( y ) ) g ( u n ( x ) ) g ( u ϖ ( x ) ) φ ( x ) d x | + | R N 1 | x | N α G ( u n ( y ) ) G ( u ϖ ( y ) ) g ( u ϖ ( x ) ) φ ( x ) d x | 0 .
Consequently, Claim 1 is proved.
Claim 2.
We verify that R N | u n | p 2 u n φ d x R N | u ϖ | p 2 u ϖ φ d x for all φ W s , p ( R N ) .
Since W s , p ( R N ) is continuously embedded into L q ( R N ) for all q ( p , p s ) , then φ L q ( R N ) C φ < + . Then we have R > 0 such that
R N B R ( 0 ) | φ | p d x < ε p and R N B R ( 0 ) | φ | q d x < ε q .
Thus, we obtain
R N | u n | p 2 u n φ d x R N | u ϖ | p 2 u ϖ φ d x
as n .
Claim 3.
We prove that
R 2 N | u n ( x ) u n ( y ) | p 2 ( u n ( x ) u n ( y ) ) ( φ ( x ) φ ( y ) ) | x y | N + s p d x d y R 2 N | u ϖ ( x ) u ϖ ( y ) | p 2 ( u ϖ ( x ) u ϖ ( y ) ) ( φ ( x ) φ ( y ) ) | x y | N + s p d x d y .
Using the Hölder inequality, it is easy to obtain
R 2 N | | u n ( x ) u n ( y ) | p 2 ( u n ( x ) u n ( y ) ) ( φ ( x ) φ ( y ) ) | x y | N + s p | d x d y R 2 N | u n ( x ) u n ( y ) | p | x y | N + s p d x d y ( p 1 ) / p R 2 N | φ ( x ) φ ( y ) | p | x y | N + s p d x d y 1 / p u n p 1 φ < + .
Thus | u n ( x ) u n ( y ) | p 2 ( u n ( x ) u n ( y ) ) ( φ ( x ) φ ( y ) ) | x y | N + s p L 1 ( R 2 N ) for all n , and for all ( x , y ) R 2 N outside a set with measure zero when we have a constant K > 0 , then
| | u n ( x ) u n ( y ) | p 2 ( u n ( x ) u n ( y ) ) ( φ ( x ) φ ( y ) ) | x y | N + s p | K .
For every ε > 0 , there exists δ = ε K such that for all measurable set E R 2 N , | E | < δ , we have
E | | u n ( x ) u n ( y ) | p 2 ( u n ( x ) u n ( y ) ) ( φ ( x ) φ ( y ) ) | x y | N + s p | d x d y K | E | < ε .
Therefore, | u n ( x ) u n ( y ) | p 2 ( u n ( x ) u n ( y ) ) ( φ ( x ) φ ( y ) ) | x y | N + s p is equi-integrable on R 2 N and
| u n ( x ) u n ( y ) | p 2 ( u n ( x ) u n ( y ) ) ( φ ( x ) φ ( y ) ) | x y | N + s p | u ϖ ( x ) u ϖ ( y ) | p 2 ( u ϖ ( x ) u ϖ ( y ) ) ( φ ( x ) φ ( y ) ) | x y | N + s p
a . e . on R 2 N . For φ W s , p ( R N ) , then, there exists R > 0 such that
R 2 N B R ( 0 ) | φ ( x ) φ ( y ) | p | x y | N + s p d x d y < ε p ,
where B R ( 0 ) is a ball in R 2 N with center 0 and radius R . From (42), we know that ( u n ) is bounded in W s , p ( R N ) , then integrate on R 2 N B R ( 0 ) , for a suitable constant K > 0 ,
| R 2 N B R ( 0 ) | u n ( x ) u n ( y ) | p 2 ( u n ( x ) u n ( y ) ) ( φ ( x ) φ ( y ) ) | x y | N + s p d x d y | R 2 N B R ( 0 ) | u n ( x ) u n ( y ) | p | x y | N + s p d x d y ( p 1 ) / p × R 2 N B R ( 0 ) | φ ( x ) φ ( y ) | p | x y | N + s p d x d y 1 / p < K ε .
Thus, we prove that the Vitali’s theorem holds, so (41) holds.
According to Bartsch and Wang ([46], Lemma 2.6),
J ϖ ( u n ) = J ϖ ( u ϖ ) + J ϖ ( u n ) + o n ( 1 )
and
Ψ ϖ ( u n ) = Ψ ϖ ( u ϖ ) + Ψ ϖ ( u n ) + o n ( 1 ) .
Above all equalities and (35), we deduce that
J ϖ ( u n ) λ ϖ Ψ ϖ ( u n ) = J ϖ ( u ϖ ) λ ϖ Ψ ϖ ( u ϖ ) + J ϖ ( u n ) λ ϖ Ψ ϖ ( u n ) + o n ( 1 ) = J ϖ ( u n ) λ ϖ Ψ ϖ ( u n ) + o n ( 1 ) ,
thus for n + ,
J ϖ ( u n ) λ ϖ Ψ ( u n ) ( W s , p ( R N ) ) 0 .
By ( g 3 ) for all t 0 , we have q 1 G ( t ) g ( t ) t . Then
0 > Φ 0 , a + ρ 1 lim inf n + J ϖ ( u n ) = lim inf n + J ϖ ( u n ) 1 p J ϖ ( u n ) u n + 1 p λ ϖ a p 1 p λ ϖ a p
and
lim sup ϖ 0 λ ϖ p ( ρ 1 + Φ 0 , a ) a p < 0 .
Hence, we have λ 1 < 0 which does not depend on ϖ such that
λ ϖ λ 1 < 0 , ϖ ( 0 , ϖ 0 ) .
According to (43), we have
R 2 N | u n ( x ) u n ( y ) | p | x y | N + s p d x d y + R N B ( ϖ x ) | u n | p d x λ ϖ R N | u n | p d x = R 2 N G ( u n ( y ) ) g ( u n ( x ) ) u n ( x ) | x y | N α d x d y + o n ( 1 ) .
Combining (44) and (45), we deduce
R 2 N | u n ( x ) u n ( y ) | p | x y | N + s p d x d y + R N B ( ϖ x ) | u n | p d x λ 1 R N | u n | p d x R 2 N G ( u n ( y ) ) g ( u n ( x ) ) u n ( x ) | x y | N α d x d y + o n ( 1 ) .
From Lemma 2, for suitable constants C > 0 and D 3 > 0 , we have
R 2 N G ( u n ( y ) ) g ( u n ( x ) ) u n ( x ) | x y | N α d x d y C G ( u n ) L 2 N N + α ( R N ) g ( u n ( x ) ) u n ( x ) L 2 N N + α ( R N ) 2 C θ g ( u n ( x ) ) u n ( x ) L 2 N N + α ( R N ) D 3 ( u n ( x ) L 2 N p N + α ( R N ) 2 p + u n L 2 N q N + α ( R N ) 2 q )
Above all, we have
R 2 N | u n ( x ) u n ( y ) | p | x y | N + s p d x d y + C 0 R N | u n | p d x R 2 N G ( u n ( y ) ) g ( u n ( x ) ) u n ( x ) | x y | N α d x d y + o n ( 1 ) D 3 ( u n ( x ) L 2 N p N + α ( R N ) 2 p + u n L 2 N q N + α ( R N ) 2 q ) + o n ( 1 ) ,
where C 0 is a constant and does not depend on ϖ ( 0 , ϖ 0 ) . With the Sobolev embedding W s , p ( R N ) L p ( R N ) ,
u n W s , p ( R N ) p D 3 ( u n ( x ) L 2 N p N + α ( R N ) 2 p + u n L 2 N q N + α ( R N ) 2 q ) + o n ( 1 ) D 4 ( u n W s , p ( R N ) 2 p + u n W s , p ( R N ) 2 q ) + o n ( 1 ) ,
where D 3 and D 4 are two constants that do not depend on ϖ ( 0 , ϖ 0 ) . For u n 0 in W s , p ( R N ) , for a subsequence of ( u n ) , we assume that lim inf n + u n W s , p ( R N ) > 0 . Since 2 p > p , 2 q > p , by (47), there is a suitable constant D 5 > 0 such that
lim inf n + u n W s , p ( R N ) D 5 > 0 .
Combining (47) and (48), we have
lim inf n + u n L 2 N p N + α ( R N ) 2 p D 6 ,
or
lim inf n + u n L 2 N q N + α ( R N ) 2 q D 6 ,
where D 6 is a constant independent of ϖ ( 0 , ϖ 0 ) . Indeed, if
lim inf n + u n L 2 N p N + α ( R N ) 2 p = 0
and
lim inf n + u n L 2 N q N + α ( R N ) 2 q = 0 ,
then lim inf n + u n W s , p ( R N ) p = 0 via (47). This is a contradiction. Please note that
p , q ( p ( N + α ) 2 N , p ( N + α ) + p 2 s 2 N ) ,
then 2 N p N + α , 2 N q N + α ( p , p s ) . We denote p 1 = 2 N p N + α , q 1 = 2 N q N + α ( p , p s ) . Applying the fractional Gagliardo–Nirenberg inequality, we obtain
u n L t ( R N ) t C s , N , t u n L p ( R N ) t ( 1 a ) [ u n ] s , p t a ,
for all t { p 1 , q 1 } , then for all n N , we have
lim inf n + u n L t ( R N ) t C s , N , t ( lim inf n + u n L p ( R N ) ) t ( 1 a ) G t a ,
where G is a positive constant independent of ϖ ( 0 , ϖ 0 ) and [ u n ] s , p G . With (49), (50) and (53), we understand that there exists β > 0 independent of ϖ ( 0 , ϖ 0 ) such that
lim inf n + u n u ϖ L p ( R N ) p β .
This completes the proof of Lemma 11. □
From here, we let ρ satisfy 0 < ρ < min { 1 p , β a p } ( Φ , a Φ 0 , a ) ρ 1 .
Lemma 12.
Let ϖ ( 0 , ϖ 0 ) ,   J ϖ satisfy the ( P S ) c condition restricted on S ( a ) with c < Φ 0 , a + ρ .
Proof. 
Note that ( u n ) S ( a ) is a ( P S ) c sequence for J ϖ constrained to S ( a ) and u n u ϖ in W s , p ( R N ) while c < Φ 0 , a + ρ < 0 . Note that Ψ : W s , p ( R N ) R . As
Ψ ( u ) = 1 p R N | u | p d x , u W s , p ( R N ) ,
we find S ( a ) = Ψ 1 ( { a p / p } ) . According to Willem [27]’s Proposition 5.12 as n + , for a sequence ( λ n ) R , we have
J ϖ ( u n ) λ n Ψ ( u n ) ( W s , p ( R N ) ) 0 .
According to Lemma 11, for u n = u n u ϖ 0 in W s , p ( R N ) , and there exists β > 0 , which does not depend on ϖ ( 0 , ϖ 0 ) , such that
lim inf n + u n u ϖ L p ( R N ) p = lim inf n + u n L p ( R N ) p β ,
where ϖ 0 is given in Lemma 8.
Setting d n = u n L p ( R N ) , while assuming that u n L p ( R N ) d > 0 and u ϖ L p ( R N ) = b , we have a p = b p + d p . According to Lemma 9, for large enough n we have b > 0 and J ϖ ( u n ) Φ , d n + o n ( 1 ) , so we must obtain d n ( 0 , a ) . Hence,
c + o n ( 1 ) = J ϖ ( u n ) = J ϖ ( u n ) + J ϖ ( u ϖ ) + o n ( 1 ) Φ , d n + Φ 0 , b + o n ( 1 )
as well as Lemma 6,
ρ + Φ 0 , a d n p a p Φ , a + b p a p Φ 0 , a .
Fixing n , we deduce
ρ d p a p ( Φ , a Φ 0 , a ) β a p ( Φ , a Φ 0 , a )
which is absurd when ρ < β a p ( Φ , a Φ 0 , a ) . Thus, u n 0 in W s , p ( R N ) , and u n u ϖ in W s , p ( R N ) . Thus, u ϖ L p ( R N ) = a and when λ ϖ is the limit of some subsequence of ( λ n ) ,
( Δ ) p s u ϖ + B ( ϖ x ) | u ϖ | p 2 u ϖ = λ ϖ | u ϖ | p 2 u ϖ + 1 | x | N α G ( u ϖ ) g ( u ϖ ) in R N .
This completes the proof of Lemma 12. □

4. Multiplicity Result of Problem (1)

Let δ > 0 and w > 0 be the solution of the following problem
( Δ ) p s u = λ | u | p 2 u + 1 | x | N α G ( u ) g ( u ) in R N , R N | u | p d x = a p ,
with J 0 ( w ) = Φ 0 , a . Let η : 0 , + 0 , 1 be a smooth non-increasing cut-off function satisfying η t = 1 if 0 t δ 2 as well as η t = 0 if t δ . For any y M , we set the function Ψ ϖ , y : R N R
Ψ ϖ , y x : = η ϖ x y w ϖ x y ϖ ,
Ψ ˜ ϖ , y ( x ) = a Ψ ϖ , y ( x ) Ψ ϖ , y L p ( R N )
while denoting by Ξ ϖ : M S ( a ) the function
Ξ ϖ y = Ψ ˜ ϖ , y .
Therefore, for every y M ,   Ξ ϖ y has compact support.
Lemma 13.
The functional Ξ ϖ meets
lim ϖ 0 + J ϖ Ξ ϖ y = Φ 0 , a u n i f o r m l y   i n y M .
Proof. 
We assume by contradiction that there exist δ 0 > 0 , ( y n ) M and ϖ n 0 such that
J ϖ n ( Ξ ϖ n ( y n ) ) Φ 0 , a δ 0 , n N .
Let z = ϖ n x y n ϖ n and z ¯ = ϖ n y y n ϖ n , we can obtain
J ϖ n Ξ ϖ n y n = 1 p η ϖ n z w z s , p p + R N B ϖ n z + y n η ϖ n z w z p d z 1 2 R N R N G η ϖ n z ¯ w z ¯ G η ϖ n z w z | z z ¯ | N α d z d z ¯ .
By the Lebesgue-dominated convergence theorem as in Molica Bisci et al. [47]’s Lemma 17 and Palatucci and Pisante [48]’s Lemma 5,
lim n R N | Ψ ϖ n , y n | p d x = lim n R N | η ϖ n z w z | p d x = R N | w | p d x = a p ,
lim n R 2 N | Ξ ϖ n ( y n ) ( x ) Ξ ϖ n ( y n ) ( y ) | p | x y | N + s p d x d y = [ w ] s , p p
and
lim n R N R N G η ϖ n z ¯ w z ¯ G η ϖ n z w z | z z ¯ | N α d z d z ¯ = R N R N G w ( z ¯ ) G w ( z ) | z z ¯ | N α d z d z ¯ .
From Ambrosio and Isernia [43]’s Lemmas 2.2 and 2.5, we also have
lim n R N B ( ϖ n x ) | Ξ ϖ n ( y n ) | p d x = lim n R N a p Ψ ϖ n , y L p ( R N ) p B ( ϖ n z + y n ) | η ϖ n z w ( z ) | p d z = 0 .
As a consequence, this yields
lim n J ϖ n Ξ ϖ n y n = J 0 w = Φ 0 , a
which contradicts (56). □
Now, we fix R = R ( δ ) > 0 and choose δ > 0 such that M δ B R ( 0 ) . Then note Υ : R N R N by letting Υ ( x ) = x for | x | R as well as Υ ( x ) = R x x for | x | R . Hereafter, let β ϖ : S ( a ) R N given by
β ϖ u = R N Υ ϖ x | u | p d x a p .
Lemma 14
(Ambrosio [4]). The function β ϖ meets
lim ϖ 0 β ϖ Ξ ϖ y = y   u n i f o r m l y   i n   y M .
Proof. 
With Ambrosio and Isernia [43]’s Lemma 4.18, assuming that there exists δ 0 > 0 , ( y n ) M and ϖ n 0 such that
β ϖ n Ξ ϖ n y n y n δ 0 .
By using the definitions of Ξ ϖ n y n , β ϖ n and η , we deduce that
β ϖ n Ξ ϖ n y n = y n + R N Υ ϖ n z + y n y n η ϖ n z w z p d z a p .
With the Dominated Convergence Theorem and ( y n ) M B R ( 0 ) ,
β ϖ n Ξ ϖ n y n y n = o n 1 ,
which contradicts (57). □
Arguing as in the proof of Ambrosio [3], we have the next lemma.
Lemma 15.
Fix ϖ n 0 and ( u n ) S ( a ) be such that J ϖ n ( u n ) Φ 0 , a . Then, there exists ( y ˜ n ) R N such that u n x = u n x + y ˜ n has a convergent subsequence in W s , p ( R N ) . Additionally, up to a subsequence, y n = ϖ n y ˜ n y M .
Proof. 
Since J ϖ n ( u n ) , u n = 0 ,   J ϖ n ( u n ) Φ 0 , a and we can argue that ( u n ) is bounded. Then, for two constants R > 0 ,   β > 0 , and a sequence ( y ˜ n ) R N we have
lim inf n B R ( y ˜ n ) | u n | p d x β > 0 .
We surmise that the assumption is invalid. Hence, for all R > 0 ,
lim n sup y R N B R ( 0 ) | u n | p d x = 0 .
Since ( u n ) is bounded in W s , p ( R N ) , according to Lemma 1, for any q ( p , p s ) ,   u n 0 in L q ( R N ) , then R N 1 | x | N α G ( u n ) G ( u n ) d x 0 . Therefore, according to lim n + J ϖ n ( u n ) = Φ 0 , a < 0 , we have the contradiction with lim n + J ϖ n ( u n ) 0 .
Then, we set u n ( x ) = u n ( x + y ^ n ) . There exists u W s , p ( R N ) { 0 } and for a subsequence, u n u in W s , p ( R N ) . Because
Φ 0 , a J 0 ( u n ) = J 0 ( u n ) J ϖ n ( u n ) and ( u n ) S ( a ) ,
we have J 0 ( u n ) Φ 0 , a . Using Theorem 7, it is easy to deduce that u n u in W s , p ( R N ) and ( u n ) S ( a ) . Then, we show that ( y n ) is bounded.
Using rebuttals of evidence, we may hypothesize that there exists a subsequence of ( y n ) such that | y n | when n , and we have
Φ 0 , a = lim n + J ϖ n ( u n ) = lim inf n + ( 1 p R 2 N | u n ( x ) u n ( y ) | p | x y | N + s p d x d y + R N B ( ϖ n x + y n ) | u n | p d x 1 2 R N 1 | x | N α G ( u n ) G ( u n ) d x ) ,
i.e.,
Φ 0 , a 1 p [ u n ] s , p p + R N B | u n | p d x 1 2 R N 1 | x | N α G ( u n ) G ( u n ) d x Φ , a
which gives an absurd with (28). Therefore, we understand that ( y n ) is bounded, so in R N , we suppose that y n y .
Above all, it is easy to derive that
Φ 0 , a 1 p [ u n ] s , p p + R N B | u n | p d x 1 2 R N 1 | x | N α G ( u n ) G ( u n ) d x Φ B ( y ) , a .
If y M , with Corollary 1 and B ( y ) > 0 , we have Φ B ( y ) , a > Φ 0 , a , which is a contradiction, then B ( y ) = 0 , and y M .  □
We set h ( ϖ ) as a positive function satisfying h ( ϖ ) 0 as ϖ 0 . We define
S ˜ ( a ) = u S ( a ) : J ϖ ( u ) Φ 0 , a + h ( ϖ ) .
For any y M , according to Lemma 13, when ϖ 0 ,   h ϖ = J ϖ Ξ ϖ y Φ 0 , a 0 . Thus, Φ ϖ y S ˜ ( a ) for any ϖ > 0 .
Inspired by Alves and Figueiredo [49] and Alves and Thin [50]’s Lemma 4.5, then we give the next Lemma.
Lemma 16.
We set δ > 0 and M δ = { x R N : d i s t ( x , M ) δ } , so it holds that
lim ϖ 0 sup u S ˜ ( a ) inf z M δ | β ϖ u z | = 0 .
Proof. 
We fix ϖ n 0 as n . Then, there exists u n S ˜ ( a ) such that
inf z M δ | β ϖ u z | = sup u S ˜ ( a ) inf z M δ | β ϖ u z | + o n 1 .
Hence, there exists ( y ˜ n ) M δ such that
lim n β ϖ n u n y ˜ n = 0 .
Since u n S ˜ ( a ) ,
Φ 0 , a J 0 ( u n ) J ϖ n u n Φ 0 , a + h ϖ n ,
i.e.,
u n S ( a ) and J ϖ n u n Φ 0 , a .
Using Lemma 15, for large enough n, we obtain that there exists ( y ˜ n ) R N such that y n = ϖ n y ˜ n M δ . By setting u n = u n x + y ˜ n and using a change in variable, we deduce
β ϖ n u n = y n + R N Υ ϖ n z + y n y n u n p d z a p
and
β ϖ n u n y n = R N Υ ϖ n z + y n y n u n p d z a p 0 when n .
This completes the proof of Lemma 16. □
Proof of Theorem 1.
To prove Theorem 1, we use two steps.
Step 1. We first verify the existence of multiple normalized solutions to problem (1).
For ϖ ( 0 , ϖ 0 ) : According to Lemma 13, Lemma 14 and Lemma 16 and the arguments in Cingolani and Lazzo [51], we can understand that β ϖ Ξ ϖ is a homotopic to the inclusion map id: M M δ . Combining Ambrosio [39]’s Lemma 6.3.21, it is clear we have
c a t S ˜ ( a ) c a t M δ M .
Furthermore, let us choose a function h ϖ > 0 such that h ϖ 0 as ϖ 0 as well as Φ 0 , a + h ϖ is not a critical level for J ϖ . According to arguments as in Lemma 4, on S ( a ) , we deduce that J ϖ is bounded. For small enough ϖ > 0 , we deduce from Lemma 12 that J ϖ satisfies the Palais–Smale condition in S ( a ) . With the Lusternik–Schnirelman category theorem for critical points in Ghoussoub [52] and Wang et al. [23], it is easy to obtain that J ϖ admits at least c a t M δ M critical points on S ( a ) .
Step 2. We study the behavior of maximum points of | u ϖ | .
For h, given in (58), we fix u ϖ as a solution of problem (1) with J ϖ ( u ϖ ) Φ 0 , a + h ( ϖ ) . Using the proof of Lemma 15, for each ϖ n 0 , there exists ( y ˜ n ) R N such that y n = ϖ n y ˜ n y 0 M and u n ( x ) = u ϖ n x + y ˜ n has a convergent subsequence in W s , p ( R N ) and u 0 . Then, u n is a solution of
( Δ ) p s u n + B ( ϖ n x + y n ) | u n | p 2 u n = λ n | u n | p 2 u n + 1 | x | N α g ( u n ) in R N
and
lim sup ϖ 0 λ ϖ p ( ρ 1 + Φ 0 , a ) a p < 0 .
Since u n u in W s , p ( R N ) , then, applying the same arguments found in Alves and Figueiredo [49]’s Lemma 4.5, we obtain
lim | x | u n ( x ) = 0 uniformly   in n N .
Thus, there are R 1 > 0 ,   n 0 N and τ > 0 such that
| u n ( x ) | 1 2 τ 2 | B R 1 ( 0 ) | 1 p for | x | R 1 and n n 0 .
We know that u n L ( R N ) 0 , because u n L 2 = a , which contradicts u n 0 in W s , p ( R N ) .
Then, with (28), when n is large enough, we pick R 1 > τ 0 such that
0 < τ 2 B R 1 ( 0 ) | u n | p d x | B R 1 ( 0 ) | · u n L ( R N ) p
when we choose δ = τ 2 | B R 1 ( 0 ) | 1 p . We have that there exists δ > 0 such that u n L δ . In the following, let us consider ζ n R N such that | u n ( ζ n ) | = u n L ( R N ) for all n N . Then, ζ n = z n + y ˜ n and
lim n + B ( ϖ n ζ n ) = lim n + B ( ϖ n z n + ϖ n y ˜ n ) = B ( y ) = 0 .
 □

5. Conclusions and Future Studies

In our study above, by using variational methods, minimization techniques, and the Lusternik–Schnirelmann category, we obtain the existence of multiple normalized solutions. Moreover, under the autonomous case and nonautonomous case, we prove Theorem 1. In future studies, we will change the growth of g to exponential growth. In this process, forced proof will be affected, and we need to explore new methods to solve this problem. At the same time, we will try our best to explore the practical application of the research problem.

Author Contributions

Writing–original draft, X.Z.; Writing—review & editing, S.L.; Funding acquisition, S.L. All authors have read and agreed to the published version of the manuscript.

Funding

S. Liang was supported by the Science and Technology Development Plan Project of Jilin Province, China (Grant No. YDZJ202201ZYTS582), the Young Outstanding Talents Project of Scientific Innovation and Entrepreneurship in Jilin (No. 20240601048RC), the National Natural Science Foundation of China (Grant No. 12371455), Natural Science Foundation of Changchun Normal University (No. CSJJ2023004GZR), the Research Foundation of Department of Education of Jilin Province (Grant No. JJKH20230902KJ) and the Innovation and Entrepreneurship Talent Funding Project of Jilin Province (Grant No. 2023QN21).

Data Availability Statement

Data are contained within the article.

Conflicts of Interest

The authors declare that they have no competing interests.

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Zhang, X.; Liang, S. Multiple Normalized Solutions to a Choquard Equation Involving Fractional p-Laplacian in ℝN. Fractal Fract. 2024, 8, 310. https://doi.org/10.3390/fractalfract8060310

AMA Style

Zhang X, Liang S. Multiple Normalized Solutions to a Choquard Equation Involving Fractional p-Laplacian in ℝN. Fractal and Fractional. 2024; 8(6):310. https://doi.org/10.3390/fractalfract8060310

Chicago/Turabian Style

Zhang, Xin, and Sihua Liang. 2024. "Multiple Normalized Solutions to a Choquard Equation Involving Fractional p-Laplacian in ℝN" Fractal and Fractional 8, no. 6: 310. https://doi.org/10.3390/fractalfract8060310

APA Style

Zhang, X., & Liang, S. (2024). Multiple Normalized Solutions to a Choquard Equation Involving Fractional p-Laplacian in ℝN. Fractal and Fractional, 8(6), 310. https://doi.org/10.3390/fractalfract8060310

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