1 Introduction

For any number aR and each interval I of R, we denote N a ={a,a+1,a+2,} and I N a =I N a throughout this paper. It is also worth noting that, in what follows, we appeal to the convention that s = k k 1 u(s)=0 for any k N a , where u is a function defined on N a .

In this paper, we will consider the following discrete fractional boundary value problem with a p-Laplacian operator:

{ Δ C β [ ϕ p ( Δ C α u ) ] ( t ) = f ( t + α + β 1 , u ( t + α + β 1 ) ) , t [ 0 , b ] N 0 , Δ C α u ( t ) | t = β 1 + Δ C α u ( t ) | t = β + b = 0 , u ( α + β 2 ) + u ( α + β + b ) = 0 ,
(1.1)

where 0<α, β1, 1<α+β2, b N 1 , Δ C β and Δ C α denote the Caputo fractional differences of order α and β respectively, f: [ α + β 1 , b + α + β 1 ] N α + β 1 ×RR is a continuous function and ϕ p is the p-Laplacian operator, that is, ϕ p (u)= | u | p 2 u, p>1. Obviously, ϕ p is invertible and its inverse operator is ϕ q , where q>1 is a constant such that 1/p+1/q=1.

The continuous fractional calculus has received increasing attention within the last ten years or so, and the theory of fractional differential equations has been a new important mathematical branch due to its extensive applications in various fields of science, such as physics, mechanics, chemistry, engineering, etc. For more details, see [114] and references therein. Although the discrete fractional calculus has seen slower progress, within the recent several years, a lot of papers have appeared; see [1535]. For example, a recent paper by Atıcı and Eloe [19] explores a discrete fractional conjugate boundary value problem with the Riemann-Liouville fractional difference. To the best of our knowledge, this is a pioneering work on discussing boundary value problems in discrete fractional calculus. After that, Goodrich studied discrete fractional boundary value problems involving the Riemann-Liouville fractional difference intensively and obtained a series of excellent results; see [2025]. Particularly note that Abdeljawad introduced the conception of Caputo fractional difference and presented some useful properties of it in [28].

p-Laplacian boundary value problems for ordinary differential equations, finite difference equations and dynamic equations have been studied extensively, but there are few papers dealing with the fractional p-Laplacian boundary value problems, besides [3638], especially for discrete fractional p-Laplacian boundary value problems involving Caputo fractional differences.

Motivated by the aforementioned works, we will consider the existence of solutions to the discrete fractional boundary value problem (1.1) and establish the sufficient conditions for the existence of at least one solution to it by using Schaefer’s fixed point theorem.

The remainder of this paper is organized as follows. Section 2 preliminarily provides some necessary background material for the theory of discrete fractional calculus. In Section 3, the main existence result for problem (1.1) is established with the help of Schaefer’s fixed point theorem. Finally, in Section 4, a concrete example is provided to illustrate the possible application of the established analytical result.

2 Preliminaries

For convenience, we first present here some necessary basic definitions on discrete fractional calculus.

Definition 2.1 [15]

For any t and ν, the falling factorial function is defined as

t ν ̲ = Γ ( t + 1 ) Γ ( t + 1 ν )

provided that the right-hand side is well defined. We appeal to the convention that if t+1ν is a pole of the Gamma function and t+1 is not a pole, then t ν ̲ =0.

Definition 2.2 [17]

For any t and ν, the rising factorial function is defined as

t ν ¯ = Γ ( t + ν ) Γ ( t )

provided that the right-hand side is well defined. We employ the convention that if t is a pole of the Gamma function and t+ν is not a pole, then t ν ¯ =0.

Definition 2.3 [39]

The ν-th fractional sum of a function f: N a R, for ν>0, is defined by

Δ ν f(t)= 1 Γ ( ν ) s = a t ν ( t s 1 ) ν 1 ̲ f(s),t N a + ν .

Definition 2.4 [28]

The ν-order Caputo fractional difference of a function f: N a R, for ν>0, νN, is defined by

where n is the smallest integer greater than or equal to ν and Δ n is the n-th order forward difference operator. If ν=nN, then .

Next, we present here several lemmas which will be important in the sequel.

Lemma 2.1 [28]

Assume that ν>0 and f is defined on N a . Then

where n is the smallest integer greater than or equal to ν.

Lemma 2.2 Let n be a positive integer. Then

( t a ) n ̲ = k = 0 n ( n k ) ( 1 ) k a k ¯ t n k ̲ ,t N a .
(2.1)

Proof The proof is by induction. For n=1, (2.1) is the same as

( t a ) 1 ̲ =ta.

Assume that (2.1) is true for n=m, that is

( t a ) m ̲ = k = 0 m ( m k ) ( 1 ) k a k ¯ t m k ̲ ,t N a

holds. So, for n=m+1,

Therefore, (2.1) also holds for n=m+1, which implies that (2.1) holds for any positive integer. □

In view of Lemma 2.1 and Lemma 2.2, the following fact is obvious.

Lemma 2.3 Assume that ν>0 and f is defined on N a . Then

where c i R, i=1,2,,n1, and n is the smallest integer greater than or equal to ν.

Finally, we need the following additional lemma that will be used in Section 3 of this paper.

Lemma 2.4 [21]

Let νR and t,sR such that ( t s ) ν ̲ is well defined. Then

Δ s ( t s ) ν ̲ =ν ( t s 1 ) ν 1 ̲ .

3 Existence result

In this section, we will establish the existence of at least one solution for problem (1.1). To accomplish this, we first state and prove the following result which is of particular importance in what follows.

Lemma 3.1 Let h: [ α + β 1 , α + β 1 + b ] N α + β 1 R be given. The unique solution of

{ Δ C β [ ϕ p ( Δ C α u ) ] ( t ) = h ( t + α + β 1 ) , t [ 0 , b ] N 0 , Δ C α u ( t ) | t = β 1 + Δ C α u ( t ) | t = β + b = 0 , u ( α + β 2 ) + u ( α + β + b ) = 0 ,
(3.1)

is

u ( t ) = 1 Γ ( α ) s = β 1 t α ( t s 1 ) α 1 ̲ ϕ q ( 1 Γ ( β ) τ = 0 s β ( s τ 1 ) β 1 ̲ h ( τ + α + β 1 ) 1 2 Γ ( β ) τ = 0 b ( β + b τ 1 ) β 1 ̲ h ( τ + α + β 1 ) ) 1 2 Γ ( α ) s = β 1 β + b ( α + β + b s 1 ) α 1 ̲ ϕ q ( 1 Γ ( β ) τ = 0 s β ( s τ 1 ) β 1 ̲ h ( τ + α + β 1 ) 1 2 Γ ( β ) τ = 0 b ( β + b τ 1 ) β 1 ̲ h ( τ + α + β 1 ) ) , t [ α + β 2 , α + β + b ] N α + β 2 .

Proof Suppose that u(t) satisfies the equation of problem (3.1), then Lemma 2.3 implies that

ϕ p ( Δ C α u ( t ) ) = 1 Γ ( β ) s = 0 t β ( t s 1 ) β 1 ̲ h(s+α+β1)+ c 0 ,

for some c 0 R, t [ β 1 , β + b ] N β 1 .

From the boundary condition Δ C α u(t) | t = β 1 + Δ C α u(t) | t = β + b =0, one has

c 0 = 1 2 Γ ( β ) s = 0 b ( β + b s 1 ) β 1 ̲ h(s+α+β1).

Therefore, we have

u ( t ) = 1 Γ ( α ) s = β 1 t α ( t s 1 ) α 1 ̲ ϕ q ( 1 Γ ( β ) τ = 0 s β ( s τ 1 ) β 1 ̲ h ( τ + α + β 1 ) 1 2 Γ ( β ) τ = 0 b ( β + b τ 1 ) β 1 ̲ h ( τ + α + β 1 ) ) + c 1 ,
(3.2)

where c 1 R, t [ α + β 2 , α + β + b ] N α + β 2 .

On the other hand, by condition u(α+β2)+u(α+β+b)=0, we get

c 1 = 1 2 Γ ( α ) s = β 1 β + b ( α + β + b s 1 ) α 1 ̲ ϕ q ( 1 Γ ( β ) τ = 0 s β ( s τ 1 ) β 1 ̲ h ( τ + α + β 1 ) 1 2 Γ ( β ) τ = 0 b ( β + b τ 1 ) β 1 ̲ h ( τ + α + β 1 ) ) .

Now, substitution of c 1 into (3.2) gives

u ( t ) = 1 Γ ( α ) s = β 1 t α ( t s 1 ) α 1 ̲ ϕ q ( 1 Γ ( β ) τ = 0 s β ( s τ 1 ) β 1 ̲ h ( τ + α + β 1 ) 1 2 Γ ( β ) τ = 0 b ( β + b τ 1 ) β 1 ̲ h ( τ + α + β 1 ) ) 1 2 Γ ( α ) s = β 1 β + b ( α + β + b s 1 ) α 1 ̲ ϕ q ( 1 Γ ( β ) τ = 0 s β ( s τ 1 ) β 1 ̲ h ( τ + α + β 1 ) 1 2 Γ ( β ) τ = 0 b ( β + b τ 1 ) β 1 ̲ h ( τ + α + β 1 ) ) , t [ α + β 2 , α + β + b ] N α + β 2 .

The proof is complete. □

To prove the main result, we need Schaefer’s fixed point theorem.

Lemma 3.2 [40]

Let E be a normed linear space (possibly incomplete) and Φ:EE be a compact operator. Suppose that the set

S= { x E | x = λ Φ x , for some λ ( 0 , 1 ) }

is bounded. Then Φ has a fixed point in E.

In order to use Schaefer’s fixed point theorem to solve the problem (1.1), we first define the following operator:

F:C [ α + β 2 , α + β + b ] N α + β 2 C [ α + β 2 , α + β + b ] N α + β 2

by

F u ( t ) = 1 Γ ( α ) s = β 1 t α ( t s 1 ) α 1 ̲ ϕ q ( 1 Γ ( β ) τ = 0 s β ( s τ 1 ) β 1 ̲ N u ( τ + α + β 1 ) 1 2 Γ ( β ) τ = 0 b ( β + b τ 1 ) β 1 ̲ N u ( τ + α + β 1 ) ) 1 2 Γ ( α ) s = β 1 β + b ( α + β + b s 1 ) α 1 ̲ × ϕ q ( 1 Γ ( β ) τ = 0 s β ( s τ 1 ) β 1 ̲ N u ( τ + α + β 1 ) 1 2 Γ ( β ) τ = 0 b ( β + b τ 1 ) β 1 ̲ N u ( τ + α + β 1 ) ) ,

where C [ α + β 2 , α + β + b ] N α + β 2 denotes the Banach space of all functions u: [ α + β 2 , α + β + b ] N α + β 2 R with the norm u=max{|u(t)|:t [ α + β 2 , α + β + b ] N α + β 2 } and the operator

N:C [ α + β 2 , α + β + b ] N α + β 2 C [ α + β 2 , α + β + b ] N α + β 2

is defined by

Nu(t)=f ( t , u ( t ) ) ,t [ α + β 2 , α + β + b ] N α + β 2 .

It is easy to verify that the operator F is well defined, and the fixed points of the operator F are solutions of problem (1.1).

Now, the main result is stated as follows.

Theorem 3.1 Assume that there exist nonnegative functions a,gC [ α + β 2 , α + β + b ] N α + β 2 such that

| f ( t , u ) | a(t)+g(t) | u | p 1 ,t [ α + β 2 , α + β + b ] N α + β 2 ,uR.
(3.3)

Then the problem (1.1) has at least one solution, provided that

( 3 / 2 ) q g q 1 ( i = 1 b ( 1 + β i ) q 1 ) ( i = 1 b + 1 ( 1 + α i ) ) <1.
(3.4)

Proof The proof will be divided into the following two steps.

Step 1: F:C [ α + β 2 , α + β + b ] N α + β 2 C [ α + β 2 , α + β + b ] N α + β 2 is completely continuous.

At first, in view of the continuity of f, it is easy to verify that F is continuous. Furthermore, it is not difficult to verify that F maps bounded sets into bounded sets and equi-continuous sets. Therefore, in the light of the well-known Arzelá-Ascoli theorem, we know that F is a compact operator.

Step 2: F a priori bounds.

Set

S= { u C [ α + β 2 , α + β + b ] N α + β 2 | u = λ F u , λ ( 0 , 1 ) } .

Now, it remains to show that the set S is bounded.

For any uS, there exists a λ(0,1) such that u(t)=λFu(t). So, by (3.3), Lemma 2.4 and the monotonicity of s ι ̲ , ι(0,1], we can obtain that

| u ( t ) | = λ | F u ( t ) | 1 Γ ( α ) s = β 1 t α ( t s 1 ) α 1 ̲ ϕ q ( 1 Γ ( β ) τ = 0 s β ( s τ 1 ) β 1 ̲ | N u ( τ + α + β 1 ) | + 1 2 Γ ( β ) τ = 0 b ( β + b τ 1 ) β 1 ̲ | N u ( τ + α + β 1 ) | ) + 1 2 Γ ( α ) s = β 1 β + b ( α + β + b s 1 ) α 1 ̲ × ϕ q ( 1 Γ ( β ) τ = 0 s β ( s τ 1 ) β 1 ̲ | N u ( τ + α + β 1 ) | + 1 2 Γ ( β ) τ = 0 b ( β + b τ 1 ) β 1 ̲ | N u ( τ + α + β 1 ) | ) , 1 Γ ( α ) s = β 1 t α ( t s 1 ) α 1 ̲ ϕ q ( a + g u p 1 Γ ( β ) τ = 0 s β ( s τ 1 ) β 1 ̲ + a + g u p 1 2 Γ ( β ) τ = 0 b ( β + b τ 1 ) β 1 ̲ ) + 1 2 Γ ( α ) s = β 1 β + b ( α + β + b s 1 ) α 1 ̲ ϕ q ( a + g u p 1 Γ ( β ) τ = 0 s β ( s τ 1 ) β 1 ̲ + a + g u p 1 2 Γ ( β ) τ = 0 b ( β + b τ 1 ) β 1 ̲ ) = 1 Γ ( α ) s = β 1 t α ( t s 1 ) α 1 ̲ × ϕ q ( ( a + g u p 1 ) s β ̲ Γ ( β + 1 ) + ( a + g u p 1 ) ( β + b ) β ̲ 2 Γ ( β + 1 ) ) + 1 2 Γ ( α ) s = β 1 β + b ( α + β + b s 1 ) α 1 ̲ ϕ q ( ( a + g u p 1 ) s β ̲ Γ ( β + 1 ) + ( a + g u p 1 ) ( β + b ) β ̲ 2 Γ ( β + 1 ) ) ϕ q ( 3 ( β + b ) β ̲ ( a + g u p 1 ) 2 Γ ( β + 1 ) ) { 1 Γ ( α ) s = β 1 t α ( t s 1 ) α 1 ̲ + 1 2 Γ ( α ) s = β 1 β + b ( α + β + b s 1 ) α 1 ̲ } 3 q 1 ( ( β + b ) β ̲ ) q 1 ( a + g u p 1 ) q 1 2 q 1 ( Γ ( β + 1 ) ) q 1 3 ( α + b + 1 ) α ̲ 2 Γ ( α + 1 ) ( 3 2 ) q ( ( β + b ) β ̲ Γ ( β + 1 ) ) q 1 ( α + β + 1 ) α ̲ Γ ( α + 1 ) ( a + g u p 1 ) q 1 = ( 3 2 ) q ( Γ ( β + b + 1 ) Γ ( β + 1 ) Γ ( b + 1 ) ) q 1 Γ ( α + b + 2 ) Γ ( α + 1 ) Γ ( b + 2 ) ( a + g u p 1 ) q 1 = ( 3 2 ) q ( i = 1 b ( 1 + β i ) q 1 ) ( i = 1 b + 1 ( 1 + α i ) ) ( a + g u p 1 ) q 1 .
(3.5)

Here we will consider the following two cases: (1) g=0 or (2) g0.

Case 1: Suppose that g=0. Then it is evident that the set S is bounded from (3.5).

Case 2: Suppose that g0. It also follows from (3.5) that

u p 1 { ( 3 2 ) q g q 1 ( i = 1 b ( 1 + β i ) q 1 ) ( i = 1 b + 1 ( 1 + α i ) ) } p 1 ( a g + u p 1 ) .
(3.6)

By virtue of (3.4) and (3.6), it is obvious that there exists a constant M>0 such that

uM.

Consequently, in both Case 1 and Case 2, we have proved that the set S is bounded.

Then, we can see that F satisfies all conditions of Schaefer’s fixed point theorem. Thus, we approach a conclusion that F has at least one fixed point which is the solution of problem (1.1). The proof is complete. □

4 An illustrative example

In this section, we will illustrate the possible application of the above established analytical result with a concrete example.

Example 4.1 Consider the following discrete fractional boundary value problem:

{ Δ C 1 / 2 [ ϕ 3 ( Δ C 2 / 3 u ) ] ( t ) = 1 100 u 2 ( t + 1 / 6 ) + sin ( t + 1 / 6 ) , t [ 0 , 2 ] N 0 , Δ C 2 / 3 u ( t ) | t = 1 / 2 + Δ C 2 / 3 u ( t ) | t = 5 / 2 = 0 , u ( 5 / 6 ) + u ( 19 / 6 ) = 0 .
(4.1)

Corresponding to problem (1.1), we have p=3, q= 3 2 , α= 2 3 , β= 1 2 and

f(t,u)= 1 100 u 2 +sint,t [ 1 / 6 , 13 / 6 ] N 1 / 6 ,uR.

Choose a(t)=1, g(t)= 1 100 . By a simple calculation, we can obtain

( 3 2 ) 3 2 ( 1 100 ) 1 2 ( i = 1 2 ( 1 + 1 2 i ) 1 2 ) ( i = 1 3 ( 1 + 2 3 i ) ) 0.6832<1.

Obviously, problem (4.1) satisfies all assumptions of Theorem 3.1. Hence, we can conclude that problem (4.1) has at least one solution.