1 Introduction

Fractional differential calculus is a discipline to which many researchers are dedicating their time, perhaps because of its demonstrated applications in various fields of science and engineering [1]. Many researchers studied the existence of solutions to fractional boundary value problems, for example, [210].

The q-difference calculus or quantum calculus is an old subject that was initially developed by Jackson [11, 12]; basic definitions and properties of q-difference calculus can be found in [13, 14].

The fractional q-difference calculus had its origin in the works by Al-Salam [15] and Agarwal [16]. More recently, maybe due to the explosion in research within the fractional differential calculus setting, new developments in this theory of fractional q-difference calculus were made, for example, q-analogues of the integral and differential fractional operators properties such as Mittage-Leffler function [17], just to mention some.

El-Shahed and Hassan [18] studied the existence of positive solutions of the q-difference boundary value problem:

{ D q 2 u ( t ) = a ( t ) f ( u ( t ) ) , t J : = [ 0 , 1 ] , α u ( 0 ) β D q u ( 0 ) = 0 , γ u ( 1 ) + δ D q u ( 1 ) = 0 .

Ferreira [19] considered the existence of positive solutions to nonlinear q-difference boundary value problem:

{ ( RL D q α u ) ( t ) = f ( t , u ( t ) ) , 0 < t < 1 , 1 < α 2 , u ( 0 ) = u ( 1 ) = 0 .

Ferreira [20] studied the existence of positive solutions to nonlinear q-difference boundary value problem:

{ ( RL D q α u ) ( t ) = f ( t , u ( t ) ) , 0 < t < 1 , 2 < α 3 , u ( 0 ) = ( D q u ) ( 0 ) = 0 , ( D q u ) ( 1 ) = β 0 .

El-Shahed and Al-Askar [21] studied the existence of positive solutions to nonlinear q-difference equation:

{ D q α C u + a ( t ) f ( u ( t ) ) = 0 , 0 < t < 1 , 2 < α 3 , u ( 0 ) = ( D q 2 u ) ( 0 ) = 0 , γ ( D q u ) ( 1 ) + β D q 2 u ( 1 ) = 0 ,

where γ,β0 and D q C is the fractional q-derivative of the Caputo type.

Ahmad, Alsaedi and Ntouyas [22] discussed the existence of solutions for the second-order q-difference equation with nonseparated boundary conditions

{ D q 2 u ( t ) = f ( t , u ( t ) ) , t I , u ( 0 ) = η u ( T ) , D q u ( 0 ) = η D q u ( T ) ,

where fC(I×R,R), I=[0,T] q N ¯ , q N ¯ :={ q n :nN}{0}, and T q N ¯ is a fixed constant, and η1 is a fixed real number.

Ahmad and Nieto [23] discussed a nonlocal nonlinear boundary value problem (BVP) of third-order q-difference equations given by

{ D q 3 u ( t ) = f ( t , u ( t ) ) , t I q , u ( 0 ) = 0 , D q u ( 0 ) = 0 , u ( 1 ) = α u ( η ) ,

where fC( I q ×R,R), I q ={0,1}{ q n :nN}, and q(0,1) is a fixed constant, η{ q n :nN} and α1/ η 2 is a real number.

This paper is mainly concerned with the existence results for the following fractional q-difference equations:

{ D q α C u + f ( t , u ) = 0 , t J = [ 0 , 1 ] , 2 < α 3 , u ( 0 ) = ( D q 2 u ) ( 0 ) = 0 , γ ( D q u ) ( 1 ) + β D q 2 u ( 1 ) = 0 ,
(1.1)

where γ,β0 and D q C is the fractional q-derivative of the Caputo type. f:J×EE is a given function satisfying some assumptions that will be specified later, and E is a Banach space with norm u.

To investigate the existence of solutions of the problem above, we use Mönch’s fixed-point theorem combined with the technique of measures of weak noncompactness, which is an important method for seeking solutions of differential equations. This technique was mainly initiated in the monograph of Banaś and Goebel [24], and subsequently developed and used in many papers; see, for example, Banaś et al. [25], Guo et al. [26], Krzyska and Kubiaczyk [27], Lakshmikantham and Leela [28], Mönch [29], O’Regan [30, 31], Szufla [32, 33] and the references therein. As far as we know, there are very few results devoted to weak solutions of nonlinear fractional differential equations [3438]. Motivated by the above mentioned papers, the purpose of this paper is to establish the existence results for the boundary value problem (1.1) by virtue of the Mönch’s fixed-point theorem combined with the technique of measures of weak noncompactness.

The remainder of this article is organized as follows. In Section 2, we provide some basic definitions, preliminaries facts and various lemmas, which are needed later. In Section 3, we give main results of the problem (1.1). In the end, we also give an example for the illustration of the theories established in this paper.

2 Preliminaries and lemmas

In this section, we present some basic notations, definitions and preliminary results, which will be used throughout this paper.

Let q(0,1) and define [13]

[ a ] q = q a 1 q 1 = a a 1 ++1,aR.

The q-analogue of the power ( a b ) n is

( a b ) ( 0 ) =1, ( a b ) ( n ) = k = 0 n 1 ( a b q k ) ,a,bR,nN.

If α is not a positive integer, then

( a b ) ( α ) = a α i = 0 ( 1 ( b / a ) q i ) ( 1 ( b / a ) q α + i ) .

Note that if b=0, then a ( α ) = a α . The q-gamma function is defined by

Γ q (x)= ( 1 q ) ( x 1 ) ( 1 q ) x 1 ,xR{0,1,2,},0<q<1,

and satisfies Γ q (x+1)= [ x ] q Γ q (x).

The q-derivative of a function f is here defined by

D q f(x)= d q f ( x ) d q x = f ( q x ) f ( x ) ( q 1 ) x

and q-derivatives of higher order by

D q n f(x)={ f ( x ) , if  n = 0 , D q D q n 1 f ( x ) , if  n N .

The q-integral of a function f defined in the interval [0,b] is given by

0 x f(t) d q t=x(1q) n = 0 f ( x q n ) q n ,0|q|<1,x[0,b].

If a[0,b] and f is defined in the interval [0,b], its integral from a to b is defined by

a b f(t) d q t= 0 b f(t) d q t 0 a f(t) d q t.

Similarly, as done for derivatives, an operator I q n can be defined, namely,

( I q 0 f ) (x)=f(x), ( I q n f ) (x)= I q ( I q n 1 f ) (x),nN.

The fundamental theorem of calculus applies to these operators I q and D q , that is,

( D q I q f)(x)=f(x),

and if f is continuous at x=0, then

( I q D q f)(x)=f(x)f(0).

Basic properties of the two operators can be found in the book mentioned in [13]. We now point out three formulas that will be used later ( D q i denotes the derivative with respect to variable i) [19]

[ a ( t s ) ] ( α ) = a α ( t s ) ( α ) , D q t ( t s ) ( α ) = [ α ] q ( t s ) ( α 1 ) , ( x D q 0 x f ( x , t ) d q t ) ( x ) = 0 x x D q f ( x , t ) d q t + f ( q x , x ) .

Remark 2.1 We note that if α>0 and abt, then ( t a ) ( α ) ( t b ) ( α ) [19].

Let J:=[0,1] and L 1 (J,E) denote the Banach space of real-valued Lebesgue integrable functions on the interval J, L (J,E) denote the Banach space of real-valued essentially bounded and measurable functions defined over J with the norm L .

Let E be a real reflexive Banach space with norm and dual E , and let (E,ω)=(E,σ(E, E )) denote the space E with its weak topology. Here, C(J,E) is the Banach space of continuous functions x:JE with the usual supremum norm x :=sup{x(t):tJ}.

Moreover, for a given set V of functions v:JR, let us denote by V(t)={v(t):vV},tJ, and V(J)={v(t):vV,tJ}.

Definition 2.1 A function h:EE is said to be weakly sequentially continuous if h takes each weakly convergent sequence in E to a weakly convergent sequence in E (i.e. for any ( x n ) n in E with x n (t)x(t) in (E,ω) then h( x n (t))h(x(t)) in (E,ω) for each tJ).

Definition 2.2 [39]

The function x:JE is said to be Pettis integrable on J if and only if there is an element x J E corresponding to each IJ such that φ( x I )= I φ(x(s))ds for all φ E , where the integral on the right is supposed to exist in the sense of Lebesgue. By definition, x I = I x(s)ds.

Let P(J,E) be the space of all E-valued Pettis integrable functions in the interval J.

Lemma 2.1 [39]

If x() is Pettis integrable and h() is a measurable and an essentially bounded real-valued function, then x()h() is Pettis integrable.

Definition 2.3 [40]

Let E be a Banach space, Ω E the set of all bounded subsets of E, and B 1 the unit ball in E. The De Blasi measure of weak noncompactness is the map β: Ω E [0,) defined by

β ( X ) = inf { ϵ > 0 :  there exists a weakly compact subset  Ω  of  E such that  X ϵ B 1 + Ω } .

Lemma 2.2 [40]

The De Blasi measure of noncompactness satisfies the following properties:

  1. (a)

    STβ(S)β(T);

  2. (b)

    β(S)=0S is relatively weakly compact;

  3. (c)

    β(ST)=max{β(S),β(T)};

  4. (d)

    β( S ¯ ω )=β(S), where S ¯ ω denotes the weak closure of S;

  5. (e)

    β(S+T)β(S)+β(T);

  6. (f)

    β(aS)=|a|α(S);

  7. (g)

    β(conv(S))=β(S);

  8. (h)

    β( | λ | h λS)=hβ(S).

The following result follows directly from the Hahn-Banach theorem.

Lemma 2.3 Let E be a normed space with x 0 0. Then there exists φ E with φ=1 and φ( x 0 )= x 0 .

Definition 2.4 [16]

Let α0 and f be a function defined on [0,1]. The fractional q-integral of the Riemann-Liouville type is ( RL I q 0 f)(x)=f(x) and

( RL I q α f)(x)= a x ( x q t ) ( α 1 ) Γ q ( α ) f(t) d q t,α R + ,x[0,1].

Definition 2.5 [14]

The fractional q-derivative of the Riemann-Liouville type of order α0 is defined by ( RL D q 0 f)(x)=f(x) and

( RL D q α f)(x)= ( D q [ α ] I q [ α ] α f ) (x),α>0,

where [α] is the smallest integer greater than or equal to α.

Definition 2.6 [14]

The fractional q-derivative of the Caputo type of order α0 is defined by

( C D q α f)(x)= ( I q [ α ] α D q [ α ] f ) (x),α>0,

where [α] is the smallest integer greater than or equal to α.

Lemma 2.4 [14]

Let α,β0 and let f be a function defined on [0,1]. Then the next formulas hold:

  1. (1)

    ( I q β I q α f)(x)=( I q α + β f)(x),

  2. (2)

    ( D q β I q α f)(x)=f(x).

Lemma 2.5 [32]

Let D be a closed convex and equicontinuous subset of a metrizable locally convex vector space C(J,E) such that 0D. Assume that A:DD is weakly sequentially continuous. If the implication

V ¯ = conv ¯ ( { 0 } A ( V ) ) V is relatively weakly compact ,
(2.1)

holds for every subset V of D, then A has a fixed point.

3 Main results

Let us start by defining what we mean by a solution of the problem (1.1).

Definition 3.1 A function uC(J, E ω ) is said to be a solution of the problem (1.1) if u satisfies the equation D q α C u+f(t,u)=0 on J, and satisfy the conditions u(0)=( D q 2 u)(0)=0, γ( D q u)(1)+β D q 2 u(1)=0.

For the existence results on the problem (1.1), we need the following auxiliary lemmas.

Lemma 3.1 [19]

Let α>0 and nN. Then, the following equality holds:

( RL I q α RL D q n f)(x) = RL D q n RL I q α f(x) k = 0 α 1 x α n + k Γ q ( α + k n + 1 ) ( D q k f ) (0).

Lemma 3.2 [14]

Let α>0 and n R + N. Then the following equality holds:

( I q α C D q α f ) (x)=f(x) k = 0 [ α ] 1 x k Γ q ( k + 1 ) ( D q k f ) (0).

We derive the corresponding Green’s function for boundary value problem (1.1), which will play major role in our next analysis.

Lemma 3.3 Let ρC[0,1] be a given function, then the boundary-value problem

{ D q α C u + ρ ( t ) = 0 , t [ 0 , 1 ] , 2 < α 3 , u ( 0 ) = ( D q 2 u ) ( 0 ) = 0 , γ ( D q u ) ( 1 ) + β D q 2 u ( 1 ) = 0
(3.1)

has a unique solution

u(t)= 0 1 G(t,qs)ρ(s) d q s,
(3.2)

where G(t,s) is defined by the formula

G(t,s)={ t ( 1 s ) ( α 2 ) Γ q ( α 1 ) + β γ t ( 1 s ) ( α 3 ) Γ q ( α 2 ) , if 0 t s 1 , t ( 1 s ) ( α 2 ) Γ q ( α 1 ) + β γ t ( 1 s ) ( α 3 ) Γ q ( α 2 ) ( t s ) ( α 1 ) Γ q ( α ) , if 0 s t 1 .
(3.3)

Here, G(t,s) is called the Green’s function of boundary value problem (3.1).

Proof By Lemma 2.4 and Lemma 3.2, we can reduce the equation of problem (3.1) to an equivalent integral equation

u(t)=u(0)+ D q u ( 0 ) Γ q ( 2 ) t+ D q 2 u ( 0 ) Γ q ( 3 ) t 2 I q α ρ(t).
(3.4)

Applying the boundary conditions u(0)=( D q 2 u)(0)=0, we have

u(t)=At 0 t ( t q s ) ( α 1 ) Γ q ( α ) ρ(s) d q s.
(3.5)

So, we have

( D q u)(t)=A 0 t [ α 1 ] q ( t q s ) ( α 2 ) Γ q ( α ) ρ(s) d q s,
(3.6)
( D q 2 u ) (t)= 0 t [ α 1 ] q [ α 2 ] q ( t q s ) ( α 3 ) Γ q ( α ) ρ(s) d q s.
(3.7)

Then, by the condition γ( D q u)(1)+β D q 2 u(1)=0, we have

A= 0 1 ( 1 q s ) ( α 2 ) Γ q ( α 1 ) ρ(s) d q s+ β γ 0 1 ( 1 q s ) ( α 3 ) Γ q ( α 2 ) ρ(s) d q s.
(3.8)

Therefore, the unique solution of problem (3.1) is

u ( t ) = A t 0 t ( t q s ) ( α 1 ) Γ q ( α ) ρ ( s ) d q s = [ 0 1 ( 1 q s ) ( α 2 ) Γ q ( α 1 ) ρ ( s ) d q s + β γ 0 1 ( 1 q s ) ( α 3 ) Γ q ( α 2 ) ρ ( s ) d q s ] t 0 t ( t q s ) ( α 1 ) Γ q ( α ) ρ ( s ) d q s = 0 1 G ( t , q s ) ρ ( s ) d q s ,

which completes the proof. □

Remark 3.1 From the expression of G(t,s), it is obvious that G(t,s) is continuous on J×J. Denote by

G =sup { 0 T | G ( t , s ) | d q s : t J } .

To prove the main results, we need the following assumptions:

(H1) For each tJ, the function f(t,) is weakly sequentially continuous;

(H2) For each xC(J,E), the function f(,x()) is Pettis integrable on J;

(H3) There exists p f L (J, R + ) such that

f ( t , u ) p f (t)ufor a.e. tJ and each uE;

(H3)′ There exists p f L (J, R + ) and a continuous nondecreasing function ψ:[0,)(0,) such that

f ( t , u ) p f (t)ψ ( u ) for a.e. tJ and each uE;

(H4) For each bounded set DE, and each tJ, the following inequality holds:

β ( f ( t , D ) ) p f (t)β(D);

(H5) There exists a constant R>0 such that

R p f L ψ ( R ) G >1,

where p f L =sup{ p f (t):tJ}.

Theorem 3.1 Let E be a reflexive Banach space and assume that (H1)-(H3) are satisfied. If

p f L G <1,
(3.9)

then the problem (1.1) has at least one solution on J.

Proof Let the operator A:C(J,E)C(J,E) defined by the formula

(Au)(t):= 0 1 G(t,qs)f ( s , u ( s ) ) d q s,
(3.10)

where G(,) is the Green’s function defined by (3.3). It is well known the fixed points of the operator A are solutions of the problem (1.1).

First notice that, for xC(J,E), we have f(,x())P(J,E) (assumption (H2)). Since, sG(t,s) L (J), then G(t,)f(,x()) is Pettis integrable for all tJ by Lemma 2.1, and so the operator A is well defined.

Let R>0, and consider the set

D = { x C ( J , E ) : x R  and x ( t 1 ) x ( t 2 ) R p f L 0 1 | G ( t 2 , q s ) G ( t 1 , q s ) | d q s  for  t 1 , t 2 J } .

Clearly, the subset D is closed, convex and equicontinuous. We shall show that A satisfies the assumptions of Lemma 2.5. The proof will be given in three steps.

Step 1: We will show that the operator A maps D into itself.

Take xD, tJ and assume that Ax(t)0. Then there exists ψ E such that Ax(t)=ψ(Ax(t)). Thus,

( A x ) ( t ) = ψ ( ( A x ) ( t ) ) = 0 1 G ( t , q s ) f ( s , y ( s ) ) d q s 0 1 | G ( t , q s ) | ψ ( f ( s , x ( s ) ) ) d q s 0 1 | G ( t , q s ) | p f ( s ) x ( s ) d q s p f L R G R .

Let τ 1 , τ 2 J, τ 1 < τ 2 and xD, so Ax( τ 2 )Ax( τ 1 )0. Then there exists ψ E , such that Ax( τ 2 )Ax( τ 1 )=ψ(Ax( τ 2 )Ax( τ 1 )). Hence,

A x ( τ 2 ) A x ( τ 1 ) = 0 1 [ G ( τ 2 , q s ) G ( τ 1 , q s ) ] f ( s , x ( s ) ) d q s 0 1 | G ( τ 2 , q s ) G ( τ 1 , q s ) | f ( s , x ( s ) ) d q s R p f L 0 1 | G ( τ 2 , q s ) G ( τ 1 , q s ) | d q s ,

this means that A(D)D.

Step 2: We will show that the operator A is weakly sequentially continuous.

Let ( x n ) be a sequence in D and let ( x n (t))x(t) in (E,w) for each tJ. Fix tJ. Since f satisfies assumptions (H1), we have f(t, x n (t)) converge weakly uniformly to f(t,x(t)). Hence, the Lebesgue dominated convergence theorem for Pettis integrals implies A x n (t) converges weakly uniformly to Ax(t) in E ω . Repeating this for each tJ shows A x n Ax. Then A:DD is weakly sequentially continuous.

Step 3: The implication (2.1) holds. Now let V be a subset of D such that V conv ¯ (A(V){0}). Clearly, V(t) conv ¯ (A(V){0}) for all tJ. Hence, AV(t)AD(t), tJ, is bounded in E. Thus, AV(t) is weakly relatively compact since a subset of a reflexive Banach space is weakly relatively compact if and only if it is bounded in the norm topology. Therefore,

v ( t ) β ( A ( V ) ( t ) { 0 } ) β ( A ( V ) ( t ) ) = 0 ,

thus, V is relatively weakly compact in E. In view of Lemma 2.5, we deduce that A has a fixed point, which is obviously a solution of the problem (1.1). This completes the proof. □

Remark 3.2 In Theorem 3.1, we presented an existence result for weak solutions of the problem (1.1) in the case where the Banach space E is reflexive. However, in the nonreflexive case, conditions (H1)-(H3) are not sufficient for the application of Lemma 2.5; the difficulty is with condition (2.1).

Theorem 3.2 Let E be a Banach space, and assume assumptions (H1), (H2), (H3), (H4) are satisfied. If (3.9) holds, then the problem (1.1) has at least one solution on J.

Theorem 3.3 Let E be a Banach space, and assume assumptions (H1), (H2), (H3)′, (H4), (H5) are satisfied. If (3.9) holds, then the problem (1.1) has at least one solution on J.

Proof Assume that the operator A:C(J,E)C(J,E) is defined by the formula (3.10). It is well known the fixed points of the operator A are solutions of the problem (1.1).

First notice that, for xC(J,E), we have f(,x())P(J,E) (assumption (H2)). Since, sG(t,s) L (J), then G(t,)f(,x()) for all tJ is Pettis integrable (Lemma 2.1), and thus, the operator A makes sense.

Let R>0, and consider the set

D = { x C ( J , E ) : x R  and x ( t 1 ) x ( t 2 ) p f L ψ ( R ) 0 1 | G ( t 2 , q s ) G ( t 1 , q s ) | d q s  for  t 1 , t 2 J } ,
(3.11)

clearly, the subset D is closed, convex and equicontinuous. We shall show that A satisfies the assumptions of Lemma 2.5. The proof will be given in three steps.

Step 1: We will show that the operator A maps D into itself.

Take xD, tJ and assume that Ax(t)0. Then there exists ψ E such that Ax(t)=ψ(Ax(t)). Thus,

( A x ) ( t ) = ψ ( ( A x ) ( t ) ) = ψ ( 0 1 G ( t , q s ) f ( s , y ( s ) ) d q s ) 0 T | G ( t , q s ) | ψ ( f ( s , x ( s ) ) ) d q s 0 T | G ( t , q s ) | p f ( s ) ψ ( x ( s ) ) d q s p f L ψ ( R ) G R .

Let τ 1 , τ 2 J, τ 1 < τ 2 and xD, so Ax( τ 2 )Ax( τ 1 )0. Then there exist ψ E such that

A x ( τ 2 ) A x ( τ 1 ) =ψ ( A x ( τ 2 ) A x ( τ 1 ) ) .

Thus,

A x ( τ 2 ) A x ( τ 1 ) = ψ ( 0 1 [ G ( τ 2 , q s ) G ( τ 1 , q s ) ] f ( s , x ( s ) ) d q s ) 0 1 | G ( τ 2 , q s ) G ( τ 1 , q s ) | f ( s , x ( s ) ) d q s ψ ( R ) p f L 0 1 | G ( τ 2 , q s ) G ( τ 1 , q s ) | d q s ,

this means that A(D)D.

Step 2: We will show that the operator A is weakly sequentially continuous.

Let ( x n ) be a sequence in D and let ( x n (t))x(t) in (E,w) for each tJ. Fix tJ. Since f satisfies assumptions (H1), we have f(t, x n (t)), converging weakly uniformly to f(t,x(t)). Hence, the Lebesgue dominated convergence theorem for Pettis integral implies A x n (t) converging weakly uniformly to Ax(t) in E ω . We do it for each tJ so A x n Ax. Then A:DD is weakly sequentially continuous.

Step 3: The implication (2.1) holds. Now let V be a subset of D such that V conv ¯ (A(V){0}). Clearly, V(t) conv ¯ (A(V){0}) for all tJ. Hence, AV(t)AD(t), tJ, is bounded in E. Using this fact, assumption (H4), Lemma 2.2 and the properties of the measure β, we have for each tJ

v ( t ) β ( A ( V ) ( t ) { 0 } ) β ( A ( V ) ( t ) ) = β { 0 1 G ( t , q s ) f ( s , V ( s ) ) d q s } 0 1 | G ( t , q s ) | p f ( s ) β ( V ( s ) ) d q s p f L 0 1 | G ( t , q s ) | v ( s ) d q s p f L v G ,

which gives

v p f L v G .

This means that

v [ 1 p f L G ] 0.

By (3.9), it follows that v =0, that is v(t)=0 for each tJ, and then V(t) is relatively weakly compact in E. In view of Lemma 2.5, we deduce that A has a fixed point which is obviously a solution of the problem (1.1). This completes the proof. □