1 Introduction

Fractional calculus has recently evolved as an interesting and important field of research. The much interest in the subject owes to its extensive applications in the mathematical modeling of several phenomena in many engineering and scientific disciplines such as physics, chemistry, biophysics, biology, blood flow problems, control theory, aerodynamics, nonlinear oscillation of earthquake, the fluid-dynamic traffic model, polymer rheology, regular variation in thermodynamics, economics, fitting of experimental data, etc. [1, 2]. A significant feature of a fractional order differential operator, in contrast to its counterpart in classical calculus, is its nonlocal behavior. It means that the future state of a dynamical system or process based on the fractional differential operator depends on its current state as well its past states. It is equivalent to saying that differential equations of arbitrary order are capable of describing memory and hereditary properties of certain important materials and processes. This aspect of fractional calculus has contributed towards the growing popularity of the subject.

Nonlocal initial and boundary value problems of nonlinear fractional order differential equations have recently been investigated by several researchers. The domain of study ranges from the theoretical aspects (like existence, uniqueness, periodicity, asymptotic behavior, etc.) to the analytic and numerical methods for fractional differential equations. In fact the theory of differential equations of fractional order (parallel to the well-known theory of ordinary differential equations) has been growing independently for the last three decades. For some recent development of the subject, we refer, for instance, to a series of papers [314] and references cited therein.

In this paper, we discuss the existence of solutions for a boundary value problem of integro-differential equations of fractional order with nonlocal three-point fractional boundary conditions

{ D α x ( t ) = A f ( t , x ( t ) ) + B I β g ( t , x ( t ) ) , 2 < α 3 , t [ 0 , 1 ] , D δ x ( 0 ) = 0 , D δ + 1 x ( 0 ) = 0 , D δ x ( 1 ) D δ x ( η ) = a ,
(1)

where 0<δ1, αδ>3, 0<β<1, 0<η<1, D ( ) denotes the Riemann-Liouville fractional derivative of order (), f, g are given continuous functions, and A, B, a are real constants.

The objective of the present work is to establish the existence of solutions for the given problem by applying Sadovskii’s fixed point theorem for condensing maps. It is imperative to note that the application of Sadovskii’s fixed point theorem for condensing maps in the present scenario is new. Moreover, the right-hand side of the fractional differential equation in (1) provides a liberty to fix it in terms of non-integral and integral terms. Observe that the integral term in (1) is a Riemann-Liouville integral of order β(0,1), which reduces to the classical integral term ( 0 t g(s,x(s))ds) in the limit β 1 . The nature of the nonlinearity considered in the problem (1) becomes of non-integral type if we take B=0 in (1) and corresponds to integral type for A=0 in (1). Furthermore, the given boundary conditions are also interesting and important from a physical point of view [15, 16] as the condition D δ x(1) D δ x(η)=a is a fractional analogue of the classical flux condition x (1) x (η)=a (the difference of flux values at the right end point and at an intermediate point of the interval [0,1] remains constant).

2 Auxiliary results

We recall here the following definitions.

Definition 2.1 The Riemann-Liouville fractional integral of order q for a continuous function g is defined as

I q g(t)= 1 Γ ( q ) 0 t g ( s ) ( t s ) 1 q ds,q>0,

provided the integral exists.

Definition 2.2 The Riemann-Liouville derivative of fractional order q for a continuous function g:(0,)R is defined as

D 0 + q g(t)= 1 Γ ( n q ) ( d d t ) n 0 t ( t s ) n q 1 g(s)ds,n=[q]+1,

where [q] denotes the integer part of the real number q.

By the substitution x(t)= I δ y(t)= D δ y(t), where y(t) is a suitable continuous function, the problem (1) takes the form

{ D α δ y ( t ) = A f ( t , I δ y ( t ) ) + B I β g ( t , I δ y ( t ) ) , t [ 0 , 1 ] , y ( 0 ) = 0 , y ( 0 ) = 0 , y ( 1 ) y ( η ) = a .
(2)

Lemma 2.1 For any hC(0,1)L(0,1), the unique solution of the linear fractional boundary value problem

{ D α δ y ( t ) = h ( t ) , t [ 0 , 1 ] , y ( 0 ) = 0 , y ( 0 ) = 0 , y ( 1 ) y ( η ) = a ,
(3)

is

y(t)= I α δ h(t)+ t α δ 1 1 η α δ 1 ( a + I α δ h ( 1 ) I α δ h ( η ) ) .

Proof It is well known that the solutions of the fractional differential equation in (3) can be written as [2]

y(t)= I α δ h(t)+ c 1 t α δ 1 + c 2 t α δ 2 + c 3 t α δ 3 ,
(4)

where c 1 , c 2 , c 3 R are arbitrary constants. Using the given boundary conditions, we find that c 2 =0, c 3 =0 and

c 1 = 1 1 η α δ 1 ( a + I α δ h ( 1 ) I α δ h ( η ) ) .

Substituting these values in (4), we get

y(t)= I α δ h(t)+ t α δ 1 1 η α δ 1 ( a + I α δ h ( 1 ) I α δ h ( η ) ) .

This completes the proof. □

Thus, the solution of a linear variant of the problem (1) can be written as

x ( t ) = I δ y ( t ) = I δ [ I α δ h ( t ) + t α δ 1 1 η α δ 1 ( a + I α δ h ( 1 ) I α δ h ( η ) ) ] = I α h ( t ) + 1 1 η α δ 1 ( a + I α δ h ( 1 ) I α δ h ( η ) ) 0 t ( t s ) δ 1 Γ ( δ ) s α δ 1 d s = I α h ( t ) + 1 1 η α δ 1 ( a + I α δ h ( 1 ) I α δ h ( η ) ) { t α 1 Γ ( δ ) 0 1 ( 1 ν ) δ 1 ν α δ 1 d ν } ,

where we have used the substitution s=νt in the integral of the last term. Using the relation for beta function B(,),

B(β+1,α)= 0 1 ( 1 u ) α 1 u β du= Γ ( α ) Γ ( β + 1 ) Γ ( α + β + 1 ) ,

we get

x(t)= I α h(t)+ Γ ( α δ ) t α 1 ( 1 η α δ 1 ) Γ ( α ) ( a + I α δ h ( 1 ) I α δ h ( η ) ) .
(5)

The solution of the original nonlinear problem (1) can be obtained by replacing h with the right-hand side of the fractional equation of (1) in (5).

Let C=C([0,1],R) denote the Banach space of all continuous functions from [0,1]R endowed with the norm defined by x=sup{|x(t)|,t[0,1]}.

Definition 2.3 Let M be a bounded set in a metric space (X,d), then the Kuratowskii measure of noncompactness α(M) is defined as inf{ϵ:M covered by a finitely many sets suchthat the diameter of each setϵ}.

Definition 2.4 [17]

Let Φ:D(Φ)XX be a bounded and continuous operator on a Banach space X. Then Φ is called a condensing map if α(Φ(B))<α(B) for all bounded sets BD(Φ), where α denotes the Kuratowski measure of noncompactness.

Lemma 2.2 [[18], Example 11.7]

The map K+C is a k-set contraction with 0k<1, and thus also condensing, if

  1. (i)

    K,C:DXX are operators on the Banach space X;

  2. (ii)

    K is k-contractive, i.e.,

    KxKykxy

for all x,yD and fixed k[0,1);

  1. (iii)

    C is compact.

Theorem 2.1 [19]

Let B be a convex, bounded and closed subset of a Banach space X and let Φ:BB be a condensing map. Then Φ has a fixed point.

3 Main result

In the following we denote by L 1 / p ([0,1], R + ) the space of 1 p -Lebesgue measurable functions from [0,1] to R + with the norm μ= ( 0 1 | μ ( s ) | 1 p d s ) p .

Theorem 3.1 Let f,g:[0,1]×RR be continuous functions satisfying the following conditions:

( H 1 ) f satisfies the Lipschitz condition

| f ( t , x ) f ( t , y ) | L 1 (t)|xy| for all (t,x),(t,y)[0,1]×R,

where L 1 L 1 / p ([0,1], R + ), p=min{ q 1 , q 2 }, q 1 (0,1), q 2 (0,αδ);

( H 2 ) there exist a function m L 1 / p ([0,1], R + ) and a nondecreasing function ψ: R + R + such that

| g ( t , x ) | m(t)ψ ( x ) ,(t,x)[0,1]×R.

Then the boundary value problem (1) has at least one solution, provided

γ:= | A | L 1 Γ ( α ) ( 1 p α p ) 1 p + | A | | Q | L 1 Γ ( α δ ) ( 1 p α δ p ) 1 p ( 1 + η α δ p ) <1.

Proof Let B r ={xC:xr} be a closed bounded and convex subset of C:=C([0,1],R), where r will be fixed later. Using (5), we define a map Φ: B r C as

( Φ x ) ( t ) = A 0 t ( t s ) α 1 Γ ( α ) f ( s , x ( s ) ) d s B 0 t ( t s ) α + β 1 Γ ( α + β ) g ( s , x ( s ) ) d s + Q t α 1 [ a + A 0 1 ( 1 s ) α δ 1 Γ ( α δ ) f ( s , x ( s ) ) d s + B 0 1 ( 1 s ) α δ + β 1 Γ ( α δ + β ) g ( s , x ( s ) ) d s A 0 η ( η s ) α δ 1 Γ ( α δ ) f ( s , x ( s ) ) d s B 0 η ( η s ) α δ + β 1 Γ ( α δ + β ) g ( s , x ( s ) ) d s ] ,

where

Q= Γ ( α δ ) ( 1 η α δ 1 ) Γ ( α ) , η α δ 1 1.

Observe that the problem (1) is equivalent to a fixed point problem Φx=x.

Let us decompose Φ as Φ= Φ 1 + Φ 2 , where

( Φ 1 x ) ( t ) = A 0 t ( t s ) α 1 Γ ( α ) f ( s , x ( s ) ) d s + a Q t α 1 + A Q t α 1 [ 0 1 ( 1 s ) α δ 1 Γ ( α δ ) f ( s , x ( s ) ) d s 0 η ( η s ) α δ 1 Γ ( α δ ) f ( s , x ( s ) ) d s ] , t [ 0 , 1 ]

and

( Φ 2 x ) ( t ) = B 0 t ( t s ) α + β 1 Γ ( α + β ) g ( s , x ( s ) ) d s + B Q t α 1 [ 0 1 ( 1 s ) α δ + β 1 Γ ( α δ + β ) g ( s , x ( s ) ) d s 0 η ( η s ) α δ + β 1 Γ ( α δ + β ) g ( s , x ( s ) ) d s ] , t [ 0 , 1 ] .

Step 1. Φ( B r ) B r .

For that, we select r ω 1 γ , where

ω = | A | σ + | B | m 2 ψ ( r ) Γ ( α + β ) ( 1 p α + β p ) 1 p + | B | | Q | m 2 ψ ( r ) Γ ( α δ + β ) ( 1 p α δ + β p ) 1 p ( 1 + η α δ + β p ) , σ = | a | + M ( 1 Γ ( α + 1 ) + | Q | ( 1 + η α 1 ) Γ ( α δ + 1 ) ) , sup t [ 0 , 1 ] | f ( t , 0 ) | = M < .

Using |f(t,x(t))||f(t,x(t))f(t,0)|+|f(t,0)| L 1 (t)r+M for x B r , t[0,1], we get

| ( Φ 1 x ) ( t ) | | A | r [ 0 t ( t s ) α 1 Γ ( α ) L 1 ( s ) d s + | Q | 0 1 ( 1 s ) α δ 1 Γ ( α δ ) L 1 ( s ) d s + | Q | 0 η ( η s ) α δ 1 Γ ( α δ ) L 1 ( s ) d s ] + σ | A | | A | r Γ ( α ) ( 0 t ( t s ) α 1 1 p d s ) 1 p ( 0 1 L 1 1 p ( s ) d s ) p + σ | A | + | A | | Q | r Γ ( α δ ) ( 0 1 ( 1 s ) α δ 1 1 p d s ) 1 p ( 0 1 L 1 1 p ( s ) d s ) p + | A | | Q | r η α δ p Γ ( α δ ) ( 0 η ( η s ) α δ 1 1 p d s ) 1 p ( 0 1 L 1 1 p ( s ) d s ) p | A | r [ 1 Γ ( α ) ( 1 p α p ) 1 p + | Q | Γ ( α δ ) ( 1 p α δ p ) 1 p + | Q | η α δ p Γ ( α δ ) ( 1 p α δ p ) 1 p ] L 1 + σ | A | .

In a similar manner, we have that

| ( Φ 2 x ) ( t ) | | B | 0 t ( t s ) α + β 1 Γ ( α + β ) m ( s ) ψ ( r ) d s + | B | | Q | 0 1 ( 1 s ) α δ + β 1 Γ ( α δ + β ) m ( s ) ψ ( r ) d s + | B | | Q | 0 η ( η s ) α δ + β 1 Γ ( α δ + β ) m ( s ) ψ ( r ) d s | B | ψ ( r ) [ 1 Γ ( α + β ) ( 1 p α + β p ) 1 p + | Q | Γ ( α δ + β ) ( 1 p α δ + β p ) 1 p ( 1 + η α δ + β p ) ] m .

Thus

| ( Φ x ) ( t ) | | ( Φ 1 x ) ( t ) | + | ( Φ 2 x ) ( t ) | | A | r [ 1 Γ ( α ) ( 1 p α p ) 1 p + | Q | Γ ( α δ ) ( 1 p α δ p ) 1 p + | Q | η α δ p Γ ( α δ ) ( 1 p α δ p ) 1 p ] L 1 + σ | A | + | B | ψ ( r ) [ 1 Γ ( α + β ) ( 1 p α + β p ) 1 p + | Q | Γ ( α δ + β ) ( 1 p α δ + β p ) 1 p ( 1 + η α δ + β p ) ] m γ r + ω r ,

which implies that Φ( B r ) B r .

Step 2. Φ 1 is continuous and γ-contractive.

To show the continuity of Φ 1 for t[0,1], let us consider a sequence x n converging to x. Then, by the assumption ( H 1 ), we have

( Φ 1 x n ) ( t ) ( Φ 1 x ) ( t ) [ | A | L 1 Γ ( α ) ( 1 p α p ) 1 p + | A | | Q | L 1 Γ ( α δ ) ( 1 p α δ p ) 1 p ( 1 + η α δ p ) ] x n x .

Next, we show that Φ 1 is γ-contractive. For x,y B r , we get

( Φ 1 x ) ( t ) ( Φ 1 y ) ( t ) [ | A | L 1 Γ ( α ) ( 1 p α p ) 1 p + | A | | Q | L 1 Γ ( α δ ) ( 1 p α δ p ) 1 p ( 1 + η α δ p ) ] x y .

By the given assumption,

γ= | A | L 1 Γ ( α ) ( 1 p α p ) 1 p + | A | | Q | L 1 Γ ( α δ ) ( 1 p α δ p ) 1 p ( 1 + η α δ p ) <1,

it follows that Φ 1 is γ-contractive.

Step 3. Φ 2 is compact.

In Step 1, it has been shown that Φ 2 is uniformly bounded. Now we show that Φ 2 maps bounded sets into equicontinuous sets of C([0,1],R). Let t 1 , t 2 [0,1] with t 1 < t 2 and x B r . Then we obtain

( Φ 2 x ) ( t 2 ) ( Φ 2 x ) ( t 1 ) | B | Γ ( α + β ) 0 t 1 [ ( t 2 s ) α + β 1 ( t 1 s ) α + β 1 ] | g ( s , x ( s ) ) | d s + | B | Γ ( α + β ) t 1 t 2 ( t 2 s ) α + β 1 | g ( s , x ( s ) ) | d s + | B | | Q | | t 2 α 1 t 1 α 1 | [ 0 1 ( 1 s ) α δ + β 1 Γ ( α δ + β ) | g ( s , x ( s ) ) | d s + 0 η ( η s ) α δ + β 1 Γ ( α δ + β ) | g ( s , x ( s ) ) | d s ] | B | Γ ( α + β ) 0 t 1 [ ( t 2 s ) α + β 1 ( t 1 s ) α + β 1 ] m 2 ( s ) d s + | B | ψ ( r ) Γ ( α + β ) t 1 t 2 ( t 2 s ) α + β 1 m 2 ( s ) d s + | B | | Q | ψ ( r ) | t 2 α 1 t 1 α 1 | [ 0 1 ( 1 s ) α δ + β 1 Γ ( α δ + β ) m 2 ( s ) d s + 0 η ( η s ) α δ + β 1 Γ ( α δ + β ) m 2 ( s ) d s ] .

Obviously, the right-hand side of the above inequality tends to zero independently of x B r as t 2 t 1 0. Therefore it follows by the Arzelá-Ascoli theorem that Φ 2 :C([0,1],R)C([0,1],R) is completely continuous. Thus Φ 2 is compact on [0,1].

Step 4. Φ is condensing.

Since Φ 1 is continuous, γ-contraction and Φ 2 is compact, therefore, by Lemma 2.2, Φ: B r B r with Φ= Φ 1 + Φ 2 is a condensing map on B r .

Consequently, by Theorem 2.1, the map Φ has a fixed point which implies that the problem (1) has a solution. □

In the special case when L 1 (t)=L, L a constant, we have the following.

Corollary 3.1 Let f,g:[0,1]×RR be continuous functions. Assume that g satisfies ( H 2 ) and f satisfies the following condition:

( H 1 )′ |f(t,x)f(t,y)|L|xy| for all (t,x),(t,y)[0,1]×R, L>0 is a constant.

If

γ := | A | L Γ ( α + 1 ) + | A | | Q | L Γ ( α δ + 1 ) ( 1 + η α δ ) <1,

then the boundary value problem (1) has at least one solution.

Example 3.1 Consider a boundary value problem of integro-differential equations of fractional order with nonlocal fractional boundary conditions given by

{ D 5 / 2 x ( t ) = A f ( t , x ( t ) ) + B I β g ( t , x ( t ) ) , t [ 0 , 1 ] , D 1 / 4 x ( 0 ) = 0 , D 5 / 4 x ( 0 ) = 0 , D 1 / 4 x ( 1 ) D 1 / 4 x ( η ) = a ,
(6)

where A=B=1, β=3/4, η=2/3, f(t,x)= e t | x | ( 1 + e t ) ( 1 + | x | ) , g(t,x)= t 2 | x | 3 1 + | x | 3 .

Then we have

| f ( t , x ) f ( t , y ) | = e t 1 + e t | | x | 1 + | x | | y | 1 + | y | | e t | x y | 1 + e t L 1 ( t ) | x y | , where  L 1 ( t ) = 1 2 e t .

Also, for all xC and each t[0,1], we have

| f ( t , x ) | = e t 1 + e t | | x | 1 + | x | | e t 1 + e t < m 1 (t),where  m 1 (t)= 1 2 e t ,

and |g(t,x)| m 2 (t)ψ(x) with m 2 (t)= t 2 ( m 2 = ( 3 / 11 ) 3 / 4 ) and ψ(x)=1. Selecting p=3/4 and using the given data, we find that

γ : = | A | L 1 Γ ( α ) ( 1 p α p ) 1 p + | A | | Q | L 1 Γ ( α δ ) ( 1 p α δ p ) 1 p ( 1 + η α δ p ) 0.825717 .

As γ<1, therefore, by the conclusion of Theorem 3.1, the problem (6) has a solution.