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Article

Positive Solutions for a Hadamard Fractional p-Laplacian Three-Point Boundary Value Problem

1
School of Mathematical Sciences, Qufu Normal University, Qufu 273165, China
2
School of Mathematics, Statistics and Applied Mathematics, National University of Ireland, H91 TK33 Galway, Ireland
3
School of Mathematical Sciences, Chongqing Normal University, Chongqing 401331, China
4
State Key Laboratory of Mining Disaster Prevention and Control Co-Founded by Shandong Province and the Ministry of Science and Technology, Shandong University of Science and Technology, Qingdao 266590, China
*
Author to whom correspondence should be addressed.
Submission received: 4 April 2019 / Revised: 12 May 2019 / Accepted: 13 May 2019 / Published: 17 May 2019

Abstract

:
This article is to study a three-point boundary value problem of Hadamard fractional p-Laplacian differential equation. When our nonlinearity grows ( p 1 ) -superlinearly and ( p 1 ) -sublinearly, the existence of positive solutions is obtained via fixed point index. Moreover, using an increasing operator fixed-point theorem, the uniqueness of positive solutions and uniform convergence sequences are also established.

1. Introduction

In this paper, we study the existence and uniqueness of positive solutions for the Hadamard fractional p-Laplacian three-point boundary value problem
D α ( φ p ( D β u ( t ) ) ) = f ( t , u ( t ) ) , t ( 1 , e ) , D β u ( 1 ) = D β u ( e ) = 0 , u ( 1 ) = u ( 1 ) = 0 , u ( e ) = a u ( ξ ) ,
where α ( 1 , 2 ] , β ( 2 , 3 ] , and D α , D β are respectively the Hadamard fractional derivatives of orders α , β ; ξ ( 1 , e ) , and a 0 with a ( log ξ ) β 1 [ 0 , 1 ) ; note φ p ( s ) = | s | p 2 s is the p-Laplacian for p > 1 , s R .
Arafa et al. [1] introduced a fractional-order HIV-1 infection of CD4+T cells dynamics model and then used the generalised Euler method to find a numerical solution of the HIV-1 infection fractional order model: the model is
D α 1 ( T ) = s K V T d T + b I , D α 2 ( I ) = K V T ( b + δ ) I , D α 3 ( V ) = N δ I c V ,
where D α i ( i = 1 , 2 , 3 ) are fractional-order derivatives. Nonlinear analysis methods (such as fixed-point theorems, Leray–Schauder alternative, subsolution and supersolution methods and iterative techniques) are used to study various kinds of fractional-order equations (most of these results involve the Riemann–Liouville and Caputo-type fractional derivatives); see [2,3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,30,31,32,33,34,35,36,37,38,39,40,41,42,43,44,45,46,47,48,49,50,51,52] and the references therein. In [2], the authors used a double iterative technique to study the unique solution of the p-Laplacian fractional boundary value problem
D x α ( φ p ( D x γ z ) ) ( x ) = f ( x , z ( x ) ) , 0 < x < 1 , z ( 0 ) = 0 , D x γ z ( 0 ) = D x γ z ( 1 ) = 0 , z ( 1 ) = 0 1 z ( x ) d χ ( x ) ,
where D x α , D x γ are the standard Riemann–Liouville derivatives. For the unique solution, they constructed uniform converged sequences, and provided estimates on the error and the convergence rate. In [3], the authors adopted some fixed-point theorems on cones to study the unique solution for the fractional p-Laplacian boundary value problem
D 0 + β φ p ( D 0 + α u ( t ) ) + f ( t , u ( t ) ) = 0 , t ( 0 , 1 ) , u ( 0 ) = u ( 1 ) = u ( 0 ) = D 0 + α u ( 0 ) = 0 ,
where D 0 + α , D 0 + β are the Caputo fractional derivatives and they presented iterative schemes for the unique solution when f doesn’t satisfy a Lipschitz condition. When nonlinearities satisfy a Lipschitz condition, we refer the reader to [4,5,6,7,8,9]. For example, the authors in [4] used Banach’s contraction mapping principle to study the unique solution for the fractional Dirichlet boundary value problem
D 0 + α u ( t ) + f ( t , u ( t ) , u ( t ) ) = 0 , t ( 0 , 1 ) , u ( 0 ) = u ( 1 ) = 0 ,
where D 0 + α denotes the Riemann–Liouville fractional derivative. Positive solutions [16,17,18,19,20,21,22,23,24,25,26,27,28,29,30,31,32,33,34,35] and nontrivial solutions [36,37,38,39,40,41,42,43,44,45,46,47,48,49,50,51,52] were also studied for fractional-order equations. For example, the authors in [16] used the Guo–Krasnoselskii’s fixed-point theorem and the Leggett–Williams fixed-point theorem to study the existence and multiplicity of positive solutions for the fractional boundary-value problem
D α ( φ p ( D α u ( t ) ) ) = f ( t , u ( t ) ) , t [ 0 , 1 ] T , u ( 0 ) = u ( σ ( 1 ) ) = D α u ( 0 ) = D α u ( σ ( 1 ) ) = 0 ,
where D α is the conformable fractional derivative on time scales. In [17], the authors studied positive solutions for the fractional system
D 0 + β 1 ( φ p ( D 0 + α 1 u ( t ) ) ) + λ 1 f 1 ( t , u ( t ) , v ( t ) ) = 0 , t ( 0 , 1 ) , D 0 + β 2 ( φ p ( D 0 + α 2 u ( t ) ) ) + λ 2 f 2 ( t , u ( t ) , v ( t ) ) = 0 , t ( 0 , 1 ) , u ( 0 ) = u ( 0 ) = = u ( n 2 ) ( 0 ) = 0 , φ p ( D 0 + α 1 u ( 0 ) ) = ( φ p ( D 0 + α 1 u ( 1 ) ) ) = 0 , v ( 0 ) = v ( 0 ) = = v ( m 2 ) ( 0 ) = 0 , φ p ( D 0 + α 2 v ( 0 ) ) = ( φ p ( D 0 + α 2 v ( 1 ) ) ) = 0 , u ( 1 ) = μ 1 0 1 g 1 ( s ) v ( s ) d A 1 ( s ) , v ( 1 ) = μ 2 0 1 g 2 ( s ) u ( s ) d A 2 ( s )
and obtained existence and nonexistence of positive solutions, and considered the impact of parameters on solutions. In [36], the authors used the Kuratowski noncompactness measure and the Sadovskii fixed-point theorem to study the impulsive fractional differential equations with the p-Laplacian operator
D 0 + β ( φ p ( D 0 + α x ) ) ( t ) = f ( t , x ( t ) , x ( t ) ) , t ( 0 , 1 ) , Δ x ( t ) | t = t k = I k ( x ( t k ) ) , Δ x ( t ) | t = t k = J k ( x ( t k ) ) , D 0 + α x ( 0 ) = 0 , x ( 0 ) = x ( 0 ) = 0 1 a 1 ( x ( s ) ) d s , x ( 1 ) = x ( 1 ) = 0 1 a 2 ( x ( s ) ) d s .
Hadamard fractional-order problems were briefly discussed in the literature; see [53,54,55,56,57,58,59,60,61,62,63,64,65,66,67,68,69,70,71,72] and the references therein. Yang in [53] used the comparison principle and the monotone iterative technique combined with the subsolution and supersolution method to study the existence of extremal solutions for Hadamard fractional differential equations with Cauchy initial value conditions
( D a + α x ) ( t ) = f ( t , x ( t ) , y ( t ) ) , ( J a + 1 α x ) ( a + ) = x 0 * , α ( 0 , 1 ] , t ( a , b ] , ( D a + α y ) ( t ) = g ( t , x ( t ) , y ( t ) ) , ( J a + 1 α y ) ( a + ) = y 0 * , α ( 0 , 1 ] , t ( a , b ] ,
where D a + α , J a + α are the left-sided Hadamard fractional derivative and integral of order α , respectively. In [54], the authors used fixed point methods to study the existence of positive solutions for Hadamard fractional integral boundary value problems
D β ( φ p ( D α u ( t ) ) ) = f ( t , u ( t ) ) , t ( 1 , e ) , u ( 1 ) = D α u ( 1 ) = u ( 1 ) = u ( e ) = 0 , φ p ( D α u ( e ) ) = μ 1 e φ p ( D α u ( t ) ) d t t .
In this paper, we study the existence of positive solutions for the Hadamard fractional p-Laplacian three-point boundary value problem (1). Note: (i) we establish some relations from the corresponding problem without the p-Laplacian operator, and use some ( p 1 ) -superlinearly and ( p 1 ) -sublinearly conditions for the nonlinearity to obtain positive solutions for (1); (ii) using an increasing operator fixed-point theorem, we obtain the unique solution for (1), and establish uniformconverged sequences for this solution.

2. Preliminaries

In this paper, we only provide the definition for the Hadamard fractional derivative; for more details about Hadamard fractional calculus, see the book [73].
Definition 1.
The Hadamard derivative of fractional order q for a function g : [ 1 , ) R is defined as
D q g ( t ) = 1 Γ ( n q ) t d d t n 1 t log t log s n q 1 g ( s ) d s s , n 1 < q < n ,
where n = [ q ] + 1 , [ q ] denotes the integer part of the real number q and log ( · ) = log e ( · ) .
In what follows, we calculate the Green’s functions associated with (1). We let φ p ( D β u ( t ) ) = v ( t ) for t [ 1 , e ] . Then, from (1) we obtain
D α v ( t ) = f ( t , u ( t ) ) , t ( 1 , e ) , v ( 1 ) = v ( e ) = 0 .
Lemma 1.
The boundary value problem (10) takes the form
v ( t ) = 1 e G α ( t , s ) f ( s , u ( s ) ) d s s ,
where
G α ( t , s ) = 1 Γ ( α ) ( log t ) α 1 ( 1 log s ) α 1 ( log t log s ) α 1 , 1 s t e , ( log t ) α 1 ( 1 log s ) α 1 , 1 t s e .
Proof. 
We use ideas in Lemma 2 of [59]. For some c i R ( i = 1 , 2 ) , we have
v ( t ) = c 1 ( log t ) α 1 + c 2 ( log t ) α 2 1 Γ ( α ) 1 t ( log t log s ) α 1 f ( s , u ( s ) ) d s s .
From the condition v ( 1 ) = 0 , we have c 2 = 0 . Hence,
v ( t ) = c 1 ( log t ) α 1 1 Γ ( α ) 1 t ( log t log s ) α 1 f ( s , u ( s ) ) d s s .
Substituting e into the above equation, and using u ( e ) = 0 , we obtain
v ( e ) = c 1 1 Γ ( α ) 1 e ( 1 log s ) α 1 f ( s , u ( s ) ) d s s = 0 .
Then,
c 1 = 1 Γ ( α ) 1 e ( 1 log s ) α 1 f ( s , u ( s ) ) d s s = 0 .
Consequently, we have
v ( t ) = 1 Γ ( α ) 1 e ( log t ) α 1 ( 1 log s ) α 1 f ( s , u ( s ) ) d s s 1 Γ ( α ) 1 t ( log t log s ) α 1 f ( s , u ( s ) ) d s s = 1 e G α ( t , s ) f ( s , u ( s ) ) d s s .
This completes the proof. □
Note that φ p ( D β u ( t ) ) = v ( t ) . Then, φ p ( D β u ( t ) ) = v ( t ) and D β u ( t ) = φ q ( v ( t ) ) , where q is a constant with q 1 + p 1 = 1 . Then, from (1), we have
D β u ( t ) = φ q ( v ( t ) ) , t ( 1 , e ) , u ( 1 ) = u ( 1 ) = 0 , u ( e ) = a u ( ξ ) .
Lemma 2.
The boundary value problem (12) is equivalent to the integral equation
u ( t ) = 1 e G β ( t , s ) φ q v ( s ) d s s ,
where
G 1 β ( t , s ) = 1 Γ ( β ) ( log t ) β 1 ( 1 log s ) β 1 ( log t log s ) β 1 , 1 s t e , ( log t ) β 1 ( 1 log s ) β 1 , 1 t s e , G β ( t , s ) = G 1 β ( t , s ) + a ( log t ) β 1 ( 1 a ( log ξ ) β 1 ) Γ ( β ) G 1 β ( ξ , s ) .
Proof. 
We follow the ideas in Lemma 1. For some c i R ( i = 1 , 2 , 3 ) , we have
u ( t ) = c 1 ( log t ) β 1 + c 2 ( log t ) β 2 + c 3 ( log t ) β 3 1 Γ ( β ) 1 t ( log t log s ) β 1 φ q v ( s ) d s s .
Then, u ( 1 ) = u ( 1 ) = 0 implies c 2 = c 3 = 0 . Consequently, we have
u ( t ) = c 1 ( log t ) β 1 1 Γ ( β ) 1 t ( log t log s ) β 1 φ q v ( s ) d s s .
Substituting e , ξ into the above equation, and using u ( e ) = a u ( ξ ) , we obtain
c 1 1 Γ ( β ) 1 e ( 1 log s ) β 1 φ q v ( s ) d s s = a c 1 ( log ξ ) β 1 a Γ ( β ) 1 ξ ( log ξ log s ) β 1 φ q v ( s ) d s s .
Solving this equation, we have
c 1 = 1 ( 1 a ( log ξ ) β 1 ) Γ ( β ) 1 e ( 1 log s ) β 1 φ q v ( s ) d s s a ( 1 a ( log ξ ) β 1 ) Γ ( β ) 1 ξ ( log ξ log s ) β 1 φ q v ( s ) d s s .
As a result, we obtain
u ( t ) = ( log t ) β 1 ( 1 a ( log ξ ) β 1 ) Γ ( β ) 1 e ( 1 log s ) β 1 φ q v ( s ) d s s a ( log t ) β 1 ( 1 a ( log ξ ) β 1 ) Γ ( β ) 1 ξ ( log ξ log s ) β 1 φ q v ( s ) d s s 1 Γ ( β ) 1 t ( log t log s ) β 1 φ q v ( s ) d s s = ( log t ) β 1 ( 1 a ( log ξ ) β 1 ) Γ ( β ) 1 e ( 1 log s ) β 1 φ q v ( s ) d s s a ( log t ) β 1 ( 1 a ( log ξ ) β 1 ) Γ ( β ) 1 ξ ( log ξ log s ) β 1 φ q v ( s ) d s s 1 Γ ( β ) 1 t ( log t log s ) β 1 φ q v ( s ) d s s + 1 Γ ( β ) 1 e ( log t ) β 1 ( 1 log s ) β 1 φ q v ( s ) d s s 1 Γ ( β ) 1 e ( log t ) β 1 ( 1 log s ) β 1 φ q v ( s ) d s s = 1 e G 1 β ( t , s ) φ q v ( s ) d s s + a ( log t ) β 1 ( 1 a ( log ξ ) β 1 ) Γ ( β ) 1 e ( log ξ ) β 1 ( 1 log s ) β 1 φ q v ( s ) d s s a ( log t ) β 1 ( 1 a ( log ξ ) β 1 ) Γ ( β ) 1 ξ ( log ξ log s ) β 1 φ q v ( s ) d s s = 1 e G 1 β ( t , s ) φ q v ( s ) d s s + a ( log t ) β 1 ( 1 a ( log ξ ) β 1 ) Γ ( β ) 1 e G 1 β ( ξ , s ) φ q v ( s ) d s s = 1 e G β ( t , s ) φ q v ( s ) d s s .
This completes the proof. □
Note v ( t ) = 1 e G α ( t , s ) f ( s , u ( s ) ) d s s , t [ 1 , e ] , and we have that (1) is equivalent to the Hammerstein type integral equation
u ( t ) = 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) f ( τ , u ( τ ) ) d τ τ d s s .
Let E : = C [ 1 , e ] , u : = max t [ 1 , e ] | u ( t ) | , P : = { u E : u ( t ) 0 , t [ 1 , e ] } . Then, ( E , · ) is a real Banach space and P a cone on E. From (15), we define an operator A : E E as follows:
( A u ) ( t ) = 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) f ( τ , u ( τ ) ) d τ τ d s s , u E .
Note that our functions G α , G β , f are continuous, so the operator A is a completely continuous operator. Moreover, if there is a u E is a fixed point of A, then from Lemmas 1–2, we have that u is a solution for (1). Therefore, in what follows, we turn to study the existence of fixed points of the operator A.
Lemma 3.
(see [21] (Lemma 3.2). Let β ( n 1 , n ] , and n 3 . Then, the function G has the properties:
(R1) G ( t , s ) = G ( 1 s , 1 t ) , for t , s [ 0 , 1 ] ,
(R2) t β 1 ( 1 t ) s ( 1 s ) β 1 Γ ( β ) G ( t , s ) ( β 1 ) s ( 1 s ) β 1 , for t , s [ 0 , 1 ] ,
(R3) t β 1 ( 1 t ) s ( 1 s ) β 1 Γ ( β ) G ( t , s ) ( β 1 ) t β 1 ( 1 t ) , for t , s [ 0 , 1 ] , where
G ( t , s ) = 1 Γ ( β ) t β 1 ( 1 s ) β 1 ( t s ) β 1 , 0 s t 1 , t β 1 ( 1 s ) β 1 , 0 t s 1 .
Lemma 4.
Let ϕ ( t ) = ( log t ) β 1 ( 1 log t ) Γ ( β ) , η ( s ) = log s ( 1 log s ) β 1 Γ ( β ) , for t , s [ 1 , e ] . Then, the functions G α , G β have the properties:
(I1) G α C ( [ 1 , e ] × [ 1 , e ] , R + ) and Γ ( α ) G α ( t , s ) 1 , for t , s [ 1 , e ] ,
(I2) ϕ ( t ) η ( s ) ( 1 a ( log ξ ) β 1 + a ϕ ( ξ ) ) Γ ( β ) 1 a ( log ξ ) β 1 G β ( t , s ) ( a + ( 1 a ( log ξ ) β 1 ) Γ ( β ) ) ( β 1 ) ( 1 a ( log ξ ) β 1 ) Γ ( β ) η ( s ) , for t , s [ 1 , e ] ,
(I3) G β ( t , s ) ( 1 a ( log ξ ) β 1 + a ϕ ( ξ ) ) ( β 1 ) ( log t ) β 1 ( 1 a ( log ξ ) β 1 ) Γ ( β ) , for t , s [ 1 , e ] .
Proof. 
From the definition of G α , we easily have (I1). From Lemma 3, in G ( t , s ) , using log t , log s to replace t , s , we have
Γ ( β ) ϕ ( t ) η ( s ) G 1 β ( t , s ) ( β 1 ) η ( s ) , for t , s [ 1 , e ] ,
and
G 1 β ( t , s ) ( β 1 ) ϕ ( t ) , for t , s [ 1 , e ] .
Consequently, from (17), we have
G β ( t , s ) = G 1 β ( t , s ) + a ( log t ) β 1 ( 1 a ( log ξ ) β 1 ) Γ ( β ) G 1 β ( ξ , s ) ( β 1 ) η ( s ) + a ( log t ) β 1 ( 1 a ( log ξ ) β 1 ) Γ ( β ) ( β 1 ) η ( s ) = ( a + ( 1 a ( log ξ ) β 1 ) Γ ( β ) ) ( β 1 ) ( 1 a ( log ξ ) β 1 ) Γ ( β ) η ( s ) , for t , s [ 1 , e ] ,
and
G β ( t , s ) = G 1 β ( t , s ) + a ( log t ) β 1 ( 1 a ( log ξ ) β 1 ) Γ ( β ) G 1 β ( ξ , s ) Γ ( β ) ϕ ( t ) η ( s ) + a ( log t ) β 1 ( 1 a ( log ξ ) β 1 ) Γ ( β ) Γ ( β ) ϕ ( ξ ) η ( s ) Γ ( β ) ϕ ( t ) η ( s ) + a ( log t ) β 1 ( 1 log t ) ( 1 a ( log ξ ) β 1 ) Γ ( β ) Γ ( β ) ϕ ( ξ ) η ( s ) = Γ ( β ) ϕ ( t ) η ( s ) + a 1 a ( log ξ ) β 1 Γ ( β ) ϕ ( t ) ϕ ( ξ ) η ( s ) = Γ ( β ) ϕ ( t ) η ( s ) 1 a ( log ξ ) β 1 + a ϕ ( ξ ) 1 a ( log ξ ) β 1 , for t , s [ 1 , e ] .
This implies that (I2) holds. Finally, from (18), we obtain
G β ( t , s ) = G 1 β ( t , s ) + a ( log t ) β 1 ( 1 a ( log ξ ) β 1 ) Γ ( β ) G 1 β ( ξ , s ) ( β 1 ) ( log t ) β 1 ( 1 log t ) Γ ( β ) + a ( log t ) β 1 ( 1 a ( log ξ ) β 1 ) Γ ( β ) ( β 1 ) ϕ ( ξ ) ( β 1 ) ( log t ) β 1 Γ ( β ) 1 + a ϕ ( ξ ) 1 a ( log ξ ) β 1 = ( 1 a ( log ξ ) β 1 + a ϕ ( ξ ) ) ( β 1 ) ( log t ) β 1 ( 1 a ( log ξ ) β 1 ) Γ ( β ) , for t , s [ 1 , e ] .
Thus, (I3) holds. This completes the proof. □
For convenience, we define three positive constants
κ 1 = ( 1 a ( log ξ ) β 1 + a ϕ ( ξ ) ) Γ ( β ) 1 a ( log ξ ) β 1 , κ 2 = ( a + ( 1 a ( log ξ ) β 1 ) Γ ( β ) ) ( β 1 ) ( 1 a ( log ξ ) β 1 ) Γ ( β ) ,
κ 3 = ( 1 a ( log ξ ) β 1 + a ϕ ( ξ ) ) ( β 1 ) ( 1 a ( log ξ ) β 1 ) Γ ( β ) .
Lemma 5.
Let z P and μ ( τ ) = 1 e η ( s ) G α ( s , τ ) d s s , for τ [ 1 , e ] . Then, we have the following two integral inequalities
1 e G β ( t , s ) 1 e G α ( s , τ ) z ( τ ) d τ τ d s s κ 1 ϕ ( t ) 1 e z ( τ ) μ ( τ ) d τ τ , for t [ 1 , e ] ,
and
1 e G β ( t , s ) 1 e G α ( s , τ ) z ( τ ) d τ τ d s s κ 2 1 e z ( τ ) μ ( τ ) d τ τ , for t [ 1 , e ] .
This is a direct result from Lemma 4(I2), so we omit the details.
Lemma 6.
(see [74] (Lemma 2.6)). Let θ > 0 and φ P . Then,
0 1 φ ( t ) d t θ 0 1 φ θ ( t ) d t , if θ 1 , and 0 1 φ ( t ) d t θ 0 1 φ θ ( t ) d t , i f 0 < θ 1 .
Lemma 7.
(see [75]). Let E be a real Banach space and P a cone on E. Suppose that Ω E is a bounded open set and that A : Ω ¯ P P is a continuous compact operator. If there exists a ω 0 P \ { 0 } such that
ω A ω λ ω 0 , λ 0 , ω Ω P ,
then i ( A , Ω P , P ) = 0 , where i denotes the fixed point index on P.
Lemma 8.
(see [75]). Let E be a real Banach space and P a cone on E. Suppose that Ω E is a bounded open set with 0 Ω and that A : Ω ¯ P P is a continuous compact operator. If
ω λ A ω 0 , λ [ 0 , 1 ] , ω Ω P ,
then i ( A , Ω P , P ) = 1 .
Lemma 9.
(see [75]). Let E be a partially ordered Banach space, and x 0 , y 0 E with x 0 y 0 , D = [ x 0 , y 0 ] . Suppose that A : D E satisfies the following conditions:
(i) A is an increasing operator;
(ii) x 0 A x 0 , y 0 A y 0 , i.e., x 0 and y 0 is a subsolution and a supersolution of A;
(iii) A is a completely continuous operator.
Then, A has the smallest fixed point x * and the largest fixed point y * in [ x 0 , y 0 ] , respectively. Moreover, x * = lim n A n x 0 and y * = lim n A n y 0 .

3. Positive Solutions for (1)

For convenience, let
κ 3 = κ 1 1 e μ ( t ) ϕ ( t ) d t t , κ 4 = κ 2 1 e μ ( t ) d t t .
First, we list assumptions for our nonlinearity f:
(H1) f C ( [ 0 , 1 ] × R + , R + ) ,
(H2) there exist c 1 > 0 , a 1 > κ 3 1 p , 1 < p 2 , κ 3 1 p Γ 2 p ( α ) , p 2 , such that
f ( t , z ) a 1 z p 1 c 1 , ( t , z ) [ 1 , e ] × R + ,
(H3) there exist r 1 > 0 , a 2 ( 0 , κ 4 1 p Γ 2 p ( α ) ) , 1 < p 2 , ( 0 , κ 4 1 κ 3 2 p ) , p 2 , such that
f ( t , z ) a 2 z p 1 , ( t , z ) [ 1 , e ] × [ 0 , r 1 ] ,
(H4) there exist r 2 > 0 , a 3 > κ 3 1 p , 1 < p 2 , κ 3 1 p Γ 2 p ( α ) , p 2 , such that
f ( t , z ) a 3 z p 1 , ( t , z ) [ 1 , e ] × [ 0 , r 2 ] ,
(H5) there exist c 2 > 0 , a 4 ( 0 , κ 4 1 p 2 p 2 Γ 2 p ( α ) ) , 1 < p 2 , ( 0 , κ 4 1 κ 3 2 p ) , p 2 , such that
f ( t , z ) a 4 z p 1 + c 2 , ( t , z ) [ 1 , e ] × R + ,
(H6) there exists k ( 0 , 1 ) such that f ( t , λ u ) λ k ( p 1 ) f ( t , u ) , λ [ 0 , 1 ] , t [ 1 , e ] .
(H7) f ( t , u ) is increasing with respect to u, i.e., f ( t , u 1 ) f ( t , u 2 ) if u 1 u 2 , and f ( t , 0 ) 0 , t [ 1 , e ] .
Let
P 0 = z P : z ( t ) ( 1 a ( log ξ ) β 1 + a ϕ ( ξ ) ) Γ 2 ( β ) ( a + ( 1 a ( log ξ ) β 1 ) Γ ( β ) ) ( β 1 ) ϕ ( t ) z , t [ 1 , e ] = z P : z ( t ) κ 1 κ 2 ϕ ( t ) z , t [ 1 , e ] .
Then, we have the following lemma.
Lemma 10.
Suppose that (H1) holds. Then, A ( P ) P 0 .
Proof. 
From Lemma 4(I2), for u P , we have
( A u ) ( t ) = 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) f ( τ , u ( τ ) ) d τ τ d s s 1 e ( a + ( 1 a ( log ξ ) β 1 ) Γ ( β ) ) ( β 1 ) ( 1 a ( log ξ ) β 1 ) Γ ( β ) η ( s ) φ q 1 e G α ( s , τ ) f ( τ , u ( τ ) ) d τ τ d s s ,
and
( A u ) ( t ) 1 e Γ ( β ) ϕ ( t ) η ( s ) 1 a ( log ξ ) β 1 + a ϕ ( ξ ) 1 a ( log ξ ) β 1 φ q 1 e G α ( s , τ ) f ( τ , u ( τ ) ) d τ τ d s s = ( 1 a ( log ξ ) β 1 + a ϕ ( ξ ) ) Γ 2 ( β ) ( a + ( 1 a ( log ξ ) β 1 ) Γ ( β ) ) ( β 1 ) ϕ ( t ) 1 e ( a + ( 1 a ( log ξ ) β 1 ) Γ ( β ) ) ( β 1 ) ( 1 a ( log ξ ) β 1 ) Γ ( β ) η ( s ) · φ q 1 e G α ( s , τ ) f ( τ , u ( τ ) ) d τ τ d s s ( 1 a ( log ξ ) β 1 + a ϕ ( ξ ) ) Γ 2 ( β ) ( a + ( 1 a ( log ξ ) β 1 ) Γ ( β ) ) ( β 1 ) ϕ ( t ) A u , for t [ 1 , e ] .
Therefore, ( A u ) ( t ) ( 1 a ( log ξ ) β 1 + a ϕ ( ξ ) ) Γ 2 ( β ) ( a + ( 1 a ( log ξ ) β 1 ) Γ ( β ) ) ( β 1 ) ϕ ( t ) A u , for t [ 1 , e ] . This completes the proof. □
Let B ρ = { u P : u < ρ } , for ρ > 0 .
Theorem 1.
Suppose that (H1)–(H3) hold. Then, (1) has at least one positive solution.
Proof. 
Let S 1 = { u P : u = A u + λ ψ , λ 0 } , where ψ P 0 is a fixed element. We prove that S 1 is bounded in P. If u S 1 , then, from Lemma 10, we have u P 0 , and u ( t ) ( A u ) ( t ) for t [ 1 , e ] . Now, we consider two cases. □
Case 1. Let p 2 . Then, we have 1 p 1 ( 0 , 1 ] . From (H2), we have
f 1 p 1 ( t , z ) + c 1 1 p 1 ( f ( t , z ) + c 1 ) 1 p 1 ( a 1 z p 1 ) 1 p 1 = a 1 1 p 1 z , for ( t , z ) [ 1 , e ] × R + .
Consequently, from (19) and Lemma 6, we obtain
u ( t ) 1 e G β ( t , s ) 1 e G α ( s , τ ) f ( τ , u ( τ ) ) d τ τ 1 p 1 d s s = Γ 1 p 1 ( α ) 1 e G β ( t , s ) 1 e Γ ( α ) G α ( s , τ ) f ( τ , u ( τ ) ) d τ τ 1 p 1 d s s = Γ 1 p 1 ( α ) 1 e G β ( t , s ) 1 e Γ ( α ) G α ( s , τ ) f ( τ , u ( τ ) ) d log τ 1 p 1 d s s = Γ 1 p 1 ( α ) 1 e G β ( t , s ) 0 1 Γ ( α ) G α ( s , e x ) f ( e x , u ( e x ) ) d x 1 p 1 d s s Γ 1 p 1 ( α ) 1 e G β ( t , s ) 0 1 ( Γ ( α ) G α ( s , e x ) ) 1 p 1 f 1 p 1 ( e x , u ( e x ) ) d x d s s Γ 1 p 1 ( α ) 1 e G β ( t , s ) 0 1 ( Γ ( α ) G α ( s , e x ) ) f 1 p 1 ( e x , u ( e x ) ) d x d s s = Γ p 2 p 1 ( α ) 1 e G β ( t , s ) 1 e G α ( s , τ ) f 1 p 1 ( τ , u ( τ ) ) d τ τ d s s κ 1 ϕ ( t ) Γ p 2 p 1 ( α ) 1 e μ ( τ ) f 1 p 1 ( τ , u ( τ ) ) d τ τ κ 1 ϕ ( t ) Γ p 2 p 1 ( α ) 1 e μ ( τ ) a 1 1 p 1 u ( τ ) c 1 1 p 1 d τ τ .
Multiplying by μ ( t ) on both sides of (21) and integrating over [ 1 , e ] , we obtain
1 e u ( t ) μ ( t ) d t t κ 1 Γ p 2 p 1 ( α ) 1 e μ ( t ) ϕ ( t ) d t t 1 e μ ( t ) a 1 1 p 1 u ( t ) c 1 1 p 1 d t t = κ 3 Γ p 2 p 1 ( α ) 1 e μ ( t ) a 1 1 p 1 u ( t ) c 1 1 p 1 d t t .
Solving this inequality, we have
1 e u ( t ) μ ( t ) d t t κ 3 c 1 1 p 1 Γ p 2 p 1 ( α ) 1 e μ ( t ) d t t κ 3 a 1 1 p 1 Γ p 2 p 1 ( α ) 1 .
Note that, for u P 0 , we get
1 e κ 1 κ 2 ϕ ( t ) u μ ( t ) d t t κ 3 c 1 1 p 1 Γ p 2 p 1 ( α ) 1 e μ ( t ) d t t κ 3 a 1 1 p 1 Γ p 2 p 1 ( α ) 1 , and u κ 4 c 1 1 p 1 Γ p 2 p 1 ( α ) κ 3 a 1 1 p 1 Γ p 2 p 1 ( α ) 1 .
Case 2. Let p ( 1 , 2 ] . Then, we have p 1 ( 0 , 1 ] . Note that G β ( t , s ) κ 3 1 , for t , s [ 1 , e ] , by (H2), (19) and Lemma 6 we have
u p 1 ( t ) 1 e G β ( t , s ) 1 e G α ( s , τ ) f ( τ , u ( τ ) ) d τ τ 1 p 1 d s s p 1 = κ 3 p 1 1 e G β ( t , s ) κ 3 1 e G α ( s , τ ) f ( τ , u ( τ ) ) d τ τ 1 p 1 d log s p 1 = κ 3 p 1 0 1 G β ( t , e x ) κ 3 1 e G α ( e x , τ ) f ( τ , u ( τ ) ) d τ τ 1 p 1 d x p 1 κ 3 p 1 0 1 G β ( t , e x ) κ 3 p 1 1 e G α ( e x , τ ) f ( τ , u ( τ ) ) d τ τ d x κ 3 p 2 1 e G β ( t , s ) 1 e G α ( s , τ ) f ( τ , u ( τ ) ) d τ τ d s s κ 1 κ 3 p 2 ϕ ( t ) 1 e μ ( τ ) f ( τ , u ( τ ) ) d τ τ κ 1 κ 3 p 2 ϕ ( t ) 1 e μ ( τ ) ( a 1 u p 1 ( τ ) c 1 ) d τ τ .
Multiplying by μ ( t ) on both sides of (22) and integrating over [ 1 , e ] , we conclude that
1 e μ ( t ) u p 1 ( t ) d t t κ 1 κ 3 p 2 1 e μ ( t ) ϕ ( t ) d t t 1 e μ ( t ) ( a 1 u p 1 ( t ) c 1 ) d t t .
Solving this inequality, we have
1 e μ ( t ) u p 1 ( t ) d t t κ 3 p 1 c 1 1 e μ ( t ) d t t κ 3 p 1 a 1 1 .
Noting that u P 0 , we have
u p 1 κ 3 p 1 κ 2 p 2 κ 1 1 p c 1 κ 4 κ 3 p 1 a 1 1 1 e μ ( t ) ϕ p 1 ( t ) d t t 1 .
The above two cases imply that S 1 is bounded in P. Then, we can choose
R 1 > κ 3 p 1 κ 2 p 2 κ 1 1 p c 1 κ 4 κ 3 p 1 a 1 1 1 e μ ( t ) ϕ p 1 ( t ) d t t 1 p 1 , 1 < p 2 , κ 4 c 1 1 p 1 Γ p 2 p 1 ( α ) κ 3 a 1 1 p 1 Γ p 2 p 1 ( α ) 1 , p 2 ,
such that
u A u + λ ψ , for u B R 1 P , λ 0 .
As a result, Lemma 7 implies that
i ( A , B R 1 P , P ) = 0 .
For r 1 in (H3), we now prove that
u λ A u , for u B r 1 P , λ [ 0 , 1 ] .
If this claim isn’t true, then there exist u B r 1 P and λ [ 0 , 1 ] such that u = λ A u , and u ( t ) ( A u ) ( t ) , for t [ 1 , e ] . Now, we consider two cases.
Case 1. Let p 2 . Then, we have p 1 1 . From (20), (H3) and Lemma 6, we get
u p 1 ( t ) 1 e G β ( t , s ) 1 e G α ( s , τ ) f ( τ , u ( τ ) ) d τ τ 1 p 1 d s s p 1 = κ 3 p 1 0 1 G β ( t , e x ) κ 3 1 e G α ( e x , τ ) f ( τ , u ( τ ) ) d τ τ 1 p 1 d x p 1 κ 3 p 2 0 1 G β ( t , e x ) 1 e G α ( e x , τ ) f ( τ , u ( τ ) ) d τ τ d x = κ 3 p 2 1 e G β ( t , s ) 1 e G α ( s , τ ) f ( τ , u ( τ ) ) d τ τ d s s κ 3 p 2 κ 2 1 e μ ( τ ) a 2 u p 1 ( τ ) d τ τ .
Multiplying by μ ( t ) on both sides of (25) and integrating over [ 1 , e ] , we find
1 e μ ( t ) u p 1 ( t ) d t t κ 3 p 2 a 2 κ 4 1 e μ ( t ) u p 1 ( t ) d t t .
This implies that
1 e μ ( t ) u p 1 ( t ) d t t = 0 , and u ( t ) 0 , for t [ 1 , e ] ,
since μ ( t ) ¬ 0 , for t [ 1 , e ] . This contradicts u B r 1 P , r 1 > 0 .
Case 2. Let p ( 1 , 2 ] . Then, we have 1 p 1 1 . From (20), (H3) and Lemma 6, we obtain
u ( t ) 1 e G β ( t , s ) 1 e G α ( s , τ ) f ( τ , u ( τ ) ) d τ τ 1 p 1 d s s = Γ 1 p 1 ( α ) 1 e G β ( t , s ) 0 1 Γ ( α ) G α ( s , e x ) f ( e x , u ( e x ) ) d x 1 p 1 d s s Γ 1 p 1 ( α ) 1 e G β ( t , s ) 0 1 ( Γ ( α ) G α ( s , e x ) ) 1 p 1 f 1 p 1 ( e x , u ( e x ) ) d x d s s Γ p 2 p 1 ( α ) 1 e G β ( t , s ) 1 e G α ( s , τ ) f 1 p 1 ( τ , u ( τ ) ) d τ τ d s s Γ p 2 p 1 ( α ) κ 2 1 e μ ( τ ) a 2 1 p 1 u ( τ ) d τ τ .
Multiplying by μ ( t ) on both sides of the preceding inequalities and integrating over [ 1 , e ] , we find
1 e μ ( t ) u ( t ) d t t Γ p 2 p 1 ( α ) κ 4 a 2 1 p 1 1 e μ ( t ) u ( t ) d t t .
Note that μ ( t ) ¬ 0 , for t [ 1 , e ] , and this implies that
1 e μ ( t ) u p 1 ( t ) d t t = 0 , and u ( t ) 0 , for t [ 1 , e ] .
This contradicts u B r 1 P , r 1 > 0 .
Combining the above two cases, we have that (24) holds. Then, from Lemma 8, we obtain
i ( A , B r 1 P , P ) = 1 .
Note that we can also take R 1 > r 1 such that (23) is still true. Thus, from (23) and (27), we have
i ( A , ( B R 1 B ¯ r 1 ) P , P ) = i ( A , B R 1 P , P ) i ( A , B r 1 P , P ) = 1 ,
and hence A has at least one fixed point in ( B R 1 \ B ¯ r 1 ) P , i.e., (1) has at least one positive solution. This completes the proof.
Theorem 2.
Suppose that (H1), and (H4)–(H5) hold. Then, (1) has at least one positive solution.
Proof. 
We can use similar methods as in Theorem 1 to provide the proof. We first prove that
u A u + λ ψ ˜ , for u B r 2 P , λ 0 ,
where ψ ˜ P is a given element, and r 2 is defined in (H4). Otherwise, there exist u B r 2 P and λ 0 such that u = A u + λ ψ ˜ , and thus u ( t ) ( A u ) ( t ) , for t [ 1 , e ] . Now, we consider two cases. □
Case 1. Let p 2 . Then, we have 1 p 1 ( 0 , 1 ] . Using (21) and (H4), we conclude
u ( t ) κ 1 ϕ ( t ) Γ p 2 p 1 ( α ) 1 e μ ( τ ) f 1 p 1 ( τ , u ( τ ) ) d τ τ κ 1 ϕ ( t ) Γ p 2 p 1 ( α ) 1 e μ ( τ ) a 3 1 p 1 u ( τ ) d τ τ .
Multiplying by μ ( t ) on both sides of the preceding inequalities and integrating over [ 1 , e ] , we find
1 e μ ( t ) u ( t ) d t t a 3 1 p 1 κ 1 Γ p 2 p 1 ( α ) 1 e ϕ ( t ) μ ( t ) d t t 1 e μ ( t ) u ( t ) d t t .
This implies that
1 e μ ( t ) u ( t ) d t t = 0 , and u ( t ) 0 , for t [ 1 , e ] ,
since μ ( t ) 0 , for t [ 1 , e ] . This contradicts u B r 2 P , r 2 > 0 .
Case 2. Let p ( 1 , 2 ] . Then, we have p 1 ( 0 , 1 ] . Using (22) and (H4), we obtain
u p 1 ( t ) κ 1 κ 3 p 2 ϕ ( t ) 1 e μ ( τ ) f ( τ , u ( τ ) ) d τ τ κ 1 κ 3 p 2 ϕ ( t ) 1 e μ ( τ ) a 3 u p 1 ( τ ) d τ τ .
Multiplying by μ ( t ) on both sides of the preceding inequalities and integrating over [ 1 , e ] , we find
1 e μ ( t ) u p 1 ( t ) d t t a 3 κ 1 κ 3 p 2 1 e ϕ ( t ) μ ( t ) d t t 1 e μ ( t ) u p 1 ( t ) d t t .
This implies that
1 e μ ( t ) u p 1 ( t ) d t t = 0 , and u ( t ) 0 , for t [ 1 , e ] ,
since μ ( t ) 0 , for t [ 1 , e ] . This contradicts u B r 2 P , r 2 > 0 .
As a result, we have that (28) holds, and Lemma 7 implies that
i ( A , B r 2 P , P ) = 0 .
Let S 2 = { u P : u = λ A u , λ [ 0 , 1 ] } . Then, we claim that S 2 is bounded in P. Indeed, if u S 2 , then from Lemma 10 we have u P 0 , and u ( t ) ( A u ) ( t ) , for t [ 1 , e ] . Now, we consider two cases.
Case 1. Let p 2 . Then, we have p 1 1 . Using (25) and (H5), we have
u p 1 ( t ) κ 3 p 2 κ 2 1 e μ ( τ ) ( a 4 u p 1 ( τ ) + c 2 ) d τ τ .
Multiplying by μ ( t ) on both sides of the preceding inequalities and integrating over [ 1 , e ] , we find
1 e μ ( t ) u p 1 ( t ) d t t κ 3 p 2 κ 4 1 e μ ( t ) ( a 4 u p 1 ( t ) + c 2 ) d t t .
Solving this inequality, we have
1 e μ ( t ) u p 1 ( t ) d t t κ 3 p 2 c 2 κ 4 1 e μ ( t ) d t t 1 κ 3 p 2 a 4 κ 4 .
Note that u P 0 , and we have
u p 1 κ 3 p 2 κ 2 p 2 κ 1 1 p c 2 κ 4 2 1 κ 3 p 2 a 4 κ 4 1 e μ ( t ) ϕ p 1 ( t ) d t t 1 .
Case 2. Let p ( 1 , 2 ] . Then, we have 1 p 1 1 . Using (26) and (H5), we obtain
u ( t ) Γ p 2 p 1 ( α ) κ 2 1 e μ ( τ ) ( a 4 u p 1 ( τ ) + c 2 ) 1 p 1 d τ τ Γ p 2 p 1 ( α ) 2 2 p p 1 κ 2 1 e μ ( t ) ( a 4 1 p 1 u ( t ) + c 2 1 p 1 ) d t t .
Multiplying by μ ( t ) on both sides of the preceding inequalities and integrating over [ 1 , e ] , we find
1 e μ ( t ) u ( t ) d t t Γ p 2 p 1 ( α ) 2 2 p p 1 κ 4 1 e μ ( t ) ( a 4 1 p 1 u ( t ) + c 2 1 p 1 ) d t t .
Solving this inequality, we have
1 e μ ( t ) u ( t ) d t t Γ p 2 p 1 ( α ) 2 2 p p 1 c 2 1 p 1 κ 4 2 κ 2 ( 1 Γ p 2 p 1 ( α ) 2 2 p p 1 a 4 1 p 1 κ 4 ) .
Noting that u P 0 , we have
u Γ p 2 p 1 ( α ) 2 2 p p 1 c 2 1 p 1 κ 4 2 κ 3 ( 1 Γ p 2 p 1 ( α ) 2 2 p p 1 a 4 1 p 1 κ 4 ) .
Combining the above two cases, we have proved that S 2 is bounded in P. Then, we can choose R 2 > r 2 and
R 2 > Γ p 2 p 1 ( α ) 2 2 p p 1 c 2 1 p 1 κ 4 2 κ 3 ( 1 Γ p 2 p 1 ( α ) 2 2 p p 1 a 4 1 p 1 κ 4 ) , 1 < p 2 , κ 3 p 2 κ 2 p 2 κ 1 1 p c 2 κ 4 2 1 κ 3 p 2 a 4 κ 4 1 e μ ( t ) ϕ p 1 ( t ) d t t 1 p 1 , p 2 ,
such that
u λ A u , for u B R 2 P , λ [ 0 , 1 ] .
Then, from Lemma 8, we have
i ( A , B R 2 P , P ) = 1 .
Thus, from (29) and (31), we have
i ( A , ( B R 2 B ¯ r 2 ) P , P ) = i ( A , B R 2 P , P ) i ( A , B r 2 P , P ) = 1 ,
and hence A has at least one fixed point in ( B R 2 B ¯ r 2 ) P , i.e., (1) has at least one positive solution. This completes the proof.
In what follows, we consider the uniqueness of positive solutions for (1) with the boundary conditions D β u ( 1 ) = D β u ( e ) = 0 , u ( 1 ) = u ( 1 ) = u ( e ) = 0 . This problem is equivalent to the Hammerstein type integral equation
u ( t ) = 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) f ( τ , u ( τ ) ) d τ τ d s s ,
where G β ( t , s ) = G 1 β ( t , s ) for t , s [ 1 , e ] . Note that here we still use the operator A as in (16).
Lemma 11.
Let w 0 ( t ) = 1 e G β ( t , s ) d s s for t [ 1 , e ] . Then, for all nonnegative functions w C [ 1 , e ] ( 0 ) , there exist two positive a w , b w ( a w b w ) such that
a w w 0 ( t ) 1 e G β ( t , s ) w ( s ) d s s b w w 0 ( t ) , f o r t [ 1 , e ] .
Proof. 
We first calculate w 0 . From (14), we have
1 e G β ( t , s ) d s s = 1 Γ ( β ) 1 t ( log t ) β 1 ( 1 log s ) β 1 ( log t log s ) β 1 d s s + 1 Γ ( β ) t e ( log t ) β 1 ( 1 log s ) β 1 d s s = 1 Γ ( β ) 1 e ( log t ) β 1 ( 1 log s ) β 1 d s s 1 Γ ( β ) 1 t ( log t log s ) β 1 d s s = ( log t ) β 1 ( 1 log t ) β Γ ( β ) .
Using (17) and (18), we have
1 e Γ ( β ) ϕ ( t ) η ( s ) w ( s ) d s s 1 e G β ( t , s ) w ( s ) d s s 1 e ( β 1 ) ϕ ( t ) w ( s ) d s s .
Therefore, let a w = β Γ ( β ) 1 e η ( s ) w ( s ) d s s , and b w = β ( β 1 ) 1 e w ( s ) d s s ; then, we have that (33) holds. This completes the proof. □
Theorem 3.
Suppose that (H1), (H6)–(H7) hold. Then, (1) has a unique positive solution.
Proof. 
Note that (H7) implies that A is an increasing operator, and 0 isn’t a fixed point for A. Next, we shall prove that A has a subsolution and a supersolution. Let
ξ ( t ) = 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) f ( τ , ρ ( τ ) ) d τ τ d s s ,
where
ρ ( t ) = 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) d τ τ d s s , for t [ 1 , e ] .
From Lemma 11, there exist a ρ > 0 , b ρ > 0 such that
a ρ ρ ( t ) ξ ( t ) b ρ ρ ( t ) , for t [ 1 , e ] .
Take ξ 1 ( t ) = δ 1 ξ ( t ) , ξ 2 ( t ) = δ 2 ξ ( t ) , where 0 < δ 1 < min 1 b ρ , a ρ k 1 k , δ 2 > max 1 a ρ , b ρ k 1 k . Then, we have
( A ξ 1 ) ( t ) = 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) f ( τ , ξ 1 ( τ ) ) d τ τ d s s = 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) f ( τ , δ 1 ξ ( τ ) ) d τ τ d s s = 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) f τ , δ 1 ξ ( τ ) ρ ( τ ) ρ ( τ ) d τ τ d s s 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) δ 1 ξ ( τ ) ρ ( τ ) k ( p 1 ) f τ , ρ ( τ ) d τ τ d s s 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) δ 1 a ρ k ( p 1 ) f τ , ρ ( τ ) d τ τ d s s = δ 1 a ρ k 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) f τ , ρ ( τ ) d τ τ d s s δ 1 ξ ( t ) ,
and
A ξ 1 ξ 1 , i . e . , ξ 1 is a subsolution of A .
In addition, we have
( A ξ 2 ) ( t ) = 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) f ( τ , ξ 2 ( τ ) ) d τ τ d s s = 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) δ 2 p 1 δ 2 1 p f ( τ , ξ 2 ( τ ) ) d τ τ d s s 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) δ 2 p 1 1 δ 2 b ρ k ( p 1 ) f ( τ , ξ 2 ( τ ) ) d τ τ d s s 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) δ 2 p 1 ρ ( τ ) δ 2 ξ ( τ ) k ( p 1 ) f ( τ , ξ 2 ( τ ) ) d τ τ d s s 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) δ 2 p 1 f τ , ρ ( τ ) δ 2 ξ ( τ ) ξ 2 ( τ ) d τ τ d s s = δ 2 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) f ( τ , ρ ( τ ) ) d τ τ d s s ,
and
A ξ 2 ξ 2 , i . e . , ξ 2 is a supersolution of A .
As a result, from Lemma 9, A has the smallest fixed point u * and the largest fixed point u * in [ ξ 1 , ξ 2 ] , respectively. Moreover, u * = lim n A n ξ 1 and u * = lim n A n ξ 2 .
Next, we claim that u * ( t ) = u * ( t ) , for t [ 1 , e ] . We only prove that u * ( t ) u * ( t ) . Note that they are fixed points for A, so
u * ( t ) = 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) f ( τ , u * ( τ ) ) d τ τ d s s , u * ( t ) = 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) f ( τ , u * ( τ ) ) d τ τ d s s .
Then, from Lemma 11, there exists b i a i ( i = 1 , 2 ) such that
a 1 w 0 u * b 1 w 0 , a 2 w 0 u * b 2 w 0 .
Hence, u * a 1 b 2 u * . Let μ 0 : = sup { μ > 0 : u * μ u * } . Then, μ 0 > 0 , and u * μ 0 u * . Next, we claim that μ 0 1 . If it is not true, then μ 0 ( 0 , 1 ) . Using (H6), (H7), we have
u * ( t ) = 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) f ( τ , u * ( τ ) ) d τ τ d s s 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) f ( τ , μ 0 u * ( τ ) ) d τ τ d s s 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) μ 0 k ( p 1 ) f ( τ , u * ( τ ) ) d τ τ d s s = μ 0 k 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) f ( τ , u * ( τ ) ) d τ τ d s s .
Let
g ( t ) = φ q 1 e G α ( s , τ ) f ( τ , μ 0 u * ( τ ) ) d τ τ μ 0 k φ q 1 e G α ( s , τ ) f ( τ , u * ( τ ) ) d τ τ .
Then, from (H6) and Lemma 11, we have
a 3 w 0 ( t ) 1 e G β ( t , s ) g ( s ) d s s b 3 w 0 ( t ) .
Consequently,
u * ( t ) 1 e G β ( t , s ) g ( s ) d s s + μ 0 k 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) f ( τ , u * ( τ ) ) d τ τ d s s a 3 b 2 u * ( t ) + μ 0 k u * ( t ) a 3 b 2 + μ 0 u * ( t ) .
This contradicts the definition of μ 0 , and u * ( t ) μ 0 u * ( t ) u * ( t ) . Therefore, A has a unique positive fixed point in [ ξ 1 , ξ 2 ] , and (1) has also a unique positive solution in [ ξ 1 , ξ 2 ] . This completes the proof. □
Theorem 4.
Suppose all the assumptions in Theorem 3 hold. Let u ˜ is a unique positive solution in [ ξ 1 , ξ 2 ] . Then, for any u 0 [ ξ 1 , ξ 2 ] with f ( t , u 0 ( t ) ) ¬ 0 , the sequence
u n ( t ) = 1 e G β ( t , s ) φ q 1 e G α ( s , τ ) f ( τ , u n 1 ( τ ) ) d τ τ d s s , n = 1 , 2 , . . . ,
uniformly converges to u ˜ ( t ) , for t [ 1 , e ] .
Proof. 
From Theorem 3, we have u ˜ = lim n A n ξ 1 = lim n A n ξ 2 . Note that A is increasing, so, if u 0 [ ξ 1 , ξ 2 ] , we have
A n ξ 1 A n u 0 A n ξ 2 , n N + .
This implies that A n u 0 u ˜ as n . From the definition of A, we have u n ( t ) = ( A u n 1 ) ( t ) = A ( A u n 2 ) ( t ) = ( A 2 u n 2 ) ( t ) = = ( A n u 0 ) ( t ) , and thus u n ( t ) u ˜ ( t ) uniformly on t [ 1 , e ] . This completes the proof. □

4. Conclusions

In this paper we investigate the existence and uniqueness of positive solutions for the Hadamard fractional p-Laplacian three-point boundary value problem (1). We first establish some relations from the corresponding problem without the p-Laplacian operator, and use some ( p 1 ) -superlinearly and ( p 1 ) -sublinearly conditions for the nonlinearity to obtain positive solutions to problem (1). After, using an increasing operator fixed-point theorem, we obtain the unique solution to problem (1), and establish uniform converged sequences for this solution.

Author Contributions

All authors contributed equally to the manuscript.

Funding

This work is supported by the Talent Project of Chongqing Normal University (Grant No. 02030307-0040), the National Natural Science Foundation of China (Grant No. 11601048), the Natural Science Foundation of Chongqing (Grant No. cstc2016jcyjA0181), and the Natural Science Foundation of Chongqing Normal University (Grant No. 16XYY24).

Conflicts of Interest

The authors declare that they have no competing interests.

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MDPI and ACS Style

Jiang, J.; O’Regan, D.; Xu, J.; Cui, Y. Positive Solutions for a Hadamard Fractional p-Laplacian Three-Point Boundary Value Problem. Mathematics 2019, 7, 439. https://0-doi-org.brum.beds.ac.uk/10.3390/math7050439

AMA Style

Jiang J, O’Regan D, Xu J, Cui Y. Positive Solutions for a Hadamard Fractional p-Laplacian Three-Point Boundary Value Problem. Mathematics. 2019; 7(5):439. https://0-doi-org.brum.beds.ac.uk/10.3390/math7050439

Chicago/Turabian Style

Jiang, Jiqiang, Donal O’Regan, Jiafa Xu, and Yujun Cui. 2019. "Positive Solutions for a Hadamard Fractional p-Laplacian Three-Point Boundary Value Problem" Mathematics 7, no. 5: 439. https://0-doi-org.brum.beds.ac.uk/10.3390/math7050439

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