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Research article

On a boundary value problem for fractional Hahn integro-difference equations with four-point fractional integral boundary conditions

  • Received: 01 August 2021 Accepted: 07 October 2021 Published: 14 October 2021
  • MSC : 39A10, 39A13, 39A70

  • In this paper, we study a boundary value problem consisting of Hahn integro-difference equation supplemented with four-point fractional Hahn integral boundary conditions. The novelty of this problem lies in the fact that it contains two fractional Hahn difference operators and three fractional Hahn integrals with different quantum numbers and orders. Firstly, we convert the given nonlinear problem into a fixed point problem, by considering a linear variant of the problem at hand. Once the fixed point operator is available, we make use the classical Banach's and Schauder's fixed point theorems to establish existence and uniqueness results. An example is also constructed to illustrate the main results. Several properties of fractional Hahn integral that will be used in our study are also discussed.

    Citation: Varaporn Wattanakejorn, Sotiris K. Ntouyas, Thanin Sitthiwirattham. On a boundary value problem for fractional Hahn integro-difference equations with four-point fractional integral boundary conditions[J]. AIMS Mathematics, 2022, 7(1): 632-650. doi: 10.3934/math.2022040

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  • In this paper, we study a boundary value problem consisting of Hahn integro-difference equation supplemented with four-point fractional Hahn integral boundary conditions. The novelty of this problem lies in the fact that it contains two fractional Hahn difference operators and three fractional Hahn integrals with different quantum numbers and orders. Firstly, we convert the given nonlinear problem into a fixed point problem, by considering a linear variant of the problem at hand. Once the fixed point operator is available, we make use the classical Banach's and Schauder's fixed point theorems to establish existence and uniqueness results. An example is also constructed to illustrate the main results. Several properties of fractional Hahn integral that will be used in our study are also discussed.



    The topic of fractional differential equations has gained considerable attention and has evolved as an interesting field of research, mainly due to the fact that the tools of fractional calculus are found to be more practical and effective than the corresponding ones of classical calculus in the mathematical modeling real wold problems. In fact, fractional calculus has numerous applications in various disciplines of science and engineering such as mechanics, chemistry, biology, economics, electricity, control theory, signal and image processing, regular variation in thermodynamics, biophysics, aerodynamics, viscoelasticity and damping, etc. For the basic theory and applications of fractional calculus, as well as for some recent developments in the field we refer to [1][9] and the references cited therein.

    Many physical phenomena are described by equations involving non-differentiable functions, e.g., generic trajectories of quantum mechanics [10]. The substitution of the classical derivative by a difference operator, which allows to deal with sets of non-differentiable functions, give rise to the so-called quantum calculus. Many different types of quantum difference operators appeared in the literature, for example h-calculus, q-calculus, Hahn's calculus, forward quantum calculus and backward quantum calculus. These operators have applications in orthogonal polynomials, basic hypergeometric functions, combinatorics, the calculus of variations, particle physics, quantum mechanics and the theory of relativity (see [11][24] and the references therein for some applications and new results of the quantum calculus).

    Recently, many researchers have extensively studied calculus without limit that deals with a set of non-differentiable functions, the so-called quantum calculus. Many types of quantum difference operators are employed in several applications of mathematical areas such as the calculus of variations, particle physics, quantum mechanics and theory of relativity (see [12][24] and the references therein for some applications and new results of the quatum calculus).

    In this paper, we study the Hahn quantum calculus that is one type of quantum calculus. W. Hahn [25] introduced the Hahn difference operator Dq,ω in 1949 as follow:

    Dq,ωf(t)=f(qt+ω)f(t)t(q1)+ω,tω0:=ω1q.

    The Hahn difference operator is a combination of two well-known difference operators, the forward difference operator and the Jackson q-difference operator. Notice that

    Dq,ωf(t)=Δωf(t)whenever q=1,Dq,ωf(t)=Dqf(t)whenever ω=0,Dq,ωf(t)=f(t)whenever q=1,ω0.

    The Hahn difference operator has been employed to construct families of orthogonal polynomials and investigate some approximation problems (see [26][28] and the references therein).

    In 2009, K. A. Aldwoah [29,30] defined the right inverse of Dq,ω in the terms of both the Jackson q-integral containing the right inverse of Dq [31] and Nörlund sum contaning the right inverse of Δω [31].

    In 2010, A. B. Malinowska and D. F. M. Torres [32,33] introduced the Hahn quantum variational calculus. In 2013, A. B. Malinowska and N. Martins [34] studied the generalized transversality conditions for the Hahn quantum variational calculus. Later, A. E. Hamza and S. M. Ahmed [35,36] studied the theory of linear Hahn difference equations, and investigated the existence and uniqueness results for the initial value problems for Hahn difference equations by using the method of successive approximations. Moreover, they proved Gronwall's and Bernoulli's inequalities with respect to the Hahn difference operator and established the mean value theorems for this calculus. In 2016, A. E. Hamza and S. D. Makharesh [37] investigated the Leibniz's rule and Fubini's theorem associated with Hahn difference operator. In the same year, T. Sitthiwirattham [38] considered a nonlinear Hahn difference equation with nonlocal boundary value conditions. In 2017, U. Sriphanomwan et al. [39] considered a nonlocal boundary value problem for second-order nonlinear Hahn integro-difference equation with integral boundary condition.

    In 2010, J. ˇCermˊak and L. Nechvˊatal [40] proposed the fractional (q,h)-difference operator and the fractional (q,h)-integral for q>1. In 2011, ˇCermˊak et al. [41] studied discrete Mittag-Leffler functions in linear fractional difference equations for q>1, and M. R. S. Rahmat [42,43] studied the (q,h)-Laplace transform and some (q,h)-analogues of integral inequalities on discrete time scales for q>1. In 2016, F. Du et al. [44] presented the monotonicity and convexity for nabla fractional (q,h)-difference for q>0,q1. However, we realize that Hahn difference operator requires the condition 0<q<1. Therefore, to fill the gap, T. Brikshavana and T. Sitthiwirattham [45] have introduced the fractional Hahn difference operators for 0<q<1.

    In quantum calculus, there are apparently few research works related to boundary value problems of fractional Hahn difference equations (see [46][48]). Motivated by the above discussion, to fill the gap on contributions concerning boundary value problems of fractional Hahn difference equations, the goal of this paper is to enrich this new research area. So, in this paper, we introduce and study a four-point fractional Hahn integral boundary value problems for fractional Hahn integrodifference equation of the form

    Dαq,ωu(t)=F[t,u(t),Ψγr,ρu(t),Υνm,χu(t)],tITq,ω,u(ξ)=ϕ1(u)+λ1Iβ1p1,θ1g1(η1)u(η1),ξ,η1ITq,ω{ω0,T},ξ>η1,u(T)=ϕ2(u)+λ2Iβ2p2,θ2g2(η2)u(η2),η2ITq,ω{ω0,T}, (1.1)

    where ITq,ω:={qkT+ω[k]q:kN0}{ω0}; α(1,2],β1,β2,γ,ν(0,1],ω>0,p1,p2,q,r,m(0,1),p1=qa,p2=qb,r=qc,m=qd,a,b,c,dN, θ1=ω(1p11q),θ2=ω(1p21q),ρ=ω(1r1q),χ=ω(1m1q), λ1,λ2R+, FC(ITq,ω×R×R×R,R),g1,g2C(ITq,ω,R+) and given functions, ϕ1,ϕ2:C(ITq,ω,R)R are given functionals, and for φC(ITr,ρ×ITr,ρ,[0,)) and ψC(ITm,χ×ITm,χ,[0,)), we define

    Ψγr,ρu(t):=(Iγr,ρφu)(t)=1Γr(γ)tω0(tσr,ρ(s))γ1_r,ρφ(t,s)u(s)dr,ρs,Υνm,χu(t):=(Dνm,χψu)(t)=1Γm(ν)tω0(tσm,χ(s))ν1_m,χψ(t,s)u(s)dm,χs.

    We emphasize that our problem contains two fractional Hahn difference operators and three fractional Hahn integrals with different quantum numbers and orders. To the authors' best knowledge, this is the new development on the topic as the quantum number and order of the problems studied in the literature are the same.

    We aim to show the existence and uniqueness of a solution to the problem (1.1) by using the Banach fixed point theorem, and the existence of at least one solution by using the Schauder's fixed point theorem. In addition, an example is provided to illustrate our results in the last section.

    The rest of this paper is organized as follows: We present our existence and uniqueness result in Section 3, and our existence result in Section 4, while Section 2 contains some preliminary concepts related to our problem. An example is constructed to illustrate the main results in Section 5. Finally, Section 6 is a conclusion section.

    In this section, we briefly recall some definitions and lemmas used in this research work. In this work, we use the Banach space C=C(ITq,ω,R) of all function u with the norm defined as

    uC=u+Dνm,χu,

    where u=maxtITq,ω{|u(t)|} and Dνm,χu=maxtITm,χ{|Dνm,χu(t)|}.

    Let q(0,1), ω>0. We define the notations

    [n]q:=1qn1q=qn1++q+1and[n]q!:=nk=11qk1q,nR.

    The forward jump operator and the backward jump operator are defined as

    σkq,ω(t):=qkt+ω[k]q and ρkq,ω(t):=tω[k]qqk for kN.

    The q-analogue of the power function (ab)n_q and the q,ω-analogue of the power function (ab)n_q,ω with nN0:=[0,1,2,],a,bR are defined as

    (ab)0_q:=1,(ab)n_q:=n1k=0(abqk),(ab)0_q,ω:=1,(ab)n_q,ω:=n1k=0[a(bqk+ω[k]q)],

    respectively.

    In generally, if αR, we get

    (ab)α_q=aαn=01(ba)qn1(ba)qα+n,a0,
    (ab)α_q,ω=(aω0)αn=01(bω0aω0)qn1(bω0aω0)qα+n=((aω0)(bω0))α_q,aω0.

    Note that aα_q=aα, (aω0)α_q,ω=(aω0)α, and (0)α_q=(ω0)α_q,ω=0 for α>0. The q-gamma and q-beta functions are defined as

    Γq(x):=(1q)x1_q(1q)x1,xR{0,1,2,},Bq(x,s):=10tx1(1qt)s1_qdqt=Γq(x)Γq(s)Γq(x+s),

    respectively.

    Definition 2.1. For q(0,1), ω>0 and f defined on an interval IR which containing ω0:=ω1q, the Hahn difference of f is defined as

    Dq,ωf(t)=f(qt+ω)f(t)t(q1)+ωfortω0,

    and Dq,ωf(ω0)=f(ω0), provided that f is differentiable at ω0. We call Dq,ωf the q,ω-derivative of f, and say that f is q,ω-differentiable on I.

    The Hahn difference operator has the following properties:

    Lemma 2.1. [30] Let f,g:IR are q,ω-differentiable on I. Then we have:

    (1) Dq,ω[f(t)+g(t)]=Dq,ωf(t)+Dq,ωg(t).

    (2) Dq,ω[αf(t)]=αDq,ωf(t).

    (3) Dq,ω[f(t)g(t)]=f(t)Dq,ωg(t)+g(qt+ω)Dq,ωf(t).

    (4) Dq,ω[f(t)g(t)]=g(t)Dq,ωf(t)f(t)Dq,ωg(t)g(t)g(qt+ω).

    Definition 2.2. Let I be any closed interval of R that contains a,b and ω0. If f:IR is a given function, we define the q,ω-integral of f from a to b by

    baf(t)dq,ωt:=bω0f(t)dq,ωtaω0f(t)dq,ωt,

    where

    xω0f(t)dq,ωt:=[x(1q)ω]k=0qkf(xqk+ω[k]q),xI,

    and the series converges at x=a and x=b. We say f is q,ω-integrable on [a,b] and the sum to the right hand side of this equation is called the Jackson-Nörlund sum.

    Notice that the actual domain of function f is defined on [a,b]q,ωI.

    Next, we introduce the fundamental theorem of Hahn calculus.

    Lemma 2.2. [29] Let f:IR be continuous at ω0 and define

    F(x):=xω0f(t)dq,ωt,xI.

    Then, F is continuous at ω0. In addition, Dq,ω0F(x) exists for every xI and

    Dq,ωF(x)=f(x).

    Conversely,

    baDq,ωF(t)dq,ωt=F(b)F(a) for alla,bI.

    Lemma 2.3. [38] Let q(0,1), ω>0 and f:IR be continuous at ω0. Then

    tω0rω0x(s)dq,ωsdq,ωr=tω0tqs+ωx(s)dq,ωrdq,ωs.

    Lemma 2.4. [38] Let q(0,1) and ω>0. Then

    tω0dq,ωs=tω0andtω0[tσq,ω(s)]dq,ωs=(tω0)21+q.

    Now, we give the definitions of fractioanal Hahn integral and fractional Hahn difference of Riemann-Liouville type, as follows:

    Definition 2.3. For α,ω>0,q(0,1) and f:ITq,ωR, the fractional Hahn integral is defined by

    Iαq,ωf(t):=1Γq(α)tω0(tσq,ω(s))α1_q,ωf(s)dq,ωs=[t(1q)ω]Γq(α)n=0qn(tσn+1q,ω(t))α1_q,ωf(σnq,ω(t)),

    and (I0q,ωf)(t)=f(t).

    Definition 2.4. For α,ω>0,q(0,1) and f:ITq,ωR, the fractional Hahn difference of the Riemann-Liouville type of order α is defined by

    Dαq,ωf(t):=(DNq,ωINαq,ωf)(t)=1Γq(α)tω0(tσq,ω(s))α1_q,ωf(s)dq,ωs,

    and D0q,ωf(t)=f(t), where N1αN,NN.

    Lemma 2.5. [45] Letting α>0,q(0,1),ω>0 and f:ITq,ωR,

    Iαq,ωDαq,ωf(t)=f(t)+C1(tω0)α1++CN(tω0)αN,

    for some CiR,i=1,2,,N and N1<αN,NN.

    Next, we give some auxiliary lemmas to use in simplifying calculations.

    Lemma 2.6. [45] Let α,β>0,p,q(0,1) and ω>0,

    (i)tω0(tσq,ω(s))α1_q,ωdq,ωs=(tω0)α[α]q,(ii)tω0(tσq,ω(s))α1_q,ω(sω0)β_q,ωdq,ωs=(tω0)α+βBq(β+1,α).

    Lemma 2.7. Let α,β,ν>0,nN,q,χ(0,1),ω,m>0 and χ=ω(1m1q). Then,

    (i)tω0(tσq,ω(s))β1_q,ω(sω0)αndq,ωs=(tω0)α+βnBq(αn+1,β),(ii)tω0(tσq,ω(s))ν1_q,ω(sω0)αndq,ωs=(tω0)ανnBq(αn+1,ν),(iii)tω0xω0(tσm,χ(x))ν1_m,χ(xσq,ω(s))α1_q,ωdq,ωsdm,χx=(tω0)αν[α]qBm(α+1,ν).

    Proof. From the definition of q,ω-analogue of the power function and Definition 2.3, we obtain

    (i)tω0(tσq,ω(s))β1_q,ω(sω0)αndq,ωs=(tω0)β(1q)i=0qi(1qi+1)β1_q(qi(tω0))αn=(tω0)α+βn(1q)i=0qi(1qi+1)β1_qqi(αn)=(tω0)α+βnBq(αn+1,β).

    Similarly, we obtain (ii).

    (iii)tω0xω0(tσm,χ(x))ν1_m,χ(xσq,ω(s))α1_q,ωdq,ωsdm,χx=tω0(tσm,χ(x))ν1_m,χ[xω0(xσq,ω(s))α1_q,ωdq,ωs]dm,χx=1[α]qtω0(tσm,χ(x))ν1_m,χ(xω0)αdm,χx=(tω0)αν[β]qBm(α+1,ν).

    The following lemma, dealing with a linear variant of problem (1.1), plays an important role in the forthcoming analysis.

    Lemma 2.8. Let Ω0,ω>0,q(0,1),α(1,2], and for i=1,2, θi>0,βi(0,1], pi(0,1),pi=qmi,miN, θi=ω(1pi1q), λiR+; hC(ITq,ω,R),g1,g2C(ITq,ω,R+) are given functions, ϕ1,ϕ2:C(ITq,ω,R)R are given functionals. Then the problem

    Dαq,ωu(t)=h(t),tITq,ω,u(ξ)=ϕ1(u)+λ1Iβ1p1,θ1g1(η1)u(η1),ξ,η1ITq,ω{ω0,T},ξ>η1,u(T)=ϕ2(u)+λ2Iβ2p2,θ2g2(η2)u(η2),η2ITq,ω{ω0,T}, (2.1)

    has the unique solution

    u(t)=1Γq(α)tω0(tσq,ω(s))α1_q,ωh(s)dq,ωs+(tω0)α1Ω(BT,η2Oξ,η1[ϕ1,h]Bξ,η1OT,η2[ϕ2,h])(tω0)α2Ω(AT,η2Oξ,η1[ϕ1,h]Aξ,η1OT,η2[ϕ2,h]), (2.2)

    where the functionals Oξ,η1[ϕ1,h],OT,η2[ϕ2,h] are defined by

    Oξ,η1[ϕ1,h]:=ϕ1(u)1Γq(α)ξω0(ξσq,ω(s))α1_q,ωh(s)dq,ωs+λ1Γq(α)Γp1(β1)×η1ω0xω0(η1σp1,θ1(s))β11_p1,θ1(xσq,ω(s))α1_q,ωg1(x)h(s)dq,ωsdp1,θ1x, (2.3)
    OT,η2[ϕ2,h]:=ϕ2(u)1Γq(α)Tω0(Tσq,ω(s))α1_q,ωh(s)dq,ωs+λ2Γq(α)Γp2(β2)×η2ω0xω0(η2σp2,θ2(s))β21_p2,θ2(xσq,ω(s))α1_q,ωg2(x)h(s)dq,ωsdp2,θ2x, (2.4)

    and the constants Aξ,η1,AT,η2,Bξ,η1,BT,η2 and Ω are defined by

    Aξ,η1:=(ξω0)α1λ1Γp1(β1)η1ω0(η1σp1,θ1(s))β11_p1,θ1g1(s)(sω0)α1dp1,θ1s, (2.5)
    AT,η2:=(Tω0)α1λ2Γp2(β2)η2ω0(η2σp2,θ2(s))β21_p2,θ2g2(s)(sω0)α1dp2,θ2s, (2.6)
    Bξ,η1:=(ξω0)α2λ1Γp1(β1)η1ω0(η1σp1,θ1(s))β11_p1,θ1g1(s)(sω0)α2dp1,θ1s, (2.7)
    BT,η2:=(Tω0)α2λ2Γp2(β2)η2ω0(η2σp2,θ2(s))β21_p2,θ2g2(s)(sω0)α2dp2,θ2s, (2.8)
    Ω:=Aξ,η1BT,η2AT,η2Bξ,η1. (2.9)

    Proof. Taking fractional Hahn q,ω-integral of order α to (2.1), we obtain

    u(t)=C1(tω0)α1+C2(tω0)α2+1Γq(α)tω0(tσq,ω(s))α1_q,ωh(x)dq,ωs. (2.10)

    Next, we take fractional Hahn pi,θi-integral of order βi,i=1,2 to (2.10) to get

    Iβipi,θiu(t)=1Γpi(βi)tω0(tσpi,θi(s))βi1_pi,θi[C1(sω0)α1+C2(sω0)α2]dpi,θis+1Γq(α)Γpi(βi)tω0xω0(tσpi,θi(x))βi1_pi,θi(xσq,ω(s))α1_q,ωh(s)dq,ωsdpi,θix. (2.11)

    Substituting i=1 into (2.11) and employing the first condition of (2.1), we have

    Aξ,η1C1+Bξ,η1C2=Oξ,η1[ϕ1,h]. (2.12)

    Taking i=2 into (2.11) and employing the second condition of (2.1), we have

    AT,η2C1+BT,η2C2=OT,η2[ϕ2,h], (2.13)

    where Oξ,η1,[ϕ1,h],OT,η2[ϕ2,h],Aξ,η1,AT,η2,Bξ,η1,BT,η2 and Ω are defined as (2.3)–(2.9), respectively. The constants C1 and C2 are revealed from solving the system of equations (2.12) and (2.13) as

    C1=BT,η2Oξ,η1,[ϕ1,h]Bξ,η1OT,η2,[ϕ2,h]ΩandC2=Aξ,η1OT,η2,[ϕ2,h]AT,η2Oξ,η1,[ϕ1,h]Ω.

    Substituting the constants C1,C2 into (2.10), we obtain (2.2).

    On the other hand, it's easy to show that (2.2) is the solution of problem (2.1), by taking fractional Hahn q,ω-difference of order α to (2.2), we get (2.1).

    In this section, we show the existence and uniqueness result for problem (1.1). In view of Lemma 2.8 we define an operator A:CC as

    (Au)(t):=1Γq(α)tω0(tσq,ω(s))α1_q,ωF[s,u(s),Ψγr,ρu(s),Υνm,χu(s)]dq,ωs+(tω0)α1Ω(BT,η2Oξ,η1[ϕ1,Fu]Bξ,η1OT,η2[ϕ2,Fu])(tω0)α2Ω(AT,η2Oξ,η1[ϕ1,Fu]Aξ,η1OT,η2[ϕ2,Fu]), (3.1)

    where the functionals Oξ,η1[ϕ1,Fu],OT,η2[ϕ2,Fu] are defined by

    Oξ,η1[ϕ1,Fu]:=ϕ1(u)1Γq(α)ξω0(ξσq,ω(s))α1_q,ωF[s,u(s),Ψγr,ρu(s),Υνm,χu(s)]dq,ωs+λ1Γq(α)Γp1(β1)η1ω0xω0(η1σp1,θ1(s))β11_p1,θ1(xσq,ω(s))α1_q,ωg1(x)×F[s,u(s),Ψγr,ρu(s),Υνm,χu(s)]dq,ωsdp1,θ1x, (3.2)
    OT,η2[ϕ2,Fu]:=ϕ2(u)1Γq(α)Tω0(Tσq,ω(s))α1_q,ωF[s,u(s),Ψγr,ρu(s),Υνm,χu(s)]dq,ωs+λ2Γq(α)Γp2(β2)η2ω0xω0(η2σp2,θ2(s))β21_p2,θ2(xσq,ω(s))α1_q,ωg2(x)×F[s,u(s),Ψγr,ρu(s),Υνm,χu(s)]dq,ωsdp2,θ2x, (3.3)

    and the constants Aξ,η1,AT,η2,Bξ,η1,BT,η2 and Ω are defined by (2.5)–(2.9), respectively.

    Obviously the problem (1.1) has solutions if and only if the operator A has fixed points.

    Theorem 3.1. Assume that F:ITq,ω×R×R×RR is continuous, φ:ITr,ρ×ITr,ρ[0,), ψ:ITm,χ×ITm,χ[0,) are continuous with φ0=max{φ(t,s):(t,s)ITr,ρ×ITr,ρ} and ψ0=max{ψ(t,s):(t,s)ITm,χ×ITm,χ}. In addition, assume that the following conditions hold:

    (H1) There exist positive constants 1,2,3, such that for each tITq,ω and ui,viR,i=1,2,3,

    |F[t,u1,u2,u3]F[t,v1,v2,v3]|1|u1v1|+2|u2v2|+3|u3v3|.

    (H2) There exist positive constants τ1,τ2, such that for each u,vC,

    |ϕ1(u)ϕ1(v)|τ1uvC and |ϕ2(u)ϕ2(v)|τ2uvC.

    (H3) There exist positive constants gi,Gi,i=1,2, such that for each tITq,ω,

    gi<gi(t)<Gi.

    (H4)Ξ:=LX+τ1ΘT,η2+τ2Θξ,η1<1,

    where

    L:=1+2φ0(Tω0)γΓr(γ+1)+3ψ0(Tω0)νΓm(1ν), (3.4)
    X:=[(Tω0)αΓq(α+1)+(Tω0)ανΓm(αν+1)+Φξ,η1ΘT,η2+ΦT,η2Θξ,η1], (3.5)
    Φξ,η1:=1Γq(α+1)[(ξω0)α+λ1G1(η1ω0)α+β1Γp1(α+1)Γp1(α+β1+1)], (3.6)
    ΦT,η2:=1Γq(α+1)[(Tω0)α+λ2G2(η2ω0)α+β2Γp2(α+1)Γp2(α+β2+1)], (3.7)
    Θξ,η1:=Θξ,η1+¯Θξ,η1, (3.8)
    ΘT,η2:=ΘT,η2+¯ΘT,η2, (3.9)
    Θξ,η1:=1min|Ω|[(Tω0)α1max|Bξ,η1|+(Tω0)α2max|Aξ,η1|], (3.10)
    ¯Θξ,η1:=1min|Ω|[(Tω0)αν1Γm(α)Γm(αν)max|Bξ,η1|+(Tω0)αν2Γm(α1)Γm(αν1)max|Aξ,η1|], (3.11)
    ΘT,η2:=1min|Ω|[(Tω0)α1max|BT,η2|+(Tω0)α2max|AT,η2|], (3.12)
    ¯ΘT,η2:=1min|Ω|[(Tω0)αν1Γm(α)Γm(αν)max|BT,η2|+(Tω0)αν2Γm(α1)Γm(αν1)max|AT,η2|]. (3.13)

    Then problem (1.1) has a unique solution in ITq,ω.

    Proof. For each tITr,ρ, we have

    |Ψγr,ρu(t)Ψγr,ρv(t)|ϕ0Γr(γ)tω0(tσr,ρ(s))γ1_r,ρ|u(s)v(s)|dr,ρsϕ0Γr(γ)uvTω0(Tσr,ρ(s))γ1_r,ρdr,ρs=ϕ0(Tω0)γΓr(γ+1)uv.

    Similarly, for each tITm,χ, we obtain

    |Υνm,χu(t)Υνm,χv(t)|ψ0(Tω0)νΓm(1ν)uv.

    To show that F is contraction, we denote that

    F|uv|(t):=|F[t,u(t),Ψγr,ρu(t),Υνm,χu(t)]F[t,v(t),Ψγr,ρv(t),Υνm,χv(t)]|,

    for each tITq,ω and u,vC. We find that

    |Oξ,η1[ϕ1,Fu]Oξ,η1[ϕ1,Fv]||ϕ1(u)ϕ1(v)|+1Γq(α)ξω0(ξσq,ω(s))α1_q,ωF|uv|(s)dq,ωs+λ1Γq(α)Γp1(β1)×η1ω0xω0(η1σp1,θ1(s))β11_p1,θ1(xσq,ω(s))α1_q,ωg1(x)F|uv|(s)dq,ωsdp1,θ1xτ1uvC+(1|uv|+2|Ψγr,ρuΨγr,ρ|+3|Dνm,χuDνm,χv|)1Γq(α+1)×[(ξω0)α+λ1G1(η1ω0)α+β1Γp1(α+1)Γp1(α+β1+1)]τ1uvC+[1+2φ0(Tω0)γΓr(γ+1)+3ψ0(Tω0)νΓr(1ν)]uvΦξ,η1[τ1+LΦξ,η1]uvC. (3.14)

    Similarly, we get

    |OT,η2[ϕ2,Fu]OT,η2[ϕ2,Fv]|[τ2+LΦT,η2]uvC. (3.15)

    Next, we have

    |(Au)(t)(Av)(t)|1Γq(α)Tω0(Tσq,ω(s))α1_q,ωF|uv|(s)dq,ωs+(Tω0)α1|Ω|×+{|BT,η2||Oξ,η1[ϕ1,Fu]Oξ,η1[ϕ1,Fv]|+|Bξ,η1||OT,η2[ϕ2,Fu]OT,η2[ϕ2,Fv]|}+(Tω0)α2|Ω|{|AT,η2||Oξ,η1[ϕ1,Fu]Oξ,η1[ϕ1,Fv]|+|Aξ,η1|×|OT,η2[ϕ2,Fu]OT,η2[ϕ2,Fv]|}[L(Tω0)αΓq(α+1)+[τ1+LΦξ,η1]min|Ω|{max|BT,η2|(Tω0)α1+max|AT,η2|(Tω0)α2}+[τ2+LΦT,η2]min|Ω|{max|Bξ,η1|(Tω0)α1+max|Aξ,η1|(Tω0)α2}]uvC={L[(Tω0)αΓq(α+1)+Φξ,η1ΘT,η2+ΦT,η2Θξ,η1]+τ1ΘT,η2+τ2Θξ,η1}uvC. (3.16)

    Taking fractional Hahn m,χ-difference of order ν to (3.1), we obtain

    (Dνm,χAu)(t)=1Γq(α)Γm(ν)tω0xω0(tσm,χ(x))ν1_m,χ(xσq,ω(s))α1_q,ω×F[s,u(s),Ψγr,ρu(s),Υνm,χu(s)]dq,ωsdm,χx+1ΩΓm(ν)×(BT,η2Oξ,η1[ϕ1,Fu]Bξ,η1OT,η2[ϕ2,Fu])tω0(tσm,χ(s))ν1_m,χ(sω0)α1dm,χs1ΩΓm(ν)(AT,η2Oξ,η1[ϕ1,Fu]Aξ,η1OT,η2[ϕ2,Fu])×tω0(tσm,χ(s))ν1_m,χ(sω0)α2dm,χs. (3.17)

    By the same expression as above, we obtain

    |(Dm,χνAu)(t)(Dνm,χAv)(t)|<{L[(Tω0)ανΓm(α+1)Γm(αν+1)Γq(α+1)+Φξ,η1¯ΘT,η2+ΦT,η2¯Θξ,η1]+τ1¯ΘT,η2+τ2¯Θξ,η1}×uvC. (3.18)

    From (3.16) and (3.18), we get

    AuAvC[LX+τ1ΘT,η2+τ2Θξ,η1]uvC=ΞuvC.

    By (H_4) and Banach fixed point theorem, we get that {\mathcal{A}} is a contraction and hence {\mathcal{A}} has a fixed point. Consequently problem (1.1) has a unique solution of on I^T_{q, \omega} .

    In this section, we prove an existence result for the problem (1.1) via Schauder's fixed point theorem.

    Lemma 4.1. [49] (Schauder's fixed point theorem) Let (D, d) be a complete metric space, U be a closed convex subset of D , and T: D\rightarrow D be the map such that the set Tu:u\in U is relatively compact in D . Then the operator T has at least one fixed point u^*\in U : Tu^* = u^*.

    Theorem 4.1. Suppose that (H_1) , (H_3) and (H_4) hold. Then, problem (1.1) has at least one solution on I^T_{q, \omega} .

    Proof. The proof is organized into three steps as follows:

    Step I. {\mathcal{A}} maps bounded sets into bounded sets in B_R = \{u \in \mathcal{C}: \|u\|_{\mathcal{C}} \leq R\} . Let \; \max\limits_{t\in I^T_{q, \omega}}|F(t, 0, 0, 0)| = M, \; \sup\limits_{u\in {\mathcal{C}}} |\phi_i(u)| = N_i, \; i = 1, 2 and choose a constant

    \begin{equation} R\geq \frac{ M\mathcal{X}+ N_1\Theta^*_{T,\eta_2} +N_2 \Theta^*_{\xi,\eta_1} }{1-{\mathcal{L}}{\mathcal{X}}}. \end{equation} (4.1)

    Letting

    \big|\mathcal{F}(t,u,0)\big| = \bigg|F\big[t,u(t),\Psi_{r,\rho}^\gamma u(t),\Upsilon_{m,\chi}^\nu u(t) \big]-F\big[t,0,0,0\big]\bigg|+\big|F\big[t,0,0,0\big]\big|

    for each t\in I_{q, \omega}^T and u\in B_{R} , we obtain

    \begin{align} &\Big|{\mathcal{O}_{\xi,\eta_1}^*[\phi_1,F_u]} \Big|\\ \leq\; &N_1+ \frac{1}{\Gamma_q(\alpha)} \int_{\omega_0}^{\xi} \left(\xi-\sigma_{q,\omega}(s) \right)_{q,\omega}^{\underline{\alpha-1}}\,\big|\mathcal{F}(s,u,0)\big|\,d_{q,\omega}s\\ +&\frac{\lambda_1}{\Gamma_q(\alpha)\Gamma_{p_1}(\beta_1)}\int_{\omega_0}^{\eta_1}\int_{\omega_0}^{x}\left(\eta_1-\sigma_{p_1,\theta}(s) \right)_{p_1,\theta}^{\underline{\beta_1-1}} \left(x-\sigma_{q,\omega}(s) \right)_{q,\omega}^{\underline{\alpha-1}}g_1(x)\big|\mathcal{F}(s,u,0)\big|\,d_{q,\omega}s\,d_{p_1,\theta}x\\ \leq\; &N_1+ \Bigg( \left[ \ell_1+\ell_2\varphi_0\frac{(T-\omega_0)^{\gamma}}{\Gamma_r(\gamma+1)} +\ell_3\psi_0\frac{(T-\omega_0)^{-\nu}}{\Gamma_r(1-\nu)} \right]\|u\| +M\Bigg)\,\Phi_{\xi,\eta_1}\\ \leq\; &N_1+ \big( {\mathcal{L}}\|u\|_{\mathcal{C}}+M\big)\,\Phi_{\xi,\eta_1}. \end{align} (4.2)

    Similarly,

    \begin{align} \Big|{\mathcal{O}_{T,\eta_2}^*[\phi_2,F_u]} \Big| \leq N_2+ \big( {\mathcal{L}}\|u\|_{\mathcal{C}}+M\big)\,\Phi_{T,\eta_2}. \end{align} (4.3)

    Then, we have

    \begin{align} \big| ({\mathcal{A}}u)(t)\big| \leq\; &\big(\mathcal{L} \|u\|_{\mathcal{C}}+M\big)\left[ \frac{(T-\omega_0)^{\alpha}}{\Gamma_q(\alpha+1)} + \Phi_{\xi,\eta_1}\Theta_{T,\eta_2} +\Phi_{T,\eta_2}\Theta_{\xi,\eta_1} \right] + N_1\Theta_{T,\eta_2} +N_2\Theta_{\xi,\eta_1} \end{align} (4.4)

    and

    \begin{align} \big|\left( D^\gamma_{m,\chi}{\mathcal{A}}u\right) (t)\big| \leq\; &\big(\mathcal{L} \|u\|_{\mathcal{C}}+M\big)\left[ \frac{(T-\omega_0)^{\alpha-\nu}}{\Gamma_m(\alpha-\nu+1)} + \Phi_{\xi,\eta_1}\overline{\Theta}_{T,\eta_2} +\Phi_{T,\eta_2}\overline{\Theta}_{\xi,\eta_1}\right] \\ &+ N_1\overline{\Theta}_{T,\eta_2} +N_2\overline{\Theta}_{\xi,\eta_1}. \end{align} (4.5)

    From (4.4) and (4.5), we obtain \|{\mathcal{A}}u\|_{\mathcal{C}}\leq R . Hence {\mathcal{A}} is uniformly bounded.

    Step II. By the continuity of F , the operator {\mathcal{A}} is continuous on B_R .

    Step III. Next, we show that {\mathcal{A}} is equicontinuous on B_R . For any t_1, t_2\in I^T_{q, \omega} with t_1 < t_2 , we have

    \begin{align} \big| ({\mathcal{A}}u)&(t_2)- ({\mathcal{A}}u)(t_1) \big|\,\\ \leq\; &\frac{\|F\|}{\Gamma_q(\alpha+1)} \Big| (t_2-\omega_0)^\alpha -(t_1-\omega_0)^\alpha \Big|\\ +&\frac{ \Big| (t_2-\omega_0)^{\alpha-1} -(t_1-\omega_0)^{\alpha-1} \Big|}{|\Omega|} \Big\{ |\textbf{B}_{T,\eta_2}| \big|{\mathcal{O}_{\xi,\eta_1}^*[\phi_1,F_u]}\big| +|{\textbf{B}}_{\xi,\eta_1}|\big|{\mathcal{O}_{T,\eta_2}^*[\phi_2,F]}\big| \Big\}\\ +&\frac{\Big| (t_2-\omega_0)^{\alpha-2} -(t_1-\omega_0)^{\alpha-2} \Big|}{|\Omega|} \Big\{ |\textbf{A}_{T,\eta_2}|\big|{\mathcal{O}_{\xi,\eta_1}^*[\phi_1,F_u]}\big| +|{\textbf{A}}_{\xi,\eta_1}|\big|{\mathcal{O}_{T,\eta_2}^*[\phi_2,F]}\big| \Big\} \end{align} (4.6)

    and

    \begin{align} \big|(D_{m,\chi}&^\nu{\mathcal{F}}u)(t_1) -(D_{m,\chi}^\nu{\mathcal{F}}u)(t_2) \big|\\ \leq\,&\frac{\|F\|\Gamma_q(-\nu)}{\Gamma_m(-\nu)\Gamma_q(\alpha-\nu+1)}\Big|(t_2-\omega_0)^{\alpha-\nu} -(t_1-\omega_0)^{\alpha-\nu} \Big| \\ &+\frac{\Gamma_q(\alpha)\Gamma_q(-\nu)}{|\Omega|\Gamma_m(-\nu)\Gamma_q(\alpha-\nu)} \Big\{ |\textbf{B}_{T,\eta_2}| \big|{\mathcal{O}_{\xi,\eta_1}^*[\phi_1,F_u]}\big| +|{\textbf{B}}_{\xi,\eta_1}|\big|{\mathcal{O}_{T,\eta_2}^*[\phi_2,F]}\big| \Big\}\times\\ &\; \; \; \; \Big| (t_2-\omega_0)^{\alpha-\nu-1}-(t_1-\omega_0)^{\alpha-\nu-1} \Big| \\ &+\frac{\Gamma_q(\alpha-1)\Gamma_q(-\nu)}{|\Omega|\Gamma_m(-\nu)\Gamma_q(\alpha-\nu-1)} \Big\{ |\textbf{A}_{T,\eta_2}|\big|{\mathcal{O}_{\xi,\eta_1}^*[\phi_1,F_u]}\big| +|{\textbf{A}}_{\xi,\eta_1}|\big|{\mathcal{O}_{T,\eta_2}^*[\phi_2,F]}\big| \Big\} \times\\ & \; \; \; \; \Big| (t_2-\omega_0)^{\alpha-\nu-2}-(t_1-\omega_0)^{\alpha-\nu-2} \Big|. \end{align} (4.7)

    Clearly the right-hand side of (4.6) and (4.7) tend to be zero when |t_2-t_1|\rightarrow 0 . So {\mathcal{A}} is relatively compact on B_R .

    Hence the set {\mathcal{F}}(B_R) is an equicontinuous set. As a result of Steps I to III and the Arzelá-Ascoli theorem, we can conclude that \mathcal{A}:{\mathcal{C}}\rightarrow {\mathcal{C}} is completely continuous. By Schauder's fixed point theorem, we obtain that problem (1.1) has at least one solution.

    Consider the following fractional Hahn integro-difference equation

    \begin{eqnarray} D^{\frac{4}{3}}_{\frac{1}{2},\frac{2}{3}}u(t)& = &\frac{1}{\left( 100\pi^2+t^3\right)(1+|u(t)|)} \Bigg[ e^{-3t+1}\left( u^2+2|u|\right) + e^{-(\pi+\sin^2\pi t)}\left|\Psi_{\frac{1}{8},\frac{7}{6}}^{\frac{1}{2}}u(t) \right| \\ &&+ e^{-(2\pi+\cos^2\pi t)}\left|\Upsilon^{\frac{1}{4}}_{\frac{1}{4},1}u(t) \right| \Bigg],\; \; \; \; t\in I^{10}_{\frac{1}{2},\frac{2}{3}} \end{eqnarray} (5.1)

    with four-point fractional Hahn integral boundary condition

    \begin{eqnarray*} u\left(\frac{15}{8}\right) = 10e\, \mathcal{I}_{\frac{1}{16},\frac{5}{4}}^{\frac{1}{3}}u\left(2e+\sin \frac{699055}{524288}\right)^2 u\left( \frac{699055}{524288}\right) + \sum\limits_{i = 0}^{\infty}\frac{C_i|u(t_i)|}{1+|u(t_i)|},\; \; t_i \in \sigma_{\frac{1}{2}, \frac{2}{3}}^i(10),\nonumber\\ u\left(10\right) = \frac{1}{10\pi} \mathcal{I}_{\frac{1}{32},\frac{31}{24}}^{\frac{2}{3}}u\left(\pi+\cos \frac{65549}{49125}\right)^2 u\left( \frac{65549}{49125}\right) + \sum\limits_{i = 0}^{\infty}\frac{D_i|u(t_i)|}{1+|u(t_i)|},\; \; t_i \in \sigma_{\frac{1}{2}, \frac{2}{3}}^i(10),\nonumber \end{eqnarray*}

    where \; \varphi(t, s) = \frac{e^{-|t-s|}}{(t+20)^3}, \; \psi(t, s) = \frac{e^{-|t-s|}}{(t+30)^2} and \; C_i, D_i are given constants with \frac{1}{100t^3}\leq\sum_{i = 0}^{\infty}C_i\leq\frac{e}{100t^3} and \frac{1}{200t^2}\leq\sum_{i = 0}^{\infty}D_i\leq\frac{\pi}{200t^2} .

    Here \; \alpha = \frac{4}{3}, \; \beta_1 = \frac{1}{3}, \; \beta_2 = \frac{2}{3}, \; \gamma = \frac{1}{2}, \; \nu = \frac{1}{4}, \; q = \frac{1}{2}, \; p_1 = \frac{1}{16}, \; p_2 = \frac{1}{32}, \; r = \frac{1}{8}, \; m = \frac{1}{4}, \; \; \omega = \frac{2}{3}, \\ \theta_1 = \frac{5}{4}, \; \theta_1 = \frac{31}{24}, \; \rho = \frac{7}{6}, \; \chi = 1, \; \omega_0 = \frac{\omega}{1-q} = \frac{4}{3}, \; T = 10, \; \xi = \sigma_{\frac{1}{2}, \frac{2}{3}}^4(10) = \frac{15}{8}, \; \eta_1 = \sigma_{\frac{1}{16}, \frac{5}{4}}^5(10) = \frac{699055}{524288}, \\ \eta_2 = \sigma_{\frac{1}{32}, \frac{31}{24}}^3(10) = \frac{65549}{49125} , \; \lambda_1 = 10e, \; \lambda_2 = \frac{1}{10\pi}, \; \; \phi_1(u) = \sum_{i = 0}^{\infty}\frac{C_i|u(t_i)|}{1+|u(t_i)|}, \\ \phi_2 = \sum_{i = 0}^{\infty}\frac{D_i|u(t_i)|}{1+|u(t_i)|}, \; g_1(t) = \left(2e+\sin t\right)^2, \; g_2(t) = \left(\pi+\cos t\right)^2, \text{and} \\ F\left(t, u(t), \Psi^\gamma_{r, \rho}u(t), \Upsilon^\nu_{m, \chi}u(t)\right)\\ = \, \frac{1}{\left(100\pi^2+t^3\right)(1+|u(t)|)} \Big[ e^{-3t+1}\left(u^2+2|u|\right) + e^{-(\pi+\sin^2\pi t)} \left|\Psi_{\frac{1}{8}, \frac{7}{6}}^{\frac{1}{2}}u(t) \right| + e^{-(2\pi+\cos^2\pi t)}\left|\Upsilon^{\frac{1}{4}}_{\frac{1}{4}, 1}u(t) \right| \Big].

    For all \; t\in I^{10}_{\frac{1}{2}, \frac{2}{3}}\; and \; u, v\in {\mathbb{R}} , we have

    \begin{align*} &\left| F\left( t,u,\Psi^\gamma_{r,\rho}u,\Upsilon^\nu_{m,\chi}u\right)- F\left( t,v,\Psi^\gamma_{r,\rho}v,\Upsilon^\nu_{m,\chi}v\right)\right| \\ \leq\; & \frac{1}{e^3\left( \left( \frac{4}{3}\right)^{3} +100\pi^2\right) }|u-v| +\frac{1}{e^\pi\left( \left( \frac{4}{3}\right)^{3} +100\pi^2\right) }\left| \Psi^\gamma_{r,\rho}u-\Psi^\gamma_{r,\rho}v\right|\\ +&\frac{1}{e^{2\pi}\left( \left( \frac{4}{3}\right)^{3} +100\pi^2\right) } \left|D^\nu_{m,\chi}u-D^\nu_{m,\chi}v \right|. \end{align*}

    Thus, (H_1) holds with \; \ell_1 = 0.0000503, \; \ell_2 = 0.00004367\; and \; \ell_3 = 1.8876\times10^{-6} .

    For all \; u, v\in {\mathcal{C}} ,

    \begin{align*} |\phi_1(u)-\phi_1(v)|\, = \,&\frac{e}{100\left( \frac{4}{3}\right) ^3}\|u-v\|_{\mathcal{C}},\\ |\phi_2(u)-\phi_2(v)|\, = \,&\frac{\pi}{200\left( \frac{4}{3}\right) ^2}\|u-v\|_{\mathcal{C}}. \end{align*}

    So, (H_2) holds with \; \tau_1 = 0.011468\; and \; \tau_2 = 0.0066268.

    Moreover, (H_3) holds with g_1 = 19.6831, G_1 = 41.4294, g_2 = 4.5864 and G_2 = 17.1528 .

    We can find that

    |{\textbf{A}}_{\xi,\eta_1}|\leq1.27503,\; \; \; |{\textbf{A}}_{T,\eta_2}|\leq2.05422,\; \; \; |{\textbf{B}}_{\xi,\eta_1}|\leq61548.5314,\; \; \; |{\textbf{B}}_{T,\eta_2}|\leq0.08082 and \; \; |\Omega|\geq 60067.4763.

    Also, we can show that

    {\mathcal{L}}\, = \,0.0000503,\; \; \Phi_{\xi,\eta_1}\, = \,0.39607,\; \; \Phi_{T,\eta_2}\, = \,15.96844,\\ \Theta_{\xi,\eta_1}\, = \,2.10473,\; \; \overline{\Theta}_{\xi,\eta_1}\, = \,1.25309,\; \; \Theta_{T,\eta_2}\, = \,0.0000357,\; \; \overline{\Theta}_{T,\eta_2}\, = \,0.00001716,\\ \Theta^*_{\xi,\eta_1}\, = \,3.35782,\; \; \Theta^*_{T,\eta_2}\, = \,0.00005286,\; \; \text{and}\; \; \mathcal{X} = 79.7178.

    Hence, (H_4) holds with

    \Xi \approx 0.02626 < 1.

    Therefore, by Theorem 3.1 , problem (5.1) has a unique solution. Moreover, by Theorem 4.1 , this problem has at least one solution.

    In the present research we considered a boundary value problem for Hahn integro-difference equation subject to four-point fractional Hahn integral boundary conditions. Notice that the problem at hand contains two fractional Hahn difference operators and three fractional Hahn integrals with different quantum numbers and orders. We note that if we let q = r = m = p_1 = p_2 and \omega = \rho = \theta_1 = \theta_2 , our results reduce to the results obtained in [46][48]. After proving an auxiliary result concerning a linear variant of the considered problem, the problem at hand is transformed into a fixed point problem. Existence and uniqueness results are established via Banach's and Schauder's fixed point theorems. The main results are illustrated by a numerical example. Some properties of fractional Hahn integral needed in our study are also discussed. The results of the paper are new and enrich the subject of boundary value problems for Hahn integro-difference equations. In the future work, we may extend this work by considering new boundary value problems.

    This research was funded by the Science, Research and Innovation Promotion Fund under Basic Research Plan-Saun Dusit University.

    The authors declare no conflict of interest.



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