Research article

Rational interpolative contractions with applications in extended b-metric spaces

  • Received: 03 February 2024 Revised: 01 April 2024 Accepted: 10 April 2024 Published: 18 April 2024
  • MSC : 45E99, 47H10, 54H25, 55M20

  • In this manuscript, utilizing interpolative contractions with fractional forms, some unique fixed-point results were studied in the context of extended b-metric spaces. For the validity of the presented results some examples are given. In the last section an existence theorem is provided to study the existence of a solution for the Fredholm integral equation.

    Citation: Muhammad Sarwar, Muhammad Fawad, Muhammad Rashid, Zoran D. Mitrović, Qian-Qian Zhang, Nabil Mlaiki. Rational interpolative contractions with applications in extended b-metric spaces[J]. AIMS Mathematics, 2024, 9(6): 14043-14061. doi: 10.3934/math.2024683

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  • In this manuscript, utilizing interpolative contractions with fractional forms, some unique fixed-point results were studied in the context of extended b-metric spaces. For the validity of the presented results some examples are given. In the last section an existence theorem is provided to study the existence of a solution for the Fredholm integral equation.



    The concept of distance was axiomatically formulated in the beginning of the 19th century with the introduction of metric spaces, by Frechet and Haussdorff. Since then, many authors have developed this concept, with several results available in the literature. For the generalization of this concept, the axioms of the metric space have been relaxed in several ways (see[1]), among which the notion of a b-metric space takes great importance. Bakhtin [2] (and, independently, Czerwik [3]) presented the idea of b-metric spaces and showed different results based on the existence of fixed points. For the sake of understanding, we present here the definition of a b-metric, also called a quasi-metric (see [4]).

    Definition 1.1. (Czerwik [3]) Consider Q to be a non-empty set and b: Q×Q[0,+) to be a self-map fulfilling the below prerequisites:

    (1) b(s,p)=0 s=p;

    (2) b(s,p)=b(p,s) for all s,pQ;

    (3) b(s,u)q[b(s,p)+b(p,u)] for all s,p,uQ, where q1.

    The function b: Q×Q[0,+) is called a b-metric, while the pair (Q,b) is known as a b-metric space.

    Example 1.1. [4] The space Mp[0, 1] (where p(0,1)) of all real functions k(s), s[0,1] such that

    10|k(s)|pds<+

    together with the functional

    b(k,u)=(10|k(s)u(s)|pds)1p,for eachk,uMp[0,1]

    is a b-metric space. Here, q=21p1.

    Example 1.2. [5] Let

    Q={tk:1kJ}

    for some JN and a2. Define a function b: Q×Q[0,+) by

    b(tk,tl)={0,if k=l;a,if |kl|=1;2,if |kl|=2;1,otherwise.

    Accordingly, we obtain

    b(ti,tj)a2[b(ti,tk)+b(tk,tj)]

    for all i,j,k{1,2,,J}. The pair (Q,b) forms a b-metric space for a>2. We can observe that the standard triangular inequality does not hold in this case.

    The b-metric space shares many topological properties with traditional metric spaces but does not require continuity. Recently, Kamran et al. [6] presented a new generalization of metric spaces and proved some important fixed-point results in the newly defined space. Further more, Alqahtani et al. [7] studied common fixed point results on extended b-metric space.

    Definition 1.2. [6] Consider Q to be a non-empty set and ϑ: Q×Q[1,+). A function bϑ: Q×Q[0,+) is said to be an extended b-metric if for all s,t,uQ the given axioms are satisfied

    (1) bϑ(s,t)=0 implies s=t;

    (2) bϑ(s,t)=bϑ(t,s);

    (3) bϑ(s,u)ϑ(s,u)[bϑ(s,t)+bϑ(t,u)].

    The pair (Q,bϑ) is known as extended b-metric space.

    Remark 1.1. [5] Suppose ϑ(s,t)=a, for a1, then it is obvious that the b-metric and extended b-metric spaces (bMS) will coincide. Note that either the b-metric or the extended b-metric need to be continuous like metric spaces.

    Example 1.3. [5] Suppose p(0,1),q>1 and Q=lp(R)lq(R) equipped with the metric

    b(s,v)={bp(s,v),if s,vlp(R);bq(s,v),if s,vlq(R);0,otherwise.

    Where

    lr(R)={s={sn}R:+n=1|sn|r<+}

    for r=p,q, and

    br(s,v)=(+n=1|snvn|r)1/r

    for r=p,q, we can observe that (Q,bϑ) forms an extended bMS with

    ϑ(s,v)={21/p,if s,vlp(R);21/q,if s,vlq(R);1,otherwise.

    Example 1.4. [6] Let G={1,2,3}, ϑ: G×G[1,+) and bϑ: G×G[0,+) as ϑ(s,t)=1+s+t and

    bϑ(1,1)=bϑ(2,2)=bϑ(3,3)=0  and  bϑ(1,2)=bϑ(2,1)=80,
    bϑ(1,3)=bϑ(3,1)=1000,  and  bϑ(2,3)=bϑ(3,2)=600.

    Example 1.5. [7] Let G=[0,1],ϑ: G×G[1,+) and bϑ: G×G[0,+) be defined by

    ϑ(s,e)=1+s+es+e,   bϑ(s,e)=1se,   s,e(0,1], se;
    bϑ(s,e)=0,    s,e[0,1] s=e;
    bϑ(s,0)=bϑ(0,s)=1s,   s(0,1].

    Now we are going to discuss some basic notions like convergence, completeness, and Cauchy sequence in extended bMS that are defined as:

    Definition 1.3. [6] Suppose (Q, bϑ) be an extended b-metric space.

    (1) A sequence {sj}jK in Q will converge to tQ, if for every ζ>0 there exists K=K(ζ)K such that bϑ(sj,s)<ζ for all jK. In this case, we write

    limj+sj=s.

    (2) A sequence {sj}jK in Q is known as Cauchy sequence if for every ζ>0 exists K=K(ζ)K such that bϑ(sj,sm)<ζ, for all m,jK.

    Definition 1.4. [5] Suppose every Cauchy sequence in Q is convergent, then the extended-bMS (Q,bϑ) is said to be complete.

    Definition 1.5. [5] Let (Q,bϑ) be an extended-bMS and : QQ be a self-map. For toQ, the orbit of at to is the set

    O(to,)={to,to,2to,}.

    The function is known as orbitally continuous at a given point eQ if

    limj+jto=eimpliesjto=e.

    Besides that, suppose every Cauchy sequence {jto} in Q is convergent, then the extended-bMS (Q,bϑ) is called -orbitally complete.

    Definition 1.6. [8] Suppose (R,bϑ) be an extended b-metric. The mapping : RR is known as m-continuous, where m=1,2,, if

    limn+mtn=e,

    whenever tn is a sequence in R such that

    limn+m1tn=e.

    Remark 1.2. [1] It is notable that every continuous function is orbitally continuous in Q and every complete extended-bMS is -orbitally complete for any : QQ, but the converse is not necessarily true.

    Besides that, it is obvious that 1-continuity results in 2-continuity, which in turn will result in 3-continuity, and so on; but the converse of this is not true. This might be clearer from this example: consider the self-mapping : QQ, where Q=[0,+), defined by

    Ts={5,if s[0,5],1,if s(5,+),

    we can clearly see that is discontinuous (at s=5), while it is 2-continuous because T2s=5.

    Definition 1.7. [4] A self-mapping ¥: [0,+)[0,+) is said to be a comparison function if it is increasing and ¥n(s)0 as n+ for every s[0,+), where ¥n is the nth iterate of ¥.

    Lemma 1.1. [4] Suppose ¥: [0,+)[0,+) is a comparison function, then

    (1) ¥ is continuous at 0;

    (2) every iterate ¥k of ¥,k1 is also a comparison function;

    (3) ¥(s)<s for all s>0.

    Definition 1.8. [4] Suppose t1 be a real number. A self-mapping ¥: [0,+)[0,+) is said to be a (b)-comparison function if it is increasing and if there exist koN,a[0,1) and a convergent non-negative series +k=1wk such that

    tk+1¥k+1(s)atk¥k(s)+wk

    for kko and any s0.

    The set of all (b)-comparison functions is denoted by Θ. The (b)-comparison function is said to be a (c)-comparison function if we take t=1. It is easy to show that every (c)-comparison function is a (b)-comparison function, but the converse is not true. Another important property of (b)-comparison functions is presented by Berinde [4].

    Lemma 1.2. [4] Suppose Ξ: [0,+)[0,+) be a (b)-comparison function. Then:

    (1) The series t=0htΞt(s) converges for any s[0,+);

    (2) The function bs: [0,+)[0,+) defined as

    bs=+t=0htΞt(s)

    is increasing and is continuous at s=0.

    Remark 1.3. [5] Each (b)-comparison function Ξ satisfies Ξ(s)<s and

    limn+Ξn(t)=0

    for each s>0.

    Definition 1.9. [9] Let α: Q×Q[0,+) be a mapping and Q. A self-mapping : QQ is called α-orbital admissible if for all aQ, we have

    α(a,(a))1 implies α((a),2(a))1.

    Besides, the α-orbital admissible function is said to be triangular α-orbital admissible if

    (O) α(a,t)1 and α(a,(t))1 implies α(a,(t))1, for all a,tQ.

    Besides that, we say that the extended-bMS (Q,bϑ) is α-regular if for any sequence tn in Q such that

    limntn=tandα(tn,tn+1)1,

    we have α(tn,t)1 (for more details and examples, see [9]). Popescu [9] redefined the concept of α-admissible mapping and triangular α-admissible mapping. Qawagneha et al. [10] investigated common fixed points for pairs of triangular α -admissible mappings. The idea of interpolative contractions was very recently introduced by [11], and the well-known Kannan-type contractions were revisited in the context of interpolation. Subsequently, most famous contractions (Rus [4], Ćirić [12], Reich [13], Hardy and Rogers [14], Kannan [15], Bianchini and Grandolf [16]) have been revisited in this newly introduced context-(see [11,17,18]). Following this trend and using the idea of fractional interpolative contraction, Fulga [1] established some fixed-point results in the framework of bMS. Additionally Debnath et al. studied interpolative Hardy-Rogers and Reich-Rus-Ćirić-type contractions in b-metric and rectangular bMS [19].

    Non-linear integral equations have emerged in various fields of science and engineering, offering powerful tools for modeling physical phenomena and solving problems in diverse areas such as physics, engineering, and economics. Various researchers have studied these equations using different approaches, some of which can be found in [20,21,22].

    Motivated by the above contributions using fractional interpolative contractions some fixed-point results are studied in the setting of extended-bMS. The work here presented generalizes some well-known results from the existing literature. For the authenticity of the present work a key theorems is used to establish the existence of solutions for the Fredholm integral equations. The results obtained can be extended to investigate the existence of solutions for other integral equations (see[20,21,23]).

    We initiate with the following definition of contractive mapping to prove the main results.

    Definition 2.1. Let (Q,bϑ) be an extended-bMS. A mapping : QQ is known as Al-admissible interpolative contraction (l=1,2) if ψΘ and Ω: Q×Q[0,+) such that

    12bϑ(s,s)bϑ(s,a) implies Ω(s,a)bϑ(s,a)ψ(Al(s,a)), (2.1)

    where pj0, j=1,2,3,4,5, are such that 5j=1pj=1 and

    A1(s,a)=[bϑ(s,a)]p1[bϑ(s,s)]p2[bϑ(a,a)]p3[bϑ(a,a)(1+bϑ(s,s))1+bϑ(s,a)]p4[bϑ(s,a)+bϑ(a,s)2ϑ(s,a)]p5, (2.2)

    and

    A2(s,a)={[bϑ(s,a)]p1[bϑ(s,s)]p2[bϑ(a,a)]p3[bϑ(s,s)bϑ(a,a)+bϑ(s,a)bϑ(a,s)max{bϑ(a,a),bϑ(a,s)}]p4[bϑ(s,s)bϑ(s,a)+bϑ(a,a)bϑ(a,s)max{bϑ(s,a),bϑ(a,s)}]p5,if max{bϑ(s,a),bϑ(a,s)}0;0,otherwise, (2.3)

    for any s,aQFix(Q),(Fix(Q)={sQ|s=s}).

    Theorem 2.1. Let (Q,bϑ) be an extended-bMS and be an A1-admissible interpolative contraction, assume that a sequence {qj}jN,qj>1, for all jN, such that ϑ(aj,am)<qj for all m>j, and also satisfies:

    i) There exists aoQ such that α(ao,ao)1;

    ii) is α-orbital admissible;

    iii1) is orbitally continuous; or

    iii2) is m-continuous for m1.

    Then, possesses a fixed point ϖQ and the sequence {mao} converges to ϖ.

    Proof. Suppose aoQ and the sequence {aj} be defined as aj=jao, jN. Suppose there exists kN such that

    ak=ak+1=ak,

    then, we have that ak is a fixed point of and the proof is complete. Therefore, we suppose that ajaj+1 for any jN. Using assumption (ii), we obtain that is α-orbital admissible, so consider that we have

    α(ao,a1)=α(ao,ao)1α(a1,a2)=α(ao,(ao))1α(aj1,aj)1.

    On the other hand, we have that

    12bϑ(aj1,aj1)=12bϑ(aj1,aj)bϑ(aj1,aj).

    We mention in the beginning that is an A1-admissible interpolative contraction, so from (2.1) we get

    bϑ(aj1,aj)α(aj1,aj)bϑ(aj1,aj)ψ(A1(aj1,aj))=ψ([bϑ(aj1,aj)]p1[bϑ(aj1,aj1)]p2[bϑ(aj,aj)]p3[bϑ(aj,aj)(1+bϑ(aj1,aj1))1+bϑ(aj1,aj)]p4[bϑ(aj1,aj)+bϑ(aj,aj1)2ϑ(aj1,aj)]p5)=ψ([bϑ(aj1,aj)](p1+p2)[bϑ(aj,aj+1)](p3+p4)[ϑ(aj1,aj+1)[bϑ(aj1,aj)+bϑ(aj,aj+1)]2ϑ(aj1,aj+1)]p5)=ψ([bϑ(aj1,aj)](p1+p2).[bϑ(aj,aj+1)](p3+p4)[bϑ(aj1,aj)+bϑ(aj,aj+1)2]P5).

    So,

    bϑ(aj,aj+1)=ψ([bϑ(aj1,aj)](p1+p2)[bϑ(aj,aj+1)](p3+p4)[bϑ(aj1,aj)+bϑ(aj,aj+1)2]P5). (2.4)

    Therefore,

    bϑ(aj,aj+1)<[bϑ(aj1,aj)](p1+p2)[bϑ(aj,aj+1)]p3+p4[bϑ(aj1,aj)+bϑ(aj,aj+1)2]p5,

    i.e.,

    [bϑ(aj,aj+1)](1p3p4)<[bϑ(aj1,aj)](p1+p2)[bϑ(aj1,aj)+bϑ(aj,aj+1)2]p5.

    If exists moN such that

    bϑ(amo1,amo)bϑ(amo,amo+1),

    then the above inequality becomes

    bϑ(amo,amo+1)<[bϑ(amo1,amo)](p1+p2).[bϑ(amo,amo+1)](p5+p3+p4),

    i.e.,

    [bϑ(amo,amo+1)](p1+p2)<[bϑ(amo1,amo)](p1+p2),

    so,

    bϑ(amo,amo+1)<bϑ(amo1,amo),

    but it is a contradiction, so for any jN,

    bϑ(aj,aj+1)<bϑ(aj1,aj).

    Furthermore, returning to inequality (2.4), we have

    bϑ(aj,aj+1)ψ(bϑ(aj1,aj))ψj(bϑ(ao,a1)). (2.5)

    Let rN and j<m, then by (2.5) together with the condition (iii) of extended-bMS, we obtain

    bϑ(aj,am)ϑ(aj,am)[bϑ(aj,aj+1)+bϑ(aj+1,am)]ϑ(aj,am)[bϑ(aj,aj+1)]+ϑ(aj,am)[ϑ(aj+1,am)[bϑ(aj+1,aj+2)+bϑ(aj+2,am)]]ϑ(aj,am)[bϑ(aj,aj+1)]+ϑ(aj,am)ϑ(aj+,am)bϑ(aj+1,aj+2)++ϑ(aj,am)ϑ(aj+1,am)ϑ(aj+2,am)ϑ(am1,am)bϑ(ao,a1)ϑ(aj,am)ψj(bϑ(ao,a1))+ϑ(aj,am)ϑ(aj+1,am)ψj+1(bϑ(ao,a1))++[ϑ(aj,am)ϑ(am1,am)]ψm1(bϑ(ao,a1))ϑ(a1,am)ϑ(a2,am)ϑ(am1,am)ψj(bϑ(ao,a1))+ϑ(a1,am)ϑ(a2,am)ϑ(am1,am)ψj+1(bϑ(ao,a1))++ϑ(a1,am)ϑ(a2,am)ϑ(am1,am)ψm1(bϑ(ao,a1)).

    Let

    Sj=je=1ψe(bϑ(ao,a1))jk=1ϑ(ak,am),Sm1=m1e=1ψe(bϑ(ao,a1)),

    we deduce

    bϑ(aj,am)Sm1Sj1 for all m>j.

    Consider the series

    j=1ψj(bϑ(ao,a1))je=1ϑ(ae,am).

    Let

    q=max{q1,q2,,qj},

    we have

    uj=ψj(bϑ(ao,a1))kj=1ϑ(aj,am)ψj(bϑ(ao,a1))qj=vj.

    From Lemma 1.2, we have that k=0ψk(bϑ(ao,a1))qk converges. For the convergence of series using comparison criteria, we get that

    j=1ψj(bϑ(ao,a1))je=1ϑ(ae,am)

    converges, and hence

    limj,mbϑ(aj,am)=0.

    As a result, we say that {aj}jN is a Cauchy sequence in a -orbitally complete extended-bMS. Hence, there exists a point ϖQ, such that

    limjjao=ϖ.

    We can declare that ϖ is a fixed point of the self-mapping under of any hypothesis, (iii1) or (iii2). Indeed,

    ϖ=limjaj=limjaj1.

    Moreover,

    limjmaj=ϖ (2.6)

    for every m1.

    If is m-continuous, then

    limjmaj=ϖ,

    and by (2.6), it follows that ϖ=ϖ. Suppose is considered to be orbitally continuous on Q, then

    ϖ=limjaj=limjaj1=limj(j1ao)=ϖ.

    Therefore, ϖFix(Q).

    Theorem 2.2. Let (Q,bϑ) be an extended bMS. Suppose there exists a sequence {qj},qj>1, for all jN such that ϑ(aj,am)<qj, for all m>j, and is A2-admissible interpolative contraction, and also satisfies:

    i) There exists aoQ such that α(ao,ao)1;

    ii) is α-orbital admissible;

    iii1) is orbitally continuous; or

    iii2) is m-continuous for m1.

    Then has a fixed point ϖQ.

    Proof. From the proof of the above theorem, for aoQ, we construct the sequence {aj}, where

    aj=aj1=jao

    for any jN. Since aj1aj for any jN, keeping in mind that is assumed to be A2-admissible interpolative contraction, we have

    12bϑ(aj1,aj1)=12bϑ(aj1,aj)bϑ(aj1,aj),α(aj1,aj)bϑ(aj1,aj)ψ(A2(aj1,aj)),

    where

    A2=[bϑ(aj1,aj)]p1[bϑ(aj1,aj1)]p2[bϑ(aj,aj)]p3[bϑ(aj1,aj1)bϑ(aj,aj)+bϑ(aj1,aj)bϑ(aj,aj1)max{bϑ(aj,aj),bϑ(aj,aj1)}]p4[bϑ(aj1,aj1)bϑ(aj1,aj)+bϑ(aj,aj)bϑ(aj,aj1)max{bϑ(aj1,aj),bϑ(aj,aj1)}]p5=[bϑ(aj1,aj)]p1[bϑ(aj1,aj)]p2[bϑ(aj,aj+1)]p3[bϑ(aj1,aj)bϑ(aj,aj+1)+bϑ(aj1,aj)bϑ(aj,aj)max{bϑ(aj,aj+1),bϑ(aj,aj)}]p4[bϑ(aj1,aj)b(aj1,aj+1)+bϑ(aj,aj+1)bϑ(aj,aj)max{bϑ(aj1,aj+1),bϑ(aj,aj)}]p5=[bϑ(aj1,aj)](p1+p2+p5+p4)[bϑ(aj,aj+1)]p3.

    Since, by assumption, it follows that α(aj1,aj)1 for all jN, we have

    bϑ(aj,aj+1)α(aj1,aj)bϑ(aj1,aj)ψ(A2(aj1,aj))=ψ([bϑ(aj1,aj)](p1+p2+p4+p5)[bϑ(aj,aj+1)]p3)<[bϑ(aj1,aj)](p1+p2+p4+p5)[bϑ(aj,aj+1)]p3.

    Therefore,

    [bϑ(aj,aj+1)](1p3)<[bϑ(aj1,aj)](p1+p2+p4+p5),

    i.e.,

    bϑ(aj,aj+1)<bϑ(aj1,aj), for any jN.

    Furthermore, keeping in mind ψ2, we obtain

    bϑ(aj,aj+1)<ψ(bϑ(aj1,aj))<ψ2(bϑ(aj2,aj1))<<ψj(bϑ(ao,a1)),

    and using the same method as in the proof of Theorem 2.1, we can see that the sequence {aj} is Cauchy. Furthermore, since (Q,bϑ) is considered to be -orbitally complete, we can find a point ϖQ such that

    limjjao=ϖ.

    Consider that is m-continuous, we have

    ϖ=limjmaj=limjaj+m=ϖ,

    and suppose that is orbitally continuous, we obtain

    ϖ=limj(jao)=limjaj=limjaj+1=ϖ,

    it means that ϖ is a fixed point of .

    The following corollaries are observed from the above results.

    Corollary 2.1. Suppose (Q,bϑ) be a complete extended b-metric space. Suppose that there exists a sequence {pj}jN, pj>1 for all jN such that ϑ(sj,sm)<qj for all m>j and : QQ be a mapping such that

    α(s,v)bϑ(s,v)ψ(Al(s,v)).

    For any s,vQFix(Q), where Al,l=1,2 is defined by (2.2) and (2.3), and ψΘ. Then, has a fixed point ϖQ provided that:

    i) There exists uoQ such that α(uo,uo)1;

    ii) is α-orbital admissible;

    iii1) is orbitally continuous; or

    iii2) is m-continuous for m1.

    Corollary 2.2. Suppose (Q,bϑ) be a complete extended b-metric space. Suppose that there exists a sequence {pj}jN, pj>1, for all jN such that ϑ(sj,sm)<pj, for all m>j and : QQ be a mapping such that

    1/2bϑ(s,s)bϑ(s,v)impliesbϑ(s,v)ψ(Al(s,v)).

    For any s,vQFix(Q), where Al,l=1,2, are defined by (2.2) and (2.3), and ψΘ. Then, has a fixed point ϖQ, provided that either is orbitally continuous or is m-continuous for m1.

    Proof. Plug α(s,v)=1 in Theorems 2.1 and 2.2, respectively.

    By replacing the continuity of the function with the continuity of bϑ, we will have the following result.

    Theorem 2.3. Suppose (Q,bϑ) be a complete, α-regular extended-bMS, where bϑ is continuous, and : QQ is such that

    12ϑ(a,v)bϑ(a,a)bϑ(a,v)impliesα(a,v)bϑ(a,v)ψ(Al(a,v)),

    where ψΘ and Al, for l=1,2 are given by (2.2) and (2.3). Consider that:

    (1) There exists aoQ such that α(ao,ao)1;

    (2) is α-orbital admissible.

    Then, contains a fixed point ϖQ, and the sequence {mao} converges to this point ϖ.

    Proof. As we know from the proof of Theorem 2.1, the sequence {aj} where

    aj=aj1=jao

    converges to a point ϖQ, and this point ϖ is claimed to be a fixed point of the mapping . For this reason, we can declare that

    12ϑ(a,v)bϑ(aj,aj)bϑ(aj,ϖ) (2.7)

    or

    12ϑ(a,v)bϑ(aj,(aj))bϑ(aj,ϖ). (2.8)

    Indeed, supposing on contrary

    12ϑ(a,v)bϑ(aj,aj)>bϑ(aj,ϖ)

    and

    12ϑ(a,v)bϑ(aj,(aj))>bϑ(aj,ϖ),

    we get that

    bϑ(aj,aj+1)=bϑ(aj,aj)ϑ(a,v)[bϑ(aj,ϖ)+bϑ(ϖ,aj)]<ϑ(a,v)[12ϑ(a,v)bϑ(aj,aj)+12ϑ(a,v)bϑ(aj,(aj))]=12[bϑ(aj,aj+1)+bϑ(aj+1,aj+2)]bϑ(aj,aj+1),
    bϑ(aj,aj+1)bϑ(aj+1,aj+2)bϑ(aj,aj+1)<bϑ(aj,aj+1),

    which leads to contradiction and then (2.7) and (2.8) holds. Keeping the regularity condition of the space (Q,bϑ) in mind, we have that α(aj,ϖ)1 for any jN.

    Case 1. When l=1, if (2.7) holds, we get

    bϑ(aj+1,ϖ)α(aj,ϖ)bϑ(aj,ϖ)ψ(A1(aj,ϖ))A1(aj,ϖ)=[bϑ(aj,ϖ)]p1[bϑ(aj,ϖ)]p2[bϑ(ϖ,ϖ)]p3[bϑ(ϖ,ϖ)(1+bϑ(aj,aj+1))1+bϑ(aj,ϖ)]p4[bϑ(aj,ϖ)+bϑ(ϖ,aj+1)2ϑ(aj,ϖ)]p5,

    we can distinguish the following two situations:

    (1) p1+p2>0, letting j+ above, we obtain bϑ(ϖ,ϖ)=0, thus ϖ=ϖ.

    (2) p1=p2=0, when j above, and keeping in mind the continuity of extended-bMS we obtain

    bϑ(ϖ,ϖ)<[bϑ(ϖ,ϖ)](p3+p4+p5)=bϑ(ϖ,ϖ),

    which is a contradiction. So, we have ϖ=ϖ, i.e., ϖ is a fixed point of the mapping .

    Case 2. When l=2. If (2.7) holds, we obtain

    bϑ(aj+1,ϖ)α(am,ϖ)bϑ(aj,ϖ)ψ(A2(aj,ϖ))<A2(aj,ϖ)=[bϑ(aj,ϖ)]p1[bϑ(aj,aj+1)]p2[bϑ(ϖ,ϖ)]p3[bϑ(ϖ,ϖ)bϑ(aj,aj+1)+bϑ(ϖ,aj+1)bϑ(aj,ϖ)max{bϑ(aj,aj+1),bϑ(aj+1,ϖ)}]p4[bϑ(ϖ,ϖ)bϑ(ϖ,aj+1)+bϑ(aj,aj+1)bϑ(aj,ϖ)max{bϑ(ϖ,aj+1),bϑ(aj+1,ϖ)}]p5,

    if (2.8) holds,

    bϑ(aj+2,ϖ)α(aj+1,ϖ)bϑ(2aj,ϖ)ψ(A2(aj,ϖ))<A2(aj,ϖ)=[bϑ(aj+1,ϖ)]p1[bϑ(aj+1,aj+2)]p2[bϑ(ϖ,ϖ)]p3[bϑ(ϖ,ϖ)bϑ(aj+1,aj+2)+bϑ(ϖ,aj+2)bϑ(aj+1,ϖ)max{bϑ(aj+1,aj+2),bϑ(aj+2,ϖ)}]p4[bϑ(ϖ,ϖ)bϑ(ϖ,aj+2)+bϑ(aj+1,aj+2)bϑ(aj+1,ϖ)max{bϑ(ϖ,aj+2),bϑ(aj+2,ϖ)}]p5,

    we can distinguish the following two situations:

    (1) p1+p2+p4+p5>0, letting j above, we obtain bϑ(ϖ,ϖ)=0, thus ϖ=ϖ.

    (2) p1=p2=p4=p5=0, in this case, when j above, we get

    bϑ(ϖ,ϖ)<[bϑ(ϖ,ϖ)]p3=bϑ(ϖ,ϖ),

    which is a contradiction.

    So, we get ϖ=ϖ, i.e., ϖ is a fixed point of the mapping .

    This result possesses the below corollaries.

    Corollary 2.3. Let (Q,bϑ) be a complete extended bMS. Suppose {pj}jN be a sequence, pj>1 for all jN such that ϑ(sj,sm)<pj for all m>j and : QQ be a mapping such that k[0,1) such that

    1/2bϑ(s,s)bϑ(s,v)impliesbϑ(s,v)kAl(s,v),

    for any s,vQFie(Q) where Al,l=1,2 are defined by (2.2) and (2.3). Then, contains a fixed point ϖQ, provided that either is orbitally continuous or is m-continuous for m1.

    Proof. Plug ψ(t)=kt in the above corollary.

    Corollary 2.4. Suppose (Q,bϑ) be a complete extended-bMS such that bϑ is continuous. Suppose there exist a sequence {pj}jN,pj>1 for all jN such that ϑ(sj,sm)<pj for all m>j, and : QQ be a self-mapping. Then has a fixed point provided that

    12ϑ(s,v)bϑ(s,s)bϑ(s,v)impliesbϑ(s,v)ψ(Al(s,v)),

    where ψϝ and Al,l=1,2 are given by (2.2) and (2.3).

    Proof. Put α(s,v)=1 in Theorem 2.3.

    Corollary 2.5. Consider (Q,bϑ) be a complete extended-bMS such that bϑ is continuous. Suppose that exists {pj}jN,pj>1 for all jN such that ϑ(sj,sm)<pj for all m>j and : QQ, self-mapping. Then will have a fixed point in Q provided that there exist k[0,1) such that

    12ϑ(s,v)bϑ(s,s)bϑ(s,v)impliesbϑ(s,v)kAl(s,v),

    where Al,l=1,2 are given by (2.2) and (2.3).

    Proof. Substituted ψ(t)=kt in the above corollary.

    Now, we are going to present some examples of the above results.

    Example 2.1. Let Q=[0,+) and bϑ: Q×Q[0,+) be an extended-bMS defined as

    bϑ(s,v)={s+v,if sv for all s,vQ;0,if s=v;

    and ϑ: Q×Q[1,+) be defined as ϑ(s,v)=1+s+v for all s,vQ. Let the mapping : QQ be defined by

    (s)={15,if s[0,1);s+14,if s[1,2];ss2+9+In(s2+1)s2+7,if s(2,+);

    and a function α:Q×Q[0,+), where

    α(s,v)={s+v+1,if s,v[0,1);5,if s=0v=2;s4+v3,if s=14,v{3,9};0,otherwise.

    Let also the comparison function ψ: [0,)[0,), ψ(s)=s/3, and we choose p1=p5=1/5, p2=p4=1/10, and p3=2/5. Therefore, we can clearly see that conditions (i) and (ii) are verified, and since 2(s)=1/5 is continuous, condition (iv) is also satisfied.

    Case (1). For s,v[0,1], we have bϑ(s,v)=0, so inequality (2.1) holds.

    Case (2). For s=0 and v=2, we have 12bϑ(0,1/2)=1/42=bϑ(0,2) and bϑ(s,v)=0. Thus, the inequality (2.1) holds.

    Case(3). For s=1/4 and v=3, we have

    1/2bϑ(1/4,1/4)=0.253.25=bϑ(1/4,3)  α(1/4,3)bϑ(1/4,T3)=0.441716<0.8207=A1(1/4,3),

    hence (2.1) holds.

    Case(4). For s=1/4 and v=9, we have

    1/2bϑ(1/4,1/4)=0.2253.25=bϑ(1/4,9)   α(1/4,9)bϑ(1/4,9)=0.8513<2.0433=A1(1/4,9).

    All other cases are true because α(s,v)=0. Hence, the mapping is an A1-admissible interpolative contraction. So, as all the conditions of Theorem 2.1 are verified, we obtained that there exists a fixed point of the mapping , that is u=1/5.

    Example 2.2. Let Q={1,2,3,5} and the extended-bMS defined bϑ: Q×QR+ as bϑ(s,v)=|sv|4 with ϑ(s,v)=1+x+y and : QQ such that (1)=(5)=1  and  (2)=(3)=2. Taking α: Q×QR+,α(s,v)=3 for all s,vQ, and ψ(t)=t/2. The constants here are all equal, i.e., pi=1/5   i={1,2,3,4,5}, we have

    12ϑ(3,5)bϑ(3,3)=1/18<16=bϑ(3,5),

    which implies

    α(3,5)bϑ(3,5)=3<8.2=ψ(A2(3,5)).

    Therefore, all the requirements of Theorem 2.3 are satisfied and it is clear that has (at least) a fixed point.

    In this segment, we apply one of the observed results to study the existence of a solution for the Fredholm integral equation. Suppose Q=C([a,b],R) be the space of all continuous real-valued functions defined on [a, b]. Note that the space Q is complete by considering the extended-bMS

    bϑ(s(e),v(e))=supe[a,b]|s(e)v(e)|2

    with

    ϑ(s,v)=|s(e)|+|v(e)|+2,

    where ϑ(s,v): Q×Q[1,+) and ψΘ be the b-comparison function defined as ψ(e)=e/2. Consider the Fredholm integral equation as:

    s(e)=f(e)+baM(e,i,s(i))di for all i,e[a,b]. (3.1)

    Define a mapping : QQ, as

    (s(e))=f(e)+baM(e,i,s(i))di,i,e[a,b].

    Theorem 3.1. Consider that the following conditions hold:

    (1) Suppose M: [p,q]×[p,q]×RR and g: [p,q]R be continuous.

    (2) is Al-admissible interpolative contraction, Al,l=1,2 is defined in (2.2) and (2.3), respectively.

    (3)

    supe[p,q]|M(e,i,s(i))M(e,i,v(e))|Al(s(e),v(e))2(qp)

    for each e,i[p,q] and s,vQ.

    Then, the integral Eq (3.1) has a solution.

    Proof. Suppose (Q,bϑ) be a complete extended-bMS and α(s,v)=1. Then as

    12ϑ(s(e),v(e))bϑ(s(e),(s(e)))bϑ(s(e),s(e))=supe[p,q]|s(e)s(e)|2=supe[p,q]|f(e)+qpM(e,i,s(i))dif(e)qpM(e,i,s(i))di|2supe[p,q]|f(e)+qpM(e,i,s(i))dif(e)qpM(e,i,v(i))di|2=bϑ(s(e),v(e)),

    we have

    α(s(e),v(e))bϑ(s(e),v(e))=bϑ(s(e),v(e))=supe[p,q]|s(e)v(e)|2=supe[p,q]|f(e)+qpM(e,i,s(i))dif(e)qpM(e,i,v(i))di|2=supe[p,q]|qp(M(e,i,s(i))M(e,i,v(i)))di|2(qpsupe[p,q]|M(e,i,s(i))M(e,i,v(i))|di)2(qpAl(s(e),v(e))2(qp)di)2=Al(s(e),v(e))2=ψ(Al(s(e),v(e))).

    All the conditions of Theorem 2.3 are fulfilled. Therefore, the integral Eq (3.1) has a solution.

    Many physical problems can be described by various Fredholm integral equations. There are several methods available in the literature for the establishment of solutions to these equations. One powerful method is the fixed-point method. Therefore, in the current work, some new fractional interpolative contractions were introduced. With the help of these fractional interpolative contractions, some fixed-point results were studied in extended bMS. For the validity of the presented results, certain examples were given. Lastly, as a practical application, an existence theorem for the solution of the Fredholm integral equation was provided. This work generalizes some well-known results from the existing literature. In the future, one can explore the established work for multi-valued mapping and investigating the existence of solutions for integral inclusions.

    The authors declare they have not used artificial intelligence (AI) tools in the creation of this article.

    Authors are thankful to Prince Sultan University for the support of this work through TAS research lab.

    This work is funded by Natural Science Basic Research Plan in Shaanxi Province of China (No. 2022JQ-040).

    The authors declare no conflicts of interest.



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