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,p∈Q;
(3) b(s,u)≤q[b(s,p)+b(p,u)] for all s,p,u∈Q, where q≥1.
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,u∈Mp[0,1] |
is a b-metric space. Here, q=21p−1.
Example 1.2. [5] Let
Q={tk:1≤k≤J} |
for some J∈N and a≥2. Define a function b: Q×Q→[0,+∞) by
b(tk,tl)={0,if k=l;a,if |k−l|=1;2,if |k−l|=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,u∈Q 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 a≥1, 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,v∈lp(R);bq(s,v),if s,v∈lq(R);0,otherwise. |
Where
lr(R)={s={sn}⊂R:+∞∑n=1|sn|r<+∞} |
for r=p,q, and
br(s,v)=(+∞∑n=1|sn−vn|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,v∈lp(R);21/q,if s,v∈lq(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], s≠e; |
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}j∈K in Q will converge to t∈Q, if for every ζ>0 there exists K=K(ζ)∈K such that bϑ(sj,s)<ζ for all j≥K. In this case, we write
limj→+∞sj=s. |
(2) A sequence {sj}j∈K 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,j≥K.
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 ℸ: Q→Q be a self-map. For to∈Q, the orbit of ℸ at to is the set
O(to,ℸ)={to,ℸto,ℸ2to,…}. |
The function ℸ is known as orbitally continuous at a given point e∈Q if
limj→+∞ℸjto=eimpliesℸℸjto=ℸe. |
Besides that, suppose every Cauchy sequence {ℸjto} in Q is convergent, then the extended-bMS (Q,bϑ) is called ℸ-orbitally complete.
Definition 1.6. [8] Suppose (R,bϑ) be an extended b-metric. The mapping ℸ: R→R is known as m-continuous, where m=1,2,…, if
limn→+∞ℸmtn=ℸe, |
whenever tn is a sequence in R such that
limn→+∞ℸm−1tn=e. |
Remark 1.2. [1] It is notable that every continuous function is orbitally continuous in Q and every complete extended-bMS is ℸ-orbitally complete for any ℸ: Q→Q, 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 ℸ: Q→Q, where Q=[0,+∞), defined by
Ts={5,if s∈[0,5],1,if s∈(5,+∞), |
we can clearly see that ℸ 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 ¥,k≥1 is also a comparison function;
(3) ¥(s)<s for all s>0.
Definition 1.8. [4] Suppose t≥1 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 ko∈N,a∈[0,1) and a convergent non-negative series ∑+∞k=1wk such that
tk+1¥k+1(s)≤atk¥k(s)+wk |
for k≥ko and any s≥0.
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 ℸ: Q→Q is called α-orbital admissible if for all a∈Q, we have
α(a,ℸ(a))≥1 implies α(ℸ(a),ℸ2(a))≥1. |
Besides, the α-orbital admissible function ℸ is said to be triangular α-orbital admissible if
(ℸO) α(a,t)≥1 and α(a,ℸ(t))≥1 implies α(a,ℸ(t))≥1, for all a,t∈Q. |
Besides that, we say that the extended-bMS (Q,bϑ) is α-regular if for any sequence tn in Q such that
limn→∞tn=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 ℸ: Q→Q is known as Alℸ-admissible interpolative contraction (l=1,2) if ∃ ψ∈Θ and Ω: Q×Q→[0,+∞) such that
12bϑ(s,ℸs)≤bϑ(s,a) implies Ω(s,a)bϑ(ℸs,ℸa)≤ψ(Alℸ(s,a)), | (2.1) |
where pj≥0, j=1,2,3,4,5, are such that ∑5j=1pj=1 and
A1ℸ(s,a)=[bϑ(s,a)]p1⋅[bϑ(s,ℸs)]p2⋅[bϑ(a,ℸa)]p3⋅[bϑ(a,ℸa)(1+bϑ(s,ℸs))1+bϑ(s,a)]p4⋅[bϑ(s,ℸa)+bϑ(a,ℸs)2ϑ(s,ℸa)]p5, | (2.2) |
and
A2ℸ(s,a)={[bϑ(s,a)]p1⋅[bϑ(s,ℸs)]p2⋅[bϑ(a,ℸa)]p3⋅[bϑ(s,ℸs)bϑ(a,ℸa)+bϑ(s,ℸa)bϑ(a,ℸs)max{bϑ(a,ℸa),bϑ(a,ℸs)}]p4⋅[bϑ(s,ℸs)bϑ(s,ℸa)+bϑ(a,ℸa)bϑ(a,ℸs)max{bϑ(s,ℸa),bϑ(a,ℸs)}]p5,if max{bϑ(s,ℸa),bϑ(a,ℸs)}≠0;0,otherwise, | (2.3) |
for any s,a∈Q∖Fixℸ(Q),(Fixℸ(Q)={s∈Q|ℸs=s}).
Theorem 2.1. Let (Q,bϑ) be an extended-bMS and ℸ be an A1ℸ-admissible interpolative contraction, assume that ∃ a sequence {qj}j∈N,qj>1, for all j∈N, such that ϑ(aj,am)<qj for all m>j, and ℸ also satisfies:
i) There exists ao∈Q such that α(ao,ℸao)≥1;
ii)ℸ is α-orbital admissible;
iii1)ℸ is orbitally continuous; or
iii2)ℸ is m-continuous for m≥1.
Then, ℸ possesses a fixed point ϖ∈Q and the sequence {ℸmao} converges to ϖ.
Proof. Suppose ao∈Q and the sequence {aj} be defined as aj=ℸjao, ∀ j∈N. Suppose there exists k∈N such that
ak=ak+1=ℸak, |
then, we have that ak is a fixed point of ℸ and the proof is complete. Therefore, we suppose that aj≠aj+1 for any j∈N. Using assumption (ii), we obtain that ℸ is α-orbital admissible, so consider that we have
α(ao,a1)=α(ao,ℸao)≥1⇒α(a1,a2)=α(ℸao,ℸ(ℸao))≥1⇒⋯⇒α(aj−1,aj)≥1. |
On the other hand, we have that
12bϑ(aj−1,ℸaj−1)=12bϑ(aj−1,aj)≤bϑ(aj−1,aj). |
We mention in the beginning that ℸ is an A1ℸ-admissible interpolative contraction, so from (2.1) we get
bϑ(ℸaj−1,ℸaj)≤α(aj−1,aj)bϑ(ℸaj−1,aj)≤ψ(A1ℸ(aj−1,aj))=ψ([bϑ(aj−1,aj)]p1⋅[bϑ(aj−1,ℸaj−1)]p2⋅[bϑ(aj,ℸaj)]p3⋅[bϑ(aj,ℸaj)(1+bϑ(aj−1,ℸaj1))1+bϑ(aj−1,aj)]p4⋅[bϑ(aj−1,ℸaj)+bϑ(aj,ℸaj−1)2ϑ(aj−1,ℸaj)]p5)=ψ([bϑ(aj−1,aj)](p1+p2)⋅[bϑ(aj,aj+1)](p3+p4)⋅[ϑ(aj−1,aj+1)[bϑ(aj−1,aj)+bϑ(aj,aj+1)]2ϑ(aj−1,aj+1)]p5)=ψ([bϑ(aj−1,aj)](p1+p2).[bϑ(aj,aj+1)](p3+p4)⋅[bϑ(aj−1,aj)+bϑ(aj,aj+1)2]P5). |
So,
bϑ(aj,aj+1)=ψ([bϑ(aj−1,aj)](p1+p2)⋅[bϑ(aj,aj+1)](p3+p4)⋅[bϑ(aj−1,aj)+bϑ(aj,aj+1)2]P5). | (2.4) |
Therefore,
bϑ(aj,aj+1)<[bϑ(aj−1,aj)](p1+p2)⋅[bϑ(aj,aj+1)]p3+p4⋅[bϑ(aj−1,aj)+bϑ(aj,aj+1)2]p5, |
i.e.,
[bϑ(aj,aj+1)](1−p3−p4)<[bϑ(aj−1,aj)](p1+p2)⋅[bϑ(aj−1,aj)+bϑ(aj,aj+1)2]p5. |
If exists mo∈N such that
bϑ(amo−1,amo)≤bϑ(amo,amo+1), |
then the above inequality becomes
bϑ(amo,amo+1)<[bϑ(amo−1,amo)](p1+p2).[bϑ(amo,amo+1)](p5+p3+p4), |
i.e.,
[bϑ(amo,amo+1)](p1+p2)<[bϑ(amo−1,amo)](p1+p2), |
so,
bϑ(amo,amo+1)<bϑ(amo−1,amo), |
but it is a contradiction, so for any j∈N,
bϑ(aj,aj+1)<bϑ(aj−1,aj). |
Furthermore, returning to inequality (2.4), we have
bϑ(aj,aj+1)≤ψ(bϑ(aj−1,aj))≤⋯≤ψj(bϑ(ao,a1)). | (2.5) |
Let r∈N 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(am−1,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(am−1,am)]ψm−1(bϑ(ao,a1))≤ϑ(a1,am)ϑ(a2,am)⋯ϑ(am−1,am)ψj(bϑ(ao,a1))+ϑ(a1,am)ϑ(a2,am)⋯ϑ(am−1,am)ψj+1(bϑ(ao,a1))+⋯+ϑ(a1,am)ϑ(a2,am)⋯ϑ(am−1,am)ψm−1(bϑ(ao,a1)). |
Let
Sj=j∑e=1ψe(bϑ(ao,a1))j∏k=1ϑ(ak,am),Sm1=m−1∑e=1ψe(bϑ(ao,a1)), |
we deduce
bϑ(aj,am)≤Sm−1−Sj−1 for all m>j. |
Consider the series
∞∑j=1ψj(bϑ(ao,a1))j∏e=1ϑ(ae,am). |
Let
q=max{q1,q2,…,qj}, |
we have
uj=ψj(bϑ(ao,a1))k∏j=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))j∏e=1ϑ(ae,am) |
converges, and hence
limj,m→∞bϑ(aj,am)=0. |
As a result, we say that {aj}j∈N is a Cauchy sequence in a ℸ-orbitally complete extended-bMS. Hence, there exists a point ϖ∈Q, such that
limj→∞ℸjao=ϖ. |
We can declare that ϖ is a fixed point of the self-mapping ℸ under of any hypothesis, (iii1) or (iii2). Indeed,
ϖ=limj→∞aj=limj→∞ℸaj−1. |
Moreover,
limj→∞ℸmaj=ϖ | (2.6) |
for every m≥1.
If ℸ is m-continuous, then
limj→∞ℸmaj=ℸϖ, |
and by (2.6), it follows that ℸϖ=ϖ. Suppose ℸ is considered to be orbitally continuous on Q, then
ϖ=limj→∞aj=limj→∞ℸaj−1=limj→∞ℸ(ℸj−1ao)=ℸϖ. |
Therefore, ϖ∈Fixℸ(Q).
Theorem 2.2. Let (Q,bϑ) be an extended bMS. Suppose there exists a sequence {qj},qj>1, for all j∈N such that ϑ(aj,am)<qj, for all m>j, and ℸ is A2ℸ-admissible interpolative contraction, and ℸ also satisfies:
i) There exists ao∈Q such that α(ao,ℸao)≥1;
ii)ℸ is α-orbital admissible;
iii1)ℸ is orbitally continuous; or
iii2)ℸ is m-continuous for m≥1.
Then ℸ has a fixed point ϖ∈Q.
Proof. From the proof of the above theorem, for ao∈Q, we construct the sequence {aj}, where
aj=ℸaj−1=ℸjao |
for any j∈N. Since aj−1≠aj for any j∈N, keeping in mind that ℸ is assumed to be A2ℸ-admissible interpolative contraction, we have
12bϑ(aj−1,ℸaj−1)=12bϑ(aj−1,aj)≤bϑ(aj−1,aj),α(aj−1,aj)bϑ(ℸaj−1,ℸaj)≤ψ(A2ℸ(aj−1,aj)), |
where
A2ℸ=[bϑ(aj−1,aj)]p1⋅[bϑ(aj−1,ℸaj−1)]p2⋅[bϑ(aj,ℸaj)]p3⋅[bϑ(aj−1,ℸaj−1)bϑ(aj,ℸaj)+bϑ(aj−1,ℸaj)bϑ(aj,ℸaj−1)max{bϑ(aj,ℸaj),bϑ(aj,ℸaj−1)}]p4⋅[bϑ(aj−1,ℸaj−1)bϑ(aj−1,ℸaj)+bϑ(aj,ℸaj)bϑ(aj,ℸaj−1)max{bϑ(aj−1,ℸaj),bϑ(aj,ℸaj−1)}]p5=[bϑ(aj−1,aj)]p1⋅[bϑ(aj−1,aj)]p2⋅[bϑ(aj,aj+1)]p3⋅[bϑ(aj−1,aj)bϑ(aj,aj+1)+bϑ(aj−1,aj)bϑ(aj,aj)max{bϑ(aj,aj+1),bϑ(aj,aj)}]p4⋅[bϑ(aj−1,aj)b(aj−1,aj+1)+bϑ(aj,aj+1)bϑ(aj,aj)max{bϑ(aj−1,aj+1),bϑ(aj,aj)}]p5=[bϑ(aj−1,aj)](p1+p2+p5+p4)⋅[bϑ(aj,aj+1)]p3. |
Since, by assumption, it follows that α(aj−1,aj)≥1 for all j∈N, we have
bϑ(aj,aj+1)≤α(aj−1,aj)bϑ(ℸaj−1,ℸaj)≤ψ(A2ℸ(aj−1,aj))=ψ([bϑ(aj−1,aj)](p1+p2+p4+p5)⋅[bϑ(aj,aj+1)]p3)<[bϑ(aj−1,aj)](p1+p2+p4+p5)⋅[bϑ(aj,aj+1)]p3. |
Therefore,
[bϑ(aj,aj+1)](1−p3)<[bϑ(aj−1,aj)](p1+p2+p4+p5), |
i.e.,
bϑ(aj,aj+1)<bϑ(aj−1,aj), for any j∈N. |
Furthermore, keeping in mind ψ2, we obtain
bϑ(aj,aj+1)<ψ(bϑ(aj−1,aj))<ψ2(bϑ(aj−2,aj−1))<⋯<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 ℸ-orbitally complete, we can find a point ϖ∈Q such that
limj→∞ℸjao=ϖ. |
Consider that ℸ is m-continuous, we have
ℸϖ=limj→∞ℸmaj=limj→∞aj+m=ϖ, |
and suppose that ℸ is orbitally continuous, we obtain
ℸϖ=limj→∞ℸ(ℸjao)=limj→∞ℸaj=limj→∞aj+1=ϖ, |
it means that ϖ is a fixed point of ℸ.
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}j∈N, pj>1 for all j∈N such that ϑ(sj,sm)<qj for all m>j and ℸ: Q→Q be a mapping such that
α(s,v)bϑ(ℸs,ℸv)≤ψ(Alℸ(s,v)). |
For any s,v∈Q∖Fix(Q), where Alℸ,l=1,2 is defined by (2.2) and (2.3), and ψ∈Θ. Then, ℸ has a fixed point ϖ∈Q provided that:
i) There exists uo∈Q such that α(uo,ℸuo)≥1;
ii)ℸ is α-orbital admissible;
iii1)ℸ is orbitally continuous; or
iii2)ℸ is m-continuous for m≥1.
Corollary 2.2. Suppose (Q,bϑ) be a complete extended b-metric space. Suppose that there exists a sequence {pj}j∈N, pj>1, for all j∈N such that ϑ(sj,sm)<pj, for all m>j and ℸ: Q→Q be a mapping such that
1/2bϑ(s,ℸs)≤bϑ(s,v)impliesbϑ(ℸs,ℸv)≤ψ(Alℸ(s,v)). |
For any s,v∈Q∖Fix(Q), where Alℸ,l=1,2, are defined by (2.2) and (2.3), and ψ∈Θ. Then, ℸ has a fixed point ϖ∈Q, provided that either ℸ is orbitally continuous or ℸ is m-continuous for m≥1.
Proof. Plug α(s,v)=1 in Theorems 2.1 and 2.2, respectively.
By replacing the continuity of the function ℸ 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 ℸ: Q→Q is such that
12ϑ(a,v)bϑ(a,ℸa)≤bϑ(a,v)impliesα(a,v)bϑ(ℶa,ℸv)≤ψ(Alℸ(a,v)), |
where ψ∈Θ and Alℸ, for l=1,2 are given by (2.2) and (2.3). Consider that:
(1) There exists ao∈Q such that α(ao,ℸao)≥1;
(2) ℸ is α-orbital admissible.
Then, ℸ contains a fixed point ϖ∈Q, and the sequence {ℸmao} converges to this point ϖ.
Proof. As we know from the proof of Theorem 2.1, the sequence {aj} where
aj=ℸaj−1=ℸjao |
converges to a point ϖ∈Q, and this point ϖ is claimed to be a fixed point of the mapping ℸ. For this reason, we can declare that
12ϑ(a,v)bϑ(aj,ℸaj)≤bϑ(aj,ϖ) | (2.7) |
or
12ϑ(a,v)bϑ(ℸaj,ℸ(ℸaj))≤bϑ(ℸaj,ϖ). | (2.8) |
Indeed, supposing on contrary
12ϑ(a,v)bϑ(aj,ℸaj)>bϑ(aj,ϖ) |
and
12ϑ(a,v)bϑ(ℸaj,ℸ(ℸaj))>bϑ(ℸaj,ϖ), |
we get that
bϑ(aj,aj+1)=bϑ(aj,ℸaj)≤ϑ(a,v)[bϑ(aj,ϖ)+bϑ(ϖ,ℸaj)]<ϑ(a,v)[12ϑ(a,v)bϑ(aj,ℸaj)+12ϑ(a,v)bϑ(ℸaj,ℸ(ℸaj))]=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 j∈N.
Case 1. When l=1, if (2.7) holds, we get
bϑ(aj+1,ϖ)≤α(aj,ϖ)bϑ(ℸaj,ℸϖ)≤ψ(A1ℸ(aj,ϖ))≤A1ℸ(aj,ϖ)=[bϑ(aj,ϖ)]p1⋅[bϑ(aj,ℸϖ)]p2⋅[bϑ(ϖ,ℸϖ)]p3⋅[bϑ(ϖ,ℸϖ)(1+bϑ(aj,aj+1))1+bϑ(aj,ϖ)]p4⋅[bϑ(aj,ℸϖ)+bϑ(ϖ,aj+1)2ϑ(aj,ℸϖ)]p5, |
we can distinguish the following two situations:
(1) p1+p2>0, letting j→+∞ above, we obtain bϑ(ϖ,ℸϖ)=0, thus ℸϖ=ϖ.
(2) p1=p2=0, when j→∞ above, and keeping in mind the continuity of extended-bMS we obtain
bϑ(ϖ,ℸϖ)<[bϑ(ϖ,ℸϖ)](p3+p4+p5)=bϑ(ϖ,ℸϖ), |
which is a contradiction. So, we have ℸϖ=ϖ, i.e., ϖ is a fixed point of the mapping ℸ.
Case 2. When l=2. If (2.7) holds, we obtain
bϑ(aj+1,ℸϖ)≤α(am,ϖ)bϑ(ℸaj,ℸϖ)≤ψ(A2ℸ(aj,ϖ))<A2ℸ(aj,ϖ)=[bϑ(aj,ϖ)]p1⋅[bϑ(aj,aj+1)]p2⋅[bϑ(ϖ,ℸϖ)]p3⋅[bϑ(ϖ,ℸϖ)bϑ(aj,aj+1)+bϑ(ϖ,aj+1)bϑ(aj,ℸϖ)max{bϑ(aj,aj+1),bϑ(aj+1,ℸϖ)}]p4⋅[bϑ(ϖ,ℸϖ)bϑ(ϖ,aj+1)+bϑ(aj,aj+1)bϑ(aj,ℸϖ)max{bϑ(ϖ,aj+1),bϑ(aj+1,ℸϖ)}]p5, |
if (2.8) holds,
bϑ(aj+2,ℸϖ)≤α(aj+1,ϖ)bϑ(ℸ2aj,ℸϖ)≤ψ(A2ℸ(ℸaj,ϖ))<A2ℸ(ℸaj,ϖ)=[bϑ(aj+1,ϖ)]p1⋅[bϑ(aj+1,aj+2)]p2⋅[bϑ(ϖ,ℸϖ)]p3⋅[bϑ(ϖ,ℸϖ)bϑ(aj+1,aj+2)+bϑ(ϖ,aj+2)bϑ(aj+1,ℸϖ)max{bϑ(aj+1,aj+2),bϑ(aj+2,ℸϖ)}]p4⋅[bϑ(ϖ,ℸϖ)bϑ(ϖ,aj+2)+bϑ(aj+1,aj+2)bϑ(aj+1,ℸϖ)max{bϑ(ϖ,aj+2),bϑ(aj+2,ℸϖ)}]p5, |
we can distinguish the following two situations:
(1) p1+p2+p4+p5>0, letting j→∞ above, we obtain bϑ(ϖ,ℸϖ)=0, thus ℸϖ=ϖ.
(2) p1=p2=p4=p5=0, in this case, when j→∞ above, we get
bϑ(ϖ,ℸϖ)<[bϑ(ϖ,ℸϖ)]p3=bϑ(ϖ,ℸϖ), |
which is a contradiction.
So, we get ℸϖ=ϖ, i.e., ϖ is a fixed point of the mapping ℸ.
This result possesses the below corollaries.
Corollary 2.3. Let (Q,bϑ) be a complete extended bMS. Suppose {pj}j∈N be a sequence, pj>1 for all j∈N such that ϑ(sj,sm)<pj for all m>j and ℸ: Q→Q be a mapping such that ∃ k∈[0,1) such that
1/2bϑ(s,ℸs)≤bϑ(s,v)impliesbϑ(ℸs,ℸv)≤kAlℸ(s,v), |
for any s,v∈Q−Fie(Q) where Alℸ,l=1,2 are defined by (2.2) and (2.3). Then, ℸ contains a fixed point ϖ∈Q, provided that either ℸ is orbitally continuous or ℸ is m-continuous for m≥1.
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}j∈N,pj>1 for all j∈N such that ϑ(sj,sm)<pj for all m>j, and ℸ: Q→Q be a self-mapping. Then ℸ has a fixed point provided that
12ϑ(s,v)bϑ(s,ℸs)≤bϑ(s,v)impliesbϑ(ℸs,ℸv)≤ψ(Alℸ(s,v)), |
where ψ∈ϝ and Alℸ,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}j∈N,pj>1 for all j∈N such that ϑ(sj,sm)<pj for all m>j and ℸ: Q→Q, self-mapping. Then ℸ will have a fixed point in Q provided that there exist k∈[0,1) such that
12ϑ(s,v)bϑ(s,ℸs)≤bϑ(s,v)impliesbϑ(ℸs,ℸv)≤kAlℸ(s,v), |
where Alℸ,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 s≠v for all s,v∈Q;0,if s=v; |
and ϑ: Q×Q→[1,+∞) be defined as ϑ(s,v)=1+s+v for all s,v∈Q. Let the mapping ℸ: Q→Q be defined by
ℸ(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 ℸ2(s)=1/5 is continuous, condition (iv) is also satisfied.
Case (1). For s,v∈[0,1], we have bϑ(ℸs,ℸv)=0, so inequality (2.1) holds.
Case (2). For s=0 and v=2, we have 12bϑ(0,1/2)=1/4≤2=bϑ(0,2) and bϑ(ℸs,ℸv)=0. Thus, the inequality (2.1) holds.
Case(3). For s=1/4 and v=3, we have
1/2bϑ(1/4,ℸ1/4)=0.25≤3.25=bϑ(1/4,3)⇒ α(1/4,3)bϑ(ℸ1/4,T3)=0.441716<0.8207=A1ℸ(1/4,3), |
hence (2.1) holds.
Case(4). For s=1/4 and v=9, we have
1/2bϑ(1/4,ℸ1/4)=0.225≤3.25=bϑ(1/4,9)⇒ α(1/4,9)bϑ(ℸ1/4,ℸ9)=0.8513<2.0433=A1ℸ(1/4,9). |
All other cases are true because α(s,v)=0. Hence, the mapping ℸ is an A1ℸ-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 ℸ, that is u=1/5.
Example 2.2. Let Q={1,2,3,5} and the extended-bMS defined bϑ: Q×Q→R+ as bϑ(s,v)=|s−v|4 with ϑ(s,v)=1+x+y and ℸ: Q→Q such that ℸ(1)=ℸ(5)=1 and ℸ(2)=ℸ(3)=2. Taking α: Q×Q→R+,α(s,v)=3 for all s,v∈Q, 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,ℸ3)=1/18<16=bϑ(3,5), |
which implies
α(3,5)bϑ(ℸ3,ℸ5)=3<8.2=ψ(A2ℸ(3,5)). |
Therefore, all the requirements of Theorem 2.3 are satisfied and it is clear that ℸ 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 ψ∈Θ 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 ℸ: Q→Q, as
ℸ(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]×R→R and g: [p,q]→R be continuous.
(2)ℸ is Alℸ-admissible interpolative contraction, Alℸ,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))|≤√Alℸ(s(e),v(e))√2(q−p) |
for each e,i∈[p,q] and s,v∈Q.
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),ℸ(s(e)))≤bϑ(s(e),ℸs(e))=supe∈[p,q]|s(e)−ℸs(e)|2=supe∈[p,q]|f(e)+∫qpM(e,i,s(i))di−f(e)−∫qpM(e,i,s(i))di|2≤supe∈[p,q]|f(e)+∫qpM(e,i,s(i))di−f(e)−∫qpM(e,i,v(i))di|2=bϑ(s(e),v(e)), |
we have
α(s(e),v(e))bϑ(ℸs(e),ℸv(e))=bϑ(ℸs(e),ℸv(e))=supe∈[p,q]|ℸs(e)−ℸv(e)|2=supe∈[p,q]|f(e)+∫qpM(e,i,s(i))di−f(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≤(∫qp√Alℸ(s(e),v(e))√2(q−p)di)2=Alℸ(s(e),v(e))2=ψ(Alℸ(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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