Abstract
In this paper, we establish the existence of fixed points of rational type contractions in the setting of extended b-metric spaces. Our results extend considerably several well-known results in the existing literature. We present some nontrivial examples to show the validity of our results. Furthermore, as applications, we obtain the existence of solution to a class of Fredholm integral equations.
1. Introduction and Preliminaries
The concept of distance between two abstract objects has received importance not only for mathematical analysis but also for its related fields. Bakhtin [1] introduced b-metric spaces as a generalization of metric spaces (see also Czerwik [2]). Recently, Kamran et al. [3] gave the notion of extended b-metric space and presented a counterpart of Banach contraction mapping principle. On the other hand, fixed point results dealing with general contractive conditions involving rational type expression are also interesting. Some well-known results in this direction are involved (see [4,5,6,7,8,9,10]).
First, of all, we recall some fixed point theorems for rational type contractions in metric spaces.
Theorem 1
([5]). Let T be a continuous self mapping on a complete metric space . If T is a rational type contraction, there exist , where such that
for all , then T has a unique fixed point in X.
Theorem 2
([4]). Let T be a continuous self mapping on a complete metric space . If T is a rational type contraction, there exist , where such that
for all , then T has a unique fixed point in X.
Fisher [11] refined the result of Khan [6] in the following way.
Theorem 3
([11]). Let T be a self mapping on a complete metric space . If T is a rational type contraction, T satisfies the inequality
for all , where . Then, T has a unique fixed point in X.
Ahmad et al. [12] extended Theorem 3 from metric spaces to generalized metric spaces (see [13] for more details). Piri et al. [14] extended the result of Ahmad et al. [12] in the following way.
Theorem 4
([14]). Let T be a self mapping on a complete generalized metric space . If T is a rational type contraction, T satisfies the inequality
for all , where and . Then, T has a unique fixed point in X.
Let us recall some basic concepts in b-metric spaces as follows.
Definition 1
([1,2]). Let X be a nonempty set and be a given real number. A function is called a b-metric on X, if, for all , the following conditions hold:
if and only if ;
;
.
In this case, the pair is called a b-metric space.
It is well-known that any b-metric space will become a metric space if . However, any metric space does not necessarily be a b-metric space if . In other words, b-metric spaces are more general than metric spaces (see [15]).
The following example gives us evidence that b-metric space is indeed different from metric space.
Example 1
([16]). Let be a metric space and for all , where is a real number. Then, is a b-metric space with . However, is not a metric space.
Definition 2
([17]). Let be a sequence in a b-metric space . Then,
(i) is called a convergent sequence, if, for each , there exists such that , for all , and we write ;
(ii) is called a Cauchy sequence, if, for each , there exists such that , for all ;
(iii) is said to be complete if every Cauchy sequence is convergent in X.
The following theorem is a basic theorem for Banach type contraction in b-metric space.
Theorem 5
([18]). Let T be a self mapping on a complete b-metric space . Then, T has a unique fixed point in X if
holds for all , where is a constant. Moreover, for any , the sequence converges to the fixed point.
Note that the distance function utilized in b-metric spaces is generally discontinuous (see [15,19]). For fixed point results and more examples in b-metric spaces, the readers may refer to [15,16,17,18].
In what follows, we recall the concept of extend b-metric space and some examples.
Definition 3
([3]). Let X be a nonempty set. Suppose that and are two mappings. If for all , the following conditions hold:
if and only if ;
;
,
then is called an extended b-metric, and the pair is called an extended b-metric space.
Note that, if (a finite constant), for all , then extended b-metric space reduces to a b-metric space. That is to say, b-metric space is a generalization of metric space, and extended b-metric space is a generalization of b-metric space.
In the following, we introduce some examples for extended b-metric spaces.
Example 2.
Let . Define two mappings and as follows: , for all , and
Then, is an extended b-metric space.
Indeed, and in Definition 3 are clear. Let . We prove that in Definition 3 is satisfied.
(i) If , then is clear.
(ii) If , , then
(iii) If , , then
(iv) If , , , then
Consider the above cases, it follows that holds. Hence, the claim holds.
Example 3.
Let . Define two mappings and as follows: , for all and
Then, is an extended b-metric space.
Indeed, and in Definition 3 are obvious. Let . We prove that in Definition 3 is satisfied.
(i) If , then is obvious.
(ii) If , , then
(iii) If , , then
(iv) If , , , then
Consider the above cases, it follows that holds. Hence, the claim holds.
Example 4.
Let . Define two mappings and as follows:
and , for all . Then, is an extended b-metric space.
Indeed, and in Definition 3 are valid. Let . We prove that in Definition 3 is satisfied.
(i) If , then holds.
(ii) If , , then
(iii) If , , then
(iv) If , , , then, by the fact that is nondecreasing on and , it follows that
Consider the above cases, it follows that holds. Hence, the claim holds.
Example 5.
Let and be a function on . Define a mapping as follows:
Then, is an extended-b metric space.
As a matter of fact, obviously, and hold. For , we have the following cases:
(i) Let such that and z are distinct each other, then
(ii) Let and , then
(iii) Let and , then
Therefore, in Definition 3 holds. Thus, the claims hold.
Remark 1.
Examples 2–5 are extended b-metric spaces but not b-metric spaces.
Similar to Definition 2, we recall some concepts in extended b-metric spaces as follows.
Definition 4
([3]). Let be a sequence in an extended b-metric space . Then,
(i) is called a convergent sequence, if, for each , there exists such that , for all , and we write ;
(ii) is called a Cauchy sequence, if, for each , there exists such that , for all ;
(iii) is said to be complete if every Cauchy sequence is convergent in X.
As we know, the limit of convergent sequence in extended b-metric space is unique provided that is a continuous mapping (see [3]).
Definition 5
([20,21]). Let T be a self mapping on an extended b-metric space . For , the set
is said to be an orbit of T at . T is said to be orbitally continuous at if implies . Moreover, if every Cauchy sequence of the form is convergent to some point in X, then is said to be a T-orbitally complete space.
Note that, if is complete extended b-metric space, then X is T-orbitally complete for any self-mapping T on X. Moreover, if T is continuous, then it is obviously orbitally continuous in X. However, the converse may not be true.
In the sequel, unless otherwise specified, we always denote .
Definition 6
([22]). Let X be a nonempty set and be a mapping. A mapping is called α-admissible, if for all implies .
Definition 7
([23]). Let X be a nonempty set and be a mapping. Then, is called α*-admissible if it is a α-admissible mapping and holds for all .
Example 6.
Let and be a mapping defined by . Let be a function defined by
Then, T is α-admissible and . Moreover, is satisfied for all . Consequently, T is α*-admissible.
Example 7
([23]). Let and be a mapping defined by . Let be a function defined by
Then, T is a α-admissible mapping and . However, is satisfied for . Thus, T is not α*-admissible.
Definition 8
([24]). Let T be a self mapping on a nonempty set X. Then, T is called α-orbitally admissible if, for all , leads to .
It is mentioned that each -admissible mapping must be an -orbitally admissible mapping (for more details, see [24]). For the uniqueness of fixed point, we will use the following definition frequently.
Definition 9.
An α-orbitally admissible mapping T is called -orbitally admissible if implies .
Definition 10
([17,25]). A function is said to be a comparison function, if it is nondecreasing and for all , where denotes the iteration of ψ.
In what follows, the set of all comparison functions is denoted by . Some examples for comparison functions, the reader may refer to [26].
Lemma 1
([27]). Let . Then, for all and .
The following lemmas will be used in the sequel.
Lemma 2
([28]). Let be an extended b-metric space, and be a sequence in X. If satisfies
and
for all , then is a Cauchy sequence in X.
Proof.
From the given conditions, we get
On taking limit as , we have
Setting for each , and , we obtain
Notice that
then, by the Ratio test the series, converges.
Let and be the sequence of partial sum. Consequently, for any and , we obtain
Taking the limit as from both side of the above inequality, we make a conclusion that is a Cauchy sequence in X. □
Lemma 3
([29]). Let be a sequence in an extended b-metric space such that
and
for any , where , then is a Cauchy sequence in X.
Proof.
Choose , where in Lemma 2. Then, the proof is completed. □
2. Fixed Points of Rational Type Contractions
In this section, we assume that is an extended b-metric space with the continuous functional . Let be a mapping. For , we always denote
Theorem 6.
Let T be a self mapping on a T-orbitally complete extended b-metric space . Assume that there exist two functions , such that
for all . That is, T is a rational type contraction. If
(i) T is α-orbitally admissible;
(ii) there exists satisfying ;
(iii) (1) is satisfied for ();
(iv) T is either continuous or, orbitally continuous on X.
Then, T possesses a fixed point . Moreover, the sequence converges to .
Proof.
By (ii), define a sequence in X such that , for all .
If , for, some , then is a fixed point of T. This completes the proof. Without loss of generality, we therefore assume that , for all .
Based on (i), implies that . Then, . Continuing this process, one has , for all .
Similar to ([10], Theorem 2.1), we can prove
In fact, we finish the proof via three cases.
(i) If , then by (3), it follows that
This is (5).
(ii) If , then by (3), we have
which is a contradiction.
(iii) If , then by (4), it is easy to say that
In this case, we discuss it with two subcases.
(i) If , then
This is in contradiction with (7).
(ii) If , then
This is in contradiction with (8).
This is to say, (iii) does not occur.
Thus, (5) is satified. Accordingly, we speculate that
Letting , we obtain that .
It follows from Lemma 2 that is a Cauchy sequence in X. Since is T-orbitally complete, then there is such that .
Assume that T is continuous, then
Therefore, T possesses a fixed point z in X.
Assume that T is orbitally continuous on X, thus, as . Since the limit of sequence in extended b-metric space is unique, then . Thus, T possesses a fixed point z in X, i.e., . □
Example 8.
Under all the conditions of Example 3, let be a continuous mapping defined by
In addition, we define a mapping as
Let be a point with , then and . Therefore, T is α-orbitally admissible.
Set , for all , where , then .
For all distinct in X, ones have
Moreover, there is with , then . Now, we deduce inductively that , where , for all . Obviously, as . Thus, is T-orbitally complete.
Note that , where , that is to say,
Thus, all the conditions of Theorem 6 hold and hence T possesses a fixed point in X and .
Theorem 7.
In addition to all the conditions of Theorem 6, suppose that the T is -orbitally admissible. Then, T possesses a unique fixed point .
Proof.
Following Theorem 6, T possesses a fixed point in X. Thus, . Assume that T is -orbitally admissible. If possible, there exist such that and , then .
Taking in (2), we obtain
which is a contradiction. Therefore, T possesses a unique fixed point in X. □
Corollary 1.
([10], Theorem 2.1) Let T be a continuous self mapping on a complete extended b-metric space such that
for all , where . That is, T is a rational type contraction. In addition, suppose that for all ,
where , . Then, T has a unique fixed point . Moreover, the sequence converges to .
Proof.
Setting , for all , then implies that . Therefore, T is -orbitally admissible.
Let , for all , where , then . Using (iii) of Theorem 6. In view of (9), then (iii) of Theorem 6 is satisfied. Thus, all the conditions of Theorem 6 hold. Therefore, T possesses a fixed point in X, i.e., . Because of , then T is -orbitally admissible and hence, by Theorem 7, T has a unique fixed point in X. □
Remark 2.
(i) The uniqueness of fixed point is not guaranteed if T is not -orbitally admissible. In Example 8, T is α-orbitally admissible and . However, so T is not -orbitally admissible. Therefore, Theorem 7 is not applicable in this case.
(ii) In Example 8, for and , we obtain
Therefore, ([3], Theorem 2) and ([10], Theorem 2.1) are not applicable in this case.
Motivated by Piri et al. [14], we extend a fixed point theorem for Khan type from metric spaces to extended b-metric spaces.
Theorem 8.
Let T be a self mapping on a T-orbitally complete extended b-metric space . Suppose that , are two functions satisfying
for all , where
If
(i) T is α-orbitally admissible;
(ii) there exists and ;
(iii) (1) is satisfied for ().
Then, T possesses a fixed point . Moreover, the sequence converges to .
Proof.
By (ii), define a sequence in X such that , for all . Since T is -orbitally admissible, then implies . Thus, inductively, we obtain that , for all . In order to show that T possesses a fixed point in X, we assume that , for all . We divide the proof into the following two cases:
Case 1
Therefore,
Furthermore,
Letting , we have
It follows from Condition (iii) and Lemma 2 that is a Cauchy sequence in X. Notice that X is T-orbitally complete, thus, there is with as .
Taking from both sides of (11), we have , which is in contradiction with .
Case 2
Thus, T possesses a fixed point in X, i.e., . □
Example 9.
Under all the conditions of Example 5, let be a mapping defined by
We also define a mapping as
Let be a point such that , then and . Therefore, T is α-orbitally admissible.
Set , for all , where . For all , we obtain
Clearly, there exists such that , then . Therefore, by the mathematical induction, we have , for all . Consequently, as . This shows that is a T-orbitally complete extended b-metric space.
Moreover, it is easy to see that
Accordingly, all the conditions of Theorem 8 hold and, therefore, T possesses a fixed point and .
Theorem 9.
In addition to Theorem 8, suppose that T is -orbitally admissible. Then, T possesses a unique fixed point .
Proof.
By Theorem 8, T possesses a fixed point in X, i.e., . For the uniqueness, let such that . Then, by the -orbital admissibility of T, we have .
As in Theorem 8, we also divide the proof into two cases as follows:
Case 1
Suppose that
and
Therefore,
This is a contradiction.
Case 2
Assume that
or
Consequently, .
Thus, T possesses a unique fixed point in X. This completes the proof. □
Corollary 2.
Let T be a self mapping on a complete extended b-metric space such that
for all , where , and are defined in Theorem 8. Furthermore, suppose, for all , that (9) is satisfied. Then, T has a unique fixed point . Moreover, the sequence converges to z.
Corollary 3.
Let T be a self mapping on a complete extended b-metric space such that
for all , where and . Further suppose, for all , that (9) is satisfied. Then, T has a unique fixed point . Moreover, the sequence converges to z.
Corollary 4.
([10], Theorem 2.2) Let T be a self mapping on a complete extended b-metric space such that
for all , where and . Further assume, for all , that (9) is satisfied. Then, T has a unique fixed point . Moreover, the sequence converges to z.
Remark 3.
(i) In Example 9, T is α-orbitally admissible. Since , but , T is not -orbitally admissible. In this case, Theorem 9 is not applicable in Example 9.
(ii) In Example 9, if and , then
This shows that Corollaries 2–4 are not applicable in Example 9.
3. Applications
In this section, by using fixed point theorems mentioned above, we cope with some problems for the unique solution to a class of Fredholm integral equations.
Let be a set of all real valued continuous functions on . Define two mappings by
and by
where is a constant. Then, is a complete extended b-metric space.
Define a Fredholm integral equation by
where , and and are continuous functions. Let be an integral operator defined by
Theorem 10.
Let be an integral operator defined in (12). Suppose that the following assumptions hold:
(i) for any , , where ,
(ii) for any , it satisfies
where and is a continuous function satisfying
Then, the integral operator T has a unique solution in X.
Proof.
Let be a constant with . Making full use of (13) and the Hölder’s inequality, we speculate that
Setting , we obtain that
Thus, all the conditions of Corollary 1 are satisfied and hence T possesses a unique fixed point in X. □
Theorem 11.
Let be an integral operator defined by (12). Assume that the following assumptions hold:
(i) , where for any ;
(ii) for all distinct in X, ones have
where
and is a continuous function such that
Then, the integral operator T has a unique solution in X.
Example 10.
Let be a set of all real valued continuous functions defined on . Then, is a complete extended b-metric space equipped with , where , for all . Let be an operator defined by
where and , for all .
We have
Taking the supremum on both sides of (16), for all , we obtain
In addition, , where and . Thus, all the conditions of Theorem 10 are satisfied and hence the integral operator T has a unique solution.
Author Contributions
H.H. designed the research and wrote the paper. Y.M.S. offered the draft preparation and gave the methodology, M.S.K. and S.R. co-wrote and made revisions to the paper. H.H. gave the support of funding acquisition. All authors have read and agreed to the published version of the manuscript.
Funding
The first author acknowledges the financial support from the Natural Science Foundation of Chongqing of China (No. cstc2020jcyj-msxmX0762), and the Initial Funding of Scientific Research for High-level Talents of Chongqing Three Gorges University of China (No. 2104/09926601).
Institutional Review Board Statement
Not applicable.
Informed Consent Statement
Not applicable.
Data Availability Statement
The data presented in this study are available upon request from the corresponding author.
Acknowledgments
The authors thank the editor and the referees for their valuable comments and suggestions which greatly improved the quality of this paper.
Conflicts of Interest
The authors declare no conflict of interest.
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