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 thatfor 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 thatfor 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 inequalityfor 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 inequalityfor 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 ifholds 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 setis 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 byThen, 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 satisfiesandfor 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 thatandfor 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 thatfor 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 .
Taking
and
, for all
in (
2), we have
where
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
(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
By (
6), we get
which means that
This is in contradiction with (
7).
(ii) If
, then
By (
6), we get
which establishes that
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 thatfor 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 satisfyingfor 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
Suppose that
and
for all
. From (
10), we obtain that
where
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 .
Assume, if possible,
. From (
10) and the triangular inequality, we obtain
where
Taking
from both sides of (
11), we have
, which is in contradiction with
.
Case 2
Assume that
or
for all
. Consider (
10), it follows that
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
From (
10), we obtain
where
This is a contradiction.
Case 2
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 thatfor 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 thatfor 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 thatfor 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 , thenThis shows that Corollaries 2–4 are not applicable in Example 9.