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Article

Non-Unique Fixed Point Results in Extended B-Metric Space †

1
Department of Mathematics, King Saud University, P.O. Box 2455, Riyadh 11451, Saudi Arabia
2
Department of Mathematics and Computer Sciences, Universitatea Transilvania Brasov, 500036 Brasov, Romania
3
Department of Mathematics, Erdal Karapınar, Atilim University, 06836 İncek, Ankara, Turkey
*
Author to whom correspondence should be addressed.
2000 Mathematics Subjects Classification 46T99, 47H10; 54H25.
Mathematics 2018, 6(5), 68; https://doi.org/10.3390/math6050068
Submission received: 5 April 2018 / Revised: 26 April 2018 / Accepted: 27 April 2018 / Published: 2 May 2018
(This article belongs to the Special Issue Fixed Point Theory)

Abstract

:
In this paper, we investigate the existence of fixed points that are not necessarily unique in the setting of extended b-metric space. We state some examples to illustrate our results.

1. Introduction and Preliminaries

Metric fixed point theory was initiated by the elegant results of Banach, the contraction mapping principle, and all researchers in this area agree on this. He formulated that every contraction in a complete metric space possesses a unique fixed point. Researchers have generalized this result by refining the contraction condition and/or by changing the metric space with a refined abstract space. One interesting generalization of metric space is b-metric space, formulated recently by Czerwik [1]. Following this result on b-metric space, several authors have reported a number of fixed point results in the framework of b-metric space (see, e.g., [2,3,4,5,6,7,8,9] and related references therein).
Throughout this manuscript, we denote N 0 : = N { 0 } , where N represents the positive integers. Further, R represents the real numbers and R 0 + : = [ 0 , ) .
Definition 1
(Czerwik [1]). For a non-empty set X, a function m b : X × X R 0 + is said to be b-metric if it satisfies the following conditions:
(mb1)
m b ( x , y ) = 0 if and only if x = y .
(mb2)
m b ( x , y ) = m b ( y , x ) for all x , y X .
(mb3)
m b ( x , y ) s [ m b ( x , z ) + m b ( z , y ) ] for all x , y , z X , where s 1 .
In addition, the pair ( X , m b ) is called a b-metric space, in short, bMS.
One of the standard examples of b-metric is the following:
Example 1.
Let X = R be the set of real numbers and m b ( x , y ) = ( x y ) 2 . Then m b is a b-metric on R with s = 2 . It is clear that m b is not a metric on R .
Remark 1.
It is worth mentioning that, for s = 1 , the b-metric becomes a usual metric.
Recently, Kamran et al. [10] introduced a new type of generalized b-metric space. Furthermore, they observed the analog of a Banach contraction mapping principle in the framework of this new space.
Definition 2.
[10] Let θ : X × X [ 1 , ) be a mapping. For a non-empty set X, a function d θ : X × X [ 0 , ) is said to be an extended b-metric if it satisfies the following state of affairs
(dθ1)
d θ ( ξ , η ) = 0 if and only if ξ = η ,
(dθ2)
d θ ( ξ , η ) = d θ ( η , ξ ) , and
(dθ3)
d θ ( ξ , ζ ) θ ( ξ , ζ ) d θ ( ξ , η ) + d θ ( η , ζ ) ,
for all ξ , η , ζ X . In addition, the pair ( X , d θ ) is called an extended b-metric space, in short extended-bMS.
Remark 2.
If θ ( ξ , η ) = s , constant, for s 1 , then it coincides with the standard definition of b-metric space.
Example 2.
Let θ : X × X [ 1 , ) be a mapping defined as θ ( x , y ) = x 2 + y 2 + 2 . For a set X = a , b , c , we set the mapping d θ : X × X [ 0 , ) as follows:
d θ ( a , b ) = d θ ( b , a ) = 5 , d θ ( a , c ) = d θ ( c , a ) = 3 , d θ ( b , c ) = d θ ( c , b ) = 1 ,
d θ ( a , a ) = d θ ( b , b ) = d θ ( c , c ) = 0 .
Obviously, ( d θ 1 ) and ( d θ 2 ) hold. For ( d θ 3 ) , we have
5 = d θ ( a , b ) θ ( a , b ) ( d θ ( a , c ) + d θ ( c , b ) ) = ( a 2 + b 2 + 2 ) · 4
3 = d θ ( a , c ) θ ( a , c ) ( d θ ( a , b ) + d θ ( b , c ) ) = ( a 2 + c 2 + 2 ) · 6
1 = d θ ( b , c ) θ ( b , c ) ( d θ ( b , a ) + d θ ( a , c ) ) = ( b 2 + c 2 + 2 ) · 8 .
In conclusion, for any ξ , η , ζ X , the third axiom
d θ ( ξ , ζ ) θ ( ξ , ζ ) d θ ( ξ , η ) + d θ ( η , ζ )
is satisfied. Accordingly, ( X , d θ ) is an extended b-metric space. Notice also that the standard triangle inequality is not satisfied for the following case
5 = d θ ( a , b ) > 4 = d θ ( a , c ) + d θ ( c , b ) .
Hence, X , d does not form a standard metric space.
In an extended-bMS, it is possible to obtain an analogy of basic topological notions, such as convergence, Cauchy sequences, and completeness. For more details, see, e.g., [10].
Definition 3.
[10] Let ( X , d θ ) be an extended-bMS.
(i)
We say that a sequence ξ n in X converges to ξ X , if for every ϵ > 0 there exists N = N ( ϵ ) N such that d θ ( ξ n , ξ ) < ϵ , for all n N , and it is denoted as lim n ξ n = ξ .
(ii)
We say that a sequence ξ n in X is Cauchy if, for every ϵ > 0 , there exists N = N ( ϵ ) N such that d θ ( ξ m , ξ n ) < ϵ , for all m , n N .
In what follows, we recollect the notion of completeness:
Definition 4.
[10]. An extended-bmetric space ( X , d θ ) is complete if every Cauchy sequence in X is convergent.
Lemma 1.
[10] Suppose that the pair ( X , d θ ) is a complete extended-bMS, where d θ is continuous. Then every convergent sequence has a unique limit.
Theorem 1.
[10] Suppose that the pair ( X , d θ ) is an complete extended-bMS, where d θ is continuous. If a self-mapping T : X X satisfies
d θ ( T ξ , T η ) k d θ ( ξ , η )
for all ξ , η X , where k 0 , 1 is such that for each x 0 X , lim n , m θ ( ξ n , ξ m ) < 1 k , where ξ n = T n ξ 0 , n = 1 , 2 , , then T has precisely one fixed point u. Moreover, for each η X , T n η u .
For our purposes, we need to recall the following definitions and results.
Definition 5.
[11] Suppose that the pair ( X , d θ ) is an extended-bMS For a self-mapping T : X X , for each ξ X and n N , we define
O ( ξ ; n ) = ξ , T ξ , , T n ξ   and   O ( ξ ; ) = ξ , T ξ , , T n ξ , .
We say that the set O ( ξ ; ) is the orbit of T.
Definition 6.
Suppose that the pair ( X , d θ ) is an extended-bMS. A self-mapping T : X X is called orbitally continuous if lim i T n i ( ξ ) = ζ for some ζ X implies that lim i T ( T n i ( ξ ) ) = T ζ . Moreover, if every Cauchy sequence of the form { T n i ( ξ ) } i = 1 , ξ X converges in ( X , d θ ) , then we say that an extended-bMS ( X , d θ ) is called T-orbitally complete.
Remark 3.
It is evident that the orbital continuity of T yields orbital continuity of any iterative power of T, that is, orbital continuity of T m for any m N .
Definition 7.
[12] Suppose that T is a self-mapping on a non-empty set X. Let α : X × X 0 , be a mapping. Then T is called an α-orbital admissible if, for all ξ X , we have
α ( ξ , T ξ ) 1 α ( T ξ , T 2 ξ ) 1 .
Remark 4.
We note that any α-admissible mapping is also an α-orbital admissible mapping. (see, e.g., [12]).

2. Main Results

Throughout the paper, we shall assume that d θ is a continuous functional.
Lemma 2.
[13] Let ( X , d θ ) be an extended b-metric space. If there exists q 0 , 1 such that the sequence x n , for an arbitrary x 0 X , satisfies lim n , m θ ( x n , x m ) < 1 q , and
0 < d θ ( x n , x n + 1 ) q d θ ( x n 1 , x n )
for any n N , then the sequence { x n } is Cauchy in X.
Proof. 
Let x n n N be a given sequence. By employing Inequality (3), recursively, we derive that
0 < d θ ( x n , x n + 1 ) q n d θ ( x 0 , x 1 ) .
Since q 0 , 1 , we find that
lim n d θ ( x n , x n + 1 ) = 0 .
On the other hand, by ( d θ 3 ) , together with triangular inequality, for p 1 , we derive that
d θ ( x n , x n + p ) θ ( x n , x n + p ) · d θ ( x n , x n + 1 ) + d θ ( x n + 1 , x n + p ) θ ( x n , x n + p ) d θ ( x n , x n + 1 ) + θ ( x n , x n + p ) d θ ( x n + 1 , x n + p ) θ ( x n , x n + p ) q n d θ ( x 0 , x 1 ) + θ ( x n , x n + p ) θ ( x n + 1 , x n + p ) [ d θ ( x n + 1 , x n + 2 ) + d θ ( x n + 2 , x n + p ) ] θ ( x n , x n + p ) · q n d θ ( x 0 , x 1 ) + θ ( x n , x n + p ) θ ( x n + 1 , x n + p ) · q n + 1 d θ ( x 0 , x 1 ) + + + θ ( x n , x n + p ) · · θ ( x n + p 1 , x n + p ) · k n + p 1 d θ ( x 0 , x 1 ) = d θ ( x 0 , x 1 ) i = 1 n + p 1 q i j = 1 i θ ( x n + j , x n + p ) .
Notice that the inequality above is dominated by i = 1 n + p 1 q i j = 1 i θ ( x n + j , x n + p ) i = 1 n + p 1 q i j = 1 i θ ( x j , x n + p ) .
On the other hand, by employing the ratio test, we conclude that the series i = 1 q i j = 1 i θ ( x j , x n + p ) converges some S ( 0 , ) . Indeed, lim i a i + 1 a i = lim i q θ ( x i , x i + p ) < 1 , which is why we obtain the desired result. Thus, we have
S = i = 1 q i j = 1 i θ ( x j , x n + p )   with   the   partial   sum   S n = i = 1 n q i j = 1 i θ ( x j , x n + p ) .
Consequently, we observe for n 1 , p 1 that
d θ ( x n , x n + p ) q n d θ ( x 0 , x 1 ) S n + p 1 S n 1 .
Letting n in Equation (7), we conclude that the constructive sequence { x n } is Cauchy in the extended b—metric space ( X , d θ ) . ☐
Lemma 3.
Let T : X X be an α-orbital admissible mapping and x n = T x n 1 , n N . If there exists x 0 X such that α ( x 0 , T x 0 ) 1 , then we have
α ( x n 1 , x n ) 1   for   all   n N 0 .
Proof. 
By assumption, there exists a point x 0 X such that α ( x 0 , T x 0 ) 1 . On account of the definition of x n X and owing to the fact that T is α -orbital admissible, we derive
α ( x 0 , x 1 ) = α ( x 0 , T x 0 ) 1 α ( T x 0 , T 2 x 0 ) = α ( x 1 , x 2 ) 1 .
Recursively, we have
α ( x n 1 , x n ) 1 ,   for   all   n N 0 .
 ☐
Theorem 2.
Suppose that T is an orbitally continuous self-mapping on the T-orbitally complete extended-bMS ( X , d θ ) . Assume that there exists k 0 , 1 and a 1 such that
α ( x , y ) min { d θ ( T x , T y ) , d θ ( x , T x ) , d θ ( y , T y ) } a   min { d θ ( x , T y ) , d θ ( T x , y ) } k d θ ( x , y ) )
for all x , y X . Furthermore, we presume that
(i)
T is α-orbital admissible;
(ii)
there exists x 0 X such that α ( x 0 , T x 0 ) 1 ;
(iii)
lim n , m θ ( x n , x m ) < 1 k .
Then, for each x 0 X , the sequence { T n x 0 } n N converges to a fixed point of T.
Proof. 
By assumption ( i i ) , there exists a point x 0 X such that α ( x 0 , T x 0 ) 1 . We construct the sequence { x n } in X such that
x n + 1 = T x n n N 0 .
If x n 0 = x n 0 + 1 = T x n 0 for some n 0 N 0 , then x * = x n 0 forms a fixed point for T that the proof finishes. Hence, from now on, we assume that
x n x n + 1   for   all   n N 0 .
On account of the assumptions ( i ) and ( i i ) , together with Lemma (3), Inequality (8) is yielded, that is,
α ( x n 1 , x n ) 1 ,   for   all   n N 0 .
By replacing x = x n 1 and y = x n in Inequality (9) and taking Equation (12) into account, we find that
min d θ ( T x n 1 , T x n ) , d θ ( x n 1 , T x n 1 ) , d θ ( x n , T x n ) a min d θ ( T x n , x n 1 ) , d θ ( T x n 1 , x n ) α ( x n 1 , x n ) min d θ ( T x n 1 , T x n ) , d θ ( x n 1 , T x n 1 ) , d θ ( x n , T x n ) a min d θ ( T x n , x n 1 ) , d θ ( T x n 1 , x n ) k d θ ( x n 1 , x n )
or,
min d θ ( x n , x n + 1 ) , d θ ( x n 1 , x n ) k d θ ( x n 1 , x n ) .
Since k 0 , 1 , the case d θ ( x n 1 , x n ) k d θ ( x n 1 , x n ) is impossible. Thus, we conclude that
d ( x n , x n + 1 ) k d θ ( x n 1 , x n ) .
On account of Lemma 2, we find that the sequence { x n } is a Cauchy sequence. By completeness of ( X , d θ ) , the sequence x n converges to some point u X as n . Owing to the construction x n = T n x 0 and the fact that ( X , d θ ) is T-orbitally complete, there is u X such that x n u . Since T , is orbital continuity, we deduce that x n T u . Accordingly, we conclude that u = T u . ☐
Example 3.
Let X = 1 , 2 , 3 , 4 be endowed with extended b-metric d θ : X × X 0 , , defined by d θ ( x , y ) = ( x y ) 2 , where θ : X × X 1 , , θ ( x , y ) = x + y + 1 . Let k = 1 4 , a = 4 and T : X X such that
T 1 = T 3 = 1 , T 2 = 4 , T 4 = 3 .
Define also α , β : X × X 0 , by
α ( x , y ) = 0 if , ( x , y ) ( 3 , 4 ) , ( 4 , 3 ) 1 otherwise .
Let us first notice that for any x 1 , 2 , 3 , 4 , the sequence T n x tends to 1 when n . For this reason, we can conclude that the mapping T is orbitally continuous and lim n , m θ ( T n x , T m x ) = 3 < 4 = 1 k , so ( i i i ) is satisfied. It can also be easily verified that T is orbital admissible.
If x = 1 or y = 1 , then d ( 1 , T 1 ) = 0 so Inequality (9) holds. We have to consider the following cases.
Case 1 . For x = 2 and y = 3 , we have
d θ ( 2 , 3 ) = 1 , d θ ( T 2 , T 3 ) = 9 , d θ ( 2 , T 2 ) = 4 , d θ ( 3 , T 3 ) = 4 , d θ ( 2 , T 3 ) = 1 , d θ ( 3 , T 2 ) = 1
and Inequality (9) yields
0 = min 9 , 4 , 4 4 · min 1 , 1 1 4 = 1 4 · d θ ( 2 , 3 ) .
Case 2 . For x = 2 and y = 4 , we have
d θ ( 2 , 4 ) = 4 , d θ ( T 2 , T 4 ) = 1 , d θ ( 2 , T 2 ) = 4 , d θ ( 4 , T 4 ) = 1 , d θ ( 2 , T 4 ) = 1 , d θ ( 4 , T 2 ) = 0
and
1 = min 1 , 4 , 1 4 · min 1 , 0 1 = 1 4 · d θ ( 2 , 4 ) .
Case 3 . For x = 3 and y = 4 , because α ( 3 , 4 ) = 0 , Inequality (9) holds.
Therefore, all the conditions of Theorem 2 are satisfied and T has a fixed point, x = 1 .
In Theorem 2, if we presume that α ( x , y ) = 1 and θ ( x , y ) = 1 , then we deduce the renowned non-unique fixed point theorem of Ćirić [14] as follows:
Corollary 1.
[Ćirić [14]] Suppose that T is an orbitally continuous self-map on the T-orbitally complete standard metric space ( X , d ) . We presume that there is a k [ 0 , 1 ) such that
min { d ( T x , T y ) , d ( x , T x ) , d ( y , T y ) } min { d ( x , T y ) , d ( T x , y ) } k d ( x , y )
for all x , y X . Then, for each x 0 X , the sequence { T n x 0 } n N converges to a fixed point of T.
Theorem 3.
Suppose that T is an orbitally continuous self-map on the T-orbitally complete extended-bMS ( X , d ) . We presume that there exists k 0 , 1 such that
α ( x , y ) Γ ( x , y ) k d θ ( x , y )
for all x , y X , where
Γ ( x , y ) = P ( x , y ) Q ( x , y ) R ( x , y ) P ( x , y ) = min { d θ ( T x , T y ) d θ ( x , y ) , d θ ( x , T x ) d θ ( y , T y ) } Q ( x , y ) = min { d θ ( x , T x ) d θ ( x , T y ) , d θ ( y , T y ) d θ ( T x , y ) } R ( x , y ) = min { d θ ( x , T x ) , d θ ( y , T y ) }
where R ( x , y ) 0 . Furthermore, we assume that
(i)
T is α-orbital admissible;
(ii)
there exists x 0 X such that α ( x 0 , T x 0 ) 1 ;
(iii)
lim n , m θ ( x n , x m ) < 1 k .
Then, for each x 0 X , the sequence { T n x 0 } n N converges to a fixed point of T.
Proof. 
As a first step, we construct an iterative sequence { x n } as in the proof of Theorem 2. For this purpose, we take an arbitrary initial value x X and define the following recursion:
x 0 : = x   and   x n = T x n 1   for   all   n N .
We also suppose that
x n x n 1   for   all   n N ,
as is discussed in the proof of Theorem 2.
For x = x n 1 and y = x n , Inequality (16) becomes (taking into account Lemma (3))
Γ ( x n 1 , x n ) α ( x n 1 , x n ) Γ ( x n 1 , x n ) k d θ ( x n 1 , x n )
where
P ( x n 1 , x n ) = min { d θ ( T x n 1 , T x n ) d θ ( x n 1 , x n ) , d θ ( x n 1 , T x n 1 ) d θ ( x n , T x n ) } = d θ ( x n , x n + 1 ) d θ ( x n 1 , x n ) Q ( x n 1 , x n ) = min { d θ ( x n 1 , T x n 1 ) d θ ( x n 1 , T x n ) , d θ ( x n , T x n ) d θ ( T x n 1 , x n ) } = 0 R ( x n 1 , x n ) = min { d θ ( x n 1 , T x n 1 ) , d θ ( x n , T x n ) } = min { d θ ( x n 1 , x n ) , d θ ( x n , x n + 1 ) Γ ( x n 1 , x n ) = P ( x n 1 , x n ) Q ( x n 1 , x n ) R ( x n 1 , x n ) .
We obtain that
d θ ( x n , x n + 1 ) d θ ( x n 1 , x n ) min { d θ ( x n 1 , x n ) , d θ ( x n , x n + 1 ) } k d θ ( x n 1 , x n ) .
If R ( x n 1 , x n ) = d θ ( x n , x n + 1 ) , then Inequality (20) turns into
d θ ( x n 1 , x n ) k d θ ( x n 1 , x n ) < d θ ( x n 1 , x n )
which is a contraction, since k 0 , 1 . Consequently, we deduce that
d θ ( x n , x n + 1 ) k d θ ( x n 1 , x n ) .
Applying Equation (22) recurrently, we find that
d θ ( x n , x n + 1 ) k d θ ( x n 1 , x n ) ) k 2 d θ ( x n 2 , x n 1 ) k n d θ ( x 0 , x 1 ) .
The rest of the proof is a verbatim restatement of the related lines in the proof of Theorem 2. ☐
Theorem 4.
Suppose that T is an orbitally continuous self-map on the T-orbitally complete extended-bMS ( X , d t h e t a ) . We presumed that there exists k 0 , 1 and a > 0 such that
α ( x , y ) P ( x , y ) a Q ( x , y ) k R ( x , y )
for all x , y X , where
P ( x , y ) = min { d θ ( T x , T y ) , d θ ( x , y ) , d θ ( x , T x ) , d θ ( y , T y ) } Q ( x , y ) = min { d θ ( x , T y ) , d θ ( T x , y ) } R ( x , y ) = min { d θ ( x , y ) , d θ ( x , T x ) }
with R ( x , y ) 0 . We also assume that
(i)
T is α-orbital admissible;
(ii)
there exists x 0 X such that α ( x 0 , T x 0 ) 1 ;
(iii)
lim n , m θ ( x n , x m ) < 1 k .
Then, for each x 0 X , the sequence { T n x 0 } n N converges to a fixed point of T.
Proof. 
Basically, we shall use the same technique that was used in the proof of Theorem 2. We built a recursive { x n } ,
x 0 : = x   and   x n = T x n 1   for   all   n N
for an arbitrary initial value x X . Regarding the discussion in the proof of Theorem 2, we presume that
x n x n 1   for   all   n N .
For x = x n 1 and y = x n , Inequality (24) becomes (taking into account Lemma 3)
P ( x n 1 , x n ) a Q ( x n 1 , x n ) α ( x n 1 , x n ) P ( x n 1 , x n ) a Q ( x n 1 , x n ) k R ( x n 1 , x n )
where
P ( x n 1 , x n ) = min { d θ ( T x n 1 , T x n ) , d θ ( x n 1 , x n ) , d θ ( x n 1 , T x n 1 ) , d θ ( x n , T x n ) } = min { d θ ( x n , x n + 1 ) , d θ ( x n 1 , x n ) } Q ( x n 1 , x n ) = min { d θ ( x n 1 , T x n ) , d θ ( T x n 1 , x n ) } = 0 R ( x n 1 , x n ) = max { d θ ( x n 1 , x n ) , d θ ( x n 1 , T x n 1 ) } = d θ ( x n 1 , x n ) .
Thus, Inequality (27) becomes
min { d θ ( x n , x n + 1 ) , d θ ( x n 1 , x n ) } k d θ ( x n 1 , x n ) .
If min { d θ ( x n , x n + 1 ) , d θ ( x n 1 , x n ) } = d θ ( x n 1 , x n ) , then Inequality (28) turns into
d θ ( x n 1 , x n ) k d θ ( x n 1 , x n ) < d θ ( x n 1 , x n ) ,
a contraction, since k 0 , 1 . Accordingly, we conclude that
d θ ( x n , x n + 1 ) k d θ ( x n 1 , x n ) .
Recursively, we derive that
d θ ( x n , x n + 1 ) k d θ ( x n 1 , x n ) ) k 2 d θ ( x n 2 , x n 1 ) ) k n d θ ( x 0 , x 1 ) .
By following the related lines in the proof of Theorem 2, we complete the proof. ☐
Theorem 5.
Assume that T is an orbitally continuous self-mapping on the T-orbitally complete extended-bMS ( X , d ) . We also presumed that there exists k 0 , 1 and a > 0 such that
α ( x , y ) m ( x , y ) n ( x , y ) k d θ ( x , T x ) d θ ( y , T y )
for all x , y X , where
n ( x , y ) = min { [ d θ ( T x , T y ) ] 2 , d θ ( x , y ) d θ ( T x , T y ) , [ d θ ( y , T y ) ] 2 } m ( x , y ) = min { d θ ( x , T x ) d θ ( y , T y ) , d θ ( x , T y ) d θ ( T x , y ) } .
Assume the following:
(i)
T is α-orbital admissible;
(ii)
there exists x 0 X such that α ( x 0 , T x 0 ) 1 ;
(iii)
lim n , m θ ( x n , x m ) < 1 k .
Then, for each x 0 X , the sequence { T n x 0 } n N converges to a fixed point of T.
Proof. 
As a first step, we shall construct an recursive sequence { x n = T x n 1 } n N , for an arbitrary initial value x 0 : = x X , as in the proof of Theorem 2. By following the same steps in the proof of Theorem 2, we deduce that adjacent terms of the sequence { x n } should be chosen distinct, that is,
x n x n 1   for   all   n N .
For x = x n 1 and y = x n , using ( i ) and Lemma (3) Inequality (32) infer that
m ( x n 1 , x n ) n ( x n 1 , x n ) α ( x n 1 , x n ) m ( x n 1 , x n ) n ( x n 1 , x n ) k d θ ( x n 1 , T x n 1 ) d θ ( x n , T x n ) ,
where
m ( x n 1 , x n ) = min { [ d θ ( T x n 1 , T x n ) ] 2 , d θ ( x n 1 , x n ) d θ ( T x n 1 , T x n ) , [ d θ ( x n , T x n ) ] 2 } = min { [ d θ ( x n , x n + 1 ) ] 2 , d θ ( x n 1 , x n ) d θ ( x n , x n + 1 ) , [ d θ ( x n , x n + 1 ) ] 2 } = min { [ d θ ( x n , x n + 1 ) ] 2 , d θ ( x n 1 , x n ) d θ ( x n , x n + 1 ) } , n ( x n 1 , x n ) = min { d θ ( x n 1 , T x n 1 ) d θ ( x n , T x n ) , d θ ( x n 1 , T x n ) d θ ( T x n 1 , x n ) } = min { d θ ( x n 1 , x n ) d θ ( x n , x n + 1 ) , d θ ( x n 1 , x n + 1 ) d θ ( x n , x n ) } = 0 .
The case m ( x n 1 , x n ) = d θ ( x n 1 , x n ) d θ ( x n , x n + 1 ) , is not possible because in this situation inequality (33) becomes
d θ ( x n 1 , x n ) d θ ( x n , x n + 1 ) k d θ ( x n 1 , x n ) d θ ( x n , x n + 1 ) < d θ ( x n 1 , x n ) d θ ( x n , x n + 1 ) ,
which is a contradiction. Consequently, we derive
[ d ( x n , x n + 1 ) ] 2 k ( d ( x n 1 , x n ) d ( x n , x n + 1 ) ) ,
which yields
d ( x n , x n + 1 ) < k d ( x n 1 , x n ) .
Iteratively, we get that
d ( x n , x n + 1 ) k d ( x n 1 , x n ) k 2 d ( x n 2 , x n 1 ) k n ( d ( x 0 , x 1 ) ) .
A verbatim repetition of the related lines in the proof of Theorem 2 completes the proof. ☐
Theorem 6.
Assume T is an orbitally continuous self-mapping on the T-orbitally complete extended-bMS ( X , d θ ) . We presumed there exists k [ 0 , 1 ) and a 0 such that
α ( x , y ) K ( x , y ) a Q ( x , y ) k S ( x , y ) ,
for all distinct x , y X where
K ( x , y ) = min d θ ( T x , T y ) , d θ ( y , T y ) , Q ( x , y ) = min { d θ ( x , T y ) , d θ ( y , T x ) } , S ( x , y ) = max { d θ ( x , y ) , d θ ( x , T x ) , d θ ( y , T y ) } .
If the following three conditions are fulfilled,
(i)
T is α-orbital admissible;
(ii)
there exists x 0 X such that α ( x 0 , T x 0 ) 1 ;
(iii)
lim n , m θ ( x n , x m ) < 1 k ,
then, for each x 0 X , the sequence { T n x 0 } n N converges to a fixed point of T.
Proof. 
Let x 0 X . Starting from this arbitrary initial value, we construct the iterative sequence x n = T x n 1 n N . As discussed in the proof of Theorem 2, we can suppose that
x n x n 1   for   all   n N .
On the other hand, from ( i ) and Lemma 3, we have that α ( x n 1 , x n ) 1 , so, for x = x n 1 and y = x n , Inequality (37) implies that
K ( x n 1 , x n ) a Q ( x n 1 , x n ) α ( x n 1 , x n ) K ( x n 1 , x n ) a Q ( x n 1 , x n ) k S ( x n 1 , x n )
where
K ( x n 1 , x n ) = min d θ ( T x n 1 , T x n ) , d θ ( x n , T x n ) = min d θ ( x n , x n + 1 ) , d θ ( x n , x n + 1 ) = d θ ( x n , x n + 1 ) Q ( x n 1 , x n ) = min { d θ ( x n 1 , T x n ) , d θ ( x n , T x n 1 ) } = 0 S ( x n 1 , x n ) = max { d θ ( x n 1 , x n ) , d θ ( x n 1 , T x n 1 ) , d θ ( x n , T x n ) } = max { d θ ( x n 1 , x n ) , d θ ( x n , x n + 1 ) } .
Obviously, since k [ 0 , 1 ) , the case S ( x n 1 , x n ) = d ( x n , x n + 1 ) is impossible. More precisely, Inequality (39) turns into
K ( x n 1 , x n ) = d ( x n , x n + 1 ) k d ( x n , x n + 1 ) < d ( x n , x n + 1 )
which is a contradiction. Hence, Inequality (39) yields that
d ( x n , x n + 1 ) k d ( x n 1 , x n ) < d ( x n 1 , x n )   and   d ( x n , x n + 1 ) k n d ( x 0 , x 1 )
for all n N . A verbatim restatement of the related lines in the proof of Theorem 2 completes the proof. ☐

3. Conclusions

We note that several consequences can be observed from the main results in distinct aspects. For example, taking θ ( x , y ) = s 1 implies corresponding fixed point results in the context of b-metric space. In addition, standard versions of the given results follow when we take θ ( x , y ) = 1 . Notice also that, as in [15], by assigning α ( x , y ) in a proper way, we can conclude results in the frame of “partially ordered spaces” and for “cyclic contraction”.

Author Contributions

All authors contributed equally and significantly in writing this article. All authors read and approved the final manuscript.

Acknowledgments

The first and third authors extend their appreciation to Distinguished Scientist Fellowship Program (DSFP) at King Saud University (Saudi Arabia).

Conflicts of Interest

The authors declare no conflict of interest.

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Alqahtani, B.; Fulga, A.; Karapınar, E. Non-Unique Fixed Point Results in Extended B-Metric Space. Mathematics 2018, 6, 68. https://doi.org/10.3390/math6050068

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Alqahtani B, Fulga A, Karapınar E. Non-Unique Fixed Point Results in Extended B-Metric Space. Mathematics. 2018; 6(5):68. https://doi.org/10.3390/math6050068

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Alqahtani, Badr, Andreea Fulga, and Erdal Karapınar. 2018. "Non-Unique Fixed Point Results in Extended B-Metric Space" Mathematics 6, no. 5: 68. https://doi.org/10.3390/math6050068

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