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Characterizations of quasi-metric and G-metric completeness involving w-distances and fixed points

  • Erdal Karapınar EMAIL logo , Salvador Romaguera and Pedro Tirado
Published/Copyright: December 13, 2022
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Abstract

Involving w -distances we prove a fixed point theorem of Caristi-type in the realm of (non-necessarily T 1 ) quasi-metric spaces. With the help of this result, a characterization of quasi-metric completeness is obtained. Our approach allows us to retrieve several key examples occurring in various fields of mathematics and computer science and that are modeled as non- T 1 quasi-metric spaces. As an application, we deduce a characterization of complete G -metric spaces in terms of a weak version of Caristi’s theorem that involves a G-metric version of w-distances.

MSC 2010: 47H10; 54H25; 54E50

1 Introduction

It has long been widely recognized that Caristi’s fixed point theorem [1, Theorem (2.1)’] constitutes one of the most prominent generalizations of the Banach contraction principle. Thus, Kirk showed in [2] that its validity characterizes the metric completeness. Furthermore, it has direct applications in functional analysis [3, Chapter 9], mathematical optimization [4], and, through a quasi-metric version, in the study of the complexity analysis of some algorithms via denotational semantics [5]. On the other hand, its equivalence with the celebrated Ekeland’s variational principle [6,7] guarantees, at least indirectly, its applicability to a variety of issues about global analysis, optimal control, equilibrium problems, etc. Since there is a vast literature on these topics, we keep citing the recent contributions [8,9,10] with references therein. Generalizations and extensions of Caristi’s theorem to b -metric spaces, quasi-metric spaces, partial metric spaces, and fuzzy metric spaces, among others, may be found in [11,12, 13,14,15, 16,17].

At this point, it is interesting to recall that the original proof of Caristi’s theorem uses transfinite induction. Several mathematicians refined and improved such a proof, for instance, via Zermelo-Fraenkel Axioms or via Zorn’s lemma-The Axiom of Choice (see [18, Section 1] and [19, Section 6] for detailed accounts on this subject). In this context, Khamsi [20, page 3] asked the question of finding a pure metric proof of Caristi’s theorem (see also [21, page 13]). If we understand as “a pure metric proof” the one reasonably suggested by Kozlowski in [22, page 134], then, and as far as we know, a purely metric proof already implicitly appeared in a remarkable generalization of Caristi’s theorem, in terms of w -distances, obtained by Kada et al. in [23, Theorem 2] as well as in [24, Theorem 2.3] within the framework of partial metric spaces. Later on, Kozlowski [22] and Du [25] also presented purely metric proofs of Caristi’s theorem (see also [26, Theorem 2]). Let us note that these proofs have in common a like starting point and the approaches of some parts of such proofs follow similar patterns.

It is also interesting to mention the recent contribution from Darko et al. [27], where the authors use the concept of w t -distance (a b -metric counterpart of the notion of w -distance) to generalize a known fixed-point theorem of Ćirić [28] as well as recent results from [29] and [30]. They also consider Fisher’s quasi-contraction in the framework of w t -distance.

In this article, we obtain a generalization of Kada-Suzuki-Takahashi’s theorem cited earlier to the realm of (non-necessarily T 1 ) quasi-metric spaces, with a purely metric proof that is inspired by the proof of [26, Theorem 2]. From this result, we characterize those quasi-metric spaces that are complete in the sense of [31,32] (a very general type of quasi-metric completeness). We emphasize that our non- T 1 approach allows us to recover several fundamental examples in the basic theory of asymmetric functional analysis (see, e.g., [33, Section 2.1.6]), in some aspects of the calculus of variations (see, e.g., [35]) and in various branches of the theory of computation (see, e.g., [36,37,38, 39,40]). The last part of the article is devoted to apply the obtained results in the quasi-metric setting to deduce a characterization of complete G -metric spaces in terms of a weak version of Caristi’s theorem that involves a G-metric version of w-distances.

Two antecedents of our study are contained in articles by Park [41] and by Al-Homidan et al. [42], respectively, where the authors obtained characterizations of complete T 1 quasi-metric spaces from versions of Kada-Suzuki-Takahashi’s theorem for T 1 quasi-metric spaces and whose proofs make use of a suitable quasi-order and the notion of maximal element.

2 Preliminaries

In this brief section, we recap several pertinent concepts and properties on quasi-metric spaces that will be useful throughout the article. Our main reference for these spaces is [33] and for general topology is [34].

By R , R + , N , and N 0 we denote the set of real numbers, the set of non-negative real numbers, the set of positive integer numbers, and the set of non-negative integer numbers, respectively.

A quasi-metric on a set X is a function q : X × X R + satisfying the following two conditions for any x , y , z X :

(qm1) q ( x , y ) = q ( y , x ) = 0 if and only if x = y ;

(qm2) q ( x , z ) q ( x , y ) + q ( y , z ) .

If q satisfies (qm2) and the following condition, stronger than (qm1), we say that q is a T 1 quasi-metric on X :

(qm1’) q ( x , y ) = 0 if and only if x = y .

A ( T 1 ) quasi-metric space is a pair ( X , q ) such that X is a set and q is a ( T 1 ) quasi-metric on X .

If q is a quasi-metric on a set X , the family { B q ( x , ε ) : x X , ε > 0 } is a base of open sets for a T 0 topology T q on X , where for each x X and ε > 0 , B q ( x , ε ) = { y X : q ( x , y ) < ε } . Note that if q is a T 1 quasi-metric, then T q is a T 1 topology on X .

Given a ( T 1 ) quasi-metric q on X , the function q : X × X R + defined by q ( x , y ) = q ( y , x ) for all x , y X , is also a ( T 1 ) quasi-metric on X , whereas the function q s : X × X R + defined by q s ( x , y ) = max { q ( x , y ) , q ( x , y ) } for all x , y X , is a metric on X .

It is clear from the definition of T q that a sequence ( x n ) n N in X is T q -convergent to some x X if and only if q ( x , x n ) 0 as n . Similarly, a sequence ( x n ) n N in X is T q -convergent to some x X if and only if q ( x n , x ) 0 as n .

The following is a basic but paradigmatic instance of a non- T 1 quasi-metric space.

Example 1

Let q : R × R R + defined by q ( x , y ) = max { x y , 0 } . Then, q is a non- T 1 quasi-metric on X , and the topology T q is the so-called lower topology on R . Note also that q s is the usual metric on R .

Due to the absence of symmetry, we can define various different types of Cauchy sequence and of completeness in the framework of quasi-metric spaces that, nevertheless, coincide with the usual notions of Cauchy sequence and completeness when dealing with a metric space (see, e.g., [33,43]).

Here, we will consider the following two notions of Cauchy sequence and of complete quasi-metric space:

A sequence ( x n ) n N in a quasi-metric space ( X , q ) is left Cauchy provided that for each ε > 0 , there is n ε N such that q ( x n , x m ) < ε whenever n ε n m , and it is Cauchy provided that is a Cauchy sequence in the metric space ( X , q s ) .

A quasi-metric space ( X , q ) is q -right complete provided that every left Cauchy sequence is T q -convergent, and it is q -half complete provided that every Cauchy sequence is T q -convergent.

In classical terminology (see, e.g., [33,43]), the notion of q -right completeness of ( X , q ) corresponds to the notion of right K-completeness of ( X , q ) , while the notion of q -half completeness of ( X , q ) corresponds to the notion of sequential completeness of ( X , q ) .

Obviously, every q -right complete quasi-metric space ( X , q ) is q -half complete. The converse does not hold, in general; in fact, the quasi-metric space ( X , q ) of Example 1 is q -half complete because ( X , q s ) is a complete metric space, but it is not q -right complete because the sequence ( n ) n N is left Cauchy but it is not T q -convergent.

3 Q -functions and w -distances

In [41], Park extended the notion of w-distance to the setting of quasi-metric spaces. Later, Al-Homidan et al. [42] introduced and discussed, in the realm of T 1 quasi-metric spaces, the notion of Q-function as a generalization of Park’s notion. In the sequel, we remind such notions.

Let ( X , q ) be a quasi-metric space and let W : X × X R + . Consider the following conditions:

(w1) W ( x , y ) W ( x , z ) + W ( z , y ) , for all x , y , z X .

(w2) For each x X , the function W ( x , ) : X R + is T q -lower semicontinuous ( T q -lsc, in short).

(Q) If x , y X , ( y n ) n N is a sequence in X that T q -converges to y and there is a constant M > 0 such that Q ( x , y n ) M for all n N , then Q ( x , y ) M .

(w3) For each ε > 0 , there exists δ > 0 such that W ( x , y ) δ and W ( x , z ) δ imply q ( y , z ) ε .

The function W is said to be a w -distance on ( X , q ) if it satisfies conditions (w1), (w2), and (w3), and it is said to be a Q-function on ( X , q ) if it satisfies conditions (w1), (Q) and (w3).

Next, we show that actually the notions of w-distance and Q-function coincide.

Proposition 2

Let ( X , q ) be a quasi-metric space. Then, a function F : X × X R + is a Q-function on ( X , q ) if and only if it is a w-distance on ( X , q ) .

Proof

It was noted in [42, page 128] that every w-distance on ( X , q ) is a Q-function on ( X , q ) .

Now suppose that F is a Q-function on ( X , q ) , which is not a w-distance on ( X , q ) . Then, there is x X for which the function F ( x , ) : X R + is not T q -lsc. Therefore, there exists a sequence ( y n ) n N in X that T q -converges to some y X , and an ε > 0 and a subsequence ( y k n ) n N of ( y n ) n N such that F ( x , y ) ε + F ( x , y k n ) , for all n N . Put M = F ( x , y ) ε / 2 . Then, M > 0 and F ( x , y k n ) < M for all n N . Since ( y k n ) n N is T q -convergent to y and F is a Q -function, we deduce that F ( x , y ) M , a contradiction. Hence, F is a w-distance on ( X , q ) .□

Remark 3

Note that although the authors of [42] worked in the realm of T 1 quasi-metric spaces, Proposition 2 remains valid for every quasi-metric space.

It is well known that any metric d on a set X is a w-distance on the metric space ( X , d ) (see [23, Example 1]). However, there are quasi-metric spaces ( X , q ) for which the quasi-metric q is not a w -distance on ( X , q ) [31, Proposition 2.3]. Despite this, the use of w -distances instead of the original quasi-metric one yields better results in extending Caristi’s theorem to the frame of non- T 1 quasi-metric spaces as we shall show in Theorem 12 in the next section.

We underline that there are many interesting examples of w -distances on quasi-metric spaces (see, e.g., [41,42,31]). Below are two of them, which are typical (cf. [42, Examples 2.1(a) and 2.1(b)]).

Example 4

Let q be the quasi-metric on R given by q ( x , x ) = 0 for all x R , and q ( x , y ) = y otherwise. Since q ( x , 0 ) = 0 for all x R , we deduce that ( R , q ) is a non- T 1 quasi-metric space. Now, let W : R × R R + defined by W ( x , y ) = y for all x , y R . Then, W is a Q -function on ( R , q ) [42, Example 1(a)], so it is a w-distance on ( R , q ) by Proposition 2. We shall show this fact directly for the sake of completeness. To this end, it suffices to verify condition (w2). Indeed, fix x R and let ( y n ) n N be a non-eventually constant sequence in R that T q -converges to some y R . Then, q ( y n , y ) 0 as n , and q ( y n , y ) = y eventually, so y = 0 . Hence, W ( x , y ) = 0 , and thus W ( x , ) is T q -lsc. We conclude that W is a w-distance on ( R , q ) .

Example 5

Let q be the quasi-metric on R given by q ( x , y ) = x y if y x , and q ( x , y ) = 2 ( y x ) otherwise. Clearly, ( R , q ) is a T 1 quasi-metric space. Now, let W : R × R R + be defined by W ( x , y ) = x y for all x , y R . Then, W is a Q -function on ( R , q ) [42, Example 1(b)], so it is a w-distance on ( R , q ) by Proposition 2. We shall show directly this fact for the sake of completeness. To this end, it suffices to verify condition (w2). Indeed, fix x R and let ( y n ) n N be a non-eventually constant sequence in R that T q -converges to some y R . Then, q ( y n , y ) 0 as n , so, by the definition of q , y n y 0 as n . Since W ( x , y ) W ( x , y n ) + y n y , we deduce that W ( x , ) is T q -lsc, so W is a w-distance on ( R , q ) .

We conclude this section with a novel example, based on the notion of a partial function, which will be used in illustrating our w -distance version of Caristi’s theorem.

It is interesting to point out that partial functions constitute an adequate instrument for modeling, through appropriate quasi-metrics, some typical procedures in symbolic computation as well as in complexity analysis of algorithms (see, e.g., [44,45]).

In our context, by a partial function, we mean a mapping f whose domain is an initial segment of N and takes values in R + . The set of all partial functions will be expressed as P F . Therefore, f P F if and only if there is k N such that f : { 1 , , k } R + . The number k is called the length of f and is denoted by ( f ) .

Example 6

On the set PF of partial functions, we define a relation PF as follows:

f PF g ( f ) = ( g ) and f ( n ) g ( n ) for all n { 1 , , ( f ) } .

It is clear that PF  is a partial order on PF (i.e., a reflexive, antisymmetric, and transitive relation).

Now, let q PF be the non- T 1 quasi-metric on PF given by q PF ( f , g ) = 0 if f PF g , and q PF ( f , g ) = 1 otherwise. It is well known, and easily checked, that the topology induced by q PF agrees with the famous Alexandroff topology on PF, that is, any topology where the intersection of an arbitrary family of open sets is open. Note that ( q PF ) s is the discrete metric on PF, i.e., ( q PF ) s ( f , g ) = 1 whenever f g , and hence the quasi-metric space ( PF , q PF ) is ( q PF ) -half complete because every Cauchy sequence in ( PF , q PF ) is eventually constant.

Let f 0 be the element of PF such that ( f 0 ) = 1 and f 0 ( 1 ) = 1 .

Define a function W PF : PF × PF R + as follows:

W PF ( f 0 , f 0 ) = 0 and W PF ( f , g ) = ( g ) otherwise.

We are going to show that W PF is a w -distance on ( PF , q PF ) , i.e., that it satisfies conditions (w1), (w2) and (w3). Indeed,

For (w1), let f , g , h PF . Since W PF ( f , g ) = W PF ( h , g ) , we immediately obtain that W PF ( f , g ) W PF ( f , h ) + W PF ( h , g ) .

For (w2), fix f PF and let ( g j ) j N be a sequence in PF that T ( q PF ) -converges to a g PF . Then, q PF ( g j , g ) 0 as j , so there is j 0 N such that q ( g j , g ) = 0 for all j j 0 . This implies that g j PF g , and hence, ( g j ) = ( g ) for all j j 0 . If f = g = f 0 , we have W PF ( f , g ) = 0 . Otherwise, we obtain W PF ( f , g ) = W PF ( f , g j ) for all j j 0 . Consequently, W PF ( f , ) is T ( q PF ) -lsc.

For (w3), fix ε > 0 . Put δ = min { 1 / 2 , ε } . Let f , g , h P F such that W PF ( f , g ) δ and W PF ( f , h ) δ . Then, f = g = h = f 0 , so q PF ( f , g ) = 0 ε .

4 Main results

The following characterization of q -right complete quasi-metric spaces is an adaptation of [26, Theorem 2] to our context.

Theorem 7

For a quasi-metric space ( X , q ) , the following statements are equivalent.

  1. ( X , q ) is q -right complete.

  2. If T is a self-mapping T of X such that there is a T q -nearly lsc function ϕ : X R + fulfilling, for every x X ,

    q ( x , T x ) ϕ ( x ) ϕ ( T x ) ,

    then, there exists u X satisfying ϕ ( u ) = ϕ ( T u ) .

Remark 8

We recall that, according to [26], given a quasi-metric space ( X , q ) , a function f : X R is T q -nearly lsc provided that whenever ( x n ) n N is a sequence of distinct points in X that T q -converges to some x X , we have f ( x ) liminf n f ( x n ) . Furthermore, the notions of T q -nearly lsc and T q -lsc coincide whenever ( X , q ) is a T 1 quasi-metric space.

Note that if in the preceding theorem ( X , q ) is a T 1 quasi-metric space, then u is a fixed point of T because from ϕ ( u ) = ϕ ( T u ) , we deduce that q ( u , T u ) = 0 , so u = T u [46, Theorem 2.12]. However, the following modification of [26, Example 2] provides an instance of a self-mapping T of a non- T 1 quasi-metric space that has no fixed points but for which there is a function ϕ : X R satisfying the conditions of (2) in the preceding theorem.

Example 9

Let X be the set of all ordinals less than the first uncountable ordinal number ω 1 . Consider the non- T 1 quasi-metric q on X given by q ( x , y ) = 0 if x y , and q ( x , y ) = 1 otherwise. It is clear that ( X , q ) is q -right complete because every left Cauchy sequence ( x n ) n N is T q -convergent to x sup { x n : n N } . Now consider the self-mapping of X given by T x = x + 1 for all x X . Then, T has no fixed points but one has q ( x , T x ) = 0 = ϕ ( x ) ϕ ( T x ) , for all x X , where ϕ ( x ) = 0 for all x X .

Our next theorem shows that the use of w -distances instead of the quasi-metric q provides two important advantages with respect to the part ( 1 ) ( 2 ) in Theorem 7. By one hand, the result remains valid for the more general class of q -half complete quasi-metric spaces, and, on the other hand, the existence of fixed point is guaranteed.

Definition 10

Let ( X , q ) be a quasi-metric space. A self-mapping T of X is called a W -Caristi mapping (on ( X , q ) ) if there exist a w -distance W on ( X , q ) and a T q -lsc function ϕ : X R + such that

W ( x , T x ) ϕ ( x ) ϕ ( T x ) ,

for all x X .

Before to establish our w -distance version of Caristi’s theorem, we give an auxiliary lemma which will help us to simplify its proof. (As usual, given a [non-empty] set X , the family of all non-empty subsets of X will be denoted by 2 X .)

Lemma 11

Let X be a (non-empty) set, : X 2 X a multivalued mapping, and ϕ a function from X to R + . Then, for each x X , there is a sequence ( x n ) n N 0 in X such that x 0 = x , x n + 1 x n , and

ϕ ( x n + 1 ) < 2 n + inf ϕ ( x n )

for all n N 0 .

If, in addition, there is a function W : X × X R + satisfying the triangle inequality and verifying

W ( x n , x n + 1 ) ϕ ( x n ) ϕ ( x n + 1 )

for all n N 0 , then, for each δ > 0 , there is n δ N 0 such that

W ( x n , x m ) < δ ,

whenever m > n n δ .

Proof

Let x X . Put x 0 = x . Since x 0 , there exists x 1 x 0 such that ϕ ( x 1 ) < 1 + inf ϕ ( x 0 ) .

Analogously, there exists x 2 x 1 such that ϕ ( x 2 ) < 2 1 inf ϕ ( x 1 ) .

Thus, we inductively deduce the existence of a sequence ( x n ) n N 0 in X such that x n + 1 x n and ϕ ( x n + 1 ) < 2 n + inf ϕ ( x n ) , for all n N 0 .

Now, suppose that there is a function W : X × X R + satisfying the triangle inequality and verifying W ( x n , x n + 1 ) ϕ ( x n ) ϕ ( x n + 1 ) , for all n N 0 .

Then, ( ϕ ( x n ) ) n N 0 is a non-increasing sequence in R + , and hence, it is a Cauchy sequence in R + when endowed with the usual metric. Consequently, given δ > 0 , there is n δ N 0 such that ϕ ( x n ) ϕ ( x m ) < δ , for all n , m n δ .

Since W satisfies the triangle inequality, we deduce that

W ( x n , x m ) k = n m 1 W ( x k , x k + 1 ) k = n m 1 ( ϕ ( x k ) ϕ ( x k + 1 ) ) = ϕ ( x n ) ϕ ( x m ) < δ ,

whenever m > n n δ .□

Theorem 12

Every W-Caristi mapping on a q -half complete quasi-metric space ( X , q ) has a fixed point.

Proof

Let T be a W -Caristi mapping on a q -half complete quasi-metric space ( X , q ) . Then, there exist a w -distance W on ( X , q ) and a T q -lsc function ϕ : X R + such that

W ( x , T x ) ϕ ( x ) ϕ ( T x )

for all x X .

Define a multivalued mapping : X 2 X by

x = { y X : W ( x , y ) ϕ ( x ) ϕ ( y ) }

for all x X .

Note that is well-defined because T x x , and thus x 2 X for all x X .

Fix now an x X . By the first part of Lemma 11, there is a sequence ( x n ) n N 0 in X such that x 0 = x , x n + 1 x n and ϕ ( x n + 1 ) < 2 n + inf ϕ ( x n ) , for all n N 0 .

Since x n + 1 x n , it follows from the definition of the multivalued mapping that W ( x n , x n + 1 ) ϕ ( x n ) ϕ ( x n + 1 ) , for all n N 0 .

Therefore, by the second part of Lemma 11, we obtain that, for each δ > 0 , there is n δ N 0 such that W ( x n , x m ) < δ , whenever m > n n δ .

Choose an arbitrary ε > 0 . Let δ δ ( ε ) for which condition (w3) is fulfilled. Then, for every j , k > n δ , we have W ( x n δ , x j ) < δ and W ( x n δ , x k ) < δ , so q ( x j , x k ) ε and q ( x k , x j ) ε .

This implies that ( x n ) n N 0 is a Cauchy sequence in the metric space ( X , q s ) . Since ( X , q ) is q -sequentially complete, there exists u X such that q ( x n , u ) 0 as n .

Next, we shall prove that w ( u , T u ) = 0 . To this end, we shall show four claims.

Claim 1. W ( x n , u ) 0 as n .

Indeed, given δ > 0 , there is n δ N 0 such that W ( x n , x m ) < δ , whenever m > n n δ . Fix n n δ . By condition (w2), there is m > n such that W ( x n , u ) < δ + W ( x n , x m ) . Hence,

W ( x n , u ) < 2 δ

for all n n δ .

Claim 2. u n N 0 x n .

Indeed, fix n N 0 . Choose an arbitrary δ > 0 . By Claim 1 and the fact that ϕ is T q -lsc, we deduce the existence of an m > n such that W ( x m , u ) < δ and ϕ ( u ) ϕ ( x m ) < δ .

Taking into account that x m x n , we obtain

W ( x n , u ) W ( x n , x m ) + W ( x m , u ) ϕ ( x n ) ϕ ( x m ) + δ ϕ ( x n ) ϕ ( u ) + 2 δ .

Since δ is arbitrary, we conclude that W ( x n , u ) ϕ ( x n ) ϕ ( u ) , so u x n .

Claim 3. ϕ ( u ) = inf n N 0 ϕ ( x n ) .

Indeed, by Claim 2, u x n for all n N 0 . So, by the definition of , ϕ ( u ) ϕ ( x n ) for all n N 0 . Thus, ϕ ( u ) inf n N 0 ϕ ( x n ) .

On the other hand, we have

ϕ ( x n + 1 ) < 2 n + inf ϕ ( x n ) 2 n + ϕ ( u )

for all n N 0 , and hence inf n N 0 ϕ ( x n ) ϕ ( u ) .

Claim 4. ϕ ( T u ) = inf n N 0 ϕ ( x n ) .

Indeed, since T is W -Caristi mapping, we have T u u , and, by Claim 2, we also have that u x n for all n N 0 . Therefore,

W ( x n , T u ) W ( x n , u ) + W ( u , T u ) ϕ ( x n ) ϕ ( T u )

for all n N 0 , so that T u n N 0 x n . As in the proof of Claim 2, we obtain that ϕ ( T u ) inf n N 0 ϕ ( x n ) , and also

ϕ ( x n + 1 ) < 2 n + inf ϕ ( x n ) 2 n + ϕ ( T u )

for all n N 0 , so inf n N 0 ϕ ( x n ) ϕ ( T u ) .

From Claims 3 and 4, we have that ϕ ( u ) = ϕ ( T u ) , and, consequently, w ( u , T u ) = 0 .

Finally, we prove that u = T u . Indeed, by Claim 1, the triangle inequality, and the fact that w ( u , T u ) = 0 , we deduce that W ( x n , T u ) 0 as n .

Now, choose an arbitrary ε > 0 . Let δ > 0 for which condition (w3) is fulfilled. Take n N 0 such that W ( x n , u ) δ and W ( x n , T u ) δ . From condition (w3), it follows that q s ( u , T u ) ε . Hence, u = T u , and thus, u is a fixed point of T . Furthermore, W ( u , u ) = 0 .□

We illustrate the preceding with the next (promised) example.

Example 13

Let ( PF , q PF ) be the quasi-metric space of Example 6, and let T be the self-mapping of PF defined as follows:

For each f P F with ( f ) 2 , T f is the only element of PF such that ( T f ) = ( f ) 1 and T f ( n ) = f ( n ) for all n { 1 , , ( T f ) } , and for each f P F with ( f ) = 1 , put T f = f 0 .

We are going to prove that T is a W PF -Caristi mapping on ( PF , q PF ) , where W PF is the w -distance constructed in Example 6.

Indeed, define a function ϕ : P F R + by ϕ ( f ) = ( ( f ) ) 2 for all f P F \ { f 0 } , and ϕ ( f 0 ) = 0 .

Clearly, ϕ is T ( q PF ) -lsc. Indeed, let ( g j ) j N be a sequence in PF that T ( q PF ) -converges to a g PF \ { f 0 } . Then, q PF ( g j , g ) 0 as j , so there is j 0 N such that q ( g j , g ) = 0 for all j j 0 . This implies that g j PF g , and hence ( g j ) = ( g ) for all j j 0 , so ϕ ( g ) = ϕ ( g j ) , for all j j 0 .

Since W PF ( f 0 , T f 0 ) = W PF ( f 0 , f 0 ) = 0 , we obtain W PF ( f 0 , T f 0 ) = ϕ ( f 0 ) ϕ ( T f 0 ) .

Now let f P F \ { f 0 } . If ( f ) 2 , we obtain

W PF ( f , T f ) = ( T f ) = ( f ) 1 < 2 ( f ) 1 = ( ( f ) ) 2 ( ( f ) 1 ) 2 = ϕ ( f ) ϕ ( T f ) ,

and if ( f ) = 1 , we obtain

W PF ( f , T f ) = W PF ( f , f 0 ) = ( f 0 ) = 1 = ( ( f ) ) 2 = ϕ ( f ) ϕ ( T f ) .

We have shown that T is a w PF -Caristi mapping on the ( q PF ) -half complete quasi-metric space ( PF , q PF ) . Hence, we can apply Theorem 12 to conclude that T has a fixed point. In fact f 0 is the unique fixed point of T .

Finally, we shall show that ( PF , q PF ) is not ( q PF ) -right complete, and thus we cannot apply Theorem 7.

Indeed, consider the sequence ( g j ) j N in PF such that ( g j ) = 1 and g j ( 1 ) = j for all j N . Since q PF ( g i , g j ) = 0 whenever i j , we deduce that ( g j ) j N is a ( q PF ) -right Cauchy sequence in ( PF , q PF ) . Suppose that there is g PF such that q PF ( g j , g ) 0 as j . Then, there is j 0 N such that q PF ( g j , g ) = 0 for all j j 0 . Hence, ( g j ) = ( g ) = 1 and g j ( 1 ) g ( 1 ) for all j j 0 , so j g ( 1 ) for all j j 0 , a contradiction. Consequently, ( PF , q PF ) is not ( q PF ) -right complete.

We conclude this section with our main result.

Theorem 14

A quasi-metric space ( X , q ) is q -half complete if and only if every W -Caristi mapping on it has a fixed point.

Proof

The “only if” part follows from Theorem 12.

To prove the “if” part suppose that ( X , q ) is not q -half complete. Then, there exists a non- τ q -convergent sequence ( x n ) n N , which is a Cauchy sequence in the metric space ( X , q s ) .

Therefore, for each n N , we can inductively find a k n N such that k 1 > 1 , k n + 1 > max { k n , n + 1 } , and q s ( x i , x j ) < 2 n for all i , j k n . So, in particular, q s ( x k n , x k m ) < 2 n whenever m n .

Put F { x k n : n N } and define a function W : X × X R + by W ( x , y ) = q s ( x , y ) if x , y F and W ( x , y ) = 1 otherwise.

We check that W is a w -distance on ( X , q ) .

We first note that W ( x , y ) < 1 / 2 for all x , y F .

Condition (w1) is clearly fulfilled.

For (w2), fix x X and let ( y n ) n N be a sequence in X and y X such that q ( y n , y ) 0 as n . If there is a subsequence ( z n ) of ( y n ) such that z n F for all n N , we deduce, by the triangle inequality, that q ( x n k , y ) 0 as n . Since ( x n ) n N is a Cauchy sequence in ( X , q s ) , we deduce that q ( x n , y ) 0 as n , a contradiction.

Consequently, there is n 0 N such that y n X \ F for all n n 0 . Thus, W ( x , y n ) = 1 for all n n 0 . Since W ( x , y ) 1 , we conclude that q ( x , ) is T q -lsc.

Finally, for (w3), choose an arbitrary ε > 0 . Put δ = min { 1 / 2 , ε / 2 } . Let x , y , z X such that W ( x , y ) δ and W ( x , z ) δ . Then, W ( x , y ) 1 / 2 and W ( x , z ) 1 / 2 , so x , y , z F . Therefore, q s ( x , y ) δ ε / 2 and q s ( x , z ) δ ε / 2 . By the triangle inequality we conclude that q s ( y , z ) ε , and thus q ( y , z ) ε .

Now define a function ϕ : X R + and a self-mapping T of X as follows:

ϕ ( x k n ) = 2 ( n 1 ) for all n N ,

ϕ ( x ) = 2 for all x X \ F ,

T x k n = x k n + 1 for all n N ,

and

T x = x k 1 for all x X \ F .

Obviously T has no fixed points. We shall show that, nevertheless, T is a W -Caristi mapping on ( X , q ) (with respect to the w -distance W and the function ϕ defined earlier).

We first check that ϕ is T q -lsc. As previously mentioned, let ( y n ) n N be a sequence in X and y X such that q ( y n , y ) 0 as n . If there is a subsequence ( z n ) of ( y n ) such that z n F for all n N , we deduce that q ( x n , y ) 0 as n , a contradiction.

Consequently, there is n 0 N such that y n X \ F for all n n 0 . Thus, ϕ ( y n ) = 2 for all n n 0 . Since ϕ ( y ) 2 , we conclude that ϕ is T q -lsc.

Now, let x X . If x F , we obtain x x k n for some n N . Therefore,

W ( x , T x ) = W ( x k n , x k n + 1 ) = q s ( x k n , x k n + 1 ) < 2 n = ϕ ( x k n ) ϕ ( x k n + 1 ) = ϕ ( x ) ϕ ( T x ) .

If x X \ F we obtain

W ( x , T x ) = W ( x , x k 1 ) = 1 = ϕ ( x ) ϕ ( x k 1 ) = ϕ ( x ) ϕ ( T x ) .

Thus, we have reached a contradiction that concludes the proof.□

5 An application to G-metric spaces

In this section, we apply Theorem 7 to obtain a characterization of complete G -metric spaces.

The concept of a G -metric space was introduced and analyzed by Mustafa and Sims in [47] motivated by the existence of several mistakes in the study of the topological structure of the so-called D -metric spaces. In fact, Mustafa-Sims’ study constituted the starting point for the development of an intensive research in fixed point theory for this kind of spaces and other related ones (cf. [48,49,50, 51,52,53, 54,55] and references therein). In particular, our basic reference for G -metric spaces will be [49, Chapter 3].

Let us recall that a G -metric on a set X is a function G : X × X × X R + that satisfies the following conditions for any x , y , z , a X :

(gm1) G ( x , y , z ) = 0 if x = y = z .

(gm2) G ( x , x , y ) > 0 if x y .

(gm3) G ( x , x , y ) G ( x , y , z ) if y z .

(gm4) G ( x , y , z ) = G ( x , z , y ) = G ( y , z , x ) = (symmetry in all 3).

(gm5) G ( x , y , z ) G ( x , a , a ) + G ( a , y , z ) (rectangle inequality).

By a G -metric space, we mean a pair ( X , G ) such that X is a set and G is a G -metric on X .

In [49, p. 34–35], one can find numerous instances of G -metric spaces.

The following properties may be found in [49, Chapter 3].

Each G -metric G on a set X induces a topology T G on X , which has as a base the family of open balls { B G ( x , ε ) : x X , ε > 0 } , where B G ( x , ε ) = { y X : G ( x , y , y ) < ε } for all x X and ε > 0 . Furthermore, the topological space ( X , T G ) is metrizable.

A G -metric space ( X , G ) is complete provided that every G -Cauchy sequence is T G -convergent, where a sequence ( x n ) n N in X is said to be G -Cauchy if for each ε > 0 , there is n 0 N such that G ( x n , x m , x k ) < ε for all n , m , k n 0 .

Given a G -metric space ( X , G ) , the function q G : X × X R + given by q G ( x , y ) = G ( x , y , y ) for all x , y X is a T 1 quasi-metric on X . (This quasi-metric is denoted by q G in [49].)

Let ( X , G ) be a G -metric space. From [49, Lemma 3.3.1], we deduce the following important properties:

(P1) The topologies T G , T q G , and T ( q G ) coincide on X .

(P2) ( X , G ) is complete if and only if ( X , q G ) is ( q G ) -half complete.

Saadati et al. introduced in [56] a G -metric version of the notion of w -distance with the aim of obtaining fixed point results for complete ordered G -metric spaces. We modify the notion given in [56] as follows:

Definition 15

Let ( X , G ) be a G -metric space. We say that a function W G : X × X R + is a w G -distance on ( X , G ) if it verifies the following conditions:

( wG 1 ) W G ( x , y , z ) W G ( x , a , a ) + W G ( a , y , z ) , for all x , y , z , a X .

( wG 2 ) For each x X , W G ( x , , ) : X × X R + is lsc in the sense that if ( y n ) n N is a sequence in X that T G -converges to some y X , then for each ε > 0 , W G ( x , y , y ) < ε + W G ( x , y n , y n ) , eventually.

( wG 3 ) For each ε > 0 , there is δ > 0 such that W G ( x , y , y ) δ and W G ( x , z , z ) δ imply G ( y , z , z ) ε .

Remark 16

Note that by exchanging y with z in condition ( wG 3 ) , we also have W G ( z , y , y ) ε .

Remark 17

It is not hard to check that every G -metric G on a set X is a w G -metric on ( X , G ) . In fact, condition ( wG 1 ) follows directly from condition (gm5). Condition ( wG 2 ) follows from conditions (gm4) and (gm5) and the fact that G ( y , y , y n ) 0 as n , whenever the sequence ( y n ) n N T G -converges to y . Finally, to show condition ( wG 3 ) choose an ε > 0 and suppose that G ( x , y , y ) ε / 3 and G ( x , z , z ) ε / 3 . Then, G ( y , z , z ) G ( y , x , x ) + G ( x , z , z ) 2 G ( y , y , x ) + G ( x , z , z ) ε .

As an immediate consequence of the preceding remark, we obtain that if ( X , G ) is a G -metric space, the quasi-metric q G is a w -distance on ( X , q G ) .

Proposition 18

Let WG be a wG-distance on a G-metric space ( X , G ) . Then, the function w : X × X R + defined as w ( x , y ) = W G ( x , y , y ) for all x , y X , is a w-distance on the quasi-metric space ( X , q G ) .

Proof

Let x , y , z X . We proceed to check the conditions of the definition of a w -distance.

(w1): From condition ( wG 1 ), we obtain

w ( x , y ) = W G ( x , y , y ) W G ( x , z , z ) + W G ( z , y , y ) = w ( x , z ) + w ( z , y ) .

(w2): Let ( y n ) n N be a sequence in X that T ( q G ) -converges to some y X . Then, ( y n ) n N T G -converges to y by property (P1). Given ε > 0 , it follows from condition ( wG 1 ) that

w ( x , y ) = W G ( x , y , y ) < ε + W G ( x , y n , y n ) = ε + w ( x , y n )

eventually.

(w3): Given ε > 0 , suppose that w ( x , y ) δ and w ( x , z ) δ , where this δ is the one associated with ε in condition ( wG 3 ) . Then, we have W G ( x , y , y ) δ and W G ( x , z , z ) δ . Therefore, W G ( y , z , z ) ε , i.e., w ( y , z ) ε .□

Proposition 19

Let ( X , G ) be a G-metric space and let q G be the quasi-metric induced by G . If w is a w-distance on ( X , q G ) , then the function W G : X × X R + defined by W G ( x , y , z ) = w ( x , y ) for all x , y , z X , is a w G -distance on ( X , G ) .

Proof

Let x , y , z , a X . We proceed to check the conditions of the definition of a w G -distance.

( wG 1 ) : Since, by definition, W G ( x , y , z ) = w ( x , y ) , W G ( x , a , a ) = w ( x , a ) , and W G ( a , y , z ) = w ( a , y ) , from condition (w1), we obtain

W G ( x , y , z ) W G ( x , a , a ) + W G ( a , y , z ) .

( wG 2 ) : Let ( y n ) n N be a sequence in X that T G -converges to some y X . By property (P1) it T ( q G ) -converges to y . Thus, by condition (w2), given ε > 0 we have, in particular, w ( x , y ) < ε + w ( x , y n ) eventually. Since, by definition, W G ( x , y , y ) = w ( x , y ) and W G ( x , y n , y n ) = w ( x , y n ) , we deduce that

W G ( x , y , y ) < ε + W G ( x , y n , y n )

eventually.

( wG 3 ): Given ε > 0 , suppose that W G ( x , y , y ) δ and W G ( x , z , z ) δ , where this δ is the one associated with ε in condition ( wG 3 ) . Since, by definition, W G ( x , y , y ) = w ( x , y ) and W G ( x , z , z ) = w ( x , z ) , we deduce that q G ( y , z ) ε , i.e., G ( y , z , z ) ε . (Note that we also obtain q G ( z , y ) ε , i.e., G ( z , y , y ) ε .)□

Remark 20

It is easy to construct w G -distances. For instance, let ( X , d ) be a metric space. Then, the function G : X × X × X R + given by

G ( x , y , z ) = d ( x , y ) + d ( x , z ) + d ( y , z )

for all x , y , z X is a G -metric on X (see [47]). Since q G is a w -distance on ( X , q G ) and q G ( x , y ) = G ( x , y , y ) = 2 d ( x , y ) , we deduce from Proposition 19 that the function W G defined by W G ( x , y , z ) = 2 d ( x , y ) for all x , y , z X is a w G -distance on ( X , G ) .

Definition 21

Let ( X , G ) be a G -metric space. A self-mapping T of X is said to be a W G -Caristi mapping (on ( X , G ) ) if there exist a w G -distance W G on ( X , G ) and a T G -lsc function ϕ : X R + such that

W G ( x , T x , T x ) ϕ ( x ) ϕ ( T x )

for all x X .

Theorem 22

A G-metric space ( X , G ) is complete if and only if every WG-Caristi mapping on it has a fixed point.

Proof

Let T be a W G -Caristi mapping on the complete G -metric space ( X , G ) . By property (P1) and Proposition 18, we deduce that T is a W -Caristi mapping on the quasi-metric space ( X , q G ) , which is q -half complete by property (P2). Therefore, T has a fixed point by Theorem 12.

Conversely, let T be a W -Caristi mapping on the quasi-metric space ( X , q G ) . By property (P1) and Proposition 19, we deduce that T is a W G -Caristi mapping on ( X , G ) , so, by hypothesis, it has a fixed point. Hence, ( X , q G ) is q -half complete by Theorem 14. We conclude that ( X , G ) is complete by property (P2).□



Acknowledgement

The authors thank the reviewers for their careful reading of the article and for their suggestions, which have contributed to improving it. Thanks also to one of them for calling our attention about the references [27].

  1. Conflict of interest: Prof. Erdal Karapinar is one of the Guest Editors of the Special Issue on Fixed Point Theory and Applications to Various Differential/Integral Equations but was not involved in the review process of this paper.

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Received: 2022-07-25
Revised: 2022-10-02
Accepted: 2022-10-14
Published Online: 2022-12-13

© 2022 the author(s), published by De Gruyter

This work is licensed under the Creative Commons Attribution 4.0 International License.

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