Common Fixed Point Results Using Generalized Altering Distances on Orbitally Complete Ordered Metric Spaces
Abstract
We prove the existence of common fixed points for three relatively asymptotically regular mappings defined on an orbitally complete ordered metric space using orbital continuity of one of the involved maps. We furnish a suitable example to demonstrate the validity of the hypotheses of our results.
1. Introduction and Preliminaries
Browder and Petryshyn introduced the concept of asymptotic regularity of a self-map at a point in a metric space.
Definition 1.1 (see [1].)A self-map 𝒯 on a metric space (𝒳, d) is said to be asymptotically regular at a point x ∈ 𝒳 if lim n→∞d(𝒯nx, 𝒯n+1x) = 0.
Recall that the set 𝒪(x0; 𝒯) = {𝒯nx0 : n = 0,1, 2, …} is called the orbit of the self-map 𝒯 at the point x0 ∈ 𝒳.
Definition 1.2 (see [2].)A metric space (𝒳, d) is said to be 𝒯-orbitally complete if every Cauchy sequence contained in 𝒪(x; 𝒯) (for some x in 𝒳) converges in 𝒳.
Here, it can be pointed out that every complete metric space is 𝒯-orbitally complete for any 𝒯, but a 𝒯-orbitally complete metric space need not be complete.
Definition 1.3 (see [1].)A self-map 𝒯 defined on a metric space (𝒳, d) is said to be orbitally continuous at a point z in 𝒳 if for any sequence {xn} ⊂ 𝒪(x; 𝒯) (for some x ∈ 𝒳), xn → z as n → ∞ implies 𝒯xn → 𝒯z as n → ∞.
Clearly, every continuous self-mapping of a metric space is orbitally continuous, but not conversely.
Sastry et al. [3] extended the above concepts to two and three mappings and employed them to prove common fixed point results for commuting mappings. In what follows, we collect such definitions for three maps.
Definition 1.4 (see [3].)Let 𝒮, 𝒯, ℛ be three self-mappings defined on a metric space (𝒳, d).
- (1)
If for a point x0 ∈ 𝒳, there exists a sequence {xn} in 𝒳 such that ℛx2n+1 = 𝒮x2n, ℛx2n+2 = 𝒯x2n+1, n = 0,1, 2, …, then the set 𝒪(x0; 𝒮, 𝒯, ℛ) = {ℛxn : n = 1,2, …} is called the orbit of (𝒮, 𝒯, ℛ) at x0.
- (2)
The space (𝒳, d) is said to be (𝒮, 𝒯, ℛ)-orbitally complete at x0 if every Cauchy sequence in 𝒪(x0; 𝒮, 𝒯, ℛ) converges in 𝒳.
- (3)
The map ℛ is said to be orbitally continuous at x0 if it is continuous on 𝒪(x0; 𝒮, 𝒯, ℛ).
- (4)
The pair (𝒮, 𝒯) is said to be asymptotically regular (in short a.r.) with respect to ℛ at x0 if there exists a sequence {xn} in 𝒳 such that ℛx2n+1 = 𝒮x2n, ℛx2n+2 = 𝒯x2n+1, n = 0,1, 2, …, and d(ℛxn, ℛxn+1) → 0 as n → ∞.
On the other side, Khan et al. [4] introduced the notion of an altering distance function, which is a control function that alters distance between two points in a metric space. This notion has been used by several authors to establish fixed point results in a number of subsequent works, some of which are noted in [5–9]. In [5], Choudhury introduced the concept of a generalized altering distance function in three variables which was further generalized by Rao et al. [10] to four variables and is defined as follows.
Definition 1.5 (see [10].)A function ψ : [0, +∞) 4 → [0, +∞) is said to be a generalized altering distance function if
- (i)
ψ is continuous,
- (ii)
ψ is nondecreasing in each variable,
- (iii)
ψ(t1, t2, t3, t4) = 0⇔t1 = t2 = t3 = t4 = 0.
On the other hand, fixed point theory has developed rapidly in metric spaces endowed with a partial ordering. The first result in this direction was given by Ran and Reurings [11] who presented its applications to matrix equations. Subsequently, Nieto and Rodríguez-López [12] extended this result for nondecreasing mappings and applied it to obtain a unique solution for a first order ordinary differential equation with periodic boundary conditions. Thereafter, several authors obtained many fixed point theorems in ordered metric spaces. For more details see [13–20] and the references cited therein.
In this paper, an attempt has been made to derive some common fixed point theorems for three relatively asymptotically regular mappings defined on an orbitally complete ordered metric space, using orbital continuity of one of the involved maps and conditions involving a generalized altering distance function. The presented theorems generalize, extend, and improve some recent results given in [7, 14, 21, 22]. In the hypotheses, we have considered the space as not necessarily complete, the maps ℛ, 𝒮, and 𝒯 as not necessarily continuous and the range of 𝒮 and 𝒯 may not be contained in the range of ℛ.
2. Results
2.1. Notations and Definitions
First, we introduce some further notations and definitions that will be used later.
If (𝒳, ≼) is a partially ordered set, then x, y ∈ 𝒳 are called comparable if x≼y or y≼x holds. A subset 𝒦 of 𝒳 is said to be well ordered if every two elements of 𝒦 are comparable. If 𝒯 : 𝒳 → 𝒳 is such that, for x, y ∈ 𝒳, x≼y implies 𝒯x≼𝒯y, then the mapping 𝒯 is said to be nondecreasing.
Definition 2.1. Let (𝒳, ≼) be a partially ordered set and 𝒮, 𝒯 : 𝒳 → 𝒳.
- (1)
[23] The pair (𝒮, 𝒯) is called weakly increasing if 𝒮x≼𝒯𝒮x and 𝒯x≼𝒮𝒯x for all x ∈ 𝒳.
- (2)
[24] The pair (𝒮, 𝒯) is called partially weakly increasing if 𝒮x≼𝒯𝒮x for all x ∈ 𝒳.
- (3)
[24] The mapping 𝒮 is called a weak annihilator of 𝒯 if 𝒮𝒯x≼x for all x ∈ 𝒳.
- (4)
[24] The mapping 𝒮 is called dominating if x≼𝒮x for each x ∈ 𝒳.
Note that none of two weakly increasing mappings need to be nondecreasing. There exist some examples to illustrate this fact in [23]. Obviously, the pair (𝒮, 𝒯) is weakly increasing if and only if the ordered pairs (𝒮, 𝒯) and (𝒯, 𝒮) are partially weakly increasing. Following is an example of an ordered pair (𝒮, 𝒯) which is partially weakly increasing but not weakly increasing.
Example 2.2 (see [24].)Let 𝒳 = [0,1] be endowed with usual ordering.
- (1)
Let 𝒮, 𝒯 : 𝒳 → 𝒳 be defined by 𝒮x = x2 and . Clearly, (𝒮, 𝒯) is partially weakly increasing. But for x ∈ (0,1) implies that (𝒯, 𝒮) is not partially weakly increasing.
- (2)
Let 𝒮, 𝒯 : 𝒳 → 𝒳 be defined by 𝒮x = x2 and 𝒯x = x3. Obviously, 𝒮𝒯x = x6 ≤ x for all x ∈ 𝒳. Thus 𝒮 is a weak annihilator of 𝒯.
- (3)
Let 𝒮 : 𝒳 → 𝒳 be defined by . Since for all x ∈ 𝒳, 𝒮 is a dominating map.
Definition 2.3 (see [25], [26].)Let (𝒳, d) be a metric space and f, g : 𝒳 → 𝒳. The mappings f and g are said to be compatible if lim n→∞d(fgxn, gfxn) = 0, whenever {xn} is a sequence in 𝒳 such that lim n→∞ fxn = lim n→∞ gxn = t for some t ∈ 𝒳.
Definition 2.4. Let 𝒳 be a nonempty set. Then (𝒳, d, ≼) is called an ordered metric space if
- (i)
(𝒳, d) is a metric space,
- (ii)
(𝒳, ≼) is a partially ordered set.
2.2. Main Results
The first main result is as follows.
Theorem 2.5. Let (𝒳, d, ≼) be an ordered metric space. Let 𝒮, 𝒯, ℛ : 𝒳 → 𝒳 be given mappings satisfying
- (i)
(𝒮, 𝒯) is a.r. with respect to ℛ at x0 ∈ 𝒳;
- (ii)
𝒳 is (𝒮, 𝒯, ℛ)-orbitally complete at x0;
- (iii)
(ℛ, 𝒮) and (ℛ, 𝒯) are partially weakly increasing;
- (iv)
𝒮 and 𝒯 are dominating maps;
- (v)
𝒮 and 𝒯 are weak annihilators of ℛ;
- (vi)
for a nondecreasing sequence {xn}, xn≼yn for all n and yn → u as n → ∞ imply that xn≼u for all n ∈ ℕ.
- (a)
𝒮 and ℛ are compatible; 𝒮 or ℛ is orbitally continuous at x0 or
- (b)
𝒯 and ℛ are compatible; 𝒯 or ℛ is orbitally continuous at x0.
Proof. Since (𝒮, 𝒯) is a.r. with respect to ℛ at x0 in 𝒳, there exists a sequence {xn} in 𝒳 such that
From (2.5), it will be sufficient to prove that {ℛx2n} is a Cauchy sequence. We proceed by negation and suppose that {ℛx2n} is not a Cauchy sequence. Then, there exists ε > 0 for which we can find two sequences of positive integers {m(i)} and {n(i)} such that for all positive integers i,
Finally, we prove the existence of a common fixed point of the three mappings 𝒮, 𝒯, and ℛ.
We have
Similarly, the result follows when condition (b) holds.
Now, suppose that the set of common fixed points of 𝒮, 𝒯, and ℛ in is well ordered. We claim that it cannot contain more than one point. Assume to the contrary that 𝒮u = 𝒯u = ℛu = u and 𝒮v = 𝒯v = ℛv = v but u ≠ v. By supposition, we can replace x by u and y by v in (2.1) to obtain
Now, it is easy to state a corollary of Theorem 2.5 involving a contraction of integral type.
Corollary 2.6. Let 𝒮, 𝒯, and ℛ satisfy the conditions of Theorem 2.5, except that condition (2.1) is replaced by the following: there exists a positive Lebesgue integrable function u on ℝ+ such that for each ε > 0 and that
Remark 2.7. If we take
Other results could be derived for other choices of ψ1 and ψ2.
As consequences of Theorem 2.5, we may state the following corollaries.
Corollary 2.8. Let (𝒳, d, ≼) be an ordered metric space. Let 𝒯, ℛ : 𝒳 → 𝒳 be given mappings satisfying
- (i)
𝒯 is a.r. with respect to ℛ at x0;
- (ii)
𝒳 is (𝒯, ℛ)-orbitally complete at x0;
- (iii)
𝒯 or ℛ is orbitally continuous at x0;
- (iv)
(𝒯, ℛ) is partially weakly increasing;
- (v)
𝒯 is a dominating map;
- (vi)
𝒯 is a weak annihilator of ℛ;
- (vii)
𝒯 and ℛ are compatible.
Then 𝒯 and ℛ have a common fixed point. Moreover, the set of common fixed points of 𝒯 and ℛ in is well ordered if and only if it is a singleton.
Corollary 2.9. Let (𝒳, d, ≼) be an ordered metric space. Let 𝒯 : 𝒳 → 𝒳 be a mapping satisfying
- (i)
𝒯 is a.r. at some point x0 of 𝒳;
- (ii)
𝒳 is 𝒯-orbitally complete at x0;
- (iii)
𝒯 is a dominating map.
Then 𝒯 has a fixed point. Moreover, the set of fixed points of 𝒯 in is well ordered if and only if it is a singleton.
We present an example showing the usage of our results.
Example 2.10. Let the set 𝒳 = [0, +∞) be equipped with the usual metric d and the order defined by
Remark 2.11. It was shown by examples in [22] that (in similar situations)
- (1)
if the contractive condition is satisfied just on 𝒪(x0; 𝒮, 𝒯, ℛ), there might not exist a (common) fixed point;
- (2)
under the given hypotheses (common), fixed point might not be unique in the whole space 𝒳.
Acknowledgment
The authors thank the referees for their careful reading of the text and for suggestions that helped to improve the exposition of the paper. The second and third authors are thankful to the Ministry of Science and Technological Development of Serbia.