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Article

Fixed Circle and Fixed Disc Results for New Types of Θc-Contractive Mappings in Metric Spaces

by
Hayel N. Saleh
1,2,†,
Salvatore Sessa
3,*,†,
Waleed M. Alfaqih
4,†,
Mohammad Imdad
1,† and
Nabil Mlaiki
5,†
1
Department of Mathematics, Aligarh Muslim University, Aligarh 202002, India
2
Department of Mathematics, Taiz University, Taiz 6803, Yemen
3
Dipartimento di Architettura, Università degli Studi di Napoli Federico II, Via Toledo 402, 80134 Napoli, Italy
4
Department of Mathematics, Hajjah University, Hajjah 1729, Yemen
5
Department of Mathematics and General Sciences, Prince Sultan University, Riyadh 11586, Saudi Arabia
*
Author to whom correspondence should be addressed.
These authors contributed equally to this work.
Symmetry 2020, 12(11), 1825; https://doi.org/10.3390/sym12111825
Submission received: 9 September 2020 / Revised: 25 October 2020 / Accepted: 26 October 2020 / Published: 4 November 2020
(This article belongs to the Section Mathematics)

Abstract

:
In this manuscript, we introduce the notions of various types of Θ c -contractions for which we establish some fixed circle and fixed disc theorems in the setting of metric spaces. Some illustrative examples are also provided to support our results. Moreover, we present some fixed circle and fixed disc results of integral type contractive self-mappings, which generalize many results of invariance and transformations in the literature.

1. Introduction and Preliminaries

Metric fixed point theory is a very natural and well-developed branch of mathematical analysis which deals with the existence and uniqueness results for fixed points of the mappings defined on metric spaces. The source of this theory is the classical result due to Banach [1] which is known as the Banach contraction principle and states that every contraction mapping defined on a complete metric space ( Y , ξ ) admits a unique fixed point. Several authors extended and generalized this principle in various directions (for instance, see [2,3,4,5,6,7,8,9,10]). In this regard, Jleli and Samet [11] introduced an attractive class of auxiliary functions Θ : ( 0 , ) ( 1 , ) satisfying some suitable properties and utilized the same functions to prove some fixed point theorems concerning a new type of contractions called Θ -contractions (or JS-contractions).
The Banach contraction principle and its generalizations have been applied in various disciplines of mathematics, economics and engineering. One of the interesting applications of Banach contraction principle is to study the graph neural network model [12]. On the other hand, in the case that the mapping S defined on a metric space ( Y , ξ ) has more than one fixed point, the number of fixed points of an activation function used in a neural network is important (see [13] and the references therein). There exist some mappings that fix all points of a circle or a disc. These kind of mappings have some applications to neural networks (for instance, see [14]). For example, let C be the set of all complex numbers with the usual metric ξ ( z , w ) = | z w | , for all z , w C and consider S : C C to be defined by
S z = 1 z ¯ , i f z 0 ; 0 , i f z = 0 ,
where z ¯ is the conjugate of z. Then, S fixes all points of the circle C 0 , 1 = { z C : | z | = 1 } . It is worth pointing out that there exist some mappings which map the circle C z 0 , r to itself but do not fix all points of the circle C z 0 , r . For instance, let T be a self-mapping on C defined by
T z = 1 z , i f z 0 ; 0 , i f z = 0 .
Then, T ( C 0 , 1 ) = C 0 , 1 , but T does not fix all points of C 0 , 1 . In fact, the mapping T fixes only two points of the unit circle.
Natural and interesting problems were found through the investigations of the geometric properties of fixed points. In this context, the fixed circle and fixed disc problem have been studied in metric and generalized metric spaces via different contractive conditions (see [15,16,17,18,19,20,21,22,23,24]). For example, in [15], some fixed circle results were proved using the Caristi type contraction on a metric space. Using Wardowski’s technique and some classical contractive conditions, some fixed circle theorems were obtained in [19]. In [20,21], the fixed circle problem was studied in the setting of S-metric spaces. In [16], some fixed disc theorems were obtained using several types of contractive conditions on rectangular metric space.
Motivated by the above, we aim to present in this paper some fixed circle (disc) results for some types of contraction self-mappings, namely Θ c -contractions, Ćirić type Θ c -contractions, Hardy–Rogers type Θ c -contractions and Khan type Θ c -contractions in the setting of metric spaces by using JS technique. Furthermore, we establish some fixed circle (disc) results of integral type contractive self-mappings. To do this, we use the notion of Θ -function introduced by Jleli and Samet [11]. The function Θ : ( 0 , ) ( 1 , ) is said to be a Θ -function, if the following conditions are satisfied:
(JS1)
Θ is nondecreasing;
(JS2)
for every sequence { α n } ( 0 , ) ,
lim n Θ ( α n ) = 1 lim n α n = 0 + ;
(JS3)
there exist λ ( 0 , 1 ) and k ( 0 , ) such that lim α 0 + Θ ( α ) 1 α λ = k .
In the sequel, we adopt the following notations:
  • Ω 1 the class of all functions Θ which satisfy ( J S 1 ) .
  • Ω 1 , 2 , 3 the class of all functions Θ which satisfy ( J S 1 ) ( J S 3 ) .
Remark 1.
Observe that the auxiliary function Θ used in [11] satisfies the conditions ( J S ) 1 ( J S 3 ) , that is, Θ Ω 1 , 2 , 3 while the auxiliary function Θ used in the present paper need not to satisfies ( J S 2 ) and ( J S 3 ) , that is, Θ Ω 1 .
For a metric space ( Y , ξ ) , the two sets C z 0 , r = { z Y : ξ ( z 0 , z ) = r } and D z 0 , r = { z Y : ξ ( z 0 , z ) r } are called circle and disc, respectively, with center z 0 and radius r. The circle C z 0 , r (disc D z 0 , r ) is said to be a fixed circle (fixed disc) of a mapping S : Y Y if S z = z , for all z C z 0 , r ( D z 0 , r ).
Before starting our main results, we would like to bring to the reader’s attention that, in the next three sections, we are working on transformations that not only fix one element but also fix a well-defined set of “fixed points” which is either a circle or a disc.

2. Fixed Circle (Disc) Results for Θ c -Contraction and Ćirić Type Θ c -Contraction

Let ( Y , ξ ) be a metric space. From now on, S is a self-mapping defined on a non-empty set Y and
r = inf { ξ ( z , S z ) : z S z } .
At first, we introduce the notion of Θ c -contraction as follows:
Definition 1.
Let ( Y , ξ ) be a metric space and Θ Ω 1 . A mapping S is said to be a Θ c -contraction if there exist λ ( 0 , 1 ) and z 0 Y such that
ξ ( z , S z ) > 0 Θ ( ξ ( z , S z ) ) [ Θ ( ξ ( z , z 0 ) ) ] λ , z Y .
Using the Θ c -contraction condition, we present the following fixed circle result.
Theorem 1.
Let ( Y , ξ ) be a metric space. Assume that S is a Θ c -contraction mapping defined on Y with z 0 Y and ξ ( z 0 , S z ) = r , for all z C z 0 , r . Then, C z 0 , r is a fixed circle of S.
Proof. 
Let z C z 0 , r and assume on contrary that ξ ( S z , z ) > 0 , that is, S z z . From the definition of r, we have ξ ( z , S z ) r . As S is a Θ c -contraction, so in view of the fact that Θ is nondecreasing, we get
Θ ( r ) Θ ( ξ ( z , S z ) ) [ Θ ( M ( z , z 0 ) ) ] λ < Θ ( M ( z , z 0 ) ) = Θ ( r ) ,
which is a contradiction. Therefore, S z = z , for all z C z 0 , r , that is, C z 0 , r is a fixed circle of S. This concludes the proof. □
Next, we prove the following fixed disc result.
Theorem 2.
Let ( Y , ξ ) be a metric space. Assume that S is a Ćirić type Θ c -contraction mapping with z 0 Y and ξ ( z 0 , S z ) = r for all z D z 0 , r . Then, D z 0 , r is a fixed disc of S.
Proof. 
In view of Theorem 1, the mapping S fixes the circle C z 0 , r . In order to show that D z 0 , r is a fixed disc of S, it is sufficient to show that S fixes any circle C z 0 , ρ with ρ < r . Let z C z 0 , ρ , and, contrarily, let us assume that z S z for some z C z 0 , ρ . Since S is a Θ c -contraction, we have
Θ ( ξ ( z , S z ) ) [ Θ ( M ( z , z 0 ) ) ] λ < Θ ( M ( z , z 0 ) ) = Θ ( ρ ) .
Since Θ is nondecreasing, we then obtain
ξ ( z , S z ) < ρ < r ,
which leads to a contradiction as r = inf { ξ ( S z , z ) : z S z } . Therefore, S z = z for all z D z 0 , r . Consequently, D z 0 , r is a fixed disc of S. □
Next, we generalize Θ c -contractions to Ćirić type Θ c -contractions and prove the following new results in this section.
Definition 2.
Let ( Y , ξ ) be a metric space and Θ Ω 1 . A mapping S is said to be a Ćirić type Θ c -contraction if there exist λ ( 0 , 1 ) and z 0 Y such that
ξ ( z , S z ) > 0 Θ ( ξ ( z , S z ) ) [ Θ ( M ( z , z 0 ) ) ] λ , z Y ,
where
M ( z , z 0 ) = max ξ ( z , z 0 ) , a ξ ( z , S z ) + ( 1 a ) ξ ( z 0 , S z 0 ) , ( 1 a ) ξ ( z , S z ) + a ξ ( z 0 , S z 0 ) , 1 2 [ ξ ( z , S z 0 ) + ξ ( z 0 , S z ) ] , 0 a < 1 .
The following proposition follows from Definition 2.
Proposition 1.
Let ( Y , ξ ) be a metric space. If S is a Ćirić type Θ c -contraction mapping with z 0 Y , then S z 0 = z 0 .
Proof. 
Assume that S z 0 z 0 . From Definition 2, we have
Θ ( ξ ( z 0 , S z 0 ) ) [ Θ ( M ( z 0 , z 0 ) ) ] λ = Θ max ξ ( z 0 , z 0 ) , a ξ ( z 0 , S z 0 ) + ( 1 a ) ξ ( z 0 , S z 0 ) , ( 1 a ) ξ ( z 0 , S z 0 ) + a ξ ( z 0 , S z 0 ) , 1 2 [ ξ ( z 0 , S z 0 ) + ξ ( z 0 , S z 0 ) ] λ = Θ max 0 , ξ ( z 0 , S z 0 ) λ = [ Θ ( ξ ( z 0 , S z 0 ) ) ] λ ,
a contradiction as λ ( 0 , 1 ) . Therefore, we must have S z 0 = z 0 . □
Using Ćirić type Θ c -contraction condition, we present the following fixed circle result.
Theorem 3.
Let ( Y , ξ ) be a metric space. Assume that S is a Ćirić type Θ c -contraction mapping with z 0 Y and ξ ( z 0 , S z ) = r for all z C z 0 , r . Then, C z 0 , r is a fixed circle of S.
Proof. 
Let z C z 0 , r and assume contrarily that S z z . From the definition of r, we have ξ ( z , S z ) r . As S is a Ćirić type Θ c -contraction, using Proposition 1, we have
Θ ( ξ ( z , S z ) ) [ Θ ( M ( z , z 0 ) ) ] λ = Θ max ξ ( z , z 0 ) , a ξ ( z , S z ) + ( 1 a ) ξ ( z 0 , S z 0 ) , ( 1 a ) ξ ( z , S z ) + a ξ ( z 0 , S z 0 ) , 1 2 [ ξ ( z , S z 0 ) + ξ ( z 0 , S z ) ] λ = Θ max r , a ξ ( z , S z ) , ( 1 a ) ξ ( z , S z ) λ < Θ max r , a ξ ( z , S z ) , ( 1 a ) ξ ( z , S z ) .
Now, we have the following possibilities:
Case 1: If max r , a ξ ( z , S z ) , ( 1 a ) ξ ( z , S z ) = r , then from Equation (2), the definition of r and the fact that the function Θ is nondecreasing, we have
Θ ( r ) Θ ( ξ ( z , S z ) ) < Θ ( r ) ,
a contradiction.
Case 2: If max r , a ξ ( z , S z ) , ( 1 a ) ξ ( z , S z ) = a ξ ( z , S z ) , then we have two possibilities: either a = 0 or 0 < a < 1 . Assuming that 0 < a < 1 from Equation (2) and the fact that the function Θ is nondecreasing, we have
Θ ( ξ ( z , S z ) ) < Θ ( a ξ ( z , S z ) ) Θ ( ξ ( z , S z ) ) ,
a contradiction. If a = 0 , then from Equation (2), we get
Θ ( ξ ( z , S z ) ) < Θ ( 0 ) ;
this inequality contradicts with the definition of Θ (as Θ : ( 0 , ) ( 1 , ) ).
Case 3: If max r , a ξ ( z , S z ) , ( 1 a ) ξ ( z , S z ) = ( 1 a ) ξ ( z , S z ) , then from Equation (2) and the fact that the function Θ is nondecreasing, we have
Θ ( ξ ( z , S z ) ) < Θ ( ( 1 a ) ξ ( z , S z ) ) Θ ( ξ ( z , S z ) ) ,
a contradiction. Therefore, S z = z for all z C z 0 , r . Consequently, C z 0 , r is a fixed circle of S. □
Next, we prove the following fixed disc result.
Theorem 4.
Let ( Y , ξ ) be a metric space. Assume that S is a Ćirić type Θ c -contraction mapping with z 0 Y and ξ ( z 0 , S z ) = r for all z D z 0 , r . Then, D z 0 , r is a fixed disc of S.
Proof. 
The mapping S fixes the circle C z 0 , r (in view of Theorem 3). Now, in order to show that D z 0 , r is a fixed disc of S, it is sufficient to show that S fixes any circle C z 0 , ρ with ρ < r . Let z C z 0 , ρ and, contrarily, let us assume that z S z for some z C z 0 , ρ . Since S is a Ćirić type Θ c -contraction, using Proposition 1, we have
Θ ( ξ ( z , S z ) ) [ Θ ( M ( z , z 0 ) ) ] λ = Θ max ρ , a ξ ( z , S z ) , ( 1 a ) ξ ( z , S z ) , ρ + r 2 λ < Θ max ρ , a ξ ( z , S z ) , ( 1 a ) ξ ( z , S z ) , ρ + r 2 .
Now, we have the following possibilities:
Case 1: If max ρ , a ξ ( z , S z ) , ( 1 a ) ξ ( z , S z ) , ρ + r 2 = ρ , then from Equation (3), the definition of r and the fact that the function Θ is nondecreasing, we have
Θ ( ρ ) < Θ ( r ) Θ ( ξ ( z , S z ) ) < Θ ( ρ ) ,
a contradiction.
Case 2: If max ρ , a ξ ( z , S z ) , ( 1 a ) ξ ( z , S z ) , ρ + r 2 = a ξ ( z , S z ) , then we have two possibilities: either a = 0 or 0 < a < 1 . Assuming that 0 < a < 1 from Equation (3) and the fact that the function Θ is nondecreasing, we have
Θ ( ξ ( z , S z ) ) < Θ ( a ξ ( z , S z ) ) Θ ( ξ ( z , S z ) )
a contradiction. If a = 0 , then from Equation (2), we get
Θ ( ξ ( z , S z ) ) < Θ ( 0 ) .
This inequality contradicts with the definition of Θ (as Θ : ( 0 , ) ( 1 , ) ).
Case 3: If max ρ , a ξ ( z , S z ) , ( 1 a ) ξ ( z , S z ) , ρ + r 2 = ( 1 a ) ξ ( z , S z ) , then from Equation (3) and the fact that the function Θ is nondecreasing, we have
Θ ( ξ ( z , S z ) ) < Θ ( ( 1 a ) ξ ( z , S z ) ) Θ ( ξ ( z , S z ) ) ,
a contradiction.
Case 4: If max ρ , a ξ ( z , S z ) , ( 1 a ) ξ ( z , S z ) , ρ + r 2 = ρ + r 2 , then by the definition of r, the inequality Equation (3) and the fact that the function Θ is nondecreasing, we have
Θ ( r ) Θ ( ξ ( z , S z ) ) < Θ ρ + r 2 Θ ( r ) ,
a contradiction. Therefore, S z = z for all z D z 0 , r . Consequently, D z 0 , r is a fixed disc of S. □
Corollary 1.
Let ( Y , ξ ) be a metric space and S a mapping defined on Y. If there exist λ ( 0 , 1 ) and z 0 Y with ξ ( z 0 , S z ) = r for all z C z 0 , r ( o r D z 0 , r ) such that
ξ ( z , S z ) > 0 Θ ( ξ ( z , S z ) ) [ Θ ( m ( z , z 0 ) ) ] λ , z Y ,
where m ( z , z 0 ) = max { ξ ( z , z 0 ) , ξ ( z , S z ) , ξ ( z 0 , S z 0 ) , 1 2 [ ξ ( z , S z 0 ) + ξ ( z 0 , S z ) ] } , then C z 0 , r ( o r D z 0 , r ) is a fixed circle (or disc) of S.
Proof. 
The result follows from Theorems 3 and 4 by taking a = 0 in the contractive condition (1). □
Example 1.
Let Y = [ 4 , ) be a metric space endowed with the usual metric ξ. Define S : Y Y as
S z = z , i f 4 z < 4 z + 3 , i f z 4 .
The self-mapping S is a Θ c -contraction. In fact, let Θ ( t ) = e t , z 0 = 0 and λ = 3 4 .
For all z [ 4 , ) such that z 4 , we have
ξ ( z , S z ) = 3 > 0 ,
and
Θ ( ξ ( z , S z ) ) = e 3 e 3 4 ( z ) = [ e ξ ( z , z 0 ) ] 3 4 = [ Θ ( ξ ( z , z 0 ) ) ] λ .
The self-mapping S is a Ćirić type Θ c -contraction. To show this, let Θ ( t ) = e t , z 0 = 0 , a = 1 2 and λ = 6 11 .
For all z [ 4 , ) such that z 4 , we have
ξ ( z , S z ) = 3 > 0 ,
M ( z , z 0 ) = max ξ ( z , 0 ) , 1 2 ξ ( z , S z ) , 1 2 ξ ( z , S z ) , ξ ( z , 0 ) + ξ ( 0 , S z ) 2 = max | z | , 3 2 , 3 2 , | z | + | z + 3 | 2 = | z | + | z + 3 | 2
and
Θ ( ξ ( z , S z ) ) = e 3 e 3 11 ( | z | + | z + 3 | ) = [ e | z | + | z + 3 | 2 ] 6 11 = [ Θ ( M ( z , z 0 ) ) ] λ .
We also have
r = inf { ξ ( z , S z ) : z S z } = 3 .
Therefore, all the conditions of Theorems 1–4 are satisfied. Observe that C 0 , 3 = { 3 , 3 } is a fixed circle and D 0 , 3 = [ 3 , 3 ] is a fixed disc of S.

3. Fixed Circle (Disc) Results for Hardy–Rogers Θ c -Contraction and Khan Type Θ c -Contraction

We start this section by introducing the concept Hardy–Rogers type Θ c -contractions as follows:
Definition 3.
Let ( Y , ξ ) be a metric space and Θ Ω 1 . A mapping S is called a Hardy–Rogers type Θ c -contraction if there exist λ ( 0 , 1 ) and z 0 Y such that
ξ ( z , S z ) > 0 Θ ( ξ ( z , S z ) ) [ Θ ( M * ( z , z 0 ) ) ] λ , z Y ,
where M * ( z , z 0 ) = α ξ ( z , z 0 ) + β ξ ( z , S z ) + γ ξ ( z 0 , S z 0 ) + δ ξ ( z , S z 0 ) + η ξ ( z 0 , S z ) with α + β + γ + δ + η < 1 and α , β , γ , δ , η 0 .
The following proposition follows from Definition 3.
Proposition 2.
Let ( Y , ξ ) be a metric space. If S is a Hardy–Rogers type Θ c -contraction mapping with z 0 Y , then S z 0 = z 0 .
Proof. 
Assume that S z 0 z 0 . From Definition 3 and the fact that Θ is nondecreasing, we obtain
Θ ( ξ ( z 0 , S z 0 ) ) [ Θ ( M * ( z 0 , z 0 ) ) ] λ < Θ ( M * ( z 0 , z 0 ) ) = Θ ( α ξ ( z 0 , z 0 ) + β ξ ( z 0 , S z 0 ) + γ ξ ( z 0 , S z 0 ) + δ ξ ( z 0 , S z 0 ) + η ξ ( z 0 , S z 0 ) ) = Θ ( ( β + γ + δ + η ) ξ ( z 0 , S z 0 ) ) Θ ( ξ ( z 0 , S z 0 ) ) ,
a contradiction. Therefore, we must have S z 0 = z 0 . □
Using a Hardy–Rogers type Θ c -contraction, we present the following fixed circle results.
Theorem 5.
Let ( Y , ξ ) be a metric space. Assume that S is a Hardy–Rogers type Θ c -contraction with z 0 Y and ξ ( z 0 , S z ) = r for all z C z 0 , r . Then, C z 0 , r is a fixed circle of S.
Proof. 
Let z C z 0 , r and assume contrarily that S z z . By the definition of r, we have ξ ( z , S z ) r . Since S is a Hardy–Rogers type Θ c -contraction, using Proposition 2 and the fact that Θ is nondecreasing, we have
Θ ( ξ ( z , S z ) ) [ Θ ( M * ( z , z 0 ) ) ] λ < Θ ( α ξ ( z , z 0 ) + β ξ ( z , S z ) + γ ξ ( z 0 , S z 0 ) + δ ξ ( z , S z 0 ) + η ξ ( z 0 , S z ) ) = Θ ( α r + β ξ ( z , S z ) + δ r + η r ) Θ ( ( α + β + δ + η ) ξ ( z , S z ) ) Θ ( ξ ( z , S z ) ) ,
a contradiction. Therefore, S z = z for all z C z 0 , r . Consequently, C z 0 , r is a fixed circle of S. □
Next, we prove the following fixed disc result.
Theorem 6.
Let ( Y , ξ ) be a metric space. Assume that S is a Hardy–Rogers type Θ c -contraction with z 0 Y and ξ ( z 0 , S z ) = r , for all z D z 0 , r . Then, D z 0 , r is a fixed disc of S.
Proof. 
In view of Theorem 5, S fixes the circle C z 0 , r . Now, in order to show that D z 0 , r is a fixed disc of the mapping S, it is sufficient to show that S fixes any circle C z 0 , ρ with ρ < r . Let z C z 0 , ρ and assume that ξ ( z , S z ) > 0 . Since S is a Hardy–Rogers type Θ c -contraction, using Proposition 2 and the fact that Θ is nondecreasing, we have
Θ ( ξ ( z , S z ) ) [ Θ ( M * ( z , z 0 ) ) ] λ < Θ ( α ξ ( z , z 0 ) + β ξ ( z , S z ) + γ ξ ( z 0 , S z 0 ) + δ ξ ( z , S z 0 ) + η ξ ( z 0 , S z ) ) = Θ ( α ρ + β ξ ( z , S z ) + δ ρ + η ρ ) Θ ( ( α + β + δ + η ) ξ ( z , S z ) ) Θ ( ξ ( z , S z ) ) ,
a contradiction. Thus, we obtain S z = z , and D z 0 , ρ is a fixed disc of S. □
From Theorems 5 and 6, we deduce the following corollaries.
Corollary 2.
Let ( Y , ξ ) be a metric space and S a mapping. If there exists λ ( 0 , 1 ) and z 0 Y with ξ ( z 0 , S z ) = r , for all z C z 0 , r ( o r D z 0 , r ) such that
ξ ( z , S z ) > 0 Θ ( ξ ( z , S z ) ) [ Θ ( α ξ ( z , z 0 ) + β ξ ( z , S z ) + γ ξ ( z 0 , S z 0 ) ) ] λ , z Y ,
where α + β + γ < 1 and α , β , γ 0 , then C z 0 , r ( o r D z 0 , r ) is a fixed circle (or disc) of S.
Proof. 
The claim follows from Theorems 5 and 6 if we take α = β = γ = 0 and δ = η in the contractive condition (4). □
Corollary 3.
Let ( Y , ξ ) be a metric space and S a mapping. If there exists λ ( 0 , 1 ) and z 0 Y with ξ ( z 0 , S z ) = r , for all z C z 0 , r ( o r D z 0 , r ) such that
ξ ( z , S z ) > 0 Θ ( ξ ( z , S z ) ) [ Θ ( η ( ξ ( z , S z 0 ) + ξ ( z 0 , S z ) ) ) ] λ , z Y ,
where η ( 0 , 1 2 ) , then C z 0 , r ( o r D z 0 , r ) is a fixed circle (or disc) of S.
Proof. 
The claim follows from Theorems 5 and 6 if we put η = δ = 0 in the contractive condition (4). □
The following example exhibits the utility of Theorems 5 and 6.
Example 2.
Let Y = { 3 , 4 , ln ( 3 e ) , ln ( 3 ) , ln ( 3 e ) } be endowed with the usual metric ξ. Define S : Y Y as
S z = 4 , i f z = 3 z , o t h e r w i s e .
Let Θ ( t ) = e t , z 0 = ln 3 , k = 3 10 3 ln 3 , α = δ = η = 1 3 and β = 0 . Then, S is a Hardy–Rogers type Θ c -contraction. Indeed, for z = 3
ξ ( z , S z ) = ξ ( 3 , T 3 ) = 1 > 0 ,
M ( z , z 0 ) = α ξ ( z , z 0 ) + β ξ ( z , S z ) + δ ξ ( z , S z 0 ) + η ξ ( z 0 , S z ) = 1 3 [ ξ ( 3 , ln 3 ) + ξ ( 3 , ln 3 ) + ξ ( ln 3 , 4 ) ] = 10 3 ln 3
and
Θ ( ξ ( z , S z ) ) = Θ ( ξ ( 3 , 4 ) ) = e [ e 10 3 ln 3 ] 3 10 3 ln 3 = [ Θ ( M ( z , z 0 ) ) ] λ .
We also have
r = inf { ξ ( z , S z ) : z S z } = { ξ ( 3 , 4 ) } = 1 .
Hence, all the conditions of Theorems 5 and 6 are satisfied. Observe that S fixes the circle C ln 3 , 1 = { ln ( 3 e ) , ln ( 3 e ) } and the disc D ln 3 , 1 = { ln ( 3 e ) , ln 3 , ln ( 3 e ) } .
We close this section by introducing the concept of the Khan type Θ c -contraction followed by the related fixed circle (disc) results.
Definition 4.
Let ( Y , ξ ) be a metric space and Θ Ω 1 . A mapping S is called a Khan type Θ c -contraction if there exist λ ( 0 , 1 ) and z 0 Y such that for all z Y , if max { ξ ( S z 0 , z 0 ) , ξ ( S z , z ) } 0 , then S z z and
Θ ( ξ ( S z , z ) ) Θ h ξ ( S z , z ) ξ ( S z 0 , z ) + ξ ( S z 0 , z 0 ) ξ ( S z , z 0 ) max { ξ ( S z 0 , z 0 ) , ξ ( S z , z ) } λ ,
where h ( 0 , 1 2 ) and if max { ξ ( S z 0 , z 0 ) , ξ ( S z , z ) } = 0 , then S z = z .
The following proposition is a direct consequence of Definition 4.
Proposition 3.
Let ( Y , ξ ) be a metric space. If S is a Khan type Θ c -contraction with z 0 Y , then S z 0 = z 0 .
Proof. 
Assume that S z 0 z 0 ; then, max { ξ ( S z 0 , z 0 ) , ξ ( S z , z ) } 0 . As S is a Khan type Θ c -contraction, we have
Θ ( ξ ( S z 0 , z 0 ) ) Θ h ξ ( S z 0 , z 0 ) ξ ( S z 0 , z 0 ) + ξ ( S z 0 , z 0 ) ξ ( S z 0 , z 0 ) ξ ( S z 0 , z 0 ) λ = [ Θ ( 2 h ξ ( S z 0 , z 0 ) ) ] λ < Θ ( 2 h ξ ( S z 0 , z 0 ) ) Θ ( ξ ( S z 0 , z 0 ) ) ,
a contradiction. Therefore, we must have S z 0 = z 0 . □
Now, utilizing the definition of the Khan type Θ c -contraction, we prove the following fixed circle and fixed disc results.
Theorem 7.
Let ( Y , ξ ) be a metric space and let S : Y Y be a Khan type Θ c -contraction with z 0 Y . Then, C z 0 , r is a fixed circle of S.
Proof. 
Let z C z 0 , r and assume contrarily that S z z ; then, max { ξ ( S z 0 , z 0 ) , ξ ( S z , z ) } 0 . From the definition of r, we have ξ ( z , S z ) r . As S is a Khan type Θ c -contraction, using Proposition 3 and the fact that Θ is nondecreasing, we have
Θ ( ξ ( S z , z ) ) Θ h ξ ( S z , z ) ξ ( S z 0 , x ) + ξ ( S z 0 , z 0 ) ξ ( S z , z 0 ) ξ ( S z , z ) λ = [ Θ ( h r ) ] λ < Θ ( h r ) Θ ( h ξ ( S z , z ) ) Θ ( ξ ( S z , z ) ) ,
a contradiction. Therefore, S z = z for all z C z 0 , r . Consequently, C z 0 , r is a fixed circle of S. □
Theorem 8.
Let ( Y , ξ ) be a metric space and let S : Y Y be a Khan type Θ c -contraction with z 0 Y . Then, D z 0 , r is a fixed disc of S.
Proof. 
In view of Theorem 7, S fixes the circle C z 0 , r . Now, in order to show that D z 0 , r is a fixed disc of the mapping S, it is sufficient to show that S fixes any circle C z 0 , ρ with ρ < r . Let z C z 0 , ρ and assume that ξ ( z , S z ) > 0 . By the Khan type Θ c -contractive condition, we have
Θ ( ξ ( z , S z ) ) [ Θ ( h ρ ) ] λ < Θ ( h ρ ) Θ ( ρ ) .
As Θ is a nondecreasing function, we get
ξ ( z , S z ) < ρ < r ,
a contradiction (as r ξ ( z , S z ) ). Thus, we obtain S z = z for all z C z 0 , ρ with ρ < r . Therefore, D z 0 , r is a fixed disc of S. □
The following example shows the utility of Theorems 7 and 8.
Example 3.
Let X = R be endowed with the usual metric ξ. Define S : R R by
S z = z , i f | z | < 4.5 , z + 1 , i f | z | 4.5 .
Then, S is a Khan type Θ-contraction with Θ ( t ) = e t , z 0 = 0 , k = 2 3 and h = 1 3 . In fact,
max { ξ ( S z 0 , z 0 ) , ξ ( S z , z ) } = 1 0 ,
for all z R such that | z | 4.5 . Now, we have
h ξ ( S z , z ) ξ ( S z 0 , x ) + ξ ( S z 0 , z 0 ) ξ ( S z , z 0 ) ξ ( S z , z ) = h ξ ( 0 , z ) = 1 3 | z |
and
Θ ( ξ ( S z , z ) ) = e e 2 9 | z | = [ e 1 3 | z | ] 2 3 = Θ ( h ξ ( S z , z ) ξ ( S z 0 , z ) + ξ ( S z 0 , z 0 ) ξ ( S z , z 0 ) ξ ( S z , z ) ) λ .
We also have
r = inf { ξ ( z , S z ) : z S z } = 1 .
Therefore, all the conditions of Theorems 7 and 8 are satisfied. Observe that S fixes the circle C 0 , 1 = { 1 , 1 } and the disc D 0 , 1 = [ 1 , 1 ] .

4. Fixed Circle (Disc) Results of Integral Type

In this section, we establish some fixed circle and disc results of the integral type.
Let φ : [ 0 , ) [ 0 , ) be a locally integrable function such that
0 t φ ( s ) d s > 0 , for all t > 0 .
Definition 5.
Let S : Y Y and Θ Ω 1 . The mapping S is called an integral type Θ c -contraction if there exist λ ( 0 , 1 ) and z 0 Y such that for all z Y
ξ ( z , S z ) > 0 0 Θ ( ξ ( z , S z ) ) φ ( t ) d t 0 [ Θ ( ξ ( z , z 0 ) ) ] λ φ ( t ) d t .
where φ : [ 0 , ) [ 0 , ) is a function defined as in Equation (5).
The following proposition is useful in the proof of the main results of this section.
Proposition 4.
Let ( Y , ξ ) be a metric space and S : Y Y . If S is an integral type Θ c -contraction with z 0 Y , then S z 0 = z 0 .
Proof. 
Assume that S z 0 z 0 . From Definition 5, we have
0 Θ ( ξ ( z 0 , S z 0 ) ) φ ( t ) d t 0 [ Θ ( ξ ( z 0 , z 0 ) ) ] λ φ ( t ) d t ,
which contradicts the definition of Θ , as Θ : ( 0 , ) ( 1 , ) and ξ ( z 0 , z 0 ) = 0 . Hence, we must have S z 0 = z 0 . □
In the following theorem, we present a fixed circle result for integral type Θ c -contraction.
Theorem 9.
Let ( Y , ξ ) be a metric space and S : Y Y . If S is an integral type Θ c -contraction with z 0 Y , then C z 0 , r is a fixed circle of S.
Proof. 
Assume that z S z for some z C z 0 , r . Making use of the definition of r, we have
r ξ ( z , S z ) .
Since Θ is a nondecreasing function, we have
Θ ( r ) Θ ( ξ ( z , S z ) )
and
0 Θ ( r ) φ ( t ) d t 0 Θ ( ξ ( z , S z ) ) φ ( t ) d t .
As S is an integral type Θ c -contraction, using Equation (6), we obtain
0 Θ ( r ) φ ( t ) d t 0 Θ ( ξ ( z , S z ) ) φ ( t ) d t 0 [ Θ ( ξ ( z , z 0 ) ) ] λ φ ( t ) d t < 0 Θ ( ξ ( z , z 0 ) ) φ ( t ) d t = 0 Θ ( r ) φ ( t ) d t ,
a contradiction. Therefore, we have S z = z . Consequently, C z 0 , r is a fixed circle of S. □
Next, we prove the following fixed disc results.
Theorem 10.
Let ( Y , ξ ) be a metric space, let φ : [ 0 , ) [ 0 , ) be defined as in Equation (5) and let S be an integral type Θ c -contraction with z 0 Y . Then, D z 0 , r is a fixed disc of S.
Proof. 
In view of Theorem 9, the mapping S fixes the circle C z 0 , r . Now, in order to show that D z 0 , r is a fixed disc of the mapping S, it is sufficient to show that S fixes any circle C z 0 , ρ with ρ < r . Let z C z 0 , ρ and assume that z S z . Making use of the definition of r, we have
ρ < r ξ ( z , S z ) .
Since Θ is a nondecreasing function, we have
Θ ( ρ ) Θ ( ξ ( z , S z ) )
and
0 Θ ( ρ ) φ ( t ) d t 0 Θ ( ξ ( z , S z ) ) φ ( t ) d t .
As S is an integral type Θ c -contraction, using Equation (7), we obtain
0 Θ ( ρ ) φ ( t ) d t 0 Θ ( ξ ( z , S z ) ) φ ( t ) d t 0 [ Θ ( ξ ( z , z 0 ) ) ] λ φ ( t ) d t < 0 Θ ( ξ ( z , z 0 ) ) φ ( t ) d t = 0 Θ ( ρ ) φ ( t ) d t ,
a contradiction. Therefore, we must have S z = z , z C z 0 , ρ . Consequently, D z 0 , r is a fixed disc of S. □
Remark 2.
Using similar arguments as in Definition 5, we can define the notions of an integral type Ćirić type Θ c -contraction, an integral Hardy–Rogers type Θ c -contraction and an integral Khan type Θ c -contraction, and we can obtain corresponding fixed circle and fixed disc theorems.

5. Conclusions

We have obtained some new generalized fixed circle and fixed disc results using our newly introduced contractive conditions in the setting of metric spaces. Precisely, by means of some known techniques which usually are used to obtain some fixed point theorems, we have generated some useful fixed circle and fixed disc results.

Author Contributions

Conceptualization, H.N.S., S.S., W.M.A., M.I. and N.M.; Funding acquisition, S.S.; Investigation, H.N.S., W.M.A., M.I. and N.M.; Methodology, H.N.S., S.S., W.M.A., M.I. and N.M.; Supervision, M.I.; Writing-original draft, H.N.S. All authors have read and agreed to the published version of the manuscript.

Funding

This research was funded by the Department of the second author.

Acknowledgments

The authors are grateful to an anonymous referees and the Editor for their valuable suggestions and fruitful comments.

Conflicts of Interest

The authors declare no conflict of interest.

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Saleh, H.N.; Sessa, S.; Alfaqih, W.M.; Imdad, M.; Mlaiki, N. Fixed Circle and Fixed Disc Results for New Types of Θc-Contractive Mappings in Metric Spaces. Symmetry 2020, 12, 1825. https://doi.org/10.3390/sym12111825

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Saleh HN, Sessa S, Alfaqih WM, Imdad M, Mlaiki N. Fixed Circle and Fixed Disc Results for New Types of Θc-Contractive Mappings in Metric Spaces. Symmetry. 2020; 12(11):1825. https://doi.org/10.3390/sym12111825

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Saleh, Hayel N., Salvatore Sessa, Waleed M. Alfaqih, Mohammad Imdad, and Nabil Mlaiki. 2020. "Fixed Circle and Fixed Disc Results for New Types of Θc-Contractive Mappings in Metric Spaces" Symmetry 12, no. 11: 1825. https://doi.org/10.3390/sym12111825

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