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Article

Optimum Solutions of Systems of Differential Equations via Best Proximity Points in b-Metric Spaces

1
Department of Mathematics, University of Management and Technology, C-II, Johar Town, Lahore 54770, Pakistan
2
Department of Electricity and Electronics, Institute of Research and Development of Processes, Faculty of Science and Technology, University of the Basque Country (UPV/EHU), Campus of Leioa, 48940 Leioa, Bizkaia, Spain
*
Author to whom correspondence should be addressed.
Mathematics 2023, 11(3), 574; https://doi.org/10.3390/math11030574
Submission received: 4 November 2022 / Revised: 16 January 2023 / Accepted: 17 January 2023 / Published: 21 January 2023
(This article belongs to the Section Difference and Differential Equations)

Abstract

:
This paper deals with the existence of an optimum solution of a system of ordinary differential equations via the best proximity points. In order to obtain the optimum solution, we have developed the best proximity point results for generalized multivalued contractions of b-metric spaces. Examples are given to illustrate the main results and to show that the new results are the proper generalization of some existing results in the literature.

1. Introduction and Preliminaries

Best proximity point theory provides basic tools to find approximate solutions of problems in mathematics and related disciplines, particularly whenever an exact solution does not exist.
For a non-self-mapping T : M N , where M and N are two nonempty subsets of a nonempty set Ω , a point m M is an exact solution or the fixed point (FP) of T if m = T m . In the case where M and T ( M ) have an empty intersection, then T has no FP. For such situations, it is better to find a point m M such that the distance between m and T m is minimized. That is,
ς ( m , T m ) = ς ( M , N )
where
ς ( M , N ) = inf m M , n N ς ( m , n ) ,
and ς is a metric on Ω . A point m in M that satisfies (1) is called the best proximity point (BPP) of T . In the literature, many mathematicians have contributed to the development of the BPP theory of metric spaces. The main objective of this theory is to develop necessary and sufficient conditions that ensure the existence of best proximity points (BPP(s)) of T (a non-self-mapping of certain distance space). For more details, one can see the references [1,2,3,4].
If M = N = Ω , in (1) (that is, T is self-mapping), then ς ( m , T m ) = 0 or m = T m . In this case, m becomes an FP of T . Therefore, BPP theory is a natural generalization of FP theory.
In 1969, Fan [5] provided a remarkable result in BPP theory. After that, many mathematicians have contributed to the development of BPP theory with different proximal contractions [6,7,8].
One interesting proximal contraction is the α ψ proximal ( α ψ ) contraction by Jleli and Samet [9], and they have developed some BPP(s) results in metric space (in short, MS). Abkar and Gabeleh [10] developed some BPP(s) for Suzuki-type contractions. Hussain et al. [11] generalized the α ψ contraction to the Suzuki-type α ψ contraction and developed some BPP(s) results for it.
Recently, Khan et al. [12] generalized the contraction used in [11] and developed some BPP(s) results in the domain of MS.
After the development of fixed points (FP) results for multivalued mappings by Nadler [13] in 1969, many mathematicians extended BPP theory from single-valued mappings to multivalued mappings. For instance, Ali et al. [14] in 2014 extended the α ψ contraction to α ψ multivalued contractions and developed some BPP(s) results for them.
Later on, MS was extended to the b-metric space (b-MS) by Bakhtin [15] in 1989 and by Czerwik [16] in 1993. After that, a new area of research for the existence of BPP in b-MS is opened up, and many researchers have developed BPP(s) results for single- as well as multivalued mappings in the domain of b-MS. For more details, one can see the references [17,18,19,20,21].
In this paper, we introduce a new multivalued Suzuki-type α ψ (cyclic) contractions in the domain of b-MS and develop some BPP(s) results. Examples have been given to explain our main results and to show that our main results are the proper generalization of results given in [12]. As an application of our results, we develop the optimum solution for a system of ordinary differential equations.
Definition 1
([15]). The mapping ς : Ω × Ω [ 0 , ) is a b-metric, and ( Ω , ς ) is called b-MS if the following hold:
( b 1 )
ς ( ϰ 1 , ϰ 2 ) = 0 if and only if ϰ 1 = ϰ 2 for all ϰ 1 , ϰ 2 Ω ;
( b 2 )
ς ( ϰ 1 , ϰ 2 ) = ς ( ϰ 2 , ϰ 1 ) for all ϰ 1 , ϰ 2 Ω ;
( b 3 )
There exists a real number k 1 such that ς ( ϰ 1 , ϰ 2 ) k [ ς ( ϰ 1 , ϰ 3 ) + ς ( ϰ 3 , ϰ 2 ) ] for all ϰ 1 , ϰ 2 , ϰ 3 Ω .
Remark 1.
If k = 1 , then ς becomes a metric.
In this article, R + , R , N , N 1 , 2 Ω , denote the set of non-negative reals, reals, positive integers, non-negative integers, and nonempty subsets of Ω , respectively. Define
M 0 = m M : ς ( m , n ) = ς ( M , N ) for some n N and N 0 = n N : ς ( m , n ) = ς ( M , N ) for some m M
where M , N 2 Ω . If M 0 is nonempty, then ( M , N ) has a weak P property (shortly as weak P p ) (compare with [22]) if
ς ( m 1 , n 1 ) = ς ( M , N ) , ς ( m 2 , n 2 ) = ς ( M , N ) , implies ς ( m 1 , m 2 ) ς ( n 1 , n 2 ) ,
for all m 1 , m 2 M and n 1 , n 2 N .
Definition 2.
A mapping T : M N 2 M 2 N is said to be cyclic if T ( m ) N for all m M and T ( n ) M for all n N .
In the following, we introduce multivalued α proximal admissibles with respect to p (for short, m α p ) for multivalued mappings (compared with [12]).
Definition 3.
A mapping T : M 2 N is m α p if
α ( m 1 , m 2 ) p ( m 1 , m 2 ) , ς ( m 3 , n 1 ) = ς ( M , N ) , ς ( m 4 , n 2 ) = ς ( M , N ) , implies α ( m 3 , m 4 ) p ( m 3 , m 4 ) ,
for all m 1 , m 2 , m 3 , m 4 M and n 1 T m 1 , n 2 T m 2 , where α : M × M [ 0 , ) and p : M × M [ 1 , ) .
Remark 2.
(i) 
If T : M 2 N is replaced by T : M N , then T is α proximal admissible with respect to p (shortly as α p ) (see [12]).
(ii) 
If p = 1 in the Definition 3, then T is called multivalued α proximal admissible (compare with [14]).
(iii) 
If p = 1 and 2 N is replaced by N in the Definition 3, then T is called α proximal admissible (compare with [9]).
(iv) 
If M = N = Ω in the Definition 3, then T is called α admissible with respect to p (for short, α p ).
Consider the following class:
Ψ is a class of functions ψ : [ 0 , ) [ 0 , ) , such that ψ is monotone increasing and there exist μ 0 N , a ( 0 , 1 ) , b [ 1 , ) , and a convergent series of non-negative numbers μ = 1 u μ such that for any Υ 0 ,
b μ + 1 ψ μ + 1 ( Υ ) a b μ ψ μ ( Υ ) + u μ
for all μ μ 0 . A function ψ Ψ is a “Bianchini-Grandolfi gauge function (also known as (c)-comparison function)”.
Lemma 1
([23]). If ψ Ψ , then
(i) 
( ψ μ ( Υ ) ) μ N converges to 0 as μ for all Υ R + ;
(ii) 
ψ ( Υ ) < Υ , for any Υ ( 0 , ) ;
(iii) 
ψ is continuous at 0 ;
(iv) 
The series μ = 0 b μ ψ μ ( Υ ) converges for any Υ R + .
Throughout this article, we denote k ς * ( ϰ 1 , ϰ 2 ) = ς ( ϰ 1 , ϰ 2 ) k ς ( M , N ) ; C L ( Ω ) as the closed subsets of Ω ; K ( Ω ) as the compact subsets of Ω ; BPP ( T ) as the set of BPP(s) of T ; and FP ( T ) as the set of FP(s) of T .
Definition 4.
Let ( Ω , ς ) be a b-MS and for every M , N 2 Ω , the Pompeiu–Hausdorff metric induced by ς is given by
H ( M , N ) = max { sup m M ς ( m , N ) , sup n N ς ( M , n ) } , if M N 0 , if M = N = + , otherwise
where ς ( m , N ) = inf { ς ( m , n ) , n N } .
Definition 5
([12]). Let ( Ω , ς ) be an MS, M , N C L ( Ω ) and α : M × M [ 0 , ) . T : M N is a Suzuki-type generalized α ψ contraction if
ς ( m 1 , T m 1 ) ς ( M , N ) α ( m 1 , m 2 ) ς ( m 1 , m 2 )
implies ς ( T m 1 , T m 2 ) ψ ( Γ ( m 1 , m 2 ) ) ,
for all m 1 , m 2 M , where ψ Ψ and
Γ ( m 1 , m 2 ) = max ς ( m 1 , m 2 ) , ς ( m 1 , T m 1 ) ς ( M , N ) , ς ( m 2 , T m 2 ) ς ( M , N ) , ς ( m 2 , T m 1 ) ς ( M , N ) , ς ( m 1 , T m 2 ) ς ( M , N ) 2 , ( ς ( m 1 , T m 1 ) ς ( M , N ) ) ( ς ( m 2 , T m 2 ) ς ( M , N ) ) 1 + ς ( m 1 , m 2 ) .
Theorem 1
([12]). Let ( Ω , ς ) be a complete MS, and M , N C L ( Ω ) with ( M , N ) has P p . T : M N is α p , a Suzuki-type generalized α ψ contraction, and for nonempty set M 0 , T ( M 0 ) N 0 . Also suppose α ( m 0 , m 1 ) p ( m 0 , m 1 ) and ς ( m 1 , T m 0 ) = ς ( M , N ) for some m 0 , m 1 in M 0 , and T are continuous. Then, BPP ( T ) is singleton.
In the following, we introduce generalized multivalued Suzuki-type α ψ contractions in b-MS.
Definition 6.
Let ( Ω , ς ) be a b-MS, M , N C L ( Ω ) . T : M C L ( N ) is called a generalized multivalued Suzuki-type α ψ contraction of ϖ type if
ς * ( m 1 , T m 1 ) α ( m 1 , m 2 ) ς ( m 1 , m 2 ) implies H ( T m 1 , T m 2 ) ψ ( ϖ ( m 1 , m 2 ) ) ,
for all m 1 , m 2 M , where α : M × M [ 0 , ) , ψ Ψ and
ϖ ( m 1 , m 2 ) = max ς ( m 1 , m 2 ) , ς ( m 1 , T m 1 ) k ς ( M , N ) k , ς ( m 2 , T m 2 ) k ς ( M , N ) k , ς ( m 2 , T m 1 ) ς ( M , N ) , ς ( m 1 , T m 2 ) k ς ( M , N ) 2 k 2 , ( ς ( m 1 , T m 1 ) k ς ( M , N ) ) ( ς ( m 2 , T m 2 ) k ς ( M , N ) ) k ( 1 + k ς ( m 1 , m 2 ) .
Definition 7.
Let ( Ω , ς ) be a b-MS, M , N C L ( Ω ) . T : M C L ( N ) is called a generalized multivalued Suzuki-type α ψ contraction of ξ type if
ς * ( m 1 , T m 1 ) α ( m 1 , m 2 ) ς ( m 1 , m 2 ) implies H ( T m 1 , T m 2 ) ψ ( ξ ( m 1 , m 2 ) ) ,
for all m 1 , m 2 M , where α : M × M [ 0 , ) , ψ Ψ and
ξ ( m 1 , m 2 ) = max ς ( m 1 , m 2 ) , ς ( m 1 , T m 1 ) k ς ( M , N ) k ς ( m 2 , T m 2 ) k ς ( M , N ) k , ς ( m 2 , T m 1 ) k ς ( M , N ) k .
Definition 8.
Let ( Ω , ς ) be a b-MS, M , N C L ( Ω ) . T : M N C L ( M ) C L ( N ) is called a generalized multivalued Suzuki-type α ψ cyclic contraction of ϖ type if
ς * ( m 1 , T m 1 ) α ( m 1 , m 2 ) ς ( m 1 , m 2 ) implies H ( T m 1 , T m 2 ) ψ ( ϖ ( m 1 , m 2 ) ) ,
for all m 1 , m 2 M N , where α : M N × M N [ 0 , ) , ψ Ψ and
ϖ ( m 1 , m 2 ) = max ς ( m 1 , m 2 ) , ς ( m 1 , T m 1 ) k ς ( M , N ) k , ς ( m 2 , T m 2 ) k ς ( M , N ) k , ς ( m 2 , T m 1 ) ς ( M , N ) , ς ( m 1 , T m 2 ) k ς ( M , N ) 2 k 2 , ( ς ( m 1 , T m 1 ) k ς ( M , N ) ) ( ς ( m 2 , T m 2 ) k ς ( M , N ) ) k ( 1 + k ς ( m 1 , m 2 ) .
Definition 9.
Let ( Ω , ς ) be a b-MS, M , N C L ( Ω ) . T : M N C L ( M ) C L ( N ) is called a generalized multivalued Suzuki-type α ψ cyclic contraction of ξ type if
ς * ( m 1 , T m 1 ) α ( m 1 , m 2 ) ς ( m 1 , m 2 ) implies H ( T m 1 , T m 2 ) ψ ( ϖ ( m 1 , m 2 ) ) ,
for all m 1 , m 2 M N , where α : M N × M N [ 0 , ) , ψ Ψ and
ξ ( m 1 , m 2 ) = max ς ( m 1 , m 2 ) , ς ( m 1 , T m 1 ) k ς ( M , N ) k ς ( m 2 , T m 2 ) k ς ( M , N ) k , ς ( m 2 , T m 1 ) k ς ( M , N ) k .
Remark 3.
(i) 
If in Definitions 6 and 7, T : M C L ( N ) is replaced by T : M N , then T is called a generalized Suzuki-type α ψ contraction of ϖ type and a generalized Suzuki-type α ψ cyclic contraction of ξ type, respectively.
(ii) 
If in Definition 6 T : M C L ( N ) is replaced by T : M N , and ϖ is replaced by ϖ , where
ϖ ( m 1 , m 2 ) = max ς ( m 1 , m 2 ) , ς ( m 1 , T m 1 ) k ς ( M , N ) k , ς ( m 2 , T m 2 ) k ς ( M , N ) k , ς ( m 2 , T m 1 ) k ς ( M , N ) k , ς ( m 1 , T m 2 ) k ς ( M , N ) 2 k 2 , ( ς ( m 1 , T m 1 ) k ς ( M , N ) ) ( ς ( m 2 , T m 2 ) k ς ( M , N ) ) k ( 1 + k ς ( m 1 , m 2 ) ,
then T is called a generalized Suzuki-type α ψ contraction of ϖ type.
(iii) 
If in Definitions 8 and 9 T : M N C L ( M ) C L ( N ) is replaced by T : M N M N , then T is called a generalized Suzuki-type α ψ cyclic contraction of ϖ type and a generalized Suzuki-type α ψ cyclic contraction of ξ type, respectively.

2. Best Proximity Points Results for Generalized Multivalued Suzuki-Type  α ψ Contractions

The following is our main result of this section.
Theorem 2.
Let ( Ω , ς ) be a complete b-MS (b-CMS) M , N C L ( Ω ) with M 0 ϕ . Let T : M C L ( N ) be a generalized multivalued Suzuki-type α ψ contraction of ϖ type satisfying:
1. 
For each m M 0 , T ( m ) N 0 and ( M , N ) has a weak P p ;
2. 
T is m α p ;
3. 
There exist elements m 0 and m 1 in M 0 and n 1 T m 0 such that ς ( m 1 , n 1 ) = ς ( M , N ) and α ( m 0 , m 1 ) p ( m 0 , m 1 ) ;
4. 
T is continuous.
Then, BPP ( T ) is nonempty.
Proof. 
From (3), there exist m 0 and m 1 in M 0 and n 1 T m 0 , such that
ς ( m 1 , n 1 ) = ς ( M , N ) , α ( m 0 , m 1 ) p ( m 0 , m 1 ) ;
if n 1 T m 1 , then
ς ( M , N ) ς ( m 1 , T m 1 ) ς ( m 1 , n 1 ) = ς ( M , N ) ,
which implies ς ( m 1 , T m 1 ) = ς ( M , N ) . That is, m 1 is the BPP of T . Next, if n 1 T m 1 , then,
ς ( m 0 , T m 0 ) ς ( m 0 , n 1 ) k ς ( m 0 , m 1 ) + k ς ( m 1 , n 1 ) , ς ( m 0 , T m 0 ) k ς ( m 0 , m 1 ) + k ς ( M , N ) ,
therefore,
k ς * ( m 0 , T m 0 ) k ς ( m 0 , m 1 ) .
Thus, we get:
ς * ( m 0 , T m 0 ) ς ( m 0 , m 1 ) p ( m 0 , m 1 ) ς ( m 0 , m 1 ) α ( m 0 , m 1 ) ς ( m 0 , m 1 ) .
From (4), we get:
H ( T m 0 , T m 1 ) ψ ( ϖ ( m 0 , m 1 ) ) ψ max ς ( m 0 , m 1 ) , ς ( m 0 , T m 0 ) k ς ( M , N ) k , ς ( m 1 , T m 1 ) k ς ( M , N ) k , ς ( m 1 , T m 0 ) ς ( M , N ) , ς ( m 0 , T m 1 ) k ς ( M , N ) 2 k 2 , ς ( m 0 , T m 0 ) k ς ( M , N ) ( ς ( m 1 , T m 1 ) k ς ( M , N ) k ( 1 + k ς ( m 0 , m 1 ) ) ψ max ς ( m 0 , m 1 ) , ς ( m 0 , n 1 ) k ς ( M , N ) k , ς ( m 1 , T m 1 ) k ς ( M , N ) k , ς ( m 1 , n 1 ) ς ( M , N ) , ς ( m 0 , T m 1 ) k 2 ς ( M , N ) 2 k 2 , ς ( m 0 , n 1 ) k ς ( M , N ) ( ς ( m 1 , T m 1 ) k ς ( M , N ) k ( 1 + k ς ( m 0 , m 1 ) ) .
Hence,
H ( T m 0 , T m 1 ) ψ max ς ( m 0 , m 1 ) , ς ( n 1 , T m 1 ) .
Consequently,
ς ( n 1 , T m 1 ) H ( T m 0 , T m 1 ) ψ max ς ( m 0 , m 1 ) , ς ( n 1 , T m 1 ) .
If max ς ( m 0 , m 1 ) , ς ( n 1 , T m 1 ) = ς ( n 1 , T m 1 ) , then
ς ( n 1 , T m 1 ) ψ ( ς ( n 1 , T m 1 ) < ς ( n 1 , T m 1 ) ,
which is a contradiction. Hence,
ς ( n 1 , T m 1 ) ψ ( ς ( m 0 , m 1 ) ) .
Now for q > 1 , there exists n 2 T m 1 such that
ς ( n 1 , n 2 ) < q ς ( n 1 , T m 1 ) ,
and using (7), we have
ς ( n 1 , n 2 ) < q ψ ( ς ( m 0 , m 1 ) ) .
As n 2 T m 1 N 0 , there exists m 2 M 0 such that
ς ( m 2 , n 2 ) = ς ( M , N ) .
Note that m 2 m 1 ; otherwise, m 1 becomes the BPP of T . From (6) and (9), we get
α ( m 0 , m 1 ) p ( m 0 , m 1 ) , ς ( m 1 , n 1 ) = ς ( M , N ) , ς ( m 2 , n 2 ) = ς ( M , N ) .
As T is m α p , and ( M , N ) satisfies the weak P p , we obtain
α ( m 1 , m 2 ) p ( m 1 , m 2 ) , ς ( m 1 , m 2 ) ς ( n 1 , n 2 ) .
From (8) and (10), we get:
ς ( m 1 , m 2 ) ς ( n 1 , n 2 ) < q ψ ( ς ( m 0 , m 1 ) ) .
Since ψ is strictly increasing, therefore,
ψ ς ( m 1 , m 2 ) < ψ ( q ψ ( ς ( m 0 , m 1 ) ) ) .
Set
q 1 = ψ ( q ψ ( ς ( m 0 , m 1 ) ) ) ψ ( ς ( m 1 , m 2 ) ) > 1 .
If n 2 T m 2 , then m 2 is the BPP of T and the proof completes. So, suppose n 2 T m 2 , then
ς ( m 1 , T m 1 ) ς ( m 1 , n 2 ) k ς ( m 1 , m 2 ) + k ς ( m 2 , n 2 ) ;
therefore,
ς * ( m 1 , T m 1 ) ς ( m 1 , m 2 ) p ( m 1 , m 2 ) ς ( m 1 , m 2 ) α ( m 1 , m 2 ) ς ( m 1 , m 2 ) .
From (4), we get:
H ( T m 1 , T m 2 ) ψ ( ϖ ( m 1 , m 2 ) ) ,
where
ϖ ( m 1 , m 2 ) = max ς ( m 1 , m 2 ) , ς ( m 1 , T m 1 ) k ς ( M , N ) k , ς ( m 2 , T m 2 ) k ς ( M , N ) k , ς ( m 2 , T m 1 ) ς ( M , N ) , ς ( m 1 , T m 2 ) k ς ( M , N ) 2 k 2 , ς ( m 1 , T m 1 ) k ς ( M , N ) ( ς ( m 2 , T m 2 ) k ς ( M , N ) k ( 1 + k ς ( m 1 , m 2 ) ) max ς ( m 1 , m 2 ) , ς ( n 2 , T m 2 ) .
Hence,
H ( T m 1 , T m 2 ) ψ max ς ( m 1 , m 2 ) , ς ( n 2 , T m 2 ) .
This implies
ς ( n 2 , T m 2 ) H ( T m 1 , T m 2 ) ψ max ς ( m 1 , m 2 ) , ς ( n 2 , T m 2 ) .
If max ς ( m 1 , m 2 ) , ς ( n 2 , T m 2 ) = ς ( n 2 , T m 2 ) , then
ς ( n 2 , T m 2 ) ψ ( ς ( n 2 , T m 2 ) < ς ( n 2 , T m 2 ) ,
which is a contradiction. Hence,
ς ( n 2 , T m 2 ) ψ ( ς ( m 1 , m 2 ) ) .
Now, again for q 1 > 1 , there exists n 3 T m 2 such that
ς ( n 2 , n 3 ) < q 1 ς ( n 2 , T m 2 ) q 1 ψ ( ς ( m 1 , m 2 ) ) .
From above and (12), we get
ς ( n 2 , n 3 ) ψ ( q ψ ( ς ( m 0 , m 1 ) ) .
As n 3 T m 2 N 0 , there exists m 3 M 0 such that
ς ( m 3 , n 3 ) = ς ( M , N ) .
Note that m 3 m 2 ; otherwise, m 2 becomes the BPP of T . From (6) and (14), we get
α ( m 1 , m 2 ) p ( m 1 , m 2 ) , ς ( m 2 , n 2 ) = ς ( M , N ) , ς ( m 3 , n 3 ) = ς ( M , N ) .
As T is m α p and ( M , N ) satisfies the weak P p , we obtain
α ( m 2 , m 3 ) p ( m 2 , m 3 ) , ς ( m 2 , m 3 ) ς ( n 2 , n 3 ) ,
From (13) and (15), we get
ς ( m 2 , m 3 ) ψ ( q ψ ( ς ( m 0 , m 1 ) ) .
Since ψ is strictly increasing, therefore
ψ ( ς ( m 2 , m 3 ) ) ψ 2 ( q ψ ( ς ( m 0 , m 1 ) ) .
Continuing this, we obtain sequences { m μ } M 0 and { n μ } N 0 , such that
α ( m μ , m μ + 1 ) p ( m μ , m μ + 1 ) , ς ( m μ + 1 , n μ + 1 ) = ς ( M , N ) , ς ( m μ + 2 , n μ + 2 ) = ς ( M , N ) ,
ς ( n μ + 1 , n μ + 2 ) < q μ ( ψ ( ς ( m μ , m μ + 1 ) ) ) ,
where
q μ = ψ μ ( q ψ ( ς ( m 0 , m 1 ) ) ) ψ ( ς ( m μ , m μ + 1 ) ) > 1 ,
for all μ N . Using (19) in (18) we get
ς ( n μ + 1 , n μ + 2 ) < ψ μ ( q ψ ( ς ( m 0 , m 1 ) ) ) ,
for all μ N . Since T is m α p and ( M , N ) satisfies the weak P p , we obtain
α ( m μ + 1 , m μ + 2 ) p ( m μ + 1 , m μ + 2 ) , ς ( m μ + 1 , m μ + 2 ) ς ( n μ + 1 , n μ + 2 ) .
Now, to prove { m μ } is a Cauchy sequence in M, let ε > 0 be given. Since
μ = 1 k μ ψ μ ( q ψ ( ς ( m 1 , m 0 ) ) < ,
there exists some positive integer h = h ( ε ) such that
l h k l ψ l ( q ψ ( ς ( m 1 , m 0 ) ) < ε .
Using the triangular inequality, we obtain
ς ( m μ , m λ ) k ς ( m μ , m μ + 1 ) + k 2 ς ( m μ + 1 , m μ + 2 ) + · · · + k λ μ ς ( m λ 1 , m λ ) . .
This implies
ς ( m μ , m λ ) k ψ μ 1 ( q ψ ( ς ( m 1 , m 0 ) + k 2 ψ μ ( q ψ ( ς ( m 1 , m 0 ) ) + · · · · · + k λ 2 ψ λ 1 ( q ψ ( ς ( m 1 , m 0 ) ) 1 k μ 2 ( k μ 1 ψ μ 1 ( q ψ ( ς ( m 1 , m 0 ) ) + k μ ψ μ ( q ψ ( ς ( m 1 , m 0 ) ) + · · · · · + k λ 2 ψ λ 2 ( q ψ ( ς ( m 1 , m 0 ) ) ) 1 k μ 2 i = μ λ 1 k i ψ i ( q ψ ( ς ( m 1 , m 0 ) ) 1 k μ 2 i h k i ψ i ( q ψ ( ς ( m 1 , m 0 ) ) < 1 k μ 2 ε ε ,
for all λ > μ > h > h , where h = max { 2 , h } . Thus, { m μ } is a Cauchy sequence in M . Similarly, { n μ } is a Cauchy sequence in N . Since ( Ω , ς ) is complete and M and N are closed, there exist m * M and n * N such that m μ m * and n μ n * as μ , respectively. Since ς ( m μ , n μ ) ς ( M , N ) for all μ N . We conclude
lim μ ς ( m μ , n μ ) = ς ( m * , n * ) = ς ( M , N ) .
Continuity of T implies
lim μ H ( T m μ , T m * ) = 0 .
As n μ + 1 T m μ :
ς ( n * , T m * ) k ς ( n * , n μ + 1 ) + k ς ( n μ + 1 , T m * ) k ς ( n * , n μ + 1 ) + k H ( T m μ , T m * ) .
Letting μ , we get:
ς ( n * , T m * ) 0 ,
which implies n * T m * ¯ = T m * . Furthermore,
ς ( M , N ) ς ( m * , T m * ) ς ( m * , n * ) = ς ( M , N ) ;
hence,
ς ( m * , T m * ) = ς ( M , N ) ,
which implies m * is a BPP ( T ) .
Next is the single-valued version of Theorem 2.
Theorem 3.
Let ( Ω , ς ) be a b-CMS, M , N C L ( Ω ) with M 0 ϕ . Let T : M N be a generalized Suzuki-type α ψ contraction of ϖ type satisfying the following:
1. 
For each m M 0 , we have T ( m ) N 0 , and ( M , N ) has the P p ;
2. 
T is α p ;
3. 
There exist elements m 0 and m 1 in M 0 such that ς ( m 1 , T m 0 ) = ς ( M , N ) and α ( m 0 , m 1 ) p ( m 0 , m 1 ) ;
4. 
T is continuous.
Then, BPP ( T ) is nonempty.
Proof. 
The proof follows from Theorem 2. □
Corollary 1.
Let ( Ω , ς ) be a b-CMS, M , N C L ( Ω ) with M 0 ϕ . Let T : M N be a generalized Suzuki-type α ψ contraction of ϖ type satisfying the following:
1. 
For each m M 0 , we have T ( m ) N 0 , and ( M , N ) has the P p ;
2. 
T is α p ;
3. 
There exist elements m 0 and m 1 in M 0 such that ς ( m 1 , T m 0 ) = ς ( M , N ) and α ( m 0 , m 1 ) p ( m 0 , m 1 ) ;
4. 
T is continuous.
Then, BPP ( T ) is singleton.
Proof. 
The existence of BPP directly follows from Theorem 2. For uniqueness, suppose on the contrary that m 1 and m 2 are two distinct BPP(s). Then,
ς ( m 1 , T m 1 ) = ς ( M , N ) , ς ( m 2 , T m 2 ) = ς ( M , N ) .
Then, P p implies
ς ( m 1 , m 2 ) = ς ( T m 1 , T m 2 ) .
Now,
ς * ( m 1 , T m 1 ) = 1 k ( ς ( m 1 , T m 1 ) k ς ( M , N ) ) = 1 k ( ς ( M , N ) k ς ( M , N ) ) 0 α ( m 1 , m 2 ) ς ( m 1 , m 2 ) ,
which implies
ς ( T m 1 , T m 2 ) ψ ( ϖ ( m 1 , m 2 ) ) .
It further implies
ς ( m 1 , m 2 ) ψ ( ϖ ( m 1 , m 2 ) ) ψ ( ς ( m 1 , m 2 ) ) < ς ( m 1 , m 2 ) ,
which is a contradiction. Hence, BPP ( T ) is singleton. □
Remark 4.
If we take b = 1 and p = 1 , then Theorem 1 becomes the corollary of Corollary 1.
Now, we prove the following result without the assumption of continuity of the mapping T .
Theorem 4.
Let ( Ω , ς ) be a b-CMS, M , N K ( Ω ) with M 0 ϕ . Let T : M K ( N ) be a generalized multivalued Suzuki-type α ψ contraction of ξ type satisfying the following:
1. 
For each m M 0 , we have T ( m ) N 0 , and ( M , N ) has a weak P p ;
2. 
T is m α p ;
3. 
There exist elements m 0 and m 1 in M 0 and n 1 T m 0 such that ς ( m 1 , n 1 ) = ς ( M , N ) and α ( m 0 , m 1 ) p ( m 0 , m 1 ) 2 k ;
4. 
If { m μ } is a sequence in M such that α ( m μ , m μ + 1 ) p ( m μ , m μ + 1 ) 2 k and m μ m M as μ , then there exists a subsequence { m μ l } of { m μ } such that α ( m μ l , m ) p ( m μ l , m ) 2 k for all l 1 .
Then, BPP ( T ) is nonempty.
Proof. 
From Theorem 2, we have:
ς ( n 1 , T m 1 ) ψ ( ς ( m 0 , m 1 ) ) ,
as T m 1 is compact; therefore, there exists n 2 T m 1 such that
ς ( n 1 , n 2 ) = ς ( n 1 , T m 1 ) .
Using (23) in (24), we get
ς ( n 1 , n 2 ) ψ ( ς ( m 0 , m 1 ) ) .
By assumption (1), we have T m 1 N 0 , so there exists m 2 m 1 M 0 such that
ς ( m 2 , n 2 ) = ς ( M , N ) ;
otherwise, m 1 is the BPP of T . From (6) and (26), we get
α ( m 0 , m 1 ) p ( m 0 , m 1 ) , ς ( m 1 , n 1 ) = ς ( M , N ) , ς ( m 2 , n 2 ) = ς ( M , N ) .
As T is m α p and ( M , N ) satisfies the weak P p , we obtain
α ( m 1 , m 2 ) p ( m 1 , m 2 ) , ς ( m 1 , m 2 ) ς ( n 1 , n 2 ) ,
so
ς ( m 1 , m 2 ) ς ( n 1 , n 2 ) < ψ ( ς ( m 0 , m 1 ) ) .
Continuing in a similar way as in Theorem 2, we get sequences { m μ } in M 0 and { n μ } in N 0 such that
α ( m μ , m μ + 1 ) p ( m μ , m μ + 1 ) and m μ m μ + 1 ,
n μ T m μ 1 and n μ T m μ ,
ς ( m μ , n μ ) = ς ( M , N ) and ς ( m μ , m μ + 1 ) ς ( n μ , n μ + 1 ) ψ ( ς ( m μ 1 , m μ ) ) ) .
Along similar lines as in Theorem 2, we can prove that { m μ } and { n μ } are Cauchy sequences in M and N, respectively. Since ( Ω , ς ) is complete and M and N are closed, there exist m * M and n * N such that m μ m * and n μ n * as μ , respectively, and ς ( m * , n * ) = ς ( M , N ) . Now, we show that m * is the BPP of T . If there exists a subsequence { m μ l } of { m μ } such that T m μ l = T m * for all l 1 , then
ς ( M , N ) ς ( m μ l + 1 , T m μ l ) ς ( m μ l + 1 , n μ l + 1 ) = ς ( M , N ) , ς ( M , N ) ς ( m μ l + 1 , T m * ) ς ( M , N ) for all l 1 .
Letting l , we obtain
ς ( M , N ) ς ( m * , T m * ) ς ( M , N ) .
Hence, m * is the BPP of T . Thus, we may assume T m μ T m * for all μ N . From assumption (4), we have a subsequence { m μ l } of { m μ } such that α ( m μ l , m * ) p ( m μ l , m * ) 2 k for all l 1 . For n μ l + 1 T m μ l
ς ( m μ l , T m μ l ) ς ( m μ l , n μ l + 1 ) k ς ( m μ l , m μ l + 1 ) + k ς ( m μ l + 1 , n μ l + 1 ) , ς ( m μ l , T m μ l ) k ς ( m μ l , m μ l + 1 ) + k ς ( M , N ) ;
therefore,
ς * ( m μ l , T m μ l ) ς ( m μ l , m μ l + 1 )
and
k ς * ( m μ l + 1 , T m μ l + 1 ) = ς ( m μ l + 1 , T m μ l + 1 ) k ς ( M , N ) k ς ( m μ l + 1 , m μ l + 2 ) + k ς ( m μ l + 2 , T m μ l + 1 ) k ς ( M , N ) k ς ( m μ l + 1 , m μ l + 2 ) + k ς ( m μ l + 2 , n μ l + 2 ) k ς ( M , N ) .
Using ς ( m μ l + 2 , n μ l + 2 ) = ς ( M , N ) and (27), we get
ς * ( m μ l + 1 , T m μ l + 1 ) ς ( m μ l + 1 , m μ l + 2 ) < ς ( m μ l , m μ l + 1 ) ,
and adding (28) and (29), we get
ς * ( m μ l , T m μ l ) + ς * ( m μ l + 1 , T m μ l + 1 ) < 2 ς ( m μ l , m μ l + 1 ) .
Now, for α ( m μ l , m * ) p ( m μ l , m * ) 2 k , if for some l N ,
ς * ( m μ l , T m μ l ) α ( m μ l , m * ) ς ( m μ l , m * )
and
ς * ( m μ l + 1 , T m μ l + 1 ) α ( m μ l + 1 , m * ) ς ( m μ l + 1 , m * )
holds, then we get
ς * ( m μ l , T m μ l ) α ( m μ l , m * ) ς ( m μ l , m * ) 2 k ς ( m μ l , m * )
and
ς * ( m μ l + 1 , T m μ l + 1 ) α ( m μ l + 1 , m * ) ς ( m μ l + 1 , m * ) 2 k ς ( m μ l + 1 , m * ) .
By triangular inequality,
2 ς ( m μ l , m μ l + 1 ) 2 k ς ( m μ l , m * ) + 2 k ς ( m μ l + 1 , m * ) ς * ( m μ l , T m μ l ) + ς * ( m μ l + 1 , T m μ l + 1 ) < 2 ς ( m μ l , m μ l + 1 ) ,
which is a contradiction. Hence, either
ς * ( m μ l + 1 , T m μ l + 1 ) α ( m μ l + 1 , m * ) ς ( m μ l + 1 , m * )
or
ς * ( m μ l , T m μ l ) α ( m μ l , m * ) ς ( m μ l , m * )
holds for infinitely many l N . If (32) holds for infinitely many l N , then from (5), we get
H ( T m μ l , T m * ) ψ ( ξ ( m μ l , m * ) ) .
For n μ l + 1 T m μ l , we have ς ( n μ l + 1 , T m * ) H ( T m μ l , T m * ) ; therefore,
ς ( n μ l + 1 , T m * ) ψ ξ ( m μ l , m * ) ) ,
where
ξ ( m μ l , m * ) = max ς ( m μ l , m * ) , ς ( m μ l , T m μ l ) k ς ( M , N ) k , ς ( m * , T m * ) k ς ( M , N ) k , ς ( m * , T m μ l ) k ς ( M , N ) k max ς ( m μ l , m * ) , ς ( m μ l , m μ l + 1 ) , ς ( m * , T m * ) k ς ( M , N ) k , ς ( m * , m μ l + 1 ) ,
if
max ς ( m μ l , m * ) , ς ( m μ l , m μ l + 1 ) , ς ( m * , T m * ) k ς ( M , N ) k , ς ( m * , m μ l + 1 ) = ς ( m * , T m * ) k ς ( M , N ) k .
Then, from (34), we have
ς ( n μ l + 1 , T m * ) ψ ς ( m * , T m * ) k ς ( M , N ) k .
By triangular inequality, we have
1 k ( ς ( m μ l + 1 , T m * ) k ς ( T m μ l , m μ l + 1 ) ) ς ( T m μ l , T m * ) ς ( n μ l + 1 , T m * ) .
Using the fact that n μ l + 1 T m μ l and by (35)
1 k ( ς ( m μ l + 1 , T m * ) k ς ( M , N ) ) ψ ς ( m * , T m * ) k ς ( M , N ) k .
Letting l and using ψ ( Υ ) < Υ , we get
ς ( m * , T m * ) k ς ( M , N ) k < ς ( m * , T m * ) k ς ( M , N ) k ,
which is a contradiction. Hence,
ς ( n μ l + 1 , T m * ) ψ max ς ( m μ l , m * ) , ς ( m μ l , m μ l + 1 ) , ς ( m * , m μ l + 1 ) .
Letting l , we get
n * T m * .
Hence,
ς ( M , N ) ς ( m * , T m * ) ς ( m * , n * ) = ς ( M , N ) .
Hence,
ς ( m * , T m * ) = ς ( M , N ) ,
which implies m * BPP ( T ) . Similarly, if (33) holds for infinitely many l N , the conclusion holds. □
Theorem 5.
Let ( Ω , ς ) be a b-CMS, M , N C L ( Ω ) with M 0 ϕ . Let T : M N be a generalized Suzuki-type α ψ contraction of ξ type satisfying the following:
1. 
For each m M 0 , we have T ( m ) N 0 , and ( M , N ) has the P p ;
2. 
T is α p ;
3. 
There exist elements m 0 and m 1 in M 0 and n 1 = T m 0 such that ς ( m 1 , n 1 ) = ς ( M , N ) and α ( m 0 , m 1 ) p ( m 0 , m 1 ) 2 k ;
4. 
If { m μ } is a sequence in M such that α ( m μ , m μ + 1 ) p ( m μ , m μ + 1 ) 2 k and m μ m M as μ , then there exists a subsequence { m μ l } of { m μ } such that α ( m μ l , m ) p ( m μ l , m ) 2 k for all l 1 .
Then, BPP ( T ) is singleton.
Proof. 
The existence of BPP(s) follows from Theorem 4, and the uniqueness follows from Theorem 3. □
We give an example to illustrate the above theorems.
Example 1.
Let Ω = R 2 , ς ( P 1 , P 2 ) = x 1 x 2 2 + y 1 y 2 2 , where
P 1 ( x 1 , y 1 ) , P 2 ( x 2 , y 2 ) Ω .
Then, ς is a b-metric with k = 2 . Let
M = ( 1 , 2 μ ) : μ N 1 , N = 0 , 1 2 μ : μ N 1 { ( 0 , 0 ) } ,
which implies
ς ( M , N ) = 1 .
Define mapping T : M 2 N as
T ( 1 , 2 μ ) = 0 , 1 2 a : 0 a μ .
We have
M 0 = { ( 1 , 1 ) } and N 0 = { ( 0 , 1 ) } ,
which implies
T ( M 0 ) N 0 .
α ( ϰ 1 , ϰ 2 ) = ς ( ϰ 1 , ϰ 2 ) if ϰ 1 ϰ 2 , 2 otherwise , , ψ ( Υ ) = 9 10 Υ , and p ( ϰ 1 , ϰ 2 ) = 2 .
Let P 1 = ( 1 , 2 μ 1 ) , P 2 = ( 1 , 2 μ 2 ) M , where μ 2 > μ 1 .
Now,
T ( P 1 ) = 0 , 1 2 μ 1 , · · · , ( 0 , 1 ) and T ( P 2 ) = 0 , 1 2 μ 2 , · · · , ( 0 , 1 ) .
It implies
H ( T ( P 1 ) , T ( P 2 ) ) = 1 2 μ 1 1 2 μ 2 2 = 2 μ 2 μ 1 1 2 μ 2 2 ,
as μ 2 μ 1 μ 2 it implies 2 μ 2 μ 1 1 2 μ 2 2 < 1 4 ; therefore,
H ( T ( P 1 ) , T ( P 2 ) ) < 1 4 .
Now, consider
ς ( P 1 , P 2 ) = 2 μ 2 2 μ 1 2 1 ;
it implies
ϖ ( x , y ) 1 .
Therefore,
ψ ( ϖ ( x , y ) ) 9 10 ,
(36) and (37) implies
H ( T ( P 1 ) , T ( P 2 ) ) < ψ ( ϖ ( x , y ) ) .
Therefore, T is generalized multivalued Suzuki-type α ψ contraction of ϖ type. Note that T ( M 0 ) N 0 and ( M , N ) satisfies a weak P p . Furthermore, T is clearly m α p . Theorem 2 implies T has a BPP, which is ( 1 , 1 ) .
Now, we give an example that satisfies all the conditions of Theorem 3, whereas Theorem 1 will not be applicable.
Example 2.
Let Ω = { 1 , 2 , 3 , 4 , 5 } , such that
ς ( 1 , 2 ) = 1 , ς ( 1 , 3 ) = 5 , ς ( 1 , 4 ) = 4 , ς ( 1 , 5 ) = 8 , ς ( 2 , 3 ) = 3 , ς ( 2 , 4 ) = 6 , ς ( 2 , 5 ) = 9 , ς ( 3 , 4 ) = 7 , ς ( 3 , 5 ) = 10 , ς ( 4 , 5 ) = 13 , ς ( x , y ) = ς ( y , x ) and ς ( x , x ) = 0 for all x , y in Ω .
ς is not metric because
ς ( 1 , 3 ) = 5 1 + 3 = ς ( 1 , 2 ) + ς ( 2 , 3 ) .
For k = 5 4 , ( Ω , ς ) is a b-MS.
Suppose M = { 2 , 4 } and N = { 1 , 3 , 5 } . Define T : M N by
T ( 2 ) = 1 , T ( 4 ) = 3 .
α ( ϰ 1 , ϰ 2 ) = ς ( ϰ 1 , ϰ 2 ) if ϰ 1 ϰ 2 , 0 otherwise , , ψ ( Υ ) = 9 10 Υ , and p ( ϰ 1 , ϰ 2 ) = 2 .
Note that
ς ( M , N ) = 1 , M 0 = { 2 } and N 0 = { 1 } .
Here, we discuss different cases. Case (i), x = 2 , y = 4 , is as follows:
ς ( 2 , T 2 ) k ς ( M , N ) = ς ( 2 , 1 ) k ς ( M , N ) = 1 5 4 = 1 4 36 = α ( 2 , 4 ) ς ( 2 , 4 ) ,
and
ς ( T 2 , T 4 ) = ς ( 1 , 3 ) = 5 9 10 ( 6 ) = ψ ( ϖ ( 2 , 4 ) ) .
Case (ii), x = 4 , y = 2 , is as follows:
ς ( 4 , T 4 ) k ς ( M , N ) = ς ( 4 , 3 ) = 7 5 4 = 23 4 36 = α ( 4 , 2 ) ς ( 4 , 2 ) ,
and
ς ( T 4 , T 2 ) = ς ( 3 , 1 ) = 5 9 10 ( 6 ) = ψ ( ϖ ( 4 , 2 ) .
Therefore T is a Suzuki-type generalized α ψ contraction of ϖ type. Note that T ( M 0 ) N 0 , and the pair ( M , N ) has P p . Furthermore, T is clearly α p . All axioms of Theorems 3, hold. Therefore, T has a unique BPP, which is 2 .
However, if we define the usual metric d ( x , y ) = x y on Ω , then Theorem 1 is not applicable. For instance, if x = 2 ,   y = 4 , then
d ( 2 , T 2 ) d ( M , N ) = d ( 2 , 1 ) d ( M , N ) = 0 4 = α ( 2 , 4 ) d ( 2 , 4 ) ,
whereas
d ( T 2 , T 4 ) = d ( 1 , 3 ) = 2 9 10 ( 2 ) = ψ ( Γ ( 2 , 4 ) .
Therefore, our results are the proper generalization of the results already exist in the literature.

3. Best Proximity Points Results for Generalized Multivalued Suzuki-Type α ψ Cyclic Contractions

In this section, we derive the existence of BPP(s) for generalized multivalued Suzuki-type α ψ cyclic contractions.
Theorem 6.
Let ( Ω , ς ) be a b-CMS, M , N C L ( Ω ) with M 0 ϕ . Let T : M N C L ( M ) C L ( N ) be a generalized multivalued Suzuki-type α ψ cyclic contraction of ϖ type satisfying the following:
(i) 
For every m M 0 , T ( m ) N 0 , and for every n N 0 , T ( n ) M 0 . ( M , N ) has the weak P p ;
(ii) 
T is m α p ;
(iii) 
For m 0 , m 1 in M 0 and n 1 T m 0 such that ς ( m 1 , n 1 ) = ς ( M , N ) and α ( m 0 , m 1 ) p ( m 0 , m 1 ) for n 0 and n 1 in N 0 and m 1 T n 0 , such that ς ( m 1 , n 1 ) = ς ( M , N ) and α ( n 0 , n 1 ) p ( n 0 , n 1 ) ;
(iv) 
T is continuous.
Then, there exist m * M such that ς ( m * , T m * ) = ς ( M , N ) and n * N such that ς ( n * , T n * ) = ς ( M , N ) .
Proof. 
Consider the restrictions T : M C L ( N ) and T : N C L ( M ) of T on M and N, defined as
T ( m ) = T ( m ) for all m M and T ( n ) = T ( n ) for all n N ,
respectively. Then, T and T satisfy all the conditions of Theorem 2. Hence, by Theorem 2, with mappings T and T , there exist m * M such that
ς ( m * , T m * ) = ς ( m * , T m * ) = ς ( M , N )
and n * N such that ς ( n * , T n * ) = ς ( n * , T n * ) = ς ( M , N ) . This completes the proof. □
Theorem 7.
Let ( Ω , ς ) be a b-CMS, M , N C L ( Ω ) with M 0 ϕ . Let T : M N M N be a generalized Suzuki-type α ψ cyclic contraction of ϖ type satisfying the following conditions:
(i) 
For every m M 0 , T ( m ) N 0 , and for every n N 0 , T ( n ) M 0 ; ( M , N ) has the P p ;
(ii) 
T is m α p ;
(iii) 
For m 0 , m 1 in M 0 and n 1 = T m 0 such that ς ( m 1 , n 1 ) = ς ( M , N ) and α ( m 0 , m 1 ) p ( m 0 , m 1 ) and for n 0 and n 1 in N 0 and m 1 = T n 0 , such that ς ( m 1 , n 1 ) = ς ( M , N ) and α ( n 0 , n 1 ) p ( n 0 , n 1 ) ;
(iv) 
T is continuous.
Then there exist m * M such that ς ( m * , T m * ) = ς ( M , N ) and n * N such that ς ( n * , T n * ) = ς ( M , N ) .
Proof. 
Following along similar lines of Theorem 6, we will obtain the required results. □
In the following, we derived some fixed-points theorems from our main results.
If we take M = N = Ω in Theorems 2 and 4, then we have the following results.
Theorem 8.
Let ( Ω , ς ) be a b-CMS and T : Ω C L ( Ω ) be an α p such that
ς ( ϰ 1 , T ϰ 1 ) k α ( ϰ 1 , y ) ς ( ϰ 1 , ϰ 2 ) implies H ( T ϰ 1 , T ϰ 2 ) ψ ( ϖ ( ϰ 1 , ϰ 2 ) ) ,
for all ϰ 1 , ϰ 2 Ω where ψ Ψ satisfying the following:
(i) 
There exists ϰ 0 Ω such that α ( ϰ 0 , T ϰ 0 ) p ( ϰ 0 , T ϰ 0 ) ;
(ii) 
T is continuous.
Then, FP ( T ) is nonempty.
Theorem 9.
Let ( Ω , ς ) be a b-CMS and T : Ω K ( Ω ) be an α p such that
ς ( ϰ 1 , T ϰ 1 ) k α ( ϰ 1 , ϰ 2 ) ς ( ϰ 1 , ϰ 2 ) implies H ( T ϰ 1 , T ϰ 2 ) ψ ( ξ ( ϰ 1 , ϰ 2 ) ) ,
for all ϰ 1 , ϰ 2 Ω , where ψ Ψ satisfies the following:
(i) 
There exists ϰ 0 Ω such that α ( ϰ 0 , T ϰ 0 ) p ( ϰ 0 , T ϰ 0 ) 2 k ;
(ii) 
If { ϰ μ } is a sequence in Ω such that α ( ϰ μ , ϰ μ + 1 ) p ( ϰ μ , ϰ μ + 1 ) 2 k and ϰ μ ϰ Ω as μ , then there exists a subsequence { ϰ μ l } of { ϰ μ } such that α ( ϰ μ l , ϰ ) p ( ϰ μ l , ϰ ) 2 k for all l 1 .
Then, FP ( T ) is nonempty.
If we take ψ ( Υ ) = q Υ in Theorems 8 and 9, where 0 q < 1 , then we can conclude the following theorems.
Theorem 10.
Let ( Ω , ς ) be a b-CMS and T : Ω C L ( Ω ) be an α p such that
ς ( ϰ 1 , T ϰ 1 ) k α ( ϰ 1 , ϰ 2 ) ς ( ϰ 1 , ϰ 2 ) implies H ( T ϰ 1 , T ϰ 2 ) q ( ϖ ( ϰ 1 , ϰ 2 ) ) ,
for all ϰ 1 , ϰ 2 Ω , where q [ 0 , 1 ) satisfies the following:
(i) 
There exists ϰ 0 Ω such that α ( ϰ 0 , T ϰ 0 ) p ( ϰ 0 , T ϰ 0 ) ;
(ii) 
T is continuous.
Then, FP ( T ) is nonempty.
Theorem 11.
Let ( Ω , ς ) be a b-CMS and T : Ω K ( Ω ) be an α p such that
ς ( ϰ 1 , T ϰ 1 ) k α ( ϰ 1 , ϰ 2 ) ς ( ϰ 1 , ϰ 2 ) implies H ( T ϰ 1 , T ϰ 2 ) q ( ξ ( ϰ 1 , ϰ 2 ) ) ,
for all ϰ 1 , ϰ 2 Ω , where q [ 0 , 1 ) satisfies the following:
(i) 
There exists ϰ 0 Ω such that α ( ϰ 0 , T ϰ 0 ) p ( ϰ 0 , T ϰ 0 ) 2 k ;
(ii) 
If { ϰ μ } is a sequence in Ω such that α ( ϰ μ , ϰ μ + 1 ) p ( ϰ μ , ϰ μ + 1 ) 2 k and ϰ μ ϰ Ω as μ , then there exists a subsequence { ϰ μ l } of { ϰ μ } such that α ( ϰ μ l , ϰ ) p ( ϰ μ l , ϰ ) 2 k for all l 1 .
Then, FP ( T ) is nonempty.

4. Applications to Differential Equations

BPP theory plays an important role in approximating many problems, especially in the fields of differential equations and integral equations. For more details, one can see [24,25,26]. In this section, we obtain the optimum solution of system of differential equations by applying our obtained results. Consider the following system of differential equations:
d ρ d σ = ϱ ( σ , ρ ) ; ρ ( σ 0 ) = ρ 1 , d η d σ = φ ( σ , η ) ; η ( σ 0 ) = η 1 ,
where ( σ 0 , ρ 0 ) R 2 and ( σ , ρ 1 ) , ( σ , η 1 ) are the points in
S = ( σ , ρ ) R 2 : σ σ 0 a , ρ ρ 0 b ,
for some a , b > 0 . The b-metric is given as follows:
ς ( ρ ( σ ) , ( σ ) ) = ρ 2 ,
where
ρ = max t [ σ 0 a , σ 0 + a ] ρ ( t ) ( t ) .
Define
C a = ρ C [ σ 0 a , σ 0 + a ] : ρ ( σ ) ρ 0 b ,
M = ρ C a : ρ ( σ 0 ) = ρ 1
and
N = ρ C a : ρ ( σ 0 ) = η 1 .
Then, for any ρ M and N , ρ 2 η 1 ρ 1 2 and ς ( M , N ) = η 1 ρ 1 2 .
Theorem 12.
Let S , M, and N be as defined in (39), (40), and (41), respectively, and let ρ 1 < η 1 . Suppose ϱ and φ are continuous functions defined on S satisfying the following:
(1) 
ϱ ( σ , ) φ ( σ , ρ ) K ρ 1 β η 1 ρ 1 for some K > 0 whenever K ρ 1 β η 1 ρ 1 ;
(2) 
ϱ ( σ , ) φ ( σ , ρ ) , if σ σ 0 and ϱ ( σ , ) φ ( σ , ρ ) , if σ σ 0 , whenever K ρ 1 β η 1 ρ 1 .
Define T : M N M N as follows:
T ( ρ ( σ ) ) = η 1 + σ 0 σ φ ( t , ρ ( t ) ) d t , ρ M , T ( ( σ ) ) = ρ 1 + σ 0 σ φ ( t , ( t ) ) d t , N ,
satisfying the following:
(i) 
For each ρ ( σ ) M 0 , we have T ρ ( σ ) N 0 , and for each ( σ ) N 0 , we have T ( ( σ ) ) M 0 ; ( M , N ) has the P p ;
(ii) 
There exist elements ρ 0 ( σ ) and η 1 ( σ ) in M 0 and 1 ( σ ) = T ρ 0 ( σ ) such that ς ( η 1 ( σ ) , 1 ( σ ) ) = ς ( M , N ) and there exist elements 0 ( σ ) and 1 ( σ ) in N 0 and η 1 ( σ ) = T 0 ( σ ) , such that ς ( η 1 ( σ ) , 1 ( σ ) ) = ς ( M , N ) . The b-metric is given as follows:
ς ( ρ ( σ ) , ( σ ) ) = ρ 2 .
Then, for any
β < min a , b η 1 ρ 0 P , b ρ 1 ρ 0 P , 1 K , η 1 ρ 1 Q ,
where P is the bound for both ϱ and φ and
Q = sup ϱ ( σ , ) φ ( σ , ρ ) : K ρ 1 β η 1 ρ 1 ,
(38) has an optimum solution; that is, there exists ρ * M such that ς ( ρ * , T ρ * ) = η 1 ρ 1 2 , and there exists * N such that ς ( * , T * ) = η 1 ρ 1 2 .
Proof. 
Let ρ M 0 ; then, T ( ρ ( σ 0 ) ) = η 1 and
T ( ρ ( σ ) ) ρ 0 = η 1 ρ 0 + σ 0 σ φ ( t , ρ ( t ) ) d t η 1 ρ 0 + σ 0 σ φ ( t , ρ ( t ) ) d t η 1 ρ 0 + P σ σ 0 η 1 ρ 0 + β P b .
This implies T ( ρ ( σ ) ) N . Hence, T ( M ) N . Similarly, we can prove T ( N ) M . To prove that T is a generalized Suzuki-type α ψ cyclic contraction of ϖ type. Take ρ M , N , and assume σ σ 0 ,
T ρ ( σ ) T ( σ ) 2 = ρ 1 η 1 + σ 0 σ ( ϱ ( t , ( t ) ) φ ( t , ρ ( t ) ) ) d t 2 .
Now,
σ 0 σ ( ϱ ( t , ( t ) ) φ ( t , ρ ( t ) ) ) ς t = [ σ 0 , σ ] ( ϱ ( t , ( t ) ) φ ( t , ρ ( t ) ) ) d t ,
where [ σ 0 , σ ] ( ϱ ( t , ( t ) ) φ ( t , ρ ( t ) ) ) d t is the Lebesgue integral of ( ϱ ( t , ( t ) ) φ ( t , ρ ( t ) ) ) over the interval [ σ 0 , σ ] . Now, let
C 1 = t [ σ 0 , σ 0 + β ] : K ρ ( t ) ( t ) > 1 β η 1 ρ 1 , C 2 = t [ σ 0 , σ 0 + β ] : K ρ ( t ) ( t ) 1 β η 1 ρ 1 .
Since ρ and are continuous functions, we have both C 1 and C 2 are disjoint measurable sets. Therefore,
σ 0 σ ( ϱ ( t , ( t ) ) φ ( t , ρ ( t ) ) ) d t = C 1 ( ϱ ( t , ( t ) ) φ ( t , ρ ( t ) ) ) d t + C 2 ( ϱ ( t , ( t ) ) φ ( t , ρ ( t ) ) ) d t .
Hence, from (43), we have
T ( ρ ( σ ) ) T ( ( σ ) ) 2 = ρ 1 η 1 + C 1 ( ϱ ( t , ( t ) ) φ ( t , ρ ( t ) ) ) ς t + C 2 ( ϱ ( t , ( t ) ) φ ( t , ρ ( t ) ) ) ς t 2 ρ 1 η 1 + C 1 ( ϱ ( t , ( t ) ) φ ( t , ρ ( t ) ) ) ς t + C 2 ( ϱ ( t , ( t ) ) φ ( t , ρ ( t ) ) ) ς t 2 .
In C 2 , K ρ ( t ) ( t ) 1 β η 1 ρ 1 , for σ σ 0 by condition (2), we get ϱ ( t , ( t ) ) φ ( t , ρ ( t ) ) , so C 2 ( ϱ ( t , ( t ) ) φ ( t , ρ ( t ) ) ) 0 and
C 2 ( ϱ ( t , ( t ) ) φ ( t , ρ ( t ) ) ) d t C 2 ( ϱ ( t , ( t ) ) φ ( t , ρ ( t ) ) ) d t Q C 2 d t Q σ σ 0 Q β < η 1 ρ 1 .
Therefore,
T ( ρ ( σ ) ) T ( ( σ ) ) 2 ρ 1 η 1 + C 1 ( ϱ ( t , ( t ) ) φ ( t , ρ ( t ) ) ) d t 2 .
Hence,
ς ( T ( ρ ( σ ) ) , T ( ( σ ) ) ) = sup T ( ρ ( σ ) ) T ( ( σ ) ) 2 ρ 1 η 1 + C 1 ( K ρ ( t ) ( t ) 1 β η 1 ρ 1 ) d t 2 , ρ 1 η 1 + β max t [ σ 0 β , σ 0 + β ] ( K ρ ( t ) ( t ) 1 β η 1 ρ 1 ) 2 ρ 1 η 1 + K β ρ η 1 ρ 1 2 K β ρ 2 K β ρ 2 ,
which implies
ς ( T ( ρ ( σ ) ) , T ( ( σ ) ) ) K β ς ( ρ ( σ ) , ( σ ) ) K β ϖ ( ρ ( σ ) , ( σ ) ) .
Hence, T is a generalized Suzuki-type α ψ cyclic contraction of ϖ type. T is clearly α p . Thus, all axioms of Theorem 7 hold for α ( x ) = x and p ( x ) = x . Therefore, by Theorem 7, there exists ρ * M such that ς ( ρ * , T ρ * ) = η 1 ρ 1 2 and * N such that ς ( * , T * ) = η 1 ρ 1 2 . This completes the proof. □

5. Conclusions

In this article, we have established multivalued generalized Suzuki-type α ψ proximal (cyclic) contractions of b-metric spaces along with the provision of the existence of BPP(s) of multivalued generalized Suzuki-type α ψ proximal (cyclic) contractions of b-metric spaces. Examples are given to explain our results and to show that our results are the proper generalization of the already existing results in the literature. In the end, we have developed the optimum solution for a system of ordinary differential equations with initial data. In the future, these results can further be investigated in the context of partially ordered asymmetric distance spaces and Riesz spaces with some example applications.

Author Contributions

B.A. and A.A.K. contributed to the conceptualization, formal analysis, supervision, methodology, investigation, and writing—original draft preparation. B.A. and M.D.l.S. contributed to the formal analysis, review and editing, project administration, and funding acquisition. All the authors contributed to the final version of the manuscript. All authors have read and agreed to the published version of the manuscript.

Funding

This study is supported financially by the Basque Government through Grant IT1207-19.

Data Availability Statement

Not applicable.

Acknowledgments

The authors are very grateful to the Basque Government by Grant IT1207-19.

Conflicts of Interest

The authors declare that they have no competing interest.

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Ali, B.; Khan, A.A.; De la Sen, M. Optimum Solutions of Systems of Differential Equations via Best Proximity Points in b-Metric Spaces. Mathematics 2023, 11, 574. https://doi.org/10.3390/math11030574

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Ali B, Khan AA, De la Sen M. Optimum Solutions of Systems of Differential Equations via Best Proximity Points in b-Metric Spaces. Mathematics. 2023; 11(3):574. https://doi.org/10.3390/math11030574

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Ali, Basit, Arshad Ali Khan, and Manuel De la Sen. 2023. "Optimum Solutions of Systems of Differential Equations via Best Proximity Points in b-Metric Spaces" Mathematics 11, no. 3: 574. https://doi.org/10.3390/math11030574

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