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Common fixed-point results for generalized Berinde-type contractions which involve altering distance functions

Abstract

In this paper, the existence and the uniqueness of a common fixed point for two self-mappings satisfying some generalized Berinde-type contractions which involve an altering distance function with λ∈[0,1] is established. Our theorems extend, unify, and generalize several existing results in the literature. An application of an integral equation is presented.

MSC:54H25, 54C60, 54E50.

1 Introduction and preliminaries

Fixed-point theory is one of the most fruitful and effective tools in mathematics which has enormous applications within as well as outside mathematics. In 1922, Banach established the famous fixed-point theorem which is called the Banach contraction principle. This principle is a forceful tool in nonlinear analysis. It has many applications in solving nonlinear equations.

Later, Berinde [1–5] studied many interesting fixed-point theorems for many kinds of contraction mappings. In [3] and [4], he defined the almost contraction map as follows.

Definition 1.1 Let (X,d) be a metric space. A map f:X→X is called an almost contraction if there exist a constant λ∈[0,1) and some L≥0 such that

d(fx,fy)≤λd(x,y)+Ld(y,fx)

for all x,y∈X.

Let (X,d) be a metric space. A map f:X→X is said to satisfy ‘condition (B)’ if there exist a constant λ∈[0,1) and some L≥0 such that for all x,y∈X.

d(fx,fy)≤λd(x,y)+Lmin { d ( x , f x ) , d ( y , f y ) , d ( x , f y ) , d ( y , f x ) } .

Recently, Babu et al. [6] considered the class of mappings that satisfy ‘condition (B)’.

More recently, Abbas and Ilic in [7] introduced the following definition.

Definition 1.2 Let f and g be two self-maps on a metric space (X,d). A map f is called generalized almost g-contraction if there exist a constant λ∈[0,1) and some L≥0 such that

d(fx,fy)≤λM(x,y)+Lmin { d ( g x , f x ) , d ( g y , f y ) , d ( g x , f y ) , d ( g y , f x ) }

for all x,y∈X, where M(x,y)=max{d(gx,gy),d(gx,fx),d(fy,gy), 1 2 (d(fx,gy)+d(gx,fy))}.

If g= I X , I X is the identity map on X, then they note that f satisfies ‘generalized condition (B)’.

Furthermore, Ćirić et al. [8] introduced the concept of the almost generalized contractive condition as follows.

Definition 1.3 Let f and g be two self-maps on a metric space (X,d). They are said to satisfy almost generalized contractive condition if there exist a constant λ∈[0,1) and some L≥0 such that

d ( f x , g y ) ≤ λ max { d ( x , y ) , d ( x , f x ) , d ( y , g y ) , 1 2 ( d ( f x , y ) + d ( x , g y ) ) } + L min { d ( x , f x ) , d ( y , g y ) , d ( x , g y ) , d ( y , f x ) }

for all x,y∈X.

A new category of contractive fixed-point problems was addressed by Khan et al. [9]. In their study they introduced the notion of an altering distance function, which is a control function that alters the distance between two points in a metric space.

Definition 1.4 The function ψ:[0,∞)→[0,∞) is called an altering distance function if the following properties are satisfied:

  1. (i)

    ψ is continuous and nondecreasing;

  2. (ii)

    ψ(t)=0⇔t=0.

In the literature, there has been extensive research on common fixed points by using Berinde-type contractions, see [10, 11], by using an altering distance function, see [12–14] and by using many other kinds of methods, see [15–17].

The aim of this work is to prove that there is a unique common fixed point for two self-mappings satisfying some generalized Berinde-type contractions which involve an altering distance function with λ∈[0,1]. These results extend and generalize several well-known compatible recent and classical results in the literature. As an application, the existence of a solution for the Urysohn integral equation is presented.

2 Main results

Theorem 2.1 Let (X,d) be a complete metric space. Suppose ψ:[0,∞)→[0,∞) is an altering distance function and φ:[0,∞)→[0,∞) is a lower semi-continuous function with φ(t)=0 if and only if t=0. Moreover, suppose that f and g are self-maps satisfying the inequality

ψ ( d ( f x , g y ) ) ≤ψ ( λ u ( x , y ) ) −φ ( λ u ( x , y ) ) +LN(x,y),
(2.1)

where

u(x,y)∈ { d ( x , y ) , d ( x , f x ) , d ( y , g y ) , 1 2 ( d ( f x , y ) + d ( x , g y ) ) }

and

N(x,y)=min { d ( x , y ) , d ( x , f x ) , d ( y , g y ) , d ( f x , y ) , d ( x , g y ) } ,

with L≥0 and 0≤λ≤1. Then f and g have a unique common fixed point.

Proof We prove the theorem in several steps.

Step 1. Let x 0 ∈X be an arbitrary point.

Taking x 1 =f x 0 and x 2 =g x 1 , then let x 3 =f x 2 and x 4 =g x 3 . Continue in this way, we can choose a sequence { x n } in X so that

x 2 n + 1 =f x 2 n

and

x 2 n + 2 =g x 2 n + 1

for all n=0,1,2,… . Let

d n =d( x n , x n + 1 ).
(2.2)

We will prove that { d n } is a decreasing sequence which converges to 0.

If n is an even number, put x= x n and y= x n − 1 in (2.1). We get

ψ ( d ( x n + 1 , x n ) ) = ψ ( d ( f x n , g x n − 1 ) ) ≤ ψ ( λ u ( x n , x n − 1 ) ) − φ ( λ u ( x n , x n − 1 ) ) + L N ( x n , x n − 1 ) ,
(2.3)

where

u( x n , x n − 1 )∈ { d ( x n , x n − 1 ) , d ( x n , f x n ) , d ( x n − 1 , g x n − 1 ) , 1 2 ( d ( f x n , x n − 1 ) + d ( x n , g x n − 1 ) ) }

and

N( x n , x n − 1 )=min { d ( x n , x n − 1 ) , d ( x n , f x n ) , d ( x n − 1 , g x n − 1 ) , d ( f x n , x n − 1 ) , d ( x n , g x n − 1 ) } ,

i.e.,

N( x n , x n − 1 )=0.

Thus, we have

ψ ( d ( x n , x n + 1 ) ) ≤ψ ( λ u ( x n , x n − 1 ) ) −φ ( λ u ( x n , x n − 1 ) ) ,

where

u( x n , x n − 1 )∈ { d ( x n − 1 , x n ) , d ( x n , x n + 1 ) , 1 2 d ( x n − 1 , x n + 1 ) } .

If x n = x n + 1 for some n≥0, then the proof will be finished. Therefore, we suppose that x n ≠ x n + 1 for all n≥0. Now, we shall show that d( x n , x n + 1 )≤d( x n − 1 , x n ). Arguing by contradiction, we assume d( x n , x n + 1 )>d( x n − 1 , x n ). Therefore, we have three cases.

Case 1: u( x n , x n − 1 )=d( x n − 1 , x n ). Then

ψ ( d ( x n , x n + 1 ) ) ≤ψ ( λ d ( x n − 1 , x n ) ) −φ ( λ d ( x n − 1 , x n ) ) <ψ ( λ d ( x n − 1 , x n ) ) .

Since ψ is increasing, we have d( x n , x n + 1 )<λd( x n − 1 , x n ), which is a contradiction.

Case 2: u( x n , x n − 1 )=d( x n , x n + 1 ). Then

ψ ( d ( x n , x n + 1 ) ) ≤ψ ( λ d ( x n , x n + 1 ) ) −φ ( λ d ( x n , x n + 1 ) ) <ψ ( λ d ( x n , x n + 1 ) ) .

Since ψ is increasing, we have d( x n , x n + 1 )<λd( x n , x n + 1 ), which is impossible.

Case 3: u( x n , x n − 1 )= 1 2 d( x n − 1 , x n + 1 ). Then

ψ ( d ( x n , x n + 1 ) ) ≤ψ ( λ 2 d ( x n − 1 , x n + 1 ) ) −φ ( λ 2 d ( x n − 1 , x n + 1 ) ) ≤ψ ( λ 2 d ( x n − 1 , x n + 1 ) ) .

Since ψ is increasing, we have

d( x n , x n + 1 )≤ λ 2 d( x n − 1 , x n + 1 )≤ λ 2 ( d ( x n − 1 , x n ) + d ( x n , x n + 1 ) ) ,

which leads to

d( x n , x n + 1 )≤ λ 2 − λ d( x n − 1 , x n ),

but d( x n , x n + 1 )>d( x n − 1 , x n ), therefore

d( x n , x n + 1 )< λ 2 − λ d( x n , x n + 1 ),

which is impossible since λ/(2−λ)≤1. Hence, from the above we obtain d( x n , x n + 1 )≤d( x n − 1 , x n ).

Similarly, we can prove that d( x n , x n + 1 )≤d( x n − 1 , x n ) also in the case when n is an odd number.

Therefore, we find that { d n } is a decreasing sequence and bounded below. Thus, { d n } is convergent. Let

d n →das n→∞.
(2.4)

Next, we want to show that d=0. We have two cases.

Case 1. When u( x n , x n − 1 )∈{d( x n − 1 , x n ),d( x n , x n + 1 )}, as ψ is continuous and φ is lower semi-continuous and from (2.4) we get

ψ(d)≤ψ(λd)−φ(λd).

If λ=0, then we have ψ(d)≤0⇒d=0. If λ≠0, then we have φ(λd)≤ψ(λd)−ψ(d)≤0. Thus φ(λd)=0, which implies d=0.

Case 2. When u( x n , x n − 1 )= 1 2 d( x n − 1 , x n + 1 ), we suppose that d≠0; then

ψ ( d n ) ≤ ψ ( λ 2 d ( x n − 1 , x n + 1 ) ) − φ ( λ 2 d ( x n − 1 , x n + 1 ) ) ≤ ψ ( λ 2 d ( x n − 1 , x n + 1 ) ) ≤ ψ ( λ 2 ( d ( x n − 1 , x n ) + d ( x n , x n + 1 ) ) ) .

Now, we have two subcases.

Subcase 1. λ<1. Then as n→∞ we obtain

ψ(d)≤ψ(λd),

which leads to a contradiction if d≠0.

Subcase 2. λ=1. Then

ψ( d n )≤ψ ( 1 2 d ( x n − 1 , x n + 1 ) ) ≤ψ ( 1 2 ( d ( x n − 1 , x n ) + d ( x n , x n + 1 ) ) ) .

As n→∞, we have

ψ(d)≤ψ ( 1 2 lim n → ∞ d ( x n − 1 , x n + 1 ) ) ≤ψ(d).

Since ψ is an increasing function, we get

lim n → ∞ d( x n − 1 , x n + 1 )=2d.
(2.5)

By taking n→∞ in ψ( d n )≤ψ( λ 2 d( x n − 1 , x n + 1 ))−φ( λ 2 d( x n − 1 , x n + 1 )) and using (2.5), we have

ψ(d)≤ψ ( 1 2 ( 2 d ) ) −φ ( 1 2 ( 2 d ) ) ,

i.e.

φ(d)≤0.

Hence, φ(d)=0 and then d=0.

From the above we obtain d=0, i.e.,

d n =d( x n , x n + 1 )→0as n→∞.
(2.6)

Step 2. We prove that { x n } is a Cauchy sequence. Suppose that { x n } is not a Cauchy sequence, then there exists ε>0 for which we can find subsequences { x n ( k ) } and { x m ( k ) } of { x n } with n(k)>m(k)≥k such that

d( x n ( k ) , x m ( k ) )≥ε/k.
(2.7)

Furthermore, corresponding to m(k), we can choose n(k) in such a way that it is the smallest integer with n(k)>m(k) and satisfying (2.7). Then

d( x n ( k ) − 1 , x m ( k ) )<ε/k.

Then we have

ε / k ≤ d ( x n ( k ) , x m ( k ) ) ≤ d ( x n ( k ) , x n ( k ) − 1 ) + d ( x n ( k ) − 1 , x m ( k ) ) ≤ d ( x n ( k ) , x n ( k ) − 1 ) + ε / k ,

by taking k→∞, we obtain

lim k → ∞ d( x n ( k ) , x m ( k ) )=0,

which is a contradiction. So, { x n } is a Cauchy sequence in a complete metric space X and hence it is convergent in X. Let

lim n → ∞ x n = x ∗ .

Step 3. Let us now prove that x ∗ is a common fixed point of f and g. Put x= x ∗ and y= x 2 n + 1 in (2.1) for all n, and we obtain

ψ ( d ( f x ∗ , g x 2 n + 1 ) ) ≤ψ ( λ u ( x ∗ , x 2 n + 1 ) ) −φ ( λ u ( x ∗ , x 2 n + 1 ) ) +LN ( x ∗ , x 2 n + 1 ) ,

where

u ( x ∗ , x 2 n + 1 ) ∈ { d ( x ∗ , x 2 n + 1 ) , d ( x ∗ , f x ∗ ) , d ( x 2 n + 1 , g x 2 n + 1 ) , 1 2 ( d ( f x ∗ , x 2 n + 1 ) + d ( x ∗ , g x 2 n + 1 ) ) }

and

N ( x ∗ , x 2 n + 1 ) =min { d ( x ∗ , x 2 n + 1 ) , d ( x ∗ , f x ∗ ) , d ( x 2 n + 1 , g x 2 n + 1 ) , d ( f x ∗ , x 2 n + 1 ) , d ( x ∗ , g x 2 n + 1 ) } .

Let n→∞, we get

ψ ( d ( f x ∗ , x ∗ ) ) ≤ψ ( λ lim n → ∞ u ( x ∗ , x 2 n + 1 ) ) −φ ( λ lim n → ∞ u ( x ∗ , x 2 n + 1 ) ) ,

where

lim n → ∞ u ( x ∗ , x 2 n + 1 ) ∈ { 0 , d ( x ∗ , f x ∗ ) , 1 2 d ( x ∗ , f x ∗ ) } .

If d( x ∗ ,f x ∗ )≠0, then

ψ ( d ( x ∗ , f x ∗ ) ) <ψ ( λ d ( x ∗ , f x ∗ ) ) orψ ( d ( x ∗ , f x ∗ ) ) <ψ ( λ 2 d ( x ∗ , f x ∗ ) ) ,

which is a contradiction. Hence, we obtain

d ( x ∗ , f x ∗ ) =0or x ∗ =f x ∗ .
(2.8)

Similarly, when we take x= x 2 n and y= x ∗ in (2.1) for all n we get

x ∗ =g x ∗ .
(2.9)

Equations (2.8) and (2.9) show that x ∗ is a common fixed point of f and g.

Step 4. Let us now show the uniqueness. Let y ∗ be another common fixed point of f and g. Then from (2.1) we have

ψ ( d ( f x ∗ , g y ∗ ) ) =ψ ( d ( x ∗ , y ∗ ) ) ≤ψ ( λ u ( x ∗ , y ∗ ) ) −φ ( λ u ( x ∗ , y ∗ ) ) +LN ( x ∗ , y ∗ ) ,

where

u ( x ∗ , y ∗ ) ∈ { 0 , d ( x ∗ , y ∗ ) } andN ( x ∗ , y ∗ ) =0.

Then we obtain x ∗ = y ∗ . □

Corollary 2.2 Let (X,d) be a complete metric space. Suppose ψ:[0,∞)→[0,∞) is an altering distance function and φ:[0,∞)→[0,∞) is a lower semi-continuous function with φ(t)=0 if and only if t=0. If f and g are self-maps satisfying the inequality

ψ ( d ( f x , g y ) ) ≤ψ ( λ M ( x , y ) ) −φ ( λ M ( x , y ) ) +LN(x,y),

where

M(x,y)=max { d ( x , y ) , d ( x , f x ) , d ( y , g y ) , 1 2 ( d ( f x , y ) + d ( x , g y ) ) }

and

N(x,y)=min { d ( x , y ) , d ( x , f x ) , d ( y , g y ) , d ( f x , y ) , d ( x , g y ) } ,

with L≥0 and 0≤λ≤1, then f has a unique fixed point.

Proof Since M(x,y)∈{d(x,y),d(x,fx),d(y,gy), 1 2 (d(fx,y)+d(x,gy))}, the result follows from Theorem 2.1. □

Remark 2.3 In Corollary 2.2:

  1. (i)

    If g=f and λ=1, we obtain a metric version of Theorem 12 of Aydi et al. [10].

  2. (ii)

    If L=0 and λ=1, we get Theorem 2.1 of Doric [18].

  3. (iii)

    If ψ(t)=t, L=0 and λ=1, we get Theorem 2.1 of Zhang and Song [19].

By taking f=g and L=0 in Corollary 2.2, we obtain the following result.

Corollary 2.4 Let (X,d) be a complete metric space. Suppose ψ:[0,∞)→[0,∞) is an altering distance function and φ:[0,∞)→[0,∞) is a lower semi-continuous function with φ(t)=0 if and only if t=0. If f is a self-map satisfying the inequality

ψ ( d ( f x , f y ) ) ≤ψ ( λ u ( x , y ) ) −φ ( λ u ( x , y ) ) ,
(2.10)

where u(x,y)∈{d(x,y),d(x,fx),d(y,fy), 1 2 (d(fx,y)+d(x,fy))}, 0≤λ≤1, then f has a unique fixed point.

Remark 2.5 Corollary 2.4 extends the main fixed-point result of Dutta and Choudhury [[20], Theorem 2.1] and Theorem 2.2 of Doric [18].

If we take ψ(t)=t and φ(t)=(1−k)t with k<1 in Theorem 2.1, we have the following corollary.

Corollary 2.6 Let (X,d) be a complete metric space. If f and g are self-maps satisfying the inequality

d(fx,gy)≤αu(x,y)+LN(x,y),
(2.11)

where

u(x,y)∈ { d ( x , y ) , d ( x , f x ) , d ( y , g y ) , 1 2 ( d ( f x , y ) + d ( x , g y ) ) }

and

N(x,y)=min { d ( x , y ) , d ( x , f x ) , d ( y , g y ) , d ( f x , y ) , d ( x , g y ) } ,

with L≥0 and 0≤α<1, then f and g have a unique common fixed point.

If we take f=g in Corollary 2.6 we obtain the following result.

Corollary 2.7 Let (X,d) be a complete metric space. If f is a self-map satisfying the inequality

d(fx,fy)≤αu(x,y)+LN(x,y),

where

u(x,y)∈ { d ( x , y ) , d ( x , f x ) , d ( y , f y ) , 1 2 ( d ( f x , y ) + d ( x , f y ) ) }

and

N(x,y)=min { d ( x , y ) , d ( x , f x ) , d ( y , f y ) , d ( f x , y ) , d ( x , f y ) } ,

with L≥0 and 0≤α<1, then f has a unique fixed point.

By the aid of Lemma 2.1 of [21], we have the following result as a consequence of Corollary 2.7.

Corollary 2.8 Let (X,d) be a complete metric space. If f and g are self-maps satisfying the inequality

d(fx,fy)≤αu(gx,gy)+LN(gx,gy),

where

u(gx,gy)∈ { d ( g x , g y ) , d ( g x , f x ) , d ( g y , f y ) , 1 2 ( d ( f x , g y ) + d ( g x , f y ) ) }

and

N(gx,gy)=min { d ( g x , g y ) , d ( g x , f x ) , d ( g y , f y ) , d ( f x , g y ) , d ( g x , f y ) } ,

with L≥0 and 0≤α<1, then f and g have a unique common fixed point.

Remark 2.9 Corollary 2.8 extends the results of Abbas et al. [[22], Theorem 2.1] and Jleli et al. [[23], Corollary 3.2].

3 Applications: existence of a common solution to Urysohn integral equations

Throughout this section we take X=C([a,b],R) (the set of continuous functions defined in I=[a,b]). We define the metric d:X×X→R by d(x,y)= ∥ x − y ∥ ∞ for every x,y∈X. Let φ: R + → R + be a function such that

  • φ is lower semi-continuous;

  • φ is increasing;

  • φ(t)=0⇔t=0.

Theorem 3.1 Consider the Urysohn integral equations

x ( t ) = ∫ a b K 1 ( t , s , x ( s ) ) d s + h ( t ) , x ( t ) = ∫ a b K 2 ( t , s , x ( s ) ) d s + q ( t ) ,
(3.1)

where t∈I⊂R and x,h,q∈X. Assume that, for K 1 , K 2 :I×I×R→R, we have

| ∫ a b K 1 ( t , s , x ( s ) ) ds− ∫ a b K 2 ( t , s , x ( s ) ) ds+h(t)−q(t)|≤|x(t)−y(t)|−φ ( sup t ∈ I | x ( t ) − y ( t ) | ) .

Then there exists a solution to (3.1).

Proof Define f,g:X→X by f(x)= ∫ a b K 1 (t,s,x(s))ds+h(t) and g(x)= ∫ a b K 2 (t,s,x(s))ds+q(t). It is obvious that

∥ f − g ∥ ∞ ≤ ∥ x − y ∥ ∞ −φ ( ∥ x − y ∥ ∞ ) .

Thus

d(fx,gy)≤d(x,y)−φ ( d ( x , y ) )

for all x,y∈X. Now, all the assumptions of Theorem 2.1 are satisfied with ψ(t)=t, for all t∈ R + , u(x,y)=d(x,y), and L=0. Therefore, f and g have a common fixed point, that is, a solution to the integral equation (3.1). □

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Acknowledgements

The authors would like to acknowledge the financial support received from Universiti Kebangsaan Malaysia under the research grant UKM-DIP-2012-31.

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Correspondence to Fawzia Shaddad.

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

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Shaddad, F., Md Noorani, M.S. & Alsulami, S.M. Common fixed-point results for generalized Berinde-type contractions which involve altering distance functions. Fixed Point Theory Appl 2014, 24 (2014). https://doi.org/10.1186/1687-1812-2014-24

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  • DOI: https://doi.org/10.1186/1687-1812-2014-24

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