SOME RESULTS ON FIXED POINT THEOREMS FOR MULTIVALUED MAPPINGS IN COMPLETE METRIC SPACES

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1 IJMMS 30: PII. S Hindawi Publishing Corp. SOME RESULTS ON FIXED POINT THEOREMS FOR MULTIVALUED MAPPINGS IN COMPLETE METRIC SPACES JEONG SHEOK UME, BYUNG SOO LEE, and SUNG JIN CHO Received 17 October 2001 Using the concept of w-distance, we improve some well-known fixed point theorems Mathematics Subject Classification: 47H Introduction. Recently, Ume [3] improved the fixed point theorems in a complete metric space using the concept of w-distance, introduced by Kada, Suzuki, and Takahashi [2], and more general contractive mappings than quasi-contractive mappings. In this paper, using the concept of w-distance, we first prove common fixed point theorems for multivalued mappings in complete metric spaces, then these theorems are used to improve Ćirić s fixed point theorem [1], Kada-Suzuki-Takahashi s fixed point theorem [2], and Ume s fixed point theorem [3]. 2. Preliminaries. Throughout, we denote by N the set of all positive integers and by R the set of all real numbers. Definition 2.1 see [2]. Let X,d be a metric space, then a function p : X X [0, is called a w-distance on X if the following are satisfied: 1 px,z px,y+py,z for all x,y,z X; 2 for any x X, px, : X [0, is lower semicontinuous; 3 for any ɛ>0, there exists δ>0 such that pz,x δ and pz,y δ imply dx,y ɛ. Definition 2.2. Let X,d be a metric space with a w-distance p, then 1 for any x X and A X, dx,a := inf{dx,y : y A} and da,x := inf{dy,x : y A}; 2 for any x X and A X, px,a := inf{px,y : y A} and pa,x := inf{py,x : y A}; 3 for any A,B X, pa,b := inf{px,y : x A, y B}; 4 CB p X ={A A is nonempty closed subset of X and sup x,y A px,y < }. The following lemmas are fundamental. Lemma 2.3 see [2]. Let X be a metric space with a metric d, let p be a w-distance on X. Let{x n } and {y n } be sequences in X, let {α n } and {β n } be sequences in [0, converging to 0, and let x,y,z X. Then the following hold:

2 320 JEONG SHEOK UME ET AL. 1 if px n,y α n and px n,z β n for any n N, then y = z. In particular, if px,y = 0 and px,z = 0, then y = z; 2 if px n,y n α n and px n,z β n for any n N, then {y n } converges to z; 3 if px n,x m α n for any n,m N with m>n, then {x n } is a Cauchy sequence; 4 if py,x n α n for any n N, then {x n } is a Cauchy sequence. Lemma 2.4 see [3]. Let X be a metric space with a metric d, let p be a w-distance on X, and let T be a mapping of X into itself satisfying ptx,ty q max { px,y,px,tx,py,ty,px,ty,py,tx } 2.1 for all x,y X and some q [0,1. Then 1 for each x X, n N, and i,j N with i,j n, p T i x,t j x q δ Ox,n ; for each x X and n N, there exist k,l N with k,l n such that δ Ox,n = max { px,x,p x,t k x,p T l x,x } ; for each x X, δ Ox, 1 { } px,x+px,tx+ptx,x ; q 4 for each x X, {T n x} n=1 is a Cauchy sequence. 3. Main results Theorem 3.1. Let X be a complete metric space with a metric d and let p be a w-distance on X. Suppose that S and T are two mappings of X into CB p X and ϕ : X X [0, is a mapping such that max { p u 1,u 2,p v1,v 2 } q ϕx,y 3.1 for all nonempty subsets A, B of X, u 1 SA, u 2 S 2 A, v 1 TB, v 2 T 2 B, x A, y B, and some q [0,1, { ϕx,y sup sup min [ px,sa,py,tb ] : x A, y B } : A,B X < 1 q, 3.2 inf { py,u+px,sx+py,ty : x,y X } > 0, 3.3 for every u X with u Su or u Tu, where SA means a A Sa.ThenS and T have a common fixed point in X. Let { ϕx,y β = sup sup min [ px,sa,py,tb ] : x A, y B } : A, B X, 3.4

3 FIXED POINT THEOREMS 321 and k = βq. Define x n+1 Sx n and y n+1 Ty n for all n N. Thenx n Sx n 1, x n+1 S 2 x n 1, y n Ty n 1, and y n+1 T 2 y n 1. From 3.1 and 3.2, we have p x n,x n+1 kp xn 1,x n k n 1 p x 1,x 2, 3.5 p y n,y n+1 kp yn 1,y n k n 1 p y 1,y 2, 3.6 for all n N and some k [0,1. Letn and m be any positive integers such that n<m. Then, from 3.6, we obtain p y n,y m p yn,y n+1 + +p ym 1,y m m n 1 = i=0 m n 1 i=0 p y n+i,y n+i+1 k n+i 1 p y 1,y kn 1 1 k p y 1,y 2. By Lemma 2.3, {y n } is a Cauchy sequence. Since X is complete, {y n } converges to u X. Then, since py n, is lower semicontinuous, from 3.7 we have p y n,u lim inf p k n 1 y n,y m m 1 k p y 1,y Suppose that u Su or u Tu. Then, by 3.3, 3.5, 3.6, and 3.8, we have 0 < inf { py,u+px,sx+py,ty : x,y X } inf { p y n,u +p } x n,x n+1 +p yn,y n+1 : n N { k n 1 inf 1 k p y 1,y 2 +k n 1 p x 1,x 2 +k n 1 p } y 1,y 2 : n N { } 2 k = 1 k p y 1,y 2 +p x1,x 2 inf { k n 1 : n N } = This is a contradiction. Therefore we have u Su and u Tu. Theorem 3.2. Let X be a complete metric space with a metric d and let p be a w-distance on X. Suppose that S and T are two mappings of X into CB p X and ϕ : X X [0, is a mapping such that max { p u 1,u 2,p v1,v 2 } q ϕx,y 3.10 for all x,y X, u 1 Sx, u 2 S 2 x, v 1 Ty, v 2 T 2 y, and some q [0,1, { ϕx,y sup sup min [ px,sx,py,ty ] : x A, y B and 3.3 is satisfied. Then S and T have a common fixed point in X. } : A,B X < 1 q, 3.11

4 322 JEONG SHEOK UME ET AL. By a method similar to that in the proof of Theorem 3.1, the result follows. Theorem 3.3. Let X be a complete metric space with a metric d and let p be a w-distance on X. Suppose that T is a mapping of X into CB p X and ψ : X [0, is a mapping such that p u 1,u 2 q ψx 3.12 for all x X, u 1 Tx, u 2 T 2 x and some q [0,1, { } ψx sup px,tx : x X < 1 q, inf { px,u+px,tx : x X } > 0, 3.13 for every u X with u Tu.ThenT has a fixed point in X. By a method similar to that in the proof of Theorem 3.1, the result follows. Theorem 3.4. Let X be a complete metric space with a metric d and let p be a w-distance on X. Suppose that S and T are self-mapping of X and ϕ : X X [0, is a mapping such that max { p Sx,S 2 x,p Ty,T 2 y } q ϕx,y 3.14 for all x,y X and some q [0,1, { sup } < 1 q, ϕx,y min [ px,sx,py,ty ] : x,y X inf { py,u+px,sx+py,ty : x,y X } > 0, 3.15 for every u X with u Su or u Tu.ThenS and T have a common fixed point in X. By a method similar to that in the proof of Theorem 3.1, the result follows. From Theorem 3.1, we have the following corollary. Corollary 3.5. Let X be a complete metric space with a metric d and let p be a w-distance on X. Suppose that S and T are two mappings of X into CB p X and ϕ : X X [0, is a mapping such that { max sup [ p u 1,u 2 : u1 Sx, u 2 S 2 x ], sup [ p v 1,v 2 : v1 Tx, v 2 T 2 x ]} 3.16 q ϕx,y for all x,y X and some q [0,1, and that 3.3 and 3.11 are satisfied. Then S and T have a common fixed point in X.

5 From Theorem 3.3, we have the following corollaries. FIXED POINT THEOREMS 323 Corollary 3.6. Let X be a complete metric space with a metric d and let p be a w-distance on X. Suppose that T is a mapping of X into CB p X and ψ : X [0, is a mapping such that sup [ p u 1,u 2 : u1 Tx, u 2 T 2 x ] q ψx 3.17 for all x X and some q [0,1, and that 3.13 is satisfied. Then T has a fixed point in X. Corollary 3.7. Let X be a complete metric space with a metric d and let p be a w-distance on X. Suppose that T is a self-mapping of X and ψ : X [0, is a mapping such that p Tx,T 2 x q ψx 3.18 for all x X and some q [0,1, { } ψx sup px,tx : x X < 1 q, inf { px,u+px,tx : x X } > 0, 3.19 for every u X with u Tu.ThenT has a fixed point in X. From Corollary 3.7, we have the following corollaries. Corollary 3.8 see [3]. Let X be a complete metric space with a metric d and let p be a w-distance on X. Suppose that T is a self-mapping of X such that ptx,ty q max { px,y,px,tx,py,ty,px,ty,py,tx } 3.20 for all x,y X and some q [0,1, and that inf { px,u+px,tx : x X } > for every u X with u Tu.ThenT has a unique fixed point in X. By 3.20 andlemma 2.43, we have sup { p T i x,t j x i, j N {0} } < 3.22 for every x X. Thus we may define a function r : X X [0, by rx,y= max { sup [ p T i x,t j x i, j N {0} ],px,y } 3.23 for every x,y X. Clearly, r is a w-distance on X.Letx be a given element of X, then, by using Lemma 2.41, 3.20, and 3.23, we have r Tx,T 2 x = sup { p T i x,t j x i, j N } q sup { p T i x,t j x i, j N {0} } 3.24 = q rx,tx.

6 324 JEONG SHEOK UME ET AL. By 3.21 and 3.23, we obtain inf { rx,u+rx,tx: x X } > for every u X with u Tu. From 3.24, 3.25, and Corollary 3.7, T has a fixed point in X. By3.20 andlemma 2.4, it is clear that the fixed point of T is unique. Corollary 3.9 see [2]. Let X be a complete metric space, let p be a w-distance on X, and let T be a mapping from X into itself. Suppose that there exists q [0,1 such that p Tx,T 2 x q px,tx 3.26 for every x X and that inf { px,y+px,tx : x X } > for every y X with y Ty.ThenT has a fixed point in X. Define ψ : X [0, by ψx = px,tx 3.28 for all x X. Thus the conditions of Corollary 3.7 are satisfied. Hence T has a fixed point in X. From Corollary 3.8, we have the following corollary. Corollary 3.10 see [1]. Let X be a complete metric space with a metric d and let T be a mapping from X into itself. Suppose that T is a quasicontraction, that is, there exists q [0,1 such that dt x,t y q max { dx,y,dx,tx,dy,ty,dx,ty,dy,tx } 3.29 for every x,y X. ThenT has a unique fixed point in X. It is clear that the metric d is a w-distance and inf { dx,y+dx,t x : x X } > for every y X with y Ty. Thus, by Corollary 3.8 or 3.9, T has a unique fixed point in X. Acknowledgment. This work was supported by grant No from the Basic Research Program of the Korea Science & Engineering Foundation. References [1] L. B. Ćirić, A generalization of Banach s contraction principle, Proc. Amer. Math. Soc , [2] O. Kada, T. Suzuki, and W. Takahashi, Nonconvex minimization theorems and fixed point theorems in complete metric spaces, Math. Japon , no. 2,

7 FIXED POINT THEOREMS 325 [3] J. S. Ume, Fixed point theorems related to Ćirić s contraction principle, J. Math. Anal. Appl , no. 2, Jeong Sheok Ume: Department of Applied Mathematics, Changwon National University, Changwon , Korea address: jsume@sarim.changwon.ac.kr Byung Soo Lee: Department of Mathematics, Kyungsung University, Pusan , Korea address: bslee@star.kyungsung.ac.kr Sung Jin Cho: Department of Applied Mathematics, Pukyong National University, Pusan , Korea address: sjcho@dolphin.pknu.ac.kr

8 Mathematical Problems in Engineering Special Issue on Space Dynamics Call for Papers Space dynamics is a very general title that can accommodate a long list of activities. This kind of research started with the study of the motion of the stars and the planets back to the origin of astronomy, and nowadays it has a large list of topics. It is possible to make a division in two main categories: astronomy and astrodynamics. By astronomy, we can relate topics that deal with the motion of the planets, natural satellites, comets, and so forth. Many important topics of research nowadays are related to those subjects. By astrodynamics, we mean topics related to spaceflight dynamics. It means topics where a satellite, a rocket, or any kind of man-made object is travelling in space governed by the gravitational forces of celestial bodies and/or forces generated by propulsion systems that are available in those objects. Many topics are related to orbit determination, propagation, and orbital maneuvers related to those spacecrafts. Several other topics that are related to this subject are numerical methods, nonlinear dynamics, chaos, and control. The main objective of this Special Issue is to publish topics that are under study in one of those lines. The idea is to get the most recent researches and published them in a very short time, so we can give a step in order to help scientists and engineers that work in this field to be aware of actual research. All the published papers have to be peer reviewed, but in a fast and accurate way so that the topics are not outdated by the large speed that the information flows nowadays. Before submission authors should carefully read over the journal s Author Guidelines, which are located at Prospective authors should submit an electronic copy of their complete manuscript through the journal Manuscript Tracking System at according to the following timetable: Lead Guest Editor Antonio F. Bertachini A. Prado, Instituto Nacional de Pesquisas Espaciais INPE, São José dos Campos, São Paulo, Brazil; prado@dem.inpe.br Guest Editors Maria Cecilia Zanardi, São Paulo State University UNESP, Guaratinguetá, São Paulo, Brazil; cecilia@feg.unesp.br Tadashi Yokoyama, Universidade Estadual Paulista UNESP, Rio Claro, São Paulo, Brazil; tadashi@rc.unesp.br Silvia Maria Giuliatti Winter, São Paulo State University UNESP, Guaratinguetá, São Paulo, Brazil; silvia@feg.unesp.br Manuscript Due July 1, 2009 First Round of Reviews October 1, 2009 Publication Date January 1, 2010 Hindawi Publishing Corporation

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