Scientia Magna, 7, no. 4

Page 1


Vol. 7, No. 4, 2011

ISSN 1556-6706

SCIENTIA MAGNA An international journal

Edited by

Department of Mathematics Northwest University Xi’an, Shaanxi, P.R.China


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ii


Contributing to Scientia Magna Authors of papers in science (mathematics, physics, philosophy, psychology, sociology, linguistics) should submit manuscripts, by email, to the Editor-in-Chief: Prof. Wenpeng Zhang Department of Mathematics Northwest University Xi’an, Shaanxi, P.R.China E-mail: wpzhang@nwu.edu.cn Or anyone of the members of Editorial Board: Dr. W. B. Vasantha Kandasamy, Department of Mathematics, Indian Institute of Technology, IIT Madras, Chennai - 600 036, Tamil Nadu, India. Dr. Larissa Borissova and Dmitri Rabounski, Sirenevi boulevard 69-1-65, Moscow 105484, Russia. Prof. Yuan Yi, Research Center for Basic Science, Xi’an Jiaotong University, Xi’an, Shaanxi, P.R.China. E-mail: yuanyi@mail.xjtu.edu.cn Dr. Zhefeng Xu, Department of Mathematic s, Northwest University, Xi’an, Shaanxi, P.R.China. E-mail: zfxu@nwu.edu.cn; zhefengxu@hotmail.com Prof. József Sándor, Babes-Bolyai University of Cluj, Romania. E-mail: jjsandor@hotmail.com; jsandor@member.ams.org Dr. Di Han, Department of Mathematics, Northwest University, Xi’an, Shaanxi, P.R.China. E-mail: handi515@163.com

iii


Contents R. Ma and Y. Zhang : On Erd¨os-Smarandache numbers

1

R. Dhavaseelan, etc. : A view on generalized intuitionistic fuzzy contra continuous functions and its applications

7

L. Huan : On the asymptotic properties of triangular base sequence

19

A. Esi : A new class of double interval numbers

23

M. Ren, etc. : Linear operators preserving commuting pairs of matrices over semirings

29

S. S. Billing : Conditions for a subclass of analytic functions

35

B. Hazarika : On ideal convergence in topological groups

42

Salahuddin : A summation formula including recurrence relation

49

A. Esi and E. Eren : Some classes of difference fuzzy numbers defined by an orlicz function

82

M. Dragan and M. Bencze : The Hadwiger-Finsler reverse in an acute triangle

92

Q. Yang and C. Fu : On mean value computation of a number theoretic function

96

Y. Lu, etc. : On Kummer’s fourier series for log Γ (x)

104

J. S´ andor : On two inequalities for the composition of arithmetic functions

109

G. Mirhosseinkhani : Compactness and proper maps in the category of generated spaces

114

iv


Scientia Magna Vol. 7 (2011), No. 4, 1-6

On Erd¨ os-Smarandache numbers1 Rong Ma† and Yulong Zhang‡ † School of Science, Northwestern Polytechnical University, Xi’an, Shaanxi, 710072, People’s Republic of China ‡ School of Electronic and Information Engineering, Xi’an Jiaotong University, Xi’an, Shaanxi, 710049, People’s Republic of China E-mail: marong@nwpu.edu.cn zzboyzyl@163.com Abstract Let A denote the set of Erd¨ os-Smarandache numbers, for any positive integer n, they can be defined by the solutions of the diophantine equation P (n) = S(n), where P (n) is the largest prime factor which divides n, S(n) is the Smarandache function defined as follows: S(n) is the smallest number, such that S(n)! is divisible by n, i.e., S(n) = min{m : m ∈ N, n|m!}. For any real number x > 1, let M (x) denote the number of natural numbers n in the set A and such that n ≤ x, in this paper, we study M (x) by the elementary and analytic methods, and give an interesting asymptotic formula of M (x). Keywords Erd¨ os-Smarandache numbers, the largest prime factor, asymptotic formula. MR(2000) Classification: 11N25, 11N37.

§1. Introduction For any positive integer n, the Smarandache function S(n) can be defined as follows: S(n) is the smallest number, such that S(n)! is divisible by n, i.e., S(n) = min{m : m ∈ N, n|m!}. αr 1 α2 According to the definition of S(n), if n = pα 1 p2 . . . pr denoting the prime powers factorization αi of n, we have S(n) = max1≤i≤r {S(pi )}. Hence we can easily get several values of S(n): S(1) = 1, S(2) = 2, S(3) = 3, S(4) = 4, S(5) = 5, S(6) = 3, S(7) = 7, S(8) = 4, S(9) = 6, · · · · · · . About the arithmetical properties of S(n), many scholars have studied them (see Ref.[4]-[8]). For example, Lu (see Ref.[4]) and Le (see Ref.[5]) studied the solutions involving the equations of S(n), i.e., the equation S(m1 + m2 + · · · + mk ) = S(m1 ) + S(m2 ) + · · · + S(mk ) has infinite many positive integer solutions. Du (see Ref.[6]) studied the conjecture on S(n), i.e., when n was a sqarefree number, the sum X 1 S(n) d|n

1 This work is supported by the 2011 Basic Research Fund of Northwestern Polytechnical University(JC201123).


2

Rong Ma and Yulong Zhang

No. 4

is impossible an integer. Xu (see Ref.[7]) got a profound result about S(n), that is X

3

2ζ( 32 )x 2 (S(n) − P (n)) = +O 3 ln x

Ã

2

n≤x

3

x2 ln2 x

! ,

where P (n) is the largest prime factor which divides n, ζ(s) is Riemann zeta-function. Now we let A denote the set of Erd¨os-Smarandache numbers (See Ref.[8] and [9]), which is defined by the solutions of the diophantine equation S(n) = P (n). According to the definitions of S(n) and P (n), we can easily get several front Erd¨os-Smarandache numbers, i.e., A = {2, 3, 5, 6, 7, 10, 11, 13, 14, 15, 17, 19, 21, 22, 23, 26, 28, 29, 30, 31, · · · }. In 1991, for any positive integer k > 3, Erd¨ os (see Ref. [10]) asserted the number of elements of the set A was X

1 = k + o(k) (k → +∞).

n≤k n∈A

After that, many scholars (see Ref.[11,12]) improved the result. Further more, in 2005, Ivic (see Ref.[1]) got the asymptotic formula X n≤k n6∈A

½ µ µ ¶¶¾ p log3 k 1 = k exp − 2 log k log2 k 1 + O , log2 k

where exp(x) = ex . Even he got the asymptotic formula involving the Dickman-de Bruijn function. Thereby he sharpened and corrected results of Ford (see Ref.[2]), Koninck and Doyon (see Ref.[3]). The authors are also very interested in this problem and want to know some more about the number of Erd¨os-Smarandache numbers. So we use the elementary method to study this problem and get a weaker asymptotic formula of the number of Erd¨os-Smarandache numbers. Although the result is weaker than those of the above, we have used the alternative approach (completely different from the Ivic’s). That is, we shall prove the following: Theorem 1.1. Let A denote the set of Erd¨os-Smarandache numbers, then for all positive integer k > 2, we have the asymptotic formula X

µ 1=k+O

n≤k n∈A

k 3

log k(log log k) 2

.

§2. Some lemmas To complete the proof of the above theorem, we need the several following lemmas. First, we give the familiar formula Abel’s identity. Lemma 2.1. Abel’s identity. For any arithmetical function a(n), let A(x) =

X n≤x

a(n),


Vol. 7

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On Erd¨ os-Smarandache numbers

where A(x) = 0 if x < 1. Assume f has a continuous derivative on the interval [x, y], where 0 < x < y. Then we have Z y X a(n)f (n) = A(y)f (y) − A(x)f (x) − A(t)f 0 (t)dt. (1) x

x<n≤y

Proof. See Ref.[13]. Lemma 2.2. Prime number theorem. For x > 0, let π(x) denote the number of primes not exceeding x. Then we have µ ¶ x x +O . π(x) = (2) log x log2 x In addition, the prime number theorem also has an equivalent form µ ¶ Z x X π(t) x ϑ(x) = log p = π(x) log x − dt = x + O . t log x 2

(3)

p≤x

Proof. See Ref.[14]. Lemma 2.3. For all 0 < x < y, we have X x<p≤y

1 1 = +O p2 x log x

µ

1 x log2 x

¶ .

Proof. Let a(n) denote the characteristic function of the primes, that is   1, if n is prime, a(n) =  0, otherwise. Then we have

X x<p≤y

Therefore if we take f (t) = X x<p≤y

1 t2

X a(n) 1 = . 2 p n2 x<n≤y

in Lemma 2.1, we find,

Z y X 1 1 X 1 X 1 = a(n) − a(n) + 2 a(n)dt. 2 2 2 3 p y x x t n≤y

From Lemma 2.2 we have π(x) =

n≤x

P

a(n) =

n≤x

X x<p≤y

1 p2

=

y log y

+ R(y) y2

x log x

x log x

+ R(x), where R(x) = O( logx2 x ), then we find

+ R(x) x2

(4)

n≤t

Z

y

+2 x

t log t

+ R(t) t3

dt

Z y Z y 1 1 R(t) 1 R(y) R(x) dt + 2 − − 2 +2 dt + 2 2 log t y log y y x log x x t t3 x x µ ¶ Z y Z y 1 1 1 1 R(t) = dt − +O + 2 dt + 2 2 2 y log y x log x t3 x log x x t log t x µ ¶ Z y Z y 1 1 1 R(t) = − dt. +O + 2 dt + 2 2 x log x t3 x log2 x x t log t x =

(5)


4

Rong Ma and Yulong Zhang

Now

Z

y

x

1 dt t2 log t

Z y 1 1 1 − − dt 2 log2 t x log x y log y t x µ ¶ 1 1 +O x log x x log2 x

= =

and Z

y

x

R(t) dt = O t3

No. 4

µZ

y

x

1 dt 2 t log2 t

µ =O

1 x log2 x

(6)

¶ (7)

,

where we used the condition R(t) = O( logt2 t ). Hence equation (5) can be expressed as follows: X x<p≤y

1 1 = +O p2 x log x

µ

1 x log2 x

¶ .

This proves the lemma.

§3. Proof of the theorem In this section, we shall complete the proof of the theorem. First we will estimate the P αr 1 α2 upper bound of In fact, for any positive integer k > 1, we let n = pα n≤k 1. 1 p2 · · · pr n6∈A denote the prime powers factorization of n, then according to the definitions and properties αi i of S(n) and P (n), we can let S(n) = S(pα i ) = mpi , where S(pi ) is the largest number of α2 αr 1 {S(pα 1 ), S(p2 ), · · · , S(pr )}. If αi = 1, then m = 1 and S(n) = pi is prime. If αi > 1, P then m > 1 and S(n) is composite. Hence n≤k 1 is the number of n (1 ≤ n ≤ k) such that n6∈A S(n) = 1 or S(n) is composite. Apparently S(n) = 1 if and only if n = 1. Therefore we have X X X X 1=1+ 1≤1+ 1+ 1, (8) npα ≤k αp>mp>M, α≥2

n≤k S(n)=S(pα ), α≥2

n≤k n6∈A

S(n)≤M

where M ¿ k ² , ² > 0 is a real number. Now we will estimate every term of (8). Firstly we will estimate the first summation. From Lemma 2.3 we have X X X X X X X 1 = 1+ 1+ 1= 1 npα ≤k αp>M, α≥2

np2 ≤k 2p>M

X

= M 2

¿

√ <p≤ k

npα ≤k αp>M, α≥3

µ

M 2

¶ k + O(1) + p2

2k +O M log M 2k +O M log M

µ

µ

√ <p≤ k n≤ pk2

µ

X pα ≤k αp≥M, 3≤α<p

k M log2 M k M log2 M

+

M <p≤ α≥3

µ

k √

M M

n≤ pkα

¶ k + O(1) + pα

X

+ ¶

pα ≤k αp>M, α≥3

k

+

X pα ≤k αp>M, α≥p

µ

¶ k + O(1) pα

¶ ¶ X µk k + O(1) + + O(1) pα pα √ p≤ k √ α> M

2

k M −1

¿

k , M log M

(9)

where M ¿ k ² . In order to estimate the other term of (8), we must estimate it in a different way. For M M any prime p ≤ M , let α(p) = [ p−1 ] denote the largest number not exceeding [ p−1 ]. Let


Vol. 7

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On Erd¨ os-Smarandache numbers

Q u = p≤M pα(p) . For any positive integer n such that S(n) ≤ M , let S(n) = S(pα ), according P∞ M to the definition of S(n), we must have pα |M !, thus we have α ≤ j=1 [ M pj ] ≤ [ p−1 ]. Hence for all positive integer n such that S(n) ≤ M , we have n|u, that is, the number of all the n like this is not exceeding all the divisors of u, then we have · ¸¶ Y µ X X Y M 1 ≤ 1= (1 + α(p)) = 1+ p−1 p≤M p≤M S(n)≤M d|u   µ · ¸¶ X M , log 1 + (10) = exp  p−1 p≤M

where exp(y) = ey . From Lemma 2.2 and (10), we have   µ ¶ X X M  1 ≤ exp  log 1 + p−1 p≤M S(n)≤M   µ ¶¸ X · 1  = exp log(p − 1 + M ) − log p − log 1 −  p  p≤M   X X 1  ≤ exp π(M ) log(2M ) − log p + p p≤M p≤M µ µ ¶¶ M log(2M ) M = exp −M +O log M log M µ ¶ M ¿ exp , log M

(11)

´ ³ √ where M ¿ k ² . Now let M = log k log log k (it determines k > 2), we have exp logMM ¿ k

3

log k(log log k) 2

, thus combining (8), (9) and (11), we immediately get X

µ 1=O

n≤k n6∈A

k

.

3

log k(log log k) 2

Therefore, we have X n≤k n∈A

1=k−

X

µ 1=k+O

n≤k n6∈A

k 3

log k(log log k) 2

.

This completes the proof of the theorem.

References [1] A. Ivic, On a Problem of Erd¨ os Involving the largest Prime Factor of n, Monatsh. Math., 145(2005), 35-46.


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Rong Ma and Yulong Zhang

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[2] K. Ford, The normal behavior of the Smarandache function, Smarandache Notions Journal, 10(1999), 81-86. [3] J-M De Koninck and N. Doyon, On a thin set of integers involving the largest prime factor function, Int. J. Math. Sci., 19(2003), 1185-1192. [4] Y. Lu, On the solutions of an equation involving the Smarandache function, Scientia Magna, 2(2006), No. 1, 76-79. [5] M. Le, A conjecture concerning the Smarandache function, Journal of natural science of Heilongjiang University, 24(2007), No. 5, 687-688. [6] F. Du, On a conjecture of the Smarandache function S(n), Pure and Applied Mathematics, 23(2007), No. 2, 205-208. [7] Z. Xu, On the value distribution of the Smarandache function, Acta Mathematica Sinica, 49(2006), No. 5, 1009-1012. [8] M. Le, Two function equations, Smarandache Notions Journal, 14(2004), 180-182. [9] P. Erd¨ os and P. C. Ashbache, Thoughts of Pal Erd¨os on Some Smarandache Notions, Smarandache Notion Journal, 8(1997), 220-224. [10] P. Erd¨ os, Problem 6674, Amer Math Monthly, 98(1991), 965. [11] I. Kastanas, Solution to Problem 6674, Amer Math Monthly, 98(1994), 179. [12] S. Akbik, On a density problem of Erd¨ os, Int J Math Sci., 22(1999), 655-658. [13] C. Pan and C. Pan, Element of the Analytic Number Theory, Science Press, Beijing, 1991 (in Chinese). [14] T. Apstol, Introduction to Analytic Number Theory, Springer-Verlag, New York, 1976. [15] F. Smarandache, Definitions, Solved and Unsolved Problems, Conjectures and Theorems in Number Theory and Geometry, Chicago, Xiquan Publishing House, 2000. [16] F. Smarandache, Only Problems, Not Solutions, Chicago, Xiquan Publishing House, 1993.


Scientia Magna Vol. 7 (2011), No. 4, 7-18

A view on generalized intuitionistic fuzzy contra continuous functions and its applications R. Dhavaseelan† , E. Roja‡ and M. K. Uma] † Department of Mathematics, Sona College of Technology, Salem, 636005, Tamil Nadu, India ‡ ] Department of Mathematics, Sri Saradha College for Women, Salem-16, Tamil Nadu, India E-mail: dhavaseelan.r@gmail.com Abstract In this paper the following concepts are generalized intuitionistic fuzzy contra continuous function, strongly generalized intuitionistic fuzzy contra continuous function and generalized intuitionistic fuzzy contra irresolute are studied. The concepts of generalized intuitionistic fuzzy S-closed and strongly generalized intuitionistic fuzzy S-closed are studied. The concepts of generalized intuitionistic fuzzy compact spaces and generalized intuitionistic fuzzy almost compact spaces are established. The concepts of generalized intuitionistic fuzzy filter and intuitionistic fuzzy C-convergent are established. Some properties are investigated with some illustrations. Keywords Generalized intuitionistic fuzzy contra continuity, strongly generalized intuitioni -stic fuzzy contra continuity, generalized intuitionistic fuzzy contra irresolute, generalized int -uitionistic fuzzy S-closed, generalized intuitionistic fuzzy compact spaces, generalized intuiti -onistic fuzzy almost compact spaces, generalized intuitionistic fuzzy filter and intuitionistic fuzzy C-convergent. 2000 Mathematics Subject Classification: 54A40, 03E72.

§1. Introduction The fuzzy concept has invaded almost all branches of mathematics ever since the introduction of fuzzy sets by L. A. Zadeh [16] . These fuzzy sets have applications in many fields such as information [14] and control [15] . The theory of fuzzy topological space was introduced and developed by C. L. Chang [7] and since then various notions in classical topology has extended the fuzzy topological space. The idea of “intuitionistic fuzzy set”was first published by Atanassov [1] and many works by the same author and his colleagues appeared in the literature [2,3,4] . Later, this concept was generalized to “intuitionistic L - fuzzy sets”by Atanassov and Stoeva [5] . The concepts of “On some generalizations of fuzzy continuous functions”was introduced by G. Balasubramanian and P. Sundaram [6] . The concepts of “Generalized intuitionistic fuzzy closed sets”was introduced by R. Dhavaseelan, E. Roja and M. K. Uma [9] . The concepts of “fuzzy contra continuous”was


8

R. Dhavaseelan, E. Roja and M. K. Uma

No. 4

introduced by E. Ekici and E. Kerre [10] . In this paper the following concepts are generalized intuitionistic fuzzy contra continuous function, strongly generalized intuitionistic fuzzy contra continuous function and generalized intuitionistic fuzzy contra irresolute are studied. The concepts of generalized intuitionistic fuzzy S-closed and strongly generalized intuitionistic fuzzy S-closed are studied. The concepts of generalized intuitionistic fuzzy compact spaces and generalized intuitionistic fuzzy almost compact spaces are established. The concepts of generalized intuitionistic fuzzy filter and intuitionistic fuzzy C-convergent are established. Some properties are investigated with some illustrations.

§2. Preliminaries Definition 2.1.[3] Let X be a nonempty fixed set. An intuitionistic fuzzy set (IF S for short) A is an object having the form A = {hx, µA (x), δA (x)i : x ∈ X} where the function µA : X → I and δA : X → I denote the degree of membership (namely µA (x)) and the degree of nonmembership (δA (x)) of each element x ∈ X to the set A, respectively, and 0 ≤ µA (x) + δA (x) ≤ 1 for each x ∈ X. Definition 2.2.[3] Let X be a nonempty set and the intuitionistic fuzzy sets A and B in the form A = {hx, µA (x), δA (x)i : x ∈ X}, B = {hx, µB (x), δB (x)i : x ∈ X}. Then (a) A ⊆ B iff µA (x) ≤ µB (x) and δA (x) ≥ δB (x) for all x ∈ X; (b) A = B iff A ⊆ B and B ⊆ A; (c) A¯ = {hx, δA (x), µA (x)i : x ∈ X}; (d) A ∩ B = {hx, µA (x) ∧ µB (x), δA (x) ∨ δB (x)i : x ∈ X}; (e) A ∪ B = {hx, µA (x) ∨ µB (x), δA (x) ∧ δB (x)i : x ∈ X}; (f) [ ]A = {hx, µA (x), 1 − µA (x)i : x ∈ X}; (g) h iA = {hx, 1 − δA (x), δA (x)i : x ∈ X}. Definition 2.3.[3] Let {Ai : i ∈ J} be an arbitrary family of intuitionistic fuzzy sets in X. Then T (a) Ai = {hx, ∧µAi (x), ∨δAi (x)i : x ∈ X}; S (b) Ai = {hx, ∨µAi (x), ∧δAi (x)i : x ∈ X}. Since our main purpose is to construct the tools for developing intuitionistic fuzzy topological spaces, we must introduce the intuitionistic fuzzy sets 0∼ and 1∼ in X as follows: Definition 2.4.[3] 0∼ = {hx, 0, 1i : x ∈ X} and 1∼ = {hx, 1, 0i : x ∈ X}. Here are the basic properties of inclusion and complementation: Corollary 2.1.[3] Let A, B, C be intuitionistic fuzzy sets in X. Then (a) A ⊆ B and C ⊆ D ⇒ A ∪ C ⊆ B ∪ D and A ∩ C ⊆ B ∩ D; (b) A ⊆ B and A ⊆ C ⇒ A ⊆ B ∩ C; (c) A ⊆ C and B ⊆ C ⇒ A ∪ B ⊆ C; (d) A ⊆ B and B ⊆ C ⇒ A ⊆ C; (e) A ∪ B = A ∩ B; (f) A ∩ B = A ∪ B; (g) A ⊆ B ⇒ B ⊆ A;


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A view on generalized intuitionistic fuzzy contra continuous functions and its applications

9

(h) (A) = A; (i) 1∼ = 0∼ ; (j) 0∼ = 1∼ . Now we shall define the image and preimage of intuitionistic fuzzy sets. Let X and Y be two nonempty sets and f : X → Y be a function. Definition 2.5.[3] (a) If B = {hy, µB (y), δB (y)i : y ∈ Y } is an intuitionistic fuzzy set in Y , then the preimage of B under f , denoted by f −1 (B), is the intuitionistic fuzzy set in X defined by f −1 (B) = {hx, f −1 (µB )(x), f −1 (δB )(x)i : x ∈ X}. (b) If A = {hx, λA (x), ϑA (x)i : x ∈ X} is an intuitionistic fuzzy set in X, then the image of A under f , denoted by f (A), is the intuitionistic fuzzy set in Y defined by f (A) = {hy, f (λA )(y), (1 − f (1 − ϑA ))(y)i : y ∈ Y }. Where  sup −1 λ (x), if f −1 (y) 6= ∅; x∈f (y) A f (λA )(y) = 0, otherwise,  inf −1 (y) 6= ∅; x∈f −1 (y) ϑA (x), if f (1 − f (1 − ϑA ))(y) = 1, otherwise. For the sake of simplicity,let us use the symbol f− (ϑA ) for 1 − f (1 − ϑA ). Corollary 2.2.[3] Let A, Ai (i ∈ J) be intuitionistic fuzzy sets in X, B, Bi (i ∈ K) be intuitionistic fuzzy sets in Y and f : X → Y a function. Then (a) A1 ⊆ A2 ⇒ f (A1 ) ⊆ f (A2 ); (b) B1 ⊆ B2 ⇒ f −1 (B1 ) ⊆ f −1 (B2 ); (c) A ⊆ f −1 (f (A)) { If f is injective, then A = f −1 (f (A)) }; (d) f (f −1 (B)) ⊆ B { If f is surjective, then f (f −1 (B)) = B }; S S (e) f −1 ( Bj ) = f −1 (Bj ); T T (f) f −1 ( Bj ) = f −1 (Bj ); S S (g) f ( Ai ) = f (Ai ); T T T T (h) f ( Ai ) ⊆ f (Ai ) { If f is injective, then f ( Ai ) = f (Ai )}; (i) f −1 (1∼ ) = 1∼ ; (j) f −1 (0∼ ) = 0∼ ; (k) f (1∼ ) = 1∼ , if f is surjective; (l) f (0∼ ) = 0∼ ; (m) f (A) ⊆ f (A), if f is surjective; (n) f −1 (B) = f −1 (B). Definition 2.6.[13] An intuitionistic fuzzy set A of intuitionistic fuzzy topological space X is called a intuitionistic fuzzy regular closed set if IF cl(IF int(A)) = A. Equivalently An intuitionistic fuzzy set A of intuitionistic fuzzy topological space X is called a intuitionistic fuzzy regular open set if IF int(IF cl(A)) = A. Definition 2.7.[9] Let (X, T ) be an intuitionistic fuzzy topological space. An intuitionistic fuzzy set A in (X, T ) is said to be generalized intuitionistic fuzzy closed (in shortly GIF closed)


10

R. Dhavaseelan, E. Roja and M. K. Uma

No. 4

if IF cl (A) ⊆ G whenever A ⊆ G and G is intuitionistic fuzzy open. The complement of a GIF closed set is GIF open. Definition 2.8.[9] Let (X, T ) be an intuitionistic fuzzy topological space and A be an intuitionistic fuzzy set in X. Then intuitionistic fuzzy generalized closure (in short IF Gcl) and intuitionistic fuzzy generalized interior (in short IF Gint) of A are defined by T (a) IF Gcl(A) = {G : G is a GIF closed set in X and A ⊆ G }. S (b) IF Gint(A) = {G : G is a GIF open set in X and A ⊇ G}. Definition 2.9.[11] A nonvoid family F of GIF sets on X is said to be generalized intuitionistic fuzzy filter (in short GIF filter) if (1) 0∼ ∈ / F; (2) If A, B ∈ F then A ∩ B ∈ F; (3) If A ∈ F and A ⊂ B then B ∈ F.

§3. Generalized intuitionistic fuzzy contra continuous function Definition 3.1. Let (X, T ) and (Y, S) be any two intuitionistic fuzzy topological spaces. (a) A map f : (X, T ) → (Y, S) is called intuitionistic fuzzy contra continuous (in short IF contra continuous) if the inverse image of every open set in (Y, S) is intuitionistic fuzzy closed in (X, T ). Equivalently if the inverse image of every closed set in (Y, S) is intuitionistic fuzzy open in (X, T ). (b) A map f : (X, T ) → (Y, S) is called generalized intuitionistic fuzzy contra continuous (in short GIF contra continuous) if the inverse image of every open set in (Y, S) is GIF closed in (X, T ). Equivalently if the inverse image of every closed set in (Y, S) is GIF open in (X, T ). (c) A map f : (X, T ) → (Y, S) is called GIF contra irresolute if the inverse image of every GIF closed set in (Y, S) is GIF open in (X, T ). Equivalently if the inverse image of every GIF open set in (Y, S) is GIF closed in (X, T ). (d) A map f : (X, T ) → (Y, S) is said to be strongly GIF contra continuous if the inverse image of every GIF open set in (Y, S) is intuitionistic fuzzy closed in (X, T ). Equivalently if the inverse image of every GIF closed set in (Y, S) is intuitionistic fuzzy open in (X, T ). Proposition 3.1. Let f : (X, T ) → (Y, S) be a bijective map. Then f is GIF contra continuous mapping if IF cl(f (A)) ⊆ f (IF Gint(A)) for every intuitionistic fuzzy set A in (X, T ). Proposition 3.2. Let (X, T ) and (Y, S) be any two intuitionistic fuzzy topological spaces. Let f : (X, T ) → (Y, S) be a map. Suppose that one of the following properties hold. (a) f (IF Gcl(A)) ⊆ IF int(f (A)) for each intuitionistic fuzzy set A in (X, T ). (b) IF Gcl(f −1 (B)) ⊆ f −1 (IF int(B)) for each intuitionistic fuzzy set B in (Y, S). (c) f −1 (IF cl(B)) ⊆ IF Gint(f −1 (B)) for each intuitionistic fuzzy set B in (Y, S). Then f is GIF contra continuous mapping.


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Proposition 3.3. Let (X, T ) and (Y, S) be any two intuitionistic fuzzy topological spaces. Let f : (X, T ) → (Y, S) be a map. Suppose that one of the following properties hold. (a) f −1 (IF Gcl(A)) ⊆ IF Gint(IF Gcl(f −1 (A)) for each intuitionistic fuzzy set A in (Y, S). (b) IF Gcl(IF Gint(f −1 (A))) ⊆ f −1 (IF Gint(A)) for each intuitionistic fuzzy set A in (Y, S). (c) f (IF Gcl(IF Gint(A))) ⊆ IF Gint(f (A)) for each intuitionistic fuzzy set A in (X, T ). (d) f (IF Gcl(A)) ⊆ IF Gint(f (A)) for each intuitionistic fuzzy set A in (X, T ). Then f is GIF contra continuous mapping. Proposition 3.4. Let (X, T ) and (Y, S) be any two intuitionistic fuzzy topological spaces. If f : (X, T ) → (Y, S) is intuitionistic fuzzy contra continuous then it is GIF contra continuous. The converse of Proposition 3.4 is not true. See Example 3.1. Example 3.1. Let X = {a, b, c}. Define intuitionistic fuzzy sets A and B as follows a A = hx, ( 0.4 ,

b c 0.5 , 0.4 ),

a ( 0.4 ,

b c 0.4 , 0.4 )i

a B = hx, ( 0.3 ,

b c 0.4 , 0.3 ),

a ( 0.5 ,

b c 0.6 , 0.7 )i.

and

Then T = {0∼ , 1∼ , A} and S = {0∼ , 1∼ , B} are intuitionistic fuzzy topologies on X. Thus (X, T ) and (X, S) are intuitionistic fuzzy topological spaces. Define f : (X, T ) → (X, S) as f (a) = b, f (b) = a, f (c) = c. Clearly f is GIF contra continuous. But f is not intuitionistic fuzzy contra continuous. Since, f −1 (B) ∈ / T for B ∈ S. Proposition 3.5. Let (X, T ) and (Y, S) be any two intuitionistic fuzzy topological spaces. If f : (X, T ) → (Y, S) is GIF contra irresolute then it is GIF contra continuous. The converse of Proposition 3.5 is not true. See Example 3.2. Example 3.2. Let X = {a, b, c}. Define the intuitionistic fuzzy sets A, B and C as follows. a A = hx, ( 0.4 , a B = hx, ( 0.7 ,

b c 0.4 , 0.5 ), b c 0.6 , 0.5 ),

a ( 0.5 , a ( 0.3 ,

b c 0.5 , 0.5 )i, b c 0.4 , 0.5 )i

a C = hx, ( 0.4 ,

b c 0.5 , 0.5 ),

a ( 0.4 ,

b c 0.5 , 0.5 )i.

and

T = {0∼ , 1∼ , A, B} and S = {0∼ , 1∼ , C} are intuitionistic fuzzy topologies on X. Thus (X, T ) and (X, S) are intuitionistic fuzzy topological spaces. Define f : (X, T ) → (X, S) as follows f (a) = b, f (b) = a, f (c) = c. Clearly f is GIF contra continuous. But f is not a b c a b c GIF contra irresolute. Since D = hx, ( 0.3 , 0.4 , 0.5 ), ( 0.5 , 0.5 , 0.5 )i is GIF closed in (X, S), −1 f (D) is not GIF -open in (X, T ). Proposition 3.6. Let (X, T ) and (Y, S) be any two intuitionistic fuzzy topological spaces. If f : (X, T ) → (Y, S) is strongly GIF contra continuous then f is intuitionistic fuzzy contra continuous. The converse Proposition 3.6 is not true. See Example 3.3. Example 3.3. Let X = {a, b, c}. Define the intuitionistic fuzzy sets A, B and C as follows.


12

R. Dhavaseelan, E. Roja and M. K. Uma a A = hx, ( 0.3 , a B = hx, ( 0.1 ,

b c 0.2 , 0.2 ), b c 0.1 , 0.1 ),

a ( 0.4 , a ( 0.9 ,

b c 0.5 , 0.5 )i, b c 0.9 , 0.9 )i

a , C = hx, ( 0.9

b c 0.9 , 0.9 ),

a ( 0.1 ,

b c 0.1 , 0.1 )i.

No. 4

and

T = {0∼ , 1∼ , A, B} and S = {0∼ , 1∼ , C} are intuitionistic fuzzy topologies on X. Thus (X, T ) and (X, S) are intuitionistic fuzzy topological spaces. Define f : (X, T ) → (X, S) as follows f (a) = a, f (b) = b, f (c) = b. Clearly f is intuitionistic fuzzy contra continuous. But f b c a c a , 0.99 , 0.9 ), ( 0.1 , 0b , 0.1 )i is GIF is not strongly GIF contra continuous. Since D = hx, ( 0.9 −1 open in (X, S), f (D) is not intuitionistic fuzzy closed in (X, T ). Proposition 3.7. Let (X, T ) and (Y, S) be any two intuitionistic fuzzy topological spaces. If f : (X, T ) → (Y, S) is strongly GIF contra continuous then f is GIF contra continuous. The converse Proposition 3.7 is not true. See Example 3.4. Example 3.4. Let X = {a, b, c}. Define the intuitionistic fuzzy sets A, B and C as follows. a A = hx, ( 0.4 , a B = hx, ( 0.6 ,

b c 0.5 , 0.5 ), b c 0.7 , 0.5 ),

a ( 0.5 , a ( 0.4 ,

b c 0.5 , 0.5 )i, b c 0.3 , 0.5 )i

a C = hx, ( 0.4 ,

b c 0.4 , 0.5 ),

a ( 0.4 ,

b c 0.4 , 0.5 )i.

and

T = {0∼ , 1∼ , A, B} and S = {0∼ , 1∼ , C} are intuitionistic fuzzy topologies on X . Thus (X , T ) and (X, S) are intuitionistic fuzzy topological spaces. Define f : (X, T ) → (X, S) as follows f (a) = c, f (b) = c, f (c) = c. Clearly f is GIF contra continuous. But f is not a b c a b c strongly GIF contra continuous. Since D = hx, ( 0.4 , 0.5 , 0.5 ), ( 0.4 , 0.4 , 0.3 )i is a GIF open −1 set in (X, S), f (D) is not intuitionistic fuzzy closed in (X, T ). Proposition 3.8. Let (X, T ) and (Y, S) be any two intuitionistic fuzzy topological spaces. If f : (X, T ) → (Y, S) is strongly GIF contra continuous then f is GIF contra irresolute. The converse Proposition 3.8 is not true. See Example 3.5. Example 3.5. Let X = {a, b, c}. Define the intuitionistic fuzzy sets A, B and C as follows. a b c a b c A = hx, ( 0.9 , 0.9 , 0.9 ), ( 0.1 , 0.1 , 0.1 )i, a b c a b c B = hx, ( 0.99 , 0.99 , 0.99 ), ( 0 , 0.01 , 0 )i

and a C = hx, ( 0.9 ,

b c 0.9 , 0.9 ),

a ( 0.1 ,

b c 0 , 0.05 )i.

T = {0∼ , 1∼ , A, B} and S = {0∼ , 1∼ , C} are intuitionistic fuzzy topologies on X. Thus (X, T ) and (X, S) are intuitionistic fuzzy topological spaces. Define f : (X, T ) → (X, S) as follows f (a) = a, f (b) = c, f (c) = b. Clearly f is GIF contra irresolute. But f is not strongly


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a b c a c GIF contra continuous. Since D = hx, ( 0.99 , 0.99 , 0.99 ), ( 0.01 , 0b , 0.01 )i is a GIF open set in −1 (X, S), f (D) is not intuitionistic fuzzy closed in (X, T ). Proposition 3.9. Let (X, T ) , (Y, S) and (Z, R) be any three intuitionistic fuzzy topological spaces. Let f : (X, T ) → (Y, S) and g : (Y, S) → (Z, R) be maps. (i) If f is GIF contra irresolute and g is GIF contra continuous then g◦f is GIF continuous. (ii) If f is GIF contra irresolute and g is GIF continuous then g ◦ f is GIF contra continuous. (iii) If f is GIF irresolute and g is GIF contra continuous then g ◦ f is GIF contra continuous. (iv) If f is strongly GIF contra continuous and g is GIF contra continuous then g ◦ f is intuitionistic fuzzy continuous. (v) If f is strongly GIF contra continuous and g is GIF continuous then g◦f is intuitionistic fuzzy contra continuous. (vi) If f is strongly GIF continuous and g is GIF contra continuous then g ◦ f is intuitionistic fuzzy contra continuous. Definition 3.2. An intuitionistic fuzzy topological space (X, T ) is said to be intuitionistic fuzzy T1/2 if every GIF closed set in (X, T ) is intuitionistic fuzzy closed in (X, T ). Proposition 3.10. Let (X, T ), (Y, S) and (Z, R) be any three intuitionistic fuzzy topological spaces. Let f : (X, T ) → (Y, S) and g : (Y, S) → (Z, R) be mapping and (Y, S) be intuitionistic fuzzy T1/2 if f and g are GIF contra continuous then g ◦ f is GIF continuous. The Proposition 3.10 is not valid if (Y, S) is not intuitionistic fuzzy T1/2 . See Example 3.6. Example 3.6. Let X = {a, b, c}. Define the intuitionistic fuzzy sets A, B, C and D as follows.

a , A = hx, ( 0.3 a B = hx, ( 0.6 , a C = hx, ( 0.4 ,

b c 0.3 , 0.4 ), b c 0.6 , 0.6 ), b c 0.5 , 0.4 ),

a ( 0.4 , a ( 0.3 , a ( 0.4 ,

b c 0.5 , 0.5 )i, b c 0.3 , 0.3 )i, b c 0.4 , 0.4 )i

a , D = hx, ( 0.3

b c 0.4 , 0.3 ),

a ( 0.5 ,

b c 0.6 , 0.7 )i.

and

Then the family T = {0∼ , 1∼ , A, B}, S = {0∼ , 1∼ , C} and R = {0∼ , 1∼ , D} are intuitionistic fuzzy topologics on X. Thus (X, T ) , (X, S) and (X, R) are intuitionistic fuzzy topological spaces. Also define f : (X, T ) → (X, S) as f (a) = a, f (b) = b, f (c) = b and g : (X, S) → (X, R) as g(a) = b, g(b) = a, g(c) = c. Then f and g are GIF contra continuous functions. But g ◦ f is not GIF continuous. For D is intuitionistic fuzzy open in (X, R). f −1 (g −1 (D)) is not GIF open in (X, T ). g ◦ f is not GIF continuous. Further (X, S) is not intuitionistic fuzzy T1/2 . Proposition 3.11. Let (X, T ), (Y, S) and (Z, R) be any three intuitionistic fuzzy topological spaces. Let f : (X, T ) → (Y, S) and g : (Y, S) → (Z, R) be mapping and (Y, S) be intuitionistic fuzzy T1/2 if f is intuitionistic fuzzy contra continuous and g is GIF contra irresolute then g ◦ f is strongly GIF continuous.


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No. 4

The Proposition 3.11 is not valid if (Y, S) is not intuitionistic fuzzy T1/2 . See Example 3.7. Example 3.7. Let X = {a, b, c}. Define the intuitionistic fuzzy sets A, B, C and D as follows. a A = hx, ( 0.9 , a B = hx, ( 0.4 , a C = hx, ( 0.4 ,

b c 0.9 , 0.9 ), b c 0.4 , 0.4 ), b c 0.5 , 0.5 ),

a ( 0.1 , a ( 0.4 , a ( 0.4 ,

b c 0.1 , 0.1 )i, b c 0.4 , 0.5 )i, b c 0.4 , 0.5 )i

a D = hx, ( 0.4 ,

b c 0.2 , 0.3 ),

a ( 0.6 ,

b c 0.8 , 0.7 )i.

and

Then the family T = {0∼ , 1∼ , A, B}, S = {0∼ , 1∼ , C} and R = {0∼ , 1∼ , D} are intuitionistic fuzzy topologics on X. Thus (X, T ), (X, S) and (X, R) are intuitionistic fuzzy topological spaces. Also define f : (X, T ) → (X, S) as f (a) = a, f (b) = a, f (c) = b and g : (X, S) → (X, R) as g(a) = c, g(b) = a, g(c) = b. Then f is intuitionistic fuzzy contra continuous and g is GIF contra irresolute. But g ◦ f is not strongly GIF continuous. For D is GIF open in (X, R). f −1 (g −1 (D)) is not intuitionistic fuzzy open in (X, T ). g ◦ f is not strongly GIF continuous. Further (X, S) is not intuitionistic fuzzy T1/2 . Definition 3.3. Let X be a non-empty set and x ∈ X a fixed element in X. If r ∈ I0 , s ∈ I1 are fixed real number such that r+s ≤ 1 then the intuitionistic fuzzy set xr,s = hy, xr , xs i is called an intuitionistic fuzzy point in X, where r denotes the degree of membership of xr,s , s denotes the degree of nonmembership of xr,s . The intuitionistic fuzzy point xr,s is contained in the intuitionistic fuzzy set A iff r < µA (x), s > δA (x). Proposition 3.12. Let (X, T ) and (Y, S) be any two intuitionistic fuzzy topological spaces. For a function f : (X, T ) → (Y, S) the following statements are equivalents: (a) f is GIF contra continuous mapping. (b) For each intuitionistic fuzzy point xr,s of X and for each intuitionistic fuzzy closed set B of (Y, S) containing f (xr,s ), there exists a GIF open set A of (X, T ) containing xr,s , such that A ⊆ f −1 (B). (c) For each intuitionistic fuzzy point xr,s of X and for each intuitionistic fuzzy closed set B of (Y, S) containing f (xr,s ), there exists a GIF open set A of (X, T ) containing xr,s , such that f (A) ⊆ B. Proof. (a)⇒(b) Let f is GIF contra continuous mapping. Let B be an intuitionistic fuzzy closed set in (Y, S) and let xr,s be an intuitionistic fuzzy point of X, such that f (xr,s ) ∈ B. Then xr,s ∈ f −1 (B), xr,s ∈ f −1 (B) = IF Gint(f −1 (B)). Let A = IF Gint(f −1 (B)), then A is a GIF open set and A = IF Gint(f −1 (B)) ⊆ f −1 (B). This implies A ⊆ f −1 (B). (b)⇒(c) Let B be an intuitionistic fuzzy closed set in (Y, S) and let xr,s be an intuitionistic fuzzy point in X, such that f (xr,s ) ∈ B. Then xr,s ∈ f −1 (B). By hypothesis f −1 (B) is a GIF open set in (X, T ) and A ⊆ f −1 (B). This implies f (A) ⊆ f (f −1 (B)) ⊆ B. (c)⇒(a) Let B be an intuitionistic fuzzy closed set in (Y, S) and let xr,s be an intuitionistic fuzzy point in X, such that f (xr,s ) ∈ B. Then xr,s ∈ f −1 (B). By hypothesis there exists a GIF open set A of (X, T ), such that xr,s ∈ A and f (A) ⊆ B. This implies xr,s ∈ A ⊆


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f −1 (f (A)) ⊆ f −1 (B). Since A is GIF open, A = IF Gint(A) ⊆ IF Gint(f −1 (B)). Therefore S xr,s ∈ IF Gint(f −1 (B)), f −1 (B) = xr,s ∈f −1 (B) (xr,s ) ⊆ IF Gint(f −1 (B) ⊆ f −1 (B). Hence f −1 (B) is a GIF open set in (X, T ). Thus f is GIF contra continuous mapping. Definition 3.4. Let (X, T ) and (Y, S) be any intuitionistic fuzzy topological spaces. Let f : (X, T ) → (Y, S) be a mapping. The graph g : X → X × Y of f is defined by g(x) = (x, f (x)), ∀x ∈ X. Proposition 3.13. Let (X, T ) and (Y, S) be any two intuitionistic fuzzy topological spaces. Let f : (X, T ) → (Y, S) be any mapping. If the graph g : X → X × Y of f is GIF contra continuous then f is also GIF contra continuous. Proof. Let A be an intuitionistic fuzzy open set in (Y, S). By definition f −1 (A) = T −1 1∼ f (A) = g −1 (1∼ × A). Since g is GIF contra continuous, g −1 (1∼ × A) is GIF closed in (X, T ). Now f −1 (A) is a GIF closed set in (X, T ). Thus f is GIF contra continuous. Proposition 3.14. Let (X, T ) and (Y, S) be any two intuitionistic fuzzy topological spaces. Let f : (X, T ) → (Y, S) be any mapping. If the graph g : X → X × Y of f is strongly GIF contra continuous then f is also strongly GIF contra continuous. T Proof. Let A be an GIF open set in (Y, S). By definition f −1 (A) = 1∼ f −1 (A) = g −1 (1∼ × A). Since g is strongly GIF contra continuous, g −1 (1∼ × A) is intuitionistic fuzzy closed in (X, T ). Now f −1 (A) is a intuitionistic fuzzy closed set in (X, T ). Thus f is strongly GIF contra continuous. Proposition 3.15. Let (X, T ) and (Y, S) be any two intuitionistic fuzzy topological spaces. Let f : (X, T ) → (Y, S) be any mapping. If the graph g : X → X × Y of f is GIF contra irresolute then f is also GIF contra irresolute. T Proof. Let A be an GIF open set in (Y, S). By definition f −1 (A) = 1∼ f −1 (A) = g −1 (1∼ × A). Since g is GIF contra irresolute, g −1 (1∼ × A) is GIF closed in (X, T ). Now f −1 (A) is a GIF closed set in (X, T ). Thus f is GIF contra irresolute. Definition 3.5. Let (X, T ) be an intuitionistic fuzzy topological space. If a family S {hx, µGi , δGi i : i ∈ J} of GIF open sets in (X, T ) satisfies the condition {hx, µGi , δGi i : i ∈ J} = 1∼ then it is called a GIF open cover of (X, T ). Definition 3.6. A finite subfamily of a GIF open cover {hx, µGi , δGi i : i ∈ J} of (X, T ) which is also a GIF open cover of (X, T ) is called a finite subcover of {hx, µGi , δGi i : i ∈ J}. Definition 3.7. An intuitionistic fuzzy topological space (X, T ) is called GIF compact iff every GIF open cover of (X, T ) has a finite subcover. Proposition 3.16. Let (X, T ) and (Y, S) be any two intuitionistic fuzzy topological spaces and f : (X, T ) → (Y, S) be GIF contra continuous surjection. If (X, T ) is GIF compact then so is (Y, S). Proof. Let Gi = {hy, µGi , δGi i : i ∈ J} be an intuitionistic fuzzy closed in (Y, S). S 1 − Gi be an intuitionistic fuzzy open cover in (Y, S) with {h1 − y, 1 − µGi , 1 − δGi i : i ∈ J} S = i∈J 1 − Gi = 1∼ . Since f is GIF contra continuous, f −1 (Gi )={hx, µf −1 (Gi ) , δf −1 (Gi ) i : S S i ∈ J} is GIF open cover of (X, T ). Now i∈J f −1 (Gi ) = f −1 ( i∈J Gi ) = 1∼ . Since (X, T ) S is GIF compact, there exists a finite subcover J0 ⊂ J such that i∈J0 f −1 (Gi ) = 1∼ . Hence S S S S f ( i∈J0 f −1 (Gi )) = 1∼ , f f −1 ( i∈J0 (Gi )) = i∈J0 (1 − Gi ) = 1∼ . That is, i∈J0 (1 − Gi ) = 1∼ . Therefore (Y, S) is intuitionistic fuzzy compact.


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No. 4

Definition 3.8. (i) An intuitionistic fuzzy set A of intuitionistic fuzzy topological space X is called a GIF regular closed set if IF Gcl(IF Gint(A)) = A. Equivalently An intuitionistic fuzzy set A of intuitionistic fuzzy topological space X is called a GIF regular open set if IF Gint(IF Gcl(A)) = A. (ii) An intuitionistic fuzzy topological space (X, T ) is called a intuitionistic fuzzy S-closed space if each intuitionistic fuzzy regular closed cover of X has a finite subcover for X. (iii) An intuitionistic fuzzy topological space (X, T ) is called a GIF S-closed space if each GIF regular closed cover of X has a finite subcover for X. (iv) An intuitionistic fuzzy topological space (X, T ) is called a strongly intuitionistic fuzzy S-closed space if each intuitionistic fuzzy closed cover of X has a finite subcover for X. (v) An intuitionistic fuzzy topological space (X, T ) is called a strongly GIF S-closed space if each GIF closed cover of X has a finite subcover for X. Proposition 3.17. Every strongly GIF S-closed space of (X, T ) is GIF S-closed. S Proof. Let (X, T ) be strongly GIF S-closed space and let i∈J (Gi ) = 1∼ . Where {Gi }i∈J is a family of GIF regular closed sets in (X, T ). Since every GIF regular closed is a S GIF closed set, i∈J (Gi ) = 1∼ and (X, T ) is strongly GIF S-closed implies that there exists S a finite subfamily {Gi }i∈J0 ⊂J , such that i∈J0 (Gi ) = 1∼ . Here the finite cover of X by GIF regular closed sets has a finite subcover. Therefore (X, T ) is GIF S-closed. Proposition 3.18. Let (X, T ) and (Y, S) be any two intuitionistic fuzzy topological spaces and let f : (X, T ) → (Y, S) be GIF contra continuous function. If (X, T ) is strongly GIF S-closed space then (Y, S) is intuitionistic fuzzy compact. Proof. Let Gi = {hy, µGi (y), δGi (y)i : i ∈ J} be intuitionistic fuzzy open cover of (Y, S) S and let i∈J (Gi ) = 1∼ . Since f is GIF contra continuous, f −1 (Gi ) = {hx, µf −1 (Gi ) (x), δf −1 (Gi ) S S (x)i} is GIF closed cover of (X, T ) and i∈J f −1 (Gi ) = f −1 ( i∈J (Gi )) = 1∼ . Since (X, T ) S is strongly GIF S-closed, there exists a finite subcover J0 ⊂ J, such that i∈J0 f −1 (Gi ) = 1∼ . S S S Hence f ( i∈J0 f −1 (Gi )) = f f −1 ( i∈J0 (Gi )) = i∈J0 (Gi ) = 1∼ . Therefore (Y, S) is intuitionistic fuzzy compact. Proposition 3.19. Let (X, T ) and (Y, S) be any two intuitionistic fuzzy topological spaces and let f : (X, T ) → (Y, S) be strongly GIF contra continuous function. If (X, T ) is intuitionistic fuzzy compact space then (Y, S) is GIF S-closed. Proof. Let Gi = {hy, µGi (y), δGi (y)i : i ∈ J} be GIF regular closed cover of (Y, S). S Every GIF regular closed set is GIF closed set, let i∈J (Gi ) = 1∼ . Since f is strongly GIF contra continuous, f −1 (Gi ) = {hx, µf −1 (Gi ) (x), δf −1 (Gi ) (x)i} is intuitionistic fuzzy open cover S S of (X, T ) and i∈J f −1 (Gi ) = f −1 ( i∈J (Gi )) = 1∼ . Since (X, T ) is intuitionistic fuzzy S compact space, there exists a finite subcover J0 ⊂ J, such that i∈J0 f −1 (Gi ) = 1∼ . Hence S S S f ( i∈J0 f −1 (Gi )) = f f −1 ( i∈J0 (Gi )) = i∈J0 (Gi ) = 1∼ . Therefore (Y, S) is GIF S-closed. Proposition 3.20. Let (X, T ) and (Y, S) be any two intuitionistic fuzzy topological spaces and let f : (X, T ) → (Y, S) be GIF contra irresolute. If (X, T ) is GIF compact space then (Y, S) is strongly GIF S-closed. Proof. Let Gi = {hy, µGi (y), δGi (y)i : i ∈ J} be GIF closed cover of (Y, S) and let −1 (Gi ) = {hx, µf −1 (Gi ) (x), δf −1 (Gi ) (x)i} i∈J (Gi ) = 1∼ . Since f is GIF contra irresolute, f S S −1 is GIF open cover of (X, T ) and i∈J f (Gi ) = f −1 ( i∈J (Gi )) = 1∼ . Since (X, T ) is S


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A view on generalized intuitionistic fuzzy contra continuous functions and its applications

17

S GIF compact space, there exists a finite subcover J0 ⊂ J, such that i∈J0 f −1 (Gi ) = 1∼ . S S S Hence f ( i∈J0 f −1 (Gi )) = f f −1 ( i∈J0 (Gi )) = i∈J0 (Gi ) = 1∼ . Therefore (Y, S) is strongly GIF S-closed. Definition 3.9. An intuitionistic fuzzy topological space X is called almost compact space if each intuitionistic fuzzy open cover of X has finite subcover, the intuitionistic fuzzy closure of whose members cover X. Definition 3.10. An intuitionistic fuzzy topological space X is called GIF almost compact space if each GIF open cover of X has finite subcover, the GIF closure of whose members cover X. Proposition 3.21. Let (X, T ) and (Y, S) be any two intuitionistic fuzzy topological spaces and let f : (X, T ) → (Y, S) be GIF contra irresolute and onto mapping. If (X, T ) is GIF compact space then (Y, S) is GIF almost compact. Proof. Let Gi = {hy, µGi (y), δGi (y)i : i ∈ J} be GIF open cover of (Y, S). Then S S 1∼ = i∈J Gi ⊆ i∈J (IF Gcl(Gi )). Since f is GIF contra irresolute, f −1 (IF Gcl(Gi )) is S GIF open cover of (X, T ) and i∈J f −1 (IF Gcl(Gi )) = 1∼ . Since (X, T ) is GIF compact, S there exists a finite subcover J0 ⊂ J, such that i∈J0 f −1 (IF Gcl(Gi )) = 1∼ . Hence 1∼ = S S S f ( i∈J0 f −1 (IF Gcl(Gi ))) = f f −1 ( i∈J0 (IF Gcl(Gi ))) = i∈J0 (IF Gcl(Gi ). Therefore (Y, S) is GIF almost compact. Definition 3.11. (i) A nonempty family F of GIF open sets on (X, T ) is said to be a GIF filter if (1) 0∼ ∈ / F; (2) If A, B ∈ F then A ∩ B ∈ F; (3) If A ∈ F and A ⊂ B then B ∈ F; (ii) A nonempty family B of GIF open sets on F is said to be a GIF filter base if (1) 0∼ ∈ / B; (2) If B1 , B2 ∈ B then B3 ⊂ B1 ∩ B2 for some B3 ∈ B; (iii) A GIF filter F is called GIF convergent to a intuitionistic fuzzy point xr,s of a intuitionistic fuzzy topological space (X, T ) if for each GIF open set A of (X, T ) containing xr,s , there exists a intuitionistic fuzzy set B ∈ F such that B ⊆ A; (iv) A intuitionistic fuzzy filter F is said to be intuitionistic fuzzy C-convergent to a intuitionistic fuzzy point xr,s of a intuitionistic fuzzy topological space (X, T ) if for each intuitionistic fuzzy closed set A of (X, T ) containing xr,s , there exists a intuitionistic fuzzy set B ∈ F such that B ⊆ A. Proposition 3.22. Let (X, T ) and (Y, S) be any two intuitionistic fuzzy topological spaces. A mapping f : (X, T ) → (Y, S) is GIF contra continuous. If for each intuitionistic fuzzy point xr,s and each GIF filter F in (X, T ) is GIF convergent to xr,s then intuitionistic fuzzy filter f (F) is intuitionistic fuzzy C-convergent to f (xr,s ). Proof. Let xr,s = hx, xr , xs i be a intuitionistic fuzzy point and F be any GIF filter in (X, T ) is GIF convergent to xr,s . Since f is GIF contra continuous mapping, for each intuitionistic fuzzy closed set A containing f (xr,s ), there exists a GIF open set B of (X, T ) containing xr,s , such that f (B) ⊆ A. Since F is GIF convergent to xr,s , there exists intuitionistic fuzzy set C ∈ F such that C ⊆ B. Then f (C) ⊆ f (B) ⊆ A. That is f (C) ⊆ A. Hence the


18

R. Dhavaseelan, E. Roja and M. K. Uma

No. 4

intuitionistic fuzzy filter f (F) is intuitionistic fuzzy C-convergent to f (xr,s ).

References [1] K. Atanassov, lntuitionistic fuzzy sets, V. Sgurev, Ed., VII Itkr’s Session, Sofia (June 1983 Central Sci. and Techn. Library, Bulg. Academy of Sciences, 1984). [2] K. Atanassov, intuitionistic fuzzy sets, Fuzzy Sets and Systems, 20(1986), 87-96. [3] K. Atanassov, Review and new results on intuitionistic fuzzy sets, Preprint IM-MFAIS1-88, Sofia, 1988. [4] K. Atanassov and S. Stoeva, intuitionistic fuzzy sets, Polish Syrup. on Interval & Fuzzy Mathematics, Poznan, August, 1983, 23-26. [5] K. Atanassov and S. Stoeva, intuitionistic L-fuzzy sets, in: R. Trappl, Ed., Cybernetics and System Research, Elsevier, Amsterdam, 2(1984), 539-540. [6] G. Balasubramanian, P. Sundaram, On Some generalizations of fuzzy continuous functions, Fuzzy Sets and Systems, 86(1997), 93-100. [7] C. L. Chang, Fuzzy topological spaces, J. Math. Anal. Appl., 24(1968), 182-190. [8] D. Coker and A. Es Haydar, On fuzzy S-closed, TU. J Math., 1987, 145-152. [9] R. Dhavaseelan, E. Roja and M. K. Uma, Generalized intuitionistic Fuzzy Closed Sets, Advances in Fuzzy Mathematics, 5(2010), 152-172. [10] E. Ekici and E. Kerre, On fuzzy contra continuous, Advances in Fuzzy System, 1(2006), 35-44. [11] J. H. Park and J. K. Park, Hausdorffness on generalized intuitionistic fuzzy filter, Information Science, 168(2004), 95-110. [12] A. A. Ramadan, S. E. Abbas and A. A. Abd el-latif, Compactness in Intuitionistic fuzzy topological spaces, International Journal of Mathematics and Mathematical Science, 1(2005), 19-32. [13] R. Santhi and D. Jayathi, Intuitionistic Fuzzy Contra generalized semi pre continuous mapping, Advances in Fuzzy Mathematics, 5(2010), No. 2, 173-186. [14] Smets, P. The degree of belief in a fuzzu event, Information sciences, 25(1981), 1-19. [15] Sugeno, M. An Introductory survey of fuzzy control, Information sciences, 36(1985), 59-83. [16] L. A. Zadeh, Fuzzy sets, Inform. and Control, 8(1965), 338-353.


Scientia Magna Vol. 7 (2011), No. 4, 19-22

On the asymptotic properties of triangular base sequence Le Huan Department of Mathematics, Northwest University, Xi’an, Shaanxi, P. R. China E-mail: huanle1017@163.com Abstract Let {Tn } = {1, 2, 10, 11, 12, 100, 101, 102, 110, 1000, 1001, 1002, 1010, 1011, 10000, 10001, 10002, 10010, 10011, 10012, 100000, 100001, 100002, 100010, 100011, 100012, 100100, 1000000, 1000001, 1000002, 1000010, 1000011, 1000012, 1000100, · · · } denotes the triangular base sequence. The main purpose of this paper is using the elementary method and the properties of the geometric progression to study the convergent properties of the series consists of reciprocal elements of the set and the asymptotic properties of the triangular base P∞ 1 sequence, then proved that the series n=1 Tn is convergent and obtained an asymptotic formula for ln (Tn ). Keywords Triangular base, convergent properties, asymptotic formula, elementary method.

§1. Introduction and main results American-Romanian number theorist F. Smarandache introduced hundreds of interesting sequences and unsloved problems in reference [1] and [2], many authors had studied these problems before and obtained some interesting results, see reference [3] and [4]. In [1], he denotes triangular base sequence: {Tn } = {1, 2, 10, 11, 12, 100, 101, 102, 110, 1000, 1001, 1002, 1010, 1011, 10000, 10001, 10002, 10010, 10011, 10012, 100000, 100001, 100002, 100010, 100011, 100012, 100100, 1000000, 1000001, 1000002, 1000010, 1000011, 1000012, 1000100, . . .}. In a general case: if we want to design a base such that any number

A = (an · · · a2 a1 )B ,

n X

ai bi ,

i=1

with all ai = 0, 1, · · · , ti for i ≥ 1, where ti ≥ 1, then the base should be b1 = 1, bi+1 = (ti +1)∗bi for i ≥ 1. Numbers written in the triangular base defined as follows: t(n) =

n(n+1) , 2

n ≥ 1. So we


20

Le Huan

No. 4

can easily get the first several terms: 1 = 2 = 3 =

1(1 + 1) ; 2 1(1 + 1) 2· ; 2 2(2 + 1) 1(1 + 1) 1· +0· ; 2 2 1·

.. . 8 =

2(2 + 1) 1(1 + 1) 3(3 + 1) +0· +2· ; 2 2 2

.. . So in this sequence T1 = a1 = 1, T2 = a1 = 2, T3 = a2 a1 = 10, · · · , T8 = a3 a2 a1 = 102, · · · . we note that in the triangular base sequence ai can only to be 0, 1, 2 and an 6= 0. There have no people studied the properties of this sequence until now, at least we couldn’t find any reference about it. In this paper, we first study the properties of this sequence and obtain substantive progress. That is, we have proved these two results: Theorem 1.1. The series of positive terms which are formed by triangular base sequence S=

∞ X 1 T n=1 n

is convergent and S < 2. Theorem 1.2. Let {Tn } denotes the triangular base sequence, then we have the asymptotic formula √ ln (Tn ) = 2n · ln 10 + O(1).

§2. Proof of the theorems In this section, we shall use the elementary method and the structure of triangular base sequence to complete the proof of our theorems. The elementary methods used in this paper can be found in reference [5] and [6], we don’t repeat here. First we prove Theorem 1.1. We will classify the sequence {Tn } by the digit of each element: there are two elements 1, 2 which contain one digit in the decimal; There are three elements 10, 11, 12 which contain two digits in the decimal; There are four elements 100, 101, 102, 110 which contain three digits in the decimal· · · ; Generally, there are k + 1 elements which contain k digits in the decimal. Let u ∈ {Tn } and the digit of u is i in the decimal, then we have: i−1

i−1

10

i

z }| { z }| { 10i − 1 = 1 00 · · · 00 ≤ u ≤ 22 · · · 22 = 2 · . 9

(1)

− 1 < n ≤ (k+1)(k+2) − 1, the digit of Tn is k in the decimal, Obviously, in the interval of k(k+1) 2 2 while the total of Tn which satisfy the digit is k in the decimal is k + 1. Then from (1) we can


Vol. 7

21

On the asymptotic properties of triangular base sequence

immediately deduce the estimation formula S=

∞ ∞ X X 1 = T k(k+1) n=1 n k=1

2

X (k+1)(k+2) −1<n≤ −1 2

1 1 X k+1 <1+ + . Tn 2 10k−1

0

Now using the property of geometric series to estimate S =

∞ P k=2

S

0

(2)

k=2

k+1 , 10k−1

∞ X k+1 10k−1

=

k=2

4 5 6 3 + + 3 + 4 + ··· 10 102 10 10 ∞ 1 X k+1 10 10k−1

= 1 0 S 10

=

k=2

3 4 5 6 = + 3 + 4 + 5 + ··· 102 10 10 10 Make difference of the following formula we have (1 −

1 0 )S 10

3 1 1 1 1 + + 3 + 4 + 5 + ··· 10 102 10 10 10 1 2 + 10 1 . 10 1 − 10

= =

Thus 0

S =

2 10 1 + < . 9 81 2

(3)

Combine (2) and (3) we get S=

∞ X 1 1 1 < 1 + + = 2. T 2 2 n n=1

(4)

From (4) and the convergence rule of series of positive terms we can immediately deduce ∞ X 1 that is convergent, so we proved Theorem 1.1. T n=1 n Now we prove Theorem 1.2. For any real integer n, there insists real integer m such that m(m+1) − 1 < n ≤ (m+1)(m+2) − 1, when n satisfy m(m+1) − 1 < n ≤ (m+1)(m+2) − 1, the digit 2 2 2 2 of Tn is m in decimal scale . So from (1) we know that Tn must satisfy the inequality m−1

m

z }| { z }| { 10m − 1 . 10 = 1 00 · · · 00 ≤ Tn ≤ 22 · · · 22 = 2 · 9 Taking the logarithm of (5) in two sides we get m−1

ln (Tn ) = m · ln 10 + O (1) . −1 < n ≤ On the other hand, by the definition of m, m(m+1) 2 formula √ m = 2n + O(1).

(5)

(6) (m+1)(m+2) −1, 2

we have estimation


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Le Huan

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Combining (5) and (6) we obtain the asymptotic formula ln (Tn ) =

2n · ln 10 + O(1).

This completes the proof of our Theorems.

References [1] F. Smarandache, Sequences of numbers involved in unsolved problems, Phoenix, Hexis, 2006, 33. [2] F. Smarandache, Only Problems, Not Solutions, Chicago, Xiquan Publishing House, 1993. [3] Krassimir T. Atanassov, On some of the Smarandache’s problem, American Research Press, Lupton, AZ USA, 1999. [4] Krassimir T. Atanassov, Some Smarandache problems, Hexis, Phoenix, 2004. [5] T. M. Apostol, Introduction to Analytic Number Theory, New York, Springer-Verlag, 1976. [6] Zhang Wenpeng, The elementary number theory (in Chinese), Shaanxi Normal University Press, Xi’an, 2007.


Scientia Magna Vol. 7 (2011), No. 4, 23-28

A new class of double interval numbers Ayhan Esi Department of Mathematics, Science and Art Faculty, Adiyaman University, 02040, Adiyaman, Turkey E-mail: aesi23@hotmail.com Abstract In this paper we introduce the new concept of double interval valued sequence space 2 ` (p), where p = (pk,l ) is a double sequence of bounded strictly positive numbers. We study its different properties like completeness, solidness, converge free, symmetricity etc. We prove some inclusion relations also. Keywords Completeness, interval numbers. 2000 Mathematics Subject Classification: 40C05, 40J05, 46A45.

§1. Introduction and preliminaries Interval arithmetic was first suggested by Dwyer [2] in 1951. Development of interval arithmetic as a formal system and evidence of its value as a computational device was provided by Moore [9] in 1959 and Moore and Yang [10] 1962. Furthermore, Moore and others [2],[3],[6],[10] have developed applications to differential equations. Chiao in [1] introduced sequence of interval numbers and defined usual convergence of sequences of interval number. S¸eng¨on¨ ul and Eryilmaz in [11] introduced and studied bounded and convergent sequence spaces of interval numbers and showed that these spaces are complete metric space. Later Esi in [5] introduced and studied strongly almost λ−convergence and statistically almost λ−convergence of interval numbers. Recently Esi [4] introduced and studied the new concept of interval valued sequence space ` (p), where p = (pk ) is a sequence of bounded strictly positive numbers. A set consisting of a closed interval of real numbers x such that a ≤ x ≤ b is called an interval number. A real interval can also be considered as a set. Thus we can investigate some properties of interval numbers, for instance arithmetic properties or analysis properties. We denote the set of all real valued closed intervals by IR. Any elements of IR is called closed interval and denoted by x. That is x = {x ∈ R : a ≤ x ≤ b}. An interval number x is a closed subset of real numbers [1] . Let xl and xr be first and last points of x interval number, respectively. For x1 , x2 ∈ IR, we have x1 = x2 ⇔ x1l =x2l , x1r =x2r . x1 + x2 = {x ∈ R : x1l + x2l ≤ x ≤ x1r + x2r }, and if α ≥ 0, then αx = {x ∈ R : αx1l ≤ x ≤ αx1r } and if α < 0, then αx = {x ∈ R : αx1r ≤ x ≤ αx1l }, x1 . x2 = {x ∈ R : min {x1l x2l , x1l x2r , x1r x2l , x1r x2r} ≤ x ≤ max{x1l x2l , x1l x2r , x1r x2l , x1r x2r}} .


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Ayhan Esi

No. 4

The set of all interval numbers IR is a complete metric space defined by d (x1 , x2 ) = max {|x1l − x2l | , |x1r − x2r |} .[8] In the special case x1 = [a, a] and x2 = [b, b], we obtain usual metric of R. Let us define transformation f : N → R by k → f (k) = x, x = (xk ). Then x = (xk ) is called sequence of interval numbers. The xk is called k th term of sequence x = (xk ). wi denotes the set of all interval numbers with real terms and the algebraic properties of wi can be found in [7]. In the reference [1] definition of convergence of interval numbers is defined as follows: A sequence x = (xk ) of interval numbers is said to be convergent to the interval number xo if for each ε > 0 there exists a positive integer ko such that d (xk , xo ) < ε for all k ≥ ko and we denote it by limk xk = xo . Thus, limk xk = xo ⇔ limk xkl = xol and limk xkr = xor . Now we give new definitions for interval sequences as follows: ¡ ¢ An interval valued double sequence space 2 E is said to be solid if y = y k,l ∈ 2 E whenever ¯ ¯ ¯y k,l ¯ ≤ |xk,l | for all k, l ∈ N and x = (xk,l ) ∈ 2 E. An interval valued double sequence space 2 E is said to be monotone if 2 E contains the canonical pre-image of all its step spaces. ¡ ¢ An interval valued double sequence space 2 E is said to be convergence free if y = y k,l ∈ 2 E whenever x = (xk,l ) ∈ 2 E and xk,l = 0 implies y k,l = 0. An interval valued double sequence space 2 E is said to be symmetric if 2 S (x) ⊂ 2 E for all x = (xk,l ) ∈ 2 E, where 2 S (x) denotes the set of all permutations of the elements of x = (xk,l ). Throughout the paper, p = (pk,l ) is a double sequence of bounded strictly positive numbers. We define the following interval valued double sequence space:   ∞,∞   X £ ¡ ¢¤pk,l x = (xk,l ) : d xk,l , 0 <∞ 2 ` (p) =   k,l=1,1

and if pk,l = 1 for all k, l ∈ N, then we have   ∞,∞   X ¡ ¢ x = (xk,l ) : d xk,l , 0 < ∞ . 2` =   k,l=1,1

Lemma 1.1. If a double sequence space 2 E is solid, then it is monotone.

§2. Main results Theorem 2.1. The double sequence space 2 ` (p) is a complete metric space with respect to the metric ρ defined by  ρ (x, y) = 

∞,∞ X

k,l=1,1

 M1 £ ¡ ¢¤pk,l  , d xk,l , y k,l


Vol. 7

A new class of double interval numbers

25

¡ ¢ where M = max 1, supk,l pk,l . ¡ i¢ Proof. Let x be a Cauchy sequence in 2 ` (p). Then for a given ε > 0, there exists no ∈ N, such that ¡ ¢ ρ xi , xj < ε, for all i, j ≥ no . Then  

1 h ³ ´ipk,l M  < ε, for all i, j ≥ no d xik,l , y jk,l

∞,∞ X

k,l=1,1

h ³ ´ipk,l d xik,l , y jk,l < εM , for all i, j ≥ no

∞,∞ X k,l=1,1

³ ´ ⇒ d xik,l , y jk,l < ε, for all i, j ≥ no and all k, l ∈ N.

(1)

¡ ¢ ¡ ¢ This means that xik,l is a Cauchy sequence in R. Since R is a Banach space, xik,l is convergent. Now, let lim xik,l = xk,l for each k, l ∈ N and x = (xk,l ) .

i→∞

Taking limit as j → ∞ in (1), we have ¡ ¢ ρ xi , x < ε, for all i ≥ no . Now for all i ≥ no

¡ ¢ ¡ ¢ ¡ ¢ ρ x, 0 ≤ ρ x, xi + ρ xi , 0 < ∞.

Thus x = (xk,l ) ∈2 ` (p) and so 2 ` (p) is complete. This completes the proof. Theorem 2.2. The sequence space 2 ` (p) is solid as well as monotone. ¡ ¢ Proof. Let x = (xk,l ) ∈2 ` (p) and y = y k,l be a interval valued sequence such that ¯ ¯ ¯y k,l ¯ ≤ |xk,l | for all k, l ∈ N. Then ∞,∞ X

£ ¡ ¢¤p d xk,l , 0 k,l < ∞

k,l=1,1

and

∞,∞ X

∞,∞ X £ ¡ £ ¡ ¢¤pk,l ¢¤p d y k,l , 0 ≤ d xk,l , 0 k,l < ∞.

k,l=1,1

¡

k,l=1,1

¢

Thus y = y k,l ∈2 ` (p) and so 2 ` (p) is solid. Also by Lemma 1.1, it follows that the space 2 ` (p) is monotone. This completes the proof. Theorem 2.3. The double sequence space ` (p) is not convergence free in general. Proof. The result follows from the following example. Example 2.1. Let pk,l

  2, if k = l; =  1 , if k 6= l. kl


26

Ayhan Esi

No. 4

We consider the double interval sequence x = (xk,l ) as follows:  £  − 1 , 0¤ , if k = l; k2 xk,l = .  [0, 0] , if k = 6 l. Then

∞,∞ X

∞ X ¢¤p £ ¡ d xk,l , 0 k,l =

µ

k=1

k,l=1,1

1 k2

¶2 < ∞,

¡ ¢ so x = (xk,l ) ∈2 ` (p). Now let us consider the double interval sequence y = y k,l defined as follows:  £  −k 2 , k 2 ¤ , if k = l; . y k,l =  [0, 0] , if k 6= l. Then

∞,∞ X

∞,∞ X ¡ ¢2 ¢¤p £ ¡ d y k,l , 0 k,l = k 2 = ∞, k,l=1,1

k,l=1,1

¡

¢

so y = y k,l ∈ / 2 ` (p). Hence 2 ` (p) is not convergence free. This completes the proof. Theorem 2.4. The double sequence space 2 ` (p) is not symmetric. Proof. The result follows from the following example. Example 2.2. Let   2, if k = l; pk,l = .  1, if k 6= l. We consider the double interval sequence x = (xk,l ) as follows:  h i  − √1 , 0 , if k = l; 2k . xk,l =  [0, 0] , if k 6= l. Then

∞,∞ X

∞ X £ ¡ ¢¤p d xk,l , 0 k,l =

k,l=1,1

µ

k=1

1 √ 2k

¶2 < ∞,

so x = (xk,l ) ∈2 ` (p). Now let us consider the rearrangement the double interval sequence ¡ ¢ y = y k,l of x = (xk,l ) defined as follows: 

 x1,1

   x2,2 (yk,l ) =   x  3,3  . .. Then

∞,∞ X k,l=1,1

£ ¡ ¢¤p d y k,l , 0 k,l =

x1,2

x1,3

x2,1

x2,3

x3,2 .. .

x3,3 .. .

µ

¶2

1 √ 2k

+

···

  ···  . ···    .. . ∞ X 1 √ = ∞. 2k k=1


Vol. 7

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A new class of double interval numbers

¡ ¢ Hence y = y k,l ∈ / 2 ` (p) and so the double sequence space 2 ` (p) is not symmetric. This completes the proof. Theorem 2.5. (a) If 0 < pk,l ≤ qk,l < 1 for all k, l ∈ N, then 2 ` (p) ⊂2 ` (q) and the inclusion is proper. (b) If 0 < inf k,l pk,l ≤ pk,l for all k, l ∈ N, then 2 ` (p) ⊂2 ` and if 1 < pk,l ≤ supk,l pk,l < ∞ for all k, l ∈ N, then 2 ` ⊂2 ` (p). Proof. (a) Let x = (xk,l ) ∈2 ` (p). Then ∞,∞ X

¢¤p £ ¡ d xk,l , 0 k,l < ∞.

k,l=1,1

So there exists no ∈ N such that £ ¡ ¢¤p d xk,l , 0 k,l < 1 for all k, l ≥ no . Thus

£ ¡ ¢¤q £ ¡ ¢¤p d xk,l , 0 k,l < d xk,l , 0 k,l for all k, l ≥ no

and so,

∞,∞ X

£ ¡ ¢¤q d xk,l , 0 k,l < ∞.

k,l=1,1

Thus x = (xk,l ) ∈2 ` (q). The inclusion is strict and it follows from the following example. Example 2.3. We consider the double interval sequence x = (xk,l ) as follows:  h i  − √1 , 0 , if k = l; 3k xk,l =  [0, 0] , if k 6= l. and qk,l Then

   1, if k = l;  2 + 1 , if k = l; k ; pk = . =  2, if k 6= l.  3, if k = 6 l. ∞,∞ X

∞ X £ ¡ ¢¤q d xk,l , 0 k,l =

k,l=1,1

k=1

µ

1 √ 3k

¶2+ k1 <∞

and so x = (xk,l ) ∈2 ` (q), but ∞,∞ X

∞ X £ ¡ ¢¤p 1 √ = ∞, d xk,l , 0 k,l = 3k k,l=1,1 k=1

so x = (xk,l ) ∈ / 2 ` (p). This completes the proof. (b) The first part of the result follows from the inequality ∞,∞ X

∞,∞ X £ ¡ ¡ ¢ ¢¤p d xk,l , 0 ≤ d xk,l , 0 k,l

k,l=1,1

k,l=1,1

and the second part of the result follows from the inequality ∞,∞ X k,l=1,1

∞,∞ X ¡ ¢¤p ¢ £ ¡ d xk,l , 0 . d xk,l , 0 k,l ≤ k,l=1,1


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References [1] Kuo-Ping Chiao, Fundamental properties of interval vector max-norm, Tamsui Oxf. J. Math. Sci., 18(2002), No. 2, 219-233. [2] P. S. Dwyer, Linear Computation, New York, Wiley, 1951. [3] P. S. Dwyer, Errors of matrix computation, simultaneous equations and eigenvalues, National Bureu of Standards, Applied Mathematics Series, 29(1953), 49-58. [4] A. Esi, A new class of interval numbers, Journal of Qafqaz University, Mathematics and Computer Science, 31(2011), 98-102. [5] A. Esi, Strongly almost λ−convergence and statistically almost λ−convergence of interval numbers, Sci. Magna, 7(2011), No. 2, 117-122. [6] P. S. Fischer, Automatic propagated and round-off error analysis, paper presented at the 13th National Meeting of the Association of Computing Machinery, 6(1958). [7] S. Markov, Quasilinear spaces and their relation to vector spaces, Electronic Journal on Mathematics of Computation, 2(2005), No. 1, 1-21. [8] R. E. Moore and C. T. Yang, Theory of an interval algebra and its application to numeric analysis, RAAG Memories II, Gaukutsu Bunken Fukeyu-kai, Tokyo, 1958. [9] R. E. Moore, Automatic Error Analysis in Digital Computation, LSMD-48421, Lockheed Missiles and Space Company, 1959. [10] R. E. Moore and C. T. Yang, Interval Analysis I, LMSD-285875, Lockheed Missiles and Space Company, 1962. [11] M. S¸eng¨on¨ ul and A. Eryılmaz, On the sequence spaces of interval numbers, Thai J. Math., 8(2010), No. 3, 503-510.


Scientia Magna Vol. 7 (2011), No. 4, 29-34

Linear operators preserving commuting pairs of matrices over semirings 1 Miaomiao Ren† , Yizhi Chen‡ and Guanwei Qin] Department of Mathematics, Northwest University, Xi’an, Shaanxi, 710127, P. R. China E-mail: mralgebra@sohu.com yizhichen1980@126.com qinguanwei11@163.com Abstract In this paper we characterize linear operators ϕ on the matrices over the direct product of copies (need not be finite) of a binary Boolean algebra such that ϕ preserves commuting pairs of matrices. Keywords Linear operator, binary boolean algebra, commuting pair of matrices, direct pro -duct.

§1. Introduction and preliminaries A semiring means an algebra hS, +, ·, 0, 1i, where + and · are binary, 0 and 1 are nullary, satisfying the following conditions: (1) hS, +, 0i is a commutative monoid; (2) hS, ·, 1i is a monoid; (3) a · (b + c) = a · b + a · c and (a + b) · c = a · c + b · c, ∀a, b, c ² S; (4) a · 0 = 0 · a = 0, ∀a ² S; (5) 0 6= 1. Let S be a semiring and Mn (S) the set of all n × n matrices over S. I is the identity matrix, and O is the zero matrix. Define + and · on Mn (S) as follows: A + B = [aij + bij ]n×n , A · B = [

n P

aik bkj ]n×n .

k=1

It is easy to verify that hMn (S), +, ·, O, Ii is a semiring with the above operations. Let ϕ be an operator on Mn (S). Then we say that ϕ preserves commuting pairs of matrices if ϕ(A)ϕ(B) = ϕ(B)ϕ(A) whenever AB = BA. It is well known that commutativity of matrices is very important in the theory of matrices. Many authors have studied linear operators that preserve commuting pairs of matrices over fields and semirings. Song and Beasley [9] gave characterizations of linear operators that preserve commuting pairs of matrices over the nonnegative reals. Watkins [14] considered the same 1 This work is supported by a grant of the science foundation of Northwest University (NC0925) and a grant of the science foundation of Shaanxi Province (2011JQ1017).


30

Miaomiao Ren, Yizhi Chen and Guanwei Qin

No. 4

problem on matrices over the field of characteristic 0. Moreover, there are papers on linear operators that preserve commuting pairs of matrices over some other special fields (see [1, 2, 8]). In [10], Song and Kang characterized such linear operators over general Boolean algebras and chain semirings. Linear preserver problem (LP P for short) is one of the most active research areas in matrix theory. It concerns the classification of linear operators that preserve certain functions, relations, subsets, etc., invariant. Although the linear operators concerned are mostly linear operators on matrix spaces over fields or rings, the same problem has been extended to matrices over various semirings (see [3, 5, 6, 7, 9, 10, 13] and references therein). In the last decades, there are a series of literature on linear operators that preserve invariants of matrices over a given semiring. Idempotent preservers were investigated by Song, Kang and Beasley [11] , Dolˇzan and Oblak [3] and Orel [6] . Nilpotent preservers were discussed by Song, Kang and Jun [13] and Li and Tan [5] . Regularity preservers were studied by Song, Kang, Jun, Beasley and Sze in [4] and [12]. Pshenitsyna [7] considered invertibility preservers. Song and Kang [10] studied commuting pairs of matrices preservers. In this paper we study linear operators ϕ on the matrices over the direct product of copies (need not be finite) of a binary Boolean algebra such that ϕ preserves commuting pairs of matrices. For convenience, we use Z+ to denote the set of all positive integers. Hereafter, S will always denote an arbitrary semiring unless otherwise specified. Let A be a matrix in Mn (S). We denote entry of A in the ith row and jth column by aij and transpose of A by At . For any A ∈ Mn (S) and any λ ∈ S, define λA = [λaij ]n×n , Aλ = [aij λ]n×n . A mapping ϕ : Mn (S) → Mn (S) is called a linear operator (see [9]) if ϕ(aA + Bb) = aϕ(A) + ϕ(B)b for all a, b ∈ S and all A, B ∈ Mn (S). Given k ∈ Z+ . Let Bk be the power set of a k-element set Sk and σ1 , σ2 , · · · , σk the singleton subsets of Sk . We denote φ by 0 and Sk by 1. Define + and · on Mn (S) by A+B =A

[

B,

A·B =A

\

B.

Then hBk , +, ·, 0, 1i becomes a semiring and is called a general Boolean algebra (see [13]). In particular, if k = 1 then B1 is called the binary Boolean algebra (see [13]). A matrix A ∈ Mn (S) is said to be invertible (see [10]) if there exists B ∈ Mn (S) such that AB = BA = I. A matrix P ∈ Mn (S) is called a permutation matrix (see [3]) if it has exactly one entry 1 in each row and each column and 0’s elsewhere. If P ∈ Mn (S) is a permutation matrix, then P P t = P t P = I. Note that the only invertible matrices in Mn (B1 ) are permutation matrices (see [10]).


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Linear operators preserving commuting pairs of matrices over semirings

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§2. Main results Let (Sλ )λ∈∧ be a family of semirings and S = use aλ to denote a(λ). Define (a + b)λ = aλ + bλ ,

Q λ∈∧

(ab)λ = aλ bλ

Sλ . For any λ ∈ ∧ and any a ∈ S, we

(a, b ∈ S, λ ∈ ∧).

It is routine to check that hS, +, ·, 0, 1i is a semiring under the above operations. For any A = [aij ] ∈ Mn (S) and any λ ∈ ∧, Aλ : = [(aij )λ ] ∈ Mn (Sλ ). It is obvious that (A + B)λ = Aλ + Bλ ,

(AB)λ = Aλ Bλ and (aA)λ = aλ Aλ

for all A, B ∈ Mn (S) and all a ∈ S. Q Hereafter, S = λ∈∧ Sλ , where Sλ is a semiring for any λ ∈ ∧. In the following, we can easily obtain Lemma 2.1. Let A and B be matrices in Mn (S). Then the following statements hold: (i) A = B if and only if Aλ = Bλ for all λ ∈ ∧; (ii) AB = BA if and only if Aλ Bλ = Bλ Aλ for all λ ∈ ∧; (iii) A is invertible if and only if Aλ is invertible for all λ ∈ ∧. The following result is due to Orel [6] . Lemma 2.2. If ϕ : Mn (S) → Mn (S) is a linear operator, then for any λ ∈ ∧, there exists a unique linear operator ϕλ : Mn (Sλ ) → Mn (Sλ ) such that (ϕ(A))λ = ϕλ (Aλ ) for all A ∈ Mn (S). Now, let ϕ a linear operator on Mn (S). Suppose that ϕλ preserves commuting pairs of matrices for all λ ∈ ∧. For any A, B ∈ S, if AB = BA, then for any λ ∈ ∧, Aλ Bλ = Bλ Aλ . This implies that ϕλ (Aλ )ϕλ (Bλ ) = ϕλ (Bλ )ϕλ (Aλ ). It follows that (ϕ(A)ϕ(B))λ = (ϕ(A))λ (ϕ(B))λ = ϕλ (Aλ )ϕλ (Bλ ) = ϕλ (Bλ )ϕλ (Aλ ) = (ϕ(B))λ (ϕ(A))λ = (ϕ(B)ϕ(A))λ . Further, ϕ(A)ϕ(B) = ϕ(B)ϕ(A). Thus ϕ preserves commuting pairs of matrices. Conversely, assume that ϕ preserves commuting pairs of matrices. For any λ ∈ ∧ and A, B ∈ Mn (Sλ ), there exist X, Y ∈ Mn (S) such that Xλ = A, Yλ = B and Xµ = Yµ = O for any µ 6= λ. If AB = BA then XY = Y X. Since ϕ preserves commuting pairs of matrices, we have ϕ(X)ϕ(Y ) = ϕ(Y )ϕ(X). It follows that ϕλ (A)ϕλ (B) = (ϕ(X))λ (ϕ(Y ))λ = (ϕ(X)ϕ(Y ))λ = (ϕ(Y )ϕ(X))λ = (ϕ(Y ))λ (ϕ(X))λ = ϕλ (B)ϕλ (A). Hence ϕλ preserves commuting pairs of matrices. In fact, we have proved Lemma 2.3. Let ϕ : Mn (S) → Mn (S) be a linear operator. Then ϕ preserves commuting pairs of matrices if and only if ϕλ preserves commuting pairs of matrices for all λ ∈ ∧. Let ϕ be a linear operator on Mn (S). Suppose that ϕ is invertible. For any λ ∈ ∧ and any A, B ∈ Mn (Sλ ), there exist A, B ∈ Mn (S) such that (A)λ = A, (B)λ = B, and (A)µ = (B)µ = O for any µ 6= λ. If ϕλ (A) = ϕλ (B) then (ϕ(A))λ = ϕλ (A) = ϕλ (B) = (ϕ(B))λ .


32

Miaomiao Ren, Yizhi Chen and Guanwei Qin

No. 4

Also, (ϕ(A))µ = (ϕ(B))µ = ϕµ (O) = O for any µ 6= λ. This shows that ϕ(A) = ϕ(B). Since ϕ is injective, we have A = B. Further, A = (A)λ = (B)λ = B. Thus ϕλ is injective. On the other hand, since ϕ is surjective, it follows that there exists X ∈ Mn (S) such that ϕ(X) = B. We can deduce that B = (B)λ = (ϕ(X))λ = ϕλ (Xλ ). That is to say, ϕλ is surjective. Hence ϕλ is invertible. We have therefore established half of Lemma 2.4. Let ϕ be a linear operator on Mn (S). Then ϕ is invertible if and only if ϕλ is invertible for all λ ∈ ∧. Proof. We only need to prove the remaining half. Assume that ϕλ is invertible for any λ ∈ ∧. For any A, B ∈ Mn (S) and any λ ∈ ∧, if ϕ(A) = ϕ(B) then ϕλ (Aλ ) = (ϕ(A))λ = (ϕ(B))λ = ϕλ (Bλ ). Since ϕλ is injective, we have Aλ = Bλ . By Lemma 2.1(i) it follows that A = B. Hence ϕ is injective. Since ϕλ is surjective, there exists X (λ) ∈ Mn (Sλ ) such that ϕλ (X (λ) ) = Bλ . Let X ∈ Mn (S) satisfy Xλ = X (λ) for any λ ∈ ∧. It is clear that ϕ(X) = B, and so ϕ is surjective. Thus ϕ is invertible as required. The following lemma, due to Song and Kang [10] , characterize invertible linear operators preserveing commuting pairs of matrices over a binary Boolean algebra. Lemma 2.5. Let ϕ be a linear operator on Mn (B1 ). Then ϕ is an invertible linear operator that preserves commuting pairs of matrices if and only if there exists a permutation matrix P ∈ Mn (B1 ) such that either (a) ϕ(X) = P XP t for all X ∈ Mn (B1 ), or (b) ϕ(X) = P X t P t for all X ∈ Mn (B1 ). Next, we have Q Theorem 2.1. Let S = λ∈∧ Sλ , where Sλ = B1 for any λ ∈ ∧. Let ϕ : Mn (S) → Mn (S) be a linear operator. Then ϕ is an invertible linear operator that preserves commuting pairs of matrices if and only if there exist invertible matrix U ∈ Mn (S) and f1 , f2 ∈ S such that ϕ(X) = U (f1 X + f2 X t )U t for all X ∈ Mn (S), where (f1 )λ 6= (f2 )λ for any λ ∈ ∧. Proof. (=⇒) It follows from Lemma 2.3 and Lemma 2.4 that ϕλ is an invertible linear operator which preserves commuting pairs of matrices for any λ ∈ ∧. By Lemma 2.5, there exists U ∈ Mn (S) such that either ϕλ (X) = Uλ XUλt (1) for all X ∈ Mn (Sλ ), or ϕλ (X) = Uλ X t Uλt

(2)


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Linear operators preserving commuting pairs of matrices over semirings

33

for all X ∈ Mn (Sλ ). Moreover, Uλ is a permutation matrix for any λ ∈ ∧. We have by Lemma 2.1 (iii) that U is invertible. Let ∧i : = {λ ∈ ∧| ϕλ is the form of (i)}, i = 1, 2. It is evident T S that ∧1 ∧2 = φ, ∧1 ∧2 = ∧. For i = 1, 2, let fi ∈ S satisfy (fi )λ = 1 if λ ∈ ∧i and 0 otherwise. We conclude that ϕ(X) = U (f1 X + f2 X t )U t for all X ∈ Mn (S) as required. (⇐=) For any λ ∈ ∧ and any X ∈ Mn (Sλ ), there exists Y ∈ Mn (S) such that X = Yλ . We have ϕλ (X) = ϕλ (Yλ ) = (ϕ(Y ))λ = (U (f1 Y + f2 Y t )U t )λ . If (f1 )λ = 1, (f2 )λ = 0, then ϕλ (X) = Uλ XUλt for all X ∈ Mn (Sλ ). Otherwise, ϕλ (X) = Uλ Xλt Uλt for all X ∈ Mn (Sλ ). We have by Lemma 2.1 (iii) that Uλ is invertible. It follows from Theorem 2.1 that ϕλ is an invertible linear operator that preserves commuting pairs of matrices. Therefore, ϕ is an invertible linear operator that preserves commuting pairs of matrices by Lemma 2.3 and Lemma 2.4. Song and Kang [10] characterize invertible linear operators which preserve commuting pairs of matrices over general Boolean algebra. Recall that a general Boolean algebra is isomorphic to a direct product of binary Boolean algebras. Up to isomorphism, we obtain characterization of invertible linear operators which preserve commuting pairs of matrices over general Boolean algebra. Example 2.1. Let S = B1 × B1 × B1 . Take   (0, 0, 1) (1, 0, 0) (0, 1, 0)    U = (0, 1, 0) (0, 0, 1) (1, 0, 0) (1, 0, 0) (0, 1, 0) (0, 0, 1) in M3 (S) and f1 = (0, 1, 0), f2 = (1, 0, 1) in S. Define an operator ϕ on M3 (S) by ϕ(X) = U (f1 X + f2 X t )U t for all X ∈ M3 (S). It is obvious that Uλ (λ = 1, 2, 3) are all permutation matrices. By Theorem 2.1, ϕ is an invertible linear operator which preserves commuting pairs of matrices. Q Example 2.2. Let S = k∈Z+ Sk , where Sk = B1 for any k ∈ Z+ . Take a, b ∈ S, where a2k−1 = 1, a2k = 0, b2k−1 = 0 and b2k = 1 for any k ∈ Z+ . Let 

b

 U = a 0

a

0

0

 b 

b

a

be a matrix in M3 (S). Define an operator ϕ on M3 (S) by ϕ(X) = U (aX + bX t )U t for all X ∈ M3 (S). We have by Theorem 2.1 that ϕ is an invertible linear operator which preserves commuting pairs of matrices.


34

Miaomiao Ren, Yizhi Chen and Guanwei Qin

No. 4

References [1] L. B. Beasley, Linear transformations on matrices: the invariance of commuting pairs of matrices, 6(1978/79), No. 3, 179-183. [2] M. D. Choi, A. A. Jafarian and H. Radjavi, Linear maps preserving commutativity, Linear Algebra Appl., 87(1976), 227-241. [3] D. Dolˇzan and P. Oblak, Idempotent matrices over antirings, Linear Algebra Appl., 431(2009), No. 5-7, 823-832. [4] K. T. Kang, S. Z. Song and Y. B. Jun, Linear operators that strongly preserve regularity of fuzzy matrices, Math. Commun., 15(2010), No. 1, 243-254. [5] H. H. Li and Y. J. Tan, Linear operators that strongly preserves nilpotent matrices over antinegative semirings, Northeast. Math. J., 23(2007), No. 1, 71-86. [6] M. Orel, Nonbijective idempotents preservers over semirings, J. Korean Math. Soc., 47(2010), No. 4, 805-818. [7] O. A. Pshenitsyna, Maps preserving invertibility of matrices over semirings, Russ. Math. Surv., 64(2009), No. 1, 162-164. [8] H. Radjavi, Commtativity-preserving operators on symmetric matrices, Linear Algebra Appl., 61(1984), 219-224. [9] S. Z. Song and L. B. Beasley, Linear operators that preserve commuting pairs of nonnegative real matrices, Linear Multilinear Algebra, 51(2003), No. 3, 279-283. [10] S. Z. Song and K. T. Kang, Linear maps that preserve commuting pairs of matrices over general Boolean algebra, J. Korean Math. Soc., 43(2006), No. 1, 77-86. [11] S. Z. Song, K. T. Kang and L. B. Beasley, Idempotent matrix preservers over Boolean algebras, J. Korean Math. Soc., 44(2007), No. 1, 169-178. [12] S. Z. Song, K. T. Kang, L. B. Beasley and N. S. Sze, Regular matrices and their strong preservers over semirings, Linear Algebra Appl., 429(2008), 209-223. [13] S. Z. Song, K. T. Kang and Y. B. Jun, Linear preservers of Boolean nilpotent matrices, J. Korean Math. Soc., 43(2006), No. 3, 539-552. [14] W. Watkins, Linear maps that preserve commuting pairs of matrices, Linear Algebra Appl., 14(1976), No. 1, 29-35.


Scientia Magna Vol. 7 (2011), No. 4, 35-41

Conditions for a subclass of analytic functions Sukhwinder Singh Billing Department of Applied Sciences, Baba Banda Singh Bahadur Engineering College, Fatehgarh Sahib, 140407, Punjab, India E-mail: ssbilling@gmail.com Abstract This paper is an application of a lemma due to Miller and Mocanu we find certain sufficient conditions in terms of the differential operator ¶ µ zf 00 (z) zf 0 (z) + (µ + 1) 1 − f 0 (z) f (z)

[1]

, using which

for f ∈ A to belong to the class U (λ, µ, q(z)) where ( ) µ ¶µ+1 f (z) z U (λ, µ, q(z)) = f ∈ H : 6= 0 and f 0 (z) ≺ q(z), z ∈ E , z f (z) and q, q(z) 6= 0 is univalent in E and µ a complex number. As special cases of our main result, we find certain significant results regarding starlikeness and strongly starlikeness which extend some known results. Keywords Analytic function, differential subordination, starlike function, strongly starlike function.

§1. Introduction and preliminaries Let H be the class of functions analytic in the open unit disk E = {z : |z| < 1}. Let A be the class of all functions f which are analytic in E and normalized by the conditions that f (0) = f 0 (0) − 1 = 0. Thus, f ∈ A, has the Taylor series expansion f (z) = z +

∞ X

ak z k .

k=2

Let S denote the class of all analytic univalent functions f defined in E and normalized by the conditions f (0) = f 0 (0) − 1 = 0. A function f ∈ A is said to be starlike of order α (0 ≤ α < 1) in E if and only if µ 0 ¶ zf (z) < > α, z ∈ E. f (z) A function f ∈ A is said to be strongly starlike of order α, 0 < α ≤ 1, if ¯ ¯ 0 ¯ ¯ ¯arg zf (z) ¯ < απ , z ∈ E, ¯ f (z) ¯ 2


36 equivalently

Sukhwinder Singh Billing

zf 0 (z) ≺ f (z)

µ

1+z 1−z

No. 4

¶α , z ∈ E.

For two analytic functions f and g in the unit disk E, we say that f is subordinate to g in E and write as f ≺ g if there exists a Schwarz function w analytic in E with w(0) = 0 and |w(z)| < 1, z ∈ E such that f (z) = g(w(z)), z ∈ E. In case the function g is univalent, the above subordination is equivalent to: f (0) = g(0) and f (E) ⊂ g(E). Let φ : C2 × E → C and let h be univalent in E. If p is analytic in E and satisfies the differential subordination φ(p(z), zp0 (z); z) ≺ h(z), φ(p(0), 0; 0) = h(0),

(1)

then p is called a solution of the first order differential subordination (1). The univalent function q is called a dominant of the differential subordination (1) if p(0) = q(0) and p ≺ q for all p satisfying (1). A dominant q˜ that satisfies q˜ ≺ q for all dominants q of (1), is said to be the best dominant of (1). Let ( ) µ ¶µ+1 z f (z) 6= 0 and f 0 (z) U (λ, µ, q(z)) = f ∈ H : ≺ q(z), z ∈ E , z f (z) and q, q(z) 6= 0 is univalent in E and µ a complex number. Throughout this paper, value of the complex power taken is the principal one. Fournier and Ponnusamy [2] studied the class ¯ ¯ ( ) µ ¶µ+1 ¯ ¯ f (z) z ¯ 0 ¯ U (λ, µ) = f ∈ H : 6= 0 and ¯f (z) − 1¯ < λ, z ∈ E , ¯ ¯ z f (z) where 0 < λ ≤ 1 and µ is a complex number and estimated the range of parameters λ and µ such that the functions in the class U (λ, µ) are starlike or spirallike. Note that U (λ, µ) = U (λ, µ, 1 + λz) for 0 < λ ≤ 1. Obradovi˘c et al. [3] proved: Theorem 1.1. If f ∈ A satisfies the inequality ¯ ¯ 00 0 ¯ ¯ ¯1 + zf (z) − zf (z) ¯ < 1, z ∈ E, ¯ 0 f (z) f (z) ¯ then f is starlike. Irmak and S¸an [4] proved the following result. Theorem 1.2. If f ∈ A satisfies the inequality ¯ ¯ 00 0 ¯ ¯ ¯1 + zf (z) − zf (z) ¯ < β, z ∈ E, 0 < β ≤ 1, ¯ 0 f (z) f (z) ¯ then f is strongly starlike function of order β. In the present paper, we study the differential operator µ ¶ zf 00 (z) zf 0 (z) + (µ + 1) 1 − f 0 (z) f (z)


Vol. 7

Conditions for a subclass of analytic functions

37

and write the sufficient conditions in terms of this operator for f ∈ A to be a member of the class U (λ, µ, q(z)) and consequently of U (λ, µ). In particular, we also derive some sufficient zf 00 (z) zf 0 (z) conditions in terms of the differential operator 1 + 0 − which extend the above f (z) f (z) [3] [4] results of Obradovi˘c et al. and Irmak and S¸an for f ∈ A to be starlike and strongly starlike. To prove our main result, we shall use the following lemma of Miller and Mocanu [1] (page 76). zq 0 (z) Lemma 1.1. Let q, q(z) 6= 0 be univalent in E such that is starlike in E. If an q(z) analytic function p, p(z) 6= 0 in E, satisfies the differential subordination zq 0 (z) zp0 (z) ≺ = h(z), p(z) q(z) then

·Z

z

p(z) ≺ q(z) = exp 0

h(t) t

¸

and q is the best dominant.

§2. Main result and applications zq 0 (z) Theorem 2.1. Let q, q(z) 6= 0 be univalent in E such that (= h(z)) is starlike in q(z) µ ¶µ+1 z E. If f ∈ A, f 0 (z) 6= 0 for all z in E, satisfies the differential subordination f (z) µ ¶ zf 0 (z) zf 00 (z) + (µ + 1) 1 − ≺ h(z), z ∈ E, f 0 (z) f (z) then

µ f 0 (z)

z f (z)

¶µ+1

·Z ≺ q(z) = exp 0

z

¸ h(t) , t

i.e., f ∈ U (λ, µ, q(z)) and q is the best dominant. Here µ is a complex number. µ ¶µ+1 z Proof. By setting p(z) = f 0 (z) in Lemma 1.1, proof follows. f (z) 1 + (1 − 2α)z Remark 2.1. Consider the dominant q(z) = , 0 ≤ α < 1, z ∈ E in above 1−z theorem, we have ¶ µ ¶ µ 1 (1 − 2α)z zq 00 (z) zq 0 (z) − =< 1+ − > 0, z ∈ E < 1+ 0 q (z) q(z) 1−z 1 + (1 − 2α)z zq 0 (z) is starlike in E and we immediately get the following result. q(z) µ ¶µ+1 z 0 Theorem 2.2. For a complex number µ, if f ∈ A, f (z) 6= 0 for all z in E, f (z) satisfies the differential subordination µ ¶ zf 00 (z) zf 0 (z) 2(1 − α)z + (µ + 1) 1 − ≺ , z ∈ E, f 0 (z) f (z) (1 − z)(1 + (1 − 2α)z)

for all 0 ≤ α < 1. Therefore,


38

Sukhwinder Singh Billing

then

µ 0

f (z)

z f (z)

¶µ+1 ≺

No. 4

1 + (1 − 2α)z , 0 ≤ α < 1, z ∈ E. 1−z

Taking µ = 0 in above theorem, we obtain the following result of Billing [5] . zf 0 (z) Corollary 2.1. If f ∈ A, 6= 0 for all z in E, satisfies the condition f (z) 1+ then

zf 00 (z) zf 0 (z) 2(1 − α)z − ≺ , z ∈ E, f 0 (z) f (z) (1 − z)(1 + (1 − 2α)z) zf 0 (z) 1 + (1 − 2α)z ≺ , 0 ≤ α < 1, z ∈ E, f (z) 1−z

i.e., f is starlike of order α. Remark 2.2. Setting α = 0 in the above corollary, we obtain: Suppose f ∈ A, for all z in E, satisfies 1+

2z zf 00 (z) zf 0 (z) − ≺ = F (z), f 0 (z) f (z) 1 − z2

zf 0 (z) 6= 0 f (z) (2)

then f is starlike, where F (E) = C \ {w ∈ C : <(w) = 0, |=(w)| ≥ 1}. zf 00 (z) zf 0 (z) − f 0 (z) f (z) largely over the result of Obradovi˘c et al. [3] stated in Theorem 1.1. When the above said operator takes the values in the unit disk, then f ∈ A is starlike by Theorem 1.1. But in view of the result in (2), the same operator can take values in the complex plane C except two slits <(w) = 0, |=(w)| ≥ 1. The dark portion of the Figure 2.1 is the region of variability of zf 00 (z) zf 0 (z) the differential operator 1 + 0 − in view of Theorem 1.1 whereas the region of f (z) f (z) variability is extended to the total shaded region (dark + light) in the light of the result in (2). This result extends the region of variability of the differential operator 1 +

Figure 2.1


Vol. 7

39

Conditions for a subclass of analytic functions

Remark 2.3. Consider the dominant q(z) = 1 + λz, 0 < λ ≤ 1, z ∈ E in Theorem 2.1, we have µ ¶ µ ¶ zq 00 (z) zq 0 (z) 1 < 1+ 0 − =< > 0, z ∈ E q (z) q(z) 1 + λz zq 0 (z) is starlike in E and we have the following result. q(z) µ ¶µ+1 z Theorem 2.3. Suppose f ∈ A, f 0 (z) 6= 0 for all z in E, satisfies f (z) µ ¶ zf 0 (z) λz zf 00 (z) + (µ + 1) 1 − ≺ , z ∈ E, 0 f (z) f (z) 1 + λz

for all 0 < λ ≤ 1. Therefore,

where µ is a complex number, then ¯ ¯ ¶µ+1 µ ¯ ¯ z ¯ ¯ 0 − 1¯ < λ, 0 < λ ≤ 1, z ∈ E, ¯f (z) ¯ ¯ f (z) i.e., f ∈ U (λ, µ). Selecting µ = 0 in above theorem, we obtain: zf 0 (z) Corollary 2.2. If f ∈ A, 6= 0 for all z in E, satisfies the condition f (z) 1+ then

zf 00 (z) zf 0 (z) λz − ≺ , z ∈ E, f 0 (z) f (z) 1 + λz

¯ 0 ¯ ¯ zf (z) ¯ ¯ ¯ ¯ f (z) − 1¯ < λ, 0 < λ ≤ 1, z ∈ E. Remark 2.4. Let the dominant in Theorem 2.1 be q(z) =

α(1 − z) , α > 1, z ∈ E. A α−z

little calculation yields µ ¶ µ ¶ zq 00 (z) zq 0 (z) 1 z < 1+ 0 − =< + > 0, z ∈ E. q (z) q(z) 1−z α−z Therefore,

zq 0 (z) is starlike in E and we obtain the following result. q(z)

Theorem 2.4. Let α > 1 be a real number and let f ∈ A, f 0 (z)

µ

z f (z)

in E, satisfy the differential subordination µ ¶ zf 00 (z) zf 0 (z) (1 − α)z + (µ + 1) 1 − ≺ , z ∈ E, 0 f (z) f (z) (1 − z)(α − z) then

µ 0

f (z)

z f (z)

¶µ+1 ≺

α(1 − z) , z ∈ E, α−z

where µ is a complex number. Selecting µ = 0 in above theorem, we obtain:

¶µ+1 6= 0 for all z


40

Sukhwinder Singh Billing

Corollary 2.3. If f ∈ A, 1+

No. 4

zf 0 (z) 6= 0 for all z in E, satisfies f (z)

zf 00 (z) zf 0 (z) (1 − α)z − ≺ , z ∈ E, 0 f (z) f (z) (1 − z)(α − z)

then

zf 0 (z) α(1 − z) ≺ , α > 1, z ∈ E. f (z) α−z ¶δ µ 1+z , 0 < δ ≤ 1, z ∈ E in Theorem Remark 2.5. Selecting the dominant q(z) = 1−z 2.1, we have µ ¶ µ ¶ zq 00 (z) zq 0 (z) 1 + z2 < 1+ 0 − =< > 0, z ∈ E. q (z) q(z) 1 − z2

zq 0 (z) is starlike in E and we obtain the following result. q(z) µ ¶µ+1 z 0 Theorem 2.5. Let f ∈ A, f (z) 6= 0 for all z in E, satisfy the differential f (z) subordination µ ¶ zf 0 (z) 2δz zf 00 (z) + (µ + 1) 1 − ≺ , z ∈ E, 0 f (z) f (z) 1 − z2 Therefore,

then

µ f 0 (z)

z f (z)

¶µ+1

µ ≺

1+z 1−z

¶δ , 0 < δ ≤ 1, z ∈ E.

Taking µ = 0 in above theorem, we get: zf 0 (z) Corollary 2.4. If f ∈ A, 6= 0 for all z in E, satisfies f (z) 1+ then

2δz zf 00 (z) zf 0 (z) − ≺ , z ∈ E, f 0 (z) f (z) 1 − z2

zf 0 (z) ≺ f (z)

µ

1+z 1−z

¶δ , 0 < δ ≤ 1, z ∈ E,

i.e., f is strongly starlike of order δ. Remark 2.6. We, here, make the comparison of the result in above corollary with the result in Theorem 1.2. We notice that the region of variability of the differential operator zf 00 (z) zf 0 (z) 1+ 0 − is extended in Corollary 2.4 over the result in Theorem 1.2. To justify our f (z) f (z) claim, we consider the following particular case of both the results. For δ = 1/2 in Corollary zf 0 (z) 2.4, we obtain: Suppose f ∈ A, 6= 0 for all z in E, satisfies f (z) 1+

z zf 00 (z) zf 0 (z) = G(z), − ≺ f 0 (z) f (z) 1 − z2

then f is strongly starlike of order 1/2 where G(E) = C \ {w : <(w) = 0, |=(w)| ≥ 1/2}. For β = 1/2 in Theorem 1.2, we get: If f ∈ A satisfies the inequality ¯ ¯ 00 0 ¯ ¯ ¯1 + zf (z) − zf (z) ¯ < 1 , z ∈ E, ¯ 0 f (z) f (z) ¯ 2

(3)

(4)


Vol. 7

Conditions for a subclass of analytic functions

41

then f is strongly starlike of order 1/2.

zf 00 (z) zf 0 (z) − takes values in the f 0 (z) f (z) disk of radius 1/2 with center at origin whereas by (3), the same operator can take values in the complex plane C except two slits <(w) = 0, |=(w)| ≥ 1/2 for the same conclusion i.e. f is strongly starlike of order 1/2. We also justify our claim pictorially in Figure 2.2. The dark shaded portion of the figure shows the region of variability of the above said operator in view of the result in (4) and in the light of the result in (3), the region of variability is the total shaded region (dark + light). We see that in view of (4) the differential operator 1 +

Figure 2.2

References [1] S. S. Miller and P. T. Mocanu, Differential Subordinations, Theory and Applications, Marcel Dekker, New York and Basel, 2000, No. 225. [2] R. Fournier and S. Ponnusamy, A class of locally univalent functions defined by a differential inequality, Complex Variables and Elliptic Equations, 52(2007), No. 1, 1-8. [3] M. Obradovi˘c, S. Ponnusamy, V. Singh and P. Vasundhra, A class of locally univalent functions defined by a differential inequality, Complex Variables and Elliptic Equations, 52(2007), No. 1, 1-8. [4] H. Irmak and M. S¸an, Some relations betwwen certain inequalities concerning analytic and univalent functions, Applied Mathematics Letters, 23(2010), 897-901. [5] S. S. Billing, Differential sandwich-type results and criteria for starlikeness, Rend. Sem. Mat. Univ. Politec, Torino, 69(2011), No. 1, 57-71.


Scientia Magna Vol. 7 (2011), No. 4, 42-48

On ideal convergence in topological groups Bipan Hazarika Department of Mathematics, Rajiv Gandhi University Rono Hills, Doimukh, 791112, Arunachal Pradesh, India E-mail: bh rgu@yahoo.co.in Abstract An ideal I is a family of subsets of positive integers N which is closed under taking finite unions and subsets of its elements. In [9], Kostyrko et. al introduced the concept of ideal convergence as a sequence (xk ) of real numbers is said to be I-convergent to a real number x0 , if for each ε > 0 the set {k ∈ N : |xk − x0 | ≥ ε} belongs to I. In this article we introduced I-convergence of sequences in topological groups and extensions of a decomposition theorem and a completeness theorem to the topological group setting are proved. Keywords Ideal, I-convergence, I-cauchy, topological group. 2010 Mathematics Subject Classifications: 40A05, 40G15, 40J05, 22A05.

§1. Introduction The concept of ideal convergence as a generalization of statistical convergence, and any concept involving statistical convergence play a vital role not only in pure mathematics but also in other branches of science involving mathematics, especially in information theory, computer science, biological science, dynamical systems, geographic information systems, population modelling, and motion planning in robotics. The notion of statistical convergence is a very useful functional tool for studying the convergence problems of numerical sequences/matrices (double sequences) through the concept of density. It was first introduced by Fast [7] , and Schoenberg [13] , independently for the real sequences. Later on it was further investigated from sequence point of view and linked with the summability theory by Fridy [8] and many others. The idea is based on the notion of natural density of subsets of N, the set of positive integers, which is defined as follows: The natural density of a subset of N is denoted by δ(E) and is defined by δ(E) = lim |{k ∈ E : k ≤ n}|, n→∞

where the vertical bar denotes the cardinality of the respective set. In [5], C ¸ akalli introduced this notion in topological Hausdroff groups. The notion of I-convergence was initially introduced by Kostyrko, et. al [9] as a generalization of statistical convergence which is based on the structure of the ideal I of subset of natural numbers N. Later on it was further investigated from sequence space point of view and linked ˘ at, et. al [11−12] , Tripathy and Hazarika [14−17] and many other with summability theory by Sal´ authors.


Vol. 7

On ideal convergence in topological groups

43

A non-empty family of sets I ⊆ P (N) (power set of N) is called an ideal in N if and only if (i) for each A, B ∈ I, we have A ∪ B ∈ I; (ii) for each A ∈ I and B ⊂ A, we have B ∈ I. A family F ⊆ P (N) is called a filter on N if and only if (i) φ ∈ / F; (ii) for each A, B ∈ F, we have A ∩ B ∈ F ; (iii) for each A ∈ F and B ⊃ A, we have B ∈ F. An ideal I is called non-trivial if I 6= φ and N ∈ / I. It is clear that I ⊆ P (N) is a non-trivial ideal if and only if the class F = F (I) = N − A : A ∈ I is a filter on N. The filter F (I) is called the filter associated with the ideal I. A non-trivial ideal I ⊆ P (N) is called an admissible ideal in N if it contains all singletons, i.e., if it contains {{x} : x ∈ N}. Recall that a sequence x = (xk ) of points in R is said to be I-convergent to a real number x0 if {k ∈ N : |xk −x0 | ≥ ε} ∈ I for every ε > 0 (see [9]). In this case we write I −lim xk = x0 . Let (xk ) and (yk ) be two real sequences, then we say that xk = yk for almost all k related to I (a. a. k. r. I) if the set {k ∈ N : xk 6= yk } belongs to I. Throughout the article we consider I to be a non-trivial admissible ideal of N. The purpose of this article is to give certain characterizations of I-convergent sequences in topological groups and to obtain extensions of a decomposition theorem and a completeness theorem to topological groups.

§2. I-convergence in topological groups Throughout the article X will denotes the topological Hausdroff group, written additively, which satisfies the first axiom of countability. Definition 2.1. A sequence (xk ) of points in X is said to be I-convergent to an element x0 of X if for each neighbourhood V of 0 such that the set {k ∈ N : xk − x0 ∈ / V}∈I and it is denoted by I − limk→∞ xk = x0 . Definition 2.2. A sequence (xk ) of points in X is said to be I-Cauchy in X if for each neighbourhood V of 0, there is an integer n(V ) such that the set {k ∈ N : xk − xn(V ) ∈ / V } ∈ I. Throughout the article s(X), cI (X), cI0 (X) and C I (X) denote the set of all X-valued sequences, X-valued I-convergent sequences, X-valued I-null sequences and X-valued I-Cauchy sequences in X, respectively. Theorem 2.1. A sequence (xk ) is I-convergent if and only if for each neighbourhood V of 0 there exists a subsequence (xk0 (r) ) of (xk ) such that limr→∞ xk0 (r) = x0 and {k ∈ N : xk − xk0 (r) ∈ / V } ∈ I.


44

Bipan Hazarika

No. 4

Proof. Let x = (xk ) be a sequence in X such that I − limk→∞ xk = x0 . Let {Vn } be a sequence of nested base of neighbourhoods of 0. We write E (i) = {k ∈ N : xk −x0 ∈ / Vi } for any (i+1) (i) (i) positive integer i. Then for each i, we have E ⊂ E and E ∈ F (I). Choose n(1) such that k > n(1), then E (i) 6= φ. Then for each positive integer r such that n(p + 1) ≤ r < n(2), choose k 0 (r) ∈ E (p) i.e. xk0 (r) −x0 ∈ V1 , In general, choose n(p+1) > n(p) such that r > n(p+1), then E (p+1) 6= φ. Then for all r satisfying n(p) ≤ r < n(p + 1), choose k 0 (r) ∈ E (p) i.e. xk0 (r) − x0 ∈ Vp . Also for every neighbourhood V of 0, there is a symmetric neighbourhood W of 0 such that W ∪ W ⊂ V . Then we get {k ∈ N : xk − xk0 (r) ∈ / V } ⊂ {k ∈ N : xk − x0 ∈ / W } ∪ {r ∈ N : xk0 (r) − x0 ∈ / W }. Since I − limk→∞ xk = x0 , therefore there is a neighbourhood W of 0 such that {k ∈ N : xk − x0 ∈ / W} ∈ I and limr→∞ xk0 (r) = x0 implies that {r ∈ N : xk0 (r) − x0 ∈ / W } ∈ I. Thus we have {k ∈ N : xk − xk0 (r) ∈ / V } ∈ I. Next suppose for each neighbourhood V of 0 there exists a subsequence (xk0 (r) ) of (xk ) such that limr→∞ xk0 (r) = x0 and {k ∈ N : xk − xk0 (r) ∈ / V } ∈ I. Since V is a neighbourhood of 0, we may choose a symmetric neighbourhood W of 0 such that W ∪ W ⊂ V . Then we have {k ∈ N : xk − x0 ∈ / V } ⊂ {k ∈ N : xk − xk0 (r) ∈ / W } ∪ {r ∈ N : xk0 (r) − x0 ∈ / W }. Since both the sets on the right hand side of the above relation belong to I. Therefore {k ∈ N : xk − x0 ∈ / V } ∈ I. This completes the proof of the theorem. Theorem 2.2. If limk→∞ xk = x0 and I − limk→∞ yk = 0, then I − limk→∞ (xk + yk ) = limk→∞ xk . Proof. Let V be any neighbourhood of 0. Then we may choose a symmetric neighbourhood W of 0 such that W ∪ W ⊂ V . Since limk→∞ xk = x0 , then there exists an integer n0 such that k ≥ n0 implies that xk − x0 ∈ W . Hence {k ∈ N : xk − x0 ∈ / W } ∈ I. By assumption I − limk→∞ yk = 0, then we have {k ∈ N : yk ∈ / W } ∈ I. Thus {k ∈ N : (xk − x0 ) + yk ∈ / V } ⊂ {k ∈ N : xk − x0 ∈ / W } ∪ {k ∈ N : yk ∈ / W } ∈ I.


Vol. 7

On ideal convergence in topological groups

45

This implies that I − limk→∞ (xk + yk ) = limk→∞ xk . Theorem 2.3. If a sequence (xk ) is I-convergent to x0 , then there are sequences (yk ) and (zk ) such that I − limk→∞ yk = x0 and xk = yk + zk , for all k ∈ N and {k ∈ N : xk 6= yk } ∈ I and (zk ) is a I-null sequence. Proof. Let {Vi } be a nested base of neighbourhood of 0. Take n0 = 0 and choose an increasing sequence (ni ) of positive integer such that {k ∈ N : xk − x0 ∈ / Vi } ∈ I for k > n0 . Let us define the sequences (yk ) and (zk ) as follows: yk = xk

and zk = 0, if 0 < k ≤ n1

and suppose ni < ni+1 , for i ≥ 1, yk = xk

and zk = 0, if xk − x0 ∈ Vi ,

yk = x0 and zk = xk − x0 , if xk − x0 ∈ / Vi . We have to show that (i) I − limk→∞ yk = x0 , (ii) (zk ) is a I-null sequence. (i) Let V be any neighbourhood of 0. We may choose a positive integer i such that Vi ⊂ V. Then yk − x0 = xk − x0 ∈ Vi , for k > ni . If xk − x0 ∈ / Vi , then yk − x0 = x0 − x0 = 0 ∈ V . Hence I − limk→∞ yk = x0 . (ii) It is enough to show that {k ∈ N : zk 6= 0} ∈ I. For any neighbourhood V of 0, we have {k ∈ N : zk ∈ / V } ⊂ {k ∈ N : zk 6= 0}. If np < k ≤ np+1 , then {k ∈ N : zk 6= 0} ⊂ {k ∈ N : xk − x0 ∈ / Vp }. If p > i and np < k ≤ np+1 , then {k ∈ N : zk 6= 0} ⊂ {k ∈ N : xk − x0 ∈ / Vp } ⊂ {k ∈ N : xk − x0 ∈ / Vi }. This implies that {k ∈ N : zk 6= 0} ∈ I. Hence (zk ) is a I-null sequence.

§3. I-sequential compactness Definition 3.1. Let A ⊂ X and x0 ∈ X. Then x0 is in the I-sequential closure of A if there is a sequence (xk ) of points in A such that I − limk→∞ xk = x0 . I We denote I-sequential closure of a set A by A . We say that a set is I-sequentially closed if it contains all of the points in its I-sequential closure. By a method of sequential convergence, we mean an additive function B defined on a subgroup of s(X), denoted by cB (X) into X. Definition 3.2. A sequence x = (xk ) is said to be B-convergent to x0 if x ∈ cB (X) and B(x) = x0 .


46

Bipan Hazarika

No. 4

Definition 3.3. A method B is called regular if every convergent sequence x = (xk ) is B-convergent with B(x) = lim x. From Definition 3.3, it is clear that, if B = I, then I is a regular sequential method. Definition 3.4. A point x0 is called a I-sequential accumulation point of A (or is in the I-sequential derived set) if there is a sequence x = (xk ) of points in A − {x0 } such that I-lim x = x0 . Definition 3.5. A subset A of X is called I-sequentially countably compact if any infinite subset A has at least one I-sequentially accumulation point in A. Definition 3.6. A subset A of X is called I-sequentially compact if x = (xk ) is a sequence of points of A, there is a subsequence y = (ykn ) of x with I-lim y = x0 ∈ A. Definition 3.7. A function f is called I-sequentially continuous at x0 ∈ X provided that whenever a sequence x = (xk ) of points of X is I-convergent to x0 then the sequence f (x) = f ((xk )) is I-convergent to f (x0 ). For a subset A of X, f is I-sequentially continuous on A if it is I-sequentially continuous at every x0 ∈ A and is I-sequentially continuous if it is I-sequentially continuous on X. Lemma 3.1. Any I-convergent sequence of points in X with a I-limit x0 has a convergent subsequence with the same limit x0 in the ordinary sense. The proof of the lemma follows from [11] and [17]. From the Lemma 3.1, it is clear that I is a regular subsequential method. Theorem 3.2. Any I-sequentially closed subset of a I-sequentially compact subset of X is I-sequentially compact. Proof. Let A be a I-sequentially compact subset of X and E be a I-sequentially closed subset of A. Let x = (xk ) be a sequence of points in E. Then x is a sequence of points in A. Since A is I-sequentially compact, there exists a subsequence y = (ykn ) of the sequence (xk ) such that I − lim y ∈ A. The subsequence (ykn ) is also a sequence of points in E and E is I-sequentially closed, therefore I − lim y ∈ E. Thus x = (xk ) has a I-convergent subsequence with I − lim y ∈ E, so E is I-sequentially compact. Theorem 3.3. It Any I-sequentially compact subset of X is I-sequentially closed. I

Proof. Let A be any I-sequentially compact subset of X. For any x0 ∈ A , then there exists a sequence x = (xk ) be a sequence of points in A such that I − lim x = x0 . Since I is a subsequential method, there is a subsequence y = (yr ) = (xkr ) of the sequence x = (xk ) such that limr→∞ xkr = x0 . Since I is regular, so I − lim y = x0 . By I-sequentially compactness of A is, there is a subsequence z = (zr ) of y = (yr ) such that I − lim z = y0 ∈ A. Since limr→∞ zr = x0 and I is regular, so I − lim z = x0 . Thus x0 = y0 and hence x0 ∈ A. Hence A is I-sequentially closed. Corollary 3.4. Any I-sequentially compact subset of X is closed in the ordinary sense. Theorem 3.5. A subset of X is I-sequentially compact if and only if it is I-sequentially countably compact. Proof. Let A be any I-sequentially compact subset of X and E be an infinite subset of A. Let x = (xk ) be a sequence of different points of E. Since A is I-sequentially compact, this implies that the sequence x has a convergent subsequence y = (yr ) = (xkr ) with I − lim y = x0 . Since I is subsequential method, y has a convergent subsequence z = (zr ) of the subsequence y


Vol. 7

On ideal convergence in topological groups

47

with limr→∞ zr = x0 . By the regularity of I, we obtain that x0 is a I-sequentially accumulation point of E. Then A is I-sequentially countably compact. Next suppose A is any I-sequentially countably compact subset of X. Let x = (xk ) be a sequence of different points in A. Put G = {xk : k ∈ N}. If G is finite, then there is nothing to prove. If G is infinite, then G has a I-sequentially accumulation point in A. Also each set Gn = {xn : n ≥ k}, for each positive integer n, has a I-sequentially accumulation point in A. I I Therefore ∩∞ n=1 Gn 6= φ. So there is an element x0 ∈ A such that x0 ∈ Gn . Since I is a regular subsequential method, so x0 ∈ Gn . Then there exists a subsequence z = (zr ) = (xkr ) of the sequence x = (xk ) with I − lim z ∈ A. This completes the proof. Corollary 3.6. A subset of X is I-sequentially compact if and only if it is sequentially countably compact in the ordinary sense. Corollary 3.7. A subset of X is I-sequentially compact if and only if it is countably compact in the ordinary sense. Theorem 3.8. The I-sequential continuous image of any I-sequentially compact subset of X is I-sequentially compact. Proof. Let f be any I-sequentially continuous function on X and A be any I-sequentially compact subset of X. Let y = (yk ) = (f (xk )) be a sequence of points in f (A). Since A is I-sequentially compact, there exists a subsequence z = (zr ) = (xkr ) of the sequence x = (xk ) with I − lim zA. Then f (z) = (f (zr )) = (f (xkr )) is a subsequence of the sequence y. Since f is I-sequentially continuous, I − lim(f (zr )) = f (x) ∈ f (A). Then f (A) is I-sequentially compact. Corollary 3.9. A I-sequentially continuous image of any sequentially compact subset of X is sequentially compact. Theorem 3.10. If X is I-sequentially compact, then X is complete. Proof. Let x = (xk ) be a Cauchy sequence of points of X. As X is I-sequentially compact, there exists a convergent subsequence y = (ykr ) of the sequence x such that I − lim y = x0 ∈ A. By the Theorem 2.1, there exists a subsequence z = (zkr ) of the sequence y such that limr→∞ zkr = x0 . Hence (xk ) is converges. This completes proof of the theorem.

References ˘ at, On the A-continuity of real functions, Acta Math. Univ. [1] J. Antoni and T. Sal´ Comenian, 39(1980), 159-164. ˘ at, I-convergence and I-continuity [2] V. Balaz, J. Cervenansky, P. Kostrysko and T. Sal´ of real functions, Acta Math., 5(2002), 43-50. [3] J. Boos, Classical and Modern Methods in Summability, Oxford Univ. Press, 2000. [4] H. C ¸ akalli and B. Thorpe, On summability in topological groups and a theorem of D. L. Prullage, Ann. Soc. Math. Polon. Comm. Math. Ser I, 29(1990), 139-148. [5] H. C ¸ akalli, On statistical convergence in topological groups, Pure Appl. Math. Sci., 43(1996), No. 1-2, 27-31. [6] J. Connor and K. G. Grosse-Erdmann, Sequential definition of continuity for real functions, Rocky Mountains Jour., 33(2003), No. 1, 93-121. [7] H. Fast, Sur la convergence statistique, Colloq. Math., 2(1951), 241-244.


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[8] J. A. Fridy, On statistical convergence, Analysis, 5(1985), 301-313. ˘ at and W. Wilczy´ [9] P. Kostrysko, T. Sal´ nski, I-convergence, Real Anal. Exchange, 26(2000-2001), No. 2, 669-686. [10] D. L. Prullage, Summability in topological group, Math. Z., 96(1967), 259-279. ˘ at, B. C. Tripathy and M. Ziman, On some properties of I-convergence, Tatra [11] T. Sal´ Mt. Math. Publ., 28(2004), 279-286. ˘ at, B. C. Tripathy and M. Ziman, On I-convergence field, Italian Jour. Pure [12] T. Sal´ Appl. Math., 17(2005), 45-54. [13] I. J. Schoenberg, The integrability of certain functions and related summability methods, Amer. Math. Monthly, 66(1951), 361-375. [14] B. C. Tripathy and B. Hazarika, I-convergent sequence spaces associated with multiplier sequences, Math. Ineq. Appl., 11(2008), No. 3, 543-548. [15] B. C. Tripathy and B. Hazarika, Paranorm I-convergent sequence spaces, Math. Slovaca, 59(2009), No. 4, 485-494. [16] B. C. Tripathy and B. Hazarika, Some I-convergent sequence spaces defined by Orlicz function, Acta Mathematica Applicatae Sinica, 27(2011), No. 1, 149-154. [17] B. C. Tripathy and B. Hazarika, I-Monotonic and I-Convergent Sequences, Kyungpook Math. J., 51(2011), No. 2, 233-239.


Scientia Magna Vol. 7 (2011), No. 4, 49-81

A summation formula including recurrence relation Salahuddin P. D. M College of Engineering, Bahadurgarh, Haryana, India E-mail: sludn@yahoo.com vsludn@gmail.com Abstract The aim of the present paper is to establish a summation formula based on half argument using Gauss second summation theorem. Keywords Contiguous relation, gauss second summation theorem, recurrence relation. A. M. S. Subject Classification 2000: 33C60, 33C70.

§1. Introduction Generalized Gaussian Hypergeometric function of one variable is defined by   a1 , a2 , · · · , aA ; ∞  X  (a1 )k (a2 )k · · · (aA )k z k   = F , z A B  (b1 )k (b2 )k · · · (bB )k k! k=0 b1 , b2 , · · · , bB ; or

 A FB

  

(aA ) ; (bB )

;

   z   ≡ A FB 

(aj )A j=1 (bj )B j=1

; ;

 ∞  X ((aA ))k z k = . z   ((bB ))k k!

(1)

k=0

where the parameters b1 , b2 , · · · , bB are neither zero nor negative integers and A, B are non-negative integers. Contiguous Relation is defined by [ Andrews p.363(9.16), E.D.p.51(10), H.T.F.I p.103(32)]       a, b ; a + 1, b ; a, b + 1 ; (a − b) 2 F1  (2) z  = a 2 F1  z  − b 2 F1  z . c ; c ; c; Gauss second summation theorem is defined by [Prud., 491(7.3.7.5)]   a, b ; Γ( a+b+1 ) Γ( 12 ) 1 2  =  2 F1 b+1 a+b+1 2 Γ( a+1 ; 2 ) Γ( 2 ) 2 =

) 2(b−1) Γ( 2b ) Γ( a+b+1 2 . a+1 Γ(b) Γ( 2 )

(3)


50

Salahuddin

No. 4

In a monograph of Prudnikov et al., a summation theorem is given in the form [Prud., p.491(7.3.7.3)]  2 F1

a, b ; a+b−1 2

;

 " # Γ( a+b+1 ) 2 Γ( a+b−1 ) 1 √ 2 2 = π . + b+1 2 Γ(a) Γ(b) Γ( a+1 2 ) Γ( 2 )

(4)

Now using Legendre’s duplication formula and Recurrence relation for Gamma function, the above theorem can be written in the form  2 F1

a, b

;

a+b−1 2

;

 # " ) 2(a−b+1) Γ( a2 ) Γ( a+1 Γ( 2b ) Γ( b+2 1  2(b−1) Γ( a+b−1 2 2 ) 2 ) + = + a+1 . 2 2 Γ(b) Γ( a−1 Γ( 2 ) {Γ(a)} 2 )

(5)

Recurrence relation is defined by Γ(z + 1) = z Γ(z).

(6)

§2. Main summation formula  2 F1

=

 a, b ; a+b+32 2

;

1 2

) 2b Γ( a+b+32 2 (a − b) Γ(b) " ½ Γ( 2b ) 32768(1428329123020800a − 2322150583173120a2 + 1606274243887104a3 ) × ³ Q ´³ Q ´ 14 15 Γ( a2 ) {a − b − 2ζ} {a − b + 2η} ζ=0

η=1

32768(−636906005299200a4 + 163554924216320a5 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

32768(−29011643781120a6 + 3688786669568a7 ) + ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} ζ=0

η=1

32768(−343226083200a8 + 23578343360a9 ) + ³ 14 ´³ Q ´ 15 Q {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

32768(−1193992800a10 + 43995952a11 − 1146600a12 ) + ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} ζ=0

η=1


Vol. 7

A summation formula including recurrence relation

+

32768(20020a13 − 210a14 + a15 + 1428329123020800b + 8525223163330560a2 b) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 3

+

32768(−2182234506854400a b + 1969113895649280a4 b) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 5

+

32768(−264966591528960a b + 82650036080640a6 b) ´ ³ Q ´³ Q 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 7

+

32768(−6233334240000a b + 920583637440a8 b) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 9

+

32768(−39161191680a b + 3018684240a10 b − 67407600a11 b) ³ Q ´³ Q ´ 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 12

+

32768(2691780a b − 24360a b + 435a14 b) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

+

13

32768(2322150583173120b2 + 8525223163330560ab2 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

3 2

+

32768(5852172660080640a b − 528194276167680a4 b2 + 497028396625920a5 b2 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 6 2

+

32768(−30401221536000a b + 9824497355520a7 b2 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 8 2

+

32768(−363512823840a b + 54807626640a9 b2 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 10 2

+

32768(−1104760800a b + 85096440a11 b2 − 712530a12 b2 ) ´³ Q ´ ³ Q 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 13 2

32768(27405a b + 1606274243887104b3 ) + ³ 14 ´³ Q ´ 15 Q {a − b − 2ζ} {a − b + 2η} ζ=0

+

η=1

32768(2182234506854400ab3 + 5852172660080640a2 b3 + 1153266031104000a4 b3 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} ζ=0

η=1

51


52

Salahuddin

+

No. 4

32768(−46525375584000a5 b3 + 42437501433600a6 b3 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 7 3

+

32768(−1285763673600a b + 404597084400a8 b3 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 9 3

+

32768(−7227090000a b + 1052508600a10 b3 − 8143200a11 b3 ) ´ ³ Q ´³ Q 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 12 3

32768(593775a b + 636906005299200b4 ) + ³ 14 ´³ Q ´ 15 Q {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

+

32768(1969113895649280ab4 + 528194276167680a2 b4 + 1153266031104000a3 b4 ) ³ Q ´³ Q ´ 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 5 4

+

32768(85800120220800a b − 1679965963200a6 b4 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 7 4

+

32768(1438362021600a b − 20980485000a8 b4 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 9 4

+

32768(6230113500a b − 42921450a10 b4 + 5852925a11 b4 + 163554924216320b5 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 5

+

32768(264966591528960ab + 497028396625920a2 b5 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 3 5

+

32768(46525375584000a b + 85800120220800a4 b5 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 6 5

+

32768(2667136741920a b − 24708348000a7 b5 + 19527158700a8 b5 − 109254600a9 b5 ) ´³ Q ´ ³ Q 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 10 5

+

32768(30045015a b + 29011643781120b ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

+

6

32768(82650036080640ab6 + 30401221536000a2 b6 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} ζ=0

η=1


Vol. 7

A summation formula including recurrence relation

+

53

32768(42437501433600a3 b6 + 1679965963200a4 b6 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 5 6

+

32768(2667136741920a b + 34171477200a7 b6 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 8 6

+

32768(−119759850a b + 86493225a9 b6 + 3688786669568b7 + 6233334240000ab7 ) ´ ³ Q ´³ Q 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 2 7

+

32768(9824497355520a b + 1285763673600a3 b7 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 4 7

+

32768(1438362021600a b + 24708348000a5 b7 ) ³ Q ´³ Q ´ 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 6 7

+

32768(34171477200a b + 145422675a8 b7 + 343226083200b8 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 8

+

32768(920583637440ab + 363512823840a2 b8 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

3 8

+

32768(404597084400a b + 20980485000a4 b8 + 19527158700a5 b8 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 6 8

32768(119759850a b + 145422675a7 b8 ) + ³ 14 ´³ Q ´ 15 Q {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 9

+

32768(23578343360b + 39161191680ab9 + 54807626640a2 b9 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 3 9

+

32768(7227090000a b + 6230113500a4 b9 ) ´³ Q ´ ³ Q 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 5 9

+

32768(109254600a b + 86493225a6 b9 + 1193992800b10 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 10

+

32768(3018684240ab + 1104760800a2 b10 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} ζ=0

η=1


54

Salahuddin

+

No. 4

32768(1052508600a3 b10 + 42921450a4 b10 + 30045015a5 b10 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 11

32768(43995952b + 67407600ab11 ) + ³ 14 ´³ Q ´ 15 Q {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

2 11

+

32768(85096440a b + 8143200a3 b11 + 5852925a4 b11 ) ´ ³ Q ´³ Q 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 12

+

32768(1146600b + 2691780ab12 + 712530a2 b12 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 3 12

+

32768(593775a b

+ 20020b13 + 24360ab13 + 27405a2 b13 + 210b14 + 435ab14 + b15 ) ³ Q ´³ Q ´ 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0

+

65536b(1428329123020800 + 470423898685440a) ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

+

β=1

65536b(2328961922629632a2 + 381117697130496a3 ) ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1 4

+

65536b(316734590500864a + 29456251432960a5 ) ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1 6

+

65536b(9279610167296a + 511595950208a7 ) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1 8

+

65536b(77189562432a + 2483214240a9 + 193882832a10 ) ´ ³ Q ´³ Q 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1 11

12

65536b(3327896a + 131404a + 910a13 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1 8

+

65536b(77189562432a + 2483214240a9 + 193882832a10 ) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1 11

65536b(3327896a + 131404a + 910a13 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

12

β=1


Vol. 7

A summation formula including recurrence relation

+

65536b(15a14 − 470423898685440b + 5473573561958400ab + 503214007025664a2 b) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1 3

+

65536b(1969528317345792a b + 150112771248128a4 b) ³ Q ´³ Q ´ 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1 5

+

65536b(112539365949440a b + 5581588819072a6 b) ´³ Q ´ ³ Q 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1 7

+

65536b(1638717738496a b + 49573632864a8 b + 6999713760a9 b) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1 10

65536b(116414584a b + 8390512a11 b) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1 12

+

55

65536b(58058a b + 2030a13 b + 2328961922629632b2 − 503214007025664ab2 ) ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

65536b(3412315664252928a2 b2 + 129681106132992a3 b2 + 423536993230848a4 b2 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

65536b(16628085832320a5 b2 + 11189308499712a6 b2 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

65536b(300862325376a7 b2 + 80994977424a8 b2 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

65536b(1263236520a9 b2 + 163524504a10 b2 + 1099332a11 b2 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

65536b(71253a12 b2 − 381117697130496b3 ) + ³ 15 ´ ´³ Q 14 Q {a − b + 2β} {a − b − 2α} α=0

β=1

65536b(1969528317345792ab3 − 129681106132992a2 b3 + 645921311784960a3 b3 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

65536b(11831795932800a4 b3 + 33081548382720a5 b3 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

65536b(686621093760a6 b3 + 413821722240a7 b3 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1


56

Salahuddin

+

No. 4

65536b(5675445000a8 b3 + 1386606000a9 b3 + 8708700a10 b3 ) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1 11 3

+

65536b(1017900a b + 316734590500864b4 ) ³ Q ´³ Q ´ 15 14 {a − b + 2β} {a − b − 2α} α=0

+

β=1

65536b(−150112771248128ab4 + 423536993230848a2 b4 ) ´³ Q ´ ³ Q 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1 3 4

+

65536b(−11831795932800a b + 47032752624000a4 b4 ) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1 5 4

+

65536b(436682232000a b + 1060441956000a6 b4 ) ³ Q ´³ Q ´ 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1 7 4

+

65536b(11019106800a b + 5939968500a8 b4 ) ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

65536b(32516250a9 b4 + 7153575a10 b4 − 29456251432960b5 + 112539365949440ab5 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

65536b(−16628085832320a2 b5 + 33081548382720a3 b5 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

65536b(−436682232000a4 b5 + 1443061650240a5 b5 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

65536b(6518297520a6 b5 + 13870291680a7 b5 + 56728350a8 b5 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

65536b(27313650a9 b5 + 9279610167296b6 ) + ³ 15 ´ ´³ Q 14 Q {a − b + 2β} {a − b − 2α} α=0

β=1

65536b(−5581588819072ab6 + 11189308499712a2 b6 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

65536b(−686621093760a3 b6 + 1060441956000a4 b6 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1


Vol. 7

A summation formula including recurrence relation

+

65536b(−6518297520a5 b6 + 18331241040a6 b6 + 31935960a7 b6 ) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1 8 6

65536b(59879925a b − 511595950208b7 ) + ³ 15 ´³ Q ´ 14 Q {a − b + 2β} {a − b − 2α} α=0

+

β=1

65536b(1638717738496ab7 − 300862325376a2 b7 ) ´³ Q ´ ³ Q 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1 3 7

+

65536b(413821722240a b − 11019106800a4 b7 ) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1 5 7

+

65536b(13870291680a b − 31935960a6 b7 + 77558760a7 b7 ) ³ Q ´³ Q ´ 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1 8

65536b(77189562432b − 49573632864ab8 ) + ³ 15 ´ ´³ Q 14 Q {a − b + 2β} {a − b − 2α} α=0

β=1

65536b(80994977424a2 b8 − 5675445000a3 b8 + 5939968500a4 b8 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

65536b(−56728350a5 b8 + 59879925a6 b8 ) + ³ 15 ´ ´³ Q 14 Q {a − b + 2β} {a − b − 2α} α=0

β=1

65536b(−2483214240b9 + 6999713760ab9 − 1263236520a2 b9 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

65536b(1386606000a3 b9 − 32516250a4 b9 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1

65536b(27313650a5 b9 + 193882832b10 − 116414584ab10 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

65536b(163524504a2 b10 − 8708700a3 b10 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1

65536b(7153575a4 b10 − 3327896b11 + 8390512ab11 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

65536b(−1099332a2 b11 + 1017900a3 b11 + 131404b12 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

57


58

Salahuddin

No. 4

65536b(−58058ab12 + 71253a2 b12 − 910b13 + 2030ab13 + 15b14 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

¾

β=1

½ 2 Γ( b+1 2 ) 65536a(1428329123020800 − 470423898685440a + 2328961922629632a ) − a+1 ´³ Q ´ ³ Q 15 14 Γ( 2 ) {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

65536a(−381117697130496a3 + 316734590500864a4 ) + ´ ³ Q ´³ Q 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0

65536a(−29456251432960a5 + 9279610167296a6 ) + ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

65536a(−511595950208a7 + 77189562432a8 − 2483214240a9 ) + ³ Q ´³ Q ´ 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0

65536a(193882832a10 − 3327896a11 ) + ³ 14 ´³ Q ´ 15 Q {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

65536a(131404a12 − 910a13 + 15a14 + 470423898685440b + 5473573561958400ab) + ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

65536a(−503214007025664a2 b + 1969528317345792a3 b − 150112771248128a4 b) + ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

65536a(112539365949440a5 b − 5581588819072a6 b) + ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

65536a(1638717738496a7 b − 49573632864a8 b) + ³ Q ´³ Q ´ 15 14 {a − b − 2ζ} {a − b + 2η} ζ=0

η=1

65536a(6999713760a9 b − 116414584a10 b + 8390512a11 b − 58058a12 b + 2030a13 b) + ³ Q ´³ Q ´ 15 14 {a − b − 2ζ} {a − b + 2η} ζ=0

η=1

65536a(2328961922629632b2 + 503214007025664ab2 + 3412315664252928a2 b2 ) + ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} ζ=0

η=1

65536a(−129681106132992a3 b2 + 423536993230848a4 b2 − 16628085832320a5 b2 ) + ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} ζ=0

η=1


Vol. 7

A summation formula including recurrence relation

+

59

65536a(11189308499712a6 b2 − 300862325376a7 b2 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 8 2

+

65536a(80994977424a b − 1263236520a9 b2 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 10 2

+

65536a(163524504a b − 1099332a11 b2 + 71253a12 b2 ) ´ ³ Q ´³ Q 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 3

+

65536a(381117697130496b + 1969528317345792ab3 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

2 3

+

65536a(129681106132992a b + 645921311784960a3 b3 ) ³ Q ´³ Q ´ 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0

4 3

+

65536a(−11831795932800a b + 33081548382720a5 b3 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 6 3

+

65536a(−686621093760a b + 413821722240a7 b3 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 8 3

+

65536a(−5675445000a b + 1386606000a9 b3 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 11 3

+

65536a(1017900a b − 8708700a10 b3 + 316734590500864b4 + 150112771248128ab4 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 2 4

+

65536a(423536993230848a b + 11831795932800a3 b4 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 4 4

+

65536a(47032752624000a b − 436682232000a5 b4 ) ´³ Q ´ ³ Q 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

6 4

+

65536a(1060441956000a b − 11019106800a7 b4 + 5939968500a8 b4 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 9 4

65536a(−32516250a b + 7153575a10 b4 ) + ³ 14 ´³ Q ´ 15 Q {a − b − 2ζ} {a − b + 2η} ζ=0

η=1


60

Salahuddin

+

No. 4

65536a(29456251432960b5 + 112539365949440ab5 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

2 5

+

65536a(16628085832320a b + 33081548382720a3 b5 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 4 5

+

65536a(436682232000a b + 1443061650240a5 b5 ) ´ ³ Q ´³ Q 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 6 5

+

65536a(−6518297520a b + 13870291680a7 b5 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 8 5

+

65536a(−56728350a b + 27313650a9 b5 + 9279610167296b6 + 5581588819072ab6 ) ³ Q ´³ Q ´ 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 2 6

+

65536a(11189308499712a b + 686621093760a3 b6 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

4 6

+

65536a(1060441956000a b + 6518297520a5 b6 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 6 6

+

65536a(18331241040a b − 31935960a7 b6 + 59879925a8 b6 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 7

+

65536a(511595950208b + 1638717738496ab7 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

2 7

+

65536a(300862325376a b + 413821722240a3 b7 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 4 7

+

65536a(11019106800a b + 13870291680a5 b7 ) ´³ Q ´ ³ Q 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 6 7

+

65536a(31935960a b + 77558760a7 b7 + 77189562432b8 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 8

+

65536a(49573632864ab + 80994977424a2 b8 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} ζ=0

η=1


Vol. 7

A summation formula including recurrence relation

+

65536a(5675445000a3 b8 + 5939968500a4 b8 + 56728350a5 b8 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 6 8

65536a(59879925a b + 2483214240b9 ) + ³ 14 ´³ Q ´ 15 Q {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

+

65536a(6999713760ab9 + 1263236520a2 b9 + 1386606000a3 b9 ) ´ ³ Q ´³ Q 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 4 9

65536a(32516250a b + 27313650a5 b9 ) + ³ 14 ´³ Q ´ 15 Q {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

10

+

65536a(193882832b + 116414584ab10 + 163524504a2 b10 ) ³ Q ´³ Q ´ 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 3 10

65536a(8708700a b + 7153575a4 b10 ) + ³ 14 ´³ Q ´ 15 Q {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 11

+

65536a(3327896b + 8390512ab11 + 1099332a2 b11 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 3 11

+

65536a(1017900a b + 131404b12 + 58058ab12 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 2 12

+

65536a(71253a b + 910b13 + 2030ab13 + 15b14 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} ζ=0

+

η=1

32768(1428329123020800a + 2322150583173120a2 ) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

32768(1606274243887104a3 + 636906005299200a4 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

32768(163554924216320a5 + 29011643781120a6 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

32768(3688786669568a7 + 343226083200a8 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1

61


62

Salahuddin

+

32768(23578343360a9 + 1193992800a10 + 43995952a11 ) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1 12

+

13

32768(1146600a + 20020a + 210a14 + a15 ) ³ Q ´³ Q ´ 15 14 {a − b + 2β} {a − b − 2α} α=0

+

No. 4

β=1

32768(1428329123020800b + 8525223163330560a2 b) ´³ Q ´ ³ Q 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1 3

+

32768(2182234506854400a b + 1969113895649280a4 b) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1 5

+

32768(264966591528960a b + 82650036080640a6 b) ³ Q ´³ Q ´ 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1 7

+

32768(6233334240000a b + 920583637440a8 b) ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

32768(39161191680a9 b + 3018684240a10 b + 67407600a11 b) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

32768(2691780a12 b + 24360a13 b + 435a14 b) + ³ 15 ´ ´³ Q 14 Q {a − b + 2β} {a − b − 2α} α=0

β=1

32768(−2322150583173120b2 + 8525223163330560ab2 + 5852172660080640a3 b2 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

32768(528194276167680a4 b2 + 497028396625920a5 b2 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

32768(30401221536000a6 b2 + 9824497355520a7 b2 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

32768(363512823840a8 b2 + 54807626640a9 b2 + 1104760800a10 b2 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

32768(85096440a11 b2 + 712530a12 b2 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1


Vol. 7

A summation formula including recurrence relation

32768(27405a1 3b2 + 1606274243887104b3 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

+

β=1

32768(−2182234506854400ab3 + 5852172660080640a2 b3 ) ³ Q ´³ Q ´ 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1 4 3

+

32768(1153266031104000a b + 46525375584000a5 b3 ) ´³ Q ´ ³ Q 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1 6 3

+

32768(42437501433600a b + 1285763673600a7 b3 ) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1 8 3

+

32768(404597084400a b + 7227090000a9 b3 + 1052508600a10 b3 ) ³ Q ´³ Q ´ 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1

11 3

12 3

32768(8143200a b + 593775a b ) ´ ´³ Q 15 14 Q {a − b + 2β} {a − b − 2α} α=0

β=1

32768(−636906005299200b4 + 1969113895649280ab4 − 528194276167680a2 b4 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

32768(1153266031104000a3 b4 + 85800120220800a5 b4 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

32768(1679965963200a6 b4 + 1438362021600a7 b4 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

32768(20980485000a8 b4 + 6230113500a9 b4 + 42921450a10 b4 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

32768(5852925a11 b4 + 163554924216320b5 ) + ³ 15 ´ ´³ Q 14 Q {a − b + 2β} {a − b − 2α} α=0

β=1

32768(−264966591528960ab5 + 497028396625920a2 b5 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

32768(−46525375584000a3 b5 + 85800120220800a4 b5 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

63


64

Salahuddin

+

No. 4

32768(2667136741920a6 b5 + 24708348000a7 b5 + 19527158700a8 b5 ) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

9 5

10 5

32768(109254600a b + 30045015a b ) + ³ 15 ´³ Q ´ 14 Q {a − b + 2β} {a − b − 2α} α=0

+

β=1

32768(−29011643781120b6 + 82650036080640ab6 ) ´³ Q ´ ³ Q 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1 2 6

+

32768(−30401221536000a b + 42437501433600a3 b6 ) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1 4 6

+

32768(−1679965963200a b + 2667136741920a5 b6 ) ³ Q ´³ Q ´ 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1 7 6

32768(34171477200a b + 119759850a8 b6 ) + ³ 15 ´ ´³ Q 14 Q {a − b + 2β} {a − b − 2α} α=0

β=1

32768(86493225a9 b6 + 3688786669568b7 − 6233334240000ab7 + 9824497355520a2 b7 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

32768(−1285763673600a3 b7 + 1438362021600a4 b7 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

32768(−24708348000a5 b7 + 34171477200a6 b7 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

32768(145422675a8 b7 − 343226083200b8 + 920583637440ab8 − 363512823840a2 b8 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

3 8

32768(404597084400a b − 20980485000a4 b8 + 19527158700a5 b8 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

32768(−119759850a6 b8 + 145422675a7 b8 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1

32768(23578343360b9 − 39161191680ab9 + 54807626640a2 b9 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

32768(−7227090000a3 b9 + 6230113500a4 b9 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1


Vol. 7

65

A summation formula including recurrence relation

+

32768(−109254600a5 b9 + 86493225a6 b9 − 1193992800b10 ) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1 10

32768(3018684240ab − 1104760800a2 b10 ) + ³ 15 ´³ Q ´ 14 Q {a − b + 2β} {a − b − 2α} α=0

β=1 3 10

+

32768(1052508600a b − 42921450a4 b10 + 30045015a5 b10 ) ´³ Q ´ ³ Q 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1 11

32768(43995952b − 67407600ab11 ) ´³ Q ´ 15 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1 2 11

+

32768(85096440a b − 8143200a3 b11 + 5852925a4 b11 ) ³ Q ´³ Q ´ 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1 12

+

32768(−1146600b + 2691780ab12 − 712530a2 b12 ) ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

32768(593775a3 b12 + 20020b13 − 24360ab13 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1

) 32768(27405a b − 210b14 + 435ab14 + b15 ) + ³ 15 . ´ ´³ Q 14 Q {a − b + 2β} {a − b − 2α} 2 13

α=0

(7)

β=1

§3. Derivation of main summation formula (7) Substituting c =

a+b+32 2

 (a − b) 2 F1 

a, b

;

a+b+32 2

;

, and z =

1 2

, in equation (2), we get

  a + 1, b ; 1 = a 2 F1  a+b+32 2 ; 2

  a, b + 1 ; 1 − b 2 F1  a+b+32 2 ; 2

 1 . 2

Now using Gauss second summation theorem, we get L. H. S " ½ 2b Γ( a+b+32 ) Γ( 2b ) 16384(1428329123020800a − 2322150583173120a2 ) 2 = a ³ Q ´³ Q ´ 14 15 Γ(b) Γ( a+2 2 ) {a − b − 2ζ} {a − b + 2η} ζ=0

16384(1606274243887104a3 − 636906005299200a4 ) + ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} ζ=0

η=1

η=1


66

Salahuddin

+

16384(163554924216320a5 − 29011643781120a6 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 7

+

16384(3688786669568a − 343226083200a8 + 23578343360a9 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 10

16384(−1193992800a + 43995952a11 ) + ³ 14 ´ ´³ Q 15 Q {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 12

+

16384(−1146600a + 20020a13 − 210a14 + a15 + 1428329123020800b) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 2

16384(8525223163330560a b) ´³ Q ´ 14 15 Q {a − b + 2η} {a − b − 2ζ} η=1

ζ=0

+

16384(−2182234506854400a3 b + 1969113895649280a4 b) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 5

+

16384(−264966591528960a b + 82650036080640a6 b) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 7

+

16384(−6233334240000a b + 920583637440a8 b − 39161191680a9 b) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 10

16384(3018684240a b − 67407600a11 b) + ³ 14 ´³ Q ´ 15 Q {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 12

+

16384(2691780a b − 24360a13 b + 435a14 b) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

+

16384(2322150583173120b2 + 8525223163330560ab2 ) ´³ Q ´ ³ Q 14 15 {a − b − 2ζ} {a − b + 2η} ζ=0

η=1 3 2

+

16384(5852172660080640a b − 528194276167680a4 b2 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 5 2

+

16384(497028396625920a b − 30401221536000a6 b2 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} ζ=0

η=1

No. 4


Vol. 7

A summation formula including recurrence relation

+

67

16384(9824497355520a7 b2 − 363512823840a8 b2 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 9 2

+

16384(54807626640a b − 1104760800a10 b2 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 11 2

+

16384(85096440a b − 712530a12 b2 + 27405a13 b2 ) ´ ³ Q ´³ Q 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 3

+

16384(1606274243887104b + 2182234506854400ab3 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

2 3

+

16384(5852172660080640a b + 1153266031104000a4 b3 ) ³ Q ´³ Q ´ 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 5 3

+

16384(−46525375584000a b + 42437501433600a6 b3 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 7 3

+

16384(−1285763673600a b + 404597084400a8 b3 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 9 3

+

16384(−7227090000a b + 1052508600a10 b3 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 11 3

+

16384(−8143200a b + 593775a12 b3 + 636906005299200b4 + 1969113895649280ab4 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 2 4

+

16384(528194276167680a b + 1153266031104000a3 b4 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 5 4

+

16384(85800120220800a b − 1679965963200a6 b4 ) ´³ Q ´ ³ Q 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 7 4

+

16384(1438362021600a b − 20980485000a8 b4 + 6230113500a9 b4 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 10 4

16384(−42921450a b + 5852925a11 b4 ) + ³ 14 ´³ Q ´ 15 Q {a − b − 2ζ} {a − b + 2η} ζ=0

η=1


68

Salahuddin

+

No. 4

16384(163554924216320b5 + 264966591528960ab5 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

2 5

+

16384(497028396625920a b + 46525375584000a3 b5 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 4 5

+

16384(85800120220800a b + 2667136741920a6 b5 ) ´ ³ Q ´³ Q 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 7 5

+

16384(−24708348000a b + 19527158700a8 b5 − 109254600a9 b5 + 30045015a10 b5 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 6

+

16384(29011643781120b + 82650036080640ab6 ) ³ Q ´³ Q ´ 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0

2 6

+

16384(30401221536000a b + 42437501433600a3 b6 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 4 6

+

16384(1679965963200a b + 2667136741920a5 b6 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 7 6

+

16384(34171477200a b − 119759850a8 b6 + 86493225a9 b6 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 7

+

16384(3688786669568b + 6233334240000ab7 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

2 7

+

16384(9824497355520a b + 1285763673600a3 b7 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 4 7

+

16384(1438362021600a b + 24708348000a5 b7 ) ´³ Q ´ ³ Q 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 6 7

+

16384(34171477200a b + 145422675a8 b7 + 343226083200b8 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 8

+

16384(920583637440ab + 363512823840a2 b8 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} ζ=0

η=1


Vol. 7

A summation formula including recurrence relation

+

16384(404597084400a3 b8 + 20980485000a4 b8 + 19527158700a5 b8 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 6 8

16384(119759850a b + 145422675a7 b8 ) + ³ 14 ´³ Q ´ 15 Q {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 9

+

16384(23578343360b + 39161191680ab9 + 54807626640a2 b9 ) ´ ³ Q ´³ Q 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 3 9

+

16384(7227090000a b + 6230113500a4 b9 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 5 9

+

16384(109254600a b + 86493225a6 b9 + 1193992800b10 ) ³ Q ´³ Q ´ 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 10

+

16384(3018684240ab + 1104760800a2 b10 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

3 10

+

16384(1052508600a b + 42921450a4 b10 + 30045015a5 b10 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 11

16384(43995952b + 67407600ab11 ) + ³ 14 ´³ Q ´ 15 Q {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

2 11

+

16384(85096440a b + 8143200a3 b11 + 5852925a4 b11 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 12

+

16384(1146600b + 2691780ab12 + 712530a2 b12 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 3 12

16384(593775a b + 20020b13 + 24360ab13 ) + ³ 14 ´³ Q ´ 15 Q {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 2 13

16384(27405a b + 210b14 + 435ab14 + b15 ) + ³ 14 ´³ Q ´ 15 Q {a − b − 2ζ} {a − b + 2η} ζ=0

¾

¾

η=1

½ 2 Γ( b+1 2 ) 65536(1428329123020800 − 470423898685440a + 2328961922629632a ) − a+1 ³ ´³ ´ 14 15 Q Q Γ( 2 ) {a − b − 2ζ} {a − b + 2η} ζ=0

η=1

69


70

Salahuddin

+

No. 4

65536(−381117697130496a3 + 316734590500864a4 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 5

+

65536(−29456251432960a + 9279610167296a6 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 7

+

65536(−511595950208a + 77189562432a8 − 2483214240a9 ) ´ ³ Q ´³ Q 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 10

65536(193882832a − 3327896a11 ) + ³ 14 ´³ Q ´ 15 Q {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 12

+

65536(131404a

− 910a13 + 15a14 + 470423898685440b + 5473573561958400ab) ³ Q ´³ Q ´ 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 2

+

65536(−503214007025664a b + 1969528317345792a3 b) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 4

+

65536(−150112771248128a b + 112539365949440a5 b) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 6

+

65536(−5581588819072a b + 1638717738496a7 b) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 8

+

65536(−49573632864a b + 6999713760a9 b) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 10

65536(−116414584a b + 8390512a11 b) + ³ 14 ´³ Q ´ 15 Q {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 12

+

65536(−58058a b + 2030a13 b + 2328961922629632b2 ) ´³ Q ´ ³ Q 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 2

+

65536(503214007025664ab + 3412315664252928a2 b2 − 129681106132992a3 b2 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 4 2

+

65536(423536993230848a b − 16628085832320a5 b2 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} ζ=0

η=1


Vol. 7

A summation formula including recurrence relation

+

71

65536(11189308499712a6 b2 − 300862325376a7 b2 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 8 2

+

65536(80994977424a b − 1263236520a9 b2 + 163524504a10 b2 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 11 2

12 2

65536(−1099332a b + 71253a b ) + ³ 14 ´ ´³ Q 15 Q {a − b + 2η} {a − b − 2ζ} η=1

ζ=0

+

65536(381117697130496b3 + 1969528317345792ab3 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

2 3

+

65536(129681106132992a b + 645921311784960a3 b3 ) ³ Q ´³ Q ´ 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0

4 3

+

65536(−11831795932800a b + 33081548382720a5 b3 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 6 3

+

65536(−686621093760a b + 413821722240a7 b3 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 8 3

+

65536(−5675445000a b + 1386606000a9 b3 − 8708700a10 b3 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 11 3

+

65536(1017900a b + 316734590500864b4 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

+

65536(150112771248128ab4 + 423536993230848a2 b4 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 3 4

+

65536(11831795932800a b + 47032752624000a4 b4 ) ´³ Q ´ ³ Q 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 5 4

+

65536(−436682232000a b + 1060441956000a6 b4 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 7 4

+

65536(−11019106800a b + 5939968500a8 b4 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 9 4

+

65536(−32516250a b + 7153575a10 b4 + 29456251432960b5 + 112539365949440ab5 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} ζ=0

η=1


72

Salahuddin

+

No. 4

65536(16628085832320a2 b5 + 33081548382720a3 b5 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 4 5

+

65536(436682232000a b + 1443061650240a5 b5 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 6 5

+

65536(−6518297520a b + 13870291680a7 b5 − 56728350a8 b5 ) ´ ³ Q ´³ Q 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 9 5

65536(27313650a b + 9279610167296b6 ) + ³ 14 ´³ Q ´ 15 Q {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

+

65536(5581588819072ab6 + 11189308499712a2 b6 ) ³ Q ´³ Q ´ 14 15 {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 3 6

+

65536(686621093760a b + 1060441956000a4 b6 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 5 6

+

65536(6518297520a b + 18331241040a6 b6 − 31935960a7 b6 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 8 6

65536(59879925a b + 511595950208b7 ) + ³ 14 ´³ Q ´ 15 Q {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

+

65536(1638717738496ab7 + 300862325376a2 b7 + 413821722240a3 b7 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 4 7

14 Q

65536(11019106800a b ) ´³ Q ´ 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

5 7

+

65536(13870291680a b + 31935960a6 b7 + 77558760a7 b7 + 77189562432b8 ) ´³ Q ´ ³ Q 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 8

14 Q

65536(49573632864ab ) ´³ Q ´ 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

2 8

+

65536(80994977424a b + 5675445000a3 b8 + 5939968500a4 b8 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} ζ=0

η=1


Vol. 7

73

A summation formula including recurrence relation

65536(56728350a5 b8 + 59879925a6 b8 ) + ³ 14 ´³ Q ´ 15 Q {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 9

+

65536(2483214240b + 6999713760ab9 + 1263236520a2 b9 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 3 9

65536(1386606000a b + 32516250a4 b9 ) + ³ 14 ´ ´³ Q 15 Q {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 5 9

+

65536(27313650a b + 193882832b10 + 116414584ab10 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 2 10

65536(163524504a b + 8708700a3 b10 ) + ³ 14 ´³ Q ´ 15 Q {a − b + 2η} {a − b − 2ζ} η=1

ζ=0 4 10

+

65536(7153575a b + 3327896b11 + 8390512ab11 ) ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0 2 11

+

65536(+1099332a b + 1017900a3 b11 + 131404b12 ) ³ Q ´³ Q ´ 14 15 {a − b − 2ζ} {a − b + 2η} η=1

ζ=0

65536(58058ab12 + 71253a2 b12 + 910b13 + 2030ab13 + 15b14 ) + ´³ Q ´ ³ Q 15 14 {a − b − 2ζ} {a − b + 2η} ζ=0

−b

2

b+1

Γ( a+b+32 ) 2

Γ(b + 1)

"

η=1

Γ( b+1 2 ) a+1 Γ( 2 )

½

16384(1428329123020800a + 2322150583173120a2 ) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

16384(1606274243887104a3 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1

16384(636906005299200a4 + 163554924216320a5 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

16384(29011643781120a6 + 3688786669568a7 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

16384(343226083200a8 + 23578343360a9 + 1193992800a10 ) + ³ Q ´³ Q ´ 14 15 {a − b − 2α} {a − b + 2β} α=0

¾#

β=1


74

Salahuddin

+

No. 4

16384(43995952a11 + 1146600a12 + 20020a13 ) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1 14

15

16384(210a + a + 1428329123020800b) + ³ 15 ´³ Q ´ 14 Q {a − b + 2β} {a − b − 2α} α=0

+

β=1

16384(8525223163330560a2 b + 2182234506854400a3 b) ´³ Q ´ ³ Q 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1 4

+

16384(1969113895649280a b + 264966591528960a5 b) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1 6

+

16384(82650036080640a b + 6233334240000a7 b) ³ Q ´³ Q ´ 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1 8

+

16384(920583637440a b + 39161191680a9 b + 3018684240a10 b + 67407600a11 b) ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

16384(2691780a12 b) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1

16384(24360a13 b + 435a14 b − 2322150583173120b2 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

16384(8525223163330560ab2 + 5852172660080640a3 b2 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

16384(528194276167680a4 b2 + 497028396625920a5 b2 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

16384(30401221536000a6 b2 + 9824497355520a7 b2 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

16384(363512823840a8 b2 + 54807626640a9 b2 + 1104760800a10 b2 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

16384(+85096440a11 b2 + 712530a12 b2 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1


Vol. 7

A summation formula including recurrence relation

16384(27405a13 b2 + 1606274243887104b3 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

+

β=1

16384(−2182234506854400ab3 + 5852172660080640a2 b3 ) ³ Q ´³ Q ´ 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1 4 3

+

16384(1153266031104000a b + 46525375584000a5 b3 ) ´³ Q ´ ³ Q 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1 6 3

+

16384(42437501433600a b + 1285763673600a7 b3 ) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1 8 3

+

16384(404597084400a b + 7227090000a9 b3 + 1052508600a10 b3 ) ³ Q ´³ Q ´ 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1

11 3

12 3

16384(8143200a b + 593775a b ) ´ ´³ Q 15 14 Q {a − b + 2β} {a − b − 2α} α=0

β=1

16384(−636906005299200b4 + 1969113895649280ab4 − 528194276167680a2 b4 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

16384(1153266031104000a3 b4 + 85800120220800a5 b4 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

16384(1679965963200a6 b4 + 1438362021600a7 b4 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

16384(20980485000a8 b4 + 6230113500a9 b4 + 42921450a10 b4 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

16384(5852925a11 b4 + 163554924216320b5 ) + ³ 15 ´ ´³ Q 14 Q {a − b + 2β} {a − b − 2α} α=0

β=1

16384(2667136741920a6 b5 + 24708348000a7 b5 + 19527158700a8 b5 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

16384(109254600a9 b5 + 30045015a10 b5 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1

75


76

Salahuddin

+

No. 4

16384(−29011643781120b6 + 82650036080640ab6 ) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1 2 6

+

16384(−30401221536000a b + 42437501433600a3 b6 ) ³ Q ´³ Q ´ 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1 4 6

+

16384(−1679965963200a b + 2667136741920a5 b6 ) ´³ Q ´ ³ Q 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1 7 6

16384(34171477200a b + 119759850a8 b6 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1 9 6

16384(86493225a b + 3688786669568b7 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

+

β=1

16384(−6233334240000ab7 + 9824497355520a2 b7 ) ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

16384(−1285763673600a3 b7 + 1438362021600a4 b7 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

16384(−24708348000a5 b7 + 34171477200a6 b7 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

16384(145422675a8 b7 − 343226083200b8 + 920583637440ab8 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

16384(−363512823840a2 b8 + 404597084400a3 b8 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

16384(−20980485000a4 b8 + 19527158700a5 b8 − 119759850a6 b8 + 145422675a7 b8 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

16384(23578343360b9 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1

16384(−39161191680ab9 + 54807626640a2 b9 − 7227090000a3 b9 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1


Vol. 7

77

A summation formula including recurrence relation

16384(6230113500a4 b9 − 109254600a5 b9 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1 6 9

+

16384(86493225a b − 1193992800b10 + 3018684240ab10 ) ³ Q ´³ Q ´ 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1 2 10

+

16384(−1104760800a b + 1052508600a3 b10 ) ´³ Q ´ ³ Q 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1 4 10

+

16384(−42921450a b + 30045015a5 b10 + 43995952b1 1) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1 11

16384(−67407600ab + 85096440a2 b11 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1 3 11

+

16384(−8143200a b + 5852925a4 b11 − 1146600b12 + 2691780ab12 ) ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

16384(−712530a2 b12 + 593775a3 b12 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1

16384(20020b13 − 24360ab13 + 27405a2 b13 − 210b1 4 + 435ab14 + b15 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

¾ −

½ 65536(1428329123020800 + 470423898685440a + 2328961922629632a2 ) × ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

65536(381117697130496a3 + 316734590500864a4 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

65536(29456251432960a5 + 9279610167296a6 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

65536(511595950208a7 + 77189562432a8 + 2483214240a9 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

65536(193882832a10 + 3327896a11 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1

Γ( b+2 2 ) a+1 Γ( 2 )


78

Salahuddin

+

No. 4

65536(131404a12 + 910a13 + 15a14 − 470423898685440b + 5473573561958400ab) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

2

+

65536(503214007025664a b + 1969528317345792a3 b) ³ Q ´³ Q ´ 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1 4

+

65536(150112771248128a b + 112539365949440a5 b) ´³ Q ´ ³ Q 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1 6

+

65536(5581588819072a b + 1638717738496a7 b + 49573632864a8 b) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1 9

65536(6999713760a b + 116414584a10 b) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1 11

+

65536(8390512a b + 58058a12 b + 2030a13 b) ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

65536(2328961922629632b2 − 503214007025664ab2 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

65536(3412315664252928a2 b2 + 129681106132992a3 b2 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

65536(423536993230848a4 b2 + 16628085832320a5 b2 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

65536(11189308499712a6 b2 + 300862325376a7 b2 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

65536(80994977424a8 b2 + 1263236520a9 b2 ) + ³ 15 ´ ´³ Q 14 Q {a − b + 2β} {a − b − 2α} α=0

β=1

65536(163524504a10 b2 + 1099332a11 b2 + 71253a12 b2 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

65536(−381117697130496b3 + 1969528317345792ab3 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1


Vol. 7

A summation formula including recurrence relation

+

65536(−129681106132992a2 b3 + 645921311784960a3 b3 + 11831795932800a4 b3 ) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1 5 3

15 Q

65536(33081548382720a b ) ´³ Q ´ 14 {a − b + 2β} {a − b − 2α}

α=0

+

β=1

65536(686621093760a6 b3 + 413821722240a7 b3 + 5675445000a8 b3 ) ´³ Q ´ ³ Q 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1 9 3

65536(1386606000a b + 8708700a10 b3 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1 11 3

+

65536(1017900a b + 316734590500864b4 ) ³ Q ´³ Q ´ 14 15 {a − b − 2α} {a − b + 2β} α=0

+

β=1

65536(−150112771248128ab4 + 423536993230848a2 b4 ) ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

65536(−11831795932800a3 b4 + 47032752624000a4 b4 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

65536(436682232000a5 b4 + 1060441956000a6 b4 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

65536(11019106800a7 b4 + 5939968500a8 b4 + 32516250a9 b4 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

65536(7153575a10 b4 − 29456251432960b5 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1

65536(112539365949440ab5 − 16628085832320a2 b5 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

65536(33081548382720a3 b5 − 436682232000a4 b5 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

65536(1443061650240a5 b5 + 6518297520a6 b5 + 13870291680a7 b5 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

79


80

Salahuddin

No. 4

65536(56728350a8 b5 + 27313650a9 b5 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

+

β=1

65536(9279610167296b6 − 5581588819072ab6 ) ³ Q ´³ Q ´ 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1 2 6

+

65536(11189308499712a b − 686621093760a3 b6 ) ´³ Q ´ ³ Q 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1 4 6

+

65536(1060441956000a b − 6518297520a5 b6 + 18331241040a6 b6 + 31935960a7 b6 ) ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

8 6

15 Q

65536(59879925a b ) ´³ Q ´ 14 {a − b − 2α} {a − b + 2β}

α=0

+

β=1

65536(−511595950208b7 + 1638717738496ab7 ) ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

65536(−300862325376a2 b7 + 413821722240a3 b7 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

65536(−11019106800a4 b7 + 13870291680a5 b7 − 31935960a6 b7 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

65536(77558760a7 b7 + 77189562432b8 + 5939968500a4 b8 − 56728350a5 b8 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

65536(−49573632864ab8 + 80994977424a2 b8 − 5675445000a3 b8 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1

65536(59879925a6 b8 − 2483214240b9 + 6999713760ab9 ) + ´ ³ Q ´³ Q 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1

65536(−1263236520a2 b9 + 1386606000a3 b9 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1

65536(−32516250a4 b9 + 27313650a5 b9 + 193882832b10 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

β=1


Vol. 7

81

A summation formula including recurrence relation

65536(−116414584ab10 + 163524504a2 b10 ) + ³ 15 ´³ Q ´ 14 Q {a − b − 2α} {a − b + 2β} α=0

β=1 3 10

+

65536(−8708700a b + 7153575a4 b10 − 3327896b1 1) ³ Q ´³ Q ´ 15 14 {a − b + 2β} {a − b − 2α} α=0

β=1 11

+

65536(8390512ab − 1099332a2 b11 + 1017900a3 b11 ) ´³ Q ´ ³ Q 14 15 {a − b − 2α} {a − b + 2β} α=0

β=1

65536(131404b12 − 58058ab12 + 71253a2 b12 − 910b1 3 + 2030ab13 + 15b14 ) + ³ Q ´³ Q ´ 15 14 {a − b − 2α} {a − b + 2β} α=0

¾# .

β=1

On simplification the result (8) is proved.

References [1] Arora, Asish, Singh, Rahul and Salahuddin, Development of a family of summation formulae of half argument using Gauss and Bailey theorems, Journal of Rajasthan Academy of Physical Sciences, 7(2008), 335-342. [2] J. L. Lavoie, Some summation formulae for the series 3 F2 , Math. Comput., 49(1987), 269-274. [3] J. L. Lavoie, F. Grondin and A. K. Rathie, Generalizations of Watson’s theorem on the sum of a 3 F2 , Indian J. Math., 34(1992), 23-32. [4] J. L. Lavoie, F. Grondin and A. K. Rathie, Generalizations of Whipple’s theorem on the sum of a 3 F2 , J. Comput. Appl. Math., 72(1996), 293-300. [5] A. P. Prudnikov, Yu. A. Brychkov and O. I. Marichev, More Special Functions, Integrals and Series, 3(1986). [6] E. D. Rainville, The contiguous function relations for p Fq with applications to Bateman’s u,v Jn and Rice’s Hn (ζ, p, ν), Bull. Amer. Math. Soc., 51(1945), 714-723. [7] Salahuddin and M. P Chaudhary, Development of some summation formulae using Hypergeometric function, Global journal of Science Frontier Research, 10(2010), 36-48. [8] Salahuddin and M. P Chaudhary, Certain summation formulae associated to Gauss second summation theorem, Global journal of Science Frontier Research, 10(2010), 30-35.


Scientia Magna Vol. 7 (2011), No. 4, 82-91

Some classes of difference fuzzy numbers defined by an orlicz function Ayhan Esi† and Eda Eren‡ Department of Mathematics, Adiyaman University, 02040, Adiyaman, Turkey E-mail: aesi23@hotmail.com eeren@adiyaman.edu.tr Abstract In this paper we introduce some new classes of sequences of fuzzy numbers using by Orlicz function and examine some properties of resulting sequence classes of fuzzy numbers. Keywords Fuzzy numbers, fuzzy sets, difference sequence, Orlicz function. 2000 Mathematics Subject Classification: Primary 05C38, 15A15, Secondary 05A15, 1 5A18.

§1. Introduction and preliminaries The notion of fuzzy sets was introduced by Zadeh [7] in 1965. Afterwards many authors have studied and generalized this notion in many ways, due to potential of the introduced notion. Also it has wide range of applications in almost all the branches of studied in particular science, where mathematics in used. It attracted many workers to introduce different types of classes of fuzzy numbers. Matloka [5] introduced bounded and convergent sequences of fuzzy numbers and studied their some properties. Later on, sequences of fuzzy numbers have been discussed by Nanda [6] , Diamond and Kloeden [2] , Esi [3] and many others. Let D denote the set of all closed and bounded intervals on R, the real line. For X, Y ∈ D, we define δ (X, Y ) = max (|a1 − b1 | , |a2 − b2 |) , where X = [a1 , a2 ] and Y = [b1 , b2 ]. It is known that (D, δ) is a complete metric space. A fuzzy real number X is a fuzzy set on R, i.e., a mapping X : R → I (= [0, 1]) associating each real number t with its grade of membership X (t). The set of all upper-semi continuous, normal, convex fuzzy real numbers is denoted by L(R). Throughout the paper, by a fuzzy real number X, we mean that X ∈ L(R). α The α−cut or α−level set [X] of the fuzzy real number X, for 0 < α ≤ 1, defined by α [X] = {t ∈ R : X (t) ≥ α}; for α = 0, it is the closure of the strong 0−cut, i.e., closure of the set {t ∈ R : X (t) > 0}. The linear structure of L(R) induces the addition X + Y and the scalar multiplication µX, µ ∈ R, in terms of α−level sets, by α

α

α

α

α

[X + Y ] = [X] + [Y ] , [µX] = µ [X]


Vol. 7

Some classes of difference fuzzy numbers defined by an orlicz function

83

for each α ∈ (0, 1]. Let d : L(R) × L(R) → R be defined by α

α

d (X, Y ) = sup δ ([X] , [Y ] ) . 0≤α≤1

Then d defines a metric on L(R). It is well known that L(R) is complete with respect to d. The set R of real numbers can be embedded in L(R) if we define r ∈ L(R) by   1, if t = r ; r (t) =  0, if t 6= r . The additive identity and multiplicative identity of L(R) are denoted by 0 and 1, respectively. For r in R and X in L(R), the product rX is defined as follows   X ¡r−1 t¢ , if r 6= 0 ; rX (t) =  0, if r = 0 . A metric on L (R) is said to be translation invariant if d (X + Z, Y + Z) = d (X, Y ) for all X, Y, Z ∈ L (R). The metric d has the following properties: d (cX, cY ) = |c| d (X, Y ) for c ∈ R and d (X + Y, Z + W ) ≤ d (X, Z) + d (Y, W ) . A sequence X = (Xk ) of fuzzy numbers is a function X from the set N of natural numbers in to L(R). The fuzzy number Xk denotes the value of the function at k ∈ N and is called the k−th term of the sequence. We denote by wF the set of all sequences X = (Xk ) of fuzzy numbers. A sequence X = (Xk ) of fuzzy numbers is said to be bounded if the set {Xk : k ∈ N} of fuzzy numbers is bounded [5] . We denote by `F ∞ the set of all bounded sequences X = (Xk ) of fuzzy numbers. A sequence X = (Xk ) of fuzzy numbers is said to be convergent to a fuzzy number X0 if for every ε > 0 there is a positive integer k0 such that d (Xk , X0 ) < ε for all k > k0 [5] . We denote by cF the set of all convergent sequences X = (Xk ) of fuzzy numbers. The following inequality will be used throughout the paper: Let p = (pk ) be a positive sequence of real numbers with 0 < inf pk = h ≤ pk ≤ supk pk = H < ∞ and K = max (1, 2H−1 ). Then for ak , bk ∈ C, we have pk

|ak + bk |

pk

≤ K(|ak |

p

+ |bk | k ), for all k ∈ N.

(1)

An Orlicz function is a function M : [0, ∞) → [0, ∞) which is continuous, nondecreasing and convex with M (0) = 0, M (x) > 0 for x > 0 and M (x) → ∞ as x → ∞. An Orlicz function is a function M is said to satisfy the ∆2 −condition for all values of x, if there exist a constant T > 0 such that M (2x) ≤ T M (x), (x ≥ 0).


84

Ayhan Esi and Eda Eren

Lindenstrauss and Tzafriri follows: ( `M =

[4]

No. 4

used the Orlicz function and introduced the sequence `M as

x = (xk ) :

X k

µ M

|xk | r

)

< ∞, for some r > 0 .

They proved that `M is a Banach space normed by ( ) X µ |xk | ¶ kxk = inf r > 0 : M ≤1 . r k

Remark 1.1. An Orlicz function M satisfies the inequality M (λx) ≤ λM (x) for all λ with 0 < λ < 1. In this paper we define the following difference classes of fuzzy numbers: Let X = (Xk ) be a sequence of fuzzy numbers and M be an Orlicz function. In this paper and define the following difference classes of fuzzy numbers:

cF 0 [M,

½ · µ ¶¸pk d(∆Xk , 0) F −s =0 ∆, p, s] = X = (Xk ) ∈ w : lim k M k ρ o for some ρ > 0, s > 0 ,

cF [M, ∆, p, s] =

½ · µ ¶¸pk d(∆Xk , X0 ) X = (Xk ) ∈ wF : lim k −s M =0 k ρ o for some ρ > 0, s > 0

and `F ∞

½ · µ ¶¸pk d(∆Xk , 0) F −s [M, ∆, p, s] = X = (Xk ) ∈ w : sup k M <∞ ρ k o for some ρ > 0, s > 0 ,

where p = (pk ) is a sequence of real numbers such that pk > 0 for all k ∈ N and supk pk = H < ∞ and ∆Xk = Xk − Xk+1 , this assumption is made throughout the rest of this paper. We can some specialize these classes as follows: If s = 0, M (x) = x and pk = 1 for all k ∈ N, then ½ ¾ F F F c0 [M, ∆, p, s] = c0 [∆] = X = (Xk ) ∈ w : lim d(∆Xk , 0) = 0 , k

½ ¾ cF [M, ∆, p, s] = cF [∆] = X = (Xk ) ∈ wF : lim d(∆Xk , X) = 0 k

and F `F ∞ [M, ∆, p, s] = `∞ [∆] =

¾ ½ X = (Xk ) ∈ wF : sup d(∆Xk , 0) < ∞ , k

[1]

which were defined and studied by Ba¸sarır and Mursaleen . If s = 0, M (x) = x and pk = 1 for all k ∈ N and ∆Xk = Xk then we obtain the classes cF 0, F [6] c and `F which we defined and studied by Nanda . ∞


Vol. 7

Some classes of difference fuzzy numbers defined by an orlicz function

85

Example 1.2. Let s = 0, M (x) = x and pk = 1 for all k ∈ N. Consider the sequence of fuzzy numbers X = (Xk ) defined as follows: For k = i2 , i ∈ N, Xk = 0.   1, for 0 ≤ t ≤ k −1 ; Otherwise, Xk (t) =  0, otherwise , Then

and

  [0, 0] , for k = i2 , i ∈ N; α [Xk ] = ¤ £  0, k −1 , otherwise ,  h i −1  − (k + 1) , 0 , for k = i2 , i ∈ N;    £ ¤ α [∆Xk ] = 0, k −1 , for k = i2 − 1, i ∈ N, with i > 1;  h i    − (k + 1)−1 , k −1 , otherwise ,

F F Hence X = (Xk ) ∈ cF 0 [M, ∆, p, s] ⊂ c [M, ∆, p, s] ⊂ `∞ [M, ∆, p, s].

§2. Main results In this section we prove some results involving the classes of sequences of fuzzy numbers ∆, p, s], cF [M, ∆, p, s] and `F ∞ [M, ∆, p, s].

cF 0 [M,

F Theorem 2.1. If d is a translation invariant metric, then cF 0 [M, ∆, p, s], c [M, ∆, p, s] F and `∞ [M, ∆, p, s] are closed under the operations of addition and scalar multiplication.

Proof. Since d is a translation invariant metric implies that −

d(∆Xk + ∆Yk , 0) 6 d(∆Xk , 0) + d(∆Yk , 0)

(2)

and −

d(λ∆Xk , 0) = |λ| d(∆Xk , 0) ,

(3)

where λ is a scalar. Let X = (Xk ) and Y = (Yk ) ∈ `F ∞ [M, ∆, p, s]. Then there exists positive numbers ρ1 and ρ2 such that ¶¸pk · µ d(∆Xk , 0) sup k −s M <∞ ρ1 k and · µ ¶¸pk d(∆Yk , 0) sup k −s M < ∞. ρ2 k


86

Ayhan Esi and Eda Eren

No. 4

Let ρ3 = max(2ρ1 , 2ρ2 ). By taking into account the properties (1), (2) and since M is non-decreasing and convex function, we have · µ ¶¸pk ¶ µ ¶¸pk · µ d(∆Xk + ∆Yk , 0) d(∆Yk , 0) d(∆Xk , 0) k −s M ≤ k −s M +M ρ3 ρ3 ρ3 · µ ¶ µ ¶¸pk d(∆Xk , 0) 1 d(∆Yk , 0) −s 1 ≤k M + M 2 ρ1 2 ρ2 ¶¸pk · µ ¶¸pk · µ d(∆Yk , 0) d(∆Xk , 0) −s −s +Kk M ≤ Kk M ρ1 ρ2 < ∞. F Therefore X + Y ∈ `F ∞ [M, ∆, p, s]. Now let X = (Xk ) ∈ `∞ [M, ∆, p, s] and λ ∈ R with 0 < |λ| < 1. By taking into account the properties (3) and Remark, we have

k

−s

· µ ¶¸pk · µ ¶¸pk d(λ∆Xk , 0) d(∆Xk , 0) −s M 6k |λ| M ρ ρ · µ ¶¸pk d(∆Xk , 0) pk −s 6 k |λ| M ρ · µ ¶¸pk d(∆Xk , 0) h 6 |λ| k −s M ρ < ∞.

Therefore λX ∈ `F ∞ [M, ∆, p, s]. The proof of the other cases are routine work in view of the above proof. Theorem 2.2. Let M be an Orlicz function, then F F cF 0 [M, ∆, p, s] ⊂ c [M, ∆, p, s] ⊂ `∞ [M, ∆, p, s] . F F Proof. Clearly cF 0 [M, ∆, p, s] ⊂ c [M, ∆, p, s]. We shall prove that c [M, ∆, p, s] ⊂ F [M, ∆, p, s]. Let X = (Xk ) ∈ c [M, ∆, p, s]. Then there exists some fuzzy number X0 such that · µ ¶¸pk d(∆Xk , Xo ) −s lim k M = 0, s > 0. k ρ

`F ∞

On taking ρ1 = 2ρ and by using (1), we have · µ ¶¸pk d(∆Xk , 0) k −s M ρ1

6

µ ¶pk · µ ¶¸pk 1 d(∆Xk , X0 ) Kk −s M 2 ρ µ ¶pk · µ ¶¸pk 1 d(∆Xk , 0) + . Kk −s M 2 ρ

Since X = (Xk ) ∈ cF [M, ∆, p, s], we get X = (Xk ) ∈ `F ∞ [M, ∆, p, s]. F Theorem 2.3. cF [M, ∆, p, s], c [M, ∆, p, s] and `F ∞ [M, ∆, p, s] are complete metric 0 spaces with respect to the metric given by ( ) ½ · µ µ ¶¶¸pk ¾ H1 pn (d(∆Xk , ∆Yk ) −s g (X, Y ) = inf ρ H > 0 : sup k M ≤1 , ρ k


Vol. 7

Some classes of difference fuzzy numbers defined by an orlicz function

87

where H = max (1, supk pk ). ¡ i¢ Proof. Consider the class cF be a Cauchy sequence in cF 0 [M, ∆, p, s]. Let X 0 [M, ∆, p, s]. ε Let ε > 0 be given and r, xo > 0 be fixed. Then for each rxo > 0, there exists a positive integer no such that ¡ ¢ ε g X i, X j < , for all i, j ≥ no . rxo By definition of g, we have !!#pk ) H1 ( " Ã Ã j i d(∆X , ∆X ) k k sup k −s M ≤ 1, g (X i , X j ) k for all i, j ≥ no . Thus

"

Ã

sup k

−s

Ã

M

k

for all i, j ≥ no . It follows that k

Ã

−s

Ã

M

d(∆Xki , ∆Xkj ) g (X i , X j )

d(∆Xki , ∆Xkj ) g (X i , X j )

!!#pk ≤ 1,

!! ≤ 1,

¡ ¢ for each k ≥ 0 and for all i, j ≥ no . For r > 0 with k −s M rx2o ≥ 1, we have à à !! j ³ rx ´ i d(∆X , ∆Y ) o −s k k k −s M ≤ k M . g (X i , Y j ) 2 Since k −s 6= 0 for all k, we have à M

d(∆Xki , ∆Xkj ) g (X i , X j )

! ≤M

³ rx ´ o

2

.

This implies that

rxo ε ε d(∆Xki , ∆Xkj ) ≤ . = . 2 rxo 2 ¡ ¢ ¡ ¢ Hence ∆Xki i = ∆Xk1 , ∆Xk2 , ∆Xk3 , · · · is a Cauchy sequence in L (R). Since L (R) is complete, it is convergent. Therefore for each ε (0 < ε < 1), there exists a positive integer no such that d(∆Xki , ∆Xkj ) < ε for all i ≥ no . Using the continuity of the Orlicz function M , we can find     pk  H1   lim d(∆Xki , ∆Xkj )   j→∞ −s       sup k M ≤ 1.   ρ k≥no  Thus

 

sup k −s M  k≥no

lim d(∆Xki , ∆Xk )

j→∞

ρ

pk  H1   ≤ 1. 

Taking infimum of such ρ0 s we get   ( à á " ¢ !!#pk ) H1  pn  i d(∆X , ∆X k k inf ρ H > 0 : sup k −s M ≤ 1 < ε,   ρ k


88

Ayhan Esi and Eda Eren

No. 4

for all i ≥ no . That is X i → X in cF 0 [M, ∆, p, s], where X = (Xk ). Now let i ≥ no , then using triangular inequality, we get ¡ ¢ ¡ ¢ ¡ ¢ g X, 0 ≤ g X, X i + g X i , 0 . So we have X ∈ cF 0 [M, ∆, p, s]. This completes the proof of the theorem. Theorem 2.4. Let inf pk = h > 0 and supk pk = H < ∞. Then (a) cF [M, ∆] ⊂ cF [M, ∆, p, s]. (b) Let M be an Orlicz function which satisfies ∆2 −condition. Then cF [∆, p, s] ⊂ cF [M, ∆, p, s]. Proof. (a) Suppose that X = (Xk ) ∈ cF [M, ∆]. Since M is an Orlicz function, then µ ¶ · ¸ d(∆Xk , X0 ) d(∆Xk , X0 ) lim M = M lim = 0, for some ρ > 0. k k ρ ρ h ³ Since inf k pk = h > 0, then limk M d(∆Xρk ,

X0 )

´ih

= 0, so for 0 < ε < 1, ∃ k0 3 for all k > k0 ,

· µ ¶¸h d(∆Xk , X0 ) M <ε<1 ρ and since pk > h for all k ∈ N · µ ¶¸pk · µ ¶¸h d(∆Xk , X0 ) d(∆Xk , X0 ) M 6 M <ε<1 ρ ρ and then we get

· µ ¶¸pk d(∆Xk , X0 ) lim M = 0. k ρ

Since (k −s ) is bounded, we write · µ ¶¸pk d(∆Xk , X0 ) lim k −s M = 0. k ρ Therefore X = (Xk ) ∈ cF [M, ∆, p, s]. p (b) Let X = (Xk ) ∈ cF [∆, p, s] so that Sk = k −s [d(∆Xk , X0 )] k −→ 0 as k −→ ∞. Let ε > 0 and choose δ with 0 < δ < 1 such that M (t) < ε for 0 ≤ t ≤ δ. Now we write yk = d(∆Xρk , X0 ) for all k ∈ N and consider pk

k −s [M (yk )]

pk

= k −s [M (yk )] pk

Using by the remark we have k −s [M (yk )] make the following procedure. We have

yk ≤

pk

|yk ≤δ +k −s [M (yk )]

|yk >δ .

≤ k −s max(ε, εh ) for yk ≤ δ. For yk > δ, we will

yk yk <1+ . δ δ

Since M is non-decreasing and convex, it follows that ³ yk ´ 1 1 ≤ M (2) + (2yk δ −1 ) . M (yk ) < M 1 + δ 2 2


Vol. 7

Some classes of difference fuzzy numbers defined by an orlicz function

89

Since M satisfies ∆2 −condition, we can write M (yk ) =

T yk T yk yk M (2) + M (2) = T M (2) . 2 δ 2 δ δ

We get the following ³ £ ´ ¤H pk p k −s [M (yk )]yk>δ ≤ k −s max 1, T M (2)δ −1 [yk ] k and pk

k −s [M (yk )]

³ £ ¤H ´ ≤ k −s max(ε, εh ) + max 1, T δ −1 M (2) Sk .

Taking the limits ε → 0 and k → ∞, it follows that X = (Xk ) ∈ cF [M, 4, p, s]. Theorem 2.5. Let M , M1 and M2 be Orlicz functions and s1 , s2 ≥ 0. Then T (a) cF [M1 , 4, p, s] cF [M2 , 4, p, s] ⊂ cF [M1 + M2 , 4, p, f, s]. (b) s1 ≤ s2 implies cF [M, 4, p, s1 ] ⊂ cF [M, 4, p, s2 ]. T Proof. (a) Let X = (Xk ) ∈ cF [M1 , 4, p, s] cF [M2 , 4, p, s]. Then there exist some ρ1 , ρ2 > 0 such that · µ ¶¸pk d(∆Xk , X0 ) −s =0 lim k M1 k ρ1 and

· µ ¶¸pk d(∆Xk , X0 ) lim k −s M2 = 0. k ρ2

Let ρ = ρ1 + ρ2 . Then using the inequality (1), we have · · ¸¸pk · ¶ ¶¸pk µ µ d(∆Xk , X0 ) d(∆Xk , X0 ) d(∆Xk , X0 ) (M1 + M2 ) = M1 + M2 ρ ρ ρ · µ ¶ µ ¶¸pk ρ1 d(∆Xk , X0 ) d(∆Xk , X0 ) ρ2 M1 M2 ≤ + ρ1 + ρ2 ρ1 ρ1 + ρ2 2ρ2 · µ ¶ ¶¸pk µ d(∆Xk , X0 ) d(∆Xk , X0 ) ≤ M1 + M2 ρ1 ρ2 ¶¸pk · ¶¸pk · µ µ d(∆Xk , X0 ) d(∆Xk , X0 ) + K M2 . ≤ K M1 ρ1 ρ2 Since (k −s ) is bounded, we write · · ¸¸pk d(∆Xk , X0 ) −s k (M1 + M2 ) ρ

· ¶¸pk µ d(∆Xk , X0 ) ≤ K k M1 ρ ¶¸pk · µ d(∆Xk , X0 ) −s M2 . +K k ρ −s

Therefore we get X = (Xk ) ∈ cF [M1 + M2 , 4, p, f, s]. (b) Let s1 ≤ s2 . Then k −s2 ≤ k −s1 for all k ∈ N. Let X = (Xk ) ∈ cF [M, ∆, p, s1 ]. Since · µ ¶¸pk · µ ¶¸pk d(∆Xk , X0 ) d(∆Xk , X0 ) −s2 −s1 k ≤ k , M M ρ ρ we get X = (Xk ) ∈ cF [M, 4, p, s2 ]. Theorem 2.6. Let M be an Orlicz function. Then


90

Ayhan Esi and Eda Eren

No. 4

(a) Let 0 < inf k pk ≤ pk ≤ 1, then cF [M, ∆, p, s] ⊂ cF [M, ∆, s]. F F (b) Let 1 ≤ pk ≤ supk pk³< ∞, ´ then c [M, ∆, s] ⊂ c [M, ∆, p, s]. (c) Let 0 < pk ≤ qk and pqkk be bounded, then cF [M, ∆, q, s] ⊂ cF [M, ∆, p, s]. Proof. (a) X = (Xk ) ∈ cF [M, 4, p, s]. Since 0 < inf k pk ≤ pk ≤ 1, for each k, we get ¶¸ · µ ¶¸pk · µ d(∆Xk , X0 ) d(∆Xk , X0 ) k −s M ≤ k −s M ρ ρ for all k ∈ N, and for some ρ > 0. So we get X = (Xk ) ∈ cF [M, ∆, s]. (b) Let 1 ≤ pk ≤ supk pk < ∞, for each k and X = (Xk ) ∈ cF [M, ∆, s]. Then for each 0 < ε < 1 there exists a positive integer k0 such that · µ ¶¸ d(∆Xk , X0 ) −s k M ≤ε<1 ρ for each k ≥ k0 . This implies that · µ ¶¸pk µ ¶ d(∆Xk , X0 ) d(∆Xk , X0 ) −s −s k M ≤k M ρ ρ for some ρ > 0. Hence we get X = (Xk ) ∈ cF [M, ∆, p, s]. (c) Let X = (Xk ) ∈ cF [M, ∆, q, s]. Write · µ ¶¸qk d(∆Xk , X0 ) wk = M ρ and Tk = pqkk , so that 0 < T < Tk ≤ 1 for each k. We define the sequences (uk ) and (vk ) as follows: Let uk = wk and vk = 0 if wk ≥ 1, and let uk = 0 and wk = vk if wk < 1. Then it is clear that for each k ∈ N, we have wk = uk + vk , wkTk = uTk k + vkTk . Now it follows that uTk k ≤ uk ≤ wk and vkTk ≤ vkT . Therefore

h i k −s wkTk = k −s uTk k + vkTk ≤ k −s wk + k −s vkT .

Since T < 1 so that T −1 > 1, for each k ∈ N, k −s vkT = (k −s vk )T (k −s )1−T µh ¶ µ 1 ¶1−T ¡ −s ¢T i1/T T h¡ −s ¢1−T i 1−T ≤ k vk k ¡ ¢T = k −s vk , by H¨older’s inequality and thus k −s wkTk ≤ k −s wk + Hence X = (Xk ) ∈ cF [M, ∆, p, s].

¡

k −s vk

¢T

.


Vol. 7

Some classes of difference fuzzy numbers defined by an orlicz function

91

References [1] M. Ba繡sar覺r and M. Mursaleen, Some difference sequence spaces of fuzzy numbers, J. Fuzzy Math., 11(2003), No. 3, 1-7. [2] P. Diamond and P. Kloeden, Metric spaces of fuzzy sets, Theory and Applications, World Scientific, Singapore, 1994. [3] A. Esi, On some classes of generalized difference sequences of fuzzy numbers defined by Orlicz functions, Glob. J. Pure Appl. Math., 4(2008), No. 1, 53-64. [4] J. Lindenstrauss and L. Tzafriri, On Orlicz sequence spaces, Israel J. Math., 10(1971), 379-390. [5] M. Matloka, Sequences of fuzzy numbers, Busefal, 28(1986), 28-37. [6] S. Nanda, On sequences of fuzzy numbers, Fuzzy Sets and Systems, 33(1989), 123-126. [7] L. A. Zadeh, Fuzzy sets, Information and Control, 8(1965), 338-353.


Scientia Magna Vol. 7 (2011), No. 4, 92-95

The Hadwiger-Finsler reverse in an acute triangle Marius Dragan† and Mih´aly Bencze‡ † Bdul Timisoara nr 35, Bl. OD6, Sc. E, Ap. 176, 061311, Bucuresti , Romania ‡ str. Harmanului nr 6, 505600, Sacele-N´egyfalu, jud. Brasov, Romania E-mail: benczemihaly@gmail.com Abstract In the paper the authors proposed the following inequality: In any acute triangle are true the following inequality: √ √ ¢ 2− 3 ¡ √ (a − b)2 + (b − c)2 + (c − a)2 . a2 + b2 + c2 ≤ 4 3S + (1) 3−2 2 Keywords Geometric inequalities. 2010 Mathematics Subject Classification: 26D15, 51M16, 26D99.

§1. Main results −−→ −→ −−→ In any triangle ABC we shall denote by a = ||BC||, b = ||AC||, c = ||AB||, s = the radius of circumcircle and r the radius of incircle.

a+b+c , 2

R

In the following we shall use the next result: Lemma 1.1. In any triangle ABC are valid the following identities:

2 2

2 2

a2 + b2 + c2 = 2(s2 − r2 − 4Rr).

(2)

ab + bc + ca = s2 + r2 + 4Rr.

(3)

2 2

2

2

2

2

a b + b c + c a = (s + r + 4Rr) − 16Rrs .

(4)

Lemma 1.2. In any triangle ABC are valid the following identity: cos A cos B cos C =

s2 − r2 − 4Rr − 4R2 . 4R2

(5)

Proof. In the following we denote x = a2 + b2 + c2 . From the cosinus theorem it follows


Vol. 7

that:

93

The Hadwiger-Finsler reverse in an acute triangle

¢ ¢ Q¡ x − 2a2 b2 + c2 + a2 = cos A cos B cos C = 2 b2 c2 2 2 2 8aP P 28a2 b c 2 2 2 3 2 2 x − 2 a x + 4 a b x − 8a b c = 8a2 b2 c2 2 2 s − r − 4Rr − 4R2 . = 4R2 Q¡

Theorem 1.1. In any acute triangle is true the following inequality: (6)

s > 2R + r. Proof. Because in any acute triangle are true the following inequality: according with the identity (5) it follows that the inequality (6) is true. Theorem 1.2. (Blundon) In every triangle ABC is true the following inequality: p ¯ 2 ¡ 2 ¢¯ ¯s − 2R + 10Rr − r2 ¯ ≤ 2 (R − 2r) R (R − 2r) .

Q

cos A > 0

(7)

In the following we shall use the above result. We denote: √ 2− 3 R √ , x= λ= ≥2. r 3−2 2 By identities (2) and (3) from Lemma 1.1 it follows that inequality (1) is equivalent with the following inequality: √ (λ − 1) s2 + 2 3rs + (1 − 3λ) r2 + (4 − 12λ) Rr ≥ 0 . (8) We shall consider two cases: √ Case 1.1. 2 < x ≤ 2 + 1. According with the right side of the Blundon’s inequality in order to prove the inequality (8) it will be sufficient that: µ ¶ q 3 (λ − 1) 2R2 + 10Rr − r2 − 2 R (R − 2r) r q √ 3 +2 3r 2R2 + 10Rr − r2 − 2 R (R − 2r) + (1 − 3λ) r2 + (4 − 12λ) Rr ≥ 0, or in an equivalent from p (2λ − 2) x2 + (10λ − 10) x − λx + 1 − 2 (λ − 1) x(x − 2)3 r q √ 3 +2 3 2x2 + 10x − 1 − 2 x (x − 2) + (4 − 12λ) x + 1 − 3λ ≥ 0.

(9)

Inequality (9) may be written as: q p p (λ − 1) x2 − (λ + 3) x + 1 − 2λ + 6x2 + 30x − 3 − 6 x(x − 2)3 − (λ − 1) x(x − 2)3 ≥ 0,


94

Marius Dragan and Mih´ aly Bencze

No. 4

Or in an equivalent form: q

p p 6x2 + 30x − 3 − 6 x(x − 2)3 − 9 − (λ − 1) x(x − 2)3 ≥ 0,

(x − 2) ((λ − 1) x + λ − 5) + It follows that:

q 3 p 6x2 + 30x − 3 − 6 x (x − 2) − (λ − 1) x(x − 2)3 ≥ 0. (x − 2) ((λ − 1) x + λ − 5) + r q 3 6x2 + 30x − 3 − 6 x (x − 2) + 9 As x ≥ 2 it will be sufficient to prove that: p p 6x + 42 − 6 x (x − 2) (λ − 1) x + λ − 5 + r − (λ − 1) x(x − 2) > 0. q 3 6x2 + 30x − 3 − 6 x (x − 2) + 9 After performing some calculation we shall obtain the inequality:   ³ ´ p  6  x − x (x − 2)  q  λ − 1 + r 3 6x2 + 30x − 3 − 6 x (x − 2) + 9 42

+λ − 5 + r 6x2

+λ−5>0 . q 3 + 30x − 3 − 6 x (x − 2) + 9

(10)

√ We shall consider the following function: f, g, F : (2, 2 + 1] → R, p p f (x) = x − x (x − 2), g (x) = 6x2 + 30x − 3 − 6 x(x − 2)3 , Ã

6

F (x) = f (x) λ − 1 + p g(x) + 9

!

42 +p +λ−5 . g(x) + 9

√ The inequality (10) may be written in an equivalent form as : F (x) > 0, ∀x ∈ (2, 2 + 1]. In the following we shall prove that F is a decreasing function. It will be sufficient to prove that f is an decreasing function as : f 0 (x) = 1 − √xx−1 < 0 it follows that f is a decresing 2 −2x function. Also : ³ ´ 3 3 2 (x − 2) + 3x (x − 2) g 0 (x) = 12x + 30 − q 3 x (x − 2) ³ ´ p 6 (2x + 5) x (x − 2) − (x − 2) (2x − 1) p = x (x − 2) µq ¶ q 2 2 6 x (2x + 5) − (x − 2) (2x − 1) √ = . x


Vol. 7

95

The Hadwiger-Finsler reverse in an acute triangle

In order to prove that g 0 (x) > 0 will sufficient to prove that: x(2x + 5)2 > (x − 2)(2x − 1)2 which is equivalent with the inequality 32x2 + 16x + 2 > 0. It follows that F is a decreasing √ √ function on the (2, 2 + 1] interval. We shall obtain F (x) > F ( 2 + 1). As : √ ³√ ´ ³√ ´ 6 2 + 42 F 2 + 1 = (λ − 1) 2+1 −4+ p = 0. √ 51 + 36 2 + 9 √ We shall obtain F (x) > 0, ∀ x ∈ (2, 2 + 1] . √ Case 1.2. x > 2 + 1. In order to prove the inequality (8) according theorem (1) will be sufficient to prove that : √ ¡ ¢ (λ − 1) 4x2 + 4x + 1 + 2 3 (2x + 1) + (4 − 12λ) + 1 − 3λ > 0 or in an equivalent form: √ √ ¡ ¢ λ 2x2 − 4x − 1 > 2x2 − 2 3x − 3 .

(11)

√ √ As x > 2 + 1 > 26 + 1 it follows that : 2x2 − 4x − 1 > 0. In order to prove the inequality (11) it will be sufficient to prove that : √ √ 2x2 − 2 3x − 3 . λ> 2x2 − 4x − 1 √ We shall consider the function: f : ( 2 + 1, +∞) → R

(12)

√ √ 2x2 − 2 3x − 3 . f (x) = 2x2 − 4x − 1 We have: 0

f (x) =

√ ¢ ¡ √ ¢ ¡ √ 2 3 − 4 x2 + 2 3 − 2 x − 3 2

(2x2 − 4x + 1)

.

√ ¡√ ¢ As: 4 = 40 − 24 3 > 0 it follows that : f 0 (x) < 0 (∀) x ∈ 2 + 1, +∞ . ¡√ ¢ We shall obtain: f (x) < f 2 + 1 = λ and we have the inequality of the statement.

References [1] Cezar Lupu, Constantin Mateescu, Vlad Matei and Mihai Opincaru , A refinement of the Finsler-Hodwinger reverse inequality , GMA. 2010, No. 1-2. [2] D. S. Mitrinovic, J. E. Pekaric and V. Volonec, Recent Advances in Geometric inequalities. [3] Sorin Radulescu, Marius Dragan and I. V. Maftei, Some consequences of W. J. Blundons inequalitiy, GMB. 2011, No. 1. [4] OctogonMathematical Magazine, 1993-2011.


Scientia Magna Vol. 7 (2011), No. 4, 96-103

On mean value computation of a number theoretic function1 Qianli Yang† and Chunlan Fu‡ † Department of Mathematics, Weinan Teacher’s University, Weinan, Shaanxi, 714000, P. R. China ‡ School of Sciences, South China University of Technology, Guangzhou, Guangdong, 510640, P. R. China Abstract The power function of p in the factorization of n!. It’s mean value calculation were studied, methods of the elementary number theory and analytic theory and average method were adopted, precise calculation formulas of once mean value of function b(n, p) and second mean value of function b(n, p) were got, this conclusion for studying integer n! standard decomposition type and relevant property has important impetus. Keywords Integer standard decomposition type, number theoretic function, mean value, co -mputing formula.

§1. Introduction and results In problem 68 of [1], Professor F. Smarandache asked us to study the properties of the sequences k = ep (n), p is a prime, k denotes the power of p in the factorization of n [2] . Studies the number sequences in the integral expression [3] and [5]. Studies the mean computing problems of digital sum. In this paper, we studied the power function of p in the factorization of n! and it’s mean value calculation, let p is a prime, α(n, p) denotes the power of p in the P factorization of n!. We give an exact computing formula of the mean value α(n, p) and n<N

completes the proof. First we give two definitions as follows: Definition 1.1. Let p (p > 2) be a fixed prime, n be any positive integer and n = a1 p + a2 p2 + · · · + as ps , (0 6 ai < p, i = 1, 2, · · · , s). Let a(n, p) = a1 + a2 + · · · + as as function of integer sum in base p; Let Ak (N, p) = P k a (n, p)(k = 1, 2) as once mean value of function a(n, p) and second mean value of n<N P function a(n, p). Set B (N, p) = na (n, p) as once mean value of function na (n, p). n<N

Definition 1.2. Let p (p > 2) be a fixed prime, n be any positive integer and n! = pk11 pk22 · · · pkt t , 1 This paper is supported by the N. S. F. of project Shanxi Province (2010JM1009) and E. S. F. of project of Shanxi Province (2010JK540).


Vol. 7

97

On mean value computation of a number theoretic function

where pi is a prime. Call b(n, p) as the power function of p in the factorization of n!; Call P k Ck (N, p) = b (n, p)(k = 1, 2) as k−th mean value of function b(n, p) and second mean n<N

value of function b(n, p). In this paper [x] denotes the greatest integer not exceeding x. Theorem 1.1. Let p(p ≥ 2) be a prime, N be a fixed positive integer, assume N as follows, N = a1 p + a2 p2 + · · · + as ps , (0 6 ai < p, i = 1, 2, · · · , s), then X C(N, p) = b(n, p) n<N

1 P −1

=

Ã

N (N − 1) − 2

µX s i=1

! ¶ i (p − 1)i X ai + 1 i + aj − ai p 2 2 j=1

or C(N, p) =

à [logp N ] µ ¸ · ¸ ¶ i µ· X 1 N (N − 1) (p − 1)i X N N − + − j+1 p p−1 2 2 pj p i=1 j=1 µ· ¸ · ¸ ¶ N N ¶µ· ¸ · ¸ ¶ ! pi − pi+1 p + 1 N N − − i+1 p pi . 2 pi p

Theorem 1.2. C2 (N, p) =

(

1 2

(p − 1)

ϕ2 (N ) +

s X

¡ ¡ ¢ pi−1 ai (i − 2) ϕ2 (p) + 1 − 2pi pϕ2 (ai ) +

i=1

 ¡

¢ i

(p − 1) ϕ1 (i) ϕ1 (p) + 2i 1 − p ϕ1 (ai ) ϕ1 (p) + 2 ai i

i−1 X

 aj + i − 1 ϕ1 (p)

j=1

  2 i−1 i−1 X pi−2 − 1 2 ϕ1 2 (p) X j  +pϕ1 (ai ) aj + pai  aj  − ai p − 2ai jp  2 p j=1 j=1 j=1 i−1 X

−2

s−1 X

ai ϕ1 

i=1

+

j X

s X

aj p

j=i+1

ak −

k=1

aj + 1 2

!

aj pj

j

+ ai p

i

s X j=i+1

!!)

µ s X p−1 j 2 j=i+1

aj p + p  j

i

.

Corollary 1.1. Let N = 2k1 + 2k2 + · · · + 2ks ,where k1 > k2 > · · · > ks ; ki is a positive integer,i = 1, 2, · · · , s,then C(N, 2) =

X n<N

or C(N, 2) =

X n<N

s

N (N − 1) X + b(n, 2) = (ki 2ki −1 + (i − 1)2ki ) 2 i=1

b(n, 2) =

[log2 N ] N (N − 1) 1 X +i−1+ (ki 2ki −1 + (i − 1)2ki ). 2 2 i=1


98

Qianli Yang and Chunlan Fu

No. 4

§2. Some lemmas and proofs Lemma 2.1.[4] If n is expressed as follow in the base p, n = a0 + a1 p + · · · + ak pk where 0 6 ai < p, ai is a positive integer, 0 6 i 6 k We have the exact formula, ¸ · ¸ · £ ¤ n n (1) ai = i − i+1 p, k = logp n . p p Lemma 2.2.[4] Let n be any positive integer, p be a prime, then ¸ ∞ · X 1 n = (n − a(n, p)) . b(n, p) ≡ i p p − 1 i=

(2)

Lemma 2.3.[3] Let N = a1 p + a2 p2 + · · · + as ps where (0 6 ai < p, i = 1, 2, · · · , s). Then   s i X X X p − 1 a + 1 i   ai pi A1 (N, p) = a(n, p) = i+ aj − (3) 2 2 i=1 j=1 n<N

or A1 (N, p) i ´ ³h i h   N N ¸ · ¸ ¶ µ· ¸ · ¸ ¶ s i µ· − X X pi pi+1 p + 1 p − 1 N N N N   = i+ − j+1 p − − i+1 p pi . j i 2 p p 2 p p i=1 j=1 (4) Lemma 2.4.[5] A2 (N, p)

s X

=

{ai iϕ2 (p) + pϕ2 (ai ) + (p − 1) ϕ1 (i) ϕ1 (p) + 2iϕ1 (ai ) ϕ1 (p)

i=1

 2   i−1  X +2 [ai iϕ1 (p) + pϕ1 (ai )] pi−1 . aj + pai  aj    j=1 j=1 i−1 X

(5)

Lemma 2.5. µ ¶ k−1 X pk−2 − 1 k+1 p + ϕ2 p − (k − 1)ϕ1 (p) pk−1 + ϕ1 2 (p)pk−2 ipi 4 i=1

B(pk , p) =

+ϕ2 (p) Proof. ¡ ¢ B pk , p

=

X n<pk

+

1 − pk−2 2 p . 1 − p2

(6)

X

na (n, p) = X

n<pk−1

na (n, p) + · · · +

2pk−1 6n<3pk−1

Because X ipk−1 6n<(i+1)pk−1

na (n, p) +

na (n, p)

X

na (n, p)

pk−1 6n<2pk−1

X

(p−1)pk−1 6n<pk

na (n, p).


Vol. 7

99

On mean value computation of a number theoretic function

X

=

06n<pk−1

X

=

¡

¢ ¡ ¢ n + ipk−1 a n + ipk−1 , p

¡

¢ n + ipk−1 (a (n, p) + i)

06n<pk−1

X

=

na (n, p) + i

06n<pk−1

X

X

n + ipk−1

n<pk−1

a (n, p) + i2 p2(k−1) .

n<pk−1

From above formula ¡ ¢ p (p − 1) X = pB pk−1 , p + n 2 k−1

¡ ¢ B pk , p

n<p

p (p − 1) X p (p − 1) (2p − 1) 2(k−1) + a (n, p) + p . 2 6 k−1 k

n<p

Similarly, ¡ ¢ pB pk−1 , p

¡ ¢ p2 (p − 1) X = p2 B pk−2 , p + n 2 k−2 n<p

p (p − 1) (2p − 1) 2(k−2) p (p − 1) X a (n, p) + + p , 2 6 k−2 k

n<p

······ ¡ ¢ pk−2 B p2 , p

= pk−1 B (p, p) + +

pk−1 (p − 1) X pk (p − 1) X n+ a (n, p) 2 2 n<p n<p

p (p − 1) (2p − 1) 2 p . 6

Therefore ¡

B pk , p

¢

  X X X p − 1 p = pk−1 B (p, p) + n + p2 n + · · · + pk−1 n 2 k−1 k−2 n<p n<p

n<p

¡ ¢ ¢ p − 1 k ¡ ¡ k−1 ¢ + p A p , p + A pk−2 , p + · · · + A (p, p) 2 ´ p (p − 1) (2p − 1) ³ 2(k−1) + p + p2(k−2) + · · · + p2 . 6

(7)

Because 2

B (p, p) = 12 + 22 + 32 + · · · + (p − 1) =

p (p − 1) (2p − 1) . 6

(8)

Put (3) and (8) in (7), ¡ ¢ B pk , p

=

pk (p − 1) (2p − 1) p − 1 + 6 2 2

+

k

p (p − 1) (2p − 1) p − p 6 1 − p2

µ

pk+1 − p2k−1 (k − 1) pk − 2 (1 − p) 2

µ +

p−1 2

¶2 pk

k−1 X i=1

ipi


100

Qianli Yang and Chunlan Fu

No. 4 k−1

=

X pk−2 − 1 k+1 p + (ϕ2 (p) − (k − 1) ϕ1 (p)) pk−1 + ϕ1 2 (p) pk−2 ipi 4 i=1 +ϕ2 (p)

1 − pk−2 2 p . 1 − p2

Lemma 2.6. Let N = a1 p + a2 p2 + a3 p3 + · · · + as ps ½ pi−2 − 1 2 = p ϕ2 (ai ) pi+1 + ϕ1 (ai ) ϕ1 (p) ipi + ai p 4 i=1  i−1  X + [ϕ2 (p) − (i − 1) ϕ1 (p)] ai p + ai ϕ1 2 (p) p−1 jpj  j=1    s−1 s s  X X X + ai ϕ1  aj pj  + ai pi aj pj  i=1 j=i+1 j=i+1   Ã ! j s  X X p − 1 a + 1 j +pi  j+ ak − aj pj  .  2 2 s X

B (N, p)

i−1

j=i+1

k=1

Proof. B (N, p) =

X

X

na (n, p) =

na (n, p) +

n<a1 p

n<N

na (n, p)

a1 p6n<N

X

= B (a1 p, p) +

X

(n + a1 p) a (n + a1 p, p)

06n<N −a1 p

X

= B (a1 p, p) +

¡

na (n, p) + na1 + a1 pa (n, p) + a1 2 p

¢

n<N −a1 p

(N − a1 p) (N − a1 p − 1) 2 +a1 pA1 (N − a1 p, p) + a1 2 p (N − a1 p) .

= B (a1 p, p) + B (N − a1 p, p) + a1

Similarly B (N − a1 p, p) X = na (n, p) + n<a2 p2

¡ ¢ = B a2 p2 , p + ¡

¢ = B a2 p2 , p +

X

na (n, p)

a2 p2 6n<N −a1 p

X

¡

¢ ¡ ¢ n + a2 p2 a n + a2 p2 , p

06n<N −a1 p−a2 p2

X

¡

na (n, p) + na2 + a2 p2 a (n, p) + a2 2 p2

¢

n<N −a1 p−a2 p2

¡ ¢¡ ¢ ¡ ¢ ¡ ¢ N − a1 p − a2 p2 N − a1 p − a2 p2 − 1 = B a2 p2 , p + B N − a1 p − a2 p2 , p + a2 2 ¡ ¢ ¡ ¢ +a2 p2 A1 N − a1 p − a2 p2 , p + a1 2 p2 N − a1 p − a2 p2 . ¡ ¢ B N − a1 p − · · · − as−2 ps−2 , p

¡ ¢ as ps (as ps − 1) = B as−1 ps−1 , p + B (as ps , p) + as−1 2


Vol. 7

On mean value computation of a number theoretic function

101

+as−1 ps−1 A1 (as ps , p) + as−1 2 ps−1 (as ps ) . Therefore B (N, p)

=

s X

s−1 ¢ X B ai pi , p + ai

¡

i=1

+

Ã

s−1 X

=

j=1

i=1

ai pi A N −

i=1 s X

N−

i X

!Ã aj pj

 aj pj , p +

j=1

Ã

i P

¡ i

N−

j=1

2 s−1 X

i P

ai 2 pi N −

i=1

! aj pj − 1

i X

 aj pj 

j=1

¢

¡ ¢ ai (ai − 1) p pi − 1 ai (ai − 1) p − 1 2i ai B pi , p + + ip 2 2 2 2 i=1   Ã ! ¶ X j s−1 s X X ai (ai − 1) (2ai − 1) 2i p − 1 a + 1 j + p + ai pi  j+ ak − aj pj  6 2 2 i=1 j=i+1 k=1

s ½ X pi−2 − 1 i+1 = ϕ2 (ai ) p2i + ϕ1 (ai ) ϕ1 (p) ip2i−1 + ai p     4 i−1 s−1 s i=1  X  X X + (ϕ2 (p) − (i − 1) ϕ1 (p)) ai pi−1 + ai ϕ1 2 (p) pi−2 jpj + ai ϕ1  aj pj    j=1 i=1 j=i+1   ! Ã j s s  X X X aj + 1 p−1 j+ ak − aj pj  +ai pi aj pj + pi   2 2 j=i+1

j=i+1

k=1

½ pi−2 − 1 2 p pi−1 ϕ2 (ai ) pi+1 + ϕ1 (ai ) ϕ1 (p) ipi + ai = 4 i=1  i−1  X + [ϕ2 (p) − (i − 1) ϕ1 (p)] ai p + ai ϕ1 2 (p) p−1 jpj  j=1    s−1 s s  X X X j i  + ai ϕ1 aj p + ai p aj pj  i=1 j=i+1 j=i+1   Ã ! j s  X X p−1 aj + 1 +pi  j+ ak − aj pj  .  2 2 s X

j=i+1

k=1

This completes the proofs of the lemma.

§3. Proofs of the theorem In this section, we shall complete the proof of the theorem. Proof of Theorem 1.1. From (2) we have

B(N, P ) =

X n<N

b(n, p)

=

X n<N

1 (n − a(n, p)) P −1


102

Qianli Yang and Chunlan Fu

No. 4

Ã

! X N (N − 1) − a(n, p) 2 n<N µ ¶ N (N − 1) 1 − A(N, p) . p−1 2 1 p−1

= =

(9)

Combining (3) and (9), we have

B(N, p) =

X n<N

    s i ai + 1  1  N (N − 1) X  (p − 1)i X − + aj − ai pi  . b(n, p) = P −1 2 2 2 i=1 j=1

Combining (1)、(4) and (9), we have à [logp N ] µ ¸ · ¸ ¶ i µ· X 1 N (N − 1) N (p − 1)i X N − + − j+1 p p−1 2 2 pj p j=1 i=1 ¸ ¶ µ· ¸ · N N ¶µ· ¸ · ¸ ¶ ! pi − pi+1 p + 1 N N − i+1 p pi . − 2 pi p

C(N, p) =

This completes the proof of the Theorem 1.1. Proof of Theorem 1.2. From Lemma 2.2, we have X

C2 (N, p) =

α2 (n, p) =

n<N

=

1 X

ϕ2 (N ) − 2

2

(p − 1)

2 (n

(p − 1)

n<N

Ã

1

X

2

− a (n, p))

nα (n, p) +

n<N

X

! 2

(10)

a (n, p) .

n<N

Put (2) and Lemma 2.6 in (10) C2 (N, p)

=

(

1 2

(p − 1)

ϕ2 (N ) +

s X

¡ ¡ ¢ pi−1 ai (i − 2) ϕ2 (p) + 1 − 2pi pϕ2 (ai ) +

i=1

 ¡

¢ i

+ (p − 1) ϕ1 (i) ϕ1 (p) + 2i 1 − p ϕ1 (ai ) ϕ1 (p) − 2 ai i

i−1 X j=1

 aj + i − 1 ϕ1 (p)

  2 i−1 i−1 i−2 2 X X p −1 2 ϕ1 (p)  +pϕ1 (ai ) aj + pai  aj  − ai p − 2ai jpj  2 p j=1 j=1 j=1 i−1 X

−2

s−1 X

ai ϕ1 

i=1

+pi 

s X

 aj p

j

+ ai p

j=i+1 s X

j=i+1

Ã

p−1 j+ 2

i

s X

aj pj

j=i+1 j X

ak −

k=1

This completes the proof of the Theorem 1.2.

aj + 1 2

!

  aj pj  . 


Vol. 7

On mean value computation of a number theoretic function

103

Acknowledgments The authors express many thanks to the anonymous referees for valuable suggestions and comments.

References [1] F. Smarandache, only problem, not solutions, Xiquan Publ. House. Chicage, 1993, 54-55. [2] Li Hailong and M. Toda, Elaboration of some results of Srivastava and Choi, Journal of Analysis and Application, 25(2006), 517-533. [3] Li Hailong, On base n and related counting function, Pure and Applied Mathematics, 18(2002), No. 1, 13-15. [4] Li Hailong, Exponential function of integer factorization and its mean value calculation, Pure and applied mathematics, 19(2003), No. 1, 219-222. [5] Li Hailong, Base n Nonzero Digital Multiplication Function and Its Mean Value Formula, Mathematics of practice and cognition, 22(2002), No. 4, 683-686.


Scientia Magna Vol. 7 (2011), No. 4, 104-108

On Kummer’s fourier series for log Γ (x)1 Yulin Lu† , Youcheng Li‡ and Hailong Li] † ] Weinan Teachers College, Weinan, Shaanxi, 714000, P. R. China ‡ Weinan Vocational Technical College, Weinan, Shaanxi, 714000, P. R. China R1 Abstract In Espinosa and Moll [1] , the integral 0 log Γ(x)ζ(z, x)dx is evaluated using the Fourier coefficients an , bn of log Γ (x) found in [2]. However, in both [2] and [5], these coefficients appear as 12 an and 12 bn . In view of this, we derive in this note Kummer’s Fourier series for log Γ (x) by which we evaluate the above integral. Keywords Gamma function, kummer’s fourier series, malmsten’s formula, hurwitz zeta-fun -ction, class function.

§1. Introduction and the main result Let ζ(s, x), (0 < x 6 1) denote the Hurwitz zeta-function defined by ζ(s, x) =

∞ X

1 s , σ = Re s > 1 (n + x) n=0

(1)

and let ζ(s) = ζ(s, 1) denote the Riemann zeta-function. Let Γ(x) denote the gamma function defined by Z∞ Γ(x) = e−t tx−1 dt, Re x > 0. (2) 0

The Hurwitz zeta-function ζ(s, x) satisfies the functional equation (0 < x 6 1) ´ iΓ(1 − z) ³ πiz − πiz 2 l 2 l ζ(s, x) = − e (x) − e (1 − x) , 1−z 1−z 1−z (2π) where ls (x) =

∞ X e2πinx , σ>1 ns n=1

(3)

(4)

is the polylogarithm function. We understand that these functions are meromorphically continued over C. Espinosa and R1 Moll [1, Example 6.1] and Hashimoto [3, Corollary 3] evaluate the integral 0 log Γ(x)ζ(z, x)dx in closed form. The former appealed to their theorem and used the Fourier coefficients an and bn of log Γ (x) [2] , while the latter used Lerch’s formala Γ(x) log √ = ζ 0 (0, x). 2π 1 This

work is supported by the N. S. F. (10271093) of P. R. China.

(5)


Vol. 7

On Kummer’s fourier series for log Γ (x)

105

However, both in [2] and [5], the Fourier coefficients are stated as 12 an and 12 bn and do not lead directly to the Fourier expansion (11) below for logΓ(x). In view of this, we shall elaborate on the proof in [5] for the same, and using it, we shall prove the following Theorem 1.1. For 0 < Re z < 1, we have Z

1

ζ(z − 1) 1 Γ(1 − z) πz 0 − cos ζ (2 − z) z−1 π (2π)1−z 2 1 Γ(1 − z) πz ζ(2 − z), + sin 1−z 2 (2π) 2

log Γ(x)ζ(z, x)dx = (γ + log 2π) 0

(6)

where γ indicates the Euler constant.

§2. Proof of theorem We need some lemmas. Lemma 1. For 0 < Re z < 1 we have Z 1 ζ(z, x)dx = 0,

(7)

0

Z

1

xζ(z, x)dx = − 0

ζ(z − 1) . z−1

(8)

For Re z > 0 Z

Z

1

A1 (x)ζ(z, x)dx = − 0

1

log(2 sin πx)ζ(z, x)dx 0

=

Γ(1 − z) 1−z

(2π)

sin

πz ζ(2 − z), 2

(9)

where A1 (x) indicates the first Clausen function A1 (x) = − log(2 sin πx), 0 < x < 1.

(10)

Proof can he found in [1] or [3]. Lemma 2. (Kummer’s Fourier series, [5, p. 17, (35)]). For 0 < x < 1, ∞ X Γ(x) 1 log n log √ = A1 (x) − (γ + log 2π)B1 (x) + sin 2πnx, 2 πn 2π n=1

where B1 (x) = x − 12 is the first Bernoulli polynomial. Proof. We reproduce the proof sketched in [5, p.17] more in detail. By the reciprocity relation π Γ(z)Γ(1 − z) = , sin πz we may write for 0 < Re z < 1, 1 sin πz 1 log Γ(z) = − log + (log Γ(z) − log Γ(1 − z)) . 2 π 2

(11)

(12)


106

Yulin Lu, Youcheng Li and Hailong Li

No. 4

Substituting Malmsten’s formula [5, p.16, (25)], ¶ Z ∞µ 1 − e−(z−1)t et dt, log Γ(z) = z−1− 1 − e−t t 0

(13)

we deduce that log Γ(z) = Writing

1 1 1 log 2π + A1 (z) + 2 2 2

e−(z−1)t −e−zt −t e 1−e−t

as

sinh( 12 −z )t sinh 2t

1 Γ(z) = A1 (z) + log √ 2 2π

Z

Z

µ (2z − 1)e−t +

0

e−(z−1)t − e−zt −t e 1 − e−t

dt . t

(14)

, we deduce Kummer’s expression [5, p.16, (35)]

à −t

(2z − 1) e 0

¢ ! ¡ sinh 12 − z t dt + , 0 < Re z < 1. t sinh 2t

(15)

Now we compute the Fourier sine coefficient ¡ ¢ ! Z 1 Z Ã sinh 12 − x t dt 1 ∞ −t sin 2πnx 2xe + dx bn = 2 2 0 t sinh 2t 0 µ ¶ ¶ µ Z 1 Z ∞ Z 1 1 dt 1 sin 2πnx sinh − x tdx . = 2e−t x sin 2πnxdx + t 2 sinh 2t 0 0 0 Since µ sin 2πnx sinh

¶ µµ ¶ ¶ 1 1 − x t = −i sin 2πnx sinh − x it 2 2 ¶ µ ¶¶ µ µ i 1 1 = . cos (2πn + it) x − it − cos (2πn − it) x + it 2 2 2

We obtain µ ¶ · 1 e−t 1 1 1 bn = + sin (2πn + it) x − it 2πn t 2 t sinh 2t 2πn + it 0 µ ¶¸1 ! 1 1 − sin (2πn − it) x + it dt 2πn − it 2 0 µ ¶¶ Z ∞µ i it 1 1 e−t 1 1 = + 2 sinh + dt. 2πn t 2 t sinh 2t 2 2πn + it 2πn − it 0 Z

Hence

µ

µ

¶ ¶ Z ∞µ 4πn 1 −t dt 1 1 dt −t − e = − e . (16) 2 + (2πn)2 2+1 t πn t πn t t 0 0 ³ ´ 1 1 e−t −e−2πnt We rewrite the integrand as 1+t + (cos t − e−t ) 1t and apply the 2 − cos t t + t following formulas. ¶ Z ∞µ 1 dt γ= − cos t (17) 2 1 + t t 0 Z

bn =

[5, p.6, (36) = P.5, (28); in (36), t must be t2 ], Z ∞ ¢ dt ¡ −t e − e−zt log z = , t 0

Re z > 0

[5, p.16, (28)]

(18)


Vol. 7

On Kummer’s fourier series for log Γ (x)

and

Z

µ

¶ 1 dt − e−t 1+t t

γ= 0

We need to prove that

Z

¡

cos t − e−t

0

[5, p.5, (24)].

107

(19)

¢ dt = 0. t

Which can be done by subtracting (17) from (19) and noting that the resulting integral Z ∞ dt t2 − t = 0. 2 (t + 1)(t + 1) t 0 Hence it follows that

1 (γ + log 2πn). πn From (15) and (20), we now deduce for 0 < x < 1 that bn =

∞ ∞ ∞ X X X Γ(x) 1 1 γ + log 2πn log √ = A1 (x) + bn sin 2πnx = cos 2πnx + sin 2πnx. 2 2n πn 2π n=1 n=1 n=1

(20)

(21)

Where we used the Founer series for A1 (x): A1 (x) = − log 2πnx =

∞ X 1 cos 2πnx. n n=1

(22)

Recalling the counterpart of (22) for B1 (x), we conclude (11) from (21), B1 (x) = −

∞ 1 X sin 2πnx , 0 < x < 1. π n=1 n

(23)

This completes the proof. Proof. Solving (11) for A1 (x) and substituting in (9), we deduce that ! Z 1Ã ∞ X Γ(x) log n 1 log √ + (γ + log 2π)(x − ) − sin 2πnx ζ(z, x)dx 2 πn 2π 0 n=1 =

πz 1 Γ(1 − z) sin ζ(2 − z) 2 (2π)1−z 2

whence we see, on using (7) and (8), that Z 1 Z 1 Γ(x) log Γ(x)ζ(z, x)dx = log √ ζ(z, x)dx 2π 0 0 ζ(z − 1) 1 Γ(1 − z) πz = (γ + log 2π) sin + ζ(2 − z) + I z−1 2 (2π)1−z 2 say, where I=

1 π

Z 0

∞ 1X

log n sin 2πnxζ(z, x)dx. n n=1

Changing the order of integration and summation in (25), we find that Z ∞ 1 X log n 1 sin 2πnζ(z, x)dx. I= π n=1 n 0

(24)

(25)


108

Yulin Lu, Youcheng Li and Hailong Li

No. 4

R1 The Fourier sine coefficients bn = 2 0 sin 2πnxζ(z, x)dx are evaluated in [1, Proposition 2.1] but we give a proof in the lines of that of Corollary 1 [4] . We use (3) and the expression 2πinx −e−2πinx sin 2πnx = e and proceed as in [4]: 2i bn = −2 =− =

Z

Γ(1 − z) 1−z

2 (2π)

Γ(1 − z) 1−z

(2π) Γ(1 − z) 1−z

(2π)

Hence I=

Z

1

¡

e2πinx − e−2πinx

¢³

e

πiz 2

l1−z (x) − e

−πiz 2

´ l1−z (1 − x) dx

0 1

³ −e

−πiz 2

e2πinx l1−z (1 − x) − e

πiz 2

´ e−2πinx l1−z (x) dx

0

n1−z cos

πz . 2

∞ πz X log n πz 0 1 Γ(1 − z) 1 Γ(1 − z) cos cos =− ζ (2 − z). 1−z π (2π) 2 n=1 n2−z π (2π)1−z 2

(26)

Substituting (26) in (24), we conclude (6), completing the proof.

Acknowledgement The author would like to thank Professors S. Kanemitsu for their help and useful discussions.

References [1] O. Espinosa and V. Moll, On some integrals involving the Hurwitz zeta-function, Ramanujan J., 6(2002), 259-188. [2] I. S. Gradshteyn and I. M. Ryzhik, Tables of Integrals, Series and Products, Academic Press, New York, 1994. [3] M. Hashimoto, Examples of the Hurwitz transforms, to appear. [4] S. Kanemitsu, Y. Tanigawa and J. H. Zhang, Evaluation of Spannanintegrals of the product of zeta-functions, to appear. [5] H. M. Srivastava and J. S. Choi, Series associated with the Zeta and releted functions, Kluwer Academic Publishers, Dordrecht etc, 2001.


Scientia Magna Vol. 7 (2011), No. 4, 109-113

On two inequalities for the composition of arithmetic functions J´ozsef S´andor Department of Mathematics, Babe¸s-Bolyai University, Str. Kog˘alniceanu nr. 1, 400084, Cluj-Napoca, Romania E-mail: jsandor@math.ubbcluj.ro Abstract Let f , g be arithmetic functions satisfying certain conditions. We prove the inequalities f (g(n)) ≤ 2n − ω(n) ≤ 2n − 1 and f (g(n)) ≤ n + ω(n) ≤ 2n − 1 for any n ≥ 1, where ω(n) is the number of distinct prime factors of n. Particular cases include f (n) = Smarandache function, g(n) = σ(n) or g(n) = σ ∗ (n). Keywords Arithmetic functions, inequalities. AMS Subject Classification: 11A25.

§1. Introduction Let S(n) be the Smarandache (or Kempner-Smarandache) function, i.e., the function that associates to each positive integer n the smallest positive integer k such that n|k!. Let σ(n) denote the sum of distinct positive divisors of n, while σ ∗ (n) the sum of distinct unitary divisors of n (introduced for the first time by E. Cohen, see e.g. [7] for references and many informations on this and related functions). Put ω(n) = number of distinct prime divisors of n, where n > 1. In paper [4] we have proved the inequality S(σ(n)) ≤ 2n − ω(n),

(1)

for any n > 1, with equality if and only if ω(n) = 1 and 2n − 1 is a Mersenne prime. In what follows we shall prove the similar inequality S(σ ∗ (n)) ≤ n + ω(n)

(2)

for n > 1. Remark that n + ω(n) ≤ 2n − ω(n), as 2ω(n) ≤ n follows easily for any n > 1. On the other hand 2n − ω(n) ≤ 2n − 1, so both inequalities (1) and (2) are improvements of S(g(n)) ≤ 2n − 1,

(3)

where g(n) = σ(n) or g(n) = σ ∗ (n). We will consider more general inequalities, for the composite functions f (g(n)), where f , g are arithmetical functions satisfying certain conditions.


110

J´ ozsef S´ andor

No. 4

§2. Main results Lemma 2.1. For any real numbers a ≥ 0 and p ≥ 2 one has the inequality pa+1 − 1 ≤ 2pa − 1, p−1

(4)

with equality only for a = 0 or p = 2. Proof. It is easy to see that (4) is equivalent to (pa − 1)(p − 2) ≥ 0, which is true by p ≥ 2 and a ≥ 0, as pa ≥ 2a ≥ 1 and p − 2 ≥ 0. Lemma 2.2. For any real numbers yi ≥ 2 (1 ≤ i ≤ r) one has y 1 + · · · + y r ≤ y1 · · · y r

(5)

with equality only for r = 1. Proof. For r = 2 the inequality follows by (y1 − 1)(y2 − 1) ≥ 1, which is true, as y1 − 1 ≥ 1, y2 − 1 ≥ 1. Now, relation (5) follows by mathematical induction, the induction step y1 · · · yr + yr+1 ≤ (y1 · · · yr )yr+1 being an application of the above proved inequality for the numbers y10 = y1 · · · yr , y20 = yr+1 . Now we can state the main results of this paper. Theorem 2.1. Let f, g : N → R be two arithmetic functions satisfying the following conditions: (i) f (xy) ≤ f (x) + f (y) for any x, y ∈ N; (ii) f (x) ≤ x for any x ∈ N; (iii) g(pα ) ≤ 2pα − 1, for any prime powers pα (p prime, α ≥ 1); (iv) g is multiplicative function. Then one has the inequality f (g(n)) ≤ 2n − ω(n), n > 1. (6) Theorem 2.2. Assume that the arithmetical functions f and g of Theorem 2.1 satisfy conditions (i), (ii), (iv) and (iii)0 g(pα ) ≤ pα + 1 for any prime powers pα . Then one has the inequality f (g(n)) ≤ n + ω(n), n > 1. (7) Proof of Theorem 2.1. As f (x1 ) ≤ f (x1 ) and f (x1 x2 ) ≤ f (x1 ) + f (x2 ), it follows by mathematical induction, that for any integers r ≥ 1 and x1 , · · · , xr ≥ 1 one has f (x1 · · · xr ) ≤ f (x1 ) + · · · + f (xr ).

(8)

αr 1 Let now n = pα 1 · · · pr > 1 be the prime factorization of n, where pi are distinct primes and αi ≥ 1 (i = 1, · · · , r). Since g is multiplicative, by inequality (8) one has α1 αr αr 1 f (g(n)) = f (g(pα 1 ) · · · g(pr )) ≤ f (g(p1 )) + · · · + f (g(pr )).


Vol. 7

111

On two inequalities for the composition of arithmetic functions

By using conditions (ii) and (iii), we get α1 αr αr 1 f (g(n)) ≤ g(pα 1 ) + · · · + g(pr ) ≤ 2(p1 + · · · + pr ) − r. i As pα i ≥ 2, by Lemma 2.2 we get inequality (6), as r = ω(n). Proof of Theorem 2.2. Use the same argument as in the proof of Theorem 2.1, by remarking that by (iii)0

α1 αr r f (g(n)) ≤ (pα+1 + . . . + pα r ) + r ≤ p1 . . . pr + r = n + ω(n). 1

Remark 2.1. By introducing the arithmetical function B 1 (n) (see [7], Ch.IV.28) B 1 (n) =

X

αr 1 pα = pα 1 + . . . + pr

pα kn

(i.e., the sum of greatest prime power divisors of n), the following stronger inequalities can be stated: f (g(n)) ≤ 2B 1 (n) − ω(n),

(60 )

f (g(n)) ≤ B 1 (n) + ω(n),

(70 )

(in place of (6)); as well as:

(in place of (7)). For the average order of B 1 (n), as well as connected functions, see e.g. [2], [3], [8], [7].

§3. Applications 1. First we prove inequality (1). Let f (n) = S(n). Then inequalities (i), (ii) are well-known (see e.g. [1], [6], [4]). Put α+1 g(n) = σ(n). As σ(pα ) = p p−1−1 , inequality (iii) follows by Lemma 2.1. Theorem 2.1 may be applied. 2. Inequality (2) holds true. Let f (n) = S(n), g(n) = σ ∗ (n). As σ ∗ (n) is a multiplicative function, with σ ∗ (pα ) = pα +1, inequality (iii)0 holds true. Thus (2) follows by Theorem 2.2. 3. Let g(n) = ψ(n) be the Dedekind arithmetical function; i.e., the multiplicative function whose value of the prime power pα is ψ(pα ) = pα−1 (p + 1). Then ψ(pα ) ≤ 2pα − 1 since pα + pα−1 ≤ 2pα − 1 ⇐⇒ pα−1 + 1 ≤ pα ≤ pα−1 (p − 1) ≥ 0, which is true, with strict inequality. Thus Theorem 2.1 may be applied for any function f satisfying (i) and (ii). 4. There are many functions satisfying inequalities (i) and (ii) of Theorems 2.1 and 2.2.


112

J´ ozsef S´ andor

No. 4

Let f (n) = log σ(n). As σ(mn) ≤ σ(m)σ(n) for any m, n ≥ 1, relation (i) follows. The inequality f (n) ≤ n follows by σ(n) ≤ en , which is a consequence of e.g. σ(n) ≤ n2 < en (the last inequality may be proved e.g. by induction). Remark 3.1. More generally, assume that F (n) is a submultiplicative function, i.e., satisfying F (mn) ≤ F (m)F (n), for m, n ≥ 1. (i0 ) Assume also that F (n) ≤ en .

(ii0 )

Then f (n) = log F (n) satisfies relations (i) and (ii). 5. Another nontrivial function, which satisfies conditions (i) and (ii) is the following   p, if n = p (prime); f (n) =  1, if n = composite or n = 1.

(9)

Clearly, f (n) ≤ n, with equality only if n = 1 or n = prime. For y = 1 we get f (x) ≤ f (x) + 1 = f (x) + f (1); when x, y ≥ 2 one has f (xy) = 1 ≤ f (x) + f (y). 6. Another example is f (n) = Ω(n) = α1 + · · · + αr ,

(10)

αr 1 for n = pα 1 . . . pr ; i.e., the total number of prime factors of n. Then f (mn) = f (m) + f (n), as αr 1 Ω(mn) = Ω(m) + Ω(n) for all m, n ≥ 1. The inequality Ω(n) < n follows by n = pα 1 · · · pr ≥ 2α1 +···+αr > α1 + · · · + αr . 7. Define the additive analogue of the sum of divisors function σ, as follows: If n = α1 r p1 · · · pα r is the prime factorization of n, put

µ Σ(n) = Σ

As σ(n) =

r Y pαi +1 − 1 i

i=1

p−1

, and

pα+1 − 1 p−1

pα+1 −1 p−1

¶ =

r X pαi +1 − 1 i

i=1

pi − 1

.

(11)

> 2, clearly by Lemma 2.2 one has

Σ(n) ≤ σ(n).

(12)

Let f (n) be any arithmetic function satisfying condition (ii), i.e., f (n) ≤ n for any n ≥ 1. Then one has the inequality: f (Σ(n)) ≤ 2B 1 (n) − ω(n) ≤ 2n − ω(n) ≤ 2n − 1,

(13)

for any n > 1. Indeed, by Lemma 2.1 and Remark 2.1, the first inequality of (13) follows. Since B 1 (n) ≤ n (by Lemma 2.2), the other inequalities of (13) will follow. An example: S(Σ(n)) ≤ 2n − 1,

(14)


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which is the first and last term inequality in (13). It is interesting to study the cases of equality in (14). As S(m) = m if and only if m = 1, 4 or p (prime) (see e.g. [1], [6], [4]) and in Lemma 2.2 there is equality if ω(n) = 1, while in Lemma 2.1, as p = 2, we get that n must have the form n = 2α . Then Σ(n) = 2α+1 − 1 and 2α+1 − 1 6= 1, 2α+1 − 1 6= 4, 2α+1 − 1 = prime; we get the following theorem: There is equality in (14) iff n = 2α , where 2α+1 − 1 is a prime. In paper [5] we called a number n almost f -perfect, if f (n) = 2n − 1 holds true. Thus, we have proved that n is almost S ◦ Σ-perfect number, iff n = 2α , with 2α+1 − 1 a prime (where “◦”denotes composition of functions).

References [1] Ch. Ashbacher, An introduction to the Smarandache function, Erhus Univ. Press, Vail, 1995. [2] P. Erd¨os and A. Ivi´c, Estimates for sums involving the largest prime factor of an integer and certain related additive functions, Studia Sci. Math. Hung., 15(1980), 183-199. [3] J. M. de Koninck and A. Ivi´c, Topics in arithmetical functions, Notas de Matematica, North Holland, 1980. [4] F. Luca and J. S´andor, On the composition of a certain arithmetic function, Functiones et Approximatio, 41(2009), 185-209. [5] J. S´andor, On the composition of some arithmetic functions, Studia Univ. Babe¸s-Bolyai, Math., 34(1989), 7-14. [6] J. S´andor, Geometric theorems, diophantine equations and arithmetic functions, New Mexico, 2002. [7] J. S´andor, D. S. Mitrinovi´c and B. Crstici, Handbook of number theory I, Springer Verlag, 2006. [8] T. Z. Xuan, On some sums of large additive number theoretic functions (Chinese), Beijing Shifan Daxue Xuebao, 1984, No. 2, 11-18.


Scientia Magna Vol. 7 (2011), No. 4, 114-120

Compactness and proper maps in the category of generated spaces Ghasem Mirhosseinkhani Department of Mathematics, Hormozgan University, P. O. Box 3995, Bandarabbas, Iran E-mail: gh.mirhosseini@yahoo.com Abstract In this paper we present the notion of relative C-compactness which is a generalization of the notion of compactness in the category T opC of C-generated spaces. Also we shall study proper maps in T opC , in particular, we show that proper maps in the categories T op of all topological spaces, core compactly generated spaces, locally compactly generated spaces and compactly generated spaces coincide. Keywords Generated space, compactness, proper map. AMS Subject Classification Codes: 18B30, 54D30, 54C10.

§1. Introduction and preliminaries Recall that a continuous map f : X → Y in the category T op of topological spaces is called proper if the product map idZ × f : Z × X → Z × Y is closed, for every space Z, where idZ : Z → Z is the identity map. This is equivalent to f being universally closed, in the sense that every pullback of f is a closed map. There exist many characterizations of proper maps [1,3] , the useful characterizations of them related to compactness are presented in [5]. In particular, a continuous map f : X → Y is proper if and only if f is a closed map and the set f −1 {y} is compact for every point y ∈ Y . Proper maps were worked categorically by Clementino, Giuli and Tholen, as the notion of c-compact maps, where c is a closure operator, see [2] for details. Also some categorically properties of proper maps are discussed in [4], [8] and [9]. Let C be a fixed collection of spaces, referred to as generating spaces. By a probe over a space X we mean a continuous map from one of the generating spaces to X. The C-generated topology CX on a space X is the final topology of the probes over X, that is, the finest topology making all probes continuous. We say that a topological space X is C-generated, if X = CX. The category of continuous maps of C-generated spaces is denoted by T opC . In particular, if C consists of core compact spaces, locally compact spaces, compact Hausdorff spaces, the one-point compactification of the countable discrete space respectively, then we refer to C-generated spaces as core compactly generated spaces, locally compactly generated spaces, compactly generated spaces, sequentially generated spaces, see [7]. A collection C of


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generating spaces is called productive if every generating space is exponentiable, and also the topological product of any two generating space is C-generated. If C is productive, then T opC is a cartesian closed category. For C-generated spaces X and Y , we write X ×C Y for the binary product in the category T opC , which is equal to C(X × Y ), see [7]. Indeed, in general the topology of X ×C Y is finer than the topological product X × Y , but if the product space X × Y is itself C-generated, then X × Y = X ×C Y . A continuous map f : X → Y in the category T opC is called proper if the product map idZ ×f : Z ×C X → Z ×C Y is closed, for every C-generated space Z. In this paper we shall study proper maps in T opC . We first present the notion of relative C-compactness and C-compactness and next we present some characterizations of those maps. All maps in this paper are assumed to be continuous. Theorem 1.1.[7] Let C be a productive class of generating spaces. (i) If X and Y are C-generated spaces with Y exponentiable in T op, then the topological product X × Y is C-generated. (ii) If X and Y are C-generated, then X ×C Y = X ×E Y , where E denotes the class of all exponentiable spaces. (iii) If A, B, Y are C-generated and q : A → B is a topological quotient, then the map q × idY : A ×C Y → B ×C Y is a topological quotient.

§2. Relative C-compactness and C-compactness A generalization of compactness is the notion of relative compactness, that is, for arbitrary subsets S and T of a topological space X, we say that S is relatively compact in T , written S ¿ T , if, for every open cover of T , there exist finitely many elements in the cover that cover S. The notion of relative compactness, restricted to open sets, plays an important role in the study of core compact spaces (exponentiable spaces) and generated spaces [6,7] . For an arbitrary collection C of generating spaces, the relation ¿C , on subsets of a topological space X, is defined by S ¿C T if and only if there is a C-probe P : C → X and open subsets U ¿ V ⊆ C, such that S ⊆ P (U ) and P (V ) ⊆ T . If C is productive, then the exponential topology [X ⇒C Y ] has subbasic open sets [S, V ]C = {f | S ¿C f −1 (V )}, where S ⊆ X is arbitrary and V ⊆ Y is open [7] . In this section, we give the notion of relative C-compactness, which is a generalization of relative compactness and C-compactness. Also we present necessary and sufficient conditions for relative C-compactness. A useful characterization of relative compactness is presented in [5], that is, S ¿ T if and only if for every space Z, every z ∈ Z and every open subset W of Z × X, such that {z} × T ⊆ W , then V × S ⊆ W , for some neighborhood V of z. This is an idea for the following definition: Definition 2.1. Let S, T and Q be subsets of a C-generated space X. (i) We say that S is relatively C-compact in T , written S ¿C T , if for every C-generated space Z, every z ∈ Z and every open subset W of Z ×C X, such that {z} × T ⊆ W , then V × S ⊆ W , for some neighborhood V of z. (ii) We say that Q is C-compact, if the relation Q ¿C Q holds.


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Remark 2.1. By definition of interior, the relation S ¿C T holds if and only if for every C-generated space Z and every open subset W of Z ×C X, {z ∈ Z | {z} × T ⊆ W } ⊆ {z ∈ Z | {z} × S ⊆ W }◦ . Therefore a subset Q of a C-generated space X is C-compact if and only if for every C-generated space Z and every open subset W of Z ×C X, the set {z ∈ Z | {z} × Q ⊆ W } is open. Proposition 2.1. Let S and T be subsets of a C-generated space X. (i) If C is productive, then S ¿C T implies S ¿C T . (ii) If C is productive and X is a core compact space, then S ¿ T implies S ¿C T . Proof. (i) Suppose S ¿C T . Then there is a C-probe P : C → X and open subsets U ¿ V ⊆ C, such that S ⊆ P (U ) and P (V ) ⊆ T . Let Z be a C-generated space, W ⊆ Z ×C X be an open and assume that {z} × T ⊆ W . Applying the map idZ × P : Z ×C C → Z ×C X, we have {z} × V ⊆ {z} × P −1 (T ) ⊆ (id × P )−1 (W ). By Theorem 1.1 part (i), Z ×C C = Z × C, and hence there is a neighborhood G of z, such that G × U ⊆ (id × P )−1 (W ). Thus G × S ⊆ W , as desired. (ii) Let Z be a C-generated space, W ⊆ Z ×C X be an open and assume that {z} × T ⊆ W . By Theorem 1.1 part (i), Z ×C X = Z × X, so there is a neighborhood V of z, such that V × S ⊆ W , as desired. Recall that a C-generated space X is called C-Hausdorff, if its diagonal is closed in X ×C X, and that is C-discrete, if its diagonal is open in X ×C X [5] . Theorem 2.1. Let X and Y be C-generated spaces. (i) If F is a closed set of X and F ¿C X, then F is C-compact. (ii) If X is C-Hausdorff and S ¿C T in X, then S¯ ⊆ T . (iii) If f : X → Y is a map and S ¿C T in X, then f (S) ¿C f (T ) in Y . (iv) If S ¿C T in X and A ¿C B in Y , then S × A ¿C T × B in X ×C Y . Proof. The proofs are modifications of the classical proofs, so we prove only part (iv). Let Z be a C-generated space, W ⊆ Z ×C X ×C Y be an open and assume that {z} × T × B ⊆ W . Then for every t ∈ T , {(z, t)} × B ⊆ W , so there is a neighborhood Vt of (z, t), such that S Vt × A ⊆ W . Now let W 0 = t∈T Vt . Then W 0 ⊆ Z ×C X is open and {z} × T ⊆ W 0 . Thus there is a neighborhood Vz of z, such that Vz × S ⊆ W 0 , and hence Vz × S × A ⊆ W 0 × A ⊆ W , as desired. The Sierpinski space is the space S with two points 1 and 0, such that {1} is open but {0} is not. We denote by OC X the lattice of open sets of X endowed with the topology that makes the bijection U 7→ χU : OC X → SX into a homeomorphism, where the exponential is calculated in T opC . We henceforth assume that the Sierpinski space is a C-generated space. The following lemma can be found in [5]. Lemma 2.1. Let X be a C-generated space. (i) The topology of OC X is finer than the Scott topology. (ii) The topology of OC X coincides with the Scott topology if C generates all compact Hausdorff spaces. ¯ : Z → OC X defined by (iii) A set W ⊆ Z ×C X is open if and only if its transpose W ¯ (z) = {x ∈ X | (y, x) ∈ W } is continuous. W


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(iv) A set W ⊆ Z ×C X is open if and only if for every x ∈ X, the set Vx = {z ∈ Z | (z, x) ∈ W } is open and also for every Scott open set O of OZ, the set UO = {x ∈ X | Vx ∈ O} is open. (v) The set {(U, x) ∈ OC X ×C X | x ∈ U } is open in the C-product. For a C-generated space X and an arbitrary subset S of X, we denote by OS the set {U ∈ OC X | S ⊆ U } of OC X. ¯ −1 (OS ) = Lemma 2.2. If W is an open set of Z ×C X, then for every subset S of X, W ¯ is the map defined in Lemma 2.1. {z ∈ Z | {z} × S ⊆ W }, where W Proof. ¯ −1 (OS ) ⇔ W ¯ (z) ∈ OS z∈W ¯ (z) ⇔ S⊆W ⇔

{z} × S ⊆ W

⇔ z ∈ {z ∈ Z | {z} × S ⊆ W }. Theorem 2.2. Let X be a C-generated space. Then the following are equivalent: (i) S ¿C T in X. (ii) OT ⊆ OS ◦ , where OS ◦ is the interior of OS in the space OC X. Proof. (i)⇒(ii) Let U ∈ OT . By Lemma 2.1, the set W = {(U, x) ∈ OC X ×C X | x ∈ U } is open and {U } × T ⊆ W . Thus there is an open neighborhood O of U , such that O × S ⊆ W , which shows that U ∈ OS ◦ , as desired. (ii)⇒(i) Let Z be a C-generated space, W ⊆ Z ×C X be an open. By assumption, −1 ¯ ¯ −1 (OS ◦ ), where W ¯ is the map defined in Lemma 2.1. Thus by Lemma 2.2, W (OT ) ⊆ W ◦ {z ∈ Z | {z} × T ⊆ W } ⊆ {z ∈ Z | {z} × S ⊆ W } , and hence by Remark 2.1, the result follows. Corollary 2.1. A subset Q of a C-generated space X is C-compact if and only if the set {U ∈ OC X | Q ⊆ U } is open in the space OC X. Proof. By Theorem 2.2, we have that Q ¿C Q ⇔ OQ ⊆ OQ ◦ ⇔ OQ = OQ ◦ . Corollary 2.2. Every compact set is C-compact and if the class C generates all compact Hausdorff spaces, the converse holds. Proof. By definition of the Scott topology a subset Q of a C-generated space X is compact if and only if the set {U ∈ OC X | Q ⊆ U } is Scott open. Thus by Lemma 2.1 and Corollary 2.1, the result follows.

§3. Proper maps In this section we present some properties of proper maps in T opC , in particular, we show that f is a proper map in one of the categories, core compactly generated spaces, locally compactly generated spaces, compactly generated spaces, if and only if it is a proper map in the category T op of topological spaces.


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Ghasem Mirhosseinkhani

No. 4

Proposition 3.1. If D and C are two productive classes of generating spaces such that D ⊆ C, then the inclusion functor i : T opD → T opC reflects proper maps. Proof. By Theorem 1.1 part (ii), the finite products in the categories T opC and T opD coincide. Thus if f ∈ T opD is a proper map in T opC , then it is a proper map in T opD . Remark 3.1. A map g : A → B is closed if and only if for every open set U ⊆ A, the set B \ g(A \ U ) is open. But an easy calculation shows that this set is {b ∈ B | g −1 {b} ⊆ U }. Thus a map g : A → B is closed if and only if for every open set U ⊆ A, the set {b ∈ B | g −1 {b} ⊆ U } is open. Theorem 3.1. A map f : X → Y is proper in T opC if and only if for every C-generated space Z and every open set W ⊆ Z ×C X, the set {(z, y) ∈ Z ×C Y | {z} × f −1 {y} ⊆ W } is open. Proof. By Remark 3.1, we have that f is a proper map if and only if for every C-generated space Z and every open set W ⊆ Z ×C X, the set {(z, y) ∈ Z ×C Y | (idZ × f )−1 {(z, y)} ⊆ W } is open. Definition 3.1. Let f : X → Y be a map in T opC . We say that f reflects relative Ccompactness, if for arbitrary subsets S and T of Y , such that S ¿C T , then f −1 (S) ¿C f −1 (T ). Theorem 3.2. If f : X → Y is a proper map in T opC , then f reflects relative Ccompactness. Proof. Let S ¿C T in Y , W be an open subset of Z ×C X, and z ∈ Z such that, {z} × f −1 (T ) ⊆ W . Then by Theorem 3.1, the set M = {(z, y) | {z} × f −1 (y) ⊆ W } is open. Since {z} × T ⊆ M , by definition of relative C-compactness, V × S ⊆ M for some neighborhood V of z. Therefore V × f −1 (S) ⊆ W , as desired. Corollary 3.1. If f : X → Y is a proper map in T opC , then: (i) f is a closed map and the set f −1 (Q) is C-compact, for every C-compact set Q of Y . (ii) f is a closed map and the set f −1 {y} is C-compact, for every point y in Y . Proof. Since the one-point space is a C-generated space, so if Z is the one-point space, then every proper map is closed. Singletons are compact and hence are C-compact, so by Theorem 3.2, the result follows. We know that the converse of Corollary 3.1 in T op holds, but we show that if the class C is productive, then the converse of Corollary 3.1 in T opC holds. Remark 3.2. Recall that the saturation of a productive C is the collection C¯ of C-generated spaces which are exponentiable in T op. A space is C-generated if and only if it is a quotient of ¯ see Lemma 5.3 in [7]. a space in C, Lemma 3.1. Let f : X → Y be a closed map in T opC , such that the set f −1 {y} is C-compact, for every point y in Y . Then for every C-generated space Z, which is exponentiable in T op and every open set W ⊆ Z ×C X, the set {(z, y) ∈ Z ×C Y | {z} × f −1 {y} ⊆ W } is open. Proof. Let Z ∈ T opC be an exponentiable space and W ⊆ Z ×C X be open and assume that M = {(z, y) ∈ Z ×C Y | {z} × f −1 {y} ⊆ W }. By Remark 2.1, the set Vy = {z ∈ Z | (z, y) ∈ M } = {z ∈ Z | {z} × f −1 {y} ⊆ W } is open, for every y in Y . To show that M is open, let O be a Scott open set of OZ. By Lemma 2.1 part (iv), it suffices to show that the set UO = {y ∈ Y | Vy ∈ O} is open. Let y0 ∈ Y be such that Vyo ∈ O. Since Z is exponentiable,


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for every z ∈ Vyo , there is an open neighborhood Uz of z such that Uz ¿ Vyo . By definition S of the Scott topology, there is a finite set I of Vyo , such that z∈I Uz ∈ O. Suppose that T ¯ −1 (Oz )} Oz = {V ∈ OZ | Uz ¿ V }. By Remark 3.1, the set G = {y ∈ Y | f −1 {y} ⊆ z∈I W ¯ is the map defined in Lemma 2.1. Now we show that is an open neighborhood of y0 , where W ¯ (x), and hence G ⊆ UO . Let y ∈ G. Then for every x ∈ f −1 {y} and every z ∈ I, Uz ¿ W S T ¯ z∈I Uz ⊆ x∈f −1 {y} W (x) = Vy . Therefore Vy ∈ O, as desired. Theorem 3.3. Let f : X → Y be a map in T opC . If the class C is productive, then the following are equivalent: (i) f is a proper map in T opC . (ii) For every C-generated space Z and every open set W ⊆ Z ×C X, the set {(z, y) ∈ Z ×C Y | {z} × f −1 {y} ⊆ W } is open. (iii) f is a closed map and the set f −1 (Q) is C-compact, for every C-compact set Q of Y . (iv) f is a closed map and the set f −1 {y} is C-compact, for every point y in Y . Proof. By Theorem 3.1 and Corollary 3.1, (i)⇔(ii)⇒(iii)⇒(iv). (iv)⇒(ii) Let Z ∈ T opC and W ⊆ Z ×C X be an open subset and assume that M = {(z, y) ∈ Z ×C Y | {z} × f −1 {y} ⊆ W }. By Remark 3.2, there is a quotient map q : C → Z, ¯ By Lemma 3.1, the set G = {(c, y) ∈ C ×C Y | {c} × f −1 {y} ⊆ (q × idX )−1 (W )} with C ∈ C. is open. But an easy calculation shows that G = (q × idY )−1 (M ), by Theorem 1.1 part (iii), q × idY is a quotient map, and hence the set M is open, as desired. Corollary 3.2. (i) If the class C generates all compact Hausdorff spaces, then the inclusion functor i : T opC → T op preserves proper maps. (ii) If the class C is productive, then the inclusion functor i : T opC → T op reflects proper maps. Proof. (i) Let f ∈ T opC be a proper map. Then by Corollary 3.1, f is closed and the set f −1 {y} is C-compact, for every point y ∈ Y . By Corollary 2.2, every C-compact set is compact, so f is a proper map in T op. (ii) By Corollary 2.2 and Theorem 3.3, the result follows. Corollary 3.3. Since every compact Hausdorff space is locally compact and every locally compact space is core compact, therefore by Corollary 3.2, f is a proper map in one of the categories, core compactly generated spaces, locally compactly generated spaces, compactly generated spaces, if and only if it is a proper map in the category T op of all topological spaces.

References [1] N. Bourbaki, General topology, Addison-Wesley, London, 1(1988). [2] M. M. Clementino, E. Giuli and W. Tholen, Topology in a category: compacness, Portugaliae Mathematica, 53(1996), 397-433. [3] M. M. Clementino and D. Hofmann, On some special classes of continouous maps, Open problems in topology II, Chaper 4, (2007), 367-376. [4] M. M. Clementino, D. Hofmann and W. Tholen, The convergence approach to exponentiable maps, Portugaliae Mathematica, 60(2003), 139-160.


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[5] M. H. Escard´ o, Notes on compactness, University of Birmingham, unpublished notes, 8th April 2005. [6] M. H. Escard´ o and R. Heckmann, Topologies on spaces of continuous functions, Topology Proceedings, 26(2001-2002), No. 2, 545-565. [7] M. H. Escard´ o, J. D. Lawson and A. Simpson, Comparing cartesian closed categories of (core) compactly generated spaces, Topology and its Applications, 143(2004), 105-145. [8] G. Richter and W. Tholen, Perfect maps are exponentiable-categorically, Theory and Applications of Categories, 16(2001), No. 8, 457-464. [9] W. Tholen, A categorical guide to separation, compactness and perfectness, Homology, Homotopy and Applicatins, 1(1999), 147-161.



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