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Wright Type Hypergeometric Function and Its Properties

Snehal B. Rao1, Jyotindra C. Prajapati2, Ajay K. Shukla3 1Department of Applied Mathematics, The M.S. University of Baroda, Vadodara, India 2Department of Mathematical Sciences, Faculty of Applied Sciences, Charotar University of

Science and Technology, Anand, India

3Department of Applied Mathematics and Humenities, S.V. National Institute of Technology, Surat, India Email: [email protected], [email protected], [email protected]

Received January 7, 2013; revised February 6, 2013; accepted March 6,2013

Copyright © 2013 Snehal B. Rao et al. This is an open access article distributed under the Creative Commons Attribution License,

which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

ABSTRACT

 

s v

 

Let s and z be complex variables,  s be the Gamma function, and

 

s

s

v

 

 for any complex be the v

generalized Pochhammer symbol. Wright Type Hypergeometric Function is defined (Virchenko et al. [1]), as:

 

 

  

2 1

0

, ; ; ; k

k

a b

c

R a b c z

b c

 

  

  !,

k

k z

k k where 

0,

; ,a b c, ; Re

 

a 0,Re

 

b 0, Re

 

c 0;

which is a direct generalization of classical Gauss Hypergeometric Function 2 1F a b c z

, ; ;

2R a b c1 ;z

. The principal aim of this paper is to study the various properties of this Wright type hypergeometric function

, ; ; ; which includes differentiation and integration, representation in terms of pFq and in terms of Mellin-Barnes type integral. Euler (Beta) transforms, Laplace transform, Mellin transform, Whittaker transform have also been obtained; along with its relation-ship with Fox H-function and Wright hypergeometric function.

Keywords: Euler Transform; Fox H-Function; Wright Type Hypergeometric Function; Laplace Transform; Mellin

Transform; Whittaker Transform; Wright Hypergeometric Function

1. Introduction and Preliminaries

The Gauss Hypergeometric Function is defined [2] as:

   

 

, ! 2,

k k k

k

a b

0

, ; ;

1, 0, 1,

k F a b c z

z c

  

z

c k

 

 

 

; and (1.1)

The Generalized Hypergeometric Function, in a classi- cal sense has been defined [3] by

 

 

1 ; , , ;1

, ! 1 ;

p q

k p k

k 1

1

1 0 1 , , ;

, , , ,

1, p

p q p q

q

k

k q

k

a a z

F F a a

b b

a a

b b

p q z

 

 

 

  

 

 

b b z

z k

 

   

(1.2)

and no denominator parameter equal to zero or negative integer.

E. Wright [4] has further extended the generalization of the hypergeometric series in the following form

 

1 1

0 1 1

; ! p q

n

p p

n q q

z

n n z

n

n n

   

   

   

   

r

(1.3)

where  and t are real positive numbers such that

1 1

1 q t p r 0.

t r

 

 

 

When r and t are equal to 1, Equation (1.3) dif-fers from the generalized hypergeometric function pFq by a constant multiplier only.

The generalized form of the hypergeometric function has been investigated by Dotsenko [5], Malovichko [6] and one of the special cases considered by Dotsenko [5] as

(2)

 

 

   

,

2R1 z 2 1R a b c, ; ; , ;z

   

0 !

n

n

a n b n

c z

a b n

c n

   

 

  

 

 

 

and its integral representation expressed as

(1.4)

 

 

  

 

1

1 1

0

1 c b 1 ad ,

b

c

ttztt

  

 

(1.5) ,

2R1 z

c b b

 

  

where Re

 

 

Euler’s formul

Re 0

cb  . This is the analogue of

a for the Gauss’s hypergeometric function 001 Virchenko et a

[3]. In 2 l. [1] defined the said Wright

Type Hypergeometric Function by taking   0

   in

(1.4) as

 

 

 

  

2 1 2 1

0

, ; ; ;

!

k k

k

R z R a b c z

a b k

c

b c k k z ; 0,z 1.

  

  

  

 

(1.6)

If 1

 , then (1.3) reduces to a Gauss’s hyper- geo-metric function. Galue et al. [7] and Virchenko et al. [1] investigated some properties of the function

2 1R a b c, ; ; ; z .

The following well-known facts have been prepared for studying various properties of the function

2 1R a b c, ; ; ; z .

Euler (Beta) transform (Sneddon [8]): of the function

 

The Euler transform f z is defined

 

z d

Laplace transform (Sneddon [8]):

The Laplace transform of unction

as

 

: ,

1 a1

1

b1 .

B f z a b

z  zf z (1.7) 0

the f f z

0

is de- fined as

 

e sz

 

d .

L f z f z z

 

(1.8)  Mellin transform (Sneddon [8]):

The Mellin transform of the function f x

 

is de-fined as

 

; s1

 

d

,

 

0

Re 0,

M f x s x f x x f

 

 

 

 

s

(1.9) s

then

 

1

 

; 1

 

sd .

2πiL

f xM fs x

fs xs (1.10)

 Wright generalized hypergeometric functio stava and Manocha [9]), denoted by

n (Sriva- pq, i

as

s defined

1, 1 , , p, p ;

1 1 1 0

1

, , , , ;

! p q

q q

p k

i i i

q

k j j

j

A A z

 

B B

A k z

k B k

 

 

 

 

 

 

 

  

 

(1.11)

  

1 1 1,

, 1

1 1

1 , , , 1 ,

,

0,1 , 1 , , , 1 ,

p p p

p q

q q

A A

H z

B B

 

 

   

 

 

 

 (1.12)

where

1 1 ,

,

1 1

, , , ,

, , , ,

p p m n

p q

q q

a a

H z

b b

 

 

 

 

 

 

 denotes the Fox

ion [10].

2. Basic Properties of the Function

H-funct

2

R a b c

1

,

 

z

Theorem 2.1

 

 

 

If , ,a b c; Re a 0, Re b 0, Re c 0; then

2 1 2 1

2 1

, ; ; ; , ; 1; ;

d

, ; 1; ;

d

c R a b c z c R a b c z

z R a b c z

z

 

 

   

  (2.1 ).1

 

 

2 1 2 1

0

, ; ; ; , 1; ; ;

1 1

, ! 1 .

k k

k

R a b c z R a b c z

a b k

c z

a z

b c k k

b

   

  

   

      

  

(2.1.2)

In particular,

 

2 1 2 1

1

, ; 1; , 1; 1;

1, ; ;

c

F a b c z F a b c z

az

F a b c z

   



 

(2.1.3)

Proof. 2 1 

 

  

  

 

 

 

  

2 1

1 0

0

0

2 1 2 1

d

, ; 1; ;

d 1

1 !

! 1

1 !

, ; ; ; , ; 1; ; ,

k k

k

k k

k

k k

k

z R a b c z

z

a b k

c k z

z

b c k k

a b k

c c z

b c k k

a b k

c c z

b c k k

c R a b c z c R a b c z

 

 

  

 

 

 

 

 

 

  

   

  

  

   

   

    

(3)

which is the (2.1.1). Now,

 

  

  

  

 

  

 

2 1 2 1

0

0

0

1

, ; ; ; , 1; ; ;

! 1

1 !

1 b

  

1 1

1

! 1

1

1 1 1 !

1

k k

k

k k

k

k k

k

k k

k

R a b c z R a b c z

a b k

c z

b c k k

a b k

c z

b c k k

c

a b k z b k

c k k b

a b k

c z

b b c k k

a z b

c

   

 

   

  

 

 

 

  

   

   

   

    

    

 

      

  

    

      

    

 

 

 

1 1

1

0

0

1 1 1

1 1 1 !

1 1

1 1

!

1 1

, !

k k

k

k k

k

k k

k

a b k z

b c k k

c a z

b b

a b k z

c k k

a b k

c z

a z

b c k k

  

 

  

  

 

 

       

 

   

 

  

        

 

      

  

This is the proof of (2.1.2).

For c1 and substituting  1 in above result, this

will immediatel s to particul .1.3). 

Theorem 2.2 1)If

 

0, Re 0

c

ar case (2 y lead

 

 

 

, , , ;

Re 0, Re 0, Re

and then

a b c

a b

 

 

 

 

1

1 1

c

u  

 

2 1 0

1 , d

, ; ; ;

u R a zu u

a b c   z

(2.2.1)

2 1

c R

 

; ; ; c

b c

 

  

2)If

 

 

 

 

, , , , ;

Re 0, Re 0, Re 0, Re 0

and then

a b c

a b c

 

 

   

  

 

 

1 1

2 1 1

2 1

, ; ; ; d

, ; ; ;

x

c

t c c

x

.

s s t R a b c s t s

x t c R a b c x t

 

 

  

  

 

 

 

  

    

(2.2.2) 3)

 

 

 

, , ;

Re 0, Re 0, Re 0

and then

a b c

a b c

 

  

1 2 1 0

2 1

, ; ; ; d

, ; 1; ; .

z c

c

t R a b c t t

z

R a b c z

c

 

 

 

(2.2.3)

In particular,

1 2 1 0

2 1

, ; ; d

, ; 1; .

z c

c

t F a b c t t

z

F a b c z

c

 

2.2.4)

Proof. 1)

(

 

 

 

 

  

 

 

  

  

  

  

 

  

1

1 1

2 1 0

1

1 1

0 0

1

1 1

0 0

0

1 , ; ; ;

1 d

1 d

!

!

c

k

c k

k

k c k k

k

k k

k

c

u u R a b c zu

a b

c

u u

b c

a b k c z

u u u

b c k k

a b k

c z

c

b c k k

 

 

 

 

 

 

 

 

  

 

 

 

 

 

 

  

 

 

  

 

   

  

 

     

     

  

 

c 2 1R a b c

, ;  ; ; .z

  

  

which concludes the proof of (2.2.1). 

du

! zu k

u

k k

 

c

  

c

  

(4)

2)

 

 

 

 

  

 

 

1 1

2 1 1

1

1 2 1 1

1 1 1

2 1 0

, ; ; ; d

, ; ; ;

1 , ; ; ;

applying the transformation formula c

t

x

c

t

c c

c

x s s t R a b c s t s

x t

c x t s t

s t R a b c s t

x t

c

u u x t R a b c u x t

s t u

x t

c b

 

 

  

  

  

 

  

 

  

 

 

    

 

 

   

 

 

 

d

d , x

s

x t u

  

 

 

 

 

  

   

 

  

  

1

1 1

0 0

1

1 1

0 0

0 2 1

1 d

!

1 d

!

!

, ; ; ;

k k k

c

c k

k

k k

c k c k

k

k k

c k

k

c

a b k

c u x t

u u x t u

c k k

a b k

c c x t

x t u u u

b c k k

a b k

c x t

x t c

b c k k

x t c R a b c x t

 

 

 

 

 

 

 

    

  

   

  

 

 

 

 

 

     

      

 

     

 

  

     

 

    

.

Therefore,

  

 

1

12 1

, ; ; ;

d

1

 

2 1 , ;

c c

t c

x ss t R a b c s ts x tc R a b c

  

   

 

     

Which is the proof of (2.2.2). 

; ;

.

x

x t

 

 

3)

 

 

  

 

 

 

  

 

  

 

1 1

2 1

0 0

0 0

2 1 0

, ; ; ; d d

! !

1

, ; 1; ; .

1 !

k

z z k

c c k k

k k

k

c c

k

k

t

a b k a b k

c c

t R a b c t t t t

b c k k b c k

z

a b k

c

z z

R a b c z

c b c k k c

 

  

 

 

 

  

 

 

 

   

 

     

 

 

   

 

   

 

 

This leads the proof of (2.2.3).

1 0

d z

c k

t t

k

  

 

 

 

On putting  1, in the above expression immediately leads to (2.2.4). 

Theorem 2.3

 

 

 

c 0, then

, , ;Re 0, Re 0, Re

a b c ab

If

, ; ; ;

 

, ; ; ;

d

c c m c

R a b c z z R a b c m z

z c m

1 1

2 1 2 1

d m

z         

 

   

  (2.3.1)

Proof.

 

 

 

  

 

 

  



 

 

 

  

 

 

1 1

2 1

0

1

1 1

0

, ; ; ;

d d !

1 2

!

!

m m k k c

c k

k

k k c m

k

c m k c m

k

a b k

c z

z R a b c z

z z b c k k

a b k

c k c k c k c m z

k

z

a b k

c c m c

z z

c m b c m k k

 

   

    

  

  

   

   

 

 

  

 

     

    

 

      

 

 

     

 

d d

0

k k

bck

 

2 1R a b c, ; m; ; z .

c m

 

(5)

This establishes (2.3.1).

3. Representation of Wright Type

Hypergeometric Function

,

2 1R a b c, ; ; ; z

2

R a b c

1

  

z

in Terms of the Functio

U

n

p

F

q

sing the definition

 

 

  

2

0 !

k

bck k

  

1 , ; ; ;

k k

a b k

c z

R a b cz

  

, and taking

q

  we have

 

 

 

 

 

 

2 1

1

0 0

1

1

1

, ; ; ;

1 1

, , , , ;

1 1

, , , ;

, ; ;

, ; ;

q

k i k qk

q

k qk k

j

q q

q q

R a b c q z

1

! 1 !

qk

k k

k

qk

k

b i

a q

b z q z

c k c j k

q q

b b b q

a

q q q

F z

c c c q

q q q

a q b

F z

q c

 

   

 

 

 

   

 

 

  

 

 

 

  

 

 

 

  

(3.1)

 

a

 

where  q b; is aq-tuple b b 1 b q 1

q

  

;

, , ,

q q

 

q c; is a q-tuple

c c, 1, ,c q 1

q

  . Convergence criteria for genera

ction

q q

lized hyperfeometric fun

 

 

 

 

1 1, 2, ,

F   0

1 2 1

; , , , ;

k p

p k k

p q

k

q k

z

z  

  

 

 

:

1) If pq function

! q k k

, the pFq converges for all finite .

f p q 1 function

z

2) I , the pFq converges for

1

z  and diverges for 1.

If function

z

3) p q 1, the pFq is divergent for

0 .

If p q 1 nction

z

4) , the fu pFq is absolutely

con-n circle

verge t on the 1 if

1 1

0

q p

j i

j i

 

 

 

 

 

 .

4. Mellin-Barnes Integral Representation of

,

z

Re

2

R a b c

1

  

z

Let

 

;Re a 0,

 

Then

Theorem 4.1

is represented by the Mellin- Barnes integral

 

   

  

 

 

2 1 , ; ; ;

1

d 2πi

s

L R a b c z

c s a s b s

z s

b a c s

 

     

 

 

 

(4.1.1)

 

 

0, ; , ,

Re 0, Re 0.

a b c

b c

   

 

 

where arg

 

z π; the contour of integration beginning at  i and ending at  i , and intended to separate the poles of the integrand at s k k, 0,1,to the left and all the poles at s n a n, 0,1,as well as

, 0,1,

n b

s n

 

  to the right.

Proof. We shall use the sum of residues at the poles

, 0,1,

sk k  to obtain the integral of (4.1.1).

 

 

  

 

   

 

 

    

 

2 1

0

0 , , , ;

!

! 1

1 k k

k

k

k

k k

k R a b c z

a b k

c z

b c k k

c a k b k z

b a c k k

c b k

a k z

c k

 

 

 

 

 

  

  

    

   

  

    

  

(4.1.2) Now

 

0 1

b ak

  

,

 

 

  

 

 

 

   

  

 

 

 

   

 

 

  

 

      

0

 

 

2πi

π

sinπ

1 1

L

s k

k

k

a c s

c s a s b s z

res

b a c s

c

s

b k

a k z

b a k c

  

 

 



 

0

k

0 1

1

k

k k

s s c s

c

1

d

s

c s a s b s z

s b

 

      

 

1

lim s

s

k b s

a sz

s

b a

k

 

      

  

     

 

   

 

 

 

  

     

(4.1.3)

5. Integral Transforms of

2 1

,

 

   

   

 

(4.1.2) and (4.1.3) completes the proof of (4.1.1). 

R a b c

  

z

discussed some useful integral trans- forms like Euler transforms, Laplace transfor , Mellin transform and Whittaker transform.

Theorem 5.1 (Euler (Beta) transforms). In this section we

m

(6)

   

   

   

  

1 2 1 3 2

,1 , , , , ;

,

, , , ;

R a b c

a b x

c c a b                     (5.1.1) 1 1 0

1 , ; ; ; d

z zxzz

 

 

 

 

 

where , , , , , , ;Re 0, Re

Re 0, Re 0, Re 0, Re

a b c a

c            

0, 0, Re b   

0. Proof.

    

  

 

    

  

 

   

 

  

   

   

    

1 1 1 2 1 0

1 , ;

z z R a b

1 0 1 1 1 0 0 0 3 2

; ; d

1 d

!

!

,1 , , , , ;

k k k k k k k

c xz z

xz

b k

a c b k x

z z z

c k b k

c a k b k k

1 1 0 1 d ! k k

z z z

c k b k

a c

x

a b c k k k

a b c a b                                                             

  

, , ,

; , x c   

 

 

This is the pr f (5.1.1). 

Rem 1    

               

  oof o Putting

ark:  in (5.1.1), we get

   

   

   

  

1 1 1 2 1

3 2

1 , ; ; d

,1 , ,1 , , ;

.

,1 , , ;

z F a b c xz z

a b x

c c a b                    (5.1.2) 0

z 

Taking   ,  c and substituting  in place of the notation  ; (5.1.1) re

; ; ; d

; ; , xz z x     (5.1.3 duces to

 

1 1 1 2 1 0 2 1 1 , , , c

z z R a b c

c R a b c

      

Also, considering )

  and  c in (5.1.1), with

replacement of z by

1

1 c

z at 2R1, we get

; ; ; 1 d

; , .

c x z z

x     (5.1.4)

 

2 1 0 2 1 1 , , , ;

z z R a b

c R a b c

   

 1

 

Theorem 5.2 (Laplace transform).

 

   

    

 

, ;

1 2 1

e sz , ; ; ; d

z R a b c xz z

0

3 1

,1 , , , , ;

, x a b s c s a b                (5.2.1) c     

  

 

 

 

 

 

 

 

where , , , , , ; Re 0, Re 0,

Re 0, Re 0, Re 0, Re 0,

Re 0 and 1.

a b c a b

c s x s                 Proof.

    

  

 

 

   

 

 

   

 

 

 

   

    

1 2 1 0 1 0 0 1 0 0 0 3 1

e , ; ; ; d

e d

!

e d

!

!

,1 , , , ,

sz k sz k k k sz k k k k

z R a b c xz z

xz

a c b k

z z

c k b k

c a k b k x

z z

a b c k k

c s a k b k k x

a b c k k s

a b s c a b                                                                                    

 

; , , ; x s c            

This is the proof of (5.2.1). 

    

 

   

Theorem 5.3 (Mellin transform). 1

2 1 0

, ; ; ; d

, s

s

t R a b c t t

c s a s b s

a b c s

                

 (5.3.1)

 

 

 

 

here , , 0, Re 0,

Re 0, Re 0, Re 0.

a b a b

c

s

w c, , s ; Re

  

  

Proof. Putting zt in (4.1.1), we get

  

 

  

   

 

   

  

 

 

2 1 , ; ; ;

π

1

d 2πi

1

s s

L

s

R a b c t

s b

c s a s b s

t s

b a c s

                              

(5.3.2)

where,

 

1 d

2 i

s

L

c a s s

t s

b a c s

         

 d , 2πiL

f s t s

    

 

   

s

.

c s a s b s

f s

a b c s

 

     

   

(7)

Theorem 5.4 (Whittaker transform).

 

 

   

   

  

1 1 2

, 2 1

0

4 2

e , ; ; ; d

1

,1 , , , , ;

2 ,

, , 1 ,

pt

t W pt R a b c t t

a b

p c

p b

c

 

 

 

   

   

     

 

 

 

 

 

(5.4.1)

 

 

0, Re 0,

0. b

  

Proof. To obtain Whittaker transform, we use the fol-lowing integral:

a

 

 

 

 

 

where , , , , , , ; Re

Re 0, Re 0, Re 0, Re

a b c p a

c

  

 

 

  

 

1 2

, 0

e d

1

t v

t W  t

 

 

 

 

 

1 1

2 2 ,

t

v v

v

    

 

where 1.

2 v   Re

Substituting ptv on the L. ces to

H.S. of (5.4.1), it re-du

 

 

   

 

 

 

   

 

1 1

 

  

2

, 2 1

0

0 1

1 2

, 0

1

e , ; ; ; d

1

e d

!

1 1

2 2

1

v

k

v k

v v

W v R a b c v

p p p

c p a k b k

a b c k p

v w v v

k

c p a k b k

c

k k

 

 

 

 

 

     

 

   

   

   

   

      

   

 

 

  

 

 

    

   

       

   

  

0 k

a b  k

 

k

 

   

4 2

   

 

1 !

1

,1 , , , ;

2 .

, 1 , ;

k

k k p

a b

c p

p

a b

c

 

   

   

 

 

 

  

 

 

 

 

     

   

 

 

 

This completes the proof of (5.4.1).

6. Relationship with Some Known Spec

Functions (Fox H-Function, Wright

ergeometric Function)

6.

.1 ), we get

ial

Hyp

1. Relationship with Fox H-Function Using (4 .1

 

   

2 1R a b c, ; ; ; z

  

 

 

 

   

1,22,2

  

 

1

d 2πi

1 ,1 , 1 ,

. 0,1 , 1 ,

s

L

c s a s b s

z s

b a c s

a b

c

H z

c

b a

 

 

     

 

   

   

 

6.2. Relationship with Wright Hypergeome Function

The Generalized Hypergeometric Function

tric

2 1R a b c, ; ; ; z as in (1.3) is

 

  

2 1Rz 2R a b c, ; ; ; z

 

 

1

0

; 0, 1.

!

k k

k

a b k

c

z z

b c k k

  

  

  

 

(6.2.1)

From (1.11) and (6.2.1) yields

 

 

   

   

 

2 1 2 1

2 1

, ; ; ; ,1 , , ;

, ;

R z R a b c z

a b z

c

c

a b

 

 

 

  .

(6.2.2)

dgem

The authors are thankful to the reviewers for their valu- able suggestions to improve the quality of paper.

REFERENCES

[1] N. Virchenko, S. L. Kalla and A. Al-Zamel, “Some Re- sults on a Generalized Hypergeometric Function,” Inte- gral Transforms and Special Functions, Vol. 12, No. 1,

2001, pp. 89-100. doi:10.1080/10652460108819336

7. Acknowle

ents

[2] E. D. Rainville, “Special Functions,” The Macmillan Company, New York, 1960.

[3] A. Erdelyi, et al., “Higher Transcendental Functions,”

McGaw-Hill, New York, 1953-1954.

[4] E. M. Wright, “On the Coefficient of Power Series Hav- ing Exponential Singularities,” Journal London Mathe- matical Society, Vol. s1-8, No. 1, 1933, pp. 71-79.

doi:10.1112/jlms/s1-8.1.71

[5] M. Dotsenko, “On Some Applications of Wright’s Hy-pergeometric Function,” Comptes Rendus de lAcadémie Bulgare des Sciences, Vol. 44, 1991, pp. 13-16.

[6] V. Malovichko, “On a Generalized Hypergeometric Func-tion and Some Integral Operators,” Mathematical Physics,

lts

a-

003, pp.

0014-0

Vol. 19, 1976, pp. 99-103.

[7] L. Galue, A. Al-Zamel and S. L. Kalla, “Further Resu on Generalized Hypergeometric Functions,” Applied M thematics and Computation, Vol. 136, No. 1, 2

17-25. doi:10.1016/S0096-3003(02)0

orms,” Tata i, 1979. H. L. Manocha, “A Treatise on [8] I. N. Sneddon, “The Use of Integral Transf

McGraw-Hill Publication Co. Ltd., New Delh [9] H. M. Srivastava and

(8)

Generating Functions,” John Wiley and Sons/Ellis Hor-wood, New York/Chichester, 1984.

[10] A. M. Mathai, R. K. Saxena and H. J. Haubold, “The

H-Function,” Springer, Berlin, 2010.

References

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