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Observe thatSHreduces toS, the class of normalized univalent analytic functions, if the coan-alytic part of f is zero.. Also, denote by S∗H the subclasses ofSH consisting of functions f

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Volume 2008, Article ID 263413, 10 pages

doi:10.1155/2008/263413

Research Article

On Harmonic Functions Defined by

Derivative Operator

K Al-Shaqsi and M Darus

School of Mathematical Sciences, Faculty of Science and Technology, Universiti Kebangsaan Malaysia, Bangi 43600 Selangor D Ehsan, Malaysia

Correspondence should be addressed to M Darus, maslina@pkrisc.cc.ukm.my

Received 16 September 2007; Revised 20 November 2007; Accepted 26 November 2007

Recommended by Vijay Gupta

Let S H denote the class of functions f  h ––g that are harmonic univalent and

sense-preserv-ing in the unit disk U  {z : |z| < 1}, where hz  z ∞

k2 a k z k , gz  ∞k1 b k z k |b1| <

1 In this paper, we introduce the class M Hn, λ, α of functions f  h––g which are harmonic in U.

A sufficient coefficient of this class is determined It is shown that this coefficient bound is also

nec-essary for the class M––

Hn, λ, α if f n z  h g––n ∈ MHn, λ, α, where hz  z −∞

k2 |a k |z k , g n z 

−1n∞

k1 |b k |z k and n ∈ N 0 Coefficient conditions, such as distortion bounds, convolution

con-ditions, convex combination, extreme points, and neighborhood for the class M––

Hn, λ, α, are

ob-tained.

Copyright q 2008 K Al-Shaqsi and M Darus 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.

1 Introduction

A continuous function f  u  iv is a complex-valued harmonic function in a complex domain

C if both u and v are real harmonic in C In any simply connected domainD ⊂ C, we can write

f  h  g, where h and g are analytic in D We call h the analytic part and g the coanalytic part

of f A necessary and sufficient condition for f to be locally univalent and sense-preserving in

D is that |hz| > |gz| in D; see 2

Denote bySH the class of functions f  h  g that are harmonic, univalent, and

sense-preserving in the unit diskU  {z : |z| < 1} for which f0  h0  f z0 − 1  0 Then for

f  h  g ∈ SH, we may express the analytic functions h and g as

hz  z ∞

k2

a k z k , gz ∞

k1

b k z k , b1 < 1. 1.1

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Observe thatSHreduces toS, the class of normalized univalent analytic functions, if the

coan-alytic part of f is zero Also, denote by S∗H the subclasses ofSH consisting of functions f that

mapU onto starlike domain

For f  h  g given by 1.1, we define the derivative operator introduced by authors

see 1 of f as

Dn

λ fz  D n

λ hz  −1 nDn

λ gz, n, λ ∈ N0  N ∪ {0}, z ∈ U, 1.2 whereDn

λ hz  z ∞

k2 k n Cλ, ka k z k , D n

λ gz ∞

k1 k n Cλ, kb k z k , and Cλ, k   kλ−1

We let MHn, λ, α denote the family of harmonic functions f of the form 1.1 such that

ReDn1

Dn



whereDn

λ f is defined by 1.2

If the coanalytic part of f  h  g is identically zero, then the class MHn, λ, α turns out

to be the classRn

λ α introduced by Al-Shaqsi and Darus 1 for the analytic case

Let MHn, λ, α denote that the subclass of MHn, λ, α consists of harmonic functions

f n  h  g n such that h and g nare of the form

hz  z −∞

k2

a k z k , g n z  −1 n∞

k1

It is clear that the class MHn, λ, α includes a variety of well-known subclasses of SH For

example, MH0, 0, α ≡ S

Hα is the class of sense-preserving, harmonic, univalent functions

f which are starlike of order α in U, that is, ∂/∂θargfre > α, and MH1, 0, α ≡

MH0, 1, α ≡ HKα is the class of sense-preserving, harmonic, univalent functions f which are convex of order α in U, that is, ∂/∂θarg∂/∂θfre > α Note that the classes

S

H and HKα were introduced and studied by Jahangiri 3 Also we notice that the class

MHn, 0, α is the class of Salagean-type harmonic univalent functions introduced by Jahangiri

et al.4; and MH0, λ, α is the class of Ruscheweyh-type harmonic univalent functions

stud-ied by Murugusundaramoorthy and Vijaya5

In 1984, Clunie and Sheil-Small2 investigated the class SHas well as its geometric sub-classes and obtained some coefficient bounds Since then, there has been several related papers

onSHand its subclasses such that Silverman6, Silverman and Silvia 7, and Jahangiri 3,8 studied the harmonic univalent functions Jahangiri and Silverman 9 prove the following theorem

Theorem 1.1 Let f  h  g given by 1.1 If



k2

then f is sense-preserving, harmonic, and univalent in U and f ∈ S

Hconsists of functions inSHwhich are starlike in U.

The condition1.5 is also necessary if f ∈ TH ≡ MH0, 0, 0.

In this paper, we will give sufficient condition for functions f  h  g, where h and g are given by1.1 to be in the class MHn, λ, α; and it is shown that this coefficient condition is

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also necessary for functions in the class MHn, λ, α Also, we obtain distortion theorems and characterize the extreme points for functions in MHn, λ, α Closure theorems and application

of neighborhood are also obtained

2 Coefficient bounds

We begin with a sufficient coefficient condition for functions in MHn, λ, α.

Theorem 2.1 Let f  h  g be given by 1.1 If



k1

k − αa k   k  αb k  k n Cλ, k ≤ 21 − α, 2.1

where a1  1, n, λ ∈ N0, Cλ, k   kλ−1

λ , and 0 ≤ α < 1, then f is sense-preserving, harmonic, univalent in U, and f ∈ MHn, λ, α.

Proof If z1/ z2, then



f z1 − f z2

h

z1 − h z2



 ≥ 1 −g z1 − g z2

h

z1 − h z2





 1 −

 ∞k1 b k

z k

1− z k

2

z1− z2 ∞k2 a k

z k

1− z k

2





>1−

∞

k1 kb k

1−∞k2 ka k

≥1−

∞

k1

k  αk n Cλ, k/1 − α k

1−∞k2 k − αk n Cλ, k/1 − α k  ≥0,

2.2

which proves univalence Note that f is sense-preserving inU This is because

hz ≥ 1 −∞

k2

ka k |z| k−1

> 1 −∞

k2

k − αk n Cλ, k

1− α a k

≥∞

k1

k  αk n Cλ, k

1− α b k

>∞

k1

k  αk n Cλ, k

1− α b k |z| k−1≥∞

k1

kb k |z| k−1gz.

2.3

Using the fact that Rew > α if and only if |1 − α  w| ≥ |1  α − w|, it suffices to show that

1 − αD n

λ fz  D n1

λ fz − 1  αD n

λ fz − D n1

λ fz ≥ 0. 2.4

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λ fz in 2.4 yields, by 2.1, we obtain

1 − αD n

λ fz  D n1

λ fz − 1  αD n

λ fz − D n1





2− αz 



k2

k  1 − αk n Cλ, ka k z k− −1n∞

k1

k − 1  αk n Cλ, kb k z k





−



 −αz 



k2

k − 1 − αk n Cλ, ka k z k − −1n∞

k1

k  1  αk n Cλ, kb k z k





≥21−α|z| 1−∞

k2

k−αk n Cλ, k

1− α a k |z| k−1∞

k1

kαk n Cλ, k

1− α b k |z| k−1



≥ 21 − α 1−∞

k2

k − αk n Cλ, k

1− α a k −∞

k1

k  αk n Cλ, k

1− α b k.

2.5

This last expression is nonnegative by2.1, and so the proof is complete

The harmonic function

fz  z ∞

k2

1− α

k − αk n Cλ, k x k z k 



k1

1− α

k  αk n Cλ, k y k z k , 2.6 where n, λ∈ N0and∞

k2 |x k| ∞k1 |y k|  1 show that the coefficient bound given by 2.1 is sharp The functions of the form2.6 are in MHn, λ, α because



k1

k − α

1− α a k   k  α

1− α b kk n Cλ, k  1 ∞

k2

x k ∞

k1

In the following theorem, it is shown that the condition 2.1 is also necessary for functions

f n  h  g n , where h and g nare of the form1.4

Theorem 2.2 Let f n  h  g n be given by1.4 Then f n ∈ MHn, λ, α if and only if



k1

k − αa k   k  αb k  k n Cλ, k ≤ 21 − α, 2.8

where a1 1, n, λ ∈ N0, Cλ, k   kλ−1

λ , and 0 ≤ α < 1.

Proof Since MHn, λ, α ⊂ MHn, λ, α, we only need to prove the “if and only if” part of the theorem To this end, for functions f n of the form1.4, we notice that the condition 1.3 is equivalent to

Re 1 − αz −∞k2 k − αk n Cλ, ka k z k− −12n∞

k1 k  αk n Cλ, kb k z k

z −∞k2 k n Cλ, ka k z k −12n∞

k1 k n Cλ, kb k z k



≥ 0. 2.9

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The above required condition2.9 must hold for all values of z in U Upon choosing the values

of z on the positive real axis, where 0 ≤ z  r < 1, we must have

1− α −∞k2 k − αk n Cλ, ka k r k−1−∞k1 k  αk n Cλ, kb k r k−1

1−∞k2 k n Cλ, ka k r k−1∞k1 k n Cλ, kb k r k−1 ≥ 0. 2.10

If the condition2.8 does not hold, then the numerator in 2.10 is negative for r sufficiently close to 1 Hence there exist z0  r0 in0, 1 for which the quotient in 2.8 is negative This

contradicts the required condition for f n ∈ MHn, λ, α and so the proof is complete.

3 Distortion bounds

In this section, we will obtain distortion bounds for functions in MHn, λ, α.

Theorem 3.1 Let f n ∈ MHn, λ, α Then for |z|  r < 1, one has

f n z ≤ 1  b1

2n λ  1



1− α

2− α

1 α

2− α b1r2,

f n z ≥ 1 − b1

2n λ  1



1− α

2− α

1 α

2− α b1r2.

3.1

Proof We only prove the left-hand inequality The proof for the right-hand inequality is similar and will be omitted Let f n ∈ MHn, λ, α Taking the absolute value of f n, we obtain

f n z z −∞

k2

a k z k −1n∞

k1

b k z k





≥ 1−b1



k2

a k   b k k

≥ 1−b1 2



k2

a k   b k

2 − α2 n λ  1

∞

k2

2 − α2 n λ  1

1− α a k   2 − α2 n λ  1

1− α b kr2

2−α2 n λ1

∞

k2

k−αk n Cλ, k

1− α a k   kαk n Cλ, k

1− α b kr2

≥ 1−b1

1− α

2 − α2 n λ  1



1−1 α

1− α b1r2.

3.2 The functions

fz  z  b1z  1

2n λ  1



1− α

2− α

1 α

2− α b1z2, fz  1−b1

2n λ  1



1− α

2− α

1 α

2− α b1z2

3.3 for|b1| ≤ 1 − α/1  α show that the bounds given inTheorem 3.1are sharp

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The following covering result follows from the left-hand inequality inTheorem 3.1.

Corollary 3.2 If the function f n  h  g n , where h and g given by 1.4 are in MHn, λ, α, then



w : |w| < 2n1 λ  1 − 1 −

2n λ  1 − 1 α

2n1 λ  1 − 1 − 2n λ  1  1 α

2n λ  12 − α b1⊂f n U.

3.4

4 Convolution, convex combination, and extreme points

In this section, we show that the class MHn, λ, α is invariant under convolution and convex

combination of its member

For harmonic functions f n z  z − ∞k2 a k z k  −1n∞k1 b k z k and F n z  z −

∞

k2 A k z k −1n∞

k1 B k z k , the convolution of f n and F nis given by

f n ∗F n z  f n z∗F n z  z −∞

k2

a k A k z k −1n∞

k1

Theorem 4.1 For 0 ≤ β ≤ α < 1, let f n ∈ MHn, λ, α and F n ∈ MHn, λ, β Then f n ∗F n

∈ MHn, λ, α ⊂ MHn, λ, β.

Proof We wish to show that the coefficients of f n ∗F n satisfy the required condition given in

function f n ∗F n, we obtain



k2

k − βk n Cλ, k

1− β a k A k ∞

k1

k  βk n Cλ, k

1− β b k B k

≤∞

k2

k − βk n Cλ, k

1− β a k ∞

k1

k  βk n Cλ, k

1− β b k

≤∞

k2

k − αk n Cλ, k

1− α a k ∞

k1

k  αk n Cλ, k

1− α b k  ≤ 1,

4.2

since 0≤ β ≤ α < 1 and f n ∈ MHn, λ, α Therefore f n ∗F n ∈ MHn, λ, α ⊂ MHn, λ, β.

We now examine the convex combination of MHn, λ, α.

Let the functions f n j z be defined, for j  1, 2, , by

f n j z  z −∞

k2

a k,j z k −1n∞

k1

Theorem 4.2 Let the functions f n j z defined by 4.3 be in the class MHn, λ, α for every j 

1, 2, , m Then the functions t j z defined by

t j z m

j1

are also in the class MHn, λ, α, wherem j1 c j  1.

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Proof According to the definition of t j, we can write

t j z  z −∞

k2



j1

c j a k,j



z k −1n∞

k1



j1

c j b n,j



Further, since f n j z are in MHn, λ, α for every j  1, 2, , then by 2.8, we have



k1

k − α



j1

c j a k,j k  αm

j1

c j b k,jk n Cλ, k



m

j1

c j



k1

k − αa n,j   k  αb n,j  k n Cλ, k



≤m

j1

c j21 − α ≤ 21 − α

4.6

Hence the theorem follows

Corollary 4.3 The class MHn, λ, α is closed under convex linear combination.

Proof Let the functions f n j z j  1, 2 defined by 4.1 be in the class MHn, λ, α Then the

functionΨz defined by

is in the class MHn, λ, α Also, by taking m  2, t1  μ, and t2  1 − μ inTheorem 4.1, we have the corollary

Next we determine the extreme points of closed convex hulls of MHn, λ, α denoted by clcoMHn, λ, α.

Theorem 4.4 Let f n be given by1.4 Then f n ∈ MHn, λ, α if and only if

f n z ∞

k1

where h1z  z, h k z  z − 1 − α/k − αk n Cλ, kz k , k  2, 3, , g n k z  z 

−1n 1−α/k αk n Cλ, kz k , k  1, 2, 3, , and ∞k1 X k  Y k  1, X k ≥ 0, Y k ≥ 0 In particular, the extreme points of MHn, λ, α areh k

and

g n k



Proof For the functions f nof the form4.8, we have

f n z ∞

k1

X k h k z  Y k g n k z

∞

k1

X k  Y k z −∞

k2

1− α

k − αk n Cλ, k X k z k −1n



k1

1− α

k  αk n Cλ, k Y k z k .

4.9

Then



k2

k − αk n Cλ, k

1− α a k ∞

k1

k  αk n Cλ, k

1− α b k ∞

k2

X k∞

k1

Y k  1 − X1≤ 1, 4.10

Trang 8

and so f n ∈ clcoMHn, λ, α.

Conversely, suppose that f n ∈ clcoMHn, λ, α Setting

X k  k − αk n Cλ, k

1− α a k , 0≤ X k ≤ 1, k  2, 3, ,

Y k  k  αk n Cλ, k

1− α b k , 0≤ Y k ≤ 1, k  1, 2, 3, ,

4.11

and X1 1 −∞k2 X k−∞k1 Y k Therefore, f ncan be written as

f n z  z −∞

k2

a k z k −1n∞

k1

b k z k

 z −∞

k2

1 − αX k

k − αk n Cλ, k z k −1n



k1

1 − αY k

k  αk n Cλ, k z k

 z ∞

k2

h k z − z X k∞

k1

g n k z − z Y k

∞

k2

h k zX k∞

k1

g n k zY k  z



1−∞

k2

X k−∞

k1

Y k



∞

k1

h k zX k  g n k zY k , as required.

4.12

Using Corollary 4.3 we have clcoMHn, λ, α  MHn, λ, α Then the statement of

5 An application of neighborhood

In this section, we will prove that the functions in a neighborhood of MHn, λ, α are starlike

harmonic functions

Following10, we defined the δ-neighborhood of a function f ∈ TH by

Nδ f  Fz  z −∞

k2

A k z k−∞

k1

B k z k ,∞

k2

k a k − A k   b k − B k   b1− B1 ≤ δ, 5.1

where δ > 0.

Theorem 5.1 Let

δ  2 − α2

n λ  1 − 1  α − 2 − α2 n λ  1 − 1 − α 1

ThenNδ MHn, λ, α ⊂ TH.

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Proof Suppose f n ∈ MHn, λ, α Let F n  H  G n ∈ Nδ

f n , where H  z −∞k2 A k z k and

G n  −1n∞k1 B k z k We need to show that F n ∈ TH In other words, it suffices to show that

F nsatisfies the conditionTF ∞k2 k|A k |  |B k |  |B1| ≤ 1 We observe that

TF ∞

k2

k A k   B k   B1

∞

k2

k A k − a k  a k   B k − b k  b k   B1− b1 b1

∞

k2

k A k − a k   B k − b k ∞

k2

k a k   b k   B1− b1  b1





k2

k A k − a k   B k − b k   B1− b1∞

k2

k a k   b k   b1

 δ  b1 ∞

k2

k a k   b k

 δ  b1  1− α

2 − α2 n λ  1



k2



2− α

1− α a k   2  α

1− α b k2n λ  1

≤ δ  b1  1− α

2 − α2 n λ  1



k2

k − α

1− α a k   k  α

1− α b kk n Cλ, k

≤ δ  b1  1− α

2 − α2 n λ  1



1−1 α

1− α b1.

5.3

Now this last expression is never greater than one if

δ ≤ 1 − b1 − 1− α

2 − α2 n λ  1



1−1 α

1− α b1

 2 − α2

n λ  1 − 1  α − 2 − α2 n λ  1 − 1 − α 1

5.4

Acknowledgment

The work presented here was supported by Fundamental Research Grant Scheme UKM-ST-01-FRGS0055-2006

References

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Series A I, vol 9, pp 3–25, 1984.

3 J M Jahangiri, “Harmonic functions starlike in the unit disk,” Journal of Mathematical Analysis and

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4 J M Jahangiri, G Murugusundaramoorthy, and K Vijaya, “Salagean-type harmonic univalent

func-tions,” Southwest Journal of Pure and Applied Mathematics, no 2, pp 77–82, 2002.

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Ruscheweyh derivatives,” Bulletin of the Calcutta Mathematical Society, vol 96, no 2, pp 99–108, 2004.

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Anal-ysis and Applications, vol 220, no 1, pp 283–289, 1998.

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Mathematics, vol 28, no 2, pp 275–284, 1999.

8 J M Jahangiri, “Coefficient bounds and univalence criteria for harmonic functions with negative co-efficients,” Annales Universitatis Mariae Curie-Skłodowska Sectio A, vol 52, no 2, pp 57–66, 1998.

9 J M Jahangiri and H Silverman, “Harmonic univalent functions with varying arguments,”

Interna-tional Journal of Applied Mathematics, vol 8, no 3, pp 267–275, 2002.

10 S Ruscheweyh, “Neighborhoods of univalent functions,” Proceedings of the American Mathematical

So-ciety, vol 81, no 4, pp 521–527, 1981.

... 10

5 G Murugusundaramoorthy and K Vijaya, ? ?On certain classes of harmonic functions involving

Ruscheweyh derivatives,”...

Trang 5

The above required condition2.9 must hold for all values of z in U Upon choosing the values

of...

4 Convolution, convex combination, and extreme points

In this section, we show that the class MHn, λ, α is invariant under convolution and convex

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