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Journal of Inequalities and Applications Volume 2008, Article ID 263413,10pages 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,[email protected]

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

Recommended by Vijay Gupta

Let SH 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 zk2akzk, gz k∞1bkzk|b1| <

1. In this paper, we introduce the classMHn, λ, αof functionsfh

––

gwhich are harmonic inU.

A sufficient coefficient of this class is determined. It is shown that this coefficient bound is also nec-essary for the classM––

Hn, λ, αiffnz h

––

gnMHn, λ, α, wherehz z−∞k2|ak|zk, gnz

−1n

k1|bk|zkandn ∈ N0. Coefficient conditions, such as distortion bounds, convolution

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

Hn, λ, α, are

ob-tained.

Copyrightq2008 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 functionf uivis a complex-valued harmonic function in a complex domain Cif bothuandvare real harmonic inC. In any simply connected domainD ⊂C, we can write

f hg, wherehandgare analytic inD. We callhthe analytic part andgthe coanalytic part off. A necessary and sufficient condition forf to be locally univalent and sense-preserving in Dis that|hz|>|gz|inD; see2.

Denote bySH the class of functionsf hg that are harmonic, univalent, and

sense-preserving in the unit diskU {z : |z| < 1}for whichf0 h0 fz0−1 0. Then for

f hg ∈ SH, we may express the analytic functionshandgas

hz z

k2

akzk, gz

k1

(2)

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

coan-alytic part offis zero. Also, denote bySH the subclasses ofSH consisting of functionsf that

mapUonto starlike domain.

Forf hg given by 1.1, we define the derivative operator introduced by authors

see1offas

Dn

λfz Dnλhz −1nDnλgz, n, λ∈N0 N∪ {0}, z∈U, 1.2

whereDnλhz zk2knCλ, kakzk, Dnλgzk1knCλ, kbkzk, andCλ, k kλλ−1.

We letMHn, λ, αdenote the family of harmonic functionsfof the form1.1such that

Re

Dn1

λ fz

Dn

λfz

> α, 0≤α <1, 1.3

whereDnλfis defined by1.2.

If the coanalytic part off hgis identically zero, then the classMHn, λ, αturns out

to be the classRnλαintroduced by Al-Shaqsi and Darus1for the analytic case.

LetMHn, λ, αdenote that the subclass ofMHn, λ, αconsists of harmonic functions

fnhgnsuch thathandgnare of the form

hz z−∞

k2

akzk, g

nz −1n

k1

bkzk. 1.4

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

example,MH0,0, αSHαis 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≡ HKαis the class of sense-preserving, harmonic, univalent functionsf which are convex of order α in U, that is, ∂/∂θarg∂/∂θfre > α. Note that the classes

S

H and HKαwere introduced and studied by Jahangiri3. Also we notice that the class

MHn,0, αis the class of Salagean-type harmonic univalent functions introduced by Jahangiri et al.4; andMH0, λ, αis the class of Ruscheweyh-type harmonic univalent functions stud-ied by Murugusundaramoorthy and Vijaya5.

In 1984, Clunie and Sheil-Small2investigated the classSHas 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 Silvia7, and Jahangiri3,8

studied the harmonic univalent functions. Jahangiri and Silverman 9 prove the following theorem.

Theorem 1.1. Letf hg given by1.1. If

k2

k akbk≤1−b1, 1.5

thenfis sense-preserving, harmonic, and univalent inUandfSHconsists of functions inSHwhich

are starlike inU.

The condition1.5is also necessary iff∈ THMH0,0,0.

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also necessary for functions in the classMHn, λ, α. Also, we obtain distortion theorems and characterize the extreme points for functions inMHn, λ, α. Closure theorems and application of neighborhood are also obtained.

2. Coefficient bounds

We begin with a sufficient coefficient condition for functions inMHn, λ, α. Theorem 2.1. Letf hg be given by1.1. If

k1

kαak kαbkknCλ, k≤21−α, 2.1

wherea1 1, n, λ ∈ N0, Cλ, k kλλ−1, and0 ≤ α < 1, thenf is sense-preserving, harmonic,

univalent inU, andfMHn, λ, α.

Proof. Ifz1/z2, then

f z1

f z2

h z1

h z2

≥1−g z1

g z2

h z1

h z2

1−

k1bk zk1−z k 2

z1−z2

k2ak zk1−zk2

>1−

k1kbk 1−∞k2kak

≥1−

k1 kαknCλ, k/1−αbk

1−∞k2 kαknCλ, k/1−αak ≥0,

2.2

which proves univalence. Note thatf is sense-preserving inU. This is because

hz1

k2

kak|z|k−1

>1−

k2

kαknCλ, k

1−α ak

≥∞

k1

kαknCλ, k

1−α bk

>

k1

kαknCλ, k

1−α bk|z|

k−1

k1

kbk|z|k−1≥gz.

2.3

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

1αDn

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SubstitutingDnλfzin2.4yields, by2.1, we obtain

1αDn

λfz D1fz−1αDλnfz− Dλn1fz

2−αz

k2

k1−αknCλ, kakzk−−1n

k1

k−1αknCλ, kbkzk

αz

k2

k−1−αknCλ, kakzk −−1n

k1

k1αknCλ, kbkzk

≥21−α|z|

1−∞

k2

kαknCλ, k

1−α ak|z|

k−1∞

k1

kαknCλ, k

1−α bk|z|

k−1

≥21−α

1−

k2

kαknCλ, k

1−α ak

k1

kαknCλ, k

1−α bk

.

2.5

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

The harmonic function

fz z

k2

1−α

kαknCλ, kxkzk

k1

1−α

kαknCλ, kykzk, 2.6

wheren, λ∈ N0and∞k2|xk|

k1|yk| 1 show that the coefficient bound given by2.1is sharp. The functions of the form2.6are inMHn, λ, αbecause

k1

kα

1−αak

1−αbk

knCλ, k 1

k2

xk

k1

yk2. 2.7

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

fnhgn, wherehandgnare of the form1.4.

Theorem 2.2. Letfnhgnbe given by1.4. ThenfnMHn, λ, αif and only if

k1

kαak kαbkknCλ, k≤21−α, 2.8

wherea11, n, λ∈N0, Cλ, k kλλ−1, and0≤α <1.

Proof. SinceMHn, λ, αMHn, λ, α, we only need to prove the “if and only if” part of the

theorem. To this end, for functions fn of the form1.4, we notice that the condition 1.3is

equivalent to

Re

1−αz−∞k2kαknCλ, kakzk−−12nk1kαknCλ, kbkzk

z−∞k2knCλ, kakzk −12n

k1knCλ, kbkzk

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The above required condition2.9must hold for all values ofzinU. Upon choosing the values ofzon the positive real axis, where 0≤zr <1, we must have

1−α−∞k2kαknCλ, kakrk−1−

k1kαknCλ, kbkrk−1 1−∞k2knCλ, kakrk−1

k1knCλ, kbkrk−1

≥0. 2.10

If the condition2.8does not hold, then the numerator in2.10is negative forr sufficiently close to 1. Hence there exist z0 r0 in0,1for which the quotient in2.8is negative. This contradicts the required condition forfnMHn, λ, αand so the proof is complete.

3. Distortion bounds

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

Theorem 3.1. LetfnMHn, λ, α. Then for|z|r <1, one has

fnz≤ 1b1r 1 21

1−α 2−α

1α 2−αb1

r2,

fnz 1b1r 1 21

1−α 2−α

1α 2−αb1

r2.

3.1

Proof. We only prove the left-hand inequality. The proof for the right-hand inequality is similar

and will be omitted. LetfnMHn, λ, α. Taking the absolute value offn, we obtain

fnz

z

k2

akzk −1n

k1

bkzk

≥ 1−b1r

k2

akbkrk

≥ 1−b1rr2

k2

akbk

≥ 1−b1r− 1−

α

2−α21

k2

2−α21

1−α ak

2−α21

1−α bk

r2

≥ 1−b1r− 1−

α

2−α21

k2

kαknCλ, k

1−α ak

kαknCλ, k

1−α bk

r2

≥ 1−b1r

1−α

2−α21

1−1α 1−αb1

r2.

3.2

The functions

fz zb1z 1 21

1−α 2−α

1α 2−αb1

z2,

fz 1−b1z− 1 21

1−α 2−α

1α 2−αb1

z2

3.3

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

Corollary 3.2. If the functionfnhgn, wherehandggiven by1.4are inMHn, λ, α, then

w:|w|< 2

n1λ11 2nλ11α

212−α

2n1λ11 2nλ1 1α 212−α b1

fnU.

3.4

4. Convolution, convex combination, and extreme points

In this section, we show that the classMHn, λ, αis invariant under convolution and convex combination of its member.

For harmonic functions fnz zk∞2akzk −1

n

k1bkz

k and F

nz z

k2Akzk −1

n

k1Bkz k

, the convolution offnandFnis given by

fnFnz fnzFnz z

k2

akAkzk −1n

k1

bkBkzk. 4.1

Theorem 4.1. For 0 ≤ βα < 1, let fnMHn, λ, α and FnMHn, λ, β. Then fnFn

MHn, λ, αMHn, λ, β.

Proof. We wish to show that the coefficients of fnFn satisfy the required condition given in

Theorem 2.2. ForFnMHn, λ, β,we note that|Ak| ≤1 and|Bk| ≤1. Now, for the convolution

functionfnFn, we obtain

k2

kβknCλ, k

1−β akAk

k1

kβknCλ, k

1−β bkBk

≤∞

k2

kβknCλ, k

1−β ak

k1

kβknCλ, k

1−β bk

≤∞

k2

kαknCλ, k

1−α ak

k1

kαknCλ, k

1−α bk≤1,

4.2

since 0≤βα <1 andfnMHn, λ, α. ThereforefnFnMHn, λ, αMHn, λ, β.

We now examine the convex combination ofMHn, λ, α. Let the functionsfnjzbe defined, forj 1,2, . . . ,by

fnjz z

k2

ak,jzk −1n

k1

bk,jzk. 4.3

Theorem 4.2. Let the functions fnjz defined by 4.3 be in the class MHn, λ, α for every j 1,2, . . . , m. Then the functionstjzdefined by

tjz m

j1

cjfnjz, 0≤cj ≤1 4.4

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Proof. According to the definition oftj, we can write

tjz z

k2

m

j1

cjak,j

zk −1nk1

m

j1

cjbn,j

zk. 4.5

Further, sincefnjzare inMHn, λ, αfor everyj1,2, . . ., then by2.8, we have

k1

kα

m

j1

cjak,j

m

j1

cjbk,j

knCλ, k

m

j1

cj

k1

kαan,j kαbn,jknCλ, k

m

j1

cj21−α≤21−α.

4.6

Hence the theorem follows.

Corollary 4.3. The classMHn, λ, αis closed under convex linear combination.

Proof. Let the functionsfnjz j 1,2defined by4.1be in the classMHn, λ, α. Then the

functionΨzdefined by

Ψz μfn1z 1−μfn2z, 0≤μ≤1 4.7

is in the classMHn, λ, α. Also, by takingm 2,t1 μ, andt2 1−μinTheorem 4.1, we have the corollary.

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

Theorem 4.4. Letfnbe given by1.4. ThenfnMHn, λ, αif and only if

fnz

k1

Xkhkz Ykgnkz

, 4.8

where h1z z, hkz z − 1 − α/kαknCλ, kzk, k 2,3, . . . , gnkz z

−1n1−α/kαknCλ, kzk, k 1,2,3, . . . ,andk1 Xk Yk

1, Xk ≥ 0, Yk ≥ 0. In

particular, the extreme points ofMHn, λ, αarehkandgnk

.

Proof. For the functionsfnof the form4.8, we have

fnz

k1

Xkhkz Ykgnkz

k1

XkYkz

k2

1−α

kαknCλ, kXkzk −1n

k1

1−α

kαknCλ, kYkzk.

4.9

Then

k2

kαknCλ, k

1−α ak

k1

kαknCλ, k

1−α bk

k2

Xk

k1

(8)

and sofn∈clcoMHn, λ, α.

Conversely, suppose thatfn∈clcoMHn, λ, α. Setting

Xk kαk

nCλ, k

1−α ak, 0≤Xk ≤1, k 2,3, . . . ,

Yk kαk

nCλ, k

1−α bk, 0≤Yk ≤1, k1,2,3, . . . ,

4.11

andX11−∞k2Xk

k1Yk. Therefore,fncan be written as

fnz z

k2

akzk −1n

k1

bkzk

z−∞

k2

1−αXk

kαknCλ, kzk −1n

k1

1−αYk

kαknCλ, kzk

z

k2

hkzzXk

k1

gnkzz

Yk

k2

hkzXk

k1

gnkzYkz

1−

k2

Xk

k1

Yk

k1

hkzXkgnkzYk

, as required.

4.12

Using Corollary 4.3 we have clcoMHn, λ, α MHn, λ, α. Then the statement of Theorem 4.4is really forfMHn, λ, α.

5. An application of neighborhood

In this section, we will prove that the functions in a neighborhood ofMHn, λ, αare starlike harmonic functions.

Following10, we defined theδ-neighborhood of a functionf∈ THby

Nδf

Fz z−∞

k2

Akzk

k1

Bkzk,

k2

kakAkbkBkb1−B1≤δ

,

5.1

whereδ >0.

Theorem 5.1. Let

δ 2−α2

nλ

1−1α− 2−α21−1−αb1

2−α21 . 5.2

(9)

Proof. SupposefnMHn, λ, α. LetFn HGn ∈ Nδ fn,where H z−∞k2Akzk and

Gn −1nk1Bkzk. We need to show thatFn ∈ TH. In other words, it suffices to show that

Fnsatisfies the conditionTFk2k|Ak||Bk| |B1| ≤1. We observe that

TF

k2

kAkBkB1

k2

kAkakakBkbkbkB1−b1b1

k2

kAkakBkbk

k2

kakbkB1−b1b1

k2

kAkakBkbkB1−b1

k2

kakbkb1

δb1

k2

kakbk

δb1 1−

α

2−α21

k2

2−α 1−αak

2α 1−αbk

21

δb1

1−α

2−α21

k2

kα

1−αak

1−αbk

knCλ, k

δb1 1−α

2−α21

1−1α 1−αb1

.

5.3

Now this last expression is never greater than one if

δ≤1−b1− 1−

α

2−α21

1−1α 1−αb1

2−α2

nλ11α 2α2nλ11αb

1

2−α21 .

5.4

Acknowledgment

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

References

1K. Al-Shaqsi and M. Darus, “An operator defined by convolution involving the polylogarithms func-tions,” submitted.

2J. Clunie and T. Sheil-Small, “Harmonic univalent functions,”Annales Academiae Scientiarum Fennicae. Series A I, vol. 9, pp. 3–25, 1984.

3J. M. Jahangiri, “Harmonic functions starlike in the unit disk,”Journal of Mathematical Analysis and Applications, vol. 235, no. 2, pp. 470–477, 1999.

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5G. Murugusundaramoorthy and K. Vijaya, “On certain classes of harmonic functions involving Ruscheweyh derivatives,”Bulletin of the Calcutta Mathematical Society, vol. 96, no. 2, pp. 99–108, 2004.

6H. Silverman, “Harmonic univalent functions with negative coefficients,”Journal of Mathematical Anal-ysis and Applications, vol. 220, no. 1, pp. 283–289, 1998.

7H. Silverman and E. M. Silvia, “Subclasses of harmonic univalent functions,”New Zealand Journal of Mathematics, vol. 28, no. 2, pp. 275–284, 1999.

8J. 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.

9J. 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.

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