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Volume 2012, Article ID 915625,10pages doi:10.1155/2012/915625

Research Article

Subclass of Multivalent Harmonic Functions with

Missing Coefficients

R. M. El-Ashwah

Department of Mathematics, Faculty of Science (Damietta Branch), Mansoura University, New Damietta 34517, Egypt

Correspondence should be addressed to R. M. El-Ashwah,r [email protected]

Received 20 March 2012; Accepted 8 July 2012

Academic Editor: Attila Gil´anyi

Copyrightq2012 R. M. El-Ashwah. 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.

We have studied subclass of multivalent harmonic functions with missing coefficients in the open unit disc and obtained the basic properties such as coefficient characterization and distortion theorem, extreme points, and convolution.

1. Introduction

A continuous function f u iv is a complex-valued harmonic function in a simply connected complex domain D ⊂ C if bothuand vare real harmonic in D. It was shown by Clunie and Sheil-Small1that such harmonic function can be represented byf hg, wherehandgare analytic inD. Also, a necessary and sufficient condition forfto be locally univalent and sense preserving inDis that|hz|>|gz|see also,2–4.

Denote by Hthe family of functions f hg, which are harmonic univalent and sense-preserving in the open-unit discU{z∈C:|z|<1}with normalizationf0 h0

f

z0−10.

Form ≥ 1, 0 ≤ β < 1,and γ ≥ 0,let Rm, β, γ denote the class of all multivalent harmonic functionsf hg with missing coefficients that are sense-preserving inU, and

h, gare of the form

hz zm

nm1

an1zn1, gz

nm

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and satisfying the following condition:

Re1γeiφzf z

zfzγmeiφ

m≥1; 0≤β <1; γ≥0; φ real, 1.2

where

z

∂θ

zreiθ, fz

∂θf

reiθ. 1.3

We note that:

iRm, β,1 Rm, βwitham1; bm/0see Jahangiri et al.5;

iiR1, β, γ JHα, β, γ see Kharinar and More6;

iiiR1, β,1 GHβ witha2; b1/0see Rosy et al.7and Ahuja and Jahangiri2.

Also, the subclass denoted byTm, β, γconsists of harmonic functionsf hg, so thathandgare of the form

hz zmnm1

an1zn1, gz

nm

bn1zn1 an1; bn1≥0; m≥1; zU. 1.4

We note that:

iTm, β,1 Tm, βwitham1;bm/0 see Jahangiri et al.5;

iiT1, β, γ JHα, β, γ see Kharinar and More6;

iiiT1, β,1 GHβwitha2;b1/0 see Rosy et al.7and Ahuja and Jahangiri2.

From Ahuja and Jahangiri2with slight modification and among other things proved, iffhg is of the form1.1and satisfies the coefficient condition

nm−1

n1−

m1−β |an1|

n1

m1−β |bn1|

≤2 am1;am1bm0, 1.5

then the harmonic function f is sense-preserving, harmonic multivalent with missing coefficients and starlike of orderβ0 ≤ β < 1 inU. They also proved that the condition

1.5is also necessary for the starlikeness of functionfhg of the form1.4.

In this paper, we obtain sufficient coefficient bounds for functions in the class

Rm, β, γ. These sufficient coefficient conditions are shown to be also necessary for functions in the class Tm, β, γ. Basic properties such as distortion theorem, extreme points, and convolution for the classTm, β, γare also obtained.

2. Coefficient Characterization and Distortion Theorem

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Theorem 2.1. Letf hgbe such thathandgare given by1.1. Furthermore, let

nm−1

1γn1−mγβ

m1−β |an1|

1γn1 mγβ

m1−β |bn1|

≤2, 2.1

where am 1andam1 bm 0. Thenf is sense-preserving, harmonic multivalent in Uand

fRm, β, γ.

Proof. To provefRm, β, γ, by definition, we only need to show that the condition2.1

holds forf. Substitutinghg forfin1.2, it suffices to show that

Re

⎧ ⎨ ⎩

1γeiθzhzzgzmβγeiθhz gz

hz gz

⎫ ⎬

⎭≥0, 2.2

wherehz ∂/∂zhzandgz ∂/∂zgz. Substituting forh, g, h, andg in2.2, and dividing bym1−βzm, we obtain ReAz/Bz≥0, where

Az 1

nm1

n11γeiθmβγeiθ

m1−β an1z

nm1

z

z

m

nm1

n11γeiθmβγe

m1−β bn1z

nm1,

Bz 1

nm1

an1znm1

z

z

m

nm1

bn1znm1.

2.3

Using the fact that Rew≥0 if and only if|1w|>|1−w|inU, it suffices to show that |Az

Bz| − |AzBz| ≥0. Substituting forAzandBzgives

|Az Bz| − |AzBz|

2 ∞

nm1

n11γeiθm−12βγeiθ

m1−β an1z

nm1

z

z

m

nm

n11γeiθm−12βγe

m1−β bn1z

nm1

nm1

n11γeiθm1γeiθ

m1−β an1z

nm1

z

z

nm

n11γeiθm1γe

m1−β bn1z

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≥2− ∞

nm1

n11γm2βγ−1

m1−β |an1| |z|

nm1

−∞

nm

n11γm2βγ−1

m1−β |bn1| |z|

nm1

− ∞

nm1

n11γm1γ

m1−β |an1| |z|

nm1

−∞

nm

n11γm1γ

m1−β |bn1| |z|

nm1

≥2

1− ∞

nm1

n11γmβγ

m1−β |an1|

−∞

nm

n11γmβγ

m1−β |bn1|

≥0 by2.1

2.4

The harmonic functions

fz zm

nm1

m1−β

n11γmβγxnz

n1

nm

m1−β

n11γmβγynz

n1,

2.5

where∞nm1|xn|nm|yn|1, show that the coefficient boundary given by2.1is sharp.

The functions of the form2.5are in the classRm, β, γbecause

nm1

1γn1−mβγ

m1−β |an1| ∞

nm

1γn1 mβγ

m1−β |bn1|

nm1

|xn|

nm1

yn1. 2.6

This completes the proof ofTheorem 2.1.

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Theorem 2.2. Letfhgbe such thathandgare given by1.4. ThenfTm, β, γif and only if

nm−1

1γn1−mγβ

m1−β an1

1γn1 mγβ

m1−β bn1

≤2. 2.7

Proof. SinceRm, β, γTm, β, γ, we only need to prove the “only if” part of the theorem.

To this end, for functions f of the form 1.4, we notice that the condition Re{1

γeiθzfz/zfzγme} ≥is equivalent to

Re

⎧ ⎨ ⎩

1γeiθzhzzgzmβγeiθhz gz

hz gz

⎫ ⎬

>0, 2.8

which implies that

Re

m1γeiθmβγeiθzm−∞nm11γeiθn1−mβγeiθan1zn1

zm

nm1an1zn1∞nmbn1zn1

nm1γeiθn1 mβγeiθbn1zn1

zm

nm1an1zn1∞nmbn1zn1

Re

m1−β−∞nm11γeiθn1−mβγeiθan1znm1

1−∞nm1an1znm1∞nmbn1znm1

nm1γeiθn1 mβγeiθbn1znm1

1−∞nm1an1znm1∞nmbn1znm1

>0.

2.9

Since Reeiθ≤ |eiθ|1, the required condition is that2.9is equivalent to

1−∞nm11γn1−mβγ/m1−βan1rnm1

1−∞nm1an1rnm1∞nmbn1rnm1

nm

1γn1 mβγ/m1−βbn1rnm1

1−∞nm1an1rnm1∞nmbn1rnm1

≥0.

2.10

If the condition 2.7 does not hold, then the numerator in 2.10 is negative for z r sufficiently close to 1. Hence there exists z0 r0 in 0,1 for which the quotient in 2.10

is negative. This contradicts the required condition forfTm, β, γ, and so the proof of Theorem 2.2is completed.

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Proof. The proof follows from1.5, by putting2.7in the form

nm−1

n1−mγβ/1γ

m1−γβ/1γ an1

n1 mγβ/1γ

m1−γβ/1γ bn1

≤2. 2.11

Theorem 2.4. LetfTm, β, γ. Then for|z|r <1, we have

fz≤1bm1rrm

m1−β

m1−β21γ

m12γβ1γ

m1−β21γ bm1

rm2,

fmz≥1−bm1rrm

m1−β

m1−β21γ

m12γβ1γ

m1−β21γ bm1

rm2.

2.12

Proof. We prove the left-hand-side inequality for |f|. The proof for the right-hand-side

inequality can be done by using similar arguments. LetfTm, β, γ, then we have

fz

zm

nm1

an1zn1

nm

bn1zn1

rmb

m1rm1−

nm1

an1bn1rm2

rmb m1rm1

m

1−β

1γm2−mγβ

nm1

1γm2−mγβ

m1−β an1bn1r

n1

rmb m1rm1

m

1−β

1γm2−mγβ

nm1

1γn1−mγβ

m1−β an1

1γn1 mγβ

m1−β bn1

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≥1−bm1rrm

m

1−β

1γm2−mγβ

1−

1γm1 mγβ

m1−β bm1

rm2

≥1−bm1rrm

m1−β

m1−β21γ

m12γβ1γ

m1−β21γ bm1

rm2.

2.13

This completes the proof ofTheorem 2.4.

The following covering result follows from the left-side inequality inTheorem 2.4.

Corollary 2.5. LetfTm, β, γ,then the set

w:|w|< 2

1γ

m1−β21γ

1γ−2mγβ

m1−β21γbm1

2.14

is included infU.

3. Extreme Points

Our next theorem is on the extreme points of convex hulls of the classTm, β, γ, denoted by clcoTm, β, γ.

Theorem 3.1. Letfhgbe such thathandgare given by1.4. Thenf∈clcoTm, β, γif and

only iffcan be expressed as

fz

nm

Xn1hn1z Yn1gn1z, 3.1

where

hmz zm,

hn1z zmm

1−β

1γn1−mγβz

n1 nm1, m2, ...,

gn1z zm m

1−β

1γn1 mγβz

n1 nm, m1, m2, ...,

Xn1≥0, Yn1≥0,

nm

Xn1Yn1 1.

3.2

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Proof. For functionsfzof the form3.1, we have

fz

nm

Xn1Yn1zm

nm

m1−β

1γn1−mγβXn1z

n1

nm

m1−β

1γn1 mγβYn1z

n1.

3.3

Then

nm1

1γn1−mγβ

m1−β

m1−β

1γn1−mγβ

Xn1

nm

1γn1 mγβ

m1−β

m1−β

1γn1 mγβ

Yn1

nm1

Xn1

nm

Yn1 1−Xm≤1,

3.4

and sofz∈clcoTm, β, γ. Conversely, suppose thatfz∈clcoTm, β, γ. Set

Xn1

1γn1−mγβ

m1−β an1 nm1, ...,

Yn1

1γn1 mγβ

m1−β bn1 nm, m1, ...,

3.5

then note that byTheorem 2.2, 0≤Xn1≤1 nm1, ...and 0≤Yn1≤1 nm, m1, ....

Consequently, we obtain

fz

nm

Xn1hn1z Yn1gn1z. 3.6

Using Theorem 2.2 it is easily seen that the class Tm, β, γ is convex and closed, and so clcoTm, β, γ Tm, β, γ.

4. Convolution Result

For harmonic functions of the form

fz zmnm1

an1zn1

nm

bn1zn1, 4.1

Gz zmnm1

An1zn1

nm

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we define the convolution of two harmonic functionsfandGas

fGz fzGz

zmnm1

an1An1zn1

nm

bn1Bn1zn1.

4.3

Using this definition, we show that the classTm, β, γis closed under convolution.

Theorem 4.1. For0 ≤ β < 1, letfzTm, β, γand GzTm, β, γ. ThenfzGz

Tm, β, γ.

Proof. Let the functionsfzdefined by4.1be in the class Tm, β, γ, and let the functions

Gzdefined by4.2be in the classTm, β, γ. Obviously, the coefficients off andGmust satisfy a condition similar to the inequality2.7. So for the coefficients offG we can write

nm−1

1γn1−mγβ

m1−β an1An1

1γn1 mγβ

m1−β bn1Bn1

≤ ∞

nm−1

1γn1−mγβ

m1−β an1

1γn1 mγβ

m1−β bn1

,

4.4

where the right hand side of this inequality is bounded by 2 becausefTm, β, γ. Then,

fzGzTm, β, γ.

Finally, we show thatTm, β, γis closed under convex combinations of its members.

Theorem 4.2. The classTm, β, γ is closed under convex combination.

Proof. Fori1,2,3, .... letfiTm, β, γ,where the functionsfiare given by

fiz zm

nm1

an1,izn1

nm

bn1,izn1 an1,i;bn1,i≥0;m≥1. 4.5

For∞i1ti 1; 0≤ti≤1,the convex combination offimay be written as

i1

tifiz zm

nm1

i1

tian1,i

zn1

nm

i1

tibn1,i

(10)

Then by2.7, we have

nm−1

1γn1−mγβ

m1−β

i1

tian1,i

1γn1 mγβ

m1−β

i1

tibn1,i

i1

ti

nm−1

1γn1−mγβ

m1−β an1,i

1γn1 mγβ

m1−β bn1,i

≤2 ∞

i1

ti2.

4.7

This is the condition required by2.7, and so∞i1tifizTm, β, γ. This completes the

proof ofTheorem 4.2.

Remark 4.3. Our results form1 correct the results obtained by Kharinar and More6.

Acknowledgment

The author thanks the referees for their valuable suggestions which led to the improvement of this study.

References

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

2 O. P. Ahuja and J. M. Jahangiri, “Multivalent harmonic starlike functions,”Annales Universitatis Mariae Curie-Skłodowska A, vol. 55, pp. 1–13, 2001.

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

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

5 J. M. Jahangiri, G. Murugusundaramoorthy, and K. Vijaya, “On starlikeness of certain multivalent harmonic functions,”Journal of Natural Geometry, vol. 24, no. 1-2, pp. 1–10, 2003.

6 S. M. Kharinar and M. More, “Certain class of harmonic starlike functions with some missing coefficients,”Acta Mathematica, vol. 24, no. 3, pp. 323–332, 2008.

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