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
and satisfying the following condition:
Re1γeiφzf z
zfz−γmeiφ
≥mβ 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 zm− ∞ nm1
an1zn1, gz
∞
nm
bn1zn1 an1; bn1≥0; m≥1; z∈U. 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−mβ
m1−β |an1|
n1 mβ
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
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
f∈Rm, β, γ.
Proof. To provef ∈Rm, β, γ, by definition, we only need to show that the condition2.1
holds forf. Substitutinghg forfin1.2, it suffices to show that
Re
⎧ ⎨ ⎩
1γeiθzhz−zgz−mβγeiθhz 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
n11γeiθ−mβγeiθ
m1−β an1z
n−m1
−
z
z
m ∞
nm1
n11γe−iθmβγe−iθ
m1−β bn1z
n−m1,
Bz 1
∞
nm1
an1zn−m1
z
z
m ∞
nm1
bn1zn−m1.
2.3
Using the fact that Rew≥0 if and only if|1w|>|1−w|inU, it suffices to show that |Az
Bz| − |Az−Bz| ≥0. Substituting forAzandBzgives
|Az Bz| − |Az−Bz|
2 ∞
nm1
n11γeiθ−m−12βγeiθ
m1−β an1z
n−m1
−
z
z
m∞
nm
n11γe−iθm−12βγe−iθ
m1−β bn1z
n−m1
− ∞
nm1
n11γeiθ−m1γeiθ
m1−β an1z
n−m1
−
z
z
∞
nm
n11γe−iθm1γe−iθ
m1−β bn1z
≥2− ∞
nm1
n11γ−m2βγ−1
m1−β |an1| |z|
n−m1
−∞
nm
n11γm2βγ−1
m1−β |bn1| |z|
n−m1
− ∞
nm1
n11γ−m1γ
m1−β |an1| |z|
n−m1
−∞
nm
n11γm1γ
m1−β |bn1| |z|
n−m1
≥2
1− ∞
nm1
n11γ−mβγ
m1−β |an1|
−∞
nm
n11γmβγ
m1−β |bn1|
≥0 by2.1
2.4
The harmonic functions
fz zm ∞
nm1
m1−β
n11γ−mβγxnz
n1
∞
nm
m1−β
n11γmβγynz
n1,
2.5
where∞nm1|xn|n∞m|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.
Theorem 2.2. Letfhgbe such thathandgare given by1.4. Thenf ∈Tm, β, γif and only if
∞
nm−1
1γn1−mγβ
m1−β an1
1γn1 mγβ
m1−β bn1
≤2. 2.7
Proof. SinceRm, β, γ⊂Tm, 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/zfz−γmeiθ} ≥mβis equivalent to
Re
⎧ ⎨ ⎩
1γeiθzhz−zgz−mβγeiθhz gz
hz gz
⎫ ⎬
⎭>0, 2.8
which implies that
Re
m1γeiθ−mβγeiθzm−∞nm11γeiθn1−mβγeiθan1zn1
zm−∞
nm1an1zn1∞nmbn1zn1
−
∞
nm1γeiθn1 mβγeiθbn1zn1
zm−∞
nm1an1zn1∞nmbn1zn1
Re
m1−β−∞nm11γeiθn1−mβγeiθan1zn−m1
1−∞nm1an1zn−m1∞nmbn1zn−m1
−
∞
nm1γeiθn1 mβγeiθbn1zn−m1
1−∞nm1an1zn−m1∞nmbn1zn−m1
>0.
2.9
Since Reeiθ≤ |eiθ|1, the required condition is that2.9is equivalent to
1−∞nm11γn1−mβγ/m1−βan1rn−m1
1−∞nm1an1rn−m1∞nmbn1rn−m1
−
∞
nm
1γn1 mβγ/m1−βbn1rn−m1
1−∞nm1an1rn−m1∞nmbn1rn−m1
≥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 forf ∈ Tm, β, γ, and so the proof of Theorem 2.2is completed.
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. Letf ∈Tm, 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. Letf∈Tm, β, γ, then we have
fz
zm−
∞
nm1
an1zn1
∞
nm
bn1zn1
≥rm−b
m1rm1−
∞
nm1
an1bn1rm2
≥rm−b m1rm1
− m
1−β
1γm2−mγβ ∞
nm1
1γm2−mγβ
m1−β an1bn1r
n1
≥rm−b m1rm1
− m
1−β
1γm2−mγβ ∞
nm1
1γn1−mγβ
m1−β an1
1γn1 mγβ
m1−β bn1
≥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. Letf ∈Tm, 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 zm− m
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
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 zm− ∞ nm1
an1zn1
∞
nm
bn1zn1, 4.1
Gz zm− ∞ nm1
An1zn1
∞
nm
we define the convolution of two harmonic functionsfandGas
f∗Gz fz∗Gz
zm− ∞ nm1
an1An1zn1
∞
nm
bn1Bn1zn1.
4.3
Using this definition, we show that the classTm, β, γis closed under convolution.
Theorem 4.1. For0 ≤ β < 1, letfz ∈Tm, β, γand Gz ∈ Tm, β, γ. Thenfz∗Gz ∈
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 off∗G 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 becausef ∈ Tm, β, γ. Then,
fz∗Gz∈Tm, 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, .... letfi∈Tm, 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
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∞i1tifiz ∈ Tm, 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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