Subclass of Starlike Functions A. Y. Lashin vol. 10, iss. 2, art. 40, 2009
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ON A CERTAIN SUBCLASS OF STARLIKE FUNCTIONS WITH NEGATIVE COEFFICIENTS
A. Y. LASHIN
Department of Mathematics Faculty of Science
Mansoura University Mansoura, 35516, EGYPT.
EMail:aylashin@yahoo.com
Received: 11 December, 2007
Accepted: 29 May, 2009
Communicated by: S.S. Dragomir 2000 AMS Sub. Class.: 30C45.
Key words: Univalent functions, Starlike functions, Integral means, Neighborhoods, Partial sums.
Abstract: We introduce the classH(α, β)of analytic functions with negative coefficients.
In this paper we give some properties of functions in the classH(α, β)and we obtain coefficient estimates, neighborhood and integral means inequalities for the functionf(z) belonging to the class H(α, β).We also establish some results concerning the partial sums for the functionf(z)belonging to the classH(α, β).
Acknowledgements: The author would like to thank the referee of the paper for his helpful suggestions.
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Contents
1 Introduction 3
2 Coefficient Estimates 5
3 Some Properties of the ClassH(α, β) 7
4 Neighborhood Results 8
5 Integral Means Inequalities 10
6 Partial Sums 12
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1. Introduction
Let Adenote the class of functions of the form
(1.1) f(z) = z+
∞
X
k=2
akzk,
which are analytic in the unit discU ={z :|z|<1}.And letSdenote the subclass ofAconsisting of univalent functionsf(z)inU.
A functionf(z)inSis said to be starlike of orderαif and only if Re
zf0(z) f(z)
> α (z ∈U),
for someα(0≤ α <1). We denote by S∗(α)the class of all functions inS which are starlike of orderα. It is well-known that
S∗(α)⊆ S∗(0)≡S∗.
Further, a functionf(z)inSis said to be convex of orderαinU if and only if Re
1 + zf00(z) f0(z)
> α (z ∈U),
for someα (0≤ α <1). We denote by K(α)the class of all functions inS which are convex of orderα.
The classes S∗(α), andK(α) were first introduced by Robertson [8], and later were studied by Schild [10], MacGregor [4], and Pinchuk [7].
LetT denote the subclass ofS whose elements can be expressed in the form:
(1.2) f(z) =z−
∞
X
k=2
akzk (ak ≥0).
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We denote byT∗(α)and C(α), respectively, the classes obtained by taking the in- tersections ofS∗(α)andK(α)withT,
T∗(α) =S∗(α)∩T and C(α) = K(α)∩T.
The classesT∗(α)andC(α)were introduced by Silverman [11].
LetH(α, β)denote the class of functionsf(z)∈Awhich satisfy the condition Re
αz2f00(z)
f(z) + zf0(z) f(z)
> β
for someα≥0,0≤β <1, f(z)z 6= 0 and z ∈U.
The classesH(α, β)andH(α,0)were introduced and studied by Obraddovic and Joshi [5], Padmanabhan [6], Li and Owa [2], Xu and Yang [14], Singh and Gupta [13], and others.
Further, we denote by H(α, β) the class obtained by taking intersections of the classH(α, β)withT, that is
H(α, β) = H(α, β) ∩T.
We note that
H(0, β) =T∗(β) (Silverman [11]).
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2. Coefficient Estimates
Theorem 2.1. A functionf(z)∈T is in the classH(α, β)if and only if
(2.1)
∞
X
k=2
[(k−1)(αk+ 1) + (1−β)]ak≤1−β.
The result is sharp.
Proof. Assume that the inequality (2.1) holds and let|z|<1.Then we have
αz2f00(z)
f(z) +zf0(z) f(z) −1
=
−P∞
k=2(k−1)(αk+ 1)akzk−1 1−P∞
k=2akzk−1
≤ P∞
k=2(k−1)(αk+ 1)ak 1−P∞
k=2ak ≤1−β.
This shows that the values of αz2f
00(z)
f(z) + zff(z)0(z) lie in the circle centered at w = 1 whose radius is1−β.Hencef(z)is in the classH(α, β).
To prove the converse, assume thatf(z)defined by (1.2) is in the class H(α, β).
Then
(2.2) Re
αz2f00(z)
f(z) + zf0(z) f(z)
= Re
1−P∞
k=2[αk(k−1) +k)]akzk−1 1−P∞
k=2akzk−1
> β
forz ∈U.Choose values ofz on the real axis so that αz2f
00(z)
f(z) +zff(z)0(z) is real. Upon
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clearing the denominator in (2.2) and lettingz→1−through real values, we have β 1−
∞
X
k=2
ak
!
≤1−
∞
X
k=2
[αk(k−1) +k]ak,
which obviously is the required result (2.1).
Finally, we note that the assertion (2.1) of Theorem2.1is sharp, with the extremal function being
(2.3) f(z) = z− 1−β
[(k−1)(αk+ 1) + (1−β)]zk (k ≥2).
Corollary 2.2. Letf(z)∈T be in the classH(α, β). Then we have
(2.4) ak ≤ 1−β
[(k−1)(αk+ 1) + (1−β)] (k≥2).
Equality in (2.4) holds true for the functionf(z)given by (2.3).
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3. Some Properties of the Class H (α, β)
Theorem 3.1. Let0≤α1 < α2and0≤β <1.ThenH(α2, β)⊂H(α1, β).
Proof. It follows from Theorem2.1. That
∞
X
k=2
[(k−1)(α1k+ 1) + (1−β)]ak
<
∞
X
k=2
[(k−1)(α2k+ 1) + (1−β)]ak≤1−β
forf(z)∈H(α2, β).Hencef(z)∈H(α1, β).
Corollary 3.2. H(α, β)⊆T∗(β).
The proof is now immediate becauseα≥0.
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4. Neighborhood Results
Following the earlier investigations of Goodman [1] and Ruscheweyh [9], we define theδ−neighborhood of function f(z)∈T by:
Nδ(f) = (
g ∈T :g(z) =z−
∞
X
k=2
bkzk,
∞
X
k=2
k|ak−bk| ≤δ )
.
In particular, for the identity function
e(z) = z, we immediately have
(4.1) Nδ(e) = (
g ∈T :g(z) =z−
∞
X
k=2
bkzk,
∞
X
k=2
k|bk| ≤δ )
.
Theorem 4.1. H(α, β)⊆Nδ(e),whereδ = (2α+2−β)2(1−β) .
Proof. Letf(z)∈H(α, β).Then, in view of Theorem2.1, since[(k−1)(αk+ 1) + (1−β)]is an increasing function ofk(k ≥2), we have
(2α+ 2−β)
∞
X
k=2
ak ≤
∞
X
k=2
[(k−1)(αk+ 1) + (1−β)]ak ≤1−β,
which immediately yields (4.2)
∞
X
k=2
ak≤ 1−β (2α+ 2−β).
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On the other hand, we also find from (2.1) (α+ 1)
∞
X
k=2
kak−β
∞
X
k=2
ak ≤
∞
X
k=2
[(α(k−1) + 1)k−β)]ak
=
∞
X
k=2
[(k−1)(αk+ 1) + (1−β)]ak ≤1−β.
(4.3)
From (4.3) and (4.2), we have (α+ 1)
∞
X
k=2
kak ≤(1−β) +β
∞
X
k=2
ak
≤(1−β) +β 1−β (2α+ 2−β)
≤ 2(α+ 1)(1−β) (2α+ 2−β) , that is,
(4.4)
∞
X
k=2
kak ≤ 2 (1−β)
(2α+ 2−β) =δ, which in view of the definition (4.1), prove Theorem4.1.
Lettingα= 0,in the above theorem, we have:
Corollary 4.2. T∗(β)⊆Nδ(e),whereδ= 2(1−β)(2−β).
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5. Integral Means Inequalities
We need the following lemma.
Lemma 5.1 ([3]). Iff andgare analytic inU withf ≺g,then Z 2π
0
g(reiθ)
δdθ ≤ Z 2π
0
f(reiθ)
δdθ,
whereδ > 0, z =reiθ and0< r <1.
Applying Lemma5.1, and (2.1), we prove the following theorem.
Theorem 5.2. Letδ >0.Iff(z)∈H(α, β),then forz =reiθ,0< r <1,we have Z 2π
0
f(reiθ)
δdθ ≤ Z 2π
0
f2(reiθ)
δdθ,
where
(5.1) f2(z) =z− (1−β)
(2α+ 2−β)z2.
Proof. Letf(z)defined by (1.2) andf2(z)be given by (5.1). We must show that Z 2π
0
1−
∞
X
k=2
akzk−1
δ
dθ≤ Z 2π
0
1− (1−β) (2α+ 2−β)z
δ
dθ.
By Lemma5.1, it suffices to show that 1−
∞
X
k=2
akzk−1 ≺1− (1−β) (2α+ 2−β)z.
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Setting
(5.2) 1−
∞
X
k=2
akzk−1 = 1− (1−β)
(2α+ 2−β)w(z).
From (5.2) and (2.1), we obtain
|w(z)|=
∞
X
k=2
(2α+ 2−β) (1−β) akzk−1
≤ |z|
∞
X
k=2
[(k−1)(αk+ 1) + (1−β)]
1−β ak≤ |z|. This completes the proof of the theorem.
Lettingα= 0in the above theorem, we have:
Corollary 5.3. Letδ > 0.If f(z)∈T∗(β),then forz =reiθ,0< r <1,we have Z 2π
0
f(reiθ)
δdθ ≤ Z 2π
0
f2(reiθ)
δdθ,
where
f2(z) = z− (1−β) (2−β)z2.
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6. Partial Sums
In this section we will examine the ratio of a function of the form (1.2) to its sequence of partial sums defined byf1(z) = z andfn(z) = z−Pn
k=2akzk when the coef- ficients off are sufficiently small to satisfy the condition (2.1). We will determine sharp lower bounds forRef(z)
fn(z)
,Ref
n(z) f(z)
,Ref0(z) fn0(z)
andRef0 n(z) f0(z)
. In what follows, we will use the well known result that
Re1−w(z)
1 +w(z) >0, z ∈U, if and only if
w(z) =
∞
X
k=1
ckzk
satisfies the inequality|w(z)| ≤ |z|. Theorem 6.1. Iff(z)∈H(α, β),then
(6.1) Re f(z)
fn(z) ≥1− 1
cn+1 (z ∈U, n∈N) and
(6.2) Re
fn(z) f(z)
≥ cn+1
1 +cn+1 (z ∈U, n∈N), where
ck=: [(k−1)(αk+1)+(1−β)]
1−β
.The estimates in (6.1) and (6.2) are sharp.
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Proof. We employ the same technique used by Silverman [12]. The functionf(z)∈ H(α, β),if and only ifP∞
k=2ckak ≤1.It is easy to verify thatck+1 > ck >1.Thus, (6.3)
n
X
k=2
ak+cn+1
∞
X
k=n+1
ak ≤
∞
X
k=2
ckak ≤1.
We may write cn+1
f(z) fn(z)−
1− 1 cn+1
= 1−Pn
k=2akzk−1−cn+1P∞
k=n+1akzk−1 1−Pn
k=2akzk−1
= 1 +D(z) 1 +E(z).
Set 1 +D(z)
1 +E(z) = 1−w(z) 1 +w(z), so that
w(z) = E(z)−D(z) 2 +D(z) +E(z). Then
w(z) = cn+1P∞
k=n+1akzk−1 2−2Pn
k=2akzk−1−cn+1P∞
k=n+1akzk−1 and
|w(z)| ≤ cn+1P∞ k=n+1ak 2−2Pn
k=2ak−cn+1P∞ k=n+1ak
. Now|w(z)| ≤1if and only if
n
X
k=2
ak+cn+1
∞
X
k=n+1
ak ≤1,
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which is true by (6.3). This readily yields the assertion (6.1) of Theorem6.1.
To see that
(6.4) f(z) = z−zn+1
cn+1 gives sharp results, we observe that
f(z)
fn(z) = 1− zn cn+1. Letting z →1−,we have
f(z)
fn(z) = 1− 1 cn+1,
which shows that the bounds in (6.1) are the best possible for eachn ∈N.Similarly, we take
(1 +cn+1)
fn(z)
f(z) − cn+1 1 +cn+1
= 1−Pn
k=2akzk−1+cn+1P∞
k=n+1akzk−1 1−P∞
k=2akzk−1 := 1−w(z)
1 +w(z), where
|w(z)| ≤ (1 +cn+1)P∞ k=n+1ak 2−2Pn
k=2ak+ (1−cn+1)P∞
k=n+1ak. Now|w(z)| ≤1if and only if
n
X
k=2
ak+cn+1
∞
X
k=n+1
ak ≤1,
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which is true by (6.3). This immediately leads to the assertion (6.2) of Theorem6.1.
The estimate in (6.2) is sharp with the extremal functionf(z)given by (6.4). This completes the proof of Theorem6.1.
Lettingα= 0in the above theorem, we have:
Corollary 6.2. Iff(z)∈T∗(β),then
Re f(z)
fn(z) ≥ n
(n+ 1−β), (z ∈U) and
Refn(z)
f(z) ≥ n+ 1−β
(n+ 2−2β), (z ∈U). The result is sharp for everyn, with the extremal function
(6.5) f(z) =z− 1−β
(n+ 1−β)zn+1.
We now turn to the ratios involving derivatives. The proof of Theorem6.3below follows the pattern of that in Theorem6.1, and so the details may be omitted.
Theorem 6.3. Iff(z)∈H(α, β),then
(6.6) Ref0(z)
fn0(z) ≥1− n+ 1 cn+1
(z ∈U),
and
(6.7) Re
fn0(z) f0(z)
≥ cn+1
n+ 1 +cn+1 (z ∈U, n∈N).
The estimates in (6.6) and (6.7) are sharp with the extremal function given by (6.4).
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Lettingα= 0in the above theorem, we have:
Corollary 6.4. Iff(z)∈T∗(β),then
Re f0(z)
fn0(z) ≥ βn
(n+ 1−β), (z ∈U), and
Refn0(z)
f0(z) ≥ n+ 1−β
n+ (1−β)(n+ 2), (z∈U). The result is sharp for everyn, with the extremal function given by (6.5).
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References
[1] A.W. GOODMAN, Univalent functions and analytic curves, Proc. Amer. Math.
Soc., 8(3) (1957), 598–601.
[2] J.L. LIANDS. OWA, Sufficient conditions for starlikeness, Indian J. Pure Appl.
Math., 33 (2002), 313-318.
[3] J.E. LITTLEWOOD, On inequalities in the theory of functions, Proc. London Math. Soc., 23 (1925), 481–519.
[4] T.H. MacGREGOR, The radius for starlike functions of order 12, Proc. Amer.
Math. Soc., 14 (1963), 71–76.
[5] M. OBRADOVIC AND S.B. JOSHI, On certain classes of strongly starlike functions, Taiwanese J. Math., 2(3) (1998), 297–302.
[6] K.S. PADMANABHAN, On sufficient conditions for starlikeness, Indian J.
Pure Appl. Math., 32(4) (2001), 543–550.
[7] B. PINCHUK, On starlike and convex functions of ordera, Duke Math. J., 35 (1968), 89–103.
[8] M.S. ROBERTSON, On the theory of univalent functions, Ann. of Math., 37 (1936), 374–408.
[9] S. RUSCHEWEYH, Neighborhoods of univalent functions, Proc. Amer. Math.
Soc., 81(4) (1981), 521–527.
[10] A. SCHILD, On starlike functions of ordera, Amer. J. Math., 87 (1965), 65–70.
[11] H. SILVERMAN, Univalent functions with negative coefficients, Proc. Amer.
Math. Soc., 51 (1975), 109–116.
Subclass of Starlike Functions A. Y. Lashin vol. 10, iss. 2, art. 40, 2009
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[12] H. SILVERMAN, Partial sums of starlike and convex functions, J. Math. Anal.
Appl., 209 (1997), 221–227.
[13] S. SINGHANDS. GUPTA, First order differential subordinations and starlike- ness of analytic maps in the unit disc, Kyungpook Math. J., 45 (2005), 395–404.
[14] N. XUANDD. YANG, Some criteria for starlikeness and strongly starlikeness, Bull. Korean Math. Soc., 42(3) (2005), 579–590.