• Nem Talált Eredményt

ON A CERTAIN SUBCLASS OF STARLIKE FUNCTIONS WITH NEGATIVE COEFFICIENTS

N/A
N/A
Protected

Academic year: 2022

Ossza meg "ON A CERTAIN SUBCLASS OF STARLIKE FUNCTIONS WITH NEGATIVE COEFFICIENTS"

Copied!
18
0
0

Teljes szövegt

(1)

Subclass of Starlike Functions A. Y. Lashin vol. 10, iss. 2, art. 40, 2009

Title Page

Contents

JJ II

J I

Page1of 18 Go Back Full Screen

Close

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.

(2)

Subclass of Starlike Functions A. Y. Lashin vol. 10, iss. 2, art. 40, 2009

Title Page Contents

JJ II

J I

Page2of 18 Go Back Full Screen

Close

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

(3)

Subclass of Starlike Functions A. Y. Lashin vol. 10, iss. 2, art. 40, 2009

Title Page Contents

JJ II

J I

Page3of 18 Go Back Full Screen

Close

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).

(4)

Subclass of Starlike Functions A. Y. Lashin vol. 10, iss. 2, art. 40, 2009

Title Page Contents

JJ II

J I

Page4of 18 Go Back Full Screen

Close

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]).

(5)

Subclass of Starlike Functions A. Y. Lashin vol. 10, iss. 2, art. 40, 2009

Title Page Contents

JJ II

J I

Page5of 18 Go Back Full Screen

Close

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

(6)

Subclass of Starlike Functions A. Y. Lashin vol. 10, iss. 2, art. 40, 2009

Title Page Contents

JJ II

J I

Page6of 18 Go Back Full Screen

Close

clearing the denominator in (2.2) and lettingz→1through 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).

(7)

Subclass of Starlike Functions A. Y. Lashin vol. 10, iss. 2, art. 40, 2009

Title Page Contents

JJ II

J I

Page7of 18 Go Back Full Screen

Close

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.

(8)

Subclass of Starlike Functions A. Y. Lashin vol. 10, iss. 2, art. 40, 2009

Title Page Contents

JJ II

J I

Page8of 18 Go Back Full Screen

Close

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).

(9)

Subclass of Starlike Functions A. Y. Lashin vol. 10, iss. 2, art. 40, 2009

Title Page Contents

JJ II

J I

Page9of 18 Go Back Full Screen

Close

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).

(10)

Subclass of Starlike Functions A. Y. Lashin vol. 10, iss. 2, art. 40, 2009

Title Page Contents

JJ II

J I

Page10of 18 Go Back Full Screen

Close

5. Integral Means Inequalities

We need the following lemma.

Lemma 5.1 ([3]). Iff andgare analytic inU withf ≺g,then Z

0

g(re)

δdθ ≤ Z

0

f(re)

δdθ,

whereδ > 0, z =re 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 =re,0< r <1,we have Z

0

f(re)

δdθ ≤ Z

0

f2(re)

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

0

1−

X

k=2

akzk−1

δ

dθ≤ Z

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.

(11)

Subclass of Starlike Functions A. Y. Lashin vol. 10, iss. 2, art. 40, 2009

Title Page Contents

JJ II

J I

Page11of 18 Go Back Full Screen

Close

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 =re,0< r <1,we have Z

0

f(re)

δdθ ≤ Z

0

f2(re)

δdθ,

where

f2(z) = z− (1−β) (2−β)z2.

(12)

Subclass of Starlike Functions A. Y. Lashin vol. 10, iss. 2, art. 40, 2009

Title Page Contents

JJ II

J I

Page12of 18 Go Back Full Screen

Close

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.

(13)

Subclass of Starlike Functions A. Y. Lashin vol. 10, iss. 2, art. 40, 2009

Title Page Contents

JJ II

J I

Page13of 18 Go Back Full Screen

Close

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,

(14)

Subclass of Starlike Functions A. Y. Lashin vol. 10, iss. 2, art. 40, 2009

Title Page Contents

JJ II

J I

Page14of 18 Go Back Full Screen

Close

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,

(15)

Subclass of Starlike Functions A. Y. Lashin vol. 10, iss. 2, art. 40, 2009

Title Page Contents

JJ II

J I

Page15of 18 Go Back Full Screen

Close

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).

(16)

Subclass of Starlike Functions A. Y. Lashin vol. 10, iss. 2, art. 40, 2009

Title Page Contents

JJ II

J I

Page16of 18 Go Back Full Screen

Close

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).

(17)

Subclass of Starlike Functions A. Y. Lashin vol. 10, iss. 2, art. 40, 2009

Title Page Contents

JJ II

J I

Page17of 18 Go Back Full Screen

Close

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.

(18)

Subclass of Starlike Functions A. Y. Lashin vol. 10, iss. 2, art. 40, 2009

Title Page Contents

JJ II

J I

Page18of 18 Go Back Full Screen

Close

[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.

Hivatkozások

KAPCSOLÓDÓ DOKUMENTUMOK

In the present paper, first we determine the extreme points of the class Q(α, β, γ), then we find the coefficient bounds and radius of univalency for functions belonging to this

Applying Theorem 1.3 by Littlewood [3], Owa and Sekine [5] have con- sidered some integral means inequalities for certain analytic functions.. In the present paper, we discuss

Key words and phrases: Univalent functions, Starlike functions of order α, Convex functions of order α, Inverse functions, Coefficient estimates.. 2000 Mathematics

Also we give applications of our results to certain functions defined through convolution (or Hadamard product) and in particular we consider a class N α,β λ (φ) of functions defined

Also we give applications of our results to certain functions defined through convolution (or Hadamard product) and in particular we consider a class N α,β λ (φ) of functions defined

In this paper, we study the weakly convergent sequence coefficient and obtain its estimates for some parameters in Banach spaces, which give some sufficient conditions for a

In this paper, we introduce a new class of functions which are analytic and univalent with negative coefficients defined by using a certain fractional cal- culus and fractional

In this paper, we introduce a new class of functions which are analytic and uni- valent with negative coefficients defined by using a certain fractional calculus and fractional