• 検索結果がありません。

It is the purpose of the present paper to obtain some sufficient conditions forp- valently starlikeness for a certain class of functions which are analytic in the open unit diskE

N/A
N/A
Protected

Academic year: 2022

シェア "It is the purpose of the present paper to obtain some sufficient conditions forp- valently starlikeness for a certain class of functions which are analytic in the open unit diskE"

Copied!
5
0
0

読み込み中.... (全文を見る)

全文

(1)

http://jipam.vu.edu.au/

Volume 4, Issue 2, Article 36, 2003

A CRITERION FOR p-VALENTLY STARLIKENESS

MUHAMMET KAMALI ATATURKUNIVERSITY, FACULTY OFSCIENCE ANDARTS, DEPARTMENT OFMATHEMATICS,

25240, ERZURUM-TURKEY.

[email protected]

Received 16 December, 2002; accepted 8 May, 2003 Communicated by A. Sofo

ABSTRACT. It is the purpose of the present paper to obtain some sufficient conditions forp- valently starlikeness for a certain class of functions which are analytic in the open unit diskE.

Key words and phrases: p−valently starlikeness, Jack Lemma.

2000 Mathematics Subject Classification. 30C45, 31A05.

1. INTRODUCTION

LetA(p)be the class of functions of the form:

f(z) =zp +

X

n=p+1

anzn (p∈N={1,2,3, . . .}), which are analytic inE ={z ∈C:|z|<1}.

A functionf(z)∈A(p)is said to be p-valently starlike if and only if Re

zf0(z)

f(z)

>0 (z ∈E).

We denote byS(p)the subclass ofA(p)consisting of functions which arep-valently inE (see, e.g., Goodman [1]).

Let

(1.1) f(z) = z+

X

n=2

anzn.

A functionf(z)of the form (1.1) is said to beα−convex inEif it is regular, f(z)

z f0(z)6= 0,

ISSN (electronic): 1443-5756

c 2003 Victoria University. All rights reserved.

148-02

(2)

and

(1.2) Re

α

1 +zf00(z) f0(z)

+(1−α)zf0(z) f(z)

>0

for allzinE. The set of all such functions is denoted byα−CV, whereαis a real number. Of course, ifα = 1, then an α−convex function is convex; and ifα= 0, anα−convex function is starlike. Thus the setsα−CV give a “continuous” passage from convex functions to starlike functions. Sakaguchi considers functions of the form

f(z) =zp+

X

n=p+1

anzn,

wherepis a positive integer, and he imposes the condition

(1.3) Re

1 + zf00(z)

f0(z) +kzf0(z) f(z)

>0

for z inE. He proved that if k = −1, there is only one function that satisfies (1.3), namely f(z) ≡ zp. If−1 < k 6 0,thenf(z)is p-valent convex; and if 0 < k, then f(z) isp-valent starlike. We can pass from (1.3) back to (1.2) if we divide by1 +k >0and setα= 1+k1 [6]. We denote byS(p, k)the subclassA(p)consisting of functions which satisfy the condition (1.3).

Obradovic and Owa [7] have obtained a sufficient condition for starlikeness off(z)∈ A(1) which satisfies a certain condition for the modulus of

1 + zff000(z)(z) zf0(z)

f(z)

,

we recall their result as:

Theorem 1.1. Iff(z)∈A(1)satisfies

1 + zf00(z) f0(z)

< K

zf0(z) f(z)

(z ∈E), whereK = 1.2849...,thenf(z)∈S(1).

Nunokawa [4] improved Theorem 1.1 by proving Theorem 1.2. Iff(z)∈A(p), and if

1 + zf00(z) f0(z)

<

zf0(z) f(z)

1

plog(4ep−1) (z ∈E), thenf(z)∈S(p).

2. PRELIMINARIES

In order to obtain our main result, we need the following lemma attributed to Jack [2] (given also by Miller and Mocanu [3]).

Lemma 2.1. Letw(z)be analytic inE withw(0) = 0.If|w(z)|attains its maximum value in the circle|z| = r < 1at a pointz0, then we can write z0w0(z0) = kw(z0),where k is a real number andk≥1.

Making use of Lemma 2.1,we first prove

(3)

Lemma 2.2. Letq(z)be analytic inEwithq(0) =pand suppose that

(2.1) Re

zq0(z) [q(z)]2

< 1

p(λ+ 1) (z ∈E,06λ61), thenRe{q(z)}>0inE.

Proof. Let us put

q(z) = p 1

2 +1 2λ

1 +w(z) 1−w(z)+

1 2− 1

1−w(z) 1 +w(z)

, where06λ61.

Thenw(z)is analytic inEwithw(0) = 0and by an easy calculation, we have 1 +z q0(z)

[q(z)]2 = 1 + 2

p· (λw2(z) + 2w(z) +λ)zw0(z) (w2(z) + 2λw(z) + 1)2 .

If we suppose that there exists a pointz0 ∈E such thatmax|z|6|z0||w(z)| =|w(z0)| = 1,then, from Lemma 2.1, we havez0w0(z0) =kw(z0), (k >1).

Puttingw(z0) = e,we find that z0 q0(z0)

[q(z0)]2 = 2

p ·λw2(z0)w0(z0)z0+ 2w(z0)w0(z0)z0+λw0(z0)z0 [w2(z0) + 2λw(z0) + 1]2

= 2k

p · λe3iθ+ 2e2iθ+λe (e2iθ+ 2λe+ 1)2

= 2k

p · λe3iθ+ 2e2iθ +λe

(e2iθ+ 2λe+ 1)2 · e−2iθ + 2λe−iθ + 12

(e−2iθ + 2λe−iθ + 1)2

= k

p · λcos 3θ+ (4λ2+ 2) cos 2θ+ (11λ+ 4λ3) cosθ+ (8λ2+ 2) 4 (λ+ cosθ)4

= k

p · (1 +λcosθ) (λ+ cosθ)2 (λ+ cosθ)4

= k

p · 1 +λcosθ (λ+ cosθ)2, so that

Re

z0 q0(z0) [q(z0)]2

= k

p · 1 +λcosθ (λ+ cosθ)2 = k

p · λ2+λcosθ+ 1−λ2 (λ+ cosθ)2

= k p

λ

(λ+ cosθ) + 1−λ2 (λ+ cosθ)2

> 1 p

1 λ+ 1

.

This contradicts (2.1). Therefore, we have|w(z)| <1inE, and it follows that Re{q(z)} > 0

inE. This completes our proof of Lemma 2.2.

If we takeλ= 1in Lemma 2.2, then we have the following Lemma 2.3 by Nunokawa [5].

Lemma 2.3. Letq(z)be analytic inEwithq(0) =pand suppose that Re

zq0(z) [q(z)]2

< 1

2p (z ∈E).

(4)

ThenRe{q(z)}>0inE.

3. A CRITERION FOR p-VALENTLY STARLIKENESS

Theorem 3.1. Letf(z)∈A(p), f(z)6= 0,in0<|z|<1and suppose that

(3.1) Re



 1 +z

h

1 +zf00(z)

f0(z) +kff(z)0(z)i0 h

1 +z

f00(z)

f0(z) +kff0(z)(z)i2





<1 + 1 k+ 1

1 2p

(z ∈E).

Thenf(z)∈S(p, k).

Proof. Let us put

q(z) = 1 k+ 1

1 +zf00(z)

f0(z) +kzf0(z) f(z)

(k > 0).

Then,q(z)is analytic inE withq(0) =p, q(z)6= 0inE.We have

q0(z) q(z) =

zff000(z)(z)

0

+

kzff0(z)(z)0

1 +zff000(z)(z) +kzff(z)0(z) =

f00(z) f0(z) +z

f00(z) f0(z)

0

+kff(z)0(z) +kz

f0(z) f(z)

0

1 +zff000(z)(z) +kzff(z)0(z) . Then, we obtain

zq0(z)

q(z) = 1 +zff000(z)(z)+kzff(z)0(z) −1 1 +zff000(z)(z) +kzff(z)0(z) +z

kzf0(z) f(z)

0

+zf00(z) f0(z)

0 1 +zff000(z)(z)+kzff0(z)(z)

= 1 + z2

f00(z) f0(z)

0

+k

f0(z) f(z)

0

−1 1 +zff000(z)(z) +kzff0(z)(z) , or

(k+ 1)q(z) +zq0(z) q(z)

= 1 + z2

f00(z) f0(z)

0

+k

f0(z) f(z)

0

−1

1 +zff000(z)(z) +kzff(z)0(z) + (k+ 1)q(z)

= 1 + z2

f00(z)

f0(z) +kff(z)0(z)0

+ 2z

f00(z)

f0(z) +kff0(z)(z)

+z2

f00(z)

f0(z) +kff(z)0(z)2

1 +zff000(z)(z)+kzff0(z)(z)

= 1 +z

f00(z)

f0(z) +kf0(z) f(z)

+z

zf00(z)

f0(z) +kff0(z)(z)0

+f00(z)

f0(z) +kff(z)0(z)

1 +zff000(z)(z) +kzff(z)0(z) .

(5)

Thus,

1 + 1

k+ 1z q0(z)

[q(z)]2 = 1 +z z

f00(z)

f0(z) +kff(z)0(z)0

+

f00(z)

f0(z) +kff0(z)(z)

1 +zff000(z)(z) +kzff(z)0(z)2

= 1 +z h

1 +z

f00(z)

f0(z) +kff(z)0(z)i0

1 +zff000(z)(z) +kzff0(z)(z) 2 . From Lemma 2.3 and (3.1), we thus find that

Re

1 +zf00(z)

f0(z) +kzf0(z) f(z)

>0 (z ∈E, k > 0).

This completes our proof of Theorem 3.1.

If we takeα= 0, after writing k+11 =αin (3.1), then we obtain M. Nunokawa’s theorem as follows.

Theorem 3.2. Letf(z)∈A(p), f(z)6= 0,in0<|z|<1and suppose that Re

(1 + zff000(z)(z) zf0(z)

f(z)

)

<1 + 1

2p, z ∈E.

Thenf(z)∈S(p).

REFERENCES

[1] A.W. GOODMAN, On the Schwarz-Christoffel transformation andp-valent functions, Trans. Amer.

Math. Soc., 68 (1950), 204–223.

[2] I.S. JACK, Functions starlike and convex of orderα, J. London Math. Soc., 2(3) (1971), 469–474.

[3] S.S. MILLERAND P.T. MOCANU, Second order differential inequalities in the complex plane, J.

Math. Anal. Appl., 65 (1978), 289–305.

[4] M. NUNOKAWA, On certain multivalent functions, Math. Japon., 36 (1991), 67–70.

[5] M. NUNOKAWA, A certain class of starlike functions, in Current Topics in Analytic Function The- ory, H.M. Srivastava and S. Owa (Eds.), Singapore, New Jersey, London, Hong Kong, 1992, p.

206–211.

[6] A.W. GOODMAN, Univalent Functions, Volume I, Florida, 1983, p.142–143.

[7] M. OBRADOVICANDS. OWA, A criterion for starlikeness, Math. Nachr., 140 (1989), 97–102.

参照

関連したドキュメント

alytic functions with negative coefficients in the unit disk and discuss some properties of functions belonging to the class

Abstract: The purpose of the present paper is to investigate some argument properties for certain analytic functions in the open unit disk associated with the convolution

In this paper, we obtain some sufficient conditions for an analytic function f (z), defined on the unit disk 4, to be starlike of order α.. Key words and phrases: Starlike function

For analytic functions $f(z)$ in the open unit disk $E$ , weakly $\Phi$ -like of order $\alpha$ with. respect to a function

$\mathcal{M}\mathcal{D}(a,\beta)$ of certain analytic functions in the open unit disk $U$ , two subdasses $\mathcal{M}_{1}(\alpha,\beta)$.. and

$\mathcal{M}D(\alpha,\beta)$ and $ND(\alpha, \beta)$ of certain analytic functions in the open unit disk $\mathrm{U}$ , two. subclasses $\mathcal{M}D^{*}(a, \beta)$ and

normalized analytic functions satisfying certain coefficient inequalities in the open unit disk.. The main results of the present paper provide various interesting

The object of the present paper is to consider a sufficient condition for analytic functions in the open unit disk to be strongly starlike of order