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Volume 2009, Article ID 601597,10pages doi:10.1155/2009/601597

Research Article

Conditions for Carath ´eodory Functions

Nak Eun Cho and In Hwa Kim

Department of Applied Mathematics, Pukyong National University, Busan 608-737, South Korea

Correspondence should be addressed to Nak Eun Cho,[email protected]

Received 12 April 2009; Accepted 13 October 2009

Recommended by Yong Zhou

The purpose of the present paper is to derive some sufficient conditions for Carath´eodory functions in the open unit disk. Our results include several interesting corollaries as special cases.

Copyrightq2009 N. E. Cho and I. H. Kim. 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.

1. Introduction

LetPbe the class of functionspof the form

pz 1

n1

pnzn, 1.1

which are analytic in the open unit diskU{z∈C:|z|<1}. IfpinPsatisfies

Repz>0 z∈U, 1.2

then we say thatpis the Catath´eodory function.

LetAdenote the class of all functionsfanalytic in the open unit diskU{z:|z|<1} with the usual normalizationf0 f0−10. Iffandgare analytic inU, we say thatfis subordinate tog, writtenfgorfzgz, ifgis univalent,f0 g0andfU⊂gU. For 0< α≤1, letSTCαandSTSαdenote the classes of functionsf∈ Awhich are strongly convex and starlike of orderα; that is, which satisfy

1zf

z

fz

1z

1−z α

z∈U, 1.3

zfz fz

1z

1−z α

(2)

respectively. We note that1.3and 1.4can be expressed, equivalently, by the argument functions. The classesSTCαandSTSαwere introduced by Brannan and Kirwan1and studied by Mocanu 2 and Nunokawa 3,4. Also, we note that ifα 1, thenSTSα

coincides with S∗, the well-known class of starlikeunivalent functions with respect to origin, and if 0 < α < 1, thenSTSαconsists only of bounded starlike functions1, and hence the inclusion relationSTSα ⊂ S∗ is proper. Furthermore, Nunokawa and Thomas

4 see also5found the valueβαsuch thatSTCβα⊂ STSα.

In the present paper, we consider general forms which cover the results by Mocanu

6 and Nunokawa and Thomas 4. An application of a certain integral operator is also considered. Moreover, we give some sufficient conditions for univalentclose-to-convexand

stronglystarlike functionsof orderβas special cases of main results.

2. Main Results

To prove our results, we need the following lemma due to Nunokawa3.

Lemma 2.1. Letpbe analytic inU, p0 1 andpz/0in U. Suppose that there exists a point

z0∈Usuch that

argpz< π

2α for|z|<|z0|,

argpz0 π

2α 0< α≤1.

2.1

Then we have

z0pz0

pz0 iαk,

2.2

where

k≥ 1

2

x1

x

when argpz0

π

2α,

k≤ −1

2

x1

x

when argpz0 −

π

2α,

pz0

1±

ix x >0.

2.3

With the help ofLemma 2.1, we now derive the following theorem.

Theorem 2.2. Letpbe nonzero analytic inUwithp0 1and letpsatisfy the differential equation

ηzpz Bzpz aibAz, 2.4

whereη > 0,a∈R,0≤batanπ/2α,0< α <1,Az signImpzandBzis analytic inUwithB0 a. If

argBz< π

2β

(3)

where

βη, α, a, b 2 πtan

−1SαTαasinπ/2αbcosπ/2α ηα

SαTαacosπ/2αbsinπ/2α

, 2.6

1α1α/2, 1−α1−α/2, 2.7

then

argpz< π

2α z∈U. 2.8

Proof. If there exists a point z0 ∈ Usuch that the conditions 2.1 are satisfied, then by

Lemma 2.1we obtain2.2under the restrictions2.3. Then we obtain

Az0

⎧ ⎨ ⎩

1, ifpz0 ixα,

−1, ifpz0 −ixα,

Bz0

aibAz0

pz0 −η

z0pz0

pz0

aibAzixαiηαk

a cos

π

2α

b

xαAz0sin

±π

2α

i

b

xαAz0cos

π

2α

a sin

±π

2α

ηαk

.

2.9

Now we suppose that

pz0

1

ix x >0. 2.10

Then we have

argBz0 −tan−1

asinπ/2αbcosπ/2αηαxαk

acosπ/2αbsinπ/2α

, 2.11

where

kxα≥ 1

2

(4)

Then, by a simple calculation, we see that the functiongx takes the minimum value at

x1−α/1α. Hence, we have

argBz0≤ −tan−1

1α1α/21−α1−α/2asinπ/2αbcosπ/2α ηα

1α1α/21−α1−α/2acosπ/2αbsinπ/2α

π

2β

η, α, a, b ,

2.13

whereβη, α, a, bis given by2.6. This evidently contradicts the assumption ofTheorem 2.2. Next, we suppose that

pz0

1

ix x >0. 2.14

Applying the same method as the above, we have

argBz0≥tan−1

1α1α/21−α1−α/2asinπ/2αbcosπ/2α ηα

1α1α/21−α1−α/2acosπ/2αbsinπ/2α

π

2β

η, α, a, b ,

2.15

whereβη, α, a, bis given by2.6, which is a contradiction to the assumption ofTheorem 2.2. Therefore, we complete the proof ofTheorem 2.2.

Corollary 2.3. Letf ∈ Aandη >0,0< α <1. If

arg1−η zf

z

fz η

1zf

z

fz

< π

2β

η, α zU, 2.16

whereβη, αis given by2.6witha1andb0, thenf ∈ STSα.

Proof. Taking

pz fz

zfz, Bz

1−η zf

z

fz η

1zf

z

fz

2.17

in Theorem 2.2, we can see that 2.4 is satisfied. Therefore, the result follows from

Theorem 2.2.

(5)

By a similar method of the proof inTheorem 2.2, we have the following theorem.

Theorem 2.5. Letpbe nonzero analytic inUwithp0 1and letpsatisfy the differential equation

zpz

pz Bz aibAz, 2.18

wherea∈R,b∈R−∪ {0},Az signImpz, andBzis analytic inUwithB0 a. If

argBz< π

2αδ, a, b z∈U, 2.19

where

αδ:αδ, a, b 2 πtan

−1δb

a δ >0, 2.20

then

argpz< π

2δ z∈U. 2.21

Corollary 2.6. Letf ∈ STSαδ, whereαδis given by2.20witha1andb0. Then

argfz

z < π

2δ z∈U. 2.22

Proof. Letting

pz z

fz, Bz

zfz

fz 2.23

inTheorem 2.5, we haveCorollary 2.6immediately.

If we combine Corollaries2.4and2.6, then we obtain the following result obtained by Nunokawa and Thomas4.

Corollary 2.7. Letf ∈ STCβδ, where

βδ 2 πtan

−1

tanπ 2αδ

αδ

1αδ1αδ/21−αδ1−αδ/2cosπ/2αδ

2.24

andαδis given by2.20. Then

argfz

z < π

(6)

Corollary 2.8. Letf ∈ A,0< α <1andβ,γbe real numbers withβ /0andβγ >0. If

arg

βzf

z

fz γ

< π

2δ

α, β, γ z∈U, 2.26

where

δα, β, γ 2 πtan

−1

tanπ 2α

α

βγ 1α1α/21−α1−α/2cosπ/2α

, 2.27

then

arg

βzF

z

Fz γ

< π

2α z∈U, 2.28

whereFis the integral operator defined by

Fz

βγ

z

0

fβttγ−1dt 1

z∈U. 2.29

Proof. Let

Bz 1

βγ

βzf

z

fz γ

, 2.30

pz βγ

fβz

z

0

fβttγ−1dt. 2.31

ThenBzandpzare analytic inUwithB0 p0 1. By a simple calculation, we have

1

βγzp

z Bzpz 1. 2.32

Using a similar method of the proof inTheorem 2.2, we can obtain that

argpz< π

2α zU. 2.33

From2.29and2.31, we easily see that

(7)

Since

βzF

z

Fz γ βγ

pz, 2.35

the conclusion ofCorollary 2.8immediately follows.

Remark 2.9. Lettingα → 1 inCorollary 2.8, we have the result obtained by Miller and Mocanu

7.

The proof of the following theorem below is much akin to that ofTheorem 2.2and so we omit for details involved.

Theorem 2.10. Letpbe nonzero analytic inUwithp0 1and letpsatisfy the differential equation

zpz

pz Bzpz aibAz, 2.36

wherea∈R,b∈R−∪ {0},Az signImpzandBzis analytic inUwithB0 a. If

argBz< π

2βα, a, b z∈U, 2.37

where

βα, a, b α 2 πtan

−1αb

a 0< α≤1, 2.38

then

argpz< π

2α z∈U. 2.39

Corollary 2.11. Letf∈ Awithfz/0inUand0< α≤1. If

argfz zfz < π

2βα z∈U, 2.40

whereβαis given by2.38witha1andb0, then

argfz< π

2α z∈U, 2.41

(8)

Proof. Let

pz 1

fz, Bz f

z zfz 2.42

inTheorem 2.10. Then2.36is satisfied and so the result follows.

By applyingTheorem 2.10, we have the following result obtained by Mocanu6.

Corollary 2.12. Letf∈ Awithfz/z /0andα0be the solution of the equation given by

2α 2 πtan

−1α1 0< α <1. 2.43

If

argfz< π

21−α0 z∈U, 2.44

thenf ∈ S∗.

Proof. Let

pz z

fz, Bz f

z. 2.45

Then, byTheorem 2.10, condition2.44implies that

arg z

fz < π

2α0. 2.46

Therefore, we have

argzf

z

fz

≤argfzarg z

fz < π

2, 2.47

which completes the proof ofCorollary 2.12.

Corollary 2.13. Letf∈ Awithfzfz/z /0inUand0< α≤1. If

argzf

z

fz

2zf

z

fzzfz

fz

< π

2βα z∈U, 2.48

(9)

Finally, we have the following result.

Theorem 2.14. Letpbe nonzero analytic inUwithp0 1. If

arg1−λpz λzpz < π

2βλ, α, 2.49

βλ, α α 2 πtan

−1 λα

1−λ 0≤λ <1; 0< α <1, 2.50

then

argpz< π

2α z∈U. 2.51

Proof. If there exists a pointz0 ∈Usatisfying the conditions ofLemma 2.1, then we have

1−λpz0 λz0pz0 ±ixα1−λiλαk. 2.52

Now we suppose that

pz0

1

ix x >0. 2.53

Then we have

arg1−λpz0 λz0pz0

π

2αtan

−1 λαk

1−λ

π

2

α 2

πtan

−1 λα

1−λ

π

2βλ, α,

2.54

whereβλ, αis given by2.50. Also, for the case

pz0

1

ix x >0, 2.55

we obtain

arg1−λpz0 λz0pz0 ≤ −

π

2

α 2

πtan

−1 λα

1−λ

π

2βλ, α,

2.56

(10)

Corollary 2.15. Letf∈ Awithfzfz/z /0inUand0< α <1. If

arg

zfz

fz

1zf

z

fzzfz

fz

< π

2α1 z∈U, 2.57

thenf ∈ STSα.

Acknowledgment

This research was supported by Basic Science Research Program through the National Research Foundation of Korea NRF funded by the Ministry of Education, Science and TechnologyNo. 2009-0066192.

References

1 D. A. Brannan and W. E. Kirwan, “On some classes of bounded univalent functions,”Journal of the London Mathematical Society, vol. 1, pp. 431–443, 1969.

2 P. T. Mocanu, “On strongly-starlike and strongly-convex functions,”Studia Universitatis Babes-Bolyai— Series Mathematica, vol. 31, no. 4, pp. 16–21, 1986.

3 M. Nunokawa, “On the order of strongly starlikeness of strongly convex functions,”Proceedings of the Japan Academy, Series A, vol. 69, no. 7, pp. 234–237, 1993.

4 M. Nunokawa and D. K. Thomas, “On convex and starlike functions in a sector,” Journal of the Australian Mathematical Society (Series A), vol. 60, no. 3, pp. 363–368, 1996.

5 P. T. Mocanu, “Alpha-convex integral operator and strongly-starlike functions,”Studia Universitatis Babes-Bolyai—Series Mathematica, vol. 34, no. 2, pp. 19–24, 1989.

6 P. T. Mocanu, “Some starlikeness conditions for analytic functions,”Revue Roumaine de Math´ematiques Pures et Appliqu´ees, vol. 33, no. 1-2, pp. 117–124, 1988.

References

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