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Volume 2010, Article ID 275935,12pages doi:10.1155/2010/275935

Research Article

On Certain Classes of

p

-Valent Functions by Using

Complex-Order and Differential Subordination

Abdolreza Tehranchi

1

and Adem Kılıc¸man

2

1Department of Mathematics, Islamic Azad University, South Tehran Branch, Tehran, Iran

2Department of Mathematics and Institute for Mathematical Research, University Putra Malaysia (UPM),

Serdang, Selangor 43400, Malaysia

Correspondence should be addressed to Adem Kılıc¸man,[email protected]

Received 29 May 2010; Revised 24 September 2010; Accepted 16 October 2010

Academic Editor: Vladimir Mityushev

Copyrightq2010 A. Tehranchi and A. Kılıc¸man. 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.

The aim of the present paper is to study thep-valent analytic functions in the unit disk and satisfy the differential subordinationszIpr, λfzj1/pjIpr, λfzja aB A

Bβz/a1Bz,whereIpr, λis an operator defined by S˘al˘agean andβis a complex number. Further we define a new related integral operator and also study the Fekete-Szego problem by proving some interesting properties.

1. Introduction

LetAbe the class of analytic functions inΔ {z∈C : |z|<1}. LetApdenote the class of all analytic functions in the form of

fz ezp

2p−1

np−1

tn−p1zn−p1 2F1a, b;c;z, |z|<1, 1.1

whereF1a, b;c;zis Gaussian hypergeometric function defined by

2F1a, b;c;z

n0

a, nb, n

c, nn! z n,

a, n Γan

Γa aa1, n−1, c > b >0, c > ab,

tn−p1

a, np1b, np1

c, np1np1! , e >0.

(2)

Note that it is easy to see that these functions are analytic in the unit diskΔ; for more details on hypergeometric functions2F1a, b;c.z, see 1,2.

Definition 1.1. A functionf ∈ Apis said to be in the classS,p-valently starlike functions of orderα, if it satisfies Re{zfz/fz}> α,0≤α < p, z∈Δ. We writeSp0 Sp, the class ofp-valently starlike functions inΔ.

Similarly, a functionf∈ Apis said to be in the classC,p-valently convex of order α, if it satisfies Re{1zfz/fz}> α, 0≤α < p, z∈Δ.

Lethzbe analytic andh0 p. A functionf∈ Apis in the classSphif

zfz

fzhz, z∈Δ. 1.3

The classSphand a corresponding convex classCphwere defined by Ma and Minda in 3. Similar results which are related to the convex class can also be obtained easily from the corresponding functions inSph. For example,

iifp1 and

hz 1z

1−z, 1.4

then the classes reduce to the usual classes of starlike and convex functions;

iiifhz 1 1−2αz/1−zwhere 0≤α <1, then the classes are reduced to the usual classes of starlike and convex functions of orderα;

iiiifhz p1Az/1Bz, where−1≤B < A≤1, then the classes are reduced to the class of Janowski starlike functionsSp A, Bwhich is defined by

Sp A, B

f∈ Ap: zf

fp 1Az

1Bz, −1≤B < A≤1, z∈Δ

; 1.5

ivif hz 1z/1− where p 1 and 0 < α ≤ 1, then the classes reduce to the classes of strongly starlike and convex functions of orderαthat consists of univalent functionsf ∈ Asatisfing

arg

zfz

fz < απ

2 , 0< α≤1, z∈Δ 1.6

or equivalently we have

SSα

f ∈ Ap: zf

f

1z 1−z

α

, 0< α≤1, z∈Δ

(3)

In the literature, there are several works and many researchers have been studying the related problems. For example, Obradovi´c and Owa 4, Silverman 5, Obrad-owiˇc and Tuneski 6, and Tuneski 7have studied the properties of classes of func-tions which are defined in terms of the ratio of 1zfz/fzandzfz/fz.

Definition 1.2. A functionf∈ Apis said to bep-valent Bazilevic of typeηand orderαif there exists a functiongSpsuch that

Re

zfz f1−ηzgηz

> α z∈Δ 1.8

for someη η ≥ 0andα0 ≤ α < p. We denote byBpη, α, the subclass ofApconsisting of all such functions. In particular, a function in Bp1, α Bis said to be p-valently close-to-convex of orderαinΔ.

Definition 1.3. Letfandg be analytic functions inΔ, then we sayf is subordinate togand denoted byfgif there exists a Schwarz functionwz, analytic inΔwithw0 0 and

|wz|<1, such thatfz gwz, z∈Δ. In particular, if the functiongis univalent inΔ, the above subordination is equivalent tof0 g0andfΔ⊂gΔ. Also, we say thatgis superordinate tof; see 8.

Definition 1.4. Motivated by the multiplier transformation on A, we define the operator

Ipr, λ; by the following infinite series whenfz zpnp1anznthen

Ipr, λfz zp

n1p

r

anzn λ≥0. 1.9

S˘al˘agean derivative operator is closely related to the operator Ipr, λ; see 9. In 10, Uralegaddi and Somanatha also studied the caseI1r,1 Ir. The operatorI1r, λ Iλr was studied recently by Cho and Srivastava 11and Cho and Kim 12.

Definition 1.5. Differential operator, for eachfz zp

np1anzn, we have

fjz p! pj!z

p−jn1p

n!

nj!anz

n−j, 1.10

wheren, pN, p > j, andjN0{0} ∪N. In particular, ifj0 we havef0z fz.

Definition 1.6. A function f ∈ Ap is said to be in the class Apλ, r, j;h if it satisfies the following subordination:

zIpr, λfz

j1

pjIpr, λfz

(4)

and in this study we consider

hz 1AB a

βz

1Bz, z∈Δ, 1.12

where−1 ≤B < A ≤1, a > 0 andβ/0is a complex number; so we denoteApλ, r, j;h

Apλ, r, j, β, a, A, B. Then we say that fz is superordinate to hz if fz satisfies the following:

hzz

Ipr, λfz

j1

pjIpr, λfz

j, 1.13

wherehzis analytic inΔandh0 1. Further we note that if

zIpr, λfz

j1

Ipr, λfz

j

pjaaB ABβz

a1Bz hz. 1.14

By choosingj r 0, p 1, soh0 1, thenfzSh. Fora A β 1, B −1, andp ≥ 1, we havefzSp1. But ifa β 1 andj r 0 and−1 ≤ B < A ≤ 1, then fzSA, B, a class of Janowski starlike functions. If we putp a β A 1, B

−1, thenfzSS∗1classes of strongly starlike. ByDefinition 1.2, ifgzS∗, univalent starlike, andj r0 andpaAβ1,B−1 and ifw Re{zfz/fzg2z}>1, then

fz∈ B2,1is a class Bazilevic functions of typeη2 and orderα1.

2. Main Results

Theorem 2.1. Let the functionfzbe of the form1.1. If someA, B,−1< B < A≤1, andβ/0

are complex numbers and

mp1

γλrm, pa1Bδm, j1−δm, jpjδm, jABpjβkm

<βeABδp, j1,

2.1

thenfz∈ Apλ, r, j, β, a, A, B, whereγλrm, p mλ/pλr, δm, j m!/mj! and forr, j∈N0, λ >0, p∈N, j < p. The result is sharp.

Proof. Since the functionfzin the theorem can be expressed in the form

fz ezp

n2p

kn−p1zn−p1 or fz ezp

mp1

(5)

wheremnp1 andkm a, mb, m/c, mm!, and also we have for allr, j∈ N0,

Ipr, λfz

j ep! pj!z

p−jmp1

r m!

mj!kmz m−j

eδp, jzp−j

mp1

γλrm, pδm, jkmzm−j,

2.3

now, assume that the condition 2.1 holds true. We show that f ∈ Apλ, r, j, β, a, A, B. Equivalently, we prove that

az

Ipr, λfz

j1apjI

pr, λfz

j

pjRIpr, λfz

jBazI

pr, λfz

j1

<1, 2.4

whereRaB ABβ. But we have

az

Ipr, λfz

j1

apjIpr, λfz

j

pjRIpr, λfz

j

BazIpr, λfz

j1

amp1γr λ

m, pδm, j1−δm, jpjkmzm−j

βABδp, j1ezp−j−∞mp1γλrm, paBC −δm, jABβpjkmzm−j

< ⎧ ⎪ ⎪ ⎪ ⎪ ⎨ ⎪ ⎪ ⎪ ⎪ ⎩

amp1γλrm, pδm, j1−δm, jpjkm

βeABδ

p, j1−∞mp1γλrm, paBC −δm, jABβpjkm

⎫ ⎪ ⎪ ⎪ ⎪ ⎬ ⎪ ⎪ ⎪ ⎪ ⎭ <1. 2.5

whereCdenotesδm, j1−δm, jpj.

The last inequality is true by2.1and this completes the proof. The result is sharp for the functionsfmzdefined inΔby

fmz

ezp βeA

p, j1

γλrm, pa1Bδm, j1−δm, jpjδm, jABpjβz m

2.6

(6)

Remark 2.2. We observe that ifB /0, the converse of the above theorem needs not be true. For instance, consider the functionfzdefined by

zIpr, λfz

j1

pjIpr, λfz

j

a−SgnBpB ABβz

a1−SgnBBz , 2.7

where SgnB 1,0,−1 thus accordinglyB > 0, B 0 and B < 0. It is easily seen that fz∈ Apλ, r, j, β, a, A, Band

km

1BβeABδp, j1SgnBm−p−1Bm−p−2

a1Bδm, j1δm, jpjδm, jABpjβγλrm, p

mp1

2.8

so that

mp1

γλrm, p

a1Bδm, j1−δm, jpjβABδm, jpj βeABδp, j1

|km|

1B

mp1

Bm−p−2 1B

1−B >1,

2.9

whereA,Bare satisfying the conditions−1≤B < A≤1, 0< B <1. This establishes our claim.

Theorem 2.3. If the functionfz∈ Apλ, r, j, β, a, A, B, then

|km| ≤

βABδp, j1e aγr

λ

m, pδm, j1−δm, jpj, mp−1, 2.10

(7)

Proof. We have

zIpr, λfz

j1

pjIpr, λfz

j

aaB ABβwz

a1Bwz , 2.11

wherewzip1wi−pz

i−pis defined as in theDefinition 1.3. Now we can write

a

ip1

γr λ

i, pδi, j1−δi, jpjkizi−j

⎧ ⎨

βA

p, j1ezp−j− ∞

ip1

γλri, pδi, j1Baδi, jpjRkizi−j

⎫ ⎬ ⎭

ip1

wi−pzi−p,

2.12

whereRaB ABβ. Now if we equalize the coefficients of the same power ofzin both sides, then we have

a m

ip−1

γλri, pδi, j1−δi, jpjkizi−j

im1

cizi−j

⎧ ⎨

βA

p, j1ezp−jm−1

ip1

γλri, pδi, j1Baδi, jpjRkizi−j

⎫ ⎬ ⎭wz,

2.13

where ci’s are suitable constants. By multiplying each side of the above equation by its conjugate and letting|z|1,r → 1−, we get

a2 m

ip−1

γλ2ri, pδi, j1−δi, jpj2|ki|2

βABδp, j1e2 m−1

ip1

γλ2ri, pδi, j1Baδi, jpjR2|ki|2

2.14

so that

a2γλ2rm, pδm, j1−δm, jpj2|km|2

βABδp, j1e2−1−a2 m−1

ip1

γλ2ri, pδi, j1Baδi, jpjR2|ki|2.

(8)

Since−1< B < A≤1 and 0< a < AB <1, we have

|km| ≤

βABδp, j1e aγr

λ

m, pδm, j1−δm, jpj, mp−1 2.16

and this completes the proof. Note that the estimate in2.10is sharp for the functionsfmz defined inΔ; whenjr 0 in1.3, then

fmz exp

z

0

pψtRa t1Bψtdt

, m≥1p, 2.17

where|ψt|<1,z∈ΔandRaB ABβ. We can chooseψt tm.

Theorem 2.4 Fekete-Szego Problem. Let the functionfz, given by 2.2, be in the class

Apλ, j, β, a, A, Bandμany complex number. Then

kp2−μk2p1

A

p, j1 2aγλrp2, p

×max

⎧ ⎨ ⎩1,

r λ

p2, pδp2, jλrp1, pδp1, jμABδp, j1 aγr

λ

p1, p2

⎫ ⎬ ⎭.

2.18

Proof. On using the coefficients ofzp1andzp2, we get

kp1 ABβeδ

p, j1 λrp1, pδp1, jw1,

kp2

ABeβδp, j1 λrp2, p2δp2, jw2−

ABeβδp, j1 λrp1, pδp1, jw

2 1.

2.19

By using 13that

w2−ρw21≤max

(9)

for every complex numberρ, then we can write

kp2−μk2p1

|1

aA

p, j1

w2

r λ

p2, pδp2, j −

w2 1

γr λ

p1, pδp1, j

μ

ABδp, j1 λrp1, pδp1, j

2

w12|

| A

p, j1 2aγr

λ

p2, pδp2, jw2

A

p, j1eβaγλrp1, pδp1, j−μABδp, j12

λrp1, pδp1, j2 w

2 1|

A

p, j1 2aγr

λ

p2, p

w2−hw12,

2.21

where

hr λ

p2, pδp2, jaγr λ

p1, pδp1, j−μABeβδp, j1 aγr

λ

p1, pδp1, j2 . 2.22

3. Integral Operator

Now, we introduce a new integral operator which is denoted by Gη,pz on functions belonging toApas follows:

Gη,pz e

1−ηzpηp

z

ft

t dt

0< η <1, −→0, 3.1

and we verify the effect of this operator on1.11; with a simple calculation, we have

Gη,pz e

1−ηzpηp

⎡ ⎣z

etp−1mp1

kmtm−1

⎞ ⎠dt

⎦ 0< η <1, −→0

e1−ηzpηezp

mp1

ηp mkmz

m

ezp

mp1

dmzm,

(10)

wheredm ηp/mkm. If we putrj 0 in1.11, then we obtain

zfz pfz

aaB ABβz

a1Bz 3.3

that is denoted byApλ,0,0, β, a, A, B Apλ, β, a, A, B.

Now if we letAp,ηλ, β, a, A, Bbe a class of functionsGη,pzanalytic inΔand defined by3.1wherefz∈ Apλ, β, a, A, B. Then on using3.1and definition of subordination, we have the following theorem.

Theorem 3.1. Gη,pz∈ Ap,ηλ, β, a, A, Bif and only if

zcgη,p z z2G

η,pzep2

1−ηzp pzGη,pep2

1−ηzp

aaB ABβz

a1Bz . 3.4

Proof. The conditions3.3and3.1give

G

η,pz ep

1−ηzp−1ηpfz

z or fz

zGη,pz ηp

e1−ηzp

η ,

fz 1 η, p

G

η,pz zGη,p z

ep

η

1−ηzp−1

1

ηp

Hη,pz

ep η

1−ηzp−1,

3.5

whereHη,pz zGη,pz. By puttingfzandfzin3.3, we obtain

zfz pfz

zHη,p zep21ηzp Hη,pzep2

1−ηzp

zGη,p z z 2G

η,pzep2

1−ηzp pzGη,p zep2

1−ηzp

aaB ABβz a1Bz .

3.6

With a simple calculation onFξz, we have

Fξz

⎡ ⎣z

0

sξ−1

espmp1

kmsm

⎞ ⎠ds

⎤ ⎦

ezp

mp1

mξkmz

m

ezp

p1

bmzm wherebm mξkm.

(11)

LetAp,ξλ, β, a, A, Bbe the class of functionsFξzanalytic inΔdefined byf ∈ Apλ, β, a, A, B. We can write next theorem on using3.3and definition of subordination.

Theorem 3.2. TheFξz∈ Ap,ξλ, β, a, A, Bif and only if

1Fξz zFξz

pξFξz zFξz

a

aB ABβz

a1Bz . 3.8

Proof. Since

Fξz

z

0

sξ−1fsds, 3.9

then we have

fz 1

ξFξz zFξz

,

fz 1

ξ1Fξz zFξz.

3.10

Now by making substitutionfzandfzin3.3, we obtain

zfz pfz

z/pξξ1Fξz zFξz

p/pξξFξz zFξz

z

ξ1Fξz zFξz

pξFξz zFξz

a

aB ABβz a1Bz .

3.11

Acknowledgments

The authors would like to thank refereesfor the very useful comments that improved the quality of the paper very much. The second author also acknowledges that this research was partially supported by the University Putra Malaysia under the Research University Grant SchemeRUGSno. 05-01-09-0720RU.

References

1 C. E. Andrews, R. Askey, and R. Roy, Special Functions, Cambridge University Press, Cambridge, UK, 1991.

2 Y. C. Kim and F. Rønning, “Integral transforms of certain subclasses of analytic functions,” Journal of

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3 W. C. Ma and D. Minda, “A unified treatment of some special classes of univalent functions,” in

Proceedings of the Conference on Complex Analysis, pp. 157–169, International Press, Tianjin, China.

4 M. Obradovi´c and S. Owa, “A criterion for starlikeness,” Mathematische Nachrichten, vol. 140, pp. 97– 102, 1989.

5 H. Silverman, “Convex and starlike criteria,” International Journal of Mathematics and Mathematical

Sciences, vol. 22, no. 1, pp. 75–79, 1999.

6 M. Obradowiˇc and N. Tuneski, “On the starlike criteria defined by Silverman,” Zeszyty Naukowe

Politechniki Rzeszowskiej. Matematyka, no. 24, pp. 59–64, 2000.

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Nachrichten, vol. 248-249, pp. 200–203, 2003.

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Bucharest, Romania, 1981.

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References

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