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Vol. 8 No. 4 (1985) 779-783

ON A SUBCLASS OF BAZILEVI( FUNCTIONS

D. K. THOMAS

Department of Mathematics and Computer Science University College of Swansea

Singleton Park Swansea SA2 8PP

Wales,

U.

K.

(Received September 24, 1985)

ABSTRACT. Let B() be the class of normalised Bazilevicv functions of type 0 with respect to the starlike function g. Let

BI()

be the subclass of

B()

when g(z) z. Distortion theorems and coefficient estimates are obtained for functions belonging to

BI().

KEY

WORDS AND

PHRASES.

Bazievic

functions, subclasses of S, functions

whose

deriva-

tive has

positive heal part, cose-to-convex functions, coefficient and length-area

estimates.

1980 AMS

SUBJECT CLASSIFICATION CODE.

30C45.

I.

INTRODUCTION.

Let S be the class of normalised functions f which are regular and univalent in the unit disc D {z

IzI<1}.

Let

S*

be the subclass of S consisting of functions which are starlike, and denote by

P,

the class of functions which are regu- lar in D and satisfy there the conditions

p(O) I,

Re p(z) 0 for p

P.

v

Bazilevic [i] showed that if a and are real numbers, with a >

O,

then func- tions f, regular in

D,

and having the representation

rz tiB-1

I/a+i

f(z) [(a+i)

0

p(t)g(t)

dt]

(I.I)

S*

for g p P and z

D,

also form a subclass of S denoted by

B(a,),

which contains both S* and the class of close-to-convex functions. (Powers in (I.I) are principal values). When

B O,

we write

B(a,B) B(a).

Zamorski [2] and the author [3] gave proofs of the Bieberbach conjecture for f e

B(I/N),

N a positive integer, and more recently Leach [4] has shown that the conjecture is true for f

B(a),

0 a

I.

Si,gh [5] considered the subclass

BI()

of

B(),

obtained by taking the star- like function g(z) z and gave sharp estimates for the modules of the coefficients a2, a

3, and

a4,

where for z D,

(2)

[z) z a zn [1.z) n=2 n

We note that

BI(1)

is the subclass of S which consists of functions f for which Re f’(z) 0 for z D [6].

In this paper, we shall obtain some distortion theorems for f

Bl(a)

and give

sharp estimates for the coefficients an in (2) when f e

BI(I/N)

N is a positive

integer.

2. DISTORTION THEOREMS.

THEOREM

I.

Let f e

Bl(a)

and be given by (1.2). Then with z rei0 0 N r

I,

(i)

Q2(r)

1/a _<

If(z)I

_<

Ql(r) I/,

(ii) If 0

a-< I, I-

a-I a l-r <

if ,(z)l ra-IQ

r

Q2 (r) I+--

and if a e

(r)

where

and

a l+r 1-r

1-e 1-a

a-I

a l-r

<

f’(z)l re-IQ 2(r)

a l+r

r

Q1 (r) i+---{ I---

Ql(r)

a

I

0

rOa-I (t_0)v--l+

do,

Q2(r)

a

froa-1

0

(o)do.

Equality holds in all cases for the function

f

defined by

f(z)

(a

fz

0

ta_l.l+tei)dt)i/a

(2

I)

(l_tei

where 0 or n.

PROOF.

(i) Taking 8 0 and g(z)

-=

z in

(I.I),

it follows that f satisfies the equation

1-a l-a

z

f’(z)

f(z) p(z)

(2.2)

for z D and p

P.

Thus

f(z)a

a

f

z

ta-lp (t)dt,

0

and since

Ip(z)I

<_

_

l+r for z e D

[7],

we have at once

If(z)I

<

Ql(r) I/a.

To obtain the left-hand inequality in

(i),

we observe that, since Re p(z) > 0 for z D, Re p(z) ->

r

1-r

[5],

and so from (2.2)

Now let

Zl, [Zll

r

]a

l-r

dz >_ ara-

(]-$r)

(2.3)

be chosen so that

[f(zl)a[ -< [f(z)a[

for all z with

[z[

r.

(3)

Then, writing w

fl(z )(

it follows that the line segment from w 0 to

f(zl)a

lies entirely in the image of D. Let L be the pre-image of % then w

by (2.3) we have

If(zl)la fxldwl fL ]zl

dw

[dzl

a

fr pa-1

0

(1.1.1)d

p

Q2(r),

which is the left-hand inequality in (i).

(ii) The proof follows at once from (2.2) and (i) on noting that for p

P,

1-r

lp(z)l

1+r

1+-’-’-

[7].

Equality is attained in (i) for

f0

and in (ii) for fo when 0 and for when a e 1.

We remark that as 0, the results of Theorem should in some way correspond to the classical distortion theorems for regular starlike (univalent) functions [7].

The following shows that the bounds in Theorem are asymptotic to the classical dis- tortion theorems as 0

THEOREM 2. Let

Q1(r)

and

Q2(r)

be defined as in Theorem

I.

Then for 0 r @

I,

as

I/a

r

(i)

Ql(r)

(l_r)

2’

i/a r

(ii)

’2 r

2

(l-r) (iii)

Ql(r) Q2(r) I.

PROOF.

We prove (i), since (ii) and (iii) are similar. As a-

O,

QI(r)I/

(

fr

0 p

-I 11__+_

)do

I/a

r(l+2ar

- fr

0

i_ do

r

l_2ar-alog

(l_r))I/ -21og(l-r) r

re 2

(l-r) COROLLARY. Suppose that f(z) w for z D then

lwl Q2(1)

I/a as a 0.

PROOF. Let a

O,

and w be a point on the boundary of f(D) closest to the orgin.

Let L denote the straight line from 0 to w and L its pre-mage in D Then

lwl If(z)

for z e

e

n D. Since the circle

Izl

r, for each 0 r inter-

sects L at least once Theorem (i) gives

lw] Q2(r)

I/a and so

[w[ Q2(1)

l/a

as a 0 (from Theorem 2 (ii)).

3. A COEFFICIENT THEOREM.

n n

NOTATION.

nZ=O anZ nZ--O BnZ

means

l=.l -< lnl

for n

-> O.

(4)

THEOREM 3. Let f E

BI(I/N)

with N a positive integer, and be given by

(1.2).

Suppose also that for z

D,

fo(Z)

z

+

n=2

Yn

zn

where

fo

is given by

(2.1).

Then

(i) f(z)

fo(Z),

(ii)

Yn ()N ( N) (log

n)N-I as n

.

PROOF (i) We first note that if

lenl -< IBnl

then for m 1,2

Z

enZ

8 z

n)m

(n=l (nZ-I

n

To see this, let

(n=IZ anzn)

m

nZ=O An(m)

zn and

(nZ=O 8n zn)m nZ=O Bn(m)

z

so that

A(k) A(k_l)

a

B(k)

n

B(k_l)

n

=I

n- n

=I

We now use induction on k to show that for n

-> ’IA(k) -<

B

"k’(

Clearly for

n n

n 2

IA(1)I

D

lanl B

n Bn

(I)

Suppose now that

IA(k)

n < Bn(k) for

n 1,2 and k 1,2 ,j. Then [or n

1,2,...

n (j) n (j)

A(j+I)

n

I IA II an_

<

Z__I

Bn

B

n- Bn Thus (i) now follows at once, since from

(22)

we can write

Pk zk

N f(z) z

I+ kZ__l

k

+I/N

k and since

[pk[

< 2 [7] we have

where p(z)

+ kE__l pk

z

2 k

k

z

]N

f(z) z[l+

k+[/N f0 (z)

(ii) When e

I/N, (2.1)

gives

n 2 zn

]N

z z[ i+

I n$1/N

f0(z)

z

+ nE__2 Yn

n

n z

o(N) (.)’ (nl n+l/N

Now trivially,

n n

(nE--1

n

4-)

<< nE

n/l IN

<<

(nil

Write these three series as

(j+l)

Z

C(9)z

n

D()z

n and l

E(9)z

n= n n= n n=9 n respectively.

Then

n n

(n _.__z )

E E

())z

z

0

n+l

n= n

(5)

Now a result of Littlewood

[8,

p.

193],

states that if is a flxed positive integer and

then

n

()

Thus

Also

zn

) n()

n

(nE=O

n=0 z

(log n)-I

as n

.

n

E(V) () X(log

n)-I

n

n-v

n as n =.

C(V)zn

zn

n= n n=O

+

and so

C

()

0 -J

(j)

n

(j) (-I) n

v’--log n

-I as n n

Thus D()

(log

n)

n n and so

N

(N ()v

D

() ()()(log n)N-I

Yn v$O

n

as n

REFERENCES

I. BAZILEVIC, I. E.,

v On a case of integrability in quadratures of the Loewner-Kurafew equation, Mat. Sb. 37

(79),

471-476. (Russian)

MRIT, #356.

2.

ZAMORSKI, J.,

On Bazilevicv schlicht functions, Ann. Polon. Math.12

(1962),

83-90.

3.

THOMAS,

D.

K.,

On Bazilevic functions, Math. Z. 109

(1969), 344-348.

4.

LEACH,

R.

J.,

The coefficient problem for Bazilevic functions, Houston J. Math. 6

(1980),

543-547.

5.

SINGH, R.,

On Bazilevic functions,

Proc.

Amer. Math. Soc. 38

(1973),

261-271.

6.

MacGREGOR, T. H.,

Functions whose derivative has positive real part, Trans.

Amer.

Math. Soc. 104

(1962),

532-537.

7.

POMMERENKE,

Ch, Univalent Functions, Vandenhoeck and Ruprecht,

Gttingen,

1975.

8.

LITTLEWOOD,

J.

E.,

Theory of functions, Oxford, 1944.

(6)

Special Issue on Space Dynamics

Call for Papers

Space dynamics is a very general title that can accommodate a long list of activities. This kind of research started with the study of the motion of the stars and the planets back to the origin of astronomy, and nowadays it has a large list of topics. It is possible to make a division in two main categories: astronomy and astrodynamics. By astronomy, we can relate topics that deal with the motion of the planets, natural satellites, comets, and so forth. Many important topics of research nowadays are related to those subjects.

By astrodynamics, we mean topics related to spaceflight dynamics.

It means topics where a satellite, a rocket, or any kind of man-made object is travelling in space governed by the grav- itational forces of celestial bodies and/or forces generated by propulsion systems that are available in those objects. Many topics are related to orbit determination, propagation, and orbital maneuvers related to those spacecrafts. Several other topics that are related to this subject are numerical methods, nonlinear dynamics, chaos, and control.

The main objective of this Special Issue is to publish topics that are under study in one of those lines. The idea is to get the most recent researches and published them in a very short time, so we can give a step in order to help scientists and engineers that work in this field to be aware of actual research. All the published papers have to be peer reviewed, but in a fast and accurate way so that the topics are not outdated by the large speed that the information flows nowadays.

Before submission authors should carefully read over the journal’s Author Guidelines, which are located at http://www .hindawi.com/journals/mpe/guidelines.html. Prospective au- thors should submit an electronic copy of their complete manuscript through the journal Manuscript Tracking Sy- stem at http://mts.hindawi.com/ according to the following timetable:

Manuscript Due July 1, 2009 First Round of Reviews October 1, 2009 Publication Date January 1, 2010

Lead Guest Editor

Antonio F. Bertachini A. Prado, Instituto Nacional de Pesquisas Espaciais (INPE), São José dos Campos, 12227-010 São Paulo, Brazil; [email protected]

Guest Editors

Maria Cecilia Zanardi, São Paulo State University (UNESP), Guaratinguetá, 12516-410 São Paulo, Brazil;

[email protected]

Tadashi Yokoyama, Universidade Estadual Paulista (UNESP), Rio Claro, 13506-900 São Paulo, Brazil;

[email protected]

Silvia Maria Giuliatti Winter, São Paulo State University (UNESP), Guaratinguetá, 12516-410 São Paulo, Brazil;

[email protected]

Hindawi Publishing Corporation http://www.hindawi.com

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