Coefficient Bounds S. K. Lee, V. Ravichandran
and S. Shamani vol. 10, iss. 3, art. 71, 2009
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COEFFICIENT BOUNDS FOR MEROMORPHIC STARLIKE AND CONVEX FUNCTIONS
SEE KEONG LEE V. RAVICHANDRAN
Universiti Sains Malaysia Department of Mathematics
11800 USM Penang, University of Delhi
Malaysia Delhi 110 007, India
EMail:sklee@cs.usm.my EMail:vravi@maths.du.ac.in
SUPRAMANIAM SHAMANI
School of Mathematical Sciences Universiti Sains Malaysia 11800 USM Penang, Malaysia EMail:sham105@hotmail.com
Received: 30 January, 2008
Accepted: 03 May, 2009
Communicated by: S.S. Dragomir
2000 AMS Sub. Class.: Primary 30C45, Secondary 30C80.
Key words: Univalent meromorphic functions; starlike function, convex function, Fekete- Szegö inequality.
Coefficient Bounds S. K. Lee, V. Ravichandran
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Close Abstract: In this paper, some subclasses of meromorphic univalent functions in the
unit disk∆are extended. LetU(p)denote the class of normalized univa- lent meromorphic functionsf in∆with a simple pole atz =p >0. Let φbe a function with positive real part on∆ withφ(0) = 1,φ0(0) > 0 which maps∆onto a region starlike with respect to1which is symmetric with respect to the real axis. The classP∗
(p, w0, φ)consists of functions f ∈U(p)satisfying
−
zf0(z) f(z)−w0
+ p
z−p− pz 1−pz
≺φ(z).
The classP(p, φ)consists of functionsf ∈U(p)satisfying
−
1 +zf00(z) f0(z) + 2p
z−p− 2pz 1−pz
≺φ(z).
The bounds forw0and some initial coefficients off inP∗
(p, w0, φ)and P(p, φ)are obtained.
Acknowledgment: This research is supported by Short Term grant from Universiti Sains Malaysia and also a grant from University of Delhi.
Coefficient Bounds S. K. Lee, V. Ravichandran
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Contents
1 Introduction 4
2 Coefficients Bound Problem 7
Coefficient Bounds S. K. Lee, V. Ravichandran
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1. Introduction
LetU(p)denote the class of univalent meromorphic functions f in the unit disk ∆ with a simple pole atz=p > 0and with the normalizationf(0) = 0andf0(0) = 1.
LetU∗(p, w0)be the subclass ofU(p)such thatf(z)∈U∗(p, w0)if and only if there is aρ,0< ρ < 1, with the property that
< zf0(z) f(z)−w0 <0
for ρ < |z| < 1. The functions inU∗(p, w0) map |z| < r < ρ (for some ρ, p <
ρ < 1) onto the complement of a set which is starlike with respect to w0. Further the functions inU∗(p, w0)all omit the valuew0. This class of starlike meromorphic functions is developed from Robertson’s concept of star center points [11]. Let P denote the class of functionsP(z)which are meromorphic in∆and satisfyP(0) = 1 and<{P(z)} ≥0for allz ∈∆.
Forf(z)∈U∗(p, w0), there is a functionP(z)∈ P such that
(1.1) z f0(z)
f(z)−w0 + p
z−p− pz
1−pz =−P(z) for allz ∈ ∆. LetP∗
(p, w0)denote the class of functionsf(z)which satisfy (1.1) and the condition f(0) = 0, f0(0) = 1. ThenU∗(p, w0) is a subset ofP∗
(p, w0).
Miller [9] proved thatU∗(p, w0) =P∗
(p, w0)forp≤2−√ 3.
LetK(p)denote the class of functions which belong toU(p)and map|z|< r < ρ (for somep < ρ <1) onto the complement of a convex set. Iff ∈K(p), then there is ap < ρ <1, such that for eachz,ρ <|z|<1
<
1 + zf00(z) f0(z)
≤0.
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Iff ∈K(p),then for eachzin∆,
(1.2) <
1 +zf00(z)
f0(z) + 2p
z−p − 2pz 1−pz
≤0.
Let P
(p) denote the class of functions f which satisfy (1.2) and the conditions f(0) = 0andf0(0) = 1.The classK(p)is contained inP
(p).Royster [12] showed that for0 < p ≤ 2−√
3, iff ∈ P
(p)and is meromorphic, thenf ∈ K(p).Also, for each functionf ∈P
(p),there is a functionP ∈ P such that 1 +zf00(z)
f0(z) + 2p
z−p− 2pz
1−pz =−P(z).
The classU(p)and related classes have been studied in [3], [4], [5] and [6].
Let A be the class of all analytic functions of the form f(z) = z + a2z2 + a3z3 +· · · in∆. Several subclasses of univalent functions are characterized by the quantitieszf0(z)/f(z)or1 +zf00(z)/f0(z)lying often in a region in the right-half plane. Ma and Minda [7] gave a unified presentation of various subclasses of convex and starlike functions. For an analytic functionφwith positive real part on ∆with φ(0) = 1, φ0(0) > 0which maps the unit disk∆onto a region starlike (univalent) with respect to1which is symmetric with respect to the real axis, they considered the classS∗(φ)consisting of functionsf ∈ Afor whichzf0(z)/f(z)≺φ(z) (z ∈∆).
They also investigated a corresponding class C(φ) of functions f ∈ A satisfying 1 + zf00(z)/f0(z) ≺ φ(z) (z ∈ ∆). For related results, see [1, 2, 8, 13]. In the following definition, we consider the corresponding extension for meromorphic univalent functions.
Definition 1.1. Let φ be a function with positive real part on ∆ with φ(0) = 1, φ0(0) >0which maps∆onto a region starlike with respect to1which is symmetric
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with respect to the real axis. The classP∗
(p, w0, φ)consists of functionsf ∈U(p) satisfying
−
zf0(z)
f(z)−w0 + p
z−p − pz 1−pz
≺φ(z) (z ∈∆).
The classP
(p, φ)consists of functionsf ∈U(p)satisfying
−
1 +zf00(z)
f0(z) + 2p
z−p − 2pz 1−pz
≺φ(z) (z ∈∆).
In this paper, the bounds on|w0|will be determined. Also the bounds for some coefficients off inP∗
(p, w0, φ)andP
(p, φ)will be obtained.
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2. Coefficients Bound Problem
To prove our main result, we need the following:
Lemma 2.1 ([7]). Ifp1(z) = 1 +c1z+c2z2 +· · · is a function with positive real part in∆, then
|c2−vc21| ≤
−4v+ 2 if v ≤0, 2 if 0≤v ≤1, 4v−2 if v ≥1.
Whenv <0orv >1, equality holds if and only ifp1(z)is(1 +z)/(1−z)or one of its rotations. If0< v <1, then equality holds if and only ifp1(z)is(1+z2)/(1−z2) or one of its rotations. Ifv = 0, the equality holds if and only if
p1(z) = 1
2+ 1 2λ
1 +z 1−z +
1 2 − 1
2λ
1−z
1 +z (0≤λ ≤1)
or one of its rotations. Ifv = 1, the equality holds if and only ifp1 is the reciprocal of one of the functions such that equality holds in the case ofv = 0.
Theorem 2.2. Let φ(z) = 1 +B1z +B2z2 +· · · andf(z) = z +a2z2 +· · · in
|z|< p. Iff ∈P∗
(p, w0, φ), then
w0 = 2p
pB1c1−2p2−2 and
(2.1) p
p2+B1p+ 1 ≤ |w0| ≤ p p2−B1p+ 1.
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Also, we have
(2.2)
a2+ w0 2
p2+ 1 p2 + 1
w02
≤
|w0||B2|
2 if |B2| ≥B1,
|w0|B1
2 if |B2| ≤B1. Proof. Lethbe defined by
h(z) =−
zf0(z)
f(z)−w0 + p
z−p − pz 1−pz
= 1 +b1z+b2z2+· · · .
Then it follows that
b1 =p+ 1 p+ 1
w0
, and (2.3)
b2 =p2+ 1 p2 + 1
w20 +2a2
w0. (2.4)
Sinceφis univalent andh≺φ, the function p1(z) = 1 +φ−1(h(z))
1−φ−1(h(z)) = 1 +c1z+c2z2+· · ·
is analytic and has a positive real part in∆. Also, we have
(2.5) h(z) =φ
p1(z)−1 p1(z) + 1
and from this equation (2.5), we obtain
(2.6) b1 = 1
2B1c1
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and
(2.7) b2 = 1
2B1
c2− 1 2c21
+ 1
4B2c21.
From (2.3), (2.4), (2.6) and (2.7), we get
(2.8) w0 = 2p
pB1c1−2p2−2 and
(2.9) a2 = w0
8 (2B1c2−B1c21+B2c21)− p2w0 2 − w0
2p2 − 1 2w0. From (2.3) and (2.6), we obtain
p+1 p + 1
w0 = 1 2B1c1
and, since|c1| ≤2for a function with positive real part, we have
p+ 1 p− 1
|w0|
≤
p+ 1 p+ 1
w0
≤ 1
2B1|c1| ≤B1 or
−B1 ≤p+1 p − 1
|w0| ≤B1. Rewriting the inequality, we obtain
p
p2+B1p+ 1 ≤ |w0| ≤ p p2−B1p+ 1.
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From (2.9), we obtain
a2 +w0 2
p2+ 1 p2 + 1
w20
=
w0 2
1 2B1
c2− 1
2c21
+1 4B2c21
= |w0|B1 4
c2−
B1−B2 2B1
c21
.
The result now follows from Lemma2.1.
The classes P∗
(p, w0, φ) andP
(p, φ)are indeed a more general class of func- tions, as can be seen in the following corollaries.
Corollary 2.3 ([10, inequality 4, p. 447]). Iff(z)∈P∗
(p, w0), then p
(1 +p)2 ≤ |w0| ≤ p (1−p)2. Proof. LetB1 = 2in (2.1) of Theorem2.2.
Corollary 2.4 ([10, Theorem 1, p. 447]). Letf ∈P∗
(p, w0)andf(z) = z+a2z2+
· · · in|z|< p. Then the second coefficienta2 is given by
a2 = 1 2w0
b2−p2− 1 p2 − 1
w02
,
where the region of variability fora2 is contained in the disk
a2+ 1 2w0
p2+ 1 p2 + 1
w02
≤ |w0|.
Proof. LetB1 = 2in (2.2) of Theorem2.2.
The next theorem is for convex meromorphic functions.
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Theorem 2.5. Let φ(z) = 1 +B1z +B2z2 +· · · andf(z) = z +a2z2 +· · · in
|z|< p. Iff ∈P
(p, φ), then
2p2 −B1p+ 2
2p ≤ |a2| ≤ 2p2+B1p+ 2
2p .
Also
a3− 1 3
p2+ 1 p2
−2
3a22−µ
a2−p− 1 p
2
≤
|2B2+3µB12|
12 if |2BB2
1 + 3µB1| ≥2,
B1
6 if |2BB2
1 + 3µB1| ≤2.
Proof. Lethnow be defined by h(z) =−
1 + zf00(z)
f0(z) + 2p
z−p − 2pz 1−pz
= 1 +b1z+b2z2+· · ·
andp1 be defined as in the proof of Theorem2.2. A computation shows that b1 = 2
p+1
p −a2
, and (2.10)
b2 = 2
p2+ 1
p2 + 2a22−3a3
. (2.11)
From (2.6) and (2.10), we have
(2.12) a2 =p+1
p − B1c1 4 .
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From (2.7) and (2.11), we have (2.13) a3 = 1
24
8p2+ 8
p2 + 16a22−2B1c2+B1c21−B2c21
. From (2.12), we have
2p+2
p −2a2 = 1 2B1c1
or
2p+2
p −2|a2|
≤ |2p+ 2
p−2a2| ≤ 1
2B1|c1| ≤B1. Thus we have
−B1 ≤2p+ (2/p)−2|a2| ≤B1 or
2p2 −B1p+ 2
2p ≤ |a2| ≤ 2p2+B1p+ 2
2p .
From (2.12) and (2.13), we obtain
a3− 1 3
p2+ 1 p2
−2
3a22−µ
a2−p− 1 p
2
=
1
24 −2B1c2 +B1c21−B2c21
−µ
B12c21 16
= B1 12
c2− 1
2− B2
2B1 − 3µB1 4
c21
. The result now follows from Lemma2.1.
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References
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[11] M.S. ROBERTSON, Star center points of multivalent functions, Duke Math. J., 12 (1945), 669–684.
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