Volume 2010, Article ID 302583,11pages doi:10.1155/2010/302583
Research Article
Classes of Meromorphic Functions Defined by
the Hadamard Product
J. Dziok
Institute of Mathematics, University of Rzesz´ow, ul. Rejtana 16A, 35-310 Rzesz´ow, Poland
Correspondence should be addressed to J. Dziok,[email protected]
Received 2 July 2009; Revised 21 November 2009; Accepted 5 January 2010
Academic Editor: Vladimir Mityushev
Copyrightq2010 J. Dziok. 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 object of the present paper is to introduce new classes of meromorphic functions with varying argument of coefficients defined by means of the Hadamard productor convolution. Several properties like the coefficients bounds, growth and distortion theorems, radii of starlikeness and convexity, and partial sums are investigated. Some consequences of the main results for well-known classes of meromorphic functions are also pointed out.
1. Introduction
LetMdenote the class of functions which are analytic inDD1, where
Dr {z∈C: 0<|z|< r}, 1.1
with a simple pole in the pointz 0.ByM,we denote the class of functionsf ∈ Mof the form
fz 1 z
∞
n1
anzn z∈ D. 1.2
Also, byTε
η η ∈R, ε∈ {0,1},we denote the class of functionsf ∈ Mof the form1.2for which
Forη0,we obtain the classesT00andT10of functions with positive coefficients and negative coefficients, respectively.
Motivated by Silverman1, we define the class
Tε: η∈R
Tε
η. 1.4
It is called the class of functions with varying argument of coefficients.
Letα∈ 0,1, r ∈0,1.A functionf ∈ Mis said to be meromorphically convex of order αinDrif
Re
1zf
z
fz
<−α z∈ Dr. 1.5
A functionf ∈ Mis said to be meromorphically starlike of orderαinDrif
Re
zfz
fz
<−α z∈ Dr. 1.6
We denote byMScαthe class of all functionsf ∈ M, which are meromorphically convex of order α in D and by MS∗α, we denote the class of all functionsf ∈ M,which are meromorphically starlike of orderαinD. We also set
MScMSc0, MS∗MS∗0. 1.7
It is easy to show that for a functionf∈ T0
η,the condition1.6is equivalent to the following:
zffzz1<1−α z∈ Dr. 1.8
LetBbe a subclass of the classM. We define the radius of starlikeness of orderαand the radius of convexity of orderαfor the classBby
R∗αB inf f∈B
sup r∈0,1:f is meromorphically starlike of orderαinDr;
RcαB inf f∈B
sup r∈0,1:f is meromorphically convex of orderαinDr, 1.9
respectively.
Let functionsf, gbe analytic inU:D ∪ {0}.We say that the functionfis subordinate to the functiong, and writefz≺gz or simplyf ≺gif there exists a functionωanalytic inU,|ωz| ≤ |z|z∈ U,such that
In particular, ifFis univalent inU, we have the following equivalence:
fz≺Fz⇐⇒f0 F0, fU⊂FU. 1.11
For functionsf, g∈Mof the form
fz ∞
n−1
anzn, gz ∞
n−1
bnzn, 1.12
byf∗gwe denote the Hadamard productor convolutionoffandg, defined by
f∗gz ∞
n−1
anbnzn z∈ D. 1.13
LetA, Bbe real parameters,−1 ≤A < B ≤1,and letϕ, φbe given functions from the classM.
ByWφ, ϕ;A, B,we denote the class of functionsf ∈ Msuch thatϕ∗fz/0 z∈ D and
φ∗fz
ϕ∗fz ≺
1Az
1Bz. 1.14
Moreover, let us define
TWεφ, ϕ;A, B:Tε∩ Wφ, ϕ;A, B,
TWε η
φ, ϕ;A, B:Tεη∩ Wφ, ϕ;A, B, 1.15
where the functionsϕ, φhave the form
φz 1 z −1
ε1∞
n1
βnzn, ϕz 1 z −1
ε∞
n1
αnzn z∈ D, 1.16
and the sequences{αn},{βn}are nonnegative real, with
αnβn>0 n∈N. 1.17
Moreover, let us put
It is easy to show that
fz∈ TWzφz, zϕz;A, B⇐⇒ −zfz∈ TWφ, ϕ;A, B,
fz∈ TW0ηzφz, zϕz;A, B⇐⇒ −zfz∈ TW1ηφ, ϕ;A, B. 1.19
The object of the present paper is to investigate the coefficient estimates, distortion properties and the radii of starlikeness and convexity, and partial sums for the classes of meromorphic functions with varying argument of coefficients. Some remarks depicting consequences of the main results are also mentioned.
2. Coefficients Estimates
First we mention a sufficient condition for functions to belong to the classWφ, ϕ;A, B.
Theorem 2.1. Let{dn}be defined by1.18,−1 ≤ A < B ≤ 1. If a functionf of the form1.2 satisfies the condition
∞
n1
dn|an| ≤B−A, 2.1
thenfbelongs to the classWφ, ϕ;A, B.
Proof. A functionf of the form1.2belongs to the classWεφ, ϕ;A, Bif and only if there exists a functionω,|ωz| ≤ |z|z∈ D,such that
φ∗fz
ϕ∗fz
1Aωz
1Bωz z∈ D, 2.2
or equivalently
zφ∗fz−zϕ∗fz Bzφ∗fz−Azϕ∗fz
<1 z∈ D. 2.3
Thus, it is sufficient to prove that
z
Indeed, letting|z|r 0< r <1,we have
z
ϕ∗fz−zφ∗fz−Bzφ∗fz−Azϕ∗fz
∞ n1
βnαnanzn1−B−A− ∞
n1
BβnAαnanzn1
≤∞
n1
βnαn|an|rn1−B−A ∞
n1
BβnAαn|an|rn1
≤∞
n1
dn|an|rn1−B−A<0,
2.5
whencef∈ Wφ, ϕ;A, B.
Theorem 2.2. Let f be a function of the form 1.2, with 1.3. Then f belongs to the class
TWε
ηφ, ϕ;A, Bif and only if the condition2.1holds true.
Proof. In view of Theorem 2.1, we need only to show that each function f from the class TWε
ηφ, ϕ;A, B satisfies the coefficient inequality 2.1. Let f ∈ TWεηφ, ϕ;A, B. Then by 2.3and1.2, we have
∞
n1
βnαnanzn1
B−A−∞n1−1εBβnAαnanzn1
<1 z∈ D. 2.6
Therefore, puttingzreiη 0≤r <1,and applying1.3, we obtain
∞
n1
βnαn|an|rn1
B−A−∞n1BβnAαn|an|rn1 <1. 2.7
It is clear, that the denominator of the left hand said cannot vanish forr ∈ 0,1.Moreover, it is positive forr0,and in consequence forr ∈ 0,1.Thus, by2.7, we have
∞
n1
1Bβn 1Aαn|an|rn1< B−A, 2.8
which, upon lettingr → 1−, readily yields the assertion2.1.
FromTheorem 2.2, we obtain coefficients estimates for the classTWε
ηφ, ϕ;A, B.
Corollary 2.3. If a functionfof the form1.2belongs to the classTWε
ηφ, ϕ;A, B,then
|an| ≤B−A
dn
where{dn}is defined by1.18. The result is sharp. The functionsfn,ηof the form
fn,ηz 1 z
B−A
ei{n1η−επ}dnzn z∈ D; n∈N 2.10
are the extremal functions.
3. Distortion Theorems
FromTheorem 2.2, we have the following lemma.
Lemma 3.1. Let a functionf of the form1.2belong to the classTWε
ηφ, ϕ;A, B.If the sequence
{dn}defined by1.18satisfies the inequality
d1≤dn n∈N, 3.1
then
∞
n1
an≤ B−A
d1
. 3.2
Moreover, if
nd1 ≤dn n∈N, 3.3
then
∞
n1
nan≤ B−A
d1
. 3.4
Theorem 3.2. Let a functionf belong to the classTWε
ηφ, ϕ;A, B.If the sequence{dn}defined by 1.18satisfies3.1, then
1 r −
B−A d1 r≤
fz≤ 1 r
B−A
d1 r |z|r <1. 3.5
Moreover, if3.3holds, then
1 r2 −
B−A d1 ≤
fz≤ 1 r2
B−A d1 |
z|r <1. 3.6
Proof. Let a functionfof the form1.2belong to the classTWε
ηφ, ϕ;A, B, |z|r <1.Since
fz1 z
∞
n1
anzn
≤ 1 r ∞ n1 |an|rn
1 r r
∞
n1
|an|rn−1≤ 1 r r
∞
n1 |an|,
fzz ∞
n1
anzn
≥ 1 r − ∞ n1 |an|rn
1 r −r
∞
n1
|an|rn−1≥ 1 r −r
∞
n1 |an|,
3.7
then byLemma 3.1we have3.5. Analogously we prove3.6.
4. The Radii of Convexity and Starlikeness
Theorem 4.1. The radius of starlikeness of orderαfor the classTW0
ηφ, ϕ;A, Bis given by
R∗αTW0ηφ, ϕ;A, B inf n∈N
1−αdn n−αB−A
1/n1
, 4.1
wherednis defined by1.18.
Proof. The functionf ∈ T0
ηof the form1.2is meromorphically starlike of orderαin the disk
Dr,0< r≤1,if and only if it satisfies the condition1.8. Since
zffzz1
∞
n1n1 anzn1 1∞n1anzn1
≤
∞
n1n1|an||z|n1
1−∞n1|an||z|n1 , 4.2
putting|z|r,the condition1.8is true if
∞
n1
n−α 1−α|an|r
n1 ≤1. 4.3
ByTheorem 2.2, we have
∞
n1
dn
B−A|an| ≤1. 4.4
Thus, the condition4.3is true if
n−α 1−αr
n1 ≤ dn
that is, if
r ≤
1−αdn n−αB−A
1/n1
n∈N. 4.6
It follows that each functionf ∈ TW0
ηφ, ϕ;A, Bis meromorphically starlike of orderαin the disk Dr, where r R∗TW0
ηφ, ϕ;A, B is defined by4.1. Moreover, the radius of starlikeness of the functionsfn,ηdefined by2.10is given by
rn∗min
1,
1−αdn n−αB−A
1/n1
n∈N. 4.7
Thus we have4.1.
Theorem 4.2. The radius of convexity of orderαfor the classTW1
ηφ, ϕ;A, Bis given by
RcαTW1ηφ, ϕ;A, Binf n∈N
1−αdn nn−αB−A
1/n1
, 4.8
wherednis defined by1.18.
Proof. The proof is analogous to that ofTheorem 4.1, and we omit the details.
5. Partial Sums
Letf∈ Mbe a function of the form1.2. Motivated by Silverman2and Silvia3 see also
4, we define the partial sumsfmdefined by
fmz 1 z
m
n1
anzn m∈N. 5.1
In this section, we consider partial sums of functions from the class TWε
ηφ, ϕ;A, B and obtain sharp lower bounds for the real part of ratios offtofmandftofm.
Theorem 5.1. Letm∈Nand let the sequence{dn},defined by1.18, satisfy the inequalities
B−A≤dn≤dn1 m∈N. 5.2
If a functionfbelongs to the classTWε
ηφ, ϕ;A, B,then
Re fz
fmz
≥1−B−A dm1
z∈ D, 5.3
Re
f
mz fz
≥ dm1
B−Adm1
z∈ D. 5.4
Proof. Let a functionfof the form1.2belong to the classTWε
ηφ, ϕ;A, B.Then by5.2and Theorem 2.2, we have
m
n1 |an|
dm1
B−A ∞
nm1 |an| ≤
∞
n1
dn
B−A|an| ≤1. 5.5
If we put
gz dm1 B−A
fz
fmz−
1−B−A dm1
1dm1/B−A
∞
nm1anzn1 1mn1anzn1
z∈ D,
5.6
then it suffices to show that
Regz≥0 z∈ D, 5.7
or
ggzz−11≤1 z∈ D. 5.8
Applying5.5, we find that
ggzz−11≤ dm1/B−A∞nm1|an| 2−2nn1|an| −dm1/B−A
∞
nm1|an|
≤1 z∈ D, 5.9
which readily yields the assertion5.3. In order to see thatffm1,η gives the result sharp, we observe that forzreiηwe have
fz fmz
1−B−Arm 2
dm1
r−→→1−
1−B−A dm1
. 5.10
Similarly, if we take
hz B−Adm1 fmz
fz −
dm1
B−Adm1
z∈ D, 5.11
and make use of5.5, we can deduce that
hhzz−11≤ 1 dm1/B−A
∞
nm1|an|
2−2mn1|an| −1−dm1/B−A∞nm1|an|
≤1 z∈ D, 5.12
Theorem 5.2. Letm∈Nand let the sequence{dn},defined by1.18, satisfy the inequalities5.2. If a functionfbelongs to the classTWε
ηφ, ϕ;A, B,then
Re
fz fmz
≥1−B−Am1
dm1 z∈ D,
Re
f
mz fz
≥ dm1
B−Am1 dm1 z∈ D.
5.13
The bounds are sharp, with the extremal functionfm1,η of the form2.10.
Proof. The proof is analogous to that ofTheorem 5.1, and we omit the details.
Remark 5.3. We observe that the obtained results are true if we replace the class
TWε
ηφ, ϕ;A, BbyTWεφ, ϕ;A, B.
6. Concluding Remarks
We conclude this paper by observing that, in view of the subordination relation1.18, by choosing the functionsφ and ϕ, we can define new classes of functions. In particular, the class
Wϕ;A, B:W−zϕz, ϕz;A, B 6.1
contains functionsf ∈ M,such that
−z
ϕ∗fz
ϕ∗fz ≺
1Az
1Bz. 6.2
A functionf ∈ Mbelongs to the class
Wϕ;α:Wϕ; 2α−1, α 0≤α <1 6.3
if it satisfies the condition
Re
−z
ϕ∗fz
ϕ∗fz
> α z∈ D. 6.4
The classWϕ;αis related to the class of starlike function of orderα. In particular, we have the following relationships:
S∗α W 1 z1−z;α
,
Scα W
1−2z z1−z2;α
.
Letλbe a convex parameter. A functionf∈ Mbelongs to the class
Wλ
ϕ;A, B:W
λzϕz λ−1z2ϕz,1 z;A, B
6.6
if it satisfies the condition
λzϕ∗fz λ−1z2ϕ∗fz≺ 1Az
1Bz. 6.7
The classes Wϕ;A, B,Wϕ;α,and Wλϕ;A, Bgeneralize well-known important classes, which were investigated in earlier works; see for example5–10.
If we apply the results presented in this paper to the classes discussed above, we can obtain several additional results. Some of these results were obtained in earlier works; see for example5–10.
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