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Radius properties for analytic and p-valently starlike functions
Journal of Inequalities and Applications volume 2011, Article number: 107 (2011)
Abstract
Let be the class of functions f(z) which are analytic in the open unit disk and satisfy . Also, let denotes the subclass of consisting of f(z) which are p-valently starlike of order α(0 ≦ α < p). A new subclass of is introduced by
for some real λ > 0. The object of the present paper is to consider some radius properties for such that .
2010 Mathematics Subject Classification: Primary 30C45.
1 Introduction
Let be the class of functions f(z) of the form
which are analytic in the open unit disk and satisfy
For , we say that f(z) belongs to the class if it satisfies
for some real number λ > 0.
Let us consider a function f δ (z) given by
Then, we can write that
with
and
Thus, if δ = 2, then
This shows that for λ ≧ 1.
If δ = 3, then we have that
Which shows that for λ ≧ 5.
Further, if δ = 4, then
which shows that for λ ≧ 11.
If p = 1, then is defined by
for some real number λ > 0. Note that (1.5) is equivalent to
Therefore, this class was considered by Obradović and Ponnusamy [1]. Further-more, this class was extended as the class by Shimoda et al. [2].
Let denotes the subclass of consisting of f(z) which satisfy
for some real α (0 ≦ α < p).
A function is said to be p-valently starlike of order α in (cf. Robertson [3]).
2 Coefficient inequalities
For , we consider the sufficient condition for f(z) to be in the class .
Lemma 1 If satisfies
then .
Proof We note that
Therefore, if
then .
Example 1 If we consider a function given by
with
for n ≧ p + 2, then we see that
Thus, this function f(z) satisfies the inequality (2.1). Also, we see that
Therefore, we say that .
Next, we discuss the necessary condition for the class .
Lemma 2 If satisfies
with b n = |b n | ei(n-p)θ(n = p + 1, p + 2, p + 3,...), then
Proof Let us define the function F(z) by
It follows that
for . Letting z = |z| e-iθ, we have that
If we take |z| → 1-, we obtain that
which implies that
Remark 1 If we take p = 1 in Lemmas 1 and 2, then we have that
(i)
and
(ii)
3 Radius problems
Our main result for the radius problem is contained in
Theorem 1 Let (p - 1 ≦ α < p) with
and b n = | b n | ei(n-p)θ(n = p + 1, p + 2, p + 3, ...). If , then belongs to the class for , where |δ0(λ)| is the smallest positive root of the equation
that is,
Proof Since
we have that
In view of Lemma 1, we have to show that
Note that satisfies
Applying Cauchy-Schwarz inequality, we obtain that
Let |δ|2 = x. Then, we have that
This gives us that
Let us define the function h(|δ|) by
Then, h (|δ|) satisfies h (0) = -λ < 0 and . Indeed, we have that h (|δ0(λ) |) = 0 for
This completes the proof of the theorem.
Corollary 1 Let with
and b n = |b n | ei(n-1)θ(n = 2, 3, 4,...). If δ ∈ ℂ (|δ| < 1), then belongs to the class for , where |δ0(λ)| is the smallest positive root of the equation
that is,
Remark 2 In view of (3.2), we define the function g(λ) by
Then, we have that
for λ > 0. Therefore, |δ0(λ)| given by (3.2) is increasing for λ > 0.
Remark 3 If we put in Theorem 1, then
Therefore, if we consider , then we see that
and if we make λ = 5, then we have that
References
Obradović M, Ponnusamy S: Radius properties for subclasses of univalent functions. Analysis 2005, 25: 183–188. 10.1524/anly.2005.25.3.183
Shimoda Y, Hayami T, Owa S: Notes on radius properties of certain univalent functions. Acta Univ Apul 2009, 377–383. (Special Issue)
Robertson MS: On the theory of univalent functions. Ann Math 1936, 37: 374–408. 10.2307/1968451
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4 Competing interests
The authors declare that they have no competing interests.
5 Authors' contributions
QF carried out the main part of this article. All authors read and approved the final manuscript.
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Uyanik, N., Owa, S. Radius properties for analytic and p-valently starlike functions. J Inequal Appl 2011, 107 (2011). https://doi.org/10.1186/1029-242X-2011-107
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DOI: https://doi.org/10.1186/1029-242X-2011-107