Notes on the norm of pre-Schwarzian derivatives on bi-univalent functions of order $\alpha$
H. Mahzoon, R. Kargar

TL;DR
This paper corrects previous inaccuracies in estimating the norm of the pre-Schwarzian derivative for bi-starlike functions of order alpha, providing accurate proofs and bounds.
Contribution
It offers corrected proofs and bounds for the norm of the pre-Schwarzian derivative on bi-starlike functions of order alpha, improving upon prior work.
Findings
Corrected bounds for the pre-Schwarzian norm
Valid proofs for bi-starlike functions of order alpha
Clarification of previous inaccuracies
Abstract
In the present paper we estimate the norm of the pre-Schwarzian derivative of bi-starlike functions of order where . Initially this problem was handled by Rahmatan et al. in [Bull Iran Math Soc {\bf43}: 1037-1043, 2017]. We pointed out that the proofs and bounds by Rahmatan et al. are incorrect and present correct proofs and bounds.
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Taxonomy
TopicsAnalytic and geometric function theory
Notes on the norm of pre-Schwarzian derivatives on bi-univalent functions of order
H. Mahzoon and R. Kargar
Department of Mathematics, Islamic Azad University, West Tehran Branch, Tehran, Iran
Young Researchers and Elite Club, Ardabil Branch, Islamic Azad University, Ardabil, Iran
Abstract.
In the present paper we estimate the norm of the pre-Schwarzian derivative of bi-starlike functions of order where . Initially this problem was handled by Rahmatan et al. in [Bull Iran Math Soc 43: 1037-1043, 2017]. We pointed out that the proofs and bounds by Rahmatan et al. are incorrect and present correct proofs and bounds.
Key words and phrases:
univalent, locally univalent, bi-univalent, bi-starlike, subordination, pre-Schwarzian
2010 Mathematics Subject Classification:
30C45
1. Introduction
Let be the family of analytic functions on the open unit disc and be a subclass of that its members are normalized by the condition . This means that each has the following form
[TABLE]
We denote by the family of univalent (one–to–one) functions in . Let and belong to the class . A function is called to be subordinate to , written as
[TABLE]
if there exists a Schwarz function with the following properties
[TABLE]
such that for all . If , then the following geometric equivalence relation holds true:
[TABLE]
It is known that the Koebe function
[TABLE]
maps the open unit disc onto the entire plane minus the interval . Also, the well-known Koebe One-Quarter Theorem states that the image of the open unit disc under every function contains the disc , see [3, Theorem 2.3]. Therefore every function in the class has an inverse which satisfies the following conditions:
[TABLE]
and
[TABLE]
where
[TABLE]
A function is bi-univalent in if, and only if, both and are univalent in . We denote by the class of bi-univalent functions in . The functions
[TABLE]
with the corresponding inverse functions, respectively
[TABLE]
belong to the class .
A function is called starlike (with respect to [math]) if whenever and . We denote by the class of the starlike functions in . Also, we say that a function is starlike of order () if, and only if,
[TABLE]
The class of the starlike functions of order in is denoted by . Now by definition of the starlike functions of order we recall the following definition.
Definition 1.1**.**
Let . A function given by (1.1) is said to be in the class if the conditions (1.3) and
[TABLE]
hold true where and .
Denote by the class of all satisfying the following condition
[TABLE]
The class was considered by Obradović and Ponnusamy in [5]. Now we recall the following definition.
Definition 1.2**.**
Let . A function given by (1.1) is said to be in the class if the conditions (1.5) and
[TABLE]
hold true where and .
Denote by the subclass of consisting of all locally univalent functions, namely, . For a the pre–Schwarzian and Schwarzian derivatives of are defined as follows
[TABLE]
respectively. We note that the quantity (resp. ) is analytic on precisely when is analytic (resp. meromorphic) and locally univalent on . Since is a vector space over (see [4]), thus we can define the norm of by
[TABLE]
This norm has significance in the theory of Teichmüller spaces, see [1]. It is known that if and only if is uniformly locally univalent. Also, notice that if , then is univalent in and conversely, if univalent in , then and the equality is attained for the Koebe function and its rotation. In fact, both of these bounds are sharp, see [2]. Also, if is starlike of order , then we have the sharp estimate (see e.g. [7]).
The following theorems were wrongly proven by Rahmatan et al. [6, Theorem 2.2 and Theorem 2.4].
Theorem A. Let the function given by (1.1) be in the class where . Then
[TABLE]
Theorem B. Let the function given by (1.1) be in the class where . Then
[TABLE]
We notice that when .
In the present paper we give a correct proof for Theorem A and some remarks on the Theorem B.
2. On the Theorem A
The correct version of Theorem A is contained in the following theorem:
Theorem 2.1**.**
Let . If the function of the form (1.1) is in the class , then
[TABLE]
Proof.
Let be given by (1.1). Then by Definition 1.1 the following conditions hold true:
[TABLE]
and
[TABLE]
where and . Since (2.2) holds true by [7] we conclude that where . On the other hand, since the mapping
[TABLE]
maps onto the right half-plane having real part greater than , thus (2.3) implies that
[TABLE]
By the identity (see [6, Eq. (1.2)]) (2.5) is equivalent to
[TABLE]
Now by (2.6) and definition of subordination there exists a Schwarz function with and such that
[TABLE]
or equivalently
[TABLE]
Taking logarithm on both sides of (2.7) and differentiating, after simplification, we obtain
[TABLE]
The well-known Schwarz-Pick lemma states that for a Schwarz function the following inequality holds true:
[TABLE]
Now by (2.9) and since (see [3]), the relation (2.8) implies that
[TABLE]
However we get
[TABLE]
Now we consider the following cases.
Case 1. . In this case we have . Therefore
[TABLE]
Case 2. . In this case becomes . Also we have when . Thus
[TABLE]
Case 3. . In this case we have . Thus
[TABLE]
Because when . This completes the proof. ∎
3. On the Theorem B
In this section we give some remarks on the Theorem B. Let a function be of the form (1.1) belongs to the class . Then the conditions (1.5) and (1.6) hold true. From the geometric meaning of the function , subordination principle and (1.5) we have
[TABLE]
Using definition of subordination there exists a Schwarz function so that
[TABLE]
With a simple calculation (3.1) yields
[TABLE]
Again, from (3.1) we get
[TABLE]
By substituting (3.3) into (3.2), we have
[TABLE]
To estimate the above relationship (3.4), we need to estimate , but so far this is an open question. So this question seems to be more difficult than what is given in [6]. Also, we remark that in [6, proof of Theorem 2.4] Rahmatan et al. mistakenly used the following relation
[TABLE]
and this means that . Thus Theorem 2.4 and its proof in [6] is incorrect.
The reference list from the paper itself. Each links out to its DOI / PubMed record.
- 1[1] K. Astala and F.W. Gehring, Injectivity, the BMO norm and the universal Teichmüller space , J. Anal. Math. 46 (1986), 16–57.
- 2[2] J. Becker and Ch. Pommerenke, Schlichtheitskriterien und Jordangebiete , J. Reine Angew. Math. 354 (1984), 74–94.
- 3[3] P.L. Duren, Univalent Functions , Springer–Verlag, New York, 1983.
- 4[4] H. Hornich, Ein Banachraum analytischer Funktionen in Zusammenhang mit den schlichten Funktionen , Monatsh. Math. 73 (1969), 36–45.
- 5[5] M. Obradović and S. Ponnusamy, Radius of univalence of certain class of analytic functions , Filomat 27 (2013), 1085–1090.
- 6[6] H. Rahmatan, Sh. Najafzadeh and A. Ebadian, The norm of pre-Schwarzian derivatives on bi-univalent functions of order α 𝛼 \alpha , Bull. Iran. Math. Soc. 43 (2017), 1037–1043.
- 7[7] S. Yamashita, Norm estimates for function starlike or convex of order alpha , Hokkaido Math. J. 28 (1999), 217–230.
