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Certain Classes of Analytic Functions Involving Multiplier Transformations
J. J. Bhamare Department of Mathematics,
S. S. V. P. S. B. S. Deore, College of Engineering, Deopur,Dhule-424002
M. S., India.
S. M. Khairnar
Department of Engineering Sciences,
MIT Academy of Engineering, Alandi, Pune-412105, M. S., India
Abstract- In this paper, we study certain subclasses of analytic functions involving multiplier transformations in the open unit disc. We derive few subordination results for the functions in these subclasses and discuss the applications of subordination results with the help of complex functions. We obtain coefficient estimates, radii of starlikeness, convexity and close-to-convexity, extreme points, and integral means inequalities, growth and distortion theorems for these classes.
Keywords: multiplier transformations, radii of convexity and close-to-convexity, extreme points, subordination etc.
AMS Subject Classification: 30C45 & 30C50
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I. INTRODUCTION AND PRELIMINARIES Let 𝒩 denote the class of functions of the form
𝑓 𝑧 𝛽 = 𝑧𝛽+ 𝛽𝑎𝑛𝑧𝛽+𝑛−1
∞
𝑛=2
(1.1) which are analytic and univalent in the open disc 𝑈 = 𝑧 ∈ ∁: 𝑧 < 1 . Also consider the subclass ℳ of 𝒩 consisting of
functions of the form
𝑓 𝑧 𝛽 = 𝑧𝛽 − 𝛽𝑎𝑛𝑧𝛽+𝑛−1
∞
𝑛=2
(𝛽 > 0 , 𝑎𝑛≥ 0)
(1.2) For any integer m, we defined the multiplier transformations 𝐼𝑚𝑙 of functions 𝑓 ∈ 𝒩 by
𝐼𝑚𝑙 𝑓 𝑧 𝛽 = 𝑧𝛽 − 𝛽 𝛽 + 𝑙 𝛽 + 𝑙 + 𝑛 − 1
𝑚
𝑎𝑛𝑧𝛽+𝑛−1
∞
𝑛=2
= 𝑧𝛽− 𝛽𝑄 𝑛, 𝛽, 𝑙 𝑎𝑛𝑧𝛽+𝑛−1, 𝑙 ≥ 0, 𝑧 ∈ 𝑈
∞
𝑛=2
(1.3) 𝑤𝑒𝑟𝑒 𝑄 𝑛, 𝛽, 𝑙 𝑎𝑛 = 𝛽 +𝑙
𝛽+𝑙+𝑛−1 𝑚
A function 𝑓 𝑧 ∈ ℳ is said to be in the class 𝑈𝑆𝑇(𝛼, 𝑘) (k-Uniformly starlike functions of order 𝛼) if it satisfies the condition:
𝑅𝑒 𝑧𝑓′ 𝑧 𝛽
𝑓 𝑧 𝛽 − 𝛼 > 𝑘 𝑧𝑓′ 𝑧 𝛽
𝑓 𝑧 𝛽 − 1 , 0 ≤ 𝛼 < 1, 𝑘 ≥ 0 𝑎𝑛𝑑 𝑧 ∈ 𝑈,
(1.4) And is said to be in the class 𝑈𝐶𝑉(𝛼, 𝑘) (k-Uniformly convex functions of order 𝛼) if it satisfies the condition:
𝑅𝑒 1 + 𝑧𝑓′′ 𝑧 𝛽
𝑓′ 𝑧 𝛽 − 𝛼 > 𝑘 𝑧𝑓′′ 𝑧 𝛽
𝑓′ 𝑧 𝛽 − 1 , 0 ≤ 𝛼 < 1, 𝑘 ≥ 0 𝑎𝑛𝑑 𝑧 ∈ 𝑈,
(1.5) Indeed it follows from (4) and (5) that
𝑓 ∈ 𝑈𝐶𝑉 𝛼, 𝑘 ⇔ 𝑧𝑓′ ∈ 𝑈𝑆𝑇 𝛼, 𝑘
(1.6)
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The interesting geometric properties of these function classes were extensively studied by Waggas Galib Astan et. Al [16], Kanas et al. in [14, 15], and Murugusundaramoorthy and Magesh [3,4], Astan and Kulkarni[17].Astan and Buti[18], S. M. Khairnar and N. H. More [12], S. M. Khairnar and Meena More [10, 11].
Definition1.1: For two functions 𝑓 and 𝑔 analytic in U, we say that the function 𝑓 is subordinate to g in U, denoted by 𝑓 ≺ 𝑔, if their exist a Schwarz function 𝑤(𝑧), analytic in U with 𝑤 0 = 0 and 𝑤(𝑧) < 𝑧 < 1 (𝑧 ∈ 𝑈) , such that 𝑓 𝑧 = 𝑔 𝑤 𝑧 (𝑧 ∈ 𝑈).
In particular, if the function 𝑔 is univalent in U, the above subordination is equivalent to 𝑓 0 = 𝑔 0 , 𝑓 𝑈 = 𝑔 𝑈 . The Littlewood’s subordination theorem which we will use in our investigation to obtain the integral mean inequality.
Lemma1.2: If the functions 𝑓(𝑧) and 𝑔(𝑧) are analytic in U, with 𝑓(𝑧) ≺ 𝑔(𝑧), then 𝑓(𝑟𝑒𝑖𝜃) 𝜂𝑑𝜃 ≤
2𝜋
0
𝑔(𝑟𝑒𝑖𝜃) 𝜂𝑑𝜃
2𝜋
0
(1.7) Where 𝜂 > 0, 𝑧 = 𝑟𝑒𝑖𝜃 𝑎𝑛𝑑 0 < 𝑟 < 1. Strict inequality holds for 0 < 𝑟 < 1
Unless 𝑓 is constant or 𝑤 𝑧 = 𝛼𝑧, 𝛼 = 1.
Let 𝜑(𝑧) be an analytic function in U with 𝜑 0 = 1, 𝜑′ 0 > 0 𝑎𝑛𝑑 𝑅 𝜑 𝑧 > 0, 𝑧 ∈ 𝑈.
which maps the open unit disc U onto a region starlike with respect to 1 and is symmetric with respect to the real axis. Then, by𝑆∗ 𝜑 𝑎𝑛𝑑 𝐶 𝜑 , respectively, denote the subclass of normalized analytic function class A which satisfy the following subordination relation
𝑧𝑓′ 𝑧 𝛽
𝑓 𝑧 𝛽 ≺ 𝜑 𝑧 𝑎𝑛𝑑 1 + 𝑧𝑓′′ 𝑧 𝛽
𝑓′ 𝑧 𝛽 ≺ 𝜑 𝑧 , 𝑧 ∈ 𝑈.
These functions introduced and studied by Ma and Minda. For 𝜑 𝑧 =1 + 1 − 2𝛼 𝑧
1 − 𝑧 𝑧 ∈ 𝑈, 0 ≤ 𝛼 < 1 ;
These function classes reduce to the well known classes 𝑆∗ 𝛼 of starlike functions of order 𝛼 in U and 𝐶 𝛼 of convex functions of order 𝛼 in U.
Definition1: For 𝛽 > 0, −1 ≤ 𝛼 < 1, 𝑙, 𝑘 ≥ 0 𝑎𝑛𝑑 𝐼𝑚𝑙 𝑓 𝑧 𝛽 𝑔𝑖𝑣𝑒𝑛 𝑏𝑦 1.3 , we difined a new class 𝒩𝑚𝑙(𝛼, 𝛽, 𝜆, 𝑘) as subclass of consisting function 𝑓 𝑧 𝛽 of the form (1.2) and satisfying analytic criterion
𝑅𝑒 𝑧 𝐼𝑚𝑙 𝑓 𝑧 𝛽 ′
𝜆𝑧 𝐼𝑚𝑙 𝑓 𝑧 𝛽 ′+ 1 − 𝜆 𝐼𝑚𝑙 𝑓 𝑧 𝛽 − 𝛼 ≥ 𝑘 𝑧 𝐼𝑚𝑙 𝑓 𝑧 𝛽 ′
𝜆𝑧 𝐼𝑚𝑙 𝑓 𝑧 𝛽 ′+ 1 − 𝜆 𝐼𝑚𝑙 𝑓 𝑧 𝛽 − 1 .
(1.8) II. COEFFICIENT ESTIMATE
We obtain Necessary and Sufficient condition for the function 𝑓 𝑧 𝛽 of the form (1.2) to belong to the class 𝒩𝑚𝑙(𝛼, 𝛽, 𝜆, 𝑘) Theorem2.1: A function 𝑓 𝑧 𝛽 is in the class 𝒩𝑚𝑙(𝛼, 𝛽, 𝜆, 𝑘)if and only if
1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝛽𝑄 n, β, l 𝑎𝑛
∞
𝑛=1
≤ 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
(2.1) The result is sharp for the function
𝑎𝑛= 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝛽𝑄 n, β, l Where 𝛽 > 0, −1 ≤ 𝛼 < 1, 𝑘, 𝑙 ≥ 0, 0 ≤ 𝜆 < 1
𝐼𝑚𝑙 𝑓 𝑧 𝛽 = 𝑧𝛽− 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝑄 𝑛, 𝛽, 𝑙 𝑧𝛽+𝑛−1,
∞
𝑛=2
Proof: Suppose that (2.1) is true for 𝑧 ∈ 𝑈. Then 𝑅𝑒 𝑧 𝐼𝑚𝑙 𝑓 𝑧 𝛽 ′
𝜆𝑧 𝐼𝑚𝑙 𝑓 𝑧 𝛽 ′+ 1 − 𝜆 𝐼𝑚𝑙 𝑓 𝑧 𝛽 − 𝛼 ≥ 𝑘 𝑧 𝐼𝑚𝑙 𝑓 𝑧 𝛽 ′
𝜆𝑧 𝐼𝑚𝑙 𝑓 𝑧 𝛽 ′+ 1 − 𝜆 𝐼𝑚𝑙 𝑓 𝑧 𝛽 − 1
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𝑅𝑒 𝛽 − 𝛼 𝜆𝛽 + 1 − 𝜆 − ∞𝑛 =1𝛽𝑄 n, β, l β + n − 1 − 𝛼𝜆 β + n − 1 − 𝛼 1 − 𝜆 𝑎𝑛𝑧𝑛−1 𝜆𝛽 + 1 − 𝜆 − ∞𝑛=1𝛽𝑄 n, β, l 𝜆 β + n − 1 + 1 − 𝜆 𝑎𝑛𝑧𝑛−1
≥ 𝑘 𝛽 − 𝜆𝛽 + 1 − 𝜆 − ∞𝑛 =1𝛽𝑄 n, β, l β + n − 1 − 𝜆 β + n − 1 − 1 − 𝜆 𝑎𝑛𝑧𝑛−1 𝜆𝛽 + 1 − 𝜆 − ∞𝑛 =1𝛽𝑄 n, β, l 𝜆 β + n − 1 + 1 − 𝜆 𝑎𝑛𝑧𝑛−1 Allowing 𝑧 → 1 along with real axis, we get
1 + 𝑘 − 𝑘 + 𝛼 𝜆 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝛽𝑄 n, β, l 𝑎𝑛 ≤
∞
𝑛=1
1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
𝐶𝑜𝑛𝑣𝑒𝑟𝑠𝑒𝑙𝑦, 𝑎𝑠𝑠𝑢𝑚𝑒 𝑡𝑎𝑡 𝑓 ∈ 𝒩𝑚𝑙 𝛼, 𝛽, 𝜆, 𝑘 , 𝑡𝑒𝑛
𝑘 𝑧 𝐼𝑚𝑙 𝑓 𝑧 𝛽 ′
𝜆𝑧 𝐼𝑚𝑙 𝑓 𝑧 𝛽 ′+ 1 − 𝜆 𝐼𝑚𝑙 𝑓 𝑧 𝛽 − 1 − 𝑅𝑒 𝑧 𝐼𝑚𝑙 𝑓 𝑧 𝛽 ′
𝜆𝑧 𝐼𝑚𝑙 𝑓 𝑧 𝛽 ′+ 1 − 𝜆 𝐼𝑚𝑙 𝑓 𝑧 𝛽 − 𝛼
≤ 1 + 𝑘 𝑧 𝐼𝑚𝑙 𝑓 𝑧 𝛽 ′
𝜆𝑧 𝐼𝑚𝑙 𝑓 𝑧 𝛽 ′+ 1 − 𝜆 𝐼𝑚𝑙 𝑓 𝑧 𝛽 − 1
≤ 1 + 𝑘 𝛽 − 𝜆𝛽 − 1 − 𝜆 − ∞𝑛 =1𝛽𝑄 n, β, l β + n − 1 1 − 𝜆 − 1 − 𝜆 𝑎𝑛𝑧𝑛−1 𝜆𝛽 + 1 − 𝜆 − ∞𝑛 =1𝛽𝑄 n, β, l β + n − 1 𝜆 + 1 − 𝜆 𝑎𝑛𝑧𝑛−1 is bounded above if ≤ 1 − 𝛼 , Letting 𝑧 → 1−𝑎𝑙𝑜𝑛𝑔 𝑡𝑒 𝑟𝑒𝑎𝑙 𝑎𝑥𝑖𝑠, 𝑤𝑒 𝑎𝑣𝑒
≤ 1 + 𝑘 𝛽 − 𝜆𝛽 − 1 − 𝜆 − ∞𝑛 =1𝛽𝑄 n, β, l β + n − 1 1 − 𝜆 − 1 − 𝜆 𝑎𝑛 𝜆𝛽 + 1 − 𝜆 − ∞𝑛=1𝛽𝑄 n, β, l β + n − 1 𝜆 + 1 − 𝜆 𝑎𝑛 β + n − 1 1 + 𝑘 − 𝜆 𝑘 + 𝛼 − 𝑘 + 𝛼 1 − 𝜆 𝛽𝑄 n, β, l 𝑎𝑛
∞
𝑛=1
≤ 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆 which completes the proof.
III. RADII OF STARLIKENESS, CONVEXITY AND CLOSE-TO-CONVEXITY
We obtain the radii of convexity and close-to- convexity results for 𝑓 𝑧 functions in the class𝒩𝑚𝑙(𝛼, 𝛽, 𝜆, 𝑘) in the following theorem
Theorem3.1: Let 𝑓 ∈ 𝒩𝑚𝑙 𝛼, 𝛽, 𝜆, 𝑘 . Then 𝑓 is starlike of order 𝛿, (0 ≤ 𝛿 < 1) in the disk 𝑧 < 𝑟 = 𝑟1 𝛼, 𝛽, 𝜆, 𝑘, 𝑛, 𝛿 , where
𝑟1= 𝑖𝑛𝑓 𝑛 ≥ 2
𝛽 − 𝛿 1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝑄 𝑛, 𝛽, 𝑙 𝛽 + 𝑛 − 𝛿 − 1 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
1𝑛−1
(3.1) Proof: For 0 ≤ 𝛿 < 1, It is sufficient to show that
𝑓′ 𝑧 𝛽
𝑓 𝑧 𝛽 − 1 ≤ 1 − 𝛿 ,
(3.2) For 𝑧 ≤ 𝑟1, we have
𝑍𝑓′ 𝑧 𝛽
𝑓 𝑧 𝛽 − 1 ≤ 𝛽 − 1 − ∞𝑛=2𝛽 𝛽 + 𝑛 − 2 𝑎𝑛𝑧𝑛−1
1 − ∞𝑛 =2𝛽𝑎𝑛𝑧𝑛−1 ≤ 1 − 𝛿
(3.3) Hence, (3.3) holds true if
𝛽 + 𝑛 − 𝛿 − 1 𝛽 𝛽 − 𝛿 𝑎𝑛
∞
𝑛=2
𝑧 𝑛−1≤ 1
(3.4) With the aid of (2.1) and (3.4) is true if
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𝑧 𝑛−1≤ 𝛽 − 𝛿 1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝑄 𝑛, 𝛽, 𝑙 𝛽 + 𝑛 − 𝛿 − 1 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
(3.5) Therefore,
𝑧 ≤ 𝛽 − 𝛿 1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝑄 𝑛, 𝛽, 𝑙 𝛽 + 𝑛 − 𝛿 − 1 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
1𝑛−1
(3.6) Setting 𝑧 = 𝑟1 𝛼, 𝛽, 𝜆, 𝑘, 𝑛, 𝛿 in (3.6), we get the radius of starlikeness, which completes the proof of theorem 3.1.
Theorem3.2: Let 𝑓 ∈ 𝒩𝑚𝑙 𝛼, 𝛽, 𝜆, 𝑘 . Then 𝑓 is convex of order 𝛿, (0 ≤ 𝛿 < 1) in the disk 𝑧 < 𝑟 = 𝑟2 𝛼, 𝛽, 𝜆, 𝑘, 𝑛, 𝛿 , where
𝑟2= 𝑖𝑛𝑓 𝑛 ≥ 2
𝛽 − 𝛿 1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝑄 𝑛, 𝛽, 𝑙 𝛽 + 𝑛 − 1 𝛽 + 𝑛 − 𝛿 − 1 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
1𝑛−1
(3.7) Proof: For 0 ≤ 𝛿 < 1, it is sufficient to show
𝑧𝑓′′ 𝑧 𝛽
𝑓′ 𝑧 𝛽 ≤ 1 − 𝛿 ,
(3.8) For 𝑧 ≤ 𝑟2, we have
𝑧𝑓′′ 𝑧 𝛽
𝑓′ 𝑧 𝛽 ≤ 𝛽 − 1 − ∞𝑛 =2 β + n − 1 β + n − 2 𝑎𝑛𝑧𝑛−1
1 − ∞𝑛=2 β + n − 1 𝑎𝑛𝑧𝑛−1 ≤ 1 − 𝛿 ,
(3.9) Hence, (3.9) holds true if
𝛽 + 𝑛 − 1 𝛽 + 𝑛 − 𝛿 − 1 𝛽 − 𝛿
∞
𝑛=2
𝑎𝑛 𝑧 𝑛−1≤ 1
(3.10) With the aid of (2.1) and (3.4) is true if
𝑧 𝑛−1≤ 𝛽 − 𝛿 1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝑄 𝑛, 𝛽, 𝑙 𝛽 + 𝑛 − 1 𝛽 + 𝑛 − 𝛿 − 1 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
(3.11) 𝑧 ≤ 𝛽 − 𝛿 1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝑄 𝑛, 𝛽, 𝑙
𝛽 + 𝑛 − 1 𝛽 + 𝑛 − 𝛿 − 1 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
1𝑛−1
(3.12) Setting 𝑧 = 𝑟2 𝛼, 𝛽, 𝜆, 𝑘, 𝑛, 𝛿 in (3.14), we get the radius of convexity, which completes the proof of theorem 3.2.
Theorem3.3: Let 𝑓 ∈ 𝒩𝑚𝑙 𝛼, 𝛽, 𝜆, 𝑘 . Then 𝑓 is close to convex of order 𝛿, (0 ≤ 𝛿 < 1) in the disk 𝑧 < 𝑟 = 𝑟3 𝛼, 𝛽, 𝛾, 𝑛, 𝛿 , where
𝑟3= 𝑖𝑛𝑓 𝑛 ≥ 2
𝛽 − 𝛿 1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝑄 𝑛, 𝛽, 𝑙 𝛽 + 𝑛 − 𝛿 − 1 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
1𝑛−1
(3.13) Proof: For 0 ≤ 𝛿 < 1, it is sufficient to show that
𝑓′ 𝑧 𝛽
𝑧𝛽−1 − 1 ≤ 1 − 𝛿
(3.14) For 𝑧 ≤ 𝑟3, we have
𝑓′ 𝑧 𝛽
𝑧𝛽 −1 − 1 ≤ 𝛽 − 1 + 𝛽 𝛽 + 𝑛 − 1 𝑎𝑛𝑧𝑛−1
∞
𝑛=2
≤ 1 − 𝛿
(3.15)
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Hence, (3.15) holds true if
𝛽 𝛽 + 𝑛 − 1 𝛽 − 𝛿
∞
𝑛=2
𝑎𝑛 𝑧 𝑛−1≤ 1
(3.16) With the aid of (2.1) and (3.16) is true if
𝑧 𝑛−1 ≤ 𝛽 − 𝛿 1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝑄 𝑛, 𝛽, 𝑙 𝛽 + 𝑛 − 1 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
(3.17) Therefore,
𝑧 ≤ 𝛽 − 𝛿 1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝑄 𝑛, 𝛽, 𝑙 𝛽 + 𝑛 − 1 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
1𝑛−1
(3.16) Setting 𝑧 = 𝑟3 𝛼, 𝛽, 𝜆, 𝑘, 𝑛, 𝛿 in (3.21), we get the radius of close-to-convexity, which completes the proof of theorem 3.3.
IV. EXTREAM POINTS:
The extream points of the class 𝒩𝑚𝑙 𝛼, 𝛽, 𝜆, 𝑘 are given by the following theorem.
Theorem 4.1: Let 𝑓1 𝑧 𝛽 = 𝑧𝛽,
𝑓𝑛 𝑧 𝛽 = 𝑧𝛽 − 𝛽 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝑄 𝑛, 𝛽, 𝑙 𝑧𝛽 +𝑛−1
(4.1) For n=2,3,4,…
Then, 𝑓 ∈ 𝒩𝑚𝑙 𝛼, 𝛽, 𝜆, 𝑘 if and only if it can be expressed in the form 𝑓 𝑧 𝛽 = 𝑌𝑛
∞
𝑛 =1
𝑓𝑛 𝑧 𝛽
(4.2) Where
𝑌𝑛 ≥ 0 𝑎𝑛𝑑 𝑌𝑛
∞
𝑛=1
=
(4.3) Proof: Suppose that f can be express as in (4.2). Our aim is to show that 𝑓 ∈ 𝒩𝑚𝑙 𝛼, 𝛽, 𝜆, 𝑘 .
By (4.2), we have that 𝑓 𝑧 𝛽 = 𝑌𝑛
∞
𝑛=1
𝑓𝑛 𝑧 𝛽 = 𝑌1𝑓1 𝑧 𝛽+ 𝑌𝑛
∞
𝑛=2
𝑓𝑛 𝑧 𝛽
= 𝑌1𝑓1 𝑧 𝛽
+ 𝑌𝑛 𝑧𝛽− 𝛽 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝑄 𝑛, 𝛽, 𝑙 𝑧𝛽+𝑛−1
∞
𝑛=2
(4.4) = 𝑌𝑛𝑧𝛽− 𝑌𝑛𝛽 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝑄 𝑛, 𝛽, 𝑙 𝑧𝛽 +𝑛 −1
∞
𝑛=1
= 𝑧𝛽 − 𝛽𝑌𝑛 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝑄 𝑛, 𝛽, 𝑙 𝑧𝛽 +𝑛−1.
∞
𝑛=2
Now,
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1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝑄 𝑛, 𝛽, 𝑙 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
∞
𝑛=2
× 𝑌𝑛 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝑄 𝑛, 𝛽, 𝑙 𝑧𝛽 +𝑛−1 = 𝑌𝑛
∞
𝑛 =2
= 1 − 𝑌1≤ 1
(4.5) Thus, 𝑓 ∈ 𝒩𝑚𝑙 𝛼, 𝛽, 𝜆, 𝑘 .
Conversely, assume that 𝑓 ∈ 𝒩𝑚𝑙 𝛼, 𝛽, 𝜆, 𝑘 . Since
𝑎𝑛 ≤ 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝑄 𝑛, 𝛽, 𝑙 𝑛 ≥ 2
(4.6) We can set
𝑌𝑛= 1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝑄 𝑛, 𝛽, 𝑙
1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆 𝑎𝑛 𝑛 ≥ 2
(4.7) 𝑌1= 1 − 𝑌𝑛
∞
𝑛=2
Then,
𝑓 𝑧 𝛽 = 𝑧𝛽− 𝛽
∞
𝑛 =2
𝑎𝑛𝑧𝛽+𝑛−1
= 𝑧𝛽− 𝛽
∞
𝑛=2
𝑌𝑛 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝑄 𝑛, 𝛽, 𝑙 𝑧𝛽 +𝑛 −1
= 𝑧𝛽− 𝑌𝑛 𝑧𝛽 − 𝑓𝑛 𝑧 𝛽
∞
𝑛=2
(4.8)
= 𝑌1𝑓1 𝑧 𝛽+ 𝑌𝑛𝑓𝑛 𝑧 𝛽
∞
𝑛=2
= 𝑌𝑛𝑓𝑛 𝑧 𝛽
∞
𝑛 =1
This completes the proof of Theorem4.1
V. INTEGRAL MEANS:
Theorem 5.1: Let 𝜂 > 0. If 𝑓 ∈ 𝒩𝑚𝑙 𝛼, 𝛽, 𝜆, 𝑘 𝑎𝑛𝑑 𝜑 𝛼, 𝛽, 𝑛 𝑛=1∞ are nondecreasing sequences, then, for 𝑧 = 𝑟𝑒𝑖𝜃 𝑎𝑛𝑑 0 < 𝑟 <
1
𝑓(𝑟𝑒𝑖𝜃)𝛽 𝜂𝑑𝜃 ≤
2𝜋
0
𝑓2(𝑟𝑒𝑖𝜃)𝛽 𝜂𝑑𝜃
2𝜋
0
(5.1)
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where
𝑓2(𝑧)𝛽 = 𝑧𝛽 − 𝛽 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆 𝜑 𝛼, 𝛽, 𝜆, 𝑘, 2 𝑧𝛽 +1
(5.2) 𝜑 𝛼, 𝛽, 𝜆, 𝑘, 𝑛 = 1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝑄 𝑛, 𝛽, 𝑙 .
Proof: Let 𝑓 of the form of (1.2) and
𝑓2(𝑧)𝛽 = 𝑧𝛽 − 𝛽 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆 𝜑 𝛼, 𝛽, 𝜆, 𝑘, 2 𝑧𝛽 +1
(5.3) Then we must show that
1 − 𝛽𝑎𝑛𝑧𝑛−1
∞
𝑛=1
𝜂
𝑑𝜃 ≤
2𝜋
0
1 − 𝛽 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆 𝜑 𝛼, 𝛽, 𝜆, 𝑘, 2 𝑧
𝜂
𝑑𝜃
2𝜋
0
(5.4) By lemma 5.2, it suffices to show that
1 − 𝛽𝑎𝑛𝑧𝑛−1
∞
𝑛=1
≺ 1 − 𝛽 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆 𝜑 𝛼, 𝛽, 𝜆, 𝑘, 2 𝑧
(5.5) Setting
1 − 𝛽𝑎𝑛𝑧𝑛−1
∞
𝑛=1
= 1 − 𝛽 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆 𝜑 𝛼, 𝛽, 𝜆, 𝑘, 2 𝑤(𝑧)
(5. 6) From (5.7) and (2.1) we obtain
𝑤(𝑧) = 𝜑 𝛼, 𝛽, 𝜆, 𝑘, 2 𝛽 + 1 1 − 𝛾 + 1 − 𝛼
∞
𝑛=2
𝑎𝑛𝑧𝑛−1
≤ 𝑧 𝜑 𝛼, 𝛽, 𝜆, 𝑘, 2
1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
∞
𝑛=2
𝑎𝑛
(5.7) ≤ 𝑧 < 1.
This completes the proof of Theorem 5.1.
VI. GROWTH AND DISTORSION THEOREM:
Theorem 6.1: If 𝑓 ∈ 𝒩𝑚𝑙 𝛼, 𝛽, 𝜆, 𝑘 , then,
𝑧 𝛽−𝛽 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆
𝜑 𝛼, 𝛽, 𝜆, 𝑘, 2 𝑧 𝛽 +1≤ 𝑓 𝑧 𝛽 ≤ 𝑧 𝛽 +𝛽 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆 𝜑 𝛼, 𝛽, 𝜆, 𝑘, 2 ,
(6.1) Where 𝜑 𝛼, 𝛽, 𝜆, 𝑘, 𝑛 = 1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝑄 𝑛, 𝛽, 𝑙
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This results are sharp
Theorem 6.1: If 𝑓 ∈ 𝒩𝑚𝑙 𝛼, 𝛽, 𝜆, 𝑘 , then,
−𝛽 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆 𝛽 + 1
𝛽 𝑧 𝛽−1𝜑 𝛼, 𝛽, 𝜆, 𝑘, 2 𝑧 𝛽 ≤ 𝑓′ 𝑧 𝛽 ≤ 𝛽 𝑧 𝛽−1+𝛽 1 + 𝑘 𝛽 − 𝑘 + 𝛼 𝜆𝛽 + 1 − 𝜆 𝛽 + 1 𝜑 𝛼, 𝛽, 𝜆, 𝑘, 2 𝑧 𝛽,
(6.2) Where 𝜑 𝛼, 𝛽, 𝜆, 𝑘, 𝑛 = 1 + 𝑘 − 𝜆 𝑘 + 𝛼 β + n − 1 − 𝑘 + 𝛼 1 − 𝜆 𝑄 𝑛, 𝛽, 𝑙
This results are sharp
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