Starlikeness associated with parabolic regions
Author(s) -
Rosihan M. Ali
Publication year - 2005
Publication title -
international journal of mathematics and mathematical sciences
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.21
H-Index - 39
eISSN - 1687-0425
pISSN - 0161-1712
DOI - 10.1155/ijmms.2005.561
Subject(s) - mathematics , subordination (linguistics) , convolution (computer science) , unit disk , distortion (music) , class (philosophy) , mathematical analysis , order (exchange) , function (biology) , plane (geometry) , pure mathematics , parabolic cylinder function , unit (ring theory) , parabolic partial differential equation , geometry , partial differential equation , computer science , philosophy , cmos , electronic engineering , artificial intelligence , amplifier , linguistics , engineering , biology , machine learning , evolutionary biology , artificial neural network , mathematics education , finance , economics
A parabolic starlike function f of order ρ in the unit disk is characterized by the fact that the quantity zf′(z)/f(z) lies in a given parabolic region in the right half-plane. Denote the class of such functions by PS∗(ρ). This class is contained in the larger class of starlike functions of order ρ. Subordination results for PS∗(ρ) are established, which yield sharp growth, covering, and distortion theorems. Sharp bounds for the first four coefficients are also obtained. There exist different extremal functions for these coefficient problems. Additionally, we obtain a sharp estimate forthe Fekete-Szegö coefficient functional and investigate convolution properties for PS∗(ρ)
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