Bohr-Rogosinski and improved Bohr type inequalities for certain fully starlike harmonic mappings
Molla Basir Ahamed, Vasudevarao Allu

TL;DR
This paper extends classical Bohr inequalities to certain fully starlike harmonic mappings, establishing sharp bounds and radii for these functions, which are a generalization of analytic functions.
Contribution
It derives new sharp Bohr-Rogosinski and improved Bohr inequalities for fully starlike harmonic mappings, expanding the scope of Bohr-type inequalities.
Findings
Established sharp Bohr-Rogosinski inequalities for the class
Determined improved Bohr inequalities with explicit bounds
Calculated the Bohr radius for fully starlike harmonic functions
Abstract
The classical Bohr inequality states that if is an analytic function with the power series representation in the unit disk such that for all , then \begin{equation*} \sum_{n=0}^{\infty}|a_n|r^n\leq 1\;\; \text{for}\;\; |z|=r\leq\frac{1}{3} \end{equation*} and the constant cannot be improved. The constant is known as Bohr radius and the inequality is known as Bohr inequality. Let be the class of complex-valued harmonic mappings defined in the unit disk , where and are analytic functions in with the normalization and . Let Let $…
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Taxonomy
TopicsAdvanced Banach Space Theory · Holomorphic and Operator Theory · Functional Equations Stability Results
