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Some sufficient conditions for starlike functions associated with parabolic regions - MaRDI portal

Some sufficient conditions for starlike functions associated with parabolic regions (Q1879076)

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scientific article; zbMATH DE number 2101762
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English
Some sufficient conditions for starlike functions associated with parabolic regions
scientific article; zbMATH DE number 2101762

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    Some sufficient conditions for starlike functions associated with parabolic regions (English)
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    22 September 2004
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    \(S_{p}\) is the well known class of functions introduced and sistematically studied by F. Rønning in 1993, by using the parabolic region, related to the class of uniformly convex functions \((UCV)\) defined by Goodman in 1991. Precisely \(f\in UCV\) if and only if \(zf^{\prime} \in S_{p}\). The classes \(S_{p}\) are generalized to the classes \(S_{p}(\alpha)\) respectively \(UCV (\alpha)\) in a natural way. The author obtains some conditions for inclusion \(S_{p}(\alpha) \subset H^{\lambda}(\alpha)\) where \(H^{\lambda}(\alpha)\) is the class of all \(\lambda\)-spirallike functions of order \(\alpha\). Also he studies the operator \(g(z)= z\left(f(z)/z \right)^{\gamma}\) and the conditions so that \(f\in S^{*}[A, B]\) implies \(g(z)\in H^{\lambda}(\alpha)\). It would have been appropiate if the author had also mentioned the conditions for the choice of any branch for the power \((f(z)/z)^{\gamma}\).
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    uniformly convex functions
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    starlike functions
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    parabolic regions
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