Abstract:The authors introduced and addressed several new subclasses of the family of meromorphically multivalent -star-like functions in the punctured unit disk in this study, which makes use of several higher order -derivatives. Many fascinating properties and characteristics are extracted systematically for each of these newly identified function classes. Distortion theorems and radius problems are among these characteristics and functions. A number of coefficient inequalities for functions belonging to the subcl… Show more
“…The function 𝑙 defined by 𝑙(𝑤) = √ℎ(𝑤 𝑟 ) 𝑟 , (𝑟 ∈ {1,2,3, … }) maps and its is univalent in 𝑈 into a place that 𝑟-fold symmetry for all ℎ ∈ ℋ. If the condition of normalized is met, a function is said to be 𝑟-fold symmetric (see [17][18][19]).…”
In this paper we offer two new subclasses of an open unit disk of r-fold symmetric bi-univalent functions. The Taylor-Maclaurin coefficients have their coefficient bounds calculated. Furthermore, for functions in , we have solved Fekete- functional issues. For the applicable classes, there are also a few particular special motivator results.
“…The function 𝑙 defined by 𝑙(𝑤) = √ℎ(𝑤 𝑟 ) 𝑟 , (𝑟 ∈ {1,2,3, … }) maps and its is univalent in 𝑈 into a place that 𝑟-fold symmetry for all ℎ ∈ ℋ. If the condition of normalized is met, a function is said to be 𝑟-fold symmetric (see [17][18][19]).…”
In this paper we offer two new subclasses of an open unit disk of r-fold symmetric bi-univalent functions. The Taylor-Maclaurin coefficients have their coefficient bounds calculated. Furthermore, for functions in , we have solved Fekete- functional issues. For the applicable classes, there are also a few particular special motivator results.
“…And we denote by ∑ (𝜀) * 𝑘 the class of meromorphically convex functions of 𝜀. The class ∑ * (𝜀) and ∑ (𝜀) were introduced and studied by pommerenke [1], Miller [2], Mogra et al [3], Aouf et al [4,5], El-Ashwah et al [6], Mostafa et al [7] and Venkateswarlu et al [8,9,10].…”
Section: Introductionmentioning
confidence: 99%
“…where ℑ 𝜏,𝑢,ℎ,𝑡 𝑚,𝑘 (𝑓 * 𝑔)(𝑤) is given by (9). In addition, we state that a function(𝑓 * 𝑔)(𝑤) ∈ ∑(𝛼, 𝛿, 𝒴, 𝜏, 𝑢, ℎ, 𝑡), whenever (𝑓 * 𝑔)(𝑤) is of the form (4).…”
We obtain the coefficient estimates, extreme points, distortion and growth boundaries, radii of starlikeness, convexity, and close-to-convexity, according to the main purpose of this paper.
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