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The article derives conditions for the Rabotnov function to be q-close-to-convex in the unit disk, suggesting new mathematical insights.
The article derives sufficient conditions under which the normalized Rabotnov function becomes q-close-to-convex relative to specific starlike functions on the open unit disk. To enhance the impact of our results, we include some consequences derived from the main theorems, along with graphical illustrations. The starlikeness of the Rabotnov function with respect to different aspects also falls within the scope of this study.
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Noreen et al. (2026) studied this question.
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