Kumar–Gangania conjecture on the third Hankel determinant for cardioid starlike functions

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Let S℘∗\mathcal{S}_{\wp}^{*} be the class of functions ff analytic in the unit disk, normalized by f(0)=0f(0)=0 and f′(0)=1f'(0)=1, such that

zf′(z)f(z)≺1+zez.\frac{zf'(z)}{f(z)}\prec 1+ze^z.

For f(z)=z+a2z2+a3z3+⋯f(z)=z+a_2z^2+a_3z^3+\cdots, let H3(1)H_3(1) denote the third Hankel determinant

H3(1)=∣a1a2a3a2a3a4a3a4a5∣,a1=1.H_3(1)=\begin{vmatrix}a_1&a_2&a_3\\a_2&a_3&a_4\\a_3&a_4&a_5\end{vmatrix},\qquad a_1=1.

Kumar–Gangania conjecture. If f∈S℘∗f\in\mathcal{S}_{\wp}^{*}, then the sharp bound is

∣H3(1)∣≤19≈0.1111…,|H_3(1)|\leq \frac{1}{9}\approx 0.1111\ldots,

with extremal function

f(z)=zexp⁡(13(ez3−1))=z+13z4+29z7+⋯ .f(z)=z\exp\left(\frac{1}{3}(e^{z^3}-1)\right)=z+\frac{1}{3}z^4+\frac{2}{9}z^7+\cdots.

Kumar and Gangania had previously obtained the weaker bound ∣H3(1)∣≤0.150627|H_3(1)|\leq 0.150627 for this class; the conjecture proposes the sharp value and an extremal function. Its resolution is not supplied in the source material.

References

Primary source

Neha Verma and S. Sivaprasad Kumar, “A Conjecture on H_3(1) For Certain Starlike Functions”, arXiv:2208.02975 (2022).

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