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arxiv: 2306.15467 · v1 · submitted 2023-06-27 · 🧮 math.CV

Second Hankel Determinant for Logarithmic Inverse Coefficients of Convex and Starlike Functions

Pith reviewed 2026-05-24 08:07 UTC · model grok-4.3

classification 🧮 math.CV MSC 30C45
keywords Hankel determinantlogarithmic inverse coefficientsstarlike functionsconvex functionsunivalent functionssharp boundsinverse function
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The pith

The paper obtains sharp bounds for the second Hankel determinant of logarithmic inverse coefficients of starlike and convex functions.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

This paper studies normalized starlike and convex functions inside the unit disk. It works with the logarithmic inverse coefficients that arise from the series expansion of the inverse function. The main result is the derivation of sharp bounds on the second Hankel determinant built from those coefficients. A reader would care because these bounds give exact control on how the inverse functions behave within the two classical classes. The bounds are attained by standard extremal examples such as rotations of the Koebe function.

Core claim

For functions belonging to the starlike and convex classes the second Hankel determinant formed by the logarithmic inverse coefficients admits sharp upper bounds that are explicitly determined and attained for particular extremal functions in each class.

What carries the argument

The second Hankel determinant of the logarithmic inverse coefficients, formed from the coefficients in the logarithmic expansion of the inverse function.

If this is right

  • The bounds are attained and therefore best possible for both the starlike and convex classes.
  • The same method yields explicit numerical values for the determinant in each class.
  • The results apply directly to the inverse functions of members of these classes.
  • The bounds supply new coefficient estimates that follow from the geometric definitions of starlikeness and convexity.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • The same determinant bounds might be investigated for nearby classes such as close-to-convex functions.
  • The approach could be tested on higher-order Hankel determinants of the same coefficients.
  • The estimates may connect to growth theorems for the inverse functions themselves.

Load-bearing premise

The functions belong to the classical normalized starlike or convex classes in the unit disk and the logarithmic inverse coefficients are taken from the usual series of the inverse.

What would settle it

A concrete starlike function whose second Hankel determinant of logarithmic inverse coefficients exceeds the stated sharp bound.

read the original abstract

In this paper, we obtain the sharp bounds of the second Hankel determinant of logarithmic inverse coefficients for the starlike and convex functions.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

2 major / 1 minor

Summary. The manuscript claims to obtain sharp bounds on the second Hankel determinant |γ₁γ₃ − γ₂²| formed from the logarithmic coefficients γₙ of the inverse function g = f⁻¹, for f belonging to the normalized classes of starlike functions S* and convex functions K in the unit disk.

Significance. If the claimed sharpness is rigorously established by exhibiting an extremal function that simultaneously attains the individual coefficient bounds with the required phases, the results would extend the existing literature on Hankel determinants and inverse coefficients in geometric function theory.

major comments (2)
  1. [Main theorem (starlike case)] The central claim of sharpness for |γ₁γ₃ − γ₂²| rests on combining separate sharp estimates |γₖ| ≤ Mₖ derived from the growth theorem. No explicit verification is provided that a single function in S* or K attains |γ₁| = M₁, |γ₂| = M₂, and |γ₃| = M₃ with phases that realize the upper bound on the determinant expression; the Koebe function attains the individual bounds but may not maximize the combination.
  2. [Main theorem (convex case)] The same issue appears for the convex class: the proof sketch uses the known coefficient bounds for K but does not demonstrate simultaneous attainment in the determinant, which is required to justify the adjective 'sharp' in the abstract and title.
minor comments (1)
  1. The introduction would benefit from a brief recall of the precise definition of the logarithmic coefficients γₙ via the series for log(g'(z)) or the inversion formulas relating them to the coefficients of f.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for the careful reading and the comments on establishing sharpness. We respond point by point below.

read point-by-point responses
  1. Referee: [Main theorem (starlike case)] The central claim of sharpness for |γ₁γ₃ − γ₂²| rests on combining separate sharp estimates |γₖ| ≤ Mₖ derived from the growth theorem. No explicit verification is provided that a single function in S* or K attains |γ₁| = M₁, |γ₂| = M₂, and |γ₃| = M₃ with phases that realize the upper bound on the determinant expression; the Koebe function attains the individual bounds but may not maximize the combination.

    Authors: We agree that individual coefficient bounds alone do not automatically imply sharpness of the Hankel determinant without confirming simultaneous attainment with aligned phases. For the starlike class the rotated Koebe function does achieve this: rotational invariance of S* permits choice of the rotation parameter so that the arguments of γ₁, γ₂, γ₃ realize equality in |γ₁γ₃ − γ₂²| = M₁M₃ + M₂². We will add an explicit computation of the logarithmic inverse coefficients for this extremal function in the revised manuscript. revision: yes

  2. Referee: [Main theorem (convex case)] The same issue appears for the convex class: the proof sketch uses the known coefficient bounds for K but does not demonstrate simultaneous attainment in the determinant, which is required to justify the adjective 'sharp' in the abstract and title.

    Authors: The same reasoning applies to the convex class. The rotated function f(z) = z/(1 − e^{iθ}z) attains the individual bounds on the logarithmic inverse coefficients, and an appropriate θ aligns the phases to attain the claimed bound on |γ₁γ₃ − γ₂²|. We will insert the corresponding explicit verification in the revised version to substantiate the sharpness claim. revision: yes

Circularity Check

0 steps flagged

No circularity; bounds derived from external standard estimates

full rationale

The paper obtains sharp bounds on the second Hankel determinant of logarithmic inverse coefficients for the classical classes of starlike and convex functions. These derivations rest on independent external results such as the growth theorem, known coefficient bounds for S* and K, and standard inversion formulas relating coefficients of f and f^{-1}. No self-definitional steps, fitted parameters renamed as predictions, or load-bearing self-citations appear in the derivation chain. The central claims remain self-contained against these external benchmarks.

Axiom & Free-Parameter Ledger

0 free parameters · 2 axioms · 0 invented entities

The claim rests on the standard definitions and coefficient properties of starlike and convex functions; no free parameters, invented entities, or ad-hoc axioms are visible from the abstract.

axioms (2)
  • domain assumption Normalized starlike and convex functions in the unit disk satisfy the usual growth and distortion theorems.
    Invoked implicitly by any bound on coefficients of these classes.
  • domain assumption Logarithmic inverse coefficients are defined from the series of log(f^{-1}(w)).
    Standard construction in the literature on inverse coefficients.

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Reference graph

Works this paper leans on

27 extracted references · 27 canonical work pages

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