Second Hankel Determinant for Logarithmic Inverse Coefficients of Convex and Starlike Functions
Pith reviewed 2026-05-24 08:07 UTC · model grok-4.3
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.
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
- 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.
Referee Report
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)
- [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.
- [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)
- 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
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
-
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
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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
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
axioms (2)
- domain assumption Normalized starlike and convex functions in the unit disk satisfy the usual growth and distortion theorems.
- domain assumption Logarithmic inverse coefficients are defined from the series of log(f^{-1}(w)).
Lean theorems connected to this paper
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IndisputableMonolith/Cost/FunctionalEquation.leanwashburn_uniqueness_aczel unclear?
unclearRelation between the paper passage and the cited Recognition theorem.
Theorem 3.1 ... |H_{2,1}(F_{f^{-1}}/2)| ≤ 1/33 ... equality for p(z) = 1 + 2√(2/11)z + z² / (1 - z²)
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IndisputableMonolith/Foundation/AbsoluteFloorClosure.leanabsolute_floor_iff_bare_distinguishability unclear?
unclearRelation between the paper passage and the cited Recognition theorem.
Lemma 2.2 ... Y(A,B,C) maximizer over the unit disk
What do these tags mean?
- matches
- The paper's claim is directly supported by a theorem in the formal canon.
- supports
- The theorem supports part of the paper's argument, but the paper may add assumptions or extra steps.
- extends
- The paper goes beyond the formal theorem; the theorem is a base layer rather than the whole result.
- uses
- The paper appears to rely on the theorem as machinery.
- contradicts
- The paper's claim conflicts with a theorem or certificate in the canon.
- unclear
- Pith found a possible connection, but the passage is too broad, indirect, or ambiguous to say the theorem truly supports the claim.
Reference graph
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