Small- b expansion of the DOZZ formula for light operators

We present a systematic asymptotic small-[Formula: see text] expansion of the Liouville DOZZ three-point structure constant in the light-operator regime [Formula: see text] in the limit [Formula: see text]. In this limit the DOZZ structure constant admits the asymptotic representation [Formula: see text] where [Formula: see text] is an explicitly determined prefactor. Using Thorn’s asymptotic expansion of the [Formula: see text]-function, we derive explicit closed-form expressions for the first coefficients [Formula: see text] and show that they form a symmetric polynomial structure in the variables [Formula: see text]. The resulting asymptotic expansion provides explicit finite-[Formula: see text] corrections to the leading light-limit Liouville three-point data and furnishes a practical framework for applications in celestial holography. In particular, it provides Liouville data relevant for a perturbative program aimed at studying finite-[Formula: see text] corrections to celestial Yang–Mills amplitudes. Finally, we formulate such a perturbative Liouville framework and discuss several directions for its future development.

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Publication Details

Journal
International Journal of Modern Physics A
Published
2026-10-15
DOI
https://doi.org/10.1142/s0217751x26501885
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
0.00
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article

Small- b expansion of the DOZZ formula for light operators

Marcin Radosław Piątek, Artur R. Pietrykowski, Franco Ferrari
International Journal of Modern Physics A
Black Holes and Theoretical Physics
article

Small- b expansion of the DOZZ formula for light operators

Marcin Radosław Piątek, Artur R. Pietrykowski, Franco Ferrari
article en

Abstract

We present a systematic asymptotic small-[Formula: see text] expansion of the Liouville DOZZ three-point structure constant in the light-operator regime [Formula: see text] in the limit [Formula: see text]. In this limit the DOZZ structure constant admits the asymptotic representation [Formula: see text] where [Formula: see text] is an explicitly determined prefactor. Using Thorn’s asymptotic expansion of the [Formula: see text]-function, we derive explicit closed-form expressions for the first coefficients [Formula: see text] and show that they form a symmetric polynomial structure in the variables [Formula: see text]. The resulting asymptotic expansion provides explicit finite-[Formula: see text] corrections to the leading light-limit Liouville three-point data and furnishes a practical framework for applications in celestial holography. In particular, it provides Liouville data relevant for a perturbative program aimed at studying finite-[Formula: see text] corrections to celestial Yang–Mills amplitudes. Finally, we formulate such a perturbative Liouville framework and discuss several directions for its future development.

International Journal of Modern Physics A
Openalex Percentile: Top 17%
Black Holes and Theoretical Physics
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