Recognition: unknown
A perturbative Liouville prescription for the celestial three-gluon amplitude
Pith reviewed 2026-05-07 06:09 UTC · model grok-4.3
The pith
Resolving the Liouville-Mellin map ambiguity yields a controlled b-expansion of the celestial three-gluon amplitude whose leading term recovers tree-level Yang-Mills.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
After fixing the Liouville-Mellin parameter dictionary by global conformal covariance and semiclassical compatibility, the b squared expansion of the full Liouville DOZZ three-point function produces a leading term that matches the tree-level Yang-Mills amplitude in the small total momentum limit, while the first correction term is expressible in closed form using modified Bessel functions whose soft-gluon limit separates into geometric and logarithmic contributions.
What carries the argument
The uniquely fixed map between Liouville parameters and Mellin variables, which converts the DOZZ three-point function into a controlled perturbative series in the Liouville coupling b.
If this is right
- The same fixed dictionary supplies a systematic algorithm for computing higher orders in the b expansion of the same amplitude.
- The closed-form one-loop term gives an explicit prediction for the first quantum correction to the celestial three-gluon vertex in the presence of a dilaton.
- The separation of the soft limit into geometric and logarithmic pieces suggests that each contribution may be traceable to distinct sectors of the dual celestial theory.
- The construction extends the STZ tree-level matching to a perturbative regime that remains computable order by order.
Where Pith is reading between the lines
- The same resolution procedure could be applied to higher-point celestial amplitudes or to amplitudes involving different gauge-theory particles.
- Numerical evaluation of the Bessel-function expression in the soft region could be compared with results from other celestial-holography techniques to test the map.
- If the geometric-logarithmic split persists at higher orders, it may point to a natural factorization in the dual two-dimensional theory.
Load-bearing premise
That demanding global conformal covariance together with semiclassical compatibility uniquely determines both the Liouville-Mellin variable identification and the operator normalization.
What would settle it
An independent computation of the one-loop celestial three-gluon amplitude in the dilaton background, via standard perturbative methods, that fails to reproduce the modified-Bessel expression for the order-b squared correction.
read the original abstract
We study the celestial three-gluon amplitude in a dilaton background through the Mellin-Liouville formulation proposed by Stieberger, Taylor and Zhu (STZ). The original map contains an ambiguity in the identification of Liouville and Mellin variables; we resolve it by requiring global conformal covariance and compatibility with the semiclassical expansion of Liouville theory. This uniquely fixes the operator normalization and the parameter dictionary, and leads to a controlled expansion in the Liouville coupling $b$. Starting from the full Liouville DOZZ three-point function, we derive the leading and first subleading terms in the $b^2$ expansion. The leading term reproduces the tree-level Yang-Mills amplitude in the small total momentum limit, as anticipated in the STZ proposal. The one-loop correction can be written in closed form using modified Bessel functions, and its soft limit exhibits a clear separation into geometric and logarithmic contributions. The resulting framework extends the STZ proposal to finite-$b$ corrections in a consistent and computable way.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript develops a perturbative Liouville prescription for the celestial three-gluon amplitude in a dilaton background. The authors resolve the ambiguity in the Liouville-Mellin variable map by requiring global conformal covariance and compatibility with the semiclassical (small-b) expansion of Liouville theory. Starting from the exact DOZZ three-point function, they derive the leading and O(b²) terms in the expansion; the leading term reproduces the tree-level Yang-Mills amplitude in the small total momentum limit, while the subleading correction is expressed in closed form using modified Bessel functions whose soft limit separates geometric and logarithmic contributions.
Significance. If the derivation holds, the work supplies a controlled, parameter-free framework for finite-b corrections to celestial amplitudes, extending the STZ proposal. Notable strengths include the use of the exact DOZZ formula (no ad-hoc approximations) and the closed-form Bessel expression for the one-loop term, which enables analytic access to loop-level effects and a clean soft-limit decomposition. This could facilitate systematic higher-point calculations and strengthen the link between Liouville theory and celestial holography.
minor comments (3)
- The explicit dictionary mapping Liouville momenta to Mellin variables (fixed by the covariance and semiclassical requirements) should be displayed in a table or boxed equation to aid reproducibility and verification of the leading-order match.
- In the soft-limit analysis of the O(b²) term, a short comparison of the separated geometric and logarithmic pieces to the known soft theorems of Yang-Mills theory would clarify the physical interpretation.
- A brief remark on the radius of convergence of the b-expansion or the regime where the small-total-momentum limit remains valid would help readers assess the practical range of the results.
Simulated Author's Rebuttal
We thank the referee for their positive assessment of our manuscript, including the recognition of our resolution of the Liouville-Mellin map ambiguity via conformal covariance and semiclassical consistency, the controlled b-expansion derived from the exact DOZZ function, and the closed-form modified Bessel expression for the O(b²) term. The referee recommends minor revision but raises no specific major comments or criticisms. We will incorporate any minor editorial or presentational suggestions in the revised version.
Circularity Check
No significant circularity; derivation is self-contained
full rationale
The paper begins with the standard, externally established DOZZ three-point function of Liouville theory and executes a perturbative series expansion in the Liouville parameter b. The sole additional input is the resolution of the Liouville-Mellin variable map via the independent requirements of global conformal covariance and consistency with the known semiclassical (small-b) limit of Liouville theory; these are standard symmetry and limiting-case constraints, not data fits or self-referential definitions. The leading-order term is verified to reproduce the tree-level Yang-Mills celestial amplitude in the small-total-momentum regime (a consistency check with the prior STZ proposal by unrelated authors), while the O(b²) correction is obtained in closed form. No step reduces by construction to a fitted parameter, a self-citation chain, or an ansatz smuggled from the authors' own prior work. The derivation therefore stands on external benchmarks and is not circular.
Axiom & Free-Parameter Ledger
axioms (2)
- domain assumption Global conformal covariance must hold for the Liouville-Mellin map
- domain assumption The map must be compatible with the semiclassical expansion of Liouville theory
Reference graph
Works this paper leans on
-
[1]
Lectures on the Infrared Structure of Gravity and Gauge Theory
A. Strominger,Lectures on the Infrared Structure of Gravity and Gauge Theory, arXiv:1703.05448
-
[2]
S. Pasterski, M. Pate, A. M. Raclariu,Celestial Holography,arXiv:2111.11392
- [3]
-
[4]
Donnay,Celestial holography: An asymptotic symmetry perspective,Phys
L. Donnay,Celestial Holography: An Asymptotic Symmetry Perspective,Phys. Rept. 1073 (2024) 1-41, arXiv:2310.12922
-
[5]
Pasterski,Lectures on celestial amplitudes,Eur
S. Pasterski,Lectures on celestial amplitudes,Eur. Phys. J. C81 (2021) 12, 1062, arXiv:2108.04801
-
[6]
S. Pasterski, S. H. Shao, A. Strominger,Flat Space Amplitudes and Conformal Symmetry of the Celestial Sphere,Phys. Rev. D96 (2017) 065026, arXiv:1701.00049. – 23 –
-
[7]
A. Schreiber, A. Volovich, M. Zlotnikov,Tree-level gluon amplitudes on the celestial sphere, Phys. Lett. B781 (2018) 349-357, arXiv:1711.08435
-
[8]
Kalyanapuram,Gauge and Gravity Amplitudes on the Celestial Sphere,Phys
N. Kalyanapuram,Gauge and Gravity Amplitudes on the Celestial Sphere,Phys. Rev. D103 (2021) 085015, arXiv:2012.04579
-
[9]
S. Banerjee, S. Ghosh, P. Paul,MHV Graviton Scattering Amplitudes and Current Algebra on the Celestial Sphere,JHEP 02 (2021) 176, arXiv:2008.04330
-
[10]
Stieberger, T.R
S. Stieberger, T.R. Taylor, B. Zhu,Celestial Liouville theory for Yang–Mills amplitudes, Phys. Lett. B836 (2023) 137588
2023
- [11]
-
[12]
Giribet,Remarks on celestial amplitudes and Liouville theory,Int
G. Giribet,Remarks on celestial amplitudes and Liouville theory,Int. J. Mod. Phys. D34 (2025) 01, arXiv:2403.03374
- [13]
-
[14]
Stieberger, T.R
S. Stieberger, T.R. Taylor, B. Zhu,Yang–Mills as a Liouville theory,Phys. Lett. B846 (2023) 138229
2023
-
[15]
Belavin, A.M
A.A. Belavin, A.M. Polyakov, A.B. Zamolodchikov,Infinite conformal symmetry in 2D quantum field theories,Nucl. Phys. B241 (1984) 333
1984
-
[16]
Seiberg,Notes on Quantum Liouville Theory and Quantum Gravity, Prog
N. Seiberg,Notes on Quantum Liouville Theory and Quantum Gravity, Prog. Theor. Phys. Suppl. 102 (1990) 319-349
1990
- [17]
-
[18]
Teschner,On the Liouville three point function,Phys
J. Teschner,On the Liouville three point function,Phys. Lett. B363 (1995) 65-70, hep-th/9507109
-
[19]
A.B. Zamolodchikov, A.B. Zamolodchikov,Structure constants and conformal bootstrap in Liouville field theory,Nucl. Phys. B477 (1996) 577, hep-th/9506136
-
[20]
Teschner,Liouville theory revisited,Class
J. Teschner,Liouville theory revisited,Class. Quant. Grav. 18 (2001) R153, hep-th/0104158
-
[21]
Teschner,A lecture on the Liouville vertex operators,Int
J. Teschner,A lecture on the Liouville vertex operators,Int. J. Mod. Phys. A19 (2004) 436-458, hep-th/0303150
-
[22]
Nakayama,Liouville field theory: A Decade after the revolutionInt
Y. Nakayama,Liouville field theory: A Decade after the revolutionInt. J. Mod. Phys. A19 (2004) 2771-2930, hep-th/0402009
- [23]
-
[24]
Ribault,Conformal field theory on the plane,arXiv:1406.4290
S. Ribault,Conformal field theory on the plane,arXiv:1406.4290
-
[25]
Thorn,Liouville Perturbation Theory,Phys
Ch.B. Thorn,Liouville Perturbation Theory,Phys. Rev. D66 (2002) 027702, arXiv:hep-th/0204142
-
[26]
F. Ferrari, M. R. Pi¸ atek, A. R. Pietrykowski,Small-b expansion of the DOZZ formula for light operators,arXiv:2509.21182v2. – 24 –
discussion (0)
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