pith. sign in

Analytic Continuation of Liouville Theory

7 Pith papers cite this work. Polarity classification is still indexing.

7 Pith papers citing it
abstract

Correlation functions in Liouville theory are meromorphic functions of the Liouville momenta, as is shown explicitly by the DOZZ formula for the three-point function on the sphere. In a certain physical region, where a real classical solution exists, the semiclassical limit of the DOZZ formula is known to agree with what one would expect from the action of the classical solution. In this paper, we ask what happens outside of this physical region. Perhaps surprisingly we find that, while in some range of the Liouville momenta the semiclassical limit is associated to complex saddle points, in general Liouville's equations do not have enough complex-valued solutions to account for the semiclassical behavior. For a full picture, we either must include "solutions" of Liouville's equations in which the Liouville field is multivalued (as well as being complex-valued), or else we can reformulate Liouville theory as a Chern-Simons theory in three dimensions, in which the requisite solutions exist in a more conventional sense. We also study the case of "timelike" Liouville theory, where we show that a proposal of Al. B. Zamolodchikov for the exact three-point function on the sphere can be computed by the original Liouville path integral evaluated on a new integration cycle.

citation-role summary

background 1

citation-polarity summary

verdicts

UNVERDICTED 7

roles

background 1

polarities

background 1

representative citing papers

Quantum Liouville Cosmology

hep-th · 2025-12-17 · unverdicted · novelty 6.0

Timelike Liouville disk path integrals in fixed K-representation produce Hartle-Hawking-like states, a conjecture for all-loop wavefunctions, and a K-independent inner product for 2D quantum cosmology.

Timelike Liouville theory and AdS$_3$ gravity at finite cutoff

hep-th · 2025-08-05 · unverdicted · novelty 6.0

Proposes that AdS3 gravity at finite cutoff is dual to a CFT2 coupled to timelike Liouville theory deformed by a marginal operator, with checks via semiclassical partition functions and EOM matching.

All the D-Branes of Resurgence

hep-th · 2023-01-12 · unverdicted · novelty 6.0

Negative-tension ZZ-branes are required by resurgence to build complete transseries for minimal-string free energies, with analytic Stokes data and extensions to JT gravity and other string models.

$\mathcal{N}=2$ Liouville SCFT in Four Dimensions

hep-th · 2019-07-21 · unverdicted · novelty 6.0

Constructs an N=2 Liouville SCFT in 4D, shows no quantum correction to the classical background charge, finds c=0 and negative a depending on the charge, and derives integral expressions for superfield vertex operator correlators.

Picard-Lefschetz theory and alien calculus: a case study

math-ph · 2026-05-09 · unverdicted · novelty 6.0

Explicit calculations in the Airy, Bessel, and Gamma models show that Lefschetz thimble wall-crossing produces the same Stokes coefficients as alien operators acting on Borel singularities.

A perturbative Liouville prescription for the celestial three-gluon amplitude

hep-th · 2026-04-30 · unverdicted · novelty 6.0

By fixing the Liouville-Mellin dictionary via conformal covariance and semiclassical consistency, the authors derive the leading and subleading b^2 terms of the celestial three-gluon amplitude from the DOZZ function, with the one-loop piece expressed using modified Bessel functions.

Euclidean volume fluctuations in de Sitter quantum gravity

hep-th · 2026-04-28 · unverdicted · novelty 4.0 · 2 refs

From the de Sitter partition function in various approximations, the volume probability distribution concentrates around the classical value but shifts to favor smaller universes as quantum effects increase.

citing papers explorer

Showing 7 of 7 citing papers.

  • Quantum Liouville Cosmology hep-th · 2025-12-17 · unverdicted · none · ref 34 · internal anchor

    Timelike Liouville disk path integrals in fixed K-representation produce Hartle-Hawking-like states, a conjecture for all-loop wavefunctions, and a K-independent inner product for 2D quantum cosmology.

  • Timelike Liouville theory and AdS$_3$ gravity at finite cutoff hep-th · 2025-08-05 · unverdicted · none · ref 45 · internal anchor

    Proposes that AdS3 gravity at finite cutoff is dual to a CFT2 coupled to timelike Liouville theory deformed by a marginal operator, with checks via semiclassical partition functions and EOM matching.

  • All the D-Branes of Resurgence hep-th · 2023-01-12 · unverdicted · none · ref 96 · internal anchor

    Negative-tension ZZ-branes are required by resurgence to build complete transseries for minimal-string free energies, with analytic Stokes data and extensions to JT gravity and other string models.

  • $\mathcal{N}=2$ Liouville SCFT in Four Dimensions hep-th · 2019-07-21 · unverdicted · none · ref 28 · internal anchor

    Constructs an N=2 Liouville SCFT in 4D, shows no quantum correction to the classical background charge, finds c=0 and negative a depending on the charge, and derives integral expressions for superfield vertex operator correlators.

  • Picard-Lefschetz theory and alien calculus: a case study math-ph · 2026-05-09 · unverdicted · none · ref 8

    Explicit calculations in the Airy, Bessel, and Gamma models show that Lefschetz thimble wall-crossing produces the same Stokes coefficients as alien operators acting on Borel singularities.

  • A perturbative Liouville prescription for the celestial three-gluon amplitude hep-th · 2026-04-30 · unverdicted · none · ref 23

    By fixing the Liouville-Mellin dictionary via conformal covariance and semiclassical consistency, the authors derive the leading and subleading b^2 terms of the celestial three-gluon amplitude from the DOZZ function, with the one-loop piece expressed using modified Bessel functions.

  • Euclidean volume fluctuations in de Sitter quantum gravity hep-th · 2026-04-28 · unverdicted · none · ref 26 · 2 links

    From the de Sitter partition function in various approximations, the volume probability distribution concentrates around the classical value but shifts to favor smaller universes as quantum effects increase.