The integrable Bullough-Dodd model under celestial holography

Abstract We study celestial amplitudes for the S-matrix of the 2d integrable Bullough-Dodd model. This model has bound states that appear as poles in the physics strip of its 2d S-matrix, which complicates the computation of celestial amplitudes. However, it turns out that the celestial amplitudes a...

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Main Authors: Minjia Wang, Wei Fan
Format: Article
Language:English
Published: SpringerOpen 2025-07-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP07(2025)133
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author Minjia Wang
Wei Fan
author_facet Minjia Wang
Wei Fan
author_sort Minjia Wang
collection DOAJ
description Abstract We study celestial amplitudes for the S-matrix of the 2d integrable Bullough-Dodd model. This model has bound states that appear as poles in the physics strip of its 2d S-matrix, which complicates the computation of celestial amplitudes. However, it turns out that the celestial amplitudes are, in fact, well-structured. The celestial bootstrap (arising from the unitarity and crossing symmetry of 2d S-matrix) can be decomposed into a finite-dimensional linear space, whose base-integrals evaluate into harmonic numbers. This clean structure replaces the complicated integration with simple algebra of elementary functions, and the celestial bootstrap reduces to a programmable recursion process of simple algebra. Interestingly, this linear space has a subspace that happens to cover the celestial bootstrap of the Sinh-Gordon model studied by arXiv:2209.02776 . So the celestial dual of these 2d integrable models turns out to be ‘bootstrapable’ in the practical sense, that is, a programmable recursion process.
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spelling doaj-art-8738e7204c6c43a080ebb38ca62a7add2025-08-20T03:45:40ZengSpringerOpenJournal of High Energy Physics1029-84792025-07-012025711910.1007/JHEP07(2025)133The integrable Bullough-Dodd model under celestial holographyMinjia Wang0Wei Fan1Department of Physics, School of Science, Jiangsu University of Science and TechnologyDepartment of Physics, School of Science, Jiangsu University of Science and TechnologyAbstract We study celestial amplitudes for the S-matrix of the 2d integrable Bullough-Dodd model. This model has bound states that appear as poles in the physics strip of its 2d S-matrix, which complicates the computation of celestial amplitudes. However, it turns out that the celestial amplitudes are, in fact, well-structured. The celestial bootstrap (arising from the unitarity and crossing symmetry of 2d S-matrix) can be decomposed into a finite-dimensional linear space, whose base-integrals evaluate into harmonic numbers. This clean structure replaces the complicated integration with simple algebra of elementary functions, and the celestial bootstrap reduces to a programmable recursion process of simple algebra. Interestingly, this linear space has a subspace that happens to cover the celestial bootstrap of the Sinh-Gordon model studied by arXiv:2209.02776 . So the celestial dual of these 2d integrable models turns out to be ‘bootstrapable’ in the practical sense, that is, a programmable recursion process.https://doi.org/10.1007/JHEP07(2025)133Conformal and W SymmetryField Theories in Lower DimensionsIntegrable Field TheoriesScattering Amplitudes
spellingShingle Minjia Wang
Wei Fan
The integrable Bullough-Dodd model under celestial holography
Journal of High Energy Physics
Conformal and W Symmetry
Field Theories in Lower Dimensions
Integrable Field Theories
Scattering Amplitudes
title The integrable Bullough-Dodd model under celestial holography
title_full The integrable Bullough-Dodd model under celestial holography
title_fullStr The integrable Bullough-Dodd model under celestial holography
title_full_unstemmed The integrable Bullough-Dodd model under celestial holography
title_short The integrable Bullough-Dodd model under celestial holography
title_sort integrable bullough dodd model under celestial holography
topic Conformal and W Symmetry
Field Theories in Lower Dimensions
Integrable Field Theories
Scattering Amplitudes
url https://doi.org/10.1007/JHEP07(2025)133
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