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Autori principali: Capuano, Mattia, Ferro, Livia, Lukowski, Tomasz, Palazio, Alessandro, Zhang, Yao-Qi
Natura: Preprint
Pubblicazione: 2026
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Accesso online:https://arxiv.org/abs/2603.09965
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author Capuano, Mattia
Ferro, Livia
Lukowski, Tomasz
Palazio, Alessandro
Zhang, Yao-Qi
author_facet Capuano, Mattia
Ferro, Livia
Lukowski, Tomasz
Palazio, Alessandro
Zhang, Yao-Qi
contents In this paper we study the cluster algebraic properties of wavefunction coefficients for massless scalar theories in de Sitter cosmology. We show that the symbol of the wavefunction coefficient of the $n$-site path graph $P_n$ obeys a generalisation of cluster adjacency, where all letters in a given word belong to the same cluster of an $A_{2n-3}$ algebra, with certain additional constraints on the order of the letters. We call this property the ordered single cluster condition, and provide its physical interpretation. This condition is stronger than the usual cluster adjacency obeyed by neighbouring letters, and imposes stronger constraints for the symbol bootstrap. We also show how any tree graph satisfies a cluster-like structure in terms of tubes and tubings on the underlying graph, which allows for a similar bootstrap approach.
format Preprint
id arxiv_https___arxiv_org_abs_2603_09965
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Generalised Cluster Adjacency for Cosmology
Capuano, Mattia
Ferro, Livia
Lukowski, Tomasz
Palazio, Alessandro
Zhang, Yao-Qi
High Energy Physics - Theory
In this paper we study the cluster algebraic properties of wavefunction coefficients for massless scalar theories in de Sitter cosmology. We show that the symbol of the wavefunction coefficient of the $n$-site path graph $P_n$ obeys a generalisation of cluster adjacency, where all letters in a given word belong to the same cluster of an $A_{2n-3}$ algebra, with certain additional constraints on the order of the letters. We call this property the ordered single cluster condition, and provide its physical interpretation. This condition is stronger than the usual cluster adjacency obeyed by neighbouring letters, and imposes stronger constraints for the symbol bootstrap. We also show how any tree graph satisfies a cluster-like structure in terms of tubes and tubings on the underlying graph, which allows for a similar bootstrap approach.
title Generalised Cluster Adjacency for Cosmology
topic High Energy Physics - Theory
url https://arxiv.org/abs/2603.09965