Benoît Blossier, Mariane Mangin-Brinet, José Manuel Morgado Chávez, Teseo San José
{"title":"The $η_c$-meson leading-twist distribution amplitude","authors":"Benoît Blossier, Mariane Mangin-Brinet, José Manuel Morgado Chávez, Teseo San José","doi":"arxiv-2409.12084","DOIUrl":null,"url":null,"abstract":"In this project, we employ the short-distance factorization to compute the\ndistribution amplitude of the $\\eta_c$-meson from Lattice QCD at leading twist.\nWe employ a set of CLS $N_f=2$ ensembles at three lattice spacings and various\nquark masses to extrapolate the pseudo distribution to the physical point in\nthe isospin limit. We solve the inverse problem modeling the distribution\namplitude, and we match our results to the light-cone in the\n$\\overline{\\text{MS}}$-scheme. We include a complete error budget, and we\ncompare to two alternative approaches: non-relativistic QCD and Dyson-Schwinger\nequations, finding good agreement with the latter but not with the former.","PeriodicalId":501191,"journal":{"name":"arXiv - PHYS - High Energy Physics - Lattice","volume":"12 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - High Energy Physics - Lattice","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.12084","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
In this project, we employ the short-distance factorization to compute the
distribution amplitude of the $\eta_c$-meson from Lattice QCD at leading twist.
We employ a set of CLS $N_f=2$ ensembles at three lattice spacings and various
quark masses to extrapolate the pseudo distribution to the physical point in
the isospin limit. We solve the inverse problem modeling the distribution
amplitude, and we match our results to the light-cone in the
$\overline{\text{MS}}$-scheme. We include a complete error budget, and we
compare to two alternative approaches: non-relativistic QCD and Dyson-Schwinger
equations, finding good agreement with the latter but not with the former.