Ratio of \(J/\Psi\) and \(\Psi(2s)\) exclusive photoproduction cross-sections as an indicator for the presence of non-linear QCD evolution
We investigate the proposal that the rise with energy of the ratio of the exclusive photo-production cross-sections of vector mesons \(\Psi(2s)\) and \(J/\Psi\) can serve as an indicator for the presence of high gluon densities and associated non-linear high energy evolution; we study this proposal...
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description | We investigate the proposal that the rise with energy of the ratio of the exclusive photo-production cross-sections of vector mesons \(\Psi(2s)\) and \(J/\Psi\) can serve as an indicator for the presence of high gluon densities and associated non-linear high energy evolution; we study this proposal for both photoproduction on a proton and a lead nucleus. While previous studies were based on unintegrated gluon distributions subject to linear (Balitsky-Fadin-Kuraev-Lipatov) and non-linear (Balitsky-Kovchegov) evolution equations, the current study is based on the Golec-Biernat W\"usthoff (GBW) and Bartels Golec-Biernat Kowalski (BGK) models, which allow assessing more directly the relevance of non-linear corrections for the description of the energy dependence of the photoproduction cross-section. We find that the rise of the ratio is directly related to the presence of a node in the \(\Psi(2s)\) wave function and only manifests itself for the complete non-linear models, while it is absent for their linearized versions. We further provide predictions based on leading order collinear factorization and examine to which extent such an approach can mimic a ratio rising with energy. We also provide a description of recent ALICE data on the energy dependence of the photonuclear \(J/\Psi\) production cross-section and give predictions for the energy dependence of the ratio of \(\Psi(2s)\) and \(J/\Psi\) photoproduction cross-sections for both scattering on a proton and a lead nucleus. |
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While previous studies were based on unintegrated gluon distributions subject to linear (Balitsky-Fadin-Kuraev-Lipatov) and non-linear (Balitsky-Kovchegov) evolution equations, the current study is based on the Golec-Biernat W\"usthoff (GBW) and Bartels Golec-Biernat Kowalski (BGK) models, which allow assessing more directly the relevance of non-linear corrections for the description of the energy dependence of the photoproduction cross-section. We find that the rise of the ratio is directly related to the presence of a node in the \(\Psi(2s)\) wave function and only manifests itself for the complete non-linear models, while it is absent for their linearized versions. We further provide predictions based on leading order collinear factorization and examine to which extent such an approach can mimic a ratio rising with energy. We also provide a description of recent ALICE data on the energy dependence of the photonuclear \(J/\Psi\) production cross-section and give predictions for the energy dependence of the ratio of \(\Psi(2s)\) and \(J/\Psi\) photoproduction cross-sections for both scattering on a proton and a lead nucleus.</description><identifier>EISSN: 2331-8422</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Energy ; Gluons ; Linear evolution equations ; Photoproduction ; Protons ; Scattering cross sections ; Vector mesons ; Wave functions</subject><ispartof>arXiv.org, 2024-01</ispartof><rights>2024. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). 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While previous studies were based on unintegrated gluon distributions subject to linear (Balitsky-Fadin-Kuraev-Lipatov) and non-linear (Balitsky-Kovchegov) evolution equations, the current study is based on the Golec-Biernat W\"usthoff (GBW) and Bartels Golec-Biernat Kowalski (BGK) models, which allow assessing more directly the relevance of non-linear corrections for the description of the energy dependence of the photoproduction cross-section. We find that the rise of the ratio is directly related to the presence of a node in the \(\Psi(2s)\) wave function and only manifests itself for the complete non-linear models, while it is absent for their linearized versions. We further provide predictions based on leading order collinear factorization and examine to which extent such an approach can mimic a ratio rising with energy. 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subjects | Energy Gluons Linear evolution equations Photoproduction Protons Scattering cross sections Vector mesons Wave functions |
title | Ratio of \(J/\Psi\) and \(\Psi(2s)\) exclusive photoproduction cross-sections as an indicator for the presence of non-linear QCD evolution |
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