Heavy meson photoproduction in peripheral AA collisions
Autor(a) principal: | |
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Data de Publicação: | 2018 |
Outros Autores: | |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UFRGS |
Texto Completo: | http://hdl.handle.net/10183/182896 |
Resumo: | The exclusive photoproduction of the heavy vector mesons ψ and Y is investigated in peripheral Pb-Pb collisions for the energies available at the LHC, ffiffiffi sp ¼ 2.76 TeV and ffiffiffi ps ¼ 5.02 TeV. To evaluate the robustness of the light-cone color dipole formalism, previously tested in the ultraperipheral regime, the rapidity distribution and the nuclear modification factor (RAA) are calculated for the three centrality classes: 30%–50%, 50%–70%, and 70%–90%. The ultraperipheral to peripheral regime transition was carried out by sophisticating the photon flux description and the photonuclear cross section, taking into account the effective interaction area. In our calculations, three scenarios were considered: (scenario 1) the direct application of the usual photon flux and of the photonuclear cross section with no relevant change in relation to the ultraperipheral collision (UPCs), (scenario 2) the application of an effective photon flux keeping the photonuclear cross section unchanged, and (scenario 3) also considering an effective photonuclear cross section. The results obtained with the three different scenarios were compared with the ALICE measurements, showing a better agreement with the data (only J=ψ at the moment) in the more complete approach (scenario 3), mainly in the more central regions (30%–50% and 50%–70%) where the uncertainty is smaller. |
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Gay Ducati, Maria BeatrizMartins, Sony2018-09-28T02:34:53Z20181550-7998http://hdl.handle.net/10183/182896001072358The exclusive photoproduction of the heavy vector mesons ψ and Y is investigated in peripheral Pb-Pb collisions for the energies available at the LHC, ffiffiffi sp ¼ 2.76 TeV and ffiffiffi ps ¼ 5.02 TeV. To evaluate the robustness of the light-cone color dipole formalism, previously tested in the ultraperipheral regime, the rapidity distribution and the nuclear modification factor (RAA) are calculated for the three centrality classes: 30%–50%, 50%–70%, and 70%–90%. The ultraperipheral to peripheral regime transition was carried out by sophisticating the photon flux description and the photonuclear cross section, taking into account the effective interaction area. In our calculations, three scenarios were considered: (scenario 1) the direct application of the usual photon flux and of the photonuclear cross section with no relevant change in relation to the ultraperipheral collision (UPCs), (scenario 2) the application of an effective photon flux keeping the photonuclear cross section unchanged, and (scenario 3) also considering an effective photonuclear cross section. The results obtained with the three different scenarios were compared with the ALICE measurements, showing a better agreement with the data (only J=ψ at the moment) in the more complete approach (scenario 3), mainly in the more central regions (30%–50% and 50%–70%) where the uncertainty is smaller.application/pdfengPhysical review. D, Particles, fields, gravitation, and cosmology. College Park. Vol. 97, no. 11 (June 2018), 116013, 9 p.Fotoproducao de mesonsAceleradores de partículasColisao de ions pesadosMésons psiHeavy meson photoproduction in peripheral AA collisionsEstrangeiroinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/openAccessreponame:Repositório Institucional da UFRGSinstname:Universidade Federal do Rio Grande do Sul (UFRGS)instacron:UFRGSORIGINAL001072358.pdfTexto completo (inglês)application/pdf515435http://www.lume.ufrgs.br/bitstream/10183/182896/1/001072358.pdf6056830ce80f8056ca767ef46eb3bb96MD51TEXT001072358.pdf.txt001072358.pdf.txtExtracted Texttext/plain36147http://www.lume.ufrgs.br/bitstream/10183/182896/2/001072358.pdf.txt240c064e51d9f1db6c5be0b9523db3dfMD52THUMBNAIL001072358.pdf.jpg001072358.pdf.jpgGenerated Thumbnailimage/jpeg1868http://www.lume.ufrgs.br/bitstream/10183/182896/3/001072358.pdf.jpg9ea26f585e415c0423f87537cc0319f1MD5310183/1828962018-10-05 08:01:54.151oai:www.lume.ufrgs.br:10183/182896Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2018-10-05T11:01:54Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false |
dc.title.pt_BR.fl_str_mv |
Heavy meson photoproduction in peripheral AA collisions |
title |
Heavy meson photoproduction in peripheral AA collisions |
spellingShingle |
Heavy meson photoproduction in peripheral AA collisions Gay Ducati, Maria Beatriz Fotoproducao de mesons Aceleradores de partículas Colisao de ions pesados Mésons psi |
title_short |
Heavy meson photoproduction in peripheral AA collisions |
title_full |
Heavy meson photoproduction in peripheral AA collisions |
title_fullStr |
Heavy meson photoproduction in peripheral AA collisions |
title_full_unstemmed |
Heavy meson photoproduction in peripheral AA collisions |
title_sort |
Heavy meson photoproduction in peripheral AA collisions |
author |
Gay Ducati, Maria Beatriz |
author_facet |
Gay Ducati, Maria Beatriz Martins, Sony |
author_role |
author |
author2 |
Martins, Sony |
author2_role |
author |
dc.contributor.author.fl_str_mv |
Gay Ducati, Maria Beatriz Martins, Sony |
dc.subject.por.fl_str_mv |
Fotoproducao de mesons Aceleradores de partículas Colisao de ions pesados Mésons psi |
topic |
Fotoproducao de mesons Aceleradores de partículas Colisao de ions pesados Mésons psi |
description |
The exclusive photoproduction of the heavy vector mesons ψ and Y is investigated in peripheral Pb-Pb collisions for the energies available at the LHC, ffiffiffi sp ¼ 2.76 TeV and ffiffiffi ps ¼ 5.02 TeV. To evaluate the robustness of the light-cone color dipole formalism, previously tested in the ultraperipheral regime, the rapidity distribution and the nuclear modification factor (RAA) are calculated for the three centrality classes: 30%–50%, 50%–70%, and 70%–90%. The ultraperipheral to peripheral regime transition was carried out by sophisticating the photon flux description and the photonuclear cross section, taking into account the effective interaction area. In our calculations, three scenarios were considered: (scenario 1) the direct application of the usual photon flux and of the photonuclear cross section with no relevant change in relation to the ultraperipheral collision (UPCs), (scenario 2) the application of an effective photon flux keeping the photonuclear cross section unchanged, and (scenario 3) also considering an effective photonuclear cross section. The results obtained with the three different scenarios were compared with the ALICE measurements, showing a better agreement with the data (only J=ψ at the moment) in the more complete approach (scenario 3), mainly in the more central regions (30%–50% and 50%–70%) where the uncertainty is smaller. |
publishDate |
2018 |
dc.date.accessioned.fl_str_mv |
2018-09-28T02:34:53Z |
dc.date.issued.fl_str_mv |
2018 |
dc.type.driver.fl_str_mv |
Estrangeiro info:eu-repo/semantics/article |
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info:eu-repo/semantics/publishedVersion |
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publishedVersion |
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http://hdl.handle.net/10183/182896 |
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1550-7998 |
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001072358 |
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eng |
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eng |
dc.relation.ispartof.pt_BR.fl_str_mv |
Physical review. D, Particles, fields, gravitation, and cosmology. College Park. Vol. 97, no. 11 (June 2018), 116013, 9 p. |
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