Update on J/psi regeneration in a hadron gas
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 UNIFESP |
Texto Completo: | http://dx.doi.org/10.1103/PhysRevC.97.044902 https://repositorio.unifesp.br/handle/11600/55643 |
Resumo: | In heavy-ion collisions, after the quark-gluon plasma there is a hadronic gas phase. Using effective Lagrangians, we study the interactions of charmed mesons which lead to J/psi production and absorption in this gas. We update and extend previous calculations introducing strange meson interactions and also including the interactions mediated by the recently measured exotic charmonium resonances Z(3900) and Z(4025). These resonances open new reaction channels for the J/psi, which could potentially lead to changes in its multiplicity. We compute the J/psi production cross section in processes such as D-(s)(*) + (D) over bar(*) -> J/psi + (pi, rho, K, K*) and also the J/psi absorption cross section in the corresponding inverse processes. Using the obtained cross sections as input to solve the appropriate rate equation, we conclude that the interactions in the hadron gas phase lead to a 20-24% reduction of the J/psi abundance. Within the uncertainties of the calculation, this reduction is the same at the Relativistic Heavy Ion Collider and the large Hadron Collider. |
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Update on J/psi regeneration in a hadron gasIn heavy-ion collisions, after the quark-gluon plasma there is a hadronic gas phase. Using effective Lagrangians, we study the interactions of charmed mesons which lead to J/psi production and absorption in this gas. We update and extend previous calculations introducing strange meson interactions and also including the interactions mediated by the recently measured exotic charmonium resonances Z(3900) and Z(4025). These resonances open new reaction channels for the J/psi, which could potentially lead to changes in its multiplicity. We compute the J/psi production cross section in processes such as D-(s)(*) + (D) over bar(*) -> J/psi + (pi, rho, K, K*) and also the J/psi absorption cross section in the corresponding inverse processes. Using the obtained cross sections as input to solve the appropriate rate equation, we conclude that the interactions in the hadron gas phase lead to a 20-24% reduction of the J/psi abundance. Within the uncertainties of the calculation, this reduction is the same at the Relativistic Heavy Ion Collider and the large Hadron Collider.Univ Fed Bahia, Inst Fis, Campus Univ Ondina, BR-40170115 Salvador, BA, BrazilUniv Fed Sao Paulo, BR-01302907 Sao Paulo, BrazilUniv Sao Paulo, Inst Fis, Rua Matao 1371, BR-05508090 Sao Paulo, SP, BrazilUniv Paris Saclay, CNRS, CEA, Inst Phys Theor, F-91191 Gif Sur Yvette, FranceStanford Univ, SLAC Nacl Acelerator Lab, Stanford, CA 94309 USAUniv Fed Sao Paulo, BR-01302907 Sao Paulo, BrazilWeb of ScienceCNPqFAPESPCNPq: 310759/2016-1CNPq: 311524/2016-8FAPESP: 12/50984-4FAPESP: 17/07278-5Amer Physical Soc2020-07-20T16:31:01Z2020-07-20T16:31:01Z2018info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersion-application/pdfhttp://dx.doi.org/10.1103/PhysRevC.97.044902Physical Review C. College Pk, v. 97, n. 4, p. -, 2018.10.1103/PhysRevC.97.044902WOS000429210800001.pdf2469-9985https://repositorio.unifesp.br/handle/11600/55643WOS:000429210800001engPhysical Review CCollege Pkinfo:eu-repo/semantics/openAccessAbreu, L. M.Khemchandani, Kanchan Pradeepkumar [UNIFESP]Torres, A. MartinezNavarra, F. S.Nielsen, M.reponame:Repositório Institucional da UNIFESPinstname:Universidade Federal de São Paulo (UNIFESP)instacron:UNIFESP2024-08-11T08:04:28Zoai:repositorio.unifesp.br/:11600/55643Repositório InstitucionalPUBhttp://www.repositorio.unifesp.br/oai/requestbiblioteca.csp@unifesp.bropendoar:34652024-08-11T08:04:28Repositório Institucional da UNIFESP - Universidade Federal de São Paulo (UNIFESP)false |
dc.title.none.fl_str_mv |
Update on J/psi regeneration in a hadron gas |
title |
Update on J/psi regeneration in a hadron gas |
spellingShingle |
Update on J/psi regeneration in a hadron gas Abreu, L. M. |
title_short |
Update on J/psi regeneration in a hadron gas |
title_full |
Update on J/psi regeneration in a hadron gas |
title_fullStr |
Update on J/psi regeneration in a hadron gas |
title_full_unstemmed |
Update on J/psi regeneration in a hadron gas |
title_sort |
Update on J/psi regeneration in a hadron gas |
author |
Abreu, L. M. |
author_facet |
Abreu, L. M. Khemchandani, Kanchan Pradeepkumar [UNIFESP] Torres, A. Martinez Navarra, F. S. Nielsen, M. |
author_role |
author |
author2 |
Khemchandani, Kanchan Pradeepkumar [UNIFESP] Torres, A. Martinez Navarra, F. S. Nielsen, M. |
author2_role |
author author author author |
dc.contributor.author.fl_str_mv |
Abreu, L. M. Khemchandani, Kanchan Pradeepkumar [UNIFESP] Torres, A. Martinez Navarra, F. S. Nielsen, M. |
description |
In heavy-ion collisions, after the quark-gluon plasma there is a hadronic gas phase. Using effective Lagrangians, we study the interactions of charmed mesons which lead to J/psi production and absorption in this gas. We update and extend previous calculations introducing strange meson interactions and also including the interactions mediated by the recently measured exotic charmonium resonances Z(3900) and Z(4025). These resonances open new reaction channels for the J/psi, which could potentially lead to changes in its multiplicity. We compute the J/psi production cross section in processes such as D-(s)(*) + (D) over bar(*) -> J/psi + (pi, rho, K, K*) and also the J/psi absorption cross section in the corresponding inverse processes. Using the obtained cross sections as input to solve the appropriate rate equation, we conclude that the interactions in the hadron gas phase lead to a 20-24% reduction of the J/psi abundance. Within the uncertainties of the calculation, this reduction is the same at the Relativistic Heavy Ion Collider and the large Hadron Collider. |
publishDate |
2018 |
dc.date.none.fl_str_mv |
2018 2020-07-20T16:31:01Z 2020-07-20T16:31:01Z |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://dx.doi.org/10.1103/PhysRevC.97.044902 Physical Review C. College Pk, v. 97, n. 4, p. -, 2018. 10.1103/PhysRevC.97.044902 WOS000429210800001.pdf 2469-9985 https://repositorio.unifesp.br/handle/11600/55643 WOS:000429210800001 |
url |
http://dx.doi.org/10.1103/PhysRevC.97.044902 https://repositorio.unifesp.br/handle/11600/55643 |
identifier_str_mv |
Physical Review C. College Pk, v. 97, n. 4, p. -, 2018. 10.1103/PhysRevC.97.044902 WOS000429210800001.pdf 2469-9985 WOS:000429210800001 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Physical Review C |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
- application/pdf |
dc.coverage.none.fl_str_mv |
College Pk |
dc.publisher.none.fl_str_mv |
Amer Physical Soc |
publisher.none.fl_str_mv |
Amer Physical Soc |
dc.source.none.fl_str_mv |
reponame:Repositório Institucional da UNIFESP instname:Universidade Federal de São Paulo (UNIFESP) instacron:UNIFESP |
instname_str |
Universidade Federal de São Paulo (UNIFESP) |
instacron_str |
UNIFESP |
institution |
UNIFESP |
reponame_str |
Repositório Institucional da UNIFESP |
collection |
Repositório Institucional da UNIFESP |
repository.name.fl_str_mv |
Repositório Institucional da UNIFESP - Universidade Federal de São Paulo (UNIFESP) |
repository.mail.fl_str_mv |
biblioteca.csp@unifesp.br |
_version_ |
1814268311072931840 |