Production of charmed baryons in (p)over-barp collisions close to their thresholds
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Publication Date: | 2017 |
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Format: | Article |
Language: | eng |
Source: | Repositório Institucional da UNESP |
Download full: | http://dx.doi.org/10.1103/PhysRevD.95.014017 http://hdl.handle.net/11449/162344 |
Summary: | Cross sections for the charm-production reactions (p) over barp -> (Lambda) over bar (-)(c)Sigma(+)(c),(Sigma) over bar (c)Sigma(c), (Xi) over tilde (c)Xi(c,)and (Xi) over tilde (c)'Xi(c)' are presented, for energies near their respective thresholds. The results are based on a calculation performed in the meson-exchange framework in close analogy to earlier studies of the Julich group on the strangeness-production reactions (p) over barp -> (Lambda) over bar Sigma, (Sigma) over bar Sigma, (Xi) over tilde Xi by connecting the two sectors via SU( 4) flavor symmetry. The cross sections are found to be in the order of 0.1-1 mu b at energies of 100 MeV above the respective thresholds, for all considered channels. Complementary to meson exchange, where the charmed baryons are produced by the exchange of D and D* mesons, a charm-production potential derived in a quark model is employed for assessing uncertainties. The cross sections predicted within that picture turn out to be significantly smaller. |
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Production of charmed baryons in (p)over-barp collisions close to their thresholdsCross sections for the charm-production reactions (p) over barp -> (Lambda) over bar (-)(c)Sigma(+)(c),(Sigma) over bar (c)Sigma(c), (Xi) over tilde (c)Xi(c,)and (Xi) over tilde (c)'Xi(c)' are presented, for energies near their respective thresholds. The results are based on a calculation performed in the meson-exchange framework in close analogy to earlier studies of the Julich group on the strangeness-production reactions (p) over barp -> (Lambda) over bar Sigma, (Sigma) over bar Sigma, (Xi) over tilde Xi by connecting the two sectors via SU( 4) flavor symmetry. The cross sections are found to be in the order of 0.1-1 mu b at energies of 100 MeV above the respective thresholds, for all considered channels. Complementary to meson exchange, where the charmed baryons are produced by the exchange of D and D* mesons, a charm-production potential derived in a quark model is employed for assessing uncertainties. The cross sections predicted within that picture turn out to be significantly smaller.Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Forschungszentrum Julich, Inst Kernphys, Inst Adv Simulat, D-52425 Julich, GermanyForschungszentrum Julich, Julich Ctr Hadron Phys, D-52425 Julich, GermanyUniv Estadual Paulista, Inst Fis Teor, Rua Dr Bento Teobaldo Ferraz 271,Bloco 2, BR-01140070 Sao Paulo, SP, BrazilUniv Estadual Paulista, Inst Fis Teor, Rua Dr Bento Teobaldo Ferraz 271,Bloco 2, BR-01140070 Sao Paulo, SP, BrazilCNPq: 305894/2009-9FAPESP: 2013/01907-0Amer Physical SocForschungszentrum JulichUniversidade Estadual Paulista (Unesp)Haidenbauer, J.Krein, G. [UNESP]2018-11-26T17:15:42Z2018-11-26T17:15:42Z2017-01-18info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article14application/pdfhttp://dx.doi.org/10.1103/PhysRevD.95.014017Physical Review D. College Pk: Amer Physical Soc, v. 95, n. 1, 14 p., 2017.2470-0010http://hdl.handle.net/11449/16234410.1103/PhysRevD.95.014017WOS:000392078600001WOS000392078600001.pdfWeb of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review D1,801info:eu-repo/semantics/openAccess2024-11-22T19:49:31Zoai:repositorio.unesp.br:11449/162344Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestrepositoriounesp@unesp.bropendoar:29462024-11-22T19:49:31Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Production of charmed baryons in (p)over-barp collisions close to their thresholds |
title |
Production of charmed baryons in (p)over-barp collisions close to their thresholds |
spellingShingle |
Production of charmed baryons in (p)over-barp collisions close to their thresholds Haidenbauer, J. |
title_short |
Production of charmed baryons in (p)over-barp collisions close to their thresholds |
title_full |
Production of charmed baryons in (p)over-barp collisions close to their thresholds |
title_fullStr |
Production of charmed baryons in (p)over-barp collisions close to their thresholds |
title_full_unstemmed |
Production of charmed baryons in (p)over-barp collisions close to their thresholds |
title_sort |
Production of charmed baryons in (p)over-barp collisions close to their thresholds |
author |
Haidenbauer, J. |
author_facet |
Haidenbauer, J. Krein, G. [UNESP] |
author_role |
author |
author2 |
Krein, G. [UNESP] |
author2_role |
author |
dc.contributor.none.fl_str_mv |
Forschungszentrum Julich Universidade Estadual Paulista (Unesp) |
dc.contributor.author.fl_str_mv |
Haidenbauer, J. Krein, G. [UNESP] |
description |
Cross sections for the charm-production reactions (p) over barp -> (Lambda) over bar (-)(c)Sigma(+)(c),(Sigma) over bar (c)Sigma(c), (Xi) over tilde (c)Xi(c,)and (Xi) over tilde (c)'Xi(c)' are presented, for energies near their respective thresholds. The results are based on a calculation performed in the meson-exchange framework in close analogy to earlier studies of the Julich group on the strangeness-production reactions (p) over barp -> (Lambda) over bar Sigma, (Sigma) over bar Sigma, (Xi) over tilde Xi by connecting the two sectors via SU( 4) flavor symmetry. The cross sections are found to be in the order of 0.1-1 mu b at energies of 100 MeV above the respective thresholds, for all considered channels. Complementary to meson exchange, where the charmed baryons are produced by the exchange of D and D* mesons, a charm-production potential derived in a quark model is employed for assessing uncertainties. The cross sections predicted within that picture turn out to be significantly smaller. |
publishDate |
2017 |
dc.date.none.fl_str_mv |
2017-01-18 2018-11-26T17:15:42Z 2018-11-26T17:15:42Z |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://dx.doi.org/10.1103/PhysRevD.95.014017 Physical Review D. College Pk: Amer Physical Soc, v. 95, n. 1, 14 p., 2017. 2470-0010 http://hdl.handle.net/11449/162344 10.1103/PhysRevD.95.014017 WOS:000392078600001 WOS000392078600001.pdf |
url |
http://dx.doi.org/10.1103/PhysRevD.95.014017 http://hdl.handle.net/11449/162344 |
identifier_str_mv |
Physical Review D. College Pk: Amer Physical Soc, v. 95, n. 1, 14 p., 2017. 2470-0010 10.1103/PhysRevD.95.014017 WOS:000392078600001 WOS000392078600001.pdf |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Physical Review D 1,801 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
14 application/pdf |
dc.publisher.none.fl_str_mv |
Amer Physical Soc |
publisher.none.fl_str_mv |
Amer Physical Soc |
dc.source.none.fl_str_mv |
Web of Science reponame:Repositório Institucional da UNESP instname:Universidade Estadual Paulista (UNESP) instacron:UNESP |
instname_str |
Universidade Estadual Paulista (UNESP) |
instacron_str |
UNESP |
institution |
UNESP |
reponame_str |
Repositório Institucional da UNESP |
collection |
Repositório Institucional da UNESP |
repository.name.fl_str_mv |
Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP) |
repository.mail.fl_str_mv |
repositoriounesp@unesp.br |
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1834483214860681216 |