η→γγ Decay width via the Primakoff cross section

Detalhes bibliográficos
Autor(a) principal: Rodrigues, T. E.
Data de Publicação: 2008
Outros Autores: Arruda-Neto, J. D.T., Mesa, J. [UNESP], Garcia, C., Shtejer, K., Dale, D., Nakagawa, I., Cole, P. L.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1103/PhysRevLett.101.012301
http://hdl.handle.net/11449/225216
Resumo: Incoherent η photoproduction in nuclei is evaluated at forward angles within 4 to 9GeV using a multiple scattering MonteCarlo cascade calculation with full η-nucleus final-state interactions. The Primakoff, nuclear coherent and nuclear incoherent components of the cross sections fit remarkably well previous measurements for Be and Cu from Cornell, suggesting a destructive interference between the Coulomb and nuclear coherent amplitudes for Cu. The inelastic background of the data is consistently attributed to the nuclear incoherent part, which is clearly not isotropic as previously considered in Cornell's analysis. The respective Primakoff cross sections from Be and Cu give Γη→γγ=0.476(62)keV, where the quoted error is only statistical. This result is consistent with the Particle Data Group average of 0.510(26)keV and in sharp contrast (∼50%) with the value of 0.324(46)keV obtained at Cornell. © 2008 The American Physical Society.
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spelling η→γγ Decay width via the Primakoff cross sectionIncoherent η photoproduction in nuclei is evaluated at forward angles within 4 to 9GeV using a multiple scattering MonteCarlo cascade calculation with full η-nucleus final-state interactions. The Primakoff, nuclear coherent and nuclear incoherent components of the cross sections fit remarkably well previous measurements for Be and Cu from Cornell, suggesting a destructive interference between the Coulomb and nuclear coherent amplitudes for Cu. The inelastic background of the data is consistently attributed to the nuclear incoherent part, which is clearly not isotropic as previously considered in Cornell's analysis. The respective Primakoff cross sections from Be and Cu give Γη→γγ=0.476(62)keV, where the quoted error is only statistical. This result is consistent with the Particle Data Group average of 0.510(26)keV and in sharp contrast (∼50%) with the value of 0.324(46)keV obtained at Cornell. © 2008 The American Physical Society.Physics Institute University of São Paulo, P. O. Box 66318, CEP 05315-970, São PauloFESP-São Paulo Engineering College, São Paulo, 66318Department of Physics and Biophysics UNESP, Botucatu, 66318Center of Applied Studies for Nuclear Developments (CEADEN), Havana, 66318Department of Physics Idaho State University, Pocatello, ID 83209RIKEN, 2-1 Hirosawa, Wako, Saitama 351-0198Department of Physics and Biophysics UNESP, Botucatu, 66318Universidade de São Paulo (USP)FESP-São Paulo Engineering CollegeUniversidade Estadual Paulista (UNESP)Center of Applied Studies for Nuclear Developments (CEADEN)Idaho State UniversityRIKENRodrigues, T. E.Arruda-Neto, J. D.T.Mesa, J. [UNESP]Garcia, C.Shtejer, K.Dale, D.Nakagawa, I.Cole, P. L.2022-04-28T20:42:16Z2022-04-28T20:42:16Z2008-07-03info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevLett.101.012301Physical Review Letters, v. 101, n. 1, 2008.0031-90071079-7114http://hdl.handle.net/11449/22521610.1103/PhysRevLett.101.0123012-s2.0-46949111181Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review Lettersinfo:eu-repo/semantics/openAccess2022-04-28T20:42:17Zoai:repositorio.unesp.br:11449/225216Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T20:46:10.732118Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv η→γγ Decay width via the Primakoff cross section
title η→γγ Decay width via the Primakoff cross section
spellingShingle η→γγ Decay width via the Primakoff cross section
Rodrigues, T. E.
title_short η→γγ Decay width via the Primakoff cross section
title_full η→γγ Decay width via the Primakoff cross section
title_fullStr η→γγ Decay width via the Primakoff cross section
title_full_unstemmed η→γγ Decay width via the Primakoff cross section
title_sort η→γγ Decay width via the Primakoff cross section
author Rodrigues, T. E.
author_facet Rodrigues, T. E.
Arruda-Neto, J. D.T.
Mesa, J. [UNESP]
Garcia, C.
Shtejer, K.
Dale, D.
Nakagawa, I.
Cole, P. L.
author_role author
author2 Arruda-Neto, J. D.T.
Mesa, J. [UNESP]
Garcia, C.
Shtejer, K.
Dale, D.
Nakagawa, I.
Cole, P. L.
author2_role author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv Universidade de São Paulo (USP)
FESP-São Paulo Engineering College
Universidade Estadual Paulista (UNESP)
Center of Applied Studies for Nuclear Developments (CEADEN)
Idaho State University
RIKEN
dc.contributor.author.fl_str_mv Rodrigues, T. E.
Arruda-Neto, J. D.T.
Mesa, J. [UNESP]
Garcia, C.
Shtejer, K.
Dale, D.
Nakagawa, I.
Cole, P. L.
description Incoherent η photoproduction in nuclei is evaluated at forward angles within 4 to 9GeV using a multiple scattering MonteCarlo cascade calculation with full η-nucleus final-state interactions. The Primakoff, nuclear coherent and nuclear incoherent components of the cross sections fit remarkably well previous measurements for Be and Cu from Cornell, suggesting a destructive interference between the Coulomb and nuclear coherent amplitudes for Cu. The inelastic background of the data is consistently attributed to the nuclear incoherent part, which is clearly not isotropic as previously considered in Cornell's analysis. The respective Primakoff cross sections from Be and Cu give Γη→γγ=0.476(62)keV, where the quoted error is only statistical. This result is consistent with the Particle Data Group average of 0.510(26)keV and in sharp contrast (∼50%) with the value of 0.324(46)keV obtained at Cornell. © 2008 The American Physical Society.
publishDate 2008
dc.date.none.fl_str_mv 2008-07-03
2022-04-28T20:42:16Z
2022-04-28T20:42:16Z
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/PhysRevLett.101.012301
Physical Review Letters, v. 101, n. 1, 2008.
0031-9007
1079-7114
http://hdl.handle.net/11449/225216
10.1103/PhysRevLett.101.012301
2-s2.0-46949111181
url http://dx.doi.org/10.1103/PhysRevLett.101.012301
http://hdl.handle.net/11449/225216
identifier_str_mv Physical Review Letters, v. 101, n. 1, 2008.
0031-9007
1079-7114
10.1103/PhysRevLett.101.012301
2-s2.0-46949111181
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Physical Review Letters
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.source.none.fl_str_mv Scopus
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
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