Phi-meson-nucleus bound states
Autor(a) principal: | |
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Data de Publicação: | 2017 |
Outros Autores: | , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1103/PhysRevC.96.035201 http://hdl.handle.net/11449/163179 |
Resumo: | Phi-meson-nucleus bound state energies and absorption widths are calculated for seven selected nuclei by solving the Klein-Gordon equation with complex optical potentials. Essential input for the calculations, namely the medium-modified K and K meson masses, as well as the density distributions in nuclei, are obtained from the quark-meson coupling model. The attractive potential for the Phi meson in the nuclear medium originates from the in-medium enhanced K (K) over bar loop in the Phi-meson self-energy. The results suggest that the Phi meson should form bound states with all the nuclei considered. However, the identification of the signal for these predicted bound states will need careful investigation because of their sizable absorption widths. |
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Phi-meson-nucleus bound statesPhi-meson-nucleus bound state energies and absorption widths are calculated for seven selected nuclei by solving the Klein-Gordon equation with complex optical potentials. Essential input for the calculations, namely the medium-modified K and K meson masses, as well as the density distributions in nuclei, are obtained from the quark-meson coupling model. The attractive potential for the Phi meson in the nuclear medium originates from the in-medium enhanced K (K) over bar loop in the Phi-meson self-energy. The results suggest that the Phi meson should form bound states with all the nuclei considered. However, the identification of the signal for these predicted bound states will need careful investigation because of their sizable absorption widths.Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)University of AdelaideAustralian Research Council (ARC) through the Centre of Excellence for Particle Physics at the TerascaleUniv Cruzeiro Sul, LFTC, BR-01506000 Sao Paulo, SP, BrazilInst Politecn Nacl, Ctr Invest & Estudios Avanzados, Dept Fas, Catedra CONACyT, Apartado Postal 14-740, Mexico City 07000, DF, MexicoUniv Michoacana San Nicola Hidalgo, Inst Fis & Matemat, Edificio C 3, Morelia 58040, Michoacan, MexicoUniv Estadual Paulista, Inst Fis Teor, Rua Dr Bento Teobaldo Ferraz,271-Bloco II, BR-01140070 Sao Paulo, SP, BrazilUniv Adelaide, Dept Phys, ARC Ctr Excellence Particle Phys Terascale & CSS, Adelaide, SA 5005, AustraliaUniv Estadual Paulista, Inst Fis Teor, Rua Dr Bento Teobaldo Ferraz,271-Bloco II, BR-01140070 Sao Paulo, SP, BrazilCNPq: 152348/2016-6CNPq: 400826/2014-3CNPq: 308088/2015-8CNPq: 305894/2009-9CNPq: 313800/2014-6FAPESP: 2015/17234-0FAPESP: 2013/01907-0Australian Research Council (ARC) through the Centre of Excellence for Particle Physics at the Terascale: CE110001104Australian Research Council (ARC) through the Centre of Excellence for Particle Physics at the Terascale: DP151103101Amer Physical SocUniv Cruzeiro SulInst Politecn NaclUniv Michoacana San Nicola HidalgoUniversidade Estadual Paulista (Unesp)Univ AdelaideCobos-Martinez, J. J.Tsushima, K.Krein, G. [UNESP]Thomas, A. W.2018-11-26T17:40:24Z2018-11-26T17:40:24Z2017-09-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article8application/pdfhttp://dx.doi.org/10.1103/PhysRevC.96.035201Physical Review C. College Pk: Amer Physical Soc, v. 96, n. 3, 8 p., 2017.2469-9985http://hdl.handle.net/11449/16317910.1103/PhysRevC.96.035201WOS:000408827900006WOS000408827900006.pdfWeb of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review C1,443info:eu-repo/semantics/openAccess2023-10-23T06:08:57Zoai:repositorio.unesp.br:11449/163179Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462023-10-23T06:08:57Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Phi-meson-nucleus bound states |
title |
Phi-meson-nucleus bound states |
spellingShingle |
Phi-meson-nucleus bound states Cobos-Martinez, J. J. |
title_short |
Phi-meson-nucleus bound states |
title_full |
Phi-meson-nucleus bound states |
title_fullStr |
Phi-meson-nucleus bound states |
title_full_unstemmed |
Phi-meson-nucleus bound states |
title_sort |
Phi-meson-nucleus bound states |
author |
Cobos-Martinez, J. J. |
author_facet |
Cobos-Martinez, J. J. Tsushima, K. Krein, G. [UNESP] Thomas, A. W. |
author_role |
author |
author2 |
Tsushima, K. Krein, G. [UNESP] Thomas, A. W. |
author2_role |
author author author |
dc.contributor.none.fl_str_mv |
Univ Cruzeiro Sul Inst Politecn Nacl Univ Michoacana San Nicola Hidalgo Universidade Estadual Paulista (Unesp) Univ Adelaide |
dc.contributor.author.fl_str_mv |
Cobos-Martinez, J. J. Tsushima, K. Krein, G. [UNESP] Thomas, A. W. |
description |
Phi-meson-nucleus bound state energies and absorption widths are calculated for seven selected nuclei by solving the Klein-Gordon equation with complex optical potentials. Essential input for the calculations, namely the medium-modified K and K meson masses, as well as the density distributions in nuclei, are obtained from the quark-meson coupling model. The attractive potential for the Phi meson in the nuclear medium originates from the in-medium enhanced K (K) over bar loop in the Phi-meson self-energy. The results suggest that the Phi meson should form bound states with all the nuclei considered. However, the identification of the signal for these predicted bound states will need careful investigation because of their sizable absorption widths. |
publishDate |
2017 |
dc.date.none.fl_str_mv |
2017-09-01 2018-11-26T17:40:24Z 2018-11-26T17:40:24Z |
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/PhysRevC.96.035201 Physical Review C. College Pk: Amer Physical Soc, v. 96, n. 3, 8 p., 2017. 2469-9985 http://hdl.handle.net/11449/163179 10.1103/PhysRevC.96.035201 WOS:000408827900006 WOS000408827900006.pdf |
url |
http://dx.doi.org/10.1103/PhysRevC.96.035201 http://hdl.handle.net/11449/163179 |
identifier_str_mv |
Physical Review C. College Pk: Amer Physical Soc, v. 96, n. 3, 8 p., 2017. 2469-9985 10.1103/PhysRevC.96.035201 WOS:000408827900006 WOS000408827900006.pdf |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Physical Review C 1,443 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
8 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 |
|
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1797789486858371072 |