QCD sum rules for the Delta isobar in neutron matter

Detalhes bibliográficos
Autor(a) principal: Marques L, Jesuel [UNESP]
Data de Publicação: 2018
Outros Autores: Lee, Su Houng, Park, Aaron, Matheus, R. D. [UNESP], Jeong, Kie Sang
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1103/PhysRevC.98.025206
http://hdl.handle.net/11449/164556
Resumo: We study the properties of the Delta isobar in the symmetric and asymmetric nuclear matter using the QCD sum rules approach based on the energy dispersion relation. Allowing for different continuum thresholds for the polarization tensors with different dimensions, we find stable masses for the Delta in both the vacuum and the medium. Compared to the nucleon case, we find that the vector repulsion is smaller for the Delta while the scalar attraction is similar (75 MeV vector repulsion and 200 MeV scalar attraction in the symmetric matter). The smaller vector repulsion can be understood using the Pauli principle and a constituent quark model. Also, the isospin dependence of the quasiparticle energy, which mainly comes from the vector self-energy, is quite weak. We also allow for an explicit pi - N continuum contribution to the polarization function but find its effect to be minimal Phenomenological consequences of our results are discussed.
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spelling QCD sum rules for the Delta isobar in neutron matterWe study the properties of the Delta isobar in the symmetric and asymmetric nuclear matter using the QCD sum rules approach based on the energy dispersion relation. Allowing for different continuum thresholds for the polarization tensors with different dimensions, we find stable masses for the Delta in both the vacuum and the medium. Compared to the nucleon case, we find that the vector repulsion is smaller for the Delta while the scalar attraction is similar (75 MeV vector repulsion and 200 MeV scalar attraction in the symmetric matter). The smaller vector repulsion can be understood using the Pauli principle and a constituent quark model. Also, the isospin dependence of the quasiparticle energy, which mainly comes from the vector self-energy, is quite weak. We also allow for an explicit pi - N continuum contribution to the polarization function but find its effect to be minimal Phenomenological consequences of our results are discussed.Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Korea National Research Foundation GrantsUniv Estadual Paulista, Inst Fis Teor, BR-01140070 Sao Paulo, BrazilYonsei Univ, Dept Phys, Seoul 03722, South KoreaYonsei Univ, Inst Phys & Appl Phys, Seoul 03722, South KoreaAsia Pacific Ctr Theoret Phys, Pohang 37673, Gyeongbuk, South KoreaUniv Estadual Paulista, Inst Fis Teor, BR-01140070 Sao Paulo, BrazilFAPESP: 2017/15346-0FAPESP: 2016/02717-8Korea National Research Foundation Grants: NRF-2016R1D1A1B03930089Korea National Research Foundation Grants: NRF-2018R1D1A1B07043234Korea National Research Foundation Grants: NRF-2017R1D1A1B03033685Amer Physical SocUniversidade Estadual Paulista (Unesp)Yonsei UnivAsia Pacific Ctr Theoret PhysMarques L, Jesuel [UNESP]Lee, Su HoungPark, AaronMatheus, R. D. [UNESP]Jeong, Kie Sang2018-11-26T17:55:01Z2018-11-26T17:55:01Z2018-08-22info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article14application/pdfhttp://dx.doi.org/10.1103/PhysRevC.98.025206Physical Review C. College Pk: Amer Physical Soc, v. 98, n. 2, 14 p., 2018.2469-9985http://hdl.handle.net/11449/16455610.1103/PhysRevC.98.025206WOS:000442475700008WOS000442475700008.pdf08456584624967150000-0003-2132-8251Web of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review C1,443info:eu-repo/semantics/openAccess2023-10-11T06:08:41Zoai:repositorio.unesp.br:11449/164556Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T14:38:13.644714Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv QCD sum rules for the Delta isobar in neutron matter
title QCD sum rules for the Delta isobar in neutron matter
spellingShingle QCD sum rules for the Delta isobar in neutron matter
Marques L, Jesuel [UNESP]
title_short QCD sum rules for the Delta isobar in neutron matter
title_full QCD sum rules for the Delta isobar in neutron matter
title_fullStr QCD sum rules for the Delta isobar in neutron matter
title_full_unstemmed QCD sum rules for the Delta isobar in neutron matter
title_sort QCD sum rules for the Delta isobar in neutron matter
author Marques L, Jesuel [UNESP]
author_facet Marques L, Jesuel [UNESP]
Lee, Su Houng
Park, Aaron
Matheus, R. D. [UNESP]
Jeong, Kie Sang
author_role author
author2 Lee, Su Houng
Park, Aaron
Matheus, R. D. [UNESP]
Jeong, Kie Sang
author2_role author
author
author
author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (Unesp)
Yonsei Univ
Asia Pacific Ctr Theoret Phys
dc.contributor.author.fl_str_mv Marques L, Jesuel [UNESP]
Lee, Su Houng
Park, Aaron
Matheus, R. D. [UNESP]
Jeong, Kie Sang
description We study the properties of the Delta isobar in the symmetric and asymmetric nuclear matter using the QCD sum rules approach based on the energy dispersion relation. Allowing for different continuum thresholds for the polarization tensors with different dimensions, we find stable masses for the Delta in both the vacuum and the medium. Compared to the nucleon case, we find that the vector repulsion is smaller for the Delta while the scalar attraction is similar (75 MeV vector repulsion and 200 MeV scalar attraction in the symmetric matter). The smaller vector repulsion can be understood using the Pauli principle and a constituent quark model. Also, the isospin dependence of the quasiparticle energy, which mainly comes from the vector self-energy, is quite weak. We also allow for an explicit pi - N continuum contribution to the polarization function but find its effect to be minimal Phenomenological consequences of our results are discussed.
publishDate 2018
dc.date.none.fl_str_mv 2018-11-26T17:55:01Z
2018-11-26T17:55:01Z
2018-08-22
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.98.025206
Physical Review C. College Pk: Amer Physical Soc, v. 98, n. 2, 14 p., 2018.
2469-9985
http://hdl.handle.net/11449/164556
10.1103/PhysRevC.98.025206
WOS:000442475700008
WOS000442475700008.pdf
0845658462496715
0000-0003-2132-8251
url http://dx.doi.org/10.1103/PhysRevC.98.025206
http://hdl.handle.net/11449/164556
identifier_str_mv Physical Review C. College Pk: Amer Physical Soc, v. 98, n. 2, 14 p., 2018.
2469-9985
10.1103/PhysRevC.98.025206
WOS:000442475700008
WOS000442475700008.pdf
0845658462496715
0000-0003-2132-8251
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 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)
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