QCD sum rules for the Delta isobar in neutron matter
Autor(a) principal: | |
---|---|
Data de Publicação: | 2018 |
Outros Autores: | , , , |
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. |
id |
UNSP_6579662d590a32a6ffaa3912b834a6bc |
---|---|
oai_identifier_str |
oai:repositorio.unesp.br:11449/164556 |
network_acronym_str |
UNSP |
network_name_str |
Repositório Institucional da UNESP |
repository_id_str |
2946 |
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) |
repository.mail.fl_str_mv |
|
_version_ |
1808128392260747264 |