Quark mean-field theory and consistency with nuclear matter

Detalhes bibliográficos
Autor(a) principal: Dey, Jishnu [UNESP]
Data de Publicação: 1991
Outros Autores: Tomio, Lauro [UNESP], Dey, Mira, Frederico, T.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1103/PhysRevC.44.2181
http://hdl.handle.net/11449/223822
Resumo: 1/Nc expansion in QCD (with Nc the number of colors) suggests using a potential from meson sector (e.g., Richardson) for baryons. For light quarks a field has to be introduced to ensure chiral symmetry breaking (SB). It is found that nuclear matter properties can be used to pin down the SB modeling. All masses, MN, m, m, are found to scale with density. The equations are solved self-consistently. © 1991 The American Physical Society.
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spelling Quark mean-field theory and consistency with nuclear matter1/Nc expansion in QCD (with Nc the number of colors) suggests using a potential from meson sector (e.g., Richardson) for baryons. For light quarks a field has to be introduced to ensure chiral symmetry breaking (SB). It is found that nuclear matter properties can be used to pin down the SB modeling. All masses, MN, m, m, are found to scale with density. The equations are solved self-consistently. © 1991 The American Physical Society.Instituto de Física Teorica, Universidade Estadual Paulista, Rua Pamplona 145, 01405 Sao PauloDepartment of Physics, Maulana Azad College, Calcutta 700 013Institute for Nuclear Theory, Department of Physics, FM-15, University of Washington, Seattle, WA 98195Instituto de Física Teorica, Universidade Estadual Paulista, Rua Pamplona 145, 01405 Sao PauloUniversidade Estadual Paulista (UNESP)Institute for Nuclear Theory, Department of Physics, FM-15, University of WashingtonDey, Jishnu [UNESP]Tomio, Lauro [UNESP]Dey, MiraFrederico, T.2022-04-28T19:53:17Z2022-04-28T19:53:17Z1991-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article2181-2186http://dx.doi.org/10.1103/PhysRevC.44.2181Physical Review C, v. 44, n. 5, p. 2181-2186, 1991.0556-2813http://hdl.handle.net/11449/22382210.1103/PhysRevC.44.21812-s2.0-0000945060Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review Cinfo:eu-repo/semantics/openAccess2022-04-28T19:53:17Zoai:repositorio.unesp.br:11449/223822Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462022-04-28T19:53:17Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Quark mean-field theory and consistency with nuclear matter
title Quark mean-field theory and consistency with nuclear matter
spellingShingle Quark mean-field theory and consistency with nuclear matter
Dey, Jishnu [UNESP]
title_short Quark mean-field theory and consistency with nuclear matter
title_full Quark mean-field theory and consistency with nuclear matter
title_fullStr Quark mean-field theory and consistency with nuclear matter
title_full_unstemmed Quark mean-field theory and consistency with nuclear matter
title_sort Quark mean-field theory and consistency with nuclear matter
author Dey, Jishnu [UNESP]
author_facet Dey, Jishnu [UNESP]
Tomio, Lauro [UNESP]
Dey, Mira
Frederico, T.
author_role author
author2 Tomio, Lauro [UNESP]
Dey, Mira
Frederico, T.
author2_role author
author
author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (UNESP)
Institute for Nuclear Theory, Department of Physics, FM-15, University of Washington
dc.contributor.author.fl_str_mv Dey, Jishnu [UNESP]
Tomio, Lauro [UNESP]
Dey, Mira
Frederico, T.
description 1/Nc expansion in QCD (with Nc the number of colors) suggests using a potential from meson sector (e.g., Richardson) for baryons. For light quarks a field has to be introduced to ensure chiral symmetry breaking (SB). It is found that nuclear matter properties can be used to pin down the SB modeling. All masses, MN, m, m, are found to scale with density. The equations are solved self-consistently. © 1991 The American Physical Society.
publishDate 1991
dc.date.none.fl_str_mv 1991-01-01
2022-04-28T19:53:17Z
2022-04-28T19:53:17Z
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.44.2181
Physical Review C, v. 44, n. 5, p. 2181-2186, 1991.
0556-2813
http://hdl.handle.net/11449/223822
10.1103/PhysRevC.44.2181
2-s2.0-0000945060
url http://dx.doi.org/10.1103/PhysRevC.44.2181
http://hdl.handle.net/11449/223822
identifier_str_mv Physical Review C, v. 44, n. 5, p. 2181-2186, 1991.
0556-2813
10.1103/PhysRevC.44.2181
2-s2.0-0000945060
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Physical Review C
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 2181-2186
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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