Self-consistent solution of the Schwinger-Dyson equations for the nucleon and meson propagators

Detalhes bibliográficos
Autor(a) principal: Bracco, M. E. [UNESP]
Data de Publicação: 1994
Outros Autores: Eiras, A. [UNESP], Krein, G. [UNESP], Wilets, L.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1103/PhysRevC.49.1299
http://hdl.handle.net/11449/223839
Resumo: The Schwinger-Dyson equations for the nucleon and meson propagators are solved self-consistently in an approximation that goes beyond the Hartree-Fock approximation. The traditional approach consists in solving the nucleon Schwinger-Dyson equation with bare meson propagators and bare meson-nucleon vertices; the corrections to the meson propagators are calculated using the bare nucleon propagator and bare nucleon-meson vertices. It is known that such an approximation scheme produces the appearance of ghost poles in the propagators. In this paper the coupled system of Schwinger-Dyson equations for the nucleon and the meson propagators are solved self-consistently including vertex corrections. The interplay of self-consistency and vertex corrections on the ghosts problem is investigated. It is found that the self-consistency does not affect significantly the spectral properties of the propagators. In particular, it does not affect the appearance of the ghost poles in the propagators. © 1994 The American Physical Society.
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spelling Self-consistent solution of the Schwinger-Dyson equations for the nucleon and meson propagatorsThe Schwinger-Dyson equations for the nucleon and meson propagators are solved self-consistently in an approximation that goes beyond the Hartree-Fock approximation. The traditional approach consists in solving the nucleon Schwinger-Dyson equation with bare meson propagators and bare meson-nucleon vertices; the corrections to the meson propagators are calculated using the bare nucleon propagator and bare nucleon-meson vertices. It is known that such an approximation scheme produces the appearance of ghost poles in the propagators. In this paper the coupled system of Schwinger-Dyson equations for the nucleon and the meson propagators are solved self-consistently including vertex corrections. The interplay of self-consistency and vertex corrections on the ghosts problem is investigated. It is found that the self-consistency does not affect significantly the spectral properties of the propagators. In particular, it does not affect the appearance of the ghost poles in the propagators. © 1994 The American Physical Society.Instituto de Física Teórica, Universidade Estadual Paulista, Rua Pamplona, 145-01405-900 Sao Paulo, SPDepartment of Physics, FM-15, University of Washington, Seattle, WA 98195Instituto de Física Teórica, Universidade Estadual Paulista, Rua Pamplona, 145-01405-900 Sao Paulo, SPUniversidade Estadual Paulista (UNESP)Bracco, M. E. [UNESP]Eiras, A. [UNESP]Krein, G. [UNESP]Wilets, L.2022-04-28T19:53:21Z2022-04-28T19:53:21Z1994-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article1299-1308http://dx.doi.org/10.1103/PhysRevC.49.1299Physical Review C, v. 49, n. 3, p. 1299-1308, 1994.0556-2813http://hdl.handle.net/11449/22383910.1103/PhysRevC.49.12992-s2.0-0001602493Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review Cinfo:eu-repo/semantics/openAccess2022-04-28T19:53:21Zoai:repositorio.unesp.br:11449/223839Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-06T00:11:42.698691Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Self-consistent solution of the Schwinger-Dyson equations for the nucleon and meson propagators
title Self-consistent solution of the Schwinger-Dyson equations for the nucleon and meson propagators
spellingShingle Self-consistent solution of the Schwinger-Dyson equations for the nucleon and meson propagators
Bracco, M. E. [UNESP]
title_short Self-consistent solution of the Schwinger-Dyson equations for the nucleon and meson propagators
title_full Self-consistent solution of the Schwinger-Dyson equations for the nucleon and meson propagators
title_fullStr Self-consistent solution of the Schwinger-Dyson equations for the nucleon and meson propagators
title_full_unstemmed Self-consistent solution of the Schwinger-Dyson equations for the nucleon and meson propagators
title_sort Self-consistent solution of the Schwinger-Dyson equations for the nucleon and meson propagators
author Bracco, M. E. [UNESP]
author_facet Bracco, M. E. [UNESP]
Eiras, A. [UNESP]
Krein, G. [UNESP]
Wilets, L.
author_role author
author2 Eiras, A. [UNESP]
Krein, G. [UNESP]
Wilets, L.
author2_role author
author
author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (UNESP)
dc.contributor.author.fl_str_mv Bracco, M. E. [UNESP]
Eiras, A. [UNESP]
Krein, G. [UNESP]
Wilets, L.
description The Schwinger-Dyson equations for the nucleon and meson propagators are solved self-consistently in an approximation that goes beyond the Hartree-Fock approximation. The traditional approach consists in solving the nucleon Schwinger-Dyson equation with bare meson propagators and bare meson-nucleon vertices; the corrections to the meson propagators are calculated using the bare nucleon propagator and bare nucleon-meson vertices. It is known that such an approximation scheme produces the appearance of ghost poles in the propagators. In this paper the coupled system of Schwinger-Dyson equations for the nucleon and the meson propagators are solved self-consistently including vertex corrections. The interplay of self-consistency and vertex corrections on the ghosts problem is investigated. It is found that the self-consistency does not affect significantly the spectral properties of the propagators. In particular, it does not affect the appearance of the ghost poles in the propagators. © 1994 The American Physical Society.
publishDate 1994
dc.date.none.fl_str_mv 1994-01-01
2022-04-28T19:53:21Z
2022-04-28T19:53:21Z
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.49.1299
Physical Review C, v. 49, n. 3, p. 1299-1308, 1994.
0556-2813
http://hdl.handle.net/11449/223839
10.1103/PhysRevC.49.1299
2-s2.0-0001602493
url http://dx.doi.org/10.1103/PhysRevC.49.1299
http://hdl.handle.net/11449/223839
identifier_str_mv Physical Review C, v. 49, n. 3, p. 1299-1308, 1994.
0556-2813
10.1103/PhysRevC.49.1299
2-s2.0-0001602493
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 1299-1308
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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