Self-consistent solution of the Schwinger-Dyson equations for the nucleon and meson propagators
Autor(a) principal: | |
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Data de Publicação: | 1994 |
Outros Autores: | , , |
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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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 |
|
_version_ |
1808129594003292160 |