Symmetry energy and the Pauli exclusion principle

Autores
Dorso, Claudio Oscar; Frank, Guillermo Alberto; Lopez, Jorge A.
Año de publicación
2021
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
In this article we present a classical potential that respects the Pauli exclusion principle and can be used to describe nucleon-nucleon interactions at intermediate energies. The potential depends on the relative momentum of the colliding nucleons and reduces interactions at low momentum transfer mimicking the Pauli exclusion principle. We use the potential with Metropolis Monte Carlo methods and study the formation of finite nuclei and infinite systems. We find good agreement in terms of the binding energies, radii, and internal nucleon distribution of finite nuclei, and the binding energy in nuclear matter and neutron star matter, as well as the formation of nuclear pastas, and the symmetry energy of neutron star matter.
Fil: Dorso, Claudio Oscar. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina
Fil: Frank, Guillermo Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Tecnológica Nacional. Facultad Regional Buenos Aires. Unidad de Investigación y Desarrollo de las Ingenierías; Argentina
Fil: Lopez, Jorge A.. University of Texas at El Paso; Estados Unidos
Materia
NEUTRON STAR MATTER
NUCLEAR MATTER
NUCLEAR PASTA
NUCLEAR SYMMETRY ENERGY
NUCLEON-NUCLEON INTERACTIONS
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/166706
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/166706
network_acronym_str CONICETDig
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network_name_str CONICET Digital (CONICET)
spelling Symmetry energy and the Pauli exclusion principleDorso, Claudio OscarFrank, Guillermo AlbertoLopez, Jorge A.NEUTRON STAR MATTERNUCLEAR MATTERNUCLEAR PASTANUCLEAR SYMMETRY ENERGYNUCLEON-NUCLEON INTERACTIONShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1In this article we present a classical potential that respects the Pauli exclusion principle and can be used to describe nucleon-nucleon interactions at intermediate energies. The potential depends on the relative momentum of the colliding nucleons and reduces interactions at low momentum transfer mimicking the Pauli exclusion principle. We use the potential with Metropolis Monte Carlo methods and study the formation of finite nuclei and infinite systems. We find good agreement in terms of the binding energies, radii, and internal nucleon distribution of finite nuclei, and the binding energy in nuclear matter and neutron star matter, as well as the formation of nuclear pastas, and the symmetry energy of neutron star matter.Fil: Dorso, Claudio Oscar. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; ArgentinaFil: Frank, Guillermo Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Tecnológica Nacional. Facultad Regional Buenos Aires. Unidad de Investigación y Desarrollo de las Ingenierías; ArgentinaFil: Lopez, Jorge A.. University of Texas at El Paso; Estados UnidosMultidisciplinary Digital Publishing Institute2021-11info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/166706Dorso, Claudio Oscar; Frank, Guillermo Alberto; Lopez, Jorge A.; Symmetry energy and the Pauli exclusion principle; Multidisciplinary Digital Publishing Institute; Symmetry; 13; 11; 11-2021; 1-202073-8994CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.mdpi.com/2073-8994/13/11/2116info:eu-repo/semantics/altIdentifier/doi/10.3390/sym13112116info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:40:50Zoai:ri.conicet.gov.ar:11336/166706instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:40:50.939CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Symmetry energy and the Pauli exclusion principle
title Symmetry energy and the Pauli exclusion principle
spellingShingle Symmetry energy and the Pauli exclusion principle
Dorso, Claudio Oscar
NEUTRON STAR MATTER
NUCLEAR MATTER
NUCLEAR PASTA
NUCLEAR SYMMETRY ENERGY
NUCLEON-NUCLEON INTERACTIONS
title_short Symmetry energy and the Pauli exclusion principle
title_full Symmetry energy and the Pauli exclusion principle
title_fullStr Symmetry energy and the Pauli exclusion principle
title_full_unstemmed Symmetry energy and the Pauli exclusion principle
title_sort Symmetry energy and the Pauli exclusion principle
dc.creator.none.fl_str_mv Dorso, Claudio Oscar
Frank, Guillermo Alberto
Lopez, Jorge A.
author Dorso, Claudio Oscar
author_facet Dorso, Claudio Oscar
Frank, Guillermo Alberto
Lopez, Jorge A.
author_role author
author2 Frank, Guillermo Alberto
Lopez, Jorge A.
author2_role author
author
dc.subject.none.fl_str_mv NEUTRON STAR MATTER
NUCLEAR MATTER
NUCLEAR PASTA
NUCLEAR SYMMETRY ENERGY
NUCLEON-NUCLEON INTERACTIONS
topic NEUTRON STAR MATTER
NUCLEAR MATTER
NUCLEAR PASTA
NUCLEAR SYMMETRY ENERGY
NUCLEON-NUCLEON INTERACTIONS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv In this article we present a classical potential that respects the Pauli exclusion principle and can be used to describe nucleon-nucleon interactions at intermediate energies. The potential depends on the relative momentum of the colliding nucleons and reduces interactions at low momentum transfer mimicking the Pauli exclusion principle. We use the potential with Metropolis Monte Carlo methods and study the formation of finite nuclei and infinite systems. We find good agreement in terms of the binding energies, radii, and internal nucleon distribution of finite nuclei, and the binding energy in nuclear matter and neutron star matter, as well as the formation of nuclear pastas, and the symmetry energy of neutron star matter.
Fil: Dorso, Claudio Oscar. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina
Fil: Frank, Guillermo Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Tecnológica Nacional. Facultad Regional Buenos Aires. Unidad de Investigación y Desarrollo de las Ingenierías; Argentina
Fil: Lopez, Jorge A.. University of Texas at El Paso; Estados Unidos
description In this article we present a classical potential that respects the Pauli exclusion principle and can be used to describe nucleon-nucleon interactions at intermediate energies. The potential depends on the relative momentum of the colliding nucleons and reduces interactions at low momentum transfer mimicking the Pauli exclusion principle. We use the potential with Metropolis Monte Carlo methods and study the formation of finite nuclei and infinite systems. We find good agreement in terms of the binding energies, radii, and internal nucleon distribution of finite nuclei, and the binding energy in nuclear matter and neutron star matter, as well as the formation of nuclear pastas, and the symmetry energy of neutron star matter.
publishDate 2021
dc.date.none.fl_str_mv 2021-11
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/166706
Dorso, Claudio Oscar; Frank, Guillermo Alberto; Lopez, Jorge A.; Symmetry energy and the Pauli exclusion principle; Multidisciplinary Digital Publishing Institute; Symmetry; 13; 11; 11-2021; 1-20
2073-8994
CONICET Digital
CONICET
url http://hdl.handle.net/11336/166706
identifier_str_mv Dorso, Claudio Oscar; Frank, Guillermo Alberto; Lopez, Jorge A.; Symmetry energy and the Pauli exclusion principle; Multidisciplinary Digital Publishing Institute; Symmetry; 13; 11; 11-2021; 1-20
2073-8994
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://www.mdpi.com/2073-8994/13/11/2116
info:eu-repo/semantics/altIdentifier/doi/10.3390/sym13112116
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Multidisciplinary Digital Publishing Institute
publisher.none.fl_str_mv Multidisciplinary Digital Publishing Institute
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
_version_ 1844613292292571136
score 13.070432

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