Phase structure of cold magnetized quark matter within the SU(3) NJL model

Autores
Grunfeld, Ana Gabriela; Menezes, Débora P.; Pinto, Marcus B.; Scoccola, Norberto Nerio
Año de publicación
2014
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The possible different phases of homogeneous cold quark matter in the presence of a finite magnetic field and chemical potential are obtained within the SU(3) NJL model for two parameter sets often used in the literature. Although the general pattern is the same in both cases, the number of intermediate phases is parameter dependent. The chiral susceptibilities, as usually defined, are different not only for the s quark as compared with the two light quarks, but also for the u and d quarks, yielding nonidentical crossover lines for the light quark sector. The results for stellar matter, imposing charge neutrality and β equilibrium, are also presented for the same sets of parameters. The corresponding phase diagrams show some differences with respect to the symmetric cases. It is found that for stellar matter the inverse catalysis effect is less pronounced and the transition to the fully chiral symmetry-restored phase occurs at higher chemical potentials.
Fil: Grunfeld, Ana Gabriela. Comisión Nacional de Energía Atómica; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Menezes, Débora P.. Universidade Federal de Santa Catarina; Brasil. Universidad de Alicante; España
Fil: Pinto, Marcus B.. Universidade Federal de Santa Catarina; Brasil
Fil: Scoccola, Norberto Nerio. Universidad Favaloro; Argentina. Comisión Nacional de Energía Atómica; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Materia
Relativistic models
Quark deconfinement
Phase transitions
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/99100
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/99100
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Phase structure of cold magnetized quark matter within the SU(3) NJL modelGrunfeld, Ana GabrielaMenezes, Débora P.Pinto, Marcus B.Scoccola, Norberto NerioRelativistic modelsQuark deconfinementPhase transitionshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The possible different phases of homogeneous cold quark matter in the presence of a finite magnetic field and chemical potential are obtained within the SU(3) NJL model for two parameter sets often used in the literature. Although the general pattern is the same in both cases, the number of intermediate phases is parameter dependent. The chiral susceptibilities, as usually defined, are different not only for the s quark as compared with the two light quarks, but also for the u and d quarks, yielding nonidentical crossover lines for the light quark sector. The results for stellar matter, imposing charge neutrality and β equilibrium, are also presented for the same sets of parameters. The corresponding phase diagrams show some differences with respect to the symmetric cases. It is found that for stellar matter the inverse catalysis effect is less pronounced and the transition to the fully chiral symmetry-restored phase occurs at higher chemical potentials.Fil: Grunfeld, Ana Gabriela. Comisión Nacional de Energía Atómica; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Menezes, Débora P.. Universidade Federal de Santa Catarina; Brasil. Universidad de Alicante; EspañaFil: Pinto, Marcus B.. Universidade Federal de Santa Catarina; BrasilFil: Scoccola, Norberto Nerio. Universidad Favaloro; Argentina. Comisión Nacional de Energía Atómica; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaAmerican Physical Society2014-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/99100Grunfeld, Ana Gabriela; Menezes, Débora P.; Pinto, Marcus B.; Scoccola, Norberto Nerio; Phase structure of cold magnetized quark matter within the SU(3) NJL model; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 90; 4; 8-2014; 1-110556-28211550-7998CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.90.044024info:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/prd/abstract/10.1103/PhysRevD.90.044024info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:33:15Zoai:ri.conicet.gov.ar:11336/99100instacron: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 09:33:15.352CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Phase structure of cold magnetized quark matter within the SU(3) NJL model
title Phase structure of cold magnetized quark matter within the SU(3) NJL model
spellingShingle Phase structure of cold magnetized quark matter within the SU(3) NJL model
Grunfeld, Ana Gabriela
Relativistic models
Quark deconfinement
Phase transitions
title_short Phase structure of cold magnetized quark matter within the SU(3) NJL model
title_full Phase structure of cold magnetized quark matter within the SU(3) NJL model
title_fullStr Phase structure of cold magnetized quark matter within the SU(3) NJL model
title_full_unstemmed Phase structure of cold magnetized quark matter within the SU(3) NJL model
title_sort Phase structure of cold magnetized quark matter within the SU(3) NJL model
dc.creator.none.fl_str_mv Grunfeld, Ana Gabriela
Menezes, Débora P.
Pinto, Marcus B.
Scoccola, Norberto Nerio
author Grunfeld, Ana Gabriela
author_facet Grunfeld, Ana Gabriela
Menezes, Débora P.
Pinto, Marcus B.
Scoccola, Norberto Nerio
author_role author
author2 Menezes, Débora P.
Pinto, Marcus B.
Scoccola, Norberto Nerio
author2_role author
author
author
dc.subject.none.fl_str_mv Relativistic models
Quark deconfinement
Phase transitions
topic Relativistic models
Quark deconfinement
Phase transitions
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv The possible different phases of homogeneous cold quark matter in the presence of a finite magnetic field and chemical potential are obtained within the SU(3) NJL model for two parameter sets often used in the literature. Although the general pattern is the same in both cases, the number of intermediate phases is parameter dependent. The chiral susceptibilities, as usually defined, are different not only for the s quark as compared with the two light quarks, but also for the u and d quarks, yielding nonidentical crossover lines for the light quark sector. The results for stellar matter, imposing charge neutrality and β equilibrium, are also presented for the same sets of parameters. The corresponding phase diagrams show some differences with respect to the symmetric cases. It is found that for stellar matter the inverse catalysis effect is less pronounced and the transition to the fully chiral symmetry-restored phase occurs at higher chemical potentials.
Fil: Grunfeld, Ana Gabriela. Comisión Nacional de Energía Atómica; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Menezes, Débora P.. Universidade Federal de Santa Catarina; Brasil. Universidad de Alicante; España
Fil: Pinto, Marcus B.. Universidade Federal de Santa Catarina; Brasil
Fil: Scoccola, Norberto Nerio. Universidad Favaloro; Argentina. Comisión Nacional de Energía Atómica; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
description The possible different phases of homogeneous cold quark matter in the presence of a finite magnetic field and chemical potential are obtained within the SU(3) NJL model for two parameter sets often used in the literature. Although the general pattern is the same in both cases, the number of intermediate phases is parameter dependent. The chiral susceptibilities, as usually defined, are different not only for the s quark as compared with the two light quarks, but also for the u and d quarks, yielding nonidentical crossover lines for the light quark sector. The results for stellar matter, imposing charge neutrality and β equilibrium, are also presented for the same sets of parameters. The corresponding phase diagrams show some differences with respect to the symmetric cases. It is found that for stellar matter the inverse catalysis effect is less pronounced and the transition to the fully chiral symmetry-restored phase occurs at higher chemical potentials.
publishDate 2014
dc.date.none.fl_str_mv 2014-08
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/11336/99100
Grunfeld, Ana Gabriela; Menezes, Débora P.; Pinto, Marcus B.; Scoccola, Norberto Nerio; Phase structure of cold magnetized quark matter within the SU(3) NJL model; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 90; 4; 8-2014; 1-11
0556-2821
1550-7998
CONICET Digital
CONICET
url http://hdl.handle.net/11336/99100
identifier_str_mv Grunfeld, Ana Gabriela; Menezes, Débora P.; Pinto, Marcus B.; Scoccola, Norberto Nerio; Phase structure of cold magnetized quark matter within the SU(3) NJL model; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 90; 4; 8-2014; 1-11
0556-2821
1550-7998
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.90.044024
info:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/prd/abstract/10.1103/PhysRevD.90.044024
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
application/pdf
dc.publisher.none.fl_str_mv American Physical Society
publisher.none.fl_str_mv American Physical Society
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_ 1844613020369551360
score 13.070432

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