Rotation-driven phase transitions in the cores of pulsars

Autores
Mellinger, Richard D.; Weber, Fridolin; Spinella, William M.; Contrera, Gustavo Aníbal; Orsaria, Milva Gabriela
Año de publicación
2017
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
In this paper, we discuss the impact of rotation on the particle composition of rotating neutron stars (pulsars). Particular emphasis is put on the formation of quark matter during stellar spin-down, driven by continuous gravitational compression. Our study is based on modern models for the nuclear equation of state whose parameters are tightly constrained by nuclear data, neutron star masses, and the latest estimates of neutron star radii.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto de Física La Plata
Materia
Física
Dense matter
Equation of state
Neutron stars
Pulsars
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/123779
Acceder
id SEDICI_b7d41c0b657cf03261cd63526a772d84
oai_identifier_str oai:sedici.unlp.edu.ar:10915/123779
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling Rotation-driven phase transitions in the cores of pulsarsMellinger, Richard D.Weber, FridolinSpinella, William M.Contrera, Gustavo AníbalOrsaria, Milva GabrielaFísicaDense matterEquation of stateNeutron starsPulsarsIn this paper, we discuss the impact of rotation on the particle composition of rotating neutron stars (pulsars). Particular emphasis is put on the formation of quark matter during stellar spin-down, driven by continuous gravitational compression. Our study is based on modern models for the nuclear equation of state whose parameters are tightly constrained by nuclear data, neutron star masses, and the latest estimates of neutron star radii.Facultad de Ciencias Astronómicas y GeofísicasInstituto de Física La Plata2017-08-13info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/123779enginfo:eu-repo/semantics/altIdentifier/issn/20101945info:eu-repo/semantics/altIdentifier/arxiv/1702.05549info:eu-repo/semantics/altIdentifier/doi/10.1142/s2010194517600357info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/4.0/Creative Commons Attribution 4.0 International (CC BY 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:29:28Zoai:sedici.unlp.edu.ar:10915/123779Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:29:28.859SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Rotation-driven phase transitions in the cores of pulsars
title Rotation-driven phase transitions in the cores of pulsars
spellingShingle Rotation-driven phase transitions in the cores of pulsars
Mellinger, Richard D.
Física
Dense matter
Equation of state
Neutron stars
Pulsars
title_short Rotation-driven phase transitions in the cores of pulsars
title_full Rotation-driven phase transitions in the cores of pulsars
title_fullStr Rotation-driven phase transitions in the cores of pulsars
title_full_unstemmed Rotation-driven phase transitions in the cores of pulsars
title_sort Rotation-driven phase transitions in the cores of pulsars
dc.creator.none.fl_str_mv Mellinger, Richard D.
Weber, Fridolin
Spinella, William M.
Contrera, Gustavo Aníbal
Orsaria, Milva Gabriela
author Mellinger, Richard D.
author_facet Mellinger, Richard D.
Weber, Fridolin
Spinella, William M.
Contrera, Gustavo Aníbal
Orsaria, Milva Gabriela
author_role author
author2 Weber, Fridolin
Spinella, William M.
Contrera, Gustavo Aníbal
Orsaria, Milva Gabriela
author2_role author
author
author
author
dc.subject.none.fl_str_mv Física
Dense matter
Equation of state
Neutron stars
Pulsars
topic Física
Dense matter
Equation of state
Neutron stars
Pulsars
dc.description.none.fl_txt_mv In this paper, we discuss the impact of rotation on the particle composition of rotating neutron stars (pulsars). Particular emphasis is put on the formation of quark matter during stellar spin-down, driven by continuous gravitational compression. Our study is based on modern models for the nuclear equation of state whose parameters are tightly constrained by nuclear data, neutron star masses, and the latest estimates of neutron star radii.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto de Física La Plata
description In this paper, we discuss the impact of rotation on the particle composition of rotating neutron stars (pulsars). Particular emphasis is put on the formation of quark matter during stellar spin-down, driven by continuous gravitational compression. Our study is based on modern models for the nuclear equation of state whose parameters are tightly constrained by nuclear data, neutron star masses, and the latest estimates of neutron star radii.
publishDate 2017
dc.date.none.fl_str_mv 2017-08-13
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Articulo
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://sedici.unlp.edu.ar/handle/10915/123779
url http://sedici.unlp.edu.ar/handle/10915/123779
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/20101945
info:eu-repo/semantics/altIdentifier/arxiv/1702.05549
info:eu-repo/semantics/altIdentifier/doi/10.1142/s2010194517600357
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by/4.0/
Creative Commons Attribution 4.0 International (CC BY 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by/4.0/
Creative Commons Attribution 4.0 International (CC BY 4.0)
dc.format.none.fl_str_mv application/pdf
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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score 13.070432

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