Rotation-driven phase transitions in the cores of pulsars

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...

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Detalhes bibliográficos
Autores: Mellinger, Richard D., Weber, Fridolin, Spinella, William M., Contrera, Gustavo Aníbal, Orsaria, Milva Gabriela
Formato: artículo
Estado:Versión publicada
Fecha de publicación:2017
País:Argentina
Recursos:Universidad Nacional de La Plata
Repositorio:SEDICI (UNLP)
Idioma:inglés
OAI Identifier:oai:sedici.unlp.edu.ar:10915/123779
Acesso em linha:http://sedici.unlp.edu.ar/handle/10915/123779
Access Level:acceso abierto
Palavra-chave:Física
Dense matter
Equation of state
Neutron stars
Pulsars
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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:UNLP2024-05-08T13:07:38Zoai: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:13292024-05-08 13:07:38.738SEDICI (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
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
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (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 15.198674

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