Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observations
- Autores
- Carlomagno, Juan Pablo; Contrera, Gustavo Aníbal Gabriel; Grunfeld, Ana Gabriela; Blaschke, D.
- Año de publicación
- 2024
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We investigate the extension to finite temperatures and neutrino chemical potentials of a recentlydeveloped nonlocal chiral quark model approach to the equation of state of neutron star matter.We consider two light quark flavors and current-current interactions in the scalar-pseudoscalar,vector, and diquark pairing channels, where the nonlocality of the currents is taken into accountby a Gaussian form factor that depends on the spatial components of the 4-momentum. Withinthis framework, we analyze order parameters, critical temperatures, phase diagrams, equation ofstate, and mass-radius relations for different temperatures and neutrino chemical potentials. Forparameters of the model that are constrained by recent multi-messenger observations of neutronstars, we find that the mass-radius diagram for isothermal hybrid star sequences exhibits the thermaltwin phenomenon for temperatures above 30 MeV.
Fil: Carlomagno, Juan Pablo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina
Fil: Contrera, Gustavo Aníbal Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina
Fil: Grunfeld, Ana Gabriela. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Comisión Nacional de Energía Atómica; Argentina
Fil: Blaschke, D.. University of Wroclaw; Polonia - Materia
-
Compact stars
Chiral quark models
Nuclear Astrophysics
Quantum Chromodynamics - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
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- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/241135
Ver los metadatos del registro completo
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Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observationsCarlomagno, Juan PabloContrera, Gustavo Aníbal GabrielGrunfeld, Ana GabrielaBlaschke, D.Compact starsChiral quark modelsNuclear AstrophysicsQuantum Chromodynamicshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We investigate the extension to finite temperatures and neutrino chemical potentials of a recentlydeveloped nonlocal chiral quark model approach to the equation of state of neutron star matter.We consider two light quark flavors and current-current interactions in the scalar-pseudoscalar,vector, and diquark pairing channels, where the nonlocality of the currents is taken into accountby a Gaussian form factor that depends on the spatial components of the 4-momentum. Withinthis framework, we analyze order parameters, critical temperatures, phase diagrams, equation ofstate, and mass-radius relations for different temperatures and neutrino chemical potentials. Forparameters of the model that are constrained by recent multi-messenger observations of neutronstars, we find that the mass-radius diagram for isothermal hybrid star sequences exhibits the thermaltwin phenomenon for temperatures above 30 MeV.Fil: Carlomagno, Juan Pablo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; ArgentinaFil: Contrera, Gustavo Aníbal Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; ArgentinaFil: Grunfeld, Ana Gabriela. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Comisión Nacional de Energía Atómica; ArgentinaFil: Blaschke, D.. University of Wroclaw; PoloniaAmerican Physical Society2024-02info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/241135Carlomagno, Juan Pablo; Contrera, Gustavo Aníbal Gabriel; Grunfeld, Ana Gabriela; Blaschke, D.; Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observations; American Physical Society; Physical Review D; 109; 4; 2-2024; 1-152470-0010CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/prd/abstract/10.1103/PhysRevD.109.043050info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.109.043050info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2026-06-10T09:46:23Zoai:ri.conicet.gov.ar:11336/241135instacron: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:34982026-06-10 09:46:23.6CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observations |
| title |
Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observations |
| spellingShingle |
Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observations Carlomagno, Juan Pablo Compact stars Chiral quark models Nuclear Astrophysics Quantum Chromodynamics |
| title_short |
Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observations |
| title_full |
Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observations |
| title_fullStr |
Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observations |
| title_full_unstemmed |
Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observations |
| title_sort |
Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observations |
| dc.creator.none.fl_str_mv |
Carlomagno, Juan Pablo Contrera, Gustavo Aníbal Gabriel Grunfeld, Ana Gabriela Blaschke, D. |
| author |
Carlomagno, Juan Pablo |
| author_facet |
Carlomagno, Juan Pablo Contrera, Gustavo Aníbal Gabriel Grunfeld, Ana Gabriela Blaschke, D. |
| author_role |
author |
| author2 |
Contrera, Gustavo Aníbal Gabriel Grunfeld, Ana Gabriela Blaschke, D. |
| author2_role |
author author author |
| dc.subject.none.fl_str_mv |
Compact stars Chiral quark models Nuclear Astrophysics Quantum Chromodynamics |
| topic |
Compact stars Chiral quark models Nuclear Astrophysics Quantum Chromodynamics |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
We investigate the extension to finite temperatures and neutrino chemical potentials of a recentlydeveloped nonlocal chiral quark model approach to the equation of state of neutron star matter.We consider two light quark flavors and current-current interactions in the scalar-pseudoscalar,vector, and diquark pairing channels, where the nonlocality of the currents is taken into accountby a Gaussian form factor that depends on the spatial components of the 4-momentum. Withinthis framework, we analyze order parameters, critical temperatures, phase diagrams, equation ofstate, and mass-radius relations for different temperatures and neutrino chemical potentials. Forparameters of the model that are constrained by recent multi-messenger observations of neutronstars, we find that the mass-radius diagram for isothermal hybrid star sequences exhibits the thermaltwin phenomenon for temperatures above 30 MeV. Fil: Carlomagno, Juan Pablo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina Fil: Contrera, Gustavo Aníbal Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina Fil: Grunfeld, Ana Gabriela. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Comisión Nacional de Energía Atómica; Argentina Fil: Blaschke, D.. University of Wroclaw; Polonia |
| description |
We investigate the extension to finite temperatures and neutrino chemical potentials of a recentlydeveloped nonlocal chiral quark model approach to the equation of state of neutron star matter.We consider two light quark flavors and current-current interactions in the scalar-pseudoscalar,vector, and diquark pairing channels, where the nonlocality of the currents is taken into accountby a Gaussian form factor that depends on the spatial components of the 4-momentum. Withinthis framework, we analyze order parameters, critical temperatures, phase diagrams, equation ofstate, and mass-radius relations for different temperatures and neutrino chemical potentials. Forparameters of the model that are constrained by recent multi-messenger observations of neutronstars, we find that the mass-radius diagram for isothermal hybrid star sequences exhibits the thermaltwin phenomenon for temperatures above 30 MeV. |
| publishDate |
2024 |
| dc.date.none.fl_str_mv |
2024-02 |
| 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 |
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article |
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publishedVersion |
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http://hdl.handle.net/11336/241135 Carlomagno, Juan Pablo; Contrera, Gustavo Aníbal Gabriel; Grunfeld, Ana Gabriela; Blaschke, D.; Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observations; American Physical Society; Physical Review D; 109; 4; 2-2024; 1-15 2470-0010 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/241135 |
| identifier_str_mv |
Carlomagno, Juan Pablo; Contrera, Gustavo Aníbal Gabriel; Grunfeld, Ana Gabriela; Blaschke, D.; Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observations; American Physical Society; Physical Review D; 109; 4; 2-2024; 1-15 2470-0010 CONICET Digital CONICET |
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eng |
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eng |
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American Physical Society |
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American Physical Society |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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