Oscillating Magnetized Color Superconducting Quark Stars
- Autores
- Celi, Marcos Osvaldo; Mariani, Mauro; Orsaria, Milva Gabriela; Tonetto, Lucas
- Año de publicación
- 2022
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The main objective of this work is to study the structure, composition, and oscillation modes of color superconducting quark stars with intense magnetic fields. We adopted the MIT bag model within the color superconductivity CFL framework, and we included the effects of strong magnetic fields to construct the equation of state of stable quark matter. We calculated observable quantities, such as the mass, radius, frequency, and damping time of the oscillation fundamental f mode of quark stars, taking into account current astrophysical constraints. The results obtained show that color superconducting magnetized quark stars satisfy the constraints imposed by the observations of massive pulsars and gravitational wave events. Furthermore, the quantities associated with the oscillation f mode of these objects fit the universal relationships for compact objects. In the context of the new multi-messenger gravitational wave astronomy era and the future asteroseismology of neutron stars, we hope that our results contribute to the understanding of the behavior of dense matter and compact objects.
Fil: Celi, Marcos Osvaldo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Mariani, Mauro. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina
Fil: Orsaria, Milva Gabriela. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina
Fil: Tonetto, Lucas. Università degli studi di Roma "La Sapienza"; Italia - Materia
-
COLOR SUPERCONDUCTIVITY
DENSE MATTER
DI-QUARKS
EQUATION OF STATE
MAGNETIC FIELD
NEUTRON STARS
OSCILLATIONS (INCLUDING PULSATIONS)
QUARK STARS - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/223734
Ver los metadatos del registro completo
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oai:ri.conicet.gov.ar:11336/223734 |
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Oscillating Magnetized Color Superconducting Quark StarsCeli, Marcos OsvaldoMariani, MauroOrsaria, Milva GabrielaTonetto, LucasCOLOR SUPERCONDUCTIVITYDENSE MATTERDI-QUARKSEQUATION OF STATEMAGNETIC FIELDNEUTRON STARSOSCILLATIONS (INCLUDING PULSATIONS)QUARK STARShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The main objective of this work is to study the structure, composition, and oscillation modes of color superconducting quark stars with intense magnetic fields. We adopted the MIT bag model within the color superconductivity CFL framework, and we included the effects of strong magnetic fields to construct the equation of state of stable quark matter. We calculated observable quantities, such as the mass, radius, frequency, and damping time of the oscillation fundamental f mode of quark stars, taking into account current astrophysical constraints. The results obtained show that color superconducting magnetized quark stars satisfy the constraints imposed by the observations of massive pulsars and gravitational wave events. Furthermore, the quantities associated with the oscillation f mode of these objects fit the universal relationships for compact objects. In the context of the new multi-messenger gravitational wave astronomy era and the future asteroseismology of neutron stars, we hope that our results contribute to the understanding of the behavior of dense matter and compact objects.Fil: Celi, Marcos Osvaldo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Mariani, Mauro. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; ArgentinaFil: Orsaria, Milva Gabriela. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; ArgentinaFil: Tonetto, Lucas. Università degli studi di Roma "La Sapienza"; ItaliaMDPI2022-05info: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/11336/223734Celi, Marcos Osvaldo; Mariani, Mauro; Orsaria, Milva Gabriela; Tonetto, Lucas; Oscillating Magnetized Color Superconducting Quark Stars; MDPI; Universe; 8; 5; 5-2022; 1-182218-1997CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.3390/universe8050272info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:30:34Zoai:ri.conicet.gov.ar:11336/223734instacron: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 10:30:34.697CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Oscillating Magnetized Color Superconducting Quark Stars |
title |
Oscillating Magnetized Color Superconducting Quark Stars |
spellingShingle |
Oscillating Magnetized Color Superconducting Quark Stars Celi, Marcos Osvaldo COLOR SUPERCONDUCTIVITY DENSE MATTER DI-QUARKS EQUATION OF STATE MAGNETIC FIELD NEUTRON STARS OSCILLATIONS (INCLUDING PULSATIONS) QUARK STARS |
title_short |
Oscillating Magnetized Color Superconducting Quark Stars |
title_full |
Oscillating Magnetized Color Superconducting Quark Stars |
title_fullStr |
Oscillating Magnetized Color Superconducting Quark Stars |
title_full_unstemmed |
Oscillating Magnetized Color Superconducting Quark Stars |
title_sort |
Oscillating Magnetized Color Superconducting Quark Stars |
dc.creator.none.fl_str_mv |
Celi, Marcos Osvaldo Mariani, Mauro Orsaria, Milva Gabriela Tonetto, Lucas |
author |
Celi, Marcos Osvaldo |
author_facet |
Celi, Marcos Osvaldo Mariani, Mauro Orsaria, Milva Gabriela Tonetto, Lucas |
author_role |
author |
author2 |
Mariani, Mauro Orsaria, Milva Gabriela Tonetto, Lucas |
author2_role |
author author author |
dc.subject.none.fl_str_mv |
COLOR SUPERCONDUCTIVITY DENSE MATTER DI-QUARKS EQUATION OF STATE MAGNETIC FIELD NEUTRON STARS OSCILLATIONS (INCLUDING PULSATIONS) QUARK STARS |
topic |
COLOR SUPERCONDUCTIVITY DENSE MATTER DI-QUARKS EQUATION OF STATE MAGNETIC FIELD NEUTRON STARS OSCILLATIONS (INCLUDING PULSATIONS) QUARK STARS |
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 main objective of this work is to study the structure, composition, and oscillation modes of color superconducting quark stars with intense magnetic fields. We adopted the MIT bag model within the color superconductivity CFL framework, and we included the effects of strong magnetic fields to construct the equation of state of stable quark matter. We calculated observable quantities, such as the mass, radius, frequency, and damping time of the oscillation fundamental f mode of quark stars, taking into account current astrophysical constraints. The results obtained show that color superconducting magnetized quark stars satisfy the constraints imposed by the observations of massive pulsars and gravitational wave events. Furthermore, the quantities associated with the oscillation f mode of these objects fit the universal relationships for compact objects. In the context of the new multi-messenger gravitational wave astronomy era and the future asteroseismology of neutron stars, we hope that our results contribute to the understanding of the behavior of dense matter and compact objects. Fil: Celi, Marcos Osvaldo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Mariani, Mauro. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina Fil: Orsaria, Milva Gabriela. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina Fil: Tonetto, Lucas. Università degli studi di Roma "La Sapienza"; Italia |
description |
The main objective of this work is to study the structure, composition, and oscillation modes of color superconducting quark stars with intense magnetic fields. We adopted the MIT bag model within the color superconductivity CFL framework, and we included the effects of strong magnetic fields to construct the equation of state of stable quark matter. We calculated observable quantities, such as the mass, radius, frequency, and damping time of the oscillation fundamental f mode of quark stars, taking into account current astrophysical constraints. The results obtained show that color superconducting magnetized quark stars satisfy the constraints imposed by the observations of massive pulsars and gravitational wave events. Furthermore, the quantities associated with the oscillation f mode of these objects fit the universal relationships for compact objects. In the context of the new multi-messenger gravitational wave astronomy era and the future asteroseismology of neutron stars, we hope that our results contribute to the understanding of the behavior of dense matter and compact objects. |
publishDate |
2022 |
dc.date.none.fl_str_mv |
2022-05 |
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/11336/223734 Celi, Marcos Osvaldo; Mariani, Mauro; Orsaria, Milva Gabriela; Tonetto, Lucas; Oscillating Magnetized Color Superconducting Quark Stars; MDPI; Universe; 8; 5; 5-2022; 1-18 2218-1997 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/223734 |
identifier_str_mv |
Celi, Marcos Osvaldo; Mariani, Mauro; Orsaria, Milva Gabriela; Tonetto, Lucas; Oscillating Magnetized Color Superconducting Quark Stars; MDPI; Universe; 8; 5; 5-2022; 1-18 2218-1997 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.3390/universe8050272 |
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 application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
MDPI |
publisher.none.fl_str_mv |
MDPI |
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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 |
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1844614314496884736 |
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13.070432 |