Quark-hadron pasta phase in neutron stars: The role of medium-dependent surface and curvature tensions
- Autores
- Mariani, Mauro; Lugones, Germán
- Año de publicación
- 2024
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We investigate the properties of the hadron-quark mixed phase, often termed the pasta phase, expected to exist in the cores of massive neutron stars. To construct the equations of state (EoSs), we combine an analytical representation based on the Akmal-Pandharipande-Ravenhall EoS for hadronic matter with the MIT bag model featuring vector interactions for quark matter. For modeling the mixed phase, we utilize the compressible liquid drop model that consistently accounts for finite-size and Coulomb effects. Unlike most previous analyses that treated surface tension as a constant free parameter and neglected curvature tension, we employ microphysical calculations using the multiple reflection expansion formalism to determine these parameters, while also ensuring their self-consistency with the EoS. We construct an extensive set of mixed hybrid EoSs by varying model parameters, solve the stellar structure equations to obtain neutron star mass-radius relationships, and select the models that satisfy current astrophysical constraints. Our findings closely align with calculations using a constant surface tension in terms of EoS stiffness and resulting stellar structure. However, they reveal significant differences in the types of geometric structures and their prevalence ranges within the mixed phase. Specifically, curvature effects enhance the emergence of tubes and bubbles at high densities despite the large value of surface tension, while suppressing the existence of drops and rods at low densities.
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: Lugones, Germán. Universidad Federal do Abc; Brasil - Materia
-
EQUATIONS OF STATE OF NUCLEAR MATTER
NUCLEAR MATTER IN NEUTRON STARS
QUARK MATTER - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/239128
Ver los metadatos del registro completo
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Quark-hadron pasta phase in neutron stars: The role of medium-dependent surface and curvature tensionsMariani, MauroLugones, GermánEQUATIONS OF STATE OF NUCLEAR MATTERNUCLEAR MATTER IN NEUTRON STARSQUARK MATTERhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We investigate the properties of the hadron-quark mixed phase, often termed the pasta phase, expected to exist in the cores of massive neutron stars. To construct the equations of state (EoSs), we combine an analytical representation based on the Akmal-Pandharipande-Ravenhall EoS for hadronic matter with the MIT bag model featuring vector interactions for quark matter. For modeling the mixed phase, we utilize the compressible liquid drop model that consistently accounts for finite-size and Coulomb effects. Unlike most previous analyses that treated surface tension as a constant free parameter and neglected curvature tension, we employ microphysical calculations using the multiple reflection expansion formalism to determine these parameters, while also ensuring their self-consistency with the EoS. We construct an extensive set of mixed hybrid EoSs by varying model parameters, solve the stellar structure equations to obtain neutron star mass-radius relationships, and select the models that satisfy current astrophysical constraints. Our findings closely align with calculations using a constant surface tension in terms of EoS stiffness and resulting stellar structure. However, they reveal significant differences in the types of geometric structures and their prevalence ranges within the mixed phase. Specifically, curvature effects enhance the emergence of tubes and bubbles at high densities despite the large value of surface tension, while suppressing the existence of drops and rods at low densities.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; ArgentinaFil: Lugones, Germán. Universidad Federal do Abc; BrasilAmerican Physical Society2024-03info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/239128Mariani, Mauro; Lugones, Germán; Quark-hadron pasta phase in neutron stars: The role of medium-dependent surface and curvature tensions; American Physical Society; Physical Review D; 109; 6; 3-2024; 1-182470-00102470-0029CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://link.aps.org/doi/10.1103/PhysRevD.109.063022info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.109.063022info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:36:30Zoai:ri.conicet.gov.ar:11336/239128instacron: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 09:36:31.07CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Quark-hadron pasta phase in neutron stars: The role of medium-dependent surface and curvature tensions |
title |
Quark-hadron pasta phase in neutron stars: The role of medium-dependent surface and curvature tensions |
spellingShingle |
Quark-hadron pasta phase in neutron stars: The role of medium-dependent surface and curvature tensions Mariani, Mauro EQUATIONS OF STATE OF NUCLEAR MATTER NUCLEAR MATTER IN NEUTRON STARS QUARK MATTER |
title_short |
Quark-hadron pasta phase in neutron stars: The role of medium-dependent surface and curvature tensions |
title_full |
Quark-hadron pasta phase in neutron stars: The role of medium-dependent surface and curvature tensions |
title_fullStr |
Quark-hadron pasta phase in neutron stars: The role of medium-dependent surface and curvature tensions |
title_full_unstemmed |
Quark-hadron pasta phase in neutron stars: The role of medium-dependent surface and curvature tensions |
title_sort |
Quark-hadron pasta phase in neutron stars: The role of medium-dependent surface and curvature tensions |
dc.creator.none.fl_str_mv |
Mariani, Mauro Lugones, Germán |
author |
Mariani, Mauro |
author_facet |
Mariani, Mauro Lugones, Germán |
author_role |
author |
author2 |
Lugones, Germán |
author2_role |
author |
dc.subject.none.fl_str_mv |
EQUATIONS OF STATE OF NUCLEAR MATTER NUCLEAR MATTER IN NEUTRON STARS QUARK MATTER |
topic |
EQUATIONS OF STATE OF NUCLEAR MATTER NUCLEAR MATTER IN NEUTRON STARS QUARK MATTER |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
We investigate the properties of the hadron-quark mixed phase, often termed the pasta phase, expected to exist in the cores of massive neutron stars. To construct the equations of state (EoSs), we combine an analytical representation based on the Akmal-Pandharipande-Ravenhall EoS for hadronic matter with the MIT bag model featuring vector interactions for quark matter. For modeling the mixed phase, we utilize the compressible liquid drop model that consistently accounts for finite-size and Coulomb effects. Unlike most previous analyses that treated surface tension as a constant free parameter and neglected curvature tension, we employ microphysical calculations using the multiple reflection expansion formalism to determine these parameters, while also ensuring their self-consistency with the EoS. We construct an extensive set of mixed hybrid EoSs by varying model parameters, solve the stellar structure equations to obtain neutron star mass-radius relationships, and select the models that satisfy current astrophysical constraints. Our findings closely align with calculations using a constant surface tension in terms of EoS stiffness and resulting stellar structure. However, they reveal significant differences in the types of geometric structures and their prevalence ranges within the mixed phase. Specifically, curvature effects enhance the emergence of tubes and bubbles at high densities despite the large value of surface tension, while suppressing the existence of drops and rods at low densities. 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: Lugones, Germán. Universidad Federal do Abc; Brasil |
description |
We investigate the properties of the hadron-quark mixed phase, often termed the pasta phase, expected to exist in the cores of massive neutron stars. To construct the equations of state (EoSs), we combine an analytical representation based on the Akmal-Pandharipande-Ravenhall EoS for hadronic matter with the MIT bag model featuring vector interactions for quark matter. For modeling the mixed phase, we utilize the compressible liquid drop model that consistently accounts for finite-size and Coulomb effects. Unlike most previous analyses that treated surface tension as a constant free parameter and neglected curvature tension, we employ microphysical calculations using the multiple reflection expansion formalism to determine these parameters, while also ensuring their self-consistency with the EoS. We construct an extensive set of mixed hybrid EoSs by varying model parameters, solve the stellar structure equations to obtain neutron star mass-radius relationships, and select the models that satisfy current astrophysical constraints. Our findings closely align with calculations using a constant surface tension in terms of EoS stiffness and resulting stellar structure. However, they reveal significant differences in the types of geometric structures and their prevalence ranges within the mixed phase. Specifically, curvature effects enhance the emergence of tubes and bubbles at high densities despite the large value of surface tension, while suppressing the existence of drops and rods at low densities. |
publishDate |
2024 |
dc.date.none.fl_str_mv |
2024-03 |
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/11336/239128 Mariani, Mauro; Lugones, Germán; Quark-hadron pasta phase in neutron stars: The role of medium-dependent surface and curvature tensions; American Physical Society; Physical Review D; 109; 6; 3-2024; 1-18 2470-0010 2470-0029 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/239128 |
identifier_str_mv |
Mariani, Mauro; Lugones, Germán; Quark-hadron pasta phase in neutron stars: The role of medium-dependent surface and curvature tensions; American Physical Society; Physical Review D; 109; 6; 3-2024; 1-18 2470-0010 2470-0029 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://link.aps.org/doi/10.1103/PhysRevD.109.063022 info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.109.063022 |
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 |
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 |
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CONICET Digital (CONICET) |
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CONICET Digital (CONICET) |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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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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