Is There a Crisis in Neutron Star Physics?

Autores
Horvath, J.E.; Benvenuto, Omar Gustavo
Año de publicación
2012
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión enviada
Descripción
We shall show in this report that the theoretical evolution of a particular class of systems containing a neutron star, the so-called black widow binaries, suggest masses above the∼2M⊙, a fact that would bring serious concerns about the right description of the equation of state above the saturation density. Moreover, so far the actual determinations of masses for these systems consistently give values above2M⊙, reinforcing the quandary. In this sense, and given that the confirmation of these ideas would create problems for the microphysical description, we argue that a crisis could be in the works in neutron star physics
Materia
Astronomía
neutron star
black widow
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by/4.0/
Repositorio
CIC Digital (CICBA)
Institución
Comisión de Investigaciones Científicas de la Provincia de Buenos Aires
OAI Identificador
oai:digital.cic.gba.gob.ar:11746/4223
Acceder
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network_name_str CIC Digital (CICBA)
spelling Is There a Crisis in Neutron Star Physics?Horvath, J.E.Benvenuto, Omar GustavoAstronomíaneutron starblack widowWe shall show in this report that the theoretical evolution of a particular class of systems containing a neutron star, the so-called black widow binaries, suggest masses above the∼2M⊙, a fact that would bring serious concerns about the right description of the equation of state above the saturation density. Moreover, so far the actual determinations of masses for these systems consistently give values above2M⊙, reinforcing the quandary. In this sense, and given that the confirmation of these ideas would create problems for the microphysical description, we argue that a crisis could be in the works in neutron star physics2012info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/submittedVersionhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfhttps://digital.cic.gba.gob.ar/handle/11746/4223enginfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/4.0/reponame:CIC Digital (CICBA)instname:Comisión de Investigaciones Científicas de la Provincia de Buenos Airesinstacron:CICBA2025-09-29T13:40:01Zoai:digital.cic.gba.gob.ar:11746/4223Institucionalhttp://digital.cic.gba.gob.arOrganismo científico-tecnológicoNo correspondehttp://digital.cic.gba.gob.ar/oai/snrdmarisa.degiusti@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:94412025-09-29 13:40:02.007CIC Digital (CICBA) - Comisión de Investigaciones Científicas de la Provincia de Buenos Airesfalse
dc.title.none.fl_str_mv Is There a Crisis in Neutron Star Physics?
title Is There a Crisis in Neutron Star Physics?
spellingShingle Is There a Crisis in Neutron Star Physics?
Horvath, J.E.
Astronomía
neutron star
black widow
title_short Is There a Crisis in Neutron Star Physics?
title_full Is There a Crisis in Neutron Star Physics?
title_fullStr Is There a Crisis in Neutron Star Physics?
title_full_unstemmed Is There a Crisis in Neutron Star Physics?
title_sort Is There a Crisis in Neutron Star Physics?
dc.creator.none.fl_str_mv Horvath, J.E.
Benvenuto, Omar Gustavo
author Horvath, J.E.
author_facet Horvath, J.E.
Benvenuto, Omar Gustavo
author_role author
author2 Benvenuto, Omar Gustavo
author2_role author
dc.subject.none.fl_str_mv Astronomía
neutron star
black widow
topic Astronomía
neutron star
black widow
dc.description.none.fl_txt_mv We shall show in this report that the theoretical evolution of a particular class of systems containing a neutron star, the so-called black widow binaries, suggest masses above the∼2M⊙, a fact that would bring serious concerns about the right description of the equation of state above the saturation density. Moreover, so far the actual determinations of masses for these systems consistently give values above2M⊙, reinforcing the quandary. In this sense, and given that the confirmation of these ideas would create problems for the microphysical description, we argue that a crisis could be in the works in neutron star physics
description We shall show in this report that the theoretical evolution of a particular class of systems containing a neutron star, the so-called black widow binaries, suggest masses above the∼2M⊙, a fact that would bring serious concerns about the right description of the equation of state above the saturation density. Moreover, so far the actual determinations of masses for these systems consistently give values above2M⊙, reinforcing the quandary. In this sense, and given that the confirmation of these ideas would create problems for the microphysical description, we argue that a crisis could be in the works in neutron star physics
publishDate 2012
dc.date.none.fl_str_mv 2012
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dc.identifier.none.fl_str_mv https://digital.cic.gba.gob.ar/handle/11746/4223
url https://digital.cic.gba.gob.ar/handle/11746/4223
dc.language.none.fl_str_mv eng
language eng
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repository.mail.fl_str_mv marisa.degiusti@sedici.unlp.edu.ar
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