Dynamical evolutions of ℓ-boson stars in spherical symmetry
- Autores
- Alcubierre, Miguel; Barranco, Juan; Bernal, Argelia; Degollado, Juan Carlos; Diez Tejedor, Alberto; Megevand Politano, Miguel Federico; Núñez, Darío; Sarbach, Olivier
- Año de publicación
- 2019
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- In previous work, we have found new static, spherically symmetric boson star solutions which generalize the standard boson stars (BSs) by allowing a particular superposition of scalar fields in which each of the fields is characterized by a fixed value of its non-vanishing angular momentum number. We call such solutions 'boson stars'. Here, we perform a series of fully non-linear dynamical simulations of perturbed BSs in order to study their stability, and the final fate of unstable configurations. We show that for each value of, the configuration of maximum mass separates the parameter space into stable and unstable regions. Stable configurations, when perturbed, oscillate around the unperturbed solution and very slowly return to a stationary configuration. Unstable configurations, in contrast, can have three different final states: collapse to a black hole, migration to the stable branch, or explosion (dissipation) to infinity. Just as it happens with BSs, migration to the stable branch or dissipation to infinity depends on the sign of the total binding energy of the star: bound unstable stars collapse to black holes or migrate to the stable branch, whereas unbound unstable stars either collapse to a black hole or explode to infinity. Thus, the parameter allows us to construct a new set of stable configurations. All our simulations are performed in spherical symmetry, leaving a more detailed stability analysis including non-spherical perturbations for future work.
Fil: Alcubierre, Miguel. Universidad Nacional Autónoma de México. Instituto de Ciencias Nucleares; México
Fil: Barranco, Juan. Universidad de Guanajuato; México
Fil: Bernal, Argelia. Universidad de Guanajuato; México
Fil: Degollado, Juan Carlos. Universidad Nacional Autónoma de México; México
Fil: Diez Tejedor, Alberto. Universidad de Guanajuato; México
Fil: Megevand Politano, Miguel Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Física Enrique Gaviola. Universidad Nacional de Córdoba. Instituto de Física Enrique Gaviola; Argentina
Fil: Núñez, Darío. Universidad Nacional Autónoma de México. Instituto de Ciencias Nucleares; México
Fil: Sarbach, Olivier. Universidad Michoacana de San Nicolás de Hidalgo; México - Materia
-
BOSON STARS
CLASSICAL GENERAL RELATIVITY
NUMERICAL RELATIVITY - 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:11336/126482
Ver los metadatos del registro completo
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Dynamical evolutions of ℓ-boson stars in spherical symmetryAlcubierre, MiguelBarranco, JuanBernal, ArgeliaDegollado, Juan CarlosDiez Tejedor, AlbertoMegevand Politano, Miguel FedericoNúñez, DaríoSarbach, OlivierBOSON STARSCLASSICAL GENERAL RELATIVITYNUMERICAL RELATIVITYhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1In previous work, we have found new static, spherically symmetric boson star solutions which generalize the standard boson stars (BSs) by allowing a particular superposition of scalar fields in which each of the fields is characterized by a fixed value of its non-vanishing angular momentum number. We call such solutions 'boson stars'. Here, we perform a series of fully non-linear dynamical simulations of perturbed BSs in order to study their stability, and the final fate of unstable configurations. We show that for each value of, the configuration of maximum mass separates the parameter space into stable and unstable regions. Stable configurations, when perturbed, oscillate around the unperturbed solution and very slowly return to a stationary configuration. Unstable configurations, in contrast, can have three different final states: collapse to a black hole, migration to the stable branch, or explosion (dissipation) to infinity. Just as it happens with BSs, migration to the stable branch or dissipation to infinity depends on the sign of the total binding energy of the star: bound unstable stars collapse to black holes or migrate to the stable branch, whereas unbound unstable stars either collapse to a black hole or explode to infinity. Thus, the parameter allows us to construct a new set of stable configurations. All our simulations are performed in spherical symmetry, leaving a more detailed stability analysis including non-spherical perturbations for future work.Fil: Alcubierre, Miguel. Universidad Nacional Autónoma de México. Instituto de Ciencias Nucleares; MéxicoFil: Barranco, Juan. Universidad de Guanajuato; MéxicoFil: Bernal, Argelia. Universidad de Guanajuato; MéxicoFil: Degollado, Juan Carlos. Universidad Nacional Autónoma de México; MéxicoFil: Diez Tejedor, Alberto. Universidad de Guanajuato; MéxicoFil: Megevand Politano, Miguel Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Física Enrique Gaviola. Universidad Nacional de Córdoba. Instituto de Física Enrique Gaviola; ArgentinaFil: Núñez, Darío. Universidad Nacional Autónoma de México. Instituto de Ciencias Nucleares; MéxicoFil: Sarbach, Olivier. Universidad Michoacana de San Nicolás de Hidalgo; MéxicoIOP Publishing2019-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/126482Alcubierre, Miguel; Barranco, Juan; Bernal, Argelia; Degollado, Juan Carlos; Diez Tejedor, Alberto; et al.; Dynamical evolutions of ℓ-boson stars in spherical symmetry; IOP Publishing; Classical and Quantum Gravity; 36; 21; 10-2019; 1-27; 2150130264-9381CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/1361-6382/ab4726info:eu-repo/semantics/altIdentifier/doi/10.1088/1361-6382/ab4726info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/1906.08959info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:53:04Zoai:ri.conicet.gov.ar:11336/126482instacron: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 09:53:04.798CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Dynamical evolutions of ℓ-boson stars in spherical symmetry |
title |
Dynamical evolutions of ℓ-boson stars in spherical symmetry |
spellingShingle |
Dynamical evolutions of ℓ-boson stars in spherical symmetry Alcubierre, Miguel BOSON STARS CLASSICAL GENERAL RELATIVITY NUMERICAL RELATIVITY |
title_short |
Dynamical evolutions of ℓ-boson stars in spherical symmetry |
title_full |
Dynamical evolutions of ℓ-boson stars in spherical symmetry |
title_fullStr |
Dynamical evolutions of ℓ-boson stars in spherical symmetry |
title_full_unstemmed |
Dynamical evolutions of ℓ-boson stars in spherical symmetry |
title_sort |
Dynamical evolutions of ℓ-boson stars in spherical symmetry |
dc.creator.none.fl_str_mv |
Alcubierre, Miguel Barranco, Juan Bernal, Argelia Degollado, Juan Carlos Diez Tejedor, Alberto Megevand Politano, Miguel Federico Núñez, Darío Sarbach, Olivier |
author |
Alcubierre, Miguel |
author_facet |
Alcubierre, Miguel Barranco, Juan Bernal, Argelia Degollado, Juan Carlos Diez Tejedor, Alberto Megevand Politano, Miguel Federico Núñez, Darío Sarbach, Olivier |
author_role |
author |
author2 |
Barranco, Juan Bernal, Argelia Degollado, Juan Carlos Diez Tejedor, Alberto Megevand Politano, Miguel Federico Núñez, Darío Sarbach, Olivier |
author2_role |
author author author author author author author |
dc.subject.none.fl_str_mv |
BOSON STARS CLASSICAL GENERAL RELATIVITY NUMERICAL RELATIVITY |
topic |
BOSON STARS CLASSICAL GENERAL RELATIVITY NUMERICAL RELATIVITY |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
In previous work, we have found new static, spherically symmetric boson star solutions which generalize the standard boson stars (BSs) by allowing a particular superposition of scalar fields in which each of the fields is characterized by a fixed value of its non-vanishing angular momentum number. We call such solutions 'boson stars'. Here, we perform a series of fully non-linear dynamical simulations of perturbed BSs in order to study their stability, and the final fate of unstable configurations. We show that for each value of, the configuration of maximum mass separates the parameter space into stable and unstable regions. Stable configurations, when perturbed, oscillate around the unperturbed solution and very slowly return to a stationary configuration. Unstable configurations, in contrast, can have three different final states: collapse to a black hole, migration to the stable branch, or explosion (dissipation) to infinity. Just as it happens with BSs, migration to the stable branch or dissipation to infinity depends on the sign of the total binding energy of the star: bound unstable stars collapse to black holes or migrate to the stable branch, whereas unbound unstable stars either collapse to a black hole or explode to infinity. Thus, the parameter allows us to construct a new set of stable configurations. All our simulations are performed in spherical symmetry, leaving a more detailed stability analysis including non-spherical perturbations for future work. Fil: Alcubierre, Miguel. Universidad Nacional Autónoma de México. Instituto de Ciencias Nucleares; México Fil: Barranco, Juan. Universidad de Guanajuato; México Fil: Bernal, Argelia. Universidad de Guanajuato; México Fil: Degollado, Juan Carlos. Universidad Nacional Autónoma de México; México Fil: Diez Tejedor, Alberto. Universidad de Guanajuato; México Fil: Megevand Politano, Miguel Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Física Enrique Gaviola. Universidad Nacional de Córdoba. Instituto de Física Enrique Gaviola; Argentina Fil: Núñez, Darío. Universidad Nacional Autónoma de México. Instituto de Ciencias Nucleares; México Fil: Sarbach, Olivier. Universidad Michoacana de San Nicolás de Hidalgo; México |
description |
In previous work, we have found new static, spherically symmetric boson star solutions which generalize the standard boson stars (BSs) by allowing a particular superposition of scalar fields in which each of the fields is characterized by a fixed value of its non-vanishing angular momentum number. We call such solutions 'boson stars'. Here, we perform a series of fully non-linear dynamical simulations of perturbed BSs in order to study their stability, and the final fate of unstable configurations. We show that for each value of, the configuration of maximum mass separates the parameter space into stable and unstable regions. Stable configurations, when perturbed, oscillate around the unperturbed solution and very slowly return to a stationary configuration. Unstable configurations, in contrast, can have three different final states: collapse to a black hole, migration to the stable branch, or explosion (dissipation) to infinity. Just as it happens with BSs, migration to the stable branch or dissipation to infinity depends on the sign of the total binding energy of the star: bound unstable stars collapse to black holes or migrate to the stable branch, whereas unbound unstable stars either collapse to a black hole or explode to infinity. Thus, the parameter allows us to construct a new set of stable configurations. All our simulations are performed in spherical symmetry, leaving a more detailed stability analysis including non-spherical perturbations for future work. |
publishDate |
2019 |
dc.date.none.fl_str_mv |
2019-10 |
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/11336/126482 Alcubierre, Miguel; Barranco, Juan; Bernal, Argelia; Degollado, Juan Carlos; Diez Tejedor, Alberto; et al.; Dynamical evolutions of ℓ-boson stars in spherical symmetry; IOP Publishing; Classical and Quantum Gravity; 36; 21; 10-2019; 1-27; 215013 0264-9381 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/126482 |
identifier_str_mv |
Alcubierre, Miguel; Barranco, Juan; Bernal, Argelia; Degollado, Juan Carlos; Diez Tejedor, Alberto; et al.; Dynamical evolutions of ℓ-boson stars in spherical symmetry; IOP Publishing; Classical and Quantum Gravity; 36; 21; 10-2019; 1-27; 215013 0264-9381 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://iopscience.iop.org/article/10.1088/1361-6382/ab4726 info:eu-repo/semantics/altIdentifier/doi/10.1088/1361-6382/ab4726 info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/1906.08959 |
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 |
dc.publisher.none.fl_str_mv |
IOP Publishing |
publisher.none.fl_str_mv |
IOP Publishing |
dc.source.none.fl_str_mv |
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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1844613625231179776 |
score |
13.070432 |