Precession of neutrino-cooled accretion disks in gamma-ray burst engines

Autores
Reynoso, Matias Miguel; Romero, Gustavo Esteban; Sampayo, Oscar Alfredo
Año de publicación
2006
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Aims. We study the precession of accretion disks in the context of gamma-ray burst inner engines. Methods. With an accretion disk model that allows for neutrino cooling, we evaluate the possible periods of disk precession and nutation due to the Lense-Thirring effect. Results. Assuming jet ejection perpendicular to the disk midplane and a typical intrinsic time dependence for the burst, we find possible gamma-ray light curves with a temporal microstructure similar to what is observed in some subsamples. Conclusions. We conclude that the precession and nutation of a neutrino-cooled accretion disk in the burst engine might be responsible for some events, especially those with a slow rise and a fast decay.
Fil: Reynoso, Matias Miguel. Universidad Nacional de Mar del Plata; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Sampayo, Oscar Alfredo. Universidad Nacional de Mar del Plata; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Materia
Gamma ray bursts
Precession
Neutrino astrophysics
Accretion disks
Black hole physics
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/27846

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network_name_str CONICET Digital (CONICET)
spelling Precession of neutrino-cooled accretion disks in gamma-ray burst enginesReynoso, Matias MiguelRomero, Gustavo EstebanSampayo, Oscar AlfredoGamma ray burstsPrecessionNeutrino astrophysicsAccretion disksBlack hole physicshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Aims. We study the precession of accretion disks in the context of gamma-ray burst inner engines. Methods. With an accretion disk model that allows for neutrino cooling, we evaluate the possible periods of disk precession and nutation due to the Lense-Thirring effect. Results. Assuming jet ejection perpendicular to the disk midplane and a typical intrinsic time dependence for the burst, we find possible gamma-ray light curves with a temporal microstructure similar to what is observed in some subsamples. Conclusions. We conclude that the precession and nutation of a neutrino-cooled accretion disk in the burst engine might be responsible for some events, especially those with a slow rise and a fast decay.Fil: Reynoso, Matias Miguel. Universidad Nacional de Mar del Plata; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: Sampayo, Oscar Alfredo. Universidad Nacional de Mar del Plata; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaEDP Sciences2006-07info: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/11336/27846Reynoso, Matias Miguel; Romero, Gustavo Esteban; Sampayo, Oscar Alfredo; Precession of neutrino-cooled accretion disks in gamma-ray burst engines; EDP Sciences; Astronomy and Astrophysics; 454; 7-2006; 11-160004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20054564info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2006/28/aa4564-05/aa4564-05.htmlinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:46:41Zoai:ri.conicet.gov.ar:11336/27846instacron: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 10:46:42.012CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Precession of neutrino-cooled accretion disks in gamma-ray burst engines
title Precession of neutrino-cooled accretion disks in gamma-ray burst engines
spellingShingle Precession of neutrino-cooled accretion disks in gamma-ray burst engines
Reynoso, Matias Miguel
Gamma ray bursts
Precession
Neutrino astrophysics
Accretion disks
Black hole physics
title_short Precession of neutrino-cooled accretion disks in gamma-ray burst engines
title_full Precession of neutrino-cooled accretion disks in gamma-ray burst engines
title_fullStr Precession of neutrino-cooled accretion disks in gamma-ray burst engines
title_full_unstemmed Precession of neutrino-cooled accretion disks in gamma-ray burst engines
title_sort Precession of neutrino-cooled accretion disks in gamma-ray burst engines
dc.creator.none.fl_str_mv Reynoso, Matias Miguel
Romero, Gustavo Esteban
Sampayo, Oscar Alfredo
author Reynoso, Matias Miguel
author_facet Reynoso, Matias Miguel
Romero, Gustavo Esteban
Sampayo, Oscar Alfredo
author_role author
author2 Romero, Gustavo Esteban
Sampayo, Oscar Alfredo
author2_role author
author
dc.subject.none.fl_str_mv Gamma ray bursts
Precession
Neutrino astrophysics
Accretion disks
Black hole physics
topic Gamma ray bursts
Precession
Neutrino astrophysics
Accretion disks
Black hole physics
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Aims. We study the precession of accretion disks in the context of gamma-ray burst inner engines. Methods. With an accretion disk model that allows for neutrino cooling, we evaluate the possible periods of disk precession and nutation due to the Lense-Thirring effect. Results. Assuming jet ejection perpendicular to the disk midplane and a typical intrinsic time dependence for the burst, we find possible gamma-ray light curves with a temporal microstructure similar to what is observed in some subsamples. Conclusions. We conclude that the precession and nutation of a neutrino-cooled accretion disk in the burst engine might be responsible for some events, especially those with a slow rise and a fast decay.
Fil: Reynoso, Matias Miguel. Universidad Nacional de Mar del Plata; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Sampayo, Oscar Alfredo. Universidad Nacional de Mar del Plata; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
description Aims. We study the precession of accretion disks in the context of gamma-ray burst inner engines. Methods. With an accretion disk model that allows for neutrino cooling, we evaluate the possible periods of disk precession and nutation due to the Lense-Thirring effect. Results. Assuming jet ejection perpendicular to the disk midplane and a typical intrinsic time dependence for the burst, we find possible gamma-ray light curves with a temporal microstructure similar to what is observed in some subsamples. Conclusions. We conclude that the precession and nutation of a neutrino-cooled accretion disk in the burst engine might be responsible for some events, especially those with a slow rise and a fast decay.
publishDate 2006
dc.date.none.fl_str_mv 2006-07
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/11336/27846
Reynoso, Matias Miguel; Romero, Gustavo Esteban; Sampayo, Oscar Alfredo; Precession of neutrino-cooled accretion disks in gamma-ray burst engines; EDP Sciences; Astronomy and Astrophysics; 454; 7-2006; 11-16
0004-6361
CONICET Digital
CONICET
url http://hdl.handle.net/11336/27846
identifier_str_mv Reynoso, Matias Miguel; Romero, Gustavo Esteban; Sampayo, Oscar Alfredo; Precession of neutrino-cooled accretion disks in gamma-ray burst engines; EDP Sciences; Astronomy and Astrophysics; 454; 7-2006; 11-16
0004-6361
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20054564
info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2006/28/aa4564-05/aa4564-05.html
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
application/pdf
application/pdf
dc.publisher.none.fl_str_mv EDP Sciences
publisher.none.fl_str_mv EDP Sciences
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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