High-energy emission as signature of magnetic field amplification in neutron star mergers

Autores
Fraija Cabrera, Nissim Illich; Lee, William Henry; Veres, Peter; Barniol Duran, Rodolfo
Año de publicación
2015
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
The merger of a binary neutron star system is suggested as the central engine of short gamma-ray bursts (sGRBs). For the merger process, simulations predict that magnetic field is amplified beyond magnetar field strength by Kelvin-Helmholtz instabilities. With the Large Area Telescope (LAT), bursts have been detected that show a temporally extended component in coincidence with a short-lasting peak at the end of the prompt phase. We show that the presence of these LAT components in a sGRB could provide evidence of magnetic field amplification in the neutron star merger.
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Ciencias Astronómicas
binary neutron star system
short gamma-ray bursts
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/167889
Acceder
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oai_identifier_str oai:sedici.unlp.edu.ar:10915/167889
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network_name_str SEDICI (UNLP)
spelling High-energy emission as signature of magnetic field amplification in neutron star mergersFraija Cabrera, Nissim IllichLee, William HenryVeres, PeterBarniol Duran, RodolfoCiencias Astronómicasbinary neutron star systemshort gamma-ray burstsThe merger of a binary neutron star system is suggested as the central engine of short gamma-ray bursts (sGRBs). For the merger process, simulations predict that magnetic field is amplified beyond magnetar field strength by Kelvin-Helmholtz instabilities. With the Large Area Telescope (LAT), bursts have been detected that show a temporally extended component in coincidence with a short-lasting peak at the end of the prompt phase. We show that the presence of these LAT components in a sGRB could provide evidence of magnetic field amplification in the neutron star merger.Facultad de Ciencias Astronómicas y Geofísicas2015-10info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionObjeto de conferenciahttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdf49-54http://sedici.unlp.edu.ar/handle/10915/167889enginfo:eu-repo/semantics/altIdentifier/isbn/978-987-24948-3-4info:eu-repo/semantics/reference/url/https://sedici.unlp.edu.ar/handle/10915/167830info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-15T11:36:31Zoai:sedici.unlp.edu.ar:10915/167889Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-15 11:36:31.372SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv High-energy emission as signature of magnetic field amplification in neutron star mergers
title High-energy emission as signature of magnetic field amplification in neutron star mergers
spellingShingle High-energy emission as signature of magnetic field amplification in neutron star mergers
Fraija Cabrera, Nissim Illich
Ciencias Astronómicas
binary neutron star system
short gamma-ray bursts
title_short High-energy emission as signature of magnetic field amplification in neutron star mergers
title_full High-energy emission as signature of magnetic field amplification in neutron star mergers
title_fullStr High-energy emission as signature of magnetic field amplification in neutron star mergers
title_full_unstemmed High-energy emission as signature of magnetic field amplification in neutron star mergers
title_sort High-energy emission as signature of magnetic field amplification in neutron star mergers
dc.creator.none.fl_str_mv Fraija Cabrera, Nissim Illich
Lee, William Henry
Veres, Peter
Barniol Duran, Rodolfo
author Fraija Cabrera, Nissim Illich
author_facet Fraija Cabrera, Nissim Illich
Lee, William Henry
Veres, Peter
Barniol Duran, Rodolfo
author_role author
author2 Lee, William Henry
Veres, Peter
Barniol Duran, Rodolfo
author2_role author
author
author
dc.subject.none.fl_str_mv Ciencias Astronómicas
binary neutron star system
short gamma-ray bursts
topic Ciencias Astronómicas
binary neutron star system
short gamma-ray bursts
dc.description.none.fl_txt_mv The merger of a binary neutron star system is suggested as the central engine of short gamma-ray bursts (sGRBs). For the merger process, simulations predict that magnetic field is amplified beyond magnetar field strength by Kelvin-Helmholtz instabilities. With the Large Area Telescope (LAT), bursts have been detected that show a temporally extended component in coincidence with a short-lasting peak at the end of the prompt phase. We show that the presence of these LAT components in a sGRB could provide evidence of magnetic field amplification in the neutron star merger.
Facultad de Ciencias Astronómicas y Geofísicas
description The merger of a binary neutron star system is suggested as the central engine of short gamma-ray bursts (sGRBs). For the merger process, simulations predict that magnetic field is amplified beyond magnetar field strength by Kelvin-Helmholtz instabilities. With the Large Area Telescope (LAT), bursts have been detected that show a temporally extended component in coincidence with a short-lasting peak at the end of the prompt phase. We show that the presence of these LAT components in a sGRB could provide evidence of magnetic field amplification in the neutron star merger.
publishDate 2015
dc.date.none.fl_str_mv 2015-10
dc.type.none.fl_str_mv info:eu-repo/semantics/conferenceObject
info:eu-repo/semantics/publishedVersion
Objeto de conferencia
http://purl.org/coar/resource_type/c_5794
info:ar-repo/semantics/documentoDeConferencia
format conferenceObject
status_str publishedVersion
dc.identifier.none.fl_str_mv http://sedici.unlp.edu.ar/handle/10915/167889
url http://sedici.unlp.edu.ar/handle/10915/167889
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/isbn/978-987-24948-3-4
info:eu-repo/semantics/reference/url/https://sedici.unlp.edu.ar/handle/10915/167830
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.format.none.fl_str_mv application/pdf
49-54
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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score 13.22299

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