Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube

Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-thermal high-energy emission. High-energy neutrinos are signatures of such outflows. The detection of gravitational waves...

Descripción completa

Detalles Bibliográficos
Autores: Albert, A., André, Michel|||0000-0002-0091-7279, Anghinolfi, Marco, Ardid Ramírez, Miguel, Aubert, J.-J.
Tipo de recurso: artículo
Fecha de publicación:2019
País:España
Institución:Universitat Politècnica de Catalunya (UPC)
Repositorio:UPCommons. Portal del coneixement obert de la UPC
Idioma:inglés
OAI Identifier:oai:upcommons.upc.edu:2117/128069
Acceso en línea:https://hdl.handle.net/2117/128069
https://dx.doi.org/10.3847/1538-4357/aaf21d
Access Level:acceso abierto
Palabra clave:Astrophysics
Gravitational waves
Neutrinos
Astrofísica
Neutrins
Ones gravitacionals
Àrees temàtiques de la UPC::Física::Astronomia i astrofísica
id ES_68f8dc44e11cddb278e4a9e2dd4f63ee
oai_identifier_str oai:upcommons.upc.edu:2117/128069
network_acronym_str ES
network_name_str España
repository_id_str
spelling Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCubeAlbert, A.André, Michel|||0000-0002-0091-7279Anghinolfi, MarcoArdid Ramírez, MiguelAubert, J.-J.AstrophysicsGravitational wavesNeutrinosGravitational wavesNeutrinosAstrofísicaNeutrinsOnes gravitacionalsÀrees temàtiques de la UPC::Física::Astronomia i astrofísicaAstrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-thermal high-energy emission. High-energy neutrinos are signatures of such outflows. The detection of gravitational waves and high-energy neutrinos from common sources could help establish the connection between the dynamics of the progenitor and the properties of the outflow. We searched for associated emission of gravitational waves and high-energy neutrinos from astrophysical transients with minimal assumptions using data from Advanced LIGO from its first observing run O1, and data from the ANTARES and IceCube neutrino observatories from the same time period. We focused on candidate events whose astrophysical origins could not be determined from a single messenger. We found no significant coincident candidate, which we used to constrain the rate density of astrophysical sources dependent on their gravitational-wave and neutrino emission processesPeer ReviewedInstitute of Physics (IOP)20192019-01-1620192019-02-01journal articlehttp://purl.org/coar/resource_type/c_6501VoRhttp://purl.org/coar/version/c_970fb48d4fbd8a85info:eu-repo/semantics/articleapplication/pdfhttps://hdl.handle.net/2117/128069https://dx.doi.org/10.3847/1538-4357/aaf21dreponame:UPCommons. Portal del coneixement obert de la UPCinstname:Universitat Politècnica de Catalunya (UPC)Inglésengopen accesshttp://purl.org/coar/access_right/c_abf2Attribution-NonCommercial-NoDerivs 3.0 Spainhttp://creativecommons.org/licenses/by-nc-nd/3.0/es/info:eu-repo/semantics/openAccessoai:upcommons.upc.edu:2117/1280692026-05-27T15:37:01Z
dc.title.none.fl_str_mv Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube
title Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube
spellingShingle Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube
Albert, A.
Astrophysics
Gravitational waves
Neutrinos
Gravitational waves
Neutrinos
Astrofísica
Neutrins
Ones gravitacionals
Àrees temàtiques de la UPC::Física::Astronomia i astrofísica
title_short Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube
title_full Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube
title_fullStr Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube
title_full_unstemmed Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube
title_sort Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube
dc.creator.none.fl_str_mv Albert, A.
André, Michel|||0000-0002-0091-7279
Anghinolfi, Marco
Ardid Ramírez, Miguel
Aubert, J.-J.
author Albert, A.
author_facet Albert, A.
André, Michel|||0000-0002-0091-7279
Anghinolfi, Marco
Ardid Ramírez, Miguel
Aubert, J.-J.
author_role author
author2 André, Michel|||0000-0002-0091-7279
Anghinolfi, Marco
Ardid Ramírez, Miguel
Aubert, J.-J.
author2_role author
author
author
author
dc.subject.none.fl_str_mv Astrophysics
Gravitational waves
Neutrinos
Gravitational waves
Neutrinos
Astrofísica
Neutrins
Ones gravitacionals
Àrees temàtiques de la UPC::Física::Astronomia i astrofísica
topic Astrophysics
Gravitational waves
Neutrinos
Gravitational waves
Neutrinos
Astrofísica
Neutrins
Ones gravitacionals
Àrees temàtiques de la UPC::Física::Astronomia i astrofísica
description Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-thermal high-energy emission. High-energy neutrinos are signatures of such outflows. The detection of gravitational waves and high-energy neutrinos from common sources could help establish the connection between the dynamics of the progenitor and the properties of the outflow. We searched for associated emission of gravitational waves and high-energy neutrinos from astrophysical transients with minimal assumptions using data from Advanced LIGO from its first observing run O1, and data from the ANTARES and IceCube neutrino observatories from the same time period. We focused on candidate events whose astrophysical origins could not be determined from a single messenger. We found no significant coincident candidate, which we used to constrain the rate density of astrophysical sources dependent on their gravitational-wave and neutrino emission processes
publishDate 2019
dc.date.none.fl_str_mv 2019
2019-01-16
2019
2019-02-01
dc.type.none.fl_str_mv journal article
http://purl.org/coar/resource_type/c_6501
VoR
http://purl.org/coar/version/c_970fb48d4fbd8a85
dc.type.openaire.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.none.fl_str_mv https://hdl.handle.net/2117/128069
https://dx.doi.org/10.3847/1538-4357/aaf21d
url https://hdl.handle.net/2117/128069
https://dx.doi.org/10.3847/1538-4357/aaf21d
dc.language.none.fl_str_mv Inglés
eng
language_invalid_str_mv Inglés
language eng
dc.rights.none.fl_str_mv open access
http://purl.org/coar/access_right/c_abf2
Attribution-NonCommercial-NoDerivs 3.0 Spain
http://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.rights.openaire.fl_str_mv info:eu-repo/semantics/openAccess
rights_invalid_str_mv open access
http://purl.org/coar/access_right/c_abf2
Attribution-NonCommercial-NoDerivs 3.0 Spain
http://creativecommons.org/licenses/by-nc-nd/3.0/es/
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv Institute of Physics (IOP)
publisher.none.fl_str_mv Institute of Physics (IOP)
dc.source.none.fl_str_mv reponame:UPCommons. Portal del coneixement obert de la UPC
instname:Universitat Politècnica de Catalunya (UPC)
instname_str Universitat Politècnica de Catalunya (UPC)
reponame_str UPCommons. Portal del coneixement obert de la UPC
collection UPCommons. Portal del coneixement obert de la UPC
repository.name.fl_str_mv
repository.mail.fl_str_mv
_version_ 1869409997875576832
score 15.300719