Multimessenger search for sources of gravitational waves and high-energy neutrinos : results for initial LIGO-Virgo and IceCube

Autores: Aartsen, M. G.; Ackermann, M.; Adams, J.; Aguilar, J. A.; Ahlers, M.; Ahrens, M.; Maglione, César Germán; Reula, Oscar Alejandro; Schilman, Mauro; Wolovick, Nicolás; Domínguez, Alfredo Eduardo
Año de publicación: 2014
Idioma: inglés
Tipo de recurso: artículo
Estado: versión publicada
Descripción: Fil: Aartsen, M. G. University of Adelaide. School of Chemistry and Physics; Australia.
Fil: Adams, J. University of Canterbury. Department of Physics and Astronomy; New Zealand.
Fil: Aguilar, J. A. Université de Genéve. Département de physique nucléaire et corpusculaire; Switzerland.
Fil: Ahlers, M. University of Wisconsin. Department of Physics and Wisconsin IceCube Particle Astrophysics Center; United States of America. ,
Fil: Ahrens, M. Stockholm University. Oskar Klein Centre and Department of Physics; Sweden.
Fil: Ackermann, M. Deutsches Elektronen Synchrotron Desy; Deutschland.
Fil: Maglione, César Germán. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina.
Fil: Maglione, César Germán. Argentinian Gravitational Wave Group; Argentina.
Fil: Reula, Oscar Alejandro. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina.
Fil: Reula, Oscar Alejandro. Argentinian Gravitational Wave Group; Argentina.
Fil: Schilman, Mauro. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina.
Fil: Schilman, Mauro. Argentinian Gravitational Wave Group; Argentina.
Fil: Wolovick, Nicolás. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina.
Fil: Wolovick, Nicolás. Argentinian Gravitational Wave Group; Argentina.
Fil: Domínguez, Alfredo Eduardo. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina.
Fil: Domínguez, Alfredo Eduardo. Argentinian Gravitational Wave Group; Argentina.
We report the results of a multimessenger search for coincident signals from the LIGO and Virgo gravitational-wave observatories and the partially completed IceCube high-energy neutrino detector, including periods of joint operation between 2007-2010. These include parts of the 2005-2007 run and the 2009-2010 run for LIGO-Virgo, and IceCube’s observation periods with 22, 59 and 79 strings. We find no significant coincident events, and use the search results to derive upper limits on the rate of joint sources for a range of source emission parameters. For the optimistic assumption of gravitational-wave emission energy of 10−2 Mc 2 at ∼ 150 Hz with ∼ 60 ms duration, and high-energy neutrino emission of 10 51 erg comparable to the isotropic gamma-ray energy of gamma-ray bursts, we limit the source rate below 1.6 × 10−2 Mpc−3 yr−1 . We also examine how combining information from gravitational waves and neutrinos will aid discovery in the advanced gravitational-wave detector era.
publishedVersion
Fil: Aartsen, M. G. University of Adelaide. School of Chemistry and Physics; Australia.
Fil: Adams, J. University of Canterbury. Department of Physics and Astronomy; New Zealand.
Fil: Aguilar, J. A. Université de Genéve. Département de physique nucléaire et corpusculaire; Switzerland.
Fil: Ahlers, M. University of Wisconsin. Department of Physics and Wisconsin IceCube Particle Astrophysics Center; United States of America. ,
Fil: Ahrens, M. Stockholm University. Oskar Klein Centre and Department of Physics; Sweden.
Fil: Ackermann, M. Deutsches Elektronen Synchrotron Desy; Deutschland.
Fil: Maglione, César Germán. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina.
Fil: Maglione, César Germán. Argentinian Gravitational Wave Group; Argentina.
Fil: Reula, Oscar Alejandro. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina.
Fil: Reula, Oscar Alejandro. Argentinian Gravitational Wave Group; Argentina.
Fil: Schilman, Mauro. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina.
Fil: Schilman, Mauro. Argentinian Gravitational Wave Group; Argentina.
Fil: Wolovick, Nicolás. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina.
Fil: Wolovick, Nicolás. Argentinian Gravitational Wave Group; Argentina.
Fil: Domínguez, Alfredo Eduardo. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina.
Fil: Domínguez, Alfredo Eduardo. Argentinian Gravitational Wave Group; Argentina.
Física de partículas y campos
Fuente: ISSN: 0556-2821
Materia: Ondas gravitacionales
Neutrinos
Gravitational waves
LIGO
Virgo
IceCube
Nivel de accesibilidad: acceso abierto
Condiciones de uso
Repositorio
Institución: Universidad Nacional de Córdoba
OAI Identificador: oai:rdu.unc.edu.ar:11086/28361

Acceder

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network_acronym_str	RDUUNC
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network_name_str	Repositorio Digital Universitario (UNC)
spelling	Multimessenger search for sources of gravitational waves and high-energy neutrinos : results for initial LIGO-Virgo and IceCubeAartsen, M. G.Ackermann, M.Adams, J.Aguilar, J. A.Ahlers, M.Ahrens, M.Maglione, César GermánReula, Oscar AlejandroSchilman, MauroWolovick, NicolásDomínguez, Alfredo EduardoOndas gravitacionalesNeutrinosGravitational wavesLIGOVirgoIceCubeFil: Aartsen, M. G. University of Adelaide. School of Chemistry and Physics; Australia.Fil: Adams, J. University of Canterbury. Department of Physics and Astronomy; New Zealand.Fil: Aguilar, J. A. Université de Genéve. Département de physique nucléaire et corpusculaire; Switzerland.Fil: Ahlers, M. University of Wisconsin. Department of Physics and Wisconsin IceCube Particle Astrophysics Center; United States of America. ,Fil: Ahrens, M. Stockholm University. Oskar Klein Centre and Department of Physics; Sweden.Fil: Ackermann, M. Deutsches Elektronen Synchrotron Desy; Deutschland.Fil: Maglione, César Germán. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina.Fil: Maglione, César Germán. Argentinian Gravitational Wave Group; Argentina.Fil: Reula, Oscar Alejandro. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina.Fil: Reula, Oscar Alejandro. Argentinian Gravitational Wave Group; Argentina.Fil: Schilman, Mauro. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina.Fil: Schilman, Mauro. Argentinian Gravitational Wave Group; Argentina.Fil: Wolovick, Nicolás. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina.Fil: Wolovick, Nicolás. Argentinian Gravitational Wave Group; Argentina.Fil: Domínguez, Alfredo Eduardo. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina.Fil: Domínguez, Alfredo Eduardo. Argentinian Gravitational Wave Group; Argentina.We report the results of a multimessenger search for coincident signals from the LIGO and Virgo gravitational-wave observatories and the partially completed IceCube high-energy neutrino detector, including periods of joint operation between 2007-2010. These include parts of the 2005-2007 run and the 2009-2010 run for LIGO-Virgo, and IceCube’s observation periods with 22, 59 and 79 strings. We find no significant coincident events, and use the search results to derive upper limits on the rate of joint sources for a range of source emission parameters. For the optimistic assumption of gravitational-wave emission energy of 10−2 Mc 2 at ∼ 150 Hz with ∼ 60 ms duration, and high-energy neutrino emission of 10 51 erg comparable to the isotropic gamma-ray energy of gamma-ray bursts, we limit the source rate below 1.6 × 10−2 Mpc−3 yr−1 . We also examine how combining information from gravitational waves and neutrinos will aid discovery in the advanced gravitational-wave detector era.publishedVersionFil: Aartsen, M. G. University of Adelaide. School of Chemistry and Physics; Australia.Fil: Adams, J. University of Canterbury. Department of Physics and Astronomy; New Zealand.Fil: Aguilar, J. A. Université de Genéve. Département de physique nucléaire et corpusculaire; Switzerland.Fil: Ahlers, M. University of Wisconsin. Department of Physics and Wisconsin IceCube Particle Astrophysics Center; United States of America. ,Fil: Ahrens, M. Stockholm University. Oskar Klein Centre and Department of Physics; Sweden.Fil: Ackermann, M. Deutsches Elektronen Synchrotron Desy; Deutschland.Fil: Maglione, César Germán. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina.Fil: Maglione, César Germán. Argentinian Gravitational Wave Group; Argentina.Fil: Reula, Oscar Alejandro. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina.Fil: Reula, Oscar Alejandro. Argentinian Gravitational Wave Group; Argentina.Fil: Schilman, Mauro. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina.Fil: Schilman, Mauro. Argentinian Gravitational Wave Group; Argentina.Fil: Wolovick, Nicolás. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina.Fil: Wolovick, Nicolás. Argentinian Gravitational Wave Group; Argentina.Fil: Domínguez, Alfredo Eduardo. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina.Fil: Domínguez, Alfredo Eduardo. Argentinian Gravitational Wave Group; Argentina.Física de partículas y campos2014-11-17info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://hdl.handle.net/11086/28361https://doi.org/10.1103/PhysRevD.90.102002ISSN: 0556-2821reponame:Repositorio Digital Universitario (UNC)instname:Universidad Nacional de Córdobainstacron:UNCenghttps://doi.org/10.48550/arXiv.1407.1042info:eu-repo/semantics/openAccess2025-09-04T12:34:02Zoai:rdu.unc.edu.ar:11086/28361Institucionalhttps://rdu.unc.edu.ar/Universidad públicaNo correspondehttp://rdu.unc.edu.ar/oai/snrdoca.unc@gmail.comArgentinaNo correspondeNo correspondeNo correspondeopendoar:25722025-09-04 12:34:02.598Repositorio Digital Universitario (UNC) - Universidad Nacional de Córdobafalse
dc.title.none.fl_str_mv	Multimessenger search for sources of gravitational waves and high-energy neutrinos : results for initial LIGO-Virgo and IceCube
title	Multimessenger search for sources of gravitational waves and high-energy neutrinos : results for initial LIGO-Virgo and IceCube
spellingShingle	Multimessenger search for sources of gravitational waves and high-energy neutrinos : results for initial LIGO-Virgo and IceCube Aartsen, M. G. Ondas gravitacionales Neutrinos Gravitational waves LIGO Virgo IceCube
title_short	Multimessenger search for sources of gravitational waves and high-energy neutrinos : results for initial LIGO-Virgo and IceCube
title_full	Multimessenger search for sources of gravitational waves and high-energy neutrinos : results for initial LIGO-Virgo and IceCube
title_fullStr	Multimessenger search for sources of gravitational waves and high-energy neutrinos : results for initial LIGO-Virgo and IceCube
title_full_unstemmed	Multimessenger search for sources of gravitational waves and high-energy neutrinos : results for initial LIGO-Virgo and IceCube
title_sort	Multimessenger search for sources of gravitational waves and high-energy neutrinos : results for initial LIGO-Virgo and IceCube
dc.creator.none.fl_str_mv	Aartsen, M. G. Ackermann, M. Adams, J. Aguilar, J. A. Ahlers, M. Ahrens, M. Maglione, César Germán Reula, Oscar Alejandro Schilman, Mauro Wolovick, Nicolás Domínguez, Alfredo Eduardo
author	Aartsen, M. G.
author_facet	Aartsen, M. G. Ackermann, M. Adams, J. Aguilar, J. A. Ahlers, M. Ahrens, M. Maglione, César Germán Reula, Oscar Alejandro Schilman, Mauro Wolovick, Nicolás Domínguez, Alfredo Eduardo
author_role	author
author2	Ackermann, M. Adams, J. Aguilar, J. A. Ahlers, M. Ahrens, M. Maglione, César Germán Reula, Oscar Alejandro Schilman, Mauro Wolovick, Nicolás Domínguez, Alfredo Eduardo
author2_role	author author author author author author author author author author
dc.subject.none.fl_str_mv	Ondas gravitacionales Neutrinos Gravitational waves LIGO Virgo IceCube
topic	Ondas gravitacionales Neutrinos Gravitational waves LIGO Virgo IceCube
dc.description.none.fl_txt_mv	Fil: Aartsen, M. G. University of Adelaide. School of Chemistry and Physics; Australia. Fil: Adams, J. University of Canterbury. Department of Physics and Astronomy; New Zealand. Fil: Aguilar, J. A. Université de Genéve. Département de physique nucléaire et corpusculaire; Switzerland. Fil: Ahlers, M. University of Wisconsin. Department of Physics and Wisconsin IceCube Particle Astrophysics Center; United States of America. , Fil: Ahrens, M. Stockholm University. Oskar Klein Centre and Department of Physics; Sweden. Fil: Ackermann, M. Deutsches Elektronen Synchrotron Desy; Deutschland. Fil: Maglione, César Germán. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina. Fil: Maglione, César Germán. Argentinian Gravitational Wave Group; Argentina. Fil: Reula, Oscar Alejandro. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina. Fil: Reula, Oscar Alejandro. Argentinian Gravitational Wave Group; Argentina. Fil: Schilman, Mauro. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina. Fil: Schilman, Mauro. Argentinian Gravitational Wave Group; Argentina. Fil: Wolovick, Nicolás. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina. Fil: Wolovick, Nicolás. Argentinian Gravitational Wave Group; Argentina. Fil: Domínguez, Alfredo Eduardo. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina. Fil: Domínguez, Alfredo Eduardo. Argentinian Gravitational Wave Group; Argentina. We report the results of a multimessenger search for coincident signals from the LIGO and Virgo gravitational-wave observatories and the partially completed IceCube high-energy neutrino detector, including periods of joint operation between 2007-2010. These include parts of the 2005-2007 run and the 2009-2010 run for LIGO-Virgo, and IceCube’s observation periods with 22, 59 and 79 strings. We find no significant coincident events, and use the search results to derive upper limits on the rate of joint sources for a range of source emission parameters. For the optimistic assumption of gravitational-wave emission energy of 10−2 Mc 2 at ∼ 150 Hz with ∼ 60 ms duration, and high-energy neutrino emission of 10 51 erg comparable to the isotropic gamma-ray energy of gamma-ray bursts, we limit the source rate below 1.6 × 10−2 Mpc−3 yr−1 . We also examine how combining information from gravitational waves and neutrinos will aid discovery in the advanced gravitational-wave detector era. publishedVersion Fil: Aartsen, M. G. University of Adelaide. School of Chemistry and Physics; Australia. Fil: Adams, J. University of Canterbury. Department of Physics and Astronomy; New Zealand. Fil: Aguilar, J. A. Université de Genéve. Département de physique nucléaire et corpusculaire; Switzerland. Fil: Ahlers, M. University of Wisconsin. Department of Physics and Wisconsin IceCube Particle Astrophysics Center; United States of America. , Fil: Ahrens, M. Stockholm University. Oskar Klein Centre and Department of Physics; Sweden. Fil: Ackermann, M. Deutsches Elektronen Synchrotron Desy; Deutschland. Fil: Maglione, César Germán. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina. Fil: Maglione, César Germán. Argentinian Gravitational Wave Group; Argentina. Fil: Reula, Oscar Alejandro. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina. Fil: Reula, Oscar Alejandro. Argentinian Gravitational Wave Group; Argentina. Fil: Schilman, Mauro. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina. Fil: Schilman, Mauro. Argentinian Gravitational Wave Group; Argentina. Fil: Wolovick, Nicolás. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina. Fil: Wolovick, Nicolás. Argentinian Gravitational Wave Group; Argentina. Fil: Domínguez, Alfredo Eduardo. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina. Fil: Domínguez, Alfredo Eduardo. Argentinian Gravitational Wave Group; Argentina. Física de partículas y campos
description	Fil: Aartsen, M. G. University of Adelaide. School of Chemistry and Physics; Australia.
publishDate	2014
dc.date.none.fl_str_mv	2014-11-17
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/11086/28361 https://doi.org/10.1103/PhysRevD.90.102002
url	http://hdl.handle.net/11086/28361 https://doi.org/10.1103/PhysRevD.90.102002
dc.language.none.fl_str_mv	eng
language	eng
dc.relation.none.fl_str_mv	https://doi.org/10.48550/arXiv.1407.1042
dc.rights.none.fl_str_mv	info:eu-repo/semantics/openAccess
eu_rights_str_mv	openAccess
dc.format.none.fl_str_mv	application/pdf
dc.source.none.fl_str_mv	ISSN: 0556-2821 reponame:Repositorio Digital Universitario (UNC) instname:Universidad Nacional de Córdoba instacron:UNC
reponame_str	Repositorio Digital Universitario (UNC)
collection	Repositorio Digital Universitario (UNC)
instname_str	Universidad Nacional de Córdoba
instacron_str	UNC
institution	UNC
repository.name.fl_str_mv	Repositorio Digital Universitario (UNC) - Universidad Nacional de Córdoba
repository.mail.fl_str_mv	oca.unc@gmail.com
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Multimessenger search for sources of gravitational waves and high-energy neutrinos : results for initial LIGO-Virgo and IceCube

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