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

Roderic Mòbil

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

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dc.contributor.author LIGO Scientific Collaboration
dc.contributor.author Virgo Collaboration
dc.contributor.author Albert, Arnaud
dc.contributor.author Barrios Martí, Javier
dc.contributor.author Coleiro, A.
dc.contributor.author Colomer, M.
dc.contributor.author Hernández Rey, Juan José
dc.contributor.author Illuminati, G.
dc.contributor.author Khan-Chowdhury, N.R.
dc.contributor.author Lotze, M.
dc.contributor.author Zornoza Gómez, Juan de Dios
dc.contributor.author Zúñiga Román, Juan
dc.contributor.author Aloy Toras, Miguel Angel
dc.contributor.author Cerdá Durán, Pablo
dc.contributor.author Cordero Carrión, Isabel
dc.contributor.author Font Roda, José Antonio
dc.contributor.author Marquina Vila, Antonio
dc.contributor.author Obergaulinger, M.
dc.contributor.author Sanchis Gual, Nicolas
dc.contributor.author Torres Forné, Alejandro
dc.contributor.author ANTARES Collaboration
dc.contributor.author IceCube Collaboration
dc.date.accessioned 2020-01-13T14:29:29Z
dc.date.available 2020-01-13T14:29:29Z
dc.date.issued 2019
dc.identifier.uri https://hdl.handle.net/10550/72555
dc.description.abstract 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.
dc.language.iso eng
dc.relation.ispartof Astrophysical Journal, 2019, vol. 870, num. 2, p. 134-1-134-16
dc.rights.uri info:eu-repo/semantics/openAccess
dc.source LIGO Scientific Collaboration Virgo Collaboration Albert, Arnaud Barrios Martí, Javier Coleiro, A. Colomer, M. Hernández Rey, Juan José Illuminati, G. Khan-Chowdhury, N.R. Lotze, M. Zornoza Gómez, Juan de Dios Zúñiga Román, Juan Aloy Toras, Miguel Angel Cerdá Durán, Pablo Cordero Carrión, Isabel Font Roda, José Antonio Marquina Vila, Antonio Obergaulinger, M. Sanchis Gual, Nicolas Torres Forné, Alejandro ANTARES Collaboration IceCube Collaboration 2019 Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube Astrophysical Journal 870 2 134-1 134-16
dc.subject Gravitació
dc.subject Astrofísica
dc.title Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube
dc.type info:eu-repo/semantics/article
dc.date.updated 2020-01-13T14:29:29Z
dc.identifier.doi https://doi.org/10.3847/1538-4357/aaf21d
dc.identifier.idgrec 134014


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Roderic Mòbil