Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory

dc.creatorDova, María Teresa
dc.creatorHansen, Patricia María
dc.creatorMariazzi, Analisa Gabriela
dc.creatorSciutto, Sergio Juan
dc.creatorTueros, Matías Jorge
dc.creatorVergara Quispe, Indira Dajhana
dc.creatorWahlberg, Hernán Pablo
dc.creatorANTARES Collaboration
dc.creatorIceCube Collaboration
dc.creatorThe Pierre Auger Collaboration
dc.creatorLIGO Scientific Collaboration
dc.creatorVirgo Collaboration
dc.date2017
dc.date2019-12-11T14:46:48Z
dc.date.accessioned2023-07-14T17:40:52Z
dc.date.available2023-07-14T17:40:52Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/87230
dc.identifierissn:2041-8205
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7428424
dc.descriptionThe Advanced LIGO and Advanced Virgo observatories recently discovered gravitational waves from a binary neutron star inspiral. A short gamma-ray burst (GRB) that followed the merger of this binary was also recorded by the <i>Fermi</i> Gamma-ray Burst Monitor (<i>Fermi</i>-GBM), and the Anti-Coincidence Shield for the Spectrometer for the <i>International Gamma-Ray Astrophysics Laboratory</i> (<i>INTEGRAL</i>), indicating particle acceleration by the source. The precise location of the event was determined by optical detections of emission following the merger. We searched for high-energy neutrinos from the merger in the GeV-EeV energy range using the Antares, IceCube, and Pierre Auger Observatories. No neutrinos directionally coincident with the source were detected within ± 500 s around the merger time. Additionally, no MeV neutrino burst signal was detected coincident with the merger. We further carried out an extended search in the direction of the source for high-energy neutrinos within the 14 day period following the merger, but found no evidence of emission. We used these results to probe dissipation mechanisms in relativistic outflows driven by the binary neutron star merger. The non-detection is consistent with model predictions of short GRBs observed at a large off-axis angle.
dc.descriptionLa lista completa de autores que integran el documento puede consultarse en el archivo.
dc.descriptionFacultad de Ciencias Exactas
dc.descriptionInstituto de Física La Plata
dc.formatapplication/pdf
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by/3.0/
dc.rightsCreative Commons Attribution 3.0 Unported (CC BY 3.0)
dc.subjectCiencias Exactas
dc.subjectFísica
dc.subjectgamma-ray burst: general
dc.subjectgravitational waves
dc.subjectneutrinos
dc.titleSearch for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory
dc.typeArticulo
dc.typeArticulo


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