Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory
Author(s)ANTARES Collaboration; IceCube Collaboration; Pierre Auger Collaboration; LIGO Scientific Collaboration; Virgo Collaboration; Arguelles Delgado, Carlos A; Axani, Spencer Nicholas; Collin, G. H.; Conrad, Janet Marie; Moulai, Marjon H.; Aggarwal, Nancy; Barsotti, Lisa; Biscans, Sebastien; Buikema, Aaron; Demos, Nicholas; Donovan, Frederick J; Eisenstein, Robert Alan; Essick, Reed Clasey; Evans, Matthew J; Fernandez Galiana, Alvaro-Miguel; Fritschel, Peter K; Gras, Slawomir; Hall, Evan D.; Katsavounidis, Erotokritos; Kontos, Antonios; Lanza Jr, Robert K; Lynch, Ryan Christopher; MacInnis, Myron E; Martynov, Denis; Mason, Kenneth R; Matichard, Fabrice; Mavalvala, Nergis; McCuller, Lee P; Miller, John; Mittleman, Richard K; Ray Pitambar Mohapatra, Satyanarayan; Shoemaker, David H; Tse, Maggie; Vitale, Salvatore; Weiss, Rainer; Yu, Hang; Yu, Haocun; Zucker, Michael E; ... Show more Show less
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The 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 Fermi Gamma-ray Burst Monitor (Fermi-GBM), and the Anti-Coincidence Shield for the Spectrometer for the International Gamma-Ray Astrophysics Laboratory (INTEGRAL), 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.
DepartmentKavli Institute for Astrophysics and Space Research; Massachusetts Institute of Technology. Department of Physics; Massachusetts Institute of Technology. Laboratory for Nuclear Science
American Astronomical Society
Albert, A. et al. “Search for High-Energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory.” The Astrophysical Journal 850, 2 (November 2017): L35 © 2017 The American Astronomical Society
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