Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory
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 fo...
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author | 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 |
author2 | Massachusetts Institute of Technology. Department of Physics |
author_facet | Massachusetts Institute of Technology. Department of Physics 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 |
author_sort | ANTARES Collaboration |
collection | MIT |
description | 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. |
first_indexed | 2024-09-23T14:22:58Z |
format | Article |
id | mit-1721.1/115161 |
institution | Massachusetts Institute of Technology |
last_indexed | 2024-09-23T14:22:58Z |
publishDate | 2018 |
publisher | American Astronomical Society |
record_format | dspace |
spelling | mit-1721.1/1151612022-10-01T20:59:03Z Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory 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 Massachusetts Institute of Technology. Department of Physics Massachusetts Institute of Technology. Laboratory for Nuclear Science MIT Kavli Institute for Astrophysics and Space Research 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 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. 2018-05-02T14:57:18Z 2018-05-02T14:57:18Z 2017-11 2017-11 2018-04-24T13:29:43Z Article http://purl.org/eprint/type/JournalArticle 2041-8213 http://hdl.handle.net/1721.1/115161 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 https://orcid.org/0000-0003-4186-4182 https://orcid.org/0000-0001-8866-3826 https://orcid.org/0000-0002-6393-0438 https://orcid.org/0000-0001-7909-5812 https://orcid.org/0000-0002-0026-3877 https://orcid.org/0000-0002-9635-7527 https://orcid.org/0000-0001-9409-5757 https://orcid.org/0000-0002-3503-2032 https://orcid.org/0000-0001-8196-9267 https://orcid.org/0000-0001-8459-4499 https://orcid.org/0000-0003-1983-3187 https://orcid.org/0000-0001-9018-666X https://orcid.org/0000-0001-6550-3045 https://orcid.org/0000-0002-1347-0680 https://orcid.org/0000-0002-5163-683X https://orcid.org/0000-0003-0219-9706 https://orcid.org/0000-0002-4147-2560 https://orcid.org/0000-0003-1510-4921 https://orcid.org/0000-0003-2700-0767 https://orcid.org/0000-0002-6011-6190 https://orcid.org/0000-0002-2544-1596 http://dx.doi.org/10.3847/2041-8213/AA9AED Astrophysical Journal Creative Commons Attribution 3.0 Unported license http://creativecommons.org/licenses/by/3.0/ application/pdf American Astronomical Society IOP Publishing |
spellingShingle | 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 Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory |
title | Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory |
title_full | Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory |
title_fullStr | Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory |
title_full_unstemmed | Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory |
title_short | Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory |
title_sort | search for high energy neutrinos from binary neutron star merger gw170817 with antares icecube and the pierre auger observatory |
url | http://hdl.handle.net/1721.1/115161 https://orcid.org/0000-0003-4186-4182 https://orcid.org/0000-0001-8866-3826 https://orcid.org/0000-0002-6393-0438 https://orcid.org/0000-0001-7909-5812 https://orcid.org/0000-0002-0026-3877 https://orcid.org/0000-0002-9635-7527 https://orcid.org/0000-0001-9409-5757 https://orcid.org/0000-0002-3503-2032 https://orcid.org/0000-0001-8196-9267 https://orcid.org/0000-0001-8459-4499 https://orcid.org/0000-0003-1983-3187 https://orcid.org/0000-0001-9018-666X https://orcid.org/0000-0001-6550-3045 https://orcid.org/0000-0002-1347-0680 https://orcid.org/0000-0002-5163-683X https://orcid.org/0000-0003-0219-9706 https://orcid.org/0000-0002-4147-2560 https://orcid.org/0000-0003-1510-4921 https://orcid.org/0000-0003-2700-0767 https://orcid.org/0000-0002-6011-6190 https://orcid.org/0000-0002-2544-1596 |
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