eCite Digital Repository
Search for high-energy neutrinos from binary neutron star merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory
Citation
Albert, A and Andre, M and Siellez, K and Zweizig, J, ANTARES Collaboration, IceCube Collaboration, The Pierre Auger Collaboration, and LIGO Scientific Collaboration and Virgo Collaboration, Search for high-energy neutrinos from binary neutron star merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory, The Astrophysical Journal. Letters, 850, (2) Article L35. ISSN 2041-8205 (2017) [Refereed Article]
 | PDF 802Kb |
Copyright Statement
© 2017. The American Astronomical Society. Licensed under Creative Commons Attribution 3.0 Unported (CC BY 3.0) https://creativecommons.org/licenses/by/3.0/
DOI: doi:10.3847/2041-8213/aa9aed
Abstract
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.
Item Details
| Item Type: | Refereed Article |
|---|---|
| Keywords: | gamma-ray burst, gamma ray, gravitational waves, neutrinos, binary neutron star merger |
| Research Division: | Physical Sciences |
| Research Group: | Astronomical sciences |
| Research Field: | General relativity and gravitational waves |
| Objective Division: | Expanding Knowledge |
| Objective Group: | Expanding knowledge |
| Objective Field: | Expanding knowledge in the physical sciences |
| UTAS Author: | Siellez, K (Dr Karelle Siellez) |
| ID Code: | 151994 |
| Year Published: | 2017 |
| Web of Science® Times Cited: | 108 |
| Deposited By: | Physics |
| Deposited On: | 2022-08-09 |
| Last Modified: | 2022-10-26 |
| Downloads: | 5 View Download Statistics |
Repository Staff Only: item control page