2018
DOI: 10.1134/s0021364018240025
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Search for High-Energy Neutrinos from GW170817 with the Baikal-GVD Neutrino Telescope

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Cited by 29 publications
(21 citation statements)
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“…During the third observing run, LIGO-O3, the LIGO/Virgo collaboration initiated the online GW candidate event database (GraceDB) (LIGO Scientific Collaboration 2020), providing public alerts and a centralized location for aggregating and retrieving event information. For such transient GW events, various neutrino detectors reported correlation searches: Super-Kamiokande (Abe et al 2016), Borexino (Agostini et al 2017), NOvA (Acero et al 2020, Bikal-GVD Neutrino Telescope (Avrorin et al 2018), Daya Bay (An et al 2020), XMASS (Collaboration et al 2020), and IceCube/ANTARES (Adrián-Martínez et al 2016;Albert et al 2017b;Aartsen et al 2020). The Kamioka Liquid scintillator AntiNeutrino Detector (KamLAND) has also performed a search for electron antineutrinos in coincident with gravitational waves GW150914 and GW151226, and then candidate event LVT151012 (Gando et al 2016a).…”
Section: Introductionmentioning
confidence: 99%
“…During the third observing run, LIGO-O3, the LIGO/Virgo collaboration initiated the online GW candidate event database (GraceDB) (LIGO Scientific Collaboration 2020), providing public alerts and a centralized location for aggregating and retrieving event information. For such transient GW events, various neutrino detectors reported correlation searches: Super-Kamiokande (Abe et al 2016), Borexino (Agostini et al 2017), NOvA (Acero et al 2020, Bikal-GVD Neutrino Telescope (Avrorin et al 2018), Daya Bay (An et al 2020), XMASS (Collaboration et al 2020), and IceCube/ANTARES (Adrián-Martínez et al 2016;Albert et al 2017b;Aartsen et al 2020). The Kamioka Liquid scintillator AntiNeutrino Detector (KamLAND) has also performed a search for electron antineutrinos in coincident with gravitational waves GW150914 and GW151226, and then candidate event LVT151012 (Gando et al 2016a).…”
Section: Introductionmentioning
confidence: 99%
“…Several searches have been performed for the neutrino counterparts of either binary BH-BH merges or the binary NS-NS merger [19][20][21][22][23][24][25][26][27][28], as summarized in Table 1. However, no significant neutrino signal has been observed by the neutrino telescopes, so far.…”
Section: Neutrino Detectorsmentioning
confidence: 99%
“…Since the two-week-long electromagnetic counterpart after GW170817 was observed [59], ANTARES, IceCube, the Pierre Auger Observatory, and Baikal-GVDhave searched for neutrino signals with two different time windows [19,24]; one is ±500 s around the merger to search for neutrinos associated with prompt and extended gamma-ray emissions [60][61][62], and the other is 14 days after the merger to search for longer-lived emission processes [63].…”
Section: Introductionmentioning
confidence: 99%
“…At this time, neutrinos are still missing from the multimessenger picture of mergers [11][12][13][14]. Neutrino production is expected in compact-object mergers, i.e., binary neutron star (BNS) and neutron-star-black hole (NSBH) mergers.…”
Section: Introductionmentioning
confidence: 99%