2021
DOI: 10.48550/arxiv.2105.13160
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Probing neutrino emission at GeV energies from compact binary mergers with the IceCube Neutrino Observatory

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Cited by 9 publications
(29 citation statements)
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“…This upcoming analysis will provide additional information, complimentary to the analyses with high-energy neutrinos presented here. Additionally, a search for extremely low-energy neutrinos, with 0.5-5 GeV energies, from IceCube was conducted and found no significant emission of neutrinos (Abbasi et al 2021).…”
Section: Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…This upcoming analysis will provide additional information, complimentary to the analyses with high-energy neutrinos presented here. Additionally, a search for extremely low-energy neutrinos, with 0.5-5 GeV energies, from IceCube was conducted and found no significant emission of neutrinos (Abbasi et al 2021).…”
Section: Discussionmentioning
confidence: 99%
“…Following the first confident GW observation (Abbott et al 2016), several attempts from IceCube andAstronomy with a Neutrino Telescope and Abyss environmental RESearch (ANTARES) have not found significant emission of coincident high-energy neutrinos (Albert et al 2017a;Albert et al 2017b;Albert et al 2020;Aartsen et al 2020;Veske et al 2021b). Searches for neutrinos in the low-energy regime have also been conducted by IceCube (Abbasi et al 2021), Super-Kamioka Neutrino Detection Experiment (SuperKamiokande; Abe et al 2021a),Kamioka Liquid-scintillator Anti-Neutrino Detector(KamLAND; Abe et al 2021b), and Borexino (Agostini et al 2017).…”
Section: Introductionmentioning
confidence: 99%
“…see the appendix of Abbasi et al (2023b). The upper limit obtained with ELOWEN, an extremely low energy search with IceCube (Abbasi et al 2021), is also shown in the figure and is seen to be orders of magnitude above the sensitivity of the GRECO Astronomy data set.…”
Section: Analysis Methodsmentioning
confidence: 65%
“…No significant emission was found in any of these searches using high-energy neutrinos (Aartsen et al 2020;Abbasi et al 2023a). IceCube's search for neutrinos in the MeV-GeV energy range did not return any significant observation and has constrained the neutrino emission from GW sources at these energies (Abbasi et al 2021). Searches from other detectors like ANTARES (Albert et al 2020), KamLAND , Super-Kamiokande Borexino (Agostini et al 2017) did not yield any significant detection either.…”
Section: Introductionmentioning
confidence: 99%
“…The famous multimessenger detection of the gravitational-wave (GW) event GW170817 associated with a GRB and a kilonova/macronova was followed up by neutrino telescopes (92,93,94). Other GW events -GW170104(95), GW15226 (96) and GW150914 (97) -were also analyzed in search for neutrino counterparts, as well as entire runs of LIGO and Virgo (98,99,100,101). No associated neutrino emission was identified in these searches, and upper limits on the neutrino luminosity of these events were derived.…”
Section: Sources Of Other Messengersmentioning
confidence: 99%