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Evidence of High-Energy Neutrinos from SN1987A by Kamiokande-II and IMB

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arxiv 2108.05347 v3 pith:W2IXCDB6 submitted 2021-08-03 hep-ex astro-ph.HE

classification hep-exastro-ph.HE
keywords neutrinoswerehigh-energykamiokande-iirecordedsn1987aupward-goingevents
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High-energy neutrinos from SN1987A were searched for using upward-going muons recorded by the Kamiokande-II experiment and the IMB experiment. Between 1987 August 11 and October 20, and from an angular window of 10 degree radius, two upward-going muon events were recorded by Kamiokande-II, and also two events were recorded by IMB. The probability that these upward-going muons were explained by a chance coincidence of atmospheric neutrinos was calculated to be 0.27%. This shows possible evidence of high-energy neutrinos from SN1987A.

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    Neutrinos from newborn pulsar winds hitting supernova ejecta could be detected from a galactic source by IceCube if B/P^2 exceeds ~0.003, with parameter constraints and a detectable diffuse flux for next-generation te...

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