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Features of Kamiokande-II, IMB and Baksan observations and their interpretation in a two-component model for the signal

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arxiv 0810.0456 v1 pith:PZU23UJT submitted 2008-10-02 astro-ph

Giulia Pagliaroli , Francesco Vissani This is my paper · ORCID
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keywords expectationsinterpretationmodelsignalagreementangularantineutrinoapplied
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We consider the time, angular and energy distributions of SN1987A events discussing the quality of their agreement with the expectations. A global interpretation is performed considering a simple model, based on the standard scenario for the explosion. Despite the contrasting and confusing indications, a straightforward fit to the data provides a result that does not contradict but rather supports the expectations. The calculated electron antineutrino flux is applied to predict the relic neutrino signal.

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  1. The flux of electron antineutrinos from supernova SN1987A data

    hep-ph 2025-01 conditional novelty 4.0 of 10

    A refined fit of the SN1987A antineutrino data finds accretion at about 99% confidence and a small, theory-compatible neutron fraction, closing a tension in older analyses.

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