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

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

2008-10-02

arxiv.org/abs/0810.0456v1

Astron.Lett.35:1-6,2009.

Astronomy and Astrophysics

Astrophysics

5 pages, 5 figures. Accepted for publication in Astronomy Letters

Scientific paper

10.1134/S1063773709010010

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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