Neutrino burst from SN1987A and the solar-neutrino puzzle

Details Neutrino burst from SN1987A and the solar-neutrino puzzle Neutrino burst from SN1987A and the solar-neutrino puzzle

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987phrvl..59.1864a&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 59, Oct. 19, 1987, p. 1864-1867.

Physics

29

Solar Neutrinos, Supernova 1987A

Scientific paper

The prompt electron neutrino signal from the supernova explosion in the Large Magellanic Cloud presumably detected by Kamiokande II does not necessarily mean that the Mikheyev-Smirnov-Wolfenstein (MSW) effect on the solar-neutrino flux is not operative. The electron neutrino, once rotated to a different-flavor neutrino in the progenitor star, can come back via the matter oscillation effect in the earth, or a residual electron neutrino flux from the progenitor can directly hit the detector, saving the MSW explanation of the solar-neutrino problem for a range of mixing parameters.

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