TY - JOUR
T1 - Neutrino burst from SN1987A and the solar-neutrino puzzle
AU - Arafune, J.
AU - Fukugita, M.
AU - Yanagida, T.
AU - Yoshimura, M.
N1 - Copyright:
Copyright 2015 Elsevier B.V., All rights reserved.
PY - 1987
Y1 - 1987
N2 - The prompt signal from the supernova explosion in the Large Magellanic Cloud presumably detected by Kamiokande II does not necessarily mean that the Mikheyev-Smirnov-Wolfenstein 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 flux from the progenitor can directly hit the detector, saving the Mikheyev-Smirnov-Wolfenstein explanation of the solar-neutrino problem for a range of mixing parameters.
AB - The prompt signal from the supernova explosion in the Large Magellanic Cloud presumably detected by Kamiokande II does not necessarily mean that the Mikheyev-Smirnov-Wolfenstein 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 flux from the progenitor can directly hit the detector, saving the Mikheyev-Smirnov-Wolfenstein explanation of the solar-neutrino problem for a range of mixing parameters.
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U2 - 10.1103/PhysRevLett.59.1864
DO - 10.1103/PhysRevLett.59.1864
M3 - Article
AN - SCOPUS:33748652657
SN - 0031-9007
VL - 59
SP - 1864
EP - 1867
JO - Physical Review Letters
JF - Physical Review Letters
IS - 16
ER -