17-keV neutrino, solar-neutrino puzzle, and supernova 1987A

Details 17-keV neutrino, solar-neutrino puzzle, and supernova 1987A 17-keV neutrino, solar-neutrino puzzle, and supernova 1987A

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phrvd..45.1628c&link_type=abstract

Physical Review D (Particles and Fields), Volume 45, Issue 5, 1 March 1992, pp.1628-1635

Mathematics

Logic

7

Quark And Lepton Masses And Mixing, Supernovae

Scientific paper

We present a model of the 17-keV neutrino which naturally admits Mikheyev-Smirnov-Wolfenstein oscillations of νe and νμ in the Sun, while avoiding forbidden ντ-ν¯τ oscillations. Alternatively, the large mixing angle needed for vacuum oscillations to reduce the solar νe flux can be explained, in which case the νe mass might naturally be close to its laboratory limit. The model is consistent with all known laboratory, cosmological, and astrophysical constraints, including the supernova bound on Dirac neutrino masses.

Affiliated with

Also associated with

No associations

Rating

17-keV neutrino, solar-neutrino puzzle, and supernova 1987A does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with 17-keV neutrino, solar-neutrino puzzle, and supernova 1987A, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and 17-keV neutrino, solar-neutrino puzzle, and supernova 1987A will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1490836