Resonant spin-flavor precession of solar and supernova neutrinos

Details Resonant spin-flavor precession of solar and supernova neutrinos Resonant spin-flavor precession of solar and supernova neutrinos

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987stin...8829707l&link_type=abstract

Unknown

Physics

Magnetic Fields, Precession, Quantum Chromodynamics, Solar Neutrinos, Spin Dynamics, Supernovae, Flavor (Particle Physics), Stellar Evolution, Stellar Models, Sunspots

Scientific paper

The combined effect of matter and magnetic fields on neutrino spin and flavor precession is examined. We find a potential new kind of resonant solar neutrino conversion NueL yields NuMuR or NutauR (for Dirac neutrinos) or Nue yields Nu-barMu or Nu-bartau or (for Majorana neutrinos). Such a resonance could help account for the lower than expected solar neutrino Nue flux and/or indications of an anti-correlation between fluctuations in the Nue flux and sunspot activity. Consequences of spin-flavor precession for supernova neutrinos are also briefly discussed.

Affiliated with

Also associated with

No associations

Rating

Resonant spin-flavor precession of solar and supernova neutrinos 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 Resonant spin-flavor precession of solar and supernova neutrinos, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Resonant spin-flavor precession of solar and supernova neutrinos will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1763095