A Unique Oscillation Solution to the Solar Neutrino Problem?

Details A Unique Oscillation Solution to the Solar Neutrino Problem? A Unique Oscillation Solution to the Solar Neutrino Problem?

2002-02-08

arxiv.org/abs/hep-ex/0202020v1

Physics

High Energy Physics

High Energy Physics - Experiment

10 pages, 3 figures, to be published in the proceedings of the NOON 2001 workshop

Scientific paper

A global two-neutrino oscillation fit combining Super-Kamiokande solar neutrino data with the solar neutrino rates measured by Homestake, Gallex/GNO, SAGE and SNO prefers a single allowed area, the Large Mixing Angle solution, at about 95% confidence level. The mass^2 difference between the two mass eigenstates is Delta m^2 approx 3-25 x 10^-5 eV^2, the mixing angle theta is tan^2 theta approx 0.21-0.67.

Affiliated with

Also associated with

No associations

Rating

A Unique Oscillation Solution to the Solar Neutrino Problem? 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 A Unique Oscillation Solution to the Solar Neutrino Problem?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Unique Oscillation Solution to the Solar Neutrino Problem? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-591626