Oscillation-assisted resonance spin-flavor precession and time variations of the solar neutrino flux.

Details Oscillation-assisted resonance spin-flavor precession and time variations of the solar neutrino flux. Oscillation-assisted resonance spin-flavor precession and time variations of the solar neutrino flux.

Jan 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991svjnp..53..132a&link_type=abstract

Sov. J. Nucl. Phys., Vol. 53, No. 1, p. 132 - 135

Physics

Scientific paper

The combined effect of resonance neutrino oscillations and resonance spin-flavor precession in the convective zone of the Sun is studied. It is shown that although the oscillations themselves cannot induce time variations of the solar neutrino flux observed in the 37Cl experiment, they can effectively enhance the resonance spin-flavor precession, which can give rise to such variations. New experimental data on solar neutrinos are also discussed.

Affiliated with

Also associated with

No associations

Rating

Oscillation-assisted resonance spin-flavor precession and time variations of the solar neutrino flux. 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 Oscillation-assisted resonance spin-flavor precession and time variations of the solar neutrino flux., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Oscillation-assisted resonance spin-flavor precession and time variations of the solar neutrino flux. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1896156