Adiabatic Analysis of Gravitationally-Induced Three-Flavor Neutrino Oscillations

Details Adiabatic Analysis of Gravitationally-Induced Three-Flavor Neutrino Oscillations Adiabatic Analysis of Gravitationally-Induced Three-Flavor Neutrino Oscillations

1995-01-19

arxiv.org/abs/hep-ph/9501340v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

Latex, 2 postscript figures

Scientific paper

Some implications of the proposal that flavor nondiagonal couplings of neutrinos to gravity might resolve the solar neutrino problem are considered in the context of three neutrino flavours. Using an adiabatic approximation iso-SNU curves are calculated for the neutrinos which most likely contribute to the observed solar neutrino deficiency. We show that results obtained with two-flavor models can be recovered, and discuss the effects of the addition of a third flavor. Some results are obtained for this case, and these values are compared with recent experimental data.

Affiliated with

Also associated with

No associations

Rating

Adiabatic Analysis of Gravitationally-Induced Three-Flavor Neutrino Oscillations 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 Adiabatic Analysis of Gravitationally-Induced Three-Flavor Neutrino Oscillations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Adiabatic Analysis of Gravitationally-Induced Three-Flavor Neutrino Oscillations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-198437