Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
1996-05-28
Physics
High Energy Physics
High Energy Physics - Phenomenology
latex file, 10 pages, including 8 postscript figures, Talk given at ``XXXIst Les Rencontres de Moriond- Electroweak Interactio
Scientific paper
We present a generalization of the resonant neutrino conversion in matter, including a random component in the matter density profile. The study is focused on the effect of such matter perturbations upon both large and small mixing angle MSW solutions to the solar neutrino problem. This is carried out both for the active-active $\nu_e \ra \nu_{\mu,\tau}$ as well as active-sterile $\nu_e \ra \nu_s$ conversion channels. We find that the small mixing MSW solution is much more stable (especially in $\delta m^2$) than the large mixing solution. Future solar neutrino experiments, such as Borexino, could probe solar matter density noise at the few percent level.
No associations
LandOfFree
The stability of the MSW solution to the solar neutrino problem with respect to random matter density perturbations 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 The stability of the MSW solution to the solar neutrino problem with respect to random matter density perturbations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The stability of the MSW solution to the solar neutrino problem with respect to random matter density perturbations will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-602662