Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
1999-09-18
Physics
High Energy Physics
High Energy Physics - Phenomenology
4 pages, 1 postscript figure, 1 gif figure
Scientific paper
We have numerically computed survival probabilities of solar neutrinos interacting with matter via MSW mechanism in the full three generation formalism with $\Delta m^2_{23}=2.2\times 10^{-3}$ eV$^2$. For $\theta_{13} \lesssim 30^{\circ}$, we confirm the two regions found in the two generation case, (1) with the most likelyhood, small $\sin^2(2\theta_{12}) \sim 0.006$, (2) with less likelyhood, large $\sin^2(2\theta_{12}) \gtrsim 0.5$. For $\theta_{13}\gtrsim 30^{\circ}$, we find an additional region, (3) with even less likelyhood, $10^{-5} < \Delta m^2_{12}< 10^{-4}$ eV$^2$ and/or $10^{-4} < \sin^2(2\theta_{12}) < 0.5$. Assuming that the case (1) is valid, we predict that $\theta_{13} \simeq 15^\circ$.
Kim Chung Wook
Kim Jai Sam
No associations
LandOfFree
Full Numerical Estimation of Neutrino Mixing Parameters from Solar Neutrino Data 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 Full Numerical Estimation of Neutrino Mixing Parameters from Solar Neutrino Data, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Full Numerical Estimation of Neutrino Mixing Parameters from Solar Neutrino Data will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-349871