Full Numerical Estimation of Neutrino Mixing Parameters from Solar Neutrino Data
| dc.creator | Kim, Jai Sam | |
| dc.creator | Kim, C. W. | |
| dc.date | 1999-09-18 | |
| dc.date.accessioned | 2026-07-07T04:08:07Z | |
| dc.date.available | 2026-07-07T04:08:07Z | |
| dc.description | We have numerically computed survival probabilities of solar neutrinos interacting with matter via MSW mechanism in the full three generation formalism with $Δm^2_{23}=2.2\times 10^{-3}$ eV$^2$. For $θ_{13} \lesssim 30^{\circ}$, we confirm the two regions found in the two generation case, (1) with the most likelyhood, small $\sin^2(2θ_{12}) \sim 0.006$, (2) with less likelyhood, large $\sin^2(2θ_{12}) \gtrsim 0.5$. For $θ_{13}\gtrsim 30^{\circ}$, we find an additional region, (3) with even less likelyhood, $10^{-5} < Δm^2_{12}< 10^{-4}$ eV$^2$ and/or $10^{-4} < \sin^2(2θ_{12}) < 0.5$. Assuming that the case (1) is valid, we predict that $θ_{13} \simeq 15^\circ$. | |
| dc.description | 4 pages, 1 postscript figure, 1 gif figure | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9909428 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9909428 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/49413 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Full Numerical Estimation of Neutrino Mixing Parameters from Solar Neutrino Data | |
| dc.type | text |