Determination of Solar Neutrino Oscillation Parameters using 1496 Days of Super-Kamiokande-I Data
| dc.creator | Kamiokande Collaboration | |
| dc.date | 2002-05-22 | |
| dc.date.accessioned | 2026-07-07T10:32:11Z | |
| dc.date.available | 2026-07-07T10:32:11Z | |
| dc.description | A number of different fits to solar neutrino mixing and mass square difference were performed using 1496 days of Super-Kamiokande-I's solar neutrino data. These data select two allowed areas at large neutrino mixing when combined with either the solar $^8$B flux prediction of the standard solar model or the SNO interaction rate measurements. A global fit combining SK data with the solar neutrino interaction rates measured by Homestake, SNO, Gallex/GNO and SAGE prefers a single allowed area, the Large Mixing Angle solution, at the 98.9% confidence level. The mass square difference $Δm^2$ between the two mass eigenstates ranges from about 3 to $19\times10^{-5}$eV$^2$, while the mixing angle $θ$ is in the range of $\tan^2θ\approx$0.25--0.65. | |
| dc.description | 10 Pages, 4 figures, submitted to Physics Letters B | |
| dc.identifier | https://arxiv.org/abs/hep-ex/0205075 | |
| dc.identifier | http://arxiv.org/abs/hep-ex/0205075 | |
| dc.identifier | Phys.Lett.B539:179-187,2002 | |
| dc.identifier | doi:10.1016/S0370-2693(02)02090-7 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/178667 | |
| dc.subject | High Energy Physics - Experiment | |
| dc.title | Determination of Solar Neutrino Oscillation Parameters using 1496 Days of Super-Kamiokande-I Data | |
| dc.type | text |