Implications for Solar Neutrino Oscillations from Super-Kamiokande and SNO Data
| dc.creator | Smy, Michael B. | |
| dc.date | 2001-08-31 | |
| dc.date.accessioned | 2026-07-07T03:34:44Z | |
| dc.date.available | 2026-07-07T03:34:44Z | |
| dc.description | Super-Kamiokande uses neutrino-electron elastic scattering to measure the recoil electron spectrum and zenith-angle dependence of solar $^8$B neutrinos. SNO has measured the $^8$B neutrino--deuteron charged-current reaction rate. The elastic scattering rate, spectrum and zenith-angle dependence in conjunction with the charged-current reaction rate favors active neutrino oscillations at large mixing angles by about 3$σ$ over the no-oscillation hypothesis and small mixing angles. The analysis is independent of the absolute $^8$B and {\it hep} flux and assumes two-flavor oscillations described by mixing angle and mass$^2$ difference. Two allowed regions at large mixing are found. | |
| dc.description | 8 pages, 6 figures; to be published in the proceedings of the NO-VE Workshop held in Venice, July 24-26, 2001 | |
| dc.identifier | https://arxiv.org/abs/hep-ex/0108053 | |
| dc.identifier | http://arxiv.org/abs/hep-ex/0108053 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/37097 | |
| dc.subject | High Energy Physics - Experiment | |
| dc.title | Implications for Solar Neutrino Oscillations from Super-Kamiokande and SNO Data | |
| dc.type | text |