Resumen
The time variation of the elastic scattering rate of solar neutrinos with electrons in Super-Kamiokande-I was fit to the variations expected from active two-neutrino oscillations. The best fit in the large mixing angle solution has a mixing angle of [Formula Presented] and a mass squared difference of [Formula Presented] between the two neutrino mass eigenstates. The fitted day-night asymmetry of [Formula Presented] has improved statistical precision over previous measurements and agrees well with the expected asymmetry of [Formula Presented]
| Idioma original | Inglés |
|---|---|
| Publicación | Physical Review D - Particles, Fields, Gravitation and Cosmology |
| Volumen | 69 |
| N.º | 1 |
| DOI | |
| Estado | Publicada - 2004 |
| Publicado de forma externa | Sí |
Huella
Profundice en los temas de investigación de 'Precise measurement of the solar neutrino day-night and seasonal variation in Super-Kamiokande-I'. En conjunto forman una huella única.Citar esto
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