Analysis of Neutrino oscillation data with the recent KamLAND results
| dc.creator | Aliani, P. | |
| dc.creator | Antonelli, V. | |
| dc.creator | Ferrari, R. | |
| dc.creator | Picariello, M. | |
| dc.creator | Torrente-Lujan, E. | |
| dc.date | 2004-06-16 | |
| dc.date | 2004-06-17 | |
| dc.date.accessioned | 2026-07-07T03:52:41Z | |
| dc.date.available | 2026-07-07T03:52:41Z | |
| dc.description | We present an updated analysis of all available solar and reactor neutrino data, emphasizing in particular the totality of the KamLAND results and including the SNO phase III spectrum data. In a two active-neutrino framework, we determine the solutions in the $Δm_{\odot}^2, \tan^2θ_{\odot}$ parameter space compatible with experimental data. Combining all data, we obtain the following best-fit parameters: $Δm_{\odot}^2 =8.17*10^-5$, $\tan^2θ_{\odot}=0.40$ | |
| dc.description | 4 figures. Some references added | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0406182 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0406182 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/43558 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Analysis of Neutrino oscillation data with the recent KamLAND results | |
| dc.type | text |