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⊙2,tan2θ⊙ parameter space compatible with experimental data. Combining all data, we obtain the following best-fit parameters: Δm⊙2=8.17∗10−5, tan2θ⊙=0.40
@article{arxiv.hep-ph/0406182,
title = {Analysis of Neutrino oscillation data with the recent KamLAND results},
author = {P. Aliani and V. Antonelli and R. Ferrari and M. Picariello and E. Torrente-Lujan},
journal= {arXiv preprint arXiv:hep-ph/0406182},
year = {2007}
}