Neutrino mass parameters from Kamland, SNO and other solar evidence

Details Neutrino mass parameters from Kamland, SNO and other solar evidence Neutrino mass parameters from Kamland, SNO and other solar evidence

2002-12-15

arxiv.org/abs/hep-ph/0212212v3

Phys.Rev. D69 (2004) 013005

Physics

High Energy Physics

High Energy Physics - Phenomenology

Scientific paper

10.1103/PhysRevD.69.013005

An updated analysis of all available neutrino oscillation evidence in Reactor (Kamland, first 145 days of data) and Solar experiments (SK day and night spectra, global rates from Homestake, SAGE and GALLEX) including the $SNO CC$ and $NC$ data is presented. In the framework of two active neutrino oscillations we determine the allowed regions in neutrino parameter space, we obtain, from the Kamland spectral shape and global signal, the following antineutrino best solution parameters, $ \Delta m^2_{kl}= 7.7\times 10^{-5} \eV^2, \tan^2\theta_{kl}= 0.98.$ The overall effect of the measured observed ratio $R\sim 0.6$ is that the LMA region remains the only one which is still favored. Combining Kamland and Solar data and assuming CPT invariance, i.e. the same mass matrix for neutrino and antineutrinos, we obtain the following antineutrino best solution parameters (LMAI solution), $ \Delta m^2= 7.1\times 10^{-5} \eV^2,\tan^2\theta= 0.47.$ A second solution (LMAII) appears for values $ \Delta m^2= 1.5\times 10^{-4} \eV^2, \tan^2\theta= 0.48.$ We determine additionally individual neutrino mixing parameters and their errors from fits to marginal likelihood distributions, the values are compatible with previous results. In both methods, $\chi^2$ minimization and marginal likelihood, the combined analysis of solar and Kamland data concludes that maximal mixing is not favored at the $\sim 3\sigma $ level at least.

Affiliated with

Also associated with

No associations

Rating

Neutrino mass parameters from Kamland, SNO and other solar evidence does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Neutrino mass parameters from Kamland, SNO and other solar evidence, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Neutrino mass parameters from Kamland, SNO and other solar evidence will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-441396