Probing the neutrino mass matrix in next generation neutrino oscillation experiments
arXiv:hep-ph/0509217 · doi:10.1134/S1063778806110184
Abstract
We review the current status of the neutrino mass and mixing parameters needed to reconstruct the neutrino mass matrix. A comparative study of the precision in the measurement of oscillation parameters expected from the next generation solar, atmospheric, reactor and accelerator based experiments is presented. We discuss the potential of $0νββ$ experiments in determining the neutrino mass hierarchy and the importance of a better $θ_{12}$ measurement for it.
Prepared for 5th International Conference on Non-accelerator New Physics (NANP 05), Dubna, Russia, 20-25 Jun 2005