2002/05/21 by M. Jezabek
Physics and Astronomy · #hep-ph
published as Acta Phys.Polon. B33 (2002) 1885 · 7 pages, no figures. Dedicated to Stefan Pokorski on his 60th birthday. To appear in Acta Physica Polonica B
arxiv created 2002/05/21 · arxiv updated 2009/11/30
A large hierarchy of the Dirac masses can result in a small hierarchy for the low energy masses of the active neutrinos. This can happen even if the Majorana masses of right-handed neutrinos are all equal. A realistic description of the observed neutrino masses and mixing can be obtained starting from a large hierarchy in the Dirac masses. A large mixing for solar neutrinos results from the neutrino sector. The small value of the MNS matrix element Ue3 is a natural consequence of the scheme. The masses of the two lighter neutrinos are related to the solar neutrino mixing angle: mu1/mu2 = tan2 thetasol.