Option of three pseudo--Dirac neutrinos
Abstract
Description
As an alternative for popular see-saw mechanism, the option of three pseudo% -Dirac neutrinos is discussed, where ${1/2}(m^{(L)} + m^{(R)}) \ll m^{(D)}$ for their Majorana and Dirac masses. The actual neutrino mass matrix is assumed in the form of tensor product $ M^{(ν)} \otimes {(\{array} {cc} λ^{(L)} & 1 1 & λ^{(R)} \{array})}$, where $ M^{(ν)}$ is a neutrino family mass matrix ($ M^{(ν) \dagger} = M^{(ν)}$) and $λ^{(L,R)} \equiv m^{(L,R)}/m^{(D)}$ with $ m^{(L)}$, $ m^{(R)}$ and $ m^{(D)} $ being taken as universal for three neutrino families. It is shown that three neutrino effects (deficits of solar $ν_e $'s and atmospheric $ ν_μ$'s as well as the possible LSND excess of $ν_e $'s in accelerator $ν_μ$ beam) can be nicely described by the corresponding neutrino oscillations, though the LSND effect may, alternatively, be eliminated (by a parameter choice). Atmospheric $ν_μ$'s oscillate dominantly into $ν_τ$'s, while solar $ν_e $'s - into (existing here automatically) Majorana sterile counterparts of $ν_e $'s. A phenomenological texture for neutrinos, compatible with the proposed description, is briefly presented.
LaTeX, 10 pages
LaTeX, 10 pages