Neutrino Masses in Flipped SU(5)

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

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(14 Pages,No figures,TEX,IOA-290/92 preprint)

Scientific paper

10.1016/0370-2693(93)90114-W

We analyse the fermion masses and mixings in the flipped SU(5) model. The fermion mass matrices are evolved from the GUT scale down to $m_W$ by solving the renormalization group equations for the Yukawa couplings. The constraints imposed by the charged fermion data are then utilised to make predictions about the neutrino properties . It is found that the {\it generalized } see-saw mechanism which occurs naturally in this model can provide {\it i})a solution to the solar neutrino problem via the MSW mechanism and {\it ii})a sufficiently large $\nu _{\tau }$ mass to contribute as a hot dark matter component as indicated by the recent COBE data.

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