We developed a previous model fitting all quark and lepton – including neutrino quantities in the region of the Large Mixing Angle-MSW solar solution – order of magnitudewise by only six adjustable parameters ( Higgs vacuum expectation values ) to also give an agreeing prediction for the amount of baryogenesis produced in the early time of cosmology .
We use Fukugita-Yanagida scheme and take into account now also the effect of the remormalisation equation for the Dirac neutrino sector from Planck scale to the see-saw scale .
The present version of our model with many approximately conserved ( gauge ) charges distinguishing various left- and right-Weyl particles has the largest matrix element of the mass matrix for the three flavour see-saw neutrinos being the off-diagonal elements associated with the second- and third-proto-flavour and gives the ratio of baryon number density to the entropy density to 2.59 { +17.0 \atop - 2.25 } \times 10 ^ { -11 } which agrees perfectly well as do also all the fermion masses and their mixing angles order of magnitudewise .

PACS numbers : 12.10.Dm , 12.15.Ff , 13.35.Hb , 13.60.Rj , 14.60.Pq , 14.60.St Keywords : Fermion masses , Neutrino oscillations , See-saw mechanism , Baryogenesis , Lepton number violation , Proton decay