Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2002-04-02
Nucl.Phys. B636 (2002) 305-337
Physics
High Energy Physics
High Energy Physics - Phenomenology
36 pages, 2 feynmf figures, Latex2e; one ref. added, refree responce slightly modified
Scientific paper
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.
Nielsen Holger Bech
Takanishi Yasutaka
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