Abstract

There are only two viable low-energy E6E_6 subgroups: SU(3)C×SU(2)L×U(1)Y×U(1)NSU(3)_C \times SU(2)_L \times U(1)_Y \times U(1)_N or SU(3)C×SU(2)L×SU(2)R×U(1)YL+YRSU(3)_C \times SU(2)_L \times SU(2)'_R \times U(1)_{Y_L + Y'_R}, which would not erase any preexisting lepton asymmetry of the Universe that may have been created by the decay of heavy singlet (right-handed) neutrinos or any other mechanism. They are also the two most favored E6E_6 subgroups from a recent analysis of present neutral-current data. We study details of the leptogenesis, as well as some salient experimental signatures of the two models.Comment: 12 page

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