Decrypting SO(10)-inspired leptogenesis

Encouraged by the recent results from neutrino oscillation experiments, we perform an analytical study of S0(10)-inspired models and leptogenesis with hierarchical right-handed (RH) neutrino spectrum. Under the approximation of negligible misalignment between the neutrino Yukawa basis and the charged lepton basis, we find an analytical expression for the final asymmetry directly in terms of the low energy neutrino parameters that fully reproduces previous numerical results. This expression also shows that it is possible to identify an effective leptogenesis phase for these models. When we also impose the wash-out of a large pre-existing asymmetry N-B-L(p,i), the strong thermal (ST) condition, we derive analytically all those constraints on the low energy neutrino parameters that characterise the ST-S0(10)-inspired leptogenesis solution, confirming previous numerical results. In particular we show why, though neutrino masses have to be necessarily normally ordered, the solution implies an analytical lower bound on the effective neutrinoless double beta decay neutrino mass, m(ee) greater than or similar to meV, for N-B-L(p,i) = 10(-3), testable with next generation experiments. This, in combination with an upper bound on the atmospheric mixing angle, necessarily in the first octant, forces the lightest neutrino mass within a narrow range m(1) similar or equal to (10-30) meV (corresponding to Sigma(i) m(i) similar or equal to (75-125) meV). We also show why the solution could correctly predict a non-vanishing reactor neutrino mixing angle and requires the Dirac phase to be in the fourth quadrant, implying sin delta (and J(CP)) negative as hinted by current global analyses. Many of the analytical results presented (expressions for the orthogonal matrix, RH neutrino mixing matrix, masses and phases) can have applications beyond leptogenesis. (C) 2015 The Authors. Published by Elsevier B.V.