Testing SO(10)-inspired leptogenesis with low energy neutrino experiments

We extend the results of a previous analysis of ours showing that, when both heavy and light flavour effects are taken into account, successful minimal (type I + thermal) leptogenesis with SO(10)-inspired relations is possible. Barring fine tuned choices of the parameters, these relations enforce a hierarchical RH neutrino mass spectrum that results into a final asymmetry dominantly produced by the next-to-lightest RH neutrino decays ( N 2 dominated leptogenesis). We present the constraints on the whole set of low energy neutrino parameters. Allowing a small misalignment between the Dirac basis and the charged lepton basis as in the quark sector, the allowed regions enlarge and the lower bound on the reheating temperature gets relaxed to values as low as ∼ 10 10 GeV. It is confirmed that for normal ordering (NO) there are two allowed ranges of values for the lightest neutrino mass: m 1 ≃ (1−5) × 10 −3 eV and m 1 ≃ (0.03−0.1) eV. For m 1 ≲0.01 eV the allowed region in the plane θ 13 -θ 23 is approximately given by θ 23 ≲49°+0.65 (θ 13 −5°), while the neutrinoless double beta decay effective neutrino mass falls in the range m ee = (1−3) × 10 −3 eV for θ 13 = (6°−11.5°). For m 1 ≳0.01 eV, one has quite sharply m ee ≃ m 1 and an upper bound θ 23 ≲46°. These constraints will be tested by low energy neutrino experiments during next years. We also find that inverted ordering (IO), though quite strongly constrained, is not completely ruled out. In particular, we find approximately θ 23 ≃ 43°+12° log (0.2 eV/ m 1 ), that will be fully tested by future experiments.