Abstract

We estimate the Baryon Asymmetry of the Universe (BAU) arising from leptogenesis within a class of minimal predictive seesaw models involving two right-handed neutrinos and simple Yukawa structures with one texture zero. The two right-handed neutrinos are dominantly responsible for the "atmospheric" and "solar" neutrino masses with Yukawa couplings to (νe,νμ,ντ)(ν_e, ν_μ, ν_τ) proportional to (0,1,1)(0,1,1) and (1,n,n−2)(1,n,n-2), respectively, where nn is a positive integer. The neutrino Yukawa matrix is therefore characterised by two proportionality constants with their relative phase providing a leptogenesis-PMNS link, enabling the lightest right-handed neutrino mass to be determined from neutrino data and the observed BAU. We discuss an SU(5)SU(5) SUSY GUT example, where A4A_4 vacuum alignment provides the required Yukawa structures with n=3n=3, while a Z9\mathbb{Z}_9 symmetry fixes the relatives phase to be a ninth root of unity.

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