Successful type I Leptogenesis with SO(10)-inspired mass relations
Pasquale Di Bari, Antonio Riotto

TL;DR
This paper demonstrates that successful type I leptogenesis within SO(10)-inspired models is achievable by considering next-to-lightest neutrino decays and flavor effects, overcoming previous theoretical obstacles.
Contribution
It shows how to realize successful leptogenesis under SO(10) constraints by including flavor effects and decays of heavier right-handed neutrinos, with specific conditions on neutrino parameters.
Findings
Successful leptogenesis requires m_1 0.001 eV.
Non-zero _13 favors normal hierarchical neutrino spectrum.
Flavor effects and next-to-lightest neutrino decays are crucial for viability.
Abstract
It is well-known that thermal leptogenesis through the decays of the lightest right-handed neutrinos encounters serious difficulties when SO(10)-inspired mass conditions are imposed on the Dirac neutrino mass matrix and light neutrino masses are generated through the type I see-saw mechanism. We show that these can be circumvented when the production from the next-to-lightest right-handed neutrinos and flavor effects are properly taken into account. Some conditions on the low energy parameters have to be satisfied in order for inverse processes involving the lightest right-handed neutrino not to wash-out the asymmetry. In particular we find m_1 \gtrsim 0.001 eV, where m_1 is the mass of the lightest left-handed neutrino and that non-vanishing values of the mixing angle theta_13 are preferred in the case of a normal fully hierarchical spectrum of light neutrinos.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsParticle physics theoretical and experimental studies · Neutrino Physics Research · Dark Matter and Cosmic Phenomena
