Common Origin of Non-zero $\theta_{13}$ and Baryon Asymmetry of the Universe in a TeV scale Seesaw Model with $A_4$ Flavour Symmetry
Debasish Borah, Mrinal Kumar Das, Ananya Mukherjee

TL;DR
This paper presents a TeV-scale $A_4$ flavor symmetric model that naturally explains the origin of non-zero $ heta_{13}$ neutrino mixing angle and the baryon asymmetry of the universe through resonant leptogenesis, linking neutrino physics and cosmology.
Contribution
It introduces a novel $A_4$ symmetric framework with a specific mass matrix structure that simultaneously accounts for neutrino mixing and baryon asymmetry at TeV scale, emphasizing the role of antisymmetric triplet contractions.
Findings
Inverted hierarchy neutrino masses fit data well.
Model achieves correct baryon asymmetry via resonant leptogenesis.
Non-zero $ heta_{13}$ arises naturally from antisymmetric triplet products.
Abstract
We study the possibility of generating non-zero reactor mixing angle and baryon asymmetry of the Universe within the framework of an flavour symmetric model. Using the conventional type I seesaw mechanism we construct the Dirac and Majorana mass matrices which give rise to the correct light neutrino mass matrix. Keeping the right handed neutrino mass matrix structure trivial so that it gives rise to a (quasi) degenerate spectrum of heavy neutrinos suitable for resonant leptogenesis at TeV scale, we generate the non-trivial structure of Dirac neutrino mass matrix that can lead to the light neutrino mixing through type I seesaw formula. Interestingly, such a setup naturally leads to non-zero due to the existence of anti-symmetric contraction of the product of two triplet representations of . Such antisymmetric part of triplet products usually vanish…
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