Smooth Hybrid Inflation and Non-Thermal Type II Leptogenesis
Shaaban Khalil, Qaisar Shafi, Arunansu Sil

TL;DR
This paper explores a supersymmetric hybrid inflation model where Higgs triplets facilitate inflation and generate the universe's baryon asymmetry through non-thermal leptogenesis, linking neutrino masses to cosmological observations.
Contribution
It introduces a novel inflationary scenario based on a supersymmetric gauge model with triplet leptogenesis, connecting neutrino mass generation to baryon asymmetry.
Findings
Baryon asymmetry can be explained via non-thermal triplet leptogenesis.
Higgs triplets contribute to neutrino masses and inflation dynamics.
The model successfully links neutrino physics with cosmological baryogenesis.
Abstract
We consider a smooth hybrid inflation scenario based on a supersymmetric SU(2)_L x SU(2)_R x U(1)_B-L model. The Higgs triplets involved in the model play a key role in inflation as well as in explaining the observed baryon asymmetry of the universe. We show that the baryon asymmetry can originate via non-thermal triplet leptogenesis from the decay of SU(2)_L triplets, whose tiny vacuum expectation values also provide masses for the light neutrinos.
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