Non-thermal production of lepton asymmetry and dark matter in minimal seesaw with right handed neutrino induced Higgs potential
Rome Samanta, Anirban Biswas, Sukannya Bhattacharya

TL;DR
This paper explores a non-thermal mechanism for generating lepton asymmetry and dark matter within a minimal seesaw framework, highlighting a new parameter space where RH neutrino production from inflaton decay is viable and can address Higgs mass and neutrino mass constraints.
Contribution
It introduces a non-thermal production scenario for RH neutrinos and dark matter, expanding the viable parameter space and revealing a 'phantom window' where CP asymmetry decreases with RH mass scale.
Findings
Non-thermal RH neutrino production from inflaton decay is feasible.
Dark matter with mass up to 320 MeV can be produced in this scenario.
A 'phantom window' exists where CP asymmetry decreases with increasing RH mass.
Abstract
Within Type-I seesaw mechanism, Higgs mass can be dynamically generated via quantum effects of the right handed neutrinos assuming the potential is nearly conformal at the Ultra-Violet. The scenario, named as the "Neutrino Option" allows RH neutrino mass scale upto GeV to be consistent with light neutrino masses, mixing and Higgs mass. Therefore, it is not consistent with standard hierarchical thermal leptogenesis. Parameter space for thermal resonant leptogenesis is highly constrained in this model. We point out that non-thermal pair production of RH neutrinos from inflaton decay corresponds in general to a mild degree of resonance in the CP asymmetry parameter and allows RH mass scale to be smaller more than by an order of magnitude than the thermal strong resonance case. Within the similar parameter space of thermal leptogenesis, RH neutrinos can also be produced…
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