Extension of a radiative neutrino mass model based on a cosmological view point

Abstract

We consider an extension of the radiative neutrino mass model at TeV regions so as to give the origin for inflation of the universe. This extension also gives a consistent explanation for both the origin of baryon number asymmetry and dark matter. A small scalar coupling which plays a crucial role in the neutrino mass generation in the original model may be related to parameters which are control inflation.

14 pages, 2 figures, some remarks and references added, accepted version for publication

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Cited by in corpus (14)

• Baryon number asymmetry and dark matter in the neutrino mass model with an inert doublet
• Leptogenesis and dark matter detection in a TeV scale neutrino mass model with inverted mass hierarchy
• Inflation in a modified radiative seesaw model
• Lepton number asymmetry via inflaton decay in a modified radiative seesaw model
• Low scale leptogenesis in a hybrid model of the scotogenic type I and III seesaw
• Inflation due to a non-minimal coupling of singlet scalars in the radiative seesaw model
• Leptogenesis in a neutrino mass model coupled with inflaton
• Inflation connected to the origin of $CP$ violation
• An extension of the SM based on effective Peccei-Quinn Symmetry
• Inflation and DM phenomenology in a scotogenic model extended with a real singlet scalar
• Radiative neutrino mass model with degenerate right-handed neutrinos
• Low scale leptogenesis in a model with promising $CP$ structure
• Symmetry restoration due to preheating and lepton number asymmetry
• Type-III Scotogenic Model: Inflation, Dark Matter and Collider Phenomenology