Observational Model Explores Inflationary Effects in Cosmology, Indicating New Insights for Neutrino Masses.
The radiative neutrino mass model with inert doublet dark matter is a promising model for the present experimental issues which cannot be explained within the standard model. We study an extension of this model focusing on cosmological features brought about from the scalar sector. Inflation due to singlet scalars with hierarchical nonminimal couplings with the Ricci scalar may give a favorable solution for both neutrino masses and baryon number asymmetry in the Universe.
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Budhi et al. (2016) studied this question.
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