Are the small neutrino oscillation parameters all related?
Soumita Pramanick, Amitava Raychaudhuri (University of Calcutta)

TL;DR
This paper proposes a see-saw model linking small neutrino oscillation parameters, suggesting they originate from a common source, and predicts observable CP-violation effects, which can be tested with future precision measurements.
Contribution
It introduces a see-saw model that naturally relates small neutrino parameters and predicts large CP-violation for inverted mass ordering.
Findings
Model explains small neutrino parameters through a single source.
Predicts large CP-violation in inverted mass hierarchy.
Testable with future precision neutrino experiments.
Abstract
Neutrino oscillations reveal several small parameters, namely, , the solar mass splitting {\em vis-\`{a}-vis} the atmospheric one, and the deviation of from maximal mixing. Can these small quantities all be traced to a single source and, if so, how could that be tested? Here a see-saw model for neutrino masses is presented wherein a dominant term generates the atmospheric mass splitting with maximal mixing in this sector, keeping and zero solar splitting. A Type-I see-saw perturbative contribution results in non-zero values of , , , as well as allows to deviate from in consistency with the data while interrelating them all. CP-violation is a natural consequence and is large () for inverted mass ordering. The model will be tested as precision on the…
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