Naturalness of nearly degenerate neutrinos
J. A. Casas, J. R. Espinosa, A. Ibarra, I. Navarro

TL;DR
This paper investigates whether radiative corrections can generate small neutrino mass splittings in nearly degenerate neutrinos, supporting the large angle MSW solution and stability of bimaximal mixing, with analytical insights and a simple see-saw model.
Contribution
It provides a comprehensive analysis of radiative corrections in nearly degenerate neutrinos, demonstrating compatibility with experimental data and stability of bimaximal mixing.
Findings
Vacuum oscillation solution is excluded.
Large regions of parameter space support the large angle MSW solution.
Bimaximal structure remains stable under radiative corrections.
Abstract
If neutrinos are to play a relevant cosmological role, they must be essentially degenerate. We study whether radiative corrections can or cannot be responsible for the small mass splittings, in agreement with all the available experimental data. We perform an exhaustive exploration of the bimaximal mixing scenario, finding that (i) the vacuum oscillations solution to the solar neutrino problem is always excluded; (ii) if the mass matrix is produced by a see-saw mechanism, there are large regions of the parameter space consistent with the large angle MSW solution, providing a natural origin for the hierarchy; (iii) the bimaximal structure becomes then stable under radiative corrections. We also provide analytical expressions for the mass splittings and mixing angles and present a particularly simple see-saw ansatz consistent with all observations.
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