arXiv · hep-ph/9604242
Neutrino Oscillation based on the Mixings with a Heavy Right-Handed Neutrino
Abstract
We study a consistent explanation for both deficits of solar neutrino and atmospheric neutrino due to the neutrino oscillation induced by the mixing of light neutrinos with a heavy right-handed neutrino. We propose such a phenomenological neutrino mass matrix that realizes this scenario in the simple three generation left- and right- handed neutrino framework. Although this model contains only one nonzero mass eigenvalue $\sim$ 10 eV for these light neutrino states at the first approximation level, it can be expected to explain consistently both deficiency due to the appropriate higher order corrections. A suitable hot dark matter candidate is naturally included in it as its own feature.
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Daijiro Suematsu. 1996-11-30. Neutrino Oscillation based on the Mixings with a Heavy Right-Handed Neutrino. https://doi.org/10.1016/s0370-2693(96)01588-2
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