Model independent constraints of the averaged neutrino masses revisited
arXiv:1310.3568 · doi:10.1142/S0217732313501861
Abstract
Averaged neutrino masses defined by $\la m_ν\ra_{ab} \equiv\left| \sum_{j=1}^{3}U_{aj}U_{bj}m_j\right|$ () are reanalyzed using up-to-date observed MNS parameters and neutrino masses by the neutrino oscillation experiments together with the cosmological constraint on neutrino masses. The values of $\la m_ν\ra_{ab}$ are model-independently evaluated in terms of effective neutrino mass defined by which is observable in the single beta decay. We obtain lower bound for in the inverted hierarchy(IH) case, $17~\mbox{meV} \leq \langle m_ν\rangle_{ee}$ and one for in the normal hierarchy(NH) case, $5~\mbox{meV}\leq \langle m_ν\rangle_{τμ}$. We also obtain that all the averaged masses $\la m_ν\ra_{ab}$ have upper bounds which are at most $80~\mbox{meV}$.
8 pages, 7 figures, to appear in MPLA
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