Nucleosynthesis Limits on the Mass of Long Lived Tau and Muon Neutrinos
arXiv:hep-ph/9512321 · doi:10.1016/S0927-6505(96)00052-7
Abstract
We compute the nucleosynthesis bounds on the masses of stable Dirac and Majorana neutrinos by solving an evolution equation network comprising of all neutrino species which in the Dirac case includes different helicity states as separate species. We will not commit ourselves to any particular value of the nucleosynthesis bound on effective number of light neutrino degrees of freedom , but present all our mass bounds as {\em functions} of $\dNu$. For example, we find that the excluded region in the mass of a Majorana - or - neutrino, MeV MeV corresponding to a bound $\dNu < 0.3$ gets relaxed to MeV MeV if $\dNu < 1.0$ is used instead. For the Dirac neutrinos this latter constraint gives the upper limits (for MeV): $\mnm < 0.31$ MeV and $\mnt < 0.37$ MeV. Also, the constraint $\dNu <1$ {\it allows} a stable Dirac neutrino with MeV.
29 pages, 6 eps-figures, uses epsf.sty
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- Impact of massive tau-neutrinos on primordial nucleosynthesis. Exact calculations
- Nonequilibrium corrections to energy spectra of massive particles in expanding universe
- Mass of tau neutrino in SO(10) GUT-s
- Entropy production in the Early Universe. A new mechanism