Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
1996-10-10
Physics
High Energy Physics
High Energy Physics - Phenomenology
Latex 18 pages, 3 figures. Additional discussion of nucleosynthesis. No change in conclusions
Scientific paper
We consider nucleosynthesis constraints on models which use chiral symmetry breaking as a basis for understanding very small Dirac neutrino masses. We show that present big-bang nucleosynthesis constraints impose a well-defined upper bound of 0.1eV on the neutrino masses. This bound may become several orders of magnitude more stringent in the future as our understanding of the observational constraints on nucleosynthesis improves. We discuss the phenomenological implications for neutrino dark matter, the solar neutrino problem and the atmospheric neutrino deficit.
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