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    Does cosmology imply a dirac neutrino mass?

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    Present bounds on double beta decay and tritium decay together with cosmological bounds on early nucleosynthesis lead to stringent limits on both left-handed (mL) and right-handed (mR) Majorana masses: View the MathML source. Therefore right-handed neutrinos of masses of a few keV are no longer a plausible candidate for galaxy formation processes
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