Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phrvl..67..533k&link_type=abstract
Physical Review Letters (ISSN 0031-9007), vol. 67, July 29, 1991, p. 533-536. Research supported by DOE and NSF.
Astronomy and Astrophysics
Astrophysics
63
Astrophysics, Neutrinos, Nuclear Fusion, Particle Mass, Weak Energy Interactions, Abundance, Thermodynamic Equilibrium
Scientific paper
It is shown that primordial nucleosynthesis excludes a tau-neutrino mass from 0.3 to 25 MeV (Dirac) and 0.5 to 25 MeV (Majorana) provided that its lifetime is not less than about 1 sec, and from 0.3 to 30 MeV (Dirac) and 0.5 to 32 MeV (Majorana) for a lifetime of not less than about 1000 sec. A modest improvement in the laboratory mass limit - from 35 to 25 MeV - would imply that the tau-neutrino mass must be less than 0.5 MeV (provided the lifetime is not less than about 1 sec).
Chakravorty Alak
Kolb Edward W.
Schramm David N.
Turner Michael S.
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