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Title: Primordial nucleosynthesis with a decaying [tau] neutrino

Journal Article · · Physical Review, D (Particles Fields); (United States)
; ;  [1]
  1. NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, Illinois 60510-0500 (United States) Department of Physics, The University of Chicago, Chicago, Illinois 60637-1433 (United States) Department of Astronomy Astrophysics, Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637-1433 (United States)

Mass-lifetime limits are derived for the four generic decay modes assuming that the abundance of the massive [tau] neutrino is determined by its electroweak annihilations. In general, nucleosynthesis excludes a [tau] neutrino of mass 0.4 MeV--30 MeV for lifetimes greater than about 300 sec. These nucleosynthesis bounds are timely since the current laboratory upper bounds to the [tau]-neutrino mass are around 30 MeV, and together the two bounds very nearly exclude a long-lived [tau] neutrino more massive than about 0.4 MeV. Further, our nucleosynthesis bounds together with other astrophysical and laboratory bounds exclude a [tau] neutrino of mass 0.4 MeV--30 MeV of any lifetime that decays with EM daughter product(s). We use our results to constrain the mass times relic abundance of a hypothetical, unstable species with similar decay modes. Finally, we note that a [tau] neutrino of mass 1 MeV to 10 MeV and lifetime 0.1 sec--10 sec whose decay products include an electron neutrino can reduce the [sup 4]He yield to less than that for two massless neutrino species. This fact could be relevant if the primordial mass fraction of [sup 4]He is found to be less than about 0.23 and can also lead to a modification of the nucleosynthesis bound to the number of light ([much lt]1 MeV) neutrino (and other) particle species.

OSTI ID:
7206797
Journal Information:
Physical Review, D (Particles Fields); (United States), Vol. 49:10; ISSN 0556-2821
Country of Publication:
United States
Language:
English