Constraints from primordial nucleosynthesis on the mass of the τ neutrino

Edward W. Kolb, Michael S. Turner, A. Chakravorty, and David A. Schramm
Phys. Rev. Lett. 67, 533 – Published 29 July 1991
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Abstract

The familiar nucleosynthesis constraint on the number of neutrino species, Nν≤3.4, applies to massless neutrino species. An MeV-mass neutrino can have even greater impact, and we show that primordial nucleosynthesis excludes a τ-neutrino mass from 0.3 to 25 MeV (Dirac) and 0.5 to 25 MeV (Majorana) provided that its lifetime τν≳1 sec, and from 0.3 to 30 MeV (Dirac) and 0.5 to 32 MeV (Majorana) for τν103 sec. A modest improvement in the laboratory mass limit—from 35 to 25 MeV—would imply that the τ-neutrino mass must be less than 0.5 MeV (provided τν≳1 sec).

  • Received 4 February 1991

DOI:https://doi.org/10.1103/PhysRevLett.67.533

©1991 American Physical Society

Authors & Affiliations

Edward W. Kolb, Michael S. Turner, A. Chakravorty, and David A. Schramm

  • NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, Illinois 60510-0500
  • Department of Astronomy and Astrophysics, Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637-1433
  • Department of Physics, The University of Chicago, Chicago, Illinois 60637-1433

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Issue

Vol. 67, Iss. 5 — 29 July 1991

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