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Constraints on radiative decay of massive neutrinos

Journal Article · · Physical Review, D (Particles Fields); (United States)
 [1]
  1. Department of Astronomy and Physics, and Center for Particle Astrophysics, University of California, Berkeley, California 94720 (United States)
Recent {beta}-decay experiments provide evidence for the existence of neutrinos with a mass of 17 keV. If they do exist, they should decay into lighter particles in order to avoid overclosing the Universe. Radiative decay may leave an imprint on the relic radiation from the big bang, and energy injection into the cosmic microwave background radiation should have observational consequences. In particular, the limits recently obtained on the {ital y} distortion of the blackbody spectrum of the cosmic microwave background provide stringent constraints on the radiative-decay properties of these neutrinos. We have found that the photon branching ratio has to be {ital B}{sub {gamma}}{approx lt}10{sup {minus}5} for the neutrino lifetime {tau}{congruent}10{sup 10}--10{sup 11} s. For {tau}{approx gt}10{sup 11} s, {ital B}{sub {gamma}} is constrained by the upper limits on the extragalactic background radiation at optical and UV wavelengths; the upper limit on {ital B}{sub {gamma}} decreases to about 10{sup {minus}6} at {tau}{congruent}10{sup 12} s.
OSTI ID:
7275146
Journal Information:
Physical Review, D (Particles Fields); (United States), Journal Name: Physical Review, D (Particles Fields); (United States) Vol. 46:6; ISSN PRVDA; ISSN 0556-2821
Country of Publication:
United States
Language:
English