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Constraints on the neutron lifetime from triton decay J. Byrne
School of Mathematical and Physical Sciences, University of Sussex, Brighton, Sussex BN1 9QH, UK
The empirical data on triton - decay, 3H 3He+e-+v~e have been analysed with regard to their implications for neutron decay, n p+e-+v~e. The latter process is a primary source of information on weak interactions in the nucleonic sector1; it also has a central role in big-bang cosmology2,3 and in nuclear astrophysics in relation to the solar neutrino problem4. Unfortunately, the absolute rate of neutron decay is rather uncertain5. The Particle Data Group has recommended the value n = 925 11 s for the neutron lifetime6, based on two direct measurements7,8 which are in close accord, but barely consistent with the value n = 905 11 s derived from directional correlation data on polarized and unpolarized neutron decay9−11, and the comparative half lives of pure Fermi mirror transitions12,13. A third direct measurement has given the value n = 877 11 s (ref. 14), which is totally at variance with all other evidence. We suggest here that the triton data exclude values of n outside the range 911 10s, and deduce a weighted mean value n = 914 6 s.
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