The 17 keV neutrino and the search for anomalous γ rays in 35S decay

Details The 17 keV neutrino and the search for anomalous γ rays in 35S decay The 17 keV neutrino and the search for anomalous γ rays in 35S decay

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995phlb..347..152m&link_type=abstract

Physics Letters B, v. 347, p. 152-157

Physics

3

Scientific paper

We searched for anomalous γ rays in 35S decay as a possible explanation for the kink in the β-decay spectrum, which is claimed to be due to the emission of the heavy 17 keV neutrino. The intensity and spectrum of γ rays we observed are consistent with those of the external and internal bremsstrahlung of the β rays. It is concluded that the γ-ray spectrum has no structures which may mimic the claimed kink.

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