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A massive neutrino in nuclear beta decay?

Conference ·
OSTI ID:10112508
We have continued our studies of the p-spectrum of {sup 14}C using a germanium detector doped with {sup 14}C. There is a feature in the {beta}-spectrum 17 keV below the endpoint which could be explained by the hypothesis that there is a heavy neutrino emitted in the {beta}-decay of {sup 14}C with a mass of 17{plus_minus}1 keV and an emission probability of 1.26{plus_minus}0.25%. However, we also have performed a high statistics measurement of the inner bremsstrahlung spectrum of {sup 55}Fe and find no indication of the emission of a 17-keV neutrino. We conclude that the origin of the ``kink`` that has been observed in some recent beta spectral measurements is not a neutrino.
Research Organization:
Lawrence Berkeley Lab., CA (United States)
Sponsoring Organization:
USDOE, Washington, DC (United States)
DOE Contract Number:
AC03-76SF00098
OSTI ID:
10112508
Report Number(s):
LBL--32953; CONF-920837--30; ON: DE93004718
Country of Publication:
United States
Language:
English

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