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A massive neutrino in nuclear beta decay

Conference · · AIP Conference Proceedings (American Institute of Physics); (United States)
OSTI ID:5540199
;  [1];  [2];  [1];  [3]; ; ; ;  [1];  [4];  [5]
  1. Nuclear Science Division, Lawrence Berkeley Laboratory, Berkeley, California (United States)
  2. Nuclear Science Division, Lawrence Berkeley Laboratory, Berkeley, California (United States) Physics Institute, University of Sao Paulo, Sao Paulo (Brazil)
  3. Nuclear Science Division, Lawrence Berkeley Laboratory, Berkeley, California (United States) Physics Department, Tennessee Technological University, Cookeville, Tennessee (United States)
  4. Nuclear Science Division, Lawrence Berkeley Laboratory, Berkeley, California (United States) Physics Department, University of California, Berkeley, California (United States)
  5. Nuclear Science Division, Lawrence Berke
We have continued our studies of the [beta]-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.
DOE Contract Number:
AC03-76SF00098; FG05-87ER40314
OSTI ID:
5540199
Report Number(s):
CONF-920837--
Conference Information:
Journal Name: AIP Conference Proceedings (American Institute of Physics); (United States) Journal Volume: 272:1
Country of Publication:
United States
Language:
English