Abstract
The α spectrum following the β decay of from the isotope separator TISOL has been measured by detecting α particles in coincidence with nuclei. These data, which show a low-energy interference anomaly accompanying the main α peak, permit a more precise determination of the p-wave amplitude of the astrophysically important reaction (α,γO. The α spectrum and previous γ-ray data have been fitted simultaneously by a K-matrix parametrization; a value of S(E=0.3 MeV)=57±13 keV b has been obtained for the E1 part of the (α,γO reaction.
- Received 3 November 1992
DOI:https://doi.org/10.1103/PhysRevLett.70.726
©1993 American Physical Society