Abstract
The reaction plays a fundamental role in astrophysics and needs to be known with accuracy better than 10%. Cascade transitions through the excited states of are contributing to the uncertainty. We constrained the contribution of the (6.05 MeV) and (6.13 MeV) cascade transitions by measuring the asymptotic normalization coefficients for these states using the -transfer reaction at sub-Coulomb energy. The contribution of the and cascade transitions at 300 keV is found to be and for destructive interference of the direct and resonance capture and and for constructive interference, respectively. The combined contribution of the and cascade transitions to the reaction cross section at 300 keV does not exceed 4%. Significant uncertainties have been dramatically reduced.
- Received 17 October 2014
DOI:https://doi.org/10.1103/PhysRevLett.114.071101
© 2015 American Physical Society