Abstract
Updated stellar rates for the reactions and are calculated by using all available experimental information as well as input data from the nuclear shell model. We calculated Coulomb and Thomas-Ehrmann shifts to obtain the unknown excitation energies and the spin/parity assignments of The astrophysical consequences are discussed.
- Received 25 May 2001
DOI:https://doi.org/10.1103/PhysRevC.64.045801
©2001 American Physical Society