Abstract
The reaction was studied using an 85 MeV radioactive beam. The asymptotic normalization coefficients for the virtual transitions were determined from the measured cross section. These coefficients specify the amplitude of the tail of the overlap function in the channel, and were used to calculate the astrophysical S factor for the direct capture reaction at solar energies We find that eV b.
- Received 20 July 1999
DOI:https://doi.org/10.1103/PhysRevC.60.055803
©1999 American Physical Society