Abstract
Breakup of 63-MeV and 42-MeV near the α-t threshold is examined from the astrophysical point of view. A new approach is made to extract indirectly astrophysical S factors. The S factors are compared with those deduced from radiative-capture measurements. It is shown that the energy dependence favors the recent capture data of Schröder et al.
- Received 24 April 1990
DOI:https://doi.org/10.1103/PhysRevLett.65.847
©1990 American Physical Society