Abstract
The proton stripping reaction ,dF has been used to reinvestigate the proton widths of the states in near the proton threshold. Distorted-wave angular distributions were calculated using appropriate methods for stripping to unbound states. The deduced proton width for the level at =5.673 MeV () is significantly larger than a previous value obtained from a direct radiative capture experiment. A subthreshold state at =5.603 MeV () was found to have a rather large proton reduced width so that this state contributes significantly to the astrophysical S factor at low energy. These measurements lead to substantial changes in the stellar reaction rate for the ,αN reaction. This result is discussed in relation to recent observation of the isotopic abundance ratio O in red giant stars. In addition, the nuclear structure of is studied via the measurement of spectroscopic factors for most of the levels in bound against proton decay.
- Received 2 June 1989
DOI:https://doi.org/10.1103/PhysRevC.40.1972
©1989 American Physical Society