Abstract
The energy of the first level above the proton threshold in has been determined to be 5672.57±0.32 keV by γ-ray measurements using the (α,γF reaction. The change in the excitation energy of this level previously measured at 5668±2 keV affects significantly the calculated reaction rate for destruction during hydrogen burning in stars.
- Received 8 August 1988
DOI:https://doi.org/10.1103/PhysRevC.39.265
©1989 American Physical Society