Abstract
The O()F reaction plays an important role in hydrogen-burning nucleosynthesis. Conflicting values for the low-energy behavior of its cross section exist in the literature. We present direct measurements of the astrophysical factor of the O()F reaction at center-of-mass energies between 250 and 500 keV. These measurements were conducted in inverse kinematics at the DRAGON recoil separator.
2 More- Received 15 November 2011
DOI:https://doi.org/10.1103/PhysRevC.85.035803
©2012 American Physical Society