Abstract
The O reaction rate is crucial for understanding the final abundance of predicted by nova models. The -ray emission in the first few hours after a nova outburst is expected to be dominated by 511 keV annihilation photons from the decay of , and so understanding its production can provide important constraints on the conditions during the outburst when compared with observations. Results are presented from the lowest-energy direct measurement to date, performed at the Isotope Separator and Accelerator radioactive beam facility at the TRIUMF laboratory, Canada. Cross section measurements at center-of-mass energies of 250, 330, 453, and 673 keV are obtained and the results compared to previous data and -matrix calculations. The implications for the overall reaction rate in the context of nova explosions have been discussed.
- Received 16 December 2010
DOI:https://doi.org/10.1103/PhysRevC.83.042801
©2011 American Physical Society