Abstract
The reaction rates of neutron capture reactions on light nuclei are important for reliably simulating nucleosynthesis in a variety of stellar scenarios. Neutron capture reaction rates on neutron-rich C, N, and O isotopes are calculated in the framework of a hybrid compound and direct capture model. The results are tabulated and compared with the results of previous calculations as well as with experimental results.
- Received 25 June 1999
DOI:https://doi.org/10.1103/PhysRevC.60.064614
©1999 American Physical Society