The O-15(alpha,gamma)Ne-19 and C-13(alpha,n)O-16 reactions in a multicluster model

摘要

A microscopic multicluster model has been applied to reactions of astrophysical interest. Due to the introduction of more clusters in our alpha description, the results exhibit in general a substantial improvement compared to those obtained with simpler models. We present recent results on the O-15(alpha, gamma)Ne-19 and N-15(alpha, gamma)F-19 reactions as well as preliminary results on the C-13(alpha, n)O-16 reaction. [References: 14]