Theoretical calculation of the radiative capture reaction
arXiv:1902.05881 · doi:10.1016/j.nuclphysa.2019.04.005
Abstract
We present a new calculation of the radiative capture astrophysical -factor in a cluster model framework. We consider several intercluster potentials, adjusted to reproduce the bound state properties and the elastic scattering phase shifts. Using these potentials, we calculate the astrophysical -factor, obtaining a good agreement with available data, and the photon angular distribution. Finally, we discuss the consequences of a hypothetical resonance-like structure on the -factor.
27 pages, 9 figures