Abstract
The fusion excitation function of has been measured from well above the Coulomb barrier, down to low energies where the cross section is as small as 20 b, and the astrophysical factor possibly reaches a maximum vs energy. The results of coupled-channels calculations using the potential are presented. A detailed comparison is made with recently published data on the fusion of and of , including the excitation functions, their low-energy slopes and the barrier distributions. The presence of the fusion hindrance phenomenon in all cases is pointed out, as well as the influence of the strong octupole excitation in Ca and of nucleon transfer channels with positive values in .
- Received 28 October 2011
DOI:https://doi.org/10.1103/PhysRevC.85.024607
©2012 American Physical Society