Abstract
Interaction cross sections for nuclei with on a target are calculated in the Glauber model with matter densities obtained from Skyrme Hartree-Fock and relativistic Dirac potentials. The shell-model orbital occupations and separation energies are taken from configuration-mixing calculations and experimental spectroscopic data. Halo effects are present in the most neutron-rich C and N isotopes. The rms matter radii and interaction cross section exhibit a kink at which can be associated with a change in the mean-field potential when the orbit is being filled.
- Received 13 July 2001
DOI:https://doi.org/10.1103/PhysRevC.65.014612
©2001 American Physical Society