Abstract
Using the GXPF1A interaction for the shell nuclei, we calculate energy levels and transition rates for the semimagic nuclei within both the exact shell-model space and a number of subspaces constructed using collective nucleon pairs. We present explicitly the overlaps between wave functions of low-lying states obtained from shell-model calculations and those obtained using truncated nucleon-pair subspaces. These examples are used as touchstones of pair approximations.
- Received 20 May 2010
DOI:https://doi.org/10.1103/PhysRevC.82.034303
©2010 American Physical Society