Abstract
Three-body dynamics for the and ground states are used for the first time to investigate the shell structure of these nuclei. Shell orbital probabilities, configuration-space single-particle orbital densities, and two-particle wave-function amplitudes in coupling are calculated. The predicted orbital probabilities differ significantly from shell-model values except for those with core excitation. The need in shell models for core excitation may actually reflect required three-body dynamical effects.
- Received 19 November 1982
DOI:https://doi.org/10.1103/PhysRevLett.50.98
©1983 American Physical Society