Abstract
The structure of the neutron-rich isotopes has been studied with the Gammasphere detector array using fusion-evaporation reactions. Level schemes for these nuclei are presented which have been extended to spins of . Both isotopes exhibit regular, near-yrast γ-decay sequences which are generated by the intrusion of the orbital into the shell-model space. Lower-spin, natural-parity levels are discussed within the context of shell-model calculations using the GXPF1A interaction in the full model space. Experimental features of the high-spin bands are compared with total Routhian surface calculations.
2 More- Received 9 August 2007
DOI:https://doi.org/10.1103/PhysRevC.76.054303
©2007 American Physical Society