Journal
PHYSICAL REVIEW C
Volume 76, Issue 5, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevC.76.054303
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Funding
- STFC [EP/C516478/1, PP/F000944/1] Funding Source: UKRI
- Science and Technology Facilities Council [EP/C516478/1, PP/F000944/1] Funding Source: researchfish
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The structure of the neutron-rich isotopes Fe-59,Fe-60 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 similar to 20h. Both isotopes exhibit regular, near-yrast gamma-decay sequences which are generated by the intrusion of the g(9/2) orbital into the fp shell-model space. Lower-spin, natural-parity levels are discussed within the context of shell-model calculations using the GXPF1A interaction in the full fp model space. Experimental features of the high-spin bands are compared with total Routhian surface calculations.
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