Abstract
The neutron-rich nucleus has been studied using binary grazing reactions produced by the interaction of a 215-MeV beam of ions with a thin target. The magnetic spectrometer, PRISMA, and the -ray array, CLARA, were used in the measurements. Gamma-ray transitions of the following energies were observed: 339, 398, 466, 705, 1517, 1656, and 1724 keV. Five of the observed transitions have been tentatively assigned to the decay of excited states with spins up to (). The results of a state-of-the-art shell-model calculation of the level scheme of using the SDPF-U effective interaction are also presented. The systematic behavior of the excitation energy of the first states in the odd- isotopes of sulfur and argon is discussed in relation to the excitation energy of the first excited states of the adjacent even- isotopes. The states of that have the components in their wave functions corresponding to three neutrons in the orbital outside the core have also been discussed within the context of the 0 shell-model calculations presented here.
- Received 7 July 2016
DOI:https://doi.org/10.1103/PhysRevC.94.024325
©2016 American Physical Society