Stability of the N=50 shell gap in the neutron-rich Rb, Br, Se, and Ge isotones


Stability of the N=50 shell gap in the neutron-rich Rb, Br, Se, and Ge isotones

Zhang, Y. H.; Podolyàk, Z.; de Angelis, G.; Gadea, A.; Ur, C.; Lunardi, S.; Marginean, N.; Rusu, C.; Schwengner, R.; Kröll, T.; Napoli, D. R.; Menegazzo, R.; Bazzacco, D.; Farnea, E.; Lenzi, S.; Martinez, T.; Axiotis, M.; Tonev, D.; Gelletly, W.; Langdown, S.; Regan, P. H.; Valiente Dobon, J. J.; von Oertzen, W.; Rubio, B.; Quintana, B.; Medina, N.; Broda, R.; Bucurescu, D.; Ionescu-Bujor, M.; Iordachescu, A.

The low- and medium-spin states of the N = 50 neutron-rich, 37 87Rb, 35 85Br, 34 84Se and 32 82Ge isotones have been populated in deep-inelastic processes produced by the interaction of 460 MeV 82Se ions with a 192Os target. The subsequent gamma decay has been investigated at the Laboratori Nazionali di Legnaro using the GASP gamma-ray detector array. The comparison of the experimentally observed excited states with shell-model calculations performed with and without neutron degrees of freedom has allowed the investigation of the role of the neutron-core breaking excitations and therefore of the N = 50 shell gap. The inclusion of neutron configurations in the shell-model calculations results in an improved agreement between the experimental and calculated level energies at medium and high spin. These results highlight the considerable contribution of neutron-core particle-hole excitations across the N = 50 shell gap to the level configurations. The overall agreement of the measured excited states with the shell-model predictions is indicative of the persistence of the N = 50 shell gap down to Z = 32.

Keywords: nuclear shell model; gamma-ray spectra; deep inelastic heavy ion reactions; nuclei with mass number 190 to 219; nuclear spin; nuclear energy level transitions; high spin states; nuclei with mass number 59 to 89

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