| Literature DB >> 28474931 |
S Leoni1,2, B Fornal3, N Mărginean4, M Sferrazza5, Y Tsunoda6, T Otsuka6,7,8,9, G Bocchi1,2, F C L Crespi1,2, A Bracco1,2, S Aydin10, M Boromiza4,11, D Bucurescu4, N Cieplicka-Oryǹczak2,3, C Costache4, S Călinescu4, N Florea4, D G Ghiţă4, T Glodariu4, A Ionescu4,11, Ł W Iskra3, M Krzysiek3, R Mărginean4, C Mihai4, R E Mihai4, A Mitu4, A Negreţ4, C R Niţă4, A Olăcel4, A Oprea4, S Pascu4, P Petkov4, C Petrone4, G Porzio1,2, A Şerban4,11, C Sotty4, L Stan4, I Ştiru4, L Stroe4, R Şuvăilă4, S Toma4, A Turturică4, S Ujeniuc4, C A Ur12.
Abstract
A search for shape isomers in the ^{66}Ni nucleus was performed, following old suggestions of various mean-field models and recent ones, based on state-of-the-art Monte Carlo shell model (MCSM), all considering ^{66}Ni as the lightest nuclear system with shape isomerism. By employing the two-neutron transfer reaction induced by an ^{18}O beam on a ^{64}Ni target, at the sub-Coulomb barrier energy of 39 MeV, all three lowest-excited 0^{+} states in ^{66}Ni were populated and their γ decay was observed by γ-coincidence technique. The 0^{+} states lifetimes were assessed with the plunger method, yielding for the 0_{2}^{+}, 0_{3}^{+}, and 0_{4}^{+} decay to the 2_{1}^{+} state the B(E2) values of 4.3, 0.1, and 0.2 Weisskopf units (W.u.), respectively. MCSM calculations correctly predict the existence of all three excited 0^{+} states, pointing to the oblate, spherical, and prolate nature of the consecutive excitations. In addition, they account for the hindrance of the E2 decay from the prolate 0_{4}^{+} to the spherical 2_{1}^{+} state, although overestimating its value. This result makes ^{66}Ni a unique nuclear system, apart from ^{236,238}U, in which a retarded γ transition from a 0^{+} deformed state to a spherical configuration is observed, resembling a shape-isomerlike behavior.Entities:
Year: 2017 PMID: 28474931 DOI: 10.1103/PhysRevLett.118.162502
Source DB: PubMed Journal: Phys Rev Lett ISSN: 0031-9007 Impact factor: 9.161