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AbstractAbstract
[en] Probing shell structure at a large neutron excess has been of particular interest in recent times. Neutron-rich nuclei between the proton shell closures Z = 20 and Z = 28 offer an exotic testing ground for shell evolution. The development of the N = 40gap between neutron fp and lg9/2 shells gives rise to highly interesting variations of collectivity for nuclei in this region. While 68Ni shows doubly magic properties in level energies and transition strengths, this was not observed in neighbouring nuclei. Especially neutron-rich Fe isotopes proved particularly resistant to calculational approaches using the canonical valence space (fpg) resulting in important deviations of the predicted collectivity. Only an inclusion of the d5/2-orbital could solve the problem [1]. Hitherto no transition strengths for 66Fe have been reported. We determined B(E2,2+1→0+1) values from lifetimes measured with the recoil distance Doppler-shift method using the Cologne plunger for radioactive beams at National Superconducting Cyclotron Laboratory at Michigan State University. Excited states were populated by projectile Coulomb excitation for 62,64,66Fe. The data show a rise in collectivity for Fe isotopes towards N = 40. Results [2] are interpreted by means of a modified version of the Valence Proton Symmetry [3] and compared to shell model calculations using a new effective interaction recently developed for the fpgd valence space [4].
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Source
FINUSTAR 3 Conference on frontiers in nuclear structure, astrophysics, and reactions; Rhodes (Greece); 23-27 Aug 2010; (c) 2011 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA)
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Journal Article
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Conference
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ACCELERATORS, BARYONS, BETA DECAY RADIOISOTOPES, BETA-MINUS DECAY RADIOISOTOPES, CYCLIC ACCELERATORS, CYCLOTRONS, ELEMENTARY PARTICLES, ENERGY LEVELS, ENERGY-LEVEL TRANSITIONS, EVEN-EVEN NUCLEI, EXCITATION, FERMIONS, HADRONS, INTERMEDIATE MASS NUCLEI, IRON ISOTOPES, ISOTOPES, MATHEMATICAL MODELS, NICKEL ISOTOPES, NUCLEAR MODELS, NUCLEI, NUCLEONS, RADIOISOTOPES, SECONDS LIVING RADIOISOTOPES
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