Shell evolution and the N=34 “magic number”

increasing in the regions above closed neutron shells where the neutron binding energy is extremely low or in the region of nuclei with large neutron excess.. The nucleus

We have performed calculations to test the ability of the shell model to describe the heavy Cd and In isotopes, with proton and neutron holes outside the 132 Sn core.. In this

Moreover, it is interesting to note that the neutron and proton orbitals present in the conguration of the spherical isomer and in the deformed band of these odd-odd nuclei

The one-neutron knockout cross section to the resonance at E decay = 50 keV was determined to be σ − exp 1n = 61 ± 6 mb, after sub- tracting the non-resonant continuum. [8,24] ),

The contribution of possible E2 excitation to the spectrum obtained with the lead target has — in a first step — been determined using data taken with the aluminum target and

Level schemes were reconstructed using the γ-γ coincidence technique, with tentative spin-parity assign- ments based on the measured inclusive and exclusive cross sections..

The experimental results are in good overall agreement with self-consistent beyond-mean-field calculations based on the Gogny D1S interaction, which suggests both triaxial degree

The method used for the nuclear charge (Z) identication of this new isomer of mass 95, is shown in Fig.. Coincidence measurements were performed between the