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The experimental knowledge of the Cu-61(29)32 and Zn-61(30)31 nuclei has been largely extended via the joint results from three experiments. The fusion-evaporation reaction used a Ar-36 beam and a Si-28 target foil to produce the two nuclei via the evaporation of either three protons (Cu-61) or two protons and a neutron (Zn-61). The experimental set-ups comprised the Ge-array GAMMASPHERE as well as neutron and charged-particle detectors placed around the target position. The resulting level schemes include around ten rotational superdeformed structures in each isotope. Most of them are linked to normally deformed states and in many cases spins and parities of the low-lying states in each structure have been determined. The collective structures are compared with results from configuration dependent Cranked Nilsson-Strutinsky calculations. The different structures are in general well understood from the calculation but the results do also suggest modifications of the standard Nilsson parameters in the mass A similar to 60 region. (Less)

Lifetimes of high‐spin states have been measured for 142Gd and 134Nd with EU‐ROBALL IV and AFRODITE, respectively, using DSAM. From calculations in the cranked Nilsson‐Strutinsky model it was concluded that at the high‐spin states of the (+,0)1 band, 142Gd represents a triaxial nucleus rotating around the longest principal axis.

A method to calculate absolute values of the total nuclear binding energy in the high-spin regime is briefly described. Applications to test the position of specific orbitals are examplified on Z = 36 Kr isotopes with N = 36 - 38. Calculated binding energies of possible configurations for one dipole band in 199 Pb are compared with experiment