Abstract
The first shape-constrained high-spin Hartree-Fock-Bogoliubov calculations, using the density dependent Gogny interaction, have been carried out to investigate the energy minima in 182Os. Deep, well separated minima have been found for shapes with axis ratios of 1.5:1 and 2.2:1. Corrections for rotational zero point energies and for particle number fluctuations are taken into account. Comparisons are made with cranked Strutinsky calculations for this nucleus.
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