Abstract
Levels of Se77, Se78, Se79, Se81, and Se83 below about 5 MeV were investigated by observation of the energy and angular distributions of protons emitted in the (d, p) reactions at 15-MeV bombarding energy. Values of the transferred-neutron angular momenta and of the spectroscopic factors for levels were derived from the measurements by distorted-wave Born approximation calculations. The results for the degree of filling of shell-model states and locations of the "centers of gravity" of the shell-model levels were compared with the pairing theory of Kisslinger and Sorensen. It was found that the 32, 52, and ½ subshells are less full and the g92 more full than expected. General agreement with pairing theory was obtained with the following parameters: ε92+=3.0 MeV, ε12=2.5 MeV, ε52=1.0 MeV, ε32=0, and Δ=1.65 MeV from the odd-even mass difference. In Se83, an isomer of spin½ at 0.22 MeV was identified. Measurements on (d, t) reactions indicate that the d52 subshell from the next (50-82) major shell is filling (∼0.6 particle) in the Se nuclei, even though the lower (28-50) major shell is not completely full.