Abstract
The decays of , , , and were studied both experimentally and via shell-model calculations. The four decaying nuclei were formed by bombardment of 81% enriched by triton and deuteron beams. Gamma-ray spectroscopy was carried out with Ge detectors, either bare or surrounded by a Compton suppression NaI(Tl) shield. One new Gamow-Teller decay was observed in decay, and one new first-forbidden decay was observed in decay. Otherwise γ-ray measurements of and (and limits on for unobserved transitions) were improved significantly over previous results. Shell-model studies were undertaken in order to bring these beta decay results to bear on an understanding of the shell structure in the (sd) to (fp) transition region at A=40. An interaction was constructed in the 1, 1, 2, 1, 1, 1, 1 model space. This interaction started from the Wildenthal ‘‘USD’’ (sd) interaction and the van Hees-Glaudemans (fp) interaction, which were connected by the cross-shell Millener-Kurath interaction. Certain important two-body matrix elements and single-particle energies were adjusted to fit experimental binding energies in A=40, 41, 42. This interaction was then used to calculate level spectra for the daughter nuclei , , , and as well as Gamow-Teller and unique first-forbidden beta decays leading to these nuclei. The techniques used in these relatively large scale calculations are discussed in detail, as are the results.
- Received 28 May 1986
DOI:https://doi.org/10.1103/PhysRevC.34.1031
©1986 American Physical Society