Abstract
For pt.VIII see ibid., vol.3, no.7, p.919 (1977). The authors present the results of a shell-model investigation of the masses, spectra, Coulomb energies and beta decays of the mass-24 nuclei. They have used the effective interaction of Chung and Wildenthal together with an empirically-determined Coulomb interaction. The ab initio use of a reasonably good Coulomb interaction reveals the presence of quite large errors in the calculated energies of certain states and hence of serious imperfections in the nuclear effective interaction. The calculated Coulomb energy differences in the mass-24 system have been used to improve the empirical Coulomb matrix elements.