The addition of a T-dependent but J-independent term to the surface delta interaction greatly
improves the agreement between the values of the two-body matrix elements calculated …

Shell-model results for the binding energies and spectra of exotic nuclei in the p-shell are
presented. The calculated binding energies are compared with experimental values. The …

Binding energies, excitation energies and spectroscopic factors have been calculated for 57–67
Ni and 58–68 Cu in an unrestricted (2p 3/2 , lf 5/2 ,2p 1/2 ) shell-model space. The …

Shell model calculations on nuclei in the region 28 < A ≦ 40 are performed with the assumption
of an inert 28 Si core. The theory underlying these calculations has been described in …

The rates of electron captures which induce the collapse of the stellar cores composed of 16
O, 20 Ne and 24 Mg are calculated microscopically using the shell model wave functions of …

Several observables for the A= 4–16 p-shell nuclei, resulting from a calculation in the complete
(0+ 2) ħω model space, are presented. It is shown that the 2ħω admixtures are substantial…

Spectra, magnetic dipole moments and spectroscopic factors of a number ofA=205–209
nuclei as well asM1 transitions in 208 Pb are investigated in terms of large-scale shell-model …

The results of spurious-state free calculations in a complete (0+1)ħω model space on theA=4–16
nuclei are presented. The calculated spectra as well as electromagnetic properties of …

The contributions of central as well as noncentral two-body interactions to the matrix elements
of various effective interactions for the sd shell are studied in an SU (3) two-particle basis. …

Extensive shell-model calculations on several properties of all nuclei withZ=2–9 andA=4–30
have been performed, in order to investigate whether normal and exotic light nuclei can be …