Transition probabilities between the first excited state and the ground state in the N = 81 nuclei 139Ce, 141Nd, 143Sm and 145Gd
DOI
http://dx.doi.org/10.1016/0375-9474(80)90289-4
http://dx.doi.org/10.1016/0375-9474(80)90289-4
The level structure of 141Ce up to 3.7 MeV excitation energy has been investigated by the (d, t) and (3He, α) reactions using 17 MeV deuteron and 24 MeV 3He beams respectively. The angular distributions have been analyzed with standard DWBA calculations and spectroscopic factors are deduced. The experimental information is compared to unified model calculations involving both one-particle and two-particle one-hole configurations with quadrupole and octupole vibrations of the underlying N = 82 and N = 84 core.
http://dx.doi.org/10.1016/0375-9474(79)90084-8
http://dx.doi.org/10.1016/0375-9474(79)90653-5
http://dx.doi.org/10.1016/0375-9474(79)90655-9
The original Skyrme force is extended by a momentum dependent three-body term. A study is made on its influence on nuclear matter properties and properties of finite nuclei. The problem of spin-instability is treated in two nuclear models. A force parametrization is proposed, giving good estimates for all nuclear matter quantities (binding energy per nucleon, incompressibility, reduced mass, isospin symmetric energy, etc.), as well as properties of finite nuclei throughout the whole mass region (ground-state energy, nucleon distributions, rms radii, single-particle removal energies, etc.). The proposed parametrization satisfies the spin stability conditions. The force is able to describe satisfactorily the ground-state properties, even fine effects of two nuclear mass regions, one belonging to the light mass region (A=40-48) and one belonging to the medium heavy mass region (A=104-132).
NUCLEAR STRUCTURE Skyrme force extended with momentum dependent three-body term, spin stability conditions, application to Ca and Sn isotopes. © 1979 The American Physical Society
The extended Skyrme force has been used to calculate self-consistently ground-state properties, pairing correlations and properties of excited states of spherical nuclei throughout the whole mass region. The shell-model matrix elements exhibit the same behaviour as the bare reaction matrix elements of realistic interactions, and to be renormalized due to core polarization effects (3p-1h, 4p-2h), to generate good effective interactions. A numerical application on 42Ca is presented.
http://dx.doi.org/10.1016/0370-2693(79)90876-1
http://dx.doi.org/10.1016/0375-9474(78)90361-5
An orthonormalization method suitable to deal with an overcomplete and non-orthogonal set of vectors is derived. It is then used to obtain the orthonormal set of states connected with the angular momentum coupling of N fermions in a single j-shell.
http://dx.doi.org/10.1016/0375-9474(78)90009-X