Conference paper

The Elliott SU(3) model in the pf-shell


Authors listHirsch, JG; Hess, PO; Hernández, L; Vargas, C; Beuschel, T; Draayer, JP

Publication year1999

Pages86-91

JournalRevista Mexicana de Fisica

Volume number45

ISSN0035-001X

ConferenceXXII Symposium on Nuclear Physics

PublisherSociedad Mexicana de Fisica


Abstract
The "quasi SU(3)" symmetry, uncovered in realistic shell-model calculations in the pf-shell, describes the fact that in the case of well-deformed nuclei the quadrupole-quadrupole and spin-orbit interactions play a dominant role and pairing can be included as a perturbation. In terms of a SU(3) basis, it is shown that the ground state band is built from the S = 0 leading irrep which couples strongly to the leading S = 1 irreps in the proton and neutron subspaces. Furthermore, the quadrupole-quadrupole interaction was found to give dominant weights to the so-called "stretched" coupled representations, which supports a strong SU(3)-dictated truncation of the model space. Using this type of truncation scheme, we studied Cr-48, which has a excitation spectrum like that of a quantum rotor. The Hamiltonian that was used in the study includes a single-particle term as well as pairing and quadrupole-quadrupole interactions. All or the interaction strengths were fixed from systematics. The yrast band energies were well-reproduced up to the backbending regime. By extending this approach it should be possible to perform realistic shell-model calculations for deformed nuclei throughout the periodic table.



Citation Styles

Harvard Citation styleHirsch, J., Hess, P., Hernández, L., Vargas, C., Beuschel, T. and Draayer, J. (1999) The Elliott SU(3) model in the pf-shell, Revista Mexicana de Fisica, 45, pp. 86-91

APA Citation styleHirsch, J., Hess, P., Hernández, L., Vargas, C., Beuschel, T., & Draayer, J. (1999). The Elliott SU(3) model in the pf-shell. Revista Mexicana de Fisica. 45, 86-91.



Keywords


Cr-48CR-48NUCLEIpseudo and quasi SU(3) symmmetriesQUADRUPOLEquadrupole-quadrupole and spin-orbit forces

Last updated on 2025-02-04 at 04:32