Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Shape-excited states of $sup 28$Si

Journal Article · · Pramana, v. 1, no. 6, pp. 269-273
OSTI ID:4312211
The Hartree- Fock (HF) minima for the nucleus /sup 28/Si were obtained for the prolate, oblate, and spherical shapes by using the interaction obtained by Preedom and Wildenthal. The interaction gives rise to large energy separation between the prolate and the oblate shapes. The spherical solution is just 2 MeV above the lowest HF (oblate) minimum. The spectrum projected from the oblate HF state is in good agreement with the experimental spectrum. The transition probabilities for the different energy levels also agree reasonably well. The configuration-mixing calculations performed on the basis of states projected from the three shapes indicate that there is no signiflcart mixing of different projected states. The sccond 0+2 state thus obtained corresponds to the third 0+3 state in the experimental spectrum, and stems dominantly from the spherical HF state. It is seen that the structure of the energy levels of /sup 28/Si, especially the second 0+3 level, is very sensttive to the two-body interaction. The results are compared with those obtained using the renormalized interaction of Kuo. (1 figure, 2
Research Organization:
Physical Research Lab., Ahmedabad, India
NSA Number:
NSA-29-019655
OSTI ID:
4312211
Journal Information:
Pramana, v. 1, no. 6, pp. 269-273, Journal Name: Pramana, v. 1, no. 6, pp. 269-273; ISSN PRAMC
Country of Publication:
Country unknown/Code not available
Language:
English

Similar Records

Shape coexistence and high spin states in {sup 52}Cr
Journal Article · Sat Sep 15 00:00:00 EDT 2007 · Physical Review. C, Nuclear Physics · OSTI ID:21064329

Competing Shapes And Alignments In Neutron-Rich Hf Nuclei
Journal Article · Mon May 12 00:00:00 EDT 2008 · AIP Conference Proceedings · OSTI ID:21143358

High-spin states in /sup 28/Si from variation after angular-momentum projection
Journal Article · Sun May 01 00:00:00 EDT 1983 · Phys. Rev. C; (United States) · OSTI ID:5906028