Phys. Rev. C 68, 024312 (2003) [21 pages]

Nuclear structure of the closed subshell nucleus 90Zr studied with the (n,nγ) reaction

Download: PDF (628 kB) or Buy this Article (Use Article Pack) Export: BibTeX or EndNote (RIS)

P. E. Garrett, W. Younes, J. A. Becker, and L. A. Bernstein
Lawrence Livermore National Laboratory, Livermore, California 94551, USA

E. M. Baum, D. P. DiPrete, R. A. Gatenby, E. L. Johnson, C. A. McGrath, and S. W. Yates
University of Kentucky, Lexington, Kentucky 40506-0055, USA

M. Devlin, N. Fotiades, and R. O. Nelson
Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA

B. A. Brown
Department of Physics and Astronomy and National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA

Received 12 May 2003; published 25 August 2003

States in 90Zr have been observed with the (n,nγ) reaction using both spallation and monoenergetic accelerator-produced neutrons. A scheme comprised of 81 levels and 157 transitions was constructed concentrating on levels below 5.6 MeV in excitation energy. Spins have been determined by considering data from all experimental studies performed for 90Zr. Lifetimes have been deduced using the Doppler-shift attenuation method for many of the states, and transition rates have been obtained. A spherical shell-model interpretation in terms of particle-hole excitations assuming a 88Sr closed core is given. In some cases, enhancements in B(M1) and B(E2) values are observed that cannot be explained by assuming simple particle-hole excitations. Shell-model calculations using an extended fpg-shell-model space reproduce the spectrum of excited states very well, and the gross features of the B(M1) and B(E2) transition rates. Transition rates for individual levels show discrepancies between calculations and experimental values.


©2003 The American Physical Society

URL: http://link.aps.org/doi/10.1103/PhysRevC.68.024312
DOI: 10.1103/PhysRevC.68.024312
PACS: 27.60.+j, 23.20.Lv, 25.40.Fq

[ Abstract  |  Previous article  |  Next article  |  Issue 2 ]