Eur. Phys. J. A 14, 317-348 (2002)
DOI: 10.1140/epja/i2002-10011-3
Evolution of shapes in
C. Andreoiu1, D. Rudolph1, I. Ragnarsson2, C. Fahlander1, R.A.E. Austin3, M.P. Carpenter4, R.M. Clark5, J. Ekman1, R.V.F. Janssens4, T.L. Khoo4, F.G. Kondev4, T. Lauritsen4, T. Rodinger3, D.G. Sarantites6, D. Seweryniak4, T. Steinhardt7, C.E. Svensson5, O. Thelen7 and J.C. Waddington3
1 Department of Physics, Lund University, S-22100 Lund, Sweden
2 Department of Mathematical Physics, Lund Institute of Technology, S-22100 Lund, Sweden
3 Department of Physics and Astronomy, McMaster University, Hamilton, Ontario, Canada L8S 4M1
4 Physics Division, Argonne National Laboratory, Argonne, IL 60439, USA
5 Nuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA
6 Chemistry Department, Washington University, St. Louis, MO 63130, USA
7 Institut für Kernphysik, Universität zu Köln, D-50937 Köln, Germany
ca@ns.ph.liv.ac.uk
(Received: 15 February 2002 Communicated by D. Schwalm)
Abstract
High-spin states in
were populated using the
fusion-evaporation reaction
at a beam energy
of 122 MeV. The Gammasphere Ge-detector array in conjunction with the 4
charged-particle detector array Microball allowed for the
detection of
-rays in coincidence with evaporated
light particles. The resulting extensive high-spin
decay scheme of
is presented, which comprises more than 320
-ray transitions connecting about 150 excited states.
Their spins and parities have been assigned via directional correlations of
-rays emitted from oriented states. Average quadrupole moments of
rotational bands have been determined from the analysis of residual
Doppler shifts. Shell model calculations in the
fp shell are invoked
to study some of the low-spin states, while the experimental characteristics
of the rotational bands are analyzed in the configuration-dependent
cranked Nilsson-Strutinsky (CNS) approach.
21.60.Cs - Shell model.
23.20.Lv - Gamma transitions and level energies.
23.20.En - Angular distribution and correlation measurements.
27.50.+e -

© Società Italiana di Fisica, Springer-Verlag 2002