On the nature of the 17
s isomer of the 133Sb valence nucleus
J. Genevey1 - J.A. Pinston1 - H. Faust2 - C. Foin1 - S. Oberstedt2 - B. Weiss3
1 Institut des Sciences Nucléaires, IN2P3-CNRS/Université Joseph Fourier, 38026 Grenoble
Cedex, France
2 Institut Laue-Langevin, 38042 Grenoble Cedex, France
3 Université de Nice, 06108 Nice, France
Received: 20 January 2000 / Revised version: 28 February 2000 Communicated by J. Äystö
Abstract
The decay of the 17 s isomer of 133Sb was re-investigated experimentally.
It was produced by thermal neutron induced fission of 241Pu. Its detection
is based on time correlation between fission fragments selected by the LOHENGRIN
spectrometer at ILL (Grenoble), and the
-rays, and conversion electrons
from the isomer. The interpretation of the level scheme is based on shell model
calculations, where empirical two-body matrix elements were employed. The
good agreement between theory and experiment suggests that the isomer
is the 21/2+ member of the 2p-1h
configuration.
PACS
21.10.Tg Lifetimes -
23.20.Lv Gamma transition level energies -
25.85.Ec Neutron-induced fission -
21.60.Cs Shell model -
27.60.+j
Copyright Società Italiana di Fisica, Springer-Verlag 2000