Abstract

The gamma-ray decay of excited states of the one-valence-proton nucleus 133Sb has been studied using cold-neutron induced fission of 235U and 241Pu targets, during the EXILL campaign at the ILL reactor in Grenoble. By using a highly efficient HPGe array, coincidences between gamma-rays prompt with the fission event and those delayed up to several tens of microseconds were investigated, allowing to observe, for the first time, high-spin excited states above the 16.6 micros isomer. Lifetimes analysis, performed by fast-timing techniques with LaBr3(Ce) scintillators, reveals a difference of almost two orders of magnitude in B(M1) strength for transitions between positive-parity medium-spin yrast states. The data are interpreted by a newly developed microscopic model which takes into account couplings between core excitations (both collective and non-collective) of the doubly magic nucleus 132Sn and the valence proton, using the Skyrme effective interaction in a consistent way. The results point to a fast change in the nature of particle-core excitations with increasing spin.

Highlights

  • The γ -ray decay of excited states of the one-valence-proton nucleus 133Sb has been studied using coldneutron induced fission of 235U and 241Pu targets, during the EXILL campaign at the ILL reactor in Grenoble

  • The data are interpreted by a newly developed microscopic model which takes into account couplings between core excitations of the doubly magic nucleus 132Sn and the valence proton, using

  • Ideal systems to investigate this duality should be nuclei composed of one valence particle and a doubly magic core in which the coupling between collective core excitations and the valence nucleon strongly influences the structure of the system [1]

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Summary

Contents lists available at ScienceDirect

By using a highly efficient HPGe array, coincidences between γ -rays prompt with the fission event and those delayed up to several tens of microseconds were investigated, allowing to observe, for the first time, high-spin excited states above the 16.6 μs isomer. Taking into account the decay branchings from the two levels [33], B(M1) values were extracted for the 15/2+ → 13/2+ and 13/2+ → 11/2+ transitions, yielding > 0.24 W.u. and 0.0042(15) W.u., respectively This large difference, of almost two orders of magnitude, is clearly intriguing and brings a signature of some non-trivial change of configuration mixing in the 11/2+, 13/2+ and 15/2+ states of 133Sb. In order to interpret the experimental findings, a new microscopic model has been developed with the aim of describing states with different degrees of collectivity. Our calculation has no free parameters and is self-consistent in the sense that both single-particle states and phonons come out

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