Issue |
EPJ Web Conf.
Volume 193, 2018
6th Workshop on Nuclear Fission and Spectroscopy of Neutron-Rich Nuclei (FISSION 2017)
|
|
---|---|---|
Article Number | 05002 | |
Number of page(s) | 7 | |
Section | Spectroscopy of Neutron-Rich Nuclei | |
DOI | https://doi.org/10.1051/epjconf/201819305002 | |
Published online | 14 November 2018 |
https://doi.org/10.1051/epjconf/201819305002
Excited States and Collectivity in 88Se
1
Laboratoire de Physique Subatomique et de Cosmologie, Université Grenoble Alpes, CNRS/IN2P3, Grenoble INP, F-38026 Grenoble, France
2
Institut Laue-Langevin, 71 avenue des Martyrs, 38042 Grenoble Cedex 9, France
3
Université de Strasbourg, IPHC, 23 rue du Loess 67037 Strasbourg, CNRS, UMR7178, 67037 Strasbourg, France
4
Grand Accélérateur National d’Ions Lourds, CEA/DRF-CNRS/IN2P3, Boulevard Henri Becquerel, F-14076 Caen, France
5
INFN, via Marzolo 8, 35131 Padova, Italy
6
ELI-NP/IFIN-HH, 30 Reactorului Str., 077125 Magurele, Romania
7
Faculty of Physics University of Warsaw, ulica Pasteura 5, PL-02-093 Warsaw, Poland
* e-mail: simpson@lpsc.in2p3.fr
Published online: 14 November 2018
The γ decays of excited states in the very neutron-rich nucleus 88Se have been observed following the cold neutron-induced fission of 235U at the PF1B facility of the Institut Laue-Langevin (ILL), Grenoble. The EXILL array was used to measure γ - γ - γ coincidences, which were then analysed to build a level scheme of 88Se. A low (2+1) energy hints at the onset of quadrupole deformation and the identification of possible members of a (2+2) band provide evidence for γ vibrations. Shell-model calculations using a 78Ni core reproduce the experimental decay scheme well, implying that interactions between particles in the π f5/2 p and vsd orbits are responsible for much of the collectivity present. The algebraic collective model has also been used to interpret the experimental data, showing that that the experimental spectrum is consistent with 88Se being a transitional nucleus, possessing weak static β deformation and γ instability.
© The Authors, published by EDP Sciences, 2018
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