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Transition probabilities in neutron-rich Se 80,82 and the role of the νg9/2 orbital

Authors :
Litzinger, J.
Blazhev, A.
Dewald, A.
Didierjean, F.
Duchêne, G.
Fransen, C.
Lozeva, R.
Verney, D.
Angelis, G. de
Bazzacco, D.
Birkenbach, B.
Bottoni, S.
Bracco, A.
Braunroth, T.
Cederwall, B.
Corradi, L.
Crespi, F.C.L.
Désesquelles, P.
Eberth, J.
Ellinger, E.
Farnea, E.
Fioretto, E.
Gernhäuser, R.
Goasduff, A.
Görgen, A.
Gottardo, A.
Grebosz, J.
Hackstein, M.
Hess, H.
Ibrahim, F.
Jolie, J.
Jungclaus, Andrea
Kolos, K.
Korten, W.
Leoni, S.
Lunardi, S.
Maj, A.
Menegazzo, R.
Mengoni, D.
Michelagnoli, C.
Mijatovic, T.
Million, B.
Möller, O.
Modamio, V.
Montagnoli, G.
Montanari, D.
Morales, Ana Isabel
Napoli, D.R.
Niikura, M.
Quintana, B.
Ministerio de Economía y Competitividad (España)
Federal Ministry of Education and Research (Germany)
German Research Foundation
European Commission
Bonn-Cologne Graduate School of Physics and Astronomy
Source :
Digital.CSIC. Repositorio Institucional del CSIC, instname
Publication Year :
2018
Publisher :
American Physical Society, 2018.

Abstract

13 pags., 12 figs., 4 tabs.<br />Transition probabilities of intermediate-spin yrast and non-yrast excitations in Se80,82 were investigated in a recoil distance Doppler-shift (RDDS) experiment performed at the Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Legnaro. The Cologne Plunger device for deep inelastic scattering was used for the RDDS technique and was combined with the AGATA Demonstrator array for the γ-ray detection and coupled to the PRISMA magnetic spectrometer for an event-by-event particle identification. In Se80, the level lifetimes of the yrast (61+) and (81+) states and of a non-yrast band feeding the yrast 41+ state are determined. A spin and parity assignment of the head of this sideband is discussed based on the experimental results and supported by large-scale shell-model calculations. In Se82, the level lifetimes of the yrast 61+ state and the yrare 42+ state and lifetime limits of the yrast (101+) state and of the 51- state are determined. Although the experimental results contain large uncertainties, they are interpreted with care in terms of large-scale shell-model calculations using the effective interactions JUN45 and jj44b. The excited states' wave functions are investigated and discussed with respect to the role of the neutron g9/2 orbital.<br />This work was partially supported by the European Union Seventh Framework Program FP7/2007-2013 under Grant Agreement No. 262010 ENSAR, by the German Research Foundation (DFG) under Contract No. DE 1516/3-1, by the German BMBF under Grant No. 05P15PKFNA and by the Spanish Ministerio de Economía y Competitividad under Contract No. FPA2014-57196-C5-4-P. J.L. and A.V. thank the Bonn-Cologne Graduate School of Physics and Astronomy (BCGS) for financial support.

Details

Database :
OpenAIRE
Journal :
Digital.CSIC. Repositorio Institucional del CSIC, instname
Accession number :
edsair.dedup.wf.001..792396e5d3c5cc6481e9687d582e0b9c