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γ-ray spectroscopy of low-lying yrast and non-yrast states in neutron- rich 94,95,96Kr

Authors :
Gerst, R-B
Blazhev, A.
Moschner, K.
Doornenbal, P.
Obertelli, A.
Nomura, K.
Ebran, J-P
Hilaire, S.
Libert, J.
Authelet, G.
Baba, H.
Calvet, D.
Chateau, F.
Chen, S.
Corsi, A.
Delbart, A.
Gheller, J-M
Giganon, A.
Gillibert, A.
Lapoux, V
Motobayashi, T.
Niikura, M.
Paul, N.
Rousse, J-Y
Sakurai, H.
Santamaria, C.
Steppenbeck, D.
Taniuchi, R.
Uesaka, T.
Ando, T.
Arici, T.
Browne, F.
Bruce, A. M.
Caroll, R.
Chung, L. X.
Cortes, M. L.
Dewald, M.
Ding, B.
Flavigny, F.
Franchoo, S.
Gorska, M.
Gottardo, A.
Jolie, J.
Jungclaus, A.
Lee, J.
Lettmann, M.
Linh, B. D.
Liu, J.
Liu, Z.
Lizarazo, C.
Momiyama, S.
Nagamine, S.
Nakatsuka, N.
Nita, C. R.
Nobs, C.
Olivier, L.
Orlandi, R.
Patel, Z.
Podolyak, Zs
Rudigier, M.
Saito, T.
Shand, C.
Soderstrom, P-A
Stefan, I
Vaquero, V.
Werner, V
Wimmer, K.
Xu, Z.
Publication Year :
2022

Abstract

We report on γ -ray spectroscopy of low-lying excited states in the neutron-rich 94, 95, 96Kr isotopes measured as part of the “Shell Evolution And Search for Two-plus energies At RIBF” (SEASTAR) campaign at the RIKEN Radioactive Isotope Beam Factory. Excited yrast and non-yrast states were observed, and half-lives extracted via GEANT4 simulations. In 94, 96Kr candidates for the 3− 1 state were identified. For 95Kr, the prompt SEASTAR data were combined with delayed spectroscopic data measured with the EURICA array to observe transitions on top of the known (7/2)+ isomer at a level energy of 195.5(3) keV. The comparison of the new experimental results with five-dimensional collective Hamiltonian (5DCH) and mapped interacting boson model (IBM) calculations, both using the Gogny D1M interaction, could suggest oblate-prolate shape coexistence already in 96Kr.

Details

Language :
English
Database :
OpenAIRE
Accession number :
edsair.57a035e5b1ae..ee878177dc00e96894fbdbcb5dd57f86