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The boundary of the N=90 shape phase transition: $^{148}$Ce
Koseoglou, P.GSI* ; Werner, V. ; Pietralla, N. ; Ilieva, S. K.GSI*Extern* ; Thürauf, M. ; Bernards, C. ; Blanc, A. ; Bruce, A. M. ; Cakirli, R. B. ; Cooper, N. ; Fraile, L. M. ; de France, G. ; Jentschel, M. ; Jolie, J. ; Koester, U. ; Korten, W. ; Kröll, T. ; Lalkovski, S.GSI* ; Mach, H. ; Mărginean, N. ; Mutti, P. ; Patel, Z. ; Paziy, V. ; Podolyák, Z. ; Regan, P. H. ; Régis, J.-M. ; Roberts, O. J. ; Saed-Samii, N. ; Simpson, G. S. ; Soldner, T. ; Ur, C. A. ; Urban, W. ; Wilmsen, D. ; Wilson, E.
2018
IOP Publ.
Bristol
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Please use a persistent id in citations: doi:10.1088/1742-6596/1023/1/012022 doi:10.15120/GSI-2019-00362
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Contributing Institute(s):
- Kernspektroskopie (KSP)
Research Program(s):
- 612 - Cosmic Matter in the Laboratory (POF3-612) (POF3-612)
- HGF-IVF-VH-GS-201 - HGS-HIRe : (HGF-IVF-VH-GS-201) (HGF-IVF-VH-GS-201)
Appears in the scientific report
2018
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