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Observation of $\gamma$-vibrations and alignments built on non-ground-state configurations in 156Dy

Authors :
Majola, S. N. T.
Hartley, D. J.
Riedinger, L. L.
Sharpey-Schafer, J. F.
Allmond, J. M.
Beausang, C.
Carpenter, M. P.
Chiara, C. J.
Cooper, N.
Curien, D.
Gall, B. J. P.
Garrett, P. E.
Janssens, R. V. F.
Kondev, F. G.
Kulp, W. D.
Lauritsen, T.
McCutchan, E. A.
Miller, D.
Piot, J.
Redon, N.
Riley, M. A.
Simpson, J.
Stefanescu, I.
Werner, V.
Wang, X.
Wood, J. L.
Yu, C. -H.
Zhu, S.
Source :
Phys. Rev. C 91, 034330 (2015)
Publication Year :
2020

Abstract

The exact nature of the lowest $K^\pi =2_\gamma ^+$ rotational bands in all deformed nuclei remains obscure. Traditionally they are assumed to be collective vibrations of the nuclear shape in the $\gamma$ degree of freedom perpendicular to the nuclear symmetry axis. Very few such $\gamma$-bands have been traced past the usual back-bending rotational alignments of high-j nucleons. We have investigated the structure of positive-parity bands in the N=90 nucleus 156Dy, using the 148Nd(12C,4n)156Dy reaction at 65 MeV, observing the resulting ${\gamma}$-ray transitions with the Gammasphere array. The even- and odd-spin members of the $K^\pi =2_\gamma^+$ $\gamma$-band are observed to 32+ and 31+ respectively. This rotational band faithfully tracks the ground-state configuration to the highest spins. The members of a possible $\gamma$-vibration built on the aligned yrast S-band are observed to spins 28+ and 27+. An even-spin positive-parity band, observed to spin 24+, is a candidate for an aligned S-band built on the seniority-zero configuration of the $0_2^+$ state at 676 keV. The crossing of this band with the $0_2^+$ band is at $\hbar\omega$= 0.28(1) MeV and is consistent with the configuration of the $0_2^+$ band not producing any blocking of the monopole pairing.<br />Comment: Published in Physics Review C

Subjects

Subjects :
Nuclear Experiment
Nuclear Theory

Details

Database :
arXiv
Journal :
Phys. Rev. C 91, 034330 (2015)
Publication Type :
Report
Accession number :
edsarx.2005.04706
Document Type :
Working Paper
Full Text :
https://doi.org/10.1103/PhysRevC.91.034330