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Shapes, softness, and nonyrast collectivity in $^{186}\mathrm{W}$

Authors :
Prasher, V.S.
Mitchell, A.J.
Lister, C.J.
Chowdhury, P.
Afanasieva, L.
Albers, M.
Chiara, C.J.
Carpenter, M.P.
Cline, D.
D'Olympia, N.
Guess, C.J.
Hayes, A.B.
Hoffman, C.R.
Janssens, R.V.F.
Kay, B.P.
Khoo, T.L.
Korichi, A.
Lauritsen, T.
Merchan, E.
Qiu, Y.
Seweryniak, D.
Shearman, R.
Tandel, S.K.
Verras, A.
Wu, C.Y.
Zhu, S.
Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab)
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)
Source :
Physical Review C, Physical Review C, American Physical Society, 2021, 104 (4), pp.044318. ⟨10.1103/PhysRevC.104.044318⟩
Publication Year :
2021
Publisher :
HAL CCSD, 2021.

Abstract

International audience; Nonyrast, excited states in neutron-rich W186 were populated via inelastic-scattering reactions using beams of Xe136 nuclei accelerated to 725 and 800 MeV. Levels populated in the reactions were investigated via particle-γ coincidence techniques using the Gammasphere array of high-purity germanium detectors and the compact heavy-ion counter, CHICO2. The Kπ=2+ (γ), Kπ=0+ and Kπ=2− (octupole) rotational side bands were extended to spins 14ℏ, 12ℏ, and 13ℏ, respectively. A staggering pattern observed in the energies of levels in the Kπ=2+ band was found to be consistent with a potential that gets softer to vibration in the γ degree of freedom with increasing spin. The odd-even staggering of states in the Kπ=2− band was found to exhibit a phase opposite to that seen in the γ band; an effect most probably associated with Coriolis coupling to other, unobserved octupole vibrational bands in W186.

Details

Language :
English
ISSN :
24699985 and 24699993
Database :
OpenAIRE
Journal :
Physical Review C, Physical Review C, American Physical Society, 2021, 104 (4), pp.044318. ⟨10.1103/PhysRevC.104.044318⟩
Accession number :
edsair.dedup.wf.001..a00189cf1e1d3d5bf235d509f1c83551
Full Text :
https://doi.org/10.1103/PhysRevC.104.044318⟩