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Enhanced Quadrupole and Octupole Strength in Doubly Magic Sn132

Authors :
Marc Huyse
Karl Johnston
Daniel Cox
P. Reiter
A. Vogt
M L Lozano Benito
J. Ojala
A. Blazhev
L. Kaya
Joakim Cederkäll
Jose Rodriguez
H. Naïdja
Tomoaki Togashi
M. Seidlitz
B. Siebeck
T. Berry
A. Illana
K. O. Zell
N. Warr
C. Henrich
F. Wenander
Janne Pakarinen
F. Nowacki
M. Queiser
H. De Witte
J. Snäll
Liam Gaffney
E. Siesling
Hie-Isolde Collaborations
D. Rosiak
Yusuke Tsunoda
María José García Borge
Miniball
G. Rainovski
K. Arnswald
Gianluca Colò
P. Van Duppen
M. von Schmid
Takaharu Otsuka
R. Hirsch
Th. Kröll
Source :
Physical Review Letters. 121
Publication Year :
2018
Publisher :
American Physical Society (APS), 2018.

Abstract

The first 2+ and 3- states of the doubly magic nucleus Sn132 are populated via safe Coulomb excitation employing the recently commissioned HIE-ISOLDE accelerator at CERN in conjunction with the highly efficient MINIBALL array. The Sn132 ions are accelerated to an energy of 5.49 MeV/nucleon and impinged on a Pb206 target. Deexciting γ rays from the low-lying excited states of the target and the projectile are recorded in coincidence with scattered particles. The reduced transition strengths are determined for the transitions 0g.s.+→21+, 0g.s.+→31-, and 21+→31- in Sn132. The results on these states provide crucial information on cross-shell configurations which are determined within large-scale shell-model and Monte Carlo shell-model calculations as well as from random-phase approximation and relativistic random-phase approximation. The locally enhanced B(E2;0g.s.+→21+) strength is consistent with the microscopic description of the structure of the respective states within all theoretical approaches. The presented results of experiment and theory can be considered to be the first direct verification of the sphericity and double magicity of Sn132. (Less)

Details

ISSN :
10797114 and 00319007
Volume :
121
Database :
OpenAIRE
Journal :
Physical Review Letters
Accession number :
edsair.doi...........a19566cdfafe1e9b3488a996854d5d49
Full Text :
https://doi.org/10.1103/physrevlett.121.252501