https://doi.org/10.1140/epja/i2017-12213-x
Regular Article - Experimental Physics
Study of the
decay of 116m1In: A new interpretation of low-lying 0+ states in 116Sn
1
Department of Chemistry, Simon Fraser University, 8888 University Drive, V5A 1S6, Burnaby BC, Canada
2
TRIUMF, 4004 Wesbrook Mall, V6T 2A3, Vancouver BC, Canada
3
Department of Physics, University of Guelph, 50 Stone Road, N1G 2W1, Guelph ON, Canada
4
Department of Astronomy and Physics, Saint Mary’s University, 923 Robie Street, B3H 3C3, Halifax NS, Canada
5
CSNSM, CNRS-IN2P3, Universite Paris-Saclay, 91405, Orsay Cedex, France
6
School of Physics, Georgia Institute of Technology, 837 State Street, 30332-0430, Atlanta, GA, USA
7
Departments of Chemistry and Physics & Astronomy, University of Kentucky, 40506-0055, Lexington, KY, USA
* e-mail: jpore@lbl.gov
Received:
6
December
2016
Accepted:
24
January
2017
Published online:
16
February
2017
The 116Sn nucleus contains a collective rotational band originating from proton 2p-2h excitations across the proton
shell gap. Even though this nucleus has been extensively investigated in the past, there was still missing information on the low-energy interband transitions connecting the intruder and normal structures. The low-lying structure of 116Sn was investigated through a high-statistics study of the
decay of 116m1In with the
spectrometer and its ancillary detectors at TRIUMF. These measurements are critical in order to properly characterize the
2p-2h rotational band. Weak
-decay branches are observed utilizing
-
coincidence spectroscopy methods, leading to the first direct observation of the 85 keV
ray with a transition strength of
W.u. The analysis of these results strongly suggests that the 2027 keV
state should replace the previously assigned 1757 keV
state as the band-head of the
2p-2h rotational band.
© SIF, Springer-Verlag Berlin Heidelberg, 2017