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Identifying the spin trapped character of the $^{32}$Si isomeric state

Authors :
Williams, J.
Hackman, G.
Starosta, K.
Lubna, R. S.
Choudhary, Priyanka
Srivastava, P. C.
Andreoiu, C.
Annen, D.
Asch, H.
Badanage, M. D. H. K. G.
Ball, G. C.
Beuschlein, M.
Bidaman, H.
Bildstein, V.
Coleman, R.
Garnsworthy, A. B.
Greaves, B.
Leckenby, G.
Karayonchev, V.
Martin, M. S.
Natzke, C.
Petrache, C. M.
Radich, A.
Raleigh-Smith, E.
Rhodes, D.
Russell, R.
Satrazani, M.
Spagnoletti, P.
Svensson, C. E.
Tam, D.
Wu, F.
Yates, D.
Yu, Z.
Publication Year :
2023

Abstract

The properties of a nanosecond isomer in $^{32}$Si, disputed in previous studies, depend on the evolution of proton and neutron shell gaps near the `island of inversion'. We have placed the isomer at 5505.2(2) keV with $J^{\pi} = 5^-$, decaying primarily via an $E3$ transition to the $2^+_1$ state. The $E3$ strength of 0.0841(10) W.u. is unusually small and suggests that this isomer is dominated by the $(\nu d_{3/2})^{-1} \otimes (\nu f_{7/2})^{1}$ configuration, which is sensitive to the $N=20$ shell gap. A newly observed $4^+_1$ state is placed at 5881.4(13) keV; its energy is enhanced by the $Z=14$ subshell closure. This indicates that the isomer is located in a `yrast trap', a feature rarely seen at low mass numbers.<br />Comment: Accepted, Physical Review C

Subjects

Subjects :
Nuclear Experiment

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.2311.09163
Document Type :
Working Paper