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First Evidence of Axial Shape Asymmetry and Configuration Coexistence in $^{74}$Zn: Suggestion for a Northern Extension of the $N=40$ Island of Inversion

Authors :
Rocchini, M.
Garrett, P. E.
Zielinska, M.
Lenzi, S. M.
Dao, D. D.
Nowacki, F.
Bildstein, V.
MacLean, A. D.
Olaizola, B.
Ahmed, Z. T.
Andreoiu, C.
Babu, A.
Ball, G. C.
Bhattacharjee, S. S.
Bidaman, H.
Cheng, C.
Coleman, R.
Dillmann, I.
Garnsworthy, A. B.
Gillespie, S.
Griffin, C. J.
Grinyer, G. F.
Hackman, G.
Hanley, M.
Illana, A.
Jones, S.
Laffoley, A. T.
Leach, K. G.
Lubna, R. S.
McAfee, J.
Natzke, C.
Pannu, S.
Paxman, C.
Porzio, C.
Radich, A. J.
Rajabali, M. M.
Sarazin, F.
Schwarz, K.
Shadrick, S.
Sharma, S.
Suh, J.
Svensson, C. E.
Yates, D.
Zidar, T.
Publication Year :
2023

Abstract

The excited states of $N=44$ $^{74}$Zn were investigated via $\gamma$-ray spectroscopy following $^{74}$Cu $\beta$ decay. By exploiting $\gamma$-$\gamma$ angular correlation analysis, the $2_2^+$, $3_1^+$, $0_2^+$ and $2_3^+$ states in $^{74}$Zn were firmly established. The $\gamma$-ray branching and $E2/M1$ mixing ratios for transitions de-exciting the $2_2^+$, $3_1^+$ and $2_3^+$ states were measured, allowing for the extraction of relative $B(E2)$ values. In particular, the $2_3^+ \to 0_2^+$ and $2_3^+ \to 4_1^+$ transitions were observed for the first time. The results show excellent agreement with new microscopic large-scale shell-model calculations, and are discussed in terms of underlying shapes, as well as the role of neutron excitations across the $N=40$ gap. Enhanced axial shape asymmetry (triaxiality) is suggested to characterize $^{74}$Zn in its ground state. Furthermore, an excited $K=0$ band with a significantly larger softness in its shape is identified. A shore of the $N=40$ ``island of inversion'' appears to manifest above $Z=26$, previously thought as its northern limit in the chart of the nuclides.

Subjects

Subjects :
Nuclear Experiment
Nuclear Theory

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.2302.07394
Document Type :
Working Paper
Full Text :
https://doi.org/10.1103/PhysRevLett.130.122502