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Quasi-SU(3) coupling of (1h11/2,2f7/2) across the N=82 shell gap: Enhanced E2 collectivity and shape evolution in Nd isotopes

K. Kaneko1, N. Shimizu2, T. Mizusaki3, and Y. Sun4,*

  • 1Department of Physics, Kyushu Sangyo University, Fukuoka 813-8503, Japan
  • 2Center for Nuclear Study, The University of Tokyo, 7-3-1 Hongo Bunkyo, Tokyo 113-0033, Japan
  • 3Institute of Natural Sciences, Senshu University, Tokyo 101-8425, Japan
  • 4School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China

  • *Corresponding author: sunyang@sjtu.edu.cn

Phys. Rev. C 103, L021301 – Published 3 February, 2021

DOI: https://doi.org/10.1103/PhysRevC.103.L021301

Abstract

The essence of the quasi-SU(3) coupling scheme suggested by Zuker et al. is that the high-j intruder orbit alone is insufficient to induce required large collectivity, and it is necessary for the high-j orbit to correlate through the quadrupole interaction with another higher-lying orbit with Δj=2. To extend this idea to the medium-heavy mass region, we investigate the systematics of energy levels and B(E2) values for Sn, Te, Xe, Ba, Ce, Nd, and Sm isotopes by applying the recently proposed realistic PMMU shell model. The calculations are performed by using the projected Hartree-Fock-Bogolyubov plus generator coordinate method in the model space of (1g9/2,1g7/2,2d5/2,2d3/2,3s1/2,1h11/2). The calculations describe well the experimental data over a wide range of nuclei. However, it is found that, in some nuclei close to the neutron midshell, Ce124,126, Nd130,132, and Sm134, the calculated B(E2;21+→01+) values underestimate the data considerably. This problem can be resolved by inclusion of the 2f7/2 orbit into the model space, which, with 1h11/2, forms a quasi-SU(3) coupling scheme. It is shown that the QQ interaction between the SU(3)-partner 1h11/2−2f7/2 is a driving force for enhanced E2 collectivity in the above nuclei and is responsible for the shape evolution in Nd isotopes. In addition, the participation of the 2f7/2 orbit in the model space favors prolate shape in the ground state of N≤76 isotopes, thus subverting the oblate result from the same calculation but without 2f7/2.

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