shell model
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2022 ◽  
Vol 105 (1) ◽  
Author(s):  
H. T. Xue ◽  
X. R. Zhou ◽  
S. Y. Zhang ◽  
B. C. He ◽  
Y. A. Luo ◽  
...  

2022 ◽  
pp. 122383
Author(s):  
Manvi Rajput ◽  
Suram Singh ◽  
Preeti Verma ◽  
Veerta Rani ◽  
Arun Bharti ◽  
...  

Universe ◽  
2021 ◽  
Vol 8 (1) ◽  
pp. 23
Author(s):  
Kamila Sieja

Neutron-rich Sr nuclei around N=60 exhibit a sudden shape transition from a spherical ground state to strongly prolate-deformed. Recently, much new insight into the structure of Sr isotopes in this region has been gained through experimental studies of the excited levels, transition strengths, and spectroscopic factors. In this work, a “classic” shell model description of strontium isotopes from N=50 to N=58 is provided, using a natural valence space outside the 78Ni core. Both even–even and even–odd isotopes are addressed. In particular, spectroscopic factors are computed to shed more light on the structure of low-energy excitations and their evolution along the Sr chain. The origin of deformation at N=60 is mentioned in the context of the present and previous shell model and Monte Carlo shell model calculations.


2021 ◽  
Vol 104 (6) ◽  
Author(s):  
Long-Jun Wang ◽  
Liang Tan ◽  
Zhipan Li ◽  
Bingshui Gao ◽  
Yang Sun

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