摘要
Mirror energy difference is a key observable in isospin symmetry breaking,containing rich information about nuclear structure.Understanding the mechanisms underlying mirror energy difference is important in nuclear physics.In the present work,we extensively investigated mirror energy difference using ab initio valence-space inmedium similarity renormalization group approach,focusing specifically on sd-shell nuclei.The low-lying spectra of Al isotopes and N=8 isotones,together with their mirror nuclei,were calculated,followed by a systematic analysis of the evolution of the mirror energy difference.The results suggest that the large mirror energy difference is mainly caused by the weakly-bound effects and large average occupations of the 1s1/2 orbit.Lastly,we compare the results of our ab initio calculations with shell model results,elucidating the relationship and coherence between these two models.
作者
李红蕙
李健国
谢萌冉
左维
Hong-Hui Li;Jian-Guo Li;Meng-Ran Xie;Wei Zuo(Institute of Modern Physics,Chinese Academy of Sciences,Lanzhou 730000,China;School of Nuclear Science and Technology,University of Chinese Academy of Sciences,Beijing 100049,China)
基金
the National Natural Science Foundation of China(12205340,11975282)
the Gansu Natural Science Foundation(22JR5RA123)
the Special Research Assistant Project of the Chinese Academy of Sciences
the Strategic Priority Research Program of Chinese Academy of Sciences(XDB34000000)
the Key Research Program of the Chinese Academy of Sciences(XDPB15)
the State Key Laboratory of Nuclear Physics and Technology,Peking University(NPT2020KFY13)。