Constraining nuclear symmetry energy with the charge radii of mirror-pair nuclei
Constraining nuclear symmetry energy with the charge radii of mirror-pair nuclei
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DOI:
10.1007/s41365-023-01269-1
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发表时间:
2023-03
影响因子:
2.8
通讯作者:
R. An;Shuai Sun;Li-Gang Cao;Feng-Shou Zhang
中科院分区:
文献类型:
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作者:
R. An;Shuai Sun;Li-Gang Cao;Feng-Shou Zhang
The nuclear charge radius plays a vital role in determining the equation of state of isospin asymmetric nuclear matter. Based on the correlation between the differences in charge radii of mirror-partner nuclei and the slope parameter (L) of symmetry energy at the nuclear saturation density, an analysis of the calibrated slope parameterLwas performed in finite nuclei. In this study, relativistic and nonrelativistic energy density functionals were employed to constrain the nuclear symmetry energy through the available databases of the mirror-pair nucleiCa–S,Ca–Ar, andNi–Fe. The deduced nuclear symmetry energy was located in the range 29.89–31.85 MeV, andLof the symmetry energy essentially covered the range 22.50–51.55 MeV at the saturation density. Moreover, the extractedat the sensitivity densitywas located in the interval range 30.52–39.76 MeV.