Calculation of nuclear charge radii with a trained feed-forward neural network

IF 3.2 2区 物理与天体物理 Q2 PHYSICS, NUCLEAR Physical Review C Pub Date : 2020-11-17 DOI:10.1103/physrevc.102.054323
Di Wu, C. Bai, H. Sagawa, H. Q. Zhang
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引用次数: 16

Abstract

A feed-forward neural network model is trained to calculate the nuclear charge radii. The model is trained with the input data set of proton and neutron number Z,N, the electric quadrupole transition strength B(E2) from the first excited 2+ state to the ground state, together with the symmetry energy. The model reproduces well not only the isotope dependence of charge radii, but also the kinks of charge radii at the neutron magic numbers N=82 for Sn and Sm isotopes, and also N=126 for Pb isotopes. The important role of the B(E2) value is pointed out to reproduce the kink of the isotope dependence of charge radii in these nuclei. Moreover, with the inclusion of the symmetry energy term in the inputs, the charge radii of Ca isotopes are well reproduced. This result suggests a new correlation between the symmetry energy and charge radii of Ca isotopes. The Skyrme Hartree-Fock-Bogoliubov calculation is performed to confirm the existence of this correlation in a microscopic model.
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用训练好的前馈神经网络计算核电荷半径
训练前馈神经网络模型来计算核电荷半径。模型使用质子和中子数Z、N、从第一激发态到基态的电四极跃迁强度B(E2)以及对称能等输入数据集进行训练。该模型不仅能很好地再现电荷半径的同位素依赖性,而且还能很好地再现Sn和Sm同位素在N=82和Pb同位素在N=126处的电荷半径结。指出了B(E2)值在再现这些原子核中电荷半径的同位素依赖性方面的重要作用。此外,在输入中加入对称能项后,可以很好地再现Ca同位素的电荷半径。这一结果提示了Ca同位素的对称能与电荷半径之间的新关系。在微观模型中进行了Skyrme Hartree-Fock-Bogoliubov计算以证实这种相关性的存在。
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来源期刊
Physical Review C
Physical Review C PHYSICS, NUCLEAR-
CiteScore
5.80
自引率
35.50%
发文量
863
期刊介绍: Physical Review C (PRC) is a leading journal in theoretical and experimental nuclear physics, publishing more than two-thirds of the research literature in the field. PRC covers experimental and theoretical results in all aspects of nuclear physics, including: Nucleon-nucleon interaction, few-body systems Nuclear structure Nuclear reactions Relativistic nuclear collisions Hadronic physics and QCD Electroweak interaction, symmetries Nuclear astrophysics
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