Origin of symmetry energy in finite nuclei and density dependence of nuclear matter symmetry energy from measured alpha-decay energies
Jianmin Dong, Wei Zuo, Jianzhong Gu

TL;DR
This paper investigates the origin of symmetry energy in finite nuclei, showing the surface contribution dominates, and develops a macroscopic method using alpha decay energies to analyze the density dependence of nuclear matter symmetry energy.
Contribution
It introduces a surface-focused analysis of symmetry energy and a novel macroscopic method to determine symmetry energy coefficients from experimental alpha decay data.
Findings
Surface symmetry energy dominates in heavy nuclei.
The macroscopic method yields consistent symmetry energy coefficients.
Neutron skin thickness of 208Pb aligns with pygmy dipole resonance data.
Abstract
Based on the Skyrme energy density functional, the spatial distribution of the symmetry energy of a finite nucleus is derived in order to examine whether the symmetry energy of a finite nucleus originates from its interior or from its surface. It is found that the surface part of a heavy nucleus contributes dominantly to its symmetry energy compared to its inner part. The symmetry energy coefficient is then directly extracted and the ratio of the surface symmetry coefficient to the volume symmetry coefficient is estimated. Meanwhile, with the help of experimental alpha decay energies, a macroscopic method is developed to determine the symmetry energy coefficient of heavy nuclei. The resultant is used to analyze the density dependence of the symmetry energy coefficient of nuclear matter around the saturation density, and furthermore,…
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