Constraint on the symmetry energy at high densities from neutron star observations using relativistic mean-field models
收藏DataCite Commons2025-04-27 更新2025-04-16 收录
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资源简介：
In this paper, we constrain the symmetry energy at high densities in nuclear matter using recent observations of neutron stars based on the calculations of relativistic mean-field (RMF) models. Using the observations of the neutron stars, we obtain the constraint on the symmetry energy at high densities, S(2ρ0) = 40.54±12.47MeV, and S(3ρ0) = 44.12±29.38MeV.
提供机构：
Science Data Bank
创建时间：
2025-03-25
