手征平均场模型下的中子星状态方程
Tabulated Neutron Star Equations of State Modeled within the Chiral Mean Field Model
摘要：
在这篇特刊文章中，我回顾了手征平均场（CMF）模型的一些成就，它包含核子、超子和夸克的自由度，以及它在原中子星和中子星中的应用。我还提出了一套状态方程和粒子的人口表使用CMF模型的物理约束条件下，需要重现不同的环境，如那些存在于冷中子星，核心坍缩超新星爆炸和不同阶段的紧凑型恒星合并。
英文摘要：
In this special issue article, I review some of the accomplishments of the chiral mean field (CMF) model, which contains nucleon, hyperon, and quark degrees of freedom, and its applications to proto-neutron and neutron stars. I also present a set of equation of state and particle population tables built using the CMF model subject to physical constraints necessary to reproduce different environments, such as those present in cold neutron stars, core-collapse supernova explosions and different stages of compact star mergers.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
