摘要
应用相对论核场理论，采用手征对称及其自发破缺模型得到了中子体系的场方程，计算了中子星的几个常见的宏观物理参量，得到了较为理想的计算结果．
The saturating chiral breaking field theory is applied to study the equation of the state in the framework of mean field theory.The macroscopic properties of dense neutron system are calculated with the general relativistic stellar structure equations.
出处
《宁夏大学学报（自然科学版）》
CAS
1997年第3期241-244,共4页
Journal of Ningxia University(Natural Science Edition)
关键词
手征对称
平均场近似
中子星
the chiral symmetry
the Hartree approximation
neutron stars
