摘要
对中子星状态方程作了简介,对核物质能量密度的计算的近似方法作了说明。以此为基础,研究了相互能对总能量的贡献,把相互能引入计算中,得到中子星质量、半径及密度的关系。
In this paper,we have made a brief introduction to the equation of state of neutron star and the approximation method to calculate the energy density of nuclear matter.On this basis,we researched the contribution that the correlation energy had done to the total energy,and by introducing it into the calculation,we got the relation between the mass,radius and density of the neutron star.
出处
《山西大同大学学报(自然科学版)》
2011年第2期27-29,共3页
Journal of Shanxi Datong University(Natural Science Edition)
关键词
中子星
核物质
能量密度
neutron star
nuclear matter
energy density