Reconstructing the equation of state for cold nuclear matter from the relationship of any two properties of neutron stars
Reconstructing the equation of state for cold nuclear matter from the relationship of any two properties of neutron stars
复制标题
根据中子星任意两个性质的关系重建冷核物质的状态方程
DOI：
10.1103/physrevc.64.048801
复制
发表时间：
2001
影响因子：
3.1
通讯作者：
T. Harada
中科院分区：
文献类型：
--
作者：
T. Harada
发展了一种直接的方法，从中子星的质量、半径、转动惯量、重子质量、结合能、引力红移及其组合等任意两个性质之间的关系，重建高密度核物质的物态方程。
A direct method is developed to reconstruct the equation of state for high-density nuclear matter from the relationship between any two properties of neutron stars, such as masses, radii, moments of inertia, baryonic masses, binding energies, gravitational redshifts, and their combinations.