论文标题
在有限温度和恒星稳定性下状态的微观核方程
Microscopic nuclear equation of state at finite temperature and stellar stability
论文作者
论文摘要
与在Brueckner-Hartree-fock形式主义中构建的所有当前天体物理构造兼容的状态核方程式均以一致的方式呈现并扩展到有限温度。详细研究了有限温度对中子恒星特性的影响，并提出了有关恒星稳定性的普遍关系。
A microscopic nuclear equation of state compatible with all current astrophysical constraints constructed within the Brueckner-Hartree-Fock formalism is presented and extended in a consistent way to finite temperature. The effects of finite temperature on the properties of neutron stars are studied in detail and a universal relation regarding stellar stability is proposed.
