论文标题
中子星核中的QCD
QCD in the cores of neutron stars
论文作者
论文摘要
我讨论为什么在渐近高密度下可靠的巨大化学电位状态方程的最先进的QCD计算限制了中子星密度下相同的状态方程。我描述了这些理论计算如何在较低密度下影响EOS。我认为，QCD中的AB-Initio计算提供了有关中子星形物质状态方程的重要信息，这与当前的天体物理观察互补。
I discuss why state-of-the art perturbative QCD calculations of the equation of state at large chemical potential that are reliable at asymptotically high densities constrain the same equation of state at neutron-star densities. I describe how these theoretical calculations affect the EOS at lower density. I argue that the ab-initio calculations in QCD offer significant information about the equation of state of the neutron-star matter, which is complementary to the current astrophysical observations.
