标题： 中子星结构来自QCD 显示英文标题

标题： Neutron star structure from QCD

摘要： 在本综述文章中，我们主张利用源自高密度和低密度下第一性原理计算的冷QCD物质热力学性质的当前理解，有效地约束中子星的宏观性质。 特别是，我们证明结合从手征有效理论和微扰QCD得到的前沿结果以及中子星质量的现有界限，可以以优于30%的精度获得中子星物质的状态方程的所有密度范围。 显示英文摘要

摘要： In this review article, we argue that our current understanding of the thermodynamic properties of cold QCD matter, originating from first principles calculations at high and low densities, can be used to efficiently constrain the macroscopic properties of neutron stars. In particular, we demonstrate that combining state-of-the-art results from Chiral Effective Theory and perturbative QCD with the current bounds on neutron star masses, the Equation of State of neutron star matter can be obtained to an accuracy better than 30% at all densities.