标题： 中子星状态方程：QMF建模与应用 显示英文标题

标题： Neutron star equation of state: QMF modeling and applications

摘要： 由于核物质多体理论的发展，密集物质的状态方程（EOS）这一长期悬而未决的问题可能通过理论计算与实验室测量的核性质和反应以及天文学中日益精确的观测结果的对比，在不久的将来得到理解。 在本综述中，我们关注以下六个方面：1）提供对夸克平均场（QMF）模型的概述，该模型从夸克势出发，一致地描述核子和多体核子系统；2）将QMF应用于核物质和中子星；3）将QMF形式扩展到对超核和超子物质以及超子星的描述；4）通过结合具有声速特征的夸克物质模型来探索强子-夸克相变和混合星；5）通过双星合并事件GW170817的引力波信号和电磁信号来约束夸克间相互作用；6）讨论进一步研究致密物质EOS的机会，例如通过致密天体，如中子星冷却和脉冲星跳变。 显示英文摘要

摘要： Because of the development of many-body theories of nuclear matter, the long-standing, open problem of the equation of state (EOS) of dense matter may be understood in the near future through the confrontation of theoretical calculations with laboratory measurements of nuclear properties \& reactions and increasingly accurate observations in astronomy. In this review, we focus on the following six aspects: 1) providing a survey of the quark mean-field (QMF) model, which consistently describes a nucleon and many-body nucleonic system from a quark potential; 2) applying QMF to both nuclear matter and neutron stars; 3) extending QMF formalism to the description of hypernuclei and hyperon matter, as well as hyperon stars; 4) exploring the hadron-quark phase transition and hybrid stars by combining the QMF model with the quark matter model characterized by the sound speed; 5) constraining interquark interactions through both the gravitational wave signals and electromagnetic signals of binary merger event GW170817; and 6) discussing further opportunities to study dense matter EOS from compact objects, such as neutron star cooling and pulsar glitches.