论文标题
中子星级残留
Neutron Star Merger Remnants
论文作者
论文摘要
二进制中子恒星合并观察是极端限制基本物理和天体物理学的独特方法。重力波事件及其电磁对应物的解释至关重要地依赖于合并残余的一般性模型。定量模型只能通过在3+1个维数的数值相对性模拟中获得，包括核物质，电磁和弱相互作用的详细输入物理。这篇综述总结了当前对合并残余物的理解，这些遗迹重点介绍了与多中文观察相关的某些方面。
Binary neutron star mergers observations are a unique way to constrain fundamental physics and astrophysics at the extreme. The interpretation of gravitational-wave events and their electromagnetic counterparts crucially relies on general-relativistic models of the merger remnants. Quantitative models can be obtained only by means of numerical relativity simulations in 3+1 dimensions including detailed input physics for the nuclear matter, electromagnetic and weak interactions. This review summarizes the current understanding of merger remnants focusing on some of the aspects that are relevant for multimessenger observations.
