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中子星合并遗迹

Neutron star merger remnants.

作者信息

Bernuzzi Sebastiano

机构信息

Theoretisch-Physikalisches Institut, Friedrich-Schiller-Universität Jena, Max-Wien-Platz 1, 07743 Jena, Germany.

出版信息

Gen Relativ Gravit. 2020;52(11):108. doi: 10.1007/s10714-020-02752-5. Epub 2020 Nov 10.

DOI:10.1007/s10714-020-02752-5
PMID:39247669
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC11377492/
Abstract

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 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.

摘要

双中子星合并观测是在极端条件下限制基础物理学和天体物理学的独特方式。引力波事件及其电磁对应物的解释关键依赖于合并残骸的广义相对论模型。只有通过包含核物质、电磁和弱相互作用详细输入物理的多维数值相对论模拟才能获得定量模型。本综述总结了对合并残骸的当前理解，重点关注与多信使观测相关的一些方面。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4def/11377492/be9609fd273d/10714_2020_2752_Fig9_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4def/11377492/94c81322bda8/10714_2020_2752_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4def/11377492/4241341e84a1/10714_2020_2752_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4def/11377492/142ee412a09c/10714_2020_2752_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4def/11377492/8fca63faaec2/10714_2020_2752_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4def/11377492/9f6170133f97/10714_2020_2752_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4def/11377492/6dc423d88e82/10714_2020_2752_Fig6_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4def/11377492/996710849210/10714_2020_2752_Fig7_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4def/11377492/837a3b756336/10714_2020_2752_Fig8_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4def/11377492/be9609fd273d/10714_2020_2752_Fig9_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4def/11377492/94c81322bda8/10714_2020_2752_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4def/11377492/4241341e84a1/10714_2020_2752_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4def/11377492/142ee412a09c/10714_2020_2752_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4def/11377492/8fca63faaec2/10714_2020_2752_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4def/11377492/9f6170133f97/10714_2020_2752_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4def/11377492/6dc423d88e82/10714_2020_2752_Fig6_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4def/11377492/996710849210/10714_2020_2752_Fig7_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4def/11377492/837a3b756336/10714_2020_2752_Fig8_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4def/11377492/be9609fd273d/10714_2020_2752_Fig9_HTML.jpg

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Phys Rev D. 2020 Mar 15;101(6). doi: 10.1103/physrevd.101.064042. Epub 2020 Mar 19.
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Equation of State Constraints from the Threshold Binary Mass for Prompt Collapse of Neutron Star Mergers.中子星合并瞬间坍缩的阈值双星质量所产生的状态方程约束
Phys Rev Lett. 2020 Oct 2;125(14):141103. doi: 10.1103/PhysRevLett.125.141103.
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Kilonovae.
千新星
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Black-Hole Remnants from Black-Hole-Neutron-Star Mergers.黑洞-中子星合并的黑洞残余物。
Phys Rev Lett. 2019 Jul 26;123(4):041102. doi: 10.1103/PhysRevLett.123.041102.
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Identifying a First-Order Phase Transition in Neutron-Star Mergers through Gravitational Waves.通过引力波识别中子星合并中的一级相变。
Phys Rev Lett. 2019 Feb 15;122(6):061102. doi: 10.1103/PhysRevLett.122.061102.
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Signatures of Quark-Hadron Phase Transitions in General-Relativistic Neutron-Star Mergers.在广义相对论中子星合并中夸克-强子相变的特征。
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GW170817: Measurements of Neutron Star Radii and Equation of State.GW170817：测量中子星半径和物态方程。
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