Properties of Neutron Stars Related to Gravitational Waves

IF 1 4区物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS

Astronomische Nachrichten Pub Date : 2025-06-29 DOI:10.1002/asna.70028

Yan Yan, Weifeng Zhang, Zhifu Gao, Hui Wang

引用次数: 0

Abstract

Neutron stars are natural laboratories of cold, dense strong interacting matter. In this article, we briefly review the gravitational waves related to neutron stars. Tidal deformability is a significant value that relates the observation of gravitational waves to the equation of state of cold, dense matter. The implicants of GW170817 and GW190814 are discussed. We also give an outlook for future work.

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与引力波有关的中子星特性

中子星是冷、密、强相互作用物质的天然实验室。在这篇文章中，我们简要地回顾了与中子星有关的引力波。潮汐可变形性是将引力波观测与冷致密物质的状态方程联系起来的一个重要值。讨论了GW170817和GW190814的含义。并对今后的工作进行了展望。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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来源期刊

Astronomische Nachrichten 地学天文-天文与天体物理

CiteScore

1.80

自引率

11.10%

发文量

审稿时长

4-8 weeks

期刊介绍： Astronomische Nachrichten, founded in 1821 by H. C. Schumacher, is the oldest astronomical journal worldwide still being published. Famous astronomical discoveries and important papers on astronomy and astrophysics published in more than 300 volumes of the journal give an outstanding representation of the progress of astronomical research over the last 180 years. Today, Astronomical Notes/ Astronomische Nachrichten publishes articles in the field of observational and theoretical astrophysics and related topics in solar-system and solar physics. Additional, papers on astronomical instrumentation ground-based and space-based as well as papers about numerical astrophysical techniques and supercomputer modelling are covered. Papers can be completed by short video sequences in the electronic version. Astronomical Notes/ Astronomische Nachrichten also publishes special issues of meeting proceedings.