Constraining the properties of dense matter and neutron stars by combining nuclear physics and gravitational waves from GW170817

机译：通过组合GW170817结合核物理学和引力波来限制致密物质和中子恒星的性质

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Gravitational waves from neutron-star mergers are expected to provide stringent constraints on the structure of neutron stars. At the same time, recent advances in nuclear theory have enabled reliable calculations of the low density equation of state using effective field theory based Hamiltonians and advanced techniques to solve the quantum many-body problem. In this paper, we address how the first observation of gravitational waves from GW170817 can be combined with modern calculations of the equation of state to extract useful insights about the equation of state of matter encountered inside neutron stars. We analyze the impact of various uncertainties and we show that the tidal deformability extracted from GW170817 is compatible, while less constraining, than modern nuclear physics knowledge.

机译：预计来自中子 - 星相用的引力波是在中子恒星的结构上提供严格的约束。与此同时，核理论的最近进步使得使用基于有效的场理论的哈密顿人和先进的技术来实现对状态的低密度方程的可靠计算，以解决量子的多体问题。在本文中，我们解决了来自GW170817的首次观察来自GW170817的重力波动可以与现代计算的现代计算结合，以提取关于中子恒星内遇到的物质状态等式的有用见解。我们分析了各种不确定性的影响，我们表明，从GW170817提取的潮汐可变形性与现代核物理知识相比兼容。

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《Xiamen-CUSTIPEN Workshop on the Equation of State of Dense Neutron-Rich Matter in the Era of Gravitational Wave Astronomy》|2019年|1 v. (various pagings) :|共11页
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I. Tews; J. Margueron; S. Reddy;
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中图分类 P1-532;
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dense matter; neutron stars; gravitational waves;

机译：致密的物质;中子恒星;引力波;

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专利

1. Constraining Nuclear-Matter Equations of Stateby Gravitational Waves from Black Hole-Neutron Star Binaries [J] . Masaru SHIBATA, Koutarou KYUTOKU Progress of Theoretical Physics. Supplement . 2010,第186期

机译：黑洞-中子星双星的引力波约束状态的核物质方程
2. Optimal Neutron-star Mass Ranges to Constrain the Equation of State of Nuclear Matter with Electromagnetic and Gravitational-wave Observations [J] . L. R. Weih, E. R. Most, L. Rezzolla The Astrophysical journal . 2019,第1期

机译：电磁和引力波观测的约束核物质状态方程的最佳中子星质量范围
3. GW170817: Constraining the nuclear matter equation of state from the neutron star tidal deformability [J] . Malik Tuhin, Alam N., Fortin M., Physical review, C . 2018,第3期

机译：GW170817：将状态的核物质方程从中子恒星潮汐变形制约
4. Constraining the properties of dense matter and neutron stars by combining nuclear physics and gravitational waves from GW170817 [C] . I. Tews, J. Margueron, S. Reddy Xiamen-CUSTIPEN Workshop on the Equation of State of Dense Neutron-Rich Matter in the Era of Gravitational Wave Astronomy . 2019

机译：通过组合GW170817结合核物理学和引力波来限制致密物质和中子恒星的性质
5. Constraining the r-mode saturation amplitude from a hypothetical detection of r-mode gravitational waves from a newborn neutron star: Detection strategies and machine learning algorithms. [D] . Mitidis, Andonis. 2015

机译：通过假设检测来自新生中子星的r模式引力波来约束r模式饱和幅度：检测策略和机器学习算法。
6. Gravitational waves from neutron stars and asteroseismology [O] . Wynn C. G. Ho -1

机译：来自中子星和星震学的引力波
7. Constraining the properties of dense matter and neutron stars by combining nuclear physics and gravitational waves from GW170817 [O] . I. Tews, J. Margueron, S. Reddy 2019

机译：通过组合GW170817结合核物理学和引力波来限制致密物质和中子恒星的性质

Constraining the properties of dense matter and neutron stars by combining nuclear physics and gravitational waves from GW170817

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