Equation of state of neutron star matter

Weber F

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Equation of state of neutron star matter

机译：中子星物质的状态方程

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摘要

The physical properties of neutron star matter at supernuclear densities are highly uncertain and the associated equation of state is only very poorly known. This has its origin in numerous sources which are discussed in this paper.

机译：中子星物质在超核密度下的物理特性是高度不确定的，并且相关的状态方程只是鲜为人知。这源于本文讨论的众多来源。

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《International journal of modern physics, D. Gravitation, astrophysics, cosmology 》 |2004年第7期| 共12页
作者
Weber F;
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正文语种 eng
中图分类物理学 ;
关键词
equation of state; dense matter; phase transitions; THOMAS-FERMI MODEL; HEAVY-ION COLLISIONS; MEAN-FIELD THEORY; NUCLEAR-MATTER; COMPACT STARS; COLOR SUPERCONDUCTIVITY; HADRONIC MATTER; UNSTABLE NUCLEI; KAON PRODUCTION; QUARK MATTER;

机译：状态方程;稠密物质;相变;托马斯-费米模型;重离子碰撞;均质理论;核物质;压紧星;色超导;

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机译：从双重魔术核，AB初始中子物质的AB Initio计算和中子恒星的Skyrme方程的限制
2. Role of the symmetry energy and the neutron-matter stiffness on the tidal deformability of a neutron star with unified equations of state [J] . Perot L., Chamel N., Sourie A. Physical review, C . 2019 ,第3期

机译：对称能量的作用与中子物质刚度对中子星的潮汐可变形性，具有统一状态的统一方程
3. How Well Do We Know the Neutron-Matter Equation of State at the Densities Inside Neutron Stars? A Bayesian Approach with Correlated Uncertainties [J] . Drischler C., Furnstahl R. J., Melendez J. A., Physical review letters . 2020 ,第20期

机译：我们如何在中子恒星内部的密度知道状态的中子物质方程？具有相关不确定性的贝叶斯方法
4. Nuclear Matter Equations of State and the Neutron Stars [C] . M. Urbanec, E. Běták, Z. Stuchlík International Conference on Frontiers in Nuclear Structure, Astrophysics and Reactions . 2008

机译：状态和中子恒星的核物质方程
5. Neutron stars and the equation of state of dense matter. [D] . Carriere, Josef. 2005

机译：中子星和致密物质的状态方程。
6. Inner Workings: Physicists look to a new telescope to understand neutron stars and matter at the extremes [O] . Stephen Ornes 2020

机译：内在工作：物理学家向一个新的望远镜看了解中子恒星和极端物质
7. How Well Do We Know the Neutron-Matter Equation of State at the Densities Inside Neutron Stars? A Bayesian Approach with Correlated Uncertainties [O] . C. Drischler, R. J. Furnstahl, J. A. Melendez, 2020

机译：我们如何在中子恒星内部的密度知道状态的中子物质方程？具有相关不确定性的贝叶斯方法

Equation of state of neutron star matter

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