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arXiv 1805.04780nucl-thastro-ph.SRnucl-ex
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多信使天文学新时代的核天体物理

Nuclear Astrophysics in the New Era of Multimessenger Astronomy

J. Piekarewicz

摘要:

中子星是在密度和中子质子不对称的极端条件下探索物质的独特宇宙实验室。由于其巨大的动态范围,中子星展示了无数奇异的物质状态,在正常的实验室条件下是不可能重现的。在这三个讲座中,我将讨论核物理学和天体物理学之间的强大协同作用将如何揭示这些迷人物体背后的一些最深层次的秘密。特别是,我将强调的巨大影响,第一次检测到的引力波从双中子星合并GW 170817是在约束的组成,结构和动力学的中子星。

英文摘要:

Neutron stars are unique cosmic laboratories for the exploration of matter under extreme conditions of density and neutron-proton asymmetry. Due to their enormous dynamic range, neutron stars display a myriad of exotic states of matter that are impossible to recreate under normal laboratory conditions. In these three lectures I will discuss how the strong synergy that has developed between nuclear physics and astrophysics will uncover some of the deepest secrets behind these fascinating objects. In particular, I will highlight the enormous impact that the very first detection of gravitational waves from the binary neutron-star merger GW170817 is having in constraining the composition, structure, and dynamics of neutron stars.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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