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General Relativity and Quantum Cosmology

arXiv:1608.02582v1 (gr-qc)
[Submitted on 8 Aug 2016 (this version) , latest version 24 Mar 2023 (v2) ]

Title: Approximate Universal Relations for Neutron Stars and Quark Stars

Title: 中子星和夸克星的近似普遍关系

Authors:Kent Yagi, Nicolas Yunes
Abstract: Neutron stars and quark stars are ideal laboratories to study fundamental physics at supra nuclear densities and strong gravitational fields. Astrophysical observables, however, depend strongly on the star's internal structure, which is currently unknown due to uncertainties in the equation of state. Universal relations, however, exist among certain stellar observables that do not depend sensitively on the star's internal structure. One such set of relations is between the star's moment of inertia ($I$), its tidal Love number (Love) and its quadrupole moment ($Q$), the so-called I-Love-Q relations. Similar relations hold among the star's multipole moments, which resemble the well-known black hole no-hair theorems. Universal relations break degeneracies among astrophysical observables, leading to a variety of applications: (i) X-ray measurements of the nuclear matter equation of state, (ii) gravitational wave measurements of the intrinsic spin of inspiraling compact objects, and (iii) gravitational and astrophysical tests of General Relativity that are independent of the equation of state. We here review how the universal relations come about and all the applications that have been devised to date.
Abstract: 中子星和夸克星是研究超核密度和强引力场下基本物理的理想实验室。 天体物理可观测量却强烈依赖于恒星的内部结构,而由于状态方程的不确定性,目前尚不清楚内部结构。 然而,某些恒星可观测量之间存在普遍关系,这些关系对恒星的内部结构不敏感。 其中一组关系是恒星的转动惯量($I$)、潮汐洛夫数(Love)和四极矩($Q$)之间的关系,即所谓的I-Love-Q关系。 类似的關係也存在于恒星的多極矩之間,這些關係類似於著名的黑洞無毛定理。 普遍關係打破了天體物理可觀測量之間的歧義,導致了多種應用:(i) X射線測量核物質狀態方程,(ii) 通過引力波測量漸近緊密天體的固有自旋,以及 (iii) 獨立於狀態方程的廣義相對論的引力和天體物理測試。 我們在此回顧普遍關係是如何產生的,以及迄今為止設計的所有應用。
Comments: 89 pages, 38 figures; review article submitted to Physics Reports
Subjects: General Relativity and Quantum Cosmology (gr-qc) ; High Energy Astrophysical Phenomena (astro-ph.HE)
Cite as: arXiv:1608.02582 [gr-qc]
  (or arXiv:1608.02582v1 [gr-qc] for this version)
  https://doi.org/10.48550/arXiv.1608.02582
arXiv-issued DOI via DataCite
Related DOI: https://doi.org/10.1016/j.physrep.2017.03.002
DOI(s) linking to related resources

Submission history

From: Kent Yagi [view email]
[v1] Mon, 8 Aug 2016 20:00:00 UTC (3,829 KB)
[v2] Fri, 24 Mar 2023 02:39:08 UTC (3,837 KB)
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