用引力波探测黑洞与相对论恒星
广义相对论与量子宇宙学
2007-05-23 v1
摘要
在未来十年中,引力波将把黑洞与恒星的广义相对论方面的研究从主要理论性的工作转变为高度互动的观测/理论工作。例如,引力波观测应能使我们以观测方式绘制静态黑洞周围的时空几何,定量研究黑洞碰撞中弯曲时空的高度非线性振动,探测中子星的结构及其状态方程,搜寻玻色子星、孤子星和裸奇点等奇异类型的广义相对论天体,并探测引力子的引力场和引力波尾对辐射反作用的影响等尚未观测到的广义相对论方面。
引用
@article{arxiv.gr-qc/9706079,
title = {Probing Black Holes and Relativistic Stars with Gravitational Waves},
author = {Kip S. Thorne},
journal= {arXiv preprint arXiv:gr-qc/9706079},
year = {2007}
}
备注
Latex Manuscript with nine eps figures included via "special" commands. Submitted for publication in the book Black Holes and Relativistic Stars, Proceedings of a Conference in Memory of S. Chandrasekhar, Ed. R. M. Wald (University of Chicago Press, Chicago). Large portions are adapted and updated from the author's previous gravitational-wave review articles