中子星致密结构与引力波
天体物理学
2007-05-23 v1
摘要
目录：1.引言 2.致密晕体的形成与成分 3.晕体底层：异种核形状与拓扑结构 4.致密晕体对星体质量与转动惯性的贡献 5.致密核心 6.变形、弹性应变与山丘 7.旋转部分致密中子星的形状与能量 8.椭圆率与预cession 9.来自预cession 脉冲星的引力波 10.来自预cession 脉冲星的引力波与脉冲计 11.探测可行性
关键词
引用
@article{arxiv.astro-ph/9605164,
title = {Solid interiors of neutron stars and gravitational radiation},
author = {P. Haensel},
journal= {arXiv preprint arXiv:astro-ph/9605164},
year = {2007}
}
备注
26 pages, Latex, uses l-school.sty, epsf.tex. Four figures. Lectures delivered at Les Houches Summer School 1995 ``Astrophysical Sources of Gravitational Radiation''. To be published in the Proceedings (eds. J.-A.Marck and J.-P.Lasota)