具有自旋致密双星系统的次领头阶引力波辐射与动力学演化
广义相对论与量子宇宙学
2008-11-26 v2
摘要
本文研究了具有自旋分量的致密双星系统，并考虑了由旋转形变引起的有限尺寸效应。在计入直至一阶后牛顿近似 (first post-Newtonian approximation) 的轨道运动情况下，计算了系统的动力学演化及次领头阶 (next to leading order) 引力波波形。
引用
@article{arxiv.0710.0258,
title = {Next to leading order gravitational wave emission and dynamical evolution of compact binary systems with spin},
author = {Dörte Hansen},
journal= {arXiv preprint arXiv:0710.0258},
year = {2008}
}
备注
typos corrected; version submitted to Class. Quant. Grav