孤立中子星的引力波
天体物理学
2007-05-23 v1 广义相对论与量子宇宙学
摘要
讨论了来自孤立旋转中子星的持续型引力波。给出了各种已知脉冲星的总体波形及�幅尺度。具体讨论了由于星体磁场引起的形变导致的引力波。最后讨论了关于整个银河系中中子星群体信号的初步结果。
引用
@article{arxiv.astro-ph/9605150,
title = {Gravitational waves from isolated neutron stars},
author = {E. Gourgoulhon and S. Bonazzola},
journal= {arXiv preprint arXiv:astro-ph/9605150},
year = {2007}
}
备注
11 pages, 2 PostScript figures, to appear in the Proceedings of the International Conference on Gravitational Waves: Sources and Detectors, Cascina (Pisa), Italy --- March 19-23, 1996 (World Scientific, in press)