与脉冲星自转突变相关的r模频率处瞬态引力波的前景
广义相对论与量子宇宙学
2012-09-28 v1
摘要
脉冲星的自转突变很可能触发中子星流体内部的振荡模式。我们专门研究了r模频率下的这些振荡。被激发的r模将发射引力波，并可能具有较长的阻尼时间尺度（数量级为分钟到天）。我们使用简单估计来估算自转突变可能注入r模的能量，并评估未来干涉仪探测所发射引力波的可能性。
引用
@article{arxiv.1203.0401,
title = {Prospects for transient gravitational waves at r-mode frequencies associated with pulsar glitches},
author = {I. Santiago-Prieto and I. S. Heng and D. I. Jones and J. Clark},
journal= {arXiv preprint arXiv:1203.0401},
year = {2012}
}
备注
5 pages, 1 figure. Submitted to Journal of Physics: Conference Series, Proceedings of 9th Amaldi Conference on Gravitational Waves/ NRDA 2012, Cardiff (UK) July 2011