聆听 ringing 黑洞
广义相对论与量子宇宙学
2007-05-23 v1
摘要
双星黑洞在旋进、并合和铃宕阶段产生的引力辐射，是有望被第一代或第二代公里级干涉式引力波天线探测到的候选信号。最后一阶段即准正态铃宕的波形已被充分理解。我基于加州理工 40 米干涉仪数据的分析，讨论探测黑洞准正态铃宕的可行性。
引用
@article{arxiv.gr-qc/9712044,
title = {Listening for Ringing Black Holes},
author = {Jolien D. E. Creighton},
journal= {arXiv preprint arXiv:gr-qc/9712044},
year = {2007}
}
备注
8 pages LaTeX, 1 eps figure included with epsfig, based on a talk given at the 7th Canadian Conference on General Relativity and Relativistic Astrophysics