.png){kind=icon}
返回
Binary inspiral: finding the right approximation
.png){kind=icon}
PRE
AI
DOI：10.1088/0264-9381/21/3/017.png)
.png){kind=icon}
原文求助.png){kind=icon}
分享.png){kind=icon}
收藏
摘要
En 中文
In searching for and interpreting signals from binary mergers, gravitational wave detectors need information about the features of gravitational wave bursts generated by these strong field events. Numerical relativity will ultimately provide the answers, but not on the time scale needed by the first detectors. We propose here a method in which exact numerical solutions to Einstein's equations, for periodic sources and standing waves, are used as an approximation to the strong field quasistationary epoch of inspiral. We discuss how this approximation changes the mathematical nature of the computation, and we report on progress with this problem and on remaining challenges.
Keyword:
COLLAPSING RELATIVISTIC STARS
COLLIDING BLACK-HOLES
RADIATION
COLLISION
AI总结
对已上传原文的论文进行重点信息的提取，主要内容包括：简要概述、研究摘要、背景介绍、关键亮点、图文解析、展望与总结。
期刊
IF:
3.7
论文数:
1.3W
被引数:
3.0W
机构
暂无机构信息
引用论文
分享收藏Anastomoses between Extracardiac Vessels and Coronary Arteries — II — Via Internal Mammary Arteries
PREAI
分享收藏Expression mediated by three partial sequences of the human tyrosine hydroxylase promoter in vivo
OAAI
OAAI分享收藏Enhanced or reduced concentration polarization by membrane fouling in seawater reverse osmosis (SWRO) processes.png)
Desalination
DesalinationIF0
PREAI
分享收藏Surface characterization and performance evaluation of commercial fouling resistant low-pressure RO membranesDesalination
DesalinationIF0
PREAI
分享收藏
查看更多内容