Searching for gravitational waves with the LIGO and Virgo interferometers

被引：6
|
作者：
Bizouard, Marie-Anne [1 ]
Papa, Maria Alessandra [2 ,3 ]
机构：
[1] Univ Paris 11, CNRS IN2P3, Lab Accelerateur Lineaire, F-91898 Orsay, France
[2] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-14476 Golm, Germany
[3] Univ Wisconsin, Milwaukee, WI 53201 USA
来源：
COMPTES RENDUS PHYSIQUE | 2013年 / 14卷 / 04期
关键词：
Gravitational waves; Neutron stars; Black holes; Supernova core collapse; LIGO; Virgo; GAMMA-RAY BURSTS; SCIENCE RUN 5; BLACK-HOLES; RADIATION; PULSARS; RUNAWAY; ORIGIN; LIMIT;
D O I：
10.1016/j.crhy.2013.03.001
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The first generation of ground-based interferometric gravitational wave detectors, LIGO, GEO, and Virgo, have operated and taken data at their design sensitivities over the last few years. The data has been examined for the presence of gravitational wave signals. Presented here is a comprehensive review of the most significant results. The network of detectors is currently being upgraded and extended, providing a large likelihood for observations. These future prospects will also be discussed. (C) 2013 Academie des sciences. Published by Elsevier Masson SAS. All rights reserved.
引用
收藏
页码：352 / 365
页数：14
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