Advanced LIGO: non-Gaussian beams

被引：20
作者：
D'Ambrosio, E [1 ]
O'Shaugnessy, R
Thorne, K
Willems, P
Strigin, S
Vyatchanin, S
机构：
[1] CALTECH, Pasadena, CA 91125 USA
[2] Moscow MV Lomonosov State Univ, Moscow, Russia
来源：
CLASSICAL AND QUANTUM GRAVITY | 2004年 / 21卷 / 05期
关键词：
D O I：
10.1088/0264-9381/21/5/074
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
By using non-Gaussian, flat-topped beams in the advanced gravitational wave interferometers currently being designed, one can reduce the impact on the interferometer sensitivity of a variety,of fundamental disturbances (thermoelastic noise, noise in mirror coatings, thermal lensing, etc). This may make beating the standard quantum limit an achievable goal.
引用
收藏
页码：S867 / S873
页数：7
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