Design study of the KAGRA output mode cleaner

被引：6
|
作者：
Kumeta, Ayaka [1 ]
Bond, Charlotte [2 ]
Somiya, Kentaro [1 ]
机构：
[1] Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, Japan
[2] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England
来源：
OPTICAL REVIEW | 2015年 / 22卷 / 01期
基金：
日本学术振兴会;
关键词：
Interferometer; Simulation; Gravitational waves;
D O I：
10.1007/s10043-015-0028-2
中图分类号：
O43 [光学];
学科分类号：
070207 ; 0803 ;
摘要：
Most second-generation gravitational-wave detectors employ an optical resonator called an output mode cleaner (OMC), which filters out junk light from the signal and the reference light, before it reaches the detection photodiode located at the asymmetric port of the large-scale interferometer. The optical parameters of the OMC should be carefully chosen to satisfy the requirements to filter out unwanted light whilst transmitting the gravitational-wave signal. We use the simulation program FINESSE and realistic mirror phase maps that have the same surface quality as the KAGRA test masses to find out a proper design of the KAGRA OMC.
引用
收藏
页码：149 / 152
页数：4
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