Author/Authors :
Kawamura، Seiji نويسنده , , Somiya، Kentaro نويسنده , , Beyersdorf، Peter نويسنده , , Arai، Koji نويسنده , , Sato، Shuichi نويسنده , , Miyakawa، Osamu نويسنده , , Kawazoe، Fumiko نويسنده , , Sakata، Shihori نويسنده , , Sekido، Aya نويسنده , , Mio، Norikatsu نويسنده ,
Abstract :
We report on our prototype experiment that uses a 4-m detuned resonant sideband extraction interferometer with suspended mirrors, which has almost the same configuration as the nextgeneration, gravitational-wave detectors. We have developed a new control scheme and have succeeded in the operation of such an interferometer with suspended mirrors for the first time ever as far as we know. We believe that this is the first such instrument that can see the radiation pressure signal enhancement, which can improve the sensitivity of next-generation gravitationalwave detectors.
Keywords :
instrumentation , Measurement , Metrology , Fabry-Perot , Interferometry , Phase measurement , Other areas of optics , astrophysics , Astronomy