Precise measurements, such as those made with interferometric gravitational-wave detectors, require the measurement device to be properly controlled so that the sensitivity can be as high as possible. Mirrors in the interferometer are to be located at specific operation points to isolate laser noise and to accumulate the signal in resonant cavities. On the other hand, rigid control of an auxiliary degree of freedom may result in imposing sensing noise of the control on the target object as excess force noise. Evaluation of this so-called loop noise is important in order to design a decent control scheme of the measurement device. In this paper, we show the method to calculate the level of loop noise, which has been recently implemented in simulation tools that are broadly used for designing gravitational-wave detectors.
© 2010 Optical Society of AmericaFull Article | PDF Article
Kentaro Somiya, Peter Beyersdorf, Koji Arai, Shuichi Sato, Seiji Kawamura, Osamu Miyakawa, Fumiko Kawazoe, Shihori Sakata, Aya Sekido, and Norikatsu Mio
Appl. Opt. 44(16) 3179-3191 (2005)
Jun Mizuno and Ichirou Yamaguchi
J. Opt. Soc. Am. A 16(7) 1730-1739 (1999)
Peter T. Beyersdorf, Seiji Kawamura, Kentaro Somiya, Fumiko Kawazoe, and Marcel Agüeros
Appl. Opt. 44(17) 3413-3424 (2005)