Details
| Original language | English |
|---|---|
| Article number | 012017 |
| Journal | Journal of Physics: Conference Series |
| Volume | 122 |
| Publication status | Published - 2008 |
| Externally published | Yes |
Abstract
LCGT plans to use tuned RSE as the optical configuration for its interferometer. A tuned RSE interferometer has five degrees of freedom that need to be controlled in order to operate a gravitational-wave detector, although it is expected to be very challenging because of the complexity of its optical configuration. A new control scheme for a tuned RSE interferometer has been developed and tested with a prototype interferometer to demonstrate successful control of the tuned RSE interferometer. The whole RSE interferometer was successfully locked with the control scheme. Here the control scheme and the current status of the experiment are presented.
ASJC Scopus subject areas
- Physics and Astronomy(all)
- General Physics and Astronomy
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In: Journal of Physics: Conference Series, Vol. 122, 012017, 2008.
Research output: Contribution to journal › Article › Research › peer review
}
TY - JOUR
T1 - Experimental investigation of a control scheme for a tuned resonant sideband extraction interferometer for next-generation gravitational-wave detectors
AU - Kawazoe, F.
AU - Sato, S.
AU - Leonhardt, V.
AU - Miyakawa, O.
AU - Morioka, T.
AU - Nishizawa, A.
AU - Yamazaki, T.
AU - Fukushima, M.
AU - Kawamura, S.
AU - Sugamoto, A.
PY - 2008
Y1 - 2008
N2 - LCGT plans to use tuned RSE as the optical configuration for its interferometer. A tuned RSE interferometer has five degrees of freedom that need to be controlled in order to operate a gravitational-wave detector, although it is expected to be very challenging because of the complexity of its optical configuration. A new control scheme for a tuned RSE interferometer has been developed and tested with a prototype interferometer to demonstrate successful control of the tuned RSE interferometer. The whole RSE interferometer was successfully locked with the control scheme. Here the control scheme and the current status of the experiment are presented.
AB - LCGT plans to use tuned RSE as the optical configuration for its interferometer. A tuned RSE interferometer has five degrees of freedom that need to be controlled in order to operate a gravitational-wave detector, although it is expected to be very challenging because of the complexity of its optical configuration. A new control scheme for a tuned RSE interferometer has been developed and tested with a prototype interferometer to demonstrate successful control of the tuned RSE interferometer. The whole RSE interferometer was successfully locked with the control scheme. Here the control scheme and the current status of the experiment are presented.
UR - http://www.scopus.com/inward/record.url?scp=65649112438&partnerID=8YFLogxK
U2 - 10.1088/1742-6596/122/1/012017
DO - 10.1088/1742-6596/122/1/012017
M3 - Article
AN - SCOPUS:65649112438
VL - 122
JO - Journal of Physics: Conference Series
JF - Journal of Physics: Conference Series
SN - 1742-6588
M1 - 012017
ER -