Published July 25, 2008
| Published
Journal Article
Open
Experimental investigation of a control scheme for a tuned resonant sideband extraction interferometer for next-generation gravitational-wave detectors
Chicago
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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.
Additional Information
© 2008 IOP Publishing Ltd. 7th Edoardo Amaldi Conference on Gravitational Waves (Amaldi7). This research is supported in part by a Grant-in-Aid for Scientific Research on Priority Areas (415) of the Ministry of Education, Culture, Sports, Science, and Technology, from Japan, and also partially supported by the US National Science Foundation under cooperative agreement PHY-0107417.Attached Files
Published - KAWjpcs08a.pdf
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Additional details
- Eprint ID
- 13828
- Resolver ID
- CaltechAUTHORS:KAWjpcs08a
- Ministry of Education, Culture, Sports, Science and Technology (MEXT)
- NSF
- PHY-0107417
- Created
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2009-04-06Created from EPrint's datestamp field
- Updated
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2022-07-12Created from EPrint's last_modified field