Published January 1, 2005
| public
Journal Article
Open
Development of a frequency-detuned interferometer as a prototype experiment for next-generation gravitational-wave detectors
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 next-generation, 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 gravitational-wave detectors.
Additional Information
© 2005 Optical Society of America Received 14 July 2004; revised manuscript received 6 December 2004; accepted 19 December 2004. We thank the members of the TAMA projects and the members of the Advanced Interferometer Configuration Committee from the LIGO Science Collaboration (LSC) for many comments. This research is supported by a grant-in-aid for Creative Basic Research of the Ministry of Education, Science, Sports, and Culture. Also we acknowledge support from a Japan Society for the Promotion of Science (JSPS) fellowship.Files
SOMao05.pdf
Files
(1.8 MB)
| Name | Size | Download all |
|---|---|---|
|
md5:14a005fec6069cc0831f6fffe52c3dd3
|
1.8 MB | Preview Download |
Additional details
- Eprint ID
- 8718
- Resolver ID
- CaltechAUTHORS:SOMao05
- Created
-
2007-09-10Created from EPrint's datestamp field
- Updated
-
2019-10-02Created from EPrint's last_modified field