Multicolor cavity metrology
Abstract
Long-baseline laser interferometers used for gravitational-wave detection have proven to be very complicated to control. In order to have sufficient sensitivity to astrophysical gravitational waves, a set of multiple coupled optical cavities comprising the interferometer must be brought into resonance with the laser field. A set of multi-input, multi-output servos then lock these cavities into place via feedback control. This procedure, known as lock acquisition, has proven to be a vexing problem and has reduced greatly the reliability and duty factor of the past generation of laser interferometers. In this article, we describe a technique for bringing the interferometer from an uncontrolled state into resonance by using harmonically related external fields to provide a deterministic hierarchical control. This technique reduces the effect of the external seismic disturbances by 4 orders of magnitude and promises to greatly enhance the stability and reliability of the current generation of gravitational-wave detectors. The possibility for using multicolor techniques to overcome current quantum and thermal noise limits is also discussed.
Additional Information
© 2012 Optical Society of America. Received May 9, 2012; revised August 2, 2012; accepted August 17, 2012; posted August 17, 2012 (Doc. ID 167857); published September 12, 2012. We gratefully acknowledge illuminating discussions with Bram Slagmolen, Nicolas Smith-Lefebvre, and Peter Fritschel. We also thank the National Science Foundation for support under grant PHY-0555406.Attached Files
Published - Izumi_264.pdf
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Additional details
- Eprint ID
- 35395
- Resolver ID
- CaltechAUTHORS:20121109-140606927
- NSF
- PHY-0555406
- Created
-
2012-11-13Created from EPrint's datestamp field
- Updated
-
2021-11-09Created from EPrint's last_modified field
- Caltech groups
- TAPIR, LIGO