Published April 7, 2002
| Submitted
Journal Article
Open
Path-finding towards a cryogenic interferometer for LIGO
- Creators
- DeSalvo, Riccardo
Abstract
LIGO is exploring cryogenics as a technique of last resort to reduce the thermal noise of mirrors and suspensions in gravitational wave interferometric detectors. Some of the cryogenic, or cryogenic-related, R&D done at LIGO is reported here. Some ideas being considered to make cryogenics possible may be useful even for room temperature detectors.
Additional Information
© 2002 IOP Publishing. Received 31 October 2001. Published 18 March 2002. This research was supported by the National Science Foundation under Cooperative Agreement PHY98-01158.Attached Files
Submitted - download?doi=10.1.1.383.8174_rep=rep1_type=pdf.pdf
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LIGO-P010032-00-D.pdf
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Additional details
- Eprint ID
- 75889
- DOI
- 10.1088/0264-9381/19/7/408
- Resolver ID
- CaltechAUTHORS:20170408-135557409
- PHY98-01158
- NSF
- Created
-
2017-04-13Created from EPrint's datestamp field
- Updated
-
2022-07-12Created from EPrint's last_modified field
- Caltech groups
- LIGO