Resonant dampers for parametric instabilities in gravitational wave detectors
Advanced gravitational wave interferometric detectors will operate at their design sensitivity with nearly ~1 MW of laser power stored in the arm cavities. Such large power may lead to the uncontrolled growth of acoustic modes in the test masses due to the transfer of optical energy to the mechanic...
| Main Authors: | , , , |
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| Other Authors: | |
| Format: | Article |
| Language: | English |
| Published: |
American Physical Society
2015
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| Online Access: | http://hdl.handle.net/1721.1/99141 https://orcid.org/0000-0001-8459-4499 https://orcid.org/0000-0003-1983-3187 |