Abstract
A new optical control scheme for interferometric gravitational wave detectors was proposed, which involves resonating the rf sidebands in an arm cavity. This procedure achieves a high degree of tolerance to interferometer spatial distortions and noise on the input light.
Original language | English |
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Pages (from-to) | 1014-1016 |
Number of pages | 3 |
Journal | Optics Letters |
Volume | 24 |
Issue number | 15 |
DOIs | |
Publication status | Published - 1 Aug 1999 |