Parametric Oscillatory Instability in a Fabry-Perot Cavity of the Einstein Telescope with different mirror's materials
arXiv:1702.03142 · doi:10.1016/j.physleta.2017.05.049
Abstract
We discuss the parametric oscillatory instability in a Fabry-Perot cavity of the Einstein Telescope. Unstable combinations of elastic and optical modes for two possible configurations of gravitational wave third-generation detector are deduced. The results are compared with the results for gravita- tional wave interferometers LIGO and LIGO Voyager.
4 pages, 3 tables
References in corpus (9)
- Characterization of the LIGO detectors during their sixth science run
- LIGO: The Laser Interferometer Gravitational-Wave Observatory
- Analysis of Parametric Oscillatory Instability in Power Recycled LIGO Interferometer
- Observation of Parametric Instability in Advanced LIGO
- Parametric instabilities and their control in advanced interferometer GW detectors
- A General Approach to Optomechanical Parametric Instabilities
- Observation of the Three-Mode Parametric Instability
- Time evolution of parametric instability in large-scale gravitational-wave interferometers
- Suppression of parametric oscillatory instability in third generation gravitational wave detectors