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Abstract
Parametric Instability (PI) is a phenomenon that results from resonant
interactions between optical and acoustic modes of a laser cavity. This
is problematic in gravitational wave interferometers where the high
intra-cavity power and low mechanical loss mirror suspension systems
create an environment where three mode PI will occur without
intervention. We demonstrate a technique for real time imaging of the
amplitude and phase of the optical modes of PI yielding the first ever
images of this phenomenon which could form part of active control
strategies for future detectors.
Original language | English |
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Publisher | arXiv |
Number of pages | 4 |
Publication status | Published - Jan 2022 |
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Dive into the research topics of 'Observing the optical modes of parametric instability'. Together they form a unique fingerprint.Projects
- 1 Finished
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Advanced Technologies for Next Generation Gravitational Wave Detectors
Blair, C. (Investigator 01)
ARC Australian Research Council
17/06/19 → 30/06/23
Project: Research