Data analysis and figure generation were carried out using MATLAB software provided by The MathWorks, Inc. LIGO was constructed by the California Institute of Technology and Massachusetts Institute of Technology with funding from the National Science Foundation, and operates under cooperative Agreement PHY-1764464.
Substoichiometric silica in a multimaterial highly reflective coating
Creators
Abstract
Gravitational-wave detectors impose exceptionally rigorous demands on optical coatings, which include high reflectivity, low thermal noise, low absorption, low scatter, and minimal defect counts. Simultaneously satisfying the thermal noise and absorption requirements is particularly challenging. One promising approach is to use three or more materials in a single coating. In this work we characterize such a multimaterial coating made using low index silica (SiO2), high index tantala (Ta2O5), and high index substoichiometric silica (SiO). We find that by using a multi-material structure, we achieve a more than 1000-fold reduction in optical absorption relative to a mirror made solely of SiO and SiO2. Exploration of the SiO_x deposition parameter space may allow for further optimization and we present one possible optimized coating design that may reduce coating thermal noise by 20% relative to the coatings used in current detectors.
Copyright and License
© 2025 IOP Publishing Ltd. All rights, including for text and data mining, AI training, and similar technologies, are reserved.
Acknowledgement
Data Availability
The data that support the findings of this study are openly available at the following URL/DOI: https://dcc.ligo.org/P2500332/public.
Additional details
Related works
- Featured in
- Journal Article: https://iopscience.iop.org/collections/0264-9381_low-noise-thin-film-coatings (URL)
Funding
- National Science Foundation
- PHY-1764464
Dates
- Accepted
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2025-04-30
- Available
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2025-05-27Published