Comprehensive study of amorphous metal oxide and Ta$_2$O$_5$-based mixed oxide coatings for gravitational-wave detectors
Mariana A. Fazio, Gabriele Vajente, Le Yang, Alena Ananyeva, Carmen S., Menoni

TL;DR
This study systematically investigates amorphous metal oxide and Ta₂O₅-based mixed oxide coatings, revealing their potential for reducing thermal noise in gravitational-wave detectors by analyzing their mechanical and optical properties.
Contribution
It provides a comprehensive analysis of the relationship between amorphous structure and mechanical loss, and evaluates various mixed oxide coatings for low thermal noise applications.
Findings
Metal oxide loss correlates with amorphous morphology.
SiO₂ and GeO₂ have the lowest loss angles.
TiO₂-doped Ta₂O₅ is optimal for low thermal noise.
Abstract
High finesse optical cavities of current interferometric gravitational-wave detectors are significantly limited in sensitivity by laser quantum noise and coating thermal noise. The thermal noise is associated with internal energy dissipation in the materials that compose the test masses of the interferometer. Our understanding of how the internal friction is linked to the amorphous material structure is limited due to the complexity of the problem and the lack of studies that span over a large range of materials. We present a systematic investigation of amorphous metal oxide and TaO-based mixed oxide coatings to evaluate their suitability for low Brownian noise experiments. It is shown that the mechanical loss of metal oxides is correlated to their amorphous morphology, with continuous random network materials such as SiO and GeO featuring the lowest loss angles. We…
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