Designing a low-loss high reflectivity mirror for gravitational waves detectors by combining a dielectric metasurface and a multilayer stack
Edith Hartmann, Michel Lequime, Jerome Degallaix, Michael T. Hartman, Paul Rouquette, Claude Amra, Myriam Zerrad

TL;DR
This paper proposes a novel mirror design combining a dielectric metasurface with a multilayer stack to achieve high reflectivity with fewer layers, aiming to reduce thermal noise in gravitational wave detectors.
Contribution
It introduces a new mirror architecture that reduces the number of layers and thermal noise, enhancing the sensitivity of gravitational-wave observatories.
Findings
The combined mirror design maintains high reflectivity with fewer layers.
The total thickness of high-noise material is reduced by over three times.
Potential for significant thermal noise reduction in gravitational wave detectors.
Abstract
The design of new low-mechanical-loss, high reflectivity mirrors is crucial in the development of the next generation of gravitational-wave observatories. Currently, the state-of-the-art amorphous multilayer reflective coatings which are deposited at the surface of the test masses in interferometric gravitational-wave detectors present the limiting factor in detector sensitivity due to their thermal noise. These coatings require a large number of thin layers to achieve ultra-high reflectivity. However, the thermal noise generated by this type of stack increases with the number of layers used. These dielectric mirrors represent a very mature technology, with current research producing only incremental improvements, highlighting the need for new technical solutions that can address this specific issue. Here, we provide insights into the expected performance of mirrors that combine a…
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