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    Revealing the role of hydrogen in reducing optical absorption and mechanical loss in magnetron-sputtered amorphous silicon for gravitational-wave detectors

    M. Molina-Ruiz1,*,†, R. Zhou2,*, A. Markosyan3, R. Bassiri3, M. M. Fejer3, A. Ananyeva4, S. C. Tait4, G. Vajente4, A. Davenport5 et al.

    C. S. Menoni5 and F. Hellman1,2

    • *These authors contributed equally to this work.
    • †Contact author: manelmolinaruiz@gmail.com

    Phys. Rev. Materials 9, 105602 – Published 10 October, 2025

    DOI: https://doi.org/10.1103/5n1c-tjhq

    Abstract

    Hydrogenated a-Si films grown by magnetron sputtering have greatly reduced subgap optical absorption, down to 122 ppm (9.0 cm−1) at 1064 nm, 6 ppm (0.4 cm−1) at 1550 nm, and 2 ppm (0.1 cm−1) at 2000 nm for quarter-wavelength-thick films, and they reduced room-temperature mechanical loss below 2×10−5. The dangling bond density is reduced to 1017cm−3 and the refraction index remains above that of crystalline silicon for all wavelengths. The above wavelengths are well below the Urbach edge of a-Si, and thus absorption is associated with deep-trap states. Although reductions in absorption and dissipation increase with increasing hydrogen content in the working gas, the hydrogen concentration in the films remains low (below 1 at.%), and neither absorption nor mechanical loss correlate with dangling bond density. Raman-derived bond angle deviation measurements of a-Si show a reduction in structural disorder as the films are further processed by vacuum annealing and post-hydrogenation, while a-Si:H films show a lower disorder in the as-deposited state without further reductions after thermal processing. These results suggest that the presence of hydrogen during film growth, acting as a catalyst, facilitates local rearrangement of atoms and removes strained Si–Si bonds that are more responsible for sub-band-gap absorption and dissipative mechanisms than dangling bonds.

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