Non-stoichiometric silicon nitride for future gravitational wave detectors

G S Wallace, M Ben Yaala*, S C Tait, G Vajente, T McCanny, C Clark, D Gibson, J Hough, I W Martin, S Rowan, S Reid

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

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    Abstract

    Silicon nitride thin films were deposited at room temperature employing a custom ion beam deposition (IBD) system. The stoichiometry of these films was tuned by controlling the nitrogen gas flow through the ion source and a process gas ring. A correlation is established between the process parameters, such as ion beam voltage and ion current, and the optical and mechanical properties of the films based on post-deposition heat treatment. The results show that with increasing heat treatment temperature, the mechanical loss of these materials as well as their optical absorption decreases producing films with an extinction coefficient as low as k = 6.2 ( ± 0.5 ) × 10 − 7 at 1064 nm for samples annealed at 900 C. This presents the lowest value for IBD SiNx within the context of gravitational wave detector applications. The mechanical loss of the films was measured to be ϕ = 2.1 ( ± 0.6 ) × 10 − 4 once annealed post deposition to 900 C.

    Original languageEnglish
    Article number095005
    JournalClassical and Quantum Gravity
    Volume41
    Issue number9
    DOIs
    Publication statusPublished - 2 May 2024

    Keywords

    • gravitational wave detectors
    • ion beam deposition
    • optical absorption
    • silicon nitride
    • thermal noise

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