Amorphous silicon with extremely low absorption: beating thermal noise in gravitational astronomy

Ross Birney, J. Steinlechner, Z. Tornasi, Sean Macfoy, David Vine, A.S. Bell, Desmond Gibson, Jim Hough, Sheila Rowan, P. Sortais, S. Sproules, S. Tait, Iain W. Martin, Stuart Reid

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33 Citations (Scopus)
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Amorphous silicon has ideal properties for many applications in fundamental research and industry. However, the optical absorption is often unacceptably high, particularly for gravitational wave detection. We report a novel ion beam deposition method for fabricating amorphous silicon with unprecedentedly low unpaired electron spin density and optical absorption; the spin-limit on absorption being surpassed for the first time. At low unpaired electron density, the absorption is no longer correlated with electron spins, but with the electronic mobility gap. Compared to standard ion beam deposition, the absorption at 1550,nm is lower by a factor of ≈100. This breakthrough shows that amorphous silicon could be exploited as an extreme performance optical coating in near-infra-red applications and it represents an important proof-of-concept for future gravitational wave detectors.
Original languageEnglish
Article number191101
JournalPhysical Review Letters
Early online date6 Nov 2018
Publication statusE-pub ahead of print - 6 Nov 2018


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