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2018 ; 376
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Quasi-monolithic mirror suspensions in ground-based gravitational-wave detectors:
an overview and look to the future
#MMPMID29661973
van Veggel AA
Philos Trans A Math Phys Eng Sci
2018[May]; 376
(2120
): ä PMID29661973
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At the commencement of a new era in astrophysics, with added information from
direct detections of gravitational-wave (GW) signals, this paper is a testament
to the quasi-monolithic suspensions of the test masses of the GW detectors that
have enabled the opening of a new window on the universe. The quasi-monolithic
suspensions are the final stages in the seismic isolation of the test masses in
GW detectors, and are specifically designed to introduce as little thermal noise
as possible. The history of the development of the fused-silica quasi-monolithic
suspensions, which have been so essential for the first detections of GWs, is
outlined and a glimpse into the status of research towards quasi-monolithic
suspensions made of sapphire and silicon is given.This article is part of a
discussion meeting issue 'The promises of gravitational-wave astronomy'.