Quasi-monocrystalline silicon for low-noise end mirrors in cryogenic gravitational-wave detectors

Mirrors made of silicon have been proposed for use in future cryogenic gravitational-wave detectors, which will be significantly more sensitive than current room-temperature detectors. These mirrors are planned to have diameters of ≈50 cm and a mass of ≈200 kg. While single-crystalline float-zone si...

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Bibliographic Details
Published in:Physical Review Research
Main Authors: Frank M. Kiessling, Peter G. Murray, Maya Kinley-Hanlon, Iryna Buchovska, Torunn K. Ervik, Victoria Graham, Jim Hough, Ross Johnston, Mike Pietsch, Sheila Rowan, Roman Schnabel, Simon C. Tait, Jessica Steinlechner, Iain W. Martin
Format: Article
Language:English
Published: American Physical Society 2022-10-01
Online Access:http://doi.org/10.1103/PhysRevResearch.4.043043