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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Hauptverfasser:	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:	Artigo
Sprache:	Inglês
Veröffentlicht:	American Physical Society 2022-10-01
Schriftenreihe:	Physical Review Research
Online-Zugang:	http://doi.org/10.1103/PhysRevResearch.4.043043
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