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- W2056214912 abstract "The thermal noise of optical components (e.g., end mirrors, beam splitters) is one of the limiting factors of the sensitivity of most of the present interferometric gravitational wave detectors, and it will be limiting in the advanced detectors now being designed. This thermal noise occurs mainly in the optical substrates and their mirror coatings. One possible method for minimizing thermal noise is cooling to cryogenic temperatures, maximizing the mechanical Q and maximizing the eigenfrequencies of the substrate. A new cryogenic apparatus for investigations of the temperature dependency of the Q-factor of several substrate materials down to 4.2 K is proposed. Possible methods of mode excitation and ring down measurement are discussed." @default.
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- W2056214912 date "2004-02-12" @default.
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- W2056214912 title "Proposed cryogenic Q -factor measurement of mirror substrates" @default.
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- W2056214912 doi "https://doi.org/10.1088/0264-9381/21/5/111" @default.
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