https://www.selleckchem.com/pr....oducts/abc294640.htm
75 dB, and a -10 dB RCS reduction characteristic in the wide band of 6∼20.7 GHz with a fractional band of 110%.In order to increase the number of detectable gravitational-wave sources, future gravitational-wave detectors will operate with cryogenically cooled mirrors. However, recent studies showed that cryogenic mirrors can suffer from the molecular layer formation, which introduces an additional optical loss, and the detector's performance degrades. In order to evaluate the impact of the molecular layer on future cryogenic gravitati
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