Crystalline supermirrors for gravitational-wave detection
Modern precision optical instruments are increasingly limited not by light sources, electronics, or vibration isolation but by the microscopic thermal motion of mirror coatings that form the reflecting surfaces of optical cavities. In optical atomic clocks, ultrastable lasers, stabilized frequency combs, and gravitational-wave detectors, this inherent thermomechanical noise from multilayer mirror coatings sets a noise
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