作者: John A. Sidles , Daniel Sigg
DOI: 10.1016/J.PHYSLETA.2006.01.051
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摘要: Abstract High-power Fabry–Perot cavities with suspended mirrors are employed in gravitational wave detection. The such interferometers subject to forces and torques that exerted by light pressure. This Letter derives a closed-form expression for the static torsional stiffness due this effect. is shown scale as fourth power of beam spot size. In proposed designs next-generation interferometric detectors be large enough dominate dynamics mirror suspensions.