Sun K X, Byer R L
Opt Lett. 1998 Apr 15;23(8):567-9. doi: 10.1364/ol.23.000567.
All-reflective Michelson, Sagnac, and Fabry-Perot interferometers based on grating beam splitters are experimentally demonstrated at a wavelength of 1064 nm. A 1200-groove/mm grating diffracting 0 and -1 orders with an efficiency of 48.2% for each order was used as a near-50/50 beam splitter. The all-reflective Sagnac and Michelson interferometers were formed by reintroducing both of the diffracted beams back to the grating. The Fabry-Perot interferometer was formed in a Littrow configuration by using a 1700-groove/mm grating with a blazing efficiency of 91% as a cavity coupler. These interferometers encompass all the fundamental configurations of all-reflective laser interferometric gravitational-wave detectors, promising improved wave-front quality by avoiding volume thermal effects in transmissive optics under high-power laser illumination.
基于光栅分束器的全反射迈克尔逊、萨格纳克和法布里-珀罗干涉仪在1064 nm波长下通过实验得到了验证。一个每毫米1200条刻槽、衍射0级和-1级且每级效率为48.2%的光栅被用作近50/50分束器。全反射萨格纳克和迈克尔逊干涉仪是通过将两条衍射光束都重新引入光栅而形成的。法布里-珀罗干涉仪是在 Littrow 配置下通过使用一个闪耀效率为91%的每毫米1700条刻槽的光栅作为腔耦合器而形成的。这些干涉仪涵盖了全反射激光干涉引力波探测器的所有基本配置,有望通过避免高功率激光照射下透射光学元件中的体积热效应来提高波前质量。