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Loss factors of mirrors for a gravitational wave antenna

机译:重力波天线反射镜的损耗因子

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Low-loss mirrors fabricated by ion-beam-sputtering machines for possible application in an interfere-metric gravitational wave antenna were evaluated by use of Nd:YAG laser light (λ = 1064 nm) with two distinct measurements: a tabletop experiment that used a short cavity with a small beam with a beam waist of approximately 2w_(0) = 0.82 mm, and an optical test that used a 20-m prototypical gravitational-wave detector with a large beam with a beam waist of approximately 2W_(0) = 4.4 mm. A multilayer coating comprised 29 layers of SiO_(2)/Ta_(2)O_(5) and one protective coating SiO_(2). The best values obtained as a result of these measurements were 16 ppm (parts in 10~(6)) and 30 ppm in total loss, respectively. Also, a two-dimensional loss map generated by use of a small beam successfully revealed the existence of a loss structure within the coating surface. These results imply that a high-reflectance multilayer coating has some inhomogeneities and a loss distribution with a typical scale of a few millimeters and that the total measured losses depend on the beam spot size.
机译:使用Nd:YAG激光(λ= 1064 nm)进行了两种不同的测量,评估了由离子束溅射机制造的可能在干涉式重力波天线中使用的低损耗反射镜:一项台式实验短腔,其小束腰的束腰大约为2w_(0)= 0.82 mm,并且进行了光学测试,该实验使用了20 m原型重力波探测器,大束的束腰大约为2W_(0)= 4.4毫米多层涂层包括29层SiO_(2)/ Ta_(2)O_(5)和一层保护涂层SiO_(2)。通过这些测量获得的最佳值分别是总损耗为16 ppm(10〜(6)的一部分)和30 ppm。同样,通过使用小光束产生的二维损耗图成功地揭示了涂层表面内存在损耗结构。这些结果表明,高反射率多层涂层具有一些不均匀性,并且损耗分布通常为几毫米,并且总的测量损耗取决于光束斑的大小。

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