Loss factors of mirrors for a gravitational wave antenna.
Loss factors of mirrors for a gravitational wave antenna.
复制标题
引力波天线镜子的损耗因数。
DOI:
10.1364/ao.38.002880
复制
发表时间:
1999
期刊:
影响因子:
1.9
通讯作者:
I. Kataoka
中科院分区:
文献类型:
--
作者:
S. Sato;S. Miyoki;M. Ohashi;M. Fujimoto;T. Yamazaki;M. Fukushima;A. Ueda;K. Ueda;K. Watanabe;K. Nakamura;K. Etoh;N. Kitajima;K. Ito;I. Kataoka
Low-loss mirrors fabricated by ion-beam-sputtering machines for possible application in an interferometric gravitational wave antenna were evaluated by use of Nd:YAG laser light (lambda = 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 of 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.