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Development of large size sapphire crystals for laser interferometer gravitational-wave observatory

机译:激光干涉仪重力波天文台大尺寸蓝宝石晶体的研制

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摘要

Because of its high density and superior quality factor, sapphire crystal, as a candidate material for test masses, has attracted much attention in gravitation wave communities. The use of sapphire crystal, however, is limited by its size, homogeneity, and absorption. An effort has been made to overcome these difficulties at the Shanghai Institute of Optics and Fine Mechanics in collaboration with the Laser Interferometer Gravitational-Wave Observatory Laboratory. By using a directional temperature gradient technique (TGT), sapphire crystals of 11 cm in diameter and 8 cm in length were grown at the C plane (0001). The results indicate that a homogeneity of >5/spl times/10/sup -7/ and an absorption of 35-65 ppm/cm have been achieved at wavelength of 1.06 /spl mu/m. This paper presents the TGT growth of sapphire crystals, their transmittance spectra, optical homogeneity, and absorption. Future applications for gravitational wave experiments are discussed.
机译:由于蓝宝石晶体具有高密度和优良的品质因数,因此作为测试质量的候选材料在引力波界引起了广泛关注。然而,蓝宝石晶体的使用受到其尺寸,均质性和吸收性的限制。上海光学精密机械研究所与激光干涉仪引力波天文台实验室合作,努力克服这些困难。通过使用定向温度梯度技术(TGT),在C平面(0001)上生长了直径11厘米,长度8厘米的蓝宝石晶体。结果表明,在1.06 / spl mu / m的波长下,均质性> 5 / spl乘以/ 10 / sup -7 /,吸收率达到35-65 ppm / cm。本文介绍了蓝宝石晶体的TGT生长,其透射光谱,光学均匀性和吸收性。讨论了重力波实验的未来应用。

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