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The Simons Observatory: metamaterial microwave absorber and its cryogenic applications

机译:西蒙斯天文台:超材料微波吸收器及其低温应用

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摘要

Controlling stray light at millimeter wavelengths requires special optical design and selection of absorptive materials that should be compatible with cryogenic operating environments. While a wide selection of absorptive materials exists, these typically exhibit high indices of refraction and reflect/scatter a significant fraction of light before absorption. For many lower index materials such as commercial microwave absorbers, their applications in cryogenic environments are challenging. In this paper, we present a new tool to control stray light: metamaterial microwave absorber tiles. These tiles comprise an outer metamaterial layer that approximates a lossy gradient index anti-reflection coating. They are fabricated via injection molding commercially available carbon-loaded polyurethane (25% by mass). The injection molding technology enables mass production at low cost. The design of these tiles is presented, along with thermal tests to 1 K. Room temperature optical measurements verify their control of reflectance to less than 1% up to 65 degrees angles of incidence, and control of wide angle scattering below 0.01%. The dielectric properties of the bulk carbon-loaded material used in the tiles is also measured at different temperatures, confirming that the material maintains similar dielectric properties down to 3 K. (C) 2021 Optical Society of America
机译:控制毫米波的杂散光需要特殊的光学设计和吸收材料的选择,这些材料应与低温操作环境兼容。虽然存在各种各样的吸收材料,但这些材料通常表现出高折射率,并在吸收前反射/散射大量光。对于许多低折射率材料,如商用微波吸收器,其在低温环境中的应用具有挑战性。在本文中,我们提出了一种控制杂散光的新工具:超材料微波吸收砖。这些瓷砖包括一个外部超材料层,近似于有损梯度折射率防反射涂层。它们是通过注塑商用载碳聚氨酯(质量分数为25%)制成的。注射成型技术能够以低成本实现大规模生产。介绍了这些瓷砖的设计,以及1K的热试验。室温光学测量验证了其反射率控制在小于1%到65度的入射角,广角散射控制在0.01%以下。在不同温度下测量了砖中所用的块状碳负载材料的介电性能,确认该材料保持类似的介电性能,直到美国3 K.(C)2021光学学会。

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  • 来源
    《Applied optics》 |2021年第4期|共11页
  • 作者单位

    Univ Penn Dept Phys &

    Astron 209 South 33rd St Philadelphia PA 19104 USA;

    Univ Chicago Dept Phys 5720 South Ellis Ave Chicago IL 60637 USA;

    Kyoto Univ Grad Sch Sci Div Phys &

    Astron Sakyo Ku Kitashirakawa Oiwakecho Kyoto 6068502 Japan;

    Univ Calif Berkeley Dept Phys Berkeley CA 94720 USA;

    Princeton Univ Dept Phys Princeton NJ 08544 USA;

    Univ Penn Dept Phys &

    Astron 209 South 33rd St Philadelphia PA 19104 USA;

    Univ Penn Dept Phys &

    Astron 209 South 33rd St Philadelphia PA 19104 USA;

    Devlin Design Inc 1 Fitchburg St Somerville MA 02143 USA;

    Univ Penn Dept Phys &

    Astron 209 South 33rd St Philadelphia PA 19104 USA;

    Cornell Univ Dept Phys Ithaca NY 14853 USA;

    Univ Chicago Dept Phys 5720 South Ellis Ave Chicago IL 60637 USA;

    Stockholm Univ Oskar Klein Ctr Dept Phys AlbaNova SE-10691 Stockholm Sweden;

    Univ Penn Dept Phys &

    Astron 209 South 33rd St Philadelphia PA 19104 USA;

    Tohoku Univ Grad Sch Sci Astron Inst Aoba Ku 6-3 Aramaki Aza Aoba Sendai Miyagi 9808578 Japan;

    Univ Penn Dept Phys &

    Astron 209 South 33rd St Philadelphia PA 19104 USA;

    Univ Tokyo Dept Phys Bunkyo Ku 7-3-1 Hongo Tokyo 1130033 Japan;

    Tohoku Univ Grad Sch Sci Astron Inst Aoba Ku 6-3 Aramaki Aza Aoba Sendai Miyagi 9808578 Japan;

    Univ Penn Dept Phys &

    Astron 209 South 33rd St Philadelphia PA 19104 USA;

    Univ Tokyo Inst Adv Study Kavli Inst Phys &

    Math Universe WPI Kashiwa Chiba 2778583 Japan;

    Univ Chicago Dept Phys 5720 South Ellis Ave Chicago IL 60637 USA;

    Univ Milano Bicocca Dept Phys Piazza Sci 3 I-20126 Milan MI Italy;

    Cornell Univ Dept Phys Ithaca NY 14853 USA;

    Lawrence Berkeley Natl Lab Phys Div 1 Cyclotron Rd Berkeley CA 94720 USA;

    Univ Calif San Diego Dept Phys La Jolla CA 92093 USA;

    Univ Penn Dept Phys &

    Astron 209 South 33rd St Philadelphia PA 19104 USA;

    Goddard Space Flight Ctr 8800 Greenbelt Rd Greenbelt MD 20771 USA;

    Univ Milano Bicocca Dept Phys Piazza Sci 3 I-20126 Milan MI Italy;

    Univ Penn Dept Phys &

    Astron 209 South 33rd St Philadelphia PA 19104 USA;

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