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Bibliographic Details
Main Authors: Lam, Rex, Cray, Scott, Dietterich, Sam, Firth, Calvin, Hanany, Shaul, Izawa, Takumi, Koch, Jürgen, Konishi, Kuniaki, Matsumura, Tomotake, Sakurai, Haruyuki, Sakurai, Yuki, Takaku, Ryota, Yan, Andrew
Format: Preprint
Published: 2026
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Online Access:https://arxiv.org/abs/2602.00304
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Table of Contents:
  • We present millimeter and sub-millimeter room temperature transmission and loss measurements of 3D printed alumina disc and of a disc with one-sided 3D printed sub-wavelength structures anti-reflection coatings (SWS-ARC). For four bands spanning 158 - 700~GHz we find an index of refraction consistent with $n= 3.107 \pm 0.007$. The loss over the entire frequency band between 158~GHz and 700~GHz spans $ 1 \cdot 10^{-3} \leq \tan δ\leq 2.49 \cdot 10^{-3}$ with 10%-30% uncertainty at the lower range of frequencies shrinking to $\sim\!2\%$ at the higher frequencies. As expected, constructive and destructive interference fringes that are apparent with the flat disc data are absent with the disc that has SWS-ARC. The measured data are consistent with finite element analysis predictions that are based on the measured shape of the SWS. At frequencies between 158~GHz and 200~GHz, below the onset of diffraction effects, reflectance is reduced from a maximum of 64% to about 25%, closely matching predictions. These measurements of the index, loss, and SWS-ARC of 3D printed alumina suggest that the material and fabrication technique could be useful for astrophysical applications.