With moderate cooling requirements, YBCO-based superconducting detectors are promising for space applications from microwave to the terahertz regime. Their sensitivities, however, are still rather limited. The dielectric loss of the substrate on which YBCO films are deposited might play an important role in the detector performance. This study systematically characterizes the dielectric properties of three common commercially available substrates for YBCO film, i.e., Sapphire (Al2O3), Lanthanum aluminate (LaAlO3), and Magnesium oxide (MgO), from 0.22 to 3 THz at 300 K, 77 K, and 20 K. It has been found that both Al2O3and MgO substrates exhibit significantly reduced loss tangents (tanδ-5) at cryogenic temperatures (77 K and 20 K), whereas LaAlO3maintains high dielectric loss tangents (tanδ > 3×10-3) across all measured temperatures and frequencies
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Zhou et al. (2025) studied this question.
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