Abstract
Superconducting circuit elements used in millimeter-submillimeter (mm-submm) astronomy would greatly benefit from deposited dielectrics with small dielectric loss and noise. This will enable the use of multilayer circuit elements and thereby increase the efficiency of mm-submm filters and allow for a miniaturization of microwave kinetic inductance detectors (MKIDs). Amorphous dielectrics introduce excess loss and noise compared with their crystalline counterparts, due to two-level system defects of unknown microscopic origin. We deposited hydrogenated amorphous silicon films using plasma-enhanced chemical vapor deposition, at substrate temperatures of 100°C, 250°C, and 350°C. The measured void volume fraction, hydrogen content, microstructure parameter, and bond-Angle disorder are negatively correlated with the substrate temperature. All three films have a loss tangent below 10-5 for a resonator energy of 105 photons, at 120 mK and 4 to 7 GHz. This makes these films promising for MKIDs and on-chip mm-submm filters.
| Original language | English |
|---|---|
| Article number | 028006 |
| Number of pages | 13 |
| Journal | Journal of Astronomical Telescopes, Instruments, and Systems |
| Volume | 8 |
| Issue number | 2 |
| DOIs | |
| Publication status | Published - 2022 |
Keywords
- amorphous silicon
- dielectric loss
- filter bank
- kinetic inductance detectors
- millimeter-submillimeter
- spectrometer
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