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Ultra-Stable Kinetic Inductance Detectors for Astrophysical Observations

Completed TRL 2 (started at 1, targeting 2)

Description

This proposal seeks to implement a new KID design to reduce the low-frequency 1/f noise limiting the performance of this detector technology. This innovative design is based on work demonstrating near theoretically achievable current density in superconducting Nb nano-wires To reduce the 1/f noise, the inductive element in the resonator will be fabricated as a mesh. The proposed tasks involve fabrication of nano-mesh inductors out of Nb, TiN, and Al. The nano-meshes will be elements of superconducting resonators enabling characterization of the DC critical current and microwave response. The detailed microwave properties of the resonators, including quality factor, Q, and noise, will be characterized using existing instrumentation.

Benefits

This effort represents fundamantal research into KIDs, which are a type of sensor that has significant potential for future astrophysical applications.

Details

Technology areaSensors and Instruments > Remote Sensing Instruments and Sensors > Detectors and Focal Planes
ProgramCenter Innovation Fund: GSFC CIF (GSFC CIF)
Lead organizationGoddard Space Flight Center, Greenbelt, MD
Start date2017-10-01
End date2018-09-30

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