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High-Efficiency Feedhorn-Coupled Detector Arrays to Enable Next-Generation Space-Based CMB Polarization Missions

Completed TRL 4 (started at 3, targeting 4)

Description

We aim to develop highly efficient and uniform arrays of polarization-sensitive microwave bolometers for future cosmic microwave background missions. This project will develop on-chip broadband calibrator loads to test the detector circuit on an element-by-element basis. This work is key in demonstrating the ability of this detector technology to achieve the required sensitivity and control over systematic error to enable next-generation cosmic microwave missions.

Benefits

This technology will enable next-generation cosmic microwave background missions to peer back to the first moments after the Big Bang, shed light on the nature of dark matter and dark energy, and search for new fundamental particles.

Details

Technology areaSensors and Instruments > Remote Sensing Instruments and Sensors > Detectors and Focal Planes
ProgramCenter Independent Research & Development: GSFC IRAD (GSFC IRAD)
Lead organizationGoddard Space Flight Center, Greenbelt, MD
Start date2019-10-01
End date2020-09-30

Project contacts

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How to get involved

This is early/mid-stage (TRL 4) — the most realistic path in is NASA SBIR/STTR, which funds small businesses and research institutions to develop technology aligned with NASA's needs (equity-free, phased funding). Check whether a current SBIR/STTR solicitation topic overlaps with this project's technology area, or contact the project directly (above) to ask.

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