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Lumped-Element Kinetic Inductance Detectors for Cosmic Microwave Background Polarimetry
Completed
Description
NASA's Science Mission Directorate (SMD) calls out understanding how the universe began as a major goal. The Cosmic Microwave Background (CMB) is a nearly isotropic radiation that fills the universe and contains unique cosmological information. The CMB contains polarization anisotropies and a measurement of the primordial B-mode polarization signal from inflationary gravitational waves could uniquely confirm the theory of inflation. In order to make this measurement, thousands of detectors with photon-noise limited sensitivity are needed. The NESSF fellowship has enabled me to work on the development of Lumped Element Kinetic Inductance Detectors (LEKIDs) for measuring CMB anisotropies. Specifically, I am conducting research for dual-polarization LEKIDs that are sensitive to spectral bands in the millimeter wavelengths where the CMB spectrum peaks. In the first year of the NESSF fellowship, I accomplished all stated goals, most importantly to demonstrate sensitive dual-polarization LEKIDs with low noise. We have been invited to deploy the dual-polarization LEKIDs at the Keck Array, a B-mode polarization experiment, for an on-sky test in the coming year. I will be part of the team to integrate and deploy the detectors and to analyze the experimental data. Additionally, as part of a collaboration, I have begun work towards developing multichroic KIDs, meaning the detectors are simultaneously sensitive to multiple spectral bands, that could be used in future CMB missions. In this progress report, I give a summary of work accomplished and present the research plan for 2016-2017. This research works to fulfill the NASA objectives of 1. Developing technological advances for future missions and 2. Measuring or a setting an upper limit on the primordial B-mode polarization signal.
Details
| Technology area | Sensors and Instruments > Remote Sensing Instruments and Sensors > Detectors and Focal Planes |
| Program | Astrophysics (APD) |
| Start date | 2016-09-01 |
| End date | 2017-08-31 |
Project contacts
Listed on TechPort itself — the most direct way to ask about this specific project.
- Bradley R Johnson
- Heather Horgan
- Heather L Mccarrick
How to get involved
This is a mature technology (TRL 7+) — the realistic path in is usually NASA's Technology Transfer Program: licensing an existing NASA patent, or a Space Act Agreement to use NASA facilities/expertise directly. NASA also runs a startup licensing program with no upfront fee for companies formed to commercialize a specific NASA technology.
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