Journal article
Development of multi-chroic MKIDs for next-generation CMB polarization studies
- Abstract:
- We report on the status of an ongoing effort to develop arrays of horn-coupled, polarization-sensitive microwave kinetic inductance detectors (MKIDs) that are each sensitive to two spectral bands between 125 and 280 GHz. These multi-chroic MKID arrays are tailored for next-generation, large-detector-count experiments that are being designed to simultaneously characterize the polarization properties of both the cosmic microwave background and Galactic dust emission. We present our device design and describe laboratory-based measurement results from two 23-element prototype arrays. From dark measurements of our first engineering array, we demonstrated a multiplexing factor of 92, showed the resonators respond to bath temperature changes as expected, and found that the fabrication yield was 100%. From our first optically loaded array, we found the MKIDs respond to millimeter-wave pulses; additional optical characterization measurements are ongoing. We end by discussing our plans for scaling up this technology to kilo-pixel arrays over the next 2 years.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
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- Files:
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(Preview, Accepted manuscript, pdf, 13.1MB, Terms of use)
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- Publisher copy:
- 10.1007/s10909-018-2032-y
Authors
- Publisher:
- Springer Verlag
- Journal:
- Journal of Low Temperature Physics More from this journal
- Volume:
- 193
- Issue:
- 3-4
- Pages:
- 103–112
- Publication date:
- 2018-07-30
- Acceptance date:
- 2018-07-18
- DOI:
- EISSN:
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1573-7357
- ISSN:
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0022-2291
- Language:
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English
- Keywords:
- Pubs id:
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pubs:922977
- UUID:
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uuid:fc8e856b-7f77-488b-9bbd-b7505774dc7f
- Local pid:
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pubs:922977
- Source identifiers:
-
922977
- Deposit date:
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2019-01-29
Terms of use
- Copyright holder:
- Springer Science+Business Media
- Copyright date:
- 2018
- Notes:
- © Springer Science+Business Media, LLC, part of Springer Nature 2018. This is the accepted manuscript version of the article. The final version is available online from Springer at: https://doi.org/10.1007/s10909-018-2032-y
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