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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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Publisher copy:
10.1007/s10909-018-2032-y

Authors


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Role:
Author
ORCID:
0000-0002-6898-8938
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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics
Sub department:
Astrophysics
Department:
Unknown
Role:
Author
ORCID:
0000-0001-8071-6735


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:
1573-7357
ISSN:
0022-2291


Language:
English
Keywords:
Pubs id:
pubs:922977
UUID:
uuid:fc8e856b-7f77-488b-9bbd-b7505774dc7f
Local pid:
pubs:922977
Source identifiers:
922977
Deposit date:
2019-01-29

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