TY - JOUR
T1 - Novel frequency-domain multiplexing MKID readout for the LiteBIRD satellite
AU - Hattori, K.
AU - Ariyoshi, S.
AU - Hazumi, M.
AU - Ishino, H.
AU - Kibayashi, A.
AU - Mima, S.
AU - Otani, C.
AU - Satoh, N.
AU - Tomaru, T.
AU - Yoshida, M.
AU - Watanabe, H.
N1 - Funding Information:
Acknowledgements This work was partly supported by Grants-in-Aid for Scientific Research on Innovative Areas No. 21111002 and No. 21111003. We acknowledge support from the Department of Physics, Okayama University, and the Detector Technology Project at the High Energy Accelerator Research Organization (KEK).
PY - 2012/6
Y1 - 2012/6
N2 - The satellite LiteBIRD (Light satellite for the studies of B-mode polarization and Inflation from cosmic background Radiation Detection) is being designed to detect the B-mode polarization of the cosmic microwave background radiation. LiteBIRD will carry about 2,000 detectors for measurements in five bands (60, 80, 100, 150, and 220 GHz). Microwave kinetic inductance detectors (MKIDs) that can be multiplexed in a single readout line are suitable for the large focal plane detector array. We develop an MKID readout system for LiteBIRD to monitor the amplitude, phase, and resonant frequency of each MKID resonator simultaneously and follow movements of the resonant frequency caused by changes in the input radiation intensity. This mechanism enables us to have a larger dynamic range for the MKIDs, compared with a system that monitors the amplitude and phase on the resonant frequency. We also propose an MKID having a half-wavelength resonator. This MKID transmits the resonant microwave signal from one feedline to another. It can offer clear microwaves passing through the resonators, even if the coupling and internal quality factors are mismatched. With this MKID, our readout system can track resonance frequency changes much more easily. We present the status of the readout system development and demonstrate the performance with the half-wavelength MKID.
AB - The satellite LiteBIRD (Light satellite for the studies of B-mode polarization and Inflation from cosmic background Radiation Detection) is being designed to detect the B-mode polarization of the cosmic microwave background radiation. LiteBIRD will carry about 2,000 detectors for measurements in five bands (60, 80, 100, 150, and 220 GHz). Microwave kinetic inductance detectors (MKIDs) that can be multiplexed in a single readout line are suitable for the large focal plane detector array. We develop an MKID readout system for LiteBIRD to monitor the amplitude, phase, and resonant frequency of each MKID resonator simultaneously and follow movements of the resonant frequency caused by changes in the input radiation intensity. This mechanism enables us to have a larger dynamic range for the MKIDs, compared with a system that monitors the amplitude and phase on the resonant frequency. We also propose an MKID having a half-wavelength resonator. This MKID transmits the resonant microwave signal from one feedline to another. It can offer clear microwaves passing through the resonators, even if the coupling and internal quality factors are mismatched. With this MKID, our readout system can track resonance frequency changes much more easily. We present the status of the readout system development and demonstrate the performance with the half-wavelength MKID.
KW - Cosmic microwave background radiation
KW - Frequency-domain multiplexing
KW - Microwave kinetic inductance detectors
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U2 - 10.1007/s10909-012-0506-x
DO - 10.1007/s10909-012-0506-x
M3 - Article
AN - SCOPUS:84905044142
SN - 0022-2291
VL - 167
SP - 671
EP - 677
JO - Journal of Low Temperature Physics
JF - Journal of Low Temperature Physics
IS - 5-6
ER -