TY - JOUR
T1 - Half-meter Scale Superconducting Magnetic Bearing for Cosmic Microwave Background Polarization Experiments
AU - Sakurai, Yuki
AU - Ashton, Peter
AU - Kusaka, Akito
AU - Hill, Charles A.
AU - Kiuchi, Kenji
AU - Katayama, Nobuhiko
AU - Tajima, Osamu
N1 - Funding Information:
This work was supported by MEXT KAKENHI Grant Numbers, JP19H00674, 17H06134, 16K21744 JP17K14272, and JP19K14732. This workaws also supportedybJPSSoCre-to-CoreProgram, Advanced Research Networks and World Premier International Research Center Initiative (WPI) MEXTJapan, andJSPSeLading Initiative for Excellent YoungeRsearchers (LEADER).Theworkat LBNL is supported in part by the U.S. Department of Energy, Office of Science, Office of High Energy Physics, under contract No. DE-AC02-05CH11231. The authors would like to thank Shin-Etsu Chemical Co., Ltd. for the cooperation of the manufacturing of the ring magnet. We would like to thank dEitage (www.editage.com) and American Manuscript Editors (www.americanmanuscripteditors.com)for Englishnlguaagedeitg.in
Publisher Copyright:
© Published under licence by IOP Publishing Ltd.
PY - 2020/7/31
Y1 - 2020/7/31
N2 - We report the development of a large-diameter superconducting magnetic bearing (SMB) used in a continuously rotating cryogenic half-wave plate (HWP) polarization modulator for cosmic microwave background (CMB) polarization experiments. A precise measurement of the CMB polarization will place tighter constrains on cosmic inflation, describing the rapid expansion of the early universe. The polarization modulator is a critical instrument for suppressing 1/f contamination, which is mainly caused by atmospheric noise, and for mitigating systematic uncertainties that arise when differencing orthogonal polarization detectors. To ensure a sufficient field of view and to reduce thermal emission, the polarization modulator must have a clear-aperture diameter of > 500 mm and must operate at cryogenic temperatures. We constructed a superconducting magnetic bearing (SMB) with an inner diameter of 550 mm, which is the largest used in any CMB polarization experiment to date. We tested the friction and stiffness of the bearing at liquid nitrogen temperatures. The measured total loss is 0.4 W and the spring constant is >105 N/m, which satisfies typical experimental requirements. Furthermore, we performed a performance test by changing the number of disk-shaped YBCO tiles, and then confirmed that the SMB performance was proportional to the YBCO volume.
AB - We report the development of a large-diameter superconducting magnetic bearing (SMB) used in a continuously rotating cryogenic half-wave plate (HWP) polarization modulator for cosmic microwave background (CMB) polarization experiments. A precise measurement of the CMB polarization will place tighter constrains on cosmic inflation, describing the rapid expansion of the early universe. The polarization modulator is a critical instrument for suppressing 1/f contamination, which is mainly caused by atmospheric noise, and for mitigating systematic uncertainties that arise when differencing orthogonal polarization detectors. To ensure a sufficient field of view and to reduce thermal emission, the polarization modulator must have a clear-aperture diameter of > 500 mm and must operate at cryogenic temperatures. We constructed a superconducting magnetic bearing (SMB) with an inner diameter of 550 mm, which is the largest used in any CMB polarization experiment to date. We tested the friction and stiffness of the bearing at liquid nitrogen temperatures. The measured total loss is 0.4 W and the spring constant is >105 N/m, which satisfies typical experimental requirements. Furthermore, we performed a performance test by changing the number of disk-shaped YBCO tiles, and then confirmed that the SMB performance was proportional to the YBCO volume.
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U2 - 10.1088/1742-6596/1590/1/012060
DO - 10.1088/1742-6596/1590/1/012060
M3 - Conference article
AN - SCOPUS:85090024293
SN - 1742-6588
VL - 1590
JO - Journal of Physics: Conference Series
JF - Journal of Physics: Conference Series
IS - 1
M1 - 012060
T2 - 32nd International Symposium on Superconductivity, ISS 2019
Y2 - 3 December 2019 through 5 December 2019
ER -