Development of Multi-chroic MKIDs for Next-Generation CMB Polarization Studies

Development of Multi-chroic MKIDs for Next-Generation CMB Polarization Studies
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开发用于下一代 CMB 偏振研究的多色 MKID

DOI:
10.1007/s10909-018-2032-y
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发表时间:
2018
影响因子:
2
通讯作者:
Irwin, K.
Irwin, K.
中科院分区:
物理与天体物理3区
文献类型:
--
作者:
Johnson, B. R.;Flanigan, D.;Abitbol, M. H.;Ade, P. A.;Bryan, S.;Cho, H.-M.;Datta, R.;Day, P.;Doyle, S.;Irwin, K.

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我们报告的状态正在进行的努力,开发阵列的喇叭耦合,极化敏感的微波动力学电感探测器(MKID),每个敏感的两个光谱波段之间的125和280 GHz。这些多色MKID阵列是为下一代大探测器数量的实验量身定制的,这些实验旨在同时表征宇宙微波背景和银河尘埃发射的偏振特性。我们提出了我们的设备设计,并描述了基于实验室的测量结果,从两个23元素的原型阵列。从我们的第一个工程阵列的暗测量,我们证明了一个复用因子为92,显示谐振器响应浴温度变化的预期,并发现,制造产量为100%。从我们的第一个光学加载阵列,我们发现MKID响应毫米波脉冲;其他光学特性测量正在进行中。最后,我们讨论了我们在未来2年内将这项技术扩展到千像素阵列的计划。
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.
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