Lithographed Superconducting Resonator Development for Next-Generation Frequency Multiplexing Readout of Transition-Edge Sensors

被引:0
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作者
F. Faramarzi
T. De Haan
A. Kusaka
A. Lee
B. Neuhauser
R. Plambeck
C. Raum
A. Suzuki
B. Westbrook
机构
[1] San Francisco State University,Department of Physics and Astronomy
[2] University of California,Department of Physics
[3] Lawrence Berkeley National Laboratory,Department of Physics
[4] University of California,Radio Astronomy Laboratory
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关键词
Cosmic microwave background radiation; Transition-edge sensors; Frequency-domain multiplexing; Superconducting LC resonators;
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摘要
Ground-based cosmic microwave background (CMB) experiments are undergoing a period of exponential growth. Current experiments are observing with 1000–10,000 detectors, and the next-generation experiment (CMB stage 4) is proposing to deploy approximately 500,000 detectors. This order of magnitude increase in detector count will require a new approach for readout electronics. We have developed superconducting resonators for next-generation frequency-domain multiplexing (fMUX) readout architecture. Our goal is to reduce the physical size of resonators, such that resonators and detectors can eventually be integrated on a single wafer. To reduce the size of these resonators, we have designed spiral inductors and interdigitated capacitors that resonate around 10–100 MHz, an order of magnitude higher frequency compared to current fMUX readout systems. The higher frequency leads to a wider bandwidth and would enable higher multiplexing factor than the current ∼\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\sim $$\end{document} 50 detectors per readout channel. We will report on the simulation, fabrication method, characterization technique, and measurement of quality factor of these resonators.
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页码:498 / 504
页数:6
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