Low Loss Superconducting Microstrip Development at Argonne National Lab
Journal Article
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· IEEE Transactions on Applied Superconductivity
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- Argonne National Lab. (ANL), Argonne, IL (United States). High-Energy Physics Division; Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics. Dept. of Astronomy and Astrophysics
- Cardiff Univ. (United Kingdom). School of Physics and Astronomy
- Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology. Dept. of Physics; SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Univ. of California, San Diego, CA (United States). Dept. of Physics
- Univ. of Colorado, Boulder, CO (United States). Center for Astrophysics and Space Astronomy. Dept. of Astrophysical and Planetary Sciences
- McGill Univ., Montreal, QC (Canada). Dept. of Physics
- Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics; Argonne National Lab. (ANL), Argonne, IL (United States). High-Energy Physics Division
- Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics. Dept. of Astronomy and Astrophysics
- Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics. The Enrico Fermi Inst. Dept. of Physics. Dept. of Astronomy and Astrophysics; Argonne National Lab. (ANL), Argonne, IL (United States). High-Energy Physics Division
- SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Argonne National Lab. (ANL), Argonne, IL (United States). High-Energy Physics Division
- Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics. Dept. of Astronomy and Astrophysics
- Univ. of California, Berkeley, CA (United States). Dept. of Physics
- Argonne National Lab. (ANL), Argonne, IL (United States). Materials Sciences Division
- McGill Univ., Montreal, QC (Canada). Dept. of Physics; Canadian Inst. for Advanced Research, Toronto, ON (Canada). CIFAR Program in Cosmology and Gravity
- Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics. Dept. of Physics
- Univ. of Colorado, Boulder, CO (United States). Center for Astrophysics and Space Astronomy. Dept. of Astrophysical and Planetary Sciences. Dept. of Physics
- High Energy Accelerator Research Organization (KEK), Tsukuba (Japan)
- National Inst. of Standards and Technology (NIST), Boulder, CO (United States). Quantum Devices Group
- National Inst. of Standards and Technology (NIST), Boulder, CO (United States)
- Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology. Dept. of Physics
- Univ. of California, Davis, CA (United States). Dept. of Physics
- Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
- Univ. of California, Berkeley, CA (United States). Dept. of Physics; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). Physics Division
- Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States). Kavli Inst. for Astrophysics and Space Research
- Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics. The Enrico Fermi Inst. Dept. of Physics. Dept. of Astronomy and Astrophysics
- Argonne National Lab. (ANL), Argonne, IL (United States). Materials Science Division
- California Inst. of Technology (CalTech), Pasadena, CA (United States)
- Univ. of Melbourne, VIC (Australia). School of Physics; Univ. of California, Berkeley, CA (United States). Dept. of Physics
- Case Western Reserve Univ., Cleveland, OH (United States). Dept. of Physics
- Three-Speed Logic, Inc., Vancouver, BC (Canada)
- Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
- Univ. of Toronto, ON (Canada). Dunlap Inst. for Astronomy and Astrophysics. Dept. of Astronomy and Astrophysics
- Univ. of Illinois, Urbana, IL (United States). Dept. of Astronomy. Dept. of Physics
Low loss superconducting microstrip is an essential component in realizing 100 kilo-pixel multichroic cosmic microwave background detector arrays. In this paper, we have been developing a low loss microstrip by understanding and controlling the loss mechanisms. We present the fabrication of the superconducting microstrip, the loss measurements at a few GHz frequencies using half-wavelength resonators, and the loss measurements at 220 GHz frequencies with the superconducting microstrip coupled to slot antennas at one end and to TES detectors at the other end. Finally, the measured loss tangent of the microstrip made of sputtered Nb and SiOx is 1-2e-3.
- Research Organization:
- Argonne National Lab. (ANL), Argonne, IL (United States); SLAC National Accelerator Lab., Menlo Park, CA (United States); Univ. of Chicago, IL (United States); Stanford Univ., CA (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Sponsoring Organization:
- USDOE Office of Science (SC), Basic Energy Sciences (BES); National Science Foundation (NSF); The Kavli Foundation (United States); Gordon and Betty Moore Foundation (United States)
- Grant/Contract Number:
- AC02-06CH11357; ANT-0638937; PHY-1125897; AST-0956135
- OSTI ID:
- 1357457
- Journal Information:
- IEEE Transactions on Applied Superconductivity, Vol. 25, Issue 3; ISSN 1051-8223
- Publisher:
- Institute of Electrical and Electronics Engineers (IEEE)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
Cited by: 5 works
Citation information provided by
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