Magnetic flux noise in dc SQUIDs: temperature and geometry dependence

The spectral density S(Φ)(f) = A(2)/(f/1 Hz)(α) of magnetic flux noise in ten dc superconducting quantum interference devices (SQUIDs) with systematically varied geometries shows that α increases as the temperature is lowered; in so doing, each spectrum pivots about a nearly constant frequency. The...

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Veröffentlicht in:Physical review letters 2013-04, Vol.110 (14), p.147002-147002, Article 147002
Hauptverfasser: Anton, S M, Birenbaum, J S, O'Kelley, S R, Bolkhovsky, V, Braje, D A, Fitch, G, Neeley, M, Hilton, G C, Cho, H-M, Irwin, K D, Wellstood, F C, Oliver, W D, Shnirman, A, Clarke, John
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container_end_page 147002
container_issue 14
container_start_page 147002
container_title Physical review letters
container_volume 110
creator Anton, S M
Birenbaum, J S
O'Kelley, S R
Bolkhovsky, V
Braje, D A
Fitch, G
Neeley, M
Hilton, G C
Cho, H-M
Irwin, K D
Wellstood, F C
Oliver, W D
Shnirman, A
Clarke, John
description The spectral density S(Φ)(f) = A(2)/(f/1 Hz)(α) of magnetic flux noise in ten dc superconducting quantum interference devices (SQUIDs) with systematically varied geometries shows that α increases as the temperature is lowered; in so doing, each spectrum pivots about a nearly constant frequency. The mean-square flux noise, inferred by integrating the power spectra, grows rapidly with temperature and at a given temperature is approximately independent of the outer dimension of a given SQUID. These results are incompatible with a model based on the random reversal of independent, surface spins.
doi_str_mv 10.1103/PhysRevLett.110.147002
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title Magnetic flux noise in dc SQUIDs: temperature and geometry dependence
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