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Distribution of flux-pinning energies in YBa sub 2 Cu sub 3 O sub 7 minus. delta. and Bi sub 2 Sr sub 2 CaCu sub 2 O sub 8+. delta. from flux noise

Journal Article · · Physical Review Letters; (USA)
; ; ;  [1]; ; ; ; ; ;  [2]
  1. Department of Physics, University of California, Berkeley, CA (USA) Center for Advanced Materials, Materials and Chemical Sciences Division, Lawrence Berkeley Laboratory, 1 Cyclotron Road, Berkeley, California 94720 (USA)
  2. Department of Applied Physics, Stanford University, Stanford, California 94305 (USA)
The spectral density of the magnetic flux noise measured in high-temperature superconductors in low magnetic fields scales approximately as the inverse of the frequency and increases with temperature. We use the temperature and frequency dependence of the noise to determine the pinning energies of individual flux vortices in thermal equilibrium. The distribution of pinning energies peaks below 0.1 eV in YBa{sub 2}Cu{sub 3}O{sub 7-{delta}} and near 0.2 eV in Bi{sub 2}Sr{sub 2}CaCu{sub 2}O{sub 8+{delta}}. The noise power is proportional to the ambient magnetic field, indicating that the vortex motion is uncorrelated.
DOE Contract Number:
AC03-76SF00098
OSTI ID:
7242797
Journal Information:
Physical Review Letters; (USA), Journal Name: Physical Review Letters; (USA) Vol. 64:1; ISSN PRLTA; ISSN 0031-9007
Country of Publication:
United States
Language:
English

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