2004
DOI: 10.1134/1.1687853
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Distribution of a local magnetic field in superconductors with an uncorrelated random lattice of abrikosov vortices

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Cited by 5 publications
(4 citation statements)
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“…18 Such disorder in the VL can produce a symmetric lineshape, 38,50 and can broaden the field distribution significantly compared to that of the corresponding ordered state. 51 Weak random pinning or point-like disorder due to oxygen deficiency may slightly distort the VL, and may also broaden the lineshape.…”
mentioning
confidence: 99%
“…18 Such disorder in the VL can produce a symmetric lineshape, 38,50 and can broaden the field distribution significantly compared to that of the corresponding ordered state. 51 Weak random pinning or point-like disorder due to oxygen deficiency may slightly distort the VL, and may also broaden the lineshape.…”
mentioning
confidence: 99%
“…18 Such disorder in the VL can produce a symmetric lineshape, 38,50 and can broaden the field distribution significantly compared to that of the corresponding ordered state. 51 Weak random pinning or point-like disorder due to oxygen deficiency may slightly distort the VL, and may also broaden the lineshape. 39 However, the correlated disorder due to the twin and grain boundaries is dominant at long wavelengths, 40,52 and therefore we are mostly sensitive to the twin/grain boundaries.…”
Section: Discussionmentioning
confidence: 99%
“…In particular, it is well known that for regular lattices the line shapes are significantly different for lattices of different symmetries [8]. When, however, σ is increasing, these differences tend to average, and the distribution function approximates that of a Gaussian distribution [11]. The calculations demonstrated that a non-uniform field quite rapidly, already at a distance 0.2 (measured in λ units), becomes uniform; hence, the thickness of the films selected should not exceed 0.2.…”
Section: Irregularly Distributed Abrikosov's Vorticesmentioning
confidence: 95%
“…It is well known that an Abrikosov vortex lattice is formed in HTSC in an external magnetic field Н (Н с1 < H < H c2 , H c1 , H c2 are the first and second critical fields). However, the distribution of local magnetic field has so far been calculated for either regular vortex lattices [8 -10] or for the case of complete chaos in the distribution of Abrikosov's vortices -random non-correlated distribution of vortices [11], with no signs of a regular vortex lattice. Nonetheless, the case of a irregular vortex lattice is quite common.…”
mentioning
confidence: 99%