2014
DOI: 10.1007/s10971-014-3275-y
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Enhanced flux pinning in YGdBCO film grown by sol–gel approach

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Cited by 7 publications
(4 citation statements)
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“…Figure 6a shows the HAADF STEM overview of the YBCO-Gd 5% layer on the STO substrate. No precipitate particles or secondary phases ascribable to RE 2 O 3 were present, in contrast with the previously reported study by [20]. The vertical brighter/darker contrast corresponded to YBCO twin grains with an average size of 18.5 nm in [100]/[010]YBCO projection (giving ~13 nm in [110]YBCO projection).…”
Section: Structural Properties and Morphologycontrasting
confidence: 83%
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“…Figure 6a shows the HAADF STEM overview of the YBCO-Gd 5% layer on the STO substrate. No precipitate particles or secondary phases ascribable to RE 2 O 3 were present, in contrast with the previously reported study by [20]. The vertical brighter/darker contrast corresponded to YBCO twin grains with an average size of 18.5 nm in [100]/[010]YBCO projection (giving ~13 nm in [110]YBCO projection).…”
Section: Structural Properties and Morphologycontrasting
confidence: 83%
“…Li et al observed an increase in both T c and J c in the whole field range at 77 K. These authors ascribed the enhancement to the significant presence of RE 2 O 3 phases in their films. In our work, instead, we observed a different behavior: T c was not affected by Gd addition (Table 4), whereas J c behaviors were more markedly improved at lower temperatures rather than at 77 K. This result, in agreement with the structural and morphological characterizations, evidenced the effect of the different nature of the introduced defects (no RE 2 O 3 phases were recognized in our samples), likely due to the different growth methods [20].…”
Section: Temperature (K)supporting
confidence: 68%
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