Twins and Intergrowth Defects in High-<I>T</I><SUB>c</SUB> Bi–Sr–Ca–Cu–O Superconductor Examined by High-Resolution Electron Microscopy

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説明

Twinned structure with twin plane (510) and with the composition plane (001) is observed in a high-Tc Bi–Sr–Ca–Cu–O superconductor which is orthorhombic with a=0.54, b=2.7 and c=3.08 nm. Directions of “Bi-concentrated bands” in both twin individuals are perpendicular to each other. Local intergrowths of perovskite-related layers with 1.8 and 2.1 nm thickness are observed among the major layers of 1.5 nm. The material includes small amounts of crystal with c=3.6 nm, which may be responsible for the superconductivity at 105 K, as already suggested by Muromachi et al. (Jpn. J. Appl. Phys. 27 (1988) L556).

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詳細情報 詳細情報について

  • CRID
    1570291227384104704
  • NII論文ID
    110003928126
  • NII書誌ID
    AA10650595
  • 本文言語コード
    en
  • データソース種別
    • CiNii Articles

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