Defect structure and superconducting properties of La1.8SrxCa1.2xCu2O6δ

H. Shaked, J. D. Jorgensen, B. A. Hunter, R. L. Hitterman, K. Kinoshita, F. Izumi, and T. Kamiyama
Phys. Rev. B 48, 12941 – Published 1 November 1993
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Abstract

We have studied the relationship between structural defects and superconductivity in La1.8SrxCa1.2xCu2O6δ (0≤x≤0.8). The samples were prepared by synthesis under different oxygen pressures, P(O2)=50, 250, and 400 atm. Six of the seven samples were found to be superconducting with 22≤Tc≤58 K. The structural properties were determined by neutron powder diffraction. The inter-CuO2-plane spacing, dCuCu, increases as Ca on the M(1) site between these planes is replaced by the larger Sr and La ions. The metal-site ordering is influenced by the oxygen pressure during synthesis. We have used the inter-CuO2-plane spacing, neutron-diffraction measurements of the scattering from the metal sites, and chemical constraints to determine the occupancies of La, Sr, and Ca at the M(1) site. For the same overall composition, higher oxygen pressure leads to a larger fraction of La on the M(1) site. Oxygen occupancy of the vacant O(3) site in the M(1) plane increases sharply when dCuCu exceeds 3.5 Å. The superconducting transition temperature Tc decreases systematically as the occupancy of O(3) increases for samples that would otherwise be expected to be superconducting.

  • Received 2 August 1993

DOI:https://doi.org/10.1103/PhysRevB.48.12941

©1993 American Physical Society

Authors & Affiliations

H. Shaked, J. D. Jorgensen, B. A. Hunter, and R. L. Hitterman

  • Materials Science Division, Argonne National Laboratory, Argonne, Illinois 60439

K. Kinoshita

  • Nippon Telegraph and Telephone Corporation Basic Research Laboratories, Musashino, Tokyo 180, Japan

F. Izumi

  • National Institute for Research in Inorganic Materials, 1-1 Namiki, Tsukuba, Ibaraki 305, Japan

T. Kamiyama

  • Institute of Materials Science, University of Tsukuba, Tsukuba, Ibaraki 305, Japan

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Vol. 48, Iss. 17 — 1 November 1993

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