Magnetic interaction in hole-doped high- Tc superconductors observed by angle-resolved photoemission spectroscopy

T. Sato, H. Matsui, K. Terashima, T. Takahashi, H. Ding, H. B. Yang, S. C. Wang, T. Fujii, T. Watanabe, A. Matsuda, T. Terashima, K. Kadowaki

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Abstract

We have performed a high-resolution angle-resolved photoemission spectroscopy (ARPES) on high-Tc superconductors (HTSCs) Bi 2Sr2Can-1CunO2n+4 (n=1-3) to study the systematics of the electronic structure and the origin of many-body interactions responsible for superconductivity. We find that a large hole-like Fermi surface and d-wave superconducting gap are generic features of Bi-based HTSCs. For n=2 and 3, a sudden change in the energy dispersion, so-called "kink", becomes pronounced on approaching (π,0) in the superconducting state, while a kink appears only around the nodal direction in the normal state. The kink around (π,0) disappears at Tc. For n=1, the kink shows no significant temperature dependence even across Tc. This could suggest that the coupling of electrons with Q=(π,π) magnetic mode is dominant in the superconducting state for multi-layered cuprates, while the interaction at the normal state and that of single-layered cuprates have a different origin.

Original languageEnglish
Pages (from-to)51-58
Number of pages8
JournalPhysica C: Superconductivity and its applications
Volume412-414
Issue numberSPEC. ISS.
DOIs
Publication statusPublished - Oct 1 2004

Keywords

  • ARPES
  • Bi-based cuprates
  • Electronic structure

ASJC Scopus subject areas

  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics
  • Energy Engineering and Power Technology
  • Electrical and Electronic Engineering

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    Sato, T., Matsui, H., Terashima, K., Takahashi, T., Ding, H., Yang, H. B., Wang, S. C., Fujii, T., Watanabe, T., Matsuda, A., Terashima, T., & Kadowaki, K. (2004). Magnetic interaction in hole-doped high- Tc superconductors observed by angle-resolved photoemission spectroscopy. Physica C: Superconductivity and its applications, 412-414(SPEC. ISS.), 51-58. https://doi.org/10.1016/j.physc.2003.11.063