Enhanced Superconducting Gaps in the Trilayer High-Temperature Bi2Sr2Ca2Cu3O10+δ Cuprate Superconductor

S. Ideta, K. Takashima, M. Hashimoto, T. Yoshida, A. Fujimori, H. Anzai, T. Fujita, Y. Nakashima, A. Ino, M. Arita, H. Namatame, M. Taniguchi, K. Ono, M. Kubota, D. H. Lu, Z.-X. Shen, K. M. Kojima, and S. Uchida
Phys. Rev. Lett. 104, 227001 – Published 1 June 2010

Abstract

We report the first observation of the multilayer band splitting in the optimally doped trilayer cuprate Bi2Sr2Ca2Cu3O10+δ (Bi2223) by angle-resolved photoemission spectroscopy. The observed energy bands and Fermi surfaces are originated from the outer and inner CuO2 planes (OP and IP). The OP band is overdoped with a large d-wave gap around the node of Δ043meV while the IP is underdoped with an even large gap of Δ060meV. These energy gaps are much larger than those for the same doping level of the double-layer cuprates, which leads to the large Tc in Bi2223. We propose possible origins of the large superconducting gaps for the OP and IP: (1) minimal influence of out-of-plane disorder and a proximity effect and (2) interlayer tunneling of Cooper pairs between the OP and IP.

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  • Received 20 April 2009

DOI:https://doi.org/10.1103/PhysRevLett.104.227001

©2010 American Physical Society

Authors & Affiliations

S. Ideta1, K. Takashima1, M. Hashimoto1, T. Yoshida1, A. Fujimori1, H. Anzai2, T. Fujita2, Y. Nakashima2, A. Ino2, M. Arita3, H. Namatame3, M. Taniguchi2,3, K. Ono4, M. Kubota4, D. H. Lu5, Z.-X. Shen5, K. M. Kojima1, and S. Uchida1

  • 1Department of Physics, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan
  • 2Graduate School of Science, Hiroshima University, Higashi-Hiroshima 739-8526, Japan
  • 3Hiroshima Synchrotron Center, Hiroshima University, Higashi-Hiroshima 739-0046, Japan
  • 4Photon Factory, Institute of Materials Structure Science, KEK, Tsukuba, Ibaraki 305-0801, Japan
  • 5Department of Applied Physics and Stanford Synchrotron Radiation Lightsource, Stanford University, Stanford, California, 94305, USA

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Vol. 104, Iss. 22 — 4 June 2010

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