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Infrared pseudogap in cuprate and pnictide high-temperature superconductors

S. J. Moon, Y. S. Lee, A. A. Schafgans, A. V. Chubukov, S. Kasahara, T. Shibauchi, T. Terashima, Y. Matsuda, M. A. Tanatar, R. Prozorov, A. Thaler, P. C. Canfield, S. L. Bud'ko, A. S. Sefat, D. Mandrus, K. Segawa, Y. Ando, and D. N. Basov
Phys. Rev. B 90, 014503 – Published 8 July 2014

Abstract

We investigate infrared manifestations of the pseudogap in the prototypical cuprate and pnictide superconductors, YBa2Cu3Oy and BaFe2As2 (Ba122) systems. We find remarkable similarities between the spectroscopic features attributable to the pseudogap in these two classes of superconductors. The hallmarks of the pseudogap state in both systems include a weak absorption feature at about 500cm1 followed by a featureless continuum between 500 and 1500cm1 in the conductivity data and a significant suppression in the scattering rate below 700–900 cm1. The latter result allows us to identify the energy scale associated with the pseudogap ΔPG. We find that in the Ba122-based materials the superconductivity-induced changes of the infrared spectra occur in the frequency region below 100–200 cm1, which is much lower than the energy scale of the pseudogap. We performed theoretical analysis of the scattering rate data of the two compounds using the same model, which accounts for the effects of the pseudogap and electron-boson coupling. We find that the scattering rate suppression in Ba122-based compounds below ΔPG is solely due to the pseudogap formation, whereas the impact of the electron-boson coupling effects is limited to lower frequencies. The magnetic resonance modes used as inputs in our modeling are found to evolve with the development of the pseudogap, suggesting an intimate correlation between the pseudogap and magnetism.

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  • Received 27 January 2014
  • Revised 9 June 2014

DOI:https://doi.org/10.1103/PhysRevB.90.014503

©2014 American Physical Society

Authors & Affiliations

S. J. Moon1,2,*, Y. S. Lee1,3, A. A. Schafgans1, A. V. Chubukov4, S. Kasahara5, T. Shibauchi6, T. Terashima5, Y. Matsuda6, M. A. Tanatar7, R. Prozorov7, A. Thaler7, P. C. Canfield7, S. L. Bud'ko7, A. S. Sefat8, D. Mandrus8,9, K. Segawa10, Y. Ando10, and D. N. Basov1

  • 1Department of Physics, University of California, San Diego, La Jolla, California 92093, USA
  • 2Department of Physics, Hanyang University, Seoul 133-791, Republic of Korea
  • 3Department of Physics, Soongsil University, Seoul 156-743, Republic of Korea
  • 4Department of Physics, University of Wisconsin-Madison, 1150 Univ. Ave., Madison, Wisconsin 53706-1390, USA
  • 5Research Center for Low Temperature and Materials Science, Kyoto University, Kyoto 606-8502, Japan
  • 6Department of Physics, Kyoto University, Kyoto 606-8502, Japan
  • 7Ames Laboratory and Department of Physics and Astronomy, Iowa State University, Ames, Iowa 50011, USA
  • 8Materials Science and Technology Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
  • 9Department of Materials Science and Engineering, University of Tennessee, Knoxville, Tennessee 37996, USA
  • 10Institute of Scientific and Industrial Research, Osaka University, Ibaraki, Osaka 560-0047, Japan

  • *soonjmoon@hanyang.ac.kr

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Issue

Vol. 90, Iss. 1 — 1 July 2014

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