Synchrotron x-ray scattering study of charge-density-wave order in HgBa2CuO4+δ

W. Tabis, B. Yu, I. Bialo, M. Bluschke, T. Kolodziej, A. Kozlowski, E. Blackburn, K. Sen, E. M. Forgan, M. v. Zimmermann, Y. Tang, E. Weschke, B. Vignolle, M. Hepting, H. Gretarsson, R. Sutarto, F. He, M. Le Tacon, N. Barišić, G. Yu, and M. Greven
Phys. Rev. B 96, 134510 – Published 10 October 2017

Abstract

We present a detailed synchrotron x-ray scattering study of the charge-density-wave (CDW) order in simple tetragonal HgBa2CuO4+δ (Hg1201). Resonant soft x-ray scattering measurements reveal that short-range order appears at a temperature that is distinctly lower than the pseudogap temperature and in excellent agreement with a prior transient reflectivity result. Despite considerable structural differences between Hg1201 and YBa2Cu3O6+δ, the CDW correlations exhibit similar doping dependencies, and we demonstrate a universal relationship between the CDW wave vector and the size of the reconstructed Fermi pocket observed in quantum oscillation experiments. The CDW correlations in Hg1201 vanish already below optimal doping, once the correlation length is comparable to the CDW modulation period, and they appear to be limited by the disorder potential from unit cells hosting two interstitial oxygen atoms. A complementary hard x-ray diffraction measurement, performed on an underdoped Hg1201 sample in magnetic fields along the crystallographic c axis of up to 16 T, provides information on the form factor of the CDW order. As expected from the single-CuO2-layer structure of Hg1201, the CDW correlations vanish at half-integer values of L and appear to be peaked at integer L. We conclude that the atomic displacements associated with the short-range CDW order are mainly planar, within the CuO2 layers.

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  • Received 2 February 2017
  • Revised 15 September 2017

DOI:https://doi.org/10.1103/PhysRevB.96.134510

©2017 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

W. Tabis1,2,3,*, B. Yu1, I. Bialo2, M. Bluschke4,5, T. Kolodziej2,6, A. Kozlowski2, E. Blackburn7, K. Sen8, E. M. Forgan7, M. v. Zimmermann9, Y. Tang1, E. Weschke4, B. Vignolle3, M. Hepting5, H. Gretarsson5, R. Sutarto10, F. He10, M. Le Tacon8, N. Barišić1,11, G. Yu1, and M. Greven1,†

  • 1School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
  • 2AGH University of Science and Technology, Faculty of Physics and Applied Computer Science, 30-059 Krakow, Poland
  • 3Laboratoire National des Champs Magnetiques Intenses (CNRS, INSA, UJF, UPS), 31400 Toulouse, France
  • 4Helmholtz-Zentrum Berlin fur Materialien und Energie, D-12489 Berlin, Germany
  • 5Max Planck Institute for Solid State Research, D-70569 Stuttgart, Germany
  • 6Advanced Photon Source, Argonne National Laboratory, Lemont, Illinois 60439, USA
  • 7School of Physics and Astronomy, University of Birmingham, Birmingham B15 2TT, United Kingdom
  • 8Institut für Festkörperphysik, Karlsruher Institut für Technologie, 76021 Karlsruhe, Germany
  • 9Deutsches Elektronen-Synchrotron DESY, 22603 Hamburg, Germany
  • 10Canadian Light Source, Saskatoon, Saskatchewan, Canada S7N 2V3
  • 11Institute of Solid State Physics, TU Wien, 1040 Vienna, Austria

  • *wojciech.tabis@lncmi.cnrs.fr
  • greven@umn.edu

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Vol. 96, Iss. 13 — 1 October 2017

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