Persistent insulating state at megabar pressures in strongly spin-orbit coupled Sr2IrO4

Chunhua Chen, Yonghui Zhou, Xuliang Chen, Tao Han, Chao An, Ying Zhou, Yifang Yuan, Bowen Zhang, Shuyang Wang, Ranran Zhang, Lili Zhang, Changjin Zhang, Zhaorong Yang, Lance E. DeLong, and Gang Cao
Phys. Rev. B 101, 144102 – Published 15 April 2020
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Abstract

It is commonly anticipated that an insulating state will collapse in favor of an emergent metallic state at high pressures: The average electron density must increase with pressure, while the electronic bandwidth is expected to broaden and fill the insulating energy band gap. Here we report an unusually stable insulating state that persists up to at least 185 GPa in Sr2IrO4, the archetypical spin-orbit-driven Jeff=1/2 insulator. This study shows that the electrical resistance R of single-crystal Sr2IrO4 initially decreases with applied pressure P, reaches a minimum in the range 32–38 GPa, then abruptly rises to recover the insulating state with increasing P up to 185 GPa. However, evidence of a saturation of R below 80 K for P124GPa GPa raises the possibility of a low-temperature exotic state. Our synchrotron x-ray diffraction and Raman scattering data show the emergence of the rapid increase in R is accompanied by a structural phase transition from the native tetragonal I41/acd phase to an orthorhombic Pbca phase (with much reduced symmetry) at 40.6 GPa. The clear correspondence of the onset pressures of these two anomalies is key to understanding the stability of the insulating state at megabar pressures: Pressure-induced, structural distortions prevent the expected onset of metallization, despite the sizable volume compression attained at the highest pressure accessed in this study.

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  • Received 29 January 2020
  • Revised 6 March 2020
  • Accepted 20 March 2020

DOI:https://doi.org/10.1103/PhysRevB.101.144102

©2020 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

Chunhua Chen1,2, Yonghui Zhou1,*, Xuliang Chen1, Tao Han3, Chao An3, Ying Zhou3, Yifang Yuan1,2, Bowen Zhang1,2, Shuyang Wang1,2, Ranran Zhang1, Lili Zhang4, Changjin Zhang1,3,5, Zhaorong Yang1,3,5,†, Lance E. DeLong6, and Gang Cao7,‡

  • 1Anhui Province Key Laboratory of Condensed Matter Physics at Extreme Conditions, High Magnetic Field Laboratory, Chinese Academy of Sciences, Hefei 230031, China
  • 2Science Island Branch of Graduate School, University of Science and Technology of China, Hefei 230026, China
  • 3Institutes of Physical Science and Information Technology, Anhui University, Hefei 230601, China
  • 4Shanghai Synchrotron Radiation Facility, Shanghai Advanced Research Institute, Chinese Academy of Sciences, Shanghai 201204, China
  • 5Collaborative Innovation Center of Advanced Microstructures, Nanjing University, Nanjing 210093, China
  • 6Department of Physics and Astronomy, University of Kentucky, Lexington, Kentucky 40506, USA
  • 7Department of Physics, University of Colorado at Boulder, Boulder, Colorado 80309, USA

  • *Corresponding author: yhzhou@hmfl.ac.cn
  • Corresponding author: zryang@issp.ac.cn
  • Corresponding author: gang.cao@colorado.edu

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Issue

Vol. 101, Iss. 14 — 1 April 2020

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