Intertwined magnetic, structural, and electronic transitions in V2O3

Benjamin A. Frandsen, Yoav Kalcheim, Ilya Valmianski, Alexander S. McLeod, Z. Guguchia, Sky C. Cheung, Alannah M. Hallas, Murray N. Wilson, Yipeng Cai, Graeme M. Luke, Z. Salman, A. Suter, T. Prokscha, Taito Murakami, Hiroshi Kageyama, D. N. Basov, Ivan K. Schuller, and Yasutomo J. Uemura
Phys. Rev. B 100, 235136 – Published 23 December 2019
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Abstract

We present a coordinated study of the paramagnetic-to-antiferromagnetic, rhombohedral-to-monoclinic, and metal-to-insulator transitions in thin-film specimens of the classic Mott insulator V2O3 using low-energy muon spin relaxation, x-ray diffraction, and nanoscale-resolved near-field infrared spectroscopic techniques. The measurements provide a detailed characterization of the thermal evolution of the magnetic, structural, and electronic phase transitions occurring in a wide temperature range, including quantitative measurements of the high- and low-temperature phase fractions for each transition. The results reveal a stable coexistence of the high- and low-temperature phases over a broad temperature range throughout the transition. Careful comparison of temperature dependence of the different measurements, calibrated by the resistance of the sample, demonstrates that the electronic, magnetic, and structural degrees of freedom remain tightly coupled to each other during the transition process. We also find evidence for antiferromagnetic fluctuations in the vicinity of the phase transition, highlighting the important role of the magnetic degree of freedom in the metal-insulator transition.

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  • Received 15 October 2019
  • Revised 3 December 2019

DOI:https://doi.org/10.1103/PhysRevB.100.235136

©2019 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

Benjamin A. Frandsen1,2,*, Yoav Kalcheim3, Ilya Valmianski3, Alexander S. McLeod3, Z. Guguchia1,4, Sky C. Cheung1, Alannah M. Hallas5, Murray N. Wilson5, Yipeng Cai5, Graeme M. Luke5,6, Z. Salman4, A. Suter4, T. Prokscha4, Taito Murakami7, Hiroshi Kageyama7, D. N. Basov3,1, Ivan K. Schuller3, and Yasutomo J. Uemura1,†

  • 1Department of Physics, Columbia University, New York, New York 10027, USA
  • 2Department of Physics and Astronomy, Brigham Young University, Provo, Utah 84602, USA
  • 3Department of Physics, University of California San Diego, 9500 Gilman Drive, La Jolla, California 92093, USA
  • 4Laboratory for Muon Spin Spectroscopy, Paul Scherrer Institut, CH-5232 Villigen PSI, Switzerland
  • 5Department of Physics and Astronomy, McMaster University, Hamilton, Ontario, Canada L8S 4M1
  • 6Canadian Institute for Advanced Research, Toronto, Ontario, Canada L8S 4M1
  • 7Department of Energy and Hydrocarbon Chemistry, Graduate School of Engineering, Kyoto University, Nishikyo, Kyoto 615-8510, Japan

  • *benfrandsen@byu.edu
  • yu2@columbia.edu

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Issue

Vol. 100, Iss. 23 — 15 December 2019

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