Electronic structure and direct observation of ferrimagnetism in multiferroic hexagonal YbFeO3

Shi Cao, Kishan Sinha, Xin Zhang, Xiaozhe Zhang, Xiao Wang, Yuewei Yin, Alpha T. N'Diaye, Jian Wang, David J. Keavney, Tula R. Paudel, Yaohua Liu, Xuemei Cheng, Evgeny Y. Tsymbal, Peter A. Dowben, and Xiaoshan Xu
Phys. Rev. B 95, 224428 – Published 26 June 2017

Abstract

The magnetic interactions between rare-earth and Fe ions in hexagonal rare-earth ferrites (hRFeO3), may amplify the weak ferromagnetic moment on Fe, making these materials more appealing as multiferroics. To elucidate the interaction strength between the rare-earth and Fe ions as well as the magnetic moment of the rare-earth ions, element-specific magnetic characterization is needed. Using x-ray magnetic circular dichroism, we have studied the ferrimagnetism in hYbFeO3 by measuring the magnetization of Fe and Yb separately. The results directly show antialignment of magnetization of Yb and Fe ions in hYbFeO3 at low temperature, with an exchange field on Yb of about 17 kOe. The magnetic moment of Yb is about 1.6μB at low temperature, significantly reduced compared with the 4.5μB moment of a free Yb3+. In addition, the saturation magnetization of Fe in hYbFeO3 has a sizable enhancement compared with that in hLuFeO3. These findings directly demonstrate that ferrimagnetic order exists in hYbFeO3; they also account for the enhancement of magnetization and the reduction of coercivity in hYbFeO3 compared with those in hLuFeO3 at low temperature, suggesting an important role for the rare-earth ions in tuning the multiferroic properties of hRFeO3.

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  • Received 22 March 2017
  • Revised 21 May 2017

DOI:https://doi.org/10.1103/PhysRevB.95.224428

©2017 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

Shi Cao1, Kishan Sinha1, Xin Zhang1, Xiaozhe Zhang2,1, Xiao Wang3, Yuewei Yin1, Alpha T. N'Diaye4, Jian Wang5, David J. Keavney6, Tula R. Paudel1, Yaohua Liu7, Xuemei Cheng3, Evgeny Y. Tsymbal1,8, Peter A. Dowben1,8, and Xiaoshan Xu1,8,*

  • 1Department of Physics and Astronomy, University of Nebraska, Lincoln, Nebraska 68588, USA
  • 2Department of Physics, Xi'an Jiaotong University, Xi'an 710049, People's Republic of China
  • 3Department of Physics, Bryn Mawr College, Bryn Mawr, Pennsylvania 19010, USA
  • 4Advanced Light Source, Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
  • 5Canadian Light Source, Saskatoon, SK, S7N 2V3 Canada
  • 6Advanced Photon Source, Argonne National Laboratory, Argonne, Illinois 60439, USA
  • 7Quantum Condensed Matter Division, Oak Ridge National Lab, Oak Ridge, Tennessee 37831, USA
  • 8Nebraska Center for Materials and Nanoscience, University of Nebraska, Lincoln, Nebraska 68588, USA

  • *Corresponding author: xiaoshan.xu@unl.edu

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Vol. 95, Iss. 22 — 1 June 2017

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