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Direct observation of oxygen polarization in Sr2IrO4 by O K-edge x-ray magnetic circular dichroism

R. Kadono1,*, M. Miyazaki2, M. Hiraishi3, H. Okabe4, A. Koda1,5, K. Amemiya5,6, and H. Nakao5,6

  • 1Muon Science Laboratory, Institute of Materials Structure Science, High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
  • 2Muroran Institute of Technology, Muroran, Hokkaido 050-8585, Japan
  • 3Graduate School of Science and Engineering, Ibaraki University, Bunkyo, Mito, Ibaraki 310-8512, Japan
  • 4Institute for Materials Research (IMR), Tohoku University, Katahira, Aoba-ku, Sendai 980-8577, Japan
  • 5Department of Materials Structure Science, Graduate University for Advanced Studies, Tsukuba, Ibaraki 305-0801, Japan
  • 6Photon Factory, Institute of Materials Structure Science, High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan

  • *ryosuke.kadono@kek.jp

Phys. Rev. B 107, L201122 – Published 31 May, 2023

DOI: https://doi.org/10.1103/PhysRevB.107.L201122

Abstract

X-ray absorption spectroscopy (XAS) and magnetic circular dichroism (XMCD) measurements at the oxygen (O) K edge were performed to investigate the magnetic polarization of ligand O atoms in the weak ferromagnetic (WFM) phase of the Ir perovskite compound Sr2IrO4. With the onset of the WFM phase below TN≃240 K, XMCD signals corresponding to XAS peaks respectively identified as originating from the magnetic moments of apical and planar oxygen (OA and OP) in the IrO6 octahedra were observed. The observation of magnetic moments at OA sites is consistent (except for the relative orientation) with that suggested by prior muon spin rotation (µSR) experiment in the noncollinear antiferromagnetic (NC-AFM) phase below TM≈100 K. Assuming that the OA magnetic moment observed by µSR is also responsible for the corresponding XMCD signal, the magnetic moment of OP is estimated to be consistent with the previous µSR result. Since the OA XMCD signal is mainly contributed by Ir 5dzx and yz orbitals which also hybridize with OP, it is inferred that the relatively large OP magnetic moment is induced by Ir 5dxy orbitals. Moreover, the inversion of OA moments relative to Ir moments between the two magnetic phases revealed by XMCD suggests the presence of competing magnetic interactions for OA, with which the ordering of OA moments in the NC-AFM phase may be suppressed to TM.

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