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Connection between magnetic interactions and the spin-wave gap of the insulating phase of NaOsO3
Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden.
Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden.
Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden.
Örebro University, School of Science and Technology.ORCID iD: 0000-0001-8007-5392
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2021 (English)In: Physical Review B, ISSN 2469-9950, E-ISSN 2469-9969, Vol. 104, no 13, article id 134433Article in journal (Refereed) Published
Abstract [en]

The scenario of a metal-insulator transition driven by the onset of antiferromagnetic order in NaOsO3 calls for a trustworthy derivation of the underlying effective spin Hamiltonian. To determine the latter we rely on ab initio electronic-structure calculations, linear spin-wave theory, and comparison to experimental data of the corresponding magnon spectrum. We arrive this way to Heisenberg couplings that are less than or similar to 45 to less than or similar to 63% smaller than values presently proposed in the literature and Dzyaloshinskii-Moriya interactions in the region of 15% of the Heisenberg exchange J. These couplings together with the symmetric anisotropic exchange interaction and single-ion magnetocrystalline anisotropy successfully reproduce the magnon dispersion obtained by resonant inelastic x-ray scattering measurements. In particular, the spin-wave gap fully agrees with the measured one. We find that the spin-wave gap is defined from a subtle interplay between the single-ion anisotropy, the Dzyaloshinskii-Moriya exchange, and the symmetric anisotropic exchange interactions. The results reported here underpin the local-moment description of NaOsO3, when it comes to analyzing the magnetic excitation spectra. Interestingly, this comes about from a microscopic theory that describes the electron system as Bloch states, adjusted to a mean-field solution to Hubbard-like interactions.

Place, publisher, year, edition, pages
American Physical Society , 2021. Vol. 104, no 13, article id 134433
National Category
Condensed Matter Physics
Identifiers
URN: urn:nbn:se:oru:diva-97359DOI: 10.1103/PhysRevB.104.134433ISI: 000746135800001Scopus ID: 2-s2.0-85118935797OAI: oai:DiVA.org:oru-97359DiVA, id: diva2:1636247
Funder
Knut and Alice Wallenberg Foundation, 2018.0060Swedish Research Council, 2015-04608 2016-05980 2019-05304 20190-3666 2017-03832 2019-03569 2016-07213EU, European Research Council, 854843
Note

Funding agencies:

eSSENCE, Swedish National Infrastructure for Computing (SNIC)

High Performance Computing Center North (HPC2N), Umeå

Available from: 2022-02-09 Created: 2022-02-09 Last updated: 2022-02-15Bibliographically approved

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Thonig, DannyEriksson, Olle

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