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Magnetic structure and excitation spectrum of the hyperhoneycomb Kitaev magnet β-Li2IrO3

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posted on 2018-07-03, 10:16 authored by Samuel Ducatman, Ioannis RousochatzakisIoannis Rousochatzakis, Natalia B. Perkins
© 2018 American Physical Society. We present a theoretical study of the static and dynamical properties of the three-dimensional, hyperhoneycomb Kitaev magnet β-Li2IrO3. We argue that the observed incommensurate order can be understood in terms of a long-wavelength twisting of a nearby commensurate period-3 state, with the same key qualitatively features. The period-3 state shows very different structure when either the Kitaev interaction K or the off-diagonal exchange anisotropy Γ is dominant. A comparison of the associated static spin structure factors with reported scattering experiments in zero and finite fields gives strong evidence that β-Li2IrO3 lies in the regime of dominant Kitaev coupling, and that the Heisenberg exchange J is much weaker than both K and Γ. Our predictions for the magnon excitation spectra, the dynamical spin structure factors, and their polarization dependence provide additional distinctive fingerprints that can be checked experimentally.

History

School

  • Science

Department

  • Physics

Published in

Physical Review B

Volume

97

Issue

12

Citation

DUCATMAN, S., ROUSOCHATZAKIS, I. and PERKINS, N.B., 2018. Magnetic structure and excitation spectrum of the hyperhoneycomb Kitaev magnet β-Li2IrO3. Physical Review B, 97: 125125.

Publisher

© American Physical Society

Version

  • AM (Accepted Manuscript)

Publisher statement

This work is made available according to the conditions of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0) licence. Full details of this licence are available at: https://creativecommons.org/licenses/by-nc-nd/4.0/

Acceptance date

2018-02-21

Publication date

2018-03-16

Notes

This paper was accepted for publication in the journal Physical Review B and the definitive published version is available at https://doi.org/10.1103/PhysRevB.97.125125

ISSN

2469-9950

eISSN

2469-9969

Language

  • en

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