Spin-orbit transitions in α- and γCoV2O6

F. Wallington, A. M. Arevalo-Lopez, J. W. Taylor, J. R. Stewart, V. Garcia-Sakai, J. P. Attfield, and C. Stock
Phys. Rev. B 92, 125116 – Published 9 September 2015
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Abstract

γ-triclinic and α-monoclinic polymorphs of CoV2O6 are two of the few known transition-metal ion-based materials that display stepped 13 magnetization plateaus at low temperatures. Neutron diffraction [M. Markkula et al., Phys. Rev. B 86, 134401 (2012)], x-ray dichroism [N. Hollmann et al., Phys. Rev. B 89, 201101(R) (2014)], and dielectric measurements [J. Singh et al., J. Mater. Chem. 22, 6436 (2012)] have shown a coupling between orbital, magnetic, and structural orders in CoV2O6. We apply neutron inelastic scattering to investigate this coupling by measuring the spin-orbit transitions in both α and γ polymorphs. We find the spin exchange and anisotropy in monoclinic αCoV2O6 to be weak in comparison with the spin-orbit coupling λ and estimate an upper limit of |J/λ|0.05. However, the spin exchange is larger in the triclinic polymorph and we suggest the excitations are predominately two dimensional. The local compression of the octahedra surrounding the Co2+ ion results in a direct coupling between higher-energy orbital levels, the magnetic ground state, and elastic strain. CoV2O6 is therefore an example where the local distortion along with the spin-orbit coupling provides a means of intertwining structural and magnetic properties. We finish the paper by investigating the low-energy magnetic fluctuations within the ground-state doublet and report a magnetic excitation that is independent of the local crystalline electric field. We characterize the temperature and momentum dependence of these excitations and discuss possible connections to the magnetization plateaus.

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  • Received 1 May 2015
  • Revised 12 August 2015

DOI:https://doi.org/10.1103/PhysRevB.92.125116

©2015 American Physical Society

Authors & Affiliations

F. Wallington1, A. M. Arevalo-Lopez2,3, J. W. Taylor4, J. R. Stewart4, V. Garcia-Sakai4, J. P. Attfield2,3, and C. Stock1,2

  • 1School of Physics and Astronomy, University of Edinburgh, Edinburgh EH9 3FD, United Kingdom
  • 2Centre for Science at Extreme Conditions, University of Edinburgh, Edinburgh EH9 3FD, United Kingdom
  • 3School of Chemistry, University of Edinburgh, Edinburgh EH9 3FD, United Kingdom
  • 4ISIS Facility, Rutherford Appleton Laboratory, Chilton, Didcot OX11 0QX, United Kingdom

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Issue

Vol. 92, Iss. 12 — 15 September 2015

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