Non-Kitaev vs. Kitaev Honeycomb Cobaltates
arXiv:2211.03737 · doi:10.1103/PhysRevB.107.054420
Abstract
Recently, honeycomb cobaltates with 3 were proposed to display Kitaev physics despite weak spin-orbit coupling. However, other theoretical and experimental works found leading XXZ Heisenberg and negligible Kitaev interactions in BaCo(AsO) (BCAO), which calls for a further study to clarify the origin of the discrepancies. Here we derive the analytical expressions of the spin model using strong-coupling perturbation theory. With tight binding parameters obtained by {\it ab-initio} calculations for idealized honeycomb BCAO, we find that the largest intraorbital exchange path, which was assumed to be small in the earlier theory proposal, leads to a ferromagnetic (FM) Heisenberg interaction. This becomes the dominant interaction, as other and contributions almost cancel each other. Exactly the same assumed-to-be-small channel also generates an antiferromagnetic Kitaev interaction, which then cancels a FM Kitaev interaction from paths, resulting in a small Kitaev interaction. Under the trigonal distortion, the preeminent isotropic Heisenberg becomes an anisotropic XXZ model as expected, which is the case for BCAO. However, in NaCoSbO the intraorbital hopping is smaller and comparable to the hopping, leading to a delicate competition between enhanced Kitaev and reduced Heisenberg interactions.
10 pages, 4 figures
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