Abstract
The recent prediction that honeycomb lattices of Co2+ (3d7) ions could host dominant Kitaev interactions provides an exciting direction for exploration of new routes to stabilizing Kitaev's quantum spin liquid in real materials. Na3Co2SbO6 has been singled out as a potential material candidate provided that spin and orbital moments couple into a Jeff=12 ground state, and that the relative strength of trigonal crystal field and spin-orbit coupling acting on Co ions can be tailored. Using x-ray linear dichroism (XLD) and x-ray magnetic circular dichroism (XMCD) experiments, alongside configuration interaction calculations, we confirm the counterintuitive positive sign of the trigonal crystal field acting on Co2+ ions and test the validity of the Jeff=12 description of the electronic ground state. The results lend experimental support to recent theoretical predictions that a compression (elongation) of CoO6 octahedra along (perpendicular to) the trigonal axis would drive this cobaltate toward the Kitaev limit, assuming the Jeff=12 character of the electronic ground state is preserved.
| Original language | English |
|---|---|
| Article number | 214443 |
| Journal | Physical Review B |
| Volume | 107 |
| Issue number | 21 |
| DOIs | |
| State | Published - Jun 1 2023 |
Funding
Work at the Advanced Photon Source of Argonne National Laboratory was supported by the U.S. DOE, Office of Science, Office of Basic Energy Sciences, under Contract No. DE-AC02-06CH11357. Work in the Materials Science Division of Argonne National Laboratory (powder synthesis and characterization) was supported by the U.S. Department of Energy, Office of Science, Basic Energy Sciences, Materials Science and Engineering Division. We acknowledge Diamond Light Source for time on beamline I10. E.H.T.P. and R.J.H. were supported by National Science Foundation Grant No. DMR-2104881 and DOE-NNSA through the Chicago/DOE Alliance Center (CDAC) Cooperative Agreement No. DE-NA0003975. R.T. was supported by FAPESP Grant No. 2021/11170-0. J.-Q.Y. was supported by the U.S. Department of Energy, Office of Science, Basic Energy Sciences, Division of Materials Sciences and Engineering.
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