# Crystalline Electric Field Randomness in the Triangular Lattice   Spin-Liquid YbMgGaO$_4$

**Authors:** Yuesheng Li, Devashibhai Adroja, Robert I. Bewley, David, Voneshen, Alexander A. Tsirlin, Philipp Gegenwart, Qingming Zhang

arXiv: 1702.01981 · 2017-03-13

## TL;DR

This study investigates the crystalline electric field levels in the spin-liquid candidate YbMgGaO$_4$ using inelastic neutron scattering, revealing broadening effects due to site disorder that influence magnetic excitations.

## Contribution

It demonstrates that CEF level broadening in YbMgGaO$_4$ arises from Mg/Ga site mixing, affecting magnetic properties and excitation spectra.

## Key findings

- CEF excitations at 39, 61, and 97 meV with broadening
- Site disorder causes distribution of Yb--O distances and CEF parameters
- Broadening explains low-energy excitation features in the polarized phase

## Abstract

We apply moderate-high-energy inelastic neutron scattering (INS) measurements to investigate Yb$^{3+}$ crystalline electric field (CEF) levels in the triangular spin-liquid candidate YbMgGaO$_4$. Three CEF excitations from the ground-state Kramers doublet are centered at the energies $\hbar \omega$ = 39, 61, and 97\,meV in agreement with the effective \mbox{spin-1/2} $g$-factors and experimental heat capacity, but reveal sizable broadening. We argue that this broadening originates from the site mixing between Mg$^{2+}$ and Ga$^{3+}$ giving rise to a distribution of Yb--O distances and orientations and, thus, of CEF parameters that account for the peculiar energy profile of the CEF excitations. The CEF randomness gives rise to a distribution of the effective spin-1/2 $g$-factors and explains the unprecedented broadening of low-energy magnetic excitations in the fully polarized ferromagnetic phase of YbMgGaO$_4$, although a distribution of magnetic couplings due to the Mg/Ga disorder may be important as well.

## Full text

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## Figures

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## References

66 references — full list in the complete paper: https://tomesphere.com/paper/1702.01981/full.md

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Source: https://tomesphere.com/paper/1702.01981