Semiclassical Routes to the $α$-RuCl$_3$ Scattering Continuum via Model Meta$-$Analysis
Chaebin Kim, Martin Mourigal
TL;DR
This study examines the origin of a broad, Γ-point-centered spin continuum in the proximate Kitaev magnet $\alpha$-RuCl$_3$ by combining semi-classical stochastic Landau-Lifshitz dynamics with quantum-corrections to compute the temperature evolution of the dynamical spin structure factor across correlated and conventional paramagnetic regimes. Through a meta-analysis of 38 proposed exchange-parameter sets and Bayesian optimization, the authors identify parameter families that reproduce the observed continuum, including a best-fit set that features a dominant off-diagonal $\Gamma'$ term, and demonstrate that spectral features collapse when temperatures are scaled by the Curie-Weiss scale $\bar{\theta}_{\mathrm{CW}}$, indicating the high-$T$ dynamics are governed primarily by correlated paramagnetism rather than Kitaev fractionalization. Complementary 24-site exact diagonalization clarifies finite-size effects and the proximity to zigzag/incommensurate order, yielding distinct low-temperature spectra that help discriminate between competing parameterizations. The resulting data-driven, reproducible framework enables inference of effective spin models in magnets with broad continua and offers a path to applying this approach to other candidate Kitaev materials beyond $\alpha$-RuCl$_3$.
Abstract
$α$-RuCl$_3$ is a leading material for proximate Kitaev magnetism. We address the origin of the broad, $Γ$-point centered excitation continuum observed by inelastic neutron scattering at elevated temperatures in this compound. Using stochastic Landau-Lifshitz dynamics augmented with quantum-equivalent corrections, we reproduce the temperature-dependent dynamical spin structure factor across both the correlated and conventional paramagnetic regimes. A meta-analysis of 38 published exchange parameter sets identifies those most consistent with the full temperature evolution. A Bayesian optimization procedure is used to derive parameters that capture the low-energy star-like momentum dependence and the overall bandwidth of the continuum. Rescaling temperatures by the Curie--Weiss scale produces a collapse of spectral measures, demonstrating that the high-$T$ dynamics are governed by correlated paramagnetism below $θ_{\mathrm{CW}}$ rather than by the Kitaev crossover to fractionalized excitations. Complementary 24-site exact diagonalization clarifies finite-size systematics at low temperature and the proximity to zigzag/incommensurate ordering. Beyond $α$-RuCl$_3$, our simulation pipeline provides a reproducible, data-driven framework to infer effective spin models in magnets that exhibit broad continua.
