arXiv · 2405.13215
Role of stacking defects on the magnetic behavior of CrCl$_3$
Abstract
In the study of van der Waals-layered magnetic materials, the properties of CrCl$_3$ continue to attract attention. This compound is reported to undergo antiferromagnetic (AFM) ordering below $\sim$14 K, with a ferromagneticlike region proposed to exist between 14 and 17 K. Ideally, the crystal structure is rhombohedral (R) below $\sim$235 K, separated from a higher-temperature monoclinic (M) phase by a layer-sliding structural phase transition. However, the structural transition is often inhibited even in bulk single crystals, allowing M-type layer stacking, reported to have a tenfold greater interlayer magnetic coupling than R-type stacking, to be present at low temperature. To clarify the effect of stacking defects on CrCl$_3$, we report magnetization measurements on samples of varying crystalline quality. At low applied magnetic field, some crystals predominantly show the $T_N=14$ K peak, but other crystals show hysteretic behavior and a magnetization enhancement at a slightly higher temperature ($14 < T \lesssim 17$ K.) Samples with anomalous behavior exhibit a transition around $\sim$2 T in isothermal magnetization-field data, providing evidence that M-type stacking defects are the source of these anomalies. Ground powder samples are especially likely to show strongly anomalous behavior. We suggest that the anomalous behavior arises from few-layer magnetic domains that form just above $T_N$ in an environment of mixed interlayer magnetic coupling strength. We argue that the influence of M-type stacking boundaries on sublattice magnetization is already observable in reported neutron scattering data, and may be responsible for a certain feature in reported specific heat data.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
John A. Schneeloch, Adam A. Aczel, Feng Ye, Despina Louca. 2024-05-21. Role of stacking defects on the magnetic behavior of CrCl$_3$. https://doi.org/10.1103/physrevb.110.144439
Cite the original work for its findings. Save a collection to share your selection of sources.