# High-pressure magnetization and NMR studies on $\alpha$-RuCl$_3$

**Authors:** Y. Cui, J. Zheng, K. Ran, Jinsheng Wen, Zhengxin Liu, B. Liu, Wenan, Guo, and Weiqiang Yu

arXiv: 1706.02697 · 2017-12-06

## TL;DR

This study investigates how high pressure affects the magnetic properties and phase behavior of $	ext{α-RuCl}_3$, revealing phase separation, suppression of magnetic order, and potential emergence of a disordered state.

## Contribution

It provides new insights into pressure-induced phase transitions and magnetic suppression in $	ext{α-RuCl}_3$, combining magnetization and NMR techniques up to 1.5 GPa.

## Key findings

- Magnetic ordering persists up to 0.45 GPa with phase separation at higher pressures.
- Magnetic volume fraction is fully suppressed above 1.05 GPa.
- A high-pressure phase with nearly absent static susceptibility emerges below 100 K.

## Abstract

We report high-pressure magnetization and $^{35}$Cl NMR studies on $\alpha$-RuCl$_3$ with pressure up to 1.5~GPa. At low pressures, the magnetic ordering is identified by both the magnetization data and the NMR data, where the $T_N$ shows a concave shape dependence with pressure. These data suggest stacking rearrangement along the $c$-axis. With increasing pressure, phase separation appears prominently at $P\ge$~0.45~GPa, and the magnetic volume fraction is completely suppressed at $P\ge$~1.05~GPa. Meanwhile, a phase-transition-like behavior emerges at high pressures in the remaining volume by a sharp drop of magnetization $M(T)$ upon cooling, with the transition temperature $T_x$ increased to ~250~K at 1~GPa. The $1/^{35}T_1$ is reduced by over three orders of magnitude when cooled below 100~K. This characterizes a high-pressure, low-temperature phase with nearly absent static susceptibility and low-energy spin fluctuations. The nature of the high-pressure ground state is discussed, where a magnetically disordered state is proposed as a candidate state.

## Full text

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## Figures

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## References

44 references — full list in the complete paper: https://tomesphere.com/paper/1706.02697/full.md

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Source: https://tomesphere.com/paper/1706.02697