# Negative-vector-chirality 120$^\circ$ spin structure in the defect- and   distortion-free quantum kagome antiferromagnet YCu$_3$(OH)$_6$Cl$_3$

**Authors:** A. Zorko, M. Pregelj, M. Gomilsek, M. Klanjsek, O. Zaharko, W. Sun,, and J.-X. Mi

arXiv: 1907.07489 · 2019-10-17

## TL;DR

This study reveals a long-range 120-degree magnetic order with negative vector spin chirality in the defect-free quantum kagome antiferromagnet YCu$_3$(OH)$_6$Cl$_3$, highlighting the role of anisotropy and further-neighbor interactions.

## Contribution

It provides the first detailed magnetic structure of a defect- and distortion-free quantum kagome antiferromagnet, emphasizing the influence of Dzyaloshinskii-Moriya interactions and further-neighbor exchanges.

## Key findings

- Magnetic order with negative vector spin chirality observed
- Ordered moments are significantly reduced, indicating strong quantum fluctuations
- Magnetic order persists despite absence of typical perturbations

## Abstract

The magnetic ground state of the ideal quantum kagome antiferromagnet (QKA) has been a long-standing puzzle, mainly because perturbations to the nearest-neighbor isotropic Heisenberg Hamiltonian can lead to various fundamentally different ground states. Here we investigate a recently synthesized QKA representative YCu$_3$(OH)$_6$Cl$_3$, where perturbations commonly present in real materials, like lattice distortion and intersite ion mixing, are absent. Nevertheless, this compound enters a long-range magnetically ordered state below $T_N=15$ K. Our powder neutron diffraction experiment reveals that its magnetic structure corresponds to a coplanar $120^\circ$ state with negative vector spin chirality. The ordered magnetic moments are suppressed to $0.42(2)\mu_B$, which is consistent with the previously detected spin dynamics persisting to the lowest experimentally accessible temperatures. This indicates either a coexistence of magnetic order and disorder or the presence of strong quantum fluctuations in the ground state of YCu$_3$(OH)$_6$Cl$_3$. The origin of the magnetic order is sought in terms of Dzyaloshinskii-Moriya magnetic anisotropy and further-neighbor isotropic exchange interactions.

## Full text

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## Figures

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## References

53 references — full list in the complete paper: https://tomesphere.com/paper/1907.07489/full.md

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Source: https://tomesphere.com/paper/1907.07489