# Spin-order dependent anomalous Hall effect and magneto-optical effect in   noncollinear antiferromagnets Mn$_{3}X$N ($X$ = Ga, Zn, Ag, and Ni)

**Authors:** Xiaodong Zhou, Jan-Philipp Hanke, Wanxiang Feng, Fei Li, Guang-Yu Guo,, Yugui Yao, Stefan Bl\"ugel, and Yuriy Mokrousov

arXiv: 1903.11038 · 2019-03-27

## TL;DR

This paper investigates how different spin orders in noncollinear antiferromagnets Mn$_{3}X$N influence their anomalous Hall and magneto-optical effects using first-principles calculations, revealing large effects and symmetry-dependent behaviors.

## Contribution

It provides a systematic first-principles analysis of spin-order dependent AHE and MOE in Mn$_{3}X$N, highlighting the role of symmetry and band structure in these phenomena.

## Key findings

- Large intrinsic anomalous Hall conductivity, e.g., 359 S/cm in Mn$_{3}$AgN.
- Symmetry determines tensor components of AHE for different spin chiralities.
- Spin order significantly affects magneto-optical anisotropy and optical isotropy.

## Abstract

Noncollinear antiferromagnets (AFMs) have recently attracted a lot of attention owing to the potential emergence of exotic spin orders on geometrically frustrated lattices, which can be characterized by corresponding spin chiralities. By performing first-principles density functional calculations together with group-theory analysis and tight-binding modelling, here we systematically study the spin-order dependent anomalous Hall effect (AHE) and magneto-optical effect (MOE) in representative noncollinear AFMs Mn$_{3}X$N ($X$ = Ga, Zn, Ag, and Ni). The symmetry-related tensor shape of the intrinsic anomalous Hall conductivity (IAHC) for different spin orders is determined by analyzing the relevant magnetic point groups. We show that while only the ${xy}$ component of the IAHC tensor is nonzero for right-handed spin chirality, all other elements, $\sigma_{xy}$, $\sigma_{yz}$, and $\sigma_{zx}$, are nonvanishing for a state with left-handed spin chirality owing to lowering of the symmetry. Our tight-binding arguments reveal that the magnitude of IAHC relies on the details of the band structure and that $\sigma_{xy}$ is periodically modulated as the spin rotates in-plane. The IAHC obtained from first principles is found to be rather large, e.g., it amounts to 359 S/cm in Mn$_{3}$AgN. By extending our analysis to finite frequencies, we calculate the optical isotropy [$\sigma_{xx}(\omega)\approx\sigma_{yy}(\omega)\approx\sigma_{zz}(\omega)$] and the magneto-optical anisotropy [$\sigma_{xy}(\omega)\neq\sigma_{yz}(\omega)\neq\sigma_{zx}(\omega)$] of Mn$_{3}X$N. We argue that the spin-order dependent AHE and MOE are indispensable in detecting complex spin structures in noncollinear AFMs.

## Full text

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## Figures

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## References

76 references — full list in the complete paper: https://tomesphere.com/paper/1903.11038/full.md

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Source: https://tomesphere.com/paper/1903.11038