# Asymmetric splitting of an antiferromagnetic resonance via quartic   exchange interactions in multiferroic hexagonal HoMnO$_3$

**Authors:** N. J. Laurita, Yi Luo, Rongwei Hu, Meixia Wu, S. W. Cheong, O., Tchernyshyov, N. P. Armitage

arXiv: 1706.04141 · 2017-12-05

## TL;DR

This study uncovers asymmetric antiferromagnetic resonance splitting in HoMnO3 caused by quartic exchange interactions, revealed through THz spectroscopy and supported by theoretical modeling, highlighting complex Ho-Mn interactions.

## Contribution

It demonstrates the necessity of including quartic spin interactions in models to explain AFR asymmetry in low-symmetry multiferroic materials.

## Key findings

- Asymmetric AFR splitting observed in HoMnO3
- g-factor difference of approximately 50% between branches
- Quartic exchange interactions are essential for theoretical explanation

## Abstract

The symmetric splitting of two spin-wave branches in an antiferromagnetic resonance (AFR) experiment has been an essential measurement of antiferromagnets for over half a century. In this work, circularly polarized time-domain THz spectroscopy experiments performed on the low symmetry multiferroic h-HoMnO$_3$ reveal an AFR of the Mn sublattice to split asymmetrically in applied magnetic field, with an $\approx$ 50\% difference in $g$-factors between the high and low energy branches of this excitation. The temperature dependence of the $g$-factors, including a drastic renormalization at the Ho spin ordering temperature, reveals this asymmetry to unambiguously stem from Ho-Mn interactions. Theoretical calculations demonstrate the AFR asymmetry is not explained by conventional Ho-Mn exchange mechanisms alone and are only reproduced if quartic spin interactions are also included in the spin Hamiltonian. Our results provide a paradigm for the optical study of such novel interactions in hexagonal manganites and low symmetry antiferromagnets in general.

## Full text

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## Figures

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## References

90 references — full list in the complete paper: https://tomesphere.com/paper/1706.04141/full.md

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Source: https://tomesphere.com/paper/1706.04141