# On the origin of magnetic anisotropy in two dimensional CrI$_3$

**Authors:** J. L. Lado, J. Fern\'andez-Rossier

arXiv: 1704.03849 · 2018-03-28

## TL;DR

This paper investigates the origins of magnetic anisotropy in monolayer CrI$_3$, combining computational and theoretical models to identify key contributions that enable ferromagnetic order in two dimensions.

## Contribution

It identifies two main sources of magnetic anisotropy in CrI$_3$, clarifies their roles, and establishes an effective spin Hamiltonian for the system.

## Key findings

- Both super-exchange and single ion anisotropy favor off-plane magnetization.
- The XXZ Hamiltonian with small single ion anisotropy models the system accurately.
- Magnetic anisotropy-induced gap is crucial for magnetic order in 2D.

## Abstract

The observation of ferromagnetic order in a monolayer of CrI$_3$ has been recently reported, with a Curie temperature of 45 Kelvin and off-plane easy axis. Here we study the origin of magnetic anisotropy, a necessary ingredient to have magnetic order in two dimensions, combining two levels of modeling, density functional calculations and spin model Hamiltonians. We find two different contributions to the magnetic anisotropy of the material, both favoring off-plane magnetization and contributing to open a gap in the spin wave spectrum. First, ferromagnetic super-exchange across the $\simeq $ 90 degree Cr-I-Cr bonds, are anisotropic, due to the spin orbit interaction of the ligand I atoms. Second, a much smaller contribution that comes from the single ion anisotropy of the $S=3/2$ Cr atom. Our results permit to establish the XXZ Hamiltonian, with a very small single ion anisotropy, as the adequate spin model for this system. Using spin wave theory we estimate the Curie temperature and we highlight the essential role played by the gap that magnetic anisotropy induces on the magnon spectrum.

## Full text

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## Figures

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## References

61 references — full list in the complete paper: https://tomesphere.com/paper/1704.03849/full.md

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Source: https://tomesphere.com/paper/1704.03849