# Perpendicular magnetic anisotropy at the Fe/MgAl$_2$O$_4$ interface:   Comparative first-principles study with Fe/MgO

**Authors:** Keisuke Masuda, Yoshio Miura

arXiv: 1803.10428 · 2018-12-31

## TL;DR

This study uses first-principles calculations to compare interfacial magnetic anisotropy in Fe/MgAl$_2$O$_4$ and Fe/MgO, revealing potential for enhanced perpendicular magnetic anisotropy with interface engineering.

## Contribution

It provides a detailed theoretical comparison of interfacial magnetic anisotropy between Fe/MgAl$_2$O$_4$ and Fe/MgO, and suggests methods to enhance PMA.

## Key findings

- Fe/MgAl$_2$O$_4$ exhibits interfacial PMA with $K_i \\approx 1.2$ mJ/m$^2$
- Difference in $K_i$ attributed to spin-flip scattering contributions
- Insertion of tungsten layers can increase $K_i$ to over 3 mJ/m$^2$

## Abstract

We present a theoretical study on interfacial magnetocrystalline anisotropy for Fe/MgAl$_2$O$_4$. This system has a very small lattice mismatch at the interface and therefore is suitable for realizing a fully coherent ferromagnet/oxide interface for magnetic tunnel junctions. On the basis of density functional theory, we calculate the interfacial anisotropy constant $K_{\rm i}$ and show that this system has interfacial perpendicular magnetic anisotropy (PMA) with $K_{\rm i} \approx 1.2\,{\rm mJ/m^2}$, which is a little bit smaller than that of Fe/MgO ($K_{\rm i} \approx$ 1.5--1.7$\,{\rm mJ/m^2}$). Second-order perturbation analysis with respect to the spin-orbit interaction clarifies that the difference in $K_{\rm i}$ between Fe/MgAl$_2$O$_4$ and Fe/MgO originates from the difference in contributions from spin-flip scattering terms at the interface. We propose that the insertion of tungsten layers into the interface of Fe/MgAl$_2$O$_4$ is a promising way to obtain huge interfacial PMA with $K_{\rm i} \gtrsim 3\,{\rm mJ/m^2}$.

## Full text

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## Figures

10 figures with captions in the complete paper: https://tomesphere.com/paper/1803.10428/full.md

## References

56 references — full list in the complete paper: https://tomesphere.com/paper/1803.10428/full.md

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Source: https://tomesphere.com/paper/1803.10428