# Non-equilibrium spin density and spin-orbit torque in three dimensional   topological insulators - antiferromagnet heterostructure

**Authors:** Sumit Ghosh, Aurelien Manchon

arXiv: 1901.08314 · 2019-07-17

## TL;DR

This paper investigates non-equilibrium spin density and spin-orbit torque in topological insulator-antiferromagnet heterostructures, highlighting the preservation of Dirac cones and the robustness of staggered spin density against impurities.

## Contribution

It reveals the existence of a robust staggered spin density and analyzes the angular dependence of torques, incorporating both surface and bulk topological insulator contributions.

## Key findings

- Staggered spin density corresponds to damping-like torque.
- Spin-orbit torque exhibits angular dependence similar to Rashba systems.
- Robustness of spin density against scalar impurities in the surface energy regime.

## Abstract

We study the behavior of non-equilibrium spin density and spin-orbit torque in a topological insulator - antiferromagnet heterostructure. Unlike ferromagnetic heterostructures where Dirac cone is gapped due to time-reversal symmetry breaking, here the Dirac cone is preserved. We demonstrate the existence of a staggered spin density corresponding to a damping like torque, which is quite robust against the scalar impurity, when the transport energy is in the topological insulator surface energy regime. We show the contribution to the non-equilibrium spin density due to both surface and bulk topological insulator bands. Finally, we show that the torques in topological insulator-antiferromagnet heterostructure exhibit an angular dependence that is consistent with the standard spin-orbit torque obtained in Rashba system with some additional nonlinear effects arising from the interfacial coupling.

## Full text

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## Figures

13 figures with captions in the complete paper: https://tomesphere.com/paper/1901.08314/full.md

## References

46 references — full list in the complete paper: https://tomesphere.com/paper/1901.08314/full.md

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Source: https://tomesphere.com/paper/1901.08314