Abstract
Using relativistic first-principles calculations, we show that the chemical trend of the Dzyaloshinskii-Moriya interaction (DMI) in ultrathin films follows Hund’s first rule with a tendency similar to their magnetic moments in either the unsupported monolayers or interfaces. We demonstrate that, besides the spin-orbit coupling (SOC) effect in inversion asymmetric noncollinear magnetic systems, the driving force is the orbital occupations and their spin-flip mixing processes with the spin-orbit active states control directly the sign and magnitude of the DMI. The magnetic chirality changes are discussed in the light of the interplay between SOC, Hund’s first rule, and the crystal-field splitting of orbitals.
- Received 19 May 2016
DOI:https://doi.org/10.1103/PhysRevLett.117.247202
© 2016 American Physical Society