Abstract

A combined approach using first-principles calculations and spin dynamics simulations is applied to study $\mathrm{Ni}/{\mathrm{Ir}}_{n}/\mathrm{Pt}(111)$ ($n=0,1,2$) films. The lowest-energy states are predicted to be spin spirals but with a minute (of the order of a few $\ensuremath{\mu}\mathrm{eV}/\mathrm{atom}$) energy difference with skyrmionic states. The spontaneous low-temperature skyrmions, with $\ensuremath{\sim}15$ nm to $\ensuremath{\sim}35$ nm size, arise from a large Dzyaloshinskii-Moriya (DM) and Heisenberg exchange interactions ratio and, in particular, from a large in-plane DM vector component for nearest neighbors. The skyrmions become larger and more dispersed with the enhancement of the Ir buffer thickness. Also, with increasing $n$, the skyrmions' stability decreases when an external magnetic field is applied or the temperature is raised. For $n=0$ and $n=1$, we find that metastable skyrmioniums can occur, which are characterized by a slightly lower stability with respect to the external fields and larger critical currents, compared to skyrmions.

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