# Thermal Creation of Skyrmions in Ferromagnetic Films with Perpendicular   Anisotropy and Dzyaloshinskii-Moriya Interaction

**Authors:** Dmitry A. Garanin, Eugene M. Chudnovsky, Senfu Zhang, and Xixiang, Zhang

arXiv: 1906.05952 · 2025-02-17

## TL;DR

This study uses Monte Carlo simulations to demonstrate how thermal fluctuations facilitate the formation and stabilization of skyrmion lattices in ferromagnetic films with specific magnetic properties, aligning with recent experimental findings.

## Contribution

It provides a theoretical and computational analysis of thermally induced skyrmion creation, revealing conditions for stable skyrmion lattices in ferromagnetic films with Dzyaloshinskii-Moriya interaction.

## Key findings

- Thermal fluctuations promote skyrmion formation at elevated temperatures.
- Skyrmion lattices can be stabilized by cooling after formation.
- Skyrmion lattices have lower energy than labyrinth domains in certain fields.

## Abstract

We study theoretically, via Monte Carlo simulations on lattices containing up to 1000 x 1000 spins, thermal creation of skyrmion lattices in a 2D ferromagnetic film with perpendicular magnetic anisotropy and Dzyaloshinskii-Moriya interaction. At zero temperature, skyrmions only appear in the magnetization process in the presence of static disorder. Thermal fluctuations violate conservation of the topological charge and reduce the effective magnetic anisotropy that tends to suppress skyrmions. In accordance with recent experiments, we find that elevated temperatures assist the formation of skyrmion structures. Once such a structure is formed, it can be frozen into a regular skyrmion lattice by reducing the temperature. We investigate topological properties of skyrmion structures and find the average skyrmion size. Energies of domain and skyrmion states are computed. It is shown that skyrmion lattices have lower energy than labyrinth domains within a narrow field range.

## Full text

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## Figures

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## References

69 references — full list in the complete paper: https://tomesphere.com/paper/1906.05952/full.md

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Source: https://tomesphere.com/paper/1906.05952