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Main Author: Barton-Singer, Bruno
Format: Preprint
Published: 2024
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Online Access:https://arxiv.org/abs/2401.04569
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author Barton-Singer, Bruno
author_facet Barton-Singer, Bruno
contents Two recently developed methods of modelling chiral magnetic soliton elliptical instability are applied in two novel scenarios, the tilted ferromagnetic phase of chiral magnets dominated by easy-plane anisotropy and the general case of the chiral magnet with tilted applied field and arbitrary uniaxial anisotropy. In the former case, the analytical predictions are found to exactly match previous numerical results. In the latter case, instability of isolated chiral skyrmions has not yet been studied, although the predictions correspond interestingly to previous numerical investigation of the phase diagram.
format Preprint
id arxiv_https___arxiv_org_abs_2401_04569
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Modelling the elliptical instability of magnetic skyrmions
Barton-Singer, Bruno
Mesoscale and Nanoscale Physics
High Energy Physics - Theory
Mathematical Physics
Two recently developed methods of modelling chiral magnetic soliton elliptical instability are applied in two novel scenarios, the tilted ferromagnetic phase of chiral magnets dominated by easy-plane anisotropy and the general case of the chiral magnet with tilted applied field and arbitrary uniaxial anisotropy. In the former case, the analytical predictions are found to exactly match previous numerical results. In the latter case, instability of isolated chiral skyrmions has not yet been studied, although the predictions correspond interestingly to previous numerical investigation of the phase diagram.
title Modelling the elliptical instability of magnetic skyrmions
topic Mesoscale and Nanoscale Physics
High Energy Physics - Theory
Mathematical Physics
url https://arxiv.org/abs/2401.04569