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Chiral magnetic skyrmions across length scales

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Stavros Komineas, Christof Melcher, Stephanos Venakides

Mesoscale and Nanoscale Physics · Submitted 9 Jun 2022

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim Using fitting techniques, we modify these formulae so that their validity extends to almost the entire range of skyrmion radii.

how it is stated · asserted 1.00 read the record →

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arXiv ID2206.04761 (version 1)
Pith IDP63FNVGW, Pith's permanent record of this paper and its review
CitationChristof Melcher, Stavros Komineas, Stephanos Venakides. "Chiral magnetic skyrmions across length scales." arXiv:2206.04761 (2022). https://pith.science/paper/P63FNVGW
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The compiled record

The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

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Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 4,327 input tokens.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.24 · human participants 0.01 · controlled comparison 0.75 · randomized assignment 0.01 · states quantitative result 0.07 · compares with prior results 0.76 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; .

The profile and energy of chiral skyrmions, found in magnetic materials with the Dzyaloshinskii-Moriya interaction, can be approximated by formulae obtained through asymptotic analysis in the limits of small and large skyrmion radius. Using fitting techniques, we modify these formulae so that their validity extends to almost the entire range of skyrmion radii. Such formulae are obtained for skyrmions that are stabilised in the presence of an external field or easy-axis anisotropy or a combination of these. We further study the effect of the magnetostatic field on the skyrmion profile. We compare the profile of magnetic bubbles, stabilized without the chiral Dzyaloshinskii-Moriya interaction to that of a chiral skyrmion.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 The profile and energy of chiral skyrmions, found in magnetic materials with the Dzyaloshinskii-Moriya interaction, can be approximated by formulae obtained through asymptotic analysis in the limits of small and large skyrmion radius. background 0.76 0.32 0.22 asserted 0.76
s1 Using fitting techniques, we modify these formulae so that their validity extends to almost the entire range of skyrmion radii. method 0.57 0.95 0.23 asserted 1.00
s2 Such formulae are obtained for skyrmions that are stabilised in the presence of an external field or easy-axis anisotropy or a combination of these. contribution 0.82 0.86 0.13 asserted 1.00
s3 We further study the effect of the magnetostatic field on the skyrmion profile. contribution 0.99 0.92 0.05 unclear 0.56
s4 We compare the profile of magnetic bubbles, stabilized without the chiral Dzyaloshinskii-Moriya interaction to that of a chiral skyrmion. contribution 0.88 0.88 0.07 asserted 0.86

What kind of paper the classifier reports this is: theoretical result 0.98 · evidence from proof or derivation 0.98.

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Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper
Original abstract

The profile and energy of chiral skyrmions, found in magnetic materials with the Dzyaloshinskii-Moriya interaction, can be approximated by formulae obtained through asymptotic analysis in the limits of small and large skyrmion radius. Using fitting techniques, we modify these formulae so that their validity extends to almost the entire range of skyrmion radii. Such formulae are obtained for skyrmions that are stabilised in the presence of an external field or easy-axis anisotropy or a combination of these. We further study the effect of the magnetostatic field on the skyrmion profile. We compare the profile of magnetic bubbles, stabilized without the chiral Dzyaloshinskii-Moriya interaction to that of a chiral skyrmion.

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