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Lifetime of racetrack skyrmions

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dc.contributor Háskóli Íslands
dc.contributor University of Iceland
dc.contributor.author Bessarab, Pavel
dc.contributor.author Müller, Gideon Philipp
dc.contributor.author Lobanov, Igor S.
dc.contributor.author Rybakov, Filipp N.
dc.contributor.author Kiselev, Nikolai S.
dc.contributor.author Jónsson, Hannes
dc.contributor.author Uzdin, Valery M.
dc.contributor.author Blügel, Stefan
dc.contributor.author Bergqvist, Lars
dc.contributor.author Delin, Anna
dc.date.accessioned 2018-05-02T14:25:39Z
dc.date.available 2018-05-02T14:25:39Z
dc.date.issued 2018-02-21
dc.identifier.citation Bessarab, P. F., Müller, G. P., Lobanov, I. S., Rybakov, F. N., Kiselev, N. S., Jónsson, H., . . . Delin, A. (2018). Lifetime of racetrack skyrmions. Scientific Reports, 8(1), 3433. doi:10.1038/s41598-018-21623-3
dc.identifier.issn 2045-2322
dc.identifier.uri https://hdl.handle.net/20.500.11815/709
dc.description.abstract The skyrmion racetrack is a promising concept for future information technology. There, binary bits are carried by nanoscale spin swirls–skyrmions–driven along magnetic strips. Stability of the skyrmions is a critical issue for realising this technology. Here we demonstrate that the racetrack skyrmion lifetime can be calculated from first principles as a function of temperature, magnetic field and track width. Our method combines harmonic transition state theory extended to include Goldstone modes, with an atomistic spin Hamiltonian parametrized from density functional theory calculations. We demonstrate that two annihilation mechanisms contribute to the skyrmion stability: At low external magnetic field, escape through the track boundary prevails, but a crossover field exists, above which the collapse in the interior becomes dominant. Considering a Pd/Fe bilayer on an Ir(111) substrate as a well-established model system, the calculated skyrmion lifetime is found to be consistent with reported experimental measurements. Our simulations also show that the Arrhenius pre-exponential factor of escape depends only weakly on the external magnetic field, whereas the pre-exponential factor for collapse is strongly field dependent. Our results open the door for predictive simulations, free from empirical parameters, to aid the design of skyrmion-based information technology.
dc.description.sponsorship e acknowledge financial support from the Icelandic Research Fund (Grant No. 163048-052), the mega-grant of the Ministry of Education and Science of the Russian Federation (grant no. 14. Y26.31.0015), Göran Gustafsson Foundation, the Russian Foundation for Basic Research (Grant No. 18-02-00267 A), Vetenskapsrådet (VR), Carl Tryggers Stiftelse (CTS), the European Union’s Horizon 2020 research and innovation programme (grant agreement no. 665095–FET-Open project MAGicSky), Academy of Finland (grant no. 278260), and SwedishEnergy Agency (STEM). Calculations of skyrmion lifetimes were supported by the Russian Science Foundation (Grant No. 17-72-10195). Some of the computations were performed on resources provided by the Swedish National Infrastructure for Computing (SNIC) at the National Supercomputer Center (NSC), Linköping University, the PDC Centre for High Performance Computing (PDC-HPC), KTH, and the High Performance Computing Center North (HPC2N), Umeå University.
dc.format.extent 3433
dc.language.iso en
dc.publisher Springer Nature
dc.relation "info:eu-repo/grantAgreement/EC/H2020/665095-FET"
dc.relation.ispartofseries Scientific Reports;8(1)
dc.rights info:eu-repo/semantics/openAccess
dc.subject Condensed-matter physics
dc.subject Magnetic properties and materials
dc.subject Þéttefnisfræði
dc.subject Segulmagn
dc.subject Reiknirit
dc.title Lifetime of racetrack skyrmions
dc.type info:eu-repo/semantics/article
dcterms.license This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. Te images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.
dc.description.version Peer Reviewed
dc.identifier.journal Scientific Reports
dc.identifier.doi 10.1038/s41598-018-21623-3
dc.contributor.department Raunvísindastofnun (HÍ)
dc.contributor.department Science Institute (UI)
dc.contributor.school Verkfræði- og náttúruvísindasvið (HÍ)
dc.contributor.school School of Engineering and Natural Sciences (UI)


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