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Pathways to bubble and skyrmion lattice formation in Fe/Gd multilayers

  • Tim Titze
  • , Sabri Koraltan
  • , Mailin Matthies
  • , Timo Schmidt
  • , Dieter Suess
  • , Manfred Albrecht
  • , Stefan Mathias (Corresponding author)
  • , Daniel Steil (Corresponding author)

Publications: Contribution to journalArticlePeer Reviewed

Abstract

The creation and control of magnetic spin textures is of great interest in fundamental research and future device-oriented applications. Fe/Gd multilayers host a rich variety of magnetic textures including topologically trivial type-2 bubbles and topologically protected chiral type-1 bubbles, also known as dipolar-stabilized skyrmions. Using time-resolved Kerr spectroscopy, we highlight how various control strategies, including temperature, out-of-plane magnetic fields and femtosecond light excitation, can be used to create such textures via different pathways. We find that varying the magnetic field for constant temperature leads to a different (H, T) phase diagram of magnetic textures than moving along a temperature trajectory for constant magnetic field. Micromagnetic simulations corroborate this finding and allow us to visualize the different paths taken. Furthermore, we show that the creation of bubbles and skyrmions in this material via impulsive light excitation is not solely governed by temperature-driven processes, since bubbles and skyrmions can be stabilized in parts of the (H, T) phase diagram, where neither the constant temperature nor the constant magnetic field trajectory predict their existence. Using this phase diagram, we reason why bubble and skyrmion creation in this particular system is only possible from the stripe domain state. Our observations provide a versatile toolkit for tailoring the creation of magnetic spin textures in Fe/Gd multilayers.
Original languageEnglish
Article number064413
Number of pages12
JournalPhysical Review B
Volume112
Issue number6
DOIs
Publication statusPublished - 1 Aug 2025

Funding

T.T. and D.S. gratefully acknowledge funding by the Deutsche Forschungsgemeinschaft (DFG), Grant No. 217133147 (SFB1073, Project No. A02). T.S. and M.A. gratefully acknowledge funding by the DFG, Grant No. 507821284. S.K. and D.Su. acknowledge the Austrian Science Fund (FWF) for support through Grant No. I 6267 (CHIRALSPIN). S.K. thanks the Vienna Doctoral School in Physics for funding the Mobility Fellowship. S.K. acknowledges funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme, Grant Agreement No. 101001290 (3DNANOMAG).

Austrian Fields of Science 2012

  • 103015 Condensed matter
  • 103017 Magnetism
  • 103018 Materials physics

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