Shahbazi, K orcid.org/0000-0002-1082-4535, Hrabec, A orcid.org/0000-0002-2895-1962, Moretti, S orcid.org/0000-0002-7586-2217 et al. (5 more authors) (2018) Magnetic properties and field-driven dynamics of chiral domain walls in epitaxial Pt/Co/AuxPt1-x trilayers. Physical Review B - Condensed Matter and Materials Physics, 98 (21). ARTN 214413. ISSN 1098-0121
Abstract
Chiral domain walls in ultrathin perpendicularly magnetized layers have a Néel structure stabilized by a Dzyaloshinskii-Moriya interaction (DMI) that is generated at the interface between the ferromagnet and a heavy metal. Different interface materials or properties are required above and below a ferromagnetic film in order to generate the structural inversion asymmetry needed to ensure that the DMI arising at the two interfaces does not cancel. Here we report on the magnetic properties of epitaxial Pt/Co/AuxPt1−x trilayers grown by sputtering onto sapphire substrates with 0.6 nm thick Co. As x rises from 0 to 1, a structural inversion asymmetry is progressively generated. We characterize the epilayer structure with x-ray diffraction and cross-sectional transmission electron microscopy, revealing (111) stacking. The saturation magnetization falls as the proximity magnetization in Pt is reduced, whilst the perpendicular magnetic anisotropy Ku rises. The micromagnetic DMI strength D was determined using the bubble expansion technique and also rises from a negligible value when x=0 to ∼1 mJ/m2 for x=1. The depinning field at which field-driven domain wall motion crosses from the creep to the depinning regime rises from ∼40 to ∼70 mT, attributed to greater spatial fluctuations of the domain wall energy with increasing Au concentration. Meanwhile, the increase in DMI causes the Walker field to rise from ∼10 to ∼280 mT, meaning that only in the x=1 sample is the steady flow regime accessible. The full dependence of domain wall velocity on driving field bears little resemblance to the prediction of a simple one-dimensional model, but can be described very well using micromagnetic simulations with a realistic model of disorder. These reveal a rise in Gilbert damping as x increases.
Metadata
Item Type: | Article |
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Authors/Creators: |
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Copyright, Publisher and Additional Information: | ©2018 American Physical Society.This is an author produced version of a paper published in Physical Review B - Condensed Matter and Materials Physics. Uploaded in accordance with the publisher's self-archiving policy. |
Keywords: | cond-mat.mtrl-sci |
Dates: |
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Institution: | The University of Leeds |
Academic Units: | The University of Leeds > Faculty of Engineering & Physical Sciences (Leeds) > School of Physics and Astronomy (Leeds) > Condensed Matter (Leeds) |
Depositing User: | Symplectic Publications |
Date Deposited: | 23 Jan 2019 11:09 |
Last Modified: | 17 Dec 2024 11:47 |
Status: | Published |
Publisher: | American Physical Society |
Identification Number: | 10.1103/PhysRevB.98.214413 |
Related URLs: | |
Open Archives Initiative ID (OAI ID): | oai:eprints.whiterose.ac.uk:137662 |