Optically and Microwave-Induced Magnetization Precession in [Co/Pt]/NiFe Exchange Springs.

X-ray detected ferromagnetic resonance (XFMR) X-ray magnetic circular dichroism (XMCD) exchange spring magnets ferromagnetic resonance interfacial domains spin transfer torque (STT) time-resolved magneto-optical Kerr effect (TRMOKE)

Journal

ACS applied materials & interfaces
ISSN: 1944-8252
Titre abrégé: ACS Appl Mater Interfaces
Pays: United States
ID NLM: 101504991

Informations de publication

Date de publication:
18 Nov 2020
Historique:
pubmed: 7 11 2020
medline: 7 11 2020
entrez: 6 11 2020
Statut: ppublish

Résumé

Microwave and heat-assisted magnetic recordings are two competing technologies that have greatly increased the capacity of hard disk drives. The efficiency of the magnetic recording process can be further improved by employing non-collinear spin structures that combine perpendicular and in-plane magnetic anisotropy. Here, we investigate both microwave and optically excited magnetization dynamics in [Co/Pt]/NiFe exchange spring samples. The resulting canted magnetization within the nanoscale [Co/Pt]/NiFe interfacial region allows for optically stimulated magnetization precession to be observed for an extended magnetic field and frequency range. The results can be explained by formation of an imprinted domain structure, which locks the magnetization orientation and makes the structures more robust against external perturbations. Tuning the canted interfacial domain structure may provide greater control of optically excited magnetization reversal and optically generated spin currents, which are of paramount importance for future ultrafast magnetic recording and spintronic applications.

Identifiants

pubmed: 33156990
doi: 10.1021/acsami.0c14058
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

52116-52124

Auteurs

Maciej Da Browski (M)

Department of Physics and Astronomy, University of Exeter, Stocker Road, Exeter, Devon EX4 4QL, U.K.

Andreas Frisk (A)

Diamond Light Source, Harwell Science and Innovation Campus, Didcot OX11 0DE, U.K.

David M Burn (DM)

Diamond Light Source, Harwell Science and Innovation Campus, Didcot OX11 0DE, U.K.

David G Newman (DG)

Department of Physics and Astronomy, University of Exeter, Stocker Road, Exeter, Devon EX4 4QL, U.K.

Christoph Klewe (C)

Advanced Light Source, Lawrence Berkeley National Laboratory, Berkeley, California 94720, United States.

Alpha T N'Diaye (AT)

Advanced Light Source, Lawrence Berkeley National Laboratory, Berkeley, California 94720, United States.

Padraic Shafer (P)

Advanced Light Source, Lawrence Berkeley National Laboratory, Berkeley, California 94720, United States.

Elke Arenholz (E)

Advanced Light Source, Lawrence Berkeley National Laboratory, Berkeley, California 94720, United States.
Cornell High Energy Synchrotron Source, Cornell University, Ithaca, New York 14853, United States.

Graham J Bowden (GJ)

School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, U.K.

Thorsten Hesjedal (T)

Department of Physics, Clarendon Laboratory, University of Oxford, Oxford OX1 3PU, U.K.

Gerrit van der Laan (G)

Diamond Light Source, Harwell Science and Innovation Campus, Didcot OX11 0DE, U.K.

Gino Hrkac (G)

College of Engineering, Mathematics and Physical Sciences, University of Exeter, Stocker Road, Exeter, Devon EX4 4QL, U.K.

Robert J Hicken (RJ)

Department of Physics and Astronomy, University of Exeter, Stocker Road, Exeter, Devon EX4 4QL, U.K.

Classifications MeSH