Abstract

The magnetic properties of Co(10 Å)/NiO(40 Å)/Fe trilayer epitaxially grown on W(110) substrate were investigated with use of x-ray magnetic linear dichroism (XMLD) and x-ray magnetic circular dichroism (XMCD). We showed that magnetic anisotropy of Fe film that can be controlled by a thickness-driven spin reorientation transition is transferred via interfacial exchange coupling not only to NiO layer but further to ferromagnetic Co overlayer as well. Similarly, a temperature driven spin reorientation of Fe sublayer induces a reorientation of NiO spin orientation and simultaneous switching of the Co magnetization direction. Finally, by element specific XMCD and XMLD magnetic hysteresis loop measurements we proved that external magnetic field driven reorientation of Fe and Co magnetizations as well as NiO Néel vector are strictly correlated and magnetic anisotropy fields of Fe and Co sublayers are identical despite the different crystal structures.

Details

Title
Transfer of magnetic anisotropy in epitaxial Co/NiO/Fe trilayers
Author
Szpytma, M. 1   VIAFID ORCID Logo  ; Ślęzak, M. 1 ; Janus, W. 1 ; Nayyef, H. 1 ; Ślęzak, T. 1 ; Mandziak, A. 2 ; Zając, M. 2 ; Wilgocka-Ślęzak, D. 3 ; Menteş, T. O. 4 ; Jugovac, M. 4 ; Locatelli, A. 4   VIAFID ORCID Logo  ; Kozioł-Rachwał, A. 1 

 AGH University of Krakow, Faculty of Physics and Applied Computer Science, Krakow, Poland (GRID:grid.9922.0) (ISNI:0000 0000 9174 1488) 
 Jagiellonian University, National Synchrotron Radiation Centre SOLARIS, Krakow, Poland (GRID:grid.5522.0) (ISNI:0000 0001 2162 9631) 
 Polish Academy of Sciences, Jerzy Haber Institute of Catalysis and Surface Chemistry, Krakow, Poland (GRID:grid.413454.3) (ISNI:0000 0001 1958 0162) 
 Elettra – Sincrotrone Trieste, Basovizza, Trieste, Italy (GRID:grid.5942.a) (ISNI:0000 0004 1759 508X) 
Pages
1680
Publication year
2024
Publication date
2024
Publisher
Nature Publishing Group
e-ISSN
20452322
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
2916553664
Copyright
© The Author(s) 2024. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.