Abstract

The remanent domain structures of composite element magnetic barcodes have been imaged using photo-emission electron microscopy with contrast from x-ray magnetic circular dichroism (XMCD-PEEM) and analysed with reference to the results of micromagnetic simulations. The magnetisation configuration at the end of wide strips is found to be perpendicular to the majority magnetisation direction. This transitions to an incomplete rotation for nominal strip widths below 300 nm and is found to affect the mechanics of magnetisation reversal for nominal strip widths below 200 nm, owing to a difference in magnetisation orientation when an external magnetic field is applied that is just smaller than the magnetic coercivity of the structures and a corresponding change in reversal dynamics. This change in domain structure as strip width decreases is consistent with both the influence of shape anisotropy and with measurements of magnetic hysteresis. The magnetisation reversal characteristics of composite element structures are found to be dependent on the relative magnetisation configurations of neighbouring strips, which in turn are found to vary stochastically upon the application and removal of a magnetic field along the easy axis of the structure. It is found that the application of a canted field is necessary to ensure sharp, consistent magnetisation reversal of bits when writing a binary code. These results confirm that either improved lithography of narrower strips or non-rectangular elements would be necessary to further increase the number of individually programmable bits in a barcode.

Details

Title
Magnetisation configuration in arrays of permalloy rectangles and its impact on magnetisation reversal
Author
Newton, P J 1   VIAFID ORCID Logo  ; Devlin, N B 1   VIAFID ORCID Logo  ; Masur, S M 1 ; Ghidini, M 2   VIAFID ORCID Logo  ; Backes, D 3   VIAFID ORCID Logo  ; Maccherozzi, F 3   VIAFID ORCID Logo  ; Pacheco-Pumaleque, A A 4 ; González Esqueche, M A 5 ; Barnes, C H W 1   VIAFID ORCID Logo 

 Department of Physics, Cavendish Laboratory, University of Cambridge, J. J. Thomson Avenue, Cambridge CB3 0HE, United Kingdom 
 SMFI, Department of Mathematics, Physics and Computer Science, University of Parma, viale G.P. Usberti 7/A, 43124 Parma, Italy; Department of Materials Science and Metallurgy, University of Cambridge, 27 Charles Babbage Road, Cambridge CB3 0FS, United Kingdom; Diamond Light Source, Harwell Science and Innovation Campus, Didcot, OX11 0DE, United Kingdom 
 Diamond Light Source, Harwell Science and Innovation Campus, Didcot, OX11 0DE, United Kingdom 
 Escuela Profesional de Ingeniería de Sistemas, Universidad Nacional de Cañete, Jr San Agustín 124, San Vicente de Cañete, Lima, Peru 
 Laboratorio de Celdas Solares, Universidad Nacional de Barranca, Av. Toribio de Luzuriaga Nro. 376, Mz J, Urbanización La Florida, Distrito y Provincia de Barranca, Peru 
Publication year
2021
Publication date
Sep 2021
Publisher
IOP Publishing
e-ISSN
20531591
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
2574786476
Copyright
© 2021. 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.