Abstract

Chiral magnets are an emerging class of topological matter harboring localized and topologically protected vortex-like magnetic textures called skyrmions, which are currently under intense scrutiny as an entity for information storage and processing. Here, on the level of micromagnetics we rigorously show that chiral magnets can not only host skyrmions but also antiskyrmions as least energy configurations over all non-trivial homotopy classes. We derive practical criteria for their occurrence and coexistence with skyrmions that can be fulfilled by (110)-oriented interfaces depending on the electronic structure. Relating the electronic structure to an atomistic spin-lattice model by means of density functional calculations and minimizing the energy on a mesoscopic scale by applying spin-relaxation methods, we propose a double layer of Fe grown on a W(110) substrate as a practical example. We conjecture that ultra-thin magnetic films grown on semiconductor or heavy metal substrates with C2v symmetry are prototype classes of materials hosting magnetic antiskyrmions.

Details

Title
Antiskyrmions stabilized at interfaces by anisotropic Dzyaloshinskii-Moriya interactions
Author
Hoffmann, Markus 1   VIAFID ORCID Logo  ; Zimmermann, Bernd 1   VIAFID ORCID Logo  ; Müller, Gideon P 2   VIAFID ORCID Logo  ; Schürhoff, Daniel 1 ; Kiselev, Nikolai S 1   VIAFID ORCID Logo  ; Melcher, Christof 3 ; Blügel, Stefan 1   VIAFID ORCID Logo 

 Peter Grünberg Institut and Institute for Advanced Simulation, Forschungszentrum Jülich and JARA, Jülich, Germany 
 Peter Grünberg Institut and Institute for Advanced Simulation, Forschungszentrum Jülich and JARA, Jülich, Germany; Science Institute of the University of Iceland, Reykjavík, Iceland 
 Department of Mathematics I & JARA FIT, RWTH Aachen University, Aachen, Germany 
Pages
1-9
Publication year
2017
Publication date
Aug 2017
Publisher
Nature Publishing Group
e-ISSN
20411723
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
1930810990
Copyright
© 2017. 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.