Room temperature skyrmions in symmetric multilayers

Author:

He Min1ORCID,Li Jinzhi2,Hu Chaoqun3,Zhang Jine3,Gao Yang3ORCID,Li Zhuolin34,Wang Xinran5,Zhao Yinchang1,Dai Zhenhong1ORCID,Xiao Dongdong3,Cai Jianwang34,Zhang Ying234ORCID

Affiliation:

1. School of Physics and Electronic Information, Yantai University, Yantai 264005, China

2. Songshan Lake Materials Laboratory, Dongguan 523808, People's Republic of China

3. Beijing National Laboratory for Condensed Matter Physics, Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China

4. School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100049, China

5. Fert Beijing Institute, MIIT Key Laboratory of Spintronics, School of Integrated Circuit Science and Engineering, Beihang University, Beijing 100191, China

Abstract

We experimentally demonstrate the generation of skyrmions (166 ± 42 nm) by controlling and modulating the skyrmion stability parameter κ through changing the Co layer thickness in the multilayer with repetitions of the symmetric Pt/Co/Pt trilayer. The magnetic field dependence of skyrmion evolution is reversible. Dzyaloshinskii–Moriya interaction constant D is quantitatively measured by Brillouin spectroscopy to understand the mechanism. Surprisingly, the D value is high enough to generate skyrmions in a symmetric sandwich structure although the value is smaller than that in an antisymmetric Pt/Co/Ta trilayer. The decreased D value with the increase in the Co layer thickness indicates that the Dzyaloshinskii–Moriya interaction is still contributed from the interfaces. This work broadens the flexibility to generate skyrmions by engineering skyrmion-based devices with nominally symmetric multilayer without the requirement of very large DMI.

Funder

National Natural Science Foundation of China

Shandong Natural Science Funds for Doctoral Program

The Strategic Priority Research Program of the Chinese Academy of Science

Youth Innovation Promotion Association

Publisher

AIP Publishing

Subject

Physics and Astronomy (miscellaneous)

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