Chiral Magnetism and High-Temperature Skyrmions in B20-Ordered Co-Si

Magnets with chiral crystal structures and helical spin structures have recently attracted much attention as potential spin-electronics materials, but their relatively low magnetic-ordering temperatures are a disadvantage. While cobalt has long been recognized as an element that promotes high-temper...

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Veröffentlicht in:Physical review letters 2020-02, Vol.124 (5), p.057201-057201, Article 057201
Hauptverfasser: Balasubramanian, Balamurugan, Manchanda, Priyanka, Pahari, Rabindra, Chen, Zhen, Zhang, Wenyong, Valloppilly, Shah R, Li, Xingzhong, Sarella, Anandakumar, Yue, Lanping, Ullah, Ahsan, Dev, Pratibha, Muller, David A, Skomski, Ralph, Hadjipanayis, George C, Sellmyer, David J
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Sprache:eng
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Zusammenfassung:Magnets with chiral crystal structures and helical spin structures have recently attracted much attention as potential spin-electronics materials, but their relatively low magnetic-ordering temperatures are a disadvantage. While cobalt has long been recognized as an element that promotes high-temperature magnetic ordering, most Co-rich alloys are achiral and exhibit collinear rather than helimagnetic order. Crystallographically, the B20-ordered compound CoSi is an exception due to its chiral structure, but it does not exhibit any kind of magnetic order. Here, we use nonequilibrium processing to produce B20-ordered Co_{1+x}Si_{1-x} with a maximum Co solubility of x=0.043. Above a critical excess-Co content (x_{c}=0.028), the alloys are magnetically ordered, and for x=0.043, a critical temperature T_{c}=328  K is obtained, the highest among all B20-type magnets. The crystal structure of the alloy supports spin spirals caused by Dzyaloshinskii-Moriya interactions, and from magnetic measurements we estimate that the spirals have a periodicity of about 17 nm. Our density-functional calculations explain the combination of high magnetic-ordering temperature and short periodicity in terms of a quantum phase transition where excess-cobalt spins are coupled through the host matrix.
ISSN:0031-9007
1079-7114
DOI:10.1103/PhysRevLett.124.057201