Microwave response of chiral magnetic soliton in Yb(Ni1−xCux)3Al9

Author:

Meng Fanying12,Liu Wei3,Rahman Azizur4,Zhao Jun12,Wang Aina12,Tong Wei15ORCID,Fan Jiyu6ORCID,Ma Chunlan7ORCID,Ge Min4,Pi Li145,Du Haifeng15,Zhang Lei15ORCID,Zhang Yuheng145

Affiliation:

1. Anhui Key Laboratory of Condensed Matter Physics at Extreme Conditions, High Magnetic Field Laboratory, Hefei Institutes of Physical Science, Chinese Academy of Sciences, Hefei 230031, China

2. University of Science and Technology of China, Hefei 230026, China

3. Institutes of Physical Science and Information Technology, Anhui University, Hefei 230601, China

4. Hefei National Research Center for Physical Sciences at the Microscale, University of Science and Technology of China, Hefei 230026, China

5. The High Magnetic Field Laboratory of Anhui Province, Hefei 230031, China

6. Department of Applied Physics, Nanjing University of Aeronautics and Astronautics, Nanjing 210016, China

7. Jiangsu Key Laboratory of Micro and Nano Heat Fluid Flow Technology and Energy Application, School of Physical Science and Technology, Suzhou University of Science and Technology, Suzhou 215009, China

Abstract

A chiral soliton lattice (CSL) is a topological spin-texture that has potential applications in next-generation spintronic devices. In this work, we performed angle-dependence of magnetization and electron spin resonance (ESR) investigations on the CSL host Yb(Ni1− xCu x)3Al9 with x = 0.06 (YNCA). The angle-dependent magnetization reveals a peculiar variable magnetic anisotropy. The maximum magnetization axis is parallel to the ab-plane below the field of ∼35.7 kOe while shifts to the c-axis at higher fields. The microwave responses of the CSL helicoid and ferromagnetic resonance (FMR) of the forced ferromagnetic state (FFM) are observed and appear as two resonance lines on ESR spectra with the highest intensities in the ab-plane. When the external field is rotated from [Formula: see text] to [Formula: see text], the resonance field [Formula: see text] corresponding to the CSL helicoid decreases while [Formula: see text] correlated with the FMR increases. Furthermore, the temperature-dependent ESR shows that the CSL persists until 15 K much higher than TC (6.4 K), which suggests a precursor phenomenon. The microwave response in YNCA provides a powerful tool for modulating and researching the CSL.

Funder

National key R&D Program of China

National Natural Science Foundation of China Anhui Provincial Natural Science Foundation

Alliance of International Science Organizations

Collaborative Innovation Program of Hefei Science Center, CAS

Publisher

AIP Publishing

Subject

Physics and Astronomy (miscellaneous)

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