2018
DOI: 10.1063/1.5027800
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Crystal-orientation dependence of magnetic domain structures in the skyrmion-hosting magnets MnNiGa

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Cited by 14 publications
(15 citation statements)
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“…6(d)]. This phenomenon has been observed in the study of the crystal direction dependence of the domains in off-stoichiometric (Mn 1−x Ni x ) 65 Ga 35 alloys [26]. With lowering K u , the biskyrmion state can be stabilized under a certain field and maintained when K u is tilted.…”
Section: Resultsmentioning
confidence: 73%
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“…6(d)]. This phenomenon has been observed in the study of the crystal direction dependence of the domains in off-stoichiometric (Mn 1−x Ni x ) 65 Ga 35 alloys [26]. With lowering K u , the biskyrmion state can be stabilized under a certain field and maintained when K u is tilted.…”
Section: Resultsmentioning
confidence: 73%
“…Yao et al [24] and Loudon et al [25] have argued that the biskyrmions under Lorentz transmission electron microscopy (TEM) can possibly be depicted as an inclined type-II (topological trivial) bubble. But we notice that there are distinguished features in the Lorentz TEM images of biskyrmion and its trivial bubble that are obtained in the same material, for example, in the different crystal orientations of (Mn 1−x Ni x ) 65 Ga 35 [26] or in the small-Ga-substituted MnNiGa alloys [20]. Therefore, as an important type of skyrmion state, its formation origin and stability condition deserves in-depth study.…”
Section: Introductionmentioning
confidence: 75%
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“…The ma- chirality of the skyrmion bubbles. 7 Various magnetic domains were observed on the wedge-shaped alloy specimen [35], in the present study, we only focus on the magnetic stripes along the [001] axis as shown in Fig. 1(d).…”
Section: Micromagnetic Simulationsmentioning
confidence: 99%
“…The material parameters of MnNiGa alloy are listed as follows [17]: exchange stiffness A = 2 × 10 −11 J • m −1 , saturation magnetization M s = 5.16 × 10 5 A • m −1 , and uniaxial anisotropy K u = 8.7 × 10 4 J • m −3 . Previous studies report that the crystal orientation, thus the magnetic easy axis direction, is a key ingredient to form biskyrmions [33]. Hence, we perform simulations with the easy axis at a tilted angle of 31 • as in the [12 2] crystal [33].…”
mentioning
confidence: 99%