1981
DOI: 10.1088/0022-3719/14/31/016
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Wavevector and spin reorientation in MnSi

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Cited by 64 publications
(59 citation statements)
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“…The pitch vector Q points along 111 and the magnetic moments lie perpendicular to it. 16 If an external magnetic field is applied in a direction other than 111 , Q will rotate in the direction of the magnetic field and become parallel to it at a field μ 0 H C1 ≃ 0.1 T, as shown theoretically by Plumer and Walker, 17 and confirmed more recently with small-angle neutron scattering (SANS). 18 Above H C1 , the magnetic moments form a conical phase, which collapses into a ferromagnetic state at μ 0 H C2 = 0.6 T. In cubic helimagnets, there is a narrow temperature interval between the paramagnetic phase and the region of regular chiral modulations where a number of complex multidimensional states and numerous physical anomalies have been observed.…”
mentioning
confidence: 64%
“…The pitch vector Q points along 111 and the magnetic moments lie perpendicular to it. 16 If an external magnetic field is applied in a direction other than 111 , Q will rotate in the direction of the magnetic field and become parallel to it at a field μ 0 H C1 ≃ 0.1 T, as shown theoretically by Plumer and Walker, 17 and confirmed more recently with small-angle neutron scattering (SANS). 18 Above H C1 , the magnetic moments form a conical phase, which collapses into a ferromagnetic state at μ 0 H C2 = 0.6 T. In cubic helimagnets, there is a narrow temperature interval between the paramagnetic phase and the region of regular chiral modulations where a number of complex multidimensional states and numerous physical anomalies have been observed.…”
mentioning
confidence: 64%
“…37,38 It is characterized by a strongly anisotropic susceptibility, induced by the last term in Eq. (31).…”
Section: Response Of the Single-spiral Statementioning
confidence: 99%
“…Helimagnets are special cases of a large family of periodic non collinear spin structures called frustrated systems of XY and Heisenberg spins. The frustration has several origins: (i) it can be due to the geometry of the lattice such as the triangular lattice, the face-centered cubic (FCC) and hexagonalclose-packed (HCP) lattices, with antiferromagnetic NN interaction [11][12][13] (ii) it can be due to competing interactions between NN and NNN such as the case of helimagnets [1,2] shown in Fig. 1 (iii) it can be due to the * sahbi.el-hog@u-cergy.fr † diep@u-cergy.fr, corresponding author competition between the exchange interaction which favors collinear spin configurations and the DzyaloshinskiiMoriya (DM) interaction which favors perpendicular spin arrangements.…”
mentioning
confidence: 99%