TY - JOUR
T1 - Free energy of twisting spins in Mn3Sn
AU - Li, Xiaokang
AU - Jiang, Shan
AU - Meng, Qingkai
AU - Zuo, Huakun
AU - Zhu, Zengwei
AU - Balents, Leon
AU - Behnia, Kamran
N1 - Publisher Copyright:
© 2022 American Physical Society.
PY - 2022/7/1
Y1 - 2022/7/1
N2 - The magnetic free energy is usually quadratic in the magnetic field and depends on the mutual orientation of the magnetic field and the crystalline axes. Tiny in magnitude, this magnetocrystalline anisotropy energy (MAE) is nevertheless indispensable for the existence of permanent magnets. Here, we show that in Mn3Sn, a noncollinear antiferromagnet that has attracted much attention following the discovery of its large anomalous Hall effect, the free energy of the spins has superquadratic components, which drive the MAE. We experimentally demonstrate that the thermodynamic free energy includes terms odd in the magnetic field [F(H3)+F(H5)] and generating sixfold and 12-fold angular oscillations in the torque response. We show that they are quantitatively explained by theory, which can be used to quantify relevant energy scales (Heisenberg, Dzyaloshinskii-Moriya, Zeeman, and single-ion anisotropy) of the system. Based on the theory, we conclude that in contrast to common magnets, what drives the MAE in Mn3Sn is the field-induced deformation of the spin texture.
AB - The magnetic free energy is usually quadratic in the magnetic field and depends on the mutual orientation of the magnetic field and the crystalline axes. Tiny in magnitude, this magnetocrystalline anisotropy energy (MAE) is nevertheless indispensable for the existence of permanent magnets. Here, we show that in Mn3Sn, a noncollinear antiferromagnet that has attracted much attention following the discovery of its large anomalous Hall effect, the free energy of the spins has superquadratic components, which drive the MAE. We experimentally demonstrate that the thermodynamic free energy includes terms odd in the magnetic field [F(H3)+F(H5)] and generating sixfold and 12-fold angular oscillations in the torque response. We show that they are quantitatively explained by theory, which can be used to quantify relevant energy scales (Heisenberg, Dzyaloshinskii-Moriya, Zeeman, and single-ion anisotropy) of the system. Based on the theory, we conclude that in contrast to common magnets, what drives the MAE in Mn3Sn is the field-induced deformation of the spin texture.
U2 - 10.1103/PhysRevB.106.L020402
DO - 10.1103/PhysRevB.106.L020402
M3 - Article
AN - SCOPUS:85135691660
SN - 2469-9950
VL - 106
JO - Physical Review B
JF - Physical Review B
IS - 2
M1 - L020402
ER -