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    Observation of fluctuation driven topological Hall effect in the chiral magnet Mn1/3NbS2 with weak Dzyaloshinskii–Moriya interactions

    Haocheng Liao1,2,3,4, Wenhao Li1,2,3,4, Ziyi Zhou1,2,3,4, Qisheng Jiang1,2,3,4, Hui Cheng5,6, Taisen Zuo5,6, He Cheng5,6, Xinzhi Liu1,2,3,*, and Yue Zheng1,2,3,4

    • *Contact author: liuxzh39@mail.sysu.edu.cn

    Phys. Rev. B 113, 214409 – Published 1 June, 2026

    DOI: https://doi.org/10.1103/6l9v-4gg8

    Abstract

    Chiral magnets with Dzyaloshinskii–Moriya interaction host topological spin textures that generate emergent transport. We report a comprehensive study of Mn1/3NbS2, a less-understood member of the T1/3MS2 chiral helimagnet family. Small-angle neutron scattering confirms a chiral helimagnetic ground state with a long helical period of 300 nm, indicating weak DMI. Under a c-axis field, the system evolves through a chiral conical phase (CCP) before reaching the forced ferromagnetic state; a pronounced topological Hall effect (ρxyT∼70 nΩ cm) emerges in the CCP. Detailed analysis shows that THE in CCP phases is dominated by a fluctuation-driven mechanism: thermal magnon excitations generate net scalar spin chirality even when static χ vanishes. The intrinsic lattice chirality (P6322) and DMI break left/right magnon degeneracy, allowing a longitudinal field alone to produce an imbalance. This accounts for the strong temperature dependence, boundary enhancement, and comparable topological Hall conductivity σxyT (∼30(Ωcm)−1) of Mn1/3NbS2 versus well-known CSL Cr1/3NbS2 (∼6.5(Ωcm)−1) despite much weaker DMI in the former. Our results establish Mn1/3NbS2 as a distinct platform for fluctuation-driven topological transport in weakly DMI, strongly anisotropic chiral magnets.

    Physics Subject Headings (PhySH)

    Corrections

    1 July, 2026

    Correction: The penultimate sentence of the Acknowledgment section was missing information and has been fixed.

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