Published December 2019 | v1
Journal Article Open

Creating Weyl nodes and controlling their energy by magnetization rotation

Abstract

As they do not rely on the presence of any crystal symmetry, Weyl nodes are robust topological features of an electronic structure that can occur at any momentum and energy. Acting as sinks and sources of Berry curvature, Weyl nodes have been predicted to strongly affect the transverse electronic response, like in the anomalous Hall or Nernst effects. However, to observe large anomalous effects the Weyl nodes need to be close to or at the Fermi level, which implies the band structure must be tuned by an external parameter, e.g., chemical doping. Here we show that in a ferromagnetic metal tuning of the Weyl node energy and momentum can be achieved by rotation of the magnetization. First, taking as example the elementary magnet hcp-Co, we use electronic structure calculations based on density-functional theory to show that by canting the magnetization away from the easy axis, Weyl nodes can be driven exactly to the Fermi surface. Second, we show that the same phenomenology applies to the kagome ferromagnet Co₃Sn₂S₂, in which we additionally show how the dynamics in energy and momentum of the Weyl nodes affects the calculated anomalous Hall and Nernst conductivities. Our results highlight how the intrinsic magnetic anisotropy can be used to engineer Weyl physics.

Copyright and License

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI.

Acknowledgement

We thank Ulrike Nitzsche for technical assistance. M.R. and J.v.d.B. acknowledge support from the German Research Foundation (DFG) via SFB 1143, Project A5. M.P.G. and J.I.F. thank the Alexander von Humboldt Foundation for financial support through the Georg Forster Research Fellowship Program. J.I.F. and J.-S.Y. thank the IFW excellence programme. J.G.C. acknowledges support by the Betty Moore Foundation EPiQS Initiative, Grant No. GBMF3848 and the United States—Israel Binational Science Foundation (BSF, Grant No. 2016389). L.Y. acknowledges support by the Tsinghua Education Foundation. E.K. and S.F. were supported by the STC Center for Integrated Quantum Materials, NSF Grant No. DMR-1231319, and by ARO MURI Award No. W911NF-14-0247. 

M.P.G. and J.I.F. contributed equally to this work.

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Additional details

Created:
October 24, 2023
Modified:
October 24, 2023