Published July 2, 2025 | Published
Journal Article Open

Fermi surface origin of the low-temperature magnetoresistance anomaly

  • 1. ROR icon Okinawa Institute of Science and Technology
  • 2. ROR icon University of Tennessee at Knoxville
  • 3. ROR icon California Institute of Technology
  • 4. ROR icon University of Chicago
  • 5. ROR icon Colorado State University

Abstract

Magnetoresistance (MR) at a fixed field can demonstrate a non-monotonic temperature dependence—an anomaly—in many systems, including low-dimensional chalcogenides, spin- and charge-density-wave metals, and topological semimetals. These systems are often low-carrier-density compensated metals, and the physics are expected to be quasi-classical. Nevertheless, the MR anomaly also exists in the highly conductive metals Cr, Mo, and W for both linear and quadratic field dependence, with their non-saturation attributed to either open orbit or electron-hole compensation. We argue that quantum transport across sharp Fermi surface arcs, but not necessarily the full cyclotron orbit, governs this MR anomaly, thereby accounting for the profound effects of disorder. In Cr, an overlay exists between three temperature dependences: MR at a constant high field, linear MR at a low field, and Shubnikov-de Haas (SdH) oscillations of the smallest orbit. In Mo, the MR anomaly extends beyond the temperature of its SdH oscillations but disappears before Kohler's scaling reemerges.

Copyright and License

© 2025 The Authors. Published by Elsevier Inc.
This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/).

Acknowledgement

Y.F. acknowledges support from the Okinawa Institute of Science and Technology Graduate University with subsidy funding from the Cabinet Office, Government of Japan. Y.W. acknowledges startup support from the University of Tennessee, Knoxville. T.F.R. acknowledges support from US Department of Energy Basic Energy Science award no. DE-SC0014866. P.B.L. is funded by the Gordon and Betty Moore Foundation (grant GBMF12763). H.C. acknowledges support from US NSF CAREER grant DMR-1945023.

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Additional details

Created:
July 8, 2025
Modified:
July 8, 2025