Kondo Insulator to Semimetal Transformation Tuned by Spin-Orbit Coupling

S. Dzsaber, L. Prochaska, A. Sidorenko, G. Eguchi, R. Svagera, M. Waas, A. Prokofiev, Q. Si, and S. Paschen
Phys. Rev. Lett. 118, 246601 – Published 16 June 2017
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Abstract

Recent theoretical studies of topologically nontrivial electronic states in Kondo insulators have pointed to the importance of spin-orbit coupling (SOC) for stabilizing these states. However, systematic experimental studies that tune the SOC parameter λSOC in Kondo insulators remain elusive. The main reason is that variations of (chemical) pressure or doping strongly influence the Kondo coupling JK and the chemical potential μ—both essential parameters determining the ground state of the material—and thus possible λSOC tuning effects have remained unnoticed. Here, we present the successful growth of the substitution series Ce3Bi4(Pt1xPdx)3 (0x1) of the archetypal (noncentrosymmetric) Kondo insulator Ce3Bi4Pt3. The Pt-Pd substitution is isostructural, isoelectronic, and isosize, and it therefore is likely to leave JK and μ essentially unchanged. By contrast, the large mass difference between the 5d element Pt and the 4d element Pd leads to a large difference in λSOC, which thus is the dominating tuning parameter in the series. Surprisingly, with increasing x (decreasing λSOC), we observe a Kondo insulator to semimetal transition, demonstrating an unprecedented drastic influence of the SOC. The fully substituted end compound Ce3Bi4Pd3 shows thermodynamic signatures of a recently predicted Weyl-Kondo semimetal.

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  • Received 14 December 2016

DOI:https://doi.org/10.1103/PhysRevLett.118.246601

© 2017 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

S. Dzsaber1, L. Prochaska1, A. Sidorenko1, G. Eguchi1, R. Svagera1, M. Waas1, A. Prokofiev1, Q. Si2, and S. Paschen1,2,*

  • 1Institute of Solid State Physics, Vienna University of Technology, Wiedner Hauptstraße 8–10, 1040 Vienna, Austria
  • 2Department of Physics and Astronomy, Rice University, Houston, Texas 77005, USA

  • *Corresponding author. paschen@ifp.tuwien.ac.at

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Issue

Vol. 118, Iss. 24 — 16 June 2017

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