AI Article Synopsis

  • Tantalum arsenide (TaAs) is a noncentrosymmetric monopnictide that shows promise as a Weyl semimetal, allowing for the study of chiral massless quasiparticles known as Weyl fermions.
  • The research involved detailed measurements of TaAs's bulk Fermi surface topology using advanced techniques like angle-dependent Shubnikov-de Haas and de Haas-van Alphen measurements, revealing three different types of Fermi surface pockets.
  • TaAs stands out among similar materials as it has the Fermi energy positioned close to Weyl points, which is essential for generating chiral quasiparticles, leading to potential discoveries in novel quantum phenomena.

Article Abstract

Tantalum arsenide is a member of the noncentrosymmetric monopnictides, which are putative Weyl semimetals. In these materials, three-dimensional chiral massless quasiparticles, the so-called Weyl fermions, are predicted to induce novel quantum mechanical phenomena, such as the chiral anomaly and topological surface states. However, their chirality is only well defined if the Fermi level is close enough to the Weyl points that separate Fermi surface pockets of opposite chirality exist. In this Letter, we present the bulk Fermi surface topology of high quality single crystals of TaAs, as determined by angle-dependent Shubnikov-de Haas and de Haas-van Alphen measurements combined with ab initio band-structure calculations. Quantum oscillations originating from three different types of Fermi surface pockets were found in magnetization, magnetic torque, and magnetoresistance measurements performed in magnetic fields up to 14 T and temperatures down to 1.8 K. Of these Fermi pockets, two are pairs of topologically nontrivial electron pockets around the Weyl points and one is a trivial hole pocket. Unlike the other members of the noncentrosymmetric monopnictides, TaAs is the first Weyl semimetal candidate with the Fermi energy sufficiently close to both types of Weyl points to generate chiral quasiparticles at the Fermi surface.

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http://dx.doi.org/10.1103/PhysRevLett.117.146401DOI Listing

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