Phonon-induced rotation of the electronic nematic director in superconducting Bi2Se3

Matthias Hecker and Rafael M. Fernandes
Phys. Rev. B 105, 174504 – Published 2 May 2022

Abstract

The doped topological insulator AxBi2Se3, with A={Cu,Sr,Nb}, becomes a nematic superconductor below Tc3–4 K. The associated electronic nematic director is described by an angle α and is experimentally manifested in the elliptical shape of the in-plane critical magnetic field Hc2. Because of the threefold rotational symmetry of the lattice, α is expected to align with one of three high-symmetry directions corresponding to the in-plane nearest-neighbor bonds, consistent with a Z3-Potts nematic transition. Here, we show that the nematic coupling to the acoustic phonons, which makes the nematic correlation length tend to diverge along certain directions only, can fundamentally alter this phenomenology in trigonal lattices. Compared to hexagonal lattices, the former possesses a sixth independent elastic constant c14 due to the fact that the in-plane shear strain doublet (εxxεyy,2εxy) and the out-of-plane shear strain doublet (2εyz,2εzx) transform as the same irreducible representation. We find that, when c14 overcomes a threshold value, which is expected to be the case in doped Bi2Se3, the nematic director α unlocks from the high-symmetry directions due to the competition between the quadratic phonon-mediated interaction and the cubic nematic anharmonicity. This implies the breaking of the residual in-plane twofold rotational symmetry (C2x), resulting in a triclinic phase. We discuss the implications of these findings for the structure of nematic domains, for the shape of the in-plane Hc2 in AxBi2Se3, and for the presence of nodes inside the superconducting state.

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  • Received 19 November 2021
  • Revised 1 March 2022
  • Accepted 19 April 2022

DOI:https://doi.org/10.1103/PhysRevB.105.174504

©2022 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

Matthias Hecker and Rafael M. Fernandes

  • School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA

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Vol. 105, Iss. 17 — 1 May 2022

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