Spin-orbit interaction and Dirac cones in d-orbital noble metal surface states

Ryan Requist, Polina M. Sheverdyaeva, Paolo Moras, Sanjoy K. Mahatha, Carlo Carbone, and Erio Tosatti
Phys. Rev. B 91, 045432 – Published 28 January 2015

Abstract

Band splittings, chiral spin polarization, and topological surface states generated by spin-orbit interactions at crystal surfaces are receiving a lot of attention for their potential device applications as well as fascinating physical properties. Most studies have focused on sp states near the Fermi energy, which are relevant for transport and have long lifetimes. Far less explored, though in principle stronger, are spin-orbit interaction effects within d states, including those deep below the Fermi energy. Here, we report a joint photoemission and ab initio study of spin-orbit effects in the deep d-orbital surface states of a 24-layer Au film grown on Ag(111) and a 24-layer Ag film grown on Au(111), singling out a conical intersection (Dirac cone) between two surface states in a large surface-projected gap at the time-reversal symmetric M¯ points. Unlike the often isotropic dispersion at Γ¯ point Dirac cones, the M¯ point cones are strongly anisotropic. An effective k·p Hamiltonian is derived to describe the anisotropic band splitting and spin polarization near the Dirac cone.

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  • Received 21 November 2014

DOI:https://doi.org/10.1103/PhysRevB.91.045432

©2015 American Physical Society

Authors & Affiliations

Ryan Requist1, Polina M. Sheverdyaeva2, Paolo Moras2, Sanjoy K. Mahatha2,3, Carlo Carbone2, and Erio Tosatti1,3,4

  • 1International School for Advanced Studies (SISSA), Via Bonomea 265, 34136 Trieste, Italy
  • 2Istituto di Struttura della Materia, Consiglio Nazionale delle Ricerche, Trieste, Italy
  • 3International Centre for Theoretical Physics (ICTP), Strada Costiera 11, 34151 Trieste, Italy
  • 4Democritos Simulation Center, Istituto Officina dei Materiali, Consiglio Nazionale delle Ricerche, Via Bonomea 265, 34136 Trieste, Italy

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Issue

Vol. 91, Iss. 4 — 15 January 2015

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