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Relativistic k.p Hamiltonians for centrosymmetric topological insulators from ab initio wave functions

2016/07/21 by I. A. Nechaev, E. E. Krasovskii · 1 citation
Physics and Astronomy · #cond-mat.mes-hall #cond-mat.mtrl-sci

paper · pdf · doi:10.1103/physrevb.94.201410

published as Phys. Rev. B 94, 201410 (2016) · 6 pages, 4 figures, 1 table

arxiv created 2016/07/21 · arxiv updated 2016/12/07

Abstract

We present a method to microscopically derive a small-size k⋅p Hamiltonian in a Hilbert space spanned by physically chosen ab initio spinor wave functions. Without imposing any complementary symmetry constraints, our formalism equally treats three- and two-dimensional systems and simultaneously yields the Hamiltonian parameters and the true ℤ2 topological invariant. We consider bulk crystals and thin films of Bi2Se3, Bi2Te3, and Sb2Te3. It turns out that the effective continuous k⋅p models with open boundary conditions often incorrectly predict the topological character of thin films.

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