Non-Born effects in scattering of electrons in a conducting tube with a low concentration of impurities

A. S. Ioselevich and N. S. Peshcherenko
Phys. Rev. B 99, 035414 – Published 9 January 2019

Abstract

Quasi-one-dimensional systems demonstrate Van Hove singularities in the density of states νF and the resistivity ρ, occurring when the Fermi level E crosses a bottom EN of some subband of transverse quantization. We demonstrate that the character of smearing of the singularities crucially depends on the concentration of impurities. There is a crossover concentration nc|λ|,λ1 being the dimensionless amplitude of scattering. For nnc, the singularities are simply rounded at ɛEENτ1—the Born scattering rate. For nnc, the single-impurity non-Born effects in scattering become essential despite λ1. The peak of the resistivity is asymmetrically split in a Fano-resonance manner (however, with a more complex structure). Namely, for ɛ>0, there is a broad maximum at ɛλ2, while for ɛ<0, there is a deep minimum at |ɛ|n2λ2. The behavior of ρ below the minimum depends on the sign of λ. In case of repulsion, ρ monotonically grows with |ɛ| and saturates for |ɛ|λ2. In case of attraction, ρ has a sharp maximum at |ɛ|λ2. The latter feature is due to resonant scattering at quasistationary bound states that inevitably arise just below the bottom of each subband for any attracting impurity.

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  • Received 24 October 2018

DOI:https://doi.org/10.1103/PhysRevB.99.035414

©2019 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

A. S. Ioselevich*

  • Condensed-matter physics laboratory, National Research University Higher School of Economics, Moscow 101000, Russia and L. D. Landau Institute for Theoretical Physics, Moscow 119334, Russia

N. S. Peshcherenko

  • Moscow Institute of Physics and Technology, Moscow 141700, Russia and Skolkovo Institute of Science and Technology, Moscow 121205, Russia

  • *iossel@itp.ac.ru
  • peshcherenko@phystech.edu

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Vol. 99, Iss. 3 — 15 January 2019

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