Dependence of the optical conductivity on the uniaxial and biaxial strains in black phosphorene

C. H. Yang, J. Y. Zhang, G. X. Wang, and C. Zhang
Phys. Rev. B 97, 245408 – Published 12 June 2018

Abstract

By using the Kubo formula, the optical conductivity of strained black phosphorene was studied. The anisotropic band dispersion gives rise to an orientation dependent optical conductivity. The energy gap can be tuned by the uniaxial and biaxial strains which can be observed from the interband optical conductivity polarized along the armchair (x) direction. The preferential conducting direction is along the x direction. The dependence of the intraband optical conductivity along the zigzag (y) direction on the Fermi energy and strain exhibits increasing or decreasing monotonously. However, along the x direction this dependence is complicated which originates from the carriers' inverse-direction movements obtained by two types of the nearest phosphorus atom interactions. The modification of the biaxial strain on the energy structure and optical-absorption property is more effective. The imaginary part of the total optical conductivity (Imσ) can be negative around the threshold of the interband optical transition by modifying the chemical potential. Away from this frequency region, Imσ exhibits positive value. It can be used in the application of the surface plasmon propagations in multilayer dielectric structures.

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  • Received 26 November 2017
  • Revised 2 April 2018

DOI:https://doi.org/10.1103/PhysRevB.97.245408

©2018 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

C. H. Yang1,2, J. Y. Zhang1, G. X. Wang3, and C. Zhang2,*

  • 1School of Physics and Optoelectronic Engineering, Nanjing University of Information Science and Technology, Nanjing 210044, China
  • 2School of Physics and Institute for Superconducting and Electronic Materials, University of Wollongong, New South Wales 2552, Australia
  • 3Center for Clean Energy Technology, School of Mathematical and Physical Sciences, University of Technology Sydney, Sydney NSW 2007, Australia

  • *Corresponding author: czhang@uow.edu.au

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Vol. 97, Iss. 24 — 15 June 2018

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