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Monte Carlo Solution of High Electric Field Hole Transport Processes in Avalanche Amorphous Selenium

[Image: see text] Amorphous selenium lacks the structural long-range order present in crystalline solids. However, the stark similarity in the short-range order that exists across its allotropic forms, augmented with a shift to non-activated extended-state transport at high electric fields beyond th...

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Autores principales: Mukherjee, Atreyo, Vasileska, Dragica, Akis, John, Goldan, Amir H.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: American Chemical Society 2021
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7905821/
https://www.ncbi.nlm.nih.gov/pubmed/33644565
http://dx.doi.org/10.1021/acsomega.0c04922
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author Mukherjee, Atreyo
Vasileska, Dragica
Akis, John
Goldan, Amir H.
author_facet Mukherjee, Atreyo
Vasileska, Dragica
Akis, John
Goldan, Amir H.
author_sort Mukherjee, Atreyo
collection PubMed
description [Image: see text] Amorphous selenium lacks the structural long-range order present in crystalline solids. However, the stark similarity in the short-range order that exists across its allotropic forms, augmented with a shift to non-activated extended-state transport at high electric fields beyond the onset of impact ionization, allowed us to perform this theoretical study, which describes the high-field extended-state hole transport processes in amorphous selenium by modeling the band-transport lattice theory of its crystalline counterpart trigonal selenium. An in-house bulk Monte Carlo algorithm is employed to solve the semiclassical Boltzmann transport equation, providing microscopic insight to carrier trajectories and relaxation dynamics of these non-equilibrium “hot” holes in extended states. The extended-state hole–phonon interaction and the lack of long-range order in the amorphous phase is modeled as individual scattering processes, namely acoustic, polar and non-polar optical phonons, disorder and dipole scattering, and impact ionization gain, which is modeled using a power law Keldysh fit. We have used a non-parabolic approximation to the density functional theory calculated valence band density of states. To validate our transport model, we calculate and compare our time of flight mobility, impact ionization gain, ensemble energy and velocity, and high field hole energy distributions with experimental findings. We reached the conclusion that hot holes drift around in the direction perpendicular to the applied electric field and are subject to frequent acceleration/deceleration caused by the presence of high phonon, disorder, and impurity scattering. This leads to a certain determinism in the otherwise stochastic impact ionization phenomenon, as usually seen in elemental crystalline solids.
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spelling pubmed-79058212021-02-26 Monte Carlo Solution of High Electric Field Hole Transport Processes in Avalanche Amorphous Selenium Mukherjee, Atreyo Vasileska, Dragica Akis, John Goldan, Amir H. ACS Omega [Image: see text] Amorphous selenium lacks the structural long-range order present in crystalline solids. However, the stark similarity in the short-range order that exists across its allotropic forms, augmented with a shift to non-activated extended-state transport at high electric fields beyond the onset of impact ionization, allowed us to perform this theoretical study, which describes the high-field extended-state hole transport processes in amorphous selenium by modeling the band-transport lattice theory of its crystalline counterpart trigonal selenium. An in-house bulk Monte Carlo algorithm is employed to solve the semiclassical Boltzmann transport equation, providing microscopic insight to carrier trajectories and relaxation dynamics of these non-equilibrium “hot” holes in extended states. The extended-state hole–phonon interaction and the lack of long-range order in the amorphous phase is modeled as individual scattering processes, namely acoustic, polar and non-polar optical phonons, disorder and dipole scattering, and impact ionization gain, which is modeled using a power law Keldysh fit. We have used a non-parabolic approximation to the density functional theory calculated valence band density of states. To validate our transport model, we calculate and compare our time of flight mobility, impact ionization gain, ensemble energy and velocity, and high field hole energy distributions with experimental findings. We reached the conclusion that hot holes drift around in the direction perpendicular to the applied electric field and are subject to frequent acceleration/deceleration caused by the presence of high phonon, disorder, and impurity scattering. This leads to a certain determinism in the otherwise stochastic impact ionization phenomenon, as usually seen in elemental crystalline solids. American Chemical Society 2021-02-05 /pmc/articles/PMC7905821/ /pubmed/33644565 http://dx.doi.org/10.1021/acsomega.0c04922 Text en © 2021 The Authors. Published by American Chemical Society Permits non-commercial access and re-use, provided that author attribution and integrity are maintained; but does not permit creation of adaptations or other derivative works (https://creativecommons.org/licenses/by-nc-nd/4.0/).
spellingShingle Mukherjee, Atreyo
Vasileska, Dragica
Akis, John
Goldan, Amir H.
Monte Carlo Solution of High Electric Field Hole Transport Processes in Avalanche Amorphous Selenium
title Monte Carlo Solution of High Electric Field Hole Transport Processes in Avalanche Amorphous Selenium
title_full Monte Carlo Solution of High Electric Field Hole Transport Processes in Avalanche Amorphous Selenium
title_fullStr Monte Carlo Solution of High Electric Field Hole Transport Processes in Avalanche Amorphous Selenium
title_full_unstemmed Monte Carlo Solution of High Electric Field Hole Transport Processes in Avalanche Amorphous Selenium
title_short Monte Carlo Solution of High Electric Field Hole Transport Processes in Avalanche Amorphous Selenium
title_sort monte carlo solution of high electric field hole transport processes in avalanche amorphous selenium
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7905821/
https://www.ncbi.nlm.nih.gov/pubmed/33644565
http://dx.doi.org/10.1021/acsomega.0c04922
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