2024 APS March Meeting
Monday–Friday, March 4–8, 2024;
Minneapolis & Virtual
Session S56: First-Principles Computations of Electronic Transport
8:00 AM–11:00 AM,
Thursday, March 7, 2024
Room: 205AB
Sponsoring
Unit:
DCOMP
Chair: Yuanyue Liu, University of Texas at Austin; William G. Vandenberghe
Abstract: S56.00002 : An ab initio approach to closing the "10-100 eV gap" for charge-carrier thermalization in semiconductors
8:30 AM–9:00 AM
Abstract
Presenter:
Massimo V Fischetti
(University of Texas at Dallas)
Author:
Massimo V Fischetti
(University of Texas at Dallas)
We present here an ab inito study of the energy-loss processes and thermalization of hot carriers (electrons, holes, and/or electron-hole pairs) that are generated by high-energy radiation in solids, considering wurtzite GaN as an example. In particular, we focus on the 10-100 eV range of kinetic energy (which we define as the "10-100 eV gap"), since this range is poorly understood. Indeed, the nuclear/particle physics community has a long-standing track record of understanding the thermalization in the higher-energy range (above about 100 eV), whereas the electronic-device community has studied extensively carrier transport in the lower-energy range (below ∼ 10 eV). However, the 10-100 eV gap has been studied only using the free-electron approximation and semi-empirical models for the energy-loss processes. In order to close this 'gap', we employ density functional theory (DFT) to obtain the band structure and dielectric function of GaN for energies up to about 100 eV. DFT perturbation theory and Fermi's Golden Rule/first Born approximation are used to calculate the charge-carrier scattering rates for the major charge-carrier interactions (phonon scattering, impact ionization, and plasmon emission), A full- band Monte Carlo solution of the Boltzmann transpoirt equation is then used to study the thermalization of electrons with kinetic enetrgies as high as 100. The results show that the full thermalization of electrons and holes is complete within ∼ 1 and 0.5 ps, respectively. Hot electrons dissipate about 90% of their initial kinetic energy to the electron-hole gas during the first ∼ 0.1 fs, due to rapid plasmon emission and impact ionization at high energies. The remaining energy is lost at a much slower rate via phonon emission at lower energies (below ∼ 10 eV). During the thermalization, hot electrons generate pairs with an average energy of ∼ 8.9 eV/pair (11-12 pairs per hot electron). Additionally, during the thermalization, the maximum electron displacement from its original position is found to be on the order of 100 nm.