Understanding the Average Electron-Hole Pair-Creation Energy in Silicon and Germanium Based on Full-Band Monte Carlo Simulations

被引:14
|
作者
Fang, Jingtian [1 ,2 ]
Reaz, Mahmud [3 ]
Weeden-Wright, Stephanie L. [4 ]
Schrimpf, Ronald D. [2 ]
Reed, Robert A. [2 ]
Weller, Robert A. [2 ]
Fischetti, Massimo V. [5 ]
Pantelides, Sokrates T. [1 ,2 ]
机构
[1] Vanderbilt Univ, Dept Phys & Astron, Nashville, TN 37235 USA
[2] Vanderbilt Univ, Dept Elect Engn & Comp Sci, 221 Kirkland Hall, Nashville, TN 37235 USA
[3] Vanderbilt Univ, Interdisciplinary Mat Sci Program, 221 Kirkland Hall, Nashville, TN 37235 USA
[4] Lipscomb Univ, Dept Elect & Comp Engn, Nashville, TN 37204 USA
[5] Univ Texas Dallas, Dept Mat Sci & Engn, Richardson, TX 75080 USA
基金
美国国家科学基金会;
关键词
Electron-hole-pair (EHP); impact ionization; Monte Carlo; single-event effects (SEEs); FANO FACTOR; TEMPERATURE-DEPENDENCE; IMPACT IONIZATION; SCATTERING; LIFETIME;
D O I
10.1109/TNS.2018.2879593
中图分类号
TM [电工技术]; TN [电子技术、通信技术];
学科分类号
0808 ; 0809 ;
摘要
The thermalization process of sub-10-eV charge carriers is examined with treating carrier transport with full-band Monte Carlo simulations. The average energy loss (3.69 eV in Si and 2.62 eV in Ge) required to create a thermalized electron-hole pair, obtained from the simulations, is very close to the experimentally measured radiation-ionization energies of Si and Ge irradiated with high-energy particles. These results suggest that only interactions that occur after the radiation-generated charge carriers decay to energies of similar to 10 eV or less determine the fundamental property of the radiation-ionization energies. In addition to an energy loss equal to the band gap energy via impact ionization, acoustic-phonon emission, which has been omitted in prior work, contributes 30% of the remaining carrier energy loss, while optical-phonon emission contributes the other 70%.
引用
收藏
页码:444 / 451
页数:8
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