1981
DOI: 10.1103/physrevb.24.3519
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Theory of electron-avalanche breakdown in solids

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Cited by 262 publications
(98 citation statements)
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“…Knowledge of two physical properties is needed to make useful predictions: the interaction strength (which determines the magnitude of the factor multiplying the δ-function) and the kinematics of a collision between an electron and phonon (which determines the zeros of the δ-function argument). Our understanding of electrons and phonons is based on standard models [15][16][17][18][19][22][23][24]36,37 which assume effective mass dispersion. In this work we have replaced semi-phenomenological and ad hoc assumptions about the interaction strength with ab initio calculations, finding that it is stronger than the interaction in the standard models.…”
Section: Resultsmentioning
confidence: 99%
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“…Knowledge of two physical properties is needed to make useful predictions: the interaction strength (which determines the magnitude of the factor multiplying the δ-function) and the kinematics of a collision between an electron and phonon (which determines the zeros of the δ-function argument). Our understanding of electrons and phonons is based on standard models [15][16][17][18][19][22][23][24]36,37 which assume effective mass dispersion. In this work we have replaced semi-phenomenological and ad hoc assumptions about the interaction strength with ab initio calculations, finding that it is stronger than the interaction in the standard models.…”
Section: Resultsmentioning
confidence: 99%
“…Attempts to make realistic predictions for energy and momentum transfer were made by Sparks et al 22 and Akkerman et al 23 who used phenomenological arguments to parametrize and estimate the electron-phonon matrix elements. We are unaware of any more definitive work.…”
Section: 21mentioning
confidence: 99%
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“…However, a very useful approximate solution can be obtained for the total electron density, N(t), in the limit that the electron heating rate is much greater than the rate of energy transfer to the lattice. Note that, 5 = & j;N(E,t)de (6) Inserting equations 2-5 into eq. 1 and integrating over energy, we can write the time dependence of the electron density as,…”
Section: S(e T)dand = S(eand + S(et)hpactmentioning
confidence: 99%
“…This is to be expected as the probability for the ion generation differs between air and vacuum. High vacuum increases the mean electron free path and consequently reduces the concentration of ions generated in the gap by an impact ionization avalanche process [13]. In a high vacuum environment, the reduction of the available ion concentration between non-ideally contacted spots will tend to suppress the formation of the ionic layer since the neutralization occurs at a constant rate but there does not exist sufficient ion concentration to rebuild the surface ion layer immediately.…”
mentioning
confidence: 99%