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An empirical relationship for ionization coefficient for microscale gaps and high reduced electric fields
The importance of gas discharges for numerous applications with increasingly small device size motivates a more fundamental understanding of breakdown mechanisms. Gas breakdown theories for these gap sizes unify field emission with the Townsend avalanche, which depends on Townsend's first ioniz...
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Published in: | Journal of applied physics 2022-08, Vol.132 (7) |
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Main Authors: | , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | The importance of gas discharges for numerous applications with increasingly small device size motivates a more fundamental understanding of breakdown mechanisms. Gas breakdown theories for these gap sizes unify field emission with the Townsend avalanche, which depends on Townsend's first ionization coefficient
α; however, the ratio of the electric field E to gas pressure p for microscale gas breakdown exceeds the range of validity for the typical empirical equation. While some studies have used particle-in-cell simulations to assess
α in this range, they only examined a narrow range of experimental conditions. This work extends this approach to characterize ionization in microscale gaps for N2, Ar, Ne, and He for a broader range of pressure, gap distance d, and applied voltage V. We calculated
α at steady state for
0.75
≤
d
≤
10
μ
m and p = 190, 380, and 760 Torr. As expected,
α
/
p is not a function of reduced electric field
E
/
p for microscale gaps, where the electron mean free path is comparable to d and
E
/
p is high at breakdown. For
d
<
2
μ
m,
α
/
p scales with V and is independent of p. For
d
>
10
μ
m,
α
/
p approaches the standard empirical relationship for
E
/
p
≲
1000
V
Tor
r
−
1
c
m
−
1 and deviates at higher levels because the ionization cross section decreases. We develop a more rigorous semiempirical model for
α, albeit not as universal or simple, for a wider range of d and p for different gas species that may be incorporated into field emission-driven breakdown theories to improve their predictive capability. |
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ISSN: | 0021-8979 1089-7550 |
DOI: | 10.1063/5.0098961 |