Decreasing electronics size necessitates better characterization of electron emission at the micro- and nanoscales for applications including microplasmas, micro- and nanoelectromechanical systems, and directed energy. While Paschen's law (PL) has historically predicted breakdown voltage based on the Townsend avalanche, field emission must be incorporated for gap sizes below ∼15 μm. Extensive studies have modified PL to explicitly include field emission for planar geometries; however, many practical experiments use pin-to-plate geometries. We modify a previous theory coupling PL and field emission to account for pin-to-plate geometries by replacing the field enhancement factor, which has been used primarily as a fitting parameter, with the appropriate vacuum electric field. This requires explicitly accounting for the spatial dependence of ionization and non-uniform space charge in Poisson's equation. We derive a breakdown equation of the form previously obtained for planar geometry [Venkattraman and Alexeenko, Phys. Plasmas 19, 123515 (2012)] that agrees well with experimental data with the work function as the fitting parameter. The work function was consistently lower (∼2 eV) than anticipated (∼4.5 eV) but was generally fairly consistent (∼ ± 7%). We then derived closed form solutions in the limit of low ionization, corresponding to the field emission regime, and recovered an analytic solution for a parallel plate geometry in the limit of small gap distance that differed from prior analytic results because of the explicit consideration of spatial dependence in charge density. This theory may ultimately be applied to other nonplanar geometries by applying the appropriate equation for the vacuum electric field.
I. INTRODUCTION
The continuous reduction in the device size of electronics toward micro- and nanoscales makes accurately predicting breakdown voltage Vb for safe and optimum device operation increasingly important. Specifically, predicting Vb is paramount for device reliability for applications in high voltage devices,1 pulsed power,2 switches and switchgear,3,4 high power microwaves,5,6 directed energy,7 fusion,8–11 and accelerator applications.12 Conversely, combustion13–16 and various biomedical applications17–21 motivate accurate predictions of Vb to ensure the generation of the resultant plasmas.
Historically, Paschen's law (PL)22,23 has been used to predict breakdown voltage, driven by electron avalanches occurring based on electron collisions. However, as the gap distance decreases, PL begins to deviate from experimental values because the strong electric fields generated at smaller gaps reduce the potential barrier at the cathode sufficiently for electrons to tunnel into the gap by field emission.24,25 These field-emitted electrons ionize the neutral gas near the cathode, creating positive ions. The positive ions subsequently collide with the cathode to create an additional component of secondary emission in the Townsend avalanche and a space-charge electric field that enhances the surface electric field and, thus, the field emission current.23,25–29 These phenomena combine to increase the total current density in the gap, leading to a higher breakdown electric field for a given voltage and causing Vb to decrease with decreasing gap distance d rather than increasing as predicted by PL.25,27 Recent analytic theories have derived from first principles that in the field emission dominated regime.23
While gas, gap distance, and pressure are common parameters of interest for breakdown models, an additional consideration is device geometry. Many original models are derived based on a parallel plate geometry;23,27,30 however, practical devices often use other electrode shapes, such as spherical31,32 or pin-to-plate.33,34 Despite the practical importance of these nonplanar geometries, few theoretical studies have investigated these designs.30,35
A common issue with previous breakdown models23,26,36–38 is how to determine the field enhancement factor a priori to allow for a truly predictive model. The difficulty in achieving this has led to the common treatment of the field enhancement factor as a fitting parameter.23 One recent study eliminates the need to use the field enhancement factor as a fitting parameter and incorporates a non-uniform electric field.35 Here, we combine the recent work by Fu et al. on electric field non-uniformity35 with prior work deriving microscale gas breakdown for a planar diode coupling field emission and Townsend avalanche26,36 to obtain a dimensionless breakdown model for microscale gas breakdown for a pin-to-plate geometry, which is more common for typical field emission and breakdown applications due to the greater field enhancement than in planar diodes.33,34 In the process, we now use the work function as the fitting factor and observe a relatively slight variation (∼15%) across various gap conditions. Also, electrode surface waviness impacts the measured (or effective) work function,39 which may account for some of this variation, particularly for multiple breakdown events that can alter the electrode surface, and even cause significant cratering.34
II. MODEL
Figure 1 shows the pin-to-plate geometry considered in this analysis with the pin anode with a tip radius of 0.5 μm at x = 0 and a copper plate as the cathode at x = d set at a gap distance of 1, 5, or 10 μm ± 0.5 μm from the tip.34
Pin-to-plate geometry considered in the analysis, where the pin represents the anode set at x = 0 with a tip radius of r and the plate is the cathode at a gap distance of d from the tip. Processes for electron emission include secondary electron emission, ionization, and field emission, which create the space-charge region near the cathode.
Pin-to-plate geometry considered in the analysis, where the pin represents the anode set at x = 0 with a tip radius of r and the plate is the cathode at a gap distance of d from the tip. Processes for electron emission include secondary electron emission, ionization, and field emission, which create the space-charge region near the cathode.
Following an analogous procedure to Ref. 26, we begin by writing Poisson's equation assuming all spatial variation in the electric field E is in the x direction as
where is the total electric field [, where is the vacuum electric field and is the space-charge electric field], is the ion current density, given by
where is the total current density, and
is the ion drift velocity with all terms and variables are described in Table I. Note that the total electric field is a function of position x in the geometry in Fig. 1, which makes the ionization coefficient spatially dependent and given by
Parameter definitions, values, and units used in the derivation.
Parameter . | Definition . | Value or equation . | Unit . |
---|---|---|---|
Ap | Material constant of air | 15 | cm−1 Torr−1 |
Bp | Material constant of air | 365 | V cm−1 Torr−1 |
AFN | Fowler–Nordheim constant | 6.2 × 10−6 | A eV V−2 |
BFN | Fowler–Nordheim constant | 6.85 × 107 | |
Modified Fowler–Nordheim parameter | V cm−1 | ||
ɛ0 | Permittivity of free space | 8.854 × 10−12 | F m−1 |
e | Electron charge | 1.602 × 10−19 | C |
k | Boltzmann's constant | 1.38 × 10−23 | J K−1 |
Tg | Gas temperature | 300 | K |
m | Mass of gas molecule | 4.82 × 10−26 | kg |
σce | Charge exchange cross section | 10−18 | m2 |
p | Gas pressure | Variable | Torr |
x | Position along gap | Variable | m |
r | Anode tip radius | Variable | m |
ϕ | Effective cathode surface work function | Variable | eV |
d | Gap distance | Variable | m |
γSE | Secondary emission coefficient of cathode from ion impact | Variable | Dimensionless |
t2(y) | Approximate correction factor for elliptical integrals in Fowler–Nordheim equation | 1.1 | Dimensionless |
ρ | Ion charge density | C m−3 | |
vd | Ion drift velocity | cf. (3) | m s−1 |
Parameter . | Definition . | Value or equation . | Unit . |
---|---|---|---|
Ap | Material constant of air | 15 | cm−1 Torr−1 |
Bp | Material constant of air | 365 | V cm−1 Torr−1 |
AFN | Fowler–Nordheim constant | 6.2 × 10−6 | A eV V−2 |
BFN | Fowler–Nordheim constant | 6.85 × 107 | |
Modified Fowler–Nordheim parameter | V cm−1 | ||
ɛ0 | Permittivity of free space | 8.854 × 10−12 | F m−1 |
e | Electron charge | 1.602 × 10−19 | C |
k | Boltzmann's constant | 1.38 × 10−23 | J K−1 |
Tg | Gas temperature | 300 | K |
m | Mass of gas molecule | 4.82 × 10−26 | kg |
σce | Charge exchange cross section | 10−18 | m2 |
p | Gas pressure | Variable | Torr |
x | Position along gap | Variable | m |
r | Anode tip radius | Variable | m |
ϕ | Effective cathode surface work function | Variable | eV |
d | Gap distance | Variable | m |
γSE | Secondary emission coefficient of cathode from ion impact | Variable | Dimensionless |
t2(y) | Approximate correction factor for elliptical integrals in Fowler–Nordheim equation | 1.1 | Dimensionless |
ρ | Ion charge density | C m−3 | |
vd | Ion drift velocity | cf. (3) | m s−1 |
Additionally, the Fowler–Nordheim current density24,26,40 is given by
where is the total electric field at the cathode and the total current density is given by
Additionally, the vacuum (or space-charge independent) electric field for the geometry in Fig. 1 is given by35
The positive space charge in the gap incrementally increases the electric field by E+.25,26 Thus, jFN from (5) becomes the modified Fowler–Nordheim current density, given by
At breakdown, the electric field in jFN is defined as the surface field, or the electric field at the cathode x = d. Strictly speaking, Etot(x) = Ev(x) + E+(x); however, we can make a few observations about the contributions of these terms to streamline our derivation. First, since E+ arises due to the ions formed at the cathode, the maximum contribution due to space charge will occur for the surface electric field at the cathode in field emission and the secondary emission coefficient γSE in the Townsend avalanche condition.23,26 The peak E+ at x = d is consistent with prior theories for planar microscale gas breakdown, which assumed that the charge density was constant from the cathode to the center of the gap and absent from the center to the anode.23,26 Here, we relax the requirement of constant charge density from the cathode to the center of the gap, but retain the assumptions of peak space-charge contribution at the cathode and negligible space-charge contribution due to the ions at the anode.
For α(x), including E+(x) explicitly in (4) would greatly complicate the solution, particularly since E+(x) is at its highest near the cathode and approaches zero at the anode and, more generally, throughout the gap. Because the physical importance of E+(x) is its influence on field emission at the cathode surface at x = d,23,26 its impact on Etot(x) and, consequently, α(x), throughout the remainder of the gap is minimal, we assume Etot(x) ≈ Ev(x) across the gap for determining α(x). As before,23,26 the surface electric field at the cathode (x = d) for determining the contribution of field emission must include this space-charge electric field, so Etot(d) = Ev(d) + E+(d). Because of the difficulty in extracting space-charge effects from , we cannot readily determine the applied breakdown voltage at the anode from the cathode condition. Instead, we again appeal to and, more specifically, to estimate Vb at the anode from the vacuum breakdown electric field at the anode, given by
While throughout the gap, we emphasize that E+(x) is at its maximum at the cathode and at its minimum [we explicitly assumed ] at the anode, making (11) a more accurate approach for determining Rearranging (11) gives the voltage applied at the anode (x = 0) to achieve breakdown as
Integrating along the gap to substitute into (7) gives
From here, we nondimensionalize by36
where
Considering the cathode at x = d, we next incorporate space charge into the total current density through the modified Fowler–Nordheim current from (9) as
where represents the enhancement in the electric field at the cathode due to the positive space charge induced by the additional ionization due to the electrons that enter the gap due to field emission. Inserting (17) into the nondimensionalized form of (6) and assuming which generally holds until transitioning to PL,23 yields
where , and we have used to obtain for ultimately determining Vb. Solving (18) is challenging due to the spatial dependence of , which comes from in (3); however, the variation of leads to at most a variation in of ∼20% at 1 μm and <10% at ∼0.1 μm. Thus, for the purposes of solving (18), we may neglect this spatial variation and set for simplicity. This is reasonable since (generally considered between 10−3 and 10−1)23,38,41,42 and numerical solutions show that prior to transitioning to PL for gaps ∼10 μm.23 While this assumption may hinder predictive capability in the transition regime between the field emission driven regime and PL, at smaller gaps where field emission clearly drives breakdown,23 making this assumption more accurate in the more field emission driven regime. Furthermore, sensitivity analysis using error propagation showed that had minimal impact on Vb when field emission dominated in a parallel plate geometry,43 providing additional justification for neglecting this term for calculations in the field emission regime. Thus, we may neglect the second term in the parentheses of the denominator of (18) since in the FE dominant breakdown regime, allowing us to rewrite (18) as
Integrating (19) across the gap (0 to ) yields
This differs from the planar case, which assumed that the space charge was constant from the center of the gap to the cathode (d/2 ≤ x ≤ d), making .26 Subtracting from both sides of (20) to obtain on the left-hand-side (LHS) and setting gives
Finally, setting the LHS = g(y) and minimizing (21) yields the breakdown condition as
where . This is analogous to the final planar breakdown condition,26 but accounts for the non-uniform electric field and resulting non-uniform space charge across the gap for a pin-to-plate geometry.
III. RESULTS
We first apply the breakdown model described in (22) to experimental data from Ref. 34 using a pin with a 0.5 μm tip radius and gap distances of 1, 5, and 10 μm. Figures 2–4 show the fitted as a function of breakdown event for all data collected in Ref. 34 determined from numerically solving (22). Because we incorporate the work function into the scaling parameters, changing the work function changes all of the scaling terms in (15), which changes every subsequent variable (all of the dimensionless terms). Thus, care must be taken when comparing nondimensional values for different work functions. We numerically determine that equates from (22) with the experimentally determined, nondimensionalized breakdown voltage. Furthermore, (5) explicitly shows the dependence of jFN on .
Work function as a function of breakdown event for 400 grit polishing at initial interelectrode gap distances (neglecting potential changes due to crater formation) of (a) 1 μm, (b) 5 μm, and (c) 10 μm. Each point represents data from each individual breakdown event from Ref. 34. Data from Brayfield et al., J. Appl. Phys. 125, 203302 (2019). Copyright 2019 AIP Publishing LLC.
Work function as a function of breakdown event for 400 grit polishing at initial interelectrode gap distances (neglecting potential changes due to crater formation) of (a) 1 μm, (b) 5 μm, and (c) 10 μm. Each point represents data from each individual breakdown event from Ref. 34. Data from Brayfield et al., J. Appl. Phys. 125, 203302 (2019). Copyright 2019 AIP Publishing LLC.
Work function as a function of breakdown event for 800 grit polishing at initial interelectrode gap distances (neglecting potential changes due to crater formation) of (a) 1 μm, (b) 5 μm, and (c) 10 μm. Each point represents a single breakdown event. Data from Brayfield et al., J. Appl. Phys. 125, 203302 (2019). Copyright 2019 AIP Publishing LLC.
Work function as a function of breakdown event for 800 grit polishing at initial interelectrode gap distances (neglecting potential changes due to crater formation) of (a) 1 μm, (b) 5 μm, and (c) 10 μm. Each point represents a single breakdown event. Data from Brayfield et al., J. Appl. Phys. 125, 203302 (2019). Copyright 2019 AIP Publishing LLC.
Work function as a function of breakdown event for 1200 grit polishing at initial interelectrode gap distances (neglecting potential changes due to crater formation) of (a) 1 μm, (b) 5 μm, and (c) 10 μm. Each point represents a single breakdown event. Data from Brayfield et al., J. Appl. Phys. 125, 203302 (2019). Copyright 2019 AIP Publishing LLC.
Work function as a function of breakdown event for 1200 grit polishing at initial interelectrode gap distances (neglecting potential changes due to crater formation) of (a) 1 μm, (b) 5 μm, and (c) 10 μm. Each point represents a single breakdown event. Data from Brayfield et al., J. Appl. Phys. 125, 203302 (2019). Copyright 2019 AIP Publishing LLC.
Next, we consider the data pertaining to the first and tenth breakdown events and the depths of the craters formed. Taking the sum of the initial interelectrode gap distance and the crater depth as deff, we fit . Given the relative consistency of over the wide range of , we averaged and compared predicted by the average with the experimental . Figure 5(b) shows that the predicted and measured differed by an average of ∼16%. We note that is lower than typically stated in the literature (e.g., ∼4.5 eV for copper). We surmise that this behavior replaces a semiempirical correction factor that is usually accounted for by , which is now a purely geometrical effect; the role of the correction factor has shifted to . Another possible contributory factor to the reduced is that ions near the cathode may suppress the potential barrier, allowing the field-emitted electrons to tunnel into the gap which may lower the work function of the cathode. While some studies44,45 have suggested that space charge could lower , further investigation is required. For instance, Malayter and Garner theoretically investigated the effect of surface waviness on measured using a scanning Kelvin probe (SKP); they calculated the change in the charge in the gap, and ultimately the capacitance, of each step of the SKP.39 It may be possible to modify this theory to account for the change in as space charge builds up in the gap.
(a) Work function as a function of effective gap distance deff (interelectrode gap distance + crater depth) based on fitting the experimental data34 before and after crater formation. Each data point is an individual experiment. (b) Measured34 and predicted breakdown voltage using the average work function as a function of deff.
(a) Work function as a function of effective gap distance deff (interelectrode gap distance + crater depth) based on fitting the experimental data34 before and after crater formation. Each data point is an individual experiment. (b) Measured34 and predicted breakdown voltage using the average work function as a function of deff.
Figure 6 uses (22) and the appropriate scaling parameters to predict breakdown voltage as a function of work function for various pressures. Increasing the work function increases the breakdown voltage, since increasing the work function increases the energy required for electrons to overcome the potential barrier and tunnel through the cathode. Figure 6 also suggests that pressure does not have a significant effect on the breakdown voltage in (a)–(c), but increases the breakdown voltage for (d) at the largest work function. We will explicitly investigate gap distance and pressure next.
Breakdown voltage as a function of work function for various gap distances at pressures of (a) 1000 Torr, (b) 760 Torr, (c) 380 Torr, and (d) 50 Torr.
Breakdown voltage as a function of work function for various gap distances at pressures of (a) 1000 Torr, (b) 760 Torr, (c) 380 Torr, and (d) 50 Torr.
Next, we consider the nondimensionalized version of the model. While our most recent nondimensionalized breakdown models23,38 considered work function as a separate dimensionless variable and derived corresponding scaling parameters, the present study keeps the work function within the scaling parameters as in our earlier studies.36 Thus, the scaling parameters for each gas in the present study are only constant for a given work function. Figure 7 shows the dimensionless breakdown voltage as a function of dimensionless gap distance for various dimensionless pressures and work functions. Figure 8 shows the dimensionless breakdown voltage as a function of dimensionless pressure for various dimensionless gap distances and work functions. Overall, these results indicate that breakdown voltage depends more strongly on gap distance than pressure in the field emission driven regime, in agreement with prior sensitivity analyses of field emission breakdown theories for a parallel plate geometry.43
Dimensionless breakdown voltage as a function of dimensionless gap distance for various dimensionless pressures for work function of (a) 1 eV, (b) 2 eV, and (c) 3 eV. Because changing the work function changes the scaling parameters, the dimensionless values in (a)–(c) should not be compared to one another.
Dimensionless breakdown voltage as a function of dimensionless gap distance for various dimensionless pressures for work function of (a) 1 eV, (b) 2 eV, and (c) 3 eV. Because changing the work function changes the scaling parameters, the dimensionless values in (a)–(c) should not be compared to one another.
Dimensionless breakdown voltage as a function of dimensionless pressure for various dimensionless gap distances for work function of (a) 1 eV, (b) 2 eV, and (c) 3 eV. Because changing the work function changes the scaling parameters, the dimensionless values in (a)–(c) should not be compared to one another.
Dimensionless breakdown voltage as a function of dimensionless pressure for various dimensionless gap distances for work function of (a) 1 eV, (b) 2 eV, and (c) 3 eV. Because changing the work function changes the scaling parameters, the dimensionless values in (a)–(c) should not be compared to one another.
Furthermore, we can assess the impact of tip radius on breakdown voltage. Figure 9(a) shows the breakdown voltage as a function of gap distance for tip radii of 0.5, 1, and 3 μm at a pressure of 760 Torr and work function of 2 eV, Fig. 9(b) shows the dependence on the ratio of gap distance to tip radius, d/r, for the same conditions, and Fig. 9(c) shows breakdown voltage as a function of tip radius for gap distances of 0.5 and 2 μm. As demonstrated, the sharpest tip corresponds to the lowest breakdown voltage, and increasing tip radius for a constant gap distance shows the breakdown voltage approaching a constant, as expected. As d/r becomes small, the geometry begins to more closely resemble a parallel plate geometry, so the breakdown voltage becomes less sensitive to r.
(a) Breakdown voltage as a function of gap distance for tip radii of 0.5, 1, and 3 μm. (b) Breakdown voltage as a function of the ratio of gap distance to tip radius d/r for tip radii of 0.5, 1, and 3 μm. (c) Breakdown voltage as a function of tip radius for gap distances of 0.5 and 2 μm.
(a) Breakdown voltage as a function of gap distance for tip radii of 0.5, 1, and 3 μm. (b) Breakdown voltage as a function of the ratio of gap distance to tip radius d/r for tip radii of 0.5, 1, and 3 μm. (c) Breakdown voltage as a function of tip radius for gap distances of 0.5 and 2 μm.
As discussed above, this model eliminates the dependence on the secondary emission coefficient in the field emission driven breakdown regime after (17) due to the series expansion, similar to our initial microscale gas breakdown study.36 This assumption begins to weaken as we approach the PL regime. We can identify the condition for transitioning from this simplified field emission driven regime theory to the traditional PL by considering
which is a dimensionless, position-dependent modified Townsend avalanche condition. Inserting our definitions from above and solving for γSE yields
which determines γSE to transition to the traditional PL. Figure 10 plots this transition value of for the parameters considered in Fig. 7. For all but the largest and considered, achieving the transition to the classical PL requires γSE much larger than typical magnitudes. Thus, assuming that γSE minimally impacts the breakdown voltage calculation is reasonable for the majority of the parameter space considered here. For reference, the dimensional pressures and gap distances considered here correspond to 50–1000 Torr and 0.1–5 μm, respectively.
Secondary emission coefficient γSE as a function of dimensionless gap distance for various pressures at work function of (a) 1 eV, (b) 2 eV, and (c) 3 eV.
Secondary emission coefficient γSE as a function of dimensionless gap distance for various pressures at work function of (a) 1 eV, (b) 2 eV, and (c) 3 eV.
IV. CONCLUSION
This work derived a dimensionless breakdown model for a pin-to-plate geometry considering a non-uniform electric field, field emission, and Townsend effects. We compared the theory to experimental data to determine work function values to assess variation of the theoretical predictions over the course of several breakdown events. Additionally, we showed the variation of breakdown voltage with both pressure and gap distance, demonstrating a stronger dependence on gap distance, as expected based on previous analyses for planar diodes.43
The lower work function obtained by fitting to experimental data rather than may be due to the presence of additional space charge lowering the energy needed for electrons to tunnel into the gap or an artifact of residual effects from the semiempirical correction factor usually accounted for by fitting . Further investigation is needed to elucidate the physics behind the ∼2–3 eV difference in work function compared to typically reported values from the literature.
Additionally, further experimental data assessing crater depth is needed to distinguish changes in breakdown voltage due to surface morphology effects on work function and crater depth induced changes on modified gap distance. Future work will further examine the effects of electrode geometry and the resulting charge buildup on work function and the application of this technique to other relevant geometries, such as sphere-to-sphere.31,32,46
ACKNOWLEDGMENTS
This material is based on work supported by the Air Force Office of Scientific Research under Award No. FA9550-18-1-0218 and the Office of Naval Research under Grant No. N00014-17-1-2702. A.M.L. gratefully acknowledges funding from a graduate scholarship from the Directed Energy Professional Society.
DATA AVAILABILITY
The data that support the findings of this study are available from the corresponding author upon reasonable request.