SLIDE 2 1 10 100
Log10 k (m
3/s)
Electron temperature (eV) Log10 k01 Log10 k02 Log10 k03 Log10 k04 Log10 k05 Log10 k06 Log10 k07 Log10 k08 Log10 k09 Log10 k10 Log10 k11 Log10 k12 Log10 k13 Log10 k14 RATE CONSTANTS OF BF3 PLASMA DISCHARGE (PRESENT)
- Fig. 1. Rate coefficients of reactions used in the present
model.
According to the assumptions in the present model, we formulate the particle balance equations for all neutral and ion species as following [1,2,7] : 𝑂3𝑜𝑓𝑙07 + 𝑙14𝑜4𝑜𝑓 − 𝑂
1𝑜𝑓𝑙08 − 𝑂 1𝑜𝑓𝑙09 −
𝛿 𝑂
1 𝑈 1
⁄ = 0 (1) 𝑂5𝑜𝑓𝑙02 + 𝑂5𝑜𝑓𝑙03 + 𝑂4𝑜𝑓𝑙05 + 𝑂3𝑜𝑓𝑙07 + 𝑙14𝑜4𝑜𝑓 + 𝑙13𝑜5𝑜𝑓 + 𝑙12𝑜6𝑜𝑓 − 𝑂2𝑜𝑓𝑙10 − 𝛿 𝑂2 𝑈
2
⁄ = 0 (2) 𝑂4𝑜𝑓𝑙05 + 𝑙13𝑜5𝑜𝑓 − 𝑂3𝑜𝑓𝑙06 − 𝑂3𝑜𝑓𝑙07 − 𝛿 𝑂3 𝑈
3
⁄ = 0 (3) 𝑂5𝑜𝑓𝑙03 + 𝑙12𝑜6𝑜𝑓 − 𝑂4𝑜𝑓𝑙04 − 𝑂4𝑜𝑓𝑙05 − 𝛿 𝑂4 𝑈
4
⁄ = 0 (4) 𝑂
1𝑜𝑓𝑙08 − 𝑜1𝑜𝑓𝑙11 − 𝑜1 𝜐1
⁄ = 0 (5) 𝑂
1𝑜𝑓𝑙09 + 𝑜1𝑜𝑓𝑙11 − 𝑜2 𝜐2
⁄ = 0 (6) 𝑂2𝑜𝑓𝑙10 − 𝑜3 𝜐3 ⁄ = 0 (7) 𝑂3𝑜𝑓𝑙06 − 𝑜4 𝜐4 ⁄ − 𝑙14𝑜4𝑜𝑓 = 0 (8) 𝑂5𝑜𝑓𝑙02 + 𝑂4𝑜𝑓𝑙04 − 𝑜5 𝜐5 ⁄ − 𝑙13𝑜5𝑜𝑓 = 0 (9) 𝑂5𝑜𝑓𝑙01 − 𝑜6 𝜐6 ⁄ − 𝑙12𝑜6𝑜𝑓 = 0 . (10) The charge and particle number conservations are [1,2,7] : 𝑜1 +
1 2 𝑜2 + 𝑜3 + 𝑜4 + 𝑜5 + 𝑜6 = 𝑜𝑓 (11)
𝑂
1 + 𝑜1 + 𝑜2 + 𝑂3 + 𝑜4 + 𝑂4 + 𝑜5 + 𝑂5 + 𝑜6 = 𝑂0 =
𝑞 𝑙𝑈 ⁄ (12) 𝑂2 + 𝑜3 + 𝑂3 + 𝑜4 + 2𝑂4 + 2𝑜5 + 3𝑂5 + 3𝑜6 = 3𝑂0 = 3 𝑞 𝑙𝑈 ⁄ (13) where 𝑂
1, 𝑂2, 𝑂3, 𝑂4, 𝑂5 are the densities of B, F, BF,
BF2, BF3, respectively; 𝑜1, 𝑜2, 𝑜3, 𝑜4, 𝑜5, 𝑜6 are the densities of B+, B++, F+, BF+, BF2+, BF3+, respectively; 𝑈
1,
𝑈
2, 𝑈 3, 𝑈 4 are the transit times of B, F, BF, BF2 across the
chamber, respectively; 𝜐1 , 𝜐2 , 𝜐3 , 𝜐4 , 𝜐5 , 𝜐6 are the containment times of B+, B++, F+, BF+, BF2+, BF3+, respectively; and the containment times of B, F, BF, BF2 would be 𝑈
1/𝛿, 𝑈 2/𝛿, 𝑈 3/𝛿, 𝑈 4/𝛿; γ is the sticking factor
- f B, F, BF, BF2 at the wall; p is the BF3 gas pressure; 𝑈
is the ion and neutral temperature (= 600 K); 𝑜𝑓 is the electron density; 𝑂0 is the density of BF3 molecules before discharge. In the equations which are expressed above, we consider the ratio of 𝜐1, 𝜐2, 𝜐3, 𝜐4, 𝜐5, 𝜐6 to be the ratio
- f the square root of the respective ion masses, and also
consider the ratio of 𝑈
1, 𝑈 2, 𝑈 3, 𝑈 4 to be the ratio of the
square root of the respective atomic or molecular masses [2,7]. 𝜐1 and 𝑈
1 are calculated as two unknown variables.
As preliminary results, we calculate the dependence
- f ion species fractions on plasma density, gas pressure
without considering the relation between pressure and electron temperature. Figure 2 illustrates the ion species fractions when changing the plasma density from 1015 m-
3 to 1019 m-3 at fixed operating pressure p = 20 mTorr, the
recombination coefficient and the electron temperature are set as γ = 0.1 and Te = 3 eV, respectively [2]. We can see that the ion species fraction is greatly influenced by the plasma density. When the plasma density increases, the ion species fractions of B+, F+, BF+, and BF2+ increase, while the ion species fraction of BF3+ decreases significantly, indicating the BF3+ is negligible at very high plasma density regime. The ion species fraction of BF2+ is always higher than that of B+, B++, F+, and BF+.
1E15 1E16 1E17 1E18 1E19 20 40 60 80 100
Ion species fraction (%) Plasma density (m
B
+
B
++
F
+
BF
+
BF2
+
BF3
+
Fixed parameters : p = 20 mTorr, = 0.1, Te = 3 eV (Present)
- Fig. 2. The dependence of ion species fractions on plasma
density.
10 20 30 40 50 20 40 60 80 100
Ion species fraction (%) Pressure (mTorr) B
+
B
++
F
+
BF
+
BF2
+
BF3
+
Fixed parameters : ne = 10
17 m
- 3, = 0.1, Te = 3 eV (Present)
Transactions of the Korean Nuclear Society Virtual Spring Meeting July 9-10, 2020