| 1 | \documentclass{article} |
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| 2 | \usepackage{fullpage} |
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| 3 | \newcommand{\PSbox}[3]{\mbox{\rule{0in}{#3}\special{psfile=#1}\hspace{#2}}} |
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| 4 | \begin{document} |
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| 5 | \begin{enumerate} |
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| 6 | \item Chemical vapor deposition |
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| 7 | |
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| 8 | \begin{enumerate} |
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| 9 | \item The mass transfer Prandtl number is given by: |
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| 10 | $${\rm Pr}=\frac{\mu}{\rho D};\ \rho=\frac{MP}{RT},$$ |
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| 11 | where $M$ is the molar mass. Since 1atm=101300 Pa, this pressure is 10130 |
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| 12 | Pa; Pascals are equivalent to Joules per cubic meter. This therefore |
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| 13 | evaluates to: |
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| 14 | $$\rm\rho = \frac{0.040\frac{kg}{mol}\cdot10130\frac{J}{m^3}} |
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| 15 | {8.314\frac{J}{K\cdot mol}\cdot 500K} = 0.097\frac{kg}{m^3};\ |
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| 16 | Pr=\frac{3\times10^{-5}\frac{N\cdot s}{m^2}}{0.097\frac{kg}{m^3}\cdot |
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| 17 | 2\times10^{-4}\frac{m^2}{s}} = 1.54.$$ |
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| 18 | This is not far from one, which is not atypical for a gas (yes, that was a |
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| 19 | double-negative). |
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| 20 | |
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| 21 | \item With a flow rate of $0.3\rm\frac{m^3}{s}$, and box width and height of |
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| 22 | 2m$\times$0.75m, the average velocity is 0.2m/s. The Reynolds number is |
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| 23 | then: |
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| 24 | $${\rm Re} = \frac{\rho u_{av}H}{\mu} = |
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| 25 | \frac{\rm 0.097\frac{kg}{m^3}\cdot0.2\frac{m}{s}\cdot0.75m} |
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| 26 | {3\times10^{-5}\frac{N\cdot s}{m^2}} = 485.$$ |
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| 27 | Looks like flow will remain laminar. |
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| 28 | |
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| 29 | \item The velocity boundary layer thickness will grow as: |
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| 30 | $$\delta_u=5.0\sqrt{\frac{\nu x}{U_\infty}},$$ |
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| 31 | for which we can use $u_{av}$ as $U_\infty$; this gives a maximum thickness |
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| 32 | of 0.27m at $x=2m$. The velocity boundary layers will just meet at the end |
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| 33 | of the reactor. |
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| 34 | |
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| 35 | With a Prandtl number just above one, the concentration boundary layer will |
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| 36 | be somewhat smaller than the velocity boundary layer, but our expression |
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| 37 | for relative boundary layer thickness won't quite be right. So we can |
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| 38 | estimate that the velocity and concentration boundary layers will look |
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| 39 | something like: |
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| 40 | \begin{center} |
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| 41 | \PSbox{cvdboxBL.ps}{420pt}{176pt} |
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| 42 | \end{center} |
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| 43 | |
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| 44 | \item Though the concentration boundary layer thickness correlation is not |
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| 45 | quite right, the high-Pr Nusselt number correlation is accurate down to a |
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| 46 | Prandtl number of 0.5, so we can use that: |
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| 47 | $${\rm Nu}_x = 0.332{\rm Re}_x^{1/2}{\rm Pr}^{1/3},$$ |
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| 48 | along with expressions for the local mass transfer coefficient $h_{Dx}$ and |
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| 49 | diffusive flux: |
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| 50 | $${\rm Nu}_x = \frac{h_{Dx}x}{D_{fl}} \Rightarrow |
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| 51 | h_{Dx} = \frac{{\rm Nu}_xD_{fl}}{x};\ |
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| 52 | J_y|_{y=0} = h_{Dx}(C_\infty-C_s).$$ |
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| 53 | The molar density of the gas mixture is $P/RT$, so with 1 mol\% silane, we |
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| 54 | can use one percent of the overall pressure as the silane partial pressure |
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| 55 | and set $C_\infty=P_{\rm SiH_4}/RT$. The problem states that we can |
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| 56 | estimate $C_s=0$. The results are summarized as follows: |
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| 57 | \begin{center} |
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| 58 | \begin{tabular}{c|cccc|} |
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| 59 | Distance $x$ & Re$_x$ & Nu$_x$ & $h_{Dx}$ & $J_y|_{y=0}$ \\ \hline |
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| 60 | 0.10m & 65 & 3.08 & $6.17\times10^{-3}$m/s & |
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| 61 | $1.5\times10^{-4}$mol/m$^2$sec \\ |
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| 62 | 0.30m & 195 & 5.34 & $3.56\times10^{-3}$m/s & |
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| 63 | $8.68\times10^{-5}$mol/m$^2$sec \\ \hline |
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| 64 | \end{tabular} |
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| 65 | \end{center} |
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| 66 | Note that this close to the entrance, we're really pushing the envelope of |
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| 67 | validity of this solution (since $\delta_C\ll x$ is not so valid). Call it |
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| 68 | a rough estimate. |
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| 69 | |
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| 70 | \item We can just divide the flux by molar density of the solid to calculate |
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| 71 | the deposition rate: |
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| 72 | $\frac{dY}{dt} = \frac{J\cdot M_{\rm Si}}{\rho_{solid}}.$ |
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| 73 | At 10 cm, this will be 1.7 nm/sec; at 30 cm, 0.97 nm/sec. This means a 20 |
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| 74 | cm wafer placed 10 cm from the entrance (from $x=10$cm to $x=30$cm) will |
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| 75 | have a 70\% variation in deposition rate across it, which is a huge |
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| 76 | variation! |
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| 77 | |
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| 78 | \item There are various ways to make the deposition more uniform. A common |
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| 79 | one is to place the substrates on an incline tilting upward about |
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| 80 | 30$^\circ$, so the velocity increases with $x$, flattening out the |
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| 81 | concentration boundary layer a bit. One can also run under conditions more |
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| 82 | likely to be reaction-limited ({\em e.g.} at lower temperature), so the |
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| 83 | silane concentration in the gas will be roughly uniform throughout the |
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| 84 | chamber and right up to the wafers, making deposition roughly uniform. |
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| 85 | |
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| 86 | But the real answer is to ditch this reactor design, and go to something |
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| 87 | very different. Many modern reactors use stagnation flow produced by |
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| 88 | something like a shower head directing reactant gas at an individual wafer, |
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| 89 | or individual wafer rotation, to achieve near-uniform velocity and |
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| 90 | concentration boundary layers. (In response to a similar question on last |
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| 91 | year's final, a student suggested ``Rotisserie CVD'' with wafers moving |
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| 92 | around like chickens in an oven...) Because it processes just a single |
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| 93 | wafer per chamber, this equipment is more expensive, but is worth it to |
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| 94 | deliver uniformity to within a few percent across each wafer. |
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| 95 | \end{enumerate} |
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| 96 | \end{enumerate} |
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| 97 | \end{document} |
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