We plan to reduce the energy balance into a more usable form. To achieve this form for plug-flow reactors, we begin by applying the balance to a small differential volume,, in which there are no spatial variations (Figure R9.6-1). The number of moles of species i inis |
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Figure CD9-6 |
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Substituting for Ni in Equation (9-3) and dividingby gives |
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Taking the limit asand noting that gives |
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Rearranging, we have |
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(R9.6-1) |
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Comparing Equations (R9.6-1) and (9-26) |
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(R9.6-2) |
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we note that the term in parentheses is just ri. The rate of reaction of species i is related to the rate of disappearance of species A through the stoichiometric coefficient, |
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Then |
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Finally, |
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To include radial variations in temperature, see Problem P8-29 |
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where a is the heat exchange area per unit volume. Differentiating yields |
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Recalling that |
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we substitute these equations into Equation (9-22) to obtain |
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Neglecting shaft work and changes in pressure with respect to time, we obtain |
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Transient energy |
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(R9.6-3) |
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This equation must be coupled with the mole balances, |
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(R9.6-4) |
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Numerical solution |
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and the rate law, |
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(R9.6-5) |
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and solved numerically. A variety of numerical techniques
for solving equations of this type can be found in the book Applied Numerical
Methods.1 For steady-state operation in which no work is done by the system, Equation (R9.6-3) reduces to |
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(8-60) |
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Substitution for the molar flow rates Fi in terms of conversion gives Equation (8-56). |
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Use this |
(8-56) |
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As stated previously, this equation is solved simultaneously with the mole balance. |