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23-Chem-B1 Transport Phenomena · December 2019

Question 6 of 6: C2 — Deriving the diffusion equation in spherical coordinates

Nivaar worked solution (AI-drafted; not reviewed by a licensed engineer)

Notes on this paper

Paper format. 16-Chem-B1 Transport Phenomena, December 2019 — open-book, 3 hours, six problems (25 marks each) in three sections: A Fluid Mechanics (A1, A2), B Heat Transfer (B1, B2), C Mass Transfer (C1, C2). The rubric asks the candidate to attempt one problem from each section plus a fourth; all six are worked here as a complete study resource. Pages 9–12 of the paper are an appendix of the equations of change (continuity, Navier–Stokes, energy, species) and are used as the reference tables rather than re-derived.

Reference texts: R. B. Bird, W. E. Stewart & E. N. Lightfoot, Transport Phenomena (2nd ed., Wiley) — the equations of change and the film/annular differential balances (A1, C1, C2); J. R. Welty, C. E. Wicks, R. E. Wilson & G. L. Rorrer, Fundamentals of Momentum, Heat and Mass Transfer (Wiley) — pipe friction, the Moody chart and the internal-/external-flow convection correlations (A2, B1, B2); F. P. Incropera & D. P. DeWitt, Fundamentals of Heat and Mass Transfer (8th ed., Wiley) — radiation enclosures, Dittus–Boelter, Churchill–Chu natural convection and air properties (B1, B2); C. J. Geankoplis, Transport Processes and Separation Process Principles (Prentice Hall) — the film model for diffusion with reaction (C1); R. H. Perry & D. W. Green, Perry’s Chemical Engineers’ Handbook — transport properties of air and water.

Question 6: C2 — Deriving the diffusion equation in spherical coordinates (25 marks)

Question text not reproduced: the examination questions are © Engineers and Geoscientists BC. Open the official past paper (linked at the top of this page) to read the question, then follow the worked solution below.

Given. A stationary medium ($\mathbf u=0$), no chemical reaction ($\dot R_{A}=0$), and constant molecular diffusivity $D$. Find. The transient diffusion (Fick’s second law) equation written out fully in spherical coordinates $(r,\theta,\phi)$.

z r θ φ spherical control volume: r² sinθ dr dθ dφ
Fig. C2: Spherical polar coordinates. A differential control volume has faces of area $r^2\sin\theta\,d\theta\,d\phi$ (radial), $r\sin\theta\,dr\,d\phi$ ($\theta$), and $r\,dr\,d\theta$ ($\phi$). Balancing the diffusive flux across these curved faces produces the geometric $2/r$ and $\cot\theta$ terms.

This is a derivation rather than a numerical problem, so the argument is developed as connected reasoning from the species conservation law down to the fully-expanded operator.

  1. Start from the species continuity equation. For component A the general conservation of moles is $$\frac{\partial C_A}{\partial t}+(\nabla\cdot\mathbf N_A)=\dot R_A,$$ where $\mathbf N_A=-D\,\nabla C_A+C_A\mathbf u$ is the combined diffusive-plus-convective molar flux (Appendix Table A.5).
  2. Apply the stated simplifications. A stationary medium sets $\mathbf u=0$ (no convection), and no reaction sets $\dot R_A=0$. With constant $D$ the flux is purely diffusive, $\mathbf N_A=-D\nabla C_A$, and the balance collapses to Fick’s second law: $$\frac{\partial C_A}{\partial t}=D\,\nabla^2C_A\quad\Longleftrightarrow\quad\frac1D\frac{\partial C_A}{\partial t}=\nabla^2C_A.$$
  3. Write the Laplacian in spherical coordinates. In $(r,\theta,\phi)$ the Laplacian operator is $$\nabla^2C_A=\frac1{r^2}\frac{\partial}{\partial r}\!\left(r^2\frac{\partial C_A}{\partial r}\right)+\frac1{r^2\sin\theta}\frac{\partial}{\partial\theta}\!\left(\sin\theta\frac{\partial C_A}{\partial\theta}\right)+\frac1{r^2\sin^2\theta}\frac{\partial^2C_A}{\partial\phi^2}.$$ This is exactly $\nabla\cdot(\nabla C_A)$ evaluated with the spherical control-volume face areas of Fig. C2.
  4. Expand the radial term. Differentiating the product, $$\frac1{r^2}\frac{\partial}{\partial r}\!\left(r^2\frac{\partial C_A}{\partial r}\right)=\frac1{r^2}\!\left(2r\frac{\partial C_A}{\partial r}+r^2\frac{\partial^2C_A}{\partial r^2}\right)=\frac{\partial^2C_A}{\partial r^2}+\frac2r\frac{\partial C_A}{\partial r}.$$ The $2/r$ term is the geometric consequence of the radial area growing as $r^2$.
  5. Expand the polar ($\theta$) term. $$\frac1{r^2\sin\theta}\frac{\partial}{\partial\theta}\!\left(\sin\theta\frac{\partial C_A}{\partial\theta}\right)=\frac1{r^2\sin\theta}\!\left(\cos\theta\frac{\partial C_A}{\partial\theta}+\sin\theta\frac{\partial^2C_A}{\partial\theta^2}\right)=\frac1{r^2}\frac{\partial^2C_A}{\partial\theta^2}+\frac{\cot\theta}{r^2}\frac{\partial C_A}{\partial\theta}.$$
  6. Assemble the result. The azimuthal term is already expanded, so collecting all three contributions gives $$\boxed{\frac1D\frac{\partial C_A}{\partial t}=\frac{\partial^2C_A}{\partial r^2}+\frac2r\frac{\partial C_A}{\partial r}+\frac1{r^2}\frac{\partial^2C_A}{\partial\theta^2}+\frac{\cot\theta}{r^2}\frac{\partial C_A}{\partial\theta}+\frac1{r^2\sin^2\theta}\frac{\partial^2C_A}{\partial\phi^2},}$$ which is precisely the equation to be shown.
ContributionExpanded form
Radial$\partial^2C_A/\partial r^2+(2/r)\,\partial C_A/\partial r$
Polar ($\theta$)$(1/r^2)\partial^2C_A/\partial\theta^2+(\cot\theta/r^2)\partial C_A/\partial\theta$
Azimuthal ($\phi$)$(1/r^2\sin^2\theta)\,\partial^2C_A/\partial\phi^2$
Full equation$\tfrac1D\,\partial C_A/\partial t=\nabla^2C_A$ (spherical, as boxed above)
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