Question 1 of 6: A1 — Laminar flow of water between parallel plates
Nivaar worked solution (AI-drafted; not reviewed by a licensed engineer)
Notes on this paper
Paper format: National Exams, May 2014 — 04-CHEM-B1 Transport Phenomena; 3 hours, open book. Six problems in three sections (A Fluid Mechanics, B Heat Transfer, C Mass Transfer); candidates attempt one from each section plus a fourth from any section (four of six marked, 25 marks each). The worked solutions below cover all six problems. A summary of the conservation equations (continuity, Navier–Stokes, energy, species) is provided as Appendix A in the paper and is used throughout.
Reference texts: R. S. Brodkey & H. C. Hershey, Transport Phenomena — A Unified Approach (McGraw-Hill) — the paper’s own reference and source of the appended conservation-equation tables; R. B. Bird, W. E. Stewart & E. N. Lightfoot, Transport Phenomena (2nd ed., Wiley) — equations of change and the differential momentum / energy / species balances; J. R. Welty, C. E. Wicks, R. E. Wilson & G. L. Rorrer, Fundamentals of Momentum, Heat and Mass Transfer (Wiley) — differential balances and diffusion with reaction; F. P. Incropera & D. P. DeWitt, Fundamentals of Heat and Mass Transfer (Wiley) — conduction with generation, composite walls, combined convection–radiation.
Question 1: A1 — Laminar flow of water between parallel plates
Given. Fully-developed, steady laminar flow of water (constant $\rho$, $\mu$) between infinite parallel plates a distance $2\delta$ apart; $y$ measured from the mid-plane, so the walls are at $y=\pm\delta$. Flow is driven along $x$ by a constant pressure gradient $dP/dx$. For part (b), inlet temperature $T_{in}$, wall temperature $T_s$.
Find. (a) the velocity profile $u(y)$; (b) the governing PDE for $T$ together with its boundary conditions.
Fig. A1: Fully-developed laminar flow between parallel plates spaced $2\delta$ apart. The pressure gradient drives a symmetric parabolic velocity profile, zero at each wall and maximum on the mid-plane $y=0$.
Part (a) — velocity profile
Reduce the Navier–Stokes equation. For steady, fully-developed unidirectional flow, $\vec{u}=u(y)\,\hat{\imath}$ with $u_y=u_z=0$; continuity then gives $\partial u/\partial x=0$ automatically. The $x$-momentum equation (Table A.2) loses its transient, inertial and $z$-terms, leaving a balance of pressure and viscous stress: $$0=-\frac{1}{\rho}\frac{\partial P}{\partial x}+\nu\frac{\partial^2 u}{\partial y^2}\;\Longrightarrow\;\mu\frac{d^2u}{dy^2}=\frac{dP}{dx}.$$
Integrate twice. With $dP/dx$ constant across the gap, $\dfrac{du}{dy}=\dfrac{1}{\mu}\dfrac{dP}{dx}\,y+C_1$ and $u=\dfrac{1}{2\mu}\dfrac{dP}{dx}\,y^2+C_1 y+C_2.$
Apply symmetry and no-slip. Symmetry about the mid-plane requires $du/dy=0$ at $y=0$, so $C_1=0$. No-slip at either wall, $u(\pm\delta)=0$, gives $C_2=-\dfrac{1}{2\mu}\dfrac{dP}{dx}\,\delta^2.$
Assemble the profile. Substituting the constants, $$u(y)=-\frac{1}{2\mu}\frac{dP}{dx}\left(\delta^2-y^2\right)=-\frac{\delta^2}{2\mu}\frac{dP}{dx}\left(1-\left(\frac{y}{\delta}\right)^2\right).$$ The centre-line value $u(0)=-\dfrac{\delta^2}{2\mu}\dfrac{dP}{dx}$ is by definition $u_{max}$ (positive, since a driving flow has $dP/dx<0$), giving the required result. $\boxed{\,u=u_{max}\left(1-\left(\dfrac{y}{\delta}\right)^2\right)\,}$
Part (b) — temperature-profile equation
The flow is now thermally developing: the fluid enters at $T_{in}$ and is heated (or cooled) toward the wall value $T_s$ as it moves downstream, so $T=T(x,y)$. Applying the energy equation for an incompressible medium (Table A.3) in rectangular coordinates and discarding the terms that vanish gives the governing PDE.
Reduce the energy equation. Steady state removes $\partial T/\partial t$; with $u_y=u_z=0$ only the axial convection term $u_x\,\partial T/\partial x$ survives on the left. On the right, axial conduction $\partial^2T/\partial x^2$ is negligible next to transverse conduction $\partial^2T/\partial y^2$ (large Péclet number), and there is no volumetric generation. With constant $k$: $$\rho\hat{C}_P\,u(y)\,\frac{\partial T}{\partial x}=k\,\frac{\partial^2 T}{\partial y^2}.$$
Insert the known velocity profile. Substituting $u(y)=u_{max}\!\left(1-(y/\delta)^2\right)$ from part (a) gives the differential equation describing the temperature field: $$\boxed{\;\rho\hat{C}_P\,u_{max}\!\left(1-\left(\frac{y}{\delta}\right)^2\right)\frac{\partial T}{\partial x}=k\,\frac{\partial^2 T}{\partial y^2}\;}$$ This is the classic Graetz (thermal-entry) problem; as instructed we stop here without solving.
Boundary and inlet conditions. Three conditions close the second-order-in-$y$, first-order-in-$x$ equation:
Inlet: $T(0,y)=T_{in}$ for all $y$.
Both walls isothermal: $T(x,+\delta)=T(x,-\delta)=T_s$.
Equivalently, by symmetry the centre-line has zero transverse gradient: $\left.\dfrac{\partial T}{\partial y}\right|_{y=0}=0$ (may replace one wall condition).
Check — modelling assumptions
Viscous dissipation is neglected (water at ordinary shear rates: the Brinkman number is very small), axial conduction is dropped relative to axial convection (high Péclet number), and properties are taken constant. If dissipation were retained, a source term $+\mu(du/dy)^2$ would be added to the right-hand side.