UNIT 1: Heat and Mass Transfer – Comprehensive Short Notes
(Aligned with RGPV Past Paper Analysis)
I. Fundamentals and Basic Concepts
Modes of Heat Transfer
-
Conduction: Transfer due to temperature gradient in a medium (Fourier’s law).
-
Convection: Transfer between solid surface and moving fluid (Newton’s law of cooling).
-
Radiation: Transfer via electromagnetic waves (Stefan-Boltzmann law).
Basic Laws
| Law | Statement | Formula |
|---|---|---|
| Fourier’s Law | Heat flux proportional to temperature gradient | $$\displaystyle q'' = -k \frac{dT}{dx} $$ |
| Newton’s Law of Cooling | Convective heat flux proportional to surface-ambient ΔT | $$\displaystyle q'' = h (T_s - T_\infty) $$ |
| Stefan-Boltzmann Law | Radiant energy from a black body | $$\displaystyle E_b = \sigma T^4 $$ |
| Planck’s Distribution Law | Spectral emissive power of a black body | $$\displaystyle E_{b\lambda} = \frac{2\pi h c^2}{\lambda^5(e^{hc/\lambda kT}-1)} $$ |
| Wien’s Displacement Law | Peak wavelength shifts with temperature | $$\displaystyle \lambda_{max} T = b $$ (constant) |
| Kirchhoff’s Law | For a body in thermal equilibrium: $$\displaystyle \alpha = \varepsilon $$ (for same wavelength/direction) |
Thermal Properties
-
Thermal conductivity ($k$): W/m·K, material’s ability to conduct heat.
-
Convective heat transfer coefficient ($h$): W/m²·K, depends on flow, geometry.
-
Emissivity ($\varepsilon$): Ratio of actual to black body radiation (0–1).
-
Absorptivity ($\alpha$), Reflectivity ($\rho$), Transmissivity ($\tau$): $$\displaystyle \alpha + \rho + \tau = 1 $$.
Key Distinctions
| Concept | Difference |
|---|---|
| Heat vs. Internal Energy vs. Thermal Energy | Heat: energy in transit. Internal energy: total microscopic energy. Thermal energy: part of internal energy related to temperature. |
| Conduction vs. Convection | Conduction: no bulk motion; Convection: fluid motion enhances transfer. |
| Evaporation vs. Boiling | Evaporation: surface phenomenon at any T; Boiling: bulk phenomenon at saturation T with vapor bubbles. |
| Film vs. Dropwise Condensation | Film: continuous liquid film (lower h); Dropwise: discrete droplets (higher h, ~5–10×). |
| Forced vs. Natural Convection | Forced: external means (fan/pump); Natural: buoyancy-driven ($$\displaystyle Gr > 10^9 $$). |
| Laminar vs. Turbulent Flow | Laminar: smooth layers ($$\displaystyle Re < 2300 $$ in pipes); Turbulent: chaotic mixing ($$\displaystyle Re > 4000 $$). |
| Grashof vs. Rayleigh Number | $$\displaystyle Gr = \frac{g \beta (T_s - T_\infty) L^3}{\nu^2} $$ (buoyancy/inertia); $$\displaystyle Ra = Gr \cdot Pr $$ (buoyancy/viscous+diffusion). |
Radiation Shield
-
Thin, low-emissivity material placed between surfaces to reduce net radiation exchange.
-
Effectiveness: $$\displaystyle \varepsilon_{eff} \approx \frac{1}{1/\varepsilon_1 + 1/\varepsilon_2 - 1} $$ for two parallel plates.
-
Application: Thermocouples, spacecraft insulation, building windows.
Thermocouple
-
Principle: Seebeck effect – two dissimilar metals generate voltage proportional to temperature difference.
-
Use: Temperature measurement; junction at measurement point, reference at known T.
[!TIP]
- Common Pitfall: Confusing thermal energy (stored) with heat (transfer).
- Exam Focus: Kirchhoff’s law applies at thermal equilibrium for same wavelength/direction.
II. Steady-State Heat Conduction
One-Dimensional Conduction
Plane Wall
-
Governing Equation: $$\displaystyle \frac{d^2T}{dx^2} = 0 $$ (steady, 1D, constant $k$).
-
Temperature Distribution: Linear: $$\displaystyle T(x) = C_1 x + C_2 $$.
-
Heat Transfer Rate: $$\displaystyle Q = k A \frac{T_1 - T_2}{L} $$.
-
Composite Wall:
$$Q = \frac{A (T_{hot} - T_{cold})}{\sum \frac{L_i}{k_i} + \frac{1}{h_i} + \frac{1}{h_o}} = U A \Delta T_{overall}$$
where $$\displaystyle U = \left[ \sum \frac{L_i}{k_i} + \frac{1}{h_i} + \frac{1}{h_o} \right]^{-1} $$.
- Thermal Contact Resistance: Additional resistance at interfaces due to imperfect contact.
Cylinder
-
Governing Equation (radial, steady): $$\displaystyle \frac{1}{r} \frac{d}{dr} \left( r \frac{dT}{dr} \right) = 0 $$.
-
Temperature Distribution: $$\displaystyle T(r) = C_1 \ln r + C_2 $$.
-
Heat Transfer Rate:
$$Q = \frac{2\pi k L (T_i - T_o)}{\ln(r_o/r_i)}$$
- Critical Radius of Insulation:
$$\boxed{r_{cr} = \frac{k}{h}}$$
For $$\displaystyle r < r_{cr} $$, adding insulation increases heat loss; for $$\displaystyle r > r_{cr} $$, it decreases loss.
Physical Significance: Balance between increased area and increased thermal resistance.
Sphere
-
Governing Equation: $$\displaystyle \frac{1}{r^2} \frac{d}{dr} \left( r^2 \frac{dT}{dr} \right) = 0 $$.
-
Temperature Distribution: $$\displaystyle T(r) = -\frac{C_1}{r} + C_2 $$.
-
Heat Transfer Rate:
$$Q = \frac{4\pi k r_i r_o (T_i - T_o)}{r_o - r_i}$$
- Critical Radius:
$$\boxed{r_{cr} = \frac{2k}{h}}$$
Applications
-
Composite Walls: Windows, cold storage, oven walls – calculate $Q$ and interface temperatures.
-
Critical Radius Design:
-
Refrigeration pipes: Insulation thickness > $$\displaystyle r_{cr} $$ to minimize heat gain.
-
Electrical wires: Insulation < $$\displaystyle r_{cr} $$ to avoid overheating (but usually wires operate below $$\displaystyle r_{cr} $$).
-
-
Plot of Q vs. r for Cylinder:
- Initially rises (area effect dominates), peaks at $$\displaystyle r_{cr} $$, then falls (resistance effect dominates).
[!TIP]
- Critical Radius Formula: Cylinder: $k/h$; Sphere: $2k/h$.
- Common Error: Forgetting that $$\displaystyle r_{cr} $$ applies to outer radius of insulation.
III. Transient Heat Conduction
Lumped Capacitance Method
-
Assumption: Infinite thermal conductivity → uniform temperature throughout solid at any time.
-
Biot Number Criterion: $$\displaystyle Bi = \frac{h L_c}{k} < 0.1 $$ (where $$\displaystyle L_c = V/A_s $$).
-
Energy Balance:
$$\rho V c_p \frac{dT}{dt} = -h A_s (T - T_\infty)$$
- Solution:
$$\frac{T(t) - T_\infty}{T_i - T_\infty} = \exp \left( -\frac{h A_s}{\rho V c_p} t \right) = \exp(-Bi \cdot Fo)$$
where $$\displaystyle Fo = \frac{\alpha t}{L_c^2} $$ (Fourier number).
- Time to Reach Temperature $T$:
$$t = -\frac{\rho V c_p}{h A_s} \ln \frac{T - T_\infty}{T_i - T_\infty}$$
Infinite Thermal Conductivity Method
-
Same as lumped capacitance; term sometimes used interchangeably.
-
Temperature-Time Plot: Exponential decay from $$\displaystyle T_i $$ to $$\displaystyle T_\infty $$.
[!TIP]
- Biot Number: $$\displaystyle Bi < 0.1 $$ required; if violated, use Heisler charts or numerical methods.
- Exam Problem: Often given $\rho$, $$\displaystyle c_p $$, $k$, $h$, $V$, $$\displaystyle A_s $$ – first check $Bi$.
IV. Convection Heat Transfer
Boundary Layer Theory
-
Hydrodynamic Boundary Layer: Region where velocity changes from 0 to $$\displaystyle U_\infty $$.
-
Momentum Equation Derivation (for flat plate, steady, incompressible, constant $\mu$):
Start from Navier-Stokes, apply boundary layer approximations ($\partial/\partial x \ll \partial/\partial y$, $u \approx u(x,y)$, $v \ll u$), simplify to:
-
$$u \frac{\partial u}{\partial x} + v \frac{\partial u}{\partial y} = \nu \frac{\partial^2 u}{\partial y^2}$$
-
Thermal Boundary Layer: Region where $T$ changes from $$\displaystyle T_s $$ to $$\displaystyle T_\infty $$.
- Energy Equation:
$$u \frac{\partial T}{\partial x} + v \frac{\partial T}{\partial y} = \alpha \frac{\partial^2 T}{\partial y^2}$$
-
Boundary Layer Thickness ($\delta$): $$\displaystyle u/\delta \sim U_\infty/\delta $$, $$\displaystyle \delta \propto \sqrt{\frac{\nu x}{U_\infty}} $$ (laminar).
-
Displacement Thickness ($$\displaystyle \delta^* $$): $$\displaystyle \delta^* = \int_0^\infty \left(1 - \frac{u}{U_\infty}\right) dy $$.
Dimensionless Numbers
| Number | Definition | Physical Significance |
|---|---|---|
| Reynolds ($Re$) | $$\displaystyle \frac{\rho U L}{\mu} $$ | Inertia/viscous forces; flow regime. |
| Prandtl ($Pr$) | $$\displaystyle \frac{\nu}{\alpha} = \frac{\mu c_p}{k} $$ | Momentum/thermal diffusivity ratio. |
| Nusselt ($Nu$) | $$\displaystyle \frac{h L}{k} $$ | Convective/conduction resistance ratio. |
| Grashof ($Gr$) | $$\displaystyle \frac{g \beta (T_s - T_\infty) L^3}{\nu^2} $$ | Buoyancy/inertia (natural conv). |
| Rayleigh ($Ra$) | $Gr \cdot Pr$ | Buoyancy/viscous+diffusion (natural conv). |
| Stanton ($St$) | $$\displaystyle \frac{h}{\rho c_p U} $$ | Heat transfer/thermal capacity rate. |
Flow Regimes
-
Laminar: Smooth, $$\displaystyle Re_x < 5 \times 10^5 $$ (flat plate).
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Transition: $$\displaystyle 5 \times 10^5 < Re_x < 3 \times 10^6 $$.
-
Turbulent: Chaotic, $$\displaystyle Re_x > 3 \times 10^6 $$.
Diagram:
DiagramSEARCH: boundary layer development flat plate laminar turbulent
Forced Convection
External (Flow over surfaces)
- Flat Plate (Laminar):
$$Nu_x = 0.332 \, Re_x^{1/2} \, Pr^{1/3} \quad (Pr > 0.6)$$
-
Cylinder/Sphere: Use Churchill-Bernstein or Hilpert correlations.
Example (cylinder, $$\displaystyle Re_D Pr > 0.2 $$):
$$Nu_D = C \, Re_D^m \, Pr^{1/3}$$
with $C$, $m$ from table (e.g., $$\displaystyle Re_D=40–4000 $$: $$\displaystyle C=0.683 $$, $$\displaystyle m=0.466 $$).
Internal (Flow in tubes)
-
Hydrodynamically Fully Developed: Velocity profile invariant in flow direction.
-
Thermally Fully Developed: Temperature profile invariant.
-
Entrance Length:
-
Laminar: $$\displaystyle L_{h,th} \approx 0.05 \, Re \, Pr \, D $$ (thermal).
-
Turbulent: $$\displaystyle L_{h,th} \approx 10–60 \, D $$.
-
-
Correlation (Laminar, constant $$\displaystyle T_s $$):
$$Nu = 3.66 \quad \text{(fully developed)}$$
Dimensional Analysis for Forced Convection
Buckingham Pi Theorem: If $n$ variables involve $r$ fundamental dimensions, then $(n-r)$ independent $\pi$ terms describe the relationship.
Application to Forced Convection:
-
Variables: $$\displaystyle h, L, k, \mu, c_p, \rho, U $$. ($$\displaystyle n=7 $$)
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Dimensions: $M, L, T, \Theta$ ($$\displaystyle r=4 $$).
-
Repeating Variables: $L, k, \mu, \rho$ (include all dimensions).
-
$\pi$ Terms:
$$\displaystyle \pi_1 = \frac{h L}{k} = Nu $$, $$\displaystyle \pi_2 = \frac{\rho U L}{\mu} = Re $$, $$\displaystyle \pi_3 = \frac{\mu c_p}{k} = Pr $$.
-
Functional Form:
$$\boxed{Nu = f(Re, Pr)}$$
Natural Convection
- Vertical Plate (laminar, $$\displaystyle Ra_x < 10^9 $$):
$$Nu_x = 0.59 \, (Ra_x)^{1/4} \quad \text{or} \quad Nu_x = 0.68 + \frac{0.67 \, Ra_x^{1/4}}{[1+(0.492/Pr)^{9/16}]^{4/9}}$$
- Horizontal Cylinder (average):
$$Nu_D = C \, Ra_D^m$$
(e.g., $$\displaystyle 10^4 < Ra_D < 10^7 $$: $$\displaystyle C=0.53 $$, $$\displaystyle m=1/4 $$).
[!TIP]
- Forced vs. Natural: Check $$\displaystyle Gr/Re^2 $$: if $$\displaystyle > 0.1 $$, natural convection significant.
- Correlation Selection: Ensure geometry, $Re$, $Pr$ range match.
V. Radiation Heat Transfer
Fundamental Concepts
-
Black Body: Ideal emitter/absorber ($$\displaystyle \varepsilon = \alpha = 1 $$).
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Gray Body: $\varepsilon$, $\alpha$ constant (independent of $\lambda$), $$\displaystyle <1 $$.
Radiation Between Surfaces
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Shape Factor (View Factor) $$\displaystyle F_{i\to j} $$: Fraction of radiation leaving surface $i$ that strikes $j$ directly.
-
Properties:
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Reciprocity: $$\displaystyle A_i F_{i\to j} = A_j F_{j\to i} $$.
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Summation: $$\displaystyle \sum_{j=1}^N F_{i\to j} = 1 $$.
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Symmetry: $$\displaystyle F_{i\to j} = F_{i\to j'} $$ if $j$, $j'$ symmetric w.r.t. $i$.
-
Reciprocity Theorem Derivation
Consider differential areas $$\displaystyle dA_i $$, $$\displaystyle dA_j $$:
$$dF_{i\to j} = \frac{\cos \theta_i \cos \theta_j}{\pi S^2} dA_j$$
Integrate:
$$F_{i\to j} = \frac{1}{A_i} \int_{A_i} \int_{A_j} \frac{\cos \theta_i \cos \theta_j}{\pi S^2} dA_j dA_i$$
Swap integration order:
$$A_i F_{i\to j} = \int_{A_j} \int_{A_i} \frac{\cos \theta_i \cos \theta_j}{\pi S^2} dA_i dA_j = A_j F_{j\to i}$$
Thus, $$\displaystyle \boxed{A_i F_{i\to j} = A_j F_{j\to i}} $$.
Shape Factor Derivations
- Parallel Plates (equal area $A$, spaced $L$ apart, $L \gg$ dimensions):
$$F_{1\to2} = 1, \quad F_{2\to1} = 1$$
- Perpendicular Plates (edge-to-edge):
$$F_{1\to2} = \frac{1}{2} \left[ 1 + \frac{X^2+Y^2-1}{XY\sqrt{1+X^2+Y^2}} \right]$$
where $$\displaystyle X = a/L $$, $$\displaystyle Y = b/L $$.
- Cylinder to Coaxial Disk:
$$F_{1\to2} = \frac{1}{2} \left[ X \sqrt{X^2-1} - \ln(X + \sqrt{X^2-1}) \right]$$
where $$\displaystyle X = L/r + 1 $$.
Net Radiation Exchange
- Between Black Bodies ($i$ and $j$):
$$Q_{i\to j} = \frac{\sigma (T_i^4 - T_j^4)}{\frac{1}{A_i F_{i\to j}}}$$
- Between Gray Bodies (using Radiosity $$\displaystyle J_i $$ and Irradiation $$\displaystyle G_i $$):
$$J_i = \varepsilon_i \sigma T_i^4 + (1-\varepsilon_i) G_i$$
$$G_i = \sum_{j=1}^N F_{i\to j} J_j$$
Solve linear system for $$\displaystyle J_i $$, then $$\displaystyle Q_i = A_i (J_i - G_i) $$.
Special Cases
-
Hemispherical Cavity (radius $R$, emissivity $\varepsilon$, inner surface $T$):
Radiation leaving opening = black body radiation from a surface of area $$\displaystyle \pi R^2 $$:
$$Q = \varepsilon \sigma (\pi R^2) T^4$$
(since cavity acts like black body for $L \gg R$).
- Large Parallel Plates (1 & 2, $$\displaystyle \varepsilon_1 $$, $$\displaystyle \varepsilon_2 $$):
$$Q_{12} = \frac{\sigma (T_1^4 - T_2^4)}{\frac{1}{\varepsilon_1} + \frac{1}{\varepsilon_2} - 1} \cdot A$$
[!TIP]
- Radiation Shield: Two shields reduce heat transfer to $\approx 1/3$ of single-plate case.
- Common Error: Forgetting reciprocity when $$\displaystyle A_i \neq A_j $$.
VI. Heat Exchangers
Classification
| Type | Diagram | Characteristics |
|---|---|---|
| Parallel Flow | DiagramSEARCH: parallel flow heat exchanger diagram |
Both fluids same direction; lower LMTD. |
| Counter Flow | DiagramSEARCH: counter flow heat exchanger diagram |
Opposite direction; higher LMTD, more efficient. |
| Cross Flow | DiagramSEARCH: cross flow heat exchanger diagram |
Fluids perpendicular; often use $\varepsilon$-NTU method. |
| Shell-and-Tube | DiagramSEARCH: shell and tube heat exchanger |
One fluid in tubes, other in shell; versatile. |
| Plate | DiagramSEARCH: plate heat exchanger |
High area/volume; gasketed, easy maintenance. |
LMTD Method
- Definition:
$$\Delta T_{lm} = \frac{\Delta T_1 - \Delta T_2}{\ln(\Delta T_1 / \Delta T_2)}$$
where $$\displaystyle \Delta T_1 $$, $$\displaystyle \Delta T_2 $$ are temperature differences at each end.
-
Parallel Flow:
$$\displaystyle \Delta T_1 = T_{h,in} - T_{c,in} $$, $$\displaystyle \Delta T_2 = T_{h,out} - T_{c,out} $$.
-
Counter Flow:
$$\displaystyle \Delta T_1 = T_{h,in} - T_{c,out} $$, $$\displaystyle \Delta T_2 = T_{h,out} - T_{c,in} $$.
-
Derivation: From energy balance and $$\displaystyle \frac{dT}{dx} \propto \Delta T $$, integrate:
$$Q = U A \Delta T_{lm}$$
Design/Analysis
Given $U$, $A$, flow rates, inlet $T$:
-
Calculate $$\displaystyle C_{min} $$, $$\displaystyle C_{max} $$ ($$\displaystyle C = \dot{m} c_p $$).
-
Compute $$\displaystyle \Delta T_1 $$, $$\displaystyle \Delta T_2 $$ based on flow arrangement.
-
Find $$\displaystyle \Delta T_{lm} $$.
-
$$\displaystyle Q = U A \Delta T_{lm} = C_{min} (T_{c,out} - T_{c,in}) $$ (or hot side).
-
Solve for unknown exit temperature.
Fouling
-
Definition: Deposition of scales, corrosion products on heat transfer surfaces.
-
Effects: Increases thermal resistance → $U$ decreases, $Q$ drops, pressure drop increases.
-
Fouling Factor $$\displaystyle R_f $$: Added resistance in $$\displaystyle 1/U = 1/U_{clean} + R_f $$.
Temperature Profiles
-
Parallel Flow: Both fluids approach same exit T; $\Delta T$ decreases along length.
-
Counter Flow: Can achieve outlet $$\displaystyle T_{c,out} > T_{h,out} $$; $\Delta T$ more uniform.
-
Equal Slope Condition: When $$\displaystyle C_h = C_c $$ (heat capacity rates equal), temperature lines are parallel in counter flow.
[!TIP]
- LMTD Correction: For cross flow, use correction factor $F$: $$\displaystyle Q = U A F \Delta T_{lm} $$.
- Exam Tip: Always sketch temperature profiles to identify $$\displaystyle \Delta T_1 $$, $$\displaystyle \Delta T_2 $$.
VII. Extended Surfaces (Fins)
Purpose & Applications
-
Increase surface area to enhance heat transfer from small base areas.
-
Used in: radiators, engine cylinders, electronic cooling, heat exchangers.
Types
- Straight (rectangular, cylindrical), annular, pin.
Governing Equation (Straight Fin, Uniform Cross-Section)
Assumptions: steady, 1D, constant $k$, $h$, no radiation.
- Energy Balance on differential element:
$$-k A_c \frac{dT}{dx} + h P (T - T_\infty) dx = \frac{d}{dx} \left( -k A_c \frac{dT}{dx} dx \right)$$
where $$\displaystyle A_c $$ = cross-sectional area, $P$ = perimeter.
- Simplified:
$$\frac{d^2T}{dx^2} - m^2 (T - T_\infty) = 0$$
where $$\displaystyle \boxed{m^2 = \frac{h P}{k A_c}} $$.
Boundary Conditions
-
Base: $$\displaystyle T(0) = T_b $$.
-
Tip:
-
Convective: $$\displaystyle -k A_c \left. \frac{dT}{dx} \right|_{x=L} = h A_t (T_L - T_\infty) $$.
-
Insulated: $$\displaystyle \left. \frac{dT}{dx} \right|_{x=L} = 0 $$.
-
Infinite Fin: $$\displaystyle T(L) = T_\infty $$.
-
Solution & Performance Parameters
- Temperature Distribution (insulated tip):
$$\frac{T(x) - T_\infty}{T_b - T_\infty} = \frac{\cosh[m(L-x)]}{\cosh(mL)}$$
- Fin Efficiency $$\displaystyle \eta_f $$:
$$\eta_f = \frac{Q_{actual}}{Q_{if\,no\,fin}} = \frac{\tanh(mL)}{mL} \quad \text{(insulated tip)}$$
$$\eta_f = \frac{\sinh(mL)}{\cosh(mL) + (h/(m k)) \sinh(mL)} \quad \text{(convective tip)}$$
- Fin Effectiveness $$\displaystyle \varepsilon_f $$:
$$\varepsilon_f = \frac{Q_{actual}}{Q_{without\,fin}} = \eta_f \frac{A_f}{A_b}$$
where $$\displaystyle A_f = A_b + P L $$ (rectangular).
[!TIP]
- Efficiency Limit: $$\displaystyle \eta_f \approx 1/(mL) $$ for $$\displaystyle mL > 2 $$; fin too long → diminishing returns.
- Common Mistake: Using $mL$ with $L$ as total length, not exposed length.
VIII. Mass Transfer
Analogy with Heat Transfer
| Heat Transfer | Mass Transfer |
|---|---|
| Temperature $T$ | Concentration $C$ |
| Heat flux $q''$ | Mass flux $j''$ |
| Fourier’s law: $$\displaystyle q'' = -k \nabla T $$ | Fick’s first law: $$\displaystyle j'' = -D \nabla C $$ |
| Thermal diffusivity $$\displaystyle \alpha = k/(\rho c_p) $$ | Mass diffusivity $D$ |
Modes
-
Diffusion: Molecular motion (Fick’s laws).
-
Convection: Bulk motion + diffusion.
Fick’s Laws
-
First Law (steady diffusion): $$\displaystyle j'' = -D \frac{dC}{dx} $$.
-
Second Law (transient): $$\displaystyle \frac{\partial C}{\partial t} = D \nabla^2 C $$.
Convective Mass Transfer
- Mass Transfer Coefficient $$\displaystyle h_m $$:
$$j'' = h_m (C_s - C_\infty)$$
- Analogy (Chilton-Colburn):
$$St_h \cdot Pr^{2/3} = St_m \cdot Sc^{2/3}$$
where $$\displaystyle St_m = \frac{h_m}{U} $$, $$\displaystyle Sc = \nu/D $$.
Binary Mixtures
For ideal gas: $$\displaystyle p_i V = n_i R T $$ → $$\displaystyle C_i = \frac{p_i}{R T} $$ (molar concentration).
-
Mass Density $$\displaystyle \rho_i = C_i M_i $$.
-
Mass Fraction $$\displaystyle Y_i = \frac{\rho_i}{\rho} = \frac{p_i M_i}{p M_{avg}} $$.
-
Molar Fraction $$\displaystyle x_i = \frac{p_i}{p} $$.
Example (O₂/N₂, $$\displaystyle p=1.1 $$ bar, $$\displaystyle T=15^\circ $$C, $$\displaystyle p_{O_2}:p_{N_2}=0.21:0.79 $$):
-
$$\displaystyle p_{O_2} = 0.21 \times 1.1 = 0.231 $$ bar, $$\displaystyle p_{N_2} = 0.869 $$ bar.
-
$$\displaystyle C_{O_2} = p_{O_2}/(R T) $$, $$\displaystyle R=8314 $$ J/kmol·K, $$\displaystyle T=288 $$ K.
-
$$\displaystyle M_{O_2}=32 $$, $$\displaystyle M_{N_2}=28 $$ → $$\displaystyle M_{avg} = 0.21\times32 + 0.79\times28 = 28.84 $$ kg/kmol.
-
$$\displaystyle \rho_{O_2} = C_{O_2} M_{O_2} $$, etc.
General Equation of Mass Diffusion (Stationary Medium)
For species $A$ in mixture:
$$\frac{\partial C_A}{\partial t} = D \nabla^2 C_A + \text{source/sink terms}$$
Derived from species continuity + Fick’s first law.
[!TIP]
- Mass Average Velocity: $$\displaystyle v = \sum Y_i v_i $$; used in convective term.
- Exam Problem: Often ask to compute $$\displaystyle x_i $$, $$\displaystyle Y_i $$, $$\displaystyle \rho_i $$ from partial pressures.
IX. Dimensional Analysis
Buckingham Pi Theorem
-
Statement: If a physical relation involves $n$ variables and $r$ fundamental dimensions, the relation can be expressed as a function of $(n-r)$ independent dimensionless $\pi$ terms.
-
Steps:
-
List all variables ($n$).
-
Choose $r$ repeating variables (include all dimensions, independent).
-
Form $\pi$ terms: $$\displaystyle \pi = (\text{non-repeating}) \times (\text{repeating})^a $$.
-
Determine exponents by dimensional homogeneity.
-
Write functional relation: $$\displaystyle F(\pi_1, \pi_2, ...) = 0 $$.
-
Application to Forced Convection (as in Section IV)
-
Variables: $$\displaystyle h, L, k, \mu, c_p, \rho, U $$ → $$\displaystyle n=7 $$, $$\displaystyle r=4 $$ ($M, L, T, \Theta$) → $3$ $\pi$ terms.
-
Repeating: $L, k, \mu, \rho$.
-
$$\displaystyle \pi_1 = h L / k = Nu $$, $$\displaystyle \pi_2 = \rho U L / \mu = Re $$, $$\displaystyle \pi_3 = \mu c_p / k = Pr $$.
-
Relation: $$\displaystyle \boxed{Nu = f(Re, Pr)} $$.
Dimensionless Groups
-
$Re$: Flow regime.
-
$Pr$: Relative thickness of velocity/thermal boundary layers.
-
$Nu$: Convective/conductive heat transfer.
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$Gr$, $Ra$: Natural convection strength.
-
$$\displaystyle Sc = \nu/D $$: Mass transfer analog of $Pr$.
-
$$\displaystyle Sh = h_m L / D $$: Mass transfer analog of $Nu$.
Advantages & Limitations
| Advantages | Limitations |
|---|---|
| Reduces number of variables | Does not give exact functional form |
| Guides experimental design | Constants depend on variable choice |
| Predicts correlation form | Cannot account for all physics (e.g., radiation) |
[!TIP]
- Choosing Repeating Variables: Must include all dimensions; avoid dimensionless groups.
- Common Pitfall: Using $h$, $T$ as repeating variables (they are dependent).
X. Boiling and Condensation
Boiling
-
Pool Boiling Curve (surface $$\displaystyle T_s $$ vs. $q''$):
-
Natural Convection ($$\displaystyle T_s < T_{sat} $$): $q''$ increases with $\Delta T$.
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Nucleate Boiling: Bubbles form at nucleation sites; $q''$ high, $\Delta T$ moderate (5–30°C).
-
Critical Heat Flux (CHF): Maximum $q''$ before film boiling; burnout point.
-
Transition Boiling: Unstable, $q''$ drops.
-
Film Boiling: Stable vapor film; $q''$ increases again with $\Delta T$ (Leidenfrost effect).
-
-
Mechanisms:
-
Nucleate: Micro-convection, latent heat removal by bubbles.
-
Film: Vapor film insulates; heat transfer by conduction/radiation through vapor.
-
Condensation
-
Film Condensation:
- Nusselt’s Theory (laminar film, vertical plate):
$$q'' = 0.943 \left[ \frac{\rho_l (\rho_l - \rho_v) g h_{fg} k_l^3 \Delta T}{\mu_l L} \right]^{1/4}$$
for vertical plate of height $L$.
- Horizontal Tube:
$$q'' = 0.725 \left[ \frac{\rho_l (\rho_l - \rho_v) g h_{fg} k_l^3 \Delta T}{\mu_l D} \right]^{1/4}$$
-
Dropwise Condensation:
-
Droplets form, coalesce, fall; bare surface exposed → higher $h$ (5–10× film).
-
Requires hydrophobic surface treatment; hard to maintain.
-
Comparison
| Film Condensation | Dropwise Condensation |
|---|---|
| Continuous liquid film | Discrete droplets |
| Lower $h$ (~1000 W/m²·K) | Higher $h$ (~5000–10,000 W/m²·K) |
| Reliable, sustained | Requires surface treatment, unstable |
[!TIP]
- Boiling Curve: Remember regimes and CHF.
- Condensation: Nusselt’s formulas for vertical plate/tube are key.
END OF UNIT 1 NOTES
These notes synthesize all high-frequency topics from RGPV past papers (2023–2025). Focus on boxed formulas and derivations for 8-mark questions.