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ME-701 · Heat and Mass Transfer/Quick Revision Short Notes

Heat and Mass Transfer (ME-701) - Unit 1 Short Notes

UNIT 1: Heat and Mass Transfer – Comprehensive Short Notes

(Aligned with RGPV Past Paper Analysis)


I. Fundamentals and Basic Concepts

Modes of Heat Transfer

  1. Conduction: Transfer due to temperature gradient in a medium (Fourier’s law).

  2. Convection: Transfer between solid surface and moving fluid (Newton’s law of cooling).

  3. 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).

  • 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: $$\displaystyle h, L, k, \mu, c_p, \rho, U $$. ($$\displaystyle n=7 $$)

  • 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 ($$\displaystyle \varepsilon = \alpha = 1 $$).

  • Gray Body: $\varepsilon$, $\alpha$ constant (independent of $\lambda$), $$\displaystyle <1 $$.

Radiation Between Surfaces

  • Shape Factor (View Factor) $$\displaystyle F_{i\to j} $$: Fraction of radiation leaving surface $i$ that strikes $j$ directly.

  • Properties:

    1. Reciprocity: $$\displaystyle A_i F_{i\to j} = A_j F_{j\to i} $$.

    2. Summation: $$\displaystyle \sum_{j=1}^N F_{i\to j} = 1 $$.

    3. 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

  1. Parallel Plates (equal area $A$, spaced $L$ apart, $L \gg$ dimensions):

$$F_{1\to2} = 1, \quad F_{2\to1} = 1$$

  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 $$\displaystyle X = a/L $$, $$\displaystyle Y = b/L $$.

  1. 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 $T$:

  1. Calculate $$\displaystyle C_{min} $$, $$\displaystyle C_{max} $$ ($$\displaystyle C = \dot{m} c_p $$).

  2. Compute $$\displaystyle \Delta T_1 $$, $$\displaystyle \Delta T_2 $$ based on flow arrangement.

  3. Find $$\displaystyle \Delta T_{lm} $$.

  4. $$\displaystyle Q = U A \Delta T_{lm} = C_{min} (T_{c,out} - T_{c,in}) $$ (or hot side).

  5. 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

  1. Base: $$\displaystyle T(0) = T_b $$.

  2. 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, $$\displaystyle p_{O_2}:p_{N_2}=0.21:0.79 $$):

  1. $$\displaystyle p_{O_2} = 0.21 \times 1.1 = 0.231 $$ bar, $$\displaystyle p_{N_2} = 0.869 $$ bar.

  2. $$\displaystyle C_{O_2} = p_{O_2}/(R T) $$, $$\displaystyle R=8314 $$ J/kmol·K, $$\displaystyle T=288 $$ K.

  3. $$\displaystyle M_{O_2}=32 $$, $$\displaystyle M_{N_2}=28 $$ → $$\displaystyle M_{avg} = 0.21\times32 + 0.79\times28 = 28.84 $$ kg/kmol.

  4. $$\displaystyle \rho_{O_2} = C_{O_2} M_{O_2} $$, 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:

    1. List all variables ($n$).

    2. Choose $r$ repeating variables (include all dimensions, independent).

    3. Form $\pi$ terms: $$\displaystyle \pi = (\text{non-repeating}) \times (\text{repeating})^a $$.

    4. Determine exponents by dimensional homogeneity.

    5. 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.

  • $Gr$, $Ra$: 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. $q''$):

    1. Natural Convection ($$\displaystyle T_s < T_{sat} $$): $q''$ increases with $\Delta T$.

    2. Nucleate Boiling: Bubbles form at nucleation sites; $q''$ high, $\Delta T$ moderate (5–30°C).

    3. Critical Heat Flux (CHF): Maximum $q''$ before film boiling; burnout point.

    4. Transition Boiling: Unstable, $q''$ drops.

    5. 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.

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