4. Introduction to Heat & Mass Transfer. This section will cover the following
concepts: • A rudimentary introduction to mass transfer. • Mass transfer from a ...
4. Introduction to Heat & Mass Transfer This section will cover the following concepts: • A rudimentary introduction to mass transfer. • Mass transfer from a molecular point of view. • Fundamental similarity of heat and mass transfer. • Application of mass transfer concepts: - Evaporation of a liquid layer - Evaporation of a liquid droplet
4. Heat & Mass Transfer
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Mass Transfer: Mass-Transfer Rate Laws: • Fick’s Law of Diffusion: Describes, in its basic form, the rate at which two gas species diffuse through each other. • For one-dimensional binary diffusion: m ˙A , 1
mass flow of A per unit area
4. Heat & Mass Transfer
= YA (m ˙ A+m ˙ B) − , 1 mass flow of A associated with bulk flow per unit area
2
dYA ρDAB , dx1
mass flow of A associated with molecular diffusion
(4.1)
AER 1304–ÖLG
• A is transported by two means: (a) bulk motion of the fluid, and (b) molecular diffusion. • Mass flux is defined as the mass flowrate of species A per unit area perpendicular to the flow: m ˙A=m ˙ A /A
(4.2)
m ˙ A has the units kg/(s m2 ). • The binary diffusivity, or the molecular diffusion coefficient, DAB is a property of the mixture and has units of m2 /s. 4. Heat & Mass Transfer
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• In the absence of diffusion: m ˙ A = YA (m ˙ A+m ˙ B ) = YA m ˙ ≡ Bulk flux of species A
(4.3a)
where m ˙ is the mixture mass flux. • The diffusional flux adds an additional component to the flux of A: dYA −ρDAB ≡ Diffusional flux of A, m ˙ A,diff dx (4.3b) 4. Heat & Mass Transfer
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• Note that the negative sign causes the flux to be postive in the x-direction when the concentration gradient is negative. • Analogy between the diffusion of heat (conduction) and molecular diffusion. - Fourier’s law of heat conduction: dT ˙ Qx = −k (4.4) dx • Both expressions indicate a flux (m ˙ A,diff or Q˙ x ) being proportional to the gradient of a scalar quantity [(dYA /dx) or (dT /dx)]. 4. Heat & Mass Transfer
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• A more general form of Eqn 4.1: −→ −→ −→ ˙ A+m ˙ B ) − ρDAB ∇YA m ˙ A = YA (m
(4.5)
symbols with over arrows represent vector quantities. Molar form of Eqn 4.5 −→ −→ −→ N˙ A = χA (N˙ A + N˙ B ) − cDAB ∇χA
(4.6)
where N˙ A , (kmol/(s m2 ), is the molar flux of species A; χA is mole fraction, and c is the molar concentration, kmol/m3 . 4. Heat & Mass Transfer
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• Meanings of bulk flow and diffusional flux can be better explained if we consider that: m ˙ = m ˙A + m ˙B , 1 , 1 , 1
mixture mass flux
species A mass flux
(4.7)
species B mass flux
• If we substitute for individual species fluxes from Eqn 4.1 into 4.7: dYA dYB m ˙ = YA m ˙ − ρDAB + YB m ˙ − ρDBA dx dx (4.8a) 4. Heat & Mass Transfer
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• Or: dYA dYB m ˙ = (YA + YB )m ˙ − ρDAB − ρDBA dx dx (4.8b) • For a binary mixture, YA + YB = 1; then: dYA dYB − ρDAB − ρDBA =0 , dx1 , dx1 diffusional flux of species A
• In general
4. Heat & Mass Transfer
(4.9)
diffusional flux of species B
m ˙i =0 8
AER 1304–ÖLG
• Some cautionary remarks: - We are assuming a binary gas and the diffusion is a result of concentration gradients only (ordinary diffusion). - Gradients of temperature and pressure can produce species diffusion. - Soret effect: species diffusion as a result of temperature gradient. - In most combustion systems, these effects are small and can be neglected.
4. Heat & Mass Transfer
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Molecular Basis of Diffusion: • We apply some concepts from the kinetic theory of gases. - Consider a stationary (no bulk flow) plane layer of a binary gas mixture consisting of rigid, non-attracting molecules. - Molecular masses of A and B are identical. - A concentration (mass-fraction) gradient exists in x-direction, and is sufficiently small that over smaller distances the gradient can be assumed to be linear. 4. Heat & Mass Transfer
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4. Heat & Mass Transfer
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• Average molecular properties from kinetic of gases: p 8k T Q1/2 Mean speed B of species A v¯ ≡ molecules = πmA pn Q Wall collision 1 A frequency of A ZA ≡ molecules per unit area = v¯ 4 V 1 λ ≡ Mean free path = √ 2π(ntot /V )σ 2 Average perpendicular distance 2 from plane of last collision to a ≡ plane where next collision occurs = λ 3 4. Heat & Mass Transfer
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theory
(4.10a) (4.10b) (4.10c) (4.10d)
AER 1304–ÖLG
-
where kB : Boltzmann’s constant. mA : mass of a single A molecule. (nA /V ): number of A molecules per unit volume. (ntot /V ): total number of molecules per unit volume. σ: diameter of both A and B molecules.
• Net flux of A molecules at the x-plane: m ˙A=m ˙ A,(+)x−dir − m ˙ A,(−)x−dir 4. Heat & Mass Transfer
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(4.11)
AER 1304–ÖLG
• In terms of collision frequency, Eqn 4.11 becomes m ˙A , 1
Net mass flux of species A
=
(ZA )x−a , 1
mA −
Number of A crossing plane x originating from plane at (x−a)
(ZA )x+a , 1
mA
Number of A crossing plane x originating from plane at (x+a)
(4.12) • Since ρ ≡ mtot /Vtot , then we can relate ZA to mass fraction, YA (from Eqn 4.10b) 1 nA mA 1 ZA mA = ρ¯ v = YA ρ¯ v 4 mtot 4
4. Heat & Mass Transfer
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(4.13)
AER 1304–ÖLG
• Substituting Eqn 4.13 into 4.12 1 m ˙ A = ρ¯ v (YA,x−a − YA,x+a ) 4
(4.14)
• With linear concentration assumption dY YA,x−a − YA,x+a = dx 2a YA,x−a − YA,x+a = 4λ/3
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(4.15)
AER 1304–ÖLG
• From the last two equations, we get v¯λ dYA m ˙ A = −ρ 3 dx
(4.16)
• Comparing Eqn. 3.16 with Eqn. 3.3b, DAB is DAB = v¯λ/3
(4.17)
• Substituting for v¯ and λ, along with ideal-gas equation of state, P V = nkB T 3 2 p kB T Q1/2 T DAB = (4.18a) 3 2 3 π mA σ P 4. Heat & Mass Transfer
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or DAB ∝ T 3/2 P −1
(4.18b)
• Diffusivity strongly depends on temperature and is inversely proportional to pressure. • Mass flux of species A, however, depends on ρDAB , which then gives: ρDAB ∝ T 1/2 P 0 = T 1/2
(4.18c)
• In some practical/simple combustion calculations, the weak temperature dependence is neglected and ρD is treated as a constant. 4. Heat & Mass Transfer
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Comparison with Heat Conduction: • We apply the same kinetic theory concepts to the transport of energy. • Same assumptions as in the molecular diffusion case. • v¯ and λ have the same definitions. • Molecular collision frequency is now based on the total number density of molecules, ntot /V , p Q 1 ntot Average wall collision Z = frequency per unit area = v¯ (4.19) 4 V 4. Heat & Mass Transfer
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4. Heat & Mass Transfer
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• In the no-interaction-at-a-distance hard-sphere model of the gas, the only energy storage mode is molecular translational (kinetic) energy. • Energy balance at the x-plane; Net energy flow in x−direction
=
kinetic energy flux with molecules from x−a to x
−
kinetic energy flux with molecules from x+a to x
Q˙ x = Z (ke)x−a − Z (ke)x+a • ke is given by
4. Heat & Mass Transfer
3 1 2 v = kB T ke = m¯ 2 2 20
(4.20)
(4.21)
AER 1304–ÖLG
heat flux can be related to temperature as 3 ˙ Qx = kB Z (Tx−a − Tx+a ) 2
(4.22)
• The temperature gradient dT Tx+a − Tx−a = dx 2a
(4.23)
• Eqn. 4.23 into 3.22, and definitions of Z and a p n Q dT 1 Q˙ x = − kB v¯λ (4.24) 2 V dx 4. Heat & Mass Transfer
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Comparing to Eqn. 4.4, k is Q p 1 n k = kB v¯λ 2 V
(4.25)
• In terms of T and molecular size, p k3 Q1/2 1/2 B k= T π 3 mσ 4
(4.26)
• Dependence of k on T (similar to ρD) k ∝ T 1/2
(4.27)
- Note: For real gases T dependency is larger. 4. Heat & Mass Transfer
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4. Heat & Mass Transfer
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Species Conservation: • One-dimensional control volume • Species A flows into and out of the control volume as a result of the combined action of bulk flow and diffusion. • Within the control volume, species A may be created or destroyed as a result of chemical reaction. • The net rate of increase in the mass of A within the control volume relates to the mass fluxes and reaction rate as follows:
4. Heat & Mass Transfer
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AER 1304–ÖLG
dmA,cv dt , 1
Rate of increase of mass A within CV
= [m ˙ A A]x − [m ˙ A A]x+∆x + m ˙ AV , 1 , 1 , 1 Mass flow of A into CV
Mass flow of A out of the CV
Mass prod. rate of A by reaction
(4.28)
- where - m ˙ A is the mass production rate of species A per unit volume. - m ˙ A is defined by Eqn. 4.1.
4. Heat & Mass Transfer
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• Within the control volume mA,cv = YA mcv = YA ρVcv , and the volume Vcv = A · ∆x; Eqn. 4.28 ∂(ρYA ) ∂YA = A∆x = A YA m ˙ − ρDAB ∂t ∂x x = ∂YA A YA m ˙ − ρDAB +m ˙ A A∆x ∂x x+∆x (4.29) • Dividing by A∆x and taking limit as ∆x → 0, ∂(ρYA ) ∂ ∂YA = =− YA m ˙ − ρDAB +m ˙A ∂t ∂x ∂x (4.30) 4. Heat & Mass Transfer
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• For the steady-flow, d dYA = YA m ˙ − ρDAB =0 m ˙A− dx dx
(4.31)
• Eqn. 4.31 is the steady-flow, one-dimensional form of species conservation for a binary gas mixture. For a multidimensional case, Eqn. 4.31 can be generalized as −→ m ˙A − ∇·m ˙A = 0 (4.32) , 1 , 1 Net rate of species A production by chemical reaction
4. Heat & Mass Transfer
Net flow of species A out of control volume
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Some Applications of Mass Transfer: The Stefan Problem:
4. Heat & Mass Transfer
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• Assumptions: - Liquid A in the cylinder maintained at a fixed height. - Steady-state - [A] in the flowing gas is less than [A] at the liquid-vapour interface. - B is insoluble in liquid A • Overall conservation of mass: ˙ A+m ˙B m ˙ (x) = constant = m
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(4.33)
AER 1304–ÖLG
Since m ˙ B = 0, then m ˙A=m ˙ (x) = constant Then, Eqn.4.1
(4.34)
now becomes
dYA m ˙ A = YA m ˙ A − ρDAB dx
(4.35)
Rearranging and separating variables m ˙A dYA − dx = ρDAB 1 − YA 4. Heat & Mass Transfer
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(4.36)
AER 1304–ÖLG
Assuming ρDAB to be constant, integrate Eqn. 4.36 m ˙A − x = − ln[1 − YA ] + C (4.37) ρDAB With the boundary condition YA (x = 0) = YA,i
(4.38)
We can eliminate C; then m = ˙ Ax YA (x) = 1 − (1 − YA,i ) exp ρDAB 4. Heat & Mass Transfer
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(4.39)
AER 1304–ÖLG
• The mass flux of A, m ˙ A , can be found by letting YA (x = L) = YA,∞ Then, Eqn. 4.39 reads ρDAB 1 − YA,∞ = m ˙A= ln L 1 − YA,i
(4.40)
• Mass flux is proportional to ρD, and inversely proportional to L.
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Liquid-Vapour Interface: • Saturation pressure PA,i = Psat (Tliq,i )
(4.41)
• Partial pressure can be related to mole fraction and mass fraction YA,i
Psat (Tliq,i ) M WA = P M Wmix,i
(4.42)
- To find YA,i we need to know the interface temperature. 4. Heat & Mass Transfer
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• In crossing the liquid-vapour boundary, we maintain continuity of temperature Tliq,i (x = 0− ) = Tvap,i (x = 0+ ) = T (0) (4.43) and energy is conserved at the interface. Heat is transferred from gas to liquid, Q˙ g−i . Some of this heats the liquid, Q˙ i−l , while the remainder causes phase change. Q˙ g−i − Q˙ i−l = m(h ˙ vap − hliq ) = mh ˙ fg (4.44) or
Q˙ net = mh ˙ fg 4. Heat & Mass Transfer
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(4.45) AER 1304–ÖLG
Droplet Evaporation:
4. Heat & Mass Transfer
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AER 1304–ÖLG
• Assumptions: - The evaporation process is quasi-steady. - The droplet temperature is uniform, and the temperature is assumed to be some fixed value below the boiling point of the liquid. - The mass fraction of vapour at the droplet surface is determined by liquid-vapour equilibrium at the droplet temperature. - We assume constant physical properties, e.g., ρD.
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Evaporation Rate: • Same approach as the Stefan problem; except change in coordinate sysytem. • Overall mass conservation: m(r) ˙ = constant = 4πr2 m ˙
(4.46)
• Species conservation for the droplet vapour: dYA m ˙ A = YA m ˙ A − ρDAB dr
4. Heat & Mass Transfer
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(4.47)
AER 1304–ÖLG
• Substitute Eqn. 4.46 into 4.47 and solve for m, ˙ ρDAB dYA m ˙ = −4πr 1 − YA dr 2
(4.48)
• Integrating and applying the boundary condition YA (r = rs ) = YA,s
(4.49)
- yields (1 − YA,s ) exp [−m/(4πρD ˙ AB r) YA (r) = 1 − exp [−m/(4πρD ˙ AB rs )] (4.50) 4. Heat & Mass Transfer
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AER 1304–ÖLG
• Evaporation rate can be determined from Eqn. 4.50 by letting YA = YA,∞ for r → ∞: (1 − Y
= ) A,∞ m ˙ = 4πrs ρDAB ln (1 − YA,s )
(4.51)
• In Eqn. 4.51, we can define the dimensionless transfer number, BY , 1 − YA,∞ 1 + BY ≡ 1 − YA,s 4. Heat & Mass Transfer
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(4.52a)
AER 1304–ÖLG
or
YA,s − YA,∞ BY = 1 − YA,s
• Then the evaporation rate is
m ˙ = 4πrs ρDAB ln (1 + BY )
• Droplet Mass Conservation: dmd = −m ˙ dt where md is given by md = ρl V = ρl πD3 /6 4. Heat & Mass Transfer
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(4.52b)
(4.53)
(4.54)
(4.55) AER 1304–ÖLG
where D = 2rs , and V is the volume of the droplet. • Substituting Eqns 4.55 and 4.53 into 4.54 and differentiating dD 4ρDAB =− ln (1 + BY ) dt ρl D
(4.56)
• Eqn 4.56 is more commonly expressed in term of D2 rather than D, dD2 8ρDAB =− ln (1 + BY ) dt ρl 4. Heat & Mass Transfer
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(4.57)
AER 1304–ÖLG
• Equation 4.57 tells us that time derivative of the square of the droplet diameter is constant. D2 varies with t with a slope equal to RHS of Eqn.4.57. This slope is defined as evaporation constant K: 8ρDAB K= ln (1 + BY ) (4.58) ρl • Droplet evaporation time can be calculated from: 80
dD2 = −
Kdt
(4.59)
0
Do2 4. Heat & Mass Transfer
8td
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AER 1304–ÖLG
which yields td = Do2 /K
(4.60)
• We can change the limits to get a more general relationship to provide a general expression for the variation of D with time: D2 (t) = Do2 − Kt
(4.61)
• Eq. 4.61 is referred to as the D2 law for droplet evaporation.
4. Heat & Mass Transfer
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AER 1304–ÖLG
D2 law for droplet evaporation:
4. Heat & Mass Transfer
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