Chapter2 Introduction to Conduction · – There are no moving parts in conductive heat transfer....
Transcript of Chapter2 Introduction to Conduction · – There are no moving parts in conductive heat transfer....
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Chapter2Introduction to Conduction
• Conduction is the transfer of energy from
OverviewCo duct o s t e t a s e o e e gy othe more energetic to the less energetic particles of a substance due to interactions between the particles.– There must be a thermal gradient in a stationary
(no moving parts) medium (solid/liquid/gas). – There are no moving parts in conductive heat
transfer. Most problems dealing with conduction involve solids.
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• Conduction is governed by Fourier’s Law: (heat rate)ddTkAqx −=
The Conduction Rate EquationConduction is governed by Fourier s Law: (heat rate)
• For the heat flux:
where k = the thermal conductivity (W/m·K), A = the area of the object (m2), dT/dx = temperature gradient of the object.
• Since heat flux is a vector quantity, a more general statement of Fourier’s Law (conduction rate equation) is:
dxqx
dxdTkqx −=′′
⎟⎟⎞
⎜⎜⎛
++−=∇−=′′dTkdTjdTikTkq( q )
– where is the three-dimensional del operator and T(x,y,z) is the scalar temperature field.
• From the previous equations it follows that:
⎟⎟⎠
⎜⎜⎝
++∇dz
kdy
jdx
ikTkq
∇
dxdTkqx −=′′
dydTkqy −=′′
dzdTkqz −=′′
Heat Flux Components
• Cartesian Coordinates: ( ), ,T x y zT T Tq k i k j k kx y z
→ → → →∂ ∂ ∂′′ = − − −∂ ∂ ∂
xq′′ yq′′ zq′′
(2.3)
(2.22)T T Tq k i k j k kr r zφ
→ → → →∂ ∂ ∂′′ = − − −∂ ∂ ∂
rq′′ qφ′′ zq′′
• Cylindrical Coordinates: ( ), ,T r zφ
• Spherical Coordinates: ( ), ,T r φ θ
sinT T Tq k i k j k kr r rθ θ φ
→ → → →∂ ∂ ∂′′ = − − −∂ ∂ ∂
(2.25)
rq′′ qθ′′ qφ′′
Spherical Coordinates: ( ), ,φ
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Heat Flux Components (cont.)
In angular coordinates , the temperature gradient is still based on temperature change over a length scale and hence has units of °C/m and not °C/deg.
( ) or ,φ φ θ
• Heat rate for one-dimensional, radial conduction in a cylinder or sphere:
– Cylinder2r r r rq A q rLqπ′′ ′′= =
or,2r r r rq A q rqπ′ ′ ′′ ′′= =
– Sphere– Sphere24r r r rq A q r qπ′′ ′′= =
Properties
Thermophysical PropertiesThermal Conductivity: A measure of a material’s ability to transfer thermal
energy by conduction.
Thermal Diffusivity: A measure of a material’s ability to respond to changesin its thermal environmentin its thermal environment.
•Property Tables:• Solids: Tables A.1 – A.3• Gases: Table A.4• Liquids: Tables A.5 – A.7
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• Physical Meaning
Thermal Conductivityy g
– property of the material, how quickly heat can be delivered• How to Determine k
– experimentally, determined from equations (example: k = -qx’’/ (∂T/∂x) )• How to Use It
– use k to find temperature distribution, which can then find the heat transfer in any direction
• For a given material: ks > kl >> kgh lid l li idwhere s: solid; l: liquid; g: gas.
• This is only true assuming that they (solid, liquid, gas) are all stationary and not moving.
• k is usually assumed to be constant but it can be a function of temperature, k = f(T)– If the material is non-isotropic, heat transfer is directional (direction dependent, such as a
composite), k = f(T,x,y,z). – Therefore for an isotropic material, k= f(T)
Properties (Micro- and Nanoscale Effects)
Micro- and Nanoscale Effects• Conduction may be viewed as a consequence of energy carrier (electron or
phonon) motion.
• For the solid state:1k Cc λ= (2 7)
• Energy carriers also collide with physical boundaries, affecting their propagation.External boundaries of a film of material
average energy carrier velocity, c < ∞.
3 mfpk Cc λ=
energy carrierspecific heat perunit volume.
mean free path → averagedistance traveled by an energycarrier before a collision.
(2.7)
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Properties (Micro- and Nanoscale Effects)
( )( )
For 1
1 2 3
1 3
mfp
x mfp
y mfp
L
k k L
k k L
λ
λ π
λ
<
= −
= −
/ ,/ // /
Grain boundaries within a solid
(2.9a)
(2.9b)
Measured thermal conductivity of a ceramic material vs. grain size, L. at 300K 25nm.mfp Tλ ≈ =
• Fourier’s law does not accurately describe the finite energy carrier propagation velocity. This limitation is not important except in problems involving extremely small time scales.
• Thermal diffusivity α is the ratio of the thermal conductivity to
Thermal Diffusivity Thermal diffusivity, α, is the ratio of the thermal conductivity to the heat capacity.
– where ρ=density, Cp = specific heat (heat required to raise one gram of material 1 K), and k = thermal conductivity
• Physical MeaningeHeatStorag
tionHeatConducT
tT
Ck
=Δ
Δ•=
ρα
• If k increases and Cp decreases, the thermal diffusivity of the material will increase
eHeatStoragtTCp
Δρ
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• Physical Meaning
Thermal Diffusivity (continued) Physical Meaning
– Several factors affect how fast heat will transfer through a material• Thermal Conductivity, k: the higher the value of a material’s heat conductivity, k,
the faster that heat will transfer through the material.• Heat Storage: when heat transfers through a material, some of the heat will be
stored in the material. Materials that have a large heat capacity will let more heat through than materials with a low heat capacity.
– Low Cp ↑Heat Transfer, ↓Heat Storage– High Cp ↓Heat Transfer, ↑ Heat Storage
• How Can We Determine It?
• How can We Use It?– The heat diffusion equation:
dtdTcq
dzdTk
dzd
dydTk
dyd
dxdTk
dxd
pρ=+⎟⎠⎞
⎜⎝⎛+⎟⎟
⎠
⎞⎜⎜⎝
⎛+⎟⎠⎞
⎜⎝⎛
• The heat diffusion equation: dtdTcq
dzdTk
dzd
dydTk
dyd
dxdTk
dxd
pρ=+⎟⎠⎞
⎜⎝⎛+⎟⎟
⎠
⎞⎜⎜⎝
⎛+⎟⎠⎞
⎜⎝⎛
The Heat Diffusion Equation q
• How did we get this equation?Derivation:T(t,x,y,z) = Temperature Distribution
dtdzdzdydydxdx ⎠⎝⎠⎝⎠⎝
Imagine a small cube of material as shown at right
Substituting gives
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The Heat Diffusion Equation (continued)
The Heat Diffusion Equation (continued)
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• 1
Simplifications: 1-D, stead state, constant properties
• 1.
• 2.
• 3.
Heat Equation (Radial Systems)
• Cylindrical Coordinates:
21 1
pT T T Tkr k k q c
r r r z z trρ
φ φ⎛ ⎞∂ ∂ ∂ ∂ ∂ ∂ ∂⎛ ⎞ ⎛ ⎞+ + + =⎜ ⎟⎜ ⎟ ⎜ ⎟∂ ∂ ∂ ∂ ∂ ∂ ∂⎝ ⎠ ⎝ ⎠⎝ ⎠
•(2.24)
• Spherical Coordinates:
22 2 2 2
1 1 1 sinsin sin p
T T T Tkr k k q cr r tr r r
θ ρφ φ θ θθ θ⎛ ⎞∂ ∂ ∂ ∂ ∂ ∂ ∂⎛ ⎞ ⎛ ⎞+ + + =⎜ ⎟⎜ ⎟ ⎜ ⎟∂ ∂ ∂ ∂ ∂ ∂ ∂⎝ ⎠ ⎝ ⎠⎝ ⎠
•(2.27)
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Heat Equation (Special Case)
One Dimensional Conduction in a Planar Medium with Constant Properties• One-Dimensional Conduction in a Planar Medium with Constant Propertiesand No Generation
2
21T T
tx α∂ ∂
=∂∂
thermal diffu osivit f the medy iumkα ≡ → ypcρ
Boundary Conditions
Boundary and Initial Conditions• For transient conduction, heat equation is first order in time, requiring
specification of an initial temperature distribution: ( ) ( )0, ,0tT x t T x= =
• Since heat equation is second order in space, two boundary conditionsmust be specified. Some common cases: Constant Surface Temperature:Constant Surface Temperature:
( )0, sT t T=
Constant Heat Flux:
T∂
Applied Flux Insulated Surface
T∂0|x s
Tk qx =
∂ ′′− =∂
0| 0xTx =
∂=
∂
Mixed surface condition:
( )0| 0,xTk h T T tx = ∞
∂− = −⎡ ⎤⎣ ⎦∂
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• For the 3-Dcase, 6 BCs and 1 IC are required to get the complete solution.
Boundary Conditions (BCs) and Initial Conditions (ICs)
For the 3 Dcase, 6 BCs and 1 IC are required to get the complete solution. However, a unique solution may still not be arrived at.
• E.g., the 1-Dimensional case:
Boundary Conditions (continued)( )1(0, )T t T t ⎫=
⎪
However:
1(0, ) ( )T t T t= ⎫⎪
0
( ) ill-defined w ith no unique solution
( , 0) ( )x
dT w tdx
T x f x=
⎪⎪= ⎬⎪⎪= ⎭
1
2
( , ) ( )( , ) ( ) well defined with a unique solution( ,0) ( )
T L t T tT x f x
⎫⎪= ⎬⎪= ⎭
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Conduction Analysis
Methodology of a Conduction Analysis
• Solve appropriate form of heat equation to obtain the temperature
• Consider possible micro- or nano-scale effects in problems involving verysmall physical dimensions or very rapid changes in heat or cooling rates.
• Solve appropriate form of heat equation to obtain the temperaturedistribution.
• Knowing the temperature distribution, apply Fourier’s Law to obtain theheat flux at any time, location and direction of interest.
• Applications:Applications:
Chapter 3: One-Dimensional, Steady-State ConductionChapter 4: Two-Dimensional, Steady-State ConductionChapter 5: Transient Conduction
Problem: Thermal Response of Plane Wall
Problem 2.46 Thermal response of a plane wall to convection heat transfer.
KNOWN: Plane wall, initially at a uniform temperature, is suddenly exposed to convective heating.
FIND: (a) Differential equation and initial and boundary conditions which may be used to find the temperature distribution, T(x,t); (b) Sketch T(x,t) for the following conditions: initial (t ≤ 0), steady-state (t → ∞), and two intermediate times; (c) Sketch heat fluxes as a function of time at the two surfaces; (d) Expression for total energy transferred to wall per unit volume (J/m3).
SCHEMATIC:
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Problem: Thermal Response (Cont).
ASSUMPTIONS: (1) One-dimensional conduction, (2) Constant properties, (3) No internal heat generation.
ANALYSIS: (a) For one-dimensional conduction with constant properties, the heat equation has the form,
2
2T 1 T
t x∂ ∂
α ∂∂=
( ) i
0
L
Initial, t 0 : T x,0 T uniform temperature
Boundaries: x=0 T/ x 0 adiabatic surface
x=L k T/ x = h T L
∂ ∂
∂ ∂
≤ =
=
− ( ),t T surface convection∞
⎧⎪⎪⎨⎪
⎡ − ⎤⎪ ⎣ ⎦⎩
and the conditions are:
(b) The temperature distributions are shown on the sketch.
Note that the gradient at x = 0 is always zero, since this boundary is adiabatic. Note also that the gradient at x = L decreases with time.
c) The heat flux, ( )xq x,t ,′′ as a function of time, is shown on the sketch for the surfaces x = 0 and x = L.
Problem: Thermal Response (Cont).
in conv s0E q A dt
∞′′= ∫
d) The total energy transferred to the wall may be expressed as
( )( )in s 0E hA T T L,t dt
∞∞= −∫
0
Dividing both sides by AsL, the energy transferred per unit volume is
( ) 3in0
E h T T L,t dt J/mV L
∞∞ ⎡ ⎤= −⎡ ⎤⎣ ⎦ ⎣ ⎦∫
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Problem 2.28 Surface heat fluxes, heat generation and total rate of radiationabsorption in an irradiated semi-transparent material with a
prescribed temperature distribution.
Problem: Non-uniform Generation due to Radiation Absorption
KNOWN: Temperature distribution in a semi-transparent medium subjected to radiative flux.
FIND: (a) Expressions for the heat flux at the front and rear surfaces, (b) The heat generation rate ( )q x , and (c) Expression for absorbed radiation per unit surface area.
SCHEMATIC:
Problem : Non-uniform Generation (Cont.)
ASSUMPTIONS: (1) Steady-state conditions, (2) One-dimensional conduction in medium, (3) Constant properties, (4) All laser irradiation is absorbed and can be characterized by an internal volumetric heat generation term ( )q x .
ANALYSIS: (a) Knowing the temperature distribution, the surface heat fluxes are found using Fourier’s law,
( ) -axx 2
dT Aq k k - a e Bdx k
⎡ ⎤⎡ ⎤′′ = − = − − +⎢ ⎥⎢ ⎥⎣ ⎦ ⎣ ⎦ 2dx ka⎢ ⎥⎢ ⎥⎣ ⎦ ⎣ ⎦
Front Surface, x=0: ( )xA Aq 0 k + 1 B kBka a
⎡ ⎤ ⎡ ⎤′′ = − ⋅ + = − +⎢ ⎥ ⎢ ⎥⎣ ⎦ ⎣ ⎦ <
Rear Surface, x=L: ( ) -aL -aLx
A Aq L k + e B e kB .ka a
⎡ ⎤ ⎡ ⎤′′ = − + = − +⎢ ⎥ ⎢ ⎥⎣ ⎦ ⎣ ⎦ <
(b) The heat diffusion equation for the medium is
d dT q d dT0 or q=-k
dx dx k dx dx⎛ ⎞ ⎛ ⎞+ =⎜ ⎟ ⎜ ⎟⎝ ⎠ ⎝ ⎠
( ) -ax -axd Aq x k e B Ae .dx ka
⎡ ⎤= − + + =⎢ ⎥⎣ ⎦
( c ) Performing an energy balance on the medium, in out gE E E 0− + =
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On a unit area basis
( ) ( ) ( )-aLg in out x x
AE E E q 0 q L 1 e .a
′′ ′′ ′′ ′′ ′′= − + = − + = + − <
Alternatively, evaluate gE′′ by integration over the volume of the medium,
Problem : Non-uniform Generation (Cont.)
( ) ( )LL L -ax -ax -aLg 0 0 0
A AE q x dx= Ae dx=- e 1 e .a a⎡ ⎤′′ = = −⎣ ⎦∫ ∫