16a

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Overall Shell Energy Balance
Forms of Energy Generation:
(Se) 1. Degradation of electrical energy to heat
(Sn) 2. Heat from nuclear source (by fission)
(Sv) 3. Heat from viscous dissipation
Let S = rate of heat production
per unit volume (W/m3)
Energy
Generation
Electrical Heat Source
Consider an electrical wire
(solid cylinder):
Shell Heat Balance:
2πœ‹π‘ŸπΏπ‘žπ‘Ÿ
π‘Ÿ
− 2πœ‹π‘ŸπΏπ‘žπ‘Ÿ
π‘Ÿ+βˆ†π‘Ÿ
+ 2πœ‹π‘Ÿβˆ†π‘ŸπΏ 𝑆𝑒 = 0
Rate of Heat IN:
2πœ‹π‘ŸπΏπ‘žπ‘Ÿ
Rate of Heat OUT:
2πœ‹π‘ŸπΏπ‘žπ‘Ÿ
Generation:
2πœ‹π‘Ÿβˆ†π‘ŸπΏ 𝑆𝑒
π‘Ÿ
π‘Ÿ+βˆ†π‘Ÿ
Electrical Heat Source
Rate of Heat IN
2πœ‹π‘ŸπΏπ‘žπ‘Ÿ
Area perpendicular
to qr at r = r
π‘Ÿ
= (2πœ‹π‘ŸπΏ) βˆ™ π‘žπ‘Ÿ
π‘Ÿ
The Shell:
Rate of Heat IN:
2πœ‹π‘ŸπΏπ‘žπ‘Ÿ
Rate of Heat OUT:
2πœ‹π‘ŸπΏπ‘žπ‘Ÿ
Generation:
2πœ‹π‘Ÿβˆ†π‘ŸπΏ 𝑆𝑒
π‘Ÿ
π‘Ÿ+βˆ†π‘Ÿ
Electrical Heat Source
Rate of Heat OUT
2πœ‹π‘ŸπΏπ‘žπ‘Ÿ
π‘Ÿ+βˆ†π‘Ÿ
Area perpendicular
to qr at r = r + dr
= (2πœ‹(π‘Ÿ + βˆ†π‘Ÿ)𝐿) βˆ™ π‘žπ‘Ÿ
π‘Ÿ+βˆ†π‘Ÿ
The Shell:
Rate of Heat IN:
2πœ‹π‘ŸπΏπ‘žπ‘Ÿ
Rate of Heat OUT:
2πœ‹π‘ŸπΏπ‘žπ‘Ÿ
Generation:
2πœ‹π‘Ÿβˆ†π‘ŸπΏ 𝑆𝑒
π‘Ÿ
π‘Ÿ+βˆ†π‘Ÿ
Electrical Heat Source
Generation = Volume X Se
𝑉 = πœ‹ π‘Ÿ + βˆ†π‘Ÿ
2
− π‘Ÿ2 𝐿
∴ 𝑉 = πœ‹ 2π‘Ÿβˆ†π‘Ÿ 𝐿
Too small
= πœ‹ π‘Ÿ 2 + 2π‘Ÿβˆ†π‘Ÿ + βˆ†π‘Ÿ
2
− π‘Ÿ2 𝐿
∴ 𝐺𝑒𝑛 = 2πœ‹π‘Ÿβˆ†π‘ŸπΏ βˆ™ 𝑆𝑒
The Shell:
Rate of Heat IN:
2πœ‹π‘ŸπΏπ‘žπ‘Ÿ
Rate of Heat OUT:
2πœ‹π‘ŸπΏπ‘žπ‘Ÿ
Generation:
2πœ‹π‘Ÿβˆ†π‘ŸπΏ 𝑆𝑒
π‘Ÿ
π‘Ÿ+βˆ†π‘Ÿ
Electrical Heat Source
Consider an electrical wire
(solid cylinder):
Shell Heat Balance:
2πœ‹π‘ŸπΏπ‘žπ‘Ÿ
2πœ‹π‘ŸπΏπ‘žπ‘Ÿ
π‘Ÿ
− 2πœ‹π‘ŸπΏπ‘žπ‘Ÿ
π‘Ÿ
π‘Ÿ+βˆ†π‘Ÿ
− 2πœ‹π‘ŸπΏπ‘žπ‘Ÿ
+ 2πœ‹π‘Ÿβˆ†π‘ŸπΏ 𝑆𝑒 = 0
π‘Ÿ+βˆ†π‘Ÿ
= − 2πœ‹π‘Ÿβˆ†π‘ŸπΏ 𝑆𝑒
Dividing by 2πœ‹βˆ†π‘ŸπΏ:
π‘Ÿπ‘žπ‘Ÿ
π‘Ÿ
− π‘Ÿπ‘žπ‘Ÿ
βˆ†π‘Ÿ
π‘Ÿ+βˆ†π‘Ÿ
= −𝑆𝑒 π‘Ÿ
Q: Why did we divide by
2πœ‹βˆ†π‘ŸπΏ and not by 2πœ‹π’“βˆ†π‘ŸπΏ?
Electrical Heat Source
Consider an electrical wire
(solid cylinder):
We now have:
π‘Ÿπ‘žπ‘Ÿ π‘Ÿ − π‘Ÿπ‘žπ‘Ÿ
βˆ†π‘Ÿ
π‘Ÿ+βˆ†π‘Ÿ
= −𝑆𝑒 π‘Ÿ
Taking the limit as βˆ†π‘Ÿ → 0:
𝑑
π‘Ÿπ‘žπ‘Ÿ = −𝑆𝑒 π‘Ÿ
π‘‘π‘Ÿ
Q: Is this correct?
NO!
Electrical Heat Source
Consider an electrical wire
(solid cylinder):
We now have:
π‘Ÿπ‘žπ‘Ÿ π‘Ÿ − π‘Ÿπ‘žπ‘Ÿ
βˆ†π‘Ÿ
π‘Ÿ+βˆ†π‘Ÿ
= −𝑆𝑒 π‘Ÿ
We must adhere to the
definition of the derivative:
π‘Ÿπ‘žπ‘Ÿ
lim
βˆ†π‘Ÿ→0
π‘Ÿπ‘žπ‘Ÿ
− π‘Ÿπ‘žπ‘Ÿ
βˆ†π‘Ÿ
π‘Ÿ+βˆ†π‘Ÿ
− π‘Ÿπ‘žπ‘Ÿ
βˆ†π‘Ÿ
π‘Ÿ+βˆ†π‘Ÿ
π‘Ÿ
π‘Ÿ
= +𝑆𝑒 π‘Ÿ
𝑑
=
π‘Ÿπ‘žπ‘Ÿ = 𝑆𝑒 π‘Ÿ
π‘‘π‘Ÿ
Electrical Heat Source
Consider an electrical wire
(solid cylinder):
𝑑
π‘Ÿπ‘žπ‘Ÿ = 𝑆𝑒 π‘Ÿ
π‘‘π‘Ÿ
We now have:
Integrating:
𝑆𝑒 π‘Ÿ 𝐢1
π‘žπ‘Ÿ =
+
2
π‘Ÿ
Boundary conditions:
π‘Žπ‘‘ π‘Ÿ = 0,
π‘Žπ‘‘ π‘Ÿ = 𝑅,
π‘žπ‘Ÿ = 𝑓𝑖𝑛𝑖𝑑𝑒
𝑇 = 𝑇0
Note: The problem statement will
tell you hints about what boundary
conditions to use.
Electrical Heat Source
Consider an electrical wire
(solid cylinder):
We now have:
𝑆𝑒 π‘Ÿ 𝐢1
π‘žπ‘Ÿ =
+
2
π‘Ÿ
Applying B.C. 1: π‘Žπ‘‘ π‘Ÿ = 0, π‘žπ‘Ÿ = 𝑓𝑖𝑛𝑖𝑑𝑒
Because q has to be finite at r = 0, all
the terms with radius, r, below the
denominator must vanish. Therefore:
𝐢1 = 0
𝑆𝑒 π‘Ÿ
π‘žπ‘Ÿ =
2
Electrical Heat Source
Consider an electrical wire
(solid cylinder):
We now have:
𝑆𝑒 π‘Ÿ
π‘žπ‘Ÿ =
2
Substituting Fourier’s Law:
𝑑𝑇 𝑆𝑒 π‘Ÿ
−π‘˜
=
π‘‘π‘Ÿ
2
𝑑𝑇 −𝑆𝑒 π‘Ÿ
=
π‘‘π‘Ÿ
2π‘˜
−𝑆𝑒 π‘Ÿ 2
𝑇=
+ 𝐢2
4π‘˜
Electrical Heat Source
Consider an electrical wire
(solid cylinder):
We now have:
−𝑆𝑒 π‘Ÿ 2
𝑇=
+ 𝐢2
4π‘˜
Applying B.C. 2: π‘Žπ‘‘ π‘Ÿ = 𝑅,
−𝑆𝑒 𝑅2
𝑇0 =
+ 𝐢2
4π‘˜
𝑆𝑒 𝑅2
𝐢2 = 𝑇0 +
4π‘˜
This is it! But,
we rewrite it
into a nicer
−𝑆𝑒 π‘Ÿ 2 𝑆𝑒 𝑅2
form…
𝑇=
+
+ 𝑇0
4π‘˜
4π‘˜
𝑇 = 𝑇0
Electrical Heat Source
Consider an electrical wire
(solid cylinder):
Temperature Profile:
𝑆𝑒 𝑅2
π‘Ÿ
𝑇 − 𝑇0 =
1−
4π‘˜
𝑅
2
Important assumptions:
1. Temperature rise is not large so that
k and Se are constant & uniform.
2. The surface of the wire is
maintained at T0.
3. Heat flux is finite at the center.
Electrical Heat Source
Other important notes…
Let:
π‘˜π‘’ = electrical conductivity
𝐼 = current density
π‘Žπ‘šπ‘
π‘π‘š2
1
Ω βˆ™ π‘π‘š
𝐸 = voltage drop over a length
These imply the following :
𝐼2
𝑆𝑒 =
π‘˜π‘’
𝐸
𝐼 = π‘˜π‘’
𝐿
𝑉
𝑆𝑒 𝑅2
π‘Ÿ
𝑇 − 𝑇0 =
1−
4π‘˜
𝑅
2
𝑆𝑒 𝑅2 𝐸 2 𝑅2 π‘˜π‘’
=
4π‘˜
4𝐿2 π‘˜
Electrical Heat Source
Heat flux profile:
𝑆𝑒 π‘Ÿ
π‘žπ‘Ÿ =
2
The stress profile versus
the temperature profile:
Temperature Profile:
𝑆𝑒 𝑅2
π‘Ÿ
𝑇 − 𝑇0 =
1−
4π‘˜
𝑅
2
Electrical Heat Source
Quantities that might be asked for:
1. Maximum Temperature
Substituting r = 0
to the profile T(r):
π‘‡π‘šπ‘Žπ‘₯
𝑆𝑒 𝑅2
= 𝑇0 +
4π‘˜
2. Average Temperature Rise
𝑇 − 𝑇0 =
2πœ‹ 𝑅
𝑇 − 𝑇0 π‘Ÿ π‘‘π‘Ÿ
0
0
2πœ‹ 𝑅
π‘Ÿ π‘‘π‘Ÿ π‘‘πœƒ
0
0
π‘‘πœƒ
𝑆𝑒 𝑅2 1
𝑇 − 𝑇0 =
= π‘‡π‘šπ‘Žπ‘₯
8π‘˜
2
3. Heat Outflow Rate at the Surface
𝑄
𝑄
𝑆𝑒 π‘Ÿ
π‘žπ‘Ÿ = =
=
𝐴 2πœ‹π‘…πΏ
2
π‘Ÿ=𝑅
𝑄 = πœ‹π‘…2 𝐿 βˆ™ 𝑆𝑒
Electrical Heat Source
Examples for Review:
Example 10.2-1 and Example 10.2-2
Bird, Stewart, and Lightfoot, Transport
Phenomena, 2nd Ed., p. 295
Nuclear Heat Source
Consider a spherical
nuclear fuel assembly
(solid sphere):
Before doing a balance, let:
𝑆𝑛 = volumetric heat rate of
production within the
fissionable material only
𝑆𝑛0 = volumetric heat rate of
production at r = 0
Sn depends on radius parabolically:
𝑏 = a dimensionless positive constant
Nuclear Heat Source
Consider a spherical
nuclear fuel assembly
(solid sphere):
Before doing a balance, let:
π‘‡π‘Ÿ
𝐹
= temperature profile in the
fissionable sphere
(𝐢)
π‘‡π‘Ÿ
= temperature profile in the
Alcladding
(𝐹)
= heat flux in the fissionable
sphere
(𝐢)
= heat flux in the Al cladding
π‘žπ‘Ÿ
π‘žπ‘Ÿ
Nuclear Heat Source
Consider a spherical
nuclear fuel assembly
(solid sphere):
For the fissionable material:
(𝐹)
4πœ‹π‘Ÿ 2 π‘žπ‘Ÿ
(𝐹)
π‘Ÿ
− 4πœ‹π‘Ÿ 2 π‘žπ‘Ÿ
π‘Ÿ+βˆ†π‘Ÿ
+ 4πœ‹π‘Ÿ 2 βˆ†π‘Ÿ 𝑆𝑛 = 0
Rate of Heat IN:
(𝐹)
2
4πœ‹π‘Ÿ π‘žπ‘Ÿ
Rate of Heat OUT:
4πœ‹π‘Ÿ 2 π‘žπ‘Ÿ
Generation:
4πœ‹π‘Ÿ 2 βˆ†π‘Ÿ 𝑆𝑛
π‘Ÿ
(𝐹)
π‘Ÿ+βˆ†π‘Ÿ
Electrical Heat Source
Generation = Volume X Sn
4
𝑉 = πœ‹ π‘Ÿ + βˆ†π‘Ÿ
3
3
−
π‘Ÿ3
∴ 𝑉 = 4πœ‹ π‘Ÿ 2 βˆ†π‘Ÿ
Too small
4
= πœ‹ π‘Ÿ 3 + 3π‘Ÿ 2 βˆ†π‘Ÿ + 3π‘Ÿ βˆ†π‘Ÿ
3
2
+ βˆ†π‘Ÿ
3
− π‘Ÿ3
∴ 𝐺𝑒𝑛 = 4πœ‹π‘Ÿ 2 βˆ†π‘Ÿ 𝑆𝑛
Rate of Heat IN:
(𝐹)
2
4πœ‹π‘Ÿ π‘žπ‘Ÿ
Rate of Heat OUT:
4πœ‹π‘Ÿ 2 π‘žπ‘Ÿ
Generation:
4πœ‹π‘Ÿ 2 βˆ†π‘Ÿ 𝑆𝑛
π‘Ÿ
(𝐹)
π‘Ÿ+βˆ†π‘Ÿ
Nuclear Heat Source
For the fissionable material:
(𝐹)
4πœ‹π‘Ÿ 2 π‘žπ‘Ÿ
(𝐹)
π‘Ÿ
− 4πœ‹π‘Ÿ 2 π‘žπ‘Ÿ
π‘Ÿ+βˆ†π‘Ÿ
No
generation
here!
+ 4πœ‹π‘Ÿ 2 βˆ†π‘Ÿ 𝑆𝑛 = 0
For the Al cladding:
(𝐢)
4πœ‹π‘Ÿ 2 π‘žπ‘Ÿ
Dividing by 4πœ‹βˆ†π‘Ÿ:
(𝐹)
π‘Ÿ 2 π‘žπ‘Ÿ
𝐹
2
π‘Ÿ+βˆ†π‘Ÿ − π‘Ÿ π‘žπ‘Ÿ
βˆ†π‘Ÿ
(𝐢)
π‘Ÿ
− 4πœ‹π‘Ÿ 2 π‘žπ‘Ÿ
π‘Ÿ+βˆ†π‘Ÿ
=0
Dividing by 4πœ‹βˆ†π‘Ÿ:
π‘Ÿ
(𝐢)
= 𝑆𝑛 π‘Ÿ
2
π‘Ÿ 2 π‘žπ‘Ÿ
𝐢
2π‘ž
−
π‘Ÿ
π‘Ÿ+βˆ†π‘Ÿ
π‘Ÿ
βˆ†π‘Ÿ
π‘Ÿ
=0
Nuclear Heat Source
For the fissionable material:
(𝐹)
4πœ‹π‘Ÿ 2 π‘žπ‘Ÿ
(𝐹)
π‘Ÿ
− 4πœ‹π‘Ÿ 2 π‘žπ‘Ÿ
π‘Ÿ+βˆ†π‘Ÿ
No
generation
here!
+ 4πœ‹π‘Ÿ 2 βˆ†π‘Ÿ 𝑆𝑛 = 0
For the Al cladding:
(𝐢)
4πœ‹π‘Ÿ 2 π‘žπ‘Ÿ
Taking βˆ†π‘Ÿ → 0:
𝑑 2 (𝐹)
π‘Ÿ π‘žπ‘Ÿ
= 𝑆𝑛 π‘Ÿ 2
π‘‘π‘Ÿ
(𝐢)
π‘Ÿ
− 4πœ‹π‘Ÿ 2 π‘žπ‘Ÿ
Taking βˆ†π‘Ÿ → 0:
𝑑 2 (𝐢)
π‘Ÿ π‘žπ‘Ÿ
=0
π‘‘π‘Ÿ
π‘Ÿ+βˆ†π‘Ÿ
=0
Nuclear Heat Source
For the fissionable material:
(𝐹)
4πœ‹π‘Ÿ 2 π‘žπ‘Ÿ
(𝐹)
π‘Ÿ
− 4πœ‹π‘Ÿ 2 π‘žπ‘Ÿ
π‘Ÿ+βˆ†π‘Ÿ
No
generation
here!
+ 4πœ‹π‘Ÿ 2 βˆ†π‘Ÿ 𝑆𝑛 = 0
For the Al cladding:
(𝐢)
4πœ‹π‘Ÿ 2 π‘žπ‘Ÿ
Taking βˆ†π‘Ÿ → 0:
𝑑 2 (𝐹)
π‘Ÿ
π‘Ÿ π‘žπ‘Ÿ
= 𝑆𝑛0 1 + 𝑏
π‘‘π‘Ÿ
𝑅𝐹
(𝐢)
π‘Ÿ
− 4πœ‹π‘Ÿ 2 π‘žπ‘Ÿ
Taking βˆ†π‘Ÿ → 0:
2
π‘Ÿ2
𝑑 2 (𝐢)
π‘Ÿ π‘žπ‘Ÿ
=0
π‘‘π‘Ÿ
π‘Ÿ+βˆ†π‘Ÿ
=0
Nuclear Heat Source
For the fissionable material:
(𝐹)
4πœ‹π‘Ÿ 2 π‘žπ‘Ÿ
(𝐹)
π‘Ÿ
− 4πœ‹π‘Ÿ 2 π‘žπ‘Ÿ
π‘Ÿ+βˆ†π‘Ÿ
No
generation
here!
+ 4πœ‹π‘Ÿ 2 βˆ†π‘Ÿ 𝑆𝑛 = 0
For the Al cladding:
(𝐢)
4πœ‹π‘Ÿ 2 π‘žπ‘Ÿ
Integrating:
(𝐢)
π‘Ÿ
− 4πœ‹π‘Ÿ 2 π‘žπ‘Ÿ
Integrating:
π‘Ÿ+βˆ†π‘Ÿ
=0
Nuclear Heat Source
Boundary Conditions:
π‘Žπ‘‘ π‘Ÿ = 0,
(𝐹)
𝐢1
π‘žπ‘Ÿ 𝑖𝑠 𝑓𝑖𝑛𝑖𝑑𝑒
=0
Integrating:
For the fissionable material
Boundary Conditions:
(𝐹)
π‘Žπ‘‘ π‘Ÿ = 𝑅(𝐹) ,
(𝐢)
𝐢1
= 𝑆𝑛0
π‘žπ‘Ÿ
1 𝑏
+
𝑅
3 5
Integrating:
For the Al cladding
(𝐢)
= π‘žπ‘Ÿ
𝐹 3
Nuclear Heat Source
For the fissionable material
Inserting Fourier’s Law:
For the Al cladding
Inserting Fourier’s Law:
Nuclear Heat Source
For the fissionable material
For the Al cladding
Boundary Conditions:
Boundary Conditions:
R(C)
At r = R(F),
T(F) = T(C)
R(F)
At r = R(C),
T(C) = T0
Nuclear Heat Source
For the fissionable material
For the Al cladding
Overall Shell Energy Balance
Recall the Overall Shell Energy Balance:
Q by Convective Transport
W by Molecular Transport
Q by Molecular Transport
W by
External
Forces
Energy
Generation
SteadyState!
Overall Shell Energy Balance
We need all these terms for viscous dissipation:
Q by Convective Transport
Q by Molecular Transport
How can we account for
all these terms at once?
W by Molecular Transport
Combined Energy Flux Vector
We introduce something new to replace q:
Combined Energy Flux Vector:
Heat Rate from Molecular Motion
Convective Energy Flux
1 2
𝒆=
πœŒπ‘£ + πœŒπ‘ˆ 𝒗 + 𝝅 βˆ™ 𝒗 + 𝒒
2
Work Rate from Molecular Motion
Combined Energy Flux Vector
We introduce something new to replace q:
Combined Energy Flux Vector:
Recall the molecular stress tensor:
When dotted with v:
𝝅 = π‘πœΉ + 𝝉
𝝅 βˆ™ 𝒗 = 𝑝𝒗 + [𝝉 βˆ™ 𝒗]
Substituting into e:
1 2
𝒆=
πœŒπ‘£ + πœŒπ‘ˆ 𝒗 + 𝑝𝒗 + [𝝉 βˆ™ 𝒗] + 𝒒
2
Combined Energy Flux Vector
We introduce something new to replace q:
Combined Energy Flux Vector:
1 2
𝒆=
πœŒπ‘£ + πœŒπ‘ˆ 𝒗 + 𝑝𝒗 + [𝝉 βˆ™ 𝒗] + 𝒒
2
Simplifying the boxed expression:
𝑝
πœŒπ‘ˆπ’— + 𝑝𝒗 = 𝜌 π‘ˆ +
𝒗 = 𝜌 π‘ˆ + 𝑝𝑉 𝒗 = πœŒπ»π’—
𝜌
Finally:
1 2
𝒆=
πœŒπ‘£ + 𝜌𝐻 𝒗 + [𝝉 βˆ™ 𝒗] + 𝒒
2
Viscous Dissipation Source
Consider the flow of an incompressible Newtonian fluid
between 2 coaxial cylinders:
π‘₯
𝑣𝑧 π‘₯ = 𝑣𝑏
𝑏
Viscous Dissipation Source
Consider the flow of an incompressible Newtonian fluid
between 2 coaxial cylinders:
We now make a shell
balance shown in red
on the left.
Rate of
Energy IN:
π‘ŠπΏπ’†π’™
Rate of
Energy OUT:
π‘ŠπΏπ’†π’™
When the combined energy flux vector is used, the
generation term will automatically appear from e.
π‘₯
π‘₯+βˆ†π‘₯
Viscous Dissipation Source
Consider the flow of an incompressible Newtonian fluid
between 2 coaxial cylinders:
π‘ŠπΏπ’†π’™
π‘₯+βˆ†π‘₯
− π‘ŠπΏπ’†π’™
𝑑𝒆𝒙
=0
𝑑π‘₯
𝒆𝒙 = 𝐢1
π‘₯
=0
We now make a shell
balance shown in red
on the left.
Rate of
Energy IN:
π‘ŠπΏπ’†π’™
Rate of
Energy OUT:
π‘ŠπΏπ’†π’™
When the combined energy flux vector is used, the
generation term will automatically appear from e.
π‘₯
π‘₯+βˆ†π‘₯
Viscous Dissipation Source
Consider the flow of an incompressible Newtonian fluid
between 2 coaxial cylinders:
1 2
𝒆=
πœŒπ‘£ + 𝜌𝐻 𝒗 + [𝝉 βˆ™ 𝒗] + 𝒒
2
𝒆𝒙 = 𝐢1
Fourier’s Law:
Newton’s Law:
𝑑𝑇
π‘žπ‘₯ = −π‘˜
𝑑π‘₯
𝜏π‘₯𝑧
𝑑𝑣𝑧
= −πœ‡
𝑑π‘₯
When the combined energy flux vector is used, the
generation term will automatically appear from e.
Viscous Dissipation Source
Consider the flow of an incompressible Newtonian fluid
between 2 coaxial cylinders:
𝒆𝒙 = 𝐢1
Substituting the
velocity profile:
Integrating:
𝑑𝑇
𝑑𝑣𝑧
−π‘˜
− πœ‡π‘£π‘§
= 𝐢1
𝑑π‘₯
𝑑π‘₯
𝑑𝑇
𝑣𝑏
−π‘˜
− πœ‡π‘₯
𝑑π‘₯
𝑏
πœ‡ 𝑣𝑏
𝑇=−
π‘˜ 𝑏
2
2
= 𝐢1
π‘₯ 2 𝐢1
− π‘₯ + 𝐢2
2
π‘˜
When the combined energy flux vector is used, the
generation term will automatically appear from e.
Viscous Dissipation Source
Consider the flow of an incompressible Newtonian fluid
between 2 coaxial cylinders:
Boundary Conditions:
πœ‡ 𝑣𝑏
𝑇=−
π‘˜ 𝑏
2
π‘₯ 2 𝐢1
− π‘₯ + 𝐢2
2
π‘˜
After applying the B.C.:
𝑇 − 𝑇0
1
πœ‡π‘£π‘2
=
𝑇𝑏 − 𝑇0 2 π‘˜ 𝑇𝑏 − 𝑇0
π‘₯
𝑏
π‘₯
π‘₯
1− +
𝑏
𝑏
When the combined energy flux vector is used, the
generation term will automatically appear from e.
Viscous Dissipation Source
Consider the flow of an incompressible Newtonian fluid
between 2 coaxial cylinders:
πœ‡ 𝑣𝑏
𝑇=−
π‘˜ 𝑏
2
π‘₯2
𝐢1
− π‘₯ + 𝐢2
2
π‘˜
Q: So where is Sv?
𝑣𝑏
𝑆𝑣 = πœ‡
𝑏
After applying the B.C.:
𝑇 − 𝑇0
1
πœ‡π‘£π‘2
=
𝑇𝑏 − 𝑇0 2 π‘˜ 𝑇𝑏 − 𝑇0
π‘₯
𝑏
π‘₯
π‘₯
1− +
𝑏
𝑏
When the combined energy flux vector is used, the
generation term will automatically appear from e.
2
Viscous Dissipation Source
Consider the flow of an incompressible Newtonian fluid
between 2 coaxial cylinders:
Temperature
Profile:
𝑇 − 𝑇0
1
πœ‡π‘£π‘2
=
𝑇𝑏 − 𝑇0 2 π‘˜ 𝑇𝑏 − 𝑇0
π‘₯
𝑏
π‘₯
π‘₯
1− +
𝑏
𝑏
New Dimensionless Number:
Dim. Group
Brinkman, Br
Ratio
viscous heat dissipation/
molecular heat transport
Equation
πœ‡π‘£π‘2
π‘˜ 𝑇𝑏 − 𝑇0
Viscous Dissipation Source
Scenarios when viscous heating is significant:
1. Flow of lubricant between rapidly moving parts.
2. Flow of molten polymers through dies in highspeed extrusion.
3. Flow of highly viscous fluids in high-speed
viscometers.
4. Flow of air in the boundary layer near an earth
satellite or rocket during reentry into the earth’s
atmosphere.
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