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COMPUTATIONAL HEAT TRANSFER AND FLUID FLOWTRANSFER AND FLUID FLOW
PRADIP DUTTADEPARTMENT OF MECHANICAL ENGINEERINGDEPARTMENT OF MECHANICAL ENGINEERING
INDIAN INSTITUTE OF SCIENCEBANGALORE
OutlineOutline
B i f H t T fBasics of Heat Transfer
M h i l d i i f fl id fl d hMathematical description of fluid flow and heattransfer: conservation equations for mass,momentum energy and chemical speciesmomentum, energy and chemical species,classification of partial differential equationsgeneralized control volume approach in Euleriang ppframe
What is Heat Transfer?What is Heat Transfer?
“Energy in transit due to temperature difference.”gy pThermodynamics tells us: How much heat is transferred (Q)
H h k i d (W) How much work is done (W) Final state of the systemHeat transfer tells us:eat t ansfe te s us: How (by which mechanism) Q is transferred At what rate Q is transferred Temperature distribution within the body
Heat transfer ThermodynamicscomplementaryHeat transfer Thermodynamicscomplementary
MODESMODES
Conduction- needs matter- molecular phenomenon (diffusion process)
i h b lk i- without bulk motion of matterConvection
heat carried away by bulk motion of fluid- heat carried away by bulk motion of fluid- needs fluid matter
Radiationd o- does not need matter- transmission of energy by electromagnetic waves
APPLICATIONS OF HEAT TRANSFER
Energy production and conversion Energy production and conversion- steam power plant, solar energy conversion etc.
Refrigeration and air-conditioning D ti li ti Domestic applications
- ovens, stoves, toaster Cooling of electronic equipment Manufacturing / materials processing
- welding, casting, forming, heat treatment, laser machining Automobiles / aircraft design Automobiles / aircraft design Nature (weather, climate etc)
(Needs medium, Temperature gradient)TT >T
.. . . . . . . . . T2T1
T1>T2. . . . . .
. . . . . . . . . . . . . . . . . . . . . . .
q’’
. . . . .
. . . . . .. . . . . . . .. . . . . .
. . . . . . . . . . . q
. . . . .solid or stationary fluid………….. . ..
RATE:
. . . . . . .solid or stationary fluid
RATE:
q(W) or (J/s) (heat flow per unit time)
Conduction (contd )(contd…)
xRate equations (1D conduction):
T1
T
A Differential Formq = - k A dT/dx, Wk = Thermal Conductivity W/mKq T2 k = Thermal Conductivity, W/mKA = Cross-sectional Area, m2
T = Temperature, K or oCk x = Heat flow path, m
Difference Form q = - k A (T2 – T1) / (x2 – x1)q k A (T2 T1) / (x2 x1)
Heat flux: q” = q / A = - kdT/dx (W/m2)
(negative sign denotes heat transfer in the direction of decreasing temperature)
Rate equation(convection)
q”y y
U TT(y)u(y)
U
Heat transfer rate q = hA( T T ) W
q T(y)Ts
u(y)
Heat transfer rate q = hA( Ts-T ) W
Heat flux q” = h( Ts-T ) W / m2
h=heat transfer co-efficient (W /m2K)
not a fluid property alone, but also depends on flow p p y , pgeometry, nature of flow (laminar/turbulent), thermodynamics properties etc.
Convection (contd…)
Free or natural convection (induced by buoyancy forces) May occur with
phase change (boiling,
Forced convection (induced by external
(boiling, condensation)
(induced by external means)
Convection (contd…)( )
Typical values of h (W/m2K)yp ( )
Free convection gases: 2 - 25
liquid: 50 - 100
Forced convection gases: 25 - 250
liquid: 50 - 20,000q ,
Boiling/Condensation 2500 -100,000
T1q1”
T2q2”
RATE:q(W) or (J/s) Heat flow per unit timeq(W) or (J/s) Heat flow per unit time.
Flux : q” (W/m2)
Rate equations (Radiation)
RADIATION:
Heat Transfer by electro-magnetic waves or photons( no medium required. )
Emissive power of a surface (energy released per unit area):Emissive power of a surface (energy released per unit area):
E=Ts4 (W/ m2)
= emissivity (property)……..
=Stefan Boltzmann constant=Stefan-Boltzmann constant
Rate equations (Contd )(Contd….)
”q” d
Ts u r
q”co n v.q r a d.
Area = AT Area = ATs
R di ti h b t l f dRadiation exchange between a large surface and surrounding
Q” = (T 4 T 4) W/ m2Q r a d = (Ts4-Tsur
4) W/ m2
Substantial derivativeSubstantial derivative txxx ,,, 321
ddx
ddx
ddxD 321
dtxdtxdtxtDt 321
dxD dtdx
xtDtD i
i
D
tilocallsubstantia
ii x
utDt
D
componentconvectivecomponent
ocaderivativesubsta t a
Conservation principle(s)Conservation principle(s)• mass is conserved• momentum is conserved• energy is conservedgy• chemical species are conserved•• …
txxx ,,, 321
DDD
V
dV
source
VVVchange
dVdVDtDdV
DtD
DtD
Conservation principlep pfor an elementary volume dV ::
dVdVDtD
dVDtD
DtDdVdV
DtD
DtDtDt
dV
dVDtD
DtDdV
dVDt
dVuD i
dV
xDt i
i
Conservation principleConservation principlefor an elementary volume dV ::
D
i
i
xu
DtD
i d f fi l l V ui V
ii
uxt
integrated for a final volume V bounded by a surface A ::
ui
ni dAdV V
AA
V V
iiV
dVux
dVt
dVDtD
called as “Reynolds Transport Equation
VV A
ii dVdAundVt
(RTE)” - a relation between a system and control volume.
Conservation of massConservation of massTotal mass remains constant. For a control volume, the balance of mass flux gives the mass accumulation ratethe balance of mass flux gives the mass accumulation rate.
0dVD 0dVDt
set : - thendensity,
- mass V
dV
- 0 source no
Conservation of massConservation of masscontinuity equation
for an elementary volume dV::
V
i t t d f fi l l V b d d b
ui
ni dAdV V
A
ii
uxt
integrated for a final volume V bounded by
a surface A ::
ni A
dAundVtV A
ii Here (ni ui ) is a scalar quantity:
-for outward flow (away from the surface)- positive V
-for inward flow- negative
Incompressible flowIncompressible flowfor an incompressible fluid: =const :f p f written for an elementary volume dV ::
V0
i
i
xu
or a final volume V bounded by a surface A ::
ui
ni dAdV V
AA0
Aii dAun
A
Conservation of momentumConservation of momentumRate of change of momentum will cause fluid acceleration. For a control volume we consider the balance of momentum fluxesFor a control volume, we consider the balance of momentum fluxes.
jj FdVuDtD
jj F
DudV
jjDt
thl itd itu
force
j
onacceleratimass Dt
set :
momentum
thenvelocity,density
-
-
j
j
dVu
u
eunit volumper force - j
V
F
Conservation of momentumConservation of momentummomentum equation
for an elementary volume dV :
jiji
j Fuux
ut
i
ijjij
ij x
fuux
ut
dijp
ij xx
Conservation of momentum
V ui dV Vintegrated for a final volume Vbounded by a surface A ::
ui
ni dAdV
A
inletoutlet
convectionchange momentum
).(
d
Aiij
Vj
dAdAdVf
dAunudVut
stressn deformatiostress sphericalforcesbody
A
idij
Aj
Vj dAndApndVf
Stress - strain relationshipp
xx22 211 xuu 21
xx22
xx11
p d
dVxx
pdVx
dFi
ij
iij
i
ijj
3
3
2
232 00
uxu
xuuu
11 uuu 2111
1 0 xuuxu
2
1
2
1
1
212 2
121
xu
xu
xu
Stress-strain relationshipStress strain relationshipfor Newtonian fluids :
1 2u
generalized :
122
112 2
x
dij
dij 2
deformation stress = = 2 X viscosity X deformationstrain rate
dijkkijij
31
jjj 3
kijd uuu
112
k
kij
j
i
i
jdij xxx
32
2
Navier-Stokes equationsNavier Stokes equations
dp i
ij
jjij
ij xx
pfuux
ut
i
j
ii
dij
xu
xx
k
kij
ij
i
i xu
xxu
x
32
d uu 1
i
i
ji
j
ii
ij
xu
xxu
xx
31
Navier-Stokes equationsNavier Stokes equations
j
iji
j
uup
uux
ut
1
i
i
ji
j
ijj x
uxx
uxx
pf 31
for an incompressible fluid =constwith a constant viscosity=constwith a constant viscosity const
21 jj upfuu
u
2ij
jiji xx
fuuxt
Surface force decompositionSurface force decomposition
dVpdVdFdijij
dVxx
dVx
dFii
iji
j
since:
jiij x
pxp
the total stress Fj can be separated into the spherical and deformation components:
dVdVpdFdij
j
xx ij
j
Work decompositionWork decompositiondxdx33
dVdVdxdx22
uu22 11
22 dx
xuu
12 dx
dxdx11xx11
xx221
112 dx
x12
total work done on an elementary volume:
dxdx11xx11xx33
total work done on an elementary volume:
12
232112
12 dxxuudxdxdx
x
23212
11
udxdxxx
Work decompositionWork decomposition
dVux
dxdxdxxu
xu 122
1321
1
212
1
122
generalized total work done on an elementary volume can be separatedgeneralized - total work done on an elementary volume can be separatedinto the kinetic and deformation components:
i
jijjjijj
i xu
Fuux
workndeformatio
workkinetic
worktotal
Conservation of mechanical energy
"change of kinetic energy is a result of work d b t l f "
start with the momentum equation :
done by external forces"
jj FdVuDtD
juDt
ijjj udVdVfuu
dVD
forces externalby work changeenergy kinetic
2 ji
jj
jj udVx
dVfdVDt
Conservation of thermal (or internal) energy( ) gy
Net heat flux entering a control volume results in rate of change of internal energyof change of internal energy
ijijiqdV
DtD
qi dV V
jjixDt
Tk ni dA
dV
Aii x
kq
i
jij
ii xu
xTk
xdV
DtD
sferheat trann workdeformatio
sferheat tranconductionchangeenergy internal
Conservation of thermal energyset :
etemperaturheat specific - cT
gy
energy internal - V
uT
dVcT
ferheat trans - i
jij
ii xu
xTk
x
thermal energy equation
for an elementary volume dV :
ii
T
cTux
cTt
i
jij
ii xu
xTk
x
Conservation of thermal energy
integrated for a final volume V ui dV V
gy
bounded by a surface A :i
ni dAdV
A
outlet inlet
convectionenergy internalchangeenergy internal
dAucTndVcT
A
iiV
uT
dAucTndVcTt
kd f id ti
V i
jij
Ai
i
dVxu
dAnxTk
sferheat trann work deformatio
sferheat tranconduction
Conservation of chemical species
Net species mass transfer across the control volume faces + chemical reactionwithin the control volume results in a change of concentration of chemicalg f fSpecies in the control volume
ssis RqdVmD
qis dV V
i
Rx
dVmDt
sni dA
dV
Ai
sss
i xmq
D
chemicaltoduek source/sin
s
i
ss
i
s Rxm
xdVm
DtD
D
reactionchemical todue
transfermassdiffusionchangeion concentrat
Conservation of chemical species
set : ionconcentrat mass pecies - sm s
mass species -
s
V
s dVm
reaction chemical
and diffusion -s
i
ss
i
Rxm
x
D
mass transfer equation
for an elementary volume for an elementary volume dV :
is
i
s umx
mt
s
i
ss
i
Rxm
x
D
Conservation of chemical species
integrated for a final volume V qis dV V
bounded by a surface A : ni dAA
tii
outlet inlet
convection specieschangeion concentrat species
Aii
s
V
s dAunmdVmt
V
s
Ai
i
ss
AV
dVRdAnxm
t
D
reaction chemical toduek source/sin
transfermassdiffusion species
VA i
Class of Linear Second-order PDEs
• Linear second order PDEs are of the form• Linear second-order PDEs are of the form
h A H f ti f d lHGuFuEuCuBuAu yxyyxyxx 2
where A - H are functions of x and y only• Elliptic PDEs: B2 - AC < 0
( d h i i h h )(steady state heat equations without heat source)
• Parabolic PDEs: B2 - AC = 0(t i t h t t f ti )(transient heat transfer equations)
• Hyperbolic PDEs: B2 - AC > 0 (wave equations)(wave equations)
MODULE 1: Review Questions• What is the driving force for (a) heat transfer (b) electric current flow
and (c) fluid flow?Whi h f th f ll i i t t i l t ?• Which one of the following is not a material property?(a) thermal conductivity (b) heat transfer coefficient (c)emissivity
• What is the order of magnitude of thermal conductivity for (a) metals(b) solid insulating materials (c) liquids (d) gases?
• What are the orders of magnitude for free convection heat transfercoefficient, forced convection and boiling?
• Under what circumstances can one expect radiation heat transfer to besignificant?
• An ideal gas is heated from 40ºC to 60ºC (a) at constant volume andg ( )(b) at constant pressure. For which case do you think the energyrequired will be greater? Explain why?
• A person claims that heat cannot be transferred in a vacuum. Evaluatepthis claim.
MODULE 1: Review Questions (contd )(contd...)
• In which of the three states (solid/liquid/gas) of a matter, conductionheat transfer is high/low? Explain your claimheat transfer is high/low? Explain your claim.
• Name some good and some poor conductors of heat.• Show that heat flow lines and isotherms in conduction heat transfer are
l t h th Will thi diti h ld f ti h tnormal to each other. Will this condition hold for convection heattransfer?
• Distinguish between Eulerian and Lagrangian approach in fluidh i Wh i th E l i h ll d?mechanics. Why is the Eulerian approach normally used?
• Derive the Reynolds transport equation.• Derive the continuity (mass conservation) equation in differential form
for incompressible flow.• Define substantial derivative. What is the physical significance of the
substantial derivative in an Eulerian framework?