TP323Lecture2-2(2)

Embed Size (px)

Citation preview

  • 8/10/2019 TP323Lecture2-2(2)

    1/31

    Momentum TransferLecture 3: Equations of Change for

    Isothermal Systems

    Transport Phenomena

  • 8/10/2019 TP323Lecture2-2(2)

    2/31

    From last week

    Shell balances for isothermal systems

    Boundary conditions Where shell balances cannot be applied

    Solutions for class examples on Blackboard

    Go through tutorial questions to get more understanding

    Shell balances as introduction to equations of continuity and

    momentum

    (i.e. TP is not all about shell balances, just in case you were

    wondering.)

  • 8/10/2019 TP323Lecture2-2(2)

    3/31

    Relevant Learning

    Equations of change:

    Continuity

    Motion

    Significance, usage, special cases (inviscid

    and creeping flows)

  • 8/10/2019 TP323Lecture2-2(2)

    4/31

    Equation of Continuity

    [Mass accumulation] = [Mass in] [Mass out]

    Substitute all equations

    Divide by xyz, and asx, y, z 0, we get:

    dz

    v

    dy

    v

    dx

    v

    t

    zyx

    zzzzz

    yyyyy

    xxxxx

    vyxvyx

    vzxvzx

    vzyvzyt

    zyx

  • 8/10/2019 TP323Lecture2-2(2)

    5/31

    Equation of Continuity

    Local change of with time at a fixed point of x, y, and

    z.

    PARTIAL time derivative

    t

    vxdx

    vy

    dy vzdz

    v Divergence of v

  • 8/10/2019 TP323Lecture2-2(2)

    6/31

    Equation of Continuity

    What happens if we (as observers) float along with the

    velocity of the flowing stream? Derivative that follows the motion

    Partial time derivative (as before) + velocity x gradient of property

    Total time change of a quantity as observed by an observer

    following the motion of the fluid

    SUBSTANTIAL time derivative

    Dt

    D

    dz

    dv

    dy

    dv

    dx

    dv

    dt

    dzyx

  • 8/10/2019 TP323Lecture2-2(2)

    7/31

    Equation of Continuity Substantial time derivative of ?

    t

    vxdx

    vy

    dyvz

    dz

    vx

    dx vy

    dy vz

    dz

    DDt

    .v Substantial derivative of

    t vx

    dx vy

    dy vz

    dz

    vx

    dxvy

    dyvz

    dz

    Divergence of v

    dz

    v

    dy

    v

    dx

    v

    t

    zyx

    v

    .dt

    d

  • 8/10/2019 TP323Lecture2-2(2)

    8/31

    Equation of Continuity

    For incompressible fluids (constant ):

    v dvxdx

    dvy

    dydvz

    dz0

    d

    dt0

    vx

    dx vx

    dx

    vy

    dy vy

    dy

    vz

    dz vz

    dz

    0

  • 8/10/2019 TP323Lecture2-2(2)

    9/31

    Equation of Momentum

    [Mom. accumulation] = [Mom. in] [Mom. out] + [Forces]

    Momentum enters and leaves control volume throughconvective momentum transfer and viscous action through

    velocity gradient

    y

    vx)x vx)x+x

    z

    x

  • 8/10/2019 TP323Lecture2-2(2)

    10/31

    Equation of momentum

    Rate of accumulation of x-momentum:

    Considering the continuity equation:

    we get:

    d vx dt

    d vxvx dx

    d vxvy dy

    dvxvz dz

    dxx

    dx

    dyx

    dy dzx

    dz

    dp

    dx gx

    t

    vx

    dxvy

    dyvz

    dz

    dvx

    dt vx

    dvx

    dx vy

    dvx

    dy vz

    dvx

    dz

    dxx

    dxdyx

    dydzx

    dz

    dp

    dxgx

  • 8/10/2019 TP323Lecture2-2(2)

    11/31

    More on viscous flux

    Recall Newtons law of viscosity:

    The viscous term in the momentum equation: derivative

    of the shear stress:

    So, this term is a function of the second-derivative ofvelocity!

    yx dvx

    dy

    dxx dx

    dyx dy

    dzx dz

  • 8/10/2019 TP323Lecture2-2(2)

    12/31

    More on viscous flux

    For incompressible, Newtonian fluids, we can simplify to:

    d

    2vx

    dx 2 d

    2vx

    dy 2 d

    2vx

    dz2

    2v

  • 8/10/2019 TP323Lecture2-2(2)

    13/31

    Equation of momentum

    For Newtonian and incompressible fluids:

    Navier-Stokes equation What you learned in Fluid Mech!

    Same treatment for y- and z-momentum

    x

    xxx

    xz

    xy

    xx

    x

    gdx

    dp

    dz

    vd

    dy

    vd

    dx

    vd

    dz

    dvv

    dy

    dvv

    dx

    dvv

    dt

    dv

    2

    2

    2

    2

    2

    2

  • 8/10/2019 TP323Lecture2-2(2)

    14/31

    ???

    Further reading on this:

    Welty et al. (2001), Fundamentals of Momentum, Heat and Mass

    Transfer 4th ed., ch. 7-9

    Bird, Stewart, Lightfoot (2007), Transport Phenomena, ch. 1-3

    McCabe, Smith, Harriot (2004), Unit Operations of Chemical

    Engineering, ch. 4

    Note: in the first 2 books, the normal stress (xx, yy, zz) are

    denoted differently (xx, yy, zz), and the pressure effects are

    included in here.

  • 8/10/2019 TP323Lecture2-2(2)

    15/31

    Class example

    Similar to the case of parallel plates, but with the plates

    vertical

    Effects of gravity

    Newtonian

    Laminar

    Incompressible

    Steady state

    From: Welty et al., 2001

  • 8/10/2019 TP323Lecture2-2(2)

    16/31

    Class example

    From: Welty et al., 2001

    v0 = 0

  • 8/10/2019 TP323Lecture2-2(2)

    17/31

    Other examples

    Flow on inclined surface

    Try to do this problem yourself!

    Pipe flow

    a bit more difficult, as we need to use cylindrical coordinates!

  • 8/10/2019 TP323Lecture2-2(2)

    18/31

    Cylindrical coordinates

    Equation of continuity:

    011 zr vdz

    dv

    d

    d

    rrv

    dr

    d

    rdt

    d

    cosrx

    zz

    sinry

    x

    y1tan

    22 yxr

  • 8/10/2019 TP323Lecture2-2(2)

    19/31

    Cylindrical coordinates

    Equation of motion for fluids with constant

    and :

  • 8/10/2019 TP323Lecture2-2(2)

    20/31

    Pipe Flow

    Fully-developed (steady) flow

    Far from entrances/exits Flow is laminar and 1 directional:

    vr= 0

    v = 0

    vz = vz(r)

    p = p(z)

  • 8/10/2019 TP323Lecture2-2(2)

    21/31

    Pipe Flow

    Continuity eqn:

    For constant density:

    As vr= v = 0, we get:

    011

    zr vdz

    dv

    d

    d

    r

    rv

    dr

    d

    rdt

    d

    0dz

    dvz

    011

    0

    dzdv

    ddv

    rrv

    drd

    r

    dt

    d

    zr

  • 8/10/2019 TP323Lecture2-2(2)

    22/31

    Pipe Flow

    Eqn of motion in the z-direction

    Flow is symmetrical about the z-axis d2vz/d2 = 0

    So, we get:

    Integrating once:

    z

    z gdz

    dp

    dr

    dvr

    dr

    d

    r

    rg

    dz

    dp

    dr

    dvr

    dr

    dz

    z

    1

    2

    2C

    rg

    dz

    dp

    dr

    dvr z

    z

    r

    Crg

    dz

    dp

    dr

    dvz

    z 1

    2

    dvz/dr doesnt

    become infinite

    when r = 0

  • 8/10/2019 TP323Lecture2-2(2)

    23/31

    Pipe Flow

    Integrate again to get vz:

    Use the boundary condition to evaluate C2, and we get:

    As before, we use P = p + gL:

    Another integration:

    2

    2

    4

    Cr

    g

    dz

    dpv zz

    224

    1Rrg

    dz

    dpv zz

    224

    1Rr

    dz

    dPvz

    LP

    P

    L

    z PRrzv

    0

    22

    04

    1

    220

    4rR

    L

    PPv Lz

  • 8/10/2019 TP323Lecture2-2(2)

    24/31

    Special case (Creeping flow)

    Creeping flow & Stokes law

    Very slow flows

    Therefore, we have:

    (also for other directions)

    Negligible effects of inertia, Re

  • 8/10/2019 TP323Lecture2-2(2)

    25/31

    Special case (Creeping flow)

    Flow past a sphere

    The creeping flow equation has been used to solve the velocityand pressure distribution in slow flows past a sphere

    cos2

    1

    2

    31

    3

    r

    R

    r

    Rvvr

    sin4

    1

    4

    31

    3

    r

    R

    r

    Rvv

    0v

    cos2

    3 2

    0

    r

    R

    R

    vgzpp

  • 8/10/2019 TP323Lecture2-2(2)

    26/31

    Special case (Creeping flow)

    Flow past a sphere

    Total drag over the surface of the sphere = [form drag] + [viscousdrag]

    Stokes equation

    Valid for

    RvFD 6

    0.12

    Re 0

    Rv

    Occurs as fluid needs to

    change direction to pass

    around the sphere

    Due to shear stress at the

    sphere surface

  • 8/10/2019 TP323Lecture2-2(2)

    27/31

    Special case (Inviscid flow)

    Euler equations for ideal fluids

    Fluids with constant density and very low viscosity inviscid flow

    Aerodynamics & hydrodynamics

    Re >> 1 and 0

    xx

    zx

    yx

    xx g

    dx

    dp

    dz

    dvv

    dy

    dvv

    dx

    dvv

    dt

    dv

  • 8/10/2019 TP323Lecture2-2(2)

    28/31

    Special case (Inviscid flow)

    The Euler equation of motion could be re-arranged to get

    the Bernoulli equation

    Bird, Stewart, & Lightfoot, Section 3.3 and example 3.5-1.

    Conditions:

    Steady, fully-developed flow

    Viscosity plays a minor role

    Or, in a more familiar format:

    02

    112

    2

    2

    2

    2

    2

    1

    hhgdpvvp

    p

    2

    2

    22

    1

    2

    11

    22

    Pugz

    Pugz

  • 8/10/2019 TP323Lecture2-2(2)

    29/31

    Another example

    Similar treatment andassumptions: Fully-developed (steady)

    flow

    Far from entrances/exits

    Flow is laminar and 1

    directional:vr= 0

    v = 0

    vz = vz(r)

    p = p(z) Consider boundary

    conditions to evaluatevelocity profile

  • 8/10/2019 TP323Lecture2-2(2)

    30/31

    Summary

    More on equations of change (isothermal)

    Continuity Mass balance

    Momentum equation Effects of convective flux,shear stress and viscous flux, pressure, and gravity

    Common assumptions and boundary conditions

    Limitations

    Important concepts:

    laminar and turbulent flows

    Creeping and inviscid flows

  • 8/10/2019 TP323Lecture2-2(2)

    31/31

    Questions?