Plug Flow Reactor Non Isothermal

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    Plug flow is a simplified and idealized picture of the

    motion of a fluid, whereby all the fluid elementsmove with a uniform velocity along parallelstreamlines.

    This perfectly ordered flow is the only transportmechanism accounted for in the plug flow reactormodel.

    Because of the uniformity of conditions in a crosssection the steady-state continuity equation is a verysimple ordinary differential equation.

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    z z + zz = 0

    z

    z = L

    z

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    MASS BALANCE

    VAF

    VVAFVrA

    0FVrFVVAAVA

    dtdN A

    VrFFAVAVVA

    Rate of flowof A into avolumeelement

    Rate of flowof A out ofthe volumeelement

    Rate ofgeneration of A bychemical reactionwithin the volumeelement

    Rate ofaccumulationof A withinthe volumeelement

    + =

    For steady-state process: 0dt

    dN A

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    Arz

    FFA

    zAzzA

    0zlim

    AVAVVA

    rV

    FF

    AA r

    dVdF

    VrFF AVAVVA

    By definition of the conversion X1FF 0AA

    dXFdF 0AA

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    So that the continuity for A becomes:

    dVrdXF A0A

    A0A

    rF

    dXdV

    (1.1)

    Design equation

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    To design an isothermal tubular/plug-flow reactor, thefollowing information is needed:

    1. Design equation

    2. Rate law

    (for first order reaction)

    3. Stoichiometry (liquid phase)

    A0A

    rF

    dXdV

    AA Ckr

    X1CC 0AA

    (1.1)

    (1.2)

    (1.3)

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    Combining eqs. (1.2) and (1.3) yields:

    X1Ckr 0AA

    Introducing eq. (1.4) into eq. (1.1) yields:

    XX

    0A

    X

    X 0A0A0

    0

    X1lnCk 1X1kC dXFV

    X1X1

    lnkCF

    X1X1

    lnkCF

    V 0

    0A

    0A

    00A

    0A

    (1.4)

    X1

    X1ln

    k

    v

    X1

    X1ln

    k

    vV 00

    0

    0

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    T1

    T1

    RE

    expkk1

    1

    (1.5)

    (1.6)

    Combining eqs. (1.5) and (1.6) yields:

    (1.7)

    Combining eqs. (1.1), (1.3), and (1.4) yields:

    00A

    0A

    v X1kF X1kCdVdX

    Recalling the Arrhenius equation:

    T1

    T1

    TE

    expX1vk

    dVdX

    10

    1

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    For an open system in which some of the energy exchangeis brought about by the flow of mass across the system

    boundaries, the energy balance for the case of only onespecies entering and leaving becomes:

    Rate of

    accumu-lation ofenergy

    within thesystem

    + =

    Rate of flowof heat tothe systemfrom the

    surrounding

    Rate workdone by thesystem on

    thesurrounding

    Rate of

    energy addedto the systemby mass flow

    into thesystem

    Rate energyleaving

    system bymass flow outof the system

    outoutininsys EFEFWQ

    dt

    dE (1.9)

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    The unsteady-state energy balance for an open system

    that has n species, each entering and leaving the system atits respective molar flow rate F i (mole of i per time) andwith its respective energy E i (joules per mole of i), is:

    out

    n

    1iii

    in

    n

    1iii

    sys FEFEWQ dt

    dE (1.10)

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    It is customary to separate the work term, , into:

    flow work: work that is necessary to get the mass intoand out of the system

    other work / shaft work, .

    For example, when shear stresses are absent:

    W

    SW

    S

    out

    n

    1i

    ii

    in

    n

    1i

    ii WPVFPVFW

    [rate of flow work]

    (1.11)

    where P is the pressure and V i is the specific volume.

    Stirrer in a CSTR Turbine in a PFR

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    Combining eqs. (1.10) and (1.11) yields:

    outn

    1iiii

    in

    n

    1iiiiS

    sys

    PVEFPVEFWQ dt

    dE

    (1.12)

    The energy E i is the sum of the internal energy (U i), thekinetic energy , the potential energy (gzi), and any

    other energies, such as electric energy or light: 2u 2i

    othergz2u

    UE i2i

    ii (1.13)

    In almost all chemical reactor situations, the Kinetic,potential, and other energy terms are negligible incomparison with the enthalpy, heat transfer:

    ii UE (1.14)

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    Recall the definition of enthalpy:

    iii PVUH (1.15)

    Combining eqs. (1.16), (1.15), and (1.13) yields:

    out

    n

    1iii

    in

    n

    1iiiS

    sys HFHFWQ dt

    dE (1.16)

    We shall let the subscript 0 represent the inletconditions. The un-subscripted variables represent the

    conditions at the outlet of the chosen system volume.

    n

    1iii

    n

    1i0i0iS

    sys HFHFWQ dt

    dE(1.17)

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    The steady-state energy balance is obtained by setting(dEsys/dt) equal to zero in eq. (1.17) in order to yield:

    0HFHFWQ n

    1iii

    n

    1i0i0iS (1.18)

    To carry out the manipulations to write eq. (1.18) interms of the heat of reaction we shall use the

    generalized reaction:

    (1.19)DdCcBbA

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    The inlet and outlet terms in Equation (1.19) areexpanded, respectively, to:

    0I0I0D0D0C0C0B0B0A0A0i0i FHFHFHFHFHFH

    IIDDCCBBAAii FHFHFHFHFHFH

    In:

    Out:

    (1.20)

    (1.21)

    We first express the molar flow rates in terms of conversion

    X1FF 0AA

    XbFFFXFbFF

    0A

    0B0A0A0BB

    XbFF B0AB (1.23)

    (1.22)

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    XcF

    FFXFcFF

    0A

    0C0A0A0CC

    XcFF C0AC (1.24)

    XdFF D0AD (1.25)

    I0A0A

    0I0A0II FF

    FFFF (1.26)

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    The term in parentheses that is multiplied by F A0X is calledthe heat of reaction at temperature T and is designated

    HRx.

    THTHbTHcTHdH ABCDRx (1.28)

    All of the enthalpies (e.g., H A, HB) are evaluated at thetemperature at the outlet of the system volume, andconsequently, [ HRx(T)] is the heat of reaction at thespecific temperature ip: The heat of reaction is alwaysgiven per mole of the species that is the basis ofcalculation [i.e., species A (joules per mole of A reacted)].

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    Substituting eq. (1. 28) into (1. 27) and reverting to

    summation notation for the species, eq. (1. 28) becomes

    XFHHHFFHFH 0ARxn

    1ii0ii0A

    n

    1iii

    n

    1i0i0i (1.29)

    Substituting eq. (1.29) into (1.18) yields:

    0XFHHHFWQ 0ARx

    n

    1i i0ii0AS (1.30)

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    The enthalpy changes on mixing so that the partial molalenthalpies are equal to the molal enthalpies of the purecomponents.

    The molal enthalpy of species i at a particular temperatureand pressure, H i, is usually expressed in terms of anenthalpy of formation of species i at some referencetemperature T R, Hi (TR), plus the change in enthalpy that

    results when the temperature is raised from the referencetemperature to some temperature T, H Qi

    QiR0ii HTHH (1.31)

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    The reference temperature at which H i is given is usually25C. For any substance i that is being heated from T 1 to T 2 inthe absence of phase change

    2

    1

    T

    TPQi dTCH (1.32)

    A large number of chemical reactions carried out inindustry do not involve phase change. Consequently, weshall further refine our energy balance to apply to single-phase chemical reactions. Under these conditions the

    enthalpy of species i at temperature T is related to theenthalpy of formation at the reference temperature T R by

    T

    T

    piR0ii

    R

    dTCTHH (1.33)

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    The heat of reaction at temperature T is given in eq. (1.28):

    THTHbTHcTHdH ABCDRx (1.28)

    where the enthalpy of each species is given by eq. (1.33):

    T

    TpiR

    0ii

    R

    dTCTHH (1.33)

    If we now substitute for the enthalpy of each species, we have

    R0AR

    0BR

    0CR

    0DRx THTbHTcHTdHH

    T

    T

    pApBpCpDR

    dTCbCcCdC (1.37)

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    The first set of terms on the right-hand side of eq. (1.37) isthe heat of reaction at the reference temperature T R ,

    R0AR

    0BR

    0CR

    0DR

    0Rx THTHbTHcTHdTH (1.38)

    The second term in brackets on the right-hand side of eq.

    (1.37) is the overall change in the heat capacity per mole of Areacted, C p,

    pApBpCpDp CbCcCdCC (1.39)

    Combining Equations (1.38), (1.39), and (1.37) gives us

    T

    TpR

    0RxRx

    R

    dTCTHTH (1.40)

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    The heat flow to the reactor, Q , is given in terms of the overallheat-transfer coefficient, U, the heat-exchange area, A, andthe difference between the ambient temperature, T a, and thereaction temperature, T.

    When the heat flow vanes along the length of the reactor,such as the case in a tubular flow reactor, we must integratethe heat flux equation along the length of the reactor toobtain the total heat added to the reactor,

    V

    0a

    A

    0a dVTTUadATTUQ

    where a is the heat-exchange area per unit volume of reactor.

    (1.41)

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    The variation in heat added along the reactor length (i.e.,volume) is found by differentiating with respect to V :

    TTUadVQ d

    a (1.42)

    For a tubular reactor of diameter D, a = D/4For a packed-bed reactor, we can write eq. (1.43) in terms of

    catalyst weight by simply dividing by the bulk catalystdensity

    TTUa

    dV

    Q d1a

    BB

    (1.43)

    Recalling dW = B dV, then

    TTUa

    dW

    Q da

    B

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    Substituting eq. (1.40) into eq. (1.36), the steady-state energy

    balance becomes

    0XFdTCTHdTCFWQ 0AT

    TpR

    0Rx

    n

    1i

    T

    Tpii0AS

    R0i

    (1.44)

    For constant of mean heat capacity:

    n

    1i0ipii0A0ARpR

    0RxS TTC

    FXFTTC

    THWQ

    (1.45)

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    EXAMPLE 1.1Calculate the heat of reaction for the synthesis of ammoniafrom hydrogen and nitrogen at 150C in kcal/mol of N

    2reacted.

    SOLUTION

    Reaction: N2

    + 3H2 2NH

    3

    R0NR

    0HR

    0NHR

    0Rx THTH3TH2TH 223

    = 2 ( 11.02) 3 (0) 0 = 20.04 kcal/mol N 2

    K.Hmolcal992.6C 2p2H

    K.Nmolcal984.6C 2p2N

    K.NHmolcal92.8C 3p 3NH

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