Page 59 - Bird R.B. Transport phenomena
P. 59

44  Chapter 2  Shell Momentum Balances and Velocity Distributions in Laminar Flow

                          When  this equation is divided  by LW Ax, and the limit  taken as Ax approaches  zero, we
                          get

                                                               ^
                                                              • ' " ° ~ ^  z z l z = L  = pg cos p  (2.2-7)
                          The  first  term on the left  side is exactly  the definition  of the derivative  of ф  with  respect
                                                                                         Х1
                          to  x. Therefore  Eq. 2.2-7 becomes
                                                          г-Ъ-фгАг-L     ^
                                                                     =  p g  p                 ( 2  2  g  )
                                                  dx         L
                          At  this point we have  to write  out explicitly  what  the components ф  and ф  are, mak-
                                                                                    хг
                                                                                           2г
                          ing use of the definition  of ф in Eqs.  1.7-1 to 3 and the expressions  for r xz  and r zz  in Ap-
                          pendix  B.I. This  ensures  that we do not miss  out on any of the forms  of momentum
                          transport. Hence we get
                                                        v v
                                              Фхг  =  T xz + P x z  =  ~t*>  y  1  + pv v      (2.2-9a)
                                                                        x z
                                              ф 2г  — p  H~ T , + pv v  = p — 2fji  —^ + pv v  (2.2-9b)
                                                        Z
                                                                              z 7
                                                             z z
                          In  accordance with  the postulates  that v z  = v (x), v x  = 0, v y  = 0, and p = p(x), we see that
                                                                z
                           (i)  since  v x  =  0, the pv v  term  in  Eq. 2.2-9a  is  zero;  (ii) since  v z  =  v (x),  the term
                                                                                         z
                                               x z
                           -2l±(d /dz)  in Eq. 2.2-9b is zero; (iii) since v z  = v (x), the term pv v  is the same  at z = 0
                                z
                                                                    z
                                                                                 z z
                          and  z = L; and (iv) since p = p(x), the contribution p is the same at z = 0 and z = L. Hence
                          T XZ  depends  only on x, and Eq. 2.2-8 simplifies  to
                                                                                               (2.2-10)
                          This is the differential  equation for the momentum flux T . It may be integrated  to give
                                                                           XZ
                                                       r xz  = (pg cos p)x + C,                (2.2-11)
                          The  constant  of  integration  may be evaluated  by  using  the boundary  condition  at the
                           gas-liquid  interface  (see §2.1):
                           B.C.I:                      atx = 0,   r xz  = 0                    (2.2-12)
                          Substitution  of this boundary  condition into Eq. 2.2-11 shows  that C }  = 0. Therefore the
                           momentum-flux  distribution is
                                                         r  = (pg cos P)x                      (2.2-13)
                                                          xz
                           as shown  in Fig. 2.2-3.
                              Next we substitute  Newton's law of viscosity
                                                          *«=-"£                             a2 i4)
                                                                                                -

                           into the left side of Eq. 2.2-13 to obtain
                                                       dv^   Jpg  cos p
                                                        dx    \  V-

                           which  is the differential  equation  for the velocity  distribution.  It can be integrated  to
                           give
                                                           /oe cos B
                                                              2    У  + С 2                    (2.2-16)
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