Page 315 - Bird R.B. Transport phenomena
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§10.4  Heat Conduction with a Viscous Heat Source  299

                  Top surface moves with velocity v  = ЯП  Щ-  10.4-2.  Modification of a portion of the flow
                                          b
                                                 system  in Fig. 10.4-1, in which the curvature  of the
                                                                is neglected.
                                                 bounding surfaces
                                           J
                "t  2    /          \     Л(х)


                       Stationary  surface



                    As  the outer cylinder  rotates, each cylindrical  shell  of  fluid  "rubs"  against  an  adja-
                cent  shell  of  fluid.  This  friction  between  adjacent  layers  of  the  fluid  produces heat; that
                is, the mechanical energy  is  degraded  into thermal energy.  The volume  heat source re-
                sulting  from  this "viscous  dissipation," which can be designated  by  S , appears automat-
                                                                          v
                ically  in the shell balance when we  use the combined energy  flux  vector  e defined  at the
                end  of Chapter 9, as we  shall  see presently.
                    If the slit width  b is small with respect to the radius R of  the outer cylinder, then the
                problem  can  be  solved  approximately  by  using  the  somewhat  simplified  system  de-
                picted  in Fig. 10.4-2. That is, we  ignore curvature  effects  and solve the problem in Carte-
                sian coordinates. The velocity  distribution is then v z  = v {x/b),  where v b  = UR.
                                                               b
                    We  now make an energy balance over a shell  of thickness  Ax, width  W, and length L.
                Since the  fluid  is  in motion, we  use  the combined energy  flux  vector  e as  written  in Eq.
                9.8-6. The balance then reads

                                            WLe \  -  WLe \  =  0                   (10.4-1)
                                               x x     x x+Ax
                Dividing by  WL Ax and letting the shell thickness  Ax go to zero then gives

                                                                                    (10.4-2)
                                                  T
                This equation may be integrated to give  dx
                                                  e  =  Q                           (10.4-3)
                                                   x
                Since we  do  not know  any  boundary  conditions for  e x/  we  cannot evaluate  the integra-
                tion constant at this point.
                    We  now  insert the expression  for  e x  from  Eq. 9.8-6. Since the velocity  component in
                the x direction is zero, the term (\pv 2  +  pLOv can be discarded. The x-component of  q  is
                -k(dT/dx)  according  to Fourier's law.  The x-component  of  [т  •  v]  is,  as  shown  in  Eq.
                9.8-1,  T V  +  T v y  +  T V . Z  Since the  only  nonzero component of  the velocity  is  v z  and
                             xy
                       XX
                                    XZ
                         X
                since r xz  =  -\xidvjdx)  according to Newton's law  of viscosity, the x-component of  [т • v]
                is  -ixv (dv /dx).  We  conclude, then, that Eq. 10.4-3 becomes
                        z
                     z
                                                                                    (10.4-4)
                When  the linear velocity  profile  v z  = v (x/b)  is inserted, we  get
                                                b
                                                                                    (10.4-5)
                              2
                in which /ji(v /b)  can be identified  as the rate of viscous  heat production per unit volume S . v
                           b
                    When  Eq. 10.4-5 is integrated we  get
                                         т  -  - г  Ч  л  -  [                      (10.4-6)
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