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78   Chapter 3  The Equations of Change for  Isothermal Systems

                            Here  (V • pv)  is  called  the "divergence  of pv,"  sometimes written as  "div  pv."  The vector
                            pv  is the mass flux, and its divergence  has a simple meaning: it is the net rate of mass  ef-
                            flux per  unit volume. The derivation in Problem 3D.1 uses  a volume element of  arbitrary
                            shape; it is not necessary  to use a rectangular volume element as we have done here.
                               A very important special  form  of the equation of continuity is that for  a  fluid  of con-
                            stant density, for  which  Eq. 3.1-4 assumes  the particularly simple  form

                            (incompressible  fluid)          (V • v)  = 0                        (3.1-5)
                            Of  course, no  fluid  is truly  incompressible, but  frequently  in engineering and  biological
                            applications,  the  assumption  of  constant density  results  in  considerable  simplification
                            and  very little error. '
                                             1 2

       EXAMPLE 3.1-1        Show that for  any kind  of flow pattern, the normal stresses  are zero at fluid-solid boundaries,
                            for  Newtonian  fluids  with  constant density.  This  is  an  important result  that  we  shall  use
      Normal  Stresses  at  often.
      Solid Surf aces  for
      Incompressible        SOLUTION
      Newtonian  Fluids
                            We  visualize  the flow of  a fluid near some solid  surface,  which  may  or may  not be flat. The
                            flow may be quite general, with  all three velocity  components being  functions  of  all three co-
                            ordinates  and  time. At  some  point P on the surface  we  erect a Cartesian coordinate system
                            with the origin at P. We now ask what the normal stress  r  is at P.
                                                                         22
                               According to Table B.I or Eq. 1.2-6, T  = —lyXdvJdz), because  (V • v)  = 0 for incompress-
                                                             ZZ
                            ible fluids. Then at point P on the surface  of the solid
                                                         to,
                                              r zz \ z=0 =  -                                    (3.1-6)
                                                        ' dz
                            First we  replaced  the derivative  dvjdz  by  using  Eq. 3.1-3  with  p constant. However,  on the
                            solid  surface  at z  = 0, the velocity  v x  is zero by  the no-slip condition (see §2.1), and  therefore
                            the  derivative  dv /dx  on the surface  must be zero. The same is true  of  dv /dy  on the  surface.
                                         x
                                                                                      y
                            Therefore r,  is zero. It is also true that т  and r yy  are zero at the surface  because  of the vanish-
                                     2
                                                            хх
                            ing  of  the derivatives  at z  =  0. (Note:  The vanishing  of  the normal stresses  on solid  surfaces
                            does  not apply  to polymeric fluids,  which  are viscoelastic.  For compressible  fluids,  the nor-
                            mal  stresses  at solid  surfaces  are zero  if  the density  is not changing with time, as is shown in
                            Problem 3C.2.)
      §3.2  THE EQUATION       OF MOTION

                            To  get  the equation  of  motion we  write  a momentum balance over  the volume element
                            Ax  Ay  Az in Fig. 3.2-1  of the form
                                          rate of         rate of       rate of     external
                                         increase   = momentum -      momentum + force on        (3.2-1)
                                       of momentum         in            out        the  fluid



                                1
                                L. D. Landau and E.  M. Lifshitz, Fluid Mechanics, Pergamon Press, Oxford  (1987), p. 21, point out
                            that, for steady, isentropic flows, commonly encountered in aerodynamics, the incompressibility
                            assumption is valid when the fluid velocity  is small  compared to the velocity  of sound  (i.e., low Mach
                            number).
                               2
                                 Equation 3.1-5 is the basis for Chapter 2 in G. K. Batchelor, An Introduction to Fluid Dynamics,
                            Cambridge  University  Press  (1967), which is a lengthy  discussion  of the kinematical consequences  of the
                            equation of continuity.
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