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336  Chapter  11  The Equations  of Change for Nonisothermal  Systems
                           opposed  to the gravitational  field. For terrestrial  problems, where  the gravitational  field  is
                           independent  of  time, we  can  write
                           p(v-g)  = -(p                                                       (11.1-8)
                                  =  -(V     +  Ф(У  •  pv)       Use vector  identity  in Eq. A.4-19
                                                 dp
                                  =  -(V     -  Ф                 Use Eq.  3.1-4
                                                 dt
                                                                  Use Ф independent  of t

                           When  this result  is inserted  into Eq. 11.1-7 we  get

                                            j -  (\pv 2  + pU  + рФ) = -(V  •  {\pv 2  + pU  + рФ)у)

                                                               -(V-q)-(V-pv)-(V-[T-v])         (11.1-9)
                           Sometimes  it is convenient  to have  the energy  equation in this  form.


     §11.2  SPECIAL FORMS OF THE ENERGY EQUATION

                           The most  useful  form  of  the energy  equation  is  one  in  which  the temperature  appears.
                           The object  of  this  section  is  to arrive  at such  an  equation, which  can be  used  for  predic-
                           tion  of temperature  profiles.
                              First we  subtract  the mechanical energy  equation  in  Eq. 3.3-1  from  the energy  equa-
                           tion in  11.1-7. This leads  to the following equation of change for  internal energy:


                                                    U=     -(V-pl/v)   -(V-q)
                                                  dt  P
                                                 rate of  net rate of  rate  of  internal
                                                 increase  in  addition  of  energy addition
                                                 internal  internal energy  by heat conduction,
                                                 energy   by  convective  per unit
                                                 per unit  transport,  volume
                                                 volume   per unit  volume
                                                                                               (11.2-1)
                                                       -  p(V  • v)  -  (T:VV)
                                                       reversible rate  irreversible rate
                                                       of internal  of internal energy
                                                       energy increase  increase  per unit
                                                       per unit volume  volume  by
                                                       by  compression  viscous  dissipation


                           It  is  now  of  interest  to compare  the mechanical  energy  equation  of  Eq.  3.3-1  and  the in-
                           ternal  energy  equation  of  Eq.  11.2-1. Note that  the  terms  p(V  •  v)  and  (T:VV)  appear  in
                           both  equations—but  with  opposite  signs.  Therefore,  these  terms  describe  the intercon-
                           version  of  mechanical  and  thermal  energy.  The  term  p(V  •  v)  can  be  either  positive  or
                           negative,  depending  on whether  the fluid  is expanding  or contracting; therefore  it repre-
                           sents  a  reversible mode  of  interchange.  On  the  other  hand,  for  Newtonian  fluids,  the
                           quantity  — (T:VV)  is always positive  (see  Eq. 3.3-3) and  therefore  represents  an irreversible
                           degradation  of  mechanical  into  internal  energy.  For  viscoelastic  fluids,  discussed  in
                           Chapter  8, the quantity  -(T:VV)  does  not have  to be  positive,  since  some  energy  may  be
                           stored  as  elastic  energy.
                              We  pointed  out in  §3.5 that the equations  of  change  can be  written  somewhat  more
                           compactly  by  using  the  substantial  derivative  (see  Table  3.5-1).  Equation  11.2-1  can  be
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