Page 353 - Bird R.B. Transport phenomena
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§11.2  Special Forms of the Energy Equation  337

                 put  in  the  substantial  derivative  form  by  using  Eq.  3.5-4.  This  gives,  with  no  further
                 assumptions

                                        t^±=  -(V-q)-p(V-v)-(T:Vv)                   (11.2-2)

                 Next  it  is  convenient  to switch  from  internal energy  to enthalpy, as  we  did  at  the very
                 end  of  §9.8. That is, in  Eq. 11.2-2 we  set  U  = H  -  pV  = H  -  (p/p), making  the standard
                 assumption  that  thermodynamic formulas  derived  from  equilibrium  thermodynamics
                 may  be  applied  locally  for  nonequilibrium  systems.  When  we  substitute  this  formula
                 into Eq. 11.2-2 and use the equation of continuity (Eq. A  of Table 3.5-1), we  get

                                                                                     (11.2-3)

                 Next  we  may  use  Eq. 9.8-7, which  presumes  that the enthalpy  is  a  function  of  p  and T
                 (this restricts  the subsequent  development  to Newtonian fluids). Then we  may  get  an  ex-
                 pression  for  the change in the enthalpy in an element  of  fluid  moving  with  the fluid  ve-
                 locity, which  is
                                                                  Dp
                                      DH     ~  DT
                                       Dt   p ^  Dt               Dt
                                             ~  DT
                                            p L
                                             ?  Dt                   Dt
                                                                  ' P .
                                                                  Dp
                                            ^   Dt                Dt                 (11.2-4)
                 Equating the right sides  of  Eqs. 11.2-3 and  11.2-4 gives

                                                                                     (11.2-5)


                 This  is  the equation  of change for  temperature,  in  terms  of  the heat flux vector  q  and  the
                 viscous  momentum flux tensor  т.  То use  this  equation  we  need  expressions  for  these
                 fluxes:
                    (i)  When  Fourier's law  of  Eq. 9.1-4  is used, the term  -(V  •  q) becomes  +(V * kVT),
                                                                        2
                         or, if the thermal conductivity is assumed  constant, +kV T.
                    (ii)  When Newton's law  of  Eq. 1.2-7  is used, the term  — (T:VV) becomes дФ  + к"Фу,
                                                                                     у
                         the quantity given explicitly  in Eq. 3.3-3.
                 We  do not perform  the substitutions  here, because  the equation  of  change  for  tempera-
                 ture is almost never used  in its complete generality.
                    We  now discuss  several  special restricted versions  of the equation  of change for tem-
                 perature.  In all  of  these we  use  Fourier's law  with  constant k, and  we  omit the  viscous
                 dissipation  term, since it is important only in flows with enormous velocity  gradients:
                                                      -
                    (i)  For an ideal gas, (d In p/д  In T)  = 1 , and
                                                  p
                                                 oC  ^ -                             (11.2-6)
                                                 pC
                                                  ?Dt   ~       Dt
                         Or, if use  is made of  the relation C  — C  = R, the equation  of  state in the form
                                                      p   v
                        pM = pRT, and the equation of continuity as written in Eq. A  of Table 3.5-1, we get

                                                          2
                                                      =  kV T  -   v)                (11.2-7)
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