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                                                  APPENDIX A. DERIVATION OF TRANSPORT EQUATIONS
                               respectively. Such equations are called nonconservative forms of momentum
                               equations.
                            2. Equations A.5, A.11, A.12, and A.13 define the fluid motion completely.
                               However, they contain twelve unknowns (three velocity components and nine
                               stresses). By invoking the rule of complementarity of stresses (i.e., τ ij = τ ji , i  =
                                j), the unknowns can be reduced to nine. Still, the number of unknowns exceeds
                               the number of available equations (four).
                            3. A solvable system must have the same number of unknowns and equations. To
                               do this, Stokes’s stress laws are invoked:
                               Stress Laws


                                                                ∂u i  ∂u j
                                                       τ ij = µ     +       ,                 (A.14)
                                                                ∂x j   ∂x i


                                                                   ∂u i

                                        σ i =−p + σ =−p + 2µ                (no summation),   (A.15)
                                                    i
                                                                   ∂x i
                                                                  2

                               where σ is called the deviatoric stress, p is pressure (compressive), and µ is
                                      i
                               the viscosity of the fluid. 3
                            4. When Equations A.14 and A.15 are substituted in Equations A.11, A.12, and
                               A.13, the new equations can be compactly written in tensor notation as
                               Momentum Equations u i (i =1,2,3)
                                   ∂(ρ m u i )  ∂(ρ m u j u i )  ∂     ∂u i     ∂p
                                           +            =       µ eff    −     + ρ m B i + S u i  . (A.16)
                                      ∂t         ∂x j      ∂x j     ∂x j   ∂x i
                               This equation is the same as Equation 1.3 in Chapter 1. The three equations
                               (A.16) now contain only four unknowns (u 1 , u 2 , u 3 , and p). Along with Equa-
                               tion A.5, therefore, there are as many unknowns as there are equations.



                            2  In Chapter 1, the deviatoric stress is expressed as


                                                                  ∂u i
                                                         σ = 2 µ      + q

                                                          i
                                                                  ∂x i
                              and significance of q is explained in Section 1.5.
                            3  In turbulent flows, the total stress comprises additive contributions of laminar and turbulent com-
                                                    t
                              ponents. The turbulent stress τ =−ρ m u u is again represented in the manner of Equation A.14


                                                    ij      i  j
                              by invoking turbulent viscosity µ t . This is known as the Boussinesq approximation. Then the total
                              stress τ  tot  in a turbulent flow is given by
                                   ij
                                                                              2
                                                       t
                                             τ ij tot  = τ ij + τ = (µ + µ t )  ∂u i  +  ∂u j  −  ρ m e δ ij ,
                                                      ij
                                                                  ∂x j  ∂x i  3
                                                             3


                              where δ ij is the Kronecker delta and e =  i=1  u u /2 is the kinetic energy of velocity fluctuations.
                                                                i
                                                                  i
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