Page 304 - Intro to Tensor Calculus
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               we cannot interchange the order of differentiation and integration in this term. Here we must use the result
               that                             Z        Z
                                             D                ∂e t
                                                                         ~
                                                   e t dτ =      + ∇· (e t V )  dτ.
                                             Dt               ∂t
                                                 V         V
               To prove this result we consider a more general problem. Let A denote the amount of some quantity per
               unit mass. The quantity A can be a scalar, vector or tensor. The total amount of this quantity inside the
                                   R
               control volume is A =  %A dτ and therefore the rate of change of this quantity is
                                    V
                                             Z                Z         Z
                                        ∂A      ∂(%A)      D
                                                                              ~
                                           =          dτ =       %A dτ −   %AV · ˆndS,
                                        ∂t        ∂t       Dt
                                              V                V         S
               which represents the rate of change of material within the control volume plus the influx into the control
               volume. The minus sign is because ˆn is always a unit outward normal. By converting the surface integral to
               a volume integral, by the Gauss divergence theorem, and rearranging terms we find that
                                              Z         Z
                                           D                ∂(%A)
                                                                           ~
                                                 %A dτ =          + ∇· (%AV ) dτ.
                                           Dt                 ∂t
                                               V          V
                                                                                           ij
                                                                                                       i
                   In equation (2.5.46) we neglect all isolated external forces and substitute F i  = σ n j , F i  = b where
                                                                                     (s)         (b)
               σ ij = −pδ ij + τ ij . We then replace all surface integrals by volume integrals and find that the conservation of
               energy can be represented in the form
                                        ∂e t                                     ∂Q
                                                               ~
                                                    ~
                                                                          ~ ~
                                            + ∇· (e t V )= ∇(σ · V ) −∇· ~q + %b · V +                (2.5.47)
                                         ∂t                                       ∂t
                                         2
                                2
                                    2
                                                                                   e
               where e t = %e + %(v + v + v )/2 is the total energy and σ =  P 3 i=1  P 3 j=1  σ ij ˆ i ˆ j is the second order stress
                                                                                     e
                                         3
                                    2
                                1
               tensor. Here
                                              3           3            3
                                             X           X            X
                                                                                     ~
                                  ~
                                                                                            ~
                                         ~
                              σ · V = −pV +     τ 1j v j ˆ 1 +  τ 2j v j ˆ 2 +  τ 3j v j ˆ 3 = −pV + τ · V
                                                                 e
                                                     e
                                                                              e
                                             j=1         j=1          j=1
                         ∗
               and τ ij = µ (v i,j + v j,i )+ λ δ ij v k,k is the viscous stress tensor. Using the identities
                                       ∗
                                                                                        2
                                  D(e t /%)  ∂e t                 D(e t /%)  De     D(V /2)
                                                       ~
                                 %        =     + ∇· (e t V )  and %      = %   + %
                                    Dt       ∂t                     Dt       Dt       Dt
                                                                    ~
               together with the momentum equation (2.5.25) dotted with V as
                                                ~
                                              DV
                                                   ~
                                                                               ~
                                                                   ~
                                                        ~ ~
                                            %     · V = %b · V −∇p · V +(∇·τ ) · V
                                              Dt
               the energy equation (2.5.47) can then be represented in the form
                                               De                      ∂Q
                                                          ~
                                                                    q
                                              %    + p(∇· V )= −∇ · ~ +    +Φ                         (2.5.48)
                                                Dt                      ∂t
               where Φ is the dissipation function and can be represented
                                                                     ~
                                                                                  ~
                                         Φ=(τ ij v i ) ,j − v i τ ij,j = ∇· (τ · V ) − (∇·τ ) · V.
                                                                                                          ∗
                                                                                                ∗
               As an exercise it can be shown that the dissipation function can also be represented as Φ = 2µ D ij D ij +λ Θ 2
               where Θ is the dilatation. The heat flow vector is determined from the Fourier law of heat conduction in
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