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26   Ch a p t e r  O n e


              1.6.4.5 Angular Momentum
              For any finite domain (body), the angular momentum equilibrium equation can be rep-
              resented as:
                                      ∫∫  x t dS + ∫∫∫  ρ x bdV = 0             (1-127)
                                                      ×
                                         ×
                                            n ()
                                       S         V
                 The indicial format can be represented as:
                                        ×=
                                      x t   ex t e =  ex n σ  e
                                             pqr  p q r  pqr  p  j  jq r
                                            xb×=  e x b e
                                                  pqr  p q r
                 Using the divergence theorem for surface integral one obtains:
                                          ⎧  ∂            ⎫ ⎪
                                          ⎪
                                    ∫∫∫  e pqr ⎨  x ∂  x ( σ jq ) + ρ x b dV = 0
                                                       p q ⎬
                                                p
                                     V    ⎩ ⎪  j          ⎭ ⎪
                                           ⎧ ∂( x σ  )  ⎫
                                                        ⎪
                                           ⎪
                                        e pqr ⎨  p  jq  + ρ xb ⎬ = 0
                                                      pq
                                           ⎩ ⎪  x ∂  j  ⎭ ⎪
                                            ⎛ ∂σ     ⎞
                                      e { x ⎜  jq  + ρ b ⎟ +σ  } = 0
                                       pqr  p  x ∂  q   pq
                                            ⎝  j     ⎠
                 Since:
                                             ∂σ
                                               jq
                                                + ρb  = 0
                                             ∂x     q
                                               j
                                              e σ  = 0
                                               pqr  pq
                 or
                                              σ  = σ                            (1-128)
                                                pq  qp
                 This actually means that stress tensor is symmetric. The condition is that there is no
              distributed angular momentum.
              1.6.4.6 Energy Conservation
              The energy conservation principle can be stated as: for any domain of interest, the rate
              of change of the kinetic and internal energy is equal to the rate of work done by the
              surface tractions and body forces, plus other rates of energies entering or leaving the
              surface. Other energies may include all types of energies but are limited to thermal and
              mechanical energies in this book. While a small section may focus on some polar me-
              dium, the majority of the book deals with non-polar media.

                                                1
              The kinetic energy in any domain: K(t) =   ∫  ρvv dV              (1-129)
                                                2  V  ii

              The rate of work by surface traction:   V ∫  tv dS                (1-130)
                                              ∂  ii
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