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Mathematical preliminaries – vector and tensor analysis  23

                                                                                         k
                          We have seen in eqn (1.125) that, for a second-order tensor T, ∂T/∂x can be
                                                                                       3
                                                                     3
                        regarded as a linear operator, acting on vectors in E to give vectors in E .When it
                                                         k
                        acts on the contravariant base vector g , the resulting vector is called the divergence
                        of T, and we write

                                                              ∂T   k
                                                    ∇· T =        g                       (1.153)
                                                             ∂x k
                        with summation over k.Inother words,
                                         ij        k    ij      k     ij  k    ij
                                ∇· T = (T g i ⊗ g j )g = T g i (g j · g ) = T g i δ = T g i ,  (1.154)
                                         ,k            ,k             ,k  j    ,j
                        expressed in terms of the covariant derivatives of the contravariant components of T.

                        Exercise 13. Verify the formulas
                                       1  ∂  √    ij       1  ∂  √    ij    kj  i
                              ∇· T = √       ( gT g i ) =  √     ( gT ) + T    kj  g i .  (1.155)
                                        g ∂x j              g ∂x j

                        Exercise 14. Show that if p is a scalar field and I is the unit second-order tensor
                        (defined in eqn (1.87)), then
                                                      ∇· (pI) =∇p.                        (1.156)



                           1.8 Summary of formulas in two dimensions

                        For two-dimensional situations in which field variables depend only on the rectangular
                        cartesian co-ordinates x and y but not z, it is straightforward to establish the reduced
                        form of the above results. We give a summary here of some of the main results for
                        convenience.
                                                                              1
                                                                                      2
                          With y 1 = x, y 2 = y, and curvilinear co-ordinates with x = ξ, x = η (and
                                                             3
                        occasionally finding it useful to put y 3 = x = z = ς), wehavebasevectors
                                          g 1 = ix ξ + jy ξ ,  g 2 = ix η + jy η ,  g 3 = k,  (1.157)
                        where suffixes denote partial differentiation, e.g. x ξ = ∂x/∂ξ. The components of the
                        covariant metric tensor are given by

                                                    2    2                    
                                  g 11  g 12  g 13    x + y ξ     x ξ x η + y ξ y η  0
                                                       ξ
                                                                    2
                                g 12  g 22  g 23    =    x ξ x η + y ξ y η  x + y 2 η  0    ,  (1.158)
                                                                   η
                                  g 13  g 23  g 33    0           0            1
                        with determinant
                                                                    2
                                                    g = g 11 g 22 − (g 12 ) .             (1.159)
                          Moreover

                                                         x ξ  x η
                                                                 0
                                      √
                                       g = g 1 × g 2 · g 3 =     y ξ  y η  0     = (x ξ y η − x η y ξ ).  (1.160)

                                                         0   0   1
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