Page 91 - Intro to Tensor Calculus
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               form. We observe that the direction cosines can be written as

                                  ˆ                       ˆ                        ˆ
                         ` 11 = b e 1 · e 1 =cos θ 11  ` 12 = b e 1 · e 2 =cos θ 12  ` 13 = b e 1 · e 3 =cos θ 13
                                  ˆ                       ˆ                        ˆ
                         ` 21 = b e 2 · e 1 =cos θ 21  ` 22 = b e 2 · e 2 =cos θ 22  ` 23 = b e 2 · e 3 =cos θ 23  (1.3.41)
                                  ˆ                       ˆ                        ˆ
                         ` 31 = b e 3 · e 1 =cos θ 31  ` 32 = b e 3 · e 2 =cos θ 32  ` 33 = b e 3 · e 3 =cos θ 33
               which enables us to write the equations (1.3.39) and (1.3.40) in the form

                                                y i = ` ij y j  and  y = ` ji y j .                   (1.3.42)
                                                                     i

               Using the index notation we represent the unit vectors as:

                                                ˆ                          ˆ
                                                e r = ` pr b e p  or  b e p = ` pr e r                (1.3.43)

               where ` pr are the direction cosines. In both the barred and unbarred system the unit vectors are orthogonal
               and consequently we must have the dot products

                                             ˆ   ˆ
                                             e r · e p = δ rp  and  b e m · b e n = δ mn              (1.3.44)

               where δ ij is the Kronecker delta. Substituting equation (1.3.43) into equation (1.3.44) we find the direction
               cosines ` ij must satisfy the relations:

                                   ˆ  ˆ
                                   e r · e s = ` pr b e p · ` ms b e m = ` pr ` ms b e p · b e m = ` pr ` ms δ pm = ` mr ` ms = δ rs
                                                                ˆ
                                              ˆ
                                                     ˆ
                                                                     ˆ
                           and     b e r · b e s = ` rm e m · ` sn e n = ` rm ` sn e m · e n = ` rm` sn δ mn = ` rm` sm = δ rs .
               The relations
                                                            and     ` rm ` sm = δ rs ,                (1.3.45)
                                             ` mr ` ms = δ rs
               with summation index m, are important relations which are satisfied by the direction cosines associated with
               a rotation of axes.
                   Combining the rotation and translation equations we find


                                                   y i = ` ij y j  +  b i  .                          (1.3.46)
                                                                  |{z}
                                                         |{z}
                                                        rotation  translation
               We multiply this equation by ` ik and make use of the relations (1.3.45) to find the inverse transformation


                                                       y = ` ik (y i − b i ).                         (1.3.47)
                                                        k
               These transformations are called linear or affine transformations.
                   Consider the x i axes as fixed, while the x i axes are rotating with respect to the x i axes where both sets
                                                ~
                                                     i
               of axes have a common origin. Let A = A b e i denote a vector fixed in and rotating with the x i axes. We
                          ~         ~
                         dA       dA
                                                       ~
               denote by       and      the derivatives of A with respect to the fixed (f) and rotating (r) axes. We can
                         dt        dt
                            f         r
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