Page 46 - Intro to Tensor Calculus
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                                              Figure 1.2-2. Cylindrical coordinates.

                   In this symbolic notation, we let T θ denote the identity transformation. That is, using the parameter
               value of θ in the given set of transformation equations produces the identity transformation. The inverse
               transformation can then be expressed in the form of finding the parameter value β such that T α T β = T θ .

               Cartesian Coordinates

                   At times it is convenient to introduce an orthogonal Cartesian coordinate system having coordinates
                i
               y ,  i =1, 2,...,N. This space is denoted E N and represents an N-dimensional Euclidean space. Whenever
                                                     i
               the generalized independent coordinates x ,i =1,... ,N are functions of the y s, and these equations are
                                                                                     0
               functionally independent, then there exists independent transformation equations
                                                       2
                                                    1
                                                  i
                                                              N
                                              i
                                            y = y (x ,x ,...,x ),  i =1, 2,...,N,                     (1.2.34)
               with Jacobian different from zero. Similarly, if there is some other set of generalized coordinates, say a barred
                       i
                                                                               0
                                               0
               system x ,i =1,... ,N where the x s are independent functions of the y s, then there will exist another set
               of independent transformation equations
                                                    1
                                              i
                                                              N
                                                       2
                                                  i
                                            y = y (x , x ,..., x ),  i =1, 2,...,N,                   (1.2.35)
               with Jacobian different from zero. The transformations found in the equations (1.2.34) and (1.2.35) imply
                                                          0
                                                   0
               that there exists relations between the x s and x s of the form (1.2.30) with inverse transformations of the
               form (1.2.32). It should be remembered that the concepts and ideas developed in this section can be applied
               to a space V N of any finite dimension. Two dimensional surfaces (N = 2) and three dimensional spaces
               (N = 3) will occupy most of our applications. In relativity, one must consider spaces where N =4.
               EXAMPLE 1.2-1. (cylindrical coordinates (r, θ, z)) Consider the transformation
                                x = x(r, θ, z)= r cos θ  y = y(r, θ, z)= r sin θ  z = z(r, θ, z)= z
               from rectangular coordinates (x, y, z) to cylindrical coordinates (r, θ, z), illustrated in the figure 1.2-2. By
               letting
                                                                                  3
                                                                 1
                                                                          2
                                                        3
                                       1
                                               2
                                      y = x,  y = y,   y = z    x = r,   x = θ,  x = z
               the above set of equations are examples of the transformation equations (1.2.8) with u = r, v = θ, w = z as
               the generalized coordinates.
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