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Introduction and Fundamentals for Mathematics and Continuum Mechanics   5


              compresses one or two of the three dimensions to zero, one can have two-dimensional
              (2D) vectors and a 1D vector (a scalar). A vector is also called a first-order tensor, having
               1
              3 = 3 independent bases. Mathematically, a set of mutually independent N variables
              can be considered as an N dimensional vector. Lower-case characters such as v and u
              are used to represent vectors in this chapter. Vectors can be also represented in indicial
              format as v i and u i  (i = 1~3). Vectors in rigorous sense (2D and 3D) follow the triangle
              rule for “add” and “subtract.” Abstract extension to an N dimensional vector may not
              follow such rules.
                 A vector can be represented in its indicial format as follows:
                                                         3
                                      ν = ν e  + ν e  +  ν e  =  ∑ ν e            (1-1)
                                          11   2 2  3 3    ii
                                                        i  =1
                 Where e i  are the three bases (with unit length). By following the Einstein convention
              (the dummy index or the repeaded index will sum running from 1 to 3), it can be simply
              represented as Equation 1-2:
                                               n = n i  e i                       (1-2)
                  v =  v + v +  v  is the magnitude of a vector or the “normal/mod/length” of a
                               2
                        2
                           2
                        1  2   3
              vector (see Figure 1.1a). The vector can be generally represented as scalar (magnitude)
              in an orientation where e is the orientation. It is this orientation that needs a reference
              system to measure it. The above representation (Equation 1-1) is for a Cartesian refer-
              ence system.
                 Addition or subtraction of vectors will follow the following rules (Figure 1.1b):
                                           u v w e =,
                                        w =±         ( u ± )                      (1-3)
                                                         v e
                                                 ii   i   i  i
                                 X 2


                                                                      b
                                                             a
                                  a 3  a
                                                                    c
                                a 1
                                       a 2
                                                  X 1            a + b = c
                        X 3        (a)                           (b)

                                   b                    c
                                                               b

                                                                     a
                                     c      a
                           a · b = c                              a   b = c
                                   (c)                           (d)

              FIGURE 1.1  Illustration of typical vector operations.
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