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0593_C02_fm  Page 24  Monday, May 6, 2002  1:46 PM





                       24                                                  Dynamics of Mechanical Systems



                       A
                                                        B                A                          B



                                                                                   θ


                      FIGURE 2.5.1                                       FIGURE 2.5.2
                      Two nonzero vectors.                               Vectors A and B connected tail to tail.


                       However, the angle that a vector makes with itself is zero (see Problem P2.5.1); hence, we
                       have:


                                                      ⋅
                                                                   2
                                                    AA =   A A =  A =  A 2                      (2.6.4)
                                                             2
                       where the last equality is a definition of A .
                        Suppose in this last case that A is a unit vector, say n. Then,

                                                                  2
                                                        ⋅
                                                       nn = n =  n = 1                          (2.6.5)
                                                              2
                       Next, suppose that n , n , and n  are mutually perpendicular unit vectors parallel to the
                                         1
                                            2
                                                   3
                       X-, Y-, and Z-axes as shown in Figure 2.6.1. Then, the various scalar products of these unit
                       vectors may be expressed as:
                                                  ⋅
                                                                        ⋅
                                                            ⋅
                                               n n =  1,    nn =   1,    nn =  1                (2.6.6)
                                                              2
                                                                          3
                                                           2
                                                    1
                                                                      3
                                                 1
                                                        ⋅
                                         ⋅
                                       n n =  n ⋅ n =  n n = n ⋅ n =  n ⋅ n =  n ⋅ n =  0       (2.6.7)
                                        1  2    2  1   1  3    3  1   2  3    3  2
                        These results may be expressed in the compact form:
                                                                 1  i =  j
                                                                 
                                                     nn = δ    =                               (2.6.8)
                                                        ⋅
                                                       i  j   ij
                                                                   i ≠  j
                                                                 0
                       where δ  is often called Kronecker’s delta function.
                              ij
                        Next, suppose that n is a unit vector parallel to a line L and that A is a nonzero vector,
                       as in Figure 2.6.2. Then, A • n is:
                                                     ⋅
                                                   An =  A n cosθ  =  A cosθ                    (2.6.9)
                       We can interpret this result as the “projection” of A onto L. Indeed, suppose we express
                       A in terms of two components: one parallel to L, called A , and the other perpendicular
                                                                          
                       to L, called A . Then,
                                   ⊥
                                                         A =  A +  A                           (2.6.10)
                                                              ||   ⊥
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