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0593_C13_fm  Page 457  Monday, May 6, 2002  3:21 PM





                       Introduction to Vibrations                                                  457


                       or

                                                     ξ +(           ξ )  =
                                                     ˙˙
                                                             2
                                                      1  2 − )(km    1  0                     (13.8.10)
                       or


                                                         ˙˙ ξ + ω ξ =
                                                              2
                                                          1   1  1  0                          (13.8.11)
                                                      ˙˙
                                                ˙˙
                        Similarly, by considering  ξ 2  and  ξ 3  we have:
                                                         ˙˙  ω ξ =
                                                         ξ +
                                                              2
                                                          2   2  2  0                         (13.8.12)
                       and

                                                         ˙˙  ω ξ =
                                                         ξ +
                                                              2
                                                          3   3  3  0                         (13.8.13)
                        We can recognize Eqs. (13.8.11), (13.8.12), and (13.8.13) as being in the form of the
                       undamped linear oscillator equation, Eq. (13.2.1). The solutions of the equations may thus
                       be expressed as:


                                                                +
                                                    ξ = A cos ω t B sin ω t                   (13.8.14)
                                                     1   1    1    1    1
                                                                +
                                                   ξ = A cos ω t B sin  ω t                   (13.8.15)
                                                    2   2     2    2    2
                                                                +
                                                   ξ = A cos ω t B sin  ω t                   (13.8.16)
                                                    3   3     3    3    3
                       where, as before, the constants A  and B  (i = 1, 2, 3) are to be evaluated from auxiliary
                                                           i
                                                     i
                       conditions.
                        Equations (13.8.14), (13.8.15), and (13.8.16) show that. given suitable auxiliary conditions.
                       the three-particle system will have sinusoidal oscillation, with the “shape,” or mode, of
                       the oscillation being in the form of ξ , ξ , or ξ  as defined by Eqs. (13.8.4), (13.8.5), and
                                                                3
                                                           2
                                                        1
                       (13.8.6).
                        This, however, raises a question: suppose the auxiliary conditions (say, the initial con-
                       ditions) are such that they do not correspond to a shape of one of the modes ξ , ξ , or ξ ;
                                                                                                     3
                                                                                               2
                                                                                             1
                       what, then, is the subsequent motion of the system? The answer is that the subsequent
                       motion may be expressed as a linear combination of the ξ , ξ , and ξ . That is, the ξ , ξ ,
                                                                           1
                                                                                                  1
                                                                                    3
                                                                              2
                                                                                                     2
                       and  ξ  may be regarded as  “base vectors” in a three-dimensional space (for the three
                            3
                       degrees of freedom of the system).
                        To see this, consider again the solutions of Eqs. (13.8 .11), (13.8.12), and (13.8.13) in the
                       form of Eqs. (13.8.14), (13.8.15), and (13.8.16). The derivatives of  ξ ,  ξ , and  ξ  may be
                                                                                      2
                                                                                   1
                                                                                              3
                       expressed as:
                                                 ˙
                                                 ξ =−A  ω  sinω +t B  ω  cosω t               (13.8.17)
                                                  1    1  1   1    1  1    1
                                                 ˙
                                                ξ =−A   ω  sinω +t B  ω  cosω t               (13.8.18)
                                                 2     2  2   2    2  2    2
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