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0593_C11_fm  Page 401  Monday, May 6, 2002  2:59 PM





                       Generalized Dynamics: Kinematics and Kinetics                               401


                                                                                 θ
                                                         θ
                                                                            ˙ ˙
                                        *
                                                 32
                                       F =−mr 2 [ ( ) ψ ˙˙ sin +( ) ˙˙  2 θ +( ) φθsin cos θ
                                                            32
                                                                φsin
                                                                        52
                                        φ
                                                                                              (11.12.33)
                                            +( ) ˙˙  θ   1  ψθcos θ]
                                                            ˙ ˙
                                                 φcos −( ) 2
                                             14
                       and
                                                                            ˙ ˙
                                                                ˙˙
                                                                    θ
                                            *
                                           F =−mr  2 [ ( ) ψ ˙˙ +( ) φsin +( )  θφcos θ ]     (11.12.34)
                                                     32
                                                                       52
                                                            32
                                            ψ
                        While Eqs. (11.12.29), (11.12.30), and (11.12.31) are similar to Eqs. (11.12.32), (11.12.33),
                       and (11.12.34), they are not identical; therefore, Eq. (11.12.5) is not valid for nonholonomic
                       systems. It happens, however, that Eq. (11.12.5) may be modified and expanded to also
                       accommodate nonholonomic systems. Although the details of this expansion are beyond
                       the scope of this text, the interested reader is referred to References 11.2 and 11.4.
                       11.13 Closure
                       Our objective in this chapter has been to introduce the principles and procedures of
                       generalized dynamics. Our intention was to obtain a working knowledge of the elementary
                       procedures. More advanced procedures, such as those applicable with large multibody
                       systems and, to some extent, those concerned with nonholonomically constrained systems,
                       have not been discussed because they are beyond our scope at this time. The interested
                       reader may want to refer to References 11.2 and 11.4 and later chapters for a discussion
                       of these topics.
                        The examples are intended to demonstrate the principal advantages of the generalized
                       procedures over the procedures used in elementary mechanics, including: (1) non-working
                       constraint forces do not contribute to the generalized forces so these forces may be simply
                       ignored in the analysis; and (2) for holonomic systems (which include the vast majority
                       of systems of interest in machine dynamics), generalized inertia forces may be computed
                       from kinetic energy functions. This in turn means that vector acceleration need not be
                       computed, thus saving considerable analysis effort.
                        In addition to these advantages, if a system possesses a potential energy function, the
                       generalized active (or applied) forces may be obtained by a single derivative of the
                       potential energy function. Moreover, for gravity and spring forces (which are prevalent
                       in machine dynamics), the potential energy functions may often be directly obtained from
                       Eqs. (11.11.5) and (11.11.10). In the next chapter, we will consider the application of these
                       procedures in obtaining equations of motion.





                       References
                       11.1. Kane, T. R., Dynamics, Holt, Rinehart & Winston, New York, 1968, p. 78.
                       11.2. Kane, T. R., and Levinson, D. A., Dynamics: Theory and Applications, McGraw-Hill, New York,
                           1985, p. 100.
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