Page 354 - Dynamics of Mechanical Systems
P. 354

0593_C10_fm  Page 335  Monday, May 6, 2002  2:57 PM





                       Introduction to Energy Methods                                              335



                                                              O

                                                         θ  i

                                                        θ
                                                         f

                                                                                     P
                       FIGURE 10.8.3
                       A simple pendulum released from
                       rest and falling through angle θ i  – θ f .            P

                       or

                                                                i)
                                                    (
                                                 mgl cosθ − cosθ =  1 m lθ ˙ f ( ) 2           (10.8.8)
                                                         f
                                                                   2
                       Solving for   we have:θ ˙  f

                                                  ˙
                                                  θ = 2  g l ( cosθ − cosθ i)  / 12            (10.8.9)
                                                   f             f
                        The result of Eq. (10.8.9) could also have been obtained by integrating the governing
                       differential equations of motion obtained in Chapter 8. Recall from Eq. (8.4.4) that for a
                       simple pendulum the governing equation is:

                                                       ˙˙  g  sinθ = 0                        (10.8.10)
                                                       θ +( ) l
                                                                      θ
                                                                      ˙
                       Then, by multiplying both sides of this equation by  , we have:
                                                      ˙˙˙
                                                                   ˙
                                                      θθ +( ) l  sinθθ = 0                     (10.8.11)
                                                           g
                                                                  2 ˙
                                                                 θ
                       Because  θθ  may be recognized as being (1/2)d /dt, we can integrate the equation and
                               ˙ ˙˙
                       obtain:
                                                 ( 12)θ 2 ˙  −( )cosθ  =  constant            (10.8.12)
                                                          g
                                                            l
                       Because   is zero when θ is θ , the constant is –(g/ )cosθ . Therefore, we have:θ ˙  i  i

                                                        2 )(
                                                    ˙ 2
                                                    θ = ( g l  cosθ − cosθ )                  (10.8.13)
                                                                        i
                       When θ is θ , Eqs. (10.8.9) and (10.8.13) are seen to be equivalent.
                                 f
                        The work–energy principle may also be used to determine the pendulum rise angle
                       when the speed at the equilibrium position (θ = 0) is known. Specifically, suppose the
                       angular speed of the pendulum when  θ is zero is  θ ˙  o . Then, the work W  done on the
                       pendulum as it rises to an angle θ  is:
                                                     f
                                                                  (
                                                         ∆
                                                  W = mg h = − mgl 1 cosθ f)                  (10.8.14)
                                                                   −
   349   350   351   352   353   354   355   356   357   358   359