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0593_C14_fm  Page 502  Tuesday, May 7, 2002  6:56 AM





                       502                                                 Dynamics of Mechanical Systems


                       From Eq. (14.6.45) we see after computation and simplification that:

                                        c c − c c − c c −( 15 8) M r +( 27 2) mMr +  24 m r   (14.6.62)
                                                                            2
                                                              24
                                                                                  2 4
                                         26   4 5  1 8
                       Therefore, the inequality of Eq. (14.6.61) is inherently satisfied.
                        Next, the second inequality of Eq. (14.6.58) will be satisfied if AC is positive. By inspec-
                       tion of Eqs. (14.6.54) and (14.6.56) we see immediately that both A and C are positive, thus
                       the second inequality of Eq. (14.6.58) is satisfied. Therefore, the motion of the pivoting
                       disk with the rim mass in the upper-most position is stable if  φ ˙ 0  is sufficiently large to
                       satisfy Eq. (14.6.60). From Eq. (14.6.45) we see that:

                                                                              ]
                                            cc + c c = ( [  3 2) M +( 33 4) Mm 12 m gr 3      (14.6.63)
                                                                        +
                                                            2
                                                                             2
                                            35   1 7
                       Hence, from Eqs. (14.6.60), (14.6.62), and (14.6.63) we have the stability criterion:
                                                      4M 2  + 22Mm +  32m 2 
                                                φ >                   (gr )                 (14.6.64)
                                                 ˙ 2
                                                 0    5M 2  +  36Mm +  64m 2 
                       Finally, observe that if m = 0, the stability criterion reduces to:

                                                         φ > (   5 )
                                                         ˙ 2
                                                          0   4gr                             (14.6.65)
                       which is identical to Eq. (14.5.38).


                       14.6.2  Rim Mass in the Lowermost Position

                       Next, let there be a small disturbance to the equilibrium position with the rim mass in its
                                                                               ˙
                                                                              φ
                       lower-most position as defined by Eq. (14.6.35). That is, let θ, , and ψ have the forms:
                                                                 * ˙
                                                             ˙
                                                                          +
                                                          ˙
                                               θ =+  θ ,  φ =  φ +  φ ,  ψ =  π ψ ˙  *        (14.6.66)
                                                  0
                                                      *
                                                              0
                                                              *
                       where, as before, the quantities with the ( ) are small. The governing equations, Eqs.
                       (14.6.28), (14.6.29), and (14.6.30), then become (after simplification):
                                                   ( 54)Mr θ  − ( 3 2)Mr φ ψ
                                                                     2 ˙ ˙ *
                                                          2˙˙*
                                                                       0
                                                    [    +(       2 2 ˙ 0]  *                 (14.6.67)
                                                   − Mgr   54)Mr φθ    =  0
                                             ( 32)Mr ˙˙ *  + ( 52)Mr φ θ  + mgrψ *  =  0      (14.6.68)
                                                     ψ
                                                    2
                                                                2 ˙ ˙ *
                                                                  0
                       and
                                                            φ= 0                              (14.6.69)
                                                            ˙˙*
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