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0593_C14_fm  Page 483  Tuesday, May 7, 2002  6:56 AM





                       Stability                                                                   483


                                               *
                       Then, to the first order in θ , sinθ and cosθ may be approximated as:
                                                     sinθ =  sin(0 + θ ) = θ  *
                                                                  *

                       and

                                                     cosθ =  cos(0 +  θ ) = 1                  (14.3.5)
                                                                   *
                        By substituting from Eqs. (14.3.4) and (14.3.5) into (14.3.1), we obtain:

                                                     θ + ( [  gr ) = Ω 2 ] θ = 0               (14.3.6)
                                                                    *
                                                     ˙˙*

                                                                                                  2
                       By referring to the solutions of Eqs. (14.2.5) and (14.2.12), we see that if [(g/r) – Ω ] is
                       positive, the solution of Eq. (14.3.6) may be expressed in terms of trigonometric functions
                                                                               2
                       and thus will be bounded and stable. Alternatively, if [g/r – Ω ] is negative, the solution
                       of Eq. (14.3.6) will be expressed in terms of exponential or hyperbolic functions and thus
                       will be unbounded and unstable. Hence, the equilibrium position θ = 0 is stable if:

                                                    gr > Ω 2  or  Ω  2  <  gr                  (14.3.7)



                       Case 2: θθ θθ = θθ θθ  = 0
                                   2
                       Consider next the equilibrium position θ = π. A small disturbance about θ = π may be
                       expressed as:

                                                          θ =+    *                            (14.3.8)
                                                              π θ
                                                                                *
                       Then, sinθ and cosθ may be approximated to the first order in θ  as:
                                                             (
                                                     sinθ = sin π θ ) =− θ *
                                                               +
                                                                  *
                                                                                               (14.3.9)
                                                             (
                                                     cosθ =  cos π θ ) =−1
                                                                +
                                                                  *
                       By substituting from Eqs. (14.3.8) and (14.3.9) into (14.3.1) we obtain:
                                                         [
                                                     θ − Ω 2  +(gr  θ )]  *  = 0              (14.3.10)
                                                     ˙˙*
                                                  *
                       In this case, the coefficient of θ  is negative for all values of Ω. Therefore, the solution of
                       Eq. (14.3.10) will involve exponential or hyperbolic functions; thus, the equilibrium posi-
                       tion is unstable.


                                          –1
                                                2
                       Case 3: θθ θθ = θθ θθ  = cos (g/rΩΩ ΩΩ )
                                   3
                                                                         2
                                                                   –1
                       Finally, consider the equilibrium position θ = cos (g/rΩ ). Observe that this equilibrium
                                                     2
                                                                               2
                       position will not exist unless g/rΩ  is smaller than 1. That is, Ω  must be greater than g/r
                                             –1
                                                    2
                       for equilibrium at θ = cos (g/rΩ ).
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