Page 214 - Intro to Tensor Calculus
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                                               Figure 2.2-8. Compound pendulum

                             dx i  ∂H             dp i   ∂H
                (d) Show that    =        and        = −    . These are a set of differential equations describing the
                              dt   ∂p i           dt     ∂x i
                   position change and momentum change of the particle and are known as Hamilton’s equations of motion
                   for a particle.


                                                  i
                                   i
                                                        i
              I 21.   Let  δT  i  = κN and  δN  i  = τB − κT and calculate the intrinsic derivative of the cross product
                           δs             δs
                 i
               B =   ijk T j N k and find  δB i  in terms of the unit normal vector.
                                     δs
              I 22. For T the kinetic energy of a particle and V the potential energy of a particle, define the Lagrangian
                                        1      i j                                             i  i
                          i
                       i
               L = L(x , ˙x )= T − V =    Mg ij ˙x ˙x − V as a function of the independent variables x , ˙x . Define the
                                        2
                                                     1  ij                                               i
                                    i
               Hamiltonian H = H(x ,p i )= T + V =     g p i p j + V, as a function of the independent variables x ,p i ,
                                                    2M
               where p i is the momentum vector of the particle and M is the mass of the particle.
                                  ∂T
                (a) Show that p i =  .
                                  ∂ ˙x i
                             ∂H      ∂L
                (b) Show that    = −
                             ∂x i    ∂x i
              I 23.   When the Euler angles, figure 2.2-6, are applied to the motion of rotating objects, θ is the angle
               of nutation, φ is the angle of precession and ψ is the angle of spin. Take projections and show that the
               time derivative of the Euler angles are related to the angular velocity vector components ω x ,ω y ,ω z by the
               relations
                                                       ˙
                                                                ˙
                                                  ω x = θ cos ψ + φ sin θ sin ψ
                                                         ˙
                                                                 ˙
                                                  ω y = −θ sin ψ + φ sin θ cos ψ
                                                           ˙
                                                        ˙
                                                  ω z = ψ + φ cos θ
               where ω x ,ω y ,ω z are the angular velocity components along the x 1 , x 2 , x 3 axes.
              I 24. Find the equations of motion for the compound pendulum illustrated in the figure 2.2-8.
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