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0593_C10_fm  Page 329  Monday, May 6, 2002  2:57 PM





                       Introduction to Energy Methods                                              329


                       where M is the mass of B (the total mass of all the particles composing B), and the middle
                       term is zero because G is the mass center of B.
                        Consider the last term of Eq. (10.5.5). By expanding and rearranging the terms we have:

                                     N
                                                                          N
                                                    N
                                                                             i [
                                        i (
                                                        i (
                                  1 ∑  m ωω × ) =  1 ∑ m ωω × )⋅( ωω × r i) =  1 ∑ m ωω⋅ r  ×( ωω × r i)]
                                               2
                                                             r
                                             r
                                  2           i   2          i         2          i
                                    i= 1            i= 1                 i= 1
                                                       N
                                                                          N
                                                                              i[
                                                                                 ×
                                                =  1 ωω⋅ ∑ m ×( ωω × r i) =  1 ωω⋅ ∑  m r i ( nω  × r i)]
                                                           r
                                                  2       ii          2               ω
                                                      i= 1                i= 1                 (10.5.6)
                                                =  1  ωω⋅I BG ω ω =  1 ωω ⋅I BG  ⋅n  ω
                                                  2   ω     2         ω
                                                =  1 ωω ⋅I BG ⋅ωω
                                                  2
                       where ω is the magnitude of ωω ωω, n  is a unit vector parallel to ωω ωω,  I BG  is the second moment
                                                    ω
                                                                                ω
                       vector of B for G for the direction of n , and I B/G  is the central inertia dyadic of B (see
                                                          ω
                       Sections 7.4 and 7.6.).
                        By substituting from Eq. (10.5.6) into (10.5.5), the kinetic energy of B becomes:
                                                              1
                                                     K =  1  v  2  + ωω ⋅I BG  ⋅ωω             (10.5.7)
                                                         2  G  2
                       Finally, suppose that n , n , and n  are mutually perpendicular principal unit vectors of
                                                     3
                                              2
                                           1
                       B for G (see Section 7.7), then K may be expressed as:
                                                          1
                                              K =  1  Mv 2  + ( 11  2  + I ω 2 + I ω 2 )       (10.5.8)
                                                            I ω
                                                  2   G   2     1  22  2  33  3
                       where I , I , and I  are the corresponding principal moments of inertia of B for B, and
                                22
                                        33
                             11
                       the ω  (i = 1, 2, 3) are the n  components of ωω ωω. Observe that in all the expressions for kinetic
                                             i
                           i
                       energy no accelerations appear, only velocities.
                       10.6 Work–Energy Principles

                       We can obtain a relationship between work and kinetic energy by integrating equations
                       obtained from Newton’s laws. To this end, consider first a particle P with mass m subjected
                       to a force F as in Figure 10.6.1. Then, from Newton’s laws (see Section 8.2), we have:


                                                           F = m a                             (10.6.1)

                       where a is the acceleration of P in an inertial frame R. If we project the terms of Eq. (10.6.1)
                       along the velocity v of P in R we have:

                                                                 ⋅
                                                         Fv⋅= m av                             (10.6.2)
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