Page 221 - Thomson, William Tyrrell-Theory of Vibration with Applications-Taylor _ Francis (2010)
P. 221

Lagrange’s Equation   Chap. 7
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                                  The  excess  coordinates  exceeding  the  number  of degrees of freedom  of the
                              system  are  called  superfluous  coordinates,  and  constraint  equations  equal  in  num­
                              ber to the  superfluous coordinates are necessary for their elimination.  Constraints
                              are  called  holonomie  if  the  excess  coordinates  can  be  eliminated  through  equa­
                              tions of constraint.  We will  deal  only with holonomie systems in  this text.
                                  Examine now the problem of defining the position of the double pendulum of

                              Fig.  7.1-2.  The  double  pendulum  has  only  2  DOF  and  the  angles  6 ^ and  62
                              completely  define  the  position  of   and  m2.  Thus,   and  62  are  generalized
                              coordinates,  i.e.,  6 ^ =   and  82  = Q2-

                                  The position of   and  m 2  can also be expressed in rectangular coordinates
                             X, y.  However they are  related by the constraint equations
                                                   If = x'i  + yj
                                                   l¡  =  (X2  - X ^   +  (y 2 - y i f
                              and  hence are not independent. We can express the rectangular coordinates  x¿,  y¿
                              in terms of the  generalized coordinates   and  62
                                              C  = /j sin   .  ^2  =  li sin 6 ^ +  ¡2 sin 62

                                              j
                                                = /i cos    y2   ^     +  ^2   ^2
                              and these  can  also be considered  as constraint  equations.
                                  To determine the kinetic energy, the squares of the velocity can be written in
                              terms of the  generalized coordinates:
                                                    ^2
                                                (MO

                                    u j   = i |   + 3)2 =  [ / i ^ i   +  I282 cos (02  “  ^1)]  T  [¡2^2  {^2  ~  ^1)]

                              The  kinetic energy
                                                      -r   1   2 . 1    2
                                                      T =  2^\^t  +  i^2^2
                              is then  a function  of both  q   =   6  and  q   =   9:
                                                   T =  T[q^,q2,...,q\,q2,---)            (7.1-2)
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