Page 220 - Thomson, William Tyrrell-Theory of Vibration with Applications-Taylor _ Francis (2010)
P. 220

Lagrange's

                                                      Equation












                              Joseph  L.  C.  Lagrange  (1736-1813)  developed  a  general  treatment  of dynamical
                              systems formulated from the scalar quantities of kinetic energy  T, potential energy
                              U, and work  W. Lagrange’s equations are in terms of generalized coordinates,  and
                              preliminary to  discussing these  equations,  we  must  have  clearly in  mind  the basic
                              concepts of coordinates and  their classification.

                       7.1  GENERALIZED COORDINATES

                              Generalized coordinates  are any set of independent coordinates equal in number to
                              the  degrees  of  freedom  of  the  system.  Thus,  the  equations  of  motion  of  the
                              previous chapter were formulated  in terms of generalized coordinates.
                                  In  more  complex  systems,  it  is  often  convenient  to  describe  the  system  in
                              terms  of  coordinates,  some  of which  may  not  be  independent.  Such  coordinates
                              may be related to each other by  constraint equations.
                                  Constraints.  Motions  of  bodies  are  not  always  free,  and  are  often  con­
                              strained to move in a predetermined manner. As a simple example, the position of
                              the spherical pendulm of Fig. 7.1-1  can be completely defined by the two indepen­
                              dent coordinates  if/  and  (/>.  Hence,  if/  and  cf)  are  generalized coordinates,  and  the
                              spherical pendulum represents a system of two degrees of freedom.
                                  The  position  of  the  spherical  pendulum  can  also  be  described  by  the  three
                              rectangular  coordinates,  x, y, z,  which  exceed  the  degrees  of  freedom  of  the
                              system by  1.  Coordinates  x, y, z  are,  however,  not  independent,  because  they are
                              related by the  constraint equation:
                                                        -h y^  + z^  =  0                 (7.1-1)
                              One  of  the  coordinates  can  be  eliminated  by  the  preceding  equation,  thereby
                              reducing the  number of necessary coordinates to 2.

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