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CONCEPTS. DEFINITIONS AND METHODS                     9

               where 6 denotes the variational operator and W is the work done by forces not included in
               V. The use of Hamilton's principle is especially convenient in cases of unusual boundary
               conditions, because the equation(s) of motion and boundary conditions are determined in
               a unified procedure [see, for example, Meirovitch (1967)l.
                 Special forms or interpretation of  (2.2) and (2.3) may be necessary for 'open systems',
               where the mass is not conserved, e.g. with in-flow and out-flow of mass and momentum,
               as is common in fluidelastic systems. These, however, will be discussed in the chapters
               that follow (e.g. in Section 3.3.3).


               2.1.2  Brief review of discrete systems

               A system is conservative if all noninertial forces may be derived from a potential function,
               i.e. if  they are all functions of  position alone; thus, if the system is displaced from a to
               b, the  work  is  not  path-dependent (or, equivalently, if  the  system is  returned to  a  by
               whatever path, the total work done is null). For a conservative system, the equations of
               motion may be written as
                                          [MlIiil+ IKlIql = {Ql,                     (2.4)


               a  special form  of  (2.1); the matrices are  of  the  same order  as  the  number of  degrees
               of  freedom,  N. Provided  that  (i) the  generalized  coordinates  are  measured  from  the
               (stable)  equilibrium configuration, (ii) the  potential energy is  zero  at  equilibrium, and
               (iii) the constraints are scleronomic - conditions that are not difficult to satisfy in many
               cases - the [MI and [K] matrices are symmetric.
                 Constraints  are  auxiliary  kinematical conditions; e.g. in  Figure 2.l(a) the  mass  MI
               cannot move freely in the plane but must remain at a fixed distance 11 from the point of
               support. The two constraint equations that must implicitly be  satisfied for the system of
               Figure 2.l(a) are what makes this system have two and not four degrees of  freedom. If
               a constraint equation may  be  reduced  to a form f (x, y, z, t) = 0, then  the constraint is
               said to be holonomic; a subclass of  this is when the constraint equation does not contain
               time explicitly, in which case the constraint is said to be sclerotzoniic (Meirovitch 1970;
               Nelmark & Fufaev  1972). Thus, if  11 were a prescribed function of  time, the constraint
               would be holonomic but not  scleronomic.'
                 The homogeneous form of equation (2.4), representing  free motions of  the system,




               may be re-written as
                                            I4 + [WIISI = {Ol,

               in which  [W] = [M]-'[K] - provided that [MI can be inverted, i.e. if  it is nonsingular.
               Oscillatory solutions are sought, of  the form

                                              (q} = [Ale'"',                         (2.7)

                 +These words  derive from  the  Greek  6Aas = whole or total  and  ubpas = law, hence  holonomic  means
               totally  demarcated or defined; the  first component of  scleronomic is from  UKA&S   = hard, hence the  word
               denotes a hard and fast rule!
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