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PIPES CONVEYING FLUID: LINEAR DYNAMICS I                69

               pipes with supported ends. An example of a system that loses stability by  a Hamiltonian
               Hopf bifurcation is the column subjected to a tangential follower load, a nonconservative
               circulatory system, for which u,’  = gC = 20.05.
                 Finally, Figure 3.4(d) shows another form of  coupled-mode flutter, for which Done &
               Simpson’s (1977) nomenclature of Pai;doussis ’ (coupled-mode)Jlutter will be retained, to
               distinguish it from the Hamiltonian Hopf bifurcation of  Figure 3.4(c). The distinguishing
               feature is that in this case the bifurcation originates directly form a divergent state; hence,
               at  the  onset  of  flutter  (u = u,),  the  frequency of  oscillation is  zero  [Rr(w) = 01,  and
               then %e(w) # 0 for u > u,.  This kind of bifurcation will be found to arise for pipes with
               supported ends (Section 3.4), as well as for other systems (e.g.in Chapter 8).


               3.3  THE EQUATIONS OF MOTION

               3.3.1  Preamble
               The linear equation of  motion for a pipe conveying fluid will be derived in the next two
               sections by  the Newtonian and the Hamiltonian approaches. Before embarking on  these
               derivations, however, it is useful to introduce some basic concepts.
                 The first is related to the description of the system via either Eulerian or Lagrangian
               coordinates, differentiated by  the concepts of  spatial position  and particle  individuality,
               respectively. In  the Eulerian description the coordinates are fixed in  space and may  not
               be  populated  by  the  same material particles  as  time  varies; these  are  the  coordinates
               commonly used  in  fluid mechanics (e.g. in  Section 2.2). In  the Lagrangian description,
               coordinates  are  identified  with  individual particles  (or  elemental volumes  surrounding
               marked points in the continuum).
                 To  fix ideas, let us consider the longitudinal vibration of  a bar, i.e. a one-dimensional
               continuum. In  the  Eulerian description, the position  x,  fixed in  space, may  be  used  as
               the independent space variable, and  the deflection field described as u(x, t); as the  bar
               vibrates, different particles or material points at different times will be located at x. In the
               Lagrangian description, a given particle may be identified by  its position at a given time
               (say, r  = 0) or, more usefully, by  its position when the bar is undeformed, x = XO. This
               particle will be at a different x as time varies, but will be identified with xo always (Hodge
               1970). Clearly, the deflection field may equally be described in terms of  u(x0, t). This is
               the more  ‘mechanical’ description and it is  the foundation of  Lagrangian dynamics, for
               instance.
                 Similarly, in the case of  flexural oscillations of  the pipe, treated as a beam, two coor-
               dinate  systems  may  be  utilized:  the  Eulerian  (x, z) or  the  Lagrangian  (xg, ZO) - see
               Figure 3.5(a). The  equilibrium configuration is  along  the x-axis,  and  hence  (XO,  a)
               (XO, 0) in this case. The lateral deflection of the pipe may be described as w(x, t) in Eule-
               rian coordinates or W(Q, r) in the Lagrangian ones; however, as we can see, there is also
               change in  the  axial or x-position of  each point, i.e. u(x, t) or u(x0, t). If we consider a
               point P, which in the undeformed state is at PO, then its deflection is

                                   U=X-XO       and    W=Z-ZO=Z.                    (3.12)
               In what follows we shall use both sets of coordinates, but the usefulness of this discus-
               sion  will  become most  evident when  the  nonlinear equations of  motion are derived  in
               Chapter 5.
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