Page 425 - Fluid-Structure Interactions Slender Structure and Axial Flow (Volume 1)
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PIPES CONVEYING FLUID: NONLINEAR AND CHAOTIC DYNAMICS          397

             an  analysis of  more  limited  scope, essentially redoing  some  of  the  same work  as  by
             Namachchivaya and co-workers, but via more standard and easily accessible terms, in fact
             following Namachchivaya & Ariaratnam (1987). What is presented below is a melange of
             all of this, but differentiating according to authors as appropriate; the results are discussed
             separately.
               In all these studies the nonlinear equation used is similar to Holmes’ (Sections 5.2.9(b)
             and 5.5.2), the only nonlinearity taken into account being due to the deformation-induced
             tension between laterally and axially fixed supports; the rest of the equation, including the
             terms associated with the flow pulsation (Le. the iC  terms), is linear and as in Section 4.5
             and Pai‘doussis & Issid (1974). Thus, the nonlinear dimensionless equation of  motion is
             given by variants of  equation (5.80):










             in which the parameters are defined in (3.71) and (5.81),  subject to

                                         u = UO(1 + p cos or).                   (5.144)

             Assuming y  = ad = a = 0 and taking u as in (5.144), Namachchivaya (1989) discretizes
             equation (5.143) into one of  two degrees of  freedom,





                   = [p,91/2u~w(C D) sin wt - p(2u;C + 2,9’/’uoB) cos wtlq - aAq,  (5.145)
                                 -
             in  which  @ = $dcijcklqiqjqkqi, the  ckl  being  terms of  the  type  making up  C, A  is  a
             diagonal matrix with elements h;, where hj are the dimensionless beam eigenvalues - cf.
             equation (4.70); p and a are assumed to be small (<<  1).+ To accentuate its structure, this
             equation may be written in  simplified notation as

                      4 + Gq + Kq = p(EI cos ot + E2  sin os)q -   i- f(q).      (5.146)


             This equation is  transformed into standard form by  an elegant Hamiltonian symplectic
             transformation (Namachchivaya 1989), a more standard technique via the solutions of the
             unperturbed system (Namachchivaya & Tien 1986b), and a standard method by Chang &
             Chen (1 994), all leading to variants of  the following equation:

                          u = (Bo + aBl)u + ,u(Kl cos (or +   sin on)u + f(u),   (5.147)


               +The notation  here differs from that in many of this group of papers where, to put in evidence the smallness
             of   and a, they  are scaled by  E, E  <<  1;  thus, IL = EW*  and a = <a*.
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