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DESTABILIZATION BY DAMPING:  T. BROOKE BENJAMIN’S WORK        469

             which  is  the  difference  between  the  nonconservative  energy  transfer  to  the  solid  and
             dissipation within it. Hence, this represents the balance of energy converted irreversibly
             by the disturbance (not the actual gain in energy by the solid, since the conservative forces
             may also contribute to this).
               Benjamin (1963) then considered three cases, corresponding to his three classes, A, B
             and C, of  instability of  compliant surfaces subjected to fluid flow.


               (i) Case of rn  > M, k  > K. If  c = C = 0, a simple harmonic solution with w = [(k -
             K)/(rn - M)]’”  is  obtained,  and  % = E  = i(k - K)G2, where 4  is the  amplitude.  The
             total  energy  level  is  positive.  For  finite  but  small  c  and  C,  on  the  other  hand,  the
             frequency is little changed, but the oscillation is amplified for c < C, which means that
             the rate of  irreversible energy transfer from the fluid to the solid exceeds the mean rate
             of  dissipation  - by  reference  to  (C.6).  The  activation  energy,  E  2:  i(k - K)G2, must
             be  positive  to  begin  with  (i.e.  a  positive  %O  must  be  added  in  generating  the  distur-
             bance)  and  if  C > c it  steadily increases, even  though 8 steadily decreases  in  view of
             (C.4). The  energy  of  the  initial  excitation  %O  is  eventually  lost  and 8 becomes  nega-
             tive, but  the  disturbance  continues  to  grow, because  this  is more  than compensated  by
             the  transfer  to  the  disturbance  of  energy  by  the  infinite  store  in  the  fluid. This  mech-
             anism  exemplifies  Benjamin’s  (1960, 1963) class  B  instability,  in  which  dissipation  is
             stabilizing.
               The case of class C, or Kelvin-Helmholtz,  instability will not be considered here and
             we go directly to a situation exemplifying class A instability.
               (ii)  Case of  m < M  and k  < K. For c = C = 0 we  once  more  have  simple harmonic
             motion with frequency w, but now the energy level of the disturbance is % = -; (K - k)G2
             and so is negative. This means that the absolute energy level of  the whole sistem must
             be reduced in the process of  creating a free oscillation: i.e. the system must be allowed
             to do work  against the external forces providing the excitation. For small and finite c and
             C, oscillations  are now  amplified if  c > C  and  damped if  c < C. Thus dissipation  and
             energy transfer  in  this  case  have  opposite  effects  as  compared  to  (i). In particular,  the
             effect of dissipation is always destabilizing. A physical interpretation is again provided by
             (C.6). The activation energy E  2 -i(K  - k)G2 is negative when the disturbance is first
             created (i.e. %O  < 0) and the amplitude of oscillation grows progressively by increases in
             the negative magnitude  of  E  for c > C. The significance of  E  is perhaps made clearest
             as  follows.  Suppose  that  the  irreversible  processes  were  suddenly  stopped,  so that  the
             oscillation  continued  at  constant  amplitude  4.  Then  E  is  the  absolute  energy  level  of
             the  system  if  the  same  oscillation  had  been  excited  by  external  forces,  and  we  know
             from the discussion above that E  is essentially negative, increasing in magnitude with q.
             Hence it is readily appreciated that dissipation is destabilizing since it lowers the absolute
             energy level.
               The preceding theoretical model provides the simplest possible demonstration of  how
             the removal of energy by dissipation may  destabilize  a system. However, the system of
             equations (C. 1) for case (ii) is more mathematical than physical since, for destabilization,
             rn  < M  is required;  but M  is the negative  of  the  added mass  [Section 2.2.l(a)], and  so
             for a physical system M  < 0 always, while m  > 0, rendering rn  < M  impossible. Hence.
             an  ‘ordinary’ one-degree-of-freedom  system  cannot  be  destabilized  by  dissipation;  two
             modes  and a travelling wave component in  the motion  are necessary (cf. Sections 3.2.2
             and 3.5.6).
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