Page 207 - Percolation Models for Transport in Porous Media With
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12.3  CAVITATION                                                     205

         On the other hand  [85),  the mass velocity is

                                              -lc-1
                                       - Ot
                                       "-PaP!    1                         {12.12)
         where  C1  is  the velocity of sound  in  the fluid.  In  this case,  as  in  {12.9),  after
         taking into account {12.11) we obtain

                                   vf < v >"' (< r > /r) 2

         and using {12.12) and the fact that < v >"' ii,
                                    "!:!! _1!2.._ (< r >)2

                                        P!Cf     r
         After substituting this value of v in {12.10), we finally obtain the formula for the
         pressure difference when the fluid  passes from  a thick capillary to a thin one:
                                 p=Po-!  ~ (<r>)4                          {12.13)
                                         2  P!C}    r

            For a fluid, P!C} "' 1 GPa; Pa  "'0.01- 0.1 MPa for the considered phenomena.
         As it was demonstrated above, one can take < r  >"' 10- 5  m and the minimal value
         of radius r "' 10- 6  m.  In  this case < r > fr "' 10,  ( < r > /r) 4  "' 10 4 ,  and if the
         background pressure of the order 10 MPa is  taken as Po,  we obtain from  {12.13)
         that p "' 10 7   - {1/2) · 10- 4   • 10 4   "' 10 7   - {1 + 0.1)  "' 10 Pa.  This means that
                                                            7
         in a  reasonable range of radii of the joining capillaries (rfr 0  < 10), the pressure
         difference,  as  fluid  passes from  a  thick capillary to a  thin one,  is of the order of
         the wave amplitude Pa,  and therefore no negative pressure develops with respect
         to the high reservoir pressure Po.
            If we  take an "exotic"  case < r  >  fr  "'  10 2 ,  i.e.,  r  "' w- 7  m,  then  ( < r  >
         fr ) 4  "' 10 8  and p "' -1 GPa.  At such values of negative pressure one can expect the
         effect of cavitation to work.  For the mentioned rarefaction pressure, the existing
         hydrodynamic pressure, and the given frequency  of action, estimate the range of
         radii of the cavitating gas bubbles.
            Suppose  that due  to some  reasons,  the  so-called  germs,  i.e.,  bubbles  of gas,
         exist inside the fluid.  Formed inside the cone of depression during the evolution
         of gas  because  of  the  local  temperature,  concentration  and  other  fluctuations,
         these germs can oscillate in the pressure wave and collapse with the formation of
         cumulative jets directed towards the interface of the fluid  and the solid capillary
         surface  [89,  90).  As  in  the  approach  [91),  consider  the  variation  of the  initial
         pressure Po  in the fluid  in the vicinity of the oscillating bubble with initial radius
         ao.  If we neglect the elasticity of vapor, the pressure of the gas inside the bubble
         is
                                      Pn =Po+ 2xfao
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