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Introduction  to  Mechanics  of  Continua                                                   39


             principles.  At  the  same  time,  within  the  frame  of  Noll’s  axiomatic  sys-

             tem,  the  postulate  3),  which  states  the  inertial  frame  invariance  of  [T],
             is  a  consequence  of  the  objectivity  principle.
                 At  last,  the  necessary  and  sufficient  condition  for  the  isotropy  of  a
             tensorial  dependence  (the  Cauchy—Eriksen—Rivlin  theorem)  shows  that,
             in  our  working  space  £3,  the  structure  of  this  dependence  should  be  of
             the  type





                           [T]  —  [—p(p, T)  +  yo(p, T,  hh,  qo,  T3)](I]




                                +  PI  (p, T,  qh,  Ip,  T3)[D]  +  p2(p, T,  Ii, Ie,  I3){D]?,

             where  Yo,  91,  y2  are  isotropic  scalar  functions  depending  upon  the  princi-

                                                                                                          —
             pal  invariants  J),  Iz,  Iz  of  [D],  where  J;  =  tr{D]  =  div  v,  212  =  (tr[D])?
             tr{D]?  and  I3  =  det[D],  and  with  the  obvious  restriction  yo(p,  T,  0,0,0)  =
             O  (conditions  required  by  the  postulate  4)).
                 This  general  form  for  the  constitutive  law  defines  the  so-called  Reiner—
             Rivlin  fluids,  after  the  names  of  the  scientists  who  established  it  for  the
             first  time.

                 Those  real  fluids  characterized  by  a  linear  dependence  between  [T]
              and  [D]  are  called  Newtonian  or  viscous.  By  using  the  corollary  which
             gives  the  general  form  of  a  linear  isotropic  tensorial  function  [([A]),
             observing  the  hydrostatic  form  at  rest,  we  necessarily  have  for  these
             fluids  the  constitutive  law



                           [T}]  =  [—p  (p,  T)  +  A  (e,  T)  tr[D]]  [1]  +  2p  (p,  T)  [D],


             where  the  scalars          and  A  are  called,  respectively,  the  first  and  the
              second  viscosity  coefficient.        By  accepting  the  Stokes  hypothesis  3A  +
              2u  =  0,  which  reduces  to  one  the  number  of  the  independent  viscosity
             coefficients  and  which  is  rigorously  fulfilled  by  the  monoatomic  gases
              (helium,  argon,  neon,  etc.)        and  approximately  fulfilled  by  other  gases

              (provided  that  divv  is  not  very  large)  we  would  have  (from  tr[T]  =
              —3p  +  (3A  2u)  tr[D]  ),  that  m1  +  722  +  733  =  —3p,  ie.,  the  above
                             4+
             mentioned  result  on  the  equality  of  pressure  with  the  negative  mean  of
             normal  stresses.
                 Obviously,  for  a  viscous  fluid  there  are  also  tangential  stresses  and  so
             there  is  a  resistance  to  the  fluid  layers  sliding.  The  viscosity  of  fluids  is
             basically  a  molecular  phenomenon.
                 For  the  incompressible  viscous  fluid  from  tr{[D]  =  divuv  =  0  we  get

              [T]  =  —p{T]  +  2u[D].
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