Page 34 - Bird R.B. Transport phenomena
P. 34

§1.2  Generalization of Newton's  Law  of Viscosity  19

                  sired,  this  set  of  relations  can be  written  more concisely  in the vector-tensor  notation  of
                  Appendix  A  as
                                                      +
                                       т  = -/i(Vv  +  (Vv) )  +  (|/Lt -  K)(V  • v)8  (1.2-7)
                  in  which  5  is  the  unit  tensor with  components  6 /y/  Vv  is  the velocity gradient tensor with
                  components  (d/dx)v jf  (Vv) +  is  the  "transpose"  of  the velocity  gradient  tensor  with  com-
                  ponents (d/dXj)Vj, and  (V • v)  is the divergence  of the velocity  vector.
                     The important conclusion  is that we  have  a generalization  of  Eq. 1.1-2, and  this  gen-
                  eralization  involves not one but  two  coefficients 3  characterizing  the fluid:  the viscosity /л
                  and  the  dilatational  viscosity  к.  Usually,  in  solving  fluid  dynamics  problems,  it  is  not
                  necessary  to  know  к.  If  the  fluid  is  a  gas,  we  often  assume  it  to  act  as  an  ideal
                  monoatomic gas,  for  which  к is  identically  zero.  If the  fluid  is  a liquid,  we  often  assume
                  that  it  is  incompressible,  and  in  Chapter  3  we  show  that  for  incompressible  liquids
                  (V  • v)  =  0, and  therefore  the term containing  к is  discarded  anyway. The dilational  vis-
                                                                              4
                  cosity  is  important  in describing  sound  absorption  in polyatomic  gases  and  in  describ-
                  ing  the  fluid dynamics  of  liquids  containing gas  bubbles.  5
                      Equation  1.2-7  (or  1.2-6) is  an  important equation  and  one that we  shall  use  often.
                  Therefore  it  is  written  out  in  full  in Cartesian  (x, y, z), cylindrical  (г, 0, z), and  spherical
                  (г, 0, ф) coordinates  in Table  B.I. The entries  in this table  for  curvilinear  coordinates  are
                  obtained  by  the methods  outlined  in §§A.6 and  A.7.  It is  suggested  that beginning  stu-
                  dents  not  concern  themselves  with  the  details  of  such  derivations,  but  rather  concen-
                  trate on using  the tabulated  results.  Chapters  2 and  3 will give ample  practice  in  doing
                  this.
                      In curvilinear  coordinates the stress components have  the same meaning as in Carte-
                  sian  coordinates.  For example,  т  in  cylindrical  coordinates, which  will be  encountered
                                              п
                  in Chapter  2, can be  interpreted  as:  (i) the viscous  force  in the z direction  on a unit  area
                  perpendicular  to the r direction, or  (ii) the viscous flux  of  z-momentum in the positive  r
                  direction. Figure  1.2-2  illustrates  some typical  surface  elements and stress-tensor  compo-
                  nents that arise  in  fluid  dynamics.
                     The shear  stresses are usually  easy  to visualize,  but  the normal stresses may  cause
                  conceptual  problems.  For example,  T  is  a  force  per  unit  area  in  the  z  direction  on  a
                                                   ZZ
                  plane  perpendicular  to the  z direction.  For the  flow  of  an  incompressible  fluid  in  the
                  convergent  channel  of  Fig.  1.2-3, we  know  intuitively  that  v z  increases  with  decreas-
                  ing  z; hence, according  to  Eq.  1.2-6, there  is  a nonzero stress  r zz  =  — 2jx{dv /dz)  acting
                                                                                   z
                  in the  fluid.
                  Note  on  the  Sign  Convention for  the  Stress  Tensor  We  have  emphasized  in  connection
                  with  Eq.  1.1-2  (and  in  the generalization  in  this  section)  that r  is  the force  in  the  posi-
                                                                       yx
                  tive x direction on a plane perpendicular  to the у  direction, and  that this  is  the force  ex-
                  erted  by  the  fluid  in  the  region  of  the  lesser у  on  the  fluid  of  greater y.  In  most  fluid
                  dynamics  and  elasticity  books,  the words  "lesser"  and  "greater"  are  interchanged  and
                  Eq.  1.1-2  is  written  as  r yx  =  +/jL(dv /dy).  The advantages  of  the sign convention  used  in
                                                x
                  this  book  are:  (a)  the  sign  convention  used  in  Newton's  law  of  viscosity  is  consistent
                  with  that used  in  Fourier's  law  of  heat  conduction and  Fick's  law  of  diffusion;  (b) the
                  sign  convention  for  т Х]  is  the  same  as  that  for  the  convective  momentum  flux  pvv  (see



                      3
                       Some writers refer to /л as the "shear viscosity," but this is inappropriate nomenclature inasmuch
                  as fi can arise in nonshearing flows as well as shearing flows. The term "dynamic viscosity" is also
                  occasionally seen, but this term has a very specific meaning in the field  of viscoelasticity and is an
                  inappropriate term for /A.
                      4
                       L. Landau and E. M. Lifshitz, op. cit., Ch. VIII.
                      5
                       G. K. Batchelor, An Introduction to Fluid Dynamics, Cambridge University Press (1967), pp.  253-255.
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