Page 134 - Bird R.B. Transport phenomena
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§4.1  Time-Dependent Flow  of Newtonian Fluids  119
                    We now apply the boundary and initial conditions in the following  way:

                 B.C. 1:  Because $ f  = 0 at  77 = 0, the function / must be zero at  77 = 0. Hence С must be zero.
                 B.C. 2:  Because ф  = 0 at  77 = 1, the function / must be zero at  17 = 1. This will be true if  В = 0
                               (
                 or  if  sin с is zero. The first  choice would  lead  to / = 0 for  all  17, and that would  be  physically
                 unacceptable. Therefore we  make the second choice, which leads  to the requirement that с =
                 0, ±тг, ±2тг, ±3тг, •  • •  •  We  label  these various  admissible  values  of с (called  "eigenvalues'')  as
                 c  and write
                  n
                                      c n  = птт,  with n = 0, ±1,  ±2, ±3, •  •  •    (4.1-32)

                 There are thus many  admissible  functions  /„ (called  "eigenfunctions")  that satisfy  Eq. 4.1-29
                 and the boundary conditions; namely,
                                   /„ = B  sin niTT),  with w = 0, ±1, ±2, ±3, •  •  •  (4.1-33)
                                        n
                 The corresponding functions satisfying  Eq. 4.1-28 are called g n  and are given  by
                                               2
                                            2
                                 g n  = Л ехр(-и тг т),  with n = 0, ±1, ±2, ±3, •  • •  (4.1-34)
                                      ;
                 I.C.:  The combinations f g  satisfy  the partial differential  equation for  <j> in Eq. 4.1-25, and
                                                                              t
                                     n n
                 so  will  any  superposition  of  such  products.  Therefore  we  write  for  the  solution  of  Eq.
                 4.1-25
                                                        2
                                                          2
                                        ф  =  ^  А»  ехр(-и тг т)  sin  HTTT j       (4.1-35)
                                         {
                 in which the expansion coefficients  D tl  = A B n  have yet to be determined. In the sum, the term
                                                  n
                 n  = 0 does  not contribute; also  since  sin(-7?)7ri7  =  —sin(+п)тгг1,  we  may  omit  all  the terms
                 with negative values  of n. Hence, Eq. 4.1-35 becomes
                                                         2
                                                            2
                                         <f> t  = 2  А,  ехр(-и тг т)  sin  птгт)      (4.1-36)
                                             H = l
                 According to the initial condition, <f> t  = 1 -  17 at т = 0, so that
                                                         s
                                             1  -  V = Ё  A, ^  И7Г77                (4.1-37)
                 We  now  have  to determine all  the D n  from  this  one equation! This  is  done by  multiplying
                 both  sides  of  the equation by  sin  тттт\,  where  m is  an integer, and  then  integrating  over  the
                 physically  pertinent range from  17 = 0 to  17 = 1, thus:

                                I  (1-17)  sin  min]dr\  = 2  A  I  s m  П7ГГ 1  s m  WTTTJ^TJ  (4.1-38)
                                Jo                  »=i  Jo
                 The left  side gives l/ттг; the integrals  on the right side are zero when n Ф m and \ when n =
                 m. Hence the initial condition leads to

                                                  D,,,=4                             (4.1-39)
                 The  final  expression  for  the dimensionless  velocity  profile  is  obtained  from  Eqs.  4.1-24,  36,
                 and 39 as
                                                      9
                                                                 2
                                                               2
                                     , т) = (1 -  77) -  2  (ш)  ехр(-и тг т)  sin  птгг)  (4.1-40)
                 The solution thus consists  of a steady-state-limit term minus a transient term, which fades  out
                 with increasing time.
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