Page 318 - Numerical Methods for Chemical Engineering
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The finite element method                                            307



                  We next use the divergence theorem
                                           '            '
                                             [∇ · v]dV =  v · ndS                   (6.212)
                                                        ∂
                  on the second integral of (6.211) to obtain
                          '              '                  '
                                  2
                            χ p [−∇ ϕ]dr =  [(∇χ p ) · (∇ϕ)]dr −  χ p [∇ϕ · n]dS    (6.213)
                                                            ∂
                  Equation (6.209) then becomes
                    '         '                  '                '
                      χ p Rdr =  [(∇χ p ) · (∇ϕ)]dr −  χ p [∇ϕ · n]dS −  χ p (r) f (r,ϕ)dr  (6.214)
                                                 ∂
                  The algebraic equation (6.206) for node p is therefore
                                 '                  '               '
                             0 =   [(∇χ p ) · (∇ϕ)]dr −  χ p [∇ϕ · n]dS −  χ p fdr
                                                   ∂
                                    '                 '
                                                          [n]
                                 +    w  [d] [ϕ − ϕ B ]dS +  w [∇ϕ · n]dS           (6.215)
                                   ∂  [d]            ∂  [n]
                                                        [n]
                  We next collect the integrals over ∂  [d]  and ∂  ,
                           '                  '          '
                                                              [d]
                       0 =   [(∇χ p ) · (∇ϕ)]dr −  χ p fdr +  w  (ϕ − ϕ B ) − χ p [∇ϕ · n] dS
                                                        ∂  [d]
                                      '
                                            [n]
                                   +      w  − χ p [∇ϕ · n]dS                       (6.216)
                                     ∂  [n]
                                                                              [n]
                  We are still free to choose the boundary weight functions w  [d] (r) > 0, w (r) > 0, and
                  now do so in a convenient manner to simplify (6.216).
                                                                           [n]
                    If we set in (6.216) w  [n]  = χ p , this is acceptable as if p is on ∂  ,χ p ≥ 0. If not,
                                                                          [n]
                  χ p = 0on ∂  [n]  and the value of ϕ p does nothing to affect ϕ(r)on ∂  . Thus, by setting
                  w [n]  = χ p = 0 we merely neglect this boundary condition. With this choice w [n]  = χ p , the
                  last integral of (6.216) is zero.
                    To treat the Dirichlet boundary condition, we simply remove ϕ p from the list of unknowns
                                             [d]
                                                                     [p]
                  for any node p that lies along ∂  , and replace ϕ p with ϕ B (r ) in all other equations.
                  Thus, we no longer need a boundary weight, and set w [d]  = 0. Equation (6.216) for node
                  p /∈ ∂  [d]  then simplifies to
                              '                  '          '
                          0 =  [(∇χ p ) · (∇ϕ)]dr −  χ p fdr −  χ p [∇ϕ · n]dS      (6.217)
                                                           ∂  [d]
                                                                          [d]
                  Since we only have an instance of (6.217) for nodes that are not on ∂  , the last integral
                  is zero and we have the further simplification
                                          '                  '
                                       0 =  [(∇χ p ) · (∇ϕ)]dr −  χ p fdr           (6.218)
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