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 Encyclopedia of Physical Science and Technology  En006G-249  June 27, 2001  14:7








              Fluid Dynamics (Chemical Engineering)                                                        61

              One of the better versions of the modified mixing length  being investigated, one can obtain various degrees of de-
              model is                                          tailed information about the turbulent motions. Most of
                                                                the more complex formulations require large computing
                           L = k t R(1 − ξ)(1 − E)     (135)
                                                                facilities and may result in extreme numerical stability
                                      ∗
                           E = exp[−φ (1 − ξ)]         (136)    and convergence problems. All of the different methods
                                          √                     of computing the turbulent field structure cannot be dis-

                                  ∗
                            ∗
                           φ = R − R  ∗ c  2 2B        (137)    cussed here. Therefore, only one of these other methods,
                                                                the so-called κ–ε method, which is a two-equation type
                            ∗
                          R = Re    f                  (138)
                                                                of closure model, is outlined. Models such as this have to
              The parameter R is the laminar–turbulent transition value
                           ∗
                           c                                    date been applied only to Newtonian flow problems.
              of R and has the numerical value 183.3 for Newtonian  The idea involved in the κ–ε model is to assume that
                 ∗
              fluids. For non-Newtonian fluids it would have to be com-  the Reynolds’ stress tensor can be written as
              puted from the various results presented above.
                The parameter B is called a dampening parameter, as its                 ¯   2
                                                                              ρv v = 2µ t D − κδ,        (142)

              physical significance is associated with dampening turbu-                      3
              lent fluctuations in the vicinity of a wall. For Newtonian
              pipeflowithasthenumericalvalue22.Fornon-Newtonian  where κ is the turbulent kinetic energy,
              fluids it has been found to be a function of various rheo-
              logical parameters as follows:                                      κ = v · v ,            (143)
                                                                                      1

                                                                                      2
                Bingham Plastic
                                                    2
               B BP = 22[1 + 0.00352He/(1 + 0.000504He) ] (139)  and µ t is a turbulent or eddy viscosity function quite anal-
                                                                ogous to the eddy diffusivity discussed earlier. Just as in
                Power Law
                                                                the zero-equation modeling situation, one cannot write
                               B PL = 22/n             (140)    down a general defining equation for µ t , but must resort
                                                                to modeling. In the present case the model used is
                Herschel–Bulkley
                               B HB = B BP /n          (141)                    µ t = c 1 ρκ 2    ε,     (144)
              No correlation has as yet been developed for the Casson
              model.                                            where c 1 is a (possibly) Reynolds number-dependent coef-
                These simple models of turbulent pipe flow for var-  ficient that must be determined empirically. The function ε
              ious rheological models do not produce accurate details  is the turbulent energy dissipation rate function. The func-
              regarding the structure of the turbulentflow. They do, how-  tions κ and ε are determined by the pair of simultaneous
              ever, offer the practicing design engineer the opportunity  differential equations
              to predict the gross engineering characteristics of interest
              with reasonable correctness. They are called zero-order  Dκ  	  µ t


              equations because no differential equations for the turbu-  = ∇ · c 2  ∇κ + τ : ∇v − ε     (145)
                                                                  Dt          ρ
              lence properties themselves are involved in their solutions.
              Rather, one must specify some empirical model, such as  Dε      µ t       ε            2


                                                                     = ∇ · c 3  ∇ε + c 4 τ : ∇v − c 5 ε κ  (146)
              the mixing length, to close the equations.          Dt          ρ         κ
                                                                In this model the coefficients c 1 to c 5 are commonly
              D. Other Closure Models
                                                                given the numerical values c 1 = 0.09, c 2 = 1.0, c 3 = 0.769,
              Actually, all methods of closure involve some type of mod-  c 4 = 1.44, and c 5 = 1.92, although these values can be var-
              eling with the introduction of adjustable parameters that  ied at will by the user and are definitely problem spe-
              must be fixed by comparison with data. The only ques-  cific. They can also be made functions of any variables
              tion is where in the hierarchy of equations the empiricism  necessary.
              should be introduced. Many different systems of modeling  Here ends this article’s discussion of this model, but
              have been developed. The zero-equation models have al-  extensive detail is available in numerous books on the
              ready been introduced. In addition there are one-equation  subject. Some of these models present very accurate, de-
              and two-equation models, stress-equation models, three-  tailed descriptions of the turbulence in some cases, but
              equation models, and large-eddy simulation models. De-  may be very much in error in others. Considerable skill
              pending on the complexity of the model and the problem  and experience are required for their use.
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