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Turbulent heat transport                                          275

           This chapter reports the status and future perspectives of different approaches to
           model the turbulent heat transfer for liquid-metal flows. Section 6.2.1.1 will provide
           an understanding of the peculiarities related to the modeling of the heat transfer in
           liquid-metal flows. In Section 6.2.1.2, an extensive overview of the available turbulent
           heat flux models will be provided along with their pros and cons with respect to
           their application to the liquid-metal flows. This is followed by a summary in
           Section 6.2.1.3.



           6.2.1.1   Understanding the peculiarities of heat transfer
                     modeling in turbulent liquid metal flows

           Before focusing on the turbulent heat flux modeling, it must be kept in mind that
           already there are a lot of uncertainties in the turbulence modeling of the velocity fields
           (for details, see Gr€ otzbach (2007)). In forced convection flows, for example, channel
           and rod bundle flows, these uncertainties can be reduced by selecting the best suited
           momentum transfer model. In this regard, a couple of best practice guidelines are
           available; see Casey and Wintergerste (2000), Menter et al. (2002), OECD (2007),
           and Roelofs (2017). Whereas, in buoyancy dominated flows, when the temperature
           is no longer a passive scalar, the temperature field needs to be modeled with utmost
           accuracy as it forms a source term for the velocity field.
              The Reynolds-averaged momentum and energy equations governing turbulent
           flows are as follows:


               DU i     1∂P    ∂    ∂U i
                   ¼ F i     +    ν     u i u j                         (6.2.1.1)
                Dt      ρ∂x i  ∂x j  ∂x j
               DT    q    ∂     ν ∂T
                  ¼    +           θu j                                 (6.2.1.2)
               Dt   ρc p  ∂x j σ T ∂x j

           where  D  ¼  ∂  ∂  is the material derivative, F i is the body force, and q is the inter-
                Dt  ∂t  + U k ∂x k
           nal energy source. In these equations, a closure is required for u i u j (turbulent momen-
           tum flux) and θu j (turbulent heat flux). The most frequent approaches adopted to close
           these equations are the following:

              Eddy viscosity model for turbulent momentum flux (u i u j ):
                    2         ∂U i  ∂U j
               u i u j ¼ kδ ij  ν t  +                                  (6.2.1.3)
                    3         ∂x j  ∂x i

              Eddy diffusivity model for turbulent heat flux (θu j ):
                      ν t ∂T
               θu i ¼                                                   (6.2.1.4)
                      Pr t ∂x i
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