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Large-eddy simulation:                            6.1.2


           Application to liquid metal
           fluid flow and heat transfer


           Y. Bartosiewicz*, M. Duponcheel*
           *Institute of Mechanics, Materials and Civil Engineering, UCLouvain,
           Louvain-la-Neuve, Belgium





           6.1.2.1   Introduction

           Liquid metal reactors are characterized, from the thermal-hydraulic point of view, by a
           very low Prandtl number coolant, Pr   0.01. At such Prandtl number, the temperature
           field is much smoother than the velocity field, that is, the smallest temperature scales
           are much larger than those of the velocity, and, for moderate Reynolds numbers, the
           heat transfer in a channel could be essentially molecular while the flow is fully tur-
           bulent. Consequently, simulation tools and in particular computational fluid dynamics
           (CFD) should account for such peculiar behavior.
              We can classify CFD by three distinct approaches according the level of modeling/
           simulating the flow physics: the direct numerical simulation (DNS), the large-eddy
           simulation (LES), and the Reynolds averaged numerical simulation (RANS). The
           flow physics of interest is essentially characterized by turbulent transfers (e.g.,
           momentum and energy transfers). Turbulent flows are characterized by a full spec-
           trum of space and time scales, ranging from large scales, driven by the geometry
           and boundary conditions, down to the smallest scales where the energy is finally dis-
           sipated. This feature is illustrated by the so-called energy cascade introduced by
           Kolmogorov (1941). This statistic-based theory relies on local isotropy and similarity
           assumptions. The energy cascade means that, because of the nonlinear interactions
           between the different scales, an energy transfer takes place from the large scales to
           the small ones. At some point, depending on the Reynolds number, the energy transfer
           competes with the viscous dissipation of the energy into heat, and this latter effect
           becomes dominant. The final dissipation occurs at a scale defined by Kolmogorov
           and called the Kolmogorov scale. This energy cascade is represented by a relation
           between the local characteristic wavenumber k of eddies and the turbulent kinetic
           energy contained by such eddies E(k) (see Fig. 6.1.2.1).
              The large wavenumber range (e.g., the large scales) is the production range where
           the energy is injected to turbulence because of existing gradients in the mean flow or
           any external forcing. Thus, we find here the largest eddies containing most of the
           energy; these eddies are characterized by a length scale l 0 and a velocity scale u 0 pro-
           portional to the geometric length scale L and to the characteristic velocity scale of the


           Thermal Hydraulics Aspects of Liquid Metal Cooled Nuclear Reactors. https://doi.org/10.1016/B978-0-08-101980-1.00017-X
           Copyright © 2019 Elsevier Ltd. All rights reserved.
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