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    Turbulence and CFD: Beyond k modeling

    __________________________________________

    Although two-equation closures such as the k model are arguably the most popular

    turbulence model for industrial applications of CFD, they have significant limitations

    and/or deficiencies. These are summarized below, together with some alternativeapproaches:

    1. The use of wall functions is convenient but fundamentally not sound for complexflows where the underlying assumptions are violated, e.g. for impinging flows. In

    the 1990s extensive effort was given to the development of so called lowReynolds number (LRN) models, which implement carefully designed damping

    functions to ensure the correct near-wall behaviour of important parameters

    such as the Reynolds shear stress, which behaves as 3)( + yuv in the near-wall

    region.

    2. The kequation is sometimes used together with other turbulence variables. Forexample, in the k closure, instead of the dissipation rate, one uses the

    quantity k/= , which has units of ]/1[ T , i.e. represents an inverse turbulence

    time scale. In form, this equation set is very similar to the k model, and uses

    an eddy viscosity model (EVM) relation to reconstruct the Reynolds stress, where

    the eddy viscosity is now given by /kCt= . The k closure has the

    remarkable and useful property of being applicable all the way to the wall.

    3. Most two-equation closures still suffer from the inherent limitation of using anEVM relation for the Reynolds stress terms, e.g.

    kx

    U

    x

    Uuu ij

    i

    j

    j

    itji

    3

    2 +

    +

    =

    Recall that this constitutive relation was modeled in a similar way to that ofmolecular transport, i.e. it is a gradient transport model. For complex flows,

    where there is more than one important strain-rate, this model fails. It is also

    deficient for flows with strong curvature and buoyancy.

    One alternative to EVM closures is an approach which solves the Reynolds Stress

    Transport Equations (RSTE). These equations are formidable, since the Reynoldsstress is a second-order tensor quantity. In order to closethese equations, many of

    the terms must be represented by simpler model relations. Nonetheless, the

    framework of the transport equations does allow the complex coupling betweenthe Reynolds stress terms and the mean velocity field to be much better

    represented. These models are especially applicable to flows with significant

    anisotropy, including near-wall flows.

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    A symbolic representation of the RSTE is as follows:

    ijijijijjij

    jji Puux

    Uuut

    ++=

    +

    D

    where

    ion termn/dissipatdestructiotheis

    tion termredistributheis

    termproductiontheis

    termdiffusiontheis

    ij

    ij

    ij

    ij

    P

    D

    Low Reynolds number or near-wall formulations have also been developed for

    the RSTE. As well, algebraic models can be derived from these equations byneglecting the net transport.

    4. The challenge of modeling the Reynolds stress becomes problematic for manycomplex flows. (Recall that the Reynolds stress represents the contribution of the

    turbulent motions to the mean transport.) Furthermore, in some cases onerequires specific information about the large-scale turbulent motions, e.g. in

    applications with unsteady or separated flows. This has led to the development of

    Large Eddy Simulation (LES) methods which calculate the large-scale motionsand model the smaller-scale motions. These represent very challenging

    simulations since the unsteady large-scale motions must be calculated in three-

    dimensions in a time-accurate manner. On the other hand, the expectation is that

    the residual stress (or subgrid-scale) terms can be adequately represented bysimpler models, since the small-scale motions are more isotropic. In LES the

    large-scale variable is referred to as the filtered velocity field, iU . LES typically

    uses different calculationmethods than do RANS models, although many CFDcodes try to include this option.

    5. Currently, the most accurate way to predict a turbulent flow is to use a DirectNumerical Simulation (DNS) in which all scales of motion are resolved by an

    unsteady, three-dimensional calculation. Examples of this approach include thepipe flow simulations of Wu and Moin (2008) (J Fluid Mech, Vol 608, pp. 81-

    112) and the backward-facing step study used as a benchmark for the project.

    Even with massive computing resources, these types of simulations can only

    consider flows with simple geometry and low Reynolds number. From anengineering viewpoint, they are not practical since they discard the vast majority

    of the information being calculated. However, they presently have been used asrefined experiments for exploring flow physics and calibrating turbulence models.