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Computation of a turbulent natural convection in a rectangular cavity with the low-reynolds-number differential stress and flux model

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Abstract

A numerical study of a natural convection in a rectangular cavity with the low-Reynoldsnumber differential stress and flux model is presented. The primary emphasis of the study is placed on the investigation of the accuracy and numerical stability of the low-Reynolds-number differential stress and flux model for a natural convection problem. The turbulence model considered in the study is that developed by Peeters and Henkes (1992) and further refined by Dol and Hanjalic (2001), and this model is applied to the prediction of a natural convection in a rectangular cavity together with the two-layer model, the shear stress transport model and the time-scale bound\(\overline {v^2 } - f\) model, all with an algebraic heat flux model. The computed results are compared with the experimental data commonly used for the validation of the turbulence models. It is shown that the low-Reynolds-number differential stress and flux model predicts well the mean velocity and temperature, the vertical velocity fluctuation, the Reynolds shear stress, the horizontal turbulent heat flux, the local Nusselt number and the wall shear stress, but slightly under-predicts the vertical turbulent heat flux. The performance of the\(\overline {v^2 } - f\) model is comparable to that of the low-Reynolds-number differential stress and flux model except for the over-prediction of the horizontal turbulent heat flux. The two-layer model predicts poorly the mean vertical velocity component and under-predicts the wall shear stress and the local Nusselt number. The shear stress transport model predicts well the mean velocity, but the general performance of the shear stress transport model is nearly the same as that of the two-layer model, under-predicting the local Nusselt number and the turbulent quantities.

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Abbreviations

gi :

Gravitational acceleration

Gk :

Buoyancy generation term

H:

Height of the cavity

h:

Heat transfer coefficient

k:

Turbulent kinetic energy

kf :

Conductivity of fluid

L:

Width of the cavity

ni :

i-th component of normal vector at the wall

Nu:

Nusselt number

p:

Pressure

Pk :

Generation term of turbulent kinetic energy

Pθ :

Generation term of temperature variance

Pr:

Prandtl number

Prθ :

Turbulent Prandtl number

Ra:

Rayleigh number

RT :

Turbulent Reynolds number\(\left( { = \frac{{\rho k^2 }}{{\mu \varepsilon }}} \right)\)

t:

Time

T:

Time scale

Ui :

Cartesian velocity components

\(\overline {u_i u_j } \) :

Reynolds stresses

Uτ :

Wall friction velocity\(\left( { = \left( {\frac{\mu }{\rho }\left| {\frac{{\partial U_P }}{{\partial x_n }}} \right|_w } \right)^{1/2} } \right)\)

Xi :

Cartesian Coordinates

xn :

Normal distance from the wall

x + x :

Dimensionless normal distance from the\(\left( { = \frac{{\rho U_\tau x_n }}{\mu }} \right)\)

β:

Gas expansion coefficient

Δn :

Normal distance from the wall

ε:

Dissipation rate of turbulent kinetic energy

εθ:

Dissipation rate of temperature fluctuation

γ:

Dynamic viscosity

γM ij :

Pseudo eddy-viscosity for momentum equations

γT j :

Pseudo eddy-viscosity for energy equation

γT :

Turbulent eddy viscosity

υ:

Kinematic viscosity

ρ:

Density

Θ:

Temperature

\(\overline {\theta u_i } \) :

Turbulent heat fluxes

\(\overline {\theta ^2 } \) :

Temperature variance

H:

Pertaining to hot wall

ε:

Pertaining to dissipation rate of turbulent kinetic energy

θ:

Pertaining to temperature

N-1 :

Pertaining to previous iteration level

M:

Pertaining to momentum equation

T:

Pertaining to energy equation

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Correspondence to Seok-Ki Choi.

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Choi, SK., Kim, EK., Wi, MH. et al. Computation of a turbulent natural convection in a rectangular cavity with the low-reynolds-number differential stress and flux model. KSME International Journal 18, 1782–1798 (2004). https://doi.org/10.1007/BF02984327

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  • DOI: https://doi.org/10.1007/BF02984327

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