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Prandtl's Mixing Length Hypothesis, Lecture notes of Mathematical Physics

Describes in shortcoming of mixing length hypothesis, one-equation tubulence models, modeling K-equatins and distribution length of scale.

Typology: Lecture notes

2021/2022

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Prandtl's Mixing Length Hypothesis
The general form of the Boussineq eddy viscosity model is given as
k
3
2
x
U
x
U
uu ij
i
j
j
i
Tji δ
+
ν=
, mm uu
2
1
k
=, (1)
where T
ν is the eddy viscosity. For thin shear layer, the relevant component of (1) may
be restated as
y
U
vu T
ν=
. (2)
Prandtl assumed that mT~luν, where
u
is a turbulent velocity scale and m
l is referred
to as the mixing length. Furthermore, Prnadtl postulated that
y
U
~um
l, (3)
and hence
y
U
2
mT
=νl, y
U
y
U
vu 2
m
=
l. (4)
The mixing length m
l depends on the nature of the flow and, in general, is space
dependent.
For free shear flows, m
l is proportional to the half-width of the shear layer l. For
different flows, the mixing lengths are given as
ll 09.0
m=, for plane jet,
ll 075.0
m=, for circular jet, (5)
ll 07.0
m=, for mixing layer.
For boundary layer flows, several different forms were suggested. For instance, Escudier
(1966, Imperial College Report) assumed
pf3
pf4
pf5

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Prandtl's Mixing Length Hypothesis

The general form of the Boussineq eddy viscosity model is given as

k 3

x

U

x

U

u u ij i

j

j

i i j T − δ 

− ′ ′=ν , um um 2

k = ′ ′ , (1)

where ν (^) T is the eddy viscosity. For thin shear layer, the relevant component of (1) may

be restated as

y

U

u v T ∂

− ′ ′=ν. (2)

Prandtl assumed that ν (^) T ~ ulm, where u is a turbulent velocity scale and l (^) m is referred

to as the mixing length. Furthermore, Prnadtl postulated that

y

U

u ~ m ∂

l , (3)

and hence

y

2 U

T m ∂

ν =l , y

U

y

U

u v

2 m ∂

− ′ ′=l. (4)

The mixing length l (^) m depends on the nature of the flow and, in general, is space

dependent.

For free shear flows, l (^) m is proportional to the half-width of the shear layer l. For

different flows, the mixing lengths are given as

l (^) m = 0. 09 l, for plane jet,

l (^) m = 0. 075 l, for circular jet, (5)

l (^) m = 0. 07 l, for mixing layer.

For boundary layer flows, several different forms were suggested. For instance, Escudier

(1966, Imperial College Report) assumed

Variation of mean velocity and mixing length

in a turbulent boundary layer

κ

κ ≥ δ

κδ

κ

κ ≤ δ

κ

= 0 0

0

m (^) y

y y

l. (6)

where κ = 0. 41 and κ 0 = 0. 09.

1 U/Uo

m

l

y/ δ

κ (^) o / κ 1

For pipe flows, Nikuradse suggested the following expression:

4

0

2

0 0

m

r

y

  1. 061 r

y

  1. 14 0. 081 r

l , (7)

where r 0 is the radius of the pipe.

1 y/ro

Variation of mixing length in a turbulent pipe

flow according to Nikuradse.

Rm/ro

R m =0.4 y

Eq. (7)

Another example of failure of the mixing length theory is illustrated in the

recirculating flow shown in the figure:

Experimental data indicates that the maximum heat flux that occurs at the

reattachment point, while the mixing length model leads to γ (^) T =νT= 0 (since 0 y

U

One-Equation Turbulence Models

Many of the one and multi-equation turbulence models are based on the Prandtl-

Kolmogorov equation given by

(^2) l

1 νT =k , (10)

where ui ui 2

k = ′ ′ is the kinetic energy of turbulence and l is a turbulent length scale. It

is expected that 2

1

k be a better representative of the turbulent velocity scale when

compared with y

U

l.

The general equation for dynamics of k is given as

j j

2

j

i

j

i

j

i i j

i i j j x x

k

x

u

x

u

x

U

) uu

P

uu u( x

k dt

d

∂ ∂

+ν ∂

−ν ∂

ρ

Reattachment Point

Schematics of backward facing step flows.

For a thin shear layer, equation (11) may be restated as

− ε ∂

ρ

y

U

) uv

P

uu v( dt y

dk (^) i i , (12)

where the viscous diffusion is neglected and ε is the dissipation. Equation (12) clearly

shows that the kinetic energy of turbulence is convected, diffused, produced, and

dissipated.

Modeling k-Equation

To close the k-equation, the unknown terms in equation (12) must be modeled.

We assume

y

U

u v T ∂

− ′ ′=ν , (13)

where ν (^) T is given by (10). The diffusion term in (12) is modeled by a gradient law. i.e.,

y

P k uu 2

v k

T i i ∂

σ

ν = 

ρ

where σ (^) k is a constant Prandtl number for k.

The dissipation is given as

l

2

3

D

k ε =c (15)

Therefore, the closed k-equation becomes

l

2

3

D

2

T k

T (^) c k y

U

y

k

dt y

dk  − 

+ν 

σ

ν

Here, σ (^) k and c (^) Dare constants and l is a length scale distribution.

y

u

y

U

κ

*^2 − u ′v′= u. (23)

Using (23) in (22) and solving for l , we find

m

4

1

D

4

1

l = cD κy=c l (24)

For cD = 0. 08 , κ = 0. 4 , we find

l = 0. 2 y (25)

It was suggested that to use equation (24) in the entire flow domain with lm

given by an empirical mixing length expression. Nikuradse's equation given by (7) has

been used extensively. In immediate vicinity of the wall, further modification for viscous

effects are needed.

Achievements of the Model

Heat transfer in the heat exchanger and separated flows are predicted with

reasonable accuracy.

Shortcomings

  • Transport of the turbulent length scale is not accounted for.
  • The model offers little advantage over the mixing length model.