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8/9/2019 Macro Micro Modeling of Solidification
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Proc. Natl. Sci. Counc. ROC(A)
Vol. 23, No. 5, 1999. pp. 622-629
Macro-Micro Modeling of Solidification
LONG-SUN CHAO AND WU-CHANG DU
Department of Engineering Science
National Cheng Kung University
Tainan, Taiwan, R.O.C.
(Received November 3, 1998; Accepted March 31, 1999)
ABSTRACT
To solve solidification problems, macro-models are generally applied. Macro-micro models, by
considering the formation of microstructures in terms of nucleation and growth, can obtain better results
than can macro-models. Except for temperature distributions, macro-micro models can offer more in-
formation about the solidification process, including undercooling, grain size, grain density etc. Thesedata can be used to predict the mechanical properties of materials directly. In this paper, two macro-
micro models are built to investigate the equiaxed solidification of eutectic. One macro-micro model
considers the nucleation step, and the other does not (assuming that nucleation occurs instantaneously).
An experimental example of a cylindrical casting is used to test these models. The finite difference method
is utilized to solve the heat transfer problem, and the source term method is employed to handle the released
latent heat. From a comparison with the experimental result, the computed cooling curve is found to be
very close to the experimental one. From the computational results, it is found that a higher cooling rate
yields the greater undercooling, which leads to a smaller grain size or higher grain density.
Key Words: macro-micro modeling, solidification, nucleation, cylindrical casting
− 622 −
I. Introduction
For binary alloys, macro-models based on phase
diagrams are generally used to solve solidification
problems. These models can give only rough predic-
tions of the solidification time, isotherms etc., which
do not have any direct relation with the microstructures
and physical properties of solidified alloys.
Recently, the micro-viewpoint has gradually been
incorporated into the solidification models. In these
models, the microstructure evolution during the solidi-
fication process is considered. The whole process
includes three different steps: nucleation (an increase
in the number of nuclei), growth (an increase in thevolume of the grain) and impingement. These three
steps are illustrated in Fig. 1.
In the solidification process, as the temperature
of the liquid metal falls below the melting point,
nucleation begins, as shown in Fig. 2. Crystal clusters
(or embryos) are formed. These clusters may melt or
grow. When the clusters are big enough, they will not
melt any more. At this time, they are called nuclei.
At the beginning of nucleation, the number of nuclei
increases very slowly. After a critical undercooling
value is reached (∆T n in Fig. 2), the number increases
rapidly. Nucleation proceeds until the decreasing tem-
perature starts to increase, i.e., recalescence occurs. At
Fig. 1. Equiaxed solidification of the eutectic system. [Reprint from
Rappaz (1989)]
this point, the number of nuclei reaches its maximum
value.
After nucleation, there is a long period of growth.
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L.S. Chao and W.C. Wu
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ρ c p∂T
∂t
= k [∂2T
∂r 2
+ 1
r
∂T ∂r
+ ∂2T
∂ z2
] + ρ L∂ f s
∂t
, (1)
where c p is the specific heat, ρ is the density,
k is the thermal conductivity, L is the latent heat,
and f s is the local volume fraction of the solid.
(2)Initial and boundary conditions:
(i) The initial condition is
T (r , z,t =0)=T 0, (2)
where T 0 is the pouring temperature of the
liquid metal.
(ii) The boundary conditions are,
(a) at the center line (r =0),
∂T ∂r r = 0
= 0 , and (3)
(b) at the air/metal interface ( z=16 cm),
q"=hconv(T −T ∞), (4)
where q" is the heat flux, hconv is the
convective heat transfer coefficient of
air, and T ∞ is the environment tem-
perature.
(c) At the metal/mold interface:
Since the temperature distribution of the
sand mold is of less interest and requires
a great deal of computing effort, the
equivalent heat transfer coefficient is
used for the sand mold. The boundary
condition at the metal/mold interface can
be given by
q"=heff (T −T ∞). (5)
The primary difference between macro and macro-
micro models is in how the local volume fraction of
solid, f s, is computed. In the macro model, Voller’s
method (Voller and Swa, 1991) is used to calculate f s.
In macro-micro models, since equiaxed grains are as-
sumed to be spherical, f s can be expressed as
s(t ) = 4
3π R3(t ) • N (t ) , (6)
where N (t ) is grain number per unit volume and R(t )
is the grain radius. The derivative of f s can be written
as
df sdt
= 4π R2(t ) • N (t ) •
dRdt
+ 43π R
3(t ) •
dN dt
. (7)
Because the radius is very small in the nucleation step,
the second term on the right-hand side of Eq. (7) can
be ignored, and the equation can be rewritten as
df sdt
= 4π R2(t ) • N (t ) •
dRdt
. (8)
Equations (6) and (8) are the basic equations of the
micro-macro models. The detailed computing methods
used to obtain f s for the two macro-micro models built
in this paper are described in the following.
1. Model I
Nucleation is assumed to occur instaneously. This
means that the nucleation step does not need to be
considered in this model, and that N (t ) is a constant.
Fig. 3. A schematic diagram of the (testing) cylindrical casting.
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Macro-Micro Modeling of Solidification
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Accordingly, Eqs. (6) and (8) can be rewritten as
s(t ) = 4
3π R
3(t ) • N , (9)
df sdt = 4π R
2
(t ) • N •dRdt . (10)
In the growth step, by using the Johnson-Mehl
model (Johnson and Mehl, 1939), the growth rate V can
be given by
V =µ •∆T 2, (11)
where µ is a growth constant and ∆T is the undercooling,
which is equal to the difference between T e and T . T eis the eutectic temperature. The expression for R can
be obtained by integrating Eq. (11):
R = r 0 + µ [T e – T (t )]
2dt
0
t
, (12)
where r 0 is the critical radius (Kurz and Fisher, 1989).
For the impingement step, Eq. (10) is modified
by multiplying by a factor F :
df sdt
= 4π R2(t ) • N • dR
dt • F . (13)
Here, F is taken as 1− f s (Avrami, 1940). Equation (13)
can be rewritten as
df sdt
= 4π R2(t ) • N • dR
dt • (1 – f s) . (14)
By integrating Eq. (14), the expression for f s becomes
s(t ) = 1 – exp[ – N • 4
3π R
3(t )] . (15)
2. Model II
In the nucleation step, the Gaussian distribution
(Zou and Rappaz, 1991) is used to capture the variation
in the trend of the nucleation rate. The equation for
dN / dt can be written as
dN dt
= –N max
2∆T σ exp[
– (∆T – ∆T 0)2
2∆T σ ]dT dt
, (16)
where ∆T 0 is the undercooling at the tip point of theGaussian distribution, ∆T σ is the standard deviation of
the distribution, and N max is the total grain density of
the whole distribution (integrating Eq. (16) from zero
undercooling to infinity).
When ∂ T / ∂ t >0 (i.e., the recalescence occurs),
dN =0. This is the end point of the nucleation step. In
the growth step, Eq. (11) is also used to calculate the
grain radius. The two-step Close-Pack model
(Alexandre et al., 1991) is applied in the impingement
step, and the f s is given by
Table 1. Constants Used in the Two Micro-Macro Models
Constant Value
N (in Model I) 6.0×109 m−3
µ 3.0 ×10 −8 m/s °C
∆T 0 20 °C
∆T σ 4.75 °C
nmax 1.20×1011 m−3
Fig. 4. The computed cooling curves obtained by the macro and
macro-micro models. (a) Cooling curves; (b) locally enlarged
cooling curves.
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L.S. Chao and W.C. Wu
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df sdt
= φ • 4π R2(t ) • N (t ) •
dRdt
, (17)
φ =
– 10.32log10
( f s) 1 ≥ f s ≥ 0.8
1 f s < 0.8 .(18)
In this paper, the finite difference method is used
to compute the temperature distribution. In formulat-
ing the finite difference equations, the central differ-
ence is used for the space derivative, and the backward
difference is used for the time derivative. The algebraic
equations are solved iteratively by using the line
S.O.R. method (Anderson et al., 1984).
III. Results and Discussion
In this paper, two macro-micro models have been
built to study solidification processes. The testing
material is gray cast iron, whose microstructure is
equiaxed eutectic. The constants used in these two
models are listed in Table 1. The node number of the
uniform grid used in the computation is 61×26. In
Model I, the time step can be 1 second. However, in
Model II the step can not be larger than 0.1 second,
and the relaxation factor is adjusted up to 1.2 since it
is more difficult to make it converge than it is in Model
I. For convenience, the center point of the casting isused as a reference point (Fig. 3).
Figure 4 shows the computed cooling curves of
the reference point for the macro and macro-micro
models. In Fig. 4(a), there is no big difference between
these two curves. However, the undercooling phenom-
enon can not be obtained from the macro model. In
Fig. 5. The cooling curves from the experiment and the macro-micromodel.
Fig. 6. The computed cooling curves obtained by the two macro-
micro models. (a) Cooling curves; (b) locally enlarged cooling
curves.
Fig. 4(b), the undercooling as well as the recalescence
phenomenon can be clearly seen from the cooling curve
of the macro-micro model.Figure 5 shows the computational and experimen-
tal cooling curves of the reference point. From this
figure, it can be found that the computational data of
the cooling curve and undercooling are quite close to
the experimental data (Kanetkar et al., 1988). Figure
6 illustrates the cooling curves of Model I and Model
II. Though these two models are quite different from
each other, the computational results are very similar
(Fig. 6(a)). Taking a close look (Fig. 6(b)), we can
find that Model II has a smaller degree of recalescence
(or the maximum undercooling), which is closer to the
experimental result.
Figure 7 shows f s vs. the grain radius at the ref-
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Macro-Micro Modeling of Solidification
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erence point for three different models, Model I, ModelII and Model II, without modification of φ (in Eqs. (14)
and (15)). Because of the modification of φ in Model
II (after impingement occurs, f s>0.8), the curve become
smoother than the one without modification. In Model
I, since f s increases slowly and smoothly with the grain
radius, the larger time step can be used, and the con-
vergence rate is faster than that in Model II. However,
in Model I, f s will not be one until the radius reaches
infinity. This is not reasonable. Accordingly, the end
point of solidification is set at the radius when f s=
0.999.
At the reference point, the relationship between
the nucleation rate (or grain density) and time is that
Fig. 8. The nucleation rate and grain density distributions vs. time.
Fig. 7. f s vs. the grain radius for different models.
Fig. 9. The distribution of the highest level of undercooling.
shown in Fig. 8. In the figure, it is shown that the
Gaussian distribution can successfully simulate the big
change of the nucleation rate in a short time. After
the nucleation step, the grain density reaches a constantvalue, i.e., the final grain density. It can also be found
that the nucleation time (about 18 seconds) is very short
compared to the local solidification time (about 300
seconds). This proves that the assumption of instan-
taneous nucleation is reasonable.
In general, it is thought that a higher cooling rate
(dT / dt ) yields a higher grain density since the higher
cooling rate leads to greater undercooling, which re-
sults in a larger number of nuclei (Kurz and Fisher,
1989). This is consistent with the computed results
described in the following. In Figs. 9-11, the distri-
butions of the maximum undercooling, grain density
and radius (of Model II) are shown. From these figures,
it can be found the grain radius and density are strongly
related to the undercooling. Closer to the center point
(where the cooling rate is lower), the maximum level
of undercooling is lower, the grain density is lower and
the grain radius is larger.
From this study, it can also be seen that the
advantages of Model I are that the formulation is simple,
and that the undercooling prediction is not bad.
However, Model I can not obtain the nucleation rate
or the grain density which varies with time, and the
grain radius should be infinite, which would make f s
equal to one, which is not reasonable. Therefore,Model I is only suitable for rough evaluation of the
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L.S. Chao and W.C. Wu
− 628 −
Fig. 11. The grain size distribution after solidification.Fig. 10. The grain density distribution after solidification.
solidification process. On the other hand, Model II can
obtain more information about solidification and a
better undercooling prediction than can Model I.
However, the computation for Model II is not verystable, so a small time step is needed. The convergence
rate of each time step is also low. Consequently, Model
II uses much more computation time than does Mode
I.
IV. Conclusions
In this paper, two macro-micro models have been
built in order to study the equiaxed solidification of
eutectic. Model I ignores the nucleation step by as-
suming that it occurs instantaneously; however, it is
considered in Model II. These two models can obtainthe undercooling (or recalescence), which cannot be
obtained by the macro models. From the computational
results, the following conclusions can be drawn:
(1)By using Model I or II, cooling curves as well
as undercooling can be well predicted, but the
computed results obtained by Model II are closer
to the experimental results.
(2)The formulation of Model I is simple, and the
convergence rate is fast. This model is suitable
for preliminary evaluation of the solidification
process.
(3)Model II can obtain the nucleation rate, grain
density and radius which varies with time, which
cannot be obtained by Model I. Since the varia-
tion of f s vs. the grain radius is not as smooth
as in Model I, Model II needs a smaller time step
for the computation to be stable.(4)During the solidification process, the cooling
rate and undercooling are two important factors
influencing the formation of the microstructure
and heat transfer.
(5)A higher cooling rate yields a higher level of
undercooling, which results in greater grain
density and a smaller grain radius.
Acknowledgment
This research was supported by the National Science Council,
R.O.C., under Contract NSC 85-2212-E006-025.
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