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The stability of cells in directional solidification

Wouter-Jan Rappel, E. Brener

To cite this version:

Wouter-Jan Rappel, E. Brener. The stability of cells in directional solidification. Journal de Physique

I, EDP Sciences, 1992, 2 (9), pp.1779-1790. �10.1051/jp1:1992244�. �jpa-00246659�

(2)

Classification Physics Abstracts

44.30 68.45 81.30F

The stability of cells in directional sofidilication

Wouter-Jan

Rappel

and E.A. Brener

(*)

Laboratoire de Physique Statistique

(*°),

24 rue Lhomond, 75231 Paris Cedex 05, France

(Received

6 August 1991, revised 27 February 1992, accepted 15 May

1992)

Abetract. The stability of numerically obtained cells in the one sided model of directional solidification is investigated, using a numerical approach. In particular, the shapes of the cells

corresponding

to the Saffman-Taylor branch are discussed. The possibility for an oscillatory instability is investigated and the results are compared with a recent approximate analytical stability calculation. For large thermal length we find an instability which is oscillatory for

some parametervalues. The results agree partially with the analytical stability calculation. The

possible limit cycle arising from this instability is discussed.

1. Introduction.

In directional

solidification,

one

pulls

a

binary alloy through

an

externally imposed

fixed tern~

perature

gradient.

For

high enough pulling velocities,

the

planar interface, separating

the

liquid phase

from the solid

phase,

becomes unstable and forms cells with a well defined

wavelength ill.

For

metals,

where the diffusion of

impurities

in the solid can be

neglected,

the

resulting

cells are

typically

very

deep

[2].

The

problem

of the determination of the

resulting

cells has received

considerably

attention.

Previous work includes numerical calculations

[3-6]

and

approximate

theories [7, 8].

Contrary

to the case of the

symmetric

model [9], where one assumes

equal dilfusivity

in the

liquid

and the

solid,

and to the case of

rapid

solidification

[10],

where the

pulling velocity

becomes so

large

that the

assumption

of local

thermodynamic equilibrium

at the interface is violated, a linear

stability analysis

of these cells in the one sided model has not been

performed.

In this paper, we examine the linear

stability

of cells in the one sided model. We focus

on the case of small Peclet

numbers,

for which one can make an

analogy

between directional solidification and viscous

fingering

[7]. For this case, Karma and Pelcd

ii Ii

have

recently argued

that the cells should exhibit an

oscillatory instability.

The

goal

of this paper is to introduce the

stability

calculation and

apply

this to find an

oscillatory instability.

This paper is

organized

as follows: in section 2, the basic

equations

of directional solidification

as well as the numerical

techniques

used in this paper are reviewed. Section 3 describes the (*) Pennanent address : Inst. for Solid State Physics, Chemogolovka, U.R.S.S.

(**) assoc16 aux universit£s Paris VI, VII et l'Ecole Nomlale Sup6lieure.

(3)

shapes arising

from our numerics and compare the results from the numerics with

analytical predictions.

In section

4,

the

stability

of the obtained cells is

investigated

and in section 5 we discuss the limit

cycle

which results from the

instability

of

large

thermal

length.

2. Basic

equations

and numerical

technique.

The standard set of

equation

are well described elsewhere

iii.

As is often

done,

we go in the frame

moving

with the

pulling velocity

vp and measure

lengths

in units of half the

wavelength A/2

,

the concentration c in units of cn~

(the

concentration far away from the

interface),

and time in units of l~

/4D. Then,

for the one sided

model,

we have

v ~C +

2Pe)

=

Ii

(fi

V

cL)

"

-(I k)(2pefi

§ +

vn)cL

c~ =

j

= -7~c

(1)

Here,

D is the diffusion constant in the

liquid,

k is the

partition coefficient, f

is the dimensionless thermal

length,

7 is the dimensionless

capillary length

and pe is the Peclet number: pe

=

(~.

vn is the contribution from the interface other than the constant

pulling velocity

up which is

2pe

in our

units).

Of course, we have vn

= 0 for a

steady

state.

To solve the above set of

equations

in a numerical efficient way we rewrite the

equations

as a

integrc-differential equation

and solve for the

(unknown

and

free) boundary

[3] We will do this for both the

quasi-static approximation,

where we

neglect

the time derivative term in the

diffusion

equation

and for the full

equation.

In the

quasi-static approximation

we find

-(

+

7~t(S))

=

/(@

+

7~t(S')) (h'

?

'G(S> S'))

dS'

+2Pek /(@

+

7~t(S')) niG(S> S')

dS'

+

/ vn(S') (k(f

+

7~t(S')) (f

+

~t(S'))j

G(S>

S')

dS'

(2)

where the Green's function G is the solution of

V

~G

+

2pe )

=

-6~(x x') (3)

The

explicit

form of G can be found in reference [3].

For the non

quasi-static

case we go back to the rest frame and we find

Y~S>t)~~ 2P~t) ~~c(s,i)

= i

f

ds,

f~

di,

~Y~S'>t')~- 2P~t') ~c(s,,i,))

A~ v

'G(~(s,1), ~'(/,i,);i,i,)

+

f

ds~

f~

di'

~~~~"~'~j

~~~~'~

~(s',i~))

-~

G(~(s,t), ~'(s',t');t,t')(2pen(

+ vn

(s',t')) (4)

where G is a solution of the full diffusion

equation

T7

~G ~

=

-6~(x x')6(t t') (5)

(4)

To find

steady

state solutions we

parameterize

the

(unknown) boundary

with N

points

of

equal arclength.

Our

independent

variables are then the normal

angles

at the

midpoints

of the

equal ardength

sections and the

position

of the

tip.

We solve the

integrc-difLerential equation

on the

points

of

equal arclength,

except at the

endpoints (~

= 0 and ~

=

l)

and

require

that the

slope

vanishes at both the

tip

and the tail. In

general,

we have chosen a discretization rate of l10

points.

To examine the

stability

of the

resulting cells,

we

perturb

the

steady

state solution

by adding

the normal shift:

x(S)

=

xo(S)

+

iio(S)6(S>t) (6)

where we assume that

6(s, t)

=

b(s)e~~

and

b(s)

« I. We substitute this

perturbation

in

(2)

and linearize in

b,

which

gives

us

Ids, (7~o

+

(° )(6(s')41

v

'+ b(s)ho

T7

)hl

T7 'G +

~(~'~

~(6"(s')

+

c(b(s')))

hi

V 'G

f

+

?~to

+

~°) (-b'(S')il

'v 'G

+1C0b(S')fit

?

G)j

f -2pek /

ds'

fly

(71Co +

( )(6(S')fi~

V ' +

6(~)~°

?

)~

+ ji

~(~'~ 7(b"(s')

+

c(6(s')))

G'

~

f

+

7~o

+

(° (-b'(/)iiG

+

iy~to6(s')G)j

+

~~~'~ 7(6"(S')

+

C(b(S')))

f

= w

/ dsJ(I k)

+ 7no

6(s')G (7)

f

The discretization of the

integrals gives

us a set of

equation

of the form

M M

L Aij6j

= w

L B"j

b>

(8)

>=o j=o

where M is the number of discretization

points.

This

ordinary eigenvalue problem

for w can be solved with one of the standard numerical

packages.

For the non

quasi-static approximation

we

again

substitute the normal shift in the

integrc-

difLerential

equation (4).

This

gives

us:

Ids' (7~co

+ ~°

)(b(s')fi[

V ' +

b(s)fro

V

)fi[

V

'G(w)

3~~,

+

7(b"(s')

+

n(b(s')) hi

V

'G(w) f

+

71Co

+

() (-6'(S')i~

'V

'G(W) +'~06(S')fi~

'~7

G(~°)j

-2pek /

ds'

fly

(7~co +

)(6(s')fi[

V

'+ 6(s)fro

V

)G(w)

f

(5)

fi( J)

+

~v (f 7(b"(S') '~(6(S')))

G(~°)

+

7'~o

+

() (-6'(S')I$G

+

ylCo6(S')G(W))j

+

~~l'~

7(b"(S')

+

C(b(S')))

" ~k°~

/

d~'

((

+

~0) b(S')G(W) (9)

where an

explicit

form of

G(w)

is

given

in reference [9].

Upon discretizing

the

integrals

we get

an

equation

like

£

M

Cjj(W)bj

# 0

(10)

j=0

where C is a function of w. and therefore in

general complex.

To solve the above

equation,

we

have to vary w until C has a zero

eigenvalue.

This is done with a Newton's

algorithm

which will converge to the

right

w after we have

guessed

an initial value for w.

The

technique

for

finding

the

growth

rate of the

perturbation

is the

following.

We will first examine the

stability

of the pattern in the

quasi-static

limit. We will not expect to find the

oscillatory instability

in this way but it is a useful first estimate. We then calculate the

largest eigenvalue

for

a number of

growth

rates. This will

give

us an indication where the

eigenvalue

becomes zero. We then use a Newton's solver to

pin

down the value of the

growth

rate for which the determinant, or the

largest eigenvalue

is zero. For further details we refer to

[10].

3.

Steady

state cell

shapes.

In this

section,

we will

investigate

the cell

shapes corresponding

to the

region

in parameter space where one can compare these cells with the

fingers

in the

Salfman-Taylor (ST) experiments

[7].

We have taken the diffusion constant to be D

= 2.5 x 10~~ m~

Is

,

the

capillary length

to be

do " I. x 10~~ m and the

wavelength

= 20. x 10~~ m. For the

partition

coefficient k we have

taken two

values,

k = 0.2

corresponding

to a subcritical

bifurcation,

and k

=

0.8, corresponding

to a

supercritical

bifurcation. The thermal

length

lT is used as the control parameter, but is

always large compared

to the difLusion

length 2D/vp.

This is

important,

since this enables us to check the

stability

program in a non-trivial way

(see below).

Depending

on the distance from the neutral curve, we obtain either a

deep

cell

(see Fig.

la)

or a shallow cell

(see Fig-16).

From

figure

la we see that the cell is indeed very

deep (notice

the difference in scales on the

axis)

and has a little bubble at its tail. This seems to be characteristic of these

deep

cells and has been

reported

in earlier numerical work in both the one-sided and

symmetric

model [3, 5]. This bubble is also present for the values of

lT

close to the

marginal stability

curve

(see Fig. lb).

We think that this bubble does not have

a

significant physical meaning,

in the one-sided

model,

for two reasons: first of

all,

since the cells are

propagating

into the

liquid,

the solid

just

above the bubble will melt first and then

resolidify,

as the cell moves on. This seems to be rather

unphysical

in the one-sided

model,

where one

neglects

the diffusion of

impurities

in the solid. A second argument is the numerical

result

plotted

in

figure

2 where we have

plotted

the cell

shapes

for fixed

velocity

and

wavelength

but different discretization rates. We see that the

tip

of the cells remain

essentially unchanged

and that the bubble propagates down as we increase the number of discretization

points.

It therefore seems

likely

that the cell

prefers

to be infinite

deep

and that the bubble is an artifact

(6)

-30300

-30400

1

-30500

~

-30600

-30700

O.O 2.O 4.O 6.0 8.O lO.O

x

~m) a)

-450

-soo

-550

-600

O.O 2.O 4.O 6.O 8.O lO.O

x

@m)

~~

Fig-I. a)

A typical example of a deep cell

(k

= 0.8, ~ = 144

pm/s,

IT

= 25300pm; other material parameters as given in

text). b)

An example of a cell close to the marginal stability curve, for a supercritical bifurcation

(k

= 0.2, ~ = 134

pm/s,

IT = 400

pm).

of our zero

slope

condition at the tail. This result is

typica1for

the one-sided

model;

in the

symmetric

model we do observe a similar bubble at the tail of the

cell,

but its

position

does not

change

as a function of the discretization rate.

Before we discuss the

stability

of the

cells,

let us

verify

that we are indeed in the ST

regime.

In

figure

3 we have

plotted

the

position

of the

tip

vi vs. the

pulling velocity

vp. As we can

see, this curve is non-monotonic. For vp < 600

pm/s

the

position

of the

tip

increases

by

increasing velocity.

This part of the curve we will call the ST

branch,

while the part on which the

tip position

decreases for for

increasing velocity

we will call the second branch

(see

also the discussion section

below).

In this paper we will focus on ST

branch,

for which we expect

(7)

-25

[

125

/~

~

/ 100 Points

-225

250 points

325

2 4 6 8

x

(~m)

Fig.2.

The cell shapes for fixed material parameters but different discretization rates.

-2500

_

-3000

~

<

c

° -3500

aI

+

~ -4000

-4500

O 200 400 600 BOO IOOO

Velocity ~ptn/s)

Fig.3.

The position of the tip Vt as a function of the pulling velocity ~p, for IT

" 1100 pm and

k

= 0.2. The circles represent the numerical data points, with the solid line as a guide to the eye.

the

tip position

to increase for

increasing velocity ill].

We can also

directly

compare the

steady

state cells with a ST

finger.

We know that in the limit of

large

IT

compared

to the diffusion

length,

the cell should have a width A of

ill]:

i

A= ~~

(II)

I-(I-k))

T

(8)

where

§

is the

position

of the

tip

of the cell relative to the

position

of the

planar

interface.

We have verified the above relation with our numerics. We find that the width of the

finger

agrees within 5$lo of the value

given

above.

Furthermore,

the width remains

roughly

constant for thermal

lengths typically

an order of

magnitude larger

than the difLusion

length.

We can

therefore conclude that we are on the ST branch. In other

words,

the results of Karma and Pelcd should

apply

to our cells.

There are some checks on our

stability

calculation. First of

all,

we can check that the

planar stability

calculation

gives

the

right

answer. The other check uses the fact that the nature of the bifurcation of the

planar

interface can be either super- or subcritical. For

metals,

with small

k,

the onset to cells from the

planar interface,

is

typically through

a subcritical bifurcation.

Indeed,

as we decrease the

wavelength

for fixed

velocity

for k

=

0.2,

we encounter a saddle- node bifurcation. From

elementary

bifurcation

theory,

we know the

stability assignments

of the two

resulting branches;

the upper branch should be

stable,

while the lower branch should be unstable. Our numerics also agree with this

stability picture, although

in the

vicinity

of the

saddle node we need more

points

on the interface to resolve the

stability.

The last check of the program, is a

highly

non-trivial one. If we take the thermal

length

to be much

bigger

than the diffusion

length,

we

approximate

the case of a dendrite in

a channel.

There,

we have a

single

cell

growing

in a narrow channel, in the absence of a temperature

gradient (I.e. lT

"

oo).

As has been

shown,

both

analytically

[12] and

numerically [13],

in the

case of a dendrite in a channel the ST branch is unstable. This

provides

us with an excellent check for our

stability

program: the cell should become unstable for very

large lT.

We have

indeed found that this is the case, as will be discussed in detail below.

4. The

oscillatory instability.

As mentioned

before,

Karma and Pelcd

ill]

have

recently argued

that in the limit of small Peclet

numbers,

the cells can

undergo

a

Hopf

bifurcation.

Using

an

approximate

interface

formalism, they

showed that the

growth

rate can have a

positive

real part with a non-zero

imaginary

part, which would mean an

oscillatory instability.

If one would increase the thermal

length,

one will encounter a first critical thermal

length

for which the real part of the

growth

part becomes

positive.

If one increases the thermal

length

even more, the

complex conjugate

root

pair

will

collapse

into two pure real

positive

roots at a second critical thermal

length.

One of the roots is

going

to a finite

value, corresponding

to the

instability

of the dendrite in a

channel,

and one is

going

to zero,

corresponding

to the zero mode which is present in the case

of zero temperature

gradient.

To

verify

the result of Karma and

Pelcd,

Kessler and Levine

performed

a linear

stability analysis

like we have

presented

in this paper, for the

symmetric

model [9]. That

is, they

obtained

steady

state solutions with the

integrc-difLerential method, perturbed

this solution with a normal shift and solved the

resulting eigenvalue problem

for the

growth

rate of the

perturbation.

Their conclusion was that there was no evidence for an

oscillatory instability.

These

contradictory

results have been controversial ever since. There are a few

possibilities

for the

disagreement,

apart from the fact that one of the two groups

might

have made a mistake.

One

possible

difference between the two

approaches

is that Karma and Pelcd

analyzed

the one sided model while Kessler and Levine used the

symmetric

model.

However,

we will argue below that we don't believe that there will be an essential difference between the models.

Nevertheless,

we have

performed

all our calculations in the one sided model.

For the parameter values of Kessler and

Levine,

we have not been able to find an

instability.

All the cells are

linearly stable,

consistent with the results of Kessler and Levine.

However,

as we have

pointed

out

above,

for

large

IT the

problem

of directional solidification

approaches

JOURNAL DE PHYSIOUEI T 2, N'9. SEPTEMBER 1992 64

(9)

O.3

O.2

o-1 5

j

o-o

-o.i

-O.2

SOD 1000 1500 2000 2500

~~wn)

FigA.

The real and the imaginary part of the eigenvalue as a function of the thermal length IT Here, k

= 0.2 and pe

= 0.268.

that of the dendrite in a channel.

There,

as has been shown before

[12],

the cell

corresponding

to the ST branch is unstable. It is therefore

logical

to extend the range of parameters to

larger

IT. Note that the ST branch in a channel is also unstable in the two sided model, and we

therefore expect to see the same

qualitative

behavior in that case [14].

We have

performed

the calculation for two different values of the

partition

coefficient: k

= 0.2

and k

= 0.8. For a fixed Peclet number pe we have varied the thermal

length

IT and have examined the

stability

of the

resulting

cells.

For all Peclet numbers we found that if we increased the thermal

length

above a critical

value,

say

lT,c

the cells become unstable. For

large

values of lT

(I.e.

lT »

lD),

this

instability

is

always

pure real. This is in

agreement

with the

stability

calculation for a dendrite in a

channel,

as well as Karma and Pelcd.

The results of the

eigenvalues

for k

= 0.2 and pe = 0.268 are

presented

in

figure

4.

Here,

the solid line

correspond

to the real part of the

largest eigenvalue,

and the dotted line

correspond

to the

imaginary

part of this

eigenvalue.

We see that the cell becomes unstable with for lT ~' l125 ~tm, and that the

instability

has a non-zero

imaginary

part. In other

words,

we do

have an

oscillatory instability

here.

Our numerics

show, however,

that an

oscillatory instability

occurs

only

for

larger

Peclet number

(I.e,

pe >

0.I).

For small Peclet number

we have

never found an

oscillatory instability.

There,

the

eigenvalue

becomes pure real so close the

lT,c

that we are not able to observe a

non-zero

imaginary

part for

positive

real part. Note however that the

imaginary

part of the

growth

rate at the critical thermal

length

in Karma and Pelc6's

theory

goes to zero as pe goes

to zero. It is

possible

that our numerics cannot handle such a small

imaginary

part.

In

figures

5a and 5b we have summarized our results for the two values of k. The solid line

correspond

to the

predicted

value of

lT,c.

We see that of the two curves the one for k

= 0.8

agrees better with the

prediction

of Karma and Pelc4. For this value of k, our numerics agree better with the solid curve for small values of pe. This is

expected

since their

analysis

is valid for small Peclet numbers. For

higher

values of pe the

analytical lT,c

becomes constant, while the

numerically

obtained value increases

again.

This can be

explained by noting

that

(10)

3500

2500

soo

SOD

~~

a)

isoo

iooo

soo

O

0.OO O.05 O.lO O,15 O.20

pe ~~

Fig.5. a)

Our numerical results for lT,c

(circles)

and the prediction Irom the analytical theory

(solid line).

Here k

= 0.8,

b)

Same as

figure

5a but now for k

= 0.2.

for

increasing

Peclet number we will move towards the stable second

branch,

which will be discussed in more detail in the

following

discussion

(see

also

Fig. 6).

As one moves toward the transition

point

between the two branches

lT,c

- oo since the second branch is stable.

The

analysis

of Karma and Pelcd is of course

only

valid for the ST branch.

Also, according

to Karma and

Pelcd,

the thermal

length

for which the

instability

becomes pure real is much

larger

than

lT,c.

Our numerics

however,

find no second critical thermal

length,

or one which is much closer to

lT,c.

(11)

~t

limit C

ST Second

branch branch

~ V

P

Fig.6.

A schematic drawing of the limit cycle arising Irom the instabfiity for large thermal length.

The solid line corresponds to the steady state solution branch while the dashed curve corresponds to the limit cycle. The ST branch

(or

at least the part on which point A is

located)

is unstable while the second branch,

corresponding

to the decreasing part of the non-monotonic curve is stable

(compare Fig.3)

The limit cycle will consist ofthe trajectory D - E

- C - D. For

a detailed explanation see the text.

5. Discussion.

To summarize our numerical

results,

we can say that in the ST limit the cells will become unstable for

large

IT- If we are in the unstable

region

the

instability might

or

might

not be

oscillatory

of nature,

depending

on the

parametervalues

of the system. The agreement with the

theory

of Karma and Pelcd is at most

partially.

Let us now

discuss,

what we think this

instability

will lead to. We

emphasize

that the scenario

we are

giving

here is

only

valid for the case when

wavelength

selection is not available. In other

words,

we envision a situation where the cell cannot

adjust

its

wavelength. Experimentally,

this would

correspond

to directional solidification in a channel. If the

wavelength

can be selected it is very well

possible

that the

instability

described in this paper can be avoided

altogether.

The limit

cycle

which will arise is sketched in

figure

6. We assume a

large

but not infinite thermal

length (I.e.

the temperature

gradient

is small but

non-zero).

Here we have

sketched,

as a solid

line,

the two

existing steady

state

branches,

as in

figure

3. Note that the

dependence

of vi on up is non

monotonic,

and

corresponds,

in the limit of

large lT,

to the one discussed in reference

[14].

To avoid any

possible

confusion we note that in the

problem

of a dendrite in a channel one

typically plots

the

velocity

as a function of the

undercooling, resulting

in a double valued curve.

Here,

we

plot

the

tip position

as a function of the

velocity resulting

in a non- monotonic function. In reference

[14],

it was shown that the ST branch

(where

yt increases for

increasing

vp, compare

Fig. 3)

is unstable while the second branch is stable

(we

have verified that the cells

corresponding

to the second branch of

Fig.3

are indeed

stable). Thus,

the

steady

state solution we start with

(point

A in

Fig. 6)

is unstable. If we start from this unstable solution on the ST

branch,

it is

possible

to

jump

to

point

B on the second branch. The time for this

jump

is

quite

small:

2jump

-~

1/Re

w where w is the

growth

rate of the

perturbation.

At B, the

tip position

of the cell will be

essentially unchanged

but the

tip velocity

vtip is

larger

than the

pulling velocity

vp.

(12)

Next,

the

tip

of the cell will advance in the channel towards a hotter

region,

while the

velocity

of the

tip

decreases

(B

-

C,~following

the dashed

curve).

At

point C,

the

velocity

of the

tip

is

equal

to the

pulling velocity:

vtip " vp. There is no stable

steady

state solution

however,

so that the

velocity

continues to decrease and becomes smaller than the

pulling velocity.

As

a result, the

tip position

decreases as well and the cell will follow the

trajectory

indicated

by

the arrow in

figure

6 on the dashed curve

(C

-

D).

The time for this process is of the order

of

lT/vtip,

which is

quite large.

Once vi has decreased so much that the

tip position

is smaller than the

largest possible

vi on the

branches,

we have

again

the

possibility

of a

jump

to the second branch

(D

-

E).

This will

finally give

us a

limiting cycle

D - E - C -

D,

as sketched in

figure

6

by

the dashed curve. The average

velocity

of the cell

during

this limit

cycle

should be the

pulling velocity

vp and the

period

of the

cycle

will of the order of

lT/@.

The selection of the

points

D and E on the solution branches are not known at the moment

(one

should solve the full non-linear

problem),

but

perhaps they

will be selected

by

the condition = vp. Note

that,

since yt is related to

it,

the width of the cell will

(slowly)

oscillate.

Let us conclude with a final word on

sidebranching

in dendrites. Karma and Pelc6 have ar-

gued

that their

oscillatory instability

could be a mechanism for the side

branching

in dendrites.

This idea of a linear

Hopf instability

from cells to dendrites which leads to

sidebranching

does not agree,

however,

with the

general accepted phenomena

of free space dendrites. First of

all,

one has found that the free space needle is

linearly

stable. Sidebranch

generation

can be

explained

if one introduces a noise-driven mechanism.

Secondly,

unlike the case of cellular structures, dendrites

depend

very

strongly

on the

anisotropy

of the

crystal.

We therefore do not believe that the

oscillatory instability

could lead to

sidebranching.

In

conclusion,

we have

presented

numerical results on the

stability

of cells in the one-sided model of directional solidification. We show that our program

produces

an

instability

for

large

values of the thermal

length.

We also show

that,

for some values of the parameter, we find an

oscillatory instability.

Acknowledgements.

One of us

(E.A.B.)

has been

supported by

the Minist4re de la Recherche et de la

Technologie.

Part of the work of E.A.B. was done

during

a visit at IFF-KFA Jiilich. We would like to

acknowledge

useful discussions with H. Levine.

References

ill

For a review, see e.g.

Langer

J., Rev. Mod. Phys. 52

(1980)

1;

Langer J., Chance and Matter, J. Souletie, J. Vannimenus and R. Stora Eds.

(North-Holland,

Amsterdam,

1987);

Kessler D-A-, Koplik J, and Levine H., Adv. Phys. 37

(1988)

255.

[2] de Cheveign4 S., Guthmann C, and Lebrun M., J. Phys. France 47

(1986)

2095.

[3] Kessler D-A- and Levine H., Phys. Rev. A 39

(1989)

3041.

[4] Kessler D-A- and Levine H., Phys. Rev. A 39

(1989)

3208.

[5]

Ungar

L-H- and Brown R.A., Phys. Rev. B 29

(1984)

1367, 30 3993

(1984);

31

(1985)

5923, 31

(1985)

5931.

[6] Ben Amar M. and Moussaflam B.,

Phys.

Rev. Left. 60

(1988)

317.

[7] Dombre T, and Hakim V., Phys. Rev. A 36

(1987)

2811.

[8] Weeks J.D. and van Saarloos W., Phys. Rev. A 42

(1990)

5056; See also Weeks J.D., van Saarloos W. and Grant M., J. Cryst. Growth l12

(1991)

244.

(13)

[9] Kessler D-A- and Levine H., Phys. Rev. A 41

(1990)

3197.

[10] Levine H, and Rappel W.-J., J. Phys. I France1

(1991)

1291.

[11] Karma A. and Pelcb P., Phys. Rev. A 39

(1989)

4162;

Karma A. and Pelc+ P., Europhys. Left. 9

(1989)

713, Karma A. and Pelc+ P., Phys. Rev. A 41

(1990)

6741.

[12] Pelce P.,

Europhys.

Lent. 7

(1988)

453.

[13] Levine H., private communication.

[14] Brener E.A., Geilikman M.B, and Temkin D-E-, Sov. Phys. JETP 67

(1988)

1002.

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