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HAL Id: jpa-00246957

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Growth roughness and instabilities due to the Schwoebel effect : a one-dimensional model

Ilya Elkinani, Jacques Villain

To cite this version:

Ilya Elkinani, Jacques Villain. Growth roughness and instabilities due to the Schwoebel ef- fect : a one-dimensional model. Journal de Physique I, EDP Sciences, 1994, 4 (6), pp.949-973.

�10.1051/jp1:1994238�. �jpa-00246957�

(2)

Classification Phy.n<..i Ahsn.a<.li

68.95 05.20D

Growth roughness and instabilities due to the Schwoebel

effect

: a

one.dimensional model

Ilya

Elkinani and

Jacques

Villain

CEA, Département de Recherche Fondamentale sur la Matière Condensée, SPSMS. MDN, CENG, 17 rue des Martyrs, F-38054 Grenoble Cedex 9, France

(Re<.eii'e(13 Jamiaiy 1994. a<.<.epled /4 Fehriiari 1994)

Abstract, A very simple, one-dimensional model (« Zeno model ») of

crystal

growth by

molecular beam epitaxy is studied numerically. The essentiel feature of the Zeno model is that ii takes into account the asymetry of the sticking coefficient of adatoms to steps (Schwoebel effect),

i-e-, the

diffusing

atoms stick preferably to the Upper ledge. In contrast with other, more

microscopic

descriptions, the Zeno model takes the diffusion of adatoms into account through a

determiniUic diffusion

equation,

so that the computing lime is

greatly

reduced and a

systematic

investigation of the effect of the different parameters is

possible. Deep

cracks form even for a weak Schwoebel effect, but they form after a time which is very long if the Schwoebel effect is very weak. In certain cases, the roughness increases proportionally to time, in agreement with expenments on silicon and with other calculations. In the absence of Schwoebel effect, surface defects are healed dunng

growth.

1. The Schwoebel effect and its consequences.

In the

growth

of a

crystal by

Molecular Beam

Epitaxy (MBE),

the

freshly deposited

atoms

(adatom.ç) which diffuse on the surface (as shown

by Fig.

l in the case of a

high

symmetry

Fig.

l. Schematic representation of the MBE growth of a

high

symmetry surface.

Deposited

adatoms diffuse to a step or nucleate a new tenace.

(3)

surface)

do net stick with the same

probabihty

to the

edge

of Upper and lower terraces. The importance of this

peculiarity

was first

emphasized by

Schwoebel

[1]

who showed that this mechanism

(hereafter

called Schw,oevel

effect)

generates an

instability

in the

evaporation

of a vicinal surface. More

recently,

several authors

[2-10] pointed

ont other

important

conse-

quences of the Schwoebel effect. The present work is much related to that of

Eaglesham

and Gilmer

[8]

and of

Zhang

et ai.

[9].

Before

going further,

it is of interest to recall the mechanism of the Schwoebel effect.

Generally,

adatoms stick

preferentially

to upper terraces, because there is a

potential

barrer which makes it difficult for them to go down to a lower terrace

(Fig. 2a).

The reason is

basically

that, in order to go downstairs, an adatom must either

push

another one

(Fig. 2b)

or

go

through

an uncomfortable

position (Fig. 2c)

where it has too few

neighbours

and too

high

an

energy. The

exchange

mechanism of

figure

2b

(analysed by

Hansen et ai.

Il1]

in the case of

ordinary

diffusion on a

high

symmetry

surface)

is often believed to be more favourable in

typical

menais than that of

figure

2c,

investigated by

Bourdin et ai.

il 2]. Experimentally,

the Schwoebel barrier has been evaluated to be about 2 000 K for

W(110) Il 3].

a

b

c

~> D

d

Fig. 2. The Schwoebel effect. a) Potential seen by an adatom, b) The

exchange

mechanism suggested

by

Hansen et ai. in the case of adatoms diffusion without steps. cl Mechanism treated by Bourdin et ai.

d) Probability of

jump

per unit time.

The

subject

to be addressed in the present work is the

growth

of a surface of

high

symmetry below ils

roughening

transition. It is clear

[4]

that, for such a surface, a strong Schwoebel effect

produces

an

instability.

Indeed, on any growing terrace, adatoms land from the beam and, since

they

cannot go downstairs,

they

are

obliged

to nucleate a new terrace on which

another terrace will be nucleated, etc., so that the surface

is covered

by

towers rather than flan.

Even a weak Schwoebel effect may be

expected

to

produce

an

instabihty.

Indeed, it

implies

that the current of

diffusmg

adatoms has the same direction as the

height gradient

j

=

K Vz

(1.1)

with a positive coefficient K. Under certain

fairly

realistic circumstances

(implying

in

(4)

particular

the absence of

evaporation),

the local

height z(r)

satisfies a conservation

equation,

à=/ôt

=

div

j,

which has to be modified because of the effect of the beam. Thus the

corresponding equation

is

~~

=

Fa div

j (1.2)

where F is the beam

intensity. Comparing (1.1)

and

(1.2),

one obtains

É=Fa-KV~z.

(1.3)

A Fourier component =j of

z(r)

satisfies, if k # 0, the equation

art

,

=

KL- ri

Since K is

positive,

there is an

instability. However,

this

argument

is not

fully convincing

because a nonlinear term

proportional

to

(grad z)~

should be added to

(1.3). Moreover,

the above arguments say

nothing

about the actual

shape

of the surface.

The best theoretical information about the consequences of the Schoebel effect on the

shape

of a

growing

surface has been obtained

by

Monte carlo simulations

[5,

8,

10].

Experimentally,

direct evidence of the Schwoebel effect has been obtained

by

field ion

microscopy [2].

The

instability

observed

by Eaglesham

et ai.

Il 4]

in the

growth

of the

(001)

surface of silicon has been attnbuted to the Schwoebel effect

[8].

2, The Zeno model,

In the present work we propose an

oversimplified

mortel

which,

we believe, will

usefully complement

the Monte Carlo work. For reasons which will become clear in the

following,

this model will be called Zeno model, from the

philosopher

born in the lucanian

city

of Eleas in the sth century B,C. This model was

already

described in a

preliminary

communication

Il 5].

This model is, to a great extent, deterministic. In

particular,

the fluctuations of the beam intensity F in space and time, as well as the fluctuations of the diffusion current around the average value

(1.1),

will be

neglected.

These

approximations

are

justified

if the number of

partides

in some charactenstic time is

large enough,

more

precisely

if the

typical

terrace size

Î

is much

larger

than the atomic distance.

In

comparison

with Monte Carlo

simulations,

such a deterministic model has the

advantage

(in addition to its

simplicity)

to isolate the contribution of the different factors which can be

responsible

for kinetic

roughness.

Beam fluctuations and current fluctuations are mdeed such factors [4], and it is of interest to

study

a model

deprived

of such fluctuations, in order to

study

the other causes of

roughness

more

precisely.

One of these causes is the Schwoebel effect,

although

the term «

instability

» may be more

appropriate

than «

roughness

» to

designate

a deterministic process. However, m

expenmental

data

(microscope

image or diffraction

spectrum)

the distinction is not easy to make, since stochastic

phenomena

are

always

important.

A pi-tort, there may be another source of

roughness, namely

the nucleation of new terraces of

atomic thickness which will form the successive atomic

layers.

The

place

and time where

nucleation occurs are stochastic to a

large

extent. Can

roughness

anse from this

stochasticity

?

The answer can

hardly

be obtained from an

analytic

argument because

long

time,

oscillatmg

current correlations result from nucleation

(Fig. 3).

An important result of the present work will be that nucleation

stochasticity

atone cannot

produce roughness,

at least in one dimension.

(5)

~ /

ll~~s

it'

ô~ -

/

Fig. 3. After nucleation of an island (ai the current in the vicinity of the nucleus remains directed

toward the nucleu; dunng a time

z and then in the opposite direction 16) during a time T'. z and T' depend on the distance to the nucleus, but are both of order (though smaller than)

1/(Fa ).

Another feature of the Zeno model is that it is

« + »-dimensional, i-e- the surface is one dimensional. Of course the real world is

(2

+ 1) dimensional. A

(1

+

1)-dimensional

world may appear as an

unacceptable ~implification.

However, it is such a

huge simplification

that it is a necessary first step,

just

as mean field is a nece~sary first step in the

study

of

phase

transitions. Indeed the

dynamics

of a two-dimensional surface

depends

on many parameters, in

particular

the diffusion constants of atoms

along

a step. It is of interest to

investigate

a model with few parameters.

We have used two versions of the model the continiious version and the disc.rete version.

Bath versions are discrete in the direction z

perpendicular

to the

high

symmetry surface. In the contimiou.ç version, there is no atomic distance in the

high

symmetry direction.i

parallel

to the average

surface,

so that terraces may be

mfinitely

small. The

advantage

of this approximation

is to reduce the number of parameters.

Actually,

it will be seen that the continuum model

depends only

on a

surgie

parameter, which characterizes the

strength

of the Schwoebel effect.

A discrete version, where a finite interatomic distance is introduced, will also be used. It will be descnbed in section 6. In the present section the continuous Zeno model will be defined.

Any

state of the surface is charactenzed

by

the positions of the steps. The absciwa of the n-th

step from the left will be called i,,. We need to

specify

two

points:

ai the

velocity

v,, of each step ; b) the nucleation

probability

p~,, on each terrace. The former quantity can

easily

be deduced from the dassical

theory,

it is shown in

Appendix

A that the absolute value of the

velocity

r,, of a step separating an upper tenace of width

Î,,

and a lower terrace of width Î,( is

r,, =

f (f,,

+ g

(fi (2. i)

where the

expressions

of

f

and g will be

given

below, assuming the upper terrace to be on the

left hand side of the step and the lower terrace to be on the

right

hand side, so that

v~, is positive. The opposite case will

easily

be obtained

by

symmetry.

The forms of

f

and g

depend

on the type of terrace, which may be either a « top terrace » a

« bottom terrace » or a « vicinal terrace »

(Fig. 4).

(6)

T

B

Fig.

4. T is a top tenace, B is a bottom terrace. The other tenaces are

« vicinal

»

For a top terrace, g does not exist

(since

that terrace cannot be the lower

terrace)

and

f

is given on both

sides,

if a is the atomic

distance, by f(Î)

=

FaÎ/2, independently

of the

Schwoebel effect. The rote of the Schwoebel effect is

just

to increase the nucleation

probability.

For a bottom terrace,

f

does not exist

(since

that terrace cannot be the topmost

terrace)

and

g is given on both sides

by g(Î)

=

FaÎ/2, independently

of the Schwoebel effect.

For a vicinal terrace, it is shown in

Appendix

A that

aF ail

j

(2.2)

f(~)"i

ii ~m ~f+fi

'

~z

and

g(Î)=aFÎ-Î _aFÎ Îj

~ i ~

~'

2

~

~

Î

+

Îj (2.3)

where a is the interatomic

distance,

F is the beam intensity per unit time and unit

length,

and

ii

is a

length

which characterizes the Schwoebel effect. It tutus out to be

given by

ii

=

~~Î (2.4)

where

Dla~

is the

probability

per unit time for an adatom at abscissa x to

jump

to a

position

at abscissa (x + 1) or (x

1)

if this

jump

does not reqwre a

change

of

height

for the adatom.

D'la~

is the

probabihty

per unit time for an adatom to

jump

to a

neighbouring

site when this

implies

going to a lower terrace

(Fig: 2d).

D is the diffusion constant of an adatom on the

ideally

flat surface.

After

having

given the formulae for the step

velocities,

we have to calculate the nucleation

probability

per unit time on a terrace. Its detailed form

depends

on the features of the nucleation process. For instance, if we assume that two adatoms which meet form a pair which

is stable and immobile, then the nucleation

probability

per unit time on a top terrace is found

(App. A)

to be

~~~~~~~ ÎÎÎ ~

~

~~

~~'~~

The nucleation

probability

on a bottom or vicinal terrace is given m the

Appendix. They

are

not essential since most of nucleation events take

place

on top terraces.

An important quantity is the

typical

size of a top terrace when nudeation takes

place.

It is

argued

in the

Appendix

that this size

corresponds

to a value of the above

probabihty

of the

JOURNAL DE PHYSIQUE T 4 N'6 )UNE 1994

~~

(7)

order of Fa

F~ Î) Îj

fi

~ ~

Î~

~~

~~'~~

We shall call

f~o

the value of

Î~

m the absence of Schwoebel effect. Thus

FÎ)o

m 12 Da

(2.7)

or

ij~i~

+ 6

ii)

=

ij~ (2.8)

STEP MOTION IN THE CASE OF MULTIPLE STEPS. The presence of step bunches ares net

modify

the nucleation

probability

nor the characteristic

lengths,

but does

modify

the step

velocity.

A bunch of p steps may be considered as a facet on which adatoms diffuse

freely.

The

possibibty

of nucleation on such a facet will be

neglected.

An adatom which reaches a step bunch from above will be assumed to

glide instantaneously

to the bottom of the bunch

(Fig. 5).

This

approximation

is not

satisfactory

for

large

bunches.

---l ---

a

b

c

d

Fig.

5. Advance of a multiple step.

Consider a bunch of p steps separating an upper terrace of width f and a lower terrace of

width

Î'.

As

before,

we call

f(Î)dt

the number of atoms

sticking

from above in time

dt and g

(Î')

dt the number of atoms

sticking

from below.

f(Î

and g

(Î')

are still given

by (2.2)

and

(2.3)

for vicinal terraces, and are

equal

to

FaÎ/2

in other cases. The atoms commg from

(8)

above and from below distribute themselves in different ways : an atom

coming

from above will stick above the

previous

one and an atom

coming

from the same level will stick aside the

previous one. Therefore the

f (Î )

dt atoms

coming

from above will

displace

the bunch

position by

the amount

v ~

dt

=

f

~~ ~~

(2.9a)

while the

g(Î')

dt atoms commg from the same level

(Fig. 5b)

will

displace

the lower step of the bunch atone

by

the amount

v~~

dt =

g(Î')

dt

(2.9b)

Thus,

the bunch tends to separate into an isolated step at the bottom and a bunch of

~/J

1)

steps. But this separation will

really

take

place (Fig. 5c) only

if that bunch does not

catch the bottom step

again

due to the

f(Î)dt

atoms

coming

from

above,

therefore if

vj ~ <

v~~

or

f(Î)

< ~p

1) g(Î').

In the opposite case

(Fig. 5d),

the step bunch does not dissociate and moves at the

velocity

~

f(f)

+

g(f')

(2.io)

p

3. Growth without Schwoebel effect.

3.1 NO SCHWOEBEL EFFECT, SURFACE INITIALLY FLAT. We have first

performed

simu-

lations without Schwoebel

effect, starting

from a flat surface. The

only

random process was the nudeation of new terraces, with the

probability given

in the

Appendix.

A

typical profile

is shown m

figure

6. The surface thickness is

essentially

reduced to two or three levels

(Fig. 7a),

but a few

higher bumps (or deeper holes) occasionnally

appear. If the time unit is the

layer filhng time,

the

largest

terraces have the

height

t at mteger time t, and there are small,

freshly

nucleated tenaces at

height (t

+

1),

and small terraces at

height (Î 1)

which are on the verge of

disappearing.

On the other

hand,

if the time is

half-integer,

ail terraces have

heights (Î

+

1/2)

and

1/2)

and are

approximately equal.

2002

2001

2000 z

1999

199s

~~~~.0

5.0 10.0 15.0 20.0 25.0

x

Fig.

6.

Typical

surface

shape

at integer coverage in the absence of Schwoebel effect for an

mitially

flat surface. The vertical direction is the height in monolayers ; the horizontal direction is the distance, using Î~~ as length unit.

(9)

1200 500

iooo

800

N(ZJ 600 N(1)

400

200 100

0 0

1997 1998 1999 2000 2001 2002 2003 Ô-Ô 0.4 0.8 12 1.6 2.0 2.4 2.8 3.2

z i

a) b)

Fig.

7. Growth of an

mitially

flat surface without Schwoebel effect. a)

Histogram showing

the proportion of the surface at

heights

1, and + at integer time t (there are aise two tenaces at height

( + 2 and one at1 2 which cannot be seen on the histogram), b) Terrace size distribution after filling 10 000 layers without Schwoebel effect.

The conclusion is that random nucleation does not lead to

roughness.

The size distribution of the terraces at an integer time is shown in

figure

7b.

3.2 HEALING OF DEFECTS FOR SAWTOOTH PROFILES OF SHORT WAVELENGTH. lt is weÎÎ

known

expenmentally

that defects such as

bumps

or

valleys

are healed

by

MBE

growth.

Our mortel does

reproduce

this property. For

simplicity,

we restncted our

study

to sawtooth

profiles.

We have studied

numerically

the

growth

of a

crystal

limited

by

a surface

exhibiting

a

periodic

succession of

straight

facets

(Fig. 8).

We have

imposed

a determmistic nucleation rule,

namely,

a new terrace is nucleated at the centre of each top terrace when its size reaches the value

Î~

= Î~~. Nucleation on terraces other than top terraces never occurs.

Figure

8 shows

1=0 toe20

t=40 -t=80

120

100

~---

---;

80

Z 60 .~

,

40 .'

20

0

0.00 0.20 0.40 0.60 0.80 1.00 1.20

x

Fig.

8.

Healing

of a saw-tooth

profile

without Schwoebel effect. Only one penod is

represented

at increasing limes (0, 20, 40 and 60 layers). Nucleation is determmistic.

(10)

the successive states of the

profile. They correspond

to a

period

L

=

1.2 Î~~ and to an initial

height h(0)

=

100.

Eventually,

a flat surface

corresponding

to

figure

6 is reached. In the intermediate states

(Fig. 8)

the surface consists of flat terraces at its top, which are bounded

by

a steep

edge

made of several

coalescing

atomic steps and

separated by

cracks. We will now try

to understand this structure in the case when the initial terrace width is shorter than

Î~.

This is the

experimentally interesting

case, because

Î~

is

generally

very

large

in MBE.

The variation of the interface thickness

(height

difference between topmost and lowest

point)

is

displayed

for a sawtooth

profile

in

figure

9a in a

typical

case. The initial decrease

corresponds

to the

flattening

of the top of the

profile,

when the width Î~ of the topmost terrace is smaller than Î~~. Then there is no nucleation at the top and, since bottom terraces are

annihilated,

the thickness decreases. When

Î~

become of the order of

Î~o,

the thickness decreases but very

slowly.

120

so ioo

80 60

Ah Ah 60

40

40

20

0 0

0.0 20.0 40.0 60.0 80.0 100.0 0.0 8000.0 16000.0 24000.0 32000.0

Time Tlme

a) b)

Fig.

9. Variation of the

height

difference (« interface thickness ») between the

highest

and the lowest point of the surface as a function of time. There is no Schwoebel effect. In case (a), the

period

is

L=1.2i~~

and the initial height difference is 100 atomic layers. In case (b), the penod is

~0 i~~ and the initial height difference is 100. The time unit is (1/Fa).

The evolution shown in

figure

8 is

easily

understood if the initial tenace width

is much shorter than

i~.

Indeed

(cf. Fig. loi

the topmost tenace of each

period readily

takes a width

i~ w1. Therefore, according

to

(2.2)

and

(2.3),

and because

ii

=

0 without Schwoebel

effect,

the topmost steps have a

velocity

of order

Fai~/2,

which is much

langer

than the

velocity Fai12

of the other steps. Therefore, the topmost steps coalesce with the next steps and form a bunch of two steps. This bunch will then

proceed

with a reduced

velocity.

The reduction factor is

approximately

2 because the progression of the topmost steps is

mainly

due to atoms

falling

from the upper tenaces, which are m identical

quantity

with or without

bunching,

and this

quantity

must be shared between two

steps.

Thus additional

bunching

will

follow,

and a

bunch of 3 steps, 4 steps, and so on, will form. Thus the

shape

of

figure

8 emerges.

The

healmg

time of a sawtooth

profile

with

period

2 L

~ 2

i~

is

easily

calculated. Indeed there is no nucleation until the surface is healed. Therefore the

healmg

time r~~~j is

just

the time

necessary to fill each

valley.

For a sawtooth

profile,

the

valleys

have a

height

h

=

Lli

and

an

area Lh/2

=

L~/21,

and

are filled after a time

~~~~~

2

Îa~

~~

(11)

1

_ a

Fal -

_ i

i

-

j

i b

i i i i i i i i i

C

Fig.

10. Growth of the top ofthe surface. Ifthe width

i~

of the topmost tenace is much

larger

than the width f of the lower terraces, the upper steps form bunches.

We have aise studied the case L

~

i~.

It tums eut to be

surprisingly compbcated.

The

profile

shows a step bunch near the top as

before,

but the new feature is that waves

develop

below the bunch

(Fig.

ii

).

The

wavelength

increases with time, so that the number of

bumps

decrease before

eventually vanishing.

As a consequence, the surface thickness has also an

oscillating

character

(Fig. 9b).

It decreases

abruptly

when a

bump disappears

from the

profile.

350 600

(a) (b)

330

310 560

Z

290 540

270 520

(c) (d)

s30 ioso

sio ioôo

z

790 1040

770 1020

750

0.00 4.00 8.00 12.00 16.00 u.00 4.00 8.00 12.00 16.00 20.00

x x

Fig. Il- Profile observed at successive limes (a) t =250, b) t=500, c) t=750 and d)

t 000) when heahng a sawtooth

profile.

The period is equal to 20 f~~. There is no Schwoebel effect and the nucleation process is determmistic. The units are the same as m

figure

6.

(12)

We have net been able to undestand the

origm

of this

instability.

We first

thought

of a

possible

artefact of time

discretization,

but we have checked that the time step was short

enough

to avoid any artefact.

Possibly

the

nonlinearity responsible

for the

instability

arises from collisions between steps, but we have not studied these collisions.

Healmg

of cracks has aise been

reproduced

in the case of a weak Schwoebel effect,

again

usmg a determmistic nucleation mechanism.

However,

these results are not reliable because it will be seen in the next sections that in the case of tandem

nucleation,

cracks may be

produced

even m the case of a very small Schwoebel effect.

4. Evolution of a surface with Schwoebel effect.

4.1 CRACKS. In this section we report simulations with Schwoebel

effect, starting

from an

initially

flat surface. Random nucleation is assumed. The

strength

of the Schwoebel effect is characterized, as said above,

by

the ratio ~

=

ijli~~,

note that it is convenient to

distinguish i~,

the actual characteristic

length

of nucleation on the topmost tenaces, and i~~ given

by (2.7).

i~

and

i~~

are related

by (2.8).

With a strong Schwoebel effect

(say,

for ~ ~ l cracks

develop

very

early. They

do not heal within the time of ouf

calculation,

so that their

depth

is

essentially equal

to Fat. This feature is

a consequence of the continuum

approximation.

The

density

of cracks cannot be

langer

than

lli~,

and seems to converge to a value of this order when ~ increases.

Actually,

even with a

fairly

weak Schwoebel

effect,

cracks also appear very

rapidly.

Figure

12 shows a

typical profile

obtained for

ijli~~

= 0.2. The cracks look similar to those m

a strong Schwoebel effect

they

become very

deep

while their width increases very

slowly.

However

they

appear

progressively.

For instance, if ~

=

0.20,

the first cracks

typically

appear

after

filling

20

layers (in

a

sample

of size 100

i~~).

Then the cracks'

depth

grows

nearly proportional

to time

(the

coefficient of

proportionality

is atomic size of

depth

pet

deposited layer).

The

deep

cracks observed in

figure

12a are

unphysical

because their width is smaller than

the interatomic distance.

However,

the other features

(density

of cracks, crack

shape,

roughness)

are the same as for a

physical

model with a finite atomic distance

(Fig. 12b).

We shall now try to understand the evolution of cracks. if the crack

profile

may be

approximated by

an

analytic

function z

(x)

of the « horizontal » coordinate

(parallel

to the

high

symmetry

orientation),

the evolution can be treated

by

the

theory

of Franck

[16].

The bottom and the top of the crack require

special

attention because, as will be

argued,

the

profile

there is

700 700

600

soo soo

400 400

Z Z

300 300

200

ioo ioo

o 0

0.00 20.00 40.00 60.00 80.00 100.00 0.00 20.00 40.00 60.00 80.00 100.00

X X

a) b)

Fig.

12.

Typical profile

at successive times for

ijli~~

=

0.20 in the Zeno model with random nucleation. a) Continuum limit. b) Fimte atomic distance, a

=

0.001f~~.

(13)

net

analytic.

In the next subsection we consider a

deep

crack, without caring about how it formed.

4.2 EvoLuTioN OF THE BOTTOM OF A CRACK. We consider a crack with a very

sharp

bottom. It is clear that the

profile

is not

analytic

at the bottom. A

sharp

bottom

implies

that the

tenace widths are small,

i~

«

ii.

This

implies

that the Schwoebel effect for these tenaces can

be considered as very strong. This argument is

only

valid in the continuum

approximation,

and has not

necessarily

a counterpart in a reabstic

problem.

Assummg

the Schwoebel effect to be

infinite,

the

equations

of evolution for a crack

having

a symmetry axis at ~r =

0 are

(Fig.

13a)

where

x,,(t)

denotes the

position

of the n th step at time t.

à 'Z

x ~

~

~

2

i~

~

---~----/---_

à

x~ z

x

b

1---$

Fig. 13. a) Labelhng the steps in the bottom of a deep crack (a) and at the top of the profile (b).

(14)

4.3 THE TRACK OF ZENO OF ELEAS.

Equation (4, la)

is

independent

of the other ones and its solution is

xi

(t

= A"1(0 exp

(-

Fat

(4.2)

This

apparently

harmless result

implies

that xi

(t)

never vanishes.

During

the nominal

layer filling

time, which is il

(Fa

),

only

a fraction

(1

île

)

of the lowest

layer

is filled. After a time

n/(Fa),

which is

nominally

the time to fill n

layers,

a fraction

xi

~

=xj(0)e~" (4.3)

Fa

is still unfilled. This is reminiscent of Zeno's

paradox according

to which Achilles will never catch the turtle if the latter has some initial

advantage,

say km. Indeed when Achilles will have run that kilometer, the turtle will advance, say one meter. Then, m the time necessary for Achilles to mn that meter, the turtle will mn one millimeter. At the n'th step of the argument, the turtle will still have an

advantage equal

tu

d~ = 10~ ~~ kilometers

(4.4)

The

similarity

between

(4.4)

and

(4.3) justifies

the

terminology

« Zeno

instability

» for the effect described above. There are of course differences between Zeno's

original paradox

and its modem version

applicable

to MBE. First of

ail,

ouf derivation and ouf result are

strictly

correct within the continuum model. Zeno's argument was

obviously

wrong. As fat as we

understand, it

just

reflects the

ignorance

of

Algebra

which affected the ancient Greeks. It should be remembered that Zeno's time was very

bright

for literature, but the great time of Greek Science was two centuries later On the other

hand,

Zeno's

theory

was formulated in a

dispute against

the

disciples

of

Pythagoras. Presumably [17, 18],

the latter may have known the sum of the

geometrical

series with

general

term

(4.4) although they

were not able to

formulate the calculation m a

convincmg language.

The

simple algebraic language

which is

nowadays taught

in ouf schools was not invented before the end of the sixteenth century

[19].

The

general

solution of

(4,1)

is

easily

seen to be

x,,

(t )

=

~jj' ~~ [~ Y

x,,

~

(0

exp Fat

(4.

5

Thus,

if xi, x~,

...,

x~

are known at time

0, they

are also known at a later time t.

Dur numerical simulations on the model described in section 2 confirm this result : if the Schwoebel effect is strong

enough,

cracks form their

depth

increases

proportionally

to lime, and

they

do not heal

during

the simulation.

Then,

how can one understand that, for appropnate

values of the Schwoebel effect, the crack

ultimately

heals after an initial increase ? To answer,

one should worry about the

edges

of the crack.

4.4 EVOLUTION OF THE CRACK EDGES. While it is easy, as seen m the previous section, to

study

the evolution of the bottom of a

crack,

it is more difficult to

figure

ont the evolution of a crack

edge.

A

priori,

two

simple

schemes may be

expected.

The two

possibilities

can be best

described in the case of a

periodic profile

with deterministic nucleation. In contrast with the previous

section,

it is convenient tu label the steps from the top of the

profile (Fig. 13b).

A first

possibility

is

that,

near its

edge,

the

profile

goes to a well-defined hmit. In other

words,

if one considers for instance

only

the times t where a new tenace is

nucleated,

one has for any given n

Lifrl

1,,(t

= 1~°

(4.6)

Co

(15)

Of course, in the continuum model addressed

here,

the crack

depth,

and therefore the

maximum value of n goes to

infinity

with time. Therefore the bottom of a crack cannot go to a

limit.

The other

possibility

is that the

freshly

nucleated steps merge into a step bunch, as occurred without Schwoebel effect when

healing

a sawtooth

profile. Then,

the

position

u

(t)

of the step brunch on the left of a maximum is an

increasing

function of

time,

except if a bunch appears above a bunch an event which has never been observed. Let h

(t

be the

height

of the

bunch, H(t)

the crack

depth

and L the

period. H(t)

is counted from the top of the

bunches,

so that

h(t) ~H(t).

The numerical calculation suggests that the nucleation rate, as well as the increase of H, is

approximately uniform,

so that

H(t)~F't

where F' may be different from F. The

quantity

of matter which faits mto the crack pet unit time is also

approximately uniform,

and therefore it is

bigger

than

F"i~,

where F" is a

number. This matter is to be distributed among the h steps of the bunch, so that the width

(L/2 u)

of the crack decreases

by

the amount F"/h in a time unit. Therefore

du

F"i~ F"i~ F"i~

à

h ~ H

~F't

Integration yields

F "

i~

"~~ ~

F'

~~

~~'~~

This expression goes to

infinity

with time t. This

implies

that the crack width

L/2

u(t)

vanishes after some time. Thus the cracks should heal.

The two scenarios described above

(crack reaching

a

stationary shape

and crack

heabng)

are

the

simplest possible

ones. In the absence of Schwoebel

effect,

and also m weak Schwoebel

effect, preexisting

cracks seem to heal

according

to the second scenario.

Figure

14

gives

an

idea of the evolution of a crack for a

fairly

strong Schwoebel

effect, iili~

= 0.5. As shown m

figure

lsa, the

slope

at the crack

edge regularly

increases as

,à.

This is

consistent with the second of the scenarios described above. The crack will

presumably

described above. The crack will

presumably

heal after a very

long

time,

although

this has not been observed in the present calculation.

5. Weak Schwoebel effect.

5.1 EVOLUTION OF THE PROFILE wiTH TIME.

-Figure16

shows the

profile

obtained for

ijli~~

= 0.05 at successive times from an

mitially

flat

profile, using

the velocities defined

by

(~.l-3),

and the nucleation

probability (2.5).

As in the case of a strong Schwoebel effect studied in the previous section, there are

deep cracks,

visible m

figures

16c to e.

However,

there are

significant differences,

m

particular

:

i)

For coverages lower than 1000

layers,

the

profile

is

just

a little

rougher

than without Schwoebel effect. There is no

striking

difference between the

profile shapes

observed after

deposit

of 500 and 1000

layers.

ii) Healmg

of cracks is

occasionnally

observed. For instance, the

deep

crack observed near

1= 80 in

figure

16c is no

longer

observed as a

deep

crack in

figure

16d.

However,

a small

(16)

2050

(a) (b)

iooo

9so 19so

z 900 1900

sso isso

soo

(c) (d)

3000

2950 7950

Z 2900

2850

2800 7800

2750 7750

0.00 0.20 0.40 0.60 0.80 1.00 0.00 0.20 0.40 0.60 0.80 1.00 1.20

x x

Fig.

14. Profile of a crack at coverages 1000 (a), 2000 (b), 3000 (c) and 8000(d) for

f~/f~~ = 0.5 in the continuous model. Nucleation is deterrninistic.

iooo.o

100.0

-,-__--

' '

-~

-,-

~

i

~

- .

iooo.o

Time Time

a) b)

Fig. 15.

increase as functions of t'~

depression

is observed at the same

place,

and is

presumably responsible

for the crack which reappears later at the same

place.

iii)

For coverages lower than 2000

layers,

the bottom of ail cracks moves

upward,

m

contradiction with the argument à la Zeno given m section 4.2. As seen m section

4.4,

this can

be understood as an effect of the crack

edges. Figure

17 shows the interface width for a

sample

(17)

99s

~ 990

485 ?Si

48Ù

~~j ~~j 98Ù

iioo

z

(c) (ii

iioo

145Ù

14ÙÙ Z

13so

1300

(ti (o

Ù.ÙÙ lÙ,ÙÙ 4Ù,ÙÙ lÙ,ÙÙ 8Ù.ÙÙ Ù.ÙÙ lÙ.ÙÙ 4Ù,ÙÙ lÙ,ÙÙ 8Ù.lÙ IÙÙ.ÙÙ

x x

Fig.

16. Profile at coverages 500 (a) 1000 (b) 15 000 (c) 2 000 (d) 2 500 (e) and 5 000 (fl monolayers for

fj/f~~

= 0.05. Note that the ordinate~ have different scaies in the different pictures. The

units are the same as m

figure

6.

of size 100 i~~ for a

particular

run. It shows

straight

pieces of

slope

terminated

by

an

abrupt

decrease. This decrease

corresponds

to the

healmg

of the

deepest

crack.

At

longer

times, the lifetime of the cracks becomes much

longer.

For instance, at coverages between 3 300 and 5 000, the interface width is a linear function of time with

slope (Fig.

17).

This means that the

deepest

crack dues not heal

during

this time.

5.2 ROUGHNESS. The

roughness

at time t is defined as

IL

L 1/2

ôh(t)=-

ΰ d£r

dV[h(V,t)-h(,1,t)l~) (5.1)

o o

(18)

where the

angular

brackets denote an average on many runs. In

practice,

we have made

only

one run. The results are shown m

figure

18. It is of interest to compare this

roughness

with the

experimental

observation of

Eaglesham

et ai.

[14, 8]

that the

roughness

mcreases

linearly

with

time until a critical coverage of a few hundreds of

monolayers,

when the material becomes

3000 200

2500

150 2000

" isoo " ioo

iooo

so soo

0

~~~~~ ~ 20000.0 3°°~°'°

0

~ 2000,0 3000.0 4000.0 5°°°'° ~'~

Tlme

0.0 1000.

~~

a) b)

Fig. 17. Interface thickness as a function of time : a) contmuum model with

ij/f~~

= 0.05 ; b) discrete model with f~/f~~ 0.03, and

a/f~~

O.COI. The units are the same as in

figure

9.

30.0 10.0

25.0

8.0

)

20.0

(

6.0

i~ 15.0

~

Î )

4.0

5.0 2.0

0.0 0.0

0.0 10000.0 20000.0 30000.0 0.0 1000.0 2000.0 3000.0 4000.0 5000.0

Time Time

a) b)

25.0

20.0

(

6.0

(

lS.0

Z z

Îi Î~

4.0 1 10.0

2.0 5.0

0.0

0.0 400.0 800.0 1200.0 1600.o 0.o 1000.0 2000.0 3000.0 4000.0 5000.0

Time Time

c) d)

Fig.

18.

Roughness

vs. time for

fj/f~~

0.03 (a), 0.05 (b), O.l (c) and 0.2 (b). Curves (b) and (c) correspond to the continuum model, and curves (a) and (d) correspond to an atomic distance a, with a/f~~ 0.005. The coordinates are the

same as m figure 9.

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