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Mapping of (1+1) D-Crystal Growth onto a 14-Vertex Model

F. Hontinfinde, A. Levi

To cite this version:

F. Hontinfinde, A. Levi. Mapping of (1+1) D-Crystal Growth onto a 14-Vertex Model. Journal de

Physique I, EDP Sciences, 1996, 6 (7), pp.873-890. �10.1051/jp1:1996104�. �jpa-00247220�

(2)

J. Phys. I France 6

(1996)

873-890 JULY1996, PAGE 873

Mapping of (I + I)D-Crystal Growth onto

a

14-Vertex Model

F. Hontinfinde

(*)

and A-C- Levi

(**)

Dipartimeuto di Fisica and Istituto Nazionale per la Fisica delta Materia, via Dodecaneso 33, 16146 Geuova, Italy

(Received ii January1996, received in final form 4 March 1996, accepted 19 March 1996)

PACS.02.70.Lq Monte Carlo and statistical methods

PACS.81.10.-h Methods of crystal growth; physics of crystal growth

Abstract. A restricted solid-on-solid

(SOS)

single- and double-step model is introduced and studied with Glauber dynamics. Kinetics and roughness of the growing crystal are described

in terms of a Markov process whose states are given by the crystal upper edge profile that we

map onto a 14-vertex model. We solve exactly the kinetic equation for small-size versions of the model. Extensive simulations are performed to derive the large scale properties. The present study appears as a further extension of Gates and Westcott's investigation of the single-step

model.

1. Introduction

Crystal growth, beyond

its

technological applications,

has a

long

and rich

history

of studies in basic science

ill

and has

generated,

at a fundamental

level, interesting problems

of non-

equilibrium

statistical

physics.

Its

study by

theoretical and

experimental

methods has

provided

a

deep insight

into solid state

physics

and

chemistry. Despite

the recent

significant

progress

obtained

by using

statistical-mechanical models and methods

[2-4]

to

clarify

cluster and

crystal growth phenomena, high-dimensional growth

models are still

complicated beyond

any

hope

of

an exact

solution,

even when well-known,

oversimplifying approximations (such

as

SOS)

are

applied.

In lower

dimensions,

the situation is less hard and some important results are available in the literature

concerning growth

kinetics. Garrod [5] solved several two-dimensional

growth

models where

growth

occurs

essentially

at kink sites. Gates and Westcott [6,7] studied

exactly

a restricted SOS

single-step

model defined on a

hexagonal

lattice and a non-restricted SOS model defined on a square lattice,

relying

on a

dynamic reversibility

concept valid in these models.

Their results on

growth

kinetics and

regimes supplement

those found in previous

investigations

on

polymer crystallization,

island or cellular structures and 2-D

crystal growth

[8, 9j.

Recently,

Hontinfinde and Touzani introduced a kinetic four-vertex model to

study

the

single-step

model in d

= I + I where atom

deposition, evaporation

and diffusion on the surface take

place [lo].

The main result

they

obtained is a reentrant

growth phase diagram similar,

but

probably

not equivalent to what is often observed

experimentally during

the

epitaxial growth

of metal

(*) On leave from LPT, Facultd des Sciences, BP 1014, Rabat Morocco and

IMSP(UNB),

BP 613

P/Novo

Benin

(**) Author for correspondence

(e-mail: levi@vaxgea,ge.infn.it)

© Les Editions de Physique 1996

(3)

874 JOURNAL DE PHYSIQUE I N°7

surfaces

ill].

In this paper, we reconsider some

important

features of

crystal growth

in two dimensions. We attempt a further extension of Gates and Westcott's work [6,7]

by studying,

in d = I + I, a

single-

and

double-step

model defined on a 45°-rotated square lattice where

single

and double steps are allowed on the

moving

"surface" (~

).

The

study

is made easier

by mapping

the interface

profile

onto a 14-vertex model. Net

growth

or

steady

decrescence of the

crystal

is described

by

a

Kolmogorov

forward equation which we solved

exactly

for small

samples.

The present model is not

dynamically

reversible

(see

Refs. [6,

7]); however,

a

steady

state does exist and the

growth velocity

can be

computed exactly

for very small systems. The latter

helps

us to build a precise simulation

procedure

to

investigate larger

systems. Our results show that some

asymptotic

properties of the model can

already

be obtained on

relatively

small system sizes, e.g., N

= 60. We find indications in the model for a

rough-to-rough

transition [12] where the

growth

rate or

velocity

may be

size-independent.

Our model

depends

on a parameter n related to the

spatial coupling

between two next-nearest

neighbours.

We find

that,

for

increasing

n, the

growing

surface becomes smoother and we suspect that for n-cc a

negligibly

small

growth velocity

will result. The latter appears to be consistent with the decrease of the time- exponent

fl

[13] of the surface as a function of n. We

define,

at fixed

growth

parameters,

a

time-dependent

order parameter

ifi(t)

to report results about the step

density

fluctuations

on the

growing

surface. Such parameter has been often used in the

literature,

e-g- to

study

the

dynamics

of

step-doubling

transitions [14]. We find that its

amplitude I(t)

is consistent with the

analytic

form

proposed by Hoogers

and

King [lsj

in a

simple

model introduced to interpret experiments on reaction kinetics. This order parameter has values

indicating perfect layer growth

at low temperature and

large driving

force on

relatively large

systems, whereas at

high

temperature, the

decay

of its

amplitude

expresses a continuous mode where the

growing

surface exhibits a

hill-and-valley

structure. We

give

a

qualitative growth phase diagram

for

n = 3,

relying

on the Wilson-Frenkel [16] behaviour of the

growth

rate in the continuous mode.

We also

explore

the fundamental question of effective diffusion in

crystal growth theory

where

growth

occurs

by

atom

deposition

and

evaporation.

When an atom evaporates from a

site,

and

shortly afterwards,

in the next simulation step, another atom condenses in the

vicinity

of this site, this

coupled evaporation-deposition

process may be considered as an effective diffusion.

We show

by

a statistical

analysis

that it is

possible

to find a temperature domain where such effective diffusion follows an Arrhenius law when the

evaporation

rate is

properly

chosen.

In Section 2, we describe our stochastic model. Section 3

gives

its numerical solution

(exact

on small

samples

and

by

simulation on

larger systems).

Section 4 is devoted to results and discussion.

2. The

Microscopic

Model

The model is defined on a 45°-rotated square lattice formed

by

a stack of discs

(Fig. I).

We

assume that the

growing crystal

is well-structured and the

solid-on-solid'(SOS)

condition is

fulfilled.

Single

and double steps are allowed on the

surface;

therefore, the present model appears as an extension of the

single

step model studied

exactly by

Gates and Westcott

[6,7].

The essential feature of the model arises from the condition that the

height

difference between any two surface nearest

neighbour

atoms can be either I or 3 in unit of

a/2,

where a is the

lattice repeat distance. The numerical

analysis

of the

growth

kinetics of models

including higher

steps would be

expensive

in

computation

time. We find convenient to

replace

the stack of discs

by

its upper

edge profile

and we define the interface between the

crystal

and the fluid

phase

as the line

connecting

the centers of surface atoms of successive columns. Thus the

(~) For short, in the following the model will be simply named the double-step model.

(4)

N°7 14 VERTICES IN

(1+1)D

GROWTH 875

o~o

~

jojo~ ~o

o~o o~o~o o~o~o~o~o~o~

o~o~o~o~o~ o~o~o~o~o~o~

o~o~o~o~o~o o~o~o~o~o~o~o~

o~o~o~o~o~o~o~o~o~o~o~o~o~

Fig. I. Mapping of the surface of a two-dimensional crystal onto a 14-vertex model. Simple and double steps are present on the surface. The line connecting black discs represents the growing crystal edge profile which can be thought of

as a connection of

some 14-vertex lines.

(>2

9 >o

11

f~/ ~

7 5 4

Fig. 2. The fourteen vertices used to map the crystal edge profile in Figure I. Vertices with small numbers are those shown in the figure. Vertices with big numbers are found by reversing all

arrows. At each vertex, the ice rule holds [17]. The line representation of these vertices is obtained

by replacing arrows pointing to the south-west or north-west by lines while others are deleted. In this representation, vertices 3, 4, 5 and 6 coincide with their usual line representation in the 6-vertex

model

[iii.

lateral "area" of a double step does not

belong

to the interface but to the

crystal

This line is identified to a line with

cyclic boundary

conditions in a

special

14-vertex model

(Fig. 2).

Other non-used vertices of the same type are considered as

non-physical

in the model. This line

mapping

establishes a one-to-one

correspondence

between a

given

state of the system and

a 14-vertex

configuration.

If Ah denotes the absolute value of the

height

difference between two surface next-nearest

(NN) neighbours,

the energy ev of a

given

vertex v is defined as:

e~ =

ji/2)e~jih)n

11)

(5)

816 JOURNAL DE PHYSIQUE I N°7

where e has the dimension of an energy, ~ is a coefficient which introduces a difference between vertices

by depending

on the vertex

"length" (in

the line

representation)

as follows:

~ =

12)~/~l/2a.

12)

Vertices 3,

4,

5 and 6 which

belong

to the 6-vertex model

(two-dimensional

version of the ice

model) II?]

have ~

= l. Even if n

= I, the relation

(2)

does not favour double step formation at low temperature. In the

remaining

of the article, ~

depends

on unless otherwise

specified. Expression ii

describes the

spatial coupling

between NN

neighbours

whereas nearest

neighbours

interact with infinite energy. n

=

1/2

may

correspond

to the

standard/Gaussian

SOS model. The energy e is defined as positive and assumed not to

depend

on the temperature.

The relation

ii)

insures:

ES " e6 " e7 = e8 = 0

(3)

Hence,

the

completely

flat

surface, corrugated

on atomic scale with NN

neighbours lying

in the same

layer

has zero energy. The

ground

state of the system is twice

degenerated

with four

ground configurations,

since relation

ii) gives

to the "reconstructed" surface

(787878...)

and the non-reconstructed surface

(565656...)

the same energy.

However,

the surface

(787878...)

has

larger

interface width and may evolve at low temperature to the structure

(565656...).

The 14-vertex energy of a

configuration

a is

given by:

E

=

~j

N~e~

(4)

J

where N~ is the number of vertex of type

j

in the

configuration.

Possible

configurations

of a system of linear size N are

parted

into time-conserved classes characterized

by

S:

S=Ni+N3+2Nio+N12+2N13-(N2+N4+2Ng+Nii+2N14) (5)

related to the mean

slope

of the surface. A class will be named "active" if the

corresponding configurations

can

change according

to the

growth

rules

(see below), "passive"

otherwise.

The case S

= o

implies

that the two ends of the interface have

height

difference

equal

to

a/2

or

3a/2 (see Fig. I).

For N even, S E

[-2N,

-2N + 2,.., 2N 2,

2N],

whereas for N odd, S E

[-2N

+1,-2N + 3,..,2N

-1].

The

configuration

a and its mirror

image (with

respect to an horizontal

axis)

-a,

belong

to

opposite

classes. Pure

growth

on a

corresponds

to pure decrescence on -a, but both classes have the same

steady

state distribution

probability.

Accordingly,

the present

study

will be restricted to systems with linear size N > 3 and to

positive

and active

classes,

I.e, S E

lo,..

,

2N 2] for N even and S E

[1,..

,

2N 3] for N odd.

N =1 and N

= 2 correspond to trivial cases.

Classes in the model are associated to surfaces with well-defined Miller indices.

They

are

naturally

divided into subclasses whose

configurations

differ

only by translations;

e-g-, for N

= 2, class

lo),

we have ns

= 2

subclasses,

each

containing

two

configurations: (78, 87); (56, 65)

whereas for N

= 4, ns

= 11 and for N

= 8, ns = 567. For N

= 7, class

(I),

ns

= 187.

We find also

possible

to describe the interface

using

the

following procedure.

We label as in references

[6,7],

unit steps of the interface

by

az,

Ii

= 1, 2,

.,

N)

from the left to the

right

and set az

equal

to

1/3

if I is a

single /double

up step and az

equal

to

II

3 if I is a

single /double

down step.

Therefore,

the surface

configuration

of

Figure

I which is, in the 14-vertex formulation,

a =

(8, 7,14,

6,13, lo,..

,

II)

is

represented

as:

? "

(+3,

-3, -1, +1,

+3, +1,

-3, +1,..

(6)

N°7 14 VERTICES IN 11 +

1)D

GROWTH 877

C~~E

5 6 5

,», -~

Cl

E

~~

b)

~ ~ ~

c

I)

E 6 5 6

,; - c

I j

E

~)

~~

d)

~~~

Fig. 3. Example of two

depositionlevaporation

events on a flat surface

(a,c)

and their correspon- dence in the 14-vertex formulation

(b,d).

Vertex numbers correspond to those listed in Figure 2.

The allowed surface

configurations

are such that two consecutive values of a~

equal

to 3

or -3 are

forbidden; otherwise,

the model would become a

triple

step model and much more

N

complicated.

The

cyclic boundary

conditions

impose

aN+i

= ai. When

~j

az = o, we recover

z

our usual class

(o).

Dynamics

is introduced in the model

through deposition

and evaporation of atoms on the surface considered as Markov processes. Vertices

8/6, 1/3, 2/4, 13/lo, 14/9, 6/5, 3/12, 4/11

and

5/7

show the presence of

growthlevaporation

sites. Condensation

(C)

and

evaporation (E)

at these sites

modify

the interface line on three sites which define

growth

and evaporation kink

subconfigurations.

The different events

whereby

atoms

join

or leave the

crystal edge

are

expressed

in terms of transitions between these three-site kinks as follows:

X A Y

ci jE

V B M

where

A/B

denotes the

previously

enumerated vertices. At each

position X,

Y, V, M, several vertices may lie. In the present

model,

we get loo

growth

kinks

(X

A

Y)

and loo evaporation kinks

(V

B

M).

As

examples

of the

previous

transitions, we

give

in

Figure

3 two events

leading

to an adatom creation

levaporation

on an assumed

initially

flat surface

(5656...6).

If AE represents the

change

in the surface energy

during

these

transformations,

there exist, for ~ = l and n = I, z transitions with AE

= +2e, z transitions with AE

= -2e and 2z

transitions with AE

= o, where in this case, z = 25. In the

single

step

model,

the situation is rather

simple

with z

= I, since

only

vertices 3, 4, 5 and 6 are needed to describe the

moving

surface.

An

important ingredient

of any

microscopic growth

model is the definition of

dynamical

rules. We model the

exchange

between the

crystal

and the fluid

phase by

a non-conserved

Glauber-type

kinetics [18]. The transition rates are considered in the

following

forms where a bias is

applied

in favour of the

deposition:

~a

~

~~PIA~/kT)

j~j

I +

exp(AE/kT)

(7)

878 JOURNAL DE PHYSIQUE I N°7

for

deposition

and

j~a ~

j?)

I +

exp(AE/kT)

for

evaporation

of the kink of type

(a),

where a can take loo different

values;

T is the temper- ature, k the Boltzmann factor and

A~

the

driving

force. These rates

satisfy

for

A~

= o the

detailed balance condition:

caja-a')

E~l-a- a')

~~~

with respect to the 14-vertex energy at the temperature considered. When

A~

= o, the model describes

equilibrium

of

crystal

and

fluid,

whereas for

A~

> 0, net

growth

occurs.

If we denote

by q(a; a')

a transition out of a and

q(a)

=

~jq(a; a'),

it appears that the

~, relation

q(a)

=

q(-a)

relevant for the

dynamic reversibility

of the model in the sense defined

by

Whittle [19] does not hold for all a. Our results show that there may be no reasonable

general

condition for the model to be so. Such

dynamically

non-reversible model is not

easily

tractable

analytically. Therefore, finding

an

expression

for the

growth

rate

depending

on

growth

parameters at the

thermodynamic

limit is not trivial. The above does not however

imply

the non-existence of a

steady

state for the system. We check that any initial distribution

probability tends,

when t-cc, to a

steady

state distribution. The system is

normally

driven to statistical

stability

and this results from the stochastic nature of the transition rules. The

model shows that for ~

= l and n

= I, the property:

~j C~(AE#o)

=

~j C~(AE

=

o) (9)

holds.

This relation is also valid in the

single

step model and coincides with one of Gates and West- cott's conditions for the existence of a

steady

state distribution

probability

of the system [6,7].

When e = o, all surface

configurations

are

ground configurations

and we recover a random

deposition

model where

only

the restriction on Ah could limit the

crystal growth.

This case

obviously

is

equivalent,

when

e#o,

to the infinite temperature limit of the model.

3. Numerical Solutions of the Model

3.I. EXACT STEADY GROWTH RATE CALCULATIONS.

They

are

only possible

on very

small

samples

since the number of

configurations

and subclasses increases

rapidly

with system size.

In the

model,

the

probability

of

adding

or

removing

more than one disc in a small interval

time dt is set to zero. Let us assume e-g- pure

deposition.

If P~

it)

is the

probability

of a at

time t,

q(a; a')

the

probability

of a transition out of a,

g(t)

the unconditioned

expected

total number of discs at time t,

given

a, then [6]:

glt

+

dt)

=

glt)+

<

qla)

>t dt.

(lo)

The

expected growth

rate

G(t)

per surface site is:

Glt)

"

N~~(glt)

"

N~~

<

ql?)

>t

Ill)

(8)

N°7 14 VERTICES IN (1+1)D GROWTH 879

In the I4-vertex

model, G(t)

has the

expression:

G(t)

=

N~~ ~j C~p[Pm(t) (12)

where

p[

is the

multiplicity

of the kink of type

(a)

in the m~~ subclass Sm whose

weight

Pm

it)

is defined

by:

Pmlt)

=

~j P«lt). l13)

Pm

it)

is obtained

by solving

the

Kolmogorov

forward

equation:

d

(i~~

=

~

L~~,

ji~, T, e)p~, it) j14)

where Lmm, =

£~ C~(M(~, p[6mm>)

denotes the elements of the transition matrix L of surface

configuration

between subclasses

(M(~, being

the number of ways a

configuration

of

subclass m'

can

change

to a

configuration

of subclass m via processes

taking

place at a kink of type

(a)).

The

steady

state solutions are used to compute the

steady growth

rate on which

we will

mostly

focus in the

following.

3.2. MONTE CARLO SIMULATION The simulation avoids the difficult

problem

of subclass

classification. It is based on the

ergodicity

of the model within a class and makes the

study

of

relatively large

systems

possible

and even easy. The

roughness

of the

growing

surface in the presence of

deposition

and

evaporation

processes may be studied

using

the

following algorithm.

All active

subconfigurations

are

listed, together

with their

coordinates;

then the total evolution

probability

of the surface is

computed:

Qla)

=

£IC~P$

+

E~q$) lis)

a

Let r =

£~ C~p$ /Q(a)

denote the total condensation

probability.

At each simulation step,

r must be

compared

to a random number ro

uniformly

distributed over the interval

[o,I].

If r > ro, condensation is

tried;

otherwise, evaporation is chosen. The

attempted

move is

accepted

with

probability:

pmc " uJ

/Q(a) (16)

where uJ is

equal

to C~

/E~

for

condensationlevaporation

on the kink of type

(a).

Concerning

the

growth

kinetics, sites where in

principle

both

deposition

and

evaporation

events are

possible

are treated as pure

growth

sites. Such avoided evaporation sites are more

strongly

linked to their

neighbours

than those considered. We

study essentially

the kinetics under

deposition

and evaporation in this restricted but

physical

case. For this

study,

the above

algorithm

needs some modifications before

yielding

precise results. One active

subconfiguration

must be selected among those listed and its evolution

accepted according

to the Monte Carlo

weights

in

expression (16).

The mean

growth

rate per surface site of a

given

active class after K simulations steps is defined as:

K

G =

N~~t~~ ~j(2r 1) (17)

~=i

(9)

880 JOURNAL DE PHYSIQUE~I N°7

7000

6000

sooo

4000

S=12

3000 S=2

2000

N " 8

IOOO ~ ~/

/

~~= j o

S=O

~

0.5 1.5 2 2.5 3 3.5 4 4.5 5

Temperature (kT/E)

Fig. 4. Dependence of the exact growth rate of a system of linear size N

= 8 on the mean slope

6 of vicinal surfaces (see text) and temperature. The supersaturation is kept constant:

Ap/kT

= 10

and we use

~y = I and n =1.

where t is the total real simulation time defined

by:

t =

f I/Qla) l18)

The number K needed to reach the

steady

state increases with

increasing

system size and

decreasing

values of the

supersaturation.

4. Results and Discussions

4.I. CASE r

= I. The results

reported

in this section are obtained in

far-from-equilibrium

conditions where atom

desorption

from the surface is

neglected.

We are

mostly

interested in some

time-dependent

quantities which could characterize the

growing

surface

morphology (roughness,

step

density fluctuations)

and which are

experimentally

measurable

together

with the average

velocity

of the interface between the two

phases, commonly

called

growth

rate.

Steady

decrescence and

temperature-programmed multilayer desorption

could be studied

using

the same

procedure.

Surfaces with odd size are

necessarily sloped

surfaces and we do not consider them

explicitly

in our

study.

In

Figure

4, we

give

exact results

(by solving

the master

equation)

on the

dependence

of the

growth

rate for

initially

flat and

sloped

surfaces with linear size N

= 8 at constant

deposition

rate. The

growth

rate decreases with the macroscopic inclination b

(tan

b

=

SIN)

of vicinal surfaces at

high

temperature, a consequence of the decrease of the number of active sites with

increasing

b. At low temperature,

preexisting

steps on

sloped

surfaces induce

higher growth

rate than on a flat one. In this case, the

growth proceeds layer-by-layer

on vicinal surfaces

by

step

propagation

as in

spiral growth

[20]. This mode is

destroyed

at

high

temperature

by

(10)

N°7 14 VERTICES IN

(1+1)D

GROWTH 881

40

16

35 14 ~"8, C(CSS

(0)

12

30 lo

a

25 6

Rate 4

20 2

~

~

2 2.22.42.62.8 3 3.23.43.63.8

4~

~

*

lo , ~

*

~ N = 600

e '

~ ~$i-a,,~~

.

~ ~

~ ~ *

~

l 1.5 2 2.5 3 3.5 4 4.5 5

Disequilibrium Aq/kT

Fig. 5. The simulated growth rate m. supersaturation at different temperatures. The inset curve

compares simulation results

(open circles)

and exact calculations

(lines)

for a system of linear size

N = 8, class (0) at four temperatures: T

=

2.5e/k,

T

=

1.5e/k,

T

=

elk

and T

=

0.5e/k

from the top to the bottom. Calculations are performed for

~y = I and n

= 1.

nucleation events on terraces. Surfaces with no terraces

(S

= 14;

12)

may then show

essentially

lateral

growth

at constant

velocity.

The above results are consistent with those found

by Krug

and

Spohn

[12] from the behaviour of the

growth velocity

as a function of the local

gradient

T7h of the surface. For b small, the

following

relation

approximately

holds for a system of linear size N:

G(b, N)

=

G(b

= 0,

N)

+ ~tb~

(19)

It has been

suggested

[4] that the temperature where p vanishes and

changes sign

may

correspond

to a

rough-to-rough (RR)

transition temperature where a sudden

drop

of the

early-

time

scaling

exponent fl

(defined below)

of the surface is

expected.

In

microscopic growth

models, the effects of a

change

of

physical

parameters on the

growth velocity provides

the best

understanding

of the

growth

mechanisms of real materials.

Figure

5

(inset curve), displays

the dependence of the

growth

rate on

supersaturation

at different temperatures. Simulation results

perfectly

agree with exact calculations up to several

digits.

Such

precise

results are

expected

since the simulation

procedure

relies on the basic ideas of the kinetic Monte Carlo

method;

therefore it may

obviously provide

a

high-accuracy

solution of the master

equation (14).

The main

figure gives

simulation results for N

= 600, class

(o).

At low temperature and small

driving force,

the

growth

rate G

nearly

behaves as:

G

+~

bA~/kT (20)

where the coefficient b, which

plays

the role of

mobility (corresponding

to the kinetic coefficient for

A~/kT

-

o),

increases with

increasing

temperature and saturates around T +~

1.5e/k.

When

T-o,

other results indicate that b tends

continuously

to o without any

non-linear nucleation

behaviour,

in agreement with the zero

roughening

temperature of the one-dimensional substrate. With

increasing

temperature, the

growth

rate

rapidly

saturates and

(11)

882 JOURNAL DE PHYSIQUE I N°7

BOOO

7000

h'9h

T

11

6000

~'~~ ~ ~

0,12 ~

4000

o.oa 3000

~~~~ Q ~'~~ 5 lo 15 20 25 30

Q ~

AH/kT

~~~~

low T ~

o

Fig. 6. Dependence of the simulated growth rate on system size at low temperature

(T

=

0.5e/k)

and high temperature

(T

=

4e/k)

for

Ap/kT

= 10. The high-temperature growth rates are given in arbitrary units. Inset: behaviour of the coefficient K

m. the supersaturation at T

=

4e/k;

C

=

exp(Ap/kT).

Calculations were performed for

~y = I and n

= 1.

depends exponentially

on the

supersaturation

at

large A~, following

the Wilson-Frenkel [16]

law: G

+~

exp(A~/kT)

I. In order to get

plausible

estimates of the infinite-size

limits,

we

explore

finite-size effects in our calculations.

Figure

6

displays

the

dependence

of the

growth

rate on system size at low and

high

temperature under a constant and

large supersaturation

of the fluid

phase.

The results ensure that these effects are rather weak for N > 60 at any super-

saturation. One can describe the fast convergence of the

steady growth

rate to its

asymptotic

value

by

the

scaling

form [21]:

G(N)

=

G(cc)

+

KIN" (21)

where K and uJ depend on the

growth

parameters. For N > 60, the curves are

approximately

linear and uJ

+~ I as in the

single

step model [21]. For small sizes

and/or

low temperature,

important

deviations from the

scaling

relation

(21)

are obtained due to

higher

order terms in I

IN.

The linear

region

increases with the

supersaturation.

A careful

analysis

of the results

reveals that there is a critical temperature To at which K vanishes and

changes sign;

at

To,

the

growth

rate is almost

size-independent.

Such result indicates a possible RR transition

[4,6,12,21].

A best estimation of To should be obtained at

large deposition

rate. In the inset of the

figure,

we show the isothermal behaviour of the coefficient K with the supersaturation;

it emerges that Ii is an

increasing

function of the

deposition

rate and no RR transition is

expected.

We

therefore,

argue that in the

(A~/T,T) plan,

the RR transition line may be

nearly straight

and normal to the T-axis.

Another

interesting

result concerns the difference in

growth speed

between the

single

step and the double step models that we

display

in

Figure

7. At low

deposition

rate and

high

temperature, the

growth

rates are

practically

the same, a consequence of a

nearly

identical behaviour of all surface active

subconfigurations. Hence,

the

single

and double step models have the same

asymptotic growth

rate per active site: the

corresponding

formula is

given by

the relation

(3.18)

of reference [7]. At low temperature, most convex active

subconfigurations,

(12)

N°7 14 VERTICES IN

(1+1)D

GROWTH 883

i~oo N =64

n=1

1200

iooo

4.5

800 4

* 3.5

* 3

600

~

2.5 2

400 1.5

o.5

200 °

O.5 1.5 2 2.5 3

tem~erat/re (k)le)

~ ~

Fig. 7. Comparison between simulation growth rates per active site for the single

(lines)

and double

(stars

or

circles)

step models for a system of linear size N = 64, class (0) at large supersaturation

Ap/kT

= 20

(main figure)

and low supersaturation

A~/kT

= 3.5

(inset curves).

absent in the

single

step

model,

are less active than the concave ones since their evolution is not

energetically favoured; accordingly,

most of them are

rejected during

the simulations. Such

situation

obviously

leads to

slightly

lower

growth

rate per active site than in the

single

step model. The double step nature appears at

large deposition

rate and

high

temperature. There, the double or

triple probability

of some sites to increase

successively

their

heights,

influences the

growth speed

which becomes

larger.

We have

checked, using

the relation

(21)

and the

asymptotic growth

rate of Gates [7], that the latter feature remains valid in the

thermodynamic

limit. It exists a well defined temperature

(main figure)

at which the two models are

strictly

identical

kinetically.

This temperature

slowly

increases with the

deposition

rate.

Below,

the

growing

surface in the

single

step model appears

rougher

than in the double step model since a

lower

growth

rate

corresponds

to less

potential

kink sites on the surface. The situation remained

unchanged

for

increasing

n as shown in

Figure

8. Our results reveal that for any n, there is a temperature domain where almost no

growth

occurs at small

driving

force. We found that the width of this

region

increases with n whereas it decreases for

increasing A~.

The latter feature has been also observed in d

= 2 +1 [4] where a real metastable state exists. A

sloped

surface in this

region

may however grow fast and

continuously

whereas an

initially rough

surface will

show

extremely

slow

growth

once become

completely

flat. In d

= 2 +1 or

higher dimensions,

fractal or dendritic

growth

may occur if the nucleation barrier is

artificially

overcome. The trivial random

deposition

model

corresponds

to e

= o. There is no correlation between surface sites and

particles

are launched at

randomly

selected positions above the

deposit.

The

figure

shows that at low temperature, this model

yields

very

rough

surfaces.

The

growth

rate at constant

driving

force

A~

and

varying

temperature shows the Wilson- Frenkel [16] behaviour above a well defined temperature. The latter is often considered in

a crude

approximation

as a transition point from the

layer growth

to the continuous one.

Although

this criterion is

questionable,

we use it to

display

a

qualitative growth phase diagram

(13)

884 JOURNAL DE PHYSIQUE I N°7

o.6

~~ random

deposition

A/£/c=0.5

O.4 sing

~~~ ~

n =

O.3

O.2

n=

oi

~

0 0.5 1.5 2 2.5 3

temperature (kTle)

Fig. 8. Comparison between simulation results on the growth rate defined per active site for different models. The random deposition model is obtained by taking e = 0.

a

7

6

(~ continuous

~

~4

~

N=64 2

n=3

layer-by- layer

o

~ ~ ~ ~ ~ ~~

temperature (kTle)

Fig. 9. Growth phase diagram of a system of linear size N

= 64, class (0) obtained by taking as

transition point to the continuous mode, the temperature which gives the maximum growth rate at fixed driving force.

in

Figure

9.

Sufficiently

below the transition

line, layer growth

occurs

by

birth,

spread

and coalescence of lD islands or

by

the one-cluster mode. Well

above,

the

crystal

grows

continuously

without any nucleation barrier. As discussed in reference [4], the one-cluster mode is

expected

to

disappear

with

increasing

temperature,

driving

force or system size. The one-cluster mode

prevails

when the time between two consecutive nucleation events

(adatoms

formation on the

terrace)

is

larger

than one

monolayer completion

time t

by

extension from the first nucleus [22].

(14)

N°7 14 VERTICES IN

(1+1)D

GROWTH 885

A

simple

calculation

using

~

= l and the relations

(1), (6), (17)

and

(18),

shows that at low temperature

(double

steps are not

relevant)

and

relatively large driving force,

the

growth

rate per site behaves as

N~~t~~,

I-e-:

~ '~

N(N ~l~~i(~e/kT))'

~~~~

One can

easily

check that G is

approximately proportional

to the nucleation rate, I-e-, to the rate of fixation of new adatoms on a flat surface:

exp(A~/kT)/(I

+

exp(2"e/kT)).

Such

proportionality however,

to our

knowledge,

has never been proven

experimentally,

except in

electrocrystallization

[23]. This mode

usually

exhibits

undamped

oscillations of the interface width W with

growth

time.

To get more

insight

into the

growth

modes and

roughness

of the

moving

surface, we define

an order parameter

ifi(t)

to monitor step

density

fluctuations on the

growing

surface:

ifi(t)

=

~J ~~P(llrh~ (t))

~

(2~)

where h~

(t)

is a

single-valued

function which denotes the surface

height

at substrate coordinate

j.

A similar order parameter has been considered in the literature to map the

dynamics

of

step-doubling

transitions [14]. Let us denote

by ((t)

the

quantity

I

(ifi(~(t),

and

by I(t)

the

amplitude

of (ifi(~(t). From an assumed initial

heights configuration (I,o,

I,

o,..,o)

of the

surface,

one finds

(~l(~(t)

= o. To avoid such

situation,

we consider that all the flat surface

sites have the same initial

height.

This

assumption

does not, of course, affect the

physics

of

our results. The behaviour of

((t)

is

displayed

in

Figure

lo for different temperatures. When

I(t)

= I, lateral

growth prevails

and the surface evolves while

remaining

flat

(pure

one-cluster mode on

average)

and this

happens

in the

figure

for T

=

o.3e/k.

A

layer

is finished to be formed before a new one is started on it. The

probability

that a second nucleation occurs in the

growing layer

or above the

growing

island is of the same order as

A(t)

= I

I(t).

When

I(t)

is

just

constant after one or two

periods

of oscillation of

((t),

the

growth

is

locally perfect

and takes

place

in a very few

layers.

A constant increase of

A(t)

may indicate a

precontinuous

mode where the

growth

is neither

completely

continuous nor

layer-by-layer.

At very

high

temperature, no oscillation is observed for

((t)

and the

growth

mode is continuous, even in the

early-stage

of the

growth.

The

amplitude

of

A(t)

is well fitted

by

the functional form [15]:

x(t)

=

x(~x~) 1 j

~~ ~~

(24)

where

X(cc)

= 0.90 and to is fitted to 8 MCS at T

=

e/k.

In our calculations, to is approxi-

mately

the time for

((t)

to reach the value

o.5,

which seems not to have a

particular physical meaning. Although

the oscillation

periods approximately

coincide in Monte Carlo time at all temperatures iii the

layer

or

quasi-layer mode, they strongly

differ in real time which of course

depends

on

physical

parameters. We also

analyze

the influence of n on

((t)

at fixed temper-

ature. We find for

n = 1, 2,3 a fast

damping

of the oscillations. However, it turns out that

increasing

n makes the surface smoother; which results are consistent with those

reported

in

Figures

8 and 9. A further

investigation

of the surface

morphology

is

performed by studying

the behaviour of the interface width

Wit)

defined

by:

W~(t)

=

ii IN) £(h~ it) ii IN) £ h~(t))~ (25)

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