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Decay of Grooves Cut in a Surface with Singular Orientation when the Neighbouring Orientations are

Unstable

Christophe Duport, Anna Chame, W. Mullins, Jacques Villain

To cite this version:

Christophe Duport, Anna Chame, W. Mullins, Jacques Villain. Decay of Grooves Cut in a Surface

with Singular Orientation when the Neighbouring Orientations are Unstable. Journal de Physique I,

EDP Sciences, 1996, 6 (8), pp.1095-1125. �10.1051/jp1:1996118�. �jpa-00247233�

(2)

Decay of Grooves Cut in

a

Surface with Singular Orientation when the Neighbouring Orientations

are

Unstable

Christophe Duport (~*),

Anna Chame

(~,**)

,

W-W- Mullins

(~)

and

Jacques Villain (~)

(~) CEA,

Département

de Recherche Fondamentale sur la Matière

Condensée,

SPSMS, 38054 Grenoble Cedex 9, France

(~)

Carnegie-Mellon University, Department

of Materials Science and

Engineering, Pittsburgh,

PA 15213, USA

(Received

19

February

1996,

accepted

10

April 1996)

PACS.68.35.Ja Surface and interface

dynamics

and vibrations

PACS.05.40.+j Fluctuation

phenomena,

random processes, and Brownian motion PACS.68.35.Bs Surface structure and

topography

Abstract. The

decay

of a

grooved profile

when trie average orientation is

singular

is treated in the

particular

case when the orientations close to the

singular

one are unstable. The system is assumed to

exchange

atoms with its vapour. The step fluctuations, which allow the

profile decay,

are treated

by

a

partially

exact transfer matrix method. The time T to

peel

the topmost

layer

is obtained

as a function of the width 1of a terrace: f c~

iexp(~i),

where the constant ~

depends

on the temperature.

Il. Introduction

~rhe

smoothing

of grooves

artific1ally

made in a

crystal

surface is a classical

problem (Blakely il ],

130nzel [2] and Preuss

[3])

solved

by

Mullins [4] in the case of a

non-singular

orientation. If the final

(or average)

orientation of the surface is

singular,

the non-linear

problem

which arises is

ontrovers1al.

Indeed,

it is not clear whether the facets which

temporarily

anse in

experiments

<ire a result of a miscut as claimed

by Lançon

and Villain

[Si,

or intrinsic

properties

as claimed

1)y

Spohn

[6] and

Hager

et ai. [7]. The

problem

is somewhat

simpler

if the orientations close la the

singular

one are

unstable,

because in that case the

topmost layer

is

peeled

without

perturbing

too much the lower ones. The

present

work is an

investigation

of this situation.

At

equihbrium,

the

parts

with

singular

orientations form facets with

sharp edges.

It is

i easonable to assume that the

top

and the bottom

parts

of the

decaying profile

also have facets with

sharp edges (Fig. l). Indeed,

the

sloping parts

of the surface are formed of

steps

which

interact

through

an attractive interaction

(in

contrast with the usual case discussed

by

Bonzel

<md Preuss [2] and then

by

Rettori and Villain [8] and then

by others).

The

exchange

of matter

(atom

per

atom)

may be either

by

diffusion on the

surface,

inside the solid or

by exchange

with the vapour [4]. The last process, called SALK

(surface

attachment

limited

kinetics),

is much

simpler

than the other ones. We shall restrict our attention io this

(*)

Author for

correspondence le-mail: [email protected])

(**)

Permanent address: Universidade Federal Fluminense, Instituto de Fisica, 24210-340, Niterôi RJ, Brazil

Q

Les

Éditions

de

Physique

1996

(3)

- 1+

Fig.

1. Initial state of the profile.

Fig.

2. A

typical

structure with

meandering

topmost step. The lower

layers

are not disturbed.

case. This process is

supposed

to

apply

not

only

to true

evaporation/condensation

of a

crystal

in contact with a vapour

phase,

but also in the case of surface diffusion on the

crystal

surface

(no exchange

with

vapour)

when

exchange

of the mobile species

je.

g.

adatoms)

with sources and sinks

je-g-

kinks and

steps)

is so dilficult as to be rate

limiting.

Then the mobile species may be considered to have an uniform chemical

potential

~1 as if it were a vapour

bathing

the surface. The

exchange

of matter between this mobile

layer

and the sources or sinks is assumed

proportional

to the difference between

~land

the local chemical

potent1al

~1+ ô~l determined

by

surface energy

changes resulting

from surface

displacements.

It is not clear whether this

limiting

case

actually

exists, but it has been used

extensively

as a basis for model

calculations [9].

In a realistic model of the

profile

considered

here,

the two topmost steps should be assumed to fluctuate between their lowest energy

positions.

The other steps

might

be assumed to be

straight. However,

this

simplified

model is

fairly complicated,

and we will

study

a

yet simpler

model with a

single fluctuating step (Fig. 2).

The system will be assumed to

exchange

atoms with its vapour, so that it is sulficient to consider a

single ridge.

In Sections 2 and

3,

the relaxation mechanism is

analyzed

and the

problem

is reduced to the

equilibrium

statistical mechanics of a

single fluctuating

fine attracted

by

a fixed fine. This

problem

is a dassical one and its

thermodynamical properties

will be recalled in Section 4. Its

dynamical behaviour, however,

requires a

special analysis

which is given in Section

5,

where the relaxation time is estimated. In Section 6 the

principal

results are

presented.

A

dictionary

(4)

ai

t=t

b)

~_~

2

Cl t=~£

1?ig. 3. Successive states of the

peehng

of trie topmost

layer: ai

at time ii a

junction

with the immobile step occurs and the two steps

loops

created

begin

to recoil

(trie

topmost

layer begin

to

<~vaporate), b)

at time t2 another

junction

occurs and

ci finally

at T two opposite

recoiling loops

merge

~nd the

layer

is

peeled.

>Jf the notations used is at the end of the text. The most

complicated part

of the

algebra

is

,zontained in the

appendices.

In

Appendix

A and B some

equilibrium properties

are evaluated

asing

the transfer matrix method and in

Appendix C,

the

dynamic problem

is treated using

an alternative

approach:

a Fokker-Planck

equation

is derived and solved

approximately,

and the

typical

times involved are estimated.

2. Characteristic Time and

Length

If the

topmost

step is in its

ground

state

(or nearly soi

at time t

= 0 and

begins

to

fluctuate,

one has to wait a

typical

time fi until it makes

junctions

with the immobile

step (Fig. 3a).

After a

junction

has taken

place,

both ends of the

topmost

terrace

evaporate

and recoil at the

velocity

~, which is

only

a function of the terrace width

1,

and of the fine tension

WI la

of the

step.

If one considers one of the

recoiling

step

loops,

it will merge

(Fig. 3c)

after a time f with another

loop recoiling

at the

opposite velocity,

which has been created at time t2

(Fig. 3b).

Let

Li

be the distance between the

points

where the

junctions

at times fi and t2 have taken

place.

Let pi be the

probability

per unit

length

and time to have a

junction.

The time

fi

(5)

is the time one has to wait before

observing

a

junction

in a

length

of order

Li Therefore, piLiti

Ci 1. But

(assuming

t2 >

fil

the time t2 fi is also the time one has to watt before

observing

a

junction

in a

length

of order

Li

Therefore pi

Li(t2 fi)

1. Thus:

fi t2 Ci t2 fi

j (2.1)

Pi 1 The

quantity (f fi)

is

comprised

between

Li/~ (if

t2

=

f)

and

Li/(2~) (if

t2

=

fi).

Therefore

f fi

~~ (2.2)

~

The left hand side f fi of this

equation

is of course

larger

than t2 fi, but cannot be much

larger; otherwise,

this would

imply

that the

probability

of a

junction

in a

length Li during

a time much

larger

than t2 fi is

negligible,

and this would be in contradiction with the definition of pi

Therefore,

f fi t2 ti

Comparison

with

(2.1)

and

(2.2) yields

Li

fi

(2.3)

Now, (2.2)

reads f cf fi +

Li /~

or

inserting (2.3) jnd (2.1):

f Qf

~~

Qf

(~ ~)

~

~Î~Î

Then,

it is clear that

1Ci

(2 5)

fi

Thus,

the time f necessary to

peel

the

topmost layer

will be known if we are able to calculate

~ and pi The

velocity

~ is

proportional

to the difference between the

evaporation

rate a of the curved

step

and the

evaporation

rate où of the

straight step.

This difference is itself

proportional

to the local excess ô~l of the chemical

potential.

The

precise

formulae are

~ =

a(a où)

=

aaoflô~l (2.6)

where a is the interatomic distance and

fl

is

1/(kBT).

The excess chemical

potential

is the

excess free energy per

partiale.

Since a

loop

of width 1and

length

~dt has an energy

Wi~dt la

and contains

i~dtla~ particles,

it follows

ô~l= Wia Ii

and

(2.6)

reads

~ oe

a~aofl ~ (2 7)

3. The Junction

Probability

pi

Ii)

The

junction probability

can be evaluated

ignoring

the

non-fluctuating step.

In

reality

when the

fluctuating

fine touches the immobile one, the process becomes irreversible and the two

separated

parts of the topmost

layer begin

to recoil. In our calculation we will

simply

obtain

an estimate of the

typical

time after which the

fluctuating

fine touches the other for the first time.

Consider a

part

of

length

L of the

fluctuating step.

At time t

=

0,

it is

supposed

to be

straight

at

position xiv, 0)

= 0 for any value of y. At time

t,

the maximum value

h(t)

of

xiv, fi

will be called the

elongation.

We want to know the

typicaltime Tilt, L)

after which

(6)

1

- ~

a) L

(h -'- y

~)

---

---'

L

x

~y -~-~---~~à-~-

i~

- -W

c) L

1?ig. 4.

Typical

excursion

(of elongation h)

of the top of the

profile

on a

length

L

ai explicitly iepresenting

the lower steps and the non

fluctuating

step and

b) ignoring

them. A excursion with

elongation larger

thon1, the size of the terrace, is shown in

ci.

For this

configuration

we can define

lhe distance Y

along

which all the points have a position x >1.

h(t)

reaches the value1for the first time

(Fig. 4a).

This time should

satisfy

pijtiL~ijt,Li

~ i

j3.ii

Insertion of this

equation

into

(2.5) gives

us

y ~

@13.21

The immobile

step

has no

part

in the calculation of

Ti

Therefore,

it can be

ignored.

We

now consider a

single

step

(Fig. 4b).

(7)

Rather than

calculating Tilt, L),

it may be easier to calculate the

typical

time To

Ii) during

which the

elongation

h remains

larger

than 1 if it is

larger

than 1 at a given time. It tutus out that both

quantities

are related

by

a

simple

relation which uses an

equilibrium property, namely

the

probability p)(L,1)

that the

elongation

at a

particular

time is

larger

than a

particular

value1

mjch larger

than the. thermal average

elongation. Indeed,

the

periods

in which the

elongation~is larger

than 1have a

typical

duration To

Ii)

and are

separated by

a time interval of order

Tilt, L).

Therefore

PllL'i)

~

~)j~j~ 13'3)

1 ,

The

quantity p) IL,1)

is not easy to calculate

exactly.

In order to use

lin

an

approximate

way)

the exact data which are

available,

we introduce the

equilibrium probability pj(L,

Y,

h)

that,

on a fine of given

length L,

a number

Yla (and

no

more)

of

points

have a

position

x > h.

Obviously

p)(L,1)

=

~j pj(L,Y,1) (3.4)

Y>o

On the other

hand,

consider a number

ôÎ

of

replicas

of the system

(1.e.

a fine of

length L)

taken from the canonical ensemble with the canonical

probability.

The number of

points

of a

given

ordinate y which have a

position

z > h is

ôlp)(h),

where

PI (h)

=

~j p(z) (3.5)

~>h

is the

equilibrium probability

that for a

given

y,

x(y)

> h. The

probability p(h)

is known

exactly

as recalled in the next section. The total number of

points

of the fine which have a

position

x > h is obtained

by multiplying

the number of points of a

given

ordinate y which have a

position

x > h

by

the number L

la,

and therefore it is

equal

to

(Lla)ôlp((h).

On the

other

hand,

the number of points of a given ordinate y which have a

position

x > h can also be written as

N

£

~'

pj (L, Y, h) (3.6)

y~o a

Equating

this to

IL la)ôlp) (hi,

one obtains

£ Ypj(L, Y, hi

=

Lp) (3.7)

Y>o

This formula may be

exploited

in an

approximate

way if Y is

replaced by

its average value

1:

P £ pj(L, Y, hi

=

Lp) (3.8)

Y>o Insertion into

(3.4)

now

yields

p)(L, hi

=

~~~~~~

(3 9)

Y

Now, using (3.2), (3.3)

and

(3.9)

we obtain the basic formula for the

peehng

time:

T ~

fiÎ 13.i°)

where ~ is

given by (2.7)

as

pointed

out before and

p) ii)

is

exactly

known. Its value will be

recalled in Section 4.

Before

estimating

Y and To

Ii)

we define more

precisely

our model and recall some well-known

equilibrium properties.

(8)

4.

Equilibrium Properties

of a

Fluctuating Step

In the

previous sections,

the

problem

has been reduced to the statistical mechanics of a fine which can fluctuate around a fixed fine which attracts it. As will be seen, an

"unbinding"

transition can occur for this

system:

the two fines cari be bound

(localized solution)

if the tem-

perature

is

sulficiently

low or, for a fixed temperature, if the attractive

potential

is

sulficiently strong.

The

firit

exact

theory

of

binding

of two watts in d

= 2 was done

by

Abraham

[loi iising

the transfer matrix method. Chui and Weeks [11] treated the same

problem

under a

solid-on-solid condition. A different

derivation,

with an extension to d

= 3 was

proposed by

Vallade and

Lajzerowicz [12].

The

problem

treated in

Appendix

A is the

study

of the fluctuations of a

step

which has a

stiffness

+~

(defined by (5.1) below)

and is bound

by

an attractive

potential -Wo

to a

straight

fine.

We will assume

throughout

the paper that the distance between kinks

along

the

step,

which is

of the order of +~a~

/kBT,

is

large

with

respect

to a, that is to say +~a »

kBT.

This

assumption

,ùlows one to use

equation (A.3c),

that

is,

to consider

only

transitions of one

step

away or

loward the

binding

fine.

In

Appendix A, by using

the transfer matrix

method,

it is shown that the

density

of

proba- lJility p(x)

to find a

point

of the step at a distance x of the borderline is, for x

# 0,

Plx)

=

iaoi~exPl-21~x) 14.1)

where ~ is a real number.

Since the

integral

of the

probability

is

unity,

the constant in

(4.1)

is

ao[~

oe 2~

(4.2)

The

probability

to find a

point

of the

step

at a distance

larger

than x of the borderline is

jjiven by integrating (4.1):

p)(x)

ce

exp(-2~x) (4.3)

The width of the

topmost layer

is assumed to be

large

with

respect

to the size of the thermal fluctuations which is of the order

of1/~,

then i~ » 1.

Moreover,

the continuum limit

implies

that ~a < 1.

Thus,

the relative order of the

length

scales is 1»

1/~

» a

It

might

be

argued

that the

assumption

~a < 1 is very

spec1al,

since it will be valid

only

on a very small range of

temperatures.

This

assumption imphes

that a fluctuation of

large elongation

would be

relatively

easy. If a

large

value of

Wo (say Wi/2)

is

chosen,

which would be

physically reasonable,

it could make ~a

comparable

to

unity

and would restrict allowed

fluctuations to a few times a.

However, experimentally,

for various reasons

je-

g.

feasibility),

we are interested

by

macro- or at least

mesoscopié profiles.

The

profile

width 1 then must be much

larger

than a.

Therefore,

the

product

~a should be

small,

otherwise the

product

~i will be

huge

and the relaxation time too

(as

will be seen

later).

On the other

hand,

since ~

changes rapidly

with

T,

the

temperature

range where ~i is small is very narrow. In this way the

assumption

1 »

1/~

» a is

really physical.

In this

connection,

in

Figure

5 a

plot

of ~ versus

Wo

is

presented (obtained by solving Eq.

(A.25) ),

in which ~ goes to zero as

Wo approaches

the

limiting

value

given by equation (A.26b) (as

an

equality).

Since

1/~

is the order of the average

elongation,

this

plot gives

the reader a

feel for the

dilficulty

of a

fluctuating step

to cross the top terrace.

The transfer matrix method demonstrates the existence of a transition at a certain tempera- ture

Tc

at which the constant ~ vanishes. Above this

temperature,

the

step prefers

to increase

(9)

,

/

' /

/

/

,

0.8 /

/

' ,

/ /

/

~'~ Î /

/

~Î t'

~ / ~~Î

~~

0.4 ' / ~~ ~'~

/

/

fiw =1.5

i

/

fiwi =20

°'~

' /

fiw

=2.5

,

/

fiw = 3.0

0

0 0.2 0A 0.6 0.8

)W

Fig.

5.

~ as function of

Wo,

the

binding potential.

The order of the average

elongation

of an excursion is

1/~.

The solid

curve

(flwi

=

o-à)

may be unreliable because

exp(-flwi)

would be too

big.

its

entropy

rather than its

potential

energy, and thus is not bound to the terrace

edge.

This transition is called

unbinding

transition or

delocalisation

transition. When T >

Tc,

there are

no forbidden orientations

in the

vicinity

of the average surface

orientation,

and this is the case discussed in references [5] to

[8].

In the present

work,

the condition T <

Tc

is assumed. Then

in the continuum

hmit,

which

corresponds

to ~a <

1,

we obtain the relations

(see

in

Appendix A, Eqs. (A.23)

and

(A.25),

which define ~, and

Eq. (A.46))

Wo

<

kBT (4.4a)

~~~~'~~~

~

ÎÎ~Î~ ~~'~~~

The transition

temperature

is

given by

the condition ~

= 0 and therefore

kBTc

"

@~ (4.4c)

5. Estimate of

1

Dur next task is to calculate Y and To. In this section an estimate for

1

is obtained

using

a

simple

and intuitive

argument

and in

Appendix

B it is evaluated

through

a detailed calculation.

The evaluation ofTo will also be

performed

in two ways: in Section 6

through

a

simple argument

and in

Appendix

C.

A

simple

way to estimate Y is

through

the

evaluation,

for two

limiting

cases, of the average

quadratic

difference

(ôx~ )y

between the horizontal

positions

of two

points

of the hne

separated

by

a distance y.

(10)

If y <

1,

then

(ôx~)y

must be

approximately

the same as in the absence of an attractive

potential, namely

jôx2j~

=

j jà.ii

On the other

hand,

if y

»1,

the attractive

potential

must be

considered,

and

(ôx~)y

=

/ ~ Î~ lx x')~pja;nt(y;

x,

x')dxdx' (5.2)

where pja;nt

(vi

x,

x')

is the

joint probability

that

x(0)

= x and

xiv)

=

x'

simultaneously.

It can

lJe written as the sum of an uncorrelated

probability

and a

correction, namely

Pjo>nul, X>

X')

"

AIX)piX')

+

ôpi§,

X,

X') 15.31

]Ify »

1,

the correlation term is

negligible

and

m m

~~~~~~

Î

~~

~'~~PixiPix')dxdx~ j~,~~

which can be written as

(ôx~)y

= 2

/~ x~p(x)dx

2

/~ p(x)dx)

~

(5.5)

o o

Using (4.1)

and

(4.2),

this

yields

~~~~~~

12

~~'~~

V

can then be defined as the crossover value between the behaviours

(5.1)

and

(5.6),

so that

Y

=

~( (5.7)

2~

A more elaborated evaluation

of1

is done in detail in

Appendix

B and the final result is ,£most the same as the

previous

one:

~ Y

=

0.45~) (5.8)

The above result is consistent with the

assumption1

»

$

in the hmit

~a <

1,

that is to iay, this result is vahd when

1

is much

greater

than the vertical distance between

kinks,

and

this occurs for

large

values of the

elongation.

Since1

is defined

as

(see Eq. (3.9)

for

instance)

the average

length along

which the

points

of the fine have

positions

x > h for an excursion with

elongation larger

than h

(where

h is much

larger

than the thermal average

elongation),

the fact that

1

does not

depend

on h is

surprising.

In

general1

would

depend

on

h,

however the result

(5.8)

shows that

1

does not

depend

on h if the

elongation

is

sulficiently large.

6. The

Typical

Time TO

The last unknown

quantity

is TO

Ii).

A

simple

way to estimate this

quantity

is to consider the recoil of an

exceptional

excursion of

amplitude

h.

(11)

Let a be the

evaporation probability

from the

fluctuating

curve per site and per

second,

and let

rp

be the

adsorption probability

from the vapour when this vapour has a

density

P " Po

exp(fl~l) (6.1)

The

quantity ~lis

the vapour chemical

potential

counted from an

appropriate

origin. At

equilibrium, adsorption

and emission

mutually compensate

and

a =

rpo expjp~) j6.2)

In

reality,

an excursion of

large amplitude

h is not at

equilibrium

with the vapour which has

a fixed

density

po, so that the

adsorption

rate per site has a fixed value

"

rpo (6.3)

On the

contrary,

the emission rate per site has a value

given by (6.2)

as a function of the chemical

potential ~1(h)

that the vapour would have if it were in

equilibrium

with the excursion of

amplitude

h:

a =

exp(fl~l) (6.4)

This value will be assumed to be uniform on the whole excursion.

In this way, the

velocity

of recoil of the excursion is

given by

(

"

°o(1

eXP

lfl~))a (6.5)

Assuming

that

fl~l

<

1,

one can write ôh

1 °°~~~

~~'~~

The chemical

potent1al

~1 can be written as

(+~a~)/R,

where R is the radius of curvature of

the excursion. The

quantity

which appear in this

expression

for ~1 is the hne stiffness

+~ rather than the fine tension

Wi la

as in

(2.7)

because this

expression

for

~1 is valid for weak

slope

fluctuations while

(2.7)

is related to a macroscopic

loop.

To estimate R we recall a result from

Appendix A,

where the

typical

extension of a fluctuation of

elongation

h is obtained. One finds that

~~~~ àÎ~ ~~'~~

Assuming

the excursion is an arc of ciEcle or

parabola

of base

length

and

amplitude h,

one finds R

=

(fl~+~~h) /~~ multiplied by

a constant of order

unity.

Insertion into

(6.6) yields

ôh

ao~~a~

j 16p~h (6.8)

The fact that h > 1 at t

= 0

imphes

that the

typical elongation [

that exceeds 1lies between 1 and 1+

) Therefore,

the

typical

time To necessary for

[

to become smaller than is

1/(~ () ).

Replacing () by

its expression

(6.8),

one obtains that

T0(h)

t

~j~

~

j6_gj

ao~ a

(12)

7. Results

In this

section,

the

assumptions

and the

principal

results of the

preceding

sections are

recalled,

in order to obtain a final

expression

for the time f to

peel

the

topmost layer.

We assumed that the

step

which fluctuates is bound to the

hmiting

borderline of the

topmost layer,

that is to say, the

step

is below the

unbinding

transition: the wavevector of the bound

state is ~.

The

topmost layer

is éissumed to be

large

with

respect

to the size of the thermal fluctuations which is of the order

of1/~,

then i~ » 1.

Moreover,

the continuum limit

implies

that ~a < 1.

In this way the relative order of the

length

scales is1»

1/~

» a.

Finally,

we have

supposed

that the

typical length

between kinks

along

a

step,

fl+~a~, is

larger

than the interatomic distance a and that we are near the

unbinding

transition in order that

the

large

excursions are not too

exceptional.

In this way +~a »

kBT

»

Wo.

The

quantity

we want to calculate is the

peeling

time of the

topmost layer,

which is

given by (3.10).

It is sulficient to insert into that formula the

expressions (2.7), (4.3), (5.7)

and

(6.9)

to obtain the final result

~ ~

210a2

fi~~~~'~~~

~~'~~

where ~ is defined

by (4.4b).

All these results refer to the case when the

topmost

terrace is limited

by

a

fluctuating

step and a

rigid

one. If it is limited

by

two

fluctuating

steps, a formula

analogous

to

(3.10)

should

apply, namely

" ~

i~ ~~~~

where

p)o(h)

is the

probability that,

for a

given

y, the distance between both

topmost steps

is

greater

than h. This

probability

is

given by integrating

the

probability pro(h)dh that,

for a

given

y, the distance between both

topmost steps

is between h and h + dh. Now

Poolhl

"

/ Plh qlPlqldq (7.3j

or

using (4.1)

and

(4.2):

pro(h)

=

4~~hexp(-2~h) (7A)

Integration

now

yields

m cc

p(o(1)

=

pro(h)dh

=

4~~

h

exp(-2~h)dh

=

(2~i

+

1) exp(-2~i) (7.5)

Equations (2.7), (5.7)

and

(6.9),

which

respectively yield

~,

i

and To, are still

expected

to hold.

Inserting

these relations and

(7.5)

into

(7.2),

one obtains the

peeling

time of a

layer

in the case of two

fluctuating steps

as

y~ r-

2~t3aoa2 fiexpj~ti) ah 17.6)

(13)

Acknowledgments

This work was initiated in Jülich

(Germany).

W-W- Mullins

acknowledges

the

hospitality

of the Institute für Grenzflàchen und

Vakuumphysik

and

support

from the von Humboldt

Sitftung,

and J. Villain the

hospitality

of the

Hochleistungrechenzentrum.

A. Chame

acknowledges

a

grant

from the Brazilian National Council for the Scientific and

Technologica1Development (CNPq)

and the

hospitality

of the Centre d'Etudes Nucléaires de Grenoble. We thank Prof.

Lajzerowicz

for fruitful discussions.

Appreciation

is

expressed

to

Xing

Chu for

preparation

of

Figure

5.

Notation

Dictionary

. a: interatomic distance.

. kB~ Boltzmann constant.

. i: terrace width.

. L:

length

of an

arbitrary part

of the

system.

.

Lit

distance between the

points

where the

junctions

at times fi and t2 have taken

place.

.

L(A):

number of

adsorption

sites.

. N: number of lattice sites in the x direction.

. pli

junction probability

per unit

length

and unit time.

.

pj(L,Y, h): equilibrium probability that,

on a fine of

given length L,

a number

Y/b

of

points

have a

position

x > h.

.

p(h): equilibrium probability

that for a

given

y,

x(y)

=

h, independent

of y.

. fil time one has to watt before

observing

a

junction

in a

length

of order

Li

.

p((h): equilibrium probability

that for a

given

y,

xiv)

> h.

.

p((L,1): equilibrium probability

that the

elongation

at a

particular

time is

larger

than

a

particular

value 1 much

larger

than the thermal average value of x.

.

p(y;

x,

x') joint probability

that

x(0)

= x and

xiv)

= x'.

.

p(~~ ~(y,

x,

x'):

conditional

probability

that

xiv)

= x' if

x(0)

= x.

.

pro(h): probability that,

for a

given

y, the distance between both

topmost steps

is h.

.

p)o ii) probability that,

for a given y, the distance between both

topmost steps

is

greater

than 1.

.

PL (h, t): probability

that the

elongation

at time t of a fine

segment

of

length

L is h.

. T:

temperature.

. ~: recoil

velocity

of the

topmost

terrace.

.

Woi

attractive

potential

due to the

binding

line

(Wo

>

0).

.

Wi step

free energy per atom.

Wi la

is also the line tension at low

temperature (Wi

>

0).

.

i(h):

average value of the

length Y, along

which the points have

positions

x > h for an

excursion of

elongation larger

than

h,

where h is much

larger

than the thermal average

elongation.

(14)

~

p,

1

kBT'

. ~t: line stifIness.

. r:

adsorption probability

from the vapour per site and per second when this vapour has

a

density

p

= 1.

. e:

exp(-flwi).

. < defined

by equation (A.25).

.

À(x):

extension of a fluctuation of

elongation

x; vertical distance after which the line has lost the memory and come back to its thermal

position.

. /~; vapour chemical

potential.

. pot vapour

deisity (fixed).

. a:

evaporation probability

from the

fluctuating

curve per site and per second.

.

adsorption probability

from the vapour per site and per second.

. f: time necessary to

peel

the

topmost layer

when one of the topmost

steps

is unable to fluctuate.

. f21 time necessary to

peel

the topmost

layer,

when both

topmost steps

can fluctuate.

.

Ti(1, L):

time interval between the

periods

in which the

elongation

of a

particular step segment

of

length

L is

larger

than 1.

. To

Ii): typical

time

during

which the

elongation

remains

larger

than1 if it is

larger

than 1 at a

given

time.

Appendix

A

Unbinding

llkansition in 1+1 Dimensions We consider

(Fig. 3a)

a fixed

straight

wall

ix

=

0)

and a hne which is at the

position xiv)

> 0.

The line has a stifIness which maintains it

straight

at the

temperature

T =

0,

and it is attracted

by

the fixed wall due to a

potential V(x)

< 0 for x

= 0.

It is easier to suppose that x and y are discrete

variables,

x

la

and y

la being integers,

where a is the interatomic distance. It is also easier to use

periodic boundary

conditions. The energy is

jN-1)a jN-1)a

U((X), (VI)

#

~j Vl(X(§))

+

~j V2(X(iÎ)> X(iÎ

+

~)) (~.~)

y=0 y=0

where

Aix)

=

-woôo,~ (A.2)

with

Wo

> 0 the attractive

potential

and V2

corresponds

to the stifIness. We can write

V~(x,x)

= 0

(A.3a)

V2(x,

x +

a)

=

V2(x

+ a,

x)

=

Wi

> 0

(A.3b)

and for the other

values,

V2(x, x')

= oo

(A.3c)

Equation (A.3c)

means that

x(y) x(y -1)

can

only

have the values

0,

a or -a, otherwise the Boltzmann factor is

equal

to zero.

(15)

A.I. THE PARTITION FUNCTION. The

partition

function is

Z =

£ exp[-flvi (xo

Il

exp[- flV2 (xo,

xi

Il exp[- flvi (xi

Il

~o,~i, ,xN-i

x

exp[-

flV2

(xi,

x2Il

exp[- flV2 (xN-i,

xoIl

(AA)

where xp =

x(pa).

It is useful to introduce the notation

(x[8[x')

= exp

-~Vi xii

exp[-fl%(x,x')]

exp

(-~Vi(x')j (A.5)

2 2

Now

(AA)

can be written

Z "

L iXoi8iXiiiXii8iX2i. IXPIÔIXP+ii. IXN-iiÔiXoi iA.61

The

quantity (x[8 lx')

can be considered as an element of a real Hermitian matrix 8. For the

moment we do not

give

the vector1al

meaning

to the notation

xi.

We will do it

later,

but now

this notation is

only

a part of the

quantity (xl

8

lx'),

which we can call

8xx,. Equation (A.6)

is written

Z = Tr

8~ IA.?)

The trace is easy to calculate if the

eigenvalues 0k

are known. Then Z =

£ 0f (A.8)

k

The

interesting

case is the limit N

= oo. In this case,

by supposing

that there is a gap between the

greatest eigenvalue

00 and the others

eigenvalues, equation (A.8)

is written

Z =

0/ (A.9)

This

expression

is not

universal,

because there is not

always

a gap, but is

quite general.

The calculation of the

eigenvalues, instead,

is

specific

of each

problem.

A.2. EIGENVALUES. An

eigenvalue

0 is defined from the

equation

jjxjejx'iijx'i

=

oijxi jA,ici

where we have omitted the indice k.

From

equations IA-à)

and

(A.3c), equation (A.10)

reduces to

lx181x)41x)

+

lx181x

+

a)41x

+

a)

+

lxie(z a)j(z ai

=

ojjz) jA.ii)

For x >

2a,

from

equations (A.5), (A.2)

and

(A.3),

one can written

equation (A.Il)

as

#ix)

+

e#ix

+

a)

+

e#ix a)

=

0#ix) iA.12)

where

f = exp

i-flwi) iA.13)

Equation (A.12) obviously

has the

following

solution for x > a

~k(X)

" ak

eXp(-kX) (A.14)

(16)

with the

eigenvalue

0k

" 1 +

e[exp(ka)

+

exp(-ka)] (A.15)

Since the matrix 8 is

Hermitian,

its

eigenvalues

must be real and then there are three

possibilities:

1) k is

real, ii)

k is

purely imaginary, iii)

the

imaginary

part of k is

equal

to 17r.

The third

possibility yields

an

eigenvalue (A. là)

which is smaller than one and can not be the

largest eigenvalue.

We will see that k can be or not a real value

(and only one).

To understand the

importance

of this

fact,

let us calculate the distribution of

points

of the

fluctuating

line.

A.3. DISTRIBUTION OF THE FLUCTUATING LINE. The

probability p(x)

that

x(y)

has a

value x is

independent

of y and is

given by pjx)

=

j expj- pvi ix)j expj-pV2 ix,

xi )i

expj-pvi (xi )i expj-pV21xN-1, x)j

~

xi,...,x~-i

where Z is

given by equation (AA). Transforming

this

equation

in the same way as we had transformed

equation (AA),

we obtain the

following expression,

similar to

equation (A.6):

Plx)

=

j L lx181xi)lxi181x2). lxp181xp+1) lxN-i181x) lA.16)

To obtain a

compact

relation similar to

equation IA.?)

it is suitable to introduce the vectors

[xi

and the

operators

X defined from

jx'jxi

=

ôxx, jA.17ai

and

(x'[X[x)

=

ôxx,x (A.17b)

This is a little abstract. For a

physicist

familiar with

quantum physics,

it is useful to consider

the vectors

[xi

as

representing

the states of a

partiale

that moves

along

the x axis

satisfying

the

equation

of

Schrôdinger IA.10).

From

equation (A.16)

we obtain

Plx)

=

jlx18~ix) lA.18)

To utilize this

equation,

we have to introduce the

eigenvectors [k)

of 8.

Substituting

8 =

£ jk)0k(kl lA.191

k

in

equation (A.18),

we obtain

Plx)

=

j L0ilxlk)lklx) lA.20a)

If the condition of

validity

of

equation (A.9)

is

satisfied, equation (A.20a)

can be written

Plx)

=

j0tlx10)101x)

=

lx10)101x) lA.20b)

where we have used

equation (A.9)

to write the second

equation

and we have introduced the

eigenvector loi

which

corresponds

to the

greatest eigenvalue 00.

This

eigenvector

is given

by equation (A.14),

where k has a

particular

value ~, that is to say,

loi

=

fl lx1401xl

=

aoDl0l

+ ao

L [xl exPl-~xl lA.211

x x#o

(17)

where D is a constant.

Inserting equation (A.21)

into

equation (A.20b), using equation (A.17b),

and

supposing

~ to be

real,

we

obtain,

for

x diflerent from

0, equation (4.1).

If ~ is

positive,

the

fluctuating

fine is localized. In this

article,

this condition is assumed to be fulfilled.

If ail the k were

imaginary,

the

general

term of

equation (A.20a)

is

independent

of x. The

fluctuating

fine is delocalized.

A.4. SEARCH FOR A BOUND STATE. A bound state

corresponds

to the solution

(A.14)

with real k.

Equation (A.14)

must also be solution of

equation (A.Il)

for x

= 0 and x

= a,

that is to say,

A~#o10)

+

eA#oia)

=

0#o10) jA.22a)

#oia)

+

e#o12a)

+

eA#o10)

=

0#oia) iA.22b)

where

A =

exp(flwo/2) (A.23)

By replacing

into

equation (A.22) #o(0), #o(a),

and

#o(2a)

calculated from

equation (A.21),

we find

A~D

+ CA

exp(-~a)

= 0D

(A.24a)

AD

= 1

(A.24b)

Inserting

the value for 0

given

in

equation (A.15),

we obtain the

following equation

of second order in

exp(~a):

A~

+

eA~ exp(-~a)

= +

e[exp(-~a)

+

exp(~a)]

or

f(e~~) ~2

" e~~~ e~~

(A~ -1)

= 0

(A.25)

e

The solutions of this

equation

in

exp(~a)

are

always

real and with

opposite

sign. The

positive

solution is the

only

one which

corresponds

to a real value of k. It

corresponds

to a localized solution if ~ is

positive,

that is to say if

exp(~a)

is

greater

than

1,

that is to say if

f(1)

< 0.

Then

f(1)

=1- 1+

f~ (A~ -1)

< 0

or

A~ > 1 +

~ (A.26a)

or

+ 2

exp(-flwi

(A.26b)

~~P~~~°~

~

l +

exp(-flwi

We observe that the two lines are bounded if the

temperature

is

sulficiently

low or for a fixed

temperature,

if the attractive

potential

is

sulficiently strong.

(18)

A.5. JOINT PROBABILITY. The

probability

that

x(y')

= x and

simultaneously x(y'+y)

= x'

is

p(y;

x,

x')

=

£ ~j exp[-flvi lx)] exp[-flV2(x,

xi

)1exp[-flvi (xi

~ )1

xi, ,xyla-i xyla+i, .,xN-i

~~~~~~Î~~~ÎÎ~~~~~~fI~~Î~~~~~~~ ~~~~"~~~~~~~~~~~~ ~~~~Y/~+~)Î

-,

or

piy;

x,

x~i

=

j L ixieixiiixiieiz~i iz~/~-iieiz~i

xi,..,x~/~-i

£ l~'lÔl~yla+11" l~N-llôlX)

~yla+>;. ~N-1

or

Plv;x,x')

=

jlx18~/~lx')lx'l8~~Y/~lx)

For y much smaller than the size Na of the

system,

this

expression

can be written

plu; x,x')

=

fl ())

~~~

lxlk)lklx'llx'101101xl lA.27al

or

fl Yla

pjy.

x

x')

=

~j

~

(x[k)(k[x')[ao[~ exp[-~(x

+

x')] (A.27b)

~

flo~

An useful check is obtained for y

=

0, using equations (A.27a), (A.20b)

and the relation

£~ [k)(k[

= 1:

p(0;

x,

x')

=

£(x[k)(k[x')(x'[0)(0[x)

k

=

(xix')(x'ΰ)(°Îx)

"

ô~~'P(x) (A.28)

It is convenient to

distinguish

between the localized state

loi

and the unbound state

[q).

Equation (A.27)

is written

P(Yi

X,

X')

"

P(X)P(x')

+

ôp(y;

x,

x') (A.29)

with

ôPlv; x,x'l

=

L ())

~~~

lxlqllqlx'llx'101101xl lA.30)

q#o °

The wave function of the unbounded state is written

[q)

=

Dqoq[0)

+ oq

£ sin(qx

+~q)

lx) (A.31)

~#0

where

Dq

and +~q are solutions of the

system A~Dq

+ CA

sin(qa

+~q) =

0Dq (A.32a)

sin(qa

+~q) + e

sin(2qa

+~q) +

eADq

= 0

sin(qa

+~q)

(A.32b)

(19)

or,

replacing

0

by

its

expression IA-là),

A~Dq

+ CA

sin(qa

+~q)

=

il

+ 2e

cos(qa)]Dq (A.33a)

ADq

= sin+~q

(A.33b)

Eliminating Dq,

we obtain

A~

+

eA~[cos(qa) sin(qa)

cot

+~q] = 1+

2ecos(qa) (A.34)

or

~2

1 +

f

COS(qa)(À~ ~)

~~

~~~

~~t +~~ =

~~2

sin(qa)

We see that

+~q is

proportional

to q if q is small.

The other parameters are determined:

Dq,

from

equation (A.33b);

oq, from the normaliza- tion condition. In

short,

for an infinite system in the x

direction,

ail values of q are allowed.

However,

it may be

preferable

to assume a

large

but finite size L

=

Na,

so that q takes discrete values

which,

as

usual,

are the

integer multiples

of 27r

IL. Then,

the normalisation condition takes the form

Î~QÎ~

l~

~~~~~~~ '~Q) ~

~~2'~~j ~~'~~~)

~

~

which,

for

large L,

reduces to

laql~

Cf

) lA.36b)

By using (A.30)

and

(A.31)

we obtain

o Yla

ôPlY> x,

x')

=

lac

l~

£ laq

l~

(() smjqz

~f~)

sinjqz'

~f~)

expj-~jz

+

z')j

~

o Yla

=

lac

l~

£ laq

l~ ~

coslqjz z')i expl-~jz

+

z')j

~

o

~ Yla

~l£X01~

£1£XQl~ (() C°Sl~lX

+

X')

2'fQl

~~Pl~~lX

+ X')1

lA.37él)

~

or,

substituting

the expression

(A.15)

for 0

ôp(y;

x,

x')

=

[oo

Î~

~j Îaq

[~

~ ~~

°~~(~~

~~~

cos[q(x x')] exp[-~(x

+

x')]

A

37b)

~

l + 2e cosh

~a)

~

_~ ~ +

z'

j~~

j2

j jaq

Î~

i~/Î~ÎÎÎÎ~)

~~ ~~~~~~~ ~

~'~

~'~~~

~~~~

~

It is

pretty hard,

from this

formula,

to recover

(A.28)

for y

= 0. As a matter of

fact,

formula

(A.37b)

is not very convenient for small y.

However,

if y is

large enough,

the

quantity

Il +2ecos(qa) ~f~

+ 2e

cosh(~a)

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