HAL Id: jpa-00246734
https://hal.archives-ouvertes.fr/jpa-00246734
Submitted on 1 Jan 1993
HAL is a multi-disciplinary open access archive for the deposit and dissemination of sci- entific research documents, whether they are pub- lished or not. The documents may come from teaching and research institutions in France or abroad, or from public or private research centers.
L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des établissements d’enseignement et de recherche français ou étrangers, des laboratoires publics ou privés.
Fractal terraces in MBE growth
Alberto Pimpinelli, Jacques Villain, Dietrich Wolf
To cite this version:
Alberto Pimpinelli, Jacques Villain, Dietrich Wolf. Fractal terraces in MBE growth. Journal de
Physique I, EDP Sciences, 1993, 3 (2), pp.447-457. �10.1051/jp1:1993144�. �jpa-00246734�
J.
Phys.
I France 3(1993)
447-457 FEBRUARY 1993, PAGE 447Classification
Physics
Abs tracts68.55 05.40 64.60H
fkactal terraces b1 MBE growth
Alberto
Pimpinelli(~,~), Jacques
Villain and Dietrich E.Wolf(~)
S. P. S. M.
S./M.
D.N., D4partement
de Recherche Fondamentale M. C. du Centre d'Etude Nucl4aire deGrenoble,
85X 38041 GrenobleCedex,
France(~)
Laboratoire despectrom4trie physique,
Universit4Joseph Fourier, Grenoble,
France(~) Dipartimento
di fisica, Universiti di Parma,1-43100 Parma,Italy
(~)
IFF,Forschungszentrum
KFAJfilich,
POB 1913, D-5170Jfilich,
Germany(Received
8June1992, accepted
in final form 24July1992)
Abstract. MBE
growth
onhigh
symmetry surfaces depends to some extent on theshape
of the terraces which form the
embryos
of each new atomiclayer.
The conditions for formationof compact or fractal terraces are discussed in two limits:
large
terraces, to which a continuousdescription applies,
and small terraces, whichrequire
that the discrete nature of matter be takeninto account. In both
cases it is found that terraces
are fractal if and
only
if diffusion of adatomsalong
steps is much slower than on the flat surface at the same temperature. Precise conditionsare
given
which should be accessible toexperiment.
1. Introduction.
Progress
in theunderstanding
of fractalphenomena
has been amajor
contribution of Rammal and his coworkers. In thepresent
work we address thepossibly
fractalshape
of terraces on acrystal
surfacegrowing by
molecular beamepitaxy (MBE).
An
important problem
in this field is thetypical
size £ of the islandson the
growing
surface.Indeed,
the measurement of £can
give
information on the surface diffusion constantDs,
andeven allows a
quantitative
determination ofDs itself,
at least insimple
cases[II.
Domains of size £ may also form in the surfacelayer if,
forinstance,
the adsorbate has avariety
ofpossible
equivalent superstructures.
In most theoretical
investigations [2, 3, 4],
the islandshape
has been assumed to becompact,
I.e. not fractal.However,
fractal islands have been observedby scanning tunneling microscopy (STM)
in thedeposition
of Pt on Pt at 205 K [5] and of Au on Ru(0001)
[6] at roomtempera-
ture. Fractal islands seem to be observed
only
at(relatively)
lowtemperatures.
Si on Si(001)
has been
investigated
also at lowtemperature by
Mo et al.[Ii,
but the situation iscomplicated
because both surface diffusion and
sticking-to-step
arehighly anisotropic.
The mechanism
underlying
islandfractality
is the so-called diffusion limitedaggregation
(DLA) [7, 8, 9].
DLA is agrowth
process where atoms diffuse from far away and Stick to thefirst
growing
islandthey find,
at the veryplace
wherethey
touch it for the first time. Because offluctuations,
islandsdevelop tips,
mostincoming
atoms reach islands attips,
and thus thetips
becomelonger
and the fractalshape
appears.In MBE
growth
this scheme isoversimplified
because atoms can also bedeposited right
ontop
of an island. This favours acompact shape,
since atoms diffuse to theedge
of the island both from outside and inside. For smallislands, however,
the flux from inside isnegligible.
A
theory describing
theshape
ofgrowing
islands on ahigh symmetry crystal
surface will be outlined in thepresent
article.Analogies
and differences withexisting
theories will bediscussed.
2.
Magnitude
oft for fractal islands.The effect of terrace
edge fractality
on thetypical length
£ has been discussedby
Villain et al.[10]
and willonly briefly
be summarized here.Evaporation
will beneglected
since thetemperatures
of interest are low. The basicpic-
ture is that atoms
falling
on the surfacemostly
land on terraces betweensteps.
These mobile"adatoms" diffuse
(with
a diffusion constantDs)
untilthey
reach astep
and areincorpo-
rated there.Sometimes, however, they
meet anotherdiffusing
adatom beforereaching
astep,
andthey
may therefore forma
pair.
Pairs aresupposedly
immobile and stable at the lowtemperatures
we areconsidering.
The
density
pi ofdiffusing
adatoms perabsorption
site may beeasily
evaluated. Adatoms have an average lifetime ri beforebeing incorporated
into astep,
and pi isequal
to theproduct
of ri times the rate F ofincoming
atoms per site. Thatis,
pi "Fri. During
its lifetime ri an adatom diffuses a distance of the order@S By definition,
thislength
has to be identified with thetypical
distance betweensteps,
£.Thus,
£~ mDsri
andpi >
F£~/Ds. (ii
The
sign
" m " means "of the order ofmagnitude
of'. We can now evaluate the rate ofpair
formation.Diffusing
on a two dimensionalsurface,
an adatom visitsapproximately (I.e.
disregarding logarithmic corrections) Dsri
* £~ distinct sites. The unit oflength
is the interatomic distance. Each of these £~ siteshas,
on average, aprobability
pi ofbeing occupied,
and each adatom has therefore a
probability pi£~
offorming
apair.
The rate1/rn~~
ofpair
formation
(nucleation)
per site is obtainedby multiplying by
the rate F of atomsfalling
oneach site
1/rn~~
mFpi£~
mF~£~/Ds. (2)
Now,
since £is,
among otherthings,
thetypical
island size beforecoalescence,
there should be one andonly
onepair
formation in an area £~during
the whole life of an island. Thecorresponding
lifetime isequal
to IIF
times the islanddensity,
which isI/£~f
for fractal islands with fractal dimensiondf.
DLA in 2 dimensionsgives df
= 1.7. Thereforei/Tnuc
>F/£~~ (31
Equations
2 and 3yield
I
£ m
~~
~ ~ ~~(4)
F For non-fractal
terraces, df
= 2 and [3]
~ i/6
t R
(") jsj
F
N°2 FRACTAL TERRACES IN MBE GROWTH 449
1y
a
~ O
' O
b
c
' E
Fig.
I. An adatomapproaching
a terrace(a)
stickspreferentially
at a tip, and can then be remitted(b)
and diffused intoa
gulf.
It may also diffusestraightforwardly
to agulf along
the stepedge (c).
3.
Stabilizing
effects.We will now discuss the
stability
of non-fractalshapes during growth. Compact,
non-fractal forms are stabilizedby
therearrangement
of atoms within aterrace,
which is anegligible
efLectonly
at very lowtemperature. Indeed, compact shapes
areenergetically
favoured becausethey
minimize the surface tension energy.
Thus,
atoms bound at theedge
of an island(hereafter
called
gradatoms)
will diffusealong
the sameedge
and tend torepair fractality.
This will be callededge-
orstep-diffusion rearrangement.
The word
"gradatom" (from
the Italiangradino,
the Frenchgradin
or the Latingradus)
ispreferred
to"stepatom"
to avoid the initial "s" which weprefer
tokeep
for "surface".A similar
healing
effect is due to atomstemporarily ejected
fromtips
which diffuse toa
deeper place,
or to atoms which do not stick at first hit to the island and diffuse then to a site inside somedeep gulf (Fig. I).
This will be called off-clusterrearrangement.
4. Small islands at low
temperature.
Fractal islands
actually
observedduring heteroepitaxy
of Au onRu(0001)
[6] show dendriticarms with a
typical
width r~ of some ten nanometers. The verysimple argument
that followssuggests
that this width ismainly
controlledby
the diffusion constantDg
ofgradatoms.
Weassume low
temperature,
and that twogradatoms meeting along
theedge
of a terrace form theimmobile and stable nucleus of a new
layer
for the lateralgrowth
of the terrace.Imagine
for instance a small islandgrowing
on(001)
face. At first it willkeep
its most stableform,
thatis,
a square(Fig. 2a),
eventhough
the adatomsmainly
stick to the corners. If weassume that
they
all stick to the corners, for a linear dimensionr
sufficiently large
the island will take a cross-likeshape (Fig. 2b).
Thisshape
is observed inHwang
et al.experiment
(but
with a substrate ofhexagonal symmetry!).
For a smaller size r < r~gradatoms
have the/
oo /
a b
Fig.2. a)
Stable form of a small terrace at low temperature.b)
Dendriticinstability
undergrowth
conditions.time to diffuse to the center of an
edge
and to form there a stable nucleus. Beforereaching
a
newly
formedlayer, gradatoms
have to cover a distance of the order of the linear sizer
of the island. This takes a time r m
r~/Dg.
Thedensity
ofgradatoms
on the side of an island ispf
=
Fr,
where F is the rate ofincoming
adatoms per unit site on the islandedge;
thus F
=
F£~/r. Therefore, pf
=
F£~r/Dg.
The islandundergoes
stablegrowth
if thegradatoms
are able to cover a distance of order r withoutmeeting
anothergradatom.
Thisimplies rpf
< I. This condition is notsufficient,
because itonly requires
that oneparticular gradatom
be littlelikely
to form apair
beforereaching
anadsorption
site(kink).
Infact,
wemust ask the same
requirement
from a number ofgradatoms
of the order of r. Since for eachgradatom
theprobability
ofpair
formation isrpf
for rgradatoms
it isr~pf.
Therefore the critical linear size r~beyond
which the islandgrowth
is unstable isgiven by
r(£~
=Dg/F. (6)
£ is
directly
accessible to measureby scanning tunneling microscopy,
for instance.Assuming
for £
equation (5),
one findsj~3 '
~ g~ g
j~)
~
F2Ds
Equation (6)
ismeaningful only
if r~ <£,
that is ifrf£~
<£~,
andaccording
toequation (5)
F >
D(/D(. (8)
Since F is known and both r~ and £ are
directly
measurable withSTM, equation (6)
allowsan
experimental
determination of the diffusion constant ofgradatoms Dg.
In the case of Auon Ru
[6],
thepictures
taken at 300 Ksuggest
r~ m 10 nm, £ m 100 nm, withF~~
= 30 s,
which
imply Dg
m 10~s~~ Assuming
an activated formDg
=D(
exp(-pwg) (9)
and a
typical
value of theprefactor D(
m 10~~s~~,
our estimateyields
an activation energyW~
of the order of 0.35eV,
which is not unreasonable.Equation (8) implies
that the surface diffusion constant has a lower bound ofapproximately 10~ s~~
at roomtemperature,
which inturn
gives
an activation energyWsd
* 0.29 eV for surface diffusion.N°2 FRACTAL TERRACES IN MBE GROWTH 451
The
simple argument
abovegives only
an estimate of thetypical length beyond
which an island is nolonger
able to retain itspolygonal shape.
Whathappens
when the size exceedsr~ can
only
be studiedby
numerical simulations. This has been doneby
Xiao et al.[11].
They
assumed off-cluster diffusion due to the weakness of thesticking
coefficient of adatomson islands. Since this
type
ofsticking
coefficient is assumed to increase withtemperature, they
found that islandfractality
decreases withtemperature,
in contrast withexperiments
onhomoepitaxial
Pt [5].5. Classical linear
stability analysis.
In the
previous section,
the appearance of a fractalshape
has been attributed to the fact thata small
tip
on an island tends to becomelonger
becauseincoming
adatoms landpreferentially
on that
tip.
Thisinstability
is nottypical
of a random processonly,
and itscompetition
withstabilizing
effects can be studied within a deterministicgrowth
scheme. In the case of aplanar
surface this was done
by
Mullins and Sekerka[12].
We shall not gobeyond
theiranalysis,
butwe shall
adapt
it to our purpose. Theargument (given
more in detail inAppendix I)
canbe summarized as follows.
Away
from astep,
thedensity
p of adatomsobeys
theequation T7~p+
F = 0. Theboundary
conditionalong
astep
in the case ofperfect sticking
is p = 0. Thegrowth
rate on eachpoint
of the surface isproportional
to the currentj
=
-DT7p.
From theseequations,
it can be deduced that a sinusoidalperturbation
6x-~ cos
(ky)
on astraight step parallel
to the x directiongenerates
adestabilizing
term6idest
* Const x k6x due to atomsdiffusing
toward thestep.
This term isproportional
to the wavevector k of theperturbation
as in the
analysis
of Mullins and Sekerka. The constant isproportional
to the fluxF,
but alsodepends
on the average distance £ betweenislands,
and on the radius R of the cluster of interest. Moreprecisely,
the island collects in the time t the atomsfalling
in the area £~during
that time.Therefore,
the number of atomsreaching
agiven
island per unit time is of orderF£~,
and the flux per unitstep length
is obtaineddividing by
R.Finally
6+de~~ m
~~~
x kbx
(10)
The
stabilizing
term due to off-clusterrearrangement
is[12, 13]
6i~tab
m -Const xk~6x. ill)
This formula is rederived in
Appendix
I.Instability
occurs if thewavelength I/k
of theperturbation
islarger
thanlllfl, multiplied by
sometemperature dependent
constant. Of course, I/k
has to be smaller than £. Thus theinstability
arises if £~ > ConstIF. Replacing
£by equation (5),
fractal islands are seen to be favouredby
astrong deposition
flux F. The case ofstep-diffusion
will now beinvestigated
in more detail. Thestabilizing
term6i~tab
satisfiesa
continuity equation
~
~~~~~~
3)
~~~~~Tje
current
j along
thestep
is related to thegradient
of the chemicalpotential
pby
the~~ ~ ~~~
~
£~~
~~~~
The chemical
potential
p isproportional
to thecurvature, 32~
p m
-C~. (14)
Thus,
6k~tab
=-CAgk~6x. (15)
The kinetic coefficient
A~
which appears inequation (15)
isgiven by
a Kuboformula,
whicb may be seen to be(Appendix 2)
Ag
"~ fl j dt(Um(t)Vm(°)) (16)
where m labels the adatoms and the vm 's are their velocities. The correlation function is
easily computed (Appendix 2)
and one obtainsAg
=(Ii)
T7k
where
1/7k
is the rate of emission ofgradatoms
from agiven
kink. The constant Cdepends
on the orientation of the
step.
For the easyorientation,
it can be shown that C=
~
exp
(pwo)
2 where
Wo
is the energy of a kink. ThereforeAgC
m exp(p (Wo Wk)). (18)
~k
It is more relevant to consider the uneasy orientation.
Indeed,
if the island has theshape
of a roundedpolygon
atequilibrium,
thetips
areexpected
todevelop
at the corners since thelatter are
preexisting tips. Then,
ina square
lattice,
C= 4T and
A~C
m exp(-flwk ) (19)
r~
In any case this is small at low
temperature.
A
straight step
is unstable if~~~
>AgC. (20)
Since R <
£,
theprevious
resultimplies F£~
>AgC.
At low
temperature,
t m(D~/F)~/~
andinstability
can occuronly
ifF/D~
>(AgC/D~)~ (21)
Bales and
Zangwill [14]
and Uwaha and Saito[15]
have alsoinvestigated
thestability
of astraight step
on agrowing crystal. They
took into accountevaporation,
which modifiespretty
much the aboveanalysis. Also, they
have assumed the presence of the so-called Schwoebel effect. This effect consists in theimpossibility (or difficulty)
for adatomscoming
from thetop
of a terrace to go down the
step
because of apotential
barrier. The existence of sucha barrier in certain cases,
postulated by
Schwoebel[16],
issupported by microscopic
calculations[Iii.
The Schwoebel effect is a necessary condition for the
instability
of an infinitestep,
but is not essential for small islandssince,
anyway, the number of atomscoming
from inside the island is much smaller than the number of thosecoming
from outside. On the otherhand, evaporation
of adatoins from the surface can be
neglected
at those low temperatures where fractal islandsare
expected according
to calculations and have beenactually
observed.As seen
above,
most of theanalytic
tr~atments address thestability
ofinfinitely long straight
steps. Of co(Jrse. small I;lands ha;e not
iiifinitdy long straight edges.
The case of a circularN°2 FRACTAL TERRACES IN MBE GROWTH 4s3
island can be treated. But islands are not circular either at low
temperature,
even atequi-
librium. Theequilibrium shape
attemperatures
of interest issomething
like a square withseverely
rounded corners. Thestability
of such ashape
is a nonlinearproblem.
A numerical treatment has beengiven by
Ben Amar[18].
6. Conclusion.
We have demonstrated that islands on a surface
growing by
MBE can be fractal at low tem-perature,
inagreement
withexperiment. According
to ourformulae, fractality disappears
at lowgrowth
rates. This does notseem to be confirmed
by experiments [6].
This may be an effect of a lowsticking
coefficient.Fractality
of terraces ispredicted
to increase the average terrace size £. This may beexpected
to have effects on the
quality
ofcrystals,
but these effectsdepend
on thecrystal
structure. The influence of the Schwoebel effect on thecrystal quality
is alsoexpected
to beimportant,
but this is left for furtherinvestigation.
Acknowledgments.
A.P. wishes to
acknowledge
financialsupport
from the CentroInterdisciplinare
"BeniaminoSegre"
of the Accademia dei Linceiduring part
of this work.Appendix
1.The Mullins-Sekerka
instability
in the case ofstep-diffusion rearrangement.
The usual Mullins-Sekerka
instability
takes into account off-clusterrearrangements.
Here theappropriate
formulae forstep-diffusion
will be derived.We want to
specify
conditions for the fractalgrowth
of anisland,
in the intermediate tem-perature regime
where a continuousdescription
can beproperly employed.
As a first case we will consider theboundary edge
of the island as an infinitestraight step parallel
to the y axis(Fig. I).
Since atoms havea small
probability
offalling directly
ontop
of a smallisland,
weassume that adatoms diffuse on the surface to the
step only
from oneside,
theright
one fordefiniteness. The
step
thus grows to theright (positive
x).
As we discuss in the
body
of the paper, thestep
in a diffusion field is unstable tofluctuations,
since new adatoms will
preferentially
hit theprotruding parts
of theboundary
and willamplify
the fluctuation itself. This is the assumed mechanism
leading
to a fractal structure.We
replace
this stochastic behaviourby
a deterministic process, an average current of adatoms onto theboundary edge.
We introduce also a diffusion currentalong
thestep
as astabilizing effect,
andcompute
theresulting step profile
to first order in theamplitude
of thefluctuation.
Assume a sinusoidal
perturbation,
6x =
qcos(ky). (A.I.I)
The
density
of adatomsobeys
the diffusionequation
with a constant sourcs(the deposition
flux
F);
we still consider thetemperature sufficiently
low as to allowneglecting evaporation
from the surface. To
simplify
werequire stationarity:
D~T7~p
+ F = 0.(A.1.2)
Approximating
the islandboundary
with astraight step
iscertainly
notsatisfying
when thewavelength ilk
of theperturbed profile
becomes of the order of the linear size R of theisland,
but we
expect
the results to be correct in order ofmagnitude.
The solution ofequation (A.1.2)
for q = 0 is
~°~~~ ~s
~~
~ ~ ~~~' ~~
~~where A and B are constants Since the y axis has been chosen
along
the averagestep
direction(Fig. I),
the term inx~
may be
neglected
in the linearstability analysis.
For that reason the linearstability analysis yields
the same results as in the case F = 0already
discussed inliterature
([18, 19, 20]).
Even the nonlinear version shouldgive analogous
results for F= 0
and for small F in the case of a small island.
Imperfect sticking
of adatoms to thestep
can be taken into account if we writeEq.(A.1.2)
in a discretized form
Ds(pn+i +pn-1-2pn)+F=
0(1<
n<£-1) (A.1A)
and
supplement
it withappropriate
conditions near thestep.
For n =1,
the diffusion constantDs
will be assumed to havea value D' <
Ds.
A small value of D'corresponds
to a smallsticking
coefficient.Also,
adatoms can be released from thestep,
at a rate1/rg.
Theresulting equation
isDs (p2 Pi) D'pi
+ I/rg
+ F= 0.
(A.1.5)
We shall first discuss the case of
perfect sticking.
This means that thesticking
coefficient isequal
to I(D'
=Ds)
and that no adatom is released from thestep (rg
=cc).
Then insertion of(A.1.3)
intoequation (A. IA) yields
A= 0. This means that p should vanish
along
thestep.
This should also be true for q
#
0. It turns out that a solution ofequation (A.1.2)
for q#
0 isp =
-( (x~ lx)
pi cos(ky)
exp(kx). (A.1.6)
~
The first term is the
particular
form ofequation (A.1.3)
which vanishes on bothsteps
atx = 0 and x
= £. The second term should vanish when x has the value
(A.1.1). Therefore,
for small q,
~~
~~~ ~~'~'~~
The
velocity
ofpropagation
of thestep, disregarding
any effect of linetension,
is in eachpoint equal
toD~n(n T7p),
where n is the unit vector normal to thestep.
The two
components
of thegradient
of thedensity
arem
-) ~~)~~
cos
(ky) ()
+kpi
cos(ky) (A.1.8)
)
s=
-kpi
sin(ky)
exp(kx)
ci-kpi
sin(ky). (A.1.9)
y
To first order in the
amplitude
of the fluctuation the normal vector n readsn =
1,
~f~(~~
sinky)) /
+(~ f~(~~
sinky)) (A.1.10)
~
N°2
FRAbTAL
TERRACES IN MBE GROWTH 455and we
finally
findv~ = 6k =
-F£/2
+D~pi(k Ill) cos(ky). (A.1.11)
In a
comoving
frame the first term vanishes. Since we are interested in the case k£ >I,
in thecomoving
frame we have6i =
k£F/26x. (A.1.12)
The fluctuation is therefore
exponentially amplified,
since k£F ispositive.
This formula is valid between two infinitesteps.
For a terrace of radiusR,
it is reasonable toreplace
£by
£~/R
asexplained
in the text andequation (10)
is obtained.We now discuss the case of
imperfect sticking.
Thequadratic
term inequation (A.1.3)
will beneglected. Equation (A.1.5) implies
(D~ D')B
D'A + I/rg
= 0.
(A.1.13)
Therefore the value A of the adatom
density
on thestep
isgiven by
A
= +
(~~ l)
B.(A.1.14)
D'Tg
D'In the case of two
parallel steps,
B is of orderF£/2D~,
as inequation (A.1.6).
The main difference with the case ofperfect sticking
is thatI/rg
nowdepends
on thecurvature,
since adatoms are moreeasily
released attips,
where x"=
3~x/3y~
isnegative:
A t
Au Al
x".(A.1.15)
The solution of the diffusion
problem
has still the form(A.1.6).
Theboundary
condition isp(x) equal
to(A.1.15)
when x isgiven by (A.I.I).
Then a correctionproportional
to k~should be added to
(A.1.7).
Thisyields
astabilizing
termproportional
to-k~6x
in6i,
as in theoriginal
calculation of Mullins and Sekerka.Appendix
2.Calculation of the diffusion coefficient A.
A is defined
by
j
=-Ai7p (A.2.1)
where p is the chemical
potential.
Let us assume a free energy of the formF "
jd~rP~(~) j d~rP(~)P(~l. lA.2.21
For small variations of p one has
Asp(r)
=6p(r) (A.2.3)
which
implies
j(r)
=-AAVp(r) jA.2.4)
and therefore
)(r)
= -divj(r)
=AAi7~p(r). (A.2.5)
Transforming
to Fouriercomponents
this becomesfik "
-AAk~pk (A.2.6)
which can be
readily integrated,
with solutionpk(t)
=pk(0)
exp(-AAk~t). (A.2.7)
Taking
the thermal averageaccording
to F weget
ip~(tip-~(oil
=
ip~p-~i
exp(-AAk~t). (A.2.81
Taking
the time derivative of the left-hand side we end up with thefollowing equation, ip~(t)p-~(o))
=
-AAk2ip~p-~)
exp(-AAk2t). (A.2.9) Making
use of the trivialidentity
lPklt)P-k1°))
=)~ dt'lPk lt')P-k1°)) lA.2.1°)
and
using Equation (A.2.5),
wefinally
findlPkltlP-k1°)1
=i~ ki )~ dt' lJoklt'lJ«,-k(°)1
=
=
)~ dt' lik(t').I-k(°)I (A.2.ill
Summarizing,
~~
j~~p-~)
exp(-AAk2t)
=
1i'dt' 0kit') I-k~°~~ ~~.~~~~
The latter relation is true if t is
large enough
toprovide
for anexponential
decrease of theintegral.
If we also assume that t < AA/k~,
we have
AA
lPkP-kl
=j
j~
dt'liklt'l I-k(0)1 (A.2.13)
Since the free energy is
quadratic
in thedensity,
the correlation function issimply (Pkp-k)
=
( (A.2.14)
and
Eq.(A.2.13)
becomesA "
~ j~ dt' lik It') j-k (0)) (A.2.15)
This
general
formula will now beapplied
to thespecial
case of diffusion on astep.
We take the current ofgradatoms along
astep edge,
Jk
=fi ~
vm exP
(tkxm)> iA.2.161
N°2 FRACTAL TERRACES IN MBE GROWTH 457
where m labels the
gradatoms
and N is the totallength (assumed
to belarge)
of astep
(assumed
to bestraight).
Thenequation (16)
is obtainedby inserting equation (A.2.16)
inequation (A.2.15).
The average thermal distance between
kinks
isto
" exp(Wo/T).
Agradatom
covers such distance in a time To"
£(/Dg.
Let t = To The average number ofgradatoms
emittedby
a kink per unit time is
1/7k.
A fractionI/£o
of thesegradatoms
reach a kink. Therefore the number ofgradatoms
which are effective on alength to
isgiven
asro/(Tk£o)
Since theirvelocity
is v =£o/ro,
we findA=
~~S~2_
foT
7k£oTrk (A.2.17)
which is
equation (17).
Quite surprisingly,
the result isindependent
of bothDg
andWg.
References
[ii
Y. W.Mo,
J.Kleiner,
M. B. Webb and M. G.Lagally, Phys.
Rev. Lett. 66 1998,(1991).
[2] G. Zinnsmeister, Thin Solid Films 2, 497
(1968).
[3] S. Stoyanov and G. Kashchiev, in Current
topics
in Materials Science Vol. 7, E. Kaldis ed.(1981)
[4] J. A.
Venables,
G. D.Spiller
and M. Hanb6cken,Rep. Prcg. Phys.
47, 399(1984).
[5] M. Bott, T.
Michely
and G. Comsa,preprint (1991).
[6] R.
Q. Hwang,
J.Schr6der,
C. Gfinther and R. J.Behm, Phys.
Rev. Lent. 67, 3279(1991).
[7] T. A. Witten and L. M. Sander,
Phys.
Rev. Lent. 47, 1400(1981).
[8] L. Pietronero and E. Tosatti eds., Fractals in
Physics,
North Holland,(1986).
[9] F.
Family
and T.Vicsek, Dynamics
of FractalSurfaces,
World Scientific(1991).
[io]
J.Villain,
A.Pimpinelli
and D. E.Wolf,
Comments on Cond. Mat.Phys.
16, 1(1992).
[iii
R. F.Xiao,
I. Iwan D. Alexander, F.Rosenberger (1988) Phys.
Rev. Lent. 38, 2447(1988).
[12] W.W. Mullins and R.F. Sekerka, J.
Appl. Phys.
34, 323 and 35, 444(1963).
[13] J.
Langer,
Rev. Mod. Phys. 52, 1(1980).
[14] G.S. Bales and A.
Zangwill, Phys.
Rev. 841, 5500(1990).
[15] M. Uwaha and Y. Saito,
Phys.
Rev. Lett. 68, 224(1992).
[16] R.L.
Schwoebel,
J.Appl. Phys.
40, 614(1969).
[17] J.P. Bourdin, J.P.
Ganachaud,
J.P. Jardin, D.Spanjaard
and M-C-Desjonqueres,
J.Phys.
F:Met.
Phys.
18, 1801(1988).
[18] M. Ben Amar,
Eurcphysics
Lett. 16, 367(1991).
[19] M. Ben Amar, V.
Hakim,
M. Mashaal and Y.Cruder, Phys.
Fluids A 3 No.(7) (1991);
M. Ben Amar,Phys.
Rev. A in press.[20] R. Combescot and M. Ben Amar,