A NNALES DE L ’I. H. P., SECTION B
A. D E M ASI
E. P RESUTTI
E. S CACCIATELLI
The weakly asymmetric simple exclusion process
Annales de l’I. H. P., section B, tome 25, n
o1 (1989), p. 1-38
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The weakly asymmetric simple exclusion process (*)
A. DE MASI
E. PRESUTTI and E. SCACCIATELLI Dipartimento di Matematica pura e applicata,
Universita dell’Aquila,
Institute for Theoretical Physics, U.C.S.B., Ca. 93106
Dipartimento di Matematica, Universita di Roma I, Institute for Theoretical Physics, U.C.S.B., Ca 93106
Vol. 25, n° 1, 1989, p. 1-38. Probabilités et Statistiques
ABSTRACT. - The one dimensional n.n.
simple
exclusion process withgenerator E - 2 Lo + E -1 La, E > o,
isconsidered, Lo
andLQ being respectively
the
generators
of thesymmetric
andtotally asymmetric simple
exclusionprocesses.
Propagation
of chaos and convergence to theBurgers equation
with
viscosity
are proven in the limit when 8 goes to zero. Thedensity
fluctuation field is shown to converge to a
generalized
Ornstein Uhlenbeck process with mean zero. The timeasymptotic
covariance kernel isexplicitly computed
fortraveling
waveprofiles
and the result indicates that the shockprofile
is stable while its space location fluctuates around its averageposition
like a brownian motion. Its diffusion coefficient isexplicitly computed.
Key words : Exclusion process, hydrodynamic limit, Burgers equation, shock waves.
RESUME. - On considere le processus d’exclusion
simple
a deplus proches
voisins degenerateur L~ = ~-1 Lo + La,
ouLo
etLa
sontrespective-
ment les
générateurs
des processus d’exclusionsimple symetrique
et totale-ment
asymetrique.
Lapropagation
du chaos et la convergence vers1’equa-
tion de
Burgers
avec viscosite sont demontres pour e - 0. On montre que(*) Partially supported by C.N.R. P.S. A.I.T.M., CNPq grant n.401872-85 and the National Science Foundation under grant No: PHY82-17853 supplemented by funds for the National Areonautics and Space Admnistration.
Classification A.M.S. : 60 K 35.
Annales de l’lnstitut Henri Poincaré - Probabilités et Statistiques - 0294-1449
Ie
champ
de fluctuation de la densité converge vers un processusgeneralise
de Ornstein
Uhlenbeck,
de moyenne 0. La covarianceasymptotique
estcalculee
explicitement
pour desprofils
d’ onde en mouvement et les resultatsindiquent
que leprofil
du choc est stablelorsque
saposition
fluctue commeun brownien. Autour de sa
position
moyenne, son coefficient de diffusion est calculeexplicitement.
INTRODUCTION The one dimensional
Burgers equation
(1.1) r E R, t >_ 0, ~, >_ 0,
is one of thesimplest equations
where thegrowth
and thepropagation
of shock waves can beobserved, cf
forinstance
Smoller, [26],
and referencesquoted
in. Non linearPDE’s,
like
(1.1),
describes to some extent and inparticular
situations the macro-scopic
behavior and the collectivephenomena
exhibitedby
several modelsystems,
like cellular automata and stochasticinteracting particle systems.
In the last years such
systems
have beenextensively studied,
cellularautomata for very fast
computer
simulations(cf
for instance[21],
whereeq.
( 1. 1)
wasconsidered)
and stochasticinteracting particle systems
for thepossibility
of amathematically rigorous analysis,
which seemsbeyond
the
present techniques
for more realisticparticles
models ofphysical
fluids.The use of stochastic
systems
in thestudy
of(1.1)
goes back toMcKean, [22],
and carried outby
Calderoni andPulvirenti, [6],
andSznitman, [28],
for
systems
ofsuitably interacting
Brownianparticles.
In this paper weshall consider the exclusion process. The relation between such proces and
(1.1)
with ~, = 0 is wellknown, cf [25], [20], [5], [11], [9],
and[2], [29], [3]
where a zero range processisomorphic
to the exclusion process is considered.The derivation of
( 1.1)
with ~, > 0starting
from the exclusion process is in a sense easier. In fact for drift and diffusion to have samestrength,
like in
( 1. 1),
one mustsuitably
"weaken" theasymmetry
in the exclusion process which can then be studied as a"perturbation"
of thesymmetric
one. This can be done
by applying general
methods like the Fritz’stechnique, [14], cf. [15]. Alternatively
one can use the GuoPapanicolaou
and Varadhan
approach, [17],
which has theadvantage
ofexpliciting
theconnection with the
large
deviationstheory.
The derivation of(1.1)
withAnnales de l’lnstitut Henri Poincaré - Probabilités et Statistiques
such
techniques
has beenrecently
carried out in[19].
Thesimplest
deriva-tion of
(1.1)
is in ouropinion
due to Gartner[16]
who considers aspecific weakly asymmetric simple
exclusion process and for this he is able toexploit
at theparticles’
level the transformation which maps(1.1)
into alinear differential
equation.
To conclude we mention that thesteady
statesolutions to
( 1.1)
can be deriveddirectly, cf [8],
and that there is aninteresting
relation between(1.1)
and some interface evolutionproblem, cf Spohn [27].
In this paper we rederive
(1.1)
from theweakly asymmetric simple
exclusion process, we refer to the next section for
precise
definitions and results.We use the correlation functions
technique, introducing
somespecial
correlation functions which solve a
simplified hierarchy
ofequations
andallow us to overcome the short time limitations
usually present
in theanalysis
of thehierarchy
in the Grad-Boltzmann limit. Ourapproach
isundoubtly lengthier
but it has theadvantage
ofproviding
very detailed information on the process,actually
more than what needed forproving ( 1.1).
This is notpurely
academic. Our aim is to go further in theanalysis
of the
weakly asymmetric simple
exclusion processbeyond establishing (1.1)
and tostudy
theparticle
model in a muchlonger
time scale thanthe one where
(1.1)
is proven. Inparticular
we want to know at theparticle
level thestability properties
of thetraveling
wave solutions to(1.1).
Howlong
does the shock movekeeping
itsshape ? according
to(1.1)
it isstationary,
is that true for themicroscopic
model ? Should weadd to
(1.1) correcting
terms to catch the truelimiting
behavior ? whichones in the case ? the
problem
looks like thefollowing.
Consider X to bethe space of all
density profiles.
LetpeX
be atraveling
wave solution to(1.1). Hence,
as it is wellknown,
theshape
of p is determinedby
twoparameters
p- and p+ which denote theasymptotic
densities to the leftresp.
right
of theorigin,
p _ p +(the
drift in the process is directed toward theright).
p is thencompletely
determinedby fixing
its location in space.Call
finally M (p)
the manifold in X obtainedby rigidly shifting
in allpossible
ways theprofile
p.Any
such manifold is invariant under theevolution described
by (1.1)
and eachpoint
in the manifold moves withconstant
speed c =1- p _ - p + .
Onemight
argue that the state of theparticle
model isonly approximately
describedby
thedensity profile
of atraveling
wave p, hence to a betterapproximation
it should berepresented
in X
by
some "thin tube ofprofiles".
In thelong
timeregime
such tubemight
beamplified
and becomemacroscopic.
Whatreally happens
is hardto decide
by looking
at(1.1)
alone. From one side suchequation
seemsto indicate that each
traveling
wave p is stableexcept
for a neutraldirection,
that ofM ( p).
This wouldsuggest
that theonly
effect atlong
time should be a delocalization of the solution inside
M ( p).
However suchclaim comes from the
stability analysis
w. r. t. localized initialperturb- ations,
achange
in thelimiting
densities does in factproduce
a transitionto some new manifold M and such disturbance would never vanish. It is not clear at
all, by
the way( 1. 1)
isderived,
if theparticle system’s
evolution is in any sense related to what
predicted by
somestability analysis
for themacroscopic equation and,
if such is the case, what is the correct space where thestability problems
should be considered.Partial answers to such
questions
have been obtained for theasymmetric simple exclusion,
as wereport below,
for more details we refer to[24].
Ifp- = 0
it has been proven,[29]
and[9],
thatM ( p)
is stable and that theshock, moving
with averagespeed
c, fluctuates in spacekeeping
the sameshape,
its motionbeing
brownian with diffusion coefficient D = c. Even when p _ > 0 and c = 0 there are indications for the same behavior.Andjel
Bramson and
Liggett [1]
have in fact proven thatasymptotically
in timethe state of the
system approaches
a1/2-1/2
mixture of the states withdensities p_ and p +, the left and
right asymptotic
densities at theshock, just
what should be if theprofile
wererigidly fluctuating
with Brownian motion.Finally
we mention that a numericalanalysis, [4],
showsagreement
with theabove
behavior also in other cases.Let us now return to the
weakly asymmetric simple
exclusion process.The first
step
inanalysing
thestability
of the shock is to look at thedensity
fluctuations and that is what we have done here: we have found that thedensity
fluctuation field(cf
the next section forprecise
definitions andresults)
converges to ageneralized
Ornstein-Uhlenbeck process withzero mean. Its covariance kernel
diverges
when t - oo in the same way it should if the shockprofile
were stable butfluctuating
around its average location like a Brownian with diffusion coefficient D. We havecomputed
D and we have checked that its value agrees with that found in theasymmetric
case forp_=0.
Wehope
tocomplete
theanalysis
of thelong
time behavior of the shocks for theweakly asymmetric
exclusionprocess in a
forthcoming
paper.We conclude this section
by mentioning possible byproducts
of ouranalysis
which may beinteresting
in their own. We couldeasily
consider the multidimensional case andquite arbitrary particles jumps,
for notationalsimplicity
we have restricted ourselves to the one dimensional case and to nearestneighbor jumps.
We also have thepossibility
to deriveequations
of the form
mER, r E R, f
and V smooth real functions. The case V = 0 in( 1. 2)
isobtained
by adding
to thesymmetric generator
of thesimple
exclusion asmall
asymmetric perturbation
describedby
theasymmetric generator
ofa
"speed change
exclusionprocess",
which then determines the formof f:
Annales de l’lnstitut Henri Poincaré - Probabilités et Statistiques
To obtain the full
equation ( 1. 2)
weinterpret particles
andempty
sites as 1 and -1spins, respectively.
We then add to theprevious generator
a"small"
generator describing
local Glauber interactions amongspins,
see
[7]
where theequation
withf = 0
was derived. Ourtechnique
shouldapply quite straightforwardly
also to these cases, we are indebted to Sznitman for veryhelpful
discussions on thesepoints.
It is also worthmentioning
that we canstudy
cases where the "weak"asymmetric part
of thegenerator
of thesimple
exclusion ismultiplied by
a"slowly varying"
factor which may
depend
both on space and time.In Section 2 we state the main definitions and results and in Sections 3 and 4 their
proofs.
2. DEFINITIONS AND RESULTS
Let
S~ _ ~ ~,
be the set of allparticles configuration.
We denoteby
r; a
generic
elementof n, so ~ _ ~ ~ (x),
For any E > 0 and anycylinder
functionf
on Q letwhere
We denote
by T£ (t)
the Markovsemigroup
withpregenerator Lg,
andwe call such process the
weakly asymmetric simple
exclusion process(WASEP).
We denoteby TO(t)
the Markovsemigroup
withgenerator Lo,
such process is called the
symmetric simple
exclusion process(SEP).
We shall use the
following
notation. p, v denote measures on(.)
isthe
expectation
w. r. t. p whileE~
-Jl(T£
denotes theexpect-
ation off
w. r. t. the WA SEP with initial measure p. Sometimes we shallsimply
writeE~ ( f ).
2.1. THEOREM. - Let p be a smooth
function
on R with values in[0, 1].
For
~ > 0 let ~ be the product
measure such that(11 (x))
= p(E x).
Thenfor
any r E Rand t > 0 anduniformly
in the compactsofRxR+
where p solves
For any
~~03A9
define to be the solution of thefollowing equation
where
P~
is theprobability
kernel of thesemigroup TO (t).
ThereforePE (x,
t|~)
is the discreteapproximation
to(2 . 4),
x and tbeing
"micro-scopic"
variables in contrast to themacroscopic
variablesappearing
in(2. 4) : namely microscopic
space(resp. time)
isE -1 (resp. E - 2)
times themacroscopic
space(resp. time).
Definepg(x,
as in(2. 5) with ~ (z) in
the first term in the r. h. s.
replaced by (z)) = p(EZ) (cf
Theorem2 . 1).
Define for any
t>O, n >_ 2
for anyx --_ (xl,
..., where xl, ..., xn are distinctsites,
and
2.2. PROPOSITION. - With the above notation and
definitions, for
anyn >_ I and T > 0 there is c such that
for
any r~The above
Proposition gives
thekey
estimates for ouranalysis,
all theresults we obtain are more or less
straight
corollaries ofProposition
2. 2.In fact
using
such result it ispossible
to derive astronger
version of Theorem 2.1weakening
theassumptions
on the initial state. For instance it ispossible
to consider afamily
such that for anycp E S (R)
Annales de 1’Institut Henri Poincaré - Probabilités et Statistiques
and the same result as in Theorem 2.1 holds. We shall not discuss further this kind of
generalizations
andproceed
in ouranalysis.
Next we define the fluctuation fields. For cp as above and for
~.£
as inTheorem 2. 1 we set
and let P" be the
corresponding
law onD(R+ -~S’(R))
inducedby
theprocess with initial measure
~.
We then have ,2.3. THEOREM. 2014 The law P~ defined above converges
weakly
to thelaw of a mean zero
generalized
Ornstein-Uhlenbeck process with covari-ancc kernel
C~(r, r’)
determinedby
theequation
~C~~, r)
where
Ct
satisfiesFurthermore let p in Theorem 2.1 be a
stationary
shock wave solutionto
(2. 4)
such thatnamely p ( r, t) = p (r - c t)
where thespeed c =1- p _ - p + .
Then f or any rand r’
where
p’
is tthe first derivative of p andNotice that the different time covariance solves the linearized
equation [ef
eq.(2.10)].
This is ageneral
feature related to thevalidity
of theFluctuation-Dissipation
theorem and provenrigorously
for several stochas- tichinteracting particle systems.
Thesplitting
of C* as in(2 . 10 b)
appearsnaturally
whentaking
theexpectation
of the square of the fluctuation field. Thediagonal
terms whenexpanding
the squaregive
rise to the 03B4-term in
(2 . 10 b).
The other termCt(r, r’)
is a smooth function whose evolution isagain
determinedby
the linearizedBurgers equation
to whicha term is
added,
the last term in(2 . 10 d)
which isresponsabile
for thelinear
growth
ofCt
as t - oo . To relate such a behaviour to what discussed in the Introduction we argue as follows.Let ~,E, r,
t be
theproduct
measure such thatTheref ore
is just
the initial measure shiftedby E -1 [ct + r].
Letwhere 16,
(dr) is
the law at time t of a Brownian motionstarting
from 0 andmoving
with diffusion coefficientE D,
Dbeing
the same as in Theorem 2. 3.Given
cp E S (R)
let cpt(r)
= c~(r
+ct), then, obviously,
Therefore the true covariance of the WASEP is the same as that
produced by hE, t,
hence as far as thiscomputation
is concerned it is like the initialmeasure were
only
shifted in spaceby E -1 [ct + r],
the law of rbeing
The above motivates the
conjecture
that for any t > 0 and rwhere the 1. h. s. denotes the law of the
weakly asymmetric simple
exclusionat time
E-3 t
shifted in spaceby
theinteger part
if the initial measure is thesame
as at the end of Theorem 2. 3 and y~ is the law of a Brownian motion with diffusion coefficient D.3. SHORT TIME ESTIMATES
In this section we prove
Proposition
2.2 for timest s- ~ + ~, [3 > 0.
Westart with Lemma 3. 1 where we derive an
integral equation
for the v-functions defined in eqs.
( 2 . 6), ( 2 . 7) .
Tosimplify
notationwe just
writevn
(x, t)
foreither vn (x, t Ti) or v~ (x, t ~E);
the statements below hold forAnnales de I’Institut Henri Poincare - Probabilites et Statistiques
both. We also define
1,
as the set of alln-tuplets
of ordered distinct sites ofZ,
x= (xi,
...xn) denoting
thegeneric
element inN"
andEx
theexpectation
w. r. t. the SEPstarting
from x.~
where
and
We are
using
thefollowing
notation:for
x E zn,
x(i)
--_xB{ xi}
and x(i, j)
-_-xB{
xi, xj}(3 . 3 a)
is the unit vector in the
positive i-direction, i = l, ... , n.
~
is the sum over alldisjoint pairs i and j in { 1,
...,n ~ (3. 3 b)
i, j
Proof - By
definition for anyt > 0,
We use
(2. 2)
and(2. 5) distinguishing
the cases whenparticles
are n. n.from the others. We
get
termscontaining products
of theoccupation
number
functions 11 (correlation functions)
with n,n+ 1,
n-l and n - 2-body.
To recover the v functions we add and substract themissing 03C1~’s
and we
get
For
t >__ 0
let _vt be thefollowing
function defined on the subset ofconfigurations
with nparticles.
If thenVt
(11)
= vn(x, t)
where n is the number ofparticles
in theconfiguration 11
and x are their
positions. Since vn
issymmetric
underpermutations
of theXi in x the above is well defined. For
simplicity
weidentify
the elements of withpoints
and write the first term in( 3 . 5)
as( Lo v") (x, t).
It is easy to see that the second one is
(R vn) (x, t).
We consider next theterms with Vn-1’
By adding
andsubtracting
PE(xi, t)
Vn-1(x (j), t)
we rewriteAnnales de l’Institut Henri Poincaré - Probabilités et Statistiques
the fourth sum in
(3. 5)
as a sum of a"gradient"
of Vn-1plus (x (j), t)
times
ce,
as defined in( 3 . 2 d).
Thegradients
of vn _ 1 aremultiplied
as defined in
(3 . 2 c).
From the above observations it follows that the time derivativeof vn (x, t)
isequal
to(Lo vn) (x, t) plus
the other terms. Thereforewe can use the process with
generator Lo
to write anintegral equation
for vn. We therefore
get (3.1)
since3. 2. NOTATION. - We can
interpret
theright
hand side of(3. 1 a)
as theexpectation
withrespect
to a processdescribing n
labeledstirring particles
which starts from x move for a time t - s and then
undergo
abranching
process.
[We
arethinking
of thedegree
of the v-function as a number ofparticles,
theirpositions being specified by
thearguments
of the v-functions].
We recall that thestirring
process is realizedby independently exchanging
theoccupation
numbers at allpairs
of nearestneighbor
sitesafter an
exponential
time of mean 2. The induced motion on theparticles
is the
SEP,
if the labels of theparticles
areignored.
Since
W
can beexpressed
as a linear combination of v-functions the different terms areinterpreted
as the outcome of thebranching.
To describethis structure we
specify
first of all the initial and the final number ofparticles.
So the termsappearing
inR vn
are all of"type (n, n)",
those inthe first sum of
( 3 .1 b)
are( n, n + 1 ),
the successive ones are( n, n - 2), (n, n-1)
and(n, n) respectively.
A finerdescription
is needed toclassify
the
single
terms in eachtype.
We start with the( n, n - 2)
terms. We needtwo more labels which denote the
particles appearing
in the characteristic function in(3.1 b).
Hence each of these terms is determinedby
the multi-index
( n, n - 2, j, i).
The( n,
terms aresingled
outby adding
themulti-index
(j, i, c) where j
asbefore,
denote theparticles
involvedin the characteristic function
appearing
in(3.1 b)
while 03C3equals
± 1 or 0.If a = 1 we are
considering
the first term with(x (j), s),
theterm with vn _ 1
(x (i), s),
if 03C3 = 0 the last term with v" _ 1(x (j), s).
The terms of
type (n, n)
are divided into two classes. Those in the firstone are
singled
outby specifying
apair (j, i), cf (3 .1 b).
The others comefrom
R vn.
Toclassify
them one needs thepair (i, ?).
The firstindex, i,
labels a
particle, cf (3 . 2 a),
while ~ =1 refers to the first term in( 3 . 2 a),
o = 2 to the
second,
..., 6 = 5 to the fifth one.Finally
the(n, n+ 1)
terms can be written aswhere the sum over
... , ik
is over all the subset with k elements of the set(1,
...,n).
Therefore these terms are classifiedby
thespecification ( i 1,
...,ik, cr),
wherefi, ... , ik
are as above and a =1 selects the first term in the above sum while c = 2 the second one.Therefore the
branching
processoccurring
at time( t - s)
describesbirths,
the
( n, n + 1)
terms,deaths,
the( n, n - 2)
and( n, n -1 )
terms, as well as terms with same number ofparticles,
the(n, n)
terms. In some of thesecases
particles
after thebranching
aredisplaced, and,
as we shall seebelow,
it will be convenient to relabel some of theparticles
after thebranching.
Of course new labels are needed for thenewly
bornparticles.
One more notation: to
classify
the various terms above we introduce alabel X which can take any of the multi-indexed values we have introduced above to
single
out the terms in(3.1).
Therefore a value of 03BBspecifies
one of the terms in
(3 . 1),
inparticular
a v-function and a function of E, x and a whichmultiplies
the v-function. This function will be denoted as s,03BB).
For instance if03BB = (n, n - l, j, i, 0)
then thecorresponding
d-function is xi,
s).
Because of the presence of the terms
( n, n + 1 )
theequation relating
thev-functions is an infinite
hierarchy
ofequations:
theexpression
for vn involves Vn+1 which in turns involves Vn+2 and so on.By looking
at timessmaller than
E - 2 + ~, j3 > o,
it ispossible
to control the abovehierarchy.
This is a consequence of the
integral
in( 3 . 1 a) :
the time intervalE - 2 + ~
is"so short" that the successive iterates of
( 3 . 1 a) eventually
becomenegligi-
ble. So we fix
~3 > 0
and thedegree m
of the v-function for which we want to prove(2. 8).
We then iterate(3 . 1 a)
Ntimes,
where Ndepends
on mand
fi
in a way which will bespecified
later on. At most,therefore,
therewill be m + N
particles,
but we may need to introduce otherparticles,
atmost
N,
so that the set of necessary labels for all theseparticles
is(1,
..., m,m + 1,
...,2 N).
The first m labels are used for the initial mparticles,
hereafter referred to as the "oldparticles";
then each newparticle appearing
at abranching
is namedby using
the next available label in the above list.According
to theparticular
branch that we consider we mayor may not use all the labels in the list. In
particular
no new label isneeded for all the
( n, n - 2), (n, n -1 ), (n,
n,j, i)
and( n,
n,i, ~ = 5)
terms.For all the other
(n, n)
terms we add an extraparticle.
For the term(n,
n,i, 1)
theparticle
i is atXi - 1
and the newparticle
isplaced
at Xi’ If~ = 2 the new
particle
isplaced
at if 6 = 3 the iparticle
is atwhile the new
particle
isplaced
at xi.Finally
if cr=4 the newparticle
isplaced
atXi+ 1.
For the
( n, n + 1 )
terms wealways
add 2particles
one at thebeginning
of the cluster the other at its
end, cf
Notation 3. 2 above. One of them is"real",
i. e. it appears in theargument
of thev-function,
the other one isfictitious.
Annales de l’Institut Henri Poincaré - Probabilités et Statistiques
One final notation which refers to the
(n, n - l, j, i, a) when j _ m
andi>m
or j > m
and In the first case ifa =1,0
we label theparticle
inxi
as j particle
and that inx~ (which
ismissing
from theargument
of thev-function)
asparticle i,
so that the "old"particle
survives.If j > m, i m
and
a = -1,
weagain
switch labels between iand j.
Using
the above notation we havewhere the
functions
are defined at the end of Notation3. 2;
notice also that for notationalsimplicitly
we have notexplicited
thedegree
of thev-functions which can be desumed from their
argument.
If k N then thesum is meant to be restricted to
Àk
such that the final number ofparticles (after
the k-thbranching)
is 0 hence at the end there is no v-function. If k = N then the final number ofparticles,
asspecified by might
bedifferent from
0, namely
theconfiguration
x(t
-+, appearing
after thelast
branching
may be nonempty.
The sum in(3.7)
is over all suchpossible À1,
...,Àk
and theexpectation
refers to thestirring
process in the time intervalsplus branchings
at the timest-si
asspecified by
the values of The labels of theparticles
aregiven according
to the notational convention described before.
A
separate
bound on each of the terms in(3. 7)
wouldgive
the wrong result since there areimportant
cancellations among the different terms.These
origin
from the differences among v-functionsappearing
in(3.1)
and
(3. 2).
We need to estimate differences likeThe case 1~ =1 appears in some of the
( n, n -1 ), (n, n)
and( n, n ~-1 )
terms, while k> 1 occurs in the terms(n, n + 1, ii,
...,ik, s), cf (3. 6).
From
(3.1 a)
we then havewhere
x (t - s) (i)
is aconfiguration
of n -1stirring particles
obtained from theconfiguration x(t-s) by subtracting particle i;
x(t - s) j)
is definedanalogously.
Here we have used the fact that themarginal
over the motionof a subset of
stirring particles
is still a process ofstirring particles.
To estimate
(3.9)
we use acoupling
betweenstirring
andindependent
particles, cf [12].
Coupling
nstirring
with nindependent particles
Let
a + , ~, a _ , 1, i =1,
..., n be thefollowing operators
onNn = the
subsetof Z" of n ordered distinct sites.
x+ei
if forall j
a I,
’ i x =~ x +_ ei - ( ± e~) x if there if there is j is j
such that such that x; ± 1= x~ and j
i i ( 3 .10)
If f is
a real valued function onNn,
defineGn f as
then
Gn
is thegenerator
of a Markovjump
process whose law is the sameas that of the
stirring
and the exclusion processes, for the last one the labels of theparticles
areneglected.
In fact themarginal
of such processover functions invariant under
permutation
of the labels is theSEP,
sinceGn f (x)
=Lo f (x)
iff
issymmetric.
The
independent
process has agenerator G~
which acts on the functionsDefine a
generator G~
onN"
xN~
as follows:It is
easily
seen that themarginals
of the Markov process withgenerator G,*
onNn (resp. N~)
have same law as thestirring (resp.
independent)
process, hence thejoint
process is acoupling
of the two. Inparticular
from(3.13)
it follows that withprobability
1 for any i and tXi (t)
iscompletely
determinedby
thespecification
of(s), j
=l,
..., i and 0 _ s _t ~.
In fact from(3 . 13)
it follows that anyjump
of thestirring particle
inecessarily
induces ajump
at the same timeof some
independent particle xJ with j
i. The rule is that whenever anindependent particle,
sayparticle i, jumps by +1
then thestirring particle
ialso
jumps by
±1,
unless it would go to a siteoccupied by
someparticle j with j i.
In such case thejump
issuppressed.
On the other handif j >
ithe
jump
takesplace
and thestirring particle j
makes theopposite jump,
i. e. it moves
by - ( ± 1).
We shall therefore say thatparticle
i is of first class[or
that it haspriority]
w. r. t.particle j if j >
i. In this case we alsosay
that j
is second class w. r. t. i. Particle 1 is first class w. r. t. all the others and it movesjust
the same as theindependent particle
1.Annales de l’lnstitut Henri Poincaré - Probabilites et Statistiques
Other
couplings
can be introducedby simply changing
thepriority
list:... , ~ (n) ~
be apermutation of {1,
...,n ~.
DefineG,* ,~
iseasily
seen to defineagain
acoupling
of thestirring
andindependent
processes, which will be called thex-coupled
process. In such processparticle ~ ( 1)
has thehighest priority,
it moves the same as theindependent particle ~ ( 1).
Then comesparticle ~ (2)
with secondhighest priority
and so on. Thereforex,~ ~i~ (t)
isspecified (modulo zero) by (xn ~ 1 ~ (s),
...,(s)
for all 0__ s t).
We now go back to
( 3 . 8)
and introducef or i, j, k
as in( 3 . 8)
and any s > 0 thefollowing stopping
time on the space(Nn
and for T > s we set
Then from
(3.6), setting
where the
expectation
refers to thecoupled
process with iand j having top priority; x°
is anarbitrary configuration
of nindependent particles.
To prove
(3.16)
we observe that thedisplacements
of Xi andx~
are thesame as those of
x?
andx°
till time(0),
since theparticles
iand j
havetop priority.
At time(o) +
the distribution of thestirring particles
issymmetric
under thepermutation
ofparticles
i andj.
Therefore if then the distribution ofx ( t - s)
issymmetric
under thepermutation
of thepositions
ofi and j,
hence such a subset oftrajectories
does not contribute to the difference vm
(x (z), t)
- vm(x (j), t).
Afortiori
thisoccurs when
i~k~ y (o) (t - s)/2,
so that( 3 .16)
is proven.We can now write
( 3 . 7)
aswhere the
following
notation have been used:firstly g(h)
stands for wherei, j,
k arespecified by ?~h
if~,h
refers to a branch-ing
where a difference of v-functions appears, otherwise itequals
1.8 x
denotes the
expectation
withrespect
to a process whose law isspecified
once
~,1, ... , Àk
and aregiven.
In the time intervalsthis is a
coupled stirring + independent
process whosepriority
list isspecified by Àh.
If att - sn
there was not a v-difference then thepriority
list is chosen in anarbitrary
but fixed way. If on thecontrary
there was a difference of v-functions then twoparticles
are involved in such a difference and thepriority
list has these 2particles
withhighest priority.
Theindependent
and thestirring particles
start both from x. Thebranching
for thestirring particles
isspecified by
thevalues Àh
as describedabove. The whole process is then determined
by saying
that when a newstirring particle
is added at some of thebranchings
then anindependent particle
with same label is added on the same site and when astirring particle
dies thecorresponding independent particle
alsodisappears.
Thefictitious
particles,
which are added to take into account thev-differences, play a
roleonly
in the time intervalst - Sh + (sh - sh + 1)I2~
if at theh-th
branchincing
such a v-difference waspresent.
So we say thatthey disappear/die
at the end of this time interval.We use the
following key
estimate proven in[10]:
3. 3. PROPOSITION. - Fix n,
x=(xi,
...,xn) E Nn, oc > 1 /4
and letPx be
the law
of
anyof the couplings previously defined
between thestirring and
the
independent
processes, bothstarting from
x. Thenfor
any m there is cindependent of
x such thatfor
all T > 0As a
corollary
of the aboveProposition
we have3 . 4. COROLLARY. - Let
k _ N,
s 1, ..., sk, 03BB1, ...,03BBk, Ex
be as in(3. 17).
Let a be anypositive
number. Thenfor
any n there is cso
that where h is the characteristicfunction of
the eventWe fix a sequence s i, ... , s~, ...,
Àk
and denoteby
J thecorrespond- ing
term in(3.17). Calling
G the set of valuesof Ài
for which there is adifference of
v-functions,
thenusing
theCorollary
3. 4Annales de l’lnstitut Henri Poincaré - Probabilités et Statistiques
where
and
The contribution to
( 3 . 17)
of the second term in( 3 . 19)
is boundedby
c
2N,
since there are at most Nintegrals
eachranging
in the interval[0,
£ - 2 + a].
Hencechoosing
nlarge enough
this can be made smaller than theleft side of
(2. 8),
so we canignore
it in thisproof.
Our aim now is toestimate
J~ uniformly
on theconditioning
sothat,
afterinserting
thisbound,
theexpectation
in(3.19) only
involvesindependent
random walks.The main
difficulty
consists intaking
properadvantage
of those charac- teristic functions which may appearin dE
and whichrequire
that certainpairs
ofparticles
should be atneighbor
sites. We shall useCorollary
3. 4to reduce these to conditions
involving independent particles.
Even afterthis, however,
theanalysis
will not be verysimple
because of thebranching
structure of the process which creates correlations in the motion of the
particles.
To have asimpler
structure we shallget
rid of some of these conditions. We can do this in some of the terms withoutaffecting
thebound we aim to prove. With this in mind we
give
thefollowing
DEFINITION. -
(i)
Aparticle
is calledauxiliary
if it is not "old" and it diestogether
with an oldparticle.
Particles which are neither old norauxiliary
are called "normal".(ii) Let e£ (x,
s,À)
be the function obtainedfrom d~ (x,
s,À) by dropping
those characteristic functions
possibly present
in the latter whichonly
involve normal
particles.
(iii)
Let i be the label of anauxiliary particle,
theno (i)
denotes the label of the oldparticle
which dies withparticle
i. Furthermore t(f)
denotesthe time when i was
born, t’ (i)
when it dies and xi, theposition
attime t
(i)
ofparticles i
and o(i).
We can now relax the conditions on the death of the old and the
auxiliary particles,
remind that we havedropped
the conditions on the normalparticles.
Let us consider for instance a conditionreferring
to thedeath of an old and an
auxiliary particle,
sayi,
o(i)
and let t(0, t’ (i)
beas in the definition above. Then if h =1 and