A NNALES DE L ’I. H. P., SECTION A
M. I RAC -A STAUD
Perturbation around exact solutions for nonlinear dynamical systems : application to the perturbed Burgers equation
Annales de l’I. H. P., section A, tome 53, n
o3 (1990), p. 343-358
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343
Perturbation around exact solutions for nonlinear
dynamical systems: application to the perturbed Burgers equation
M. IRAC-ASTAUD
Laboratoire de Physique Theorique et Mathématique,
Université Paris-VII, 2, place Jussieu, Paris, France
Vol. 53, n° 3, 1990, Physique théorique
ABSTRACT. - When two
dynamical
systems of nonlinearpartial
differen-tial
equations
differby
a term that can be considered as aperturbation,
their solutions
equal
at the initialtime,
can be relatedby
a linearintegral equation.
Due to thisequation,
if the solution of one of these systems isknown,
let us call itfree,
the solution of the other one, theperturbed
one,can be written as a
perturbation expansion,
the terms of which arecompletely explicit expressions
of the free solution. Thisgeneralises
theusual
perturbation
theories around free solutionssatisfying
linear equa-tions. The
perturbed Burgers equation
is taken as anexample.
wRESUME. 2014
Quand
deuxsystèmes dynamiques d’equations
non-linéairesaux derivees
partielles
different par un termequi
peut etre considerecomme une
perturbation,
leurs solutionségales
a l’instant initial sont reliees par uneequation integrale
linéaire. Grace a cetteequation,
si lasolution de l’un des
systemes
est connue, nousl’appelons
la solutionlibre,
la solution de
l’autre,
solutionperturbée,
peut etrereprésentée
par undeveloppement
enperturbations
dont les termes sontcompletement expli-
cites en fonction de la solution libre. Ceci
generalise
les theories deperturbations
autour de solutions libres satisfaisant desequations
linéaires.L’equation
deBurgers perturbee
est traitée commeapplication.
Annales de l’Institut Henri Poincare - Physique théorique - 0246-021 1
INTRODUCTION
A
dynamical
system is calledperturbed
when it differsby
aperturbation
term from a free one, the solutions of which are
supposed
known.Denoting by F
the space of the smoothmappings
of [Rn in RNand 6 the set of the
mappings
from ~ into ~we consider the system
where
v (t) belongs
to ff and F to 6. This system is assumed to be solved for vsatisfying
the initial conditionit is what we call the free system. The most
general perturbed
system can be written on the formwhere
S~)=F(~+~N(~) belongs
to C. The functionalF (t)
is the free part ofS~ (t),
and N(t)
itsperturbative
one. These functionalsdepending
on t can be local and contain differential operators with respect to x, for instance
F t y]=a(t)~ ~x1 ~ ~x2y3. They
can as well be nonlocal and asso-J - o0
interested with the solution of
(5) satisfying
the sameboundary
condition as v
The
parameter X
thatmultiplies
theperturbation
term can have aphysical significance (for instance, X
can be acoupling constant)
or can beartfully
introduced in a system that cannot be
exactly
solved in order to get anapproximate
solution. Numericalphysical perturbed
systemscorrespond
to
dynamical
systems submitted to external forces that may be random ornot, the
perturbation
term is then a stochastic or a classical function.When an exact closed-form solution of the system
(5)
can’t befound,
we intend to relate it to the solution of the system
(3), assuming
that thesolutions of the two systems
(3)
and(5) corresponding
to the same initialconditions
(4)
and(6)
areclose,
at least in aneighbourhood
of~=0,
t = s.
Supposing analytical
the solution u of theperturbed
system, theAnnales de l’Institut Henri Poincaré - Physique théorique
perturbation
method consists inseeking
it in the form of a power series in~, u = ~
The coefficientsUn
can berecursively determined, they
n>_0
satisfy
a linear system[1],
the coefficients of whichdepend
on theUi,
i n,Uo being
the solution v of the free system.Solving
this system isnot
always possible
and when itis,
notalways
easy[2].
We propose herean
explicit expression
of these coefficients in terms of the free solution v.This
expression
is obtainedby iterating
a linearintegral equation relating
the solutions u and v ; we establish this
integral equation
in Section I.In the case where the free
equation
islinear,
we show on anexample
that this
perturbation theory
leads to the usual one where theperturbed
solution is
expressed
with the Green functioncorresponding
to the freeequation.
In this paper we obtain the solution of the
perturbed
system(5)
interms of the solution of the free one even when this last is
nonlinear,
these solutions
coinciding
at the initial time ~==~. Thisapproach
differsfrom
approximate
methods that look forparticular solutions, solitons, nearly periodic [3]...
In Section
II,
weapply
this result to the case of theperturbed Burgers
equation rl1 that isHere,
isequal
Nbeing
anarbitrary
6~
6~
functional of u. The solution of
equation (7)
with~=0,
theBurgers equation, being
known[4],
the coefficientsU~
arecompletely explicit.
I. INTEGRAL
EQUATIONS
RELATING THE PERTURBED AND THE FREE SOLUTIONSFirst we deal with a more abstract and
general problem
that we willuse to solve ours in the
following.
Let
iF
be any vector space and the space of themappings
fromW
intoff o.
The flowbelonging
to is definedby
thefollowing semi-group properties
where O is the
composition
law for themappings
inlff 0
andwhere I is the
identity
in~o .
Let us introduce now the substitution
operator ~ s
related to the flowbelonging
to 2($0’ $0)
and definedby
In
particular
when F isequal
to theidentity I,
this formula readsThe
semigroup properties
of the flowgive
where the
product
in theright
hand side is theproduct
of operators. From the formula(9),
we havewhere I is the
identity
in 2(fff 0’
The field
S~ (t)
associated to theoperator ~ s
is definedby
From the
equations (12)
and(14),
we deducethat reads
The property
( 13)
acts as the initial condition.Equation (12)
whereand
equation ( 13)
lead toThe differentiation with respect to t of this last
equation
and theusing
offormula
(16) give
Assuming
that the fieldSf (t)
takes the form F*(t) +
A N*(t),
we introducethe flow 03A8 and the operator Bf*
reducing
to 0 and 1>* when A vanishes.The
problem
we are interested in is to relate theoperator ~ s
thatsatisfies the
equation ( 16)
with Aequal
to zero that isTo this
aim,
let us calculateAnnales de l’Institut Henri Poincaré - Physique theorique
and
The
integrations
of theseequalities
on the interval[s, t]
lead toand
These two
equations
relate theoperators 03A6*ts and 03A8*ts.
Their iterations canbe
performed
and lead toanalogous results,
the onecorresponding
to(23) gives
In this relation the
operator ~ s
isexpressed
in terms of ~F*. Let ussummarise this result:
Let a substitution
operator 03A6*ts belonging
to 2(80, E0), E0 being
thespace
of the mappings from
a vector spaceF0
intoitse f, satisfy
adifferential
e uation:
~ ~t
03A6*ts= 03A6*ts( F* t + 03BB N* t with the condition that 03A6*ts is theidentity
when t = s. Theoperator ~ s
is related toW*,
its value when ~, =0, by a functional equation (23)
that can be solvedby
iterationgiving
anexpression of og
in termsof
~I’*(24).
This result was
already
established in the casewhere ff 0
is a realmanifold of dimension N and
applied
toordinary
differentialequations [5].
We now use this result to deal with the initial
problem
which we wereinterested in. We first formulate it in a convenient form. We consider the
case where the space
3’
is the space ff defined in formula( 1 ). Remarking
that
u (t),
solution of theequation (5)
and(6),
is a functionalof y, depending
on the initialtime s,
we can express it with thehelp
of theflow
~
belongs
to the space $, defined in formula(2).
Vol. 53, n° 3-1990.
We introduce several linear operators
acting
on ~:We will use the operator
Vx
that associates to any element of 6 its value in x; for instanceThis is the
analogous
to the operator"projection
on acomponent"
in afinite vector space. Here both exist:
The operators
Pi
andVx
commute.We associate to an element
of
F(t),
thefield,
F*(t), belonging
tolet us remark that F*
(t)
is an operatordepending
on y.In
particular,
we haveIn the
following
we will denoteTo the two functionals and
F (t), appearing
in theequations (5)
and(3), correspond by
the definition(28)
the fieldsSi (t)
and F*(t), belonging
to ~ The
operators 0~
related to the flows andare solutions of the formulas
(16)
and(19)
if the functionsu (t)
andv (t)
are solutions of the systems
(5)
and(3).
Theproblem
ofrelating u (t)
tov (t),
solutions of(5)
and(3),
reduces to that ofrelating
O* to B}I*satisfying (16)
and(19)
for which we canapply
theprevious
result. The twoequations (22)
and(23) acting
on anarbitrary
functionalQ
of lff furnish twointegral equations relating
the functionsQ [u (t)]
andQ [v (t)]
Annales de l’Institut Henri Poincaré - Physique théorique
and
These
equations correspond
to that obtained in[V]
when the variable xdoes not appear in the
dynamical
system.They relate, by
an inte-gral equation,
anyphysical quantity
of theperturbed
system, expres- sed in terms of u, to thecorresponding
one of the free system. Forinstance,
when thedynamical
systems are theBurgers equation, (7)
with
03BB=0,
for the free one and theKorteveg
DeVriesequation,
that is~u+u~u+03B1~3 ~x3u=0
for theperturbed
one, thecorresponding
at ax ax p
physical
quantities
are relatedthrough
the formula(31)
with, v .n. / v rw
The formula
(31 ),
whenQ
isequal
toVx Pi I,
readsThis
integral equation
is linear with respect to u and therefore easy to iterate. Theanalogous
one obtainsby using (32)
is linear with respect tov and nonlinear with respect to u
This last formula is
interesting
because it furnishes anexplicit
functionalequation
for u, theintegrand
can be calculated as soon as v is known.Let us illustrate this property on an
example:
theperturbed
diffusionequation, that is
with
After
introducing
the diffusion kernelthat satisfies
the solution of the free
equation,
linear in this case, takes the formThe
integral equation (34)
reads in this caseThis
integral equation
furnishes the powerexpansion
with respect to A of the solution u of(35)
in terms of the diffusion solution v(39).
We cancompare it to the
integral equation
obtaineddirectly
from(35) by using
the Green function e
(t)
~corresponding
to the free linearequation
To furnish a power series in
~,
thisintegral equation
has to bemodified,
that is it must be put on the form
(40).
This is obtainedby suitably introducing
in theequation (41 )
the initial condition(36)
written as followsTherefore the formula
(40)
and the usualperturbation expansion
lead tothe same result in this
particular
case, this is the same for any free linearequation.
The iteration of
(33) gives
the same result as the formula(24) applied
to it furnishes the i-th component of the function
u [t,
s;y]
as apower series in À. The coefficient
Uk
of À k is atriangular integral
of orderk the
integrand
of whichffk [t,
r;1,’ .., r;k, s, x;y]
iscompletely explicit
interms of the function v and its derivatives with respect to y:
It can be
recursively
constructed from thepreceding
oneIn the next section we
apply
these results to the case of theperturbed Burgers equation (7).
Annales de l’Institut Henri Poincaré - Physique théorique
II. PERTURBED BURGERS
EQUATION
First let us recall that the
equation (7)
when ~, isequal
to zero, can be linearizedby introducing
the function v such as[4]:
where v t,
s, x;y]
is aprimitive
of v with respect to x. We can wrtie v onthe form
The function v is solution of the diffusion
equation
with the initial condition deduced from
equations (4)
and(45)
~ ~ 1
where
y(x)
is aprimitive
of y. The solution v of(47)
and(48)
takes theform
~..J,.."" ". - v
where ~ is the diffusion kernel defined in
(37).
Thisexpression replaced
informula
(46) gives
theBurgers
solution v ; for theorems of existence seefor instance
[4].
Considering
now theequation (7)
with X different from zero, we try to linearize it aspreviously;
let us define the function (D such asand
where ~, ~-;
~]
is aprimitive
of M with respect to ~-.Taking
back thisexpression
inequation (7),
we get~ ~7 ~
where ~ is the functional
equal
to aprimitive
with respect to x ofN [t,
x;u];
the constant ofintegration
with respect to x,C (t), depends
onthe choice of the
primitive ii,
and can be taken off withoutchanging
u.The function 03C9 fulfils the same initial condition
(48)
as the function v.The
theory
of the diffusion with an external source[2] gives
for thesolution of
(45)
Substituting
(o and vby
theirexpressions (45)
and(50),
we obtain anintegral equation relating
theperturbed
solution u to the free one v. Thisequation
isobviously
nonlinear in u and in v and does not suit to findeasily
the coefficientsUk,
when the directapplication
of the result of theprevious
section furnishesintegral equations
very convenient.The straithforward
application
of the formula(43) gives
theexpression
of the coefficients
Uk
The kernel Jf involved in the
chronological integral
aregiven by
for-mula
(43)
where the free solution v is
given by (46)
and(49);
theoperators ~I’ s
andN*
being
defined in(10)
and(28)
with thehelp
of the functional~ representing
the flow associated to v and of theperturbation
term Ninvolved in the
equation (7).
Let us calculate the first kernel
The functional derivative of v is obtained
by using (45)
and(49)
Recalling
theproperty
of the functional derivativeAnnales de Henri Poincaré - Physique théorique
and
replacing
vby
itsexpression (49),
we obtainPutting
this result in the formula(56)
andremarking
thatwe
finally
have for the first kernelIn this
expression
appears a modified diffusion kernelIts
primitive
with respect to x’can be written on the form
We remark that ~
trivially belongs
to[0,1].
The modified kernel satisfies a condition deduced from
(38)
Let us note that
and
A relation
analogous
to(67)
holds for ~.Introducing (62)
in(61),
the first coefficientU 1
can be written on the formAfter
performing
anintegration by
parts with respect to xl, it readswhere
JV
being
aprimitive
of N with respect to xialready
introduced in(52).
The
expression (70)
does notdepend
on theprimitive
JVchoosen,
forThe term
U 1
is theboundary
termWe can check that
Ui satisfies
the same linearpartial
differentialequation
as
U1;
thisequation
is obtainedby sustituting
uby
1 in(5)
andtaking
the first orderin À,
it readsMoreover the functions
Ui and Ü 1
fulfil the same initial conditionTherefore if
they exist,
these two functions areequal,
we say thatthey
are
formally equal.
Inpractice
we have twoexpressions
for the first coefficient(68)
and(70),
we have toverify
their existence, the one that exists is the coefficient we werelooking for;
wegive
anexample
at theend of the section.
By
ananalogous
calculus we can find the first order in A of the cinetic energyE[MJ=1/2~~
when thevelocity
u satisfies theperturbed Burgers
Annales de l’Institul Henri Poirware - Physique théorique
equation (7); using (31),
we haveThe term in À can be
easily
calculated and isequal
to theexpected
resultmvU1.
Now,
and this is the mainadvantage
of ourmethod,
the upper ordersare obtained
by
a calculusquite analogous
to thepreceding
one, that is very easy,though
the direct calculation of these termsby using
theexpressions (51 )
and(53)
isquite
difficult. Let usapply
the formula(44)
Let us first calculate
by using (59), (60), (62)
and(63)
The
straighforward
calculus of(76), using (59), (61 ),
and(77),
leads toAs for the first
order,
anintegration by
parts can beperformed
on thiskernel. It
replaces
the first term of theright
memberby
thefollowing
one,formally equal
to itLet us denote
the
primitive
ofUi
1 in which wespecify
the functionaldependence
with respect to JV. The contribution of the first term toU2
isequal
toThe last term is
just
It
corresponds
to the first order kernel ofas we can see
by writing
with thehelp
of the formula(24).
This termhappens
too in the calculationperformed
from theexpression (53)
of (o.If we don’t use the result of the
preceding
section to calculate thiskernel,
we have to do the
Taylor expansion
ofcomposed
functionals and this is not very easy.Therefore, already
for the second order kernel we can seethe
advantage
of the methodproposed
in this paper. For thefollowing
terms, the
straighforward application
of this method leads to calculations that can beperformed
without difficulties becausethey
usealways
thesame intermediate result
(77).
Finally
let us test our result in the case where the forcedBurgers equation
can beexplicitely solved,
that is in the case where N(~,
x ;y]
isequal
to a timedependent
function 11(t)
Let us consider the Miura transformation
[6]
and
Annales de l’Institut Henri Poincaré - Physique théorique
where 11 (t) and 11 (t)
arerespectively
theprimitives of 11 and 11 vanishing
for t = s. The substitution of
(83)
and(84)
into(82)
shows that u’ fulfils the freeBurgers equation
with the same initial condition as u, we therefore haveThis
explicit
solutiondevelopped
with respect to Àgives
for the two firstterms
and
Let us check that this last term coincides with
(70)
when N[t,
x ;y]
= 11(t).
We choose the
primitive
ofN,
~’[t,
x ;y]
to beequal
to 11(t)
x and wereplace
it in(70)
using
theequality
we obtain
that is
equal
to(87).
Let us remark thatcontrarily
to11
that is welldefined,
theexpression (68) giving U in
this case isambiguous,
it iswhy
we have to choose the
expression (70)
to test our result.By
ananalogous calculation,
theexpression (79)
leads to the second orderexpected
resultTo end let us
give
theintegral equation
deduced from(34)
for the presentexample
after a
integration by
parts. Inparticular,
whenthis
integral equation
stands for the solution u of theKorteveg
Devriesequation.
The
expression (91)
does nottrivially
reduce to thealready
foundequation (53).
Howeverby stressing
that theequation (53)
can be obtainedby applying
the relation(31 )
to the functionalQ[M]=co=exp( - 2014 ~
weestablish that both these
equation
result from the sameequation (31 )
or(22)
and therefore we relate themthough
it is difficult todirectly
connectthem.
In
conclusion,
the fact that theperturbation theory developped
inthis paper furnishes
completely explicit expressions
for the terms of theperturbation expansion
may be of course very useful for thestudy
of theconvergence
properties
of thisexpansion
or for thestudy
of thestability
of the
solution,
for which we have to examine eachparticular problem.
REFERENCES
[1] W. F. AMES, Nonlinear Partial Differential Equations in Engineering, Academic Press, Inc., Vol. 18, 1965, p. 208.
[2] I. N. SNEDDON, Elements of Partial Differential Equations, McGraw-Hill, New York, 1985.
[3] D. J. KAUP, A Perturbation Expansion for the Zakharov-Shabat Inverse Scattering Transform, Siam J. Appl. Math., Vol. 31, 1, 1976, p. 121; R. M. MIURA, The Korteweg- DeVries Equation: A Survey of Results. Siam. Rev., Vol. 18, 3, 1976, p. 412.
[4] E. HOPF, Commun. Pure Appl. Math., Vol. 3, 201, 1950; J. D. COLE, Quart. Appl. Math., Vol. 9, 225, 1951.
[5] M. IRAC-ASTAUD, Proceedings du XVIIe Colloque International sur la Théorie des Groupes
en Physique, 1988, Sainte Adèle, Québec.
[6] R. M. MIURA, J. Math. Phys., Vol. 9, 1968, p. 1202.
( Manuscript received July 6, 1989.)
Annales de l’Institut Henri Poincaré - Physique théorique