A NNALES DE LA FACULTÉ DES SCIENCES DE T OULOUSE
R ODICA D. C OSTIN
Power and exponential-power series solutions of evolution equations
Annales de la faculté des sciences de Toulouse 6
esérie, tome 13, n
o4 (2004), p. 551-573
<http://www.numdam.org/item?id=AFST_2004_6_13_4_551_0>
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551
Power and exponential-power series solutions
of evolution equations
RODICA D. COSTIN (1)
Annales de la Faculté des Sciences de Toulouse Vol. XIII, n° 4, 2004
ABSTRACT. - The paper studies transseries solutions of linear evolu- tion equations, and their correspondance with solutions using generalized Laplace transform. It is found that, in spite of a rich functional freedom in the form of the transseries solutions, there is a maximal exponential order possible. This is a distinguished order a growth, and others are obtained by asymptotic superpositions of transseries solutions of this order.
RÉSUMÉ. - Cet article examine les transséries solutions formelles d’équa-
tions d’évolution linéaires et leur correspondance avec les solutions, en utilisant la transformation de Laplace généralisée. On trouve que, malgré
la grande diversité des formes possibles pour une solution transsérielle, il
y a un ordre exponentiel maximal. Il s’agit d’un certain ordre de crois- sance, et les autres solutions transsérielles sont obtenues par superposition asymptotique de solutions transsérielles de cet ordre.
1. Introduction 1.1. Brief overview
The
theory
ofpartial
differentialequations
when one, or morevariables,
is in the
complex domain,
andapproaches
a characteristicvariety
hasonly recently
started todevelop.
(*) Reçu le 29 août 2003, accepté le 14 janvier 2004
(1) Rutgers University, Department of Mathematics, Hill Center, Busch Campus, Rutgers, The State University of New Jersey, 110 Frelinghuysen Rd, Piscataway, NJ 08854-801
E-mail: [email protected]
In their paper
[11], generalized
in[12],
O. Costin and S. Tanveerproved
existence and
uniqueness
of solutions withgiven
initialconditions,
forquasi-
linear
systems
of evolutionequations
in alarge enough
sector of C.Borel
summability
ofdivergent
solutions of the heatequation
wasproved by Lutz, Miyake,
and Schâfke[13],
and moregenerally,
Borelsummability
of series solutions of linear
equations
with constant coefficients wasproved,
in a
general setting, by
Balser(see [1],
and the referencestherein).
A natural
question
is to find what formalobjects
liebeyond
formal power seriessolutions,
and what is their connection to power series. Thepresent
paper contains initial results in this direction.
For
ordinary
differentialequations
acomprehensive
andgeneral theory
of formal solutions
(transseries),
in a one-to-onecorrespondence
with truesolutions,
ispresented
in the fundamental work of Ecalle[3]-[5].
The cor-respondence
between transseries and solutions was laterproved
under non-resonance
assumptions by
O.Costin,
who constructed ageneralized
Boreltransform
[6], [7].
O. Costin and Kruskal showed how formal solutions canbe used to
produce
the Stokes constants[9], [8].
Transseries solutions can be used to find thetype
and location of movable arrays ofsingularities
towardthe
irregular singular point [8], [10].
Braaksma has
recently
extended thetheory
of transseriesrepresenta-
tions to nonlinear differenceequations [2].
The structure ofsingularities
ofsolutions of difference
equations
has been obtainedby
Kuik[15].
1.2. Général Remarks
The
present
paper considers a fewsimple
evolutionequations,
and ex-amines the formal solutions that can be built with
exponentials
and powers.Some conclusions are mentioned below.
A main distinction between formal solutions of
ordinary,
versuspartial
differential
equations
is that there is an tremendous freedom in the formal solutions of apartial
differentialequation:
after each monomial there is afunctional freedom.
Perhaps surprisingly however,
there is a maximal orderpossible
for ex-ponential
solutions(for
evolutionequations
of order at leasttwo);
thesemaximal
exponentials
are alsodistinguished
in another way:they generate
the termsbeyond
all orders ofdivergent
power solutions.For the linear
equations
examined in this paper, the heatequation
andAiry equation,
solutions can be obtainedby superposition
ofsimpler
solu-tions
(which
solvesimilarity
reductions toordinary equations).
A remark-able fact is that the PDE transseries are also obtained
by superpositions
of the transseries of the
similarity
solutions. Thisprovides
robustness to atheory
of transseries for solutions ofpartial
differentialequations.
Formal series and
exponential
series solutions ofpartial
differential equa- tions are deduced in this paperusing
standard tools inasymptotic analysis;
their basic
principles
wereexposed by
Kruskal in[14].
Such calculations ap-ply
to solutions that do have a(trans)asymptotic representation,
and usethe
assumption
that monomials in thisrepresentation
do preserve their or-dering
afteroperations
with functions. In the case ofalgebraic, ordinary
differential or difference
equations,
withanalyzable
coefficients(as
is thecase of
equations arising
inapplications),
thegeneral
solutions seem to bein a one-to-one
isomorphic correspondence
with suchalgebraic representa-
tions(transseries) (see [3]
forordinary
differentialequations).
Forpartial
differential
equations however,
due to a rich functional freedom in the set ofsolutions,
it is clear thatonly
subclasses of solutions can berepresented by algebraic objects.
Thesteps
ofspecific
calculations will be shown in somedetail to uncover that
they
can bejustified
foralgebraic representations
that have the
properties
ofÉcalle’s
transseries:they
are based on monomi-als,
that can be well ordered withrespect
to the muchlarger
relation(»),
and for which all
operations
preserve theordering.
1.3.
Setting
The
formal
solutions will be derived under theassumption
that x is realpositive x ~
+00 and that t varies in acompact
subintervalof (0, +~).
1.4. Main results
Formal solutions of the heat
equation,
and their association to solutions obtainedby
inverseLaplace
transform are studied in§3.
It is shown that power series are linear combinations
(finite,
orinfinite,
in the latter case
possibly transfinite)
of pure seriessolutions,
in which allfreedoms besides the first term are taken to be 0
(3.7);
these series are gener-ically divergent.
It is shown thatexponential
terms cannot havearbitrary
order. In
fact,
there is a maximal order ofdecay.
Thesedistinguished
expo- nential series(3.11), together
with the pure power seriessatisfy
the sameordinary
differentialequations (3.13),
hence it may be inferred that theseexponentials
are thepossible
termsbeyond
all orders of the pure power series.Complex plane
solutions u of the heatequation
are then studied in§3.4 using
inverseLaplace transform,
after proper normalization in the senseof O. Costin. The power series
asymptotic
toLaplace integrals
are pre-cisely
thecorresponding superpositions
of pure power series.Moreover,
thecorresponding superposition
of thedistinguished exponentially
small termscoincides with the
loop integral
that encircles all thesingularities
of theinverse
Laplace
transform of u, thengenerating
all the termsbeyond
allorders of u
(Proposition 3.1).
In
§3.6
it is shown that initial data determines the power series andboundary
data fixes theexponentially
small terms as well.Similar results hold for the
Airy equation
and arebriefly presented
in§4.
A
simple
firstorder,
nonlinearexample
is examinedin §5.
Power seriessolutions cannot have
arbitrary order,
and there is a maximal power.2. The
simplest partial
differentialequation
Consider the
simplest
first order evolutionequation
2ct = ux
( 2 .1 )
Equation (2.1)
has thegeneral
solution u =03A6(x + t)
where 03A6 is any differ- entiable function. Then its formal solutions are anyexpressions
in x + t andnothing
morespecific
seems to emerge.3. The Heat
Equation
Consider the
simplest
second order evolutionequation:
the heatequation
The
question
is to find the formal series solutions that can be written in terms of powers of x orexponentials
of powers of x, in theasymptotic
limitof §1.3.
It willshortly
appear that the same formal solutionssatisfy
anotherlimit, namely
for t ~ +0 and x =O(1).
3.1. Power séries solutions
Formal calculation of power series solutions of
(3.1)
is standard. The mainsteps
are as follows.Looking
for solutionsu(x, t) behaving
like a power of x, substituteThen
(3.1)
becomesThe usual
assumption
at thispoint
is that since A « xn then alsoAt, 1B.,x
« xn. Thiscertainly
holds if A is in a"good"
class of functions(but
isclearly
not true in fullgenerality,
and an easycounterexample
is0394 =
xn-l sin(1/x)).
Then in
(3.3)
the termf’ (t) xn
is muchlarger
than allothers,
and itmust therefore vanish:
f(t)
= const = cn. Then u= cnxn + A
whereThe main behavior of A contains a functional
freedom,
since then A =(x) +03B4(x,t),
where 03A6 is any functionsatisfying 03A6
«xn, 03A6xx
«xn-2
and 03B4 satisfies 03B4 ~ 03A6.For
simplicity (and definiteness) only
powers of x are consideredhere, so 03A6(x)
=ckxk (where
RkRn).
Then u =
cnxn
+ckxk + 03B4(x,t) (where 03B4
«x k)
and thesteps
aboveare
repeated
to determine theleading
behavior of b(which
is thelargest
monomial in its
asymptotic représentation).
It turns out that there is a functional freedom after every monomial of the series solution u; a
simple
calculationyields
thegeneral
form of a power series solution of(3.1):
Equation (3.1)
islinear,
hence(3.5)
is asuperposition (finite,
orinfinite,
in the latter case it can be
transfinite)
where ûn
are"pure
series" : series solutions withleading
behavior xn and where allarbitrary
freedoms were chosen zero; asimple
calculationyields
Note that the series
(3.7)
is finite if n E N anddiverges
otherwise.The series
(3.6)
is anasymptotic object only
if its terms can bearranged
in a
decreasing
way. For this to bepossible
the set S must be well ordered withrespect
to the relation : n k iff xn »xk (x
~oo).
The
decomposition (3.6), (3.7)
allows todistinguish
between the diver- gence intrinsic to theequation (seen
in(3.7))
andpossible divergence
dueto
given
data(seen
in the behavior of cn, for ngoing
towardspoints
ofaccumulation in S
~ {+~}).
It is
interesting
to note that t appearsonly
in the form of powers(even
if no
assumptions
on t weremade). Also,
the series(3.6)
isasymptotic
inthe another limit as well: t ~
+0,
and xvarying
in acompact
subinterval ofR+.
3.2.
Exponential
séries.Distinguished exponentials
Unlike the case of the first order
equation (2.1),
where anyexponential growth
of solutions waspossible,
for the heatequation (and seemingly,
formost other second or
higher
orderequations)
it turns out that there is amaximal order of increase
(for representations
in a"good class").
Formal calculation of
exponential
series solutions is the WKBmethod,
whose main
steps
are outlined belowtogether
with necessaryassumptions.
With the substitution u -
exp(W) (where lW/
»1) equation (3.1)
becomes
The term
Wxx
can beneglected
in a firstapproximation,
sinceWxx «
W2x. (Indeed,
otherwiseWxx/W2x
is muchlarger,
or of order 1 whichby integration gives
that W has at mostlogarithmic order,
so u does not haveexponential growth.)
For the dominant order of W one needs then to solve
Wt ~ 1 4 W2x,
whichgives
where 03A6 is an
arbitrary
function.It turns out that solutions W of
(3.9) belonging
to a"good"
class havethe maximal order of
growth x2. Indeed,
ifWx
is muchlarger than,
or of thesame order
as 03A6(Wx)
then(3.9) implies
thatWx
is of order x. Otherwise03A6(Wx)
must have order x, henceWx
« x. ThusWx
has at most order x,so W has at most order
x2.
Note that these considerations hold for functions W in a class for which the relation » is conserved under
operations
in x(W (., t)
isanalyzable).
Looking
for thespecific
form of a maximalW,
substitute W =f (t)x2
+o(x2 )
in(3.8),
whichgives
W= -x2 t-03C4
+o(X2).
Since the heatequation
isinvariant under translations in
t,
take T ==0,
and find thedistinguished exponential
Other solutions of
(3.9)
have the form W = cxn +o(xn)
with Rn 2and c ~ C.
There is a functional freedom after each monomial in the
expansion
ofW,
and this freedom is anarbitrary
function ofx t:
An
interesting
case is03A61(z)
=203BEz (with 03BE
EC). Taking
all other free- doms to be 0 weget
the exact solutionand the
freedom 03A61 corresponds
to invariance of(3.1)
under translations in x.Another
special
freedom is03A60(z) = (-n - 1) ln z (with n
eC). Again taking
all other freedoms 0 onegets
the formal solutionsNote that the series
(3.11)
is finite if n e Z- anddiverges
otherwise.3.3.
Similarity
solutions and transseriesIn this section it is shown that the
exponentially
small termsfollowing
a series solution
(3.7)
areprecisely (3.11). Indeed,
it will be shown that the series(3.7)
and(3.11)
solve the same differentialequation (for
fixedn);
based onexisting
results in thetheory
of transseriesrepresentations
for solutions ofordinary
differentialequations
it follows then that if(3.7) diverges,
then(3.11)
must constitute the termsbeyond
all orders of that series.3.3.1 Transseries
Noting
that the formal solutions(3.7), (3.11)
are powers of tmultiplying
series in
x2 t,
denotewhich transforms
(3.1)
into theordinary
differentialequation
Equations (3.13)
areusually
calledsimilarity
reductions of(3.1)
andtheir solutions
(3.12)
aresimilarity
solutions.Transseries solutions of
(3.13)
are of course, linear combinations of twoindependent solutions,
which have the formThen
formal,
as well asactual,
solutions of the heatequation
are obtainedfrom
(3.12)
and(3.13), (3.14): they
areThe series
multiplying
the constantAn
is(3.7),
andBn
is followedby (3.11).
3.3.2
Representations using
inverseLaplace
transformAssumption:
Forsimplicity only negative integer
powers will be con-sidered in the
following:
n E Z-.Positive values of n
correspond
to solutions of the heatequation
that donot decrease to
0; they
can also be studiedusing
inverseLaplace
transformafter
subtracting
theincreasing
terms in theexpansions (see [7], [10], [11]).
Noninteger
values of n make the inverseLaplace
transform branched at theorigin,
but nomajor
differences exist otherwise inusing
the Borel spacetechniques [7].
Transseries
(3.14)
are obtainedusing generalized
inverseLaplace
trans-form
[4], [7]
in thefollowing
way. The substitution(where I!
is apath starting
at p =0, going
to oo in theright-half plane)
transforms
(3.13) toI
whose solution is
Since n was assumed
negative, G(p)
isintegrable
at p ==0,
and issingular at p = 1.
The
integral (3.16) depends
on thepath
ofintegration R only
relative toits
homotopy
class in theright half-plane
minus thepoint
p =1;
thereforeR can be assumed to be either
d+
=ei03B8R+
or d- =e-i03B8R+ (where B
is anynumber in
(0, 03C0 2)).
A solution of
(3.13)
whose transseries is a power series with no exponen-tially
small terms is the balanced average[4], [7], [6]
and a solution whose transseries is
exponentially
small is(which
amounts tointegration
in(3.16)
on aloop
around p =1).
(1) It must be assumed that G is such that the integral
(3.16)
exists and, when inte-Stating
these facts in terms of solutions of the heatequation, using (3.12), (3.13), (3.14)
consider the solutions of(3.1)
and defin(
Then
(see §6.1
fordétails) ;
the transseriesof u[p]n
has noexponentially
small terms.Also
(see §6.2
fordétails).
3.4. Solutions of the heat
equation by
inverseLaplace
transformSolutions of
linear,
or nonlinearpartial
differentialequations
have beenstudied
using
inverseLaplace
transform methodsby
O. Costin and S. Tan-veer
[11], [12].
Looking
for solutions of(3.1)
which go to 0 for x ~ +00using
inverseLaplace transform,
first normalize theequation by substituting y == x2
and
(3.1)
becomeswhich after inverse
Laplace
transformgives
with the
general
solutionwhere F is
arbitrary.
This
gives
solutions of the heatequation
in the formwhere R is a
path starting at q
=0,
which for t in aspecified
interval lies in theright-half plane
and avoids thesingularities
of theintegrand.
3.4.1
Assumptions
on F.At this
point
a discussion isrequired
on theassumptions
on thearbitrary
function F that are
needed,
or useful.First of
all,
formula(3.26)
defines a solution of(3.1)
if theintegral
existsand can be differentiated with
respect
to t and x.Also,
formula(3.26)
definesuniquely, by
Borelsummation,
a functionUF if
F(03B6)
isanalytic at
0(or,
at least has aconvergent
Frobeniusseries) .
It should be noted that the
path
ofintegration R
in(3.26)
will have tovary with
t,
since thesingularities
of theintegrand
do vary. But the value of theintegral (3.26)
should notdepend
on small variations of ~(otherwise
UF may not solve
(3.1)).
Then F must be assumedmostly analytic,
in anappropriate
sense which assures that when t isvaried,
thepath
ofintegration
can be
accordingly
varied in a domain ofanalyticity
of theintegrand,
so thatthe value of the
integral
islocally
constant in t.In
addition, considering
functions F in a moreregular class,
more in-formation on UF can be obtained
using analytic
methods. Forexample, restricting
the considerations to solutions UF which are(1) analytic
for xin a sector
containing R+ (possibly excepting
a discrete set ofpoints),
and(2)
are defined for all t >to
thenF(03B6)
would be assumed(a) analytic
inthe
complex plane
less two half-linesS03B60 = {03B6 ~ R; |03B6|
>03B60},
and(b)
theincrease of F at
points
onS(o
should allowintegrals (3.26)
to converge(see
§6.3
fordétails).
3.4.2
Asymptotic
andtransasymptotic expansions
The
asymptotic
power series of the solution UF in(3.26)
is found in astraightforward
way,using
Watson’s Lemma(which
amounts to a formalintegration,
termby term,
of theTaylor
series of(1 - tq)-3/2
F(q 1-tq) at
As a natural
generalization
of thetechniques
used forordinary
differen-tial
equations,
it is to beexpected
thatexponentially
small terms of UF aregenerated by taking
linear combinations ofuF(x,t;~)
on differentpaths
f.For linear
equations
thestudy
ofexponentially
small series iseasier,
andeasier to
put
to test.3.5.
Superpositions
ofsimilarity
solutions and transseries3.5.1
Similarity
solutionsFor
F(03B6) = (m (with
Rm >-1)
formula(3.26)
has the form(3.18)
for7T, == -2m -
2,
hence3.5.2 Finite
superpositions
ofsimilarity
solutionsFor
F(03B6)
apolynomial:
(3.26)
is a finitesuperposition
of(3.18):
and the transseries of UF is obtained
by
a direct summation and rearrange- ment of the transseries of U-2m-2, m = O..M.Similar results hold if
F (()
apolynomial
in(1/2.
3.5.3 Infinite
superpositions
ofsimilarity
solutionsSince the function F of
(3.26)
is assumedanalytic at ( - 0,
it has aconvergent Taylor
seriesexpansion
A natural
question
is toinvestigate
what formalobjects
are obtainedby
thecorresponding superposition
of the transseries ofu-2m-2, m
0.Consider then the formal
objects
obtainedby replacing u -2m-2
andu[e]-2m-2
with their formal series(3.21), (3.7), respectively (3.22), (3.11):
The power series
ûp
can berearranged
to becomeasymptotic (meaning
that the terms are
decreasing),
and this isclearly
the power series asymp- totics of UF(by
Watson’sLemma).
The
exponential
seriesF
cannot beimmediately rearranged
in an asymp-totic way
(since
the powers of xmultiply
the sameexponential
term andhave no upper
bound).
However, F
is ananalytic
function which sums all theexponentially
small terms:
PROPOSITION 3.1. - Let F have a
convergent Taylor
series(3.29)
atthe
origin.
LetûF be defined by (3.31).
Then there exists
to
0 and c > 0 such thatfor
all t >to.
The
integral (3.26)
is on theloop
which encircles all thesingularities of
the
integrand.
To be more
specific, to
and c are anypositive
constants for whichF(03B6)
is
analytic
on thedisk + 1 t0 | 1 c.
Such constantsalways
exist since F wasassumed
analytic at 0;
forexample
if F isanalytic on |03B6|
r then onecan take
to
>1/r.
Inparticular, to
can be chosen 0 if F isanalytic
on thehalf-plane R03B6
0.The of
Proposition
3.1 isgiven
in§6.4.
3.5.4
Example
1If F is entire then the
only singularity
of theintegrand
in(3.26)
isq =
1/t,
which is an essentialsingularity.
Thepaths
ofintegration f
can betaken
to be raysd7:.
as in(3.18).
To examine the transseries of solutions on a
simple example
in this classconsider
For this F the
exponential
seriestiF
can be calculatedexplicitly (either
from(3.32),
or,directly
from(6.2)), yielding
Note that the
loop integral (3.33)
contains more than onetype
of expo-nential
terms,
inspite
of the fact that there isonly
onesingularity.
3.5.5
Example
2If F is a rational
function,
then it can be written as apolynomial plus
a sum of
poles. Polynomials
were consideredalready
in§3.5.
Consider nextthe case of a
simple pole
so
Loop integrals
For F
given by (3.34)
formula(3.26)
isand the
integrand
issingular
at q, -1
and q2 =i.
There are fourpaths
of
integration f avoiding
ql and q2.Denote
by
dO"l,0"2(03C3j = ±)
thepaths
in theright half-plane starting
atq =
0, avoiding qj
from above(respectively, below)
if aj == +(respectively,
-). Elementary
calculationsgive
and
Main
loop integral
On the other
hand,
directsuperposition
of theexponentially
small terms(see (3.32)) give, using (3.36), (3.37),
3.6. Relations between initial data and transseries
representations
The structure of transseries solutions makes visible the
type
ofinitial,
or
boundary
data thatspecifies uniquely
a solution with agiven
class. In-deed,
considersimilarity
solutions with n0;
their transseries have the form(3.15),
and it is intuitive thatlooking
at the limit t ~ +0 the smallexponential
term mustvanish,
thusfixing An,
while in the limit x ---+ +0 the constantBn
becomesvisible,
since theexponential
is nolonger beyond
all orders. This means that conditions on solutions
given
at x = 0+ andat t = 0+
specifies uniquely
a solution. Remarks 3.2 and 3.3 state theseproperties.
Remark 3.2. - The initial condition determines the dominant power series. Indeed:
(i)
Thesimilarity
solutionssatisfy
for x > 0 and n
0;
therefore(ii)
Moregenerally,
ifF(03B6)
isentire,
thenand the function F is determined
by
the initial condition at t = 0.The follows
immediately
from(3.18)
and(3.26).
Further Remarks.
The
general
case, when F is notentire,
is veryinteresting
and rich inconsequences, for both
finding
an initial time whenspecifying
an initialcondition determines F
uniquely,
and for thestudy
of backwards evolution(in
the sense ofanalytic
continuation for t less than the initialtime).
Theseissues however will not be
pursued
here.Remark 3.3. - If n is not an even
integer, boundary
conditions deter- mine theexponentially
small terms. Indeed:fo
Formula
(3.39)
followsby substituting p/(l - p)
= r in(3.18)
for x = 0and
using
a formula for an Eulerianintegral
of the first kind[16].
Remark
3.4.
- The existence of a maximal order of increase of exponen- tial termsimplies
that a solutionasymptotic
to agiven
power series in a sectorlarge enough
isunique.
Thistype
ofproperty
insuresuniqueness
alsoin the
general
results of O. Costin and S. Tanveer in[11], [12].
For the heat
equation,
since thelargest possible exponent
is of orderx2 (see (3.10))
then therequirement
that a solution beasymptotic
to apower series on a sector
larger
than arg x E[0, 03C0/4] implies uniqueness
ofthe solution.
(Intuitively, exponential
terms are not small after continuation in xbeyond 1 arg x 03C0/4.)
4. The
Airy Equation
Consider the
simplest
third order evolutionequation:
theAiry Equation
4.1. Formal solutions
Consider power series and
exponential-power
series solutions of theAiry equation (4.1)
in the limitof §1.3.
The considerations on the structure of formal solutions are very similar to the case of the heat
equation,
and are notrepeated
here.Power solutions are
superpositions
ofThe series
(4.2)
terminates if n e N anddiverges
otherwise.The
largest
order of increase of solutions are theexponentials
ofx3/2;
the
distinguished exponentials
areand there are
exponential-power
series solutions of the formThe series
(4.2)
and(4.3)
are formal solutions ofsimilarity
reductionequations: substituting
equation (4.1)
becomes theordinary
differentialequation
which,
for each n, links the seriesîcn
to theexponential
seriesûn;±.
InverseLaplace
transform of(4.4) gives
with solution a combination of
hypergeometric
functions of the form(see §6.5.3
for the definition of2F1).
Next, considering
solutions of theAiry equation
which go to 0 as x -+~,
they
can beexpressed by
inverseLaplace
transform after the proper normalizationx3/2 ==
y.Substituting u(x, t)
=v(y,t) equation (4.1)
be-comes
which after inverse
Laplace
transformv(y, t)
=~~ e-qyV(q, t)dq gives
As in the case of the heat
equation,
solutions of(4.7)
can beexpressed
as
superpositions
ofsimilarity solutions;
infact,
for n anegative integer (not
amultiple
of3)
formulas(4.5)
can be written in terms ofelementary
functions.
5. A nonlinear
example
Consider the
simple
firstorder,
nonlinear evolutionequation
whose
general
solution isgiven implicitly by
where P is an
arbitrary
tunction.Consider the formal solutions of
(5.1)
in the limit of§1.3.
A
simple analysis
shows that the maximal order of a power series solution is x: u= x t + o(x) ;
other series solutions may start with any lower power:u = cxn + ...
(with
Rn1).
-Let us focus on the
distinguished
power series.Substituting u - + v
(where v
is assumed much smaller thanx),
weget
Since v « x,
then vx
« 1(if v
is in agood class),
therefore the linearpart
of(5.3)
contains thelargest terms,
whichby solving gives v - 1 t 03A6 (x t)
(with 4)
«1).
Successiveperturbations give, iteratively,
the series solutionwhich can be viewed as a "nonlinearization" of the formal and actual so-
lutions 1 t 03A6
of the linearpart, generalizing
the samephenomenon
seen forordinary
differentialequations.
Exponential
terms can be included in the function 03A6(which
is the sameas in
(5.2));
so there areclearly
nodistinguished exponentials.
6.
Appendix
6.1.
Appendix
1From
(3.16), (3.17)
and Watson’s Lemma we havewhich
yields (3.21).
6.2.
Appendix
2From
(3.16), (3.17)
we havewhere
where the last
equality
followsby
Hankel’s formula for r-functions[16].
6.3.
Appendix
3(i) Assuming
theintegrand
of(3.26)
isanalytic along ~ = ei03B8R+,
itfollows that
F(03B6)
must beanalytic
on thepath (
=q/(1 - tq), (q
Eei03B8R+)
which is the arc
At,o
of the circle centered at-1/ (2t)
+i cos03B8/(2tsin03B8) passing through
theorigin
and thepoint -l/t
which lies in the upper half-plane
for 03B8 >0, respectively
in the lowerhalf-plane
for 0 0.(ii) Assuming
in addition that the solution UF is defined forall t to
(for
someto
>0)
it follows that F isanalytic
in theregion
boundedby At0,03B8
and the x-axis(possible excluding
a finite number ofsingular points).
(iii) Assuming (i)
and(ii)
for all 0 E(0, ()o] (possibly excepting
a discreteset of
points),
this entails that F isanalytic
in the outerregion
boundedby At,03B80
and the x-axis(possible excluding
a finite number ofsingular points).
6.4.
Appendix
4Each term
ft-2m-2
is a finite sum and it will be shown that the series converges if for all t >to >
0 ifF(03B6)
isanalytic
on thedisk |03B6
-t-1 t0| 1 c
In view of
§3.5.1
we need to consider03A3m0 Fmu[e]-2m-2. BY (3.22), (3.11)
the
superposition
of thecorresponding
formal series iswhich is a series of finite sums
(by (3.11))
and
using
theduplication
formula forr-fûnction (see (6.3) )
This series cannot be reordered in an
asymptotic
way. It will however be shown that it convergesabsolutely
for tlarge enough.
Doing
for the moment a formalcalculation,
thechange
of the order o.summation
gives
and with the notation:
03A6r(03C4) = 1 r!F(r)(03C4)
it followand
using (6.5)
where
substituting 03BE
=t(l - tq) gives
Clearly
the series convergeabsolutely, justifying
thus the calculationabove,
if theTaylor
series of F at thepoint. - t ,
converges
absolutely,
foraIl ç
on the line ofintegration
c +iR,
which followsif F is
analytic
on the disk centeredat = t
and radiusexceeding 1 c.
Thisholds for all t >
to
if thepositive
numbers c andto
are such thatF(()
isanalytic
on thedisk 1 ( + 1 t0| 1 c (such
ato
and calways
exist since F wasassumed
analytic at ( = 0).
Inparticular,
the series convergesabsolutely
for all t > 0 if F is
analytic
on thehalf-plane R03B6
0.6.5.
Appendix
5: Some formulae6.5.1
Duplication
formula for ther-function:[16]
6.5.2
Laplace
and InverseLaplace
transformationsand
conversely,
6.5.3 The extended
hypergeometric
function2Fl
Acknowledgements. -
The author is verygrateful
to Frédéric Fauvet and DavidSauzin,
theorganizers
of theextremely interesting
and well runworkshop
on"Resurgence,
alienderivations, resummability
andtransseries" ,
for the invitation to
participate,
and all theirhelp
andpatience.
The author is also
grateful
toFrançois
Trêves forraising
the issue of transseries forpartial
differentialequations,
for veryinteresting discussions,
and for
encouragements.
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