A NNALES DE L ’I. H. P., SECTION A
G IANCARLO B ENETTIN
L UIGI C HIERCHIA F RANCESCO F ASSÒ
Exponential estimates on the one-dimensional
Schroedinger equation with bounded analytic potential
Annales de l’I. H. P., section A, tome 51, n
o1 (1989), p. 45-66
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45
Exponential estimates
on
the one-dimensional
Schroedinger equation
with bounded analytic potential
Giancarlo BENETTIN
Luigi
CHIERCHIAFrancesco FASSÒ
Dipartimento di Fisica dell’Universita di Padova, Via F. Marzolo, 8, 35131 Padova, Italy
Dipartimento di Matematica, II Universita di Roma, Via O. Raimondo, 00173 Roma, Italy
Scuola Internazionale Superiore di Studi Avanzati, Strada Costiera, 11, 34014 Trieste, Italy
Vol. 51, n° 1, 1989, Physique theorique
ABSTRACT. -
Using
a Nekhoroshev-likeperturbation technique,
weinvestigate
the solutions of the one-dimensionalstationary Schroedinger equation,
with boundedanalytic potential.
Forsufficiently high
energyE,
we construct
(in principle,
up to any order in1/~/E) approximate
sol-utions,
which resemble free waves, and are ’very
close" to the true solutions over verylarge distances, growing exponentially
with/E.
Forpotentials
whichdecay sufficiently rapidly
atinfinity,
we find that thescattering
matrix differs from a trivial oneby
aquantity exponentially
small in
/E (m particular,
the reflection coefficient isexponentially
smallin
Special
attention is also devoted to the case ofquasi-periodic potentials.
These resultsunify,
extend and makequantitative previous
results
by Fedoryuk,
Neishtadt andDelyon
and Foulon. Some numericalAnnales de l’Institut Henri Poincaré - Physique theorique - 0246-0211
and
analytic
tests show that ourperturbative
constructionis,
at least in the most relevantpoint,
almostoptimal.
Nous etudions les solutions de
1’equation
deSchrodinger
aune dimension avec un
potentiel analytique
en utilisant unetechnique
deperturbation inspiree
de Nekhoroshev. Pour uneenergie E
suffisammentgrande
nous construisons des solutionsapprochees (en principe
à tous lesordres en
1A/E) qui
ressemblent a des ondesplanes
et sont tresproches
des vraies solutions sur des
grandes
distancesqui
croissentexponentielle-
ment vite avec
/E.
Pour despotentiels qui
decroissent suffisamment vite à l’infini nous montrons que la matrice de diffusion ne differe de la matrice triviale que par unequantite exponentiellement petite
en/E (en particu- lier,
Ie coefficient de reflection estexponentiellement petit
en Nousetudions tout
particulièrement
Ie cas despotentiels quasi periodiques.
Lesresultats
unifient,
etendent et rendentquantitatifs
des resultats anterieurs deFedoryuk, Neishtadt, Delyon
et Foulon. Des testsnumériques
etanalytiques
montrent que notre constructionperturbative
est presqueopti- male,
au moins pour lespoints
lesplus importants.
1. INTRODUCTION We consider here the
Schroedinger equation
where V is a bounded
real-analytic function,
and E apositive parameter.
When E is
large
with respect tomax |
V(x)|
onemight naively expect
that the solutionsof (1.1) resemble,
in some sense, the free solutions of the trivial Of course, as is wellknown,
there arecases, e. g. when V is
periodic [1],
for which there arearbitrarily large
values of E
(corresponding
tospectral
gaps of theoperator
L==20142014+V),
such that solutions of(1.1)
are insteadsubstantially
different
(in fact, L2
at oneside,
and unbounded at the otherside).
Nevertheless,
we will construct aperturbation theory (for
which the"zero-order" is the free
problem),
that shows that indeed allAnnales de l’Institut Henri Poincaré - Physique theorique
of (1.1)
are very similar to free waves over a verylarge distance, growing exponentially
withE,
moreprecisely
can beexpressed
as linear combina- tions of functions of the formwhere a is some
positive
constant.Evaluating
the constant a is also oneof our tasks: we will prove that
( 1.2)
holds with where p is the width of acomplex strip
ofanalyticity
of V(around !?),
and a is any number smaller than2/e.
On the otherhand,
ingeneral,
a cannot betaken to be
larger
than2,
as will be shown below on someexamples.
For our
analysis,
thehypothesis
ofanalyticity
of thepotential
isdeeply
essential. On the other
hand,
relation( 1.2)
is not true, ingeneral,
for non-analytic potentials: indeed,
this relationimplies
that thelength
of thepossible spectral
gapsdecays
with E as exp - aJE,
while it is well known[2] that,
forperiodic V,
thespectral
gaps areexponentially
small with~ only
isanalytic.
For
relatively simple potentials,
e. g. if V has a finite number of station- arypoints,
or isperiodic,
WKB methods have turned out to be verypowerful ([3], [4])
ininvestigating
the structure of( 1.1): however,
thesemethods have not been extended yet to more difficult
situations,
likequasi-periodic
or stochasticV,
to which ourtechnique
insteadapplies.
Our method is based on a classical mechanics
interpretation
of theSchroedinger equation.
Infact, ( 1.1)
isequivalent
to the Hamilton equa- tions for a harmonic oscillator withtime-dependent frequency [E - V (x)]~~2
(here
the role of time isplayed by x).
To such asystem
weapply
aNekhoroshev-like
technique ([5], [6]) (see
also refs.[7]-[10]), carrying
outa
simple
but very carefulquantitative analysis.
The same mechanicalsystem has been studied
by
Neishtad[8],
and anapplication
to the Schroe-dinger equation
hasalready
been madeby Delyon
and Foulon[11],
inorder to prove the
exponential decay
of theLyapunov
exponents. How-ever, these studies do not carry out any
quantitative analysis,
nor report,at least
explicitly,
direct estimates on thesolution,
say of the form( 1.2).
A
novelty
of our scheme is also the use of "local norms"([12], [13]),
which allow one to take
explicitly
into account the presence ofregions
where V is
particularly
small. Forexample,
if V is L1(in
a suitablesense)
we construct
approximate solutions,
which differ from the actual solutionsof (1.1) by exp-a
over the whole real axis. Inparticular,
as abyproduct
of our localestimates,
we get anexponentially
small bound for the reflection coefficientR,
of theform
A similarbound has been obtained
by Fedoryuk [14], by
means ofasymptotic expansions; unfortunately,
aprecise comparison
cannot begiven,
since inreference
[14]
the constants are notexplicitly
evaluated.Our results cover, in
particular,
the case of aquasi-periodic potential.
Such a case has been
widely
studiedby
means of KAM-likeperturbative
techniques ([15]-[18], [24]),
with the result that there exist solutions whichare also
quasi-periodic,
forsufficiently high
values of Ebelonging
to a setof
large
measure, but with a Cantor-like structure.By
means of ourNekhoroshev-like
perturbation theory
we obtain(as usual)
acomplemen- tary result, namely that,
for any(sufficiently high)
value ofE,
the solutionsare very close to
quasi-periodic
waves, over anexponentially large length scale,
as in( 1.1 ) .
In the next Section we formulate
precisely
our main result(Proposition 1),
and illustrate it on some relevant classes ofpotentials.
InSection 3 we prove
Proposition 1,
on the basis of the result of our pertur- bativetechnique (Proposition 2),
which in turn isproved
in Section 4.Finally,
Section 5 is devoted to thecomparison
of our estimate for the constant a with an exact result(in
theparticular
case of aperiodic potential),
and also with some numerical results(for scattering problems).
ACKNOWLEDGEMENTS
We are indebted to F. Martinelli and T.
Spencer
for usefulsuggestions.
2. STATEMENT OF RESULTS
2.1. The main
Proposition
We are concerned with the one-dimensional
Schroedinger equation ( 1.1),
with
analytic potential.
Moreprecisely, denoting by
thecomplex strip
we assume that V is
analytic
in!/ p’
and real for real x(similar functions, possibly
vector- ormatrix-valued,
will becalled, throughout
the paper, realanalytic).
For anyanalytic
functionf : !/ p ~ C,
it is convenient tointroduce,
besides the usual supremum norm, denoted thefollowing family
of "local norms":For the solution of the
Schroedinger equation (1.1)
we shall use the vectornotation
w=tB)/, 1 E 03C8’), with B)/=2014’;
for vectors w2)~2
we
adopt
thenorm ~ W 112 = |w1|2 +
I W212,
while for linear operatorsacting
on (:2 we use thecorresponding norm ~I A 11= supw~
A W wII.
Poincaré - Physique théorique
Our results can be formulated in the
following general
statement:PROPOSITION 1. - Let V be real
analytic
and bounded in sp, P > O. Foy any Esatisfying
there
’ exist a 2 x 2 realanalytic
matrixT (x),
and a ’ realanalytic function
V (x),
such that:(i)
T is close to theidentity, precisely
(ii) V
is close toV, precisely
(iii)
DenoteM= 20142014 ~ ’ ~/2B-! -1/
i), B ~ ~x~ ~
0 ~),
withthen for any
constantUEC2 the
, solutionw (x) of ( 1.1 ),
withw (0) = MT (0) u,
is
"exponentially
close" to the ,function
precisely, denoting by NE
theinteger
partof
pjE/2,
one haswith
Remarks. -
(i)
Both T andV
alsodepend
onE; although they
are notanalytic
inE, they
are, ina
sense,polynomials
ofdegree NE
in1/
forinstance,
one has withVs independent
of E. Ass=o
will be clear in Section
4,
both T andV
could beexplicitly
written up to any order in1/~/E,
while(2.5)
could also bereplaced by inequalities
accurate to any order in
1/ /E.
(ii)
As remarked in theIntroduction,
one couldreplace
theexpression
for NE by NE=03B103C1 E,
abeing
any number smaller than2/e,
with acorresponding worsening
of condition(2.3) (see
Section4.5).
Proposition
1 isclearly interesting only
forsufficiently high E;
in thiscase the
expression (2.9) for P essentially
readsIn the next subsections we illustrate some consequences which can be drawn from
Proposition
1.2. 2. General consequences
Let us discuss the basic estimate
(2.8).
Thequantity
thereappearing
isuniformy
bounded: forexample, by (2.4)
and(2.3)
one hasThe
function P
remains instead small over aquite large interval, growing exponentially
with/E:
one has forinstance P (x) ~ (30,
with
as far as
Consequently,
for x in thisinterval,
the estimate(2.8) gives
II
w(x)-w (x) II
2Po ~u~ = (!) (I
V On the otherhand,
from(2.4)
and(2.7), using also I ~M~ = 1,
one obtainsIn
conclusion,
forI
~ ~
satisfying (2.11)
one getsIn -turn, the
phase
cp(x)
satisfiesBy
the way, we also notice that in intervals shorter than(2.11),
forinstance
Annales de l’Institut Henri Poincare - Physique " theorique "
one could
replace (2.12) by
anexpression
accurate up to order1 +m/2
inI
V(one
needsapproximations
for T accurate to order1 + m/2,
see theabove
remark).
Another
general
consequence ofProposition
1 is anexponential
estimateon the
Lyapunov
exponent(when
it isdefined)
of theSchroedinger equation [11]. Indeed,
from(2.7)
and(2.8)
one gets, for any solution w, and thusthis
gives,
for the(maximal) Lyapunov
exponent~+
of theSchroedinger equation,
theexponential
bound2. 3. The
scattering problem
We shall now discuss the case of a
potential V (x)
whichdecays
suffi-ciently rapidly
for x -+ ± oo;precisely,
weneed
p -+ 0 for x -+ ± oo,with
~+00
dx = C oo. From(2.8), (2.9)
one hasthen,
for any XEf~,
this means that the
approximate
solution w is now close to w for anyx
e [R,
and moreover, the error isexponentially
small inE.
Let us then
investigate
theproperties
of w.Clearly,
for x -4> ± 00 one has T(x)
-4>1,
while the limitsf.. /
I} 1
r :t 00
B h.are finite
actually,
03B3±~2E J(
VBy choosing
in
(2.7),
anddenoting
y=y+2014y-, oneimmediately deduces,
for=(, 1 E ’),
theasymptotic
behaviorwith a
corresponding expression
for-BIt’ (’).
Inparticular,
for either a or bvanishing, (2.20) represents
apurely
left- orright-travelling
wave, with noreflected wave, and small
phase-shift
03B3~1
-
From these
approximations,
we shall now deriveexponential
estimatesfor the
scattering
matrix and the reflection coefficient[14].
Thescattering
matrix
corresponding
to(2.20)
is the trivial matrix§==( B 0 ~ ~/ ; using (2.18)
one can then say that the truescattering
matrix S
(which
is known to existessentially
in ourassumptions,
see forexample [19])
differs fromS by
aquantity exponentially
small in/E:
forexample,
it is not difficult to getin
particular,
the reflection coefficient R turns out to be boundedby
2.4.
Slowly decaying potential
Let us here consider the case of a
potential
whichdecays
to zero, forx ~ ± 00, in a non
integrable
way; to bedefinite,
assume(1+H)~
forlarge
One can see, from(2.8)
and(2.9), that,
although
w now is notuniformly
close to w, nevertheless the error remains for anextremely large interval, growing
withE
essentially
as exp exp~.
In ashorter,
stillexponentially large interval,
one gets
instead,
as in thescattering
e)
Be aware that is just a notation for the second component of w: although’,
according g to (2.8), approximates
03C8’=d03C8,
in general it does not coincide with2014.
dx dx
Annales de l’Institut Henri Poincaré - Physique theorique
Concerning w,
one can notice that it does notproperly reduce, asymptoti- cally,
to apair
ofplane
waves, because thephase
shift nowdiverges logarithmically with
xj.
However, if one accepts to restrict the attention to a finite butlarge interval, growing exponentially
withE,
then thephase
shift isfinite,
and the"asymptotic"
behavior is like in(2.20),
Onthis finite but
large scale,
the overallpicture
isessentially
the same as inthe
scattering problem.
2.5.
Quasi-periodic potential
To treat this case, we assume that the
potential
fulfills thefollowing
two conditions
(which
are also needed in the KAMapproach [15]-[18]):
(i)
V isquasi-periodic
in x, with realfrequencies
0)1, ... ,by this,
we mean that one has ... , for all the func- tion ... "
being analytic
and203C0-periodic
in eachof its
arguments;
(ii)
thefrequencies
..., OOnsatisfy
theDiophantine
conditionfor some
positive
constants c and T.We shall denote
by
the Fourier coefficients ofV,
definedthrough 1/ (PI’ ...,(?~)= ~
similar notations will be used for the otherk~Zn
quasi-periodic
functions.From the
general theory
of Section 2.2 we know that the actual solutionw of the
Schroedinger equation
differsby quantities
from theapproximate
solution w definedby (2.7),
over distancesWe now prove
that,
in the presentcase, w
is aquasi-periodic
function of x, with n + 1frequencies
(00’ ro1, ..., where~o ( E) _ ~ + C~ ( 1 /~) .
To this purpose, we first observe
that,
under condition(i),
the functionsV (x)
andT (x)
ofProposition
1 turn out to bequasi-periodic,
with thesame
frequencies
asV(x) [indeed,
thisimmediately
follows from thecorresponding
statement in Lemma 2 of Section4,
if one takes intoaccount the very construction of
V (x)
andT (x)]. Furthermore, by (2.6)
the
phase
cpentering
theexpression (2.7)
for w can be written aswith
Now, using
thequasi-periodicity
ofV,
and also theDiophantine
condition(2.22),
oneeasily
proves that 9 isquasi-periodic
too, with the samefrequencies
as V:indeed,
one hasclearly
and,
as is wellknown,
theDiophantine
condition assures the convergence of the series.Moreover,
theexpression (2.23)
for cp shows that the addi- tionalfrequency
which enters w besides thefrequencies
(01’ ..., (On of thepotential,
isgiven by
in agreement with the above statement.Let us now consider more
closely
theapproximate
solution w.First,
one can
produce
a more accurateexpression
for thefrequency
(00’precisely
This
expression
is obtained from the one aboveby using
the relationV~=V~+~(1/E),
which follows from(use
is made of the fact that the flow ..., onTn is
ergodic).
Furthermore,
one caneasily verify
thatw = B)/, 1 B)/)
is a linearcombination of "Bloch waves" with
frequencies
03C90, 03C91, ... , i. e.... , ... ,
(2. 28)
the functions
being 203C0-periodic
in each argument. It is alsopossible
to show that
B)~==1+~(1/E). Indeed,
from theexpression (2.25)
for8, using
standardtechniques
and the relation(2.5),
one can estimateI
as
Annales de l’lnstitut Henri Poincare - Physique - theorique -
C = C
(c,
’t, n,p) being
a suitable constant(for instance, using
the estimatesof refs.
[20], [21],
one getsC = c-1 ~j(2t)f).
One theneasily finds, using ( 2. 7), ( 2.4), ( 2. 23), ( 2. 26)
and(2.29):
From this
analysis,
one concludes that the solutions of theSchroedinger equation
withquasi-periodic potentials
have thefollowing
structure, over distances(!) 1 ex p N : E
u p toquantities
of orderl/E they
resemble(linear
combinationsof)
Bloch waves(2.28),
which in turn differ from thefree solutions
by quantities
of order1/)E.
3. THE HAMILTONIAN
THEOREM,
AND PROOF OF PROPOSITION 1
3.1. Statement of the Hamiltonian theorem
The
proof
ofProposition
1 is obtainedby regarding
theSchroedinger equation
as adynamical
system,namely
an harmonic oscillator withfrequency [E - V (x)] 1~2 depending
on the "time" x. To this system weapply
a Nekhoroshev-likeperturbation theory, leading
to theexponential
estimates.
It is
convenient,
in ourperturbative approach,
to use canonical coor-dinates
related
toBj/, B)/
=by
dx
M
being
the matrix introduced inProposition 1;
theSchroedinger equation
( 1.1)
is thenimmediately
seen to beequivalent
to the canonicalequations
corresponding
to the Hamilton functionprecisely
The Hamiltonian
H,
as well as all functions we will dealwith,
is defined for(p,
q, and is real if x is real andq = - ip.
The corres-ponding reality
condition for linear transformations of the form(pq)=T(x) (p’q’), T (x) being
ananalytic
2 x 2matrix,
is that the relation ispreserved
for any real x; inparticular,
this conditionguarantees that,
after the substitution(p, q) H (p’, q’),
the new Hamiltonian is still real for real x and~=2014~/.
Suchreality
conditions will beimplicitly assumed,
wheneverworking
with the p, q coordinates.Proposition
1 turns out to be a direct consequence of thefollowing
PROPOSITION 2. - Consider the Hamiltonian
(3. 2),
Vbeing
realanalytic
in
// p’
and assumeE ~ 51
VIp.
Then there exist a 2 x 2analytic
matrixT
(x),
and twoanalytic functions V (x)
and F(x),
such that:(i)
T is close to theidentity, as in (2.4);
(ii) V is
close toV, as in (2.5),
while F isbounded by (iii)
thetransformation
is canonical
and, for
x EIR, gives
the new Hamiltonian H’the form
3.2. Proof of
Proposition
1We defer to the next Section_ the
proof
ofProposition 2,
and show here how one can use it to proveProposition
1. To this purpose, let us write theequations
of motion deduced from(35)
in the vector formAnnales de l’lnstitut Henri Poincaré - Physique theorique
where ~==(~ q’),
andFrom
(3.6)
one first works out thepreliminary
estimateThis
inequality
can be achievedby introducing
a variabler~ =e-‘~ ~x~ ~,
whose
equation
of motion isimmediately
seen to bed~ d~ =e-i03A6Bei03A6~
(one profits
here of the fact that the matrices 03A6and commute);
fromthis
equation
onededuces - 2014 11111121
which in turn,using
~03B6~=~~~, gives (3.8).
Let us then write(3.6)
in theintegral
formUsing ( 3. 8)
inside theintegral,
one getsand since one obtains
P being
definedby (2.9). Finally,
if one recallsand denotes one finds
(2.7) and (2.8),
withhas also been used. The
proof
ofProposition
1 iscomplete.
4. PROOF OF PROPOSITION 2
4.1. An
equivalent
autonomous systemAs a
preliminary
step in theproof,
wereplace
the non-autonomous Hamiltonian( 3. 2)
with anequivalent
autonomous one,having
one moredegree
of freedom. To this purpose, we consider x as adependent variable,
with
equation
of motion x =1 and initial datum x(0)
= 0; one then immedi-ately recognizes
that the non-autonomous Hamiltonian( 3. 2)
isequivalent,
for what concerns the variables x, p and q, to the autonomous one
K (p, q, y, x) = y + H (p,
q,x), y being
the momentumconjugated
to x.We shall work out, in the extended
phase space ~ 3
x!/ p’
a canonicaltransformation ~ which preserves the property x= 1 and extends
(3.4), namely
of the formwhere one has denoted
~~~3c)=~~~~x’);
the matrix T isobviously required
to have theproperties
stated inProposition 2,
while h is a suitableanalytic
function. The new Hamiltonian will berequired
to have the formK’ (p’, q’, y’, x’) = y’ + H’ (p’, q’, x’),
H’having
the form and the
properties
stated inProposition
2.4. 2. The
algebraic
frameworkLet us denote
by j~p
the space of allanalytic
functions:~p -~ C;
forand any
p’ ~
p, we shall use the localnorm
p’ introduced in Section 2. If let us defineF* (x) = F (x);
one hasclearly
and
20142014
= 2014 .Throughout
theproof
we shall beprimarily
concerneddx
dx
/g p p y
with
homogeneous polynomials
ofdegree
two in pand q,
with coefficients in inparticular,
a basic role will beplayed by
the spaces( GG p 77
and "m" are abbreviations for"pure"
and"mixed").
We shall alsoconsider the space
Ap
=Ag
QA;,
and denoteby TIP,
IIm theprojections
from
Ap
toAg
andrespectively A;.
Forf belonging
to eitherAp
orAP,
and any
p’
p, we shall use the normI f I x,
P, =I
FIx,
p" while forf E Ap
wedenote
I f lx,
p’ _|03A0pf|x,
p’ +I
TImf Ix,
p’.Annales de l’Institut Henri Poincare - Physique theorique
Functions f E Ap
will be alsoregarded
asy-independent
functions defined in the wholephase space 3
x03C1. Denoting by { , }
the usual Poissonbracket,
oneimmediately
deduces thefollowing elmentary algebraic
rela-tions :
and also gets the basic estimate
for any
f, gEAp,
anyp’ _
p and any4. 3.
Elementary
canonical transformationsThe canonical transformation is obtained as the
composition
of afinite number of
elementary
canonical transformationsgenerated by
theLie
method, namely
as the time-one map of a suitableauxiliary
Hamil-tonian
flow;
we shall use, in thephase space 3
xf/ p’ y-independent auxiliary
Hamiltoniansbelonging
toAP.
Theproperties
of theelementary
canonical transformations
generated
in this way are stated in thefollowing
LEMMA 1
(on
canonicaltransformations). - Consider,
in thephase-space C3 x 9’p,
theHamiltonian ~=1 X x 2 - !X* x 2
and denoteb
O4
~ )p
4
~ )
q p~ ythe
corresponding
time-one map. Then:(i)
O is ananalytic
canonicaltransformation of ([3
x ontoitself, of
the
form
(ii)
The operatorL = {~, .}
isbounded by
for
anyf
EAP,
any x E IR and anyp’ _
p.Furthermore, if f
EAP,
then onehas
f0398
=(exp L) f
EAp,
theexponential being defined by
its series, whichis convergent.
(iii)
The 2 x 2 matrix i isanalytic
in f/ p, andfor
anyp’ _
p itsatisfies
the estimate
while K E
Ap
isgiven by
Proof. -
Theequations
of motion associated to x arethe flow is
certainly
defined and invertible for any initial datum in C3 x!/ p
and any
time,
and inparticular
at t= 1 it has the form(4.5).
A trivialinte g ration gives 03C4=exp1 2(0 X 0 / ),
andconsequently (4.7).
Considernow f~039B03C1.
Theinewquality ( 4. 6)
follows from( 4. 4);
on the otherhand,
..
00
1 ~ .
one and the series converges for any fixed x.
Finally, (4.8)
is an obvious consequence of{~ .Y~
== 20142014. N
ax
4. 4. The iterative lemma It is convenient to use here the two
parameters
We aim to construct a sequence "
Oi,
...,0N
ofelementary
canonicaltransformations of
C3
x~P
onto 0itself,
suchthat, denoting
£Ko=K
and ’S = 1,
...,N,
one " haswhere is
analytic
in E, whilefs~039Bp03C1
isanalytic
in E, and divisibleby ES.
We
proceed iteratively,
anddetermine fs+1, gs+1 in
terms gs; moreprecisely, denoting
ð =p/N,
andwe work
out iterative estimatesfor | fs x,
Psand |gs|x,
ps. Let us noticethat
Ko
has mdeed the form{4.10), with |110
x, PO= |g0 |x,
po= I V |x,
P. Our estima- tes are stated in thefollowing
LEMMA 2
(Iterative Lemma). -
LetKs
be as in(4.1©),
sN,
withgs E
A: analytic
an E and~s
EA: analytic
in E and divisibleby
Es. ~,etpo, ... , PN be
defined by (4.11 ).
Then there exists a canonicaltransforma-
tion
0398s+
1 of(:3
x ontoitself,
such that:(i)
The new Hamiltonian has theform (4.10),
withgs+ 1 E
A; analytic
in E, and 1 EA: analytic
in E and divisibleby
ES+1;
Annales de l’Institut Henri Poincare - Physique theorique
Denoting
one has and(iii) Denoting
one , has x’ = x and 1with
Moreover,
if gs and fs
are ’quasi-periodic
in x,with frequencies 03C91,
... , ron(in
the , sense ,of S ection 2.5),
then so are gs+iProof -
We use Lemma *1, choosing
j ~ such thatf~ + ~
does notcontain terms of order ES. Let us denote one ’ can write
We
determine x
in such a way thatdenoting
that We then obtain of the form
(4.10),
with
Let us now estimate 03A0m03BA on the basis of its
expression (4.8).
First ofall,
since
using
thealgebraic
relations(4.3)
one obtains~ ~
nm K = -
L~ -~.
On the otherhand,
since X is assumed to~=2.4.... ~ ~
be
analytic
inf/ p’
its derivative is alsoanalytic
in9~; Cauchy inequality gives
thenõ - 1
and thus|d~ dx |
x,03C1s+1 ~
õ -(this
estimate is the
only point
whereanalyticity
is everused!). Using
the basicestimate
(4.4),
one thenimmediately
getsIn a very similar way one can estimate
03A0p 03BA,
as well as the sumsentering (4.15);
as aresult,
theinequalities (4.12)
are found.Concerning point (iii)
of the statement, it is a trivial consequence of theinequality (4.7)
of Lemma1, together
with the estimate|~|x, 03C1s=1 2(~ ~)
2|fs|x,
03C1x. To prove the last statement, one observesthat ~
is
quasi-periodic whenever~ is;
as a consequence, the matrix isquasi- periodic
too,and,
moreover, since the Poisson brackets preserve thequasi- periodicity,
the series(4.15)
definequasi-periodic
functions..4.5. Conclusion of the
proof
On the basis of Lemma
2,
theproof
ofProposition
2 iseasily accompli-
shed. Let us look at the recurrent estimates
(4.12),
andproceed,
for amoment,
heuristically, by considering
theasymptotic
behavior forThe first
inequality reduces,
in thisapproximation,
toFs+1 ~N 2 ~03C1 Fs,
whichgives (recalling ;#’0= 1) IFN (~N 2 ~03C1)N.
Asimple
computation
shows that theoptimal
choice ofN, namely
the choice which makes minimalFN
for eachgiven
E, 11 and p, is N=20142014 ] = [ ; p JE J
where[.]
denotes theinteger
part;correspond- ingly,
one has(still
within this heuristicprocedure) FN exp- [0153p JE],
with
a=2/~. Passing
now to arigorous analysis,
thesimplest (although
notcompletely optimal) procedure
is toslightly
lower 0153,taking
forexample
a== ,
L~.N = NE == [~
p infact, using
this value of N in(4.12),
Henri Poincaré - Physique théorique
e)
andassuming E2 ~ ~ (f.
~.,E ~ 51
V oneeasily verifies, by induction,
the
following
recurrentinequalities:
If we denote
i V [F ( x )h 2 - F* (x) 2
then we see2 4
that has indeed the form
K/=~+H’,
with H’ as in( 3. 5);
inparticular,
F andV satisfy
part(ii)
of the statement.Concerning
theinequality
in part(i),
it is an easy consequence of(4.13). Indeed,
one hasT(X)=’t1 (x)
i2(x)... iN (x); using (4.13),
and theinequality
N
!!~i~2’ ’ Ft (1 + II ’ts-III) -1,
which isimmediately
verified(by
s=o
induction on
N)
for any set ofmatrices,
one obtainsfor any real x. This concludes the
proof
ofProposition
2.5. TESTING THE OPTIMALITY OF OUR PERTURBATIVE APPROACH
As remarked in the
Introduction,
we devoted some attention to theevaluation of the constants
appearing throughout
the paper, withspecial
care for the
expression
ofNE.
In the statement ofPropositions
1 and2,
one finds
(forgetting
here theinteger part) however,
as commented after the statement ofProposition 1,
one could obtain(for sufficiently large E) JE,
abeing any
number smaller than2/e.
Itis
clearly interesting
to know whether this value of a, which is obtained at the end of a ratherlong
chain ofestimates,
isnevertheless,
so tospeak, reasonably good.
(2) Apparently, according to (4.11), one should impose N ~ 1, i. e.,
E ~ 1 4
03C12: but ofcourse, for smaller E the statement of Proposition 2 is trivially true, with T = 1, V==V and H’=H.
To this purpose, we made two different tests:
(i)
in the case of thescattering,
wecompared
our estimate for the reflection coefficient R(Sect. 2.3)
with the results of rather accurate numericalcomputations; (ii)
for a
periodic potential,
wecompared
our estimate from above for theLyapunov
exponents, which in turnimplies
an estimate from above for thelength
of thespectral
gaps[22],
with acorresponding
estimate frombelow,
taken from thetheory
of Hill’sequation.
(i)
Resultsof
thefirst
test. - We haveperformed
some numericalcomputations
of the reflection coefficient Rwhich, according
to ouranalysis
of Section2.3,
isexpected
todecay,
forlarge E,
asWe have considered the
following
fourpotentials:
Potential
(i)
has twopoles
in x = :t i, so that one hasp = 1;
forpotential (ii)
one hasinstead p= !.
Potential(iii)
has morepoles,
withp = 1,
andfinally, potential (iv)
is likepotential (i),
but with additional oscillations.The
Figure
reports the results of the numericalcomputations, namely -log(|R|E) versus E.
In agreement with(5.1),
one findsstraight lines,
ofslope
The value of a, and thus of (x, are rather welldefined;
as a remarkablefact,
the threepotentials
withp = 1
showexactly
the same
slope ~ ~ 2.02,
while forpotential ii (for which - 1
onehas instead ~ ~ 1.01. These values should be considered with some care;
in
particular,
we are not able toperform
any reasonable erroranalysis.
Nevertheless,
one has thestrong impression
that the law a = ap is correct, with the same a for all of the abovepotentials;
infact,
one is eventempted
to say that 03B1 = 2 is a kind of universal constant, say for a convenient class of
scattering potentials.
This value must becompared
with a =2/e, produ-
ced
by perturbation theory.
(ii)
Resultsof
the second test. - Underassumptions
weaker than ours,one can prove
[22]
that(for sufficiently large
values ofE)
if the solution of theSchroedinger equation ( 1.1)
has aLyapunov
exponent less than a Annales de l’Institut Henri Poincaré - Physique theoriqueIllustrating the results of the numerical test for oc.
number ~ 1,
then the distanee d of E from the spectrum of the Schroedin- ger operator is boundedby (here
and in thefollowing, C1, C2,
... denote convenientpositive constants).
Consider then thespecial
case of the Mathieuequation, V(x)=cos(2x);
from our estimate(2.17), taking (as
ispossible
andconvenient)
p such that the conditionE ~ 51 (Proposition 1)
isstrictly fulfilled,
oneeasily
findsOn the other
hand,
from thetheory
of the Hill’sequation ( see
refs.[ 1 ], [23]),
one knows that there exist gaps in the spectrum atarbitrarily high
energy; moreprecisely,
for any natural number n there isa gap around
n2, having length
D ~(C3 n~ - 2
" ~(C4 JE) - 2
Thecomparison
between d and D shows that a cannot exceed2;
as a remark- ablefact,
this isexactly
the same value obtainednumerically
in the caseof
scattering, i.
e. with asubstantially
differentpotential.
Asbefore,
thisvalue must be
compared
with our limit valuea=2/~.
These results suggest that a = 2 is