A NNALES DE L ’I. H. P., SECTION A
G EORGE A. H AGEDORN
Semiclassical quantum mechanics, IV : large order asymptotics and more general states in more than one dimension
Annales de l’I. H. P., section A, tome 42, n
o4 (1985), p. 363-374
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363
Semiclassical quantum mechanics, IV:
large order asymptotics and
moregeneral states
in
morethan
onedimension
George A. HAGEDORN (*)
Department of Mathematics, Virginia Polytechnic Institute
and State University, Blacksburg, Virginia 24061-4097
Vol. 42, n° 4, 1985, Physique theorique
ABSTRACT. - We solve the n-dimensional time
dependent Schrodinger equation i~03A8 ~t = - 2014
AT + V’P modulo errors which have L norms on the order of forarbitrary large
1. The initial conditions arefairly general
states whoseposition
and momentum uncertainties are propor- tional toh1~2.
RESUME. - On resout
1’equation
deSchrodinger dependant
du tempsd ~ h2
i
2014
= 2014 2014 AT + VT en dimension n modulo des erreurs dont lanorme dans L2 est d’ordre pour 1’arbitrairement
grand.
Les conditionsinitiales sont des etats relativement
generaux
dont les incertitudes deposition
etd’impulsion
sontproportionnelles
ah1~2.
§
1. INTRODUCTIONIn this paper we
study
thehigh
order semiclassicalasymptotics
ofsolutions to the n-dimensional time
dependent Schrodinger equation
(*) Supported in part by the National Science Foundation under grant number MCS-8301277.
Annales de l’Institut Henri Poincaré - Physique theorique - Vol. 42, 0246-0211 85/04/363/12/$ 3,20/CQ Gauthier-Villars
~2014= -2014A~F+V~F.
We show that there exist solutions which are concentrated near thetrajectory
of a classicalparticle
up toerrors which are on the order of ~1~2 for
arbitrarily large
l.These results are
generalizations
of some of our earlier work[3] ] [4] on
Ithe semiclassical limit of
quantum
mechanics. In[3] ] we
showed that thereare
approximate
solutions to the n-dimensionalSchrodinger equation
which are accurate up to errors on the order of ~1~2. In
[4] ]
we showedthat in one
dimension,
there areapproximate
solutions which are accurate up to errors on the order of~1~2
forarbitrary
l.Thus,
the present papergeneralizes [3] ]
tohigher
dimension and[4] ]
tohigher
order. The gene- ralizations are notstraightforward
because it is far from clearjust
whatthe n-dimensional
analogs
of the functions of[4] ]
are.They
are notsimply « products
of Hermitepolynomials
of variousarguments multiplied by
aGaussian »,
as stated in[4 ].
Thecomplication
comes fromthe fact that the
complex unitary
groupU(n, C)
enters in theproblem
where one
might
expect to see the realorthogonal
group0(n, [R).
Thisforces one to
study
somegeneralizations
of the usual Hermitepolynomials.
Once one knows that these functions are, the
generalization
of[4] is
imme-diate.
The
approximate
solutions which westudy
have momentum andposi-
tion uncertainties on the order of
~1~2.
Thisparticular
semiclassical limitwas first studied
by Hepp [9 ],
whocomputed
the first term in the small ~asymptotics
of certainexpectation
values. In thechemistry literature,
Heller[7] ]
used theapproximation
of the same type, withoutstudying
the
question
of whether or not theapproximate
solutions wereasymptotic
to exact solutions. He and Lee have also
proposed [8 an approximation
similar to the one in
[4] and
the one we describehere,
but he has not foundthe natural orthonormal basis in which to do the
expansion.
Ralston[10]
has studied
approximate
solutions tostrictly hyperbolic
systems ofpartial
differential
equations.
His results are similar to the ones which we presentbelow,
but heexpands
theapproximate
solution in terms of a non-ortho-gonal
basis for which leads to morecomplicated
evolution equa- tions for the coefficients in theexpansion.
Other semiclassical limits are studied in the literature. In this
regard,
we recommend the reader consult the work
of Yajima [7~] ] [15 ].
The timeindependent problem
for limits similar to ours has also been studied.The reader should consult the works of
Combes,
Duclos and Seiler[1] ] [2 ],
and Simon
[77] ] [12 ].
For the
potentials
which weconsider,
thequantum
HamiltonianH(h) = - 2014 A
+V(x)
= + V on isessentially self-adjoint
on the2m
l’Institut Henri Poincaré - Physique theorique
functions of compact support. Under this Hamiltonian we will
study
the evolution of states which are linear combinations of the wave functions
~k(A, B, ~,
a, ~x),
which are defined below. The state~k(A, B, ~,
a, yy,x)
is concentrated near the
position
a and near themomentum 11.
Itsposi-
tion
uncertainty
isproportional
to and is determinedby
the matrix[AA * ]1/2
and the multi-index k. Its momentumuncertainty
isproportional
to~1~2,
and is determinedby
thematrix [BB* ]1/2
and the multi-index k.
The
precise
definition of the states~k(A, B, ~, a, r~, x)
isquite compli- cated,
andrequires
thefollowing
notation :Throughout
the paper we will let n denote the space dimension. A multi- index k =(kl, k2, ... , kn)
is an orderedn-tuple
ofnon-negative integers.
n
The order of k is defined to
be |k| = ki,
and the factorial of k is definedf=i
to be k ! =
(/(i !)(k2 !)
...(kn !).
Thesymbol
Dk denotes the differentialolkl
operator Dk -...
symbol xk
denotes themonomial xk = xlkix2k2
... We denote thegradient
of a functionf
and we denote the matrix of second
partial
derivativesWith a
slight
abuse ofnotation,
we view M" as a subset ofCn,
andlet ei
denote the ith standard basis vector in ~n or ~n. The inner
product
on !R"Our
generalizations
of the zeroth and first order Hermitepolynomials
areand
where v is an
arbitrary
non-zero vector in en. Ourgeneralizations
of thehigher
order Hermitepolynomials
are definedrecursively
as follows :Let vl, v2, ...,~ be m
arbitrary
non-zero vectors in en.Then,
One can prove
inductively
that these functions do notdepend
on theordering
of the vectors ...,~.Furthermore,
if the space dimen- sion is n = 1 and the vectors v2, ...,~ are allequal
to 1 then~2? ’ ... ,
x)
isequal
to the usual Hermitepolynomial
of order m,Hm(x).
Now suppose A is a
complex
invertible n x n matrix. We defineI A I = [AA* ]1/2,
where A* denotes theadjoint
of A.By
thepolar decompo-
sition
theorem,
there exists aunique unitary
matrixUA
so that A=
Given a
multi-index k,
we define thepolynomial
We are now in a
position
to define the functions~(A, B, ~ ~
11,~).
DEFINITION. - Let A and B be
complex ~
x ~ matrices with the follow-ing properties:
A and B are
invertible; (1.1)
is
symmetric ([real symmetric]
+i [real symmetric]); (1.2)
Re
BA -1 = 1 2 [(BA -1)
+(BA -1)*] ] is strictly positive definite; (1.3)
=AA*.
(1.4)
Let a E
Rn, ~
ERn,
> O. Then for eachmulti-index k,
we defineThe choice of the branch of the square root of
[det A ] -1
in this definition willdepend
on the context, and willalways
bespecified.
Remarks.
1. Whenever we write
B, ~ ~ ~ x),
wetacitly
assume that the condi- tions( 1.1 )-( 1. 4)
are fulfilled.2. Condition
( 1. 4)
can be rewriten in a moresymmetrical
way. It isequivalent
to the conditionwhere I is the n x n
identity
matrix.3. We prove in
§
2 that for fixedA, B, ~C, a,
and r~, the functionsa, yy,
x)
form an orthonormal basis of4.
Generically, UA
andUB
arecomplex unitary matrices, and I A I and I B
are Hermitian. In thespecial
cases in whichthey
allhappen
tobe
real,
the functionsB, ~, 0, 0, x)
aresimply rotated,
scaled versions of theeigenfunctions
of the n-dimensional harmonic oscillator.Annales de l’Institut Poincaré - Physique theorique
5. The scaled Fourier transform which is
appropriate
for the semi- classical limit isIn
§
2 we prove that6. In the definition of the functions
~k(A, B, ~, a,
yy,x),
theonly place
inwhich the matrix B appears is in the exponent.
Similarly, ~k(B, A, ~,
~ - a,ç) depends
on the matrix Aonly through
theexponential
factor. This property is crucial to ourproofs.
It also makes the result of Remark 5 ratheramazing.
The main result of this paper is the
following :
THEOREM
for some constants
C1, C2,
and M. Let ao E~n, ~n,
and letAo
andBo
be n x n matricessatisfying (1.1)-(1.4).
Given apositive integer J,
aposi-
tive real number
T,
andcomplex
numbers ckfor J,
there exists aconstant
C3
such thatwhenever
T(det A(t))
is never zero, and the branch of the square root in the definitionB(~), ~ a(t ), r~(t ), x)
is deter-mined
by continuity
int ).
Here[A(t ), B(t ), a(t ), r~(t ), S(t ) is
theunique
solu-tion of the system of
ordinary
differentialequations :
subject
to the initial conditionsA(0)=Ao, B(0)=Bo, ~(0)=~o.
and4-1985.
S(O)
= O. The~)
are theunique
solution to the system ofcoupled ordinary
differential
equations
subject
to the initial conditions~)
= ckfor
J and~) ==
0for J + 1
~
In thisequation,
thequantity
is a numericalquantity
which iscomputed
in the remarks below.Remarks.
1. The
quantity
is aproduct of
somequantities
which are relatedto the
symmetric
tensorrepresentations
of thematrices A UA,
andUA.
To
explicitly
compute thesequantities,
we need some notation. Given a sequence ofintegers i ~ , i2, ... , iN
whichsatisfy 1 ~ ~ ~ ~
we defineind
(i 1, i2, ... , iN)
to be the multi-index k with the property that thenumber}
occurs in the
sequence i1, i2, ... , iN, exactly
times. Let A be a non-singular complex n
x nmatrix,
and let k and m be multi-indices withI = !
We fix~,72....Jj~)
so that ind(/ij2....~t~j)
= m, anddefine
In
addition,
and m be any threemulti-indices,
and choosei 1, i2,
... ,iN
withind (i1, i2, ... , iN)
= k. Then we definewhere l, x’ix’2
... denotes the matrix element of ...in the usual harmonic oscillator basis
(i.
e., theI, 1, 0, 0, ~)}).
With these
definitions,
the numericalquantity
which appears in the theorem is :2. The
quantities
in the above remark arise from thecomputation
ofthe matrix elements
These matrix elements do not
depend
on a and thedependence
Annales de l’Institut Henri Poincaré - Physique . theorique -
scales out to
give
a factor of TheUA dependence
is in thequantity
It enters the
computation through
the formula :The I A dependence
is in thequantity
All of these formulas may be
proved by using
the definition of,
~, x), induction,
andexplicit computation.
3. As in
[3] [4] ] [J] ] [6] ] [13 ], A(t )
andB(t)
are determinedby
the relations4. One can prove another theorem which allows some infinite linear combinations of the functions
B, ~, x)
if one iswilling
to docomputations
modulo errors on the order of ~1~2. We have not stated this theoremhere,
since it is the obviousanalog
of Theorem 1. 2 of[4 ].
Giventhe results of
§
2 of the present paper, it is easy togeneralize
theproof
ofTheorem 1. 2 of
[4] ]
to the n-dimensional case.5. One can
generalize
Theorem 1.1 to include moregeneral
Hamil-tonians. Hamiltonians which are
arbitrary
smooth functionsand t can be accommodated. In
particular,
one can includemagnetic fields,
or one can
study problems
with timedependent potentials
which are qua- dratic in x andp (jointly).
See e. g.,[5] ] [7~] and [6 for applications
of theseideas.
In the rest of the paper we
give
the technical details necessary for theproof
of Theorem 1.1. We do notactually give
aproof
of thetheorem,
since many of the steps arevirtually
identical to theanalogous
steps in the 1-dimensional case.§ 2 .
THE TECHNICALITIESIn this section we
give prooTs
of the crucial lemmasinvolving
theproperties
of the functionsB, ~,
a, ri,x).
We also present a veryrough
outline of the
proof
of Theorem 1.1. We do notgive
the fullproof
because(once
the lemmas areproved)
it isessentially
identical to theproof
of Theo-rem 1.1 of
[4 ].
LEMMA 2.1. - The functions
~k(A, B, ~, a, r~, x)
form an orthonormal basis ofProof 2014 By scaling
outthe dependence
of the functions~k(A, B, h,
a, 11,
x),
we needonly
prove this lemma for the case inwhich ! I A
== I.Furthermore,
because of relation( 1. 4),
the value of B is irrelevant in thecomputation
of innerproducts
of the with one another.So,
we canassume B =
I,
also.Similarly,
it is sufficient to consideronly
the caseof ~
= 0 and = 1. Let =UAej
for 1j
n. Define to be thedifferential
operator ~(w~) ==~~)+~,V)
defined on the Schwartz space~(tR"),
and let be itsadjoint.
On Schwartz space, actsas the differential operator
a(w~ )* _ ~
w,x ~ - W j, V ~.
Theself-adjoint
operators
N(w)
= for 1~ ~’
=$ ~ areeasily
seen to commutewith one another.
Suppose
...~ are chosen from the set(Wj).
Then, by explicit computation.
and
From these relations it is easy to see that
Thus,
v2, ... , is aneigenfunction
ofN(wj)
witheigen-
value
equal
to twice the number of occurrances of Wj in the sequence v 1, v2, ...~. Since this is true foreach j,
and the arecommuting self-adjoint operators,
the functionsB, ~, a,
~,x)
areorthogonal.
The function v2, ... ,
x)e - "2~2
isequal
toso
using
the relationsgiven above,
one caneasily
see that the functionsare
properly
normalized.To prove the
completeness
of the functionsB, ~,
a, 11,x),
one shouldn
note that the
operator N(w~) = 2014
11 +jc~
issimply
twice the usualj=i
Poincaré - Physique theorique
Harmonic oscillator Hamiltonian. The states
B, 1, 0, 0, x)
areeigen-
functions
if I A = I,
and for eacheigenvalue,
oneeasily
sees that thereare as many
B,1, 0, 0, x)’s
as the dimension of thecorresponding eigenspace.
IIProof 2014 By elementary manipulations,
it is sufficient to consider thecase
~=1,~=~=0.
For thecases k ~ = 0,1,
we prove the lemmaby explicit
calculation. For the
larger
values we use induction and thefollowing
two formulas :
and
The
only
difficultstep
in the induction is thefollowing :
Assume thelemma is correct for all multi-indices m
with M,
and let k be a multi- indexwith |k =
M + 1. Choosevectors vj = eij
for 1j
M +1,
so that ind
(fi, i2,...,iM+1)
= k. LetUAvj, wj = UBvj,
andwhere and
By
the inductionhypothesis,
this isequal
tode Poincaré - Physique theorique
With one
exception,
all the steps are eitherstraightforward applications
of standard facts about the Fourier transform or
applications
of the iden-tities
given
above. Thatexception
occurs in the second to last step, wherewe have used the
identity :
By using
thepolar decompositions
of A andB,
we see that thisidentity
is
equivalent
to the firstequality
in theidentity
This
identity
isproved
as follows :By
condition( 1. 2),
we have BtA = AtB.If we take inverses on both sides of this
equation,
we obtainAs in Remark 2 after the definition of the
~k’s,
condition( 1. 4)
isequivalent
to A*B + B*A = 21. We
multiply
thisidentity
on theright by
the twoforms of the matrix C to obtain the desired
identity.
ttGiven the two lemmas
above,
theproof
of Theorem 1.1 is obtainedby closely mimicking
theproof
of Theorem 1.1 of[4 ].
One uses the TrotterProduct Formula to separate the effects of the kinetic and
potential
termsin the Hamiltonian. Then one
expands
thepotential
in itsTaylor
series oforder l + 1 about the
point a(t ).
The errors committed are of order~~~2
due to the
dependence
of the functions03C6k(A, B, , a,
11,x).
The terms oforder less than or
equal
to 2 in the kinetic energy and theapproximate potential give
rise to theequations ( 1. 6)-( 1.10).
Thehigher
order termsfrom the
approximate potential give
rise to the system(1.11).
There isan additional error of order ~~~2 due to the fact that we have truncated the
sums which occur in the system
( 1.11 )
in order to avoiddealing
with aninfinite system.
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( M anuscrit reçu le 10 août 1984)
Annales de l’lnstitut Poincaré - Physique theorique