A NNALES DE L ’I. H. P., SECTION A
U GO M OSCHELLA
Classical limit of a quantum particle in an external Yang-Mills field
Annales de l’I. H. P., section A, tome 51, n
o4 (1989), p. 351-370
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351
Classical limit of
aquantum particle in
anexternal Yang-Mills field
Ugo MOSCHELLA
International School for Advanced Studies, Strada costiera 11, 34014 Trieste, Italy
Vol. 51, n° 4, 1989, Physique theorique
ABSTRACT. - It is studied the classical limit of a quantum
particle
inan external non-abelian gauge field. It is shown that the
unitary
groupdescribing
the quantum fluctuations around any classicphase
orbit has aclassical limit when h tends to zero under very
general
conditions on thepotentials.
It is alsoproved
theself-adjointness
of the Hamilton’s operator of the quantumtheory
for alarge
class ofpotentials.
Someapplications
of the
theory
arefinally exposed.
RESUME. 2014 On etudie la limite
classique
d’uneparticule quantique
dansun
champ
exterieur non abelien. On demontre que 1’existence de la limiteclassique
du groupe unitairequi
decrit les fluctuationsquantiques
autourd’une orbite
classique quelconque
est assuree par des conditions peu restrictives sur lespotentiels.
On demontre aussi queFoperateur
hamilton-ien de la theorie
quantique
estauto-adjoint
pour unelarge
classe depotentiels.
Onpresente
enfinquelques applications
de cette theorie.. I. INTRODUCTION AND STATEMENT OF THE PROBLEM
Wong’s equations
are known to be the classical evolutionequations
ofa
particle moving
in an externalYang-Mills
field([1], [2]); they
were/’Institut Henri Poincaré - Physique theorique - 0246-0211
obtained as the formal limit for h
tending
to zero of thecorresponding
quantumequations
ofmotion,
where h is the Planck’s constant.The aim of this paper is to
give
arigorous proof
of thiscorrespondence
under very
general hypotheses.
In this introduction the formulations of both the classical and quantum theories are stated and the ideas
underlying
the classical limitprocedure
are
explained.
Let (5 be a
semisimple
andcompact
Lie group and 9 the associated Liealgebra,
with commutation ruleswhere {e03B1}
is a basis for g(summation
overrepeated
indices is assumedhereafter unless otherwise
specified).
In several
previous
papers on this and relatedsubjects ([3], [4]
andreferences
therein)
the main idea to obtain the classical limit of the quantumtheory
consists inletting
the dimension m of therepresentation
of the group tend to
infinity
in such a way that m h = const, when h tends to zero.More
precisely
one chooses an irreduciblerepresentation
1t,parametrized by
itshighest weight
l and then to each natural number associates the irreduciblerepresentation
whose maximalweight
is nl. The classical limit may be obtained in this wayby letting h
tend to zero asn -1.
The classical
Wong equations
then include as adynamical
variable aclassical
isospin,
which is apoint
ofr,
thecoadjoint
orbitthrough
l. Thisapproach
has however thedisadvantage
that it is necessary tochange
ateach step of the limit
procedure
the Hilbert space of the quantumtheory.
A different strategy is used here: the
representation
of g is chosen infinite dimensional from thebeginning;
it is constructed in the most convenient way for toperform
the classical limit in thespirit
ofHepp [6],
i. e.
by making
use of the bosonic creation and annihilation operators a + and a.Consider to this end the
Jordan-Schwinger
transformation[5]:
let X bean m x m matrix and let
~m
be the Hilbert spacecorresponding
to mcinematically independent bosons;
a bosonicoperator L (X) representing
X on
~m
is definedby
Let now
{T}
be a faithfulrepresentation
of thealgebra
9 on a m-dimensional vector spaceV m’
{ L (T) }
constitutes arepresentation
of g on~
becauseAnnales de /’Institut Henri Poincare - Physique - theorique -
It is obvious that
{L(T)}
is a reduciblerepresentation
of 9 and that itcontains a lot of the finite dimensional irreducible
representations
of g.To see this it suffices to note that
~
may be rewritten as the direct sumof the
eigenspaces
of a quantum m-dimensional oscillator[see (4.3)]; by
construction
{ L(T) }
leaves each of these spaces invariant and therefore the restriction of{L(T)}
to any of them defines a finite dimensionalrepresentation
which is either irreducible orcompletely
reducible. To sayprecisely
which irreduciblerepresentations
of g are contained in{L(T)}
further information about
{ T}
is needed. Forexample
consider the follow-ing
realization of a basis of(complex)
su(2):
the
previous
constructionyields
an infinite dimensionalrepresentation
which contains each finite dimensional irreducible
representation exactly
once
[5].
Now it is
possible
to write the quantum Hamiltonian of aparticle moving
in an externalYang-Mills field;
to this end consider thefollowing potentials:
The minimal
coupling prescription
leads to thefollowing
Hamilton opera- tor(the
mass of theparticle
is takenequal
toone):
where
means the
representation
of thepotentials
A on the space$~.
The operators q and p are the usual
position
and momentum operators.The
potentials Aj
account for the"magnetic"
part of theYang-Mills
interaction while
A o
isresponsible
for the "electric" part. V describes an interaction that does not involve the internaldegrees
of freedom of theparticle.
H operates on a Hilbert space of the
form ,~S
0~. ~s corresponds
tothe
spatial degrees
of freedom of theparticle
while~m
to the internalones.
Clearly q
and poperate on s
while aand a+
operate onm.
The lasttwo operators should not be confused with
The
only
non zero commutators areLet z
represent
any of theoperators q,
p, a, a + . In order toperform
theclassical limit one needs a
representation
of the canonical commutation rulessymmetric
with respect toh;
to this end define[6]
The
following
hamiltonian is obtained from( 1. 5) by
aunitary scale
transformation :
Let now
çj,
1t j,~k
and9~
be the classical variablescorresponding
to the operators akh, and where the star meanscomplex conjugation;
the
symbol ç
will beadopted
to denote any of these classical variables.Bohr’s
correspondence principle implies
that has the same form ofthe classical Hamiltonian H
(Q
and so it follows that:(here
thecorrespondence principle
has been so to sayinverted).
The
only
nonzero Poisson’s brackets are:The hamilton’s
equations easily
follow:Equations analogous
to these may be found in[7].
The definition of the classical
isospin
variable isgiven by
The
equation
of motion that onegets
for theisospin
variable areexactly
those
given by Wong:
It has been
displayed
a richer structureunderlying
theYang-Mills theory (the
variables9);
this structure will beexplicitly
used toperform
theclassical limit in a way that avoids the use of the
group-theoretical properties
that are so crucial in theprevious
treatments[3]. Clearly
moreAnnales de l’Institut Henri Poincaré - Physique theorique
degrees
of freedom have been used than those that are necessary to describe the classicalisospin;
however it ispossible
to recover in asimple
way the minimal
phase
spaces where r is a certaincoadjoint
orbit of the group G: indeed one may construct a map l:
(g*
is the dual of thealgebra g)
whose definition is thefollowing:
{
is the dual of thepreviously
chosen basis of g. It is easy to check that the Poisson brackets definedby ( 1. 14)
arenothing
but thepull-back
_
through
7 of the well-known Lie-Poisson brackets ong* [8]. _
Theexplicit expression
of the Hamiltonian thenimplies
that it ispossible
to limitoneself to consider as
dynamical variables 03BE, 03C0
and(9).
The construction of Kirillov[9] finally gives
R 2 n xr~ as
thephase
space in which one candescribe the classical system. In
particular
one derivesdirectly equations ( 1.19)
withouthaving
to passthrough ( 1.17),
which however remains hidden in this way; this does not seem to be anadvantage
because theuse of the redundant
degrees
of freedom describedby
the 9 variablesgreatly simplifies
the classical limitprocedure
and may be useful in otherproblems
related to this.It is time to
explain briefly
what is themeaning
of the words "classical limit"( [3], [4], [6], [ 10], [ 11 ], [ 12]) .
It iscommonly
said that classical mechanics is the limit of quantum mechanics when h tends to zero but aconcrete mathematical definition of the limit
procedure
is needed. Themost
significant
one is thefollowing:
letAh
ah-dependent
quantum operatorrepresenting
a certain observable whose classicalexpression
isthe
phase
space function~(Q.
What one has to do is to select certain quantum states( h, ~ ~ depending
on h such thatwhere the
following
definitions have beenadopted:
The
symbol 1 >
denotes as usual the Hilbert space scalarproduct.
The
only approrpiate
quantum states fordoing
this are known as"coherent
states",
and are the states that minimize theuncertainity
rela-tions
( [ 13], [ 14]) .
Weyl’s
operators are crucial in the construction of the coherent states;their definition is the
following:
with 03C0q=03C0jqj
etc. It is well known thatThe coherent states that will be used in the
following
aregiven by
with 0/
any normalized quantum state. aLet s
-+ ss
be a solution of the canonicalequations
withgiven
initialconditions. The quantum time evolution operator is
given by
and the
Heisenberg
operators areThe mean value of the operator z~h
(t, s)
on the stateI h, ~S ~
is thenexpected
to converge to the solution of the canonical
equations
with thegiven
initial conditions. Indeed one has that:
where
The operator is the main mathematical
object
of this paper. It describes the evolution of thequantum
fluctuations around the classicalphase
orbit. It will be shown that:where
The solution of the operator
equations ( 1. 33), ( 1. 34)
can be writtenDefine
The operator
Rh (r)
is a remainder of orderh1~2.
Annales de l’Institut Henri Poincare - Physique " théorique "
If the
potentials
are smoothenough
it willhappen
thatRh
--+> 0 when h --+> 0. Indeed if one definesthen it follows that
and from
( 1. 28)
and( 1. 29)
one obtainsThe reader is referred to
[6]
and[10]
for further material about the classical limit. The main results of this paper areconcerning
theself adj ointness
ofthe operator
( 1.11)
and theproperties
of theunitary
group of operators( 1. 32) .
Inparticular
the limit( 1. 40)
will berigorously proved
while theproofs
of( 1. 41)
and( 1. 42)
will not bereproduced
here.2. NOTATIONS AND GENERAL RESULTS
Let ~
be a Hilbert space with innerproduct ~ I ~
andnorm II
Let A be a linear operator
in ~
and denote its domain withD (A).
If A is closable A denotes its closure. If A is
densely
defined A + denotesthe
adjoint
of A.The set of bounded operators
from ~
to another Hilbert space§’
isdenoted
by
thesymbol
B($, §’)
and thecorresponding
operator norm is denotedby II
Let A be a
self-adjoint
andpositive
operator; it ispossible
to associatea scale of Hilbert spaces to A
( [ 15], [ 16], [ 17]) :
let t be a real
number;
one defines with thehelp
of thespectral
theoremthe operator
The Hilbert space
is defined
by setting
If 03C41
~ 03C42
thenc densely.
Consider now the Hilbert space and define
formally
the operatorsJ
These operators
are self-adj oint
on the domainsThe operators
b~
andb~
defined in( 1. 7)
are closed operators defined onthe domain n
Fix the
index j
and defineThis operator is
self-adjoint
andpositive
on the domainFinally
defineThese operators are
self-adjoint
andpositive
on the domainsThe scales of Hilbert spaces associated *
with 1
and * N are - denoted *Some remarkable
properties
of these scales are listed here:with z any of
the q,
p,b,
b + .In the introduction all the
interesting quantities
were written in a mixed formby making
use of the operatorsposition
and momentum to describe thespatial degrees
of freedom of theparticle
and of the operators creationAnnales de /’Institut Henri Poincaré - Physique theorique
and annihilation to
describe
the internal ones. Define now the(n + m)-
vector operators q
and p by
with
analogous
definitions for their classical counterparts.Everything
can now berephrased making
use of thesegeneralized position
and momentumoperators q
andp; analogously
one could usegeneralized
creation and annihilation operatorsb
and’6+.
The scales of spaces that will be used in thefollowing
are thoseassociated with ||, Iii (
and
X;
theseoperators
are those of(2.11) (2 . 12) (2 . 13) with p = n + m.
Some well known facts about the
Weyl
operators are nowlisted;
note that( 1. 23)
isequivalent
to thefollowing expressions:
THEOREM 2. 1:
C
(~, ~c)
isL2-strongly
continuous in the 2 n + 2 m argumentsjointly (2 . 25)
C
(~, ~) belongs
to eachof
the sets B(XT, XT),
BQT),
BPt);
besides it is
jointly strongly
continuouson the spaces
QT, Pt, Xt for
each real i.(2. 26) If 03C8
E X 1/2, and thefunction
t ~St
isdifferentiable (in
some real intervalI)
then.
3. THE CLASSICAL LIMIT OF THE UNITARY GROUP
Wh(t. s.)
Consider the canonical
equations ( 1. 15), ( 1. 16), ( 1. 17).
There exists alocal solution of these
equations
if thepotentials
fulfil the usualLipschitz
conditions. This solution is defined on a real interval I and is denoted
by çt (in
thefollowing
thedependence
of the solution of the canonicalequations
on the initial conditions is leftimplicit).
HYPOTHESES 3. 1
(on
thepotentials).
For each t~I it is
given
apositive
number pt; it isrequired
that(b)
Thepotentials ( . , t)
and V( . , t)
are differentiable twice in the set
Ut
= S(çt, pj, (3 . 2)
with
(c)
The functionsV,
are continuous on the set
Uj ( 3 . 3)
with
I =
closureof {
UUt{t}}.
tEl
It is easy to
verify
that thehypotheses
3.1 areequivalent
to thehypotheses
3. 1’ in theimportant
case in which thepotentials
do notdepend explicitely
on time:HYPOTHESES 3. 1’.
(a)
For each t~I it isgiven
apositive number rt
such that the
potentials
andV ( . ) belong
to
~2 (S (~t, rt)),
the class of twicecontinuously
differentiable functions of the set S(çt, rt) ( 3 . 4)
The reason for these
hypotheses
is that in order to prove the limit( 1. 38)
it will be necessary to make a
Taylor’s expansion
of thepotentials
up to the second order in aneighborhood
of the classicalç-orbit.
Define nowT)(a)
is the operator of the dilations and is continuous.The
following hypotheses
will ensure the existence of thequantum theory:
HYPOTHESES 3. 2
(on
theoperators).
It is
given
afamily
ofself-adjoint
operatorsdepending
on theparameter h
denotedwith {Hh (zh,
>0}. (3 . 7)
It is
required
that:Annales de l’Institut Henri Poincare - Physique theorique
(b)
For each one has that(c)
There exists aL2-strongly
continuous group ofL2-unitary
operators denoted withUh (t, s)
such thatLet
Wh (t, s)
defined as in( 1. 32)
with t and sbelonging
to I andUh (t, s)
defined in
(3 .10)
with /!>0. It holds thefollowing
THEOREM 3 . 3. -
Wh (t, s) is a L 2-strongly
continuous groupofL 2-unitary
operators.
Proof. -
This iseasily
obtained from theorem2.1,
thecontinuity
of(t, s)
and thehypothesis (3 .10).
##Consider now the operator
Kh (s)
of( 1. 36).
Define its domain as follows:On
D (Kh (s))
one has:The
following
definitions have beenadopted:
LEMMA 3.4. - with
s E I,
thenProof. -
From theorem 2. 1 it follows thatThe
identity
implies
thatFrom this one
easily
gets the resultby exploiting
thehypotheses
3. 2 and(2.27).
##Consider now the operator
H2 (s)
introduced in( 1. 38).
Itsexplicit expression
is thefollowing:
with
This is not an unworkable
object;
indeed it issimply
aquadratic operator
in q, p, a and a+.
Apart
from details the situation isexactly
the same asin
[12];
so it holds thefollowing
THEOREM 3 . 5:
(a)
For each real i,t E I, H2 (t)
E B 1,Xt) (3 . 22)
(b) H2 (t)
isessentialy self-adjoint
onXt,
V i E[1, 00] (3 . 23)
Annales de I’Institut Henri Poincare - Physique theorique
(c)
It exists aL2-strongly
continuous groupof L2-unitary
operators calledU2 (t, s)
with t, s EI,
such that(d)
For each compact K cI,
it exists aconstant 03B103C4,
K such that(e) U2 (t, s) is jointly strongly
continuous inX ~
with respect to t
and s,
V t E R.(3 . 26) (1) belong to
’Xi;
thenProof. -
S ee[ 10],
theorems4 . 2,
4 . 3. # # 1The
following
£ is the fundamental theorem of this section:THEOREM 3. 6. - Let K c I
be a compact; if the
,hypotheses
3. 1 and ,3. 2
are verified
then itfollows
thatuniformly for t
and ’ sbelonging to
K.Proof. - (3 .1) implies
thatpK>0.
Choose p such that define ’Let x
a cut-off function whose definition andproperties
are listed afterthe end of the
proof. If 03C8 ~ D1 one
has:The estimation of the first addendum
gives:
because of the
unitariety
ofs),
the property(2.14)
and the definitionof the cut-off x.
The second addendum is
majorized
thanks to(3. 25):
Now the estimation of the third term in
(3. 30)
has to befaced;
observethat
It is
possible
to use the lemma 3. 4:From
( 3 . 12)
and( 3 . 20)
one gets:The
following
definitions have beenadopted:
Annales de l’lnstitut Henri Poincare - Physique ’ theorique ’
The strong
continuity
of the group and theexpression (3 . 35)
allow one to write
and so it follows that:
Now the
expression (3.35)
must be used to estimate the norm in theintegral.
The prototypes of the terms contained in this estimate are thefollowing:
from the first term one gets themajorization:
from the second term one obtains:
The estimate of the last term
gives
where the
hypotheses
3. 2 have beenused;
from the compactness ofÛK
itfollows that it exists a function
f(p)
such that/(p) -~
0 when p ~ 0 + and for which one has:The
procedure
for the estimate of the other terms is the same as in theprevious three;
note that it is necessary to use~03C8~2 to
control the terms of theexpression (3. 35)
that arequartic
in the operators z’s. From theseestimates,
thedensity
of the setD 1
in L2 and theunitarity
ofU2 (t, s)
andWh (t, s),
the result may befinally
obtained.Appendix
Properties
of cut-off functionsThe
function x
usedduring
theprevious proof
has thefollowing
defini-tion :
Let
x ERn;
defineIt follows that
4. SELF-ADJOINTNESS OF THE HAMILTONIAN OPERATOR Consider the formal Hamiltonian
defined on some dense set of
[There
is no difference inusing
this space instead ofL2 ( Rn + m)
because ofthe natural
isomorphism connecting
these twospaces.]
There are some well known facts that allow a great
simplification
inthe
study
of theproblem
of theself-adjointness
of theoperator (4.1)
onthe space
(4. 2).
Indeed one has that:where
Kp
is theeigenspace
of a quantum m-dimensional oscillator relative to theeigenvalue
p.Annales de l’Institut Henri Physique theorique
as follows from the
antihermiticity
of the matrices T.These observations allow one to
decompose
thepresent problem
in twosuccessive steps: the first one is the
study
of theself-adjointness
of(4.1)
on the space
L 2 (R n, Kp).
This is
essentialy
the same as in the case of theSchrodinger
operator withelectromagnetic potential.
Call
H 1
the restriction ofHi
to some subset ofL~ ( Rn, Kp).
THEOREM 4.1. -
If
withthen
Hp1 is essentialy self-adjoint on
Proof. -
Theproof
of this theorem follows the sameprocedures
of[18].
The modifications that are necessary are based on the observations(4. 3), (4.4), (4. 5)
and(4. 6).
~#Consider now the operator
where Vi O.
THEOREM 4 . 2. -
S uppose
thatwith b 1
J.l
=1,
... , dim g, c 1arbitrarily
small.If
thehypotheses of
theorem 4. 1 are true then Hp isessentialy self-adjoint
on
~~ (Rn, Kp).
Proof. -
Theproof
is obtained from lemma 6 of[14]
and from the Kato-Rellich theorem[ 16].
~~In the second step the
complete
Hamilton’s operator isreconstructed;
consider indeed the
following
operator:defined on the space
The action of
(4. 9)
on(4.10)
isgiven by
In this second * and * conclusive ’ remark it is shown how to
applicate
’ theresults that have ’ been obtained.
LEMMA 5 . 1. - Let
f :
R n -+ C a ’measurable and bounded function
whichis continuous in
S (ç, p), pER, ç ERn.
ThenProof -
Write theidentity
Then one
easily
gets theproof by noting
that q~h ~ 0 for h ~ 0strongly
in the resolvent sense and that
THEOREM 5 . 2. - Let
f :
Rn -~ C a , measurable bounded ’function, which
iscontinuous in a ’
neighborhood of (~t)t
e I;if
thehypotheses
3 . 1 and ’ 3 . 2 are ’true then it
follows
thatWith t, s
E I, normalized to ’ 1.Proof. -
Observe " that( 5 . 6)
isequal
toand therefore
equal
to_
Having
in mind( 5 . 5)
and the theorem 3 . 6 one can conclude thatACKNOWLEDGEMENTS
I would like to thank Professor
Giorgio
Velo whosuggested
this pro- blem to me andprovided
hispretious help during
thewriting
of thispaper. It is a
pleasure
to thank also Professor Franco Strocchi for his interest in this work and Dr. GuidoMagnano
for ahelpful
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( Manuscript received January 30th, 1989.) (Accepted May 3rd, 1989.)
l’Institut Henri Poincaré - Physique thcorique