A NNALES DE L ’I. H. P., SECTION A
M ARIA R OSA M ENZIO
W. M. T ULCZYJEW
Infinitesimal symplectic relations and generalized hamiltonian dynamics
Annales de l’I. H. P., section A, tome 28, n
o4 (1978), p. 349-367
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349
Infinitesimal symplectic relations
and generalized Hamiltonian dynamics
Maria Rosa MENZIO
W. M. TULCZYJEW
Universita di Torino, Istituto di Fisica Matematica, Via Carlo Alberto, 10, 10123 Torino, Italy
Department of Mathematics and Statistics, University of Calgary, Calgary, Alberta, Canada Ann. Henri Poincare,
Vol. XXVIII, n° 4, 1978,
Section A :
Physique ’ theorique. ’
SUMMARY. - Generalized Hamiltonian
dynamics
formulatedorigi- nally by
Dirac is reformulated in terms ofsymplectic
geometry. A classi- fication of constraints isgiven. Importance
of first class constraints is stressed.Examples
fromparticle dynamics illustrating
various aspects of thegeneralization
aregiven.
RESUME. 2014 On formule en termes de
geometric symplectique
lagenera-
lization de la
dynamique
hamiltonienne donnee par Dirac.Apres
la clas-sification des contraintes on
souligne 1’importance
des contraintes depremiere
classe. Plusieurs aspects de cettegeneralisation
sont donnes par desexemples
tires de ladynamique
d’uneparticule.
1. INTRODUCTION
In an attempt to
provide
a canonical framework for relativisticdynamics,
Dirac
[3]
formulated ageneralization
of Hamiltoniandynamics
associatedwith submanifolds of the
phase
space of aphysical
system. A classification of the Poissonalgebra
wasgiven.
Dirac’stheory
was formulated in thelanguage
Annales de l’lnstitut Henri Poincaré - Section A - Vol. XXVIII, n° 4 - 1978. 23
350 M. R. MENZIO AND W. M. TULCZYJEW
of local coordinates. A coordinate
independent
discussion ofdynamics
associated with submanifolds of a
symplectic
manifold wasgiven by
Lichnerowicz
[5].
Lichnerowicz also included the case of non-zero Hamil- tonians.We
give
asystematic
discussion of thegeneralized
Hamiltoniandyna-
mics in terms of
symplectic
concepts such aslagrangian
submanifolds andsymplectic
relations. Classification of constraints isgiven. Importance
of first class constraints and
integrability
is stressed.Lagrangian descrip-
tion of
dynamics
is not included.Examples including
both zero and non-zero Hamiltonians are
given.
The program of
symplectic interpretation
ofdynamics
with constraintswas initiated in a seminar conducted at the Warsaw Institute for Theore- tical
Physics by
one of us(W.
M.T.)
in 1967-1968. Results remained unpu- blished except for a paperby Sniatycki [7]
who as aparticipant
in the semi-nar had access to the material.
2. SYMPLECTIC MANIFOLDS
AND LAGRANGIAN SUBMANIFOLDS
DEFINITION 2.1. Let P be a
manifold,
and co a 2-form on P. Thepair (P,
is called asymplectic manifold
if :i)
co isnon-degenerate ; ii)
co is closed : d03C9 = 0.A more
explicit
statement of conditioni)
is thatfor each vector field
Y,
it follows that X = 0. Conditioni) implies
that thedimension of P is even : dim P = 2m.
If local coordinates are introduced in P and the local
expression
of co is co A
(~
then these two conditions can beexpressed
as: 2
pCoordinates
pj)
of P such that 03C9 = dqi Adpi
are called canonical coordinates. Local existence of canonical coordinates isguaranteed by
Darboux’s theorem.
DEFINITION 2.2. Let
(P,
be asymplectic
manifold. A submanifold N c P is called alagrangian submanifold
of(P, (D)
ife) We follow the tensor calculus conventions of reference [6]. In particular, the summa-
tion convention is used.
Annales de l’Institut Henri Section A
SYMPLECTIC RELATIONS AND GENERALIZED HAMILTONIAN DYNAMICS 351
A submanifold N c P is said to be
isotropic
if conditioni)
is satisfied.We show that the dimension of an
isotropic
sub manifold can be at mostequal
to m. At anypoint p E P,
wp is anon-degenerate skew-symmetric
form on
TpP.
The vector spaceTpP together
with the formgive
an exam-ple
of what is called asymplectic
vector space. For anysubspace
V ofTpP
we define the
symplectic polar
The dimension of the
symplectic polar
isobviously equal
to thecodimen-
sion of V in
TpP.
Inparticular,
if p is an element of anisotropic
submani-fold N c
P,
then thecondition 03C9 |
N = 0implies (TpN)§ ~ TpN.
Let n bethe dimension of N. Since the dimension of is
2m - n,
we have 2m - n >- n, n. Hence the dimension of N is at most m. It follows from the discussion above that alagrangian
sub manifold is anisotropic
submanifold of maximal dimension.
Let
Q
be a manifold and letT*Q
beits cotangent
bundle. We denoteby
1tQ the bundleprojection
ofT*Q
ontoQ.
A 1-form8Q
onT*Q
is definedby :
_The
mapping TT*Q -~ TQ
is the tangentmapping
oi ~Q andTT*Q ~ T*Q
is the tangent bundleprojection.
The 1-form8Q
is called the canonical
1-form
onT*Q
and the 2-form (DQ =d03B8Q
is calledthe canonical
2 form.
Let
(qi)
be local coordinates ofQ.
At eachpoint q
EQ,
the differentialsdqi
of the coordinates form a basis of the cotangent spaceT q *Q.
The com-ponents p~ of a covector
pET q *Q together
with thecoordinates qi of q
form coordinates
(qi, p~)
of the covector p. In this way we obtain coordi-nates
(qi, p~)
ofT*Q canonically
associated with coordinatesqi.
It iseasily
seen that the local
expression
of the canonical 1-form8Q
is9Q
=and the local
expression
of the canonical 2-form 03C9Q is (DQ =dpi
Adqi.
It follows that
(T*Q,
is asymplectic
manifold and the coordinatesp~)
are canonical coordinates. -If ~p is a 1-form on
Q,
then thepullback
of the canonical 1-form9Q
by Q -~ T*Q
isequal
to ~p. This property isproved by evaluating
on an
arbitrary
vectorv E TQ:
From cp, it follows that the
image
N of themapping Q ~ T*Q
is alagrangian
submanifold of(T*Q,
if andonly
if ~p is a closed 1-form. If ~p is exact, and cp =dF,
then F is called ageneratin~g function
of N. Theimage
of a closed 1-form is aspecial
case of a class ofVol. XXVIII, n° 4 - 1978.
352 M. R. MENZIO AND W. M. TULCZYJEW
lagrangian
submanifoldsgenerated
0by
functions defined 0 on submanifoldsof Q.
PROPOSITION 2.1. - Let C
c Q be a submanifold
i and let F :be a ’
differentiable function.
The setis a ,
lagrangian submanifold
1of
Proof Using
canonical coordinates ofT* Q,
one caneasily
showthat N is a submanifold of
T* Q
of dimension m = dimQ.
Let z be any vector in TN cTT*Q.
Thenwhere
F
= F oN).
It follows that9Q
N = d F andconsequently
= 0. Since N is
isotropic
and dim N= 2
dimT*Q,
it follows that N islagrangian,
q. e. d. ,2
3. THE STRUCTURE OF THE TANGENT BUNDLE OF A SYMPLECTIC MANIFOLD
Let
(P,
be asymplectic
manifold. Then the tangent bundle TP isisomorphic
to thecotangent
bundle T*P. Theisomorphism
is establishedby
the vector bundlemorphism j8
Objects
in TPcorresponding
to9p
and COp are Tp = ?Cp o/3,
x =and d) =
dx
=respectively.
We note that
(TP, cb)
is asymplectic
manifold. Since TP isisomorphic
to the cotangent bundle
T*P,
it ispossible
to generateLagrangian
sub-manifolds of
(TP, c~)
from functions defined on submanifolds of P.Appli-
cations of such sub manifolds to
particle dynamics
will be studied in sub- sequent sections.4. INFINITESIMAL RELATIONS
Let
(P, OJ)
be asymplectic
manifoldrepresenting
thephase
space of amechanical system
(2).
Let us consider the set of all differentiable curvesin P. Possible histories form a subset D of the set of all curves. The set fØ
itself,
or any law which characterizes ~completely
will be referred to as(2) In the present section we make no use of the symplectic structure x).
Annales de l’Institut Henri Poincaré - Section A
SYMPLECTIC RELATIONS AND GENERALIZED HAMILTONIAN DYNAMICS 353
the
d ynamics
of the system. Itusually happens
that the set ~ is the set ofall solutions of an
ordinary
differentialequation
of first order.DEFINITION 4 .1. A submanifold D’ of TP is called
a first
orderdiffe-
rential
equation.
A differentiablemapping
y : I ~ P is called anintegral
curve of D’ if the vector
y{t)
tangent to y at tbelongs
toD’,
for each t e I.We denoted
by
I an openneighbourhood
of 0 E IR.When a differential
equation
D’ is used to describe thedynamics
of amechanical system, it is
important
that each element of D’ is tangent toan
integral
curve.DEFINITION 4.2. A differential
equation
D’ c TP is said to be inte-grable
if for each element u E D’ there is anintegral
curve y of D’ suchthat
y(o)
= u. Anintegrable
differentialequation
will be called aninfini-
tesimal relation.
Examples.
-a)
Let X : P ~ TP be a vector field : then theimage
D’ = Im
(X)
is a differentialequation.
It follows from thegeometric
version of
Cauchy’s
theorem that D’ isintegrable.
A vector field is fre-quently
called an infinitesimal transformation since it generates a(local)
one-parameter group of transformations. An
integral
curve of D’ is calledan
integral
curve of the vector field X.b)
Let D’ be a distribution on P(3) :
D’ isagain
anexample
of a differen-tial
equation. Integrability
of distributions is thesubject
of Frobeniustheory.
Thistheory
deals with theproblem
of existence of sub manifolds of P whose tangent vectorsbelong
to the distribution. Such submanifoldsare called
integral
submanifolds. A distribution is said to becompletely integrable
if for eachpoint
there is anintegral
submanifold of dimensionequal
to the dimension of the distribution.Integrability
in the sense ofDefinition 4.2
always
holds for a distribution. Acompletely integrable
distribution leads to a foliation of P
by
maximal connectedintegral
mani-folds ;
this foliation can beinterpreted
asdefining
anequivalence
relationin P.
Consequently,
anintegrable
distribution can beregarded
as an infi-nitesimal
equivalence
relation.c)
Let(P, B, ~u)
be a differential fibration[2],
and let X : B -~ TB be avector field. We define a differential
equation
Let
belong
to D’ and let y : I ~ B be anintegral
curve of X suchthat
y(o) _ Jl(P).
It iseasily
seen that any lift of y to P is anintegral
curveof
D’ ;
inparticular
a lift can be chosen to be tangent to u. It follows that D’is an infinitesimal relation.
e) A distribution on P is a subbundle of TP, also known as a field of p-directions.
354 M. R. MENZIO AND W. M. TULCZYJEW
B be the one-parameter group of transformations
generated by
X. For each t we have a submanifoldDt
c P x P definedby
This submanifold is not the
graph
of amapping
but can still be considereda relation in P. The one-parameter
family {Dt}
of relations is in a sensegenerated by
D’. Thisjustifies
the use of the term « infinitesimal relation » for D’.5. HAMILTONIAN DYNAMICS
Dynamics
of nonrelativisticparticle
systems isusually
describedby
a hamiltonian vector field on a
symplectic
manifold(P, representing
the
phase
space of the system. We show that a hamiltonian vector fieldprovides
aspecial example
of alagrangian
submanifold of(TP, cv).
DEFINITION 5 .1. A vector field X : P ~ TP is said to be
locally
hamil-tonian if the form X J ú) is closed :
d(X
JOJ)
= 0. The field X is said tobe
globally
hamiltonian if X J OJ is exact. A function H : P ~ !? is calleda Hamiltonian for the field dH
[7].
Since =
d{X
J + and cc~ isclosed,
a vector fieldX : P -~ TP is
locally
hamiltonian if andonly
if = 0. It followsthat,
if X is
locally hamiltonian,
it generates a one-parameter groupof symplectic
transformations. For this reason,
locally
hamiltonian vector fields arecalled
infinitesimal symplectic transformations.
PROPOSITION 5.1. 2014 A
vector field
X : P ~ TP islocally hamiltonian if
and
only if
theimage
D’of
X is alagrangian submanifold of (TP, d)).
Proof
2014 It is obvious that D’ isisotropic
if andonly
We show that
X*X
is closed if andonly
if X islocally
hamiltonian :Since dim D’ = dim P
== - 2 1
dimTP,
, D’ islagrangian
if andonly
if X islocally hamiltonian,
q. e. d.Relativistic
generalizations
of hamiltoniandynamics require passing
from infinitesimal transformations to infinitesimal relations.
Proposition
5.1suggests a
generalization
of the concept of alocally
hamiltonian vector field. We consider infinitesimal relations in P which arelagrangian
sub-manifolds of
(TP, co).
DEFINITION 5.2. A differential
equation
D’ c TP is called aninfini-
tesimal
symplectic
relation if it isintegrable
and is alagrangian
submani-fold of
(TP, c~).
Annales de l’Institut Henri Poincaré - Section A
355
SYMPLECTIC RELATIONS AND GENERALIZED HAMILTONIAN DYNAMICS
6. GENERALIZED HAMILTONIAN DYNAMICS
A
generalization
of Hamiltoniandynamics
wasproposed by
Dirac[3].
The characteristic feature of this
generalization
is the appearance of aconstraint sub manifold on which the Hamiltonian is defined. We
give
aconstruction of differential
equations appearing
in Dirac’sgeneralized dynamics independent
of local coordinates.PROPOSITION 6.1. - Let K c P be a
submanifold
and H :differentiable funetion. The
setlagrangian submanifold q~ (TP, cb).
- Let
be the
lagrangian
submanifold of(T*P, generated by
H in the senseof
Proposition
2.1. The inverseimage ~3-1(N)
of this submanifoldby
thediffeomorphism ~:
TP ~ T*P defined in Section 3 is alagrangian
submanifold
of (TP, 6).
It follows from the definitionofj9
that =Tp(W)
and u,
(3(w) , _ ~
u, w J= (
w A u,o ).
We see that w e D’ if andonly
ifHence, ~3 -1 (N)
= D’ and D’ is alagrangian
submanifold of(TP, d)),
q. e. d.DEFINITION 6.1. The
lagrangian
submanifold D’ introduced in Pro-position
6.1 is said to begenerated by
the functionH,
and H is called a Hamiltonian of D’. The submanifold K is called the constraintsubmanifold
and D’ is called a
generalized
Hamiltonian system.If D’ is to describe the
dynamics
of a mechanical system, it must be inte-grable,
that is it must be an infinitesimal relation.Integrability
of D’depends
on certainproperties
of the constraint submanifold K. Wegive
a classification of constraints in the next section and return to the
problem
of
integrability
in Section 8.7. CLASSIFICATION OF CONSTRAINTS
At each
point
p of a submanifold K c P we consider spacesTpK
cTpP
and
(TpK)~.
In terms of these two spaces we have thefollowing
defini-tions
[77] :
a)
K is said to beisotropic
at p ifTpK
cb)
K is said to becoisotropic
at p ifVol. XXVIII, n° 4 - 1978.
356 M. R. MENZIO AND W. M. TULCZYJEW
A
coisotropic
submanifold K c P is also called afirst
class constraintsubmanifold.
c)
K is said to belagrangian
at p if it isisotropic
andcoisotropic : TpK
=d)
K is said to besymplectic
at p ifTpK
n(TpK)~ = {
0}.
These definitions are related to the classification of submanifolds of
P,
introducedby
Dirac[3].
We derive Dirac’s classification of constraintsby
coordinateindependent
methods.Let
Np
be the intersection ofTpK
and and let t and k denote the dimension ofNp
and the codimension ofK, respectively.
DEFINITION 7.1. The
pair
of numbers(t, k - ~
is called the class of the submanifold K at p.We note that k - l is even. The 2-form (Dp restricted to is in
general degenerate. However,
the 2-form induced .on thequotient
spaceis
non-degenerate.
Since is asymplectic
vector space, and itsdimension,
it follows that k - t is even.Further,
we note thatand
consequently
l rn .Since k - l is the rank of
03C9 |
K at p, the class of K at p can also be definedas the
pair (k -
r,r),
where k is the codimension of K and r is the rank of K at p. Theinteger r
is evenbeing
the rank of a 2-form.In terms of the class of a submanifold K we have the
following
criteria :a)
K isisotropic
at p if andonly
if t = 2m - k.b)
K iscoisotropic
at p if andonly
if = k.c)
K islangrangian
at p if andonly
if t = k = m.d)
K issymplectic
at p if andonly
if t = 0.Let K be
isotropic
at p. ThenTpK
c(TpK)~
orequivalently TpK
=Np.
The dimensions of
T)(
andNp
are 2m - k andrespectively.
It followsthat 2m - k = 1.
Conversely,
if 2m - k= t,
thenTpK
=Np
sinceNp by
its definition is contained inTpK.
It follows thatTpK
c(TpK)~.
Thisproves criterion
a).
Theremaining
criteria areequally
easy to prove.We establish a relation between our classification of
constraints,
Dirac’soriginal
classification and theinterpretation given by
Lichnerowicz.Let X denote the Lie
algebra
of vector fields on P and let H be the subal-gebra
of(globally)
hamiltonian fields. We definesubalgebras
f c !!£and
We also introduce subsets and N
Annales de l’Institut Henri Poincaré - Section A
SYMPLECTIC RELATIONS AND GENERALIZED HAMILTONIAN DYNAMICS 357
PROPOSITION 7.1. - The set N is an ideal
of
Jf.Proof
LetX,
Y and Z be elements of~, Jf
and Jfrespectively.
Then
It follows that
[X, Y]
E Hence ~ is an ideal offf,
q. e. d.Dirac’s classification of constraints is based on the Poisson bracket structure, which is
equivalent
to thesymplectic
structure[4] [10].
Let~’
and g be functions on P. The Poisson bracket
of f and g
is the functionIntroducing
a bivector field G on P such that for each1-form ~
we writeThe
family ~
of functions on Ptogether
with the Poissonbracket { , }
form a Lie
algebra
called the Poissonalgebra. Following
Lichnerowicz[5]
we define subsets and s~ of f!}J:
Elements of tfl are called constraints, elements of f!Ã
are first
classfunctions
and elements of .xl are called
first
class constraints.PROPOSITION 7 . 2. - A
function f belongs to if
andonly if
PROPOSITION 7.2. - A unction
f
’if
andonly if
The
following
conclusions can be drawn from the twopropositions
above :
i )
if andonly
ii) ~‘
is asubalgebra
of the Poissonalgebra 9, iii)
j~ is an ideal of ~.Vol.
358 M. R. MENZIO AND W. M. TULCZYJEW
Throughout
the remainder of this section it is assumed that the class of K is constant. An immediate consequence of thisassumption
is thatN = is a distribution on K. We note that N is
exactly
the charac-peK
teristic distribution of K :
PROPOSITION 7.4. - The distribution N is
completely integrable.
Proof
- Let X : K ~ TK and Y : K ~ TK be vector fields such that im(X)
c N and im(Y)
c N. Then X JK)
= 0 and Y JK)
= 0.The
identity
_holds for any differential
form p
on K.Setting
p = K we obtainHence im
( [X, Y] )
c N. It follows from Frobenius’ theorem that N iscompletely integrable,
q. e. d.The foliation of K
by
maximalintegral
manifolds of N is called the cha- racteristic foliation of03C9 |
K.In a suitable
neighbourhood
of eachpoint
of K it ispossible
to find kindependent
constraints =1, ... , k
such that = 0.Simple algebraic
considerations show that functions K form amatrix of constant rank k - t. Let functions a =
1,
... ,t
belinearly independent
solutions ofequations (Ca ~
0. Then K = 0and { I K
=(Ca
0.It
follows that functions =are first class constraints. Let a =
1, ... , l ;
A =1, ... , k -
tare
independent
constraints thenfunctions {03C6A, 03C6B}|
K form a non-singular
matrix. Dirac calls functions03C6A
second class constraints.The
following proposition
relates our classification of constraints to Dirac’s classification.PROPOSITION 7.5. - The class
of a submanifold
K c P is(l, k -
and
only if
in aneighbourhood of
eachpoint of
K there is a systemof
inde-pendent
constraintsof
which t arefirst
class and k - t are second class.One part of the
proposition
isproved
above. The other part is easy to prove.8 . INTEGRABILITY
We return to the
problem
ofintegrability
ofgeneralized
Hamiltonian systems introduced in Section 6.THEOREM 8.1. - The
generalized
Hamiltonian system D’generated by
Annales de l’lnstitut Henri Poincaré - Section A
359
SYMPLECTIC RELATIONS AND GENERALIZED HAMILTONIAN DYNAMICS
a Hamiltonian H
defined
on a constraintsubmanifold
K isintegrable if
and
only if
K isa first
class constraintmanifold
and H is constant on leavesof
the characteristicfoliation of
K.Proof
2014 We assume first that D’ isintegrable.
If y : I ~ P is anintegral
curve of
D’,
then we have E D’ andzP(y(t))
=y(t)
for each t ~ I. It follows fromTp(D’)
c K thaty(t)
E K for each t ~ I. Since D’ isintegrable,
eachvector wED’ is tangent to an
integral
curve andconsequently belongs
to TK. We conclude that D’ c TK. At each
point
p EK,
we have the setA
M,~) = - M~H)}. Comparing
thisset with the
subspace (TpK)§ _ ~
WETpP ;
Vu Ewe see that
(TpK)~
=D -
wp, where wp is any fixed element ofDp.
SinceDp
cTpK,
it follows that(TpK)~
cTpK.
We conclude that K is a firstclass constraint. For a first class constraint the characteristic distribution is
(TK)~ =
Let u be an element of(TpK)~
and let w be anypEK
element of
Dp.
Thenw ~ TpK and (
u,dH> = -
w A u, Sincew ~ TpK
and u E(TpK)§,
it followsthat
w A = O.dH )
= 0and
consequently
H is constant on the characteristic foliation of K.Now we assume that K is a first class constraint. Let w be an element of
Dp,
and let S be a local section of the characteristic foliation of03C9|
Kwhich passes
through
p and is tangent to w. We show that S is asymplectic
submanifold of
P ;
this means that at eachpoint p’
E S we haveTp.S
n(Tp.S)~ = { 0}.
Since S is a section of the characteristicfoliation,
we have
Tp.S
n(TpK)~ = { 0 }
andTp.S
+(Tp.K)§
=Tp,K.
It follows thatThe Hamiltonian H restricted to S generates a Hamiltonian vector field X : S -~ TS c TP such that X J
S)
= -S),
let y : I ~ S c= P be anintegral
curve of X. Then =X(y(t))
and for each vector u Ewe
have X(y(t))
A u,OJ ) =
u, X J= - ( u, dH ~.
It follows that y is anintegral
curve of D’. If inparticular y(o)
= p, theny(o)
=X(p).
SinceX(p)
EDp
and w is theunique
element ofDp
which is tangent toS,
we con-clude that
y(o)
= w. Hence D’ isintegrable,
q. e. d.Let K be a constraint submanifold of constant class but not
necessarily purely
first class.Integrability
does not hold for thelagrangian
submani-fold D’
generated by
a Hamiltonian H constant on the leaves of charac- teristic foliationalthough
D’ n TK can be shown to beintegrable.
Theinfinitesimal relation D’ n TK is an
isotropic
submanifold but not alagran- gian
submanifold when second class constraints are present.We do not consider second class constraints
important
fordynamics.
In our
opinion
it is unreasonable to expectdynamics
with second class constraints to be the classical limit of quantumdynamics.
No naturalVol. XXVIII, 4 - 1978.
360 M. R. MENZIO AND W. M. TULCZYJEW
examples
of second class constraints inparticle
mechanics are known.Artificial
examples
can beeasily given : interpreting
thephase
space ofa system as the
configuration
space leads topurely
second class constraints.It is our
opinion
that second class constraints ariseonly
when thephase
space of a system is
incorrectly interpreted.
9. EXAMPLES
a)
Nonrelativisticdynamics
of acharged particle. Gauge dependent
formulation.
We consider the motion of a
particle
of mass m andcharge e
in an exter-nal static
electromagnetic
field. Theconfiguration
space of theparticle
is a riemannian manifold M of dimension 3. The riemannian structure of M is
represented by
metric tensorsThe
electromagnetic
field isrepresented by
thescalar potential V :
M ~IR,
the vectorpotential
A : M ~T*M,
theelectric field
E = - dV and themagnetic
induction B = dA.The
phase
space of theparticle
is the cotangent bundle P =T* M,
there are no constraints and a Hamiltonian H : is defined
by
where x = The infinitesimal
symplectic
relation D’generated by
the Hamiltonian is the
image
of the hamiltonian vector fieldWe
decompose
this field into horizontal and vertical componentsusing
the riemannian connection in T*M.
If
(xi) ;
i =1, 2,
3 is a coordinate system of M andp~); i, j
=1, 2,
3is the induced coordinate system of P such that
9M
=pidxi
then OJM =dp~
A dxi.This is true in
particular
when(xi)
is ageodesic
normal coordinate systemat any
point x
E M. It followseasily
thatwhere u and v are vectors in
TPP
at somepoint p E P,
hor(u)
and hor(v)
are vectors in
TxM,
x = obtainedby projecting
to TM the horizontal components of uand v,
ver(u)
and ver(v)
are covectors inT*xM
obtainedby identifying
vertical components of u and v with elements of T *M.Let u E
TpP
be a vertical vector. From X J 03C9M = - dH we obtainAnnales de l’Institut Henri Poincare - Section A
SYMPLECTIC RELATIONS AND GENERALIZED HAMILTONIAN DYNAMICS 361
If
v E TpP
is a horizontal vector thenwhere is the covariant derivative of A in the direction of hor
(v).
Let
(xi) ;
i =1, 2,
3 be a coordinate system of M andPj); i, j
=1, 2,
3the induced coordinate system of P. The content of
equations (9.3)
and(9.4)
is transcribed into differentialequations
and
equivalent
to the familiar second order system :We denoted
by gij
andgkl components
of tensors gand g respectively,
D
is the absolute(covariant)
derivative and t isinterpreted
as time.dt
b)
Relativisticdynamics
of acharged particle. Gauge dependent
for-mulation.
We consider the motion of a
particle
of mass m andcharge
e in an exter-nal
electromagnetic
field inspace-time.
Theconfiguration
space of theparticle
is apseudoriemannian
manifold M of dimension 4representing space-time.
Thepseudoriemannian
structure isrepresented by
metrictensors g : M ~
T* M Q T* M
andg :
M ~ TM ~ TM. The electro-magnetic
field isrepresented by
thepotential
A : M ~ T* M and thefield
F = - dA.The
phase
space is the cotangent bundle P = T*M. A first class cons-traint submanifold K c P of codimension 1 is defined
by
and the Hamiltonian is zero. The infinitesimal
symplectic
relation D’generated by
the Hamiltonian is the characteristic distribution N oft K
Phase space
trajectories
of theparticle
arethe integral
manifolds of D’.It is convenient for technical reasons to introduce the hamiltonian
vector field X = - G L
dH,
where H is the functionVol. XXVIII, n° 4 - 1978.
362 M. R. MENZIO AND W. M. TULCZYJEW
differentiable
everywhere
except when p =eA(x).
Since H is a first classconstraint the field X =
X
Kbelongs
to the ideal N.Integral
curves of Xare
parametrized phase
spacetrajectories
of theparticle.
Fromwe obtain
for each vertical vector
u ~ TpP
andfor each horizontal vector r e
TpP.
The field X satisfies
1
for each vertical vector
MeTpP,
andfor each horizontal vector
v E TpP.
From(9.14)
we see that the horizontal component ofX(p) projected
to TM is a unit vector inTxM.
It followsthat
integral
curves of X aretrajectories parametrized by
proper time.We write differential
equations
forparametrized trajectories
in termsof coordinates
(xA); x = 0, 1, 2, 3 of M
and the induced coordinatesThese first order
equations
areequivalent
to the second order system :c)
Nonrelativisticdynamics
of acharged particle. Gauge independent
formulation.
Let M be the riemannian manifold of
Example a)
and let S be aprincipal
Annales de Henri Poincaré - Section A
SYMPLECTIC RELATIONS AND GENERALIZED HAMILTONIAN DYNAMICS 363
fibre bundle [2] with base M and projection 03BE :
S ~ M. The structure groupis the
group R
of real numbers withrespect
to addition. The action of the structure group on S defines aone-parameter
group e tR ofdifferentiable transformations of S. The infinitesional generator of thisgroup
is a vectorfield Z : S -~ TS called
the fundamental vector field.
There is a connectionform
a on S and a curvatureform ~3
= da. The connection form a is a 1-form suchthat ( Z, o: )
= 1 and = 0. Each vector w E TS has aunique decomposition
w = wv + wh into the verticalcomponent wv
in the direction of Z and the horizontalcomponent wh satisfying wh, x )
= 0. The curvatureform 03B2
satisfies conditions = 0 and = 0 necessary and suffi- cient for the existence of a 2-form B on M suchthat ~3
=ç*B.
The form Brepresents the
magnetic
induction and a is the gauge invariantpotential.
The electric field is
represented by
the 1-form E = -dv,
where V : M -~ ~ is the scalarpotential.
We consider the motion of a
particle
of mass m andcharge
e. The confi-guration
space is S and thephase
space is R = T*S. The trueconfiguration
space of a classical
particle
is M. Theprincipal
fibre bundle S is usedonly
as a device for
introducing
gaugeindependent quantities.
No direct inter-pretation
of S can begiven
except in quantum mechanics and the Hamil- ton-Jacobitheory [9].
Each element has aunique decompo-
sition r
+ r~
into the verticalcomponent r"
=r - ~ Z, r )
suchthat
u, = 0 for each vertical vector u ETSS,
and the horizontal com-ponent rh = ( Z, r ) a(s)
suchthat (
= 0 for each horizontal vec- tor m ETSS.
Thenumber q == ( Z, r ) representing
the horizontalcomponent rh
of r isinterpreted
as thecharge
of theparticle.
We introduce the mapp-ing
% : R --> T*M definedby = ç 0
~sand ( T~), x(r) ~ _ ~
for each vector = The covector p =
x(r) representing
thevertical component of r is
interpreted
as the gauge invariant canonicalmomentum of the
particle.
A constraint submanifold K c R is defined
by
and a Hamiltonian H : K ~ IR is defined
by
The
physical meaning
of the constraint is clear : thecharge q
of theparticle
is
equal
to e. The Hamiltonian represents the energy of theparticle.
The action of the structure group on S generates a one-parameter group
y*,
L E IR ofsymplectic
transformations of R. It iseasily
seen that the firstclass constraint submanifold K is invariant under the group action. It follows that orbits
belonging
to K form the characteristic foliation ofOJs I K.
It also follows that the reducedsymplectic mani, f’old.
exists[77].
The action of the structure group preserves the connection form a and the
Vol. XXVIII, n° 4 - 1978.
364 M. R. MENZIO AND W. M. TULCZYJEW
decompositions
into vertical and horizontal components defined in terms of a. We have =y*(?-")
andalso ç
0 yt =ç.
It follows thatHence
x(y*(r)~
=x(r).
Themapping x
restricted to K is a submersion onto P = T* M with one-dimensional fibres. It follows that the fibres ofx ~
K are the orbits of the structure group.Consequently
the reducedphase
space isdiffeomorphic (although
notsymplectomorphic)
to P. Inorder to find the correct reduced
symplectic
structure of P we calculate(x I K)*9M.
Let u E TR be a vectortangent
to K. ThenHence
By differentiating
we obtainThe result is that the reduced
symplectic
manifold is(P, &),
wherec5 = 03C9M +
The Hamiltonian H is constant on leaves of the characteristic foliation of
Consequently
there is the reduced Hamiltoniansuch that H =
H 0 (x ~ I K). Trajectories
of theparticle
in the reducedphase
space are
integral
curves of the hamiltonian vector fieldX generated by H.
Annales de l’Institut Henri Poincare - Section A
SYMPLECTIC RELATIONS AND GENERALIZED HAMILTONIAN DYNAMICS 365
Corresponding
to(9.2)
we have the formulafor each vertical vector
MeTpP
andfor each horizontal vector
v E TpP.
In terms of coordinatesp~) ; i, j =1, 2, 3
of P we have the differential
equations
and
equivalent
toand
These
equations
contain no gaugedependent quantities.
The above
example
is anelegant
illustration of theversion
ofgeneralized dynamics
formulatedby
Lichnerowicz[5].
The Hamiltonian is not zeroand leads to a hamiltonian vector field in the reduced
phase
space.d)
Relativisticdynamics
of acharged particle. Gauge independent
for-mulation
(cf. [81 [9] ).
Let M be the
pseudoriemannian
manifold ofExample b)
and let S bea
principal
fibre bundle with baseM, projection ~ :
S 2014~ M and structure group [R. There is a connection form a and a curvature form ~p = - da.The 2-form F on M such that ~p ===
ç*F
isinterpreted
as theelectromagne-
tic field and a is the gauge
independent potential.
The manifold S is the
configuration
space of aparticle
with mass m andcharge
e. Thephase
space is R = T*S. Thedynamics
of theparticle
isgenerated by
a zero Hamiltonian defined on the first class constraint submanifoldwhere Z and x are
objects
defined as inExample c).
The constraint subma-Vol. XXVIII, n° 4 - 1978. 24