A NNALES DE L ’I. H. P., SECTION A
A. K. P RYKARPATSKY
J. A. Z AGRODZI ´ NSKI
Lagrangian and hamiltonian aspects of Josephson type media
Annales de l’I. H. P., section A, tome 70, n
o5 (1999), p. 497-524
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497
Lagrangian and Hamiltonian aspects
of Josephson type media
A.K.
PRYKARPATSKYa,b, J.A. ZAGRODZI0144SKIc,
1a Department of Nonlinear Mathematical Analysis, Institute for Applied Problems
of Mechanics and Mathematics, NAS, Lviv, Ukraine
Institute
for Basic Research, Monteroduni, ItalyC Institute of Physics, Polish Academy of Sciences, 02-668 Warsaw, Poland Manuscript received 16 April 1997
Vol. 70, n° 5, 1999, Physique théorique
ABSTRACT. -
Dynamical properties
ofJosephson
media are studiedwithin
Lagrangian
and Hamiltonian formalisms with gaugetype
con- straints. Ageometrical interpretation
of the first class gaugetype
con- straints involved issuggested basing
on the Marsden-Weinstein momen- tum map reduction. Anequivalent operatorial approach
is also considered in detailgiving
rise to certain twoessentially
different Poisson structures upon orbits of the Abelian gauge group, the first Poisson structure be-ing nondegenerate
in contrast to the secondone2014degenerated.
The con-sideration of the Poisson structure associated with
Josephson
media areessentially augmented by
means ofintroducing
newJosephson-Vlasov
kinetic
type equations
endowed with the canonical Lie-Poisson bracket.The reduction of the
corresponding
Hamiltonian flowexplains
thephys-
ical nature of the a
priori
involved constraints. @Elsevier,
Paris3.40.Kf, 04.20Fy, 74.50+r, 74.60G, 74.76-w
RESUME. - Nous etudions les
proprietes dynamiques
des milieuxJosephson grace
a des formalismeslagrangiens
et hamiltoniens avecdes contraintes de
type j auge.
Uneinterpretation geometrique
des1 Email: zagro@ifpan.edu.pl.
Annales de l’Institut Henri Poincaré - Physique theorique - 0246-0211
Vol. 70/99/05/(c)
498
contraintes de
type jauge
depremiere
classe mises enjeu
estsuggere
par une reduction de la carte des moments de Marsden-Weinstein. Une
approche operationnelle
est aussi consideree en detail : elle donne lieu a essentiellement deux structures de Poisson differentes sur les orbites du groupede jauge abelien,
lapremiere
etant nondegeneree
et la secondedegeneree.
La structure de Poisson associee aux milieuxJosephson
estrenforcee de
fagon
essentielle en introduisant de nouvellesequations
dutype Josephson-Vlasov
munies du crochetcanonique
de Lie-Poisson. La reduction du flot hamiltoniencorrespondant explique
la naturephysique
des contraintes mises en
jeu
apriori.
(0Elsevier,
Paris1. INTRODUCTION 1.1.
Physical background
The
dynamical properties
of so-calledJosephson
media wererecently
often discussed
[1-3].
Such aspecific
medium can be considered as a limit of the two-dimensional(2D), plane Josephson junction
arrays when the"density"
ofjunctions
tends toinfinity
if thephysical background
or
history
isreported
as well as there are different motives that such a medium isinteresting.
Thepossible approaches
areoriginated
eitherby
the
spin-glass
formalism on lattice orby systems
ofpartial
differentialequations
when continuousdynamic
processes are underinvestigation.
In the first case different collective
phenomena
areconsidered,
e.g.,the existence of vortex fluids
[4],
the interaction betweenvortices, [5], topological
invariance of arrays[6],
and even 3D structures[7], although
in the one direction the structure is discrete. As a
generic,
the Hamiltonianas in
XY-Ising
model is assumed.In the second case,
usually
aphenomenological approach
isadopted starting
from a discretepicture
butequations
can be derived also either from a suitableLagrangian
or Hamiltonian. The ultimate form of aLagrangian
is in thespirit
of theGinzburg-Landau
free energy functional with modifications introducedby
Lawrence and Doniach forlayered systems [8].
The discretization coincides with thespin-glass
formalismif
self-magnetic
fields areneglected.
There are,
however,
somequestions
when one wants to compare moreprecisely
the results of bothLagrangian
and Hamiltonianapproaches.
Annales de l’Institut Poincaré - Physique theorique
The source of
problems
is found in a choice of canonical variables and next in the lineardependence
of canonical momenta if the mentioned choice was doneincorrectly.
Thepoint
is thatadopting
the classical choice of variables in theLagrangian
the space derivative ofvelocity
appears that makes a
difficulty.
To avoid the arisenproblem
in[3]
there was
proposed
thesimplest
solution: a reduction of the number ofgeneralized
coordinates which isequivalent
to the consideration someinvariant
submanifold, carrying
the canonical Poisson structure.The arguments
originating
thepresent
paper we summarizebriefly
below. For details a reader is referred to
[3],
or[9]
and to papers cited there.Let us consider the canonical
Lagrangian
in the form(~i,~2.0),
since we are interested in time evolution in 2D Euclidean space,i.e.,
03A6 :R2
x ? -+ Here and later onby (.)t
weunderstand the derivative with
respect
to the variable t E Because of thecorrespondence
with thespin-glass
formalism we assume that -and of course A =
(Ai, A2, 0)
x ]R ---+]R2; (9 :]f~
x ]R ---+M; i.e.,
V :=
9/9~2.0),
if notationrelating
to 3D space ispreserved.
Since the derivative
~t
has thephysical interpretation
of the electricfield, quantities
Aand - ~ 0398 dt
as the vector and scalarpotential, respectively,
it isnatural, following
standard classicalapproaches,
tochoose as
generalizes
canonical coordinates the scalarpotential
andcomponents
of the vectorpotential.
In ourconcrete
case these coordinates would be(9, Ai, A2 .
The relevant
Euler-Lagrange equations
lead to the
following
fieldequations
Vol. n° 5-1999.
500
and
respectively,
where we areusing
forbrevity
the shorthand mnemonotation sin A :==
(sin A i, sin A2, 0).
..The first remark is that
(4)
follows from(5). Defining
momenta via thestandard way we obtain
i.e.,
once moredependent
ones,although
the Poisson brackets have the correct form.Finally
the Hamiltonian iswith the
density
defined as usual H =pAt
+p00398t - L
has the formup to full
divergence div [ (A
+ The fieldequations
calculatedeither from the Hamiltonian or from the
Lagrangian
should be the same.The field
equations corresponding
to the Hamilton functional(7)
coincide with those
following
from theLagrangian,
butsurprisingly equations
lead to the conclusion that
(9~
==0,
which seems at leaststrange.
As it was
proposed
in[3]
asimplest
remedium makes a reduction of a number of canonical coordinates. A situation becomes more clear if instead of(9,
as canonical coordinates there are taken twonontrivial
components
of 03A6 = A + Then thecomponent
O becomesonly
a gaugeparameter
and as a result podrops
out from the furtheranalysis.
The second set of HamiltonEqs. ( 10)
reduces then to theequivalence ~t
=81i/8p
=Annales de l’Institut Henri Poincaré - Physique theorique
1.2. Problem statement
From
the mathematicalpoint
of view such aprocedure
can beconsidered as a reduction of a
starting
manifold to some submanifold but with somenontrivial,
additional restrictions.Firstly
let us notice that when theJosephson
field ~ isgiven physically
as a
3D-vector,
the condition 03C63 = 0 should be considered as an outer constraintimposed
on theLagrangian ( 1 ) . Secondly,
let us observethat the
decomposition (2)
is not alike to thecorresponding
Helmholtzdecomposition commonly
used in classicalelectrodynamics
and hasquite
different
meaning.
Andthirdly,
we must take care of thesolenoidality
condition div tP = div A + Ae = 0.
Moreover,
theLagrangian ( 1 )
andnext the Hamiltonian and field
equations
are not invariant withrespect
S02 group. Weneed, however,
to derive truedynamical equations
forfields A and (9
being compatible
with all constraints involved above and to build thecorresponding
correct additional conditions. To do this programsuccessfully
one needs to recast our initialLagrangian theory
into dual Hamiltonianpicture performing
the standardLegendre
transform
up to full
divergence, i.e., according
to(8),
where canonicalphase
variables p and 03A6
pertain
to thecotangent
space}R2
x{0}))
over the
configuration
space x{0}) 3 ~,
andgenerate
the .following symplectic
structureSince this
symplectic
structure is invariant under the gauge transform(2)
but the Hamiltonian
(8)
is not, we fail to, derive in thecommonly
usedstraightforwardly
manner all necessary reducedboundary
conditions onthe
Josephson
fields A and 0. To cope with all theseproblems generated by
thespecial
form ofLagrangian ( 1 )
in2D-space,
we intend below to discuss ageneral Lagrangian picture
with thedegeneracy
of thecorresponding Legendre
transform via Dirac reductionprocedure
whenn° 5-1999.
ZAGRODZINSKI
such reduction is not introduced a
priori.
This leads further totreating
thefirst class gauge
type
constraintsby
means of ageometric
momentummap
reduction,
see, e.g.,[16-20].
Theprice paid
in this case is anexistence of some
multipliers
as a consequence of considered constrains.In order to transform such a
problem
with adegenerate Lagrangian,
buton some invariant
submanifold,
the secondpart
of the work is devoted toanalysis
of the relatedsymplectic
structures in such cases. In the thirdpart
some
equivalent operator approach aspects
of theproblem
are discussed.The last
part
contains someimportant
corollaries as wellprospective
sketches of methods used in the case of self-consistent
Josephson
mediain
spirit
of Vlasovapproach.
Many interesting aspects
of similarphysical problems
with a gaugetype
structure were in thepast analyzed
in detail in numerous papers[ 10,11 ] .
Authors made use of theLie-algebraic theory
of Poisson bracketson duals of some
naturally
built Liealgebras. By
this way authors were able to construct gauge invariant Poisson structures forsuperfluids, spin- glasses,
chromo andmagnetohydrodynamics.
For thesephysical
modelsthere are
corresponding
gauge invariant Hamiltoniansgiving
rise torelated evolution
equations
with conditions derived from the momentum map reduction.Concerning
theproblem
treated in thepresent article,
we deal withJosephson type
media which are not describedby
a gauge invariant Hamiltonian. That a natural canonicalsymplectic
structure could notbe found via the standard
Lie-algebraic theory
of Poisson structures on duals of some Liealgebras,
eventhough
it is also gauge invariantone.
Moreover,
some additional obstacle isimposed by
aspecial
2Ddegeneration
ofJosephson
medium underregard.
2. BASIC SETTING2014LAGRANGIAN ANALYSIS
Let us be
given
thefollowing simple
form of theLagrangian ,C
on somefunctional manifold M
smoothly parametrized by
an evolutionparameter
where u E M C
m, k
EZ+,
R some ’smooth map 0 on
the j et
manifold 0M).
Annales de l’Institut Henri Poincare - Physique ’ theorique ’
The Eulerian
equation
has the formwhere
by
definitionWe see from
( 13)
that theLagrangian
can hold derivatives in timet e ? of orders
greater
orequal
to one,leading
then to thenondegenerate Lagrangian problem
iffor all u E
M; Z+ ~ n
12014the maximaldegree
of thederivative contained in the canonical
Lagrangian L[u, Mj.
If that isthe case, we can construct
[ 12-15] simply
a Hamiltoniantheory
on someextended manifold
M,~
CM)
as followswhere, by definition, j
=0, ... ,
n -1,
504
and so on, the Hamiltonian
being
built aswhere
and (-,’)
denotes the standard scalarproduct
inWe see, thus that the
system ( 15)
has the standard Hamiltonian form upon the extended manifold When theLagrangian
is
degenerate,
the aboveprocedure fails,
that is one insists to use thestandard Dirac
theory
of reduction[ 12-16]
for theLagrangian ,C
withconstraints of the first and second class
generated by
theprocedure
of
constructing
theconjugated "impulse"
variables in the Hamiltoniantheory.
To do this we need to introduce the so-calledLagrangian expansion following
from( 17):
serving
as constraints on theLagrangian ( 12).
By definition,
theimpulse
variables ==0,..., ~ 2014 1, enjoy
thecanonical Poisson brackets:
for all =
0, ... , n - 1, where 8 (.)
is the standard Dirac delta-function distribution and~~,k
the Kroneckersymbol.
Now the total Hamiltonian isgiven by
where ~, ~
E =0, ... ,
n -1,
areLagrangian
vector multi-pliers,
to be found further in anexplicit
form. The Poisson brackets of the constraints(20)
withNc
must vanish and thisrequirement
will determinevector
multipliers ~,~ , j
=0, ... ,
n -1, provided
there exist no furtherindependent
constraints in theproblem
under consideration. We have forde l’Institut Henri Poinearé - Physique theorique
If
det ~ { c, c} 0,
from(23 )
one can find vectormultipliers
~,~, j ==0,
..., ~ - 1:Thus,
the total Hamiltonian definedby (22)
takes the form:When the case det = 0 takes
place,
we need to introducesome new
secondary
nm - r constraintsfollowing
from(23),
wherer : :=
rank ~ { c,
and toproceed
furtherby
the same way as it was done before.Josephson medium Example
1To be more
precise,
let us consider thefollowing
canonicalLagrangian
from
[3]:
where (’,’)
the usual scalarproduct
in We make thefollowing change
of variables
From
(26)
and(27)
we obtain:n° 5-1999.
506 A.K. PRYKARPATSKY AND J.A. ZAGRODZINSKI
that is a new
Lagrangian
,C with newindependent
variables O and(Ai,A2,0).
Now we are in a
position
to use the basictheory presented
above. At the verybeginning
we need to introduce theconjugated impulse
variables:where 6. :==
~22014the
standardLaplacian.
The
system (29) gives
rise us to thefollowing relationships:
As it was mentioned before and once more it is seen from
(30)
that theimpulse
yr and the vectorimpulse
p are notindependent
what is needed for thequantities (9~
andAt
to be defined from(29)
in aunique
way. Thuswe must introduce a one additional restriction as follows:
which can be read as a new constraint on the
Lagrangian
on M.The nontrivial canonical Poisson brackets are
given
aswhere
~,~=1,2.
Theaugmented
Hamiltonian takes the formwhere
At
= p -~0398t
and03BB(x)
is someLagrangian multiplier.
As a resultfrom
(33)
we obtainAnnales de l’Institut Henri Physique theorique
3. SYMPLECTIC ANALYSIS
We can convince ourselves
quite simply
that the constraint(31 )
is ofthe first class and has gauge nature.
Indeed,
let us recast the canonical Hamiltoniansystem (34)
into the usualsymplectic picture.
First we definea functional
phase
manifoldM~
C xwith coordinates
(A,
p;(9, yr)
EMn . Upon
the manifoldM~.
there existsthe canonical
symplectic
structurewhere n
dAj,
withrespect
to which the Eulerequation A]
= 0 isequivalent
to thecorresponding
Hamiltoniansystem stemming
from(34):
where ~, E is some gauge function. We can see that the condition
At
= holds for all t ER,
as well.Notice that the Hamiltonian
(34)
is invariant withrespect
to thefollowing
gauge group action g~. :My~
--+M,~
of an Abelian Lie group
G, consisting
of real valued invertible functionson
R2with
an addition groupoperation:
where
xk = x 11 x22 , ~ ~n~ (x) :
:=by
definitions.The above means that the gauge group G coincides with the standard Schwartz functional space on
R2
and the invarianceproperty Nc
o g03C8 =Nc
takesplace
on the manifoldMn
for allexp()
E G. Since the Liealgebra ~
of the Lie group G coincides as a manifold with the spaceG,
we willinterpret
further the gaugeelement 1/1
E InG in(36)
as thatPRYKARPATSKY AND J.A. ZAGRODZINSKI
belonging
to the Lie group G. Notice here that the gauge action(36)
is asymplectic
one on thesymplectic
manifold(Mn, c~~2~) :
for all E G.
Indeed,
because of both the
equality d ~ ~ dx =
0 and thecompatible
constraintcondition
div p
+ jr = c on the manifoldMn. Compatibility
here meansthat the condition
holds for all times t E that is
which is
simply proved
to be true. Now we are in aposition
to use thestandard Marsden-Weinstein reduction
procedure [ 17]
withrespect
to thegroup action
(36).
Let us define a momentum map J :
Mn
2014~~*
related with the action(36). By
definition we have: forany 03C8 ~G
whence we obtain the momentum map
The result above is almost obvious since the constraint c =
co (x)
is theeven one
being
involved on thephase
manifoldMn
for the Hamiltonian flow of(34)
to becompatible.
From(42)
we see that the submanifoldAnnales de l’Institut Henri Poinearé - Physique theorique
y-i(c
==eO(X))
CM,~
can be reduced[ 12,16]
on some submanifoldMo
CM,~
withrespect
to the group action(36)
The reduced
symplectic
structurec~o2~
on the submanifoldMo
isgiven by
and the
corresponding
reduced Hamiltonian :eV(Mo)
has the form:where we have fixed the gauge invariance as follows:
The
resulting
Hamiltonian flow onMo
iscompletely equivalent
to theflow
(35)
on M:with condition
div p
+ yr =Co (x).
Thus we have built the closed Hamiltoniantheory
related to theLagrangian (28),
on thesymplectic phase
spaceM,~
CJR2))
xR)).
4. AN
EQUIVALENT
OPERATOR APPROACHLet us be
given
anydynamical system
on some functional manifold M 3 u, where 7~ : M --+
T(M)
is a smoothvector field on
M,
the flow(47)
can be recast into thefollowing
Eulerianform
Vol. n° 5-1999.
510
with the action functional S to be
if and
only
if thedynamical system (47)
is Hamiltonian on M. This meansthat if
where the
symplectic
structure ~2:T (M) ~ T * (M)
is anondegenerate skew-symmetric operator
on theadjoint
spaceT (M), satisfying
thefollowing
condition:The element E
T * (M)
isgiven by (49)
as the definition. It is obvious that theoperator
~2 in(51 )
isskew-symmetric
oneacting
onT(M).
From(49)
we can obtaineasily
that theequation
gives
rise to the Hamiltonian form as follows:using
we have
equivalently
that is we have obtained the standard Hamiltonian form of the
system (47).
Besides we claim that the local functional ET * (M)
satisfiesthe
following determining (or characteristic)
Laxtype equation [ 13, p. 216]:
where ~
ED(M)-some
canonical transformationgenerating
functionalin the Hamiltonian-Jacobi
theory. Indeed,
from(55)
we canget
thatAnnales de l’Institut Henri Poincare - Physique " theorique "
that
is,
the
generating
functional of the Hamiltoniansystem (54).
The above results are
completely
valid up to the exact form of the Hamiltonian function 1{ because of the someambiguous
definition of the local functional ET * (M) . Indeed,
we havewhere 1/1
ET * (M)
is somegradient-wise
kernel of the vector fieldK[u]: (1/1, I~)
=0, 1/1’ = 1/1’*,
it means that there exists some functionalQ
ED(M)
such thatgrad Q == 1/1
on M. Here and below thesign "’ "
denotes the standard Frechet derivative of a local functional on M.
Therefore,
for the Hamiltoniandensity H[u]
to be found in exactform,
we need to calculate the
quantity
determining
the"Lagrangian" [u ].
Further we construct the Hamil- toniandensity
as follows:stemming
from(57).
This consideration ends the formalsetting
of theHamiltonian
theory
via theoperator approach
on the manifold M with agiven dynamical system (47).
Josephson medium Example
2To use the above results to the
Lagrangian (28),
we find that itsdensity
takes the
following
form on an extended manifold M’ _(A,
q;(9, À)
n° 5-1999.
where
by
definition q :=At , ~, :
:= ET * ( M’ ) ,
v are someLagrangian multipliers,
and(Here
thesign " ~ "
denotes the usualtransposition operation. )
From(62) using
the formula(51 )
we obtain thecorresponding symplectic
operator~2 as follows:
The inverse
operator S2-1
isgiven by
theexpression:
Thus we can
represent
the Eulerdynamical system 8S[A,
q;(9, A]
= 0as a Hamiltonian one:
where
by
definitionand
It is
obviously proved
0 that thesystem
ofEqs. (67)
iscompletely equivalent
to(35).
From(67)
one " cansimply
extract the above " found oAnnales de l’Institut Henri Poinearé - Physique theorique
vector
field K[A,
q;(9~]:
We see from
(68)
thatphase
variables q and À are notindependent,
that
compels
us to involve new Clebschtype independent phase
variables7T, p as follows:
As a result we obtain a new evolution
system
on aproperly
extendedfunctional manifold
Mn:
that is the
system completely
identical with(35),
the function~(x),
x E
being interpreted
as a functionalparameter.
From(69)
we caneasily
obtain also that the constraintis satisfied on the manifold
Myr identically.
The flow(70) persists
theconstraint
(71)
as well:upon all orbits of
(70).
Theimportant
consequence of the considerationperformed
above is that theLagrangian (28)
can berepresented
in thecorrect
nondegenerate
formonly
on the extended functional manifoldMn, giving
rise to thefollowing expression:
n° 5-1999.
514
where the vector c~ E serves as a
Lagrangian multiplier subject
to the constraint p = on the manifoldMn,
the function À-serves like thatsubject
to the constraint yr+ div p
= Co(x)
on From(73)
weget
that thecorresponding vector 03C6
E isgiven
as follows:The
expression (74)
leads ususing (51 )
to thefollowing coimplectic
structure:
Unfortunately,
theoperator (75)
isstrongly degenerate
what meansthe
necessity
to make a reduction of the flow(70)
on some submanifoldMo C Mn .
To
proceed further,
let us determine the Hamiltonian function related with the flow(70).
To do this we need to calculateonly
the functional~
EV(Mn) using
the definition(66):
The necessary condition for the above vector a E
T*(Mn)
to be agradient
is thefollowing
Volterra criterium: a’ =a’*, i.e., selfadjointness
of the
corresponding
Frechet derivative. It is easy to show that this condition holdsgood
onMn.
Thus we are inposition
to calculate thefunctional ~
E via thefollowing homotopy
formula:Annales de l’Institut Henri Poinearé - Physique theorique
Whence the Hamiltonian functional 1{ E
V(Mn)
isgiven
via(66)
asfollows:
where we denoted
Thus
Thereby,
we havegot
the Hamiltonian functional which up to factor 2 coincides with thatgiven by
formula(34)
and thatgiven
in[3,9].
Fromthe structure of
(75)
one can see that thedynamical system (70)
allowsthe
nondegenerate
reduction upon the submanifoldMo
C M" with the canonicalsymplectic
structuren° 5-1999.
516 J.A. ZAGRODZINSKI that is
where
by
definition we haveadopted
thefollowing
Poisson bracket notation.Note that for the above
functional ~
E to be obtained via calculations(76),
thefollowing expressions
for Frechet derivatives I~’and K’* were used
5. SOME COROLLARIES AND PERSPECTIVES
We have demonstrated two different
approaches
togeneral
Euler-Lagrangian type dynamical systems
on functional manifolds with con-straints of a gauge
type.
The constraints
(31 ) being
found viaanalysis
theLagrangian problem (28),
as was shownby (72),
is asingle
and of the first class. This factsuggests
toperform
the standard reduction upon some invariant submanifold on which the reducedsymplectic
structure isnondegenerate.
This was the case treated in detail in this
study
of thespecial Lagrangian problem (28).
-The momentum map
y[A,p,(9,7r],
definedby (42)
in the frame of ourapproach
admits a furtherphysical interpretation being important
for thestudy
ofJosephson
media moredeeply. Especially,
the constraintAnnales de Henri Poincare - Physique theorique -
imposes
on the reducedsymplectic
manifoldMo
Csome functional
conditions,
which can beinterpreted
as acharge density a’priori
disseminatedthroughout
aJosephson
medium under consideration. This constraintimposed
on the wanted solutions to theEqs. (46)
shouldobviously play
the role of thephysical compatibility
with the flow of
charged particles
in theJosephson
medium.Indeed,
ifthese collisionless
particles
interact with the inducedelectromagnetic
Maxwell
field,
one can write down thefollowing Josephson-Vlasov (J-V) dynamical equations
on the functional manifold = M x
F,
where the lastequation
determines the ambient
charge density
as acompatibility
constraintcondition. The
quantity f
E F CR+))represents
thecharged particle density
inposition-velocity
space at time t E E M is theparticle charge
and m E is theparticle
mass. Here we consider the motion of a cloud ofcharged particles
inside aJosephson
medium of asingle species
forsimplicity.
Ageneralization introducing
severalspecies
is
pretty elementary.
We choose further the natural unitsystem
in whiche = m = c = 1. Our
goal
now is to understand a Hamiltonian structure of the J-VEqs. (88) using
the group theoretical momentum map reductionapproach
ofMarsden-Weinstein[ 17] .
Toproceed
further one needs theinvestigation
of thesymmetry properties
of thecorresponding
to(88)
Hamiltonian functional
518 ZAGRODZINSKI
Since Hamiltonian
(92)
is written inimproper phase
space variables(x, v)
E we introduce a propermomentum-position phase
space with variables(x, y)
Ecarrying
the canonicalsymplectic
struc-ture
52~2>
:= ndx~
:==(dy,
nJx),
theconsistency
conditiony = v + A
being
satisfiedthroughout
theJosephson
medium.Corresponding
to the definition of thephase
space asabove,
weintroduce a new
particle density
distribution functionf(x, y)
E F Cas follows
identically
upon for all t E ?. As a result we obtain the nextexpression
for the Hamiltonian functional(92)
Let us consider the
following
functional gauge transformationof the whole
phase
space := M x F CX
~*(R~; JR),
where we denoted
by M)
CJR2))
the dual space to the Liealgebra R)
of canonical transformations of thesymplectic
space introduced above. The gauge function
exp((9)
EG,
used
before,
is chosenarbitrary,
butsatisfying
the naturalgrowth
atinfinity.
The Liealgebra R)
consists of elementsisomorphic
to Hamiltonian vector fields on
with respect
to the canonicalsymplectic
structureSZ ~2~
==(dy,
ndx)
mentionedalready
above. Since the set of these Hamiltonian vector fields is in one to onecorrespondence
to the set of
generating
Hamiltonian functions thephase
space F C describescorrectly
an infinite-dimensional space ofparticle density
distribution functionsf(x, y)
dxdy
at thepoint (x, y)
EAnnales de l’Institut Henri Poincaré - Physique theorique
The last considerations
give
rise togetting
a canonical Poisson bracket on thephase
space F as a Lie-Poisson bracket[16,18]
as follows:for any smooth functionals E
D(F)
the bracket reads aswhere
{ ~, ~ }T* ~~2~
denotes the standard Poisson bracket oncorresponding
to the canonicalsymplectic
structure[2(2)
==In
analogous
way one can build asymplectic
structurenaturally
connected with the
Maxwell-Josephson part
of the Hamiltonian(94).
Indeed,
if as aconfiguration
space for this Hamiltonianpart
isconsidered,
the
corresponding symplectic phase
space to the space of vectorpotential
fields A E can be defined. It is some set M
pertaining
tothe
cotangent
bundleJR2)), carrying
the canonicalsymplectic
structure :== where
(A, p)
E M. One caneasily
be convinced that the
Maxwell-Josephson part
of the Hamiltonian(94)
isjust
describedby
the canonicalsymplectic
structure thatwas used
intensively
in Section 2. Thus we have constructed via the canonicalprocedure
thesymplectic
structurec~~2~; c~F ~
upon thephase
space := M x
F,
whereby c~F2~
is denoted thesymplectic
structurecorresponding
to the Lie-Poisson bracket{’, } F (96)
on the distribution functionphase
space F CTurning
now back to the gauge group transformation 2014~M~B
O ER)
definedby (95),
we claim that:( 1 )
the Hamiltonian functional(94)
is notinvariant,
but(2)
thesymplectic
structurec~~2~
is invariant withrespect
to the mentioned above gauge transformation.To cope with this situation we consider as before a new
properly augmented symplectic
functionalphase
space :=Mn
xF,
whereby
the definition CMn
x This meansthereby
thatr*(Or(G
x M -~M)),
whereby Or (G
x M -~M)
we denoted aone-parameter
orbit of the group action(95 )
on thesymplectic
manifoldM. Since the
symplectic
structure is invariant withrespect
to this groupaction,
we claim due to thegeneral theory [ 16,19,20]
and[ 17],
that this orbit of M is
necessarily
asymplectic
space with a canonical Lie-Poisson structure. In our case we obtain thefollowing symplectic
ZAGRODZINSKI structure upon this orbit
where due to the construction above
(O, ~t) E
As a consequence the inducedsymplectic
structurec~~.2~
= 0c~F ~
is asubject
to furtherconsiderations.
Let us consider now the Hamiltonian functional
(94) properly
extendedas the one on the
augmented phase
spaceIt is obvious now that both
( 1 )
the Hamiltonian functional(97)
isinvariant,
and(2)
thesymplectic
structurec~~2~
is invariant withrespect
to the extended group action(95)
uponThis means that
for all E
G,
whereby
definitionM 3
(A,
p,0,7T) -~ (A + V~,
p, 0 -~, 7T)
e M.( 100) Thus,
the same as it was in Section2,
we can find thecorresponding
to(99)
momentum map Y :~ G*
as follows: forany 03C8 ~G
Annales de l’Institut Henri Poincare - Physique " theorique "
whence at each
point (A,
p,0,7r; f )
E7~(9r(M~)) ~
where we denote some
regular
Liesub algebra
of the Liegroup G.
As the first inference of the above consideration we can conclude that the
Josephson-Vlasov dynamical system (88)-(91 )
in theproperly
extended form on the
phase
spacewith
respect
to the extended Hamiltonian functionadmits the invariant Marsden-Weinstein
type
reduction[ 17]
upon thefollowing
reducedphase
space := =Co) / G
cThis means that the
dynamical system ( 103)-( 107)
upon the invariant submanifold C definedby
the constrainttakes the form
522 ZAGRODZINSKI
for some
arbitrary
fixedparameter
function 8 E~.
It is easy to prove alsothat ct
= 0 for all t E R withrespect
to the evolutionEqs. ( 103)-( 107).
Returning
back to the Hamiltonian(92),
theresulting
J-Vequations
upon the
phase
spaceM(f)0 ~ (A,
p,f(x, v) )
due to the transformation(93)
read as follows:Introducing
newphysical
variables E := -p and B :=rot A,
the J-Vsystem ( 112)
will take the formon some
physical
spaceMo 3 (E, B, /).
The J-V evolution
system ( 115)-( 119)
admits the Lie-Poisson struc- ture[ 18 ] given by {’, naturally
induced from thesymplectic
struc-ture
c~~2~
builtabove, i.e.,
for any a,~8
ePoincaré - Physique théorique
As a
result,
the J-Vdynamical system ( 115)-( 119)
readscompactly
asfollows
The Hamiltonian structure
( 120)
for the J-Vdynamical system ( 115)- ( 119)
seems to be ofgreat
interest forsuperconductive
theories because it enables theapplication
of thepowerful techniques
ofperturbation theory
for Hamiltoniansystems.
Therelationship
between someclassical, semiclassical,
evenquantum aspects
ofJosephson
media and J-Vtheory
with its various truncations
requires
furtherdevelopment.
In this frameit seems also of interest some modification
[9]
of J-Vtype
evolutionequations
aswith
compatibility
constraints on the ambientcharge density div p -
~R2 f(x, v)
d v = 7t , that is ct = 0 for c = 7T +div p - ~R2 f (x, v)
d v uponTreating
the model( 122)-( 124)
in detail it seems also to shine a newlight
at someconceptual problems concerning
thestability
of vortextype
solutions upon aspecial type background [9].
The latter leads to the verification of collective effects
theory
viaartificially
built andproduced
discrete models which mimicJosephson
media.