A NNALES DE L ’I. H. P., SECTION C
E UGÈNE G UTKIN
Conservation laws for the nonlinear Schrödinger equation
Annales de l’I. H. P., section C, tome 2, n
o1 (1985), p. 67-74
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Conservation laws
for the nonlinear Schrödinger equation
Eugène GUTKIN (*)
Department of Mathematics, Columbia University, New York
and MSRI, 2223 Fulton Street, Berkeley, CA 94720 (**)
Vol. 2, n° 1, 1985, p. 67-74. Analyse non linéaire
ABSTRACT. - We propose a method of
calculating
the operator den- sitieshn n
=0, 1, ...
of the conservation laws for the quantum nonlinearSchrodinger equation.
It follows from the methodthat hn
are,polynomials
in fields and their derivatives and in the
coupling
constant. The densitieshn n
4 areexplicitly
calculated.Comparison
with theintegral
densitiesbn n
=0, 1,...
for the classical nonlinearSchrodinger equation
showsthat the
correspondence between hn
andbn
breaks down after n = 3.RESUME. - On propose une methode pour calculer les densites
ope-
ratoires
hn n
=0, 1,
... pour lesintégrales
de1’equation
deSchrodinger
non lineaire
quantique.
Il s’ensuit que leshn
sont des fonctionspolynomiales
des
champs,
de leurs derivees et de la constante decouplage.
Les densites4,
sont calculéesexplicitement.
En lescomparant
avec les densitesintegrales
=0, 1,
... pourl’équation
deSchrodinger
non lineaireclassique,
on voit que lacorrespondance entre bn
ethn
n’estplus
valablepour n > 3.
1. INTRODUCTION .
We consider the quantum nonlinear
Schrodinger equation (NLSE)
in 1 + 1
space-time
dimensions(*) Research supported in by NSF Grant MCS 8101739.
68 E. GUTKIN
Its Hamiltonian
is the second
quantized
form of the manybody
HamiltonianHamiltonian
(1.3)
describes the interaction of N identicalparticles
onthe line via elastic collisions and c is the
strength
of interaction.The famous
« Bethe Ansatz »
[1 ] [2] ]
exhibits the system ofgeneralized eigenstates I
...,kN) ~ _ ~
of which iscomplete
if c >_ 0. We haveSince Bethe Ansatz
eigenstates depend
on N quantum numbersk1,
...,kN
the Hamiltonian
(1.3)
must becompletely integrable.
This means that thereare N
independent
operators =1, ..., N
such thatN
=
( -
is of course the total momentum and is thei= 1
Hamiltonian
(1.3).
Existence of shouldimply
the infinite sequence ofindependent
conservation lawsHn n
=1, 2,
... for the NLSEgiven by
their operatordensities hn
Operators Hn
arecompletely
characterizedby
the property that for any NAnnales de l’lnstitut Henri Poincaré - Analyse non linéaire
It is desirable to have
explicit expressions
for the operator densitieshn.
In this paper I suggest a method for
calculating hn
for any n.Using
thismethod I calculate
h3
andh4.
In section 4 Icompare hn
with the func-tional densities
bn
of theintegrals
of motion for the classical NLSEThacker
[3] ]
has obtainedh3 using
acompletely
differentapproach.
Kulish and
Sklyanin [4] ]
and Thacker[4] ]
haveintegrated (1.1) using
the quantum inverse
scattering
method. Their method however does notyield explicit
formulasfor hn
in terms of the fields(*).
2. N-PARTICLE SECTOR
In this section we fix N and omit the
superscript
N in formulas. TheN
Hamiltonian
H2
isequal
to theLaplacean -
with theboundary
conditions
4-/
on
hyperplanes {xi - xj
= =1, ..., N.
Because of the symmetry of function F it suffices to restrict it to
x2 ... and to
impose boundary
conditionson
hyperplanes
x~ = =1,
..., N - 1.I will use the
following
fact. There is an operator P onsymmetric
func-tions in RN that intertwines
Laplacean
with the Neumannboundary
conditions
and
Laplacean
withboundary
conditions(2.2)
for c > 0. The operator P constructed as follows. For letPij
begiven by
Denote
by
S the operator from all functionsf
on f~N intosymmetric
func-tions on R~’ obtained
by restricting f
toR~
and thenextending
it to f~~’by
symmetry. Then[5 ]
70 E. GUTKIN
Denoting by A 2
theLaplacean
withboundary
conditions(2. 3)
we express theintertwining
property of Pby
N
Let
~1"
begiven by ( - i )n C~"~(~.xn
with «higher »
Neumannboundary
conditions
i=1
for i =
0, 1,
...,[n/2 ] -
1 onhyperplanes {
xk =xk + 1 ~ k
=1,
..., N -1.Let
Hn
be defined fromfor n =
1,
.... Since operatorsOn
commute,Hn
also commute. It follows from(2. 5)
that P takesboundary
conditions(2. 7)
intoboundary
conditionsN
So
Hn
isequal
to( -
withboundary
conditions(2 . 9)
fori= 1
i =
0,
...,[n/2 ] -
1. It remains to obtain formulas forHn
similar to the formula(1.3)
forH2.
Let
g(x 1,
...,xN)
be aninfinitely
differentiable function and letf satisfy
the
boundary
conditions(2.9).
ThenIntegrating by
parts andtaking (2.9)
into account we getAnnales de l’lnstitut Henri Poincaré - Analyse non linéaire
Integrating by
partsagain
After one more
integration by
parts and obvious transformations(2.12)
becomes
which
yields
For
H4
we haveIntegrating by
parts theright
hand sideIntegrating by
parts the first term in(2.16)
weget
72 E. GUTKIN
Integrating (2.17) by
partsagain
andremembering
the second term in(2.16)
we have
The last term in
(2.18)
canagain
beintegrated by
partsyielding
From
(2.18)
and(2.19)
we have3. SECOND
QUANTIZED
FORM OFH,
A standard calculation
gives
Annales de l’lnstitut Henri Poincaré - Analyse non linéaire
Thus Also
After obvious
integrations by
parts we haveThus
4. COMPARISON WITH CLASSICAL INTEGRALS The classical NLSE
(or
Zakharov-Shabatequation [6 ])
is a
completely integrable
Hamiltonian system withinfinitely
manydegrees
of freedom
[7].
Inparticular (4 .1)
has an infinite number ofintegrals
of motion
q).
The functionalsBn
are determinedby
the local den-sities
bn
The densities
bn
are found from the recurrence relationand
From
(4. 3)
and(4.4)
get74 E. GUTKIN
The local
densities hand g
that differby
a total derivative areequivalent
h ~ g because
they
define the same functionalfoo
=foo dxg(xj.
We have - °° - °°
We see from
(3 . 2)
that1i3
differs fromb3 by
the factor( - i )3 only.
Onthe other hand the difference
between h4 (3 . 5)
andb4
is essential.Replacing
h4 by
anequivalent
operatordensity h4
the closest that we can get tob4
isThe difference
corresponds
to.c~ )
which is a nontrivialdensity.
5. CONCLUSION
The nonlinear
Schrodinger equation (1.1)
has an infinite sequence of conservation lawsHn given by
the’ operator densities~P(x)).
The densities
hn
can be foundusing
the method of sections 2 and 3. It is clear from the method thathn
arepolynomials
in the fields and their derivatives.Besides hn
arepolynomials
in thecoupling
constant c. Thedegree of hn
in c is[n/2 ].
Correspondence between hn
and theintegral
densitiesbn
of the classi-cal NLSE
(4.1)
breaks down at n = 4.REFERENCES [1] E. LIEB and W. LINIGER, Phys. Rev., t. 130, 1963, p. 1605.
[2] C. N. YANG, Phys. Rev. Lett., t. 19, 1967, p. 1312.
[3] H. B. THACKER, Phys. Rev., t. D17, 1978, p. 1031.
[4] Articles in Integrable Quantum Field Theories, Proceedings, Tvarminne, Finland 1981, Lecture Notes in Physics, 151, Springer-Verlag, New York, 1982.
[5] Another intertwining operator P was constructed in E. GUTKIN, Duke Mat. J.,
t. 49, 1, 1982 on the space of all functions not regarding the symmetry.
[6] V. E. ZAKHAROV and A. B. SHABAT, Zh. Eksp. Teor. Fiz., t. 61, 1971, p. 118;
Sov. Phys., JETP, t. 34, 1972, p. 62.
[7] V. E. ZAKHAROV and S. V. MANAKOV, Teor. Mat. Fiz., t. 19, 1974, p. 332.
Theor. Math. Phys., t. 19, 1975, p. 551.
(Manuscrit reçu le 25 juin 1984)
Annales de l’lnstitut Henri Poincaré - Analyse non linéaire