Non-Noether symmetries in singular dynamical systems
Introduction
Noether's theorem associates conservation laws with particular continuous symmetries of
the Lagrangian. According to the Hojman's theorem
[1]-
[3]
there exists the definite correspondence between
non-Noether symmetries and conserved quantities. In 1998 M. Lutzky showed that several integrals of
motion might correspond to a single one-parameter group of non-Noether transformations
[4]. In the present paper, the extension of Hojman-Lutzky theorem to singular dynamical systems is considered.
First of all let us recall some basic knowledge of description of the regular dynamical systems
(see, e. g.
[5]).
In this case time evolution is governed by Hamilton's equation
iXhω + dh = 0,
where
ω is the closed
(
dω = 0) and non-degenerate
(
iXω = 0 ⇒ X = 0) 2-form,
h is the Hamiltonian and
iXω denotes contraction of
X with
ω.
Since
ω is non-degenerate, this gives rise to an isomorphism between the vector
fields and 1-forms given by
iXω + α= 0.
The vector field is said to be Hamiltonian if it corresponds to exact form
iXfω + df = 0.
The Poisson bracket is defined as follows:
{f , g} = Xf g = − Xg f = iXf
iXgω.
By introducing a bivector field
W satisfying
iXiYω = iW iXω ∧ iYω,
Poisson bracket can be rewritten as
{f , g} = iW df ∧ dg.
It's easy to show that
iXiYLZω =
i[Z,W] iXω ∧ iYω,
where the bracket
[ · , · ] is actually a supercommutator,
for an arbitrary bivector field
W = Vs ∧ Us we have
[X,W] = [X,Vs] ∧ Us
+ Vs ∧ [X,Us]
Equation
(6) is based on the following useful property of the Lie derivative
LXiWω = i[X,W]ω +
iWLXω.
Indeed, for an arbitrary bivector field
W = Vs ∧ Us we have
LXiWω = LXiVs ∧ Usω =
LX iUsiVsω
= i[X,Us]iVsω +
iUsi[X,Vs]ω +
iUsiVsLXω =
i[X,W]ω + iWLXω
where
LZ denotes the Lie derivative along the vector field
Z.
According to Liouville's theorem Hamiltonian vector field
preserves
ω
LXfω = 0;
therefore it commutes with
W:
[Xf ,W] = 0.
In the local coordinates
zs where
ω = ωrsdzr ∧ zs bivector field
W has the following form
W = Wrs∂zr ∧ ∂zs where
Wrs is matrix inverted to
ωrs.
Case of regular Lagrangian systems
We can say that a group of transformations
g(z) = ezLE generated by the vector
field
E maps the space of solutions of equation onto itself if
iXhg*(ω) + g*(dh) = 0
For
Xh satisfying
iXhω + dh = 0
Hamilton's equation.
It's easy to show that the vector field
E should satisfy
[E , Xh] = 0
Indeed,
iXhLEω + dLEh =
LE(iXhω + dh) = 0
since
[E,Xh] = 0.
When
E is not Hamiltonian,
the group of transformations
g(z) = ezLE is non-Noether
symmetry (in a sense that it maps solutions onto solutions but does not preserve action).
Theorem:
(Lutzky, 1998) If the vector field
E generates non-Noether symmetry,
then the following functions are constant along solutions:
I(k) = iWk ωEk k = 1...n,
where
Wk and
ωEk are outer
powers of
W and
LEω.
Proof:
We have to prove that
I(k) is constant along
the flow generated by the Hamiltonian. In other words, we should find that
LXhI(k) = 0 is
fulfilled. Let us consider
LXhI(1)
LXhI(1)
= LXh(iWωE) =
i[Xh , W]ωE
+ iWLXhωE,
where according to Liouville's theorem both terms
[Xh , W] = 0 and
iWLXhLEω =
iWLELXhω =
0
since
[E , Xh] = 0 and
LXhω = 0 vanish.
In the same manner one can verify that
LXhI(k) = 0
Case of irregular Lagrangian systems
The singular Lagrangian (Lagrangian with vanishing Hessian) leads to degenerate 2-form
ω and we no longer have isomorphism between vector fields and 1-forms.
Since there exists a set of "null vectors"
us such that
iusω = 0 s = 1,2 ... n − rank(ω),
every Hamiltonian vector field is
defined up to linear combination of vectors
us. By identifying
Xf
with
Xf + Csus, we can introduce equivalence class
Xf∗ (then all
us belong to
0∗ ).
The bivector field
W is also far from being unique, but if
W1 and
W2 both satisfy
iXiY ω =
iW1,2 iXω ∧ iYω,
then
i(W1 − W2) iXω ∧ iYω = 0 ∀X,Y
is fulfilled. It is possible only when
W1 − W 2 = vs ∧ us
where
vs are some vector fields and
iusω = 0
(in other words when
W1 − W2 belongs to the class
0∗)
Theorem:
If the non-Hamiltonian vector field
E
satisfies
[E , Xh∗] = 0∗ commutation
relation (generates non-Noether symmetry), then the functions
I (k)
= iWkωEk k = 1...rank(ω)
(where
ω E = LEω) are constant along trajectories.
Proof:
Let's consider
I(1)
LXh∗I(1)
= LXh∗(iWωE)
= i[Xh∗ , W]ωE +
iWLXh∗ωE = 0
The second term vanishes since
[E , Xh∗] = 0∗ and
LXh∗ω = 0. The first one is
zero as far as
[Xh∗ , W∗] = 0∗ and
[E , 0∗] = 0∗ are satisfied. So
I (1) is conserved.
Similarly one can show that
LXhI(k) = 0 is
fulfilled.
Example:
Hamiltonian description of the relativistic particle leads to the following action
A = p0dx0 + psdxs
where
p0 =
with vanishing canonical Hamiltonian and degenerate 2-form defined by
p0ω = (psdps ∧ dx0 + p0dps ∧ dxs).
ω possesses the "null vector field"
iuω = 0
u = p0∂x0 + ps∂xs.
One can check that the following non- Hamiltonian vector field
E =p0x0∂x0
+ p1x1∂x1 + ⋯ + pnxn∂xn
generates non-Noether symmetry. Indeed,
E satisfies
[E , Xh∗] = 0∗ because of
Xh∗ = 0∗ and
[E,u] = u.
Corresponding integrals of motion are combinations of momenta:
I(1) = ps
I(2) = prps
⋯
I(n) = ps
This example shows that the set of conserved quantities can be obtained from a single
one-parameter group of non-Noether transformations.
Acknowledgements.
Author is grateful to Z. Giunashvili and M. Maziashvili for
constructive discussions and particularly grateful to George Jorjadze for invaluable help.
This work was supported by INTAS (00-00561)
and Scholarship from World Federation of Scientists.
References
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1992 J. Phys. A: Math. Gen. 25 L291-295
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1994 J. Phys. A: Math. Gen. 27 L59-60
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1995 J. Phys. A: Math. Gen. 28 L637-638
- M. Lutzky, New derivation of a conserved quantity for Lagrangian systems,
1998 J. Phys. A: Math. Gen. 15 L721-722
- N.M.J. Woodhouse, Geometric Quantization, Claredon, Oxford, 1992.
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