Revisited
Analytical
Mechanics
245
which gives the ofd conditions for
a
transformation to be completely
canonical,
C(rhThr
Xk)
=
@
3
this time with the right covariance of indices!
0
The operator
that we called
Harniltonian vector
field
in Part
I,
is
just the local ex-
pression
of
the
H~iltoni~ vector field
ix,~
=
df
,
here introduced.
and the Hamilton equations,
0
A
compfete andogy exists between the intrinsic Lagrange equations
i~w~
=
-dE&,
ixw
=
-dH
.
The main difference between them, consists in the fact that, in the
Hamilton equations, the “interaction”
is
present only in the Hamilto-
nian function, while in the Lagrange equations, the “interaction,”
via
the Lagrangian function,
is
also present in the symplectic structure
WE.
In other words, the symplectic structure
w,
in the Hamilton equations,
is
universal,
in the sense that it does not depend on the considered
dynamical system. This
is
not true for Lagrange’s equations. This
feature is
a
consequence
of
the fact that the cotangent bundle
T*Q,
of
a manifold
Q,
carries a
natural
symplectic structure, while the tangent
bundle
‘T&
has not such
a
structure.
0
A
Nother-type theorem, connecting
a
symmetry to
a
first integral, cm
be stated in the Hamiltonian formalism
M
well
as
in the Lagrangian,
even more easily. Indeed, let
A
and
Xj
be globally Hamiltonian vector
fields,
with ~amiIto~ian functions given
by
H
and
f,
respectively; i.e.
iAw
=
-dH,
ix,w
=
-df
.
We thus have
Lx,
H
=
0
es
ix,
dH
=
0
~3
ix,iAw
=
0
H
w(Xf,
A)
=
0
es
{HJ}
=
0,