HAMILTON-JACOBI EQUATIONS AND QUANTUM MECHANICS 379
greater than the size of an atom (i.e. much greater than 10 angstroms or so).
We require the dependence of H(q, p) on its last n arguments to be a linear
combination of powers, giving for example
e) =
h
y
ntt az
H (qi, -'h
aq;
- 2m
aq2 +
V (qi),
(8.44)
which is the Hamiltonian of a single particle of mass m moving in a potential V
in n dimensions. The WKB ansatz
' - Ae1°(q,)/h can be expected to yield a good
approximation on a scale of many angstroms and it gives
H(g1,p1) = E,
which, since E is constant, is equivalent to (8.41) as long as we identify the de-
pendent variable with the phase u of the wave function t'.187 Thus the relation of
the wave function in quantum mechanics to the trajectories of classical mechanics
is analogous to that between the electromagnetic field and the light rays of geo-
metric optics; both hinge on the role played by the phase of the wave function.
Note that, when we identify Hamilton's equations of mechanics with Charpit's
equations for the Hamilton-Jacobi equation (8.41), the parameter t along the
characteristics must be taken to be real time. Indeed, T in (8.42) is real time in
the Lagrangian formulation. However, the parameter along the characteristics of
the eikonal equation (8.1) cannot be thus identified because (8.1) only applies to
the spatial description of a single high-frequency component in the solution of the
wave equation. Indeed, it is helpful to think of the ray parameter in this case as a
weighted distance, as explained in Exercise 8.17.
A quantity of primary practical interest in quantum mechanics is the spectrum
of energy levels E, which emerge as eigenvalues in this theory. We can attempt
to find the energy levels for small h by generalising the argument of §8.2.4, which
corresponds to a very simple case in which V = 0 in two dimensions. To do this we
must generalise the all-important conditions that the change of phase along any
closed path, in particular a ray path, if one can be found, is an integer multiple
of 21rnh. Now we already know u in principle, assuming we have been able to
integrate Hamilton's equations because, by Charpit's method,
du
rn
OH
n dqi
dt = p'8
p, _
p` at
so
J
u=u+
p;dg,
(8.45)
i=1
where uo is the value of the phase on the boundary. It is a well-known result
of classical mechanics that the minimisation of the action (8.42) yields (8.45),
167 Unfortunately, when there are many particles, each has to have its own wave function t and
the dimensionality of the resulting differential equation is the number of degrees of freedom of
the system, which may be enormous.